REPORT
OF THE
THIRTIETH MEETING
Vie
' Rieti foN
OF THE
BRITISH ASSOCIATION
FOR THE
ADVANCEMENT OF SCIENCE;
HELD AT OXFORD IN JUNE AND JULY 1860.
LONDON
JOHN MURRAY, ALBEMARLE STREET.
1861.
PRINTED BY
TAYLOR AND FRANCIS, RED LION COURT, FLEET STREET.
CONTENTS.
Onwmeers and Rules of the Association”. 25.2... .ceccscacc ccs ccouee'ees as
Places of Meeting and Officers from commencement ..........+00+00
Treasurer's Account
Table of Council from commencement ...........0.eescesescocccecccene ves
Page
XVii
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eee ema LACT CIN! bate ek cecetccidea¥odiae cbals coc caanegucednere +’ eccewececsaes KEVIIL
Officers of Sectional Committees
Corresponding Members.. siahdioale Su Uvabaiiationick
Report of the Council to the Gentstal Cendaitibe Senay asacWet clasp aet sat
Report of the Kew Committee weahes
Report of the Parliamentary Committee .......ssceeceeceeeeseeeseecee ees
Recommendations for Additional Reports and Researches in Science
XX1x
Xxx
XXX
Xxxi
xliv
xlv
PrmmmmPT ONG. GATES 5. uc cau ads cacao ceacaressaceessovevas ves ecchvsses XIVIIL
General Statement of Sums paid for Scientific Purcases Reena teen
Extracts from Resolutions of the General Committee
Arrangement of the General Meetings Raneke(canane ney atte
REESE FODUICW nu pass onicins-nnacis axeikns acandhebn sos seeson den aus seh soe
REPORTS OF RESEARCHES IN SCIENCE.
Report on Observations of Luminous Meteors, 1859-60. By a Com-
mittee, consisting of James GLAIsHER, Esq., F.R.S., F.R.A.S.,
Secretary to the British Meteorological Society, &c.; J. H. Giap-
STONE, Esq., Ph.D., F.R.S. &c.;. R. P. Ga a: BGS... &e. ;
and I. J. Lowe, Esq., F.R.A.S., M.B.MLS. &c.
Report of the Committee appointed to dredge Dublin aay ‘By ue R.
Kinauan, M.D., F.L.S., Professor of Zoology, Government School
of Science applied to Mining Aue the Arts: si..5s05s
Report on the Excavations in Dura Den. oy fis: Rey eas
PMRMBISTS (NaMNE) oP ss re eig ee ccs creclelh asic nciriee\dee's odoatcdaeee secs ssdeccterces
Report on the Experimental Plots in the Botanical Garden of the Royal
Agricultural College, Cirencester. By James Buckxmay, F.LS.,
F.S.A., F.G.S. &c., Professor of el and whe 4 mechs Agri
cultural Coles e: ep casgetoes cos vee
27
34
vi CONTENTS.
Page
Report of the Committee requested “to report to the Meeting at
Oxford as to the Scientific Objects to be sought for by continuing
the Balloon Ascents formerly undertaken to great Altitudes.” By
the Rev. Roserr Wacker, M.A.,, F.R.S., Reader in ee
Philosophy in the University of Oxford. Ae PPer oacesce ys
Report of Committee appointed to prepare a " Self-Recording Meee
spheric Electrometer tor Kew, and Portable Apparatus for observing
Atmospheric Electricity. By Professor W. Tomson, F.R.S. ...... 44
Experiments to determine the Effect of Vibratory Action and long-
continued Changes of Load upon ae iron Girders. ee Wit-
LIAM FairBalrn, Esq., LLD., F.R.S.. a ddgetsnscavees ee
A eT of Meteorites and Fireballs, coe A.D. 2 to A.D. 1860.
By R. P. Gree, Esq., F.G.S8 cw sale «=, 48
Report on the Theory of ates Spare I “By y. 1 Boe
Smitu, M.A., F.R.S., Savilian Professor of Geometry in the Uni-
versity of Oxford aiudssisseisensocieeeceesewess soe yas qeuseesanstn=: Meester 120
On the Performance of Steam- Vessels, the Functions of the Screw, and
the Relations of its Diameter and Pitch to the Form of the Vesssel.
By Vice-Admiral MGORSOM 1060. c0ssecsoscasacersdvexoes sefaatbeaeeame eu teaae
Report on the Effects of long-continued Heat, illustrative of Geological
Phenomena. By the Rev. W. Vernon Harcourt, F.R.S., F.G.S. 175
Second Report of the Committee on Steam-ship Performance............ 193
Interim Report on the Gauging of Water by Triangular Notches
List of the British Marine Invertebrate Fauna ...,.....sscccccsseeeceneenees
CONTENTS. vil
NOTICES AND ABSTRACTS
OF
MISCELLANEOUS COMMUNICATIONS TO THE SECTIONS.
MATHEMATICS AND PHYSICS.
MaTHEMATICS.
Page
Address by the Rev. Professor Price, President of the Section s.secseesseeres L
Dr. BRENNECKE on some Solutions of the Problem of Tactions of Apollonius
of Perga by means of modern Geometry ...scereseseceerereeerersennens aves waaceses
Rev. James Booru on a New General Method for establishing the Theory of
CWONIC SECHONS....050..0sccsecescceseccesceserevcncsos aoenoscec0c1-bechnAneesan Sacneaces we
——____-—____—— on the Relations between Hyperconic Sections and Elliptic
Integrals...,..... A eee saat oa tede aa acene tactic reddeveverneet soles stasiionrastsneteraceccses wn
Mr. A. Cayxey on Curves of the Fourth Order having Three Double Points... 4
Mr. Parricx Copy on the Trisection of an Angle .....sscseseeseseenereeeeerecneusens 4
Rev. T. P. Kirkman on the Roots of Substitutions .....+...ssesereeee Soenenensne ap 4
Rey. T. Rennrson on a new Proof of Pascal’s Theorem ....s.seseesseseserreenes aa 8
Professor H. J. SrepHEeN Smit on Systems of Indeterminate Linear Equations 6
Professor SyLvEsTER on a Generalization of Poncelet’s Theorems for the Linear
Representation of Quadratic Radicals ....sseeeese0 sseesevsenes Gaeressspcevasecege> Paes
Lieut, Heat.
Sir Davip Brewster on the Influence of very small Apertures on Telescopic
IWIBIOH cess ccencccscccacascnesssncassevacceccssecascccseses atvacsdepeesreedddnacsresnes hoes 2 if
——-—-—— on some Optical Illusions connected with the Inversion
of Perspective......+. ad sieacamanadanslisesrewedesa sf Goan detsmaeeaisesaicaine aaiwarpsawene sa desis 7
on Microscopic Vision, and a New Form of Microscope 8
———_——— on the decomposed Glass found at Nineveh and other
PIACES ......500c0esescnesessarssceseesscosees Se dndins ns coisidel ta cshesowandqanesttanease<¥ayieqse¢ 9
Dr. J. H. Guapsrone on his own Perception of Colours ......ssseseee caosvgeecceee 12
—________—_—- on the Chromatic Properties of the Electric Light of
Mercury ..e.csccsscseeeecesccscesccarecnscnccesetesencuscnssansesenenssasensceeesseuesegses hepeete
Professor JeLLerr on a New Instrument for determining the Plane of Polariza-
TLOT wovecccceeecrereeeess eeeeenee wevenecconecsorne ssnaupigedace cette tis sleepin Gealsnniecnelelo's oS
Professor L. L. Linpesiér on the Caustics produced by Reflexion .s.ssseseseeeee 14
Professor Maxwe tt on the Results of Bernoulli’s Theory of Gases as applied
to their Internal Friction, their Diffusion, and their Conductivity for Heat... 15
_ ——__________ on an Instrument for Exhibiting any Mixture of the Co-
) lours of the Spectrum......+. bsp eenes SCOREUED CrarSehao canoes seaeinaesasese eaauclensane 14
viii CONTENTS.
Mr. Munao Ponron’s Further Researches regarding the Laws of Chromatic
Dispersion .....ccccccssscscccscccscccscccotssccsscsascesrcrsaccccsss ssn decneestis ie: ne
Professor Witt1am B, Rocers’s Experiments and Conclusions on Binocular
WiISIONS. cevsrensseccte(erscsensaanecciureccees eonvseeroest ss -ssesaesesasessesaameemeecnen sce
M. Serrin, Régulateur Automatique de Lumiére Electrique ...+++seesesseseeeere
Mr. Batrour Stewart on some Recent Extensions of Prevost’s Theory of Ex-
CHANG CS 2200 5dc46 casctagdcadvs dace act clvatsds vat lesedec1seds ckdebecatescdseatadeenesstel wiees
Mr. G. Jounstone Stoney on Rings seen in viewing a Light through Fibrous
Specimens of Calc-spar......-sseseeeeee Sused decbouscuesiecssseaseuenteusettamadatclcsmiacs
Mr. R. Tuomas on Thin Films of Decomposed Glass found near Oxford .......
ELecrricity, MAGNETISM.
Mr. Joun Atxan Brown on certain Results of Observations in the Observa-
tory of His Highness the Rajah of Travancore ....sscsseseeceseeeeeees = debdoae ate
— on the Diurnal Variations of the Magnetic Declina-
tion at the Magnetic Equator, and the Decennial Period .........:ccsssseeeeeeeees
Sas — on a New Induction Dip-Circle ......0...ccsasessesnsanc
— ——_—_____.__.
on Magnetic Rocks in South India........s.esseeeseeee
on a Magnetic Survey of the West Coast of India...
— on the Velocity of Earthquake Shocks in the Late-
PRE OF DG cies cost as age? va 8i vadsacusates ik cedaths sad satsestesanahtnugaxcdeiees tiers ‘
Mr. A. Crarke on a Mode of correcting the Errors of the Compass in Iron
Ships ..... Sasowoerese cesses scdusoscausaviaspessrssdavessceeeccseacacite setovedesispameeeenennnd
Sir W. Svow Harris on Electrical Force ....ssssssesscccseeceeee javeatacensaeeeaesses
Rev. T. RANKIN on the different Motions of Electric Fluid ...s.....ceseees Soa otvek
Professor W. B. Rocers on the Phenomena of Electrical Vacuum Tubes, ina
letter to Mr. Gassiot ...... seeGaecevaesSis rach s cueteseelasecehe ee eec eee eee epee Sastaces
M. H. von ScutaGintwerr’s General Abstract of the Results of Messrs. de
Schlagintweit’s Magnetic Survey of India, with three Charts .....ssscesseeees &
M. Werner and Mr. C, W. Siemens, Outline of the Principles and Prac-
tice involved in dealing with the Electrical Conditions of Submarine Electric
Telégraphs POOP cee tere tneeesesdbeseos oer
——S
—_—
POCO Pere ee meee Eee ee RE R OHHH EEE E HEH OEE DEES SEES
ASTRONOMY.
Mr. W. R. Birt on the Forms of certain Lunar Craters indicative of the Ope-
ration of a peculiar degrading Force ...s0..0... itegevesecancacee osceetebelawenececss
Professor Hennessy on the Possibility of Studying the Earth’s Internal Struc-
ture from Phenomena observed at its Surface
Rev. Epwarp Hrincxs on some Recorded Observations of the Planet Venus in
the Seventh Century before Christ
Mr. R. Hopeson on the brilliant Eruption on the Sun’s Surface, 1st Septem-
berstS5Ou.n smear eee ccercenccencctsersceseene
Dr. Jonn Lex’s Prospectus of the Hartwell Variable Star Atlas, with six Speci-
men Proofs.........4; :
POPPE ee reer ee ee Peeresens Cee eeereeesnees Peete eeetee
Professor B. Pierce on the Physical Constitution of Comets...ssssesssssseeseeees
een niencmeenes On the Dynamic Condition of Saturn’s BIBUB ascbeoseenene
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CONTENTS.
Professor B. Pierce on the Motion of a Pendulum in a Vertical Plane when
the point of suspension moves uniformly on a circumference in the same
LIFE aadcdcaicoruucecarcotrdscctadcveccsilccecscdsssaetenvecMMes topernerssdsectandaseqssens
MerrEOROLOGY.
Mr. Jouw Baz on a Plan for Systematic Observations of Temperature in
Mountain Countries.........sseseereeeee Sdoetidococta semenneanenisesnd wiatecesaeces pease
Mr. W. R. Bret on Atmospheric Waves ....++.+se++++ -eridnnncce Kepsseenesis Stee casnt
M. Du Bovutay’s Observations on the Meteorological Phenomena of the Vernal
Equinoctial Week ..........++4++ Raeaece see nadi te sesh ane sPaneen Rae semaseehiee.s sachs “ce
Mr. R. DowpeEn on the Effect of a Rapid Current of Air ....+.eeesseeeess yanekaesis
Admiral FrrzRoy on British Storms, illustrated with Diagrams and Charts...
Mr. J. Park Harrrson on the Similarity of the Lunar Curves of Minimum
Temperature at Greenwich and Utrecht in the Year 1859. ticussscessansperarcsst
Professor Hennessy on the Principles of Meteorology ......... = pesoonncentearodee :
Captain Maury on Antarctic Expeditions .c.......--.++++ Rancentenpcsscasacsms ss acoso
on the Climates of the Antarctic Regions, as indicated by Ob-
servations upon the Height of the Barometer and Direction of the Winds at
Sea........ Be cates TEC Cn SLE PCR CORO EEET Cor ceeeeee Scere Lcocedent pecs seneanendees er
Rev. Henry Mosetey on the Cause of the Descent of Glaciers .....+--++++..+0+ :
Rev. T. Ranxtn on Meteorological Observations for 1859, made at Hugagate,
Yorkshire, East Riding ...... Ht SPREE tronat ss ceeset tas sieberetene ere
M. R. pe Scuracintweir on Thermo-barometers, compared with Barometers
at great Heights ............+ beattcnaecetarcctebe dese Reaack vets shee parte eeVab cues seek is
Captain W. Parker Snow on Practical Experience of the Law of Storms in
each Quarter of the Globe... ..csecsseeeceeceeeeseees eeseresasas att qaeeaease Onsen ens eee
Mr. G. J. Symons’s Results of an Investigation into the Phenomena of English
Thunder-storms during the years 1857—59.........- puacavene Sev saetseneescae
ee eeeeee
Professor Witt1am THomson’s Notes on Atmospheric Electricity ....... Banduthie
M. Verpet’s Note on the Dispersion of the Planes of Polarization of the
Coloured Rays produced by the Action of Magnetism* ....... pcb daWaouehaavege vee
Mr. E. Vivian’s Results of Self-registering Hygrometers...secsssseseereserereees re
Rev. A. WELD’s Results of Ten Years’ Meteorological Observations at Stony-
PARSE Peacisccccoscccccccscccctccccccceccccccecesansecccccncesravoccvecttnessverovessvesstoseve
GENERAL Puysics.
Mr. J. 8. Sruarr GLenniz, Physics as a Branch of the Science of Motion ...
a General Law of Rotation applied to the Planets
el
SounD.
Rev. S. Earnsnaw on the Velocity of the Sound of Thunder......seeceseeeseesane
on the Triplicity of Sound ...-..sceseesecersereeeeeeeeeeeeeneeeens
INSTRUMENTS.
Mr. Parrick Aptz’s Description of an Instrument for Measuring Actual
MIBTATICES ccccccceccecccccdsccecececacccecseascasceccocesccccssccnsrncansocoresccccensncecsres
* This should haye been placed in an earlier division.
56
58
58
58
59
> he CONTENTS.
Mr. Parrtck Apte’s Description of a New Reflecting Instrument for Angular
Measurement pcr deneauacseceaes ss saeeenet <anete Merete eae senasbale a riceien © wep aieeiiaiaee
M. E. Becqueret on a Pile with Sulphate of Lead.......... cep patie astemogel eater ~
The Hon. W. BLanp on an Atmotic Ship.....csce.cecerecccsovesees Sesawne dese eweeee sos
Rev. J. Boorn on an Improved Instrument for describing Spirals, invented by
Henry Johnson ....... BO PRRCRO CIEE rerONAGR A Idoshuctnsacne sacbae nn dee se once pareeatemas
Mr. A. Craupet on the Means of increasing the Angle of Binocular Instru-
ments, in order to obtain a Stereoscopic Effect in proportion to their Mag-
TURIN EAP OWED eee wactisavee do cvee ed daemccoeiepe sagen acicdcideemeteicees alas Ssieacseveceuverdeae
—_— on the Principles of the Solar Camera.........ssscessessssecneseees
Mr. Henry Draper on a Reflecting Telescope for Celestial Photography,
erectine at Hastings; near INewiMOrkr.;ccdcsasceasece cevecs teeter esseewtaseveenmece eee
Mr. W. Lapp on an Improved Form of Air-Pump for Philosophical Experi-
ments ...... tee ceeerecseneeccsceeeres eee ececeeceereceessereeescceences teeccveceveveccreeves eee
Mr. Joun Smira on the Chromoscope ..e.esseseeee Ninenecassnansensccascsesegamtaes bss
CHEMISTRY.
Professor ANDREWS OD OZONE ....cecsesesssecseneeseenees Sompanen tatoos ee oansyan ned amgle
Dr. Brrp on the Deodorization Of Sewage)...ccscy<csessessosecececesecrsvusoanssnseneus
Professor B. C. Broprz on the Quantitative Estimation of the Peroxide of
Ly rOpent cern ves-ncets ss aceceseessseaes SACLECET DOHCOEBE Ton J0bk ERO aC anorectic ree one
Mr. G. B. Buckton on some Reactions of Zinc-Ethy] ..........ssesssscseesecsesees
Mr. J. J. Coteman’s Note on the Destruction of the Bitter Principle of Chy-
raitta by the Agency of Caustic Alkali.........ccscossscceescesscesecsecreseeereees oes
on some remarkable Relations existing between the
Atomic Weights, Atomic Volumes, and Properties of the Chemical Elements
Dr. FrANKLAND and B. Duppa on a new Organic Compound containing Boron
Dr, GrapsTone’s Chemical Notes .......2-scccccsssccececore See teviqacodeuseedsepsigareirs
Mr. W. R. Grove on the Transmission of Electrolysis across Glass ...... beans
Mr. A. Vernon Harcourt on the Oxidation of Potassium and Sodium........
Mr. J. B. Lawes and Dr. J. H. Grtperr on the Composition of the Ash of
Wheat grown under various CIrCUMStANCES .....ssececreseceeeeeeeeesenneeeeeeeaees .
Professor W. A. Mixxer on the Atomic Weight of Oxygen.........sssseseeeees ee
C. Moritz von Bosr’s Remarks on the Volume Theory .........00e0+. coeuteye eee
Mr. Warren De ta Rue and Dr. Hugo Muxtuer on a New Acetic Ether
occurring in a Natural Resin......... Sanetps Pam uen tenants easton tcl: cctaes sen ceest items
on the Isomers of Cumol ......... Gekcaaouswases dvanoccucaeaane
Dr. Lyon Pravrarr on the Representation of Neutral Salts on the type of a
Neutral Peroxide HO, instead of a Basic Oxide Hy On ....c.secccveceseesenees rer
Professor T. H. Rowney on the Analysis of some Connemara Minerals .......
on the; CompositioniOf Jebrccc.csts.mensress coves oseewenes
Mr. T. Scorrern on Waterproof and Unalterable Small-arm Cartridges........
Dr. HerMANnn SpRENGEL on a New Form of Blowpipe for Laboratory Use...
Dr. Tuupicuum on Thiotherine, a Sulphuretted Product of Decomposition of
FAT DUMINONS SUDSEAHCES nec seinee ds ve cede once -useedal cheated Spence sebastienesa ener
Professor VoeLcKer on the Occurrence of Poisonous Metals in Cheese ..... rey
Dr, W. Wattace on the Causes of Fire in Turkey-red Stoves,........+006 Scheo:
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CONTENTS,
GEOLOGY.
Baron F. Anca’s Notes on two newly discovered Ossiferous Caves in Sicily ...
Sir Davip BrewstTer’s Details respecting a Nail found in Kingoodie Quarry,
A Voriecieianicinicis’sls ce olcoesinnie sis(cin cite slanibisie pale. 00 eves races sc@iis oturecisseceedse ceeds susecaesne
Rey. P. B. Bronte on the Stratigraphical Position of certain Species of Corals
ray id fey UTES Reeersoneeee Sesh dane oababndcne ancuddnecesaron ction sartei co Btbdo. dudenadsadadssddoon
Mr. Joun ALtan Brown on the Velocity of Earthquake Shocks in the Laterite
RMA eceadvcaengnicceainsleascicecuecsveceossvesceescnasat severest se "Sinn Hiesonudnecescn ona
Rev. J. C. Crurrersuck on the Course of the Thames from Lechlade to
Windsor, as ruled by the Geological Formations over which it passes.........
Professor DAuBENY’s Remarks on the Elevation Theory of Volcanos ......+404+
Rev. J. B. P. Dennis on the Mode of Flight of the Pterodactyles of the Copro-
lite Bed near Cambridge ....--ssssseecseseesereneees nagebaeoonDOOhOr Cote naceROnoSeteS nv
Rev. J. Dinexz on the Corrugation of Strata in the Vicinity of Mountain
Ranges ccecseceseseseeeeees Sa nencidepSaneosc nc LUO OEOCDOBRCAODL CEH Ca BEAcne Soneceacviensnaeas
Sir Parzre pE M. Grey Ecerron’s Remarks on the Ichthyolites of Farnell
FUGa ie sacesicseceaeaisesesiisics ss pecan seers Bocrenadnee aneagsdacoonaynddagode Sciggadonadanebnne
— on a New Form of Ichthyolite discovered
by Mr. Peach...cccesssesseseseeeereeass cannasboncnte deeabanace Sebensecssnrseus saneaoneincore
M. A. Favre on Circular Chains in the Savoy AIps....ccscsesesscerssecceeeerseeens
Mr. ALeuonse Gaces on some Transformations of Iron Pyrites in connexion
with Organic Remains...... scp COEEBE So SELORO IA00080N peehiterantes Ropn ee deeiaxaneeseeens
Dr. Gernitz on Snow Crystals observed at Dresden ......eseeveeseeeees SCE CDAD
— on the Silurian Formation in the District of Wilsdruff..........c0000+
Professor Harkness on the Metamorphic Rocks of the North of Ireland ......
Dr. Hecror’s Notes on the Geology of Captain Palliser’s Expedition in British
INorth AMETICA ....002:.0ceccseccenscresececesonacnccsvasasoasaccereresses J gapnr pesanagabedn
Professor F. von Hocusterrer’s Remarks on the Geology of New Zealand,
illustrated by Geological Maps, Drawings, and Photographs...... Sreidachiasendcor
——______—_ — Observations upon the Geological Fea-
tures of the Volcanic Island of St. Paul, in the South Indian Ocean, illus-
trated by a Model in Relief of the Island, made by Captain Cybulz, of the
Australian Artillery......esessee eatasratee lelesielve's cbopeaeuaeanigy estes SAR NSDUCEOD Beteenne
Mr. E. Hutt on the Six-inch Maps of the Geological Survey ......sssseseeseeenee
on the Blenheim Iron Ore; and the Thickness of the Formations
below the Great Oolite at Stonesfield, Oxfordshire ........ssesseeceeees SASEPaC AAA
Mr. T. Sterry Hunv’s Note on some Points in Chemical Geology ...sse++s0+
Mr. J. Beets Juxes on the Igneous Rocks interstratified with the Carbonife-
rous Limestones of the Basin of Limerick.......sceesseerees MPN ce cadianeeadesesss
Mr. J. A. Kwipz on the Tynedale Coal-field and the Whin-sill of Cumberland
and Northumberland.......ccssscesesereeeees EERO Ac SdoAeDeCEnCoN Rcdudemniiceswcnares
Dr. W. Lauper Lrypsay on the Eruption in May 1860, of the Kotltigja Vol-
CANO in Iceland.......ssccssoscecseecovcssrocecsesscccscscovesssccosccsssasnveccssonacceces
Rey. W. Lrsrer on some Reptilian Foot-prints from the New Red Sandstone,
north of Wolverhampton......sscssssccecseesereeecenccneassasecaeeeeueereusseseesenserees
Rev. W. Mitcue x and Professor TenNant on the Koh-i-Noor previous to
Hts Cutting....0......sccsscceveeeseetecs * Choon Bonpe a DnISS Ca pbuCenIaochC nat sabe ne bandas
Mr. C. Moors on the Contents of Three Square Yards of Triassic Drift ........
~ Mr. Wirt1am Motynevx’s Remarks on Fossil Fish from the North Stafiord-
shire Coal Fields ..sscsscsesseseeseaeres paamieoeslenstiess Seantiotogean Benatar san adeseescsiines
bt
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xli CONTENTS.
Page
Mr. J. Powrtx’s Notice ofa Fossiliferous Deposit near Farnell, in Forfarshire,
INA Bc scocnaenas ser asdecuecnrcnses daeancsoemetcnteeneanasianes creer ace arr cent neeee re eeenee 89
Professor Puriurps on the Geology of the Vicinity of Oxford .........sece0eeseeees 90
Mr. JosEpH Prestwicu on some New Facts in relation to the Section of the
Cliffvat MundesleysINortolk:s.cccseuesesseasanecrestarewsscccrecsec eee adac eeeeaaeene 90
Mr. /J.)Prich on Shckensid@ss.c..s-sssuscsessssseceseeten sv eceeds “See reeacno eaeclees Senate 91
Mr. Witi1am PeNncELLy on the Chronological and Geographical Distribution
of the Devonian Fossils of Devon and Cornwall ........,.cccssecessccecccccececsece 91
Professor H. D. Rogers on some Phenomena of Metamorpiisnts in Coal in the
SHUMILCE SCALES oe, csct ssesdeasdersacensoceccecccrescurstscsessevesenererasasarett eset eeeiaee 101
Rev. Professor Sepewicx on the Geology of the Neighbourhood of Cambridge
and the Fossils of the Upper Greensand ............. Sos voce nsceseaseastsentsisaeanperans 101
Rev. Grisert N. Smiru on three undescribed Bone-Caves near Tenby, Pem-
rOkeShivGweceacceamnceeates sass cman cresceene case inedensaneste see serer ee Wola dane «teaeeengas 101
Rev. W. S. Symonps on the Selection of a Peculiar Geological Habitat by
some OL the raremsbmbishy Elan tSiewncoacccceccoss«os sairecsesectne sie eee tie te neeme 102
Rev. H. B. Tristram on the Geological System of the Central Sahara of
ALGOMA ness erseracsncsciaccitsoadstserecscees sactoretmacdserscabecenercenee st cot tae ee mmeare 102
Mr. J. F. Wuireaves on the Invertebrate Fauna of the Lower Oolites of
OxfordShinetgascscsecceceradaess a vaceroecs slices cone secase seston teeteneoee coon ante a aieeee 104
Captain Woopatt on the Intermittent Springs of the Chalk and Oolite of the
Neizhbourhood! of Searborotgh..c.3s.: 08s <deccss.c0taessadeaveescessns-apepreseweger 108
Mr. Toomas Wricut on the Avicula contorta Beds and Lower Lias in the
South of England.......... Gvesctestacs EG SesOuensut vorbiescewanenseat saesaviesaahaw sy Rime -. 108
BOTANY AND ZOOLOGY, tncLtupinc PHYSIOLOGY.
GENERAL.
Mr. Putrre P. Carpenter on the Progress of Natural Science in the United
States and Canada...........0+« Paver ead oa ness Pov achaasceaesecrucsutes chadacaeaceset cade 109
Professor DauBeny’s Remarks on the Final Causes of the Sexuality of Plants,
with particular reference to Mr. Darwin’s Work ‘ On the Origin of Species
by Natural Selection’ ......... “Hochortncso sho. eae nceceeer eee ease phaxte anne free 109
Borany.
Professor DowpEN on a Plant Poisoning a Plant..........sccssssesecerserseees sesess 110
Dr. C. Dresser on Abnormal Forms of Passiflora c@ruled ..ccccccecseseresevenses 110
on the Morphological Laws in Plants ..........cscecesceeseeeeenes 110
Rev. Professor HeNsLow on the supposed Germination of Mummy Wheat..... 110
Mr. Joun Hoace on the Distinctions of a Plant and an Animal, and ona Fourth
Kingdom of Natures. ..~-0cescecysnesensrpnvonrivedesnecoapersetaseessaseeprensesseseseas lil
Mr. M. T. Masters on the Normal and Abnormal Variations from an assumed
My pevin Plants. .205 sco. sceasewoes co-i- cae ane=nsinexceeuecsoasscnesrerueniosserscarssecaanenas 112
Dr. G. OerLviz on the Structure of Fern Stems ....scescseeeeees cass casasueee maces sep TD
ZooLoey.
Mr. Frank T. Bucktanp on the Acclimatization of Animals, Birds, &c., in
the United Kingdom ..ccocssscsscsccenccssesscocesessecsesnccsaveusstunsecauddsvsersecaws. LAGS
CONTENTS, xiii
Page
Mr. Curusert CoLtinewoon’s Remarks on the Respiration of the Nudibran-
Ghiate Mollusca ...cccccccccsccscsens aaeencinccisecsss cans aM Ran coca asc ateE eer sc cwccsen ce 113
-————__—_————— on the Nudibranchiate Mollusca of the Mersey
PATI CE tnt ecadececccdrsscepestestsestcadsstcccsececase cdl Pasceebecavustctphedes desssescas 113
SEE IVS UEINALIC!ZOOIOPY; ovvientnavoncorseveceenueesecasaussovsvasisessWasenens+serssinesouns 114
Professor Draper on the Intellectual Development of Europe, considered with
reference to the views of Mr. Darwin and others, that the Progression of
ieanjems 1s. determined by Iawiscs.ess.ss0sesccsccsnecsesseceessices ys dnstse-cps'e seaee 115
Rev. H. H. Hicerns on some Specimens of Shells from the Liverpool Museum,
originally from the Pathological Collection formed by the late Mr. Gaskoin... 116
Rey. A. R. Hoeawn’s Notice of British Well Shrimps ....... BG Ta De « LI6
Mr. J. G. Jerrruys on the British Teredines, or Ship-Worms ............0eeeee0s 117
Mr. Cuartes W. Peacu on the Statistics of the Herring Fishery......... Preaaes 120
MPa OESPERTCH ONC yOIP PE. esseces Winn ve cwlcrece es ieteassbste cies nctetecdiencseastysstes 120
Mr. Lovett Reeve on the Aspergillum or Watering-pot Mollusk ...........0..08 120
Dr. P. L. Sctarer’s Remarks on the Geographical Distribution of recent Ter-
BEEP IMVCLECDLALAssa.ssissscessincsesciencondaesserecenersscane Seep idaniiivenasseoesatlsceests 121
Mr. H. T. Starnron on some Peculiar Forms amongst the Micro-Lepidopterous
MMR P EM na eeas erestis sauce meanest mcenctciasvece cacostsetene da tr cevecccseressesedesvs 122
Dr. Vertoren on the Effect of Temperature and Periodicity on the Develop-
ment of certain Lepidoptera............... es cewies ninelnn penetra elsigas Biss Jeocsceeeeers » 123
Biro. O., Westwoon on Mummy Beetles, .......ccsrspeosaseyseesessnspeceptenessens 123
——————— on a Lepidopterous Parasite oecurring on the Body of
BEML AR OTC RMUCLANT GD a scng's%inniomaidaisaae sss 8sdesPesehesniese ses cosy cs sesesecseceeseasere » 124
Dr, E, Percevat Wricut’s Notes on Tomopteris onisciformis........000.008 weneqe 124
PuysioLoey.
Professor Beatz on the Ultimate Arrangement of Nerves in Muscular Tissue... 125
Professor VY. Carus on the Leptocephalid@......ccccssesscovsceccoeceoteescevcocedeses 125
——_—————— on the Value of ‘ Development” in Systematic Zoology
pdm animal MOT pHOlO Ry? vascc..ssonscaesosncdecsoascavesvcghoabebevepeaesac ouaneowensees 125
Professor Corset on the Deglutition of Alimentary Fluids...........se00eecccsese 216
Dr. Ropert M‘Donne tt on the Formation of Sugar and Amyloid Substances
Rates TEAL EL CORON. os Sa ntindisc Saeasina,s nerves els sealeasoeceopep'vs ap ogosovcemss si. « +. 129
Mr. Artuur E, Duruam’s Experimental Inquiry into the Nature of Sleep..... 129
Dr. Micuarx Fosrer’s Contributions to the Theory of Cardiac Inhibition...... 129
Mr. Rosert Garner on certain Alterations in the Medulla Oblongata in cases
BMT sa) Voto micns Mesa eeeiseiciee eeck ace oleae eke ee ee eee ek ieeee odds en ckscks 129
- on the Structure of the Lepadid@.........csceeecesees aonnesere 130
Mr. Georce D. Gres on Saccharine Fermentation within the Female Breast.. 131
Sir Caarres Gray on Asiatic Cholera......ses...8 Ruenontesess atiowncdenet oa urcekesanes 132
Mr. J. Reay Greene, A Word on Embryology, with reference to the mutual
relations of the Sub-kingdoms of Animals............. seaeneaeenecemesaaecy cesponeses LSD
Mr. Epwarp R. Harvey on the Mode of Death by Aconite.......sssscssecceeasee 133
Professor Van pER Horven on the Anatomy of Stenops Potto, Perodicticus
Geoffroyt of Bennett....... dtleiese vesiseeinneiuniaesey ec teveeevesscscsesscscrscecssecsssosensens 134
X1V CONTENTS.
Professor Van prr Horven, Observations on the Teredo navalis, and the
Mischief caused by it in Holland.............065 SadeoLnonGagsncckecadodanasutidddé foc wee
Professor Huxtry on the Development of Pyrosoma .......s0eeeenee nencsuee =qpe0bon
Dr. Cuartes Kipp on the Nature of Death from the Administration of
Anesthetics, especially Chloroform and Ether, as observed in Hospitals......
ib. Lewis ona. Hydro-spirometer ..ccsor0.«arwagecduccsiesecenstundecsstcccmaeae etenciai
Mr. Joun Luspock on the Development of Buccinum .....scsscsssssscesenseeteenees
Mr. Arcuigatp MacLaren on the Influence of Systematized Exercise on the
Expansion tof theiChestsaienecskneeeaensacasmere sree sain Sappeoecriceba secede sna ce
M. Otter on the Artificial Production of Bone and Osseous Grafts .......0.+
Dr. C. B. Rapexirr’s Experiments on Muscular Action from an Electrical point
OL VIEW. 5 coisas scans sae unc chun sok saeeceuaneneeavarcurcanes eatne naa seue set aman sebews
Dr. B. W. Ricuarpson on the Process of Oxygenation in Animal Bodies .....
Dr. Epwarp Smiru, The Action of Tea and Alcohols contrasted ......seeesseeess
Page
136
136
136
139
139
142
143
143
143
145
Dr. J. L. W. Taupicuum on the Physiological relations of the Colouring —
Matteriof thesBilessepsscsscuresacess wawseenae MOEA Ncuasnecen ieee juseenaenedees eAddoae :
GEOGRAPHY AND ETHNOLOGY.
Opening Address by the President, Sir Roprrick Impry Murcuison .......+
Mr. T. W. Atkinson on the Caravan Routes from the Russian Frontier to
Khiva, Bokhara, Kokhan, and Garkand, with suggestions for opening up a
Trade Jbetween Central: Asia. and sndia .caucesmaee «cestode sa cteceeapeeereeeeeneee ee
_——_— on the Caravan Route from Yarkand to Mai-matchin,
with a Short Account of this Town, through which the Trade is carried on
between Russiasand) China ccnesctnensscassevtenoeden cmctioncsesenel teas coca 5
Capt. Sir E. Betcuer on the Manufacture of Stone Hatchets and other Imple-
ments by the Esquimaux, illustrated by Native Tools, Arrow-heads, &c....++.
Mr. Joun Crawrurp on the Aryan or Indo-Germanic Theory of Races .......
—__—_—___———— on the Influence cf Domestic Animals on the Progress of
Civilization) (BILAS) sca, casssakpeemeccetenecteone te osmeekar eee. sunetscalesseaateeeemtoeeinc
Mr. R. Cut on certain remarkable Deviations in the Stature of Europeans....
on the Existence of a true Plural of a Personal Pronoun in a
living European Language scrsnnseccciedsestsdecscssevevseencetseeme Rec doseenasantiesh's
Captain Cypuuz on a Set of Relief Models of the Alps, &C.....ccscceeceeceseeeees
Rev. Professor Graves on the Arrangement of the Forts and Dwelling-places
Gf the Ancient Ubishie: ccs sci dsnactanenset-seearecnaervades tale Arcs eee eaeen aes
Rev. Epw. Hrncxs on certain Ethnological Boulders and their probable Origin
Professor I’. von Hocusretrrer’s New Map of the Interior of the Northern
Island of New Zealand, constructed during an Inland Journey in 1859 .......
Dr. J. Hunt on the Antiquity of the Human Race.....e...secseccee sees Scinteray Oroeee
Mr. V. Hurrapo on the Geographical Distribution and Trade in the Cinchona
Rev. Professor Jarrett on Alphabets, and especially the English; and on a
New Method of Marking the Sound of English Words, without change of
Orthography cmespanceene seen ce veemsee mere cnt Sor sSStarnaonapsas Desir asonscdesodc sob anes
Mr. R. Knox on the Origin of the Arts, and the Influence of Race in their
DevelopmMentire Aescntecceceateowenes. cnesisce teeencae seme satteset Crit nenenneSnee eee nae
Mr. D. A. Laner’s brief Account of the Progress of the Works of the Isthmus
of Suez Canal...... dic bosKobOHOmadaBroncons chcccosuserbonoddac seve
Fee neeee ee ereesetesaetee
147
148
153
154
154
154
155
155
163
163
163
CONTENTS, XV
Page
Dr. R. G. Latuam on the Jaczwings, a Population of the Thirteenth Century,
on the Frontiers of Prussia and Lithuania ........scecsscsesssscscneneeeneees ae ace 163
Dr. D. Livinestone on the latest Discoveries in South-Central Africa.......... 164
Mr. W. Locxuart on the Mountain Districts of China, and their Aboriginal
Inhabitants...... Sie oc dccucecOrngdbor CEeSESd br COC NEDIGSORD< SECO RORnDar Jobe Uap ¢RUBOBROBCE DE. 168
Mr. D. May’s Journey in Bae am and Nupé Count LESmh dadeaktre si uetatdate sates 170
Dr. Macecowan’s History of the Ante-Christian Settlement of the Jews in China 170
Mr. J. Micxt1n’s Cruise in the Gulf of Pe-che-li and Leo-tung (China)....... .. 170
Captain Suzrarp Ossorn on the Formation of Oceanic Ice in the Arctic
EVE EIONS i aicoiss tied sisvelon ciceiewee seus Mesiaceidaniawers’ssltiacisionicene onatlsoaneamanairenes de daoadgnseee ee Lee
Captain J. Patiiser on the Course and Results of the British North American
Exploring Expedition, under his Command in the Years 1857, 1858, 1859... 170
Dr. Hecror’s Remarks concerning the Climate of the Saskatchewan
Psi Chirac, cocmawsenacersncncensee sponcerek. sérasheearina ben decddbocEs pAanre Ese sthomdcce i
Mr. Suxtrvan’s Remarks concerning the Tribes of Indians inhabiting the
Country examined by the Expedition............000c000 Paaisesepuidcese sapdepae lyse}
ConsulPetserick on his proposed Journey from Khartum in Upper Egypt to
meetCaptain Speke on or near the Lake Nyanza of Central Africa.......... « 174
Dr. J. Raz on the Formation of poe and Ice Action, as observed in the
RIG SON SHAY, AUG SCLalts <ccecacssaceccsieconsesessestcous cute sigebanorignseeagancor sone ye!
on the Aborigines of the etic and Sub- Arctic Se of North
AMICTICA 22-2 00eeers0es neasneiieteiefaeeese=scdnedsessiaais JodOdexcondne SesupoendecdRegapEnNCoC ce atl
M.R. von Scuztacintweir’s Remarks on some of the Hoa - India and High
' Asia (in connexion with casts exhibited) ....... wees tie Ross svalocehdussaes dosepastine A Ua.
Lieutenant Epwarp ScuLaGintWEIT on the Tribes composing the Population
WE MOLOCCO os... csevscescessscecsensesee PR EERE ROROLOn eC Ne Og cbc aiesieseiie esetens e'seaiisi wae LT
Col. Tal. P. SHarrner on the Geography of the North Atlantic Telegraph..... 178
Captain Parker Snow on the Lost Polar Expedition and Possible Recovery of
its Scientific Documents.........06000000 deatepaaseecoeecuscmatatst|s sponedodeeconuaae .. 180
Captain M. H. Synee on the Proposed Communication between the Atlantic
and Pacific, vid British North America.......sssecsssecseeresereees aonebens Succepac tsi
M. Prerre ve Tcuiuatcuer on the Geographical Distribution of Plants in
PSSIDM NL Glucnseveadiecdsicndesttineceshcae(seseoucdsiscseeahtedaverweesneci 6008903050 0s <6) LOM
Mr. Tuomas Wricut on the Excavations on the site of the Roman City of
DaRrPeENOP ACM LOXCLEL cE cncesspecocsiaveradik vedevsnacausagtessaccedepersscsaedsevicrecst LOL
STATISTICAL SCIENCE.
Opening Address by Nassau W. Senior, M.A., President of the Section ...... 182
Rev. J. Boorn on the True Principles of an Income Tax.......scssceeeeeeeeeceeees 184
Miss Mary Carpenter on Educational Help from the Government Grant to
the destitute and neglected children of Great Britain ...... ele dae Wa saates seiosis Scroce, disy:!
Mr. E. Cuapwick on the Economical Results of Military Drill in Popular
Schools ..... Muscbemacierua tees amcaee deena aie Foancbobad sph enocenebanee SeoSeugne parece 185
—-- on the Physiological as well as Psychological Limits to
_ Mental Labour...... ApeGoadecdd anthseeoubses adoungpsousuanose Fao gaonnodhs osataodatessooaeee 185
Mr. R. DowbeEn on Local Taxation for Local Purposes .......0ccseecoscscscescerees 191
Mr. Henry Fawcett, Dr. Wheweill on the Methed of Political Economy...... 191
————__——. on Co-operative Societies, their Social and Political
OREIE Ce Ltercemae apart ee metas cacti caine is dis neneaseientiabaslechhisievecescedsdkaepssestaeseseve, 101
\
(Ir. J. J. Fox on the Province of the Statistician ....scsssssussossesssescessseeseerens 1QL
Xvi CONTENTS.
Page
Mr. J. HircuMman on Sanitary Drainage of TOWNS ....cecccsscceveesesceccesesceseeee IQ]
Mr. E, Jarvis on the System of Taxation prevailing in the United States....... 191
Dr. MicHELsEN on Serfdom in Russia .......ecssseeeseaseess dadtiwssapesesason seamen ens 191
Mr. J. M. Mircuet on the Economical History and Statistics of the Her-
2111 OS aan OOeC DURE Or OnC Ec Daecemoonscccncondadclcsracoccseee ab ibileisjeserata Beasesenenones 191
Mr. W. Newmarcu on some suggested Schemes of Taxation, and the Difficul-
ties of them........... sacdawy sie eoeete cote oosemseeete ar Weg Sdasba sac sake sony uetiet eens awereel OF
Mr. Henry Joun Ker Porrer’s Hints on the best Plan of Cottage for Agri-
cultural Labourers......... sesgiee Sneed waved siisesaneneutusaceccssesatanmanclescen cee sscsee 194
Mr. F. Purpy on the Systems of Poor Law Medical Relief...........s.ss000 eevee 195
Mr. Henry Roserts’s Notes on various efforts to Improve the Domiciliary
Condition of the Labouring Classes.......ssssscseesseeneenenees ce sveepeaet SRA (61D)
MECHANICAL SCIENCE.
Mr. P. W. Bartow on the Mechanical Effects of combining Suspension Chains
and Girders, and the value of the Practical Application of this System (illus-
trated by a Model) ........+.000+ sbubcleupeccucstesscpcssantwspepecsiuecpeatepeaneseeeroeeee .- 201
Captain BLAKEEKY on Rited' Cannon’. :-c..1..-cs..0sesesuevecheucatssepmeasstes eevee» 201
Rey. Dr. Boora ona deep Sea Pressure Gauge, invented by Henry Johnson, Esq. 202
Earl of CarrHness on Road Locomotives...........ceseecessescecesessceves <onscouscsss (20
Mr. E. Cowprr’s New Mode of obtaining a Blast of very High Temperature
inthe) ManulactareOlUrOns..5essdenceereoes ores s<ciesnecvacsyses er enewepeerene veoeee 204
Mr. Jonn Exper on the Cylindrical Spiral Boiler ............sssecessssssveeeees vases 204
Mr. Wriitam Farrparrn on the Density of Saturated Steam, and on the Law
of Expansion of Superheated Steam <.ccc.c sic. cc scccceccacsevcecsscassccccccads sseene 210
Mr. Joun FisHEr on any Atmospheric Washing Machine........++sessessesseee vee 210
Mr. Witt1am Frovupse on Giffard’s Injector for Feeding Boilers..,.........0.026. 211
Mr. Watter Hatt on a Process for Covering Submarine Wires with India-
rubber for Telegraphic purposes...... sis nics sins oes anenes eas const ainecbaspeepenes ALE 211
Professor Hennessy’s Suggestions relative to Inland Navigation ....se...ss.00. 211
Mr. Caxucott Rer.ty on the Longitudinal Stress of the Plate Girder........... - 212
Dr. B. W. Ricwarpson on Suggestions for an Electro-Magnetic Railway
IBTGak'. 35,0. ciaspssncua sehen «yeu ce ngals Memeo cep = peer esaa topeset> saaeeienges saveeumnsr sass tenes 212
Mr. S. W. Srtver on the Character and Comparative Value of Gutta Percha .
and India-rubber employed as Insulators for Subaqueous Telegraphic Wires. 212
Mr. W. Simons on Improvements in Iron Shipbuilding ........-2+...ccceeeseseeeaes 212
Admiral Tayztor’s Novel Means to lessen the frightful Loss of Life round
our exposed Coasts by rendering the Element itself an Inert Barrier against
the Power of the Sea; also a Permanent Deep-water Harbour of Refuge by
Artificial Bars........... apie exp tie «codes eccipaess lessens ces as ae see dniincesse sae es ana. anaes 215
Mr. G. F. Train on Street Railways as used in the United States, illustrated
by a Model of a Tramway and Car, or Omnibus capable of conveying sixty
DETSODS ..000.cscccseseusccesss acaideswusiaselcmavelcchenictsncedae’sveasian anes esac usanvetusanees 215
Messrs. WERNER and C. W. S1emEens on a Mode of covering Wires with
India-ribber... 0. sscccesse jap teaweasssdaneeas pastes anecanes Rasen sGece Nene Catone spaeh pce, ua
APPENDIX.
PHYSIOLOGY.
/
Professor J. H. Consett on the Deglutition of Alimentary Fluids ....00000. 21°»
/
/
OBJECTS AND RULES
OF
THE ASSOCIATION.
— i
OBJECTS.
Tue Assocration contemplates no interference with the ground occupied by
other Institutions. Its objects are,—To give a stronger impulse and a more
systematic direction to scientific inquiry,—to promote the intercourse of those
who cultivate Science in different parts of the British Empire, with one an-
other, and with foreign philosophers,—to obtain a more general attention to
the objects of Science, and a removal of any disadvantages of a public kind
which impede its progress.
RULES,
ADMISSION OF MEMBERS AND ASSOCIATES.
All Persons who have attended the first Meeting shall be entitled to be-
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The Fellows and Members of Chartered Literary and Philosophical So-
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The Officers and Members of the Councils, or Managing Committees, of
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Anwnuat Susscrisrrs shall pay, on admission, the sum of Two Pounds,
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Associates for the year shall pay on admission the sum of One Pound.
They shall not receive gratuitously the Reports of the Association, nor be
eligible to serve on Committees, or to hold any office. i
1860.
XVIil RULES OF THE ASSOCIATION.
The Association consists of the following classes :—
1, Life Members admitted from 1831 to 1845 inclusive, who have paid
on admission Five Pounds as a composition.
2. Life Members who in 1846, or in subsequent years, have paid on ad-
mission Ten Pounds as a composition.
_8. Annual Members admitted from 1831 to 1839 inclusive, subject to the
payment of One Pound annually. [May resume their Membership after in-
termission of Annual Payment. |
4. Annual Members admitted in any year since 1859, subject to the pay-
ment of Two Pounds for the first year, and One Pound in each following
year. [May resume their Membership after intermission of Annual Pay-
ment. ]
5. Associates for the year, subject to the payment of One Pound.
6. Corresponding Members nominated by the Council.
And the Members and Associates will be entitled to receive the annual
volume of Reports, gratis, or to purchase it at reduced (or Members’) price,
according to the following specification, viz. :—
1. Gratis.—Old Life Members who have paid Five Pounds as a compo-
sition for Annual Payments, and previous to 1845 a further
sum of Two Pounds as a Book Subscription, or, since 1845, a
further sum of Five Pounds.
New Life Members who have paid Ten Pounds as a com-
position.
Annual Members who have not intermitted their Annual Sub-
scription.
2. At reduced or Members’ Prices, viz. two-thirds of the Publication
Price.—Old Life Members who have paid Five Pounds as a
composition for Annual Payments, but no further sum as a
Book Subscription. :
Arnual Members, who have intermitted their Annual Subscrip-
tion.
Associates for the year. [Privilege confined to the volume for
that year only. ]
3. Members may purchase (for the purpose of completing their sets) any
of the first seventeen volumes of Transactions of the Associa-
tion, and of which more than 100 copies remain, at one-third of
the Publication Price. Application to be made (by letter) to
Messrs. Taylor & Francis, Red Lion Court, Fleet St., London.
Subscriptions shall be received by the Treasurer or Secretaries.
MEETINGS.
The Association shall meet annually, for one week, or longer. The place
of each Meeting shall be appointed by the General Committee at the pre-
vious Meeting; and the Arrangements for it shall be entrusted to the Offi-
cers of the Association,
GENERAL COMMITTEE.
The General Committee shall sit during the week of the Meeting, or
longer, to transact the business of the Association. It shall consist of the
following persons :—
1. Presidents and Officers for the present and preceding years, with
authors of Reports in the Transactions of the Association.
2. Members who have communicated any Paper to a Philosophical Society,
which has been printed in its Transactions, and which relates to such subjects
as are taken into consideration at the Sectional Meetings of the Association.
RULES OF THE ASSOCIATION. X1X
3. Office-bearers for the time being, or Delegates, altogether not exceed-
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4, Office-bearers for the time being, or Delegates, not exceeding three,
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5, Foreigners and other individuals whose assistance is desired, and who
are specially nominated in writing for the Meeting of the year by the Presi-
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6. The Presidents, Vice-Presidents, and Secretaries of the Sections are
ex-officio members of the General Committee for the time being.
SECTIONAL COMMITTEES.
The General Committee shall appoint, at each Meeting, Committees, con-
sisting severally of the Members most conversant with the several branches
of Science, to advise together for the advancement thereof.
_ The Committees shall report what subjects of investigation they would
particularly recommend to be prosecuted during the ensuing year, and
brought under consideration at the next Meeting.
The Committees shall recommend Reports on the state and progress of
particular Sciences, to be drawn up from time to time by competent persons,
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: COMMITTEE OF RECOMMENDATIONS.
The General Committee shali appoint at each Meeting a Committee, which
shall receive and consider the Recommendations of the Sectional Committees,
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to be adopted for the advancement of Science.
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OFFICERS.
A President, two or more Vice-Presidents, one or more Secretaries, and a
Treasurer, shall be annually appointed by the General Committee.
: COUNCIL.
In the intervals of the Meetings, the affairs of the Association shall be
managed by a Council appointed by the General Committee. - The Council
may also assemble for the despatch of business during the week of the
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PAPERS AND COMMUNICATIONS.
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ACCOUNTS.
The Accounts of the Association shall be audited annually, by Auditors
appointed by the Meeting. ae
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MEMBERS OF THE COUNCIL.
XXV
II. Table showing the Names of Members of the British Association who
have served on the Council in former years.
Aberdeen, Earl of, LL.D., K.G., K.T.,
F.R.S. (dec‘).
Acland, Sir Thomas D., Bart., F.R.S.
Acland, Professor H. W., M.D., F.R.S.
Adams, J. Couch, M.A., F.R.S.
Adamson, John, Esq., F.L.S.
Ainslie, Rev. Gilbert, D.D., Master of Pem-
broke Hall, Cambridge.
Airy,G.B.,D.C.L.,F.R.S.,Astronomer Royal.
Alison, Professor W. P.,M.D.,F.R.S.E.(dec*).
Allen, W. J. C., Esq.
Anderson, Prof. Thomas, M.D.
Ansted, Professor D. T., M.A., F.R.S.
Argyll, George Douglas, Duke of, F.R.S.
Arnott, Neil, M.D., F.R.S.
Ashburton, William Bingham, Lord, D.C.L,
Atkinson, Rt. Hon. R.,Lord Mayor of Dublin.
Babbage, Charles, Esq., M.A., F.R.S.
Babington, Professor CO. C., M.A., F.R.S.
Baily, Francis, Esq., F.R.S. (deceased).
Baines, Rt. Hon. M.T., M.A., M.P. (dec*).
Baker, Thomas Barwick Lloyd, Esq.
Balfour, Professor John H., M.D., F.B.S.
Barker, George, Hsq., F.R.S. (deceased).
Beamish, Richard, Hsq., F.R.8.
Bell, Professor Thomas, Pres. L.S., F.R.S.
Beechey, Rear-Admiral, F.R.S. (deceased).
Bengough, George, Esq.
Bentham, George, Esq., F.LS.
Biddell, George Arthur, Esq.
Bigge, Charles, Esq.
Blakiston, Peyton, M.D., F.R.8.
Boileau, Sir John P., Bart., F.R.S.
Boyle, Rt.Hon. D., Lord Justice-Gen!. (dec*).
Brady,The Rt. Hon. Maziere, M.R.1.A., Lord
Chancellor of Ireland.
Brand, William, Esq.
Breadalbane, John, Marquis of, K.T., F.R.S.
Brewster, Sir David, K.H., D.C.L., LL.D.,
F.R.S., Principal of the University of
Edinburgh.
Brisbane, General Sir Thomas M., Bart.,
K.C.B., G.C.H., D.C.L., F.R.S. (dec*).
Brodie, Sir B. C., Bart., D.C.L., Pres. B.S.
Brooke, Charles, B.A., F.R.S.
Brown, Robert, D.C.L., F.R.S. (deceased).
Brunel, Sir M. I., F.R.S. (deceased).
Buckland, Very Rev. William, D.D., F.RB.8.,
Dean of Westminster (deceased).
Bute, John, Marquis of, K.'T. (deceased).
Carlisle, George Will. Fred., Earl of, F.R.S.
Carson, Rey. Joseph, F.T.C.D.
Cathcart, Lt.-Gen., Earlof, K.C.B., F.R.S.E.
(deceased).
Chalmers, Rev. T., D.D. (deceased).
Chance, James, Esq.
Chester, John Graham, D.D., Lord Bishop of.
Christie, Professor 8. H., M.A., F.R.S.
Clare, Peter, Esq., F.R.A.S. (deceased).
Clark, Rev. Prof., M.D., F.R.S. (Camtridge.)
Clark, Henry, M.D.
Clark, G. T., Esq.
Clear, William, Esq. (deceased),
Clerke, Major 8., K.H., R.E., F.R.S. (dec*).
Clift, William, Hsq., F’.R.S. (deceased).
Close, Very Rev. F., M.A., Dean of Carlisle.
Cobbold, John Chevalier, Esq., M.P.
Colquhoun, J. C., Esq., M.P. (deceased).
Conybeare, Very Rev. W. D., Dean of Llan-
daff (deceased).
Cooper, Sir Henry, M.D.
Corrie, John, Esq., F.R.S. (deceased).
Crum, Walter, Esq., F.R.S.
Currie, William Wallace, Esq. (deceased).
Dalton, John, D.C.L., F.R.S. (deceased).
Daniell, Professor J. F., F.R.S. (deceased).
Dartmouth, William, Earl of, D.C.L., F.R.S.
Darwin, Charles, Esq., M.A., F.R.S.
Daubeny, Prof. Charles G. B., M.D., F.R.8.
DelaBeche, Sir H. T., C.B., F.R.S8., Director-
Gen. Geol. Surv. United Kingdom (dec‘).
De la Rue, Warren, Ph.D., F.R.S.
Devonshire, William, Duke of, M.A., F.R.S.
Dickinson, Joseph, M.D., F.R.S.
Dillwyn, Lewis W., Hsq., F.R.S. (deceased).
Drinkwater, J. E., Esq. (deceased).
Ducie, The Earl, F.R.S.
Dunraven, The Earl of, F.R.S.
Egerton, Sir P, de M. Grey, Bart., M.P.,
E.R.S
Eliot, Lord, M.P.
Ellesmere, Francis, Earl of, F.G.8. (dec*).
Enniskillen, William, Earl of, D.C.L., F.R.S,
Estcourt, T. G. B., D.C.L. (deceased).
Fairbairn, William, LL.D., C.E., F.R.S.
Faraday, Professor, D.C.L., F.R.S.
FitzRoy, Rear Admiral, F.R.S.
Fitzwilliam, The Earl, D.C.L., F.R.S. (dec*).
Fleming, W., M.D.
Fletcher, Bell, M.D.
Foote, Lundy E., Esq.
Forbes, Charles, Esq. (deceased).
Forbes, Prof. Edward, F.R.S. (deceased).
Forbes, Prof. J. D., F.R.S., Sec. R.S.E.
Fox, Robert Were, Esq., F.R.8.
Frost, Charles, F.S.A.
Fuller, Professor, M.A.
Gassiot, John P., Esq., F.R.S.
Gilbert, Davies, D.C.L., F.R.S. (deceased).
Gourlie, William, Esq. (deceased).
Graham, T., M.A., F.R.S., Master of the Mint.
Gray, John E., Esq., Ph.D., F.R.S.
Gray, Jonathan, Esq. (deceased).
Gray, William, Esq., F.G.S.
Green, Prof. Joseph Henry, D.C.L., F.R.S.
Greenough, G. B., Esq., ¥.R.S. (deceased).
Griffith, Sir R. Griffith, Bt., LL.D., M.R.1.A.
Grove, W. R., Hsq., M.A., F-.R.S.
Hallam, Henry, Esq., M.A., F.R.S. (dec*).
Hamilton, W. J., Esq., F.R.S8., For. Sec. G.S.
Hamilton, Sir Wm. R., LL.D., Astronomer
Royal of Ireland, M.R.LA., F.R.AS.
Hancock, W. Neilson, LL.D.
Harcourt, Rev. Wm. Vernon, M.A., F.R.S.
Hardwicke, Charles Philip, Earl of, F.R.S.
Harford, J. §., D.C.L., F.R.S. ;
= >
XXV1
Harris, Sir W. Snow, F.R.S.
Harrowby, The Earl of, F.R.S8.
Hatfeild, William, Esq., F.G.S. (deceased).
Henry, W. C., M.D., F.R.S. [Col., Belfast.
Henry, Rev. P.S., D.D., President of Queen’s
Henslow, Rey. Professor, M.A., F.L.8. (dec®).
Herbert, Hon. and Very Rey. Wm., LL.D.,
F.L.S., Dean of Manchester (dec*).
Herschel,Sir John F.W., Bart.,D.C.L., F.R.S.
Heywood, Sir Benjamin, Bart., F.R.S.
Heywood, James, Esq., F.R.S.
Hill, Rev. Edward, M.A., F.G.S.
Hincks, Rey. Edward, D.D., M.R.I.A.
Hincks, Rev. Thomas, B.A.
Hinds,8., D.D., late Lord Bishop of Norwich.
(deceased).
Hodgkin, Thomas, M.D.
Hodgkinson, Professor Eaton, F.R.S.
Hodgson, Joseph, Esq., F.R.S.
Hooker, Sir William J., LL.D., F.R.S.
Hope, Rev. F. W., M.A., F.R.S.
Hopkins, William, Esq., M.A., F.R.S.
Horner, Leonard, Esq., F.R.S., F.G.S8.
Hovenden, V. F., Esq., M.A.
Hugall, J. W., Esq.
Hutton, Robert, Esq., F.G.S.
Hutton, William, Esq., F.G.S.
Ibbetson,Capt.L.L. Boscawen, K.R.E.,F.G.S.
Inglis, Sir R. H., Bart., D.C.L., M.P. (dec*).
Inman, Thomas, M.D.
Jacobs, Bethel, Esq.
Jameson, Professor R., F.R.S. (deceased).
Jardine, Sir William, Bart., F.R.S.E.
Jeffreys, John Gwyn, Esq., F.R.S.
Jellett, Rev. Professor.
Jenyns, Rey. Leonard, F.L.S.
Jerrard, H. B., Esq.
Johnston, Right Hon. William, late Lord
Provost of Edinburgh.
Johnston, Prof.J. F. W.,M.A., F.R.S. (dec).
Keleher, William, Esq. (deceased).
Kelland, Rey. Professor P., M.A.
Kildare, The Marquis of.
Lankester, Edwin, M.D., F.R.S.
Lansdowne, Hen., Marquisof, D.C.L.,F.R.S.
Larcom, Major, R.E., LL.D., F.R.S.
Lardner, Rey. Dr. (deceased).
Lassell, William, Esq., F.R.S. L. & E.
Latham, R. G., M.D., F.R.S.
Lee, Very Rey. John, D.D., F.R.S.E., Prin-
cipal of the University of Edinburgh.
(deceased).
Lee, Robert, M.D., F.R.S.
Lefevre, Right Hon. Charles Shaw, late
Speaker of the House of Commons.
Lemon, Sir Charles, Bart., F.R.S.
Liddell, Andrew, Esq. (deceased).
Lindley, Professor John, Ph.D., F.R.S.
Listowel, The Earl of. [Dublin (dec*).
Lloyd, Rey. B., D.D., Provost of Trin. Coll.,
Lloyd, Rev. H., D.D., D.C.L., F.R.S. L.&E.
Londesborough, Lord, F.R.S. (deceased).
Lubbock, Sir John W., Bart., M.A., F.R.S.
Luby, Rev. Thomas.
Lyell, Sir Charles, M.A., F.R.S.
MacCullagh, Prof., D.C.L., M.R.1.A. (dec*).
REPORT— 1860.
MacDonnell, Rev. R., D.D., M.R.LA., Pro-
vost of Trinity College, Dublin.
Macfarlane, The Very Rev. Principal. (dec*).
MacGee, William, M.D.
MacLeay, William Sharp, Esq., E.L.S.
MacNeill, Professor Sir John, F.R.S.
Malahide, The Lord Talbot de.
Malcolm, Vice-Ad. Sir Charles, K.C.B. (dec*).
Maltby, Edward, D.D., F.R.S., late Lord
Bishop of Durham (deceased).
Manchester, J. P. Lee, D.D., Lord Bishop of.
Marshall, J. G., Esq., M.A., F.G.8.
May, Charles, Esq., F.R.A.S8.
Meynell, Thomas, Esq., F.L.S.
Middleton, Sir William F. F., Bart.
Miller, Professor W. A., M.D., F.R.S.
Miller, Professor W. H., M.A., F.RB.S.
Moillet, J. D., Esq. (deceased).
Milnes, R. Monckton, Esq., D.C.L., M.P.
Moggridge, Matthew, Esq.
Monteagle, Lord, F.R.8.
Moody, J. Sadleir, Esq.
Moody, T. H. C., Esq.
Moody, T. F., Esq.
Morley, The Earl of.
Moseley, Rey. Henry, M.A., F.R.S.
Mount-Edgecumbe, ErnestAugustus, Earl of.
Murchison, Sir Roderick I.,G.C. St.8., F.R.S.
Neill, Patrick, M.D., F.R.S.E.
Nicol, D., M.D.
Nicol, Professor J., F.R.S.E., F.G.S.
Nicol, Rey. J. P., LL.D.
Northampton, Spencer Joshua Alwyne, Mar-
quis of, V.P.R.S. (deceased).
Northumberland, Hugh, Duke of, K.G.,M.A.,
F.R.S. (deceased).
Ormerod, G. W., Hsq., M.A., F.G.S.
Orpen, Thomas Herbert, M.D. (deceased).
Orpen, John H., LL.D.
Osler, Follett, Esq., F.R.S.
Owen, Professor Richd.,M.D., D.C.L.,F.R.S.
Oxford, Samuel Wilberforce, D.D., Lord
Bishop of, F.R.S., F.G.S.
Palmerston, Viscount, G.C.B., M.P.
Peacock, Very Rey. G., D.D., Dean of Ely,
F.R.S. (deceased). :
Peel, Rt.Hon.Sir R.,Bart.,M.P.,D.C.L.(dec*).
Pendaryes, E. W., Esq., F.R.S. (deceased).
Phillips, Professor John, M.A., LL.D.,F.R.S.
Pigott, The Rt. Hon. D. R., M.R.1.A., Lord
Chief Baron of the Exchequer in Ireland.
Porter, G. R., Esq. (deceased).
Portlock, General, R.E., F.R.S.
Powell, Rev. Professor, M.A., F.R.S. (dec*).
Price, Rey. Professor, M.A., F.R.S.
Prichard, J. C., M.D., F.R.S. (deceased).
Ramsay, Professor William, M.A.
Ransome, George, Esq., F.L.S.
Reid, Maj.-Gen. Sir W., K.C.B., R.E., F.B.S.
(deceased).
Rendlesham, Rt. Hon. Lord, M.P.
Rennie, George, Hsq., F.R.S.
Rennie, Sir John, F.R.S.
Richardson, Sir John, M.D., C.B., F.R.S.
Richmond, Duke of, K.G., F.R.S. (dec*).
Ripon, Earl of, F.R.G.S.
MEMBERS OF THE COUNCIL.
Ritchie, Rev. Prof., LL.D., F.R.S. (dec*).
Robinson, Capt., R.A.
Robinson, Rev. J., D.D.
Robinson, Rey. T. R., D.D., F.R.AS.
Robison, Sir John, Sec.R.S. Edin. (deceased).
Roche, James, Esq.
Roget, Peter Mark, M.D., F.R.S.
Ronalds, Francis, F.R.S.
Rosebery, The Harl of, K.T., D.C.L., F.R.S.
Ross, Rear-Ad. Sir J.C.,R.N., D.C.L., F.B.S.
Rosse, Wm., Earl of, M.A., F.R.S., M.R.LA.
Royle, Prof. John F., M.D., F.R.S. (dec).
Russell, James, Esq. (deceased).
Russell, J. Scott, Esq., F.R.S. [V.P.R.8.
Sabine, Maj.-General, R.A., D.C.L., Treas. &
Sanders, William, Esq., F.G.S.
Scoresby, Rev. W., D.D., F.R.S. (deceased).
Sedgwick, Rev. Prof. Adam, M.A., F.R.S.
Selby, Prideaux John, Esq., F.R.S.E.
Sharpey, Professor, M.D., Sec.R.8.
Sims, Dillwyn, Esq.
Smith, Lieut.-Colonel C. Hamilton, F.R.S.
(deceased).
Smith, James, F.R.S. L. & E.
Spence, William, Esq., F.R.S. (deceased).
Stanley, Edward, D.D., F.R.S., late Lord
Bishop of Norwich (deceased).
Staunton, Sir G. T., Bt., M.P., D.C.L., F.R.S.
St. David’s, C.Thirlwall,D.D.,LordBishop of.
Stevelly, Professor John, LL.D.
Stokes, Professor G. G., Sec.R.S.
Strang, John, Esq., LL.D.
Strickland, Hugh E., Esq., F'.R.S. (deceased).
Sykes, Colonel W. H., M.P., F.R.S.
Symonds, B. P., D.D., Warden of Wadham
College, Oxford.
Talbot, W. H. Fox, Esq., M.A., F.R.S.
Tayler, Rev. John James, B.A.
Taylor, John, Esq., F.R.S.
Taylor, Richard, Hsq., F.G.S.
XXVil
Thompson, William, Hsq., F.L.S. (deceased).
Thomson, A., Esq.
Thomson, Professor William, M.A., F.R.S.
Tindal, Captain, R.N. (deceased).
Tite, William, Esq., M.P., F.R.S.
Tod, James, Esq., F.R.S.E.
Tooke, Thomas, F.R.S. (deceased).
Traill, J. S., M.D. (deceased).
Turner, Edward, M.D., F.R.S. (deceased).
Turner, Samuel, Esq., F.R.S., F.G.8. (dec*).
Turner, Rev. W.
Tyndall, Professor, F.R.S.
Vigors, N. A., D.C.L., F.L.S. (deceased).
Vivian, J. H., M.P., F.R.S. (deceased).
Walker, James, Esq., F.R.S.
Walker, Joseph N., Esq., F.G-S.
Walker, Rev. Professor Robert, M.A., F.R.S.
Warburton, Henry, Hsq.,.M.A., F.R.S.(dec*).
Ward, W. Sykes, Esq., F.C.S.
Washington, Captain, R.N., F.R.S.
Webster, Thomas, M.A., F.R.S.
West, William, Esq., F.R.S. (deceased).
Western, Thomas Burch, Esq.
Wharncliffe, John Stuart, Lord, F.R.S.(dec*).
Wheatstone, Professor Charles, F.R.S. ’
Whewell, Rey. William, D.D., F.R.S., Master
of Trinity College, Cambridge.
White, John F., Esq.
Williams, Prof. Charles J. B., M.D., F.R.8.
Willis, Rev. Professor Robert, M.A., F.R.S.
Wills, William, Esq., ¥.G.S. (deceased).
Wilson, Thomas, EHsq., M.A.
Wilson, Prof. W. P.
Winchester, John, Marquis of.
Woollcombe, Henry, Esq., F.S.A. (deceased).
Wrottesley, John, Lord, M.A., F.R.S.
Yarborough, The Ear! of, D.C.L.
Yarrell, William, Esq., F.L.S. (deceased).
Yates, James, Esq., M.A., F.R.S.
Yates, J. B., Esq., F.S.A., F.R.G.S. (dec*).
OFFICERS AND COUNCIL, 1860-61.
TRUSTEES (PERMANENT).
51k RopERIcK I. MurcuIson, G.C.St.S., F.R.S. JOHN TAYLOR, Esq., F.R.S,
Major-General EDWARD SABINE, R.A., D.C.L., Treas. & V.P.R.S.
PRESIDENT.
THE LORD WROTTESLEY, M.A., V.P.R.S, F.R.A.S,
VICE-PRESIDENTS.
The EArt oF DERBY, P.C., D.C.L., Chancellor of | CHarLES G. B. DAuBENy, LL.D., M.D., F-.R.S.,
the University of Oxford. F.L.S., F.G.S., Professor of Botany in the Uni-
The Rey. F, JEUNE, D.D., Vice-Chancellor of the versity of Oxford.
University of Oxford. HENRY W. ACLAND, M.D., D.C.L., F.R.S., Regius
The DuKE oF MARLBOROUGH, D.C.L. Professor of Medicine in the University of Ox-
The EARL OF Rosse, K.P., M.A., F.R.S., F.R.A.S. ford.
The Lorp BIsHoP OF OXFORD, F.R.S. WILLIAM F. Donkin, Esq., M.A., F.R.S., Savilian
The Very Rev. H. G. LippELL, D.D., Dean of Professor of Astronomy in the University of Ox-
Christ Church, Oxford. ford.
PRESIDENT ELECT.
WILLIAM FAIRBAIRN, Esq., LL.D., C.E., F.R.S,
VICE-PRESIDENTS ELECT.
The EARL oF ELLESMERE, F.R.G.S. JAMES ASPINALL TURNER, Esq., M.P.
The Lorp STANLEY, M.P., D.C.L., F.R.G.S. JAMES PRESCOTT JOULE, Esq., LL.D., F.R.S., Pre-
The Lorp BisHop OF MANCHESTER, D.D., F.R.8., sident of the Literary and Philosophical Society
.G.S. of Manchester.
Sir Poitrp DE MALpas GREY EGERTON, Bart., | Eaton HopeKtnson, Esq., F.R.S., M.R.I.A.,
M.P., F.R.S., F.G.S. M.I.C.E., Professor of the Mechanical Principles
Sir Bensamin HEywoop, Bart., F.R.S, of Engineering in University College, London.
THOMAS BAazLEY, Esq., M.P. JOSEPH WHITWORTH, Esq., F'.R.S., M.I.C.E.
LOCAL SECRETARIES FOR THE MEETING AT MANCHESTER.
ROBERT DUKINFIELD DARBISHIRE, Esq., B.A., F.G.S., Brown Street, Manchester,
ALFRED NEILD, at Mayfield, Manchester.
ARTHUR RANSOME, Esq., M.A., St. Peter’s Square, Manchester.
Professor HENRY ENFIELD Roscor, B.A., Owens College, Manchester.
LOCAL TREASURER FOR THE MEETING AT MANCHESTER.
ROBERT PHILIPS GREG, Esq., F.G.S., Manchester.
ORDINARY MEMBERS OF THE COUNCIL.
BaBinGTon, C. C., M.A., F.R.S. | GLADSTONE, Dr. J. H., F.R.S. SHARPEY, Professor, Sec. B.S.
BELL, Prof. T., Pres. L.S., F.R.S. | GRovE, WILLIAM R., F.R.S. SpPorriswoopr, W., M.A., F.R.S8,
Bropik, Sir BENJAMIN C., Bart., | HoRNER, LEONARD, F.R.S. Sykes, Colonel W. Fa es
D.C.L., Pres. R.8. Huron, Ropert, F.G.S. FE.R.S.
8.
H.
DE LA RUE, WARREN, Ph.D., | LYELL, Sir C., D.C.L., F.R.S. Tire, WILLIAM, M.P., F.
E.R.S. MILLER, Prof.W. A., M.D., F.R.S. | TyNDALL, Professor, F.R
FirzRoy, Rear Admiral, F.R.S. PorTLOCK, General, R.E., F.R.S. | WEBSTER, THOMAS, F.R.
GALTON, FRANCIS, F.G.S. PRICE, Rey. Prof., M.A., F.R.S. WILLIs, Rey. Prof., M.A., F.R.S.
Gassior, JOHN P., F.R.S.
EX-OFFICIO MEMBERS OF THE COUNCIL.
The President and President Elect, the Vice-Presidents and Vice-Presidents Elect, the General and
Assistant-General Secretaries, the General Treasurer, the Trustees, and the Presidents of former years,
yiz.—Rev. Professor Sedgwick. The Marquis of Lansdowne. The Duke of Devonshire. Rey. W. V. Har-
court. The Marquis of Breadalbane. Rey. W. Whewell, D.D. The Earl of Rosse. Sir John F, W.
Herschel, Bart. Sir Roderick I. Murchison. The Rey. T. R. Robinson, D.D. Sir David Brewster.
G. B. Airy, Esq., the Astronomer Royal. General Sabine. William Hopkins, Esq., LL.D. The Earl of
Harrowby. The Duke of Argyll. Professor Daubeny, M.D. The Rev. H. Lloyd, D.D. Professor
Owen, M.D., D.C.L. His Royal Highness The Prince Consort.
GENERAL SECRETARY.
The Rey. ROBERT WALKER, M.A., F.R.S., Professor of Experimental Philosopliy in the University of
Oxford; Culham Vicarage, Abingdon.
ASSISTANT-GENERAL SECRETARY.
JouN PHILLIPS, Esq., M.A., LL.D., F.R.S., F.G.S., Professor of Geology in the University of Oxford ;
Museum House, Oxford.
CENERAL TREASURER.
JouHN TAYLOR, Esq., F.R.S., 6 Queen Street Place, Upper Thames Street, London.
LOCAL TREASURERS.
R.
8.
8
William Gray, Esq., F.G.S., York. John Gwyn Jeffreys, Esq., F.R.S., Swansea.
C. C. Babington, Esq., M.A., F.R.S., Cambridge. J. B. Alexander, Ksq., ong
William Brand, Esq., Edinburgh. Robert Patterson, Esq., M.R.LA., Belfast.
John H. Orpen, LL.D., Dublin. Edmund Smith, Esq., Hull.
William Sanders, Esq., F.G.S., Bristol. Richard Beamish, Esq., F.R.S., Cheltenham.
Robert M‘Andrew, Esq., F.R.S., Liverpool. John Metcalfe Smith, Esq., Leeds.
W. R. Wills, Esq., Birmingham. John Angus, Esq., Aberdeen.
Professor Ramsay, M.A., Glasqow. Rey. John Griffiths, M.A., Oxford.
Robert P. Greg, Esq., F.G.S., Manchester.
AUDITORS.
Robert Hutton, Esq. Dr. Norton Shaw. John P. Gassiot, Esq.
OFFICERS OF SECTIONAL COMMITTEES. XX1X
OFFICERS OF SECTIONAL COMMITTEES PRESENT AT THE
ABERDEEN MEETING,
SECTION A.—-MATHE&MATICS AND PHYSICS.
President.—Rev. B. Price, M.A., F.R.S., Professor of Natural Philosophy, Oxford.
Vice- Presidents.—Sir David Brewster, K.H.,D.C.L., F.R.S.; Rev. H. Lloyd, D.D.,
F.R.S., M.R.I.A.; Rev. R. Main, M.A., F.R.S.; Rev. W. Whewell, D.D., F.R.S.,
Hon. M.R.1.A., Master of Trinity College, Cambridge.
Secretaries.—Professor Stevelly, LL.D.; Rev. T. Rennison, M.A., Fellow of
Queen’s College; Rev. G. C. Bell, M.A., Fellow of Worcester College.
SECTION B.—CHEMISTRY AND MINERALOGY, INCLUDING THEIR APPLICATIONS
TO AGRICULTURE AND THE ARTs.
President.—B. C. Brodie, Esq., M.A., F.R.S., F.C.S., Professor of Chemistry,
Oxford.
Vice- Presidents. —Professor Andrews, M.D., F.R.S., M.R.1.A., F.C.S.; Warren
De la Rue, Ph.D., F.R.S., F.C.S.; Professor Faraday, D.C.L., F.R.S., F.C.S.;
Professor Frankland, Ph.D., F.R.S.; Professor W. A. Miller, M.D., F.R.S., F.C.S.;
Lyon Playfair, C.B., Ph.D., F.R.S., F.C.S.
Secretaries.—G. D. Liveing, M.A., F.C.S.; A. Vernon Harcourt, Esq., B.A.,
F.C.S., Student of Christ Church; A. B. Northcote, Esq., F.C.S., Queen’s College.
SECTION C.—GEOLOGY.
President.,—Rev. A. Sedgwick, M.A., LL.D., F.R.S., F.G.S., Professor of Geology,
Cambridge.
Vice-Presidents.—Sir Charles Lyell, LL.D., D.C.L., F.R.S., Hon. M.R.S.E.,
F.G.S.; L. Horner, Pres. G.S., F.R.S.; Major-General Portlock, R.E., LL.D.,
F.R.S., F.G.S.
Secretaries.—Professor Harkness, F.R.S., F.G.S.; Captain Woodall, M.A.,
F.G.S., Oriel College; Edward Hull, B.A., F.G.S.
SECTION D.—ZOOLOGY AND BOTANY, INCLUDING PHYSIOLOGY.
President.—Rev. Professor Henslow, F.L.S., Professor of Botany, Cambridge.
Vice-Presidents.— Professor Daubeny, M.D., LL.D., F.R.S., F.L.S.; Sir W. Jar-
dine, Bart., F.R.S.E., F.L.S.; Professor Owen, M.D., LL.D., F.R.S., F.L.S.
Secretaries.—E. Lankester, M.D., LL.D., F.R.S., F.L.S.; E. Percival Wright,
M.A., M.B., M.R.ILA., F.L.S.; P. L. Sclater, M.A., F.L.S., Sec. Z.S., C.C.C.;
W.S. Church, B.A., University College.
SUB-SECTION D.—PHYSIOLOGICAL SCIENCE.
President.—George Rolleston, M.D., F.L.S., Professor of Physiology.
Vice-Presidents.—Professor Acland, M.D., LL.D., F.R.S.; Sir B. Brodie, Bart.,
D.C.L., Pres. R.S.; George Busk, F.R.S.; Dr. Davy, F.R.S. L. & E.; Professor
Huxley, F.R.S.; W. Sharpey, M.D., Sec. R.S., F.R.S.E.
Secretaries.—Robert M°Donnell, M.D., M.R.I.A.; Edward Smith, M.D., F.R.S.
SECTION E.—GEOGRAPHY AND ETHNOLOGY.
President.—Sir R.I. Murchison, G.C.St.S.,D.C.L., F.R.S., V.P.R.G.S.; Director-
General of the Geological Survey of the United Kingdom.
Vice-Presidents.—Lord Ashburton, M.A., F.R.S.; John Crawfurd, Esq., F.R.S.,
Pres. Ethn. Soc.; Francis Galton, Esq., M.A., F.R.S.; Sir J. Richardson, C.B.,
M.D., LL.D., F.R.S., F.R.G.S.; Sir Walter C. Trevelyan, Bart.
Secretaries.—Norton Shaw, M.D., Sec. R.G.S.; Thomas Wright, M.A., F.S.A.;
Captain Burrows, R.N., M.A.; Charles Lempriere, D.C.L.; Dr. James Hunt, F.S.A.
SECTION F.—ECONOMIC SCIENCE AND STATISTICS.
President.—Nassau W. Senior, M.A., late Professor of Political Economy, Oxford.
Vice-Presidents.—Sir John P. Boileau, Bart., F.R.S.; James Heywood, F.R.S. ;
Lord Monteagle, F.R.S.; Monckton Milnes, M.P.; Right Hon. Joseph Napier,
LL.D., D.C.L.; Sir Andrew Orr; Sir J. Kay Shuttleworth, Bart., F.G.S.; Col. Sykes,
M.P., F.R.S.; William Tite, Esq., M.P., F.R.S,
XXX
REPORT—1860.
Secretaries.—William Newmarch; Edmund Macrory, M.A.; Rev. J. E. T.
Rogers, M.A., Magdalen Hall, Tooke Professor of Political Economy, King’s Col-
lege, London.
SECTION G.—MECHANICAL SCIENCE.
President.—W. J. Macquorn Rankine, LL.D., F.R.S., Professor of Engineering,
Glasgow.
Vice-Presidents.—J. F. Bateman, F.R.S.; W. Fairbairn, C.E., LL.D., F.R.S. ;
J. Glynn, F.R.S.; Admiral Moorsom; Sir John Rennie, F.R.S.; Marquis of Stafford,
M.P.; James Walker, C.E., LL.D., F,.R.S.; Professor Willis, M.A., F.R.S.;
T. Webster, Q.C., M.A., F.R.S.
Secretaries,—P. Le Neve Foster, M.A.; Rey. Francis Harrison, M.A.; Henry
Wright.
CORRESPONDING MEMBERS.
Professor Agassiz, Cambridge, Massa-
chusetts.
M. Babinet, Paris.
Dr. A. D. Bache, Washington.
Professor Bolzani, Kazan,
Dr. Barth.
Dr. Bergsma, Utrecht.
r. P. G. Bond, Cambridge, U.S.
M. Boutigny (d’Evreux).
Professor Braschmann, Moscow.
Dr. Carus, Leipzig.
Dr. Ferdinand Cohn, Breslau.
M. Antoine d’Abbadie.
M. De la Rive, Geneva.
Professor Dove, Berlin.
Professor Dumas, Paris.
Dr. J. Milne-Edwards, Paris.
Professor Ehrenberg, Berlin.
Dr. Eisenlohr, Carlsruhe.
Professor Encke, Berlin.
Dr. A. Erman, Berlin.
Professor Esmark, Christiania.
Prof. A. Favre, Geneva.
Professor G. Forchhammer, Copenhagen.
M. Léon Foucault, Paris.
Prof. E. Fremy, Paris.
M. Frisiani, Milan.
Dr. Geinitz, Dresden.
Professor Asa Gray, Cambridge, U.S.
Professor Henry, Washington, U.S.
Dr. Hochstetter, Vienna.
M. Jacobi, St. Petersburg.
M. Khanikoff, St. Petersburg.
Prof. A. Kolliker, Wurzburg.
Prof. De Koninck, Liége.
Professor Kreil, Vienna.
Dr. A. Kupffer, St. Petersburg.
| Dr. Lamont, Munich.
Prof. F. Lanza.
M. Le Verrier, Paris.
Baron von Liebig, Munich.
Professor Loomis, New York.
Professor Gustav Magnus, Berlin.
Professor Matteucci, Pisa.
Professor von Middendorff, St. Petersburg.
M. l’Abbé Moigno, Paris.
Professor Nilsson, Sweden.
Dr. N. Nordenskiold, Finland.
M. E. Peligot, Paris.
Prof. B. Pierce, Cambridge, U.S.
Viscenza Pisani, Florence.
Gustave Plaar, Stresburg.
Chevalier Plana, Turin.
Professor Pliicker, Bonn.
M. Constant Prévost, Paris.
M. Quetelet, Brussels.
Prof. Retzius, Stockholm.
Professor W. B. Rogers, Boston, U.S.
Professor H. Rose, Berlin.
Herman Schlagintweit, Berlin.
Robert Schlagintweit, Berlin.
M. Werner Siemens, Vienna.
Dr. Siljestrom, Stockholm.
M. Struvé, Pulkowa.
Dr. Svanberg, Stockholm.
M. Pierre Tchihatchef.
Dr. Van der Hoeven, Leyden.
Prof. E. Verdet, Paris.
Baron Sartorius von Waltershausen,
Gottingen.
Professor Wartmann, Geneva.
Report of the Council of the British Association, presented to the
General Committee at Oxford, June 27, 1860.
1. The Council were instructed by the General Committee at Aberdeen
to maintain the establishment at Kew Observatory by aid of a grant of £500.
They have received the following Report of the Committee to whom the
working of the Observatory is entrusted.
REPORT OF THE KEW COMMITTEE. XXX1
_ 2. The continuance of Magnetic Observations, at stations indicated by the
General Committee at the Leeds Meeting, has engaged the attention of H.R.H.
the President, and of the Council; and they have had the advantage of co-
operation on the part of the President and Council of the Royal Society.
Every means has been adopted for pressing the subject on the favourable
attention of the Government, but, it is to be regretted, hitherto without
success.
3. The importance of telegraphic communication between sea-ports of the
British Isles, has been the subject of much attention since it was urged on
the General Committee by the Aberdeen Meeting. The Council are happy
to find that Admiral FitzRoy has been authorized to proceed in bringing to
a practical issue the recommendations offered on this subject to the scientific
department of the Board of Trade; and they. congratulate the Association
on the share they have taken in a cause so dear to humanity.
4. The expedition suggested by the Royal Geographical Society, and con-
curred in by the General Committee of the British Association, is on its
way; Capt. Speke, under the direction of the Admiralty, with his assistant,
Capt. Grant, having sailed from Zanzibar. Sir R.1. Murchison, in reporting
on this subject, expresses the obligation which is felt by the promoters of this
great step for the exploration of Africa, to Lord John Russell, Secretary of
State for Foreign Affairs.
The Report of the Parliamentary Committee is received for presentation
to the General Committee this day.
5. At the Meeting this day, in pursuance of the Notice placed in the
Minutes of the General Committee at Aberdeen, it will be proposed —“ That
a permanent distinct Section of Anatomy and Physiology be established, in
addition to that of Zoology and Botany.”
The Council are informed that Invitations will be presented to the General
Committee at its Meeting on Monday, July 2, to hold the next Meeting in
Manchester; on behalf of the Literary and Philosophical Society of Man-
chester, and other Institutions and Public Authorities of that city, from whom
Invitations were received at previous Meetings.
Invitations will also be presented to hold an early Meeting in Newcastle,
on behalf of the Council and Borough of Newcastle-upon-Tyne, and to hold
a Meeting in Birmingham in 1862, on behalf of the Birmingham and Midland
Institute.
Report of the Kew Committee of the British Association for the
Advancement of Science for 1859-1860.
Since the last Meeting of the British Association, the self-recording mag-
netographs have been in constant operation under the able superintendence
of Mr. Chambers, the magnetical assistant.
A description of these instruments has been given by Mr. Stewart, the
Superintendent, in a Report which is printed in the Transactions of the British
Association for 1859. The drawings for the plates connected with this
Report were made with much skill by Mr. Beckley, the mechanical assistant
at Kew.
It was mentioned in the last Report of this Committee, that a set of self-
recording magnetic instruments, designed for the first of the Colonial Obser-
vatories which have been proposed to Her Majesty’s Government, had been
completed and set up in a wooden house near the Observatory.
Shortly after the meeting at Aberdeen, the Chairman received a letter from
Dr. P. A. Bergsma, Geographical Engineer for the Dutch possessions in the
XXX1l REPORT—1860.
Indian Archipelago, requesting that the Committee would assist him in pro-
curing a set of self-recording magnetic differential instruments similar to
those at Kew, the Dutch Government having resolved to erect such at their
Observatory at Java.
In consequence of this application, and as the instruments which had been
completed were not immediately required for a British Observatory, it was
resolved that they should be assigned to Dr. Bergsma; this gentleman has
since arrived, and has for the last few weeks been engaged at the Observatory
in the examination of his instruments.
The usual monthly absolute determinations of the magnetic elements con-
tinue to be made.
Application having been made through Padre Secchi, of the Collegio Ro-
mano, for a set of magnetic instruments, for both differential and absolute
determinations, for the Jesuits’ College at Havanna, the whole to cost 600
dollars, or about £150, General Sabine obtained, at a reasonable price, the
three magnetometers that had formerly been employed at Sir T. Brisbane’s
Observatory at Makerstoun, and also an altitude and azimuth instrument.
With these instruments it is expected that the application from Havanna
Observatory can be met within the sum named; the instruments are now in
the hands of the workmen, and will be ready early in July.
Two unifilars, supplied by the late Mr. Jones, for the Dutch Government
(one for Dr. Bergsma, and the other for Dr. Buys Ballot), have had their
constants determined. Observations have also been made with two 9-inch
dip-circles belonging to General Sabine, which have been repaired by Barrow,
and with two dip-circles and a Fox’s instrument designed for Dr. Bergsma.
A set of magnetical instruments, consisting of a dip-circle, an azimuth
compass, and a unifilar, previously used by Captain Blakiston, have been
re-examined, and have been taken by Colonel Smythe, of the Royal Artillery,
to the Feejee Islands.
As it was feared that the Kew Standard Barometer might have been
injured by the workmen who some time since were repairing the Observatory,
a new one has been mounted. ‘The mechanical arrangements of this instru-
ment have been completed in a very admirable manner by Mr. Beckley ; and
the mean of all the observations made shows that the new Barometer reads
precisely the same asthe old. This result is satisfactory, not only as showing
that no change has taken place in the old Barometer, but as confirming the
accuracy of the late Mr. Welsh’s process of constructing these instruments.
The height of the cistern of the new Barometer above the level of the sea is
33°74 feet.
Mr. Valentine Magrath having quitted the Observatory, at his own request,
on the 14tn of February last, Mr. George Whipple has taken his place as
Meteorological Assistant, and has given much satisfaction.
On the 12th of March, Thomas Baker was engaged at the weekly salary
of 8s., to be raised to 10s. in six months if he gave satisfaction, which has
hitherto been the case.
Since the last meeting of the Association, 173 Barometers and 222 Ther-
mometers have been verified at the Observatory.
Professor Kupffer, Director of the Russian Magnetical and Meteorological
Observatories, visited the Observatory, and was presented with a standard
thermometer.
Mr. J. C. Jackson, Lieutenant Goodall, R.E., and Mr. Francis Galton,
F.R.S., have visited the Observatory, and received instructions in the mani-
pulation of instruments.
Mr. Galton has made some experiments at Kew Observatory, to determine
.
REPORT OF THE KEW COMMITTEE. XKXIil
the most practicable method of examining sextants, and other instruments
for geographical purposes. Considering that these instruments, after having
been once adjusted, are liable to two distinct classes of error, the one constant
for any given reading, and the other variable, it is an object to form Tables
of Corrections for the constant errors of instruments sent for examination,
and also to ascertain the amount of variable errors which might affect their
readings.
As a groundwork for examination, it is found that small mirrors may be
permanently adjusted, at the distance of half a mile, so that when the rays
of a mirror of moderate size, standing by the side of an assistant, are flashed
upon them, they may re-reflect a brilliant star of solar light, towards the
sextant under examination.
By having four permanently fixed mirrors of this description, separated by
intervals of 20°, 60°, and 40° respectively, and by flashing upon them with
two looking-glasses of moderate size, it is possible, by using every combina-
tion of these angles, to measure every twentieth degree, from 0° up to 120°.
The disturbing effects of parallax are eliminated without difficulty, by
mere attention to the way in which the sextant is laid on the table, or, in
the case of a zero determination, by a simple calculation.
Moreover, the brilliancy of the permanent mirrors is perfectly under con-
trol, by the interposition of gauze shades in front of the looking-glasses that
flash upon them. This renders an examination of the coloured shades a
matter of great ease and certainty.
Based upon these principles, Mr. Galton has drawn up a system for the
thorough examination of sextants. Each would not occupy more than two
hours in having its constant errors tabulated, and its variable errors deter-
mined; nor would an outlay of more than £30 be required for the establish-
ment of fixed tables and permanent marks. Difficulty is, however, felt in
setting the system in action, owing to the absolute need of an assistant
having leisure to undertake it.
The sum of £179 12s. 6d. has been received from the Royal Society,
to defray the expense of erecting a model house for the reception of the
instruments for Colonial Magnetic Observatories.
The Photoheliograph has been an occasional source of occupation to the
mechanical assistant; but before daily records of the sun's disk can be ob-
tained, it is absolutely requisite that an assistant should be appointed to aid
Mr. Beckley, because his duties are of such a nature as to prevent his de-
voting attention at fixed periods of the day to an object requiring so much
preparation as is the case with photoheliography. Unfortunately, the funds
at the disposal of the Committee are quite inadequate for this purpose; and
unless a special grant be obtained, the Photoheliograph will remain very little
used.
At present Mr. Beckley is preparing the instrument, under Mr. De la Rue’s
direction, for its intended trip to Spain, for the purpose of photographing the
eclipse which takes place on July 18th. The expenses of these preparations,
and of the assistants who will accompany Mr. De la Rue, will be defrayed
out of the grant of the Royal Society for that object.
The requisite preparations are somewhat extensive ; for it has been deemed
necessary to construct a wooden observatory, and to make a new iron pillar
to support the instrument, adapted to the latitude of the proposed station:
both the observatory and iron pillar may be taken to pieces to facilitate their
transport,
The wooden house is 8 feet 6 inches square, and 7 feet high; it is entirely
open at the top, except that portion divided off for a photographic room.
1860. ¢
XXXiv REPORT—1860.
The open roof will be covered by canvas when the observatory is not in use ;
and when in use, the canvas will be drawn back, so as to form an outer casing
at some little distance from the wall of the photographic room; and, in order
to keep this room as cool as possible, the canvas will, in case of need, be kept
wetted.
The chemicals and chemical apparatus will be packed in duplicate sets, so
as to provide as far as possible against the contingency of loss, by breakage
or otherwise, of a part of them.
Mr. Downes, of the firm of Cundall and Downes of Bond Street, has
promised to accompany the expedition; Mr. Beckley will also go; and Mr.
De la Rue has engaged Mr. Reynolds to assist in the erection of the observa-
tory in Spain, and in the subsequent photographic operations.
The Admiralty, on the representation of the Astronomer Royal, have pro-
vided a steam-ship to convey this and other astronomical expeditions to Bil-
bao and Santander. It is proposed that the Kew party should land at Bilbao
and proceed to Miranda. Mr. Vignoles, who is constructing the Tudela and
Bilbao railway, has kindly promised his aid and that of his staff of assist-
ants, to promote the objects of the expedition, and promises, on behalf of the
contractors, the use of horses and carts for the conveyance of the apparatus.
The expedition will sail from Portsmouth on the 7th of July; and, should the
weather prove favourable, there is reasonable hope that the various phases
of the eclipse will be successfully photographed. Whether the light of the
corona and red prominences will be sufficiently bright to impress their images,
when magnified to four inches in diameter, is a problem to be solved only by
direct experiment.
Professor William Thomson (of Glasgow) having expressed a desire that
the practical utility of his self-recording electrometer should be tried at Kew,
his wish has been acceded to and the instrument received, and it is expected
that it will shortly be in operation under his direction.
A Report has been completed by the Superintendent on the results of the
Magnetic Survey of Scotland and the adjacent islands in the years 1857 and
1858, undertaken by the late Mr. Welsh. This Report is printed in the
Transactions of the British Association for 1859.
The following correspondence has taken place between General Sabine
and the Rev. William Scott, Director of the Sydney Observatory :—
“ Observatory, Sydney, March 2, 1860.
“ Srr,—The great interest which you take in the promotion of Magnetical
Science encourages me to address you on the subject of the establishment of
a Magnetical Observatory at Sydney. The report which I send you by this
mail will explain to you the character and position of the Astronomical Ob-
servatory under my direction.
“JT am convinced that an application to our Government, from influential
persons at home, for the establishment of magnetical observations on not
too expensive a scale, would be readily attended to. Iam not practically
acquainted with any magnetical observatory, with the exception of that at
Greenwich, and am ignorant of the cost of a set of instruments, and the
exact amount of space required for working them; but I believe we could
find sufficient room in the observatory without any additional building; they
would be under my own supervision, and all that would be required would
be an additional assistant, to share with myself and my one assistant in
observing and computing. The Governor-General, Sir W. Denison, would,
though powerless as regards public money, exert his influence in favour of
such an object.
REPORT OF THE KEW COMMITTEE. XXXV
“ Trusting that you will take the matter into consideration, and excuse the
liberty I have taken in addressing you,
“Tam, Sir,
‘* Your obedient Servant,
(Signed) “W. Scort,
« Astronomer for N. S. Wales.”
“ Major-General Sabine.”
“13 Ashley Place, London, May 8, 1860.
y y
« Str,—I lose no time in replying to your letter of March 2, received this
day. ‘The self-recording magnetical instruments at Kew have been in action
nearly two and a half years—a sufficient time to test their merits or defects.
I have myself completed the analysis and reduction of the first two years (1858
and 1859) of the Observations of the Declinometer, and can therefore speak of
my own knowledge of their performance, as far as that element is concerned.
The Photographic Traces, recording both the zero line and the actual move-
ments of the magnet, can be measured with tolerable confidence to the third
place of decimals of an inch, the inch in the Kew instrument being equiva-
lent to 22 minutes of arc. The reading is consequently made to the 1000th
part of 22 minutes of declination. The record is of course continuous; but,
for the purpose of computing the results, howrly readings have been tabulated.
In the first year the trace failed in 107 out of 8760 hours, chiefly from
failure in the supply of gas, which is brought by pipes from Richmond, a
considerable distance off. This inconvenience has been remedied by the
construction at the Observatory itself, at a small expense, of a water regu-
lator, through which the supply from Richmond passes, and there is now no
reason why the trace should ever fail. I have now in course of analysis and
reduction the same years of the observations of the horizontal and vertical
force magnetographs, and have no reason hitherto to believe tnat the record
of those two elements will be inferior to that of the declination. The three
instruments, with the clock which keeps the registering papers in revolution,
together with reading telescopes placed for eye observation, either to accom-
pany or to be independent of self-registry, occupy an interior space of about
16 feet by 12, including a passage round for the observer. The cost of such
a set of instruments, complete in every respect, is £250; and four months
must be allowed for making them from the date of the order, as well as an
additional month for their careful verification at Kew (should that be de-
sired), where a detached building has been erected for this particular pur-
pose, in which they may be kept in work in comparison with the Kew instru-
ments. A detailed description of these instruments is now in the press, and
will be published in June in the volume of Reports of the British Association.
The results of the first two years of the Declinometer observations, showing
what are deemed at present to be the most useful modes of eliciting the re-
sults, will be printed in the ‘ Proceedings of the Royal Society’ in the present
summer, and the first two years of the horizontal and vertical force magneto-
graphs in the same publication later in the year. A small adjoining room is
requisite, opening if possible into the instrument-room, which should contain
suitable troughs for the preparation of the paper to receive the traces, and
to fix them. It is important to diminish as much as possible the changes of
temperature in the Observatory itself, exclusive of the effect of the instrument
cases, which have adaptations for that purpose. So far in regard to differential
instruments. For absolute determinations and secular changes a small de-
tached house is required, say 12 feet by 8, in which equality of temperature
need not be regarded, but which must be at a sufficient distance from other
e2
Xxxvi REPORT—1860.
buildings containing iron, and have copper fittings. The instruments required
for these purposes are an inclinometer and a unifilar, the latter having pro-
vision for the experiments of deflection and vibration, as well as for the abso-
lute declination: the cost of the first is £30, and of the second £45; both may
be verified, if desired, at Kew. The little work which is sent to you by the
same post as this letter contains a full description of these instruments, and
directions for their use. In addition to the charges named above, making in
all £325, the cost of packing, freight, and insurance will have to be taken
into the account.
“ One assistant will suffice, as you suggest, for keeping the magnetometers
in action, and for tabulation. The absolute values, and the calculation of the
results of all the instruments, would be, I presume, the work of the Director
of the Observatory himself. Provision must also be made for a supply of
chemicals, stationery, and gas. Should it be thought desirable that the instru-
ments should be prepared and verified under the superintendence of the Com-
mittee of the Kew Observatory, a request to that effect, transmitted by your-
self through the Governor of the Colony to the Chairman of the Committee
of the Kew Observatory, Richmond Park, London, $.W., would, I am sure,
meet immediate attention. That such an institution at the head-quarters of
our Australian dominions would be as honourable to those who should be
instrumental in its establishment as it would be beneficial to magnetical
science, must be a matter of general recognition, and it would, I am per-
suaded, find a warm supporter in your present most excellent Governor.
‘TI remain, Sir,
“ Your obedient Servant,
(Signed) “ EDWARD SABINE.”
“ The Rev. W. Scott.”
From the following correspondence which has taken place between Her
Majesty’s Government and the President of the Royal Society, it will be
seen that the establishment of a Magnetical Observatory at Vancouver
Island is postponed, in consequence of the war with China precluding the
establishment at present of a corresponding observatory at Pekin :—
“Treasury Chambers, 16th May, 1860.
“ Srr,—I am directed by the Lords Commissioners of Her Majesty’s
Treasury to acquaint you that My Lords have had under their further con-
sideration the establishment of an Observatory at Vancouver Island, and
the insertion in the Estimates of this year of a vote for that service.
“ My Lords are fully sensible of the importance of obtaining a series of
accurate Magnetical Observations at the stations recommended by the Council
of the British Association, and it would give them great pleasure to assist
without further delay in forwarding objects so interesting for the cause of
science.
“The numerous and pressing claims, however, on the public finances in
the present year make it imperative upon My Lords to submit no fresh esti-
mate to Parliament which is not of a very urgent character, and where the
total limit of expense to be incurred has not been accurately ascertained.
“In the present instance My Lords must observe that you appear to be
under some misapprehension in supposing that any engagement was entered
into by the late Government to establish a Magnetic Observatory at Pekin or
elsewhere. On the contrary, the letter of this Board of 6th December, 1858,
to Lord Wrottesley states that, ‘whatever may be the public advantages to
be derived from the proposed new establishments, the object would not,
REPORT OF THE KEW COMMITTEE. XXXVI
it appears, be sacrificed by postponement, and, looking to tae extent of
the other claims upon the public finances already existing, My Lords
have thought it right to defer the consideration of the question until next
year.’
we The letter then further states, that the three Magnetical Observatories
at the Cape of Good Hope, St. Helena, and Toronto, which were originally
sanctioned in an estimate of about £3000 for three years, had in fact cost
£11,000 for that period, and, in all, had put the country to an expense of
nearly £50,000. ‘This considcration alone suffices to show the necessity for
very careful investigation by the Government before any step is taken which
might commit the country to further expense. The circumstances referred
to in the letter in question continue in full foree; and an important further
argument against undertaking the proposed Observatory at Vancouver
Island at the present moment is furnished by the political events which have
since occurred in China. In General Sabine’s able letter of the Ist January,
1859, it is stated that, ‘without entering into the comparative scientific value
of Vancouver Island and Pekin as magnetic stations,—both being highly
important,—this much is certain, that, whatever might be the value of either,
that value would be greatly enhanced—far more than doubled—by there
being a simultaneous and continuous record at both stations; and Sir John
Herschel remarks that the importance of a five years’ series of observations
at one of the proposed stations without the others would be grievously dimi-
nished, and the general scope of the project defeated.’
“ As the present state of things in China precludes the establishment of a
Magnetic Observatory at Pekin, or any point in the Chinese Empire suffi-
ciently to the north to correspond with a station at Vancouver Island
(though there is reason to hope that this state of things may be of short
duration ), it would appear desirable even in the interests of science to postpone
the consideration until something more certain can be ascertained as to the
possibility of meeting what Sir John Herschel and General Sabine consider
such an essential requisite, viz. the commencement and continuance of simul-
taneous observations at Vancouver Island and at a point in China nearly in the
same parallel of latitude. The interval which must elapse until the political
state of affairs in China may render such an establishment possible may be
usefully employed in obtaining the most accurate estimate possible of the
actual cost of founding and maintaining each station for the period requisite
for the complete attainment of the scientific objects in view, so as to enable
Her Majesty’s Government, when the proper time shall arrive, if they shall
decide on doing so, to submit a vote to Parliament with confidence as to the
amount of expense which they may ask the nation to defray in the interests
of science.
‘Cl ain, Sin
“ Your obedient Servant,
(Signed) “ Gro. A. HAMILTON.”
“ The President of the Royal Society.”
“May 23rd, 1860.
“My pear Sir,—In Mr. Hamilton's letter (returned herewith) he has
referred to Sir Charles Trevelyan’s communication to Lord Wrottesley of the
6th December, 1858, expressing the desire of the Lords Commissioners of
the Treasury to postpone to the following year the consideration of the esta-
blishment of the Colonial Magnetic Observatories which had been recom-
mended by the Royal Society and the British Association for the Advance-
XXXVili REPORT—1860.
ment of Science ; but Mr. Hamilton has omitted altogether to refer to the
interview which took place between the President of the British Association
and Sir Charles Trevelyan subsequent to that communication, viz. on the
18th of December, 1858, when Sir Charles Trevelyan stated that ‘if asingle
station for magnetical and meteorological observations were applied for [in-
timating Pekin as its locality] by the Joint Committee of the Royal Society
and the British Association, My Lords would be disposed to comply with
such application. (See Report of the Council of the British Association,
September 1859.)
“ Political events which became known shortly after that interview made
it manifestly unadvisable to apply for a station in China; but the scientific
importance of procuring systematic magnetical researches at other stations
which had been named in the original application from two Societies, in parts
of the globe which were conveniently accessible and under British dominion,
remained as before. In these respects Vancouver Island was unobjectionable,
and was therefore substituted for ‘a station in China’ in the application,
which, consistently with Sir Charles Trevelyan’s communication of the 18th
December, 1858, was made by the Joint Committee of the two Societies. The
confident expectations thus founded being known in the United States by
the publications of the Reports of the Joint Committee of the Royal Society
and British Association, the Government of the United States authorized the
establishment of Magnetical Observatories at a station on the east side of the
United States, and at another on the south coast, both designed to cooperate
with the British Observatory to be established on Vancouver Island ; the three
stations being obviously remarkably well selected for systematic researches
over that large portion of the globe. The two observatories of the United
States’ Government have been established, and commenced their work at
the beginning of the present year.
“In reference to the aggregate amount of expenditure incurred by the
magnetical researches recommended to Government by the Royal Society
and British Association in the last twenty years, it may be remarked that, the
researches being altogether of a novel character, the continuance of the
Observatories, when first asked for in 1839, was for a very limited period.
It was, in fact, an experiment, and their longer continuance would not have
been recommended had not the experiment proved eminently successful, and
such as to justify the prosecution of the researches. The subject was there-
fore brought afresh under the consideration of Government in 1845 and again
in 1849, and the further expenditure to be incurred received the sanction of
the Treasury on both occasions, as have also, on other occasions, the magnetie
surveys connected with the Observatories. It is possible that the aggregate
amount of expenditure thus sanctioned and incurred may not be overstated
at £50,000. It is an average amount not exceeding £2500 a year for this
great branch of physical science.
‘“‘T am not myself the proper authority to say whether the gain to science,
and to the estimation in scientific respects in which this country is held by
other nations, be, or be not, an equivalent for this expenditure; but I may be
permitted to refer to the opinion expressed by the Joint Committee of the
two Societies, consisting, as is well known, of persons holding high places in
public estimation for their general knowledge and good judgment, as well
as possessing the highest scientific eminence :—‘ Your Committee, looking at
this long catalogue of distinct and positive conclusions already obtained, feel
themselves fully borne out in considering that the operation, in a scientific
point of view, has proved, so far, eminently remunerative and successful, and
that its results have fully equalled in importance and value, as real accessions
REPORT OF THE KEW COMMITTEE. XXXIX
to our knowledge, any anticipations which could reasonably have been formed
at the commencement of the inquiry.’
“ Believe me, my dear Sir,
“ Faithfully yours,
(Signed) “ EDWARD SABINE.”
“ Sir B. C. Brodie, Bart., P.R.S.”
Mr. Hamilton to the President of the Royal Society, in reply to his letter of
Qnd June (not given here).
“Treasury Chambers, June 14, 1860.
“ Sir,—In reply to your letter of the 2nd inst., with its enclosure from
General Sabine relative to the establishment of Colonial Magnetic Observa-
tories, I am directed by the Lords Commissioners of Her Majesty’s Treasury
to state that, without entering into the question what verbal assurances may
have been given in December 1858 by the then Assistant Secretary, Sir Charles
Trevelyan, of which no record was made, their Lordships observe that the
main ground of their letter of the 16th May, 1860, remains unaffected, viz.
that, in the opinion of the highest scientific authorities, whatever might be
the value of observations at Vancouver Island, that value would be greatly
increased by simultaneous observations at some station in the North of China,
and, on the other hand, would be ‘ grievously diminished’ if no station in
China was established. Under these circumstances, their Lordships thought
it desirable to postpone for a short time the consideration of the question, in
the hope that it might be considered under a different state of things in China,
rendering possible the attainment of the greatest amount of scientific advan-
tage from the expenditure of public money, in case that expenditure should
be decided upon.
“Tam, Sir,
“ Your obedient Servant,
(Signed) “G. A. HamILToN.”
General Sabine has written the following letter to Dr. Bache, who had
intimated to him that, in the event of Her Majesty’s Government declining to
establish a magnetical observatory at Vancouver Island, it was the wish of
the United States’ Government to establish one in Washington Territory, in
the vicinity of Vancouver Island :—
“May 22, 1860,
“Dear Bacue,—I waited to reply to yours of April 13th until we should
have received the reply of our Government regarding the Vancouver Island
Observatory. Mr. Gladstone has availed himself of some expressions in
Sir John Herschel’s letters and mine (to the effect of the far greater import-
ance of having observations on the Chinese as well as on the American side
of the Pacific to having either separately) to postpone a decision regarding
Vancouver Island until our relations with China shall enable our Govern-
ment to consider the question of establishing both simultaneously. Our pro-
position, therefore, has fallen to the ground, and it is quite open to your
Government to occupy the field which you were willing to concede to us in
consideration of the forward part which our Government has hitherto taken
in magnetic researches.
“Now in regard to the instruments, which, as you are probably aware,
have been prepared at my own risk, in order that, should our Government
accede to the recommendation made by the Royal Society and British Asso-
xl REPORT—1860.
ciation, the time might be saved which must otherwise have been lost in their
preparation. They have been made on the model of those which have been
in use at the Kew Observatory since January 1858. An account of these isin
the press, and will be published in the volume of Reports of the British Asso-
ciation for 1859-1860, which must be in circulation next month. I have
thoroughly examined and computed the declination results for 1858 and 1859,
by means of tabulated hourly values, and am now engaged in the same cal-
culation of the Bifilar and Vertical Force Magnetometers. The Declination
Report will be presented to the Royal Society, and printed in the ‘ Proceed-
ings’ in the course of the summer, as well as the results of the Force Mag-
netometers for the same two years, as soon as I am able to draw up the report
in due form and order. But Iam able tosay, regarding all the three elements,
that the instruments are eminently successful. Independent of the continucty
of the record (which is of course a great thing in itself), the hourly tabula-
tions are far more consistent and satisfactory than were the eye-observations
at any of our observatories.
“In preparing a second set of instruments, therefore (which we have done
for the proposed Netherlands Observatory in Java), we have had very few
improvements to introduce, except the addition of reading-telescopes for each
instrument—so that we may always retain the power of eye-observation,
either in addition to or substitution for photographic records. Dr. Bergsma,
the Director of the Java Observatory, is now at Kew, observing with his in-
struments, in comparison with those in our own Observatory (as we have a
separate building for the instruments on trial), and will take them away
towards the end of June. ‘These of course will be paid for by the Netherlands
Government, having been ordered expressly for them. There will then be the
third set, which have been prepared for Vancouver, and which are ready to
succeed the Java instruments in the experimental house. A few very trifling
improvements have been introduced in these—none worthy of being noticed
here. They at present stand as mine, and I shall be indebted £250 for them.
The decision of Government, as communicated to the President of the Royal
Society, makes no reference to my responsibility on their account. I am,
therefore, to say the least, quite free to dispose of them as I may please.
Now I am not rich enough to offer them as a Joan to your ‘ Washington
Territory ’ Observatory ; but if you desire to have differential determinations
there in addition to absolute determinations, I am persuaded that you could
not have better instruments than these would be; and I consider myself as
quite free to offer you the refusal of them, asking only in return that you
will give me as early a reply as may be convenient, because I have some
reason to expect that I may receive an application from the Sydney Obser-
vatory to obtain a duplicate of the Kew instruments; in which case, if you
had not claimed them in the meantinie, I should direct these to be sent to
Sydney. -- Sincerely yours,
(Signed) “ EDWARD SABINE.”
“ Dr. Bache, F.R.S., Director of the
Coast Survey of the United States.”
The reply to this letter has not yet been received; but in the meantime
the following application has come for a set of magnetical instruments for
absolute determinations from Dr. Smallwood, Professor of Meteorology at
M°Gill College in Montreal, Canada:—
“St. Martin, Isle Jésus, May 2], 1860.
- © Srr,—I duly received yours of the 16th of July last, in reference to the
REPORT OF THE KEW COMMITTEE. xli
establishment of a Magnetic Observatory here, in connexion with observa-
tions on meteorology and atmospheric electricity, and deferred writing until
I was in a position to acquire the instruments necessary.
* You said in your communication that ‘£80 or thereabouts was required;’
and you were kind enough to add, with a spirit of generosity I could not
expect, ‘that every care should be taken to superintend the construction of
such instruments, to verify them, and to determine their constants, and have
them carefully packed and sent out.’
“ The object of the present letter is to ascertain, Ist, the exact cost (if pos-
sible); 2nd, to whom the amount shall be forwarded; Srd, when the instru-
ments would probably be ready ; 4th, a short list of what are to be sent.
“JT feel that Iam asking too much from you; but a knowledge of your
devotion to a science which you have so much extended, makes me feel less
diffident, and I have thrown myself upon your kindness.
“T have also to acknowledge the receipt of a Book of Instructions, &c.,
with thanks.
“ So soon as I get a reply from you, I will at once transmit the amount
with the order, and submit a plan of the building.
* Believe me to remain, with great consideration and respect,
“ Yours faithfully,
(Signed) “ C, SMALLWoop.”
* General Sabine, London.”
Instruments to meet this request are in preparation.
The Committee have thought that it might not prove uninteresting to the
members of the British Association, if, in this Report, a short description
were given of the Kew Observatory, and of the nature and amount of work
which is accomplished therein.
The Observatory is situated in the middle of the old Deer-park, Richmond,
Surrey, and is about three-quarters of a mile from the Richmond Railway
Station. Its longitude is 0° 18! 47" W., and its latitude is 51°28’ 6" N. It
is built north and south. The repose produced by its complete isolation is
eminently favourabie to scientific research. In one of the lower rooms a set
of self-recording magnetographs, described in the Report of the last meeting
of this Association, is constantly at work. ‘These instruments, by the aid of
photography, furnish a continuous record of the changes which take place in
the three magnetic elements, viz. the declination, the horizontal force, and the
vertical force. The light used is that of gas, in order to obtain which, pipes
have been carried across the Park to the Observatory, at an expense of £250,
which sum was generously defrayed by a grant from the Royal Society.
Attached to this room is another, of a smaller size, in which the necessary
photographic operations connected with magnetography are conducted.
In the story above the basement, the room by which the visitor enters the
Observatory is filled with apparatus. Much of this is the property of the
Royal Society, and some of the instruments possess a historical value; for
instance, the air-pump used by Boyle; and the convertible pendulum designed
by Captain Kater, and employed by him, and subsequently by General Sabine,
in determining the length of the pendulum vibrating seconds.
_ An inner room, which opens from this one, is used as a library and sitting-
room, and in it the calculations connected with the work of the Observatory
are performed. In this room dipping-needles and magnets, which it is neces-
sary to preserve from rust, are stored. Here also the MS. of the British
Association Catalogue of Stars is preserved.
A room to the east of this contains the standard barometers, and the appa-
xlii REPORT—1860.
ratus (described by Mr. Welsh in the ‘ Transactions’ of the Royal Society,
vol. 146. p. 507) for verifying and comparing marine barometers with the
standard. This room has also accommodation for the marine barometers
sent for verification. In the middle of the room is a solid block of masonry,
extending through the floor to the ground below. To this an astronomical
quadrant was formerly attached ; it is now used as a support for the standard
barometers. This room contains also a Photographic Barograph invented
by Mr. Francis Ronalds, which, though not at present in operation, may
serve as a model for any one who wishes to have an instrument of this
description. It is described by Mr. Ronalds in the Report of the British
Association for 1851.
In a room to the west of the Library, thermometers for the Board of Trade,
the Admiralty, and opticians, are compared with a standard thermometer by
means of a very simple apparatus devised by the late Mr. Welsh.
The Observatory also possesses a dividing-engine by Perreaux, by means of
which standard thermometers are graduated. It was purchased by a grant
from the Royal Society.
In this room the pure water required for photographic processes is obtained
by distillation; and here also a small transit telescope is placed for ascertain-
ing time. The transit instrument is erected in a line between two meridian
marks—one to the north and the other to the south of the Observatory ; so
that, by means of suitable openings, either of these marks may be viewed by
the telescope.
In a higher story is the workshop, containing, among other things, a slide-
lathe by Whitworth, and a planing machine by Armstead, both of which were
presented to the Kew Observatory by the Royal Society.
In the dome is placed the Photoheliograph for obtaining pictures of the
sun’s disk; attached to the dome there is a small chamber in which the
photographic processes connected with the photoheliograph are conducted.
This chambe 1's supplied with water by means of a force-pump. A self=
recording Robinsons anemometer jsalso attached to the dome.
In addition to the rooms now specified, there are the private apartments
attached to the Observatory.
On the north side of the Observatory there is an apparatus similar to that
used at the Toronto Observatory for containing the wet- and dry-bulb, the
maximum and the minimum thermometers.
The model magnetic house, elsewhere alluded to in this Report, stands at a
distance of about 60 yards from the Observatory ; and the small wooden
house in which the absolute magnetic observations are made, at a distance
of about 110 yards. These houses are within a wooden paling, which fences
them off from the remainder of the Park, and encloses about one acre of
ground attached to the Observatory.
The work done may now be briefly specified. In the first place, the self-
recording magnetographs, as already mentioned, are kept in constant opera-
tion, and record the changes continually occurring in the magnetic elements.
The photographs are sent to General Sabine’s establishment at Woolwich,
to undergo the processes of measurement and tabulation.
In the model magnetic house there is at present a set of magnetographs
which Dr, Bergsma will take to Java. When this set is removed another will
supply its place, in readiness for any other Observatory, colonial or foreign,
at which it may be required.
In the house for absolute determinations, monthly values of the declination,
dip, and horizontal magnetic force are taken, and magnetic instruments for
foreign or colonial observatories have their constants determined,
xiii
REPORT OF THE KEW COMMITTEE.
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xliv REPORT—1860.
In the meteorological department, all the barometers, thermometers, and
hydrometers required by the Board of Trade and the Admiralty have their
corrections determined; besides which, similar instruments are verified for
opticians. Standard thermometers also are graduated, and daily meteoro-
logical observations are made, an abstract of which is published in the
‘ Illustrated London News.’
Instruction is also given in the use of instruments to officers in the army
or navy, or other scientific men who obtain permission from the Committee.
All this amount of work, it is believed, can be executed by the present
staff, consisting of the superintendent, three assistants (magnetical, mecha-
nical, and meteorological), and a boy; but the expense attending it is greater
than the present income of the Observatory, furnished by the British Asso-
ciation, will support.
In the resolution of the British Association of the 14th September, 1859,
it was recommended to Government, at the instance of the joint committee of
the Royal Society and British Association, that the sum of £350 per annum
should be placed at the disposal of the general superintendent of the mag-
netical observations ; this sum was intended to have defrayed the expenses
attending the magnetical department of the Observatory and the observa-
tions of the sun’s spots. It will be seen, however, from the correspondence
contained in an earlier part of this Report, that this source of income is not
yet available.
Joun P. GAsstotT,
June 18, 1860. Chairman.
Report of the Parliamentary Committee to the Meeting of the British
Association at Oxford in June 1860.
The Parliamentary Committee have the honour to report as follows :—
No subject of sufficient importance to require any especial notice has occu-
pied their attention during the past year, nor indeed was there any matter
referred to them at the last Meeting of the Association.
There are now either two or three vacancies in that portion of the Com-
mittee which represents the House of Commons, according as it shall be de-
termined whether the vacancy caused in that Section by Lord de Grey’s
taking his seat in the House of Lords is or is not to be filled up,
WrottTeEsLey, Chairman.
May 28, 1860.
RECOMMENDATIONS OF THE GENERAL COMMITTEE. xly
RECOMMENDATIONS ADOPTED BY THE GENERAL COMMITTEE AT THE
Oxrorp MEETING IN JUNE AND JULY 1860.
[When Committees are appointed, the Member first named is regarded as the Secretary of
the Committee, except there be a specific nomination. ]
Involving Grants of Money.
That the sum of £500 be appropriated to the maintenance of the Esta-
blishment in Kew Observatory, under the direction of the Council.
That a sum not exceeding £90 be granted for one year for the payment
of an additional Photographer for carrying on the Photo-heliographic Ob-
servations at Kew.
That a sum not exceeding £30 be placed at the disposal of Mr. Broun,
Dr. Lloyd, and Mr. Stone, for the construction of an Induction Dip Circle,
in connexion with the Observatory at Kew.
That a sum not exceeding £10 be placed at the disposal of Professor
Tyndall and Mr. Ball, for providing Instruments fur making Observations in
the Alps, and for printing the formule for the use of travellers.
That the Balloon Ascent Committee, consisting of Prof. Walker, Prof,
W. Thomson, Sir D. Brewster, Dr. Sharpey, Dr. Lloyd, Col. Sykes, General
Sabine, and Prof. J. Forbes, be reappointed, with the addition of Mr. Broun ;
and that the sum of £200 be placed at their disposal for the purpose.
That Dr. Matthiessen be requested to prosecute his Experiments on the
Chemical Nature of Alloys; and that the sum of £20 be placed at his dis-
posal for the purpose.
That Prof. Sullivan be requested to continue his Experiments on the Solu-
bility of Salts at Temperatures above 100° Cent., and on the mutual Action
of Salts in Solution ; and that the sum of £20 be placed at his disposal for
the purpose.
That Prof. Voelcker be requested to continue his investigation on Field
Experiments and Laboratory Researches on the Constituents of Manures
essential to Cultivated Crops; and that the sum of £25 be placed at his
disposal for the purpose.
That Mr. Alphonse Gages be requested to continue his Experiments on the
Mechanico-Chemical Analysis of Minerals; and that the sum of £20 be
placed at his disposal for the purpose.
That Mr. Mallet be requested to carry on his Experiments on Earthquake
Waves ; and that the sum of £25 be placed at his disposal for the purpose.
That additional excavations be made at Dura Den by the Committee, now
consisting of Dr. Anderson, Prof. Ramsay, Prof. Nicol, and Mr. Page; that
Mr. J. B. Jukes be added to the Committee; and that the sum of £20 be
placed at their disposal for the purpose.
That Mr. J. Gwyu Jeffreys, Dr. Lukis, Mr. Spence Bate, Mr. A. Hancock,
and Dr. Verloren be a Committee for the purpose of Reporting on the best
mode of preventing the ravages of the different kinds of Teredo and other
Animals in our Ships and Harbours; that Mr. J. Gwyn Jeffreys be the
Secretary ; and that the sum of £10 be placed at their disposal for the purpose.
That Mr. Sclater, Dr. A. Giinther, and Mr. R. T. Tomes be a Committee
for the purpose of preparing and printing a Report on the Present State of
our Knowledge of the Terrestrial Vertebrata of the West India Islands ;
that Mr. Sclater be the Secretary ; and that the sum of £10 be placed at
their disposal for the purpose.
That Mr. Robert MacAndrew and the following gentlemen be a Com-
xlvi REPORT—1860.
mittee for General Dredging purposes :—Mr. R. MacAndrew, Chairman;
Mr. G. C. Hyndman, Dr. Edwards, Dr. Dickie, Mr. C. L. Stewart, Dr. Colling-
wood, Dr. Kinahan, Mr. J. S. Worthey, Mr. J. Gwyn Jeffreys, Dr. E. Perceval
Wright, Mr. Lucas Barrett, and Professor J. R. Greene. That Mr. Robert
MacAndrew be the Secretary ; and that the sum of £25 be placed at their
disposal for the purpose.
That Dr. Ogilvie, Dr. Dickie, Dr. Dyce, Prof. Nicol, and Mr. C. W. Peach
be a Committee for the purpose of Dredging the North and East Coasts
of Scotland. That Dr. Ogilvie be the Secretary ; and that the sum of £25
be placed at their disposal for the purpose.
That the surviving members of the Committee appointed in the year 1842,
viz. Mr. C. Darwin, Rev. Professor Henslow, Rev. L. Jenyns, Mr. W. Ogilby,
Professor Phillips, Sir John Richardson, Mr. J. O. Westwood, Professor Owen,
Mr. W. E. Shuckard, and Mr. G. R. Waterhouse, for the purpose of pre-
paring Rules for the establishment of a Uniform Zoological Nomenclature, be
reappointed, with the addition of Sir William Jardine, Bart., and Mr. P. L.
Sclater. That Sir W. Jardine be the Secretary ; and that the sum of £10 be
placed at their disposal for the purpose of revising and reprinting the Rules.
That Mr. Sclater and Dr. F. Hechstetter be a Committee for the purpose
of drawing up a Report on the Present State of our Knowledge of the Species
of Apteryz living in New Zealand. That Mr. Sclater be the Secretary ; and
that the sum of £50 be placed at their disposal for the purpose.
That Dr. Collingwood be requested to dredge in the Estuaries of tne
Mersey and Dee ; and that the sum of £5 be placed at his disposal for the
purpose.
That Dr. Edward Smith, F.R.S., and Mr. Milner be a Committee for the
purpose of prosecuting inquiries as to the effect of Prison Diet and Discipline
upon the Bodily Functions of Prisoners. That Dr. Edward Smith be the
Secretary; and that the sum of £20 be placed at their disposal for the
purpose.
That Mr. T. Wright, Mr. J. B. Davis, and Mr. A. G. Hindlay be a Com-
mittee for the purpose of exploring entirely the piece of ground at Uriconium
in which the human remains have been found, in order to examine more
fully the circumstances connected with the discovery, and to obtain the
similar Skulls which may still remain under ground. ‘That Mr. T. Wright
be the Secretary ; and that the sum of £20 be placed at their disposal for the
purpose.
That Professor James Thomson (of Belfast) be requested to continue his
Experiments on the Gauging of Water; and that the sum of £10 be placed
at his disposal for the purpose.
That the Committee on Steam-ship Performance be reappointed, to report
proceedings to the next Meeting ; that the attention of the Committee be
also directed to the obtaining of information respecting the performance of
vessels under Sail, with a view to comparing the results of the two powers
of Wind and Steam, in order to their most effective and economical combi-
nation ; and that the sum of £150 be placed at their disposal for this purpose.
The following gentlemen were nominated to serve on the Committee :—
Vice-Admiral Moorsom; The Marquis of Stafford, M.P.; The Earl of Caith-
ness; The Lord Dufferin; Mr. William Fairbairn, F.R.S.; Mr.J. Scott Russell,
F.R.S.; Admiral Paris, C.B.; The Hon. Captain Egerton, R.N.; Mr. William
Smith, C.E.; Mr. J. E. M¢Connell, C.E.; Prof. Rankine, LL.D.; Mr. J. R.
Napier, C.E.; Mr. R.Roberts,C.E.; Mr. Henry Wright, Honorary Secretary ;
with power to add to their number.
That Prof. Phillips be requested to complete and print, before the Man-
RECOMMENDATIONS OF THE GENERAL COMMITTEE. xlvii
chester Meeting, a Classified Index to the Transactions of the Association
from 1831 to 1860 inclusive; that he be authorized to employ, during this
period, an Assistant; and that the sum of £100 be placed at his disposal for
the purpose.
Applications for Reports and Researches.
That Mr. H. J. S. Smith be requested to continue his Report on the
Theory of Numbers.
That Mr. Cayley be requested to draw up a Report on certain Problems
in Higher Dynamics.
That Mr. B. Stewart be requested to draw up a Report on Prevost’s
Theory of Exchanges, and its recent extensions.
That Prof. Stokes be requested to draw up a Report on the Present State
and Recent Progress of Physical Optics.
That Dr. Dickie be requested to draw up a Report on the Flora of Ulster,
for the next Meeting of the Association.
That Dr. Carpenter be requested to draw up a Report on the Minute
Structure of Shells.
That Dr. Michael Foster be requested to report upon the Present State
of our Knowledge in reference to Muscular Irritability.
That Mr. James Oldham be requested to continue his Report on Steam
Navigation in the Port of Hull.
That the Lord Rosse, Dr. Robinson, Professor Phillips, and Mr. W. R. Birt
be a Committee for the purpose of making observations on the Moon’s sur-
face and comparing it with that of the Earth. That Professor Phillips be the
Secretary.
That the Rev. Professor Price, Dr. Whewell, Sir J. Lubbock, Admiral
FitzRoy, Sir W. S. Harris, and Rey. Professor Haughton be a Committee for
the purpose of reporting to the next Meeting of the British Association, on
the Expediency and best means of making Tidal Observations, with a view
to the completion of Dr. Whewell’s Essays in prosecution of a full Tidal
Exposition.
That, as it would be highly desirable that the observations on the Magnetic
Lines in India should be continued, His Highness The Rajah of Travancore
be requested to complete the Survey already commenced by him, through
his Astronomer.
That it is desirable that a Committee be appointed to consider the best
mode of effecting the registration and publication of the numerical facts of
Chemistry. That the Committee consist of Dr. Frankland, Dr. W. A. Miller,
Prof. W. H. Miller, Prof. Brodie, Prof. Williamson, and Dr. Lyon Playfair.
That the Lords of the Admiralty be moved to authorize some small vessel
stationed on the South-East Coast of America to take a convenient oppor-
tunity of collecting specimens of the large Vertebrate Fossils from certain
localities easy of access between the River Plata and the Straits of
Magellan.
That Sir W. Jardine, Bart., Prof. Owen, Prof. Faraday, and Mr. Andrew
Murray be a Committee for the purpose of procuring information as to the
best means of conveying Electrical Fishes alive to Europe. That Sir W.
Jardine be the Secretary.
That Mr. William Fairbairn, Mr. J. F. Bateman, and Prof. Thomson be a
Committee for .the purpose cf reporting on Experiments to be made at the
Manchester Waterworks on the Gauging of Water; with power to add to
their number.
xl vill REPORT—1860.
That the Committee to report on the Rise and Progress of Steam Naviga-
tion in the Port of London be reappointed, and that the following gentlemen
be requested to serve on it:—Mr. William Smith, C.E.; Sir John Rennie,
F.R.S.; Captain Sir Edward Belcher; Mr. George Rennie, F.R.S.; Mr. Henry
Wright, Secretary ; with power to add to their number.
Involving Applications ta Government or Public Institutions.
That the Parliamentary Committee, now consisting of the Duke of Argy!!.
Dake of Devonshire, Earl de Grey, Lord Enniskillen, Lord Harrowby.’
Lord Rosse, Lord Stanley, Lord Wrottesley, Bishop of Oxford, Sir Philip
Egerton, Sir John Packington, be requested to recommend two members of
the House of Commons to fill the two vacancies.
That Sir Roderick I. Murchison, as Trustee of the Association, and Mr.
Nassau W. Senior, as President of the Section of Economie Science and Sta-
tistics, be a Delegacy for the purpose of attending the International Sta-
tistical Congress in London on July 16.
That the Committee on Steam-ship Performance be requested to commu-
nicate with the Parliamentary Committee, for the purpose of obtaining their
assistance in accomplishing the objects for which the Committee on Steam-
ships was appointed.
Communications to be printed entire among the Reports.
That the Communications by the Rev. W. V. Harcourt, on the results of
Experiments at the Low Moor Iron Works, be printed entire among the
Reports of the Association.
That Mr. William Fairbairn’s Paper, on Experiments to determine the
effect of vibratory action and long-continued changes ef load upon Wrought-
iron Girders, be printed entire in the Reports of the Association.
That Admiral Moorsom’s Paper, on the Performance of Steam Vessels,
be printed entire among the Reports.
That Mr. Elder’s Paper, on a cylindrical spiral boiler, with comparative
evaporating power and temperatures of furnaces, flues and chimneys of
various boilers, be printed entire in the Transactions of the Sections, with
the necessary diagrams.
Synopsis of Grants of Money appropriated to Scientific Objects by the
General Committee at the Oxford Meeting in June and July 1860,
with the name of the Member, who alone, or as the First of a Com-
mittee, is entitled to draw for the Money.
Kew Observatory. pee oe Da
Kew Observatory Establishment ......... a Sth nie Sand Se nt OO ee
Mathematical and Physical Science.
Photo-heliographic Observations at Kew... .. eee. cece nece 90 0 O
TYNDALL and Bati.—Alpine Ascents ........ eeeese008 10 0 O
Carried forward i .% ccs cave cele vetenree alana 600 1) )
RECOMMENDATIONS OF THE GENERAL COMMITTEE,
£
OOS i 2 es eee ere 600
Balloon Committee ...... Li wee =e eer ye peme 0,0)
Broun and Committee. —Dip- Bletlogh PA MEE cus sas 30
Chemical Science, including Mineralogy.
Marruatessen, Dr.—Chemical Alloys...........0 00.0 ee oe 20
SuLtivan, Professor.—Solubility of Salts ............ meeps. 20
VoeEtcker, Professor.—Constituents of Manures .......... 23
Gaces, ALpHonse.—Chemistry of Rocks and Minerals .... 20
Geology.
Matter, Rosertr.— Earthquake Observations ............ 25
Committee.—Excavations at Dura Den ..........00...+22 20
Zoology and Botany.
Jerrreys, J. G., and Committee—Ravages of Teredo and
EMMI SISSY a 2 OND Pc deo ky 16 oA laid. ciara. bid'g/e 10
Scrater, P. L., and Committee.—Report on Terrestrial Verte-
brata of West PCS ae eee deals Sars mane bo Re es 10
MacAnprew, R., and Committee.—For General Dredging .. 25
Ocitvix, Dr., id Committee—Dredging the North and Rast
Coasts of Scotland . eran 25
JARDINE, Sir W., Bane mad Ooninilece. Revising iid Ret
printing Rules of Zoological Nomenclature.............. 10
ScLArEn, P: L.—Investigation of Apteryx..... sneha ie 50
CoLiinewoop, Dr —Dredging i in Mersey aud: Dee, ss salt 5
Physiology.
Dr. Epwarp Smiru, F.R.S., and Mr. Mitner.—Effect of
Prison Diet and Discipline upon the bodily functions of
BN fe oh Pia Sool oh c'g'a’s sie, nce Cb rece eeveeeweene phatase
Geography and Ethnology.
Committee for exploring Uriconium...............-. sacs e 0)
& Mechanical Science.
Tuomsoy, Professor J.—Gauging of Water .......... 0008 10
Committee on Steam-Ship Performance ......+.-... 0.0. 150
Classified Index to the Transactions.
Professor Patties (to employ an Assistant) ...........00+ 100
Total,... £1395 O O
xlix
coooc
oo
Ores oso i=)
0
coos
cook
oosco
oo
OCS Osco 6S
(6)
1860. d
REPORT—1860.
General Statement of Sums which have been paid on Account of Grants for
Scientifie Purposes.
i 8s, - de £ 3. d.
1834. Meteorology and Subterranean
Tide Discussions ....escscceseeee 20 0 0 Temperature .......0ssssesceee ee 0
1835 Vitrification Experiments........ ot) Ard
Tide Di : y 62 0 0 Cast Iron Experiments...........+ 100 0 0
Bete ce NS aiedeatnen se rar tyes Ae Railway Constants ....+.+0+... ses 28
British Fossil Ichthyology .....- 10570) 70 Tid’ ond Sen Revel Ce agreed
£167 0 0 | Steam-vessels’ Engines..,...- sees LOO. 20) 0
1836 Stars in Histoire Céleste ...... .. 331 18 6
F : : Stars in Lacaille .......00.....0 soe wile Way
Tide Discussions .........seesesees 163 0 0 Stars in BOATS Gataleous 616 6
British Fossil Ichthyology ...... 105) 0, ON ieee a apart BUS eaaies 10 10 0
Thermometric Observations, &c. 50 0 0 Steamtonwines in Gordan ee 50 0 0
Seba on Jong-continued 171.0 Atmospheric Air .........+0008 ee U6) Seg
Rain Gauges ...ccesececeeeeees ccveee 913 0 by pH ete nies its . . :
apenas fe ee Seep hs Cea Gases on Solar Spectrum ......... 22.0 0
unar Nutation........-scee Poses OO MEO Ss (0 Hourly M lomenl On
Thermometers . SCALE EC og, alii) ourly Breleoro On et ee
aancneu sees Zucit |p es eS, and Kingussie es :
OSS] Reptiles ..scscececcevereereee
1837. Mining Statistics ........s000se000. 50 0 0
Tide Discussions ....s..sseesesseee 284 1 O £1595 11.0
Chemical Constants ....--...++ aes Met an G
Tiunar Nutation\ ccccstrspostessenes 70 0 0 1840.
Observations on Waves.........00+ 100 12 0 | Bristol Tides..........6. eeeves asaare L000) 70
Tides at Bristol...cccccceccccccceces 150 © © | Subterranean Temperature ...... 13 13 6
Meteorology and Subterranean Heart Experiments ,...0...s.s0008 18 19L
Temperature ....scccccessssceeers 89 5 3 | Lungs Experiments ......+++.40 » 813 0
Vitrification Experiments....... .. 150 0 0 | Tide Discussions .........++++94 + 50 0 0
Heart Experiments .........0eesee 8 4 6 | Land and Sea Level............44 Vim Ui Sl
Barometric Observations ......... 30 0 0 | Stars (Histoire Céleste) ......... 242 10 0
IBALOMELETS Wavsesoeyoscsssescei se .» 11:18 6 | Stars (Lacaille) ......... COROCR 30 -» 415 0
Bs Stars (Catalogue) ........006 weseacw 264 0 0
eats 1438 Tae = ciseuesecs ececvevemn elo iO
1838. Water on Iron .,....... anpupee eke eee 0: “10'-V6
Tide Discussions ....ss...e0+8 eecse 29 © 0 | Heat on Organic Bodies ...... over! 0, De 20
British Fossil Fishes ....... ses. 100 0 0 | Meteorological Observations...... 52 17 6
Meteorological Observations and Foreign Scientific Memoirs ...... 1921.6
Anemometer (construction)... 100 0 0 Working Population rest eee eeeee ees 100 0 0
Cast Iron (Strength of) ...... wee 60 0 0 | School Statistics......ceeeeseerees ope at
Animal and Vegetable Substances Forms of Vessels steeteeeeeeeeeenes 184 7 0
(Preservation of) .......4. vateed 19 1 10 | Chemical and Electrical Pheno-
Railway Constants ......... be 41 12 10 MENA . uc escececesecstesecesencescsn 40 0 0
Bristol Tides .....sssseeeceeeeseereee 50 0 0 | Meteorological Observations at
Growth of Plants ..... Re amen iene) Plymouth) ccescecsenss a exe ssenetens OOO
Mudein URivers: csecssceecsentescevee 3 6 6 | Magnetical Observations ...,.,... 185 13 9
Education Committee .......... 50 0 0 £1546 16 4
Heart Experiments ............... 5 38 O ————
Land and Sea Level............0+ 267 8 7 1841.
Subterranean Temperature ...... 8 6 0 | Observations on Waves...... seeeoO ONO
Steam-vessels.........ses00+ cectecees 100 0 0O| Meteorology and Subterranean ‘
Meteorological Committee ...... Sp MOL Teel Temperature .......ssessees oe 882-0
‘RHEYMIOMELErS iesassasessereasspanss 16 4 0 | Actinometers......ecssccssesseess 10 0 0
£956 12 2 Earthquake Shocks .........scs0e 17 of eae,
Se | Acrid Poisons...........0005 on siswiewa ~ 162 000
1839. Veins and Absorbents .........4. - 38 0 0
Fossil Ichthyology......... seve sates nl LOM OlaO VINTEC A GEUIVEES uneeesece ee acceses on 5. 0670
Meteorological Observations at Marine Zoology.....sssseeesecees sos elie 2emrs
Ply mottthiveecsae’eseesere eee sorte) 60010) 10))'SkeletonMapsi \.c.-..-nssc0seckeed a. 20% 02°10
Mechanism of Waves ..........4- 144 2 0) Mountain Barometers ........... 5 GDL SiG
Bristol Tides .....se.ssseeseseeseeeee 35 18 6 | Stars (Histoire Céleste)........0+ 185 0 0
GENERAL STATEMENT.
; 5 C5 aC
Beare (Uacpille)Gosesecsscescsseecees 79 SB 10
Stars (Nomenclature of) ......... 17. 19-.6
Stars (Catalogue of) ...........0008 40 0 0
eet ON) LOM esse kecescussesess as 50 0 0
Meteorological Observations at
DBEMRESS Eo npeccy ceccserensses tect 20 0 0
Meteorological Observations (re-
duction of) ..... miihspisesste sees 25> 7.0090
Hossil Reptiles .......0..sessoseees we 504 0710
Foreign Memoirs ..... Pseanes noses en O2ee0e G
Railway Sections .......... eeResia 38 1 6
Forms of Vessels ......0++.. Beesess 1938 12 0
Meteorological Observations at
EVTATOY Cll nays ceeeeyscre renee sss 55 0 0
Magnetical Observations ......... 6118 8
Fishes of the Old Red Sandstone 100 0 0
Tides at Leith ...... Eabgasnss seats 50 0 0
Anemometer at Edinburgh ...... 69 1 10
Tabulating Observations ......... 96.33
Races of Men ....,..e0008 ero, ye Oe
Radiate Animals ............ oye OLS 0
£1235 10 11
1842,
Dynamometric Instruments ..,... 113 Ll 2
Anoplura Britannie .....,. Aneta es Wee a
Tides at Bristol............+6+ AAO Re Oe) ea
Gases on Light..... Saracen ease oF BULA OF
Chronometers ........... areanenaer 2help. (6
Marine Zoology..........000+ recat wl aT RL,
British Fossil Mammalia ....,.... 100 0 0
Statistics of Education ........... Fie ZA eeel eat
Marine Steam-vessels’ Engines... 28 0 0
Stars (Histoire Céleste)............ 59 0 0
Stars (Brit. Assoc. Cat. of) ...... 110 0 0
Railway Sections .........sss000... 161 10 0
British Belemnites...... “cohecocdcd 50 0 0
Fossil Reptiles (publication of
Report) .....,... Re eesee Shalt eld 0.40
Forms of Vessels .........0 aon ses 180 0 0
Galvanic Experiments on Rocks 5 8 6
Meteorological Experiments at
HAIGANIOUEN! 55 50¢.20rersccores ah 68 0 0
Constant Indicator and Dynamo-
metric Instruments ....... “oe LD UMD
Force of Wind ............ cvececses 10 0 0
Light on Growth of Seeds ...... ree MEL
REAUSTALISLICS cayi..cssscesccesess fe D0 10-0
Vegetative Power of Seeds ...... 8 1 11
Questions on Human Race ...... 7
£19 178
1843.
Revision of the Nomenclature of
DETTE esse ccece sce RasedaTecsienne 6 Ate a
Reduction of Stars, British Asso-
ciation Catalogue ............00. 25 0 0
Anomalous Tides, Frith of Forth 120 0 0
Hourly Meteorological Observa-
tionsat KingussieandInverness 77 12 8
Meteorological Observations at
MEP DOEN spaces eGeecwcsvieces ee dp” TOA
Whewell’s Meteorological Ane-
mometer at Plymouth .,....... 10 0 0
Ge ons
Meteorological Observations, Os-
ler’s Anemometer at Plymouth 20 0 0
Reduction of Meteorological Ob-
SET VAtLONS Mew. .ssescecsecavenies we 30 0 0
Meteorological Instruments and
Gratuities Brceseujssesnseeiereetase Be Gi
Construction of Anemometer at
Inverness ....00+0- teeeeeeeeresens 5612 2
Magnetic Co-operation ,,.......... 10 8 10
Meteorological Recorder for Kew
Observatory .......s000 ssesensvee 00 0 O
Action of Gases on Light . eeseeece 18 16 1
Establishment at Kew Observa-
tory, Wages, Repairs, Furni-
ture and Sundries ..........+5.06 1338 4 7
Experiments by Captive Balloons 81 8 0
Oxidation of the Railsof Railways 20 0 0
Publication of Report on Fossil
Reptiles .......+ Piereeousiscuseseey 40 0 0
Coloured Drawings of Railway
NEEHONSepewansarssasaveeersaresss 147 18 3
Registration of Earthquake
Shocks ...... aaRevesesesesathesers 30 0 0
Report on Zoological Nomencla-
tC Mises css on aspen snes bene® vores) 110/07 0
Uncovering Lower Red Sand-
stone near Manchester ......... 4 4 6
Vegetative Power of Seeds ..... 5 3 8
Marine Testacea (Habits of) ... 10 0 O
Marine Zoology.....sssssseeees siege LDUGIES
Marine Zoology....es.sseeceeseerace 2 14 11
Preparation of*Report on British
Fossil Mammalia .........00s.. - 100 0 0
Physiological Operations of Me-
dizinal:Agents si,cccsxesssorssse 120) 0) 0
Vital Statistics ......sse.00 paeeecgs ND) ea
Additional Experiments on the
Horms:of Vesselsipeversssensses0 0 100 Ou 2
Additional Experiments on the
Forms of Vessels ....0s.ssss+000 100 0 0
Reduction of Experiments on the
Forms of Vessels ....ssseessee0s 100 0 0
Morin’s Instrument and Constant
Indicatot) seesse sake nestsaasasane ~» ) 628).14, 10
Experiments on the Strength of
Materials; po.esseressae BOcrecsecrem. 0) et MT
£1565 10 2
1844.
Meteorological Observations at
Kingussie and Inverness ...... 12 0 0
Completing Observations at Ply-
WAGUUG) wateyentenaaesercscaseses eon Ol 10
Magnetic and Meteorological Co-
OPETAUON Wasahaceescgscreeeesan - 25 8 4
Publication of the British Asso-
ciation Catalogue of Stars...... 35 0 0
Observations on Tides on the
East coast of Scotland ......... 100 0 0
Revision of the Nomenclature of
SEATS cans vecsacnetenn se sesexs 1842 2 9 6
Maintaining the Establishment in
Kew Observatory ......0...00 117 17 3
Instruments for Kew Observatory 56 7 3
d2
lii REPORT—1860.
a) ERAGE £ os. d.
Influence of Light on Plants...... 10 0 0) Fossil Fishes of the London Clay 100 0 0
Subterraneous Temperature in Computation of the Gaussian
Treland) Wewerssadaessccestasstaee 5 0 0 Constants for 1839.......04+ sneer DORE OO
Coloured Drawings of Railway Maintaining the Establishment at
Sectionsineciscesocs teste dieorm esse 15 17 6 Kew Observatory ...scosseseeee . 146 16 7
Investigation of Fossil Fishes of Strength of Materials....., asesyesns OO MO haO
the Lower Tertiary Strata 100 0 0} Researches in Asphyxia........04- OP liGee
Registering the Shocks of Earth- Examination of Fossil Shells...... 10 0 0
CUUAIOS eine steels sslelvsisis cin ve 1842 23 11 10 | Vitality of Seeds .........00- 1844 2 15 10
Structure of Fossil Shells ......... 20 0 0 | Vitality of Seeds ...,...0.... 1845 712 3
Radiata and Mollusca of the Marine Zoology of Cornwall,..... 10 0 0
ZSgean and Red Seas.....1842 100 0 0 | Marine Zoology of Britain ...... 10 0 0
Geographical Distributions of Exotic Anoplura .secoe.eee 1844 25 0 0
Marine Zoology........+++ 1842 010 0} Expensesattending Anemometers 11 7 6
Marine Zoology of Devon and Anemometers’ Repairs ....++.. aod) 2 HOreEO
Cornwall ........ssesesvevecesees 10 0 0} Atmospheric Waves .......se0ee.0e 3.3 3
Marine Zoology of Corfu sesinees -«- 10 0 0) Captive Balloons ....... «1844 8S 19 3
Experiments on the Vitality of Varieties of the Human Race
GEUSlamecaaactcuusessiedsseseveddees 9 0 3 1844 7 6 38
Experiments on the Vitality of Statistics of Sickness and Mor-
Seedseetnecdiirarseterssaccecl GA eimOlr ot) oO tality in York ..,cccsscscensssase sla On 10
Exotic Anoplura ......cssss0e0ce aetholion +10" 40 Fe685 1610)
Strength of Materials .......... 100 0 0 ———— eee
Completing Experiments on the
Forms of Ships .....seeesereeeeee 100 0 0 : 1847. f
Inquiries into Asphyxia ......... 10 0 0 | Computation of the Gaussian
Investigations on the Internal So for 1882) RSS rorene 50 OOM
Constitution of Metals ......... 50.0 ' 0 | Habits ee Sas sssaon 10 ae
Gonctanuelidicatociandanioun's Physiological Action of Medicines 20 0 0
Instrument, 1842 ...esseseeeee D0: 5 | eamne: Zeolasyol ComirallT an eae
2 me i Ca Atmospheric Waves «sss... Peer ie Rs
TSE ess MVatalityan SCCds. z.osedscnsensenees 4 7 7
1845. Maintaining the Establishment at
Publication of the British Associa- Kew Observatory svrsseeeseere 107 8 6
tion Catalogue of Stars ....... 851 14 6 £208 5 4
Meteorological Observations at
Inverness ..... Sponpdoggcd: itacse’ 80.18 11 1848.
Magnetic and Meteorological Co- Maintaining the Establishment at
Operation... oe reneecenes vee 1616 8 Kew Observatory ssesssecessaees 171 15 11
Meteorological Instruments at Atmospheric Waves ..sseesessees oot OS HORCS
Edinburgh ....sccsvseees ieeneeaee 18 11 9] Vitality of Seeds ......ss00008 vat Da NO
Reduction of Anemometrical Ob- Completion of Catalogues of Stars 70 0 0
servations at Plymouth ........ 25 0 07} On Colouring Matters v.00. 5 0 0
Electrical Experiments at Kew On Growth of Plants........0000.-- 15 0 O
ObservatOry ...cecresssscseceass a AGL 28 £275.18
Maintaining the Hatablishtacatn in ———
Kew Observatory aeaesaiaeemanes » 149 15. 0
For Kreil’s Barometrograph ...... 25 000 F 1849,
Gases from Iron Furnaces ...... 50 0 0 | Electrical Observations at Kew
The Actinograph ....csscsessreeees ils ete Observatory sae eoy sents ousiccaniiey OO IO mel
Microscopic Structure of Shells... 20 0 0 Maintaining Establishment at
Exotic Anoplura s.sseecsee 1843 10 0 0 ditto serene aemieaitabicioie sists cosa) OMS
Vitality of Seeds.....sssseesee 1843. 2 0 7 | Vitality of Seeds ws seeseees amu Brae
Vitality of Seeds ...seeseeeee 1844 7 0 0 | OuGrowth of Plants..........+0+ 5 0 0
Marine Zoology of Cornwall...... 10 0 | Registration of Periodical Phe-
Physiological Action of Medicines 20 0 0 MOMENA seeeesseeseeneerserenee sees 10 0 0
Statistics. of Sickness and More Bill on account of Anemometrical
talitysin) York csstsspeeeeeeee 20 0 O| Observations ......... seeeeeweeens 139 0
Earthquake Shocks ....... 1843 15 14 8 £159 19 6
£330 9 9
— 1850.
1846. Maintaining the Establishment at
British Association Catalogue of Kew Observatory ........ secesee 200 18 0
Stars vsessceeevevsveveerereeet844 211 15 0 | Transit of Earthquake Wayes,.. 50 0 0
GENERAL STATEMENT,
ase es
Periodical Phenomena .,.,........ 15 0 0
Meteorological Instrument,
AZOLES wesseseesceecsseenvenscears 2hmei0L. 0
£345 18 0
1851.
Maintaining the Establishment at
Kew Observatory (includes part
of grantin 1849) .........ce0e0 309 2 2
Theory of Heat ..........s0cee0 foe Pe MEA
Periodical Phenomena of Animals
MUDECIAUIES cy adaeseccccaseceacvece 5 0 0
Vitality of Seeds ....cc.scsscereee 5 6 4
Influence of Solar Radiation.,..... 30 0 0
Ethnological Inquiries ..,......... 12 0 0
Researches on Annelida ......... 10 0 0
£391 9 7
1852,
Maintaining the Establishment at
Kew Observatory (including
balance of grant for 1850) ... 233 17 8
Experiments on the Conduction
PRMETEAC Tcadens nas -<ssescencas one. Lee
Influence of Solar Radiations ... 20 0 0
Geological Map of Ireland ..... Sapa Ol. 0
Researches on the British Anne-
11 Oca Ieeee Pree coresasn cece sdavseae £02.00 1'0
Vitality of Seeds ........ ceacncvees 10 6 2
Strength of Boiler Plates ......... Gi 10500
£304 6 7
1853.
Maintaining the Establishment at
Kew Observatory ..... “acbcknnee 165 0 0
Experiments on the Influence of
Solar Radiation............0.08. 15 0 0
Researches on the British Anne-
RS Eart tama seis Sia nce sis vsldelass op aieeids 10 0 0
Dredging on the East Coast of
EHUAN Gs cccycscesnosascetcesecosee 10)), 0,40
Ethnological Queries ....... crea PL oy, Oigi0
£205 0 0
1854,
Maintaining the Establishment at
Kew Observatory (including
balance of former grant) ...... 330 15 4
Investigations on Flax ..........+8 11 0 0
Effects of Temperature on
Wrought Iron . .3..-..00000. eset OS r OL. 0
Registration of Periodical Pha-
nomena ...., e'elele nial sinisalelselo'si'e seo lO Om 0
British Annelida .............00006 10 0 0
Watalityrol Seeds) ..:.csscssese.+0 itu, io
Conduction of Heat ............... 4 2 0
£380 19 7
1855.
Maintaining the Establishment at
Kew Observatory ...........2... 425 0 0
Earthquake Movements ........ oe OREO 0
Physical Aspect of the Moon...... 11 8 5
Vitality of Seeds ............40. -- 10 7 11
Mamonthe World.,...s.<c0s.00s 15 0 0
Ethuological Queries ...... caceen Siento)
Dredging near Belfast .4........ 4 0 0
£480 16 4
iti
& s d.
1856.
Maintaining the Establishment at
Kew Observatory :-—
1854.....£ 75 0 0
1855......£500 0 i: oer 88
Strickland’s Ornithological Syno-
TY MS cseclese pacha ae wamtandudanes vos 100 0.0
Dredging and Dredging Forms... 913 9
Chemical Action of Light........ 20 0 0
Strength of Iron Plates............ 10 0 0
Registration of Periodical Pheno-
MMETA® waecleshenseaxeeee abi Beade ses 10 0 0
Propagation of Salmon .seseeeeeee 10 0 0
£754 13 9
1857.
Maintaining the Establishment at
Kew Observatory sescsesesesees . 350 0 0
Earthquake Wave Experiments 40 0 0
Dredging near Belfast ....... seeicny item Onn O
Dredging on the West Coast of
Scotland......... tessa devsiciiasa 450 UA Ae
Investigations into the Mollusca
of California ......... caevacenoens 10 0 0
Experiments on Flax ........... 5 0 O
Natural History of Madagascar.. 20 0 O
Researches on British Annelida 25 0 0
Report on Natural Products im-
ported into Liverpool ......... 10 0 0
Artificial Propagation of Salmon 10 0 0
Temperature of Mines ,.,... spa a me,
Thermometers. for Subterranean
Observations .esccessssseees Gearee (MeOE, nia’
Hife=B0dtsisrsssscecnncscadscrescssnestan (01 m0n 0
£507 15 4
1858.
Maintaining the Establishment at
Kew Observatory ........ sesease 000 0
Earthquake Wave Experiments.. 25 0
Dredging on the West Coast of
Scotland — cevseressveveceees ida es 10 0 0
Dredging near Dublin ........-.. AEC a
Vitality of Seeds” ect ieccssseceee 5 5 0
Dredging near Belfast ....+....40. 18 13 2
Report on the British Annelida... 25 0 O
Experiments on the production
of Heat by Motion in Fluids... 20 0 0
Report on the Natural Products
imported into Scotland......... 10 0 0
£518 18 2
1859.
Maintaining the Establishment at
Kew Observatory ....+666 peeeessie O00 MeiOm nO
Dredging near Dublin ..........46 15 0 0
Osteology of Birds,......ssseseseree 50 0 0
Trish Tunicata .....c.cscecsssesenes 5 0 OU
Manure Experiments ......00+.0s 20 0 0
British Medusid@ ...........se0e00e Sy 0220)
Dredging Committee.......... aceboy Wa
Steam Vessels’ Performance...... 5 0 0
Marine Fauna of South and West
Of Ireland ieecsncsnescave ss eaaesure 19 0 0
Photographic Chemistry ......... 10 0 0
Lanarkshire Fossils ....e..s.066 20 0
Balloon’ AscentS.:cssjscrssseoeserees 09 11 1
£684 11 1
—_————EEEe
liv REPORT—1860.
1860. & s. d, & s. d.
Maintaining the Establishment Researches on the Growth of
of Kew Observatory ..........+0. S00 HO". 0 PJGWts. vscacee-.dacteccesveeteancede 10 0 0
Dredging near Belfast..........++ 16 6 0 | Researches on the Solubility of
Dredging in Dublin Bay........... 15 0 0 DHIES=sOistrassssuees-yscsomstersated 30 0 0
Inquiry into the Performance of Researches on the Constituents
Steam -vessels...csceseccseseseeeee 124 0 0 Of Manures ..........-csoceesvesoss 25 0 0
Explorations in the Yellow Sand- Balance of Captive Balloon Ac-
stone of Dura Den...........0066 20 0 O COUNES, .ccocsccvccscsccnssescocesers 113 6
Chemico-mechanical Analysis of $1241 7 0
Rocks and Minerals........s0+++ 25 0 0 areca!
Extracts from Resolutions of the General Committee.
Committees and individuals, to whom grants of money for scientific pur-
poses have been entrusted, are required to present to each following meeting
of the Association a Report of the progress which has been made; with a
statement of the sums which have been expended, and the balance which re-
mains disposable on each grant.
Grants of pecuniary aid for scientific purposes from the funds of the Asso-
ciation expire at the ensuing meeting, unless it shall appear by a Report that
the Recommendations have been acted on, or a continuation of them be
ordered by the General Committee.
In each Committee, the Member first named is the person entitled to call
on the Treasurer, John Taylor, Esq., 6 Queen Street Place, Upper Thames
Street, London, for such portion of the sum granted as may from time to
time be required.
In grants of money to Committees, the Association does not contemplate
the payment of personal expenses to the members.
In all cases where additional grants of money are made for the continua-
tion of Researches at the cost of the Association, the sum named shall be
deemed to include, as a part of the amount, the specified balance which may
remain unpaid on the former grant for the same object.
General Meetings.
On Wednesday, June 27, at 4 p.m., in the Sheldonian Theatre, His Royal
Highness, the Prince Consort, resigned the office of President to The Lord
Wrottesley, F.R.S., who took the Chair and delivered an Address, for which
see page lv.
On Thursday Evening, June 28, at 85 p.M., a Conversazione took place in
the University Museum.
On Friday Afternoon, June 29, at 4 p.m., in the Sheldonian Theatre, the
Rev. Professor Walker, F.R.S., delivered a Discourse on the Physical Con-
stitution of the Sun.
On Friday Evening, the University Museum was opened for a Soirée with
Experiments.
On Monday Afternoon, July 2, at 2 p.m., in the Sheldonian Theatre,
Captain Sherard Osborn, R.N., delivered a Discourse on Arctic Discovery.
On Monday Evening, at 8} pP.m., a Conversazione took place in the
University Museum.
On Tuesday Evening, July 3, at 8} p.m., the University Museum was
opened for a Soirée with Microscopes.
On Wednesday, July 4, at 3 p.m., the concluding General Meeting took
place in the Sheldonian Theatre, when the Proceedings of the General Com-
mittee, and the Grants of Money for Scientific purposes, were explained to
the Members.
The Meeting was then adjourned to Manchester*.
* The Meeting is appointed to take place on Wednesday, the 4th of September, 1861.
ADDRESS
BY
THE RIGHT HON. THE LORD WROTTESLEY.
GENTLEMEN,—If, on taking this Chair for the first time as your President,
I do not enlarge upon my deficiencies for adequately filling the responsible
office to which you have done me the honour to elect me, I hope you will
believe that I am not the less sensible of them.
Your last Meeting was held under the Presidency of one not more distin-
guished by his high rank and exalted station than by his many excellent
qualities, and the discriminating interest which he has ever manifested in the
promotion of Art and Science. It was one of the most successful Meetings on
record.
We are now once more assembled in this ancient and venerable seat of
learning ; and the first topic of interest which presents itself to me, who owe
to Oxford what academic training I have received, is the contrast presented
by the state of Science and the teaching of Science in this University in the
Autuinn of the year 1814, when my residence here commenced, and for five
years alterwards, with its present condition. As the private pupil of the late
Dr. Kidd, and within a few yards of the spot from which I have now the honour
to inaugurate the Meeting of this distinguished Association, I first imbibed
that love of Science from which some of the purest pleasures of my life have
been derived ; and I cannot mention the name of my former Tutor without
acknowledging the deep debt of gratitude I owe to the memory of that able,
conscientious and single-hearted man.
It was at this period that a small knot of Geologists, headed by Broderip,
Buckland, the two Conybeares and Kidd, had begun to stimulate the curiosity
of the Students and resident Graduates by Lectures and Geological excur-
sions in the neighbourhood of this town. The lively illustrations of Buck-
land, combined with genuine talent, by degrees attracted crowds to his
teaching, and the foundations of that interesting science, already advancing
under the illustrious Cuvier in France, and destinedsoon to spread over Europe,
were at this time fairly laid in England within these classical Halls. Many
atime in those days have my studies been agreeably interrupted by the
lvi REPORT—1860.
cheerful laugh which invariably accompanied the quaint and witty terms in
which Buckland usually announced to his brother Geologist some new dis-
covery, or illustrated the facts and principles of his favourite science. At
the time, however, to which I refer, the study of physical science was chiefly
confined to a somewhat scanty attendance on the Chemical Lectures of Dr.
Kidd, and on those on Experimental Philosophy by Rigaud; and in pure
mathematics the fluxional notation still kept its ground. In the year 1818
Vince’s Astronomy, and in the following year the Differential Notation, was first
introduced in the mathematical examinations for honours. At that time
that fine foundation the Radcliffe Observatory was wholly inactive; the
observer was in declining health, and the establishment was neither useful to
astronomical students, nor did it contribute in any way to the advancement
of Astronomical Science. Even from the commencement of the present
century, and in proportion as the standard of acquirement in classical learning
was gradually raised by the emulation excited by the examinations for
honours, the attendance on the above-mentioned Lectures gradually declined :
but a similar cause enhanced the acquirements of students in pure and
applied Mathematics, and the University began to number among its
Graduates and Professors men of great eminence in those departments of
knowledge. Nor were the other sciences neglected ; and as Chairs became
vacant or new Professorships were established, men of European reputation
were appointed to fill them. In proof of all this I need only direct. atten-
tion to the names on the roll of Secretaries, Vice-Presidents and Presidents
of Sections, to convince you that Oxford now contains among her resident
Graduates, men amply qualified to establish and advance the scientific fame
of that University, of which they are the distinguished ornaments.
On the progress of Astronomy I will, as becomes me, enter into more
detail, And it is not without pain that I allude to this subject, because I am
reminded that one has been removed from among us by the hand of death,
whom I had looked forward to meeting again on this occasion with peculiar
pleasure. I never knew any one who had the interests of science more truly
at heart, or laboured more diligently to advance them, than the late Radcliffe
Observer, Mr. Manuel Johnson. ; By his exertions and indefatigable zeal
the Radcliffe Observatory was enabled.to take its proper place among the
Scientific Institutions of the world. By the liberality of the Trustees and
by the exertion of his influence, new instruments were purchased, and an
extensive series of valuable astronomical observations was made; and, what
is quite as important, they were regularly reduced and published. In addi-
tion to all this, a noble array of self-recording meteorological instruments was
brought into action, and their records duly reduced and co-ordinated. I was
nyself a candidate in 1839 for that office to which Mr. Johnson was then
appointed, and I have often rejoiced that I was not successful, as it would
have retarded for a time the promotion of one, to whom Astronomy owes a
deep debt of gratitude. Mr. Johnson was suddenly taken from us at a time
ADDRESS. vii
when he was in the full career of his useful labours, and there are few
Jabourers in science whose loss has been more deplored. The University has
very lately lost another learned Professor, and myself another valued friend,
whose contributions to science are well known and duly esteemed. The
great tragic Poet of Greece introduces his hero accusing his heathen gods
of rescuing from the grave the vile and worthless, and sending thither the
good and useful :—
seers TH OG Oikata Kal Ta xpnoTa
amrooréAXovaty aéi.
Our purer faith in meek resignation trusts that they are removed from evil
to come, and that there at least they rest from their labours—rest from
earthly toil and trouble, but awake, may be, to higher aims and aspirations,
and with nobler faculties and duties.
Although a successor may be appointed to Mr. Johnson, who will, I doubt
not, admirably discharge the duties of Radcliffe Observer, I fear that the
Observatory may not continue to maintain its high reputation, unless a suffi-
cient staff of Assistants be appointed to aid the Observer in his labours.
There is no mistake more fatal in Astronomy than that of multiplying in-
strumental means without providing an adequate supply of hands to employ
them.
I have already alluded to some particulars in which this great University
has advanced in the career of scientific improvement, but everything else has
been somewhat thrown into the shade by the important event of this year,
the opening of the new Museum. The University could have given no more
substantial proof of a sincere interest in the diffusion of science than the
foundation of this noble Institution, and I am sure that among the distin-
guished cultivators of science here assembled, there is not one who does not
entertain a hearty desire for the success of the various effurts now in progress
for the purpose of stimulating our University Students to a closer contempla-
tion and more diligent study of the gloricus works of Nature; a study, which,
if prosecuted earnestly, raises us in the scale of human beings and improves
every moral and intellectual faculty. Towards the attainment of a result so
much to be desired the Museum will most powerfully contribute, and those
who frequent it will owe deep obligations to Mr. Hope and the other bene-
factors who have generously added to its stores. But there are other causes
in operation which tend to the same end; and among them, in addition to
such improvements as arise out of the changes consequent on the recent
Act of Parliament, may be mentioned the alteration in the distribution of
Dniversity Honours.
The institution of the School of Physical Science forms a most important
feature in the recent changes, and will doubtless be productive of good results,
provided that sufficient encouragement by way of reward be held out to
those whose tastes lead them to devote themselves to those departments of
knowledge, and that the compulsory arrangements in respcet of other studies
lvili REPORT—1860.
allow sufficient time to the student to accomplish his object. The great
majority of physical students must necessarily belong to that class who have
their subsistence to earn ; and however earnest may be their zeal for mental
improvement, there will be few candidates for the honours of the Physical
School unless due encouragement be given to excellence in that department.
It was therefore with sincere pleasure that I learnt that three Fellowships
had been founded at Magdalen College as prizes for proficiency in Natural
Science; and that at the same College, and at Christ Church and Queen’s,
Scholarships and Exhibitions had been provided for students who evince
during their examinations the greatest aptitude for such studies. Moreover,
the acquisition of a Radcliffe travelling Fellowship has been made to depend
upon obtaining distinction in the School of Natural Science. In addition to
all this, that beneficent and enlightened lady, Miss Burdett Coutts, has founded
two Scholarships with the view of extending among the Clergy educated at
the University a knowledge of Geology. Great hopes are justly excited in
the minds of all well-wishers to the University by these events, and by reflec-
tion on the great change of opinion which must have taken place since the
period when Dr. Kidd, with the aid of Dr. Daubeny, Mr. Greswell and others,
in vain attempted to raise a small sum by private subscription for building a
modest receptacle for the various collections of Natural History. How little
could these public-spirited individuals have foreseen, that within a few short
years a sum approaching to £100,000 would be appropriated to the building
and furnishing that splendid monument of Oxford's good will to science, the
New Museum !
It would not be right, however, if, while speaking in just and sincere terms
of praise of all that excites my admiration in the late proceedings at Oxford,
I were to withhold the honest expression of my opinion on points on which
I feel compelled to differ from the course pursued. I will therefore refer to
two measures, one of which especially I cannot but regard as a mistake,
The first is the repeal of the statute which enforced attendance on two courses
of Professorial lectures ; a requirement, which may have had no small influ-
ence in creating a taste for natural science among that large class of students,
whose only object it is to obtain, in a creditable manner if possible, but at all
events to obtain, the distinction of an Academical degree. At the same time
I cannot but be sensible that the amount of instruction imparted in this way,
even if the attendance were much more than nominal, must necessarily have
been small, not from any want of competency in the teachers, but from the
inherent defect of the system of lectures unaccompanied by examinations ;
and on this account I the less regret the change.
The second, and more serious mistake, in my humble opinion, is the re-
jection by the Congregation in 1857 of the proposal of the Hebdomadal
Council, that the Undergraduate, after passing his first two classical exami-
nations, should be permitted to select his own line of study, and submit
himself at his option to a final examination in any one of the four Schools,
ADDRESS. lix
that is, the Classical, the Mathematical, History and Law, or Natural Science.
The Hebdomadal Council were I think right in believing that such mental
discipline as classical study can impart—and far be it from me to undervalue
it in the least—would be sufficiently secured by the classical requirements of
the two first examinations; aud that the study of Mathematics and the Natural
Sciences, besides imparting much valuable information, which might be exten-
sively utilized in after-life, might equally be viewed as an important means
of improving the intellectual faculties. There is another consideration which
must not be lost sight of in deciding on the policy of the course then pursued.
I think that it cannot in fairness be expected that a young man of the average
abilities of those who contend for honours, and who is called upon to pass
two classical examinations, and prepare for a third, before he is allowed to
follow the bent of his genius and apply himself to his favourite study, can
find time to attain a sufficient proficiency in it to pass a really creditable
examination ; accordingly the necessary result will be that the Examiners will
be obliged to lower the standard of honour, the rather that most of the students
now come to the University without having acquiredeventheelements of scien-
tific knowledge, and thus the first class may almost cease to be a distinction
worth attainment.
I cannot take leave of recent University changes without adverting to that
great, that noble step, the institution of the Middle Class Examinations,
whereby Oxford has furnished substantial aid to those more humble aspirants
to knowledge, by whom a University education, however much desired, is
quite unattainable. Whether this movement be viewed in its moral effect, as
showing a kindly sympathy of the higher intellectual class with the struggling
but deserving children of a lower sphere, or as the best expedient for bringing
about a complete reform in our educational establishments, and therefore a
great engine for advancing popular education—whether this grand and
liberal step be viewed in one or both these aspects, it has given the most
unmixed and heartfelt satisfaction to all who have the moral and mental
improvement of the nation sincerely at heart; and greatly do I rejoice that
such a satisfactory proof should have been given of a desire to make Uni-
versity Institutions a general national blessing.
Oxford, then, has shown herself fully equal to her glorious mission, and it
was only a fitting sequel to such enlightened conduct, that she should be
entrusted with the grateful task of educating the Heir apparent to the Throne
of the most popular Sovereign who ever swayed the sceptre of this vast
_ Empire.
I shall perhaps be forgiven if my former connexion with Oxford, and the
interest which I must ever take in everything appertaining to my own Uni-.
versity, have induced me to dwell somewhat at length on the above matters.
It is now time that I should direct my attention to the general domain of
science ; but more particularly to that department to which my own labours,
humble though they be, have been more especially devoted,—I mean the
Ix REPORT—1860.
science of Astronomy, a science, which, whether we consider the surpassing
interest of the subjects with which it is conversant, or tbe lofty nature of the
speculations to which its inquiries lead, must ever occupy a most distinguished,
if not the first place among all others.
In a discourse addressed in May 1859 to the Imperial Academy of
Sciences of Vienna, by the distinguished Astronomer Littrow, a very full ac-
count is given of the voluntary contributions of the private observers of
all nations to the extension of the science of Astronomy ; and this discourse
concludes with a remarkable sentence, of which our English Amateurs may
well be proud: he expresses a hope that on the next occasion in which he
shall be called upon to dilate on the same theme, he shall not as then have
to mention English names in such preponderating numbers.
At the beginning of the year 1820, when the Astronomical Society was
founded, the private Observatories in this country were very few in number.
The establishment of that Society gave a most remarkable stimulus to the
cultivation of the science which it was intended to promote. 1 can give no
better proof of this than the fact thatthe Nautical Almanac now contains a
list of no less than twelve private Observatories in the United Kingdom, at
nearly all of which some good work has been done; and in addition to this,
some Observatories, which have been since discontinued, have performed most
important services—I may instance that of the two Herschels at Slough, and
that of Admiral Smyth at Bedford.
It may not be uninteresting if I describe the nature and utility of some
of the results which these several establishments have furnished to the world:
I say the world advisedly, for scientific facts are the common inheritance of
all mankind.
But first a werd as to the peculiar province of the observatories which are
properly called ‘ public,” such as the far-famed Institution at Greenwich.
Their task is now more peculiarly to establish with the last degree of accu-
racy the places of the principal heavenly bodies of our own system, and of
the brighter or fundamental fixed stars, which are about 100 in number.
But in the early stages of Astronomy, we were necessarily indebted to public
Observatories for all the data of the science. On the other hand, their vo-
luntary rivals occupy that portion of the great astronomical field which is
untilled by the professional observer; roving over it according to their own
free will and pleasure, and cultivating with industrious hand such plants as
the more continuous and severe labours of the public Astronomer leave no
time or opportunity to bring to maturity.
The observations of our private observers have been chiefly devoted to
seven important objects :—
First. The observing and mapping of the smaller stars, under which term
I include all those which do not form the peculiar province of the public
observer.
Secondly. The observations of the positions and distances of double stars.
ADDRESS. Xl
Thirdly. Observations, delineations, and Catalogues of the Nebule.
Fourthly. Observations of the minor planets.
Fifthly. Cometary observations.
Sixthly. Observations of the solar spots, and other phenomena on the
Sun’s disc.
Seventhly. Occultations of stars by the Moon, eclipses of the heavenly
bodies, and other occasional extra-meridional observations.
And first as to cataloguing and mapping the smaller stars. This means,
as you know, the accurate determination by astronomical observation of the
places of those objects, as referred to certain assumed fixed points in the
heavens. The first Star Catalogue worthy to be so called, is that which goes
by the name of Flamsteed’s, or the British Catalogue. It contains above
$000 stars, and is the produce of the labours of the first Astronomer Royal
of Greenwich, labours prosecuted under circumstances of great difficulty,
and the results of which were not given to the world in a complete form till
many years had elapsed from the time the observations were made, which
was during the latter half of the seventeenth century. About the middle
of the eighteenth century, the celebrated Dr. Bradley, who also filled the post
of Astronomer Royal, observed an almost equally extensive Catalogue
of Stars, and the beginning of the nineteenth century gave birth to that of
Piazzi of Palermo. These three are the most celebrated of what may be
now termed the ancient Catalogues. About the year 1830 the attention of
modern astronomers was more particularly directed to the expediency of re-
observing the stars in these three Catalogues, a task which was much faci-
litated by the publication of a very valuable work of the Astronomical
Society, which rendered the calculations of the observations to be made com-
paratively easy, and accordingly observations were commenced and com-
pleted in several public and private Observatories, from which some curious
results were deduced, as e. @., sundry stars were found to be missing, and
Others to have what is called proper motion. And now a word as to the
utility of this course of observation. It is well observed by Sir John
Herschel, “ that the stars are the landmarks of the Universe; every well-deter-
mined star is a point of departure which can never deceive the astronomer,
geographer, navigator, or surveyor.” We must have these fixed points in
order to refer to them all the observations of the wandering heavenly bodies,
the planets and the comets. By these fixed marks we determine the situation
of places on the earth’s surface, and of ships on the ocean. When the places of
the stars have been registered, celestial charts are constructed ; and by com-
paring these with the heavens, we at once discover whether any new body
be present in the particular locality under observation: and thus have most
of the fifty-seven small or minor planets between Mars and Jupiter been
discovered. ‘Ihe observations, however, of these smaller stars, and the re-
gistry of their places in Catalogues, and the comparisons of the results ob-
tained at different and distant periods, have revealed another extraordinary
Ixii REPORT—1860.
fact, no less than that our own Sun is not fixed in space, but that it is con-
stantly moving forward towards a point in the constellation Hercules, at the
rate, as it is supposed, of about 18,000 miles an hour, carrying with it the
whole planetary and cometary system; and if our Sun moves, probably all
the other stars or suns move also, and the whole universe is in a perpetual
state of motion through space.
The second subject to which the attention of private observers has been
more particularly directed, is that of double or multiple stars, or those which,
being situated very close to one another, appear single to the naked eye, but
when viewed through powerful telescopes are seen to consist of two or more
stars. The measuring the angles and distances from one another of the two
or more component stars of these systems, has led to the discovery that many
of these very close stars are in fact acting as suns to one another, and revol-
ving round their common centre of gravity, each of them probably carrying
with it a whole system of planets and comets, and perhaps each carried for-
ward through space like our own sun. It became then a point of great in-
terest to determine, whether bodies so far removed from us as these systems,
observed Newton’s law of gravity, and to this end it was necessary to observe
the angles and distances of a great number of these double stars scattered
everywhere through the heavens, for the purpose of obtaining data to com-
pute their orbits. This has been done, and chiefly by private observers; and
the result is that these distant bodies are found to be obedient to the same
laws that prevail in our own system. :
The Nebulz are, as it were, systems or rings of stars scattered through space
at incredible distances from our star system, and perhaps from one another;
and there are many of these mysterious clouds of light, and there may be
endless invisible regions of space similarly tenanted. Now the nearest fixed
star of our star system whose distance has been measured, is the brightest in the
constellation Centaur, one of the Southern constellations, and this nearest is
yet so far removed, that it takes light, travelling at the rate of about 192,000
miles per second, three years to arrive at the earth from that star. When
we gaze at it, therefore, we see it only as it existed three years ago; some
great convulsion of nature may have since destroyed it. But there are many
bright stars in our own system, whose distance is so much greater than this,
as a Cygni, for example, that astronomers have not succeeded in measuring it.
What, then, must be the distance of these nebule, with which so much space
is filled; every component star in which may be a sun, with its own system
of planets and comets revolving round it, each planet inhabited by myriads
of inhabitants! What an overpowering view does this give us of the extent
of creation! The component stars of these nebulz are so faint and appa-
rently so close together, that it is necessary to use telescopes of great power,
and with apertures so large as to admit a great amount of light, for their ob-
servation. We owe it more especially to four individuals, that telescopes
have been constructed, at a great cost and with great mechanical skill, suf-
ADDRESS. xiii
ficiently powerful to penetrate these depths of space. Those four indivi-
duals are the Herschels, father and son, Lord Rosse, and Mr. Wm. Lassell.
That praiseworthy nobleman, Lord Rosse, began his meritorious career by
obtaining a First Class at this University, and has, as you know, spent large
sums of money and displayed considerable mechanical genius in erecting,
near his own Castle in Ireland, an instrument of far greater power than any
other in the world; and with it he has observed these nebule, and employed
skilful artists to delineate their forms: and he has moreover made the very
curious discovery, that some of them are arranged ina spiral form, a fact
which gives rise to much interesting speculation on the kind of forces by
which their parts are held together. It were much to be wished that obser-
vations similar to these, and with instruments of nearly the same power,
should be made of the Southern nebule also; that this generation might
be able to leave to posterity a record of their present configurations. The
distinguished Astronomer, Mr. Wm. Lassell, the discoverer of Neptune’s
satellite, has just finished at his own cost an instrument equal to the task,
mounted equatorially; and I am not without hope that it may, at perhaps
no very distant period, be devoted to its accomplishment. A recent com-
munication from him to the Astronomical Society expresses satisfaction with
the mounting of his instrument, and after many trials its great speculum has
at last come forth nearly perfect from his laboratory.
I am, however, warned by the lapse of time, that it will not be possible for
me to exhaust the whole field, the limits of which I have sketched, in which
private enterprise has been assiduously at work to enlarge the bounds of
astronomical knowledge. I will therefore pass at once to the two most in-
teresting subjects which remain, the observations of Comets, and of peculiar
appearances on the Sun’s disc.
Of all the phenomena of the heavens, there are none which excite more
general interest than comets, those vagrant strangers, the gipsies as they
have been termed of our solar system, which often come we know not whence,
and at periods when we least expect them: and such is the effect produced
by the strangeness and suddenness of their appearance, and the mysterious
nature of some of the facts connected with them, that while in ignorant times
they excited alarm, they now sometimes seduce men to leave other employ-
ments and become Astronomers. Now, though the larger and brighter
comets naturally excite most general public interest, and are really valuable
to astronomers, as exhibiting appearances which tend to throw light on the
internal structure of these bodies, and the nature of the forces which must
be in operation to produce the extraordinary phenomena observed, yet some
of the smaller telescopic comets are, perhaps, more interesting in a physical
point of view. Thus the six periodical comets, the orbits of which have been
determined with tolerable accuracy, and which return at stated intervals, are
extremely useful as being likely to disclose facts, of which but for them we
should possibly have ever rernained ignorant. Thus, for example, when the
Ixiv REPORT—1860. ;
comet of Encke, which performs its revolution in a period of a little more than
three years, was observed at each return, it disclosed the important and unex-
pected fact, that its motion was continually accelerated. At each successive
approach to the Sun it arrives at its perihelion sooner and sooner ; and there
is no way of accounting for this so satisfactory as that of supposing that the
space, in which the planetary and cometary motions are performed, is every-
where pervaded by a very rarefied atmosphere or ether, so thin as to exercise
no perceptible effect on the movements of massive solid bodies like the planets,
but substantial enough to exert a very important influence on more attenuated
substances moving with great velocity. ‘The effect of the resistance of the
ether is to retard the tangential motion, and allow the attractive force of
gravity to draw the body nearer to the Sun, by which the dimensions of the
orbit are continually contracted and the velocity in it augmented. The final
result will be that after the lapse of ages this comet will fall into the Sun;
this body, a mere hazy cloud, continually flickering as it were like a celestial
moth round the great luminary, is at some distant period destined to be mer-
cilessly consumed. Now the discovery of this ether is deeply interesting as
bearing on other important physical questions, such as the undulatory theory
of light; and the probability of the future absorption of comets by the Sun
is important as connected with a very interesting speculation by Professor
William Thomson, who has suggested that the heat and light of the Sun may
be from time to time replenished by the falling in and absorption of count-
less meteors which circulate round him; and here we have a cause revealed
which may accelerate or produce such an event.
In the progress of science it often happens that a particular class of obser-
vations, all at once, and owing to some peculiar circumstance, attracts very
general attention and becomes deeply interesting. This has been the case
within the last few years in reference to observations of the Sun's dise, which
were at one time made by very few individuals, and were indeed very much
neglected both by professional and amateur Astronomers. During this sea-
son of comparative neglect, there were not, however, wanting some enthusiastic
individuals, who were in silence and seclusion obtaining data of great import-
ance.
On the 1st of September last, at 118 18™ a.M., a distinguished Astronomer,
Mr. Carrington, had directed his telescope to the Sun, and was engaged in
observing his spots, when suddenly two intensely luminous bodies burst into
view on its surface. They moved side by side through a space of about
35,000 miles, first increasing in brightness, then fading away; in 5 minutes
they had vanished. They did not alter the shape of a group of large black
spots which lay directly in their paths. Momentary as this remarkable phe-
nomenon was, it was fortunately witnessed and confirmed, as to one of the
bright lights, by another observer, Mr. Hodgson at Highgate, who by a
happy coincidence had also his telescope directed to the great luminary at
the same instant. It may be, therefore, that these two gentlemen have
ADDRESS. Ixv
actually witnessed the process of feeding the Sun, by the fall of meteoric
matter; but however this may be, it is a remarkable circumstance, that the
observations at Kew show that on the very day, and at the very hour and
minute of this unexpected and curious phenomenon, a moderate but marked
magnetic disturbance took place; and a storm or great disturbance of the
magnetic elements occurred four hours after midnight, extending to the
southern hemisphere. Thus is exhibited a seeming connexion between mag-
netic phenomena and certain actions taking place on the Sun’s disc—a con-
nexion, which the observations of Schwabe, compared with the magnetical
records of our Colonial Observatories, had already rendered nearly certain.
The remarkable results derived from the comparison of the magnetical
observations of Captain Maguire on the shores of the Polar Sea, with the
contemporaneous records of these observatories, have been described by me
on a former occasion. The delay of the Government in re-establishing the
Colonial Observatories has hitherto retarded that further development of the
magnetic laws, which would doubtless have resulted from the prosecution of
such researches.
We may derive an important lesson from the facts above alluded to.
Here are striking instances in which independent observations of natural
phenomena have been strangely and quite unexpectedly connected together :
this tends powerfully to prove, if proof were necessary, that if we are really
ever to attain toa satisfactory knowledge of Nature’s laws, it must be accom-
plished by an assiduous watching of all her phenomena, in every department
into which Natural Science is divided. Experience shows that such obser-
vations, if made with all those precautions which long practice combined
with natural acuteness teaches, often lead to discoveries, which cannot be at
all foreseen by the observers, though many years may elapse before the
whole harvest is reaped.
I cannot allude to the subject of Arctic voyages without congratulating
the Association on the safe return of Sir Leopold M‘Clintock and his gallant
band, after accomplishing safely and satisfactorily the object of their inter-
esting mission. The great results accomplished with such small means, and
chiefly by the display of those qualities of indomitable courage, energy and
perseverance which never fail the British seaman in the hour of need, are the
theme of general admiration ; but I may be permitted in passing to express
some regret, that it was left to the devoted affection of a widowed lady,
slightly aided by private contributions, to achieve a victory in which the
honour of the nation was so largely involved,—the rather that the danger of
the enterprise,—the pretext for non-interference—was much enhanced
thereby, and the accessions to our scientific and geographical knowledge
proportionably curtailed.
The instances to which I have alluded are only a few of many which
could be adduced of an insufficient appreciation of certain objects of
scientific research. Large sums are expended on matters connected
e
lxvi REPORT—1860.
with science, but this is done on no certain and uniform system; and
there is no proper security that those who are most competent to give good
advice on such questions, should be the actual persons consulted. It was
partly with the hope of remedying these defects and of generally improving
the position of science in the country in its relation to the Government, that
the Parliamentary Committee of this Association was established; and it
was partly with the same hope that I was induced to accept the honourable
office of President of the Royal Society, though conscious at the time that
there were very many far better qualified than myself to hold it. Many of
those whom I am now addressing are aware of the steps which were adopted
by the Parliamentary Committee, and subsequently by the Committee of
Recommendations of this Association, for the purpose of collecting the
opinions of the cultivators of science on the question,—- Whether any measures
could be adopted by Government or Parliament that would improve our
position? The question was afterwards referred to and discussed by thie
Council of the Royal Society, who, on the 15th of January, 1857, agreed
upon twelve resolutions in reply thereto. These resolutions recommend,
among other things, that Government grants in aid of local funds should be
applied towards the teaching of science in schools, the formation of Provincial
Museums and Libraries, and the delivery of lectures by competent persons,
accompanied by examinations; and finally, that some existing scientific body,
or some Board to be created for the purpose, should be formally recognized,
which might advise the Government on all matters connected with science,
and especially on the prosecution, reduction, and publication of scientific
researches, and the amount of Parliamentary or other grants in aid thereof ;
also on the general principles to be adopted in reference to public scientific
appointments, and on the measures necessary for the more general diffusion
of a knowledge of physical science among the nation at large; and which
might also be consulted by the Government on the grants of pensions to the
cultivators of science. 'I was requested to transmit these resolutions to Lord
Palmerston, and also to the Parliamentary Committee of this Association.
Since that period these resolutions have been discussed by that Committee ;
but partly because some of its most influential members have expressed
grave doubts as to the expediency of urging their adoption at all, and partly
from the want of a favourable opportunity for bringing them forward, nothing
further has as yet been done. I thought, however, that the time was arrived
at which it was only proper that I should explain the steps which had been
already taken, and the actual position in which the question now stands. If
it be true, as some of our friends imagine, that the recognition of such a body
as has been above described, however useful it might prove if the public
were disposed to put confidence in its suggestions, would only augment that
feeling of jealousy which is disposed to view every application for aid to
scientific research in the light of a request for some personal boon, to be
bestowed on some favoured individual, then indeed its institution would not
—"
ADDRESS. Ixvil
be expedient. I only wish that persons who entertain such views, would pay
some attention to the working of the Government Grant Committee of the
Royal Society, a body composed of forty-two persons selected from among
the most eminent cultivators of science, and which is entrusted with the
distribution of an annual sum of £1000, placed by Parliament at the disposal
of the Royal Society at the suggestion of Lord John Russell, in aid of
scientific inquiries. One of the rules of that Commiitee is, that no sum
whatever shall be given to defray the merely personal expenses of the
experimenters ; all is spent on materials and the construction or purchase of
instruments, except in a very few and rare instances in which travelling ex-
penses form the essential feature of the outlay. A list of the objects to which
the grants are devoted has been published by Parliament; among them are
interesting investigations into the laws of heat, the strength of materials used
in building, the best form of boilers, from the bursting of which so many
fatal accidents are continually occurring, the electric conductivity of metals,
so important for telegraphic communication, and into many other questions,
in the solution of which the public generally have the deepest interest. The
cost of these researches has been defrayed by these valuable grants. They
have provided also for the construction of better and standard meteorological
and magnetical instruments, for the execution of valuable drawings of scarce
fossils and zoological specimens collected with great labour by distinguished
naturalists, for the reduction and publication of astronomical observations by
some of our most highly esteemed Astronomers, and for physiological re-
searches which have an important bearing on our knowiedge of the human
frame. Time indeed would fail me were I to attempt to describe all the good
done and perhaps evil prevented by the distribution of these grants; and
yet no portion of the money can be said to be really received by those to
whom it is appropriated, inasmuch as it is all spent in the various means and
appliances of research; in short, to quote from a letter addressed to the
Secretary of the Treasury, at a time when the grant was temporarily withheld,
“by the aid of this contribution, the Government has, in fact, obtained for
the advancement of science and the national character, the personal and
gratuitous services of men of first-rate eminence, which, without this
comparatively small assistance, would not have been so applied.” I think
that we were justified in terming this assistance small; for it is really so
in comparison with the amount of other sums which are applied to analogous
objects, but without that wholesome control of intelligent distributors,
thoroughly and intimately conversant with the characters and competency of
those who apply for the grants. The recognition of such a Board as has
been sketched out by the Council of the Royal Society, may not lead to
a greater expenditure of public money, indeed it is much more likely to
curtail it; as some who now apply for aid through the interest of persons
having influence with those in authority, who are generally but ill-informed
on the subject-matter of the application, would hesitate long before they
e2
[xvill REPORT—1860.
made a similar request to those who are thoroughly conversant with it; and it
is on this account that comparatively few of the applications to the Govern-
ment Grant Committee are rejected. Moreover, inasmuch as every grant
passed by the proposed Board would afterwards receive the jealous scrutiny
of Parliament, whose sanction must of course be obtained, I am disposed to
think that were I to support the establishment of such a scientifie Council, or
the formal recognition by the State of some existing scientific body in that
capacity, I should be advocating that which would prove a valuable addition
to the Institutions of my country.
Before I finally conclude my observations on the important question I
have introduced to your notice, and on which perhaps I have already said
too much at the risk of wearying you, I must guard myself against one
misapprehension, and that is, that we are anxious to obtain a large augmenta-
tion of the £1000 now voted by Parliament. This is by no means our wish ;
that annual sum is in ordinary years sufficient, and sometimes more than
sufficient, and there is nothing that would be more deprecated than any
large increase; but there is a very general feeling among those most
competent to form an opinion on these matters, that when the well-con-
sidered interests of science and the national good demand an extraordinary
outlay, such as cannot be defrayed out of the proceeds of the ordinary yearly
grant,—as, for example, for surveying and exploring expeditions, for the
establishment and maintenanee of magnetic observatories, for the purchase
of costly astronomical instruments, for expensive astronomical excursions,
such as that to Teneriffe,—that the expediency of the grant is more likely to
be properly investigated and tested, if referred to those whose avocations have
given them the requisite knowledge, than if the concession or rejection of the
proposal be permitted to depend on such accidents, as, whether this or that
individual apply, or this or that statesman fill the office of Chancellor of the
Exchequer.
I trust that I may be pardoned the long digression in which I have
indulged, in consideration of the importance of the subject.
Having detailed some of the valuable services of our amateur Astronomers,
let me not be accused of being unjust to the professional contributors to the
data of that noble science. Most valuable Star Catalogues have resulted from
the labours of our public Observatories, and from Greenwich in particular.
There are also two Observatories which have, as it were, a quasi public
character, viz. the Radcliffe Observatory and that of Armagh, which have
contributed much to this department of Astronomy. Your former President,
the accomplished and learned Dr. Robinson of Armagh, has lately presented
to the astronomical world a Catalogue of the places of more than 5000 stars,
and in so doing has conferred a most important benefit on his favourite
science.
But it would be an unpardonable omission were I to neglect to express our
gratitude to our great National Institution at Greenwich, for the manner in
ADDRESS. xix
which it has consistently discharged the task imposed upon it by its founder
and those who inaugurated its first proceedings. The duty assigned to it
was “to rectify the tables of the motions of the heavens and the places of
the fixed stars, in order to find out the so much desired longitude at sea, for
perfecting the art of navigation ;” and gloriously has it executed its task.
For two centuries it has been at work, endeavouring to give to the determi-
nations of the places of the principal fixed stars and of the heavenly bodies
of our own solar system, and more especially of the Moon, the utmost degree
of precision; and during the same period, the master minds of Europe have
been engaged in perfecting the analytical theory, by which the many and
most perplexing inequalities of the Moon’s motion must be accounted for
and represented, before Tables can be constructed giving the place of our
satellite with that accuracy that the modern state of science demands.
The very important task of calculating such Tables has just been finished.
Our able and accomplished Director of the National Observatory, Mr. Airy,
had caused all the observations of the Moon made at Greenwich, from 1750
to 1830, to be reduced upon one uniform system, employing constants
derived from the best modern researches; and a distinguished Danish Pro-
fessor, who had been for some time engaged in calculating new Tables of the
Moon, availed himself of the data so furnished. Professor Hansen happily
brought to his task all the accomplishments of a practised observer, and of
one of the most able analysts of modern times, combined with the most
determined industry and perseverance. In the completion of it he was
liberally assisted by our Government, at a time when an unhappy war had
deprived the Danish Government of the means of further aiding their Pro-
fessor, and a great astronomical work had been suspended for want of £300,
a sum which many do not hesitate to spend on the purchase of some useless
luxury. Professor Hansen’s Tables are now finished and published. They
agree admirably with the Greenwich Observations with which they have
been compared, and the mode of their execution has been approved by those
competent to express an opinion on such a subject. They have been
rewarded also with the Gold Medal of the Astronomical Society, a distinction
never lightly bestowed.
In paying this tribute to the merit of Professor Hansen, I must not be
understood as wishing to ignore, far less depreciate, that of three very emi-
nent geometers—Plana, Lubbock, and Pontécoulant, who have devoted
years of anxious and perhaps ill-requited labour to the investigation of the
Lunar inequalities, but who have never yet embodied the results in the only
form useful to Navigation, that of Tables.
A curious controversy has lately arisen on the subject of the acceleration
of the Moon's motion, which is now exciting great interest among mathe-
maticians and physical astronomers. Professor Adams and M. Delaunay
take one view of the question; MM. Plana, Pontécoulant, and Hansen the
other. Mr. Airy, Mr. Main the President of theAstronomical Society, and
lxx REPORT—1860.
Sir John Lubbock support the conclusions at which Professor Adams has
arrived. The question in dispute is strictly mathematical; and it is a very
remarkable circumstance in the history of Astronomy, that such great names
should be ranged on opposite sides, seeing that the point invalved is really
no other than whether certain analytical operations have been conducted on
right principles ; and it is a proof therefore, if any were wanting, of the extra-
ordinary complexity and difficulty of these transcendental inquiries. The
controversy is of the following nature :—The Moon’s motion round the Earth,
which would be otherwise uniform, is disturbed by the Sun’s attraction ; any
cause therefore which affects the amount of that attraction affects also the
Moon’s motion: now, as the excentricity of the Earth’s orbit is gradually
decreasing, the average distance of the Sun is slightly increasing every year,
and his disturbing force becomes less; hence the Moon is brought nearer the
Earth, but at the rate of lessthan one inch yearly ; her gravitation towards the
Earth is greater, and her motion is proportionably accelerated. It is on the
secular acceleration of the Moon’s mean motion, arising from this minute
yearly approach, that the dispute has arisen ; so infinitesimally small are the
quantities within the reach of modern analysis. Mr. Adams asserts that his
predecessors have improperly omitted the consideration of the effect produced
by the action of that part of the Sun’s disturbing force which acts in the
direction of a tangent to the Moon’s orbit, and which increases the velocity ;
his opponents deny that it is necessary to take this into account at all. Had
not M. Delaunay, an able French analyst, by a perfectly independent pro-
cess, confirmed the results of Professor Adams, we should have had the
English and Continental Astronomers waging war on an algebraical question.
On the other hand, however, the computations of the ancient Lunar Eclipses
support the views of the Continent; but if Mr. Adams’s mathematics are
correct, this only shows that there must be other causes in operation as yet
undiscovered, which influence the result; and it is not at all unlikely that
this most curious and interesting controversy will eventually lead to some
important discovery in Physical Astronomy.
You are aware that at the suggestion of Sir John Herschel an instrument
was constructed for the Kew Observatory, to which the name of Photohelio-
graph has been given, because it is adapted solely to the purpose of obtaining
photographic representations of the appearances on the Sun’s disc. Many
difficulties have been encountered in the use of this instrument, but by the
zealous exertions of the late Mr. Welsh, Mr. Beckley, and Mr. De la Rue,
they have been overcome. It is to the last-named gentleman, so distinguished
for his successful prosecution of celestial photography, that the Royal Society
have entrusted a grant of money to enable him to transport the Photohelio-
graph to Spain, to observe the total eclipse of the Sun, which is now
approaching, and great interest will attach to records of the phenomena of
the eclipse thus obtained.
In Chemistry I am informed that great activity has been displayed, espe-
ADDRESS. lxx1
cially in the organic department of the science. For several years past pro-
cesses of substitution (or displacement of one element or organic group by
another element or group more or less analogous) have been the main agents
employed in investigation, and the results to which they have led have been
truly wonderful ; enabling the chemist to group together separate compounds
of comparatively simple constitution into others much more complex, and
thus to imitate, up to a certain point, the phenomena which take place within
the growing plant or animal. It is not indeed to be anticipated that the
chemist should ever be able to produce by the operations of the laboratory
the arrangement of the elements in the forms of the vegetable cell or the
animal fibre; but he may hope to succeed in preparing some of the complex
results of secretion or of chemical changes produced within the living
organism,—changes, which furnish definite crystallizable compounds, such
as the formiates and the acetates, and which he has actually obtained by
operations independent of the plant or the animal.
Hofmann, in pursuing the chemical investigation of the remarkable com-
pound which he has termed Triethylphosphine, has obtained some very
singular compound ammonias. Triethylphosphine is a body which takes fire
spontaneously when its vapour is mixed with oxygen, at a temperature a little
above that of the body. It may be regarded as ammonia in which an atom
of phosphorus has taken the place of nitrogen, and in which the place of each
of the three atoms of hydrogen in ammonia is supplied by ethyl, the peculiar
hydrocarbon of ordinary alcohol. From this singular base Hofmann has
succeeded in procuring other coupled bases, which though they do not cor-
respond to any of the natural alkalies of the vegetable kingdom, such as
morphia, quinia, or strychnia, yet throw some light upon the mode in which
complex bodies more or less resembling them have been formed.
The power which nitrogen possesses of forming a connecting link between
the groups of substances of comparatively simple constitution, has been
remarkably exemplified by the discovery of a new class of amide acids by
Griess, in which he has pointed out a new method, which admits of very
general application, of producing complex bodies related to the group of
acids, in some measure analogous to the Poly-ammonias of Hofmann.
Turning to the practical applications of Chemistry, we may refer to the
beautiful dyes now extracted from aniline, an organic base formerly obtained
as a chemical curiosity from the products of the distillation of coal-tar, but
now manufactured by the hundred-weight in consequence of the extensive
demand for the beautiful colours known as Mauve, Magenta, and Solferino,
which are prepared by the action of oxidizing agents, such as bichromate of
potash, corrosive sublimate, and iodide of mercury upon aniline.
Nor has the Inorganic department of Chemistry been deprived of its due
share of important advances. Schédnbein has continued his investigations
upon ozone, and has added many new facts to our knowledge of this
interesting substance; and Andrews and Tait, by their elaborate investigations,
lxxii REPORT—-1860.
have shown that ozone, whether admitted to be an allotropic modification of
oxygen or not, is certainly much more dense than oxygen in its ordinary
condition.
In Metallurgy we may point to the investigations of Deville upon the
platinum group of metals, which are especially worthy of remark on account
of the practical manner in which he has turned to account the resources of
the oxyhydrogen blowpipe, as an agent which must soon be very generally
adopted for the finer description of metallurgic operations at high tempera-
tures. By using lime as the material of his crucibles and as the support for
the metals upon which he is operating, several very important practical
advantages have been obtained. The material is sufficiently infusible to
resist the intense heat employed ; it is a sufficiently bad conductor of heat
to economize very perfectly the high temperature which is generated ; and
it may be had sufficiently free from foreign admixture to prevent it from
contaminating the metals upon which the operator is employed.
The bearing of some recent geological discoveries on the great question
of the high antiquity of Man was brought before your notice at your last
Meeting at Aberdeen by Sir Charles Lyell in his opening address to the
Geological Section. Since that time many lrench and English naturalists
have visited the valley of the Somme in Picardy, and confirmed the opinion
originally published by M. Boucher de Perthes in 1847, and afterwards con-
firmed by Mr. Prestwich, Sir C. Lyell, and other geologists from personal
examination of that region. It appears that the position of the rude flint-
implements, which are unequivocally of human workmanship, is such, at |
Abbeville and Amiens, as to show that they are as ancient as a great mass of
gravel which fills the lower parts of the valley between those two cities, ex-
tending above and below them. This gravel is an ancient fluviatile alluvium
by no means confined to the lowest depressions (where extensive and deep
peat-mosses now exist), but is sometimes also seen covering the slopes of the
boundary hills of chalk at elevations of 80 or 100 feet above the level of the
Somme. Changes therefore in the physical geography of the country, com-
prising both the filling up with sediment and drift and the partial re-excava-
tion of the valley, have happened since old river-beds were at some former {
period the receptacles of the worked flints. The number of these last, already
computed at above 1400 in an area of fourteen miles in length and half a_
mile in breadth, has afforded to a succession of visitors abundant opportunities
of verifying the true geological position of the implements.
The old alluvium, whether at higher or lower levels, consists not only of
the coarse gravel with worked flints above mentioned, but also of superim-
posed beds of sand and loam, in which are many freshwater and land shells,
for the most part entire, and of species now living in the same part of France.
With the shells are found bones of the Mammoth and an extinct Rhinoceros,
R. tichorhinus, an extinct species of deer, and fossil remains of the Horse, Ox,
and other animals. These are met with in the overlying beds, and sometimes
ADDRESS. Ixxiii
also in the gravel where the implements occur. At Menchecourt, in the sub-
urbs of Abbeville, a nearly entire skeleton of the Siberian Rhinoceros is said
to have been taken out about forty years ago, a fact affording an answer to the
question often raised, as to whether the bones of the extinct mammalia could
have been washed out of an older alluvium into a newer one, and so redepo-
sited and mingled with the relics of human workmanship. Far-fetched as wag
this hypothesis, I am informed that it would not, if granted, have seriously
shaken the proof of the high antiquity of the human productions, for that
proof is independent of organic evidence or fossil remains, and is based on
_ physical data. As was stated to us last year by Sir C. Lyell, we should still
have to allow time for great denudation of the chalk, and the removal from
place to place, and the spreading out over the length and breadth of a large
valley of heaps of chalk flints in beds from 10 to 15 feet in thickness, covered
by loams and sands cf equal thickness, these last often tranquilly deposited,
all of which operations would require the supposition of a great lapse of time.
That the mammalian fauna preserved under such circumstances should be
found to diverge from the type now established in the same region, is con-
sistent with experience; but the fact of a foreign and extinct fauna was not
needed to indicate the great age of the gravel containing the worked flints.
Another independent proof of the age of the same gravel and its asso-
ciated fossiliferous loam is derived from the large deposits of peat above
alluded to in the valley of the Somme, which contain not only monuments
of the Roman, but also those of an older Stone Period, usually called Celtic.
Bones also of the Bear, of the species still inhabiting the Pyrenees, and of
the Beaver, and many large stumps of trees, not yet well examined by bota-
nists, are found in the same peat, the oldest portion of which belongs to
times far beyond those of tradition; yet distinguished geologists are of opi-
nion that the growth of all the vegetable matter, and even the original scoop-
ing out of the hollows containing it, are events long posterior in date to the
gravel with flint implements, nay, posterior even to the formation of the up-
permost of the layers of loam with freshwater shells overlying the gravel.
The exploration of caverns, both in the British Isles and other parts of
Europe, has in the last few years been prosecuted with renewed ardour and
success, although the theoretical explanation of many of the phenomena
brought to light seems as yet to baffle the skill of the ablest geologists.
Dr. Falconer has given us an account of the remains of several hundred
Hippopotami obtained from one cavern near Palermo, in a locality where
there is now no running water. The same paleontologist, aided by Col.
Wood of Glamorganshire, has recently extracted from a single cave in the
Gower peninsula of South Wales, a vast quantity of the antlers of a reindeer
(perhaps of two species of reindeer), both allied to the living one. These
fossils are most of them shed horns; and there have been already no less
than 1100 of them dug out of the mud filling one cave.
In the cave of Brixham in Devonshire, and in another near Palermo in
Ixxiv REPORT—1860.
Sicily, flint implements were observed by Dr. Falconer, associated in such a
manner with the bones of extinct mammalia, as to lead him to infer that Man
must have coexisted with several lost species of quadrupeds; and M. de Vibraye
has also this spring called attention to analogous conclusions at which he
has arrived, by studying the position of a human jaw with teeth, accom-
panied by the remains of a mammoth, under the stalagmite of the Grotto
d’Arcis near Troyes in France.
In the recent progress of Physiology, I am informed that the feature per-
haps most deserving of note on this occasion is the more extended and suc-
cessful application of Chemistry, Physics, and the other collateral sciences
to the study of the Animal and Vegetable Economy. In proof I refer to
the great and steady advances which have, within the last few years, been
made in the chemical history of Nutrition, the statics and dynamics of the
blood, the investigation of the physical phenomena of the senses, and the
electricity of nerves and muscles. Even the velocity of the nerve-force
itself has been submitted to measurenient. Moreover, when it is now de-
sired to apply the resources of Geometry or Analysis to the elucidation of
the phenomena of life, or to obtain a mathematical expression of a physiolo-
gical law, the first care of the investigator is to acquire precise experimental
data on which to proceed, instead of setting out with vague assumptions and
ending with a parade of misdirected skill, such as brought discredit on the
school of the mathematical physicians of the Newtonian period.
But I cannot take leave of this department of knowledge without likewise
alluding to the progress made in scrutinizing the animal and vegetable
structure by means of the microscope—more particularly the intimate or-
ganization of the brain, spinal cord, and organs of the senses; also to the
extension, through means of well-directed experiment, of our knowledge of
the functions of the nervous system, the course followed by sensorial im-
pressions and motorial excitement in the spinal cord, and the influence
exerted by or through the nervous centres on the movements of the heart,
blood-vessels and viscera, and on the activity of the secreting organs ;—
subjects of inquiry, which, it may be observed, are closely related to the
question of the organic mechanism whereby our corporeal frame is influ-
enced by various mental conditions.
And now, in conclusion, I may perhaps be permitted to express the hope
that the examples I have given of some of the researches and discoveries
which occupy the attention of the cultivators of science, may have tended to
illustrate the sublime nature, engrossing interest and paramount utility of
such pursuits, from which their beneficial influence in promoting the intel-
lectual progress and the happiness and well-being of mankind may well be
inferred. But let us assume that to any of the classical writers of antiquity,
sacred or profane, a sudden revelation had been made of all the wonders
involved in Creation accessible to man; that to them had been disclosed not
only what we now know, but what we are to know hereafter, in some future
ADDRESS. Ixxv
age of improved knowledge; would they not have delighted to celebrate the
marvels of the Creator’s power? They would have described the secret
forces by which the wandering orbs of light are retained in their destined
paths; the boundless extent of the celestial spaces in which worlds on
worlds are heaped; the wonderful mechanism by which light and heat are
conveyed through distances which to mortal minds seem quite unfathom-
able; the mysterious agency of electricity, destined at one time to awaken
men’s minds to an awful sense of a present Providence, but in after-times
to become a patient minister of man’s will, and convey his thoughts with
the speed of light across the inhabited globe; the beauties and prodigies
of contrivance which the animal and vegetable world display, from man-
kind downwards to the lowest zoophyte, from the stately oak of the pri-
meval forest to the humblest plant which the microscope unfolds to view;
the history of every stone on the mountain brow, of every gay-coloured
insect which flutters in the sun-heam ;—all would have been described, and
all which the discoveries of our more fortunate posterity will in due time
disclose, and in language such as none but they could command. It is re-
served for future ages to sing such a glorious hymn to the Creator’s praise.
But is there not enough now seen and heard to make indifference to the
wonders around us a deep reproach, nay, almost acrime? If we have neither
leisure nor inclination to track the course of the planet and comet through
boundless space ; to follow the wanderings of the subtle fluid in the galvanic
coil or the nicely poised magnet; to read the world’s history written on her
ancient rocks, the sepulchres of stony relics of ages long gone past, to analyse
with curious eye the wonderful combinations of the primitive elements and
the secret mysteries of form and being in animal and plant; discovering
everywhere connecting links and startling analogies and proofs of adaptation
of means to ends ;—all tending to charm the senses, to teach, to reclaim a
being, who seems but a creeping worm in the presence of this great Creation
—What, I repeat, if we will not or cannot do these things, or any of these
things, is that any reason why these speaking marvels should be to us almost
as though they were not? Marvels indeed they are, but they are also myste-
ries, the unravelling of some of which tasks to the utmost the highest order
of human intelligence. Let us ever apply ourselves seriously to the task,
feeling assured that the more we thus exercise, and by exercising improve
our intellectual faculties, the more worthy shall we be, the better shall we
be fitted to come nearer to our God.
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REPORTS
ON
THE STATE OF SCIENCE.
Report on Observations of Luminous Meteors, 1859-60. By a Com-
mittee, consisting of JaMes GuatisHER, Esq., F.R.S., F.RA.S.,
Secretary to the British Meteorological Society, &c.; J. H. Guav-
sTONE, Esq., Ph.D., F.R.S. &c.; R. P. Gree, Esq., F.G.S. &c. ;
and K. J. Lowe, Esq., F.R.A.S., M.B.M.S. &c.
In presenting a continuation of the Reports on the Observation of Luminous
Meteors, it will be seen that the work is now placed in the hands of a Com-
mittee, and it is with sincere regret that in presenting their first report,
they have to announce the loss of Professor Powell, who died on the 11th
of June, 1860. The preceding twelve reports were carried on solely by
Professor Powell, but from the further prosecution of this labour he felt
compelled to retire some little time since on account of failing health, having
made arrangements for the continuation of the reports. Within the past
year there does not seem to have been any unusual exhibition of meteors,
either in August or in November; and there is little to be added to the ob-
servations themselves ; in one instance only was the same meteor seen by two
different persons, viz. that observed at Wrottesley Observatory and at Baldoyle
(county Dublin), on March 10, 1860: this meteor was remarkable for its
form and for its variation in colour, as noticed by both observers. It is much
to be regretted that the observations of this meteor yet collected are insuf-
ficient to trace its path, velocity, &e.; it is scarcely possible that so re-
markable a meteor, visible from points so distant, can have passed unnoticed,
and it is very desirable that if any observations may have been taken of it,
that they should be forwarded to the Committee, for the purpose of being
submitted to calculation.
M. Julius Schmidt, now of the Royal Athens Observatory, in a communi-
cation to M. W. Haidinger of Vienna, read by the latter at Vienna the 6th
of October, 1859, before the Imperial Academy, has made some valuable
observations upon some phenomena relative to the luminous tails of meteors,
of which a résumé is given in the Appendix. An interesting paper has
appeared in the Philosophical Magazine, April 1860, “On Luminosity of
Meteors from Solar Reflexion,” by R. P. Greg, Esq. ; a brief analysis is given
in the Appendix. In the Journal of the Franklin Institute there is a very
interesting account of a large meteor seen over a large extent of country by
daylight, on November 15, 1859; an abstract of this paper also appears in the
Appendix. os
1860. fs B
Oct.
Oct.
Oct.
Oct.
Oct.
REPORT—1860.
Appearance and
Brightness
and Colour.
Magnitude.
erent eee ee ee eeee
.|Globe form, twice the
size of Ist mag. x
star, as a spark.
15
21
21
22
23
=2nd mag. *
Equal to 2nd mag.
teeter nee
6 30 p.m.|= Ist mag. x
211
a.m.
Larger than
p-m.
of a lst mag, star.
Planetary m ap-
pearance.
Three times the size| Orange,
Velocity or —
F
Train or Sparks. Duration’
Peer ee ten enn eee e ee ennee
Leaving a streak............
No streak or
sparks.
Slight streak
separate
Tne eee eee emma tenner en neee
A streak composed of se-|Duration 0:3 sec.
= to 2nd mag*...... =tolstmag.x,!Leaving a small mass of|Rapid.
orange.
and
three times
path,
parate stars.
Duratie
separate stars in its| O:l sec.
track.
teen e eee teneenees
Lasting 2 or 3 se
No sparks .......... severe |Slow. Duratio
2 seconds, {
Direction or Altitude.
om near # Pegasi, passing
through y Aquarii to about
3 Capricorni.
om y Aquarii to 3 Capricorni
Much
red downwards from below
Aquarius.
oved from under « Ursee Ma-
joris, from the direction of
y Urs Majoris and fading
away 2° beyond » Urs Ma-
joris, having passed within
30! of this star.
oving horizontally from E.
W. and crossing over
2 Urse Majoris.
ssed between Cassiopeia and
the Pole Star, going towards
-E. Its course was a line
from Cephei to E group of}
Camelopardus,
Rete teen een ewenenees Reser reeeeeeeee
om the direction of Capella,
starting at No. 36 Aurige,
and fading away midway be-
ween 9 Urs Majoris and
Many
No. 26 in the Lynx in a space
devoid of stars.
General remarks.
in
W.S.W.
Moving on a slight
curve,
The meteors to-
night gave a
point of diver-
gence in Cassio-
ela,
peia.
Increased in bril-|
liancy and disap-
pearing at maxi-
mum brightness.
Much cloud.
Aurora Borealis.
Very bright for its!
size. During the
evening Aurora
Borealis and
lightning.
At Highfield House
at the time there
was Aurora Bo-
realis, lightning
and snow.
Lightning and
snow.
A singular meteor.|Ibid
cloud and
strong lightning
i W.~ and
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS, 3
Place,
Highfield House.
ener e neta enee
eee eeneneerene
One eaten eeeees
Diss, Norfolk ...
meteors.| Highfield House.
Peete e eens
Correspondent...
Reference,
Mr, Lowe’s MS.
Tide “10 cil
Thid.
Ibid.
A) Coccusnnacan Tbid.
4 REPORT—1860.
Appearance and Brightness : Velocity or '
Date. Hour Magnitude. and Colour. Train or Sparks. Duration.
1859. |h m 3s
Oct, 23) 8 1 p.m.|As a spark ............ Small S22. No sparks left............... Very rapid ; almo:
instantaneously
Oct. 23) 8 32 p.m.|= 2nd mag. «.........\Colourless .../No streak or train ......... Rapid.
O-2 sec.
Oct. 2311 46 30 |= 2nd mag. *, star-|Bright blue...|A streak left in its track. Rapid.
like. 0-2 sec.
Oct. 25) 2 O am./= 2nd mag. *......... IBIMOSscc5 5.0052 Withia train - j.ciuess ase Rapid.
0-2 sec.
ING Vie 2 Bebw een: 7. cccccecselcotecetoatsesee| cocenacarecatereetlee oan td oat tits on gu ccatoca nse aee URE senha et areeeeel
&8 p.m.
Nov. 2/12 45 a.m./= Istmag.*, appear-|...........ccc0ec.[escocsscescsccsccenccesscesectes Rapid :...\....:09
ed as a flash,
Nov. 3) 2 3 am./= 3rd mag.*......... Colowrless™. |Sireak: oerscjiecevnetoeoee RApIC y easvers
Nov. 3) 2 4 am.= 3rd mag.......... Colourless™:*:|Streak Vscc0c:essesesteveee Rapid ....... PP
Noy. 13) 2 50 am.'= 2nd mag. «......... pene Fe SELCHK sb ss sapeuersrtertane Very rapid ......
IN OMe S| 2219 AML Ds. veacaeeetanec ss: van Iprilbanta® 30). siissvceveramast aves canst Instantaneous...
orange scar-
let.
BMS LIA svi v0 vasigta tent akd assur aft dprotecgh caxcefuaned eles sect oa op ¥apesetgadare See ai a
till 3a.m.
Noy. 15) 8 55 p.m.|= in sizetoY¥. Globe Blue, bright Without sparks or train/Slow. Duration
meteor. till it burst, then broke) O-4 see.
into two or three small
fragments and disap-
peared.
NOW 20) 8 Op iis 5.cecceeacandtee tesco. eee eee ee Ree eee ae SEROPRORSEPEPRY foe cuteagnecssbacs:
Dee. 5 5 2 p.m.Twice the size of 2...'Colourless ...|.........s..0se00- Bs ott eenieee ISIOW.....0c000000eail
Dee. 5 6 30 pm. = aba heiress Colourless) °F 2\55..ssccseceees coe Pevstsetern sees Eo sowie cam
Bec, 5 9 25 ipim.j— Usbanmp.eric.s.-s--|...coecceteeteee es leer Meus sathonc te SEEROOO SEC | ero 4
om
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 5
Direction or Altitude.
m / Andromede towards §.
45°.
above t Draconis to near’
7 Herculis coming from the
direction of Polaris.
assed 15' BH. of bothsand x
Ursx Majoris crossing over
the star 36 in the Lynx,
moving over 20° of space
perpendicularly down.
erpendicularly down from
near No. 25 Canes Venatici.
N. about 20° below the Pole
Star,
ell down from under Polaris
at an angle of 80°, and fading
away as it reached the Milky
ay.
m the zenith
6 Persei.
erpendicularly down through
Cassiopeia.
above the N. horizon, seen
through a cloud.
Poe Pe CREP eee CES C USS eee eee reer er)
ell down in N.W. from 20°
above the horizon, disappear-
ing 10° above the horizon.
C Slight Aurora Bo-
downwards at an angle of] realis and distant
General remarks.
lightning.
Temperature 24°°5
at 4 feet, 18°°0
on the grass.
Many large me-
teors, chiefly in
N.E
towards;
Appeared, disap-|
peared, and re-
appeared four
times in rapid
succession, but
never moved its
situation.
Lightning in N. at!
the time.
12 meteors. Clouds!
numerous all
Place.
Highfield House.
Observatory,
Beeston.
evening and
night, and this,
added to a full
moon, caused
most of the me-
teors to be invi-
sible. Faint Au-
rora Borealis.
An auroral arch at
the time.
Majoris only, moving over
5° of space.
ell down in W. from the alti-
tude of 45°.
ell perpendicularly down in
§.W. from the altitude of
40°, moving over 5° o
space. ~
Tbid
E. J. Lowe
Highfield House.\Id. ............44.
Observer. Reference.
Mr. Lowe’s MS.
se SAO BEE ROSE Ibid.
DOR Sie cece ttae ce Ibid.
Capt. A. §. IL/Tbid.
Lowe.
spare hich board re Ibid.
6 _ REPORT—1860.
io }
Appearance and Brightness 5 Velocit;
Date. Te Magnitude. and Colour. Erain.or Bparks. or reed
1859. | h m
Dec, 7 7 Op.m. |Larger than Jupiter,|Reddish ...... Long streak .........06000- Very rapid. D
star-like. tion 2 secs.
Dec. 14) 9 20 pm. }=2nd mag. *......... Orange ...... Sparks: ...1 cc clbswaavvevenbae Rapid. Durati
2 secs
1860.
ans 62! 8 Open: |= 2p dnt BiZ0 Fh... se: 00-|vecns ska hlaess vc) oss snck cans snn4ss chess Faleren tthe Mita eer Ni ieee
Jan. 24} 9 28 p.m. |Increased rapidly un-|Blue............ Train of separate sparks.../Slow. Duration !
til four times the secs.
apparent size of|
Jupiter.
Many POA Mron 9) Ol cccssndeccesicdshistcusss{ecctecsossoatontce| dpgosneusG’s phaiteheooscesaesteds|Glaaaineetacsicce tam
10 p.m.
Feb. 24] 7 40 p.m. |=Venus .....cscceceeeelecsseceeeceeteoees With Calla ssiecesceonecsvoc|eobynntass ie eneceree
Mar. 2/10 40 p.m. |=four timessize of }|Bright ......... Long tail......s.ssesees Wiese BloWisvvssesccey ea va
Mar. 10] 8 40 p.m. |= Venus............... Bright as Ve-|Moderate speed, trail oOff.........:.cccsseeeuene
nus. Colour} sparks left in its track
of Venus. for 3 seconds after the
meteor had vanished.
Mar. 14} 8 45 p.m./Six times size of Ju-|Very bright, Burst into fragments...... Moderate speed ..
piter. almost like
lightning in
appearance.
Red in co-
lour.
Mar. 21) 7 15 p.m. |= Venus............... IBTignter than... .cs0s.cesesscesdentesse cress SIOW..:casssontagi 4
‘ Venus.
Mar. 21| 7 40 p.m. |= Venus............... Brighter’ thant|s.....:.:.ocssessasaetendtaceses Slow... ..<cs..005
Venus.
April 1) 8 10 p.m. |=2nd mag. « ......... Yellow......... Sani tall Oe ciecsscnecenevns SIGW Senseo. eee d
April 17/Between 10)............ssccsetesscceseecssenescecanseselenessecenavccensessensescectvesselssveessastcesseeeeesn
} & 11 p.m.
ne Observations of Luminous Meteors
Di.
Aug. 16,11 45 p.m. |Equaltothe sizeof Ju- Bluish white..{It was accompanied by a|Slow, but its dura-
i piter, but very supe- train. tion was short, as
rior to that planet it did not travel
1858. in brightness. above 5° or 8°. —
Aug. 8| 8 45p.m.|Very bright, and/Blue............ It left a faint yellow train|Moderate........... i
about the size o of light in its path.
Jupiter.
Aug. 8) 9 15 p.m. |Small but bright...... 13} rier cones Left a train visible for|Very slow .,....+..
several seconds.
Aug 8) 9 38 p.m. |Small, about size of/Moderately {No train ...............:0008. Rapid in its mo-
Saturn. bright. tion; visible for
about 0:5 second
only.
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS.
7
ee Sd
Direction or Altitude.
|
‘rom 45° above the E. horizon,
moved down at an angle
of 40°.
‘yom the Dragon’s Head, fell
down at an angle of 40° to-
wards W.
‘ell down from 12° above the
horizon in'8. by E.
‘rom the direction of Polaris,
passing midway between 3
and Leonis, crossing ¢
Leonis, and fading away
near 43 Leonis.
Feet eeeeenaee Preece eee e eee we nanos
Great Bear.
n §.W., falling towards W.;
half-way to zenith when first
seen.
m 60° altitude W. by N.,
falling down towards W. at
an angle of 75°.
Dee teweeeeeeeee
§., fell down a long distance
towards W., and passing
Annee twee meee ee ee ee neearaenee
m » Aurigs to Venus, over
which planets it crossed, and
then immediately vanished.
PERN e reenter a een eeeneeereeseeeee
from various Observers.
started 10° from the zenith,
ete west of the Milky
Jay.
ell down N. from about 45°|It was very light at|Blackheath
from the horizon ; disappear-
ed about 5° from horizon.
tarted from a point 10° below}........+
@ Aquile, taking a westerly
ell perpendicularly from 25°
above « Virginis to a little
south of that star.
General remarks. Place. Observer. Reference.
bsagedeccntiteds tetas Observatory, (R. Porter ....../Mz. Lowe’s MS.
Beeston.
Snow showers...... Mbidse asstas esses E. J. Lowe... |Ibid.
GalOscctssccsamessss = Dbitling§esdcsss. sc. Td, ~csaenss iitesis. Thid.
Sear eR Ricton res Oke bids, “aatverssses(lGsr wavsceracests:|EDIGs
Six meteors seen...|[bid. .......s.005 TAS 3s astro seee-(Lbids
se sEhdENOSADNEE.c5 econ 1 mile W. of |Miss OC. Drége...|Ibid.
Beeston.
SddedcunscgenacccstReant 1 mile N.E. of |Mrs. R. Felkin...|Ibid.
Beeston.
Hseriestanctacestutcases Observatory, |Mr. R. Porter Ibid.
Beeston. (assistant obs.)
After the fragments|Highfield House.|Capt. A. 8. H.Tbid.
were thrown out, Lowe.
the meteor still
moved on of the’
same size and
brightness for a
short distance.
Meesdenadsstodcaas tents Observatory, {Miss Lucy White/Ibid.
Beeston.
Similar to the last.) Ibid. ............ Mr. R. Porter Ibid
(assistant obs. )
Increased in size at\[bid. ...:..4.444- ra RT ‘bid.
last.
Severalmeteorsmo-|Ibid. ....... .....[E. J. Lowe ......|[bid.
ving veryrapidly.
A POREROPERICOCOOLT SOE Greenwich ......|Henry C. Cris-[MS. communica-
wick. tion.
pacar IMG etc estes const sa | DOIG
the time, and the
stars in the path
of the meteor
could not beseen.
pierise cdi ris fetes DIGS, hatise canes Tdi.) tiesaicaghas ,..{Lbid.
J JaaeanaGeioss sat ere tale pid gist .comsern| Ls sceeveceeerste.(Lbid.
8 REPORT—1860. '
Appearance and Brightness : Velocit:
Date. Hour Magnitude. and Colour. Train or Sparks. or Detaieonl
1858, |b m | | |
Aug. 8) 9 44 p.m. /Equal in size to a 4th Very bright.../It left a thin train visible Slow...............5
mag. * for about 1 sec,
Aug. 8 9 52 p.m. Rather larger than Remarkably {No train ..,.........:00000 Very rapid ......05
Saturn. bright.
Aug. 8} 9 55 p.m. \Sizeofa3rd mag.*... Very bright./A very bright train. visible SlOW. 1.1.60 «ian
Blue. for 3 secs. after the; 1
extinction of the nu- ‘i
1859. | cleus.
Aug. 26} 8 24 p.m. |Six times the size of/Much brighter ................ccssseeeeeeseeseleaseaeaesans vesveeoal
a Lyre. than a Lyre.)
Aug. 30/10 14 p.m. |As bright as Capella |.........:0scccseslscccssscesssecesseseensovenanses Visible for about 3
or 4 secs,
Aug. 31) 7 5S p.m. |... ceseeesceeeseneeeeeses [Brighterwiisan| 00 25, .ins.s.fncsaacewacareel toutes PEAR
any star then)
visible.
Sept. 22)Between _|Many shooting stars |............scccseleccccsecccseseeeentensenrecsecees Saree
sunset and
11 p.m.
Sept, 24 Evening ...|Many shooting stars |............5.0++- | a slelnoa evpacweniecael Cone ene eee [Fetes ot aieeee oa
Sept. 2810 20 p.m. Larger than Jupiter |Blue........+++. NQMC... wpe nccdae ccs ensnecounleceyreeksset nema :
hee ZB a. | sacs svn ay csnnvvesefcugasted|exonnundersefeaier|saonsnas alana tate an
Cig, 28}| Tsay Sark | Baprangeeseasceoosaccnonec: Very. bright....|Sceai.saasces Tee eee Visible for several
secs.
Oct. 27) 9° 9° p.m-|As lavge\as’ Capella... :|. 050: sscsepesses|-ccavecsonecaesoeantaev snes steeuelomemeetets Porcini
aero! 7 GG peal. «16, Scape caucpeeee od usg Roser eroanoasegte SE RACHA COLDS RIOTS IASB NGA: Very rapid .,..,..
Nov, 7/ 9 33 pm... .sesceeeeeseneeneerenees As, bright) Wey. cepsovasesccpsmstoeenia ends (eemeemeanene ee er
Capella.
Noy. 9} 5 30 am. About 2° long......... Colour of red-|No sparks were seen ...... Its greatest bril-
hot iron; its liancy lasted fo
illuminating 30 seconds, buti
power very remained visibl
great. for 10 minutes.
Nove 10) 9°40! pail... .cceneurcunsaeceeress Faint yellow. .'They left a train, similar'...........s00.:0000 “
to a faint streak.
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS, 9
—————
Direction or Altitude. General remarks. Place. Observer. Reference,
ell from a little KE. of the Great)... ieee eee! Blackheath ...... (Henry C. Cris--MS. communica-
Bear constellation diagonally’ | wick, | tion,
towards the N.W., disappear-
ing about 20° above the hori-
zon.
m 30° above the due §8.\Just before disap-\Ibid................ 1G BOR sacee eenre Ae ‘Tbid.
horizon ; it went by W. to! pearingbelowthe|
the horizon. horizon I di-
stinctly saw it)
separate, giving,
at the same time
a report like that!
; of a distant rifle.|
rom 40° above the E.S.B. ho-)..........cceeseeeseeees pid sesacpenve sett IGM) appear ate Thid.
rizon to §.E., disappearing
25° above the horizon.
ell perpendicularly from near)............cc.cecseeens Wrottesley Ob-)W. P. Wakelin. |Ibid.
a Ophiuchi to within 15° of servatory.
the horizon.
ell from 10° above » Ursx/This meteor paled Ibid.......,........ ees Rate Sere Tbid.
Majoris, between » and Z, to} twice, and at-
within a degree or two of] tained its maxi-
12 Canum Venaticorum. mum brightness
just before its
disappearance.
rom near w Cassiopeiz Gia-|,..............cseeeceee| Tidserocabevccstet TC Eee eee Tbid,
gonally towards a point north
of « Persei.
bout Pleiades, moving W. to)............c.ccccseees (Ballater ...,...,.| J. H. Gladstone. |Tbid.
Ee lage. ae: id. eee Ibid.
orthern hemisphere; it fell)... eee Fort William, {Myrs. J. H. Glad-|Ibid.
from W. to E. through 25°, Scotland, stone,
descending from an altitude
of 35° to about 25°.
few degrees 8. W. of y Pegasi./It attained itsmaxi-/Wrottesley Ob-|F. Morton, Tbid.
mum _ brilliancy) servatory.
immediately be-
fore it disappear-
ed.
descended vertically from the}...............s000000- 1] ays beadgnsonabponee Ne eiasgeeapsosase Thid.
constellation Draco to within
10° or 15° of the horizon.
iE, from about 35° or 25°)..........cssccesseees CL ere Rare W. P. Wakelin. |Tbid.
altitude.
om midway between the Con-|............sseeeeeeeees iQ OEE" waRHocECCONre F. Morton ,..... Tbid.
stellation Lyra and Hercules,
at an angle of 45° to S.
rom near 6 Pegasi, at an anglel............ccssece eee DIG Ona thece saa: We Srepccpapencies Ibid, e
of 45°, to within 10° of the
§.W. horizon.
bout the same altitude as the|As it paled it got\Ibid. ............ ‘The under-gar- MS.
Pleiades, and some 8° to the) gradually shorter dener at Lord
south, and wider; it at Wrottesley’s,
last looked like a the times by
faint cloud. | F. Morton.
m Capella to irius......... They were three in;Manchester ...... G. V. Vernon,
number,
10
h
37
Feb. 16
Mar. 3
Mar. 10
|Mar. 10
REA Final: emawecenesas cede daenoseag
REPORT—1860.
Appearance and
eer Magnitude.
m
10 p.m.|Its brightness was
equal to that of a
* of the Ist mag.
10 35 p.m.|2nd mag.
9 30 p.m.
9 20 p.m.
eee ee eee eee CTO eee ere eee
9 20 p.m./The appearance gave
the impression of
3 feet in length. Its
form was strictly
defined, the front
portion being in
shape like the head
of a lily, with a
petal-shaped _out-
line. From this it
diminished grace-
fully to the tail,
not in straight-
sided lines, but in
curves. The tail
was the small-
est, and apparently
the most concrete
portion of the
whole.
9 32 pm.|A bar of light in
length equal to
moon’s diameter,
its breadth 3th o
its length.
Same
Scarlet,
Brightness
and Colour.
colour
as Rigel.
Velocity or
Train or Sparks. Duration.
No apparent train Very rapid ......008 {
errr reer ere rer ererrrrire rrr creer ere reer rr
pea-
green.
and of a red-
dish colour.
Bright
brightest
moonlight.
Colour di-
stinct and
varied, the
head pearly
white, the
tail bright
ruby, with
reddish-
brown extre-
mity,and the
middle por-
tions mark-
ed by bands
of various
shades of
colour.
At first its
colour was
pure white,
and as bright
as Sirius.
In its full
the colour
changed to
green, and
afterwards to
a deep glow-
ing crimson.
as
The outer portion of the
stream was composed of,
bright scarlet scintilla-
tions.
Lasted 5 seconds,|
slow.
oe
It left behind a train of/The whole time was)
pale yellow light. 2 secs. 4
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 11
Direction or Altitude. General remarks. Place. Observer. Reference.
(t fell from near the zenith,|.................0cec00 Manchester ...... G. V. Vernon.
passing, through Orion’s Belt,
and disappeared when on a
level with Rigel.
assing nearly horizontally]...............:.cceee0s Hendon’ ......... Mr. W. Grubb.
through Ursa Major.
£ an elevation of about 600/After dropping per.'Sidmouth ...... T. H. 8. Pullen.
feet its direction was 8.8.H.| pendicularly for
a short distance
it separated
itself into about
eighteen globu-
lar masses of dif-
ferent colours,
some about 8 or
10 inches in dia-
meter, and the
others from 1 to
3 inches.
t fell from an elevation of 60°|.........ccsecseeeeeeeee Osborne ......... J. R. Mann.
and N.N.E., and disappeared
in the N. E. at an elevation
of about 10°.
bout 50° in a N.E. direction.|After falling about|Coleraine.
: 50°, it burst into
a number of|
sparks, like a
rocket.
direction was that of a/About 30 secs. after|Baldoyle(county/J. P. Culverwell, Mr. Lowe's MS.
Dublin). E
line drawn from Orion’s Belt,
through the Pleiades, and
onward to the W. of Cassio-
. disappearing in the
partion of tp hemi-
sphere.
the disappearance
of the meteor
there was a low
rumbling thun-
der in the N.E.,
which continued
sq.
fully 2 mins.
Vers ched tts MS. communica-
tion,
was seen at an altitude of 45°,|The stars for 15° Wrottesley Ob-J. H.
on each side of
its path were
paled as by the
presence of the
full moon.
and darted perpendicularly
between the Pleiades and Al-
gol to the horizon.
servatory.
12 REPORT—1860.
a
Velocity or
Duration.
Appearance and Brightness
Magnitude.’ and Colour.
Date. Hour. Train or Sparks.
1860. |h m
Mar. 10) 9 50 p.m./It appeared about/Very bright, at}...........csseeseseereeseeeeeees Visible for a secon
2rds of the size of first purple- or two.
the moon. red and
then green,
= Venus.
DME |e Ol aeIM.| eacccesveusnesresseereres- Very brightiz.:| Aessseessat Winer coneesrsteavees 2 or 3 secs. sesevenns
April 14) 9 4 pumi}.c.cesceeeeeeeesenseeseees Hiqual to VAI=| erica taevanvecsssnsssepecucen| sucnyeestshepa <x cneem re
debaran in
brightness.
April 26] 7 52 p.M.)..ccccccscesscceeereereenes At first bril-/It left a very luminous tail! It was visible about
liant white,| behind it. a second.
and = after-
wards pur-
ple-red.
APPENDIX.
No. 1.—In the Journal of the Franklin Institute, Philadelphia, February
1860, is a collection of observations of a very remarkable meteor seen by
daylight, on November 15, 1859, by Benjamin P. Marsh, Esq.
This meteor made its appearance at about half-past 9 o’clock a.m. (New
York time), the weather being perfectly clear, and the sun shining brightly.
It was seen at Salem, Boston, and New Bedford, Massachusetts; Provi-
dence, Rhode Island; New Haven, and many other places in Connecticut ;
New York City; Paterson, Medford, and Tuckerton, New Jersey ; Dover,
and other places in Delaware; Washington City ; Alexandria, Fredericks-
burg, and Petersburg, Virginia.
It was heard at Medford, New Jersey, and at all places in that State, south
of a line joining Tuckerton and Bridgeton, and throughout nearly the whole
of Delaware. :
With perhaps two or three exceptions, it was not seen by any one in New
Jersey, south of the Camden and Atlantic Railroad ; that is to say, through-
out the very region where the report was loudest.
Many persons there saw a momentary flash of light “like the reflexion of
the sun from a looking-glass,” but could not tell where it came from. The
appearance of the meteor as seen at many places is described, and the results
from their discussion are as follows :— :
1. The inclination of the meteor’s point to the vertical was probably about |
35°, and the direction of its motion nearly west. The observations at Med-
ford and Petersburg indicate a much more southerly movement, but those of .
Washington, Alexandria, and Dover, require it to have been almost due west. |
2. The column of smoke was near 1000 feet in diameter, and its base was
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 13
Direction or Altitude. General remarks. Place. Observer. Reference,
Tt fell at an inclination of N.W.|It travelled about Bradford......... M. D.
to W. 15° and then W. W. M.
burst ; it appear- E. M. C.
ed at first as J.C.
though the moon Cc. W.
had fallen to the
earth.
BING SO 5 ccosssccesssvctesoes It appeared sta-/Torquay ......... FR. Vivian.
tionary, but in-
creased in bright-
ness for 2 or 3
seconds, when it
suddenly disap-
peared.
¢ darted from a point half-Its path was con-|Wrottesley Ob-|J. H. ............ MS. communica-
way between the Pleiades} cave to the hori-| servatory. tion.
and @ Persei to a point about} zon.
one-third of the distance
from Aldebaran to « Aurige.
t fell from the zenith to the)......, eis depanySieeeaey op Manchester ...... G. V. Vernon.
vertical about four miles north of Dennisville, at a height of near eight miles,
which may be assumed to be the approximate position of one point in the
meteor’s path. The height is inferred not merely from the angular elevations
of the smoke as seen from different points, but from the interval between the
flash and the report, as observed at Beasley’s Point. This position assigned
to the base of the cloud, from local reports, coincides pretty nearly with that
indicated by distant observations.
At New Haven, latitude 40° 18’ 18", longitude 72° 55! 10", at an eleva-
tion of 6°, the bearing was S. 35° 34! W.; and at Alexandria, latitude 38° 49',
longitude 77° 4', at an elevation of 102°, it was N.763° E. These directions
meet half'a mile west of Dennisville in latitude 39° 112/, longitude 74° 502/;
the line from New Haven having a vertical height at this point of 292
miles, and that from Alexandria 243 miles. Continuing the path, as ob-
served at Alexandria, down to 94° elevation, we have corresponding azimuth
764°, and the lines then meet half a mile north-west of Dennisville at a
height of 225 miles; but this makes the nearest point in the meteor’s path
twenty-four miles from Beasley’s Point, and consequently the interval there
between the flash and the report two minutes instead of one, as observed.
Besides, the observations on the smoke show pretty clearly that the minimum
height at Dennisville could not have exceeded ten miles. We must there-
fore conclude the meteor’s actual position to have been several miles east of
that indicated by these distant observations.
3. On the above supposition, the meteor’s path would reach the earth near
Hughesville, on the north-western boundary of Cape May County, in which
Vicinity, or perhaps still further west, it is probable that the meteor or some
of its fragments will yet be found.
4. Some observers must have seen the meteor at a height of more than
14 REPORT—1860.
100 miles; and, to have completed its path within their estimates of time, it
must have had a velocity of from thirty to fifty miles per second.
The extreme shortness of the time occupied in its flight, is proved not
merely by the estimates of several observers, but by the failure of people in
the vicinity of the explosion to distinguish the source of the sudden flash of
light seen by them, and by the impression of even the most distant observers
that it fell very near them.
5. The sound was explosive, and moé caused by the falling in of the air
after the meteor. In the latter case it must have been continuous and un-
interrupted, but the testimony of Dr. Beasley and others shows that it ceased
entirely and then began again.
Supposing the meteor to have been a stony mass, we may, perhaps, con-
sider the explosion to have consisted of a series of decrepitations caused by
the sudden expansion of the surface, the whole time of flight not being suffi-
cient to allow the heat to penetrate the mass. At the forward end these ex-
plosions would take place under great pressure, which may account for the
loudness of the sound.
6. The estimated duration of the sound at Beasley’s Point was not less
than one minute, indicating that the most distant point of the explosion was
not less than twelve miles further from that place than its nearest point.
Comparing this with the position of the assumed path, we find that, during
the explosion, the meteor must have travelled fifteen or twenty miles, occu-
pying about a second of time.
7. The explosions were very numerous, arranged in two series, the whole
occupying only half a second of time, but the individual sounds were distin-
guishable, because of the different distances they had to travel to reach the
ear. The velocity of the meteor being more than 100 times that of sound,
the reports must have come in the order of distance and zoé in the order of
their occurrence, causing the end of the explosion to be heard before the
beginning. The faint rushing sounds first heard by Mr. Ashmead must
have had their origin below the explosion, and been caused by the flight of
the fragments towards the earth. If the direction of the first faint sound
could be indicated by persons further west, it might serve to point to the
place where the fragments fell.
8. The meteor lost its luminosity with the explosion or shortly after, and
hence was not seen by persons in Cape May County and vicinity, it being
too much overhead to come within the ordinary range of vision, and the time
of flight being too short to allow them to direct their eyes to it after seeing
the flash.
If the heat be due to the resistance of the air, it must be principally deve-
loped at the surface of the forward half of the meteor. Consequently
most of the explosions must occur then, and the force of each be directed
backward, tending to check the velocity of the mass. In fact, we may per-
haps consider the series of explosions to be merely one of the forms of the
atmospheric resistance. This must increase rapidly with the density, although
it may be insufficient to account for so great a reduction of speed as would
entirely destroy the luminosity of the meteor before it reached the earth.
9. Irom the tremendous force of the explosion, and from the fact that this
meteor was seen by persons who were not within 200 miles of any part of
its path, as at Salem, Massachusetts, and Petersburg, Virginia, we must cer-
tainly conclude that it was of very considerable size; but we seem to have
no data for any approximation to its actual dimensions. It was certainly
heated to a most intense brightness; and the experiments of Professor
J. Lawrence Smith, detailed in Silliman’s Journal, vol. xix. fol. 340, second
a. te
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 15
series, in which he found that a piece of lime, less than half an inch in dia-
meter, in the flame of the oxyhydrogen blowpipe, had, when viewed in a clear
evening, at the distance of half a mile, an apparent diameter twice that of the
full moon, show conclusively that no reliance can be placed upon calculations
founded upon the apparent diameter ef bodies in a state of incandescence.
10. The apparent form of the meteor, that of a cone moving base fore-
most, may have been due to its great angular velocity, combined with the
effect of irradiation above referred to. ‘The impression made upon the eye
by the incandescent body itself, would doubtless be greater than that made
by the sphere of light surrounding it. Consequently we should continue to
see the body itself after the impression of the mere glare had faded awav ;
so that the apparent diameter of the end of the tail may represent the actual
angular diameter of the body.
11. The invisibility of the meteor to persons at Philadelphia and vicinity,
was no doubt due to the position of the sun, the direction of which then
coincided with that of the meteor.
No. 2.—Abstract of a paper by R. P. Greg, Esq., F.G.S., in the Philoso-
phical Magazine, April 1860, “On Luminosity of Meteors from Solar Re-
Hexion.”
With reference to the cause of the luminosity of shooting stars, the author
proposes to prove that their luminosity cannot arise from solar reflexion,
a theory partially supported by Sir J. Lubbock and others. He observes
that the very sudden appearance and disappearance of shooting-stars and
small meteors, and their general resemblance on a small scale to comets which
shine by solar reflexion, certainly favour the idea, either that suddenly enter-
ing the cone of the earth's shadow they are instantly eclipsed, or conversely,
become visible as they emerge from it; or secondly, previously self-luminous
in planetary space, they may become suddenly extinguished on entering the
denser atmosphere of the earth; or thirdly, they may suddenly become visi-
ble and luminous only on entering the earth’s atmosphere by friction and
compression, by rapid absorption of oxygen and sudden chemical action, or
by electrical excitation.
The author then refers to Sir J. Lubbock’s paper in the Philosophical
Magazine for February 1848, and shows by a different treatment how un-
likely, if not impossible, it is that ordinary shooting-stars (those not show-
ing symptoms of active ignition within the lower limits of the earth’s atmo-
sphere) can ever shine by reflected solar light ; and this simply from the fact
that they would be too far off for us to observe such small bodies, at even
the minimum distance at which (at certain times and places on the earth’s
surface when and where we know they are very frequently seen) they
actually could be so visible; and concludes his paper by remarking that, if
his calculations, &c. be correct, the majority of shooting-stars do not shine
by reflected light.
No. 3.—M. Schmidt on the Luminous Trains left by Meteors, &c.
M. Schmidt repeats an observation of M. Faye’s in the ‘ Comptes Rendus,’
vol. xxxii. p. 667, relative to the small amount of moveability in the tails or
luminous trains not unfrequently left by meteors, which seems to prove that
the former must be found in the atmosphere belonging to and surrounding
the earth, and not in the firmament which lies beyond it. M. Faye observed
one of these tails through the telescope, and he saw it “lingering for more
than three minutes, without changing its place very perceptibly.—Other
observers have observed them to remain for more than seven minutes.” M.
16 REPORT—1860.
Schmidt remarks on the strangeness of this stationary condition of the lumi-
nous trains of meteors, likewise on the cloud-like appearances generally left
by detonating meteors even in the day-time, when we come to consider the
enormous velocity of the meteors themselves through the higher regions of
the atmosphere ; but he says, “ we must recollect an easy and interesting ex-
periment, by which we may obtain a similar result. If you take a common
lucifer match, still burning, or when it is just about to become extinguished,
and throw it from you in any direction, either quickly or slowly, you will
in many cases perceive, either a straight immoveable line, or an undulating
or curling line of white-grey smoke, standing still in the air, if the air is calm
and not in motion.”
M. Schmidt observes how important observations, whether telescopic or
otherwise, are respecting the tails of meteors,—I1st, as regards their proper
motion; 2nd, the downward curvature sometimes exhibited by them, and
the way in which they break up and disperse; and 3rd, the means they may
afford of ascertaining by parallax their height above the earth, a matter of
very great importance for ascertaining at what heights the atmosphere ceases
to have any influence.
M. Schmidt then proceeds to cite a number of instances from his own
catalogue of meteors, where tails have been observed of long duration, or as
offering very peculiar appearances: e. g.
1664. Aug. 3. A very large meteor with curved tail, seen at Papa, Hun-
gary.
1791. Nov. 11. At Gottingen and Lilienthal, a meteor left an undulating
tail of a shining white colour, in parts alternately showing the prismatic
colours ; then became more curved, and turned into vapour of a pale yellow-
ish colour before finally disappearing.
1798. Oct. 9. Brandes witnessed at Gottingen how the tail of a bright
shooting-star bent itself within 15 seconds like a bow.
1840. July 30. Ditto at Vienna, in 15 seconds also.
1845. Oct. 24. Schmidt observed at Bonn the change in the form of the
tail of a meteor in 4 minutes; it became severed and bent, and dissolved
into small grey clouds. The whole mass moved 1° from its original place at
final disappearance.
1852. Oct. 26. A large meteor seen in Pomerania, left behind it a spiral
tail 3° long, which contracted soon into a ball, and again passed into a spiral
curve, finally assuming the shape of a capital Z.
1854. Aug. 1. At Gottingen, a fine meteor left behind a bright tail 3!
wide and 2° in length, lasted 8 or 9 minutes after dividing itself into three
oval balls, and showing at first uneven undulations or knots, while the tail itself
shortened and became more likea W. Whilst these changes took place in the
tail, the whole mist-like mass moved along the sky in a nearly opposite direc-
tion to the motion of the fireball itself; the tail had thus moved 9° in 8 minutes.
1859. Aug. 9, 10, 11. During these three nights, M. Schmidt at Athens
succeeded in observing, on four different occasions, the curving of meteor-
tails through the telescope. The whole time, in three cases of visibility, was
170", 140", and 220" respectively ; in one case only 10" or 12". The curva-
ture of the tail began to be perceptible almost directly after the meteor
vanished, and the proper motion in one direction very decided. In one of
these cases, viz. on Aug. 11, a bright orange-coloured shooting-star left a tail
visible to the naked eye 4" or 5", but through the telescope 220"; the direc-
tion about from E.N.E. to*W.S.W. The following figure shows the real mo-
tion of the tail, compared with the apparent motion of the shooting-star.
The tail finally broke up into a number of small fragments.
|
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 17
ab, the apparent motion of the shooting-star.
a, tail at end of 5th second.
(, tail at end of 12th second.
y, tail at end of 180th second.
6, tail at end of 220th second.
A B, apparent motion of the tail nearly at right
angles to a b.
Aug. 9. Representing, after another meteor, a
similar movement of tail as compared with
the meteor itself.
B
M. Schmidt states that credible cases, where the tails of meteors and shoot-
ing-stars remain visible lunger than 5 seconds, are very rare and isolated. He
cites thirty-nine instances from his own catalogue, of which we select seven
instances of longest duration.
1751. May 26. 3" 30™"...... Kraschina (Agram meteoric iron fall).
fea0g.Oct. 10. 1° «...ee On the high seas.
1840. July 30. Lo én ee ae), Vieniias
1847. Jan. 10. LOM sess.» Vienua.
1847. Nov. 10. YO" ...... Benares.
1853. Aug. 26. 107 eae oe Mazzow.
1856. Oct. 29. 30™....2.. Laybach.
Among the thirty-nine instances given by M. Schmidt, there were more
than one instance of the tail winding or doubling itself up, nay, of even
vanishing and then re-appearing.
Duration of Meteors.
M. Schmidt also offers further remarks on the duration of meteors, and he
observes how rarely they are visible for more than 1 second; that 0! 2! to
1’ 5" is the usual time of visibility ; the practised observer knows that the
majority in fact of shooting-stars only shine during the fraction of a second.
In all probability the short moment during which the light shines is at the
same time the moment of its partial and final extinction.
The time during which a shooting-star is visible is a subject for the art of
more refined observation, and M. Schmidt hopes that much attention will be
directed “towards determining the duration with regard to colours and any
anomalous motions of meteors.” In his treatise on Meteors, p- 15, M. Schmidt
states how long the tails or luminous trains of meteors remain visible, with
regard to colour, viz. as follows:—
sec. Mean error.
With white meteors, the mean =1-00 in 24 observations.... 0°05
With yellow meteors, the mean=1'51 in 18 observations.... 0°15
With green meteors, the mean =1-96 in 12 observations.... 0°29
| 1860. c
18 REPORT—1860.
On the other hand, at p. 50, the time during which tails are visible upon the
whole number, with regard to these different colours :—
sec.
‘Time of duration for pe atte ay =0°85 in 64 observations. .p. 1849.
Time of duration for ae cota =0'90 in 80 observations. a.p. 1849.
ibm ot iumeaoe snd lceee oe to = 128 in 14 observations. a-p. 1849.
"Time of duration. for ite le a =1:60 in 5 observations. a.p. 1849.
aap tte tcehe Avesta ee =0-91 in 12 observations. a.p. 1849.
Likewise in the year 1850 the longer duration of the coloured meteors
showed itself in the following proportional means :—
secs.
Duration of the white =1-16 in 12 observations.
Duration of the yellow =1'25 in 8 observations.
Duration of the yellowish red=1°41 in 6 observations.
If we consider the time during which the light of the meteor itself lasted
without regard to any other phenomena, we find in his catalogue the follow-
ing instances which show that in the case of many thousand observations
it is very rare that a shooting-star or meteor remains visible for more than 5
seconds.
Date. Duration. Place of observation.
secs.
1783. August 18 s..ccocsss+scenteejn 6 GO, |Lendon.
184.2. November 1.........e0.00.6-, LO | |Hamburg.
1842. November 7......cecseeseeves} 10 | |Hamburg.
1842. November 21 ......ssseeeeee $ |Hamburg.
1843. September 19 .........ceeee 7 | |Hamburg.
1843. September 22 ,,,...seceeeeee 9 |Hamburg.
1844. August Lh ccsesssadsnare: cer 6 |Hamburg.
1846. August TO ccssesssdesces ees 8 (Bonn.
1847. November 29 ......seeserees 8 |Bonn.
1851. September 26 ..........c000. 11 Minster.
1659 November S$” \ i. .icessene. 0s 10 =‘ |Miinster.
LOS; “August Is. .5,.scessauereses< 35 _ |G6ttingen.
1854. December 8.......2.se0ceee00| 8 |Vienna.
1656: October Zon cesssevenscees 12 |Laybach.
1857. ? sda fectee to gee ne. Mae | Mere
1859, July 27 ieecdsivsgeeesaceee] «12 Athens: for 967 are
The following remarks on the hypothesis that the intensity of the light
of the meteors is caused by the oxygen in the atmosphere, are here translated
verbatim from M. Schmidt’s communication to M. Haidinger :—
“In consequence of the observations which were then being made by Ben-
zenberg, Brandes, Felder, Heiss, by myself and others, in the year 1851, I
examined into this question more closely, and I arrived at a result which was
* Mr. Greg found one account of this meteor stating it was 20”, seen in an are of 75°.
om
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS, 19
indirectly opposed to that hypothesis: since it is a difficult matter thoroughly
to refute old objections, however untenable, I may perhaps be permitted here
to refer to them, and to refer to numbers instead of to opinions.
“ We all know that the intensity of the light of shooting-stars is estimated
according to the brightness of the stars, and we therefore, e. g., say that a
meteor is of the first magnitude when its light equals that of Arcturus or
Vega. If it shines brighter than Jupiter or Venus, we designate it a small
fireball. If we put such numerical values for the shooting-stars so as to
express the intensity of their light, and if we call A the mean height of the
shining portion of the luminous track above the surface of the earth, we
obtain the following mean proportional values, which, in the year 1851, I
deduced from the observations then made (see my work, p. 111) :—
Meteor of Ist magnitude, k=16:2 geographical miles, for 14 observations,
Meteor of 2nd magnitude, A=15:°9 geographical miles, for 20 observations,
Meteor of 3rd magnitude, A=10°8 geographical miles, for 24 observations,
Meteor of 4th magnitude, k= 8:5 geographical miles, for 21 observations,
Hence, therefore, it follows that the large meteors belong to the highest
regions of the earth, where, as we generally suppose, there exists scarcely any
air at all; that, however, the small meteors which have a feeble light are seen
nearest to the earth, and occupy the limits of the atmosphere, where the latter
still exists in a greater and more perceptible degree, and that they descend
still lower. It is therefore not the oxygen of the air which is in the main the
chief cause and origin of the burning or glowing of the meteors.”
Note by Mr. Greg.—That the smaller shooting-stars are frequently nearer
than the larger meteors, may possibly be still further supposed to be true,
from the fact that usually they are seen to move more rapidly than the larger
ones. Still exceptions may exist, as in the case of very large, and probably
aérolitic fireballs moving horizontally and parallel to the horizon.
The height at which meteors are not merely luminous, but can leave nearly
stationary trains of light, is truly surprising; one would almost have
imagined, at that distance from the surface of the earth, some retardation in
space of the attenuated and upper stratum of air, as compared with the rapid
movement of the earth on its own axis.
It is to be regretted that the extreme limits of the auroral regions are not
yet more precisely ascertained ; but it is not improbable that shooting-stars
are commonly visible, or luminous, precisely in that very region, and that
their luminosity may to some extent be owing to electrical excitation.
No. 4.—In the ‘Comptes Rendus,’ vol. xxxvii. p. 547, M. Coulvier-Gravier
gives a list of 168 bolides observed from 1841 to 1853, classed as follows:—
Istisizenas sa sevetectevess Bl
Ind SiZG, ess evseenieestere OO
Brdheigers, sore yesscaied octe _98
168
of which latter, viz. those of the 3rd size, he states as being larger or brighter
than Jupiter or Sirius; the relative or absolute size of the two other classes are
notstated. These three classes described average arcs or paths as follows :—
(1) 31... are of 42° 4!
(2) 39... are of 26° 7!
(3) 98 ... are of 22° 7
c2
20 REPORT—1860.
Their directions at different hours of the night, and numbers, are given in
the annexed Table :—
6pe.m.to10p.m.|10P.m. to 2 a.m.| 2 4.m. to 6 A.M.
Directions. Number. Number. Number. Totals
N. 2 Ze Hae 4
N.N.E. 2 A 2 4.
N.E. 3 4 1 8
E.N.E. . 1 5 y 8
E. 1 Us 2 10
E.S.E. 8 8 1 qs7
S.E. 4 8 1 13
S.S.E. A 9 5) 16
8. 4. as 3 £4
S.S.W. ] 4. 5 10
S.W. oe 8 5 13
W.S.W. 3 5 1 9
Ww. 1 3 g 6
W.N.W. 6 9 8 93
N.W. 4 4 6 14
6
a ee
The 44 bolides which were observed froin 6 p.m. till 10 p.mM., were seen
during 6943 hours of observation, which gives one bolide for 15 hours
47 minutes for that part of the night, of which the average is 9 o'clock.
The 76 bolides from 10 p.m. till 2 A.M. were seen in 8483 hours of obser-
vation, which gives one bolide for every 11 hours and 10 minutes for the
second part of the night, with the mean of midnight.
The 48 bolides from 2 A.M. till 6 A.M. were observed in 340 hours, which
gives one bolide for every 7 hours and 5 minutes for the third part of the
night, the mean being 3 A.M.
The number of bolides being therefore inverse of the times as above, for
each bolide, if one allows 100 for midnight, we should find from
No. of bolides,
6 10 10, average 9 P.M. ...... = 71
10 to ¥, average midnight ... =100
2to 6, average 3 A.M. ...... =158
The number of bolides seen about 6 A.M. is triple the number of bolides
observed in the evening, a result which accords with the horary and usual
variations of shooting-stars generally.
Out of 168 bolides observed, there were 101 which left longer and shorter
trains of light of different degrees of duration.
Out of the same number there were 20 which burst into sparks after a
course more or less arrested by the rupture.
Lastly, there were 8 which changed their original velocity, or became sta-
tionary in their course; two which changed their direction towards the end
of their path, and ove which had an oscillatory movement.
M. Coulvier-Gravier elsewhere remarks that 6th magnitude falling stars
have arcs or paths of from 40° to 9°.
ca
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 21
In the ‘ Comptes Rendus,’ vol. xlv. for 1857, p. 257, M. Coulvier-Gravier
remarks, in a series of observations on the August periodical meteors during
a period of twelve years, that the maximum number per hour, from 9 P.M. to
10 p.M., are seen between the N.E. and E.N.E. to 2° 5! of N.E. From 2 to
3 A.M. between E.S.E. and S.E., 3° of E.S.E. From 9 p.m. to 3 A.M. the
maximum has advanced 65° towards the South (or 11° per hour); so that
one would conclude that at 6 a.m. the maximum would be between the S,
and S.S.E., 7° of S.S.E.
The above is also confirmed by the general result for other months of the
year, 7. e. the maximum for August being in the morning between the S. and
S.S.E., the general average for the year, of shooting-stars, being E.S.E.
Mr. G. C. Bompas’s valuable generalizations on this fact of the number
of meteors increasing regularly from 6 P.M. to 6 A.M., as that the number
appearing in the East is double the number originating in the West, are given
in a résumé at p. 131 of the volume of the British Association Reports for
1857, held at Dublin.
No. 5.—Mr. R. P. Greg gives the following results, taken from a catalogue
he has constructed of the most remarkable meteors on record, as regards
their general observed direction ; without reference, however, to the precise
hours of observation, a matter probably of less consequence in very large
meteors moving near the earth’s surface, than in the case of ordinary sporadic
shooting-stars.
Month. No. of observations. General direction.
January ...eceee. Li N.W. to S.E.
February ...... 20 ?
March | <<... 13 §.E. tO N.W.
PANU ssc ts deaees 21 N. tos.
Bae Vi ieasde- 15 E. to w.
AIRING Weck aancsec.. 18 P
Ge Tak cencbaas « 14 S.E. to N.W.
PLUSUSE f.5. casees 24 ?
September...... 22 N.W. tO S.E.
October ......... 19 w. to E.
November ...... 39 N.E. to S.W.
December ...... 15 N. to s.
The number for each month here varies quite accidentally, as details con-
cerning precise direction are frequently wanting in the various published
accounts of these phenomena.
REPORT—1860.
22
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23
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS.
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TABLE II.—Days of the Month on which Bolides cr Aérolites have been observed and recorded.—R. P. Greg.
24 REPORT—1860.
1
SH OOD 1D Hh 1D HOD OH 9 19 09 OD LD IDNA CD HINO NON SO OD HNN
lO AHKHA OCHA RDA MANANAANMH OR AN HAHAHA
HIOANIMDOOOAHARANMOWVAMM MAOH 121A HOA
= oe | .
July.| Aug. | Sept.| Oct. | Noy. | Dee.
=
= AAANAND 1NANOOCHNMAEOANHNAANHHAMAMDOUMWA
3 :
m
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as) 3 3 . : Z
; EB CODA AAAANTHA POONA AHMOANHOG Fs ENN fo
ia) r |
Bl acne IMMA aIeD fee imc
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mm 2 F see ee
a Oa st 500 A160 09 69 OD I OT 69 19 1D sets St NOD dH fie
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o e ims ie
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3 rt ’
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fat a ered, SG: 5 srt ICY SCs Sire OT as Ba | rh ae ea
by
Noy.
Oct.
nq | 3 , : aa one) -, Sans
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s|n
8 ep s : Pe ve ae A A ie rin
ct} 3 Sia: Koy Whos Tear St Nac ae OL Pea Geers swe cn chee
Fig ede
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3 a:
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o nas :
a) ae)
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5 5 IHN AAAN PARA HA IAM EP INRA in Pi inn iN
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& | btw: ei) Bsr ee ee Ai
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Sane AGA PHORM IMAGHA ? PHAN :
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& St SOT oe SS Re) ett
Lan)
A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS.
Aérolitic epochs
common to meteor
Analysis of Taste II.
Aérolitic epochs
probably distinct
Times of fewest
aérolites.
Times of fewest
bolides.
epochs ? from meteor epochs.
6—10 February? | 8—10 January. Jan. 18—Feb. 6. February ...24—31.
11—22 July. 1422 March. sAnaisly oo 20—25. | April ...... 19—26.
4— 7 August. 5 April. April 29—May 7. OMG, Yecien 3— 8.
- 1— 6 September. | 17—21 May. August ...21—31. | June 24-30.
1— 5 October? 3—16 June. September 17—30, | July...... 1—10.
9—13 November. | 3— 8 July. Dec. 16—Jan. 7. September 12—19,
27—30 November.
11—15 December.
Observations on the preceding Tables, Se.
1. While the number of bolides is considerably larger for December and
January than for June and July, the number of aérolitic falls is about as
large again for the latter as for the former period; the earth in her orbit
in the first case being at her perihelion, in the latter at her aphelion.
2. The distribution of the larger class of meteors is not so unequal
throughout the year, if we make allowance for the immense number usually
periodically observed in August and November, when meteors as large in
apparent size as Jupiter, or even Venus, are not uncommon. March, May,
June, and July furnish out of the total number generally observed of meteors
of all sizes, the largest proportion of bolides, and especially of aérolites.
3. There is a remarkable equality in the numbers of aérolitic falls for the
first half of the year as compared with the second half, viz. 103 and 101 re-
spectively. There does not appear to be any very remarkable preponderance
in this class of meteoric phenomena during the periodic epochs for shooting-
stars, 7.e. about the 9th of August and 10th of November. In the analysis of
Table II. these epochs are more fully pointed out. There appear to be
aérolitic epochs entirely distinct in themselves ; and it is worthy of remark
that these epochs are apparently most distinctly marked, with regard to shoot-
ing-stars and boiides only, during the first six months of the year; whilst all
the epochs possibly common to both classes are seen to occur in the second
six months of the year, with the single exception of one in February.
4. Analyses of several catalogues are concisely given in Table I. for the
purpose of convenient comparison. They vary more or less from each other,
though not very materially; necessarily in constructing such catalogues,
some latitude and difference of opinion may exist respecting what constitutes
a proper bolide; and recorded observations may not always be very definite.
If meteors of the size of Venus or Jupiter were included without discrimina-
tion, the list of fireballs for August and November might be swelled out in-
definitely ; e. g. hundreds of meteors of that size were seen on one night
alone, November 13, 1833, in America. The practice of late years of look-
ing out more particularly for shooting-stars at the usual August and Novem-
ber periods, probably tends to increase disproportionately in all catalogues
of bolides, the number of observations for those two months, though the
November period appears for the present to have become very much less
remarkable for meteoric displays than formerly.
In constructing his own catalogue, Mr. Greg has endeavoured merely to
insert such observations as might with most certainty be assumed to be
remarkable for size and brilliancy.
26 REPORT—1860.
The catalogue itself may possibly appear in a future volume of the Reports
of the British Association.
An attempt has been made to separate (as aérolitic) the class of detonating
meteors, of which more than 100 are separately given; great care having
been taken to obtain the fullest and most accurate list of that class of me-
teoric phenomena, as being most interesting and most important, but which
has hitherto either been statistically too much neglected, or not sufficiently
separated and distinguished from the class of fireballs without detonation ;
large fireballs being frequently said to explode or burst, though when so ex-
pressed only, it must be construed as without noise. It has likewise been
the custom with some writers and observers to rank as aé€rolitic, all the larger
class of fireballs, whether observed to burst with or without detunation.
Probably one-third of the larger fireballs, 2. e. having an apparent diameter of
15’ and upwards, burst with an audible explosion, this for those observed at
night; of those similarly observed during daytime the proportion (according
to Mr. Greg’s calculations) is greater, probably about one-half. It is a sin-
gular fact, that out of 72 stonefalls, whose precise hour of fall has been
recorded, only 13 occurred before noon, and no less than 58 fell between
fioon and 9 p.m. Why so few should have fallen at night and before noon, in
the morning, it is not easy to say, supposing it not to be the result of chance.
If true that more aérolitic falls occur during daytime than during the night,
it would seem that there is a greater tendency to encounter those bodies in
their orbits, as they recede from the sun; that side of the earth most directly
opposite to the sun being naturally most likely to come into actual contact
with them. The above observations are taken for average of latitude, say
48° north, and 10° west longitude.
Dr. D. P. Thomson, in his ‘ Introduction to Meteorology,’ p. 302, states
that meteors are of comparative rare occurrence in the Arctic Regions: this,
if true, is curious and important, and deserves corroboration from some of
the great arctic navigators now living in this country, and to whom applica-
tion for any additional information might readily be made; the long winter
nights in those parts being admirably adapted for observations (especially
horary) of shooting-stars.
The time of maximum meteor visibility being stated by M. Coulvier-
Gravier and M. Bompas to be about 6 A.., it is rather singular that the
times of maximum occurrence for aérolites and detonating meteors should
be about the same hour p.m.
5. Of the Chinese observations given by Biot, 900 were made in a period
of only 79 years, viz. from A.p. 1023—1102; they include meteors of every
apparent size from Jupiter to the Moon; likewise a certain number of aéro-
lites, detonating meteors, meteoric showers, and doubtless some few auroral
displays. The larger propurticn were observed in that portion of the sky
included between the S.W. and S.E.
M. Abel Rémusat, in 1819, has published other particulars, viz. of 100
falls of stones and detonating meteors, which have been recorded likewise in
Chinese annals, between the sixth century B.c. to 1223 a.p. In Biot’s list
the 23rd of October presented the maximum number of observations.
6. Further observations are to be desired respecting the zodiacal light, and
every possible connexion between that phenomenon and that of shooting-stars
cr meteors. Likewise further information concerning the heights at which
meteors begin to be visible, and cease being visible. The question concern-
ing the cause of luminosity in meteors is a highly interesting one, and still
an open one. The phenomena displayed by the luminous trains or tails of
shooting-stars and meteors is also a subject requiring much attention. ‘The
DUBLIN BAY DREDGING COMMITTEE. 27
theory that they shine by reflected solar light, has been refuted by Mr. R. P.
Greg inthe April Number of the Philosophical Magazine.
7. It is desirable to distinguish, if possible, between ordinary shooting-
stars and aérolites ; Olmsted, Dr. Lawrence Smith, and Mr. Greg are strongly
of opinion that a distinction may frequently exist, both orbital and physical.
8. In a paper by Prof. W. Thomson in the ‘ Philosophical Magazine’ for
December 1854, “* On the Mechanical Energies of the Solar System,” is deve-
loped more fully the idea of Mr. Waterston, that the solar heat can only be
maintained, on any known principle, by immense numbers of meteorites
constantly striking the surface or atmosphere of the sun, and thus producing
by their enormous velocity and friction a never-failing source of heat. The
chief objection to this theory arises from the fact that, as far as we prac-
tically know anything of meteors, so far from the probability of their being
swallowed up in the sun goes, we see the majority of them apparently re-
curring without waste at periodical times, and that for a long term of years:
this simple circumstance goes much against the probability of Mr. Waterston’s
and Prof Thomson’s theory.
Considering that the sun’s heat, as an effect of its light, must have been
maintained for millions of years (as proved geologically) pretty much at its
present value, it is not improbable that future calculations, and a more accu-
rate knowledge of the phenomena exhibited by solar light, may enable us to
reduce considerably the supposed absolute heat of the sun, as now measured
by ah imaginary thermometer, and thus spare us the necessity of supposing
that its heat is so great as to require myriads of meteors to be always rush-
ing itito it to create a fresh supply of it. If the majority of meteors should
be, as they probably are, merely minute and gaseous comets, not possessing
a solid or stony nature, it would still more increase the chances against
Mr. Waterston’s theory.
9. M. Haidinger has recently published at Vienna some valuable
papers on the crust and external forms of meteoric stones, in relation to the
circumstances accompanying their fall and probable condition prior to, or at
the moment of, entering the earth’s atmosphere.
Report of the Committee appointed to dredge Dublin Bay. By J.R.
Krinanan, M.D., F.L.S., Professor of Zoology, Government School
of Science applied to Mining and the Arts.
Durine the autumn and winter months (1859) the author made several ex-
ceursions to the bays fo the north of Dublin, the results of which will be em-
bodied in the final Report. In the spring of 1860, finding that, owing to
circumstances beyond their control, there was no prospect of systematic
assistance from the other members of the Committee, the author determined
to fix on a district to be worked systematically, and selected the series
of bays between the Poolbeg Lighthouse and Bray as being the most Jikely
to yield a good return as regards numberof species and variety of grounds.
Accordingly, since the beginning of March, a series of systematic dredgings
have been carried out in this district, the results of which are now communi-
cated. The district may be conveniently divided into three sub-districts :—
Ist. That between the Lighthouse wall and Kingstown east pier, including
Kingstown Harbour. 2nd. The district between Kingstown east pier and
the south end of Dalkey Sound, including the whole sound. 3rd. The bay
28 REPORT—1860.
between the latter point and Bray Head, in each case including the banks for
seven miles off shore.
Of these the following call for notice :—
Bank 1.—The North Scallop bed lying about three miles off in district I.
It consists of pure sand. Ophiurid@ are very common; Ophioconide not
uncommon; Comatulide scarce; Asteriade not uncommon: one specimen
of Asterias rosea, Miller (Cribella rosea, Forbes), occurred here. Other
Echinoderms rare; Molluses are rare; Polyzoa and Tunicata are very com-
mon; Crustacea, Decapoda, not uncommon, species few ; Amphipoda rare ;
Cirrhipeda common; Annelida are scarce; and Polypifera very common.
It may be generally noted, however, as unprofitable ground.
2. Within this a bank of Pleistocene fine sand of considerable extent, but
generally narrow in width: this contains very few living shells, but myriads
of dead shells, from which all their organic constituents have been absorbed,
and which are easily distinguished from the shells found in the next.
3. The Shell Bank.—This, which I have only partially succeeded in tracing
out, isa curious belt of broken and living shells, the dead shells being easily
distinguished from those of the Pleistocene (Teleocene) beds. Many spe-
cies of Crustacea are here found; Zoophytes are abundant in certain parts
of it; Echinodermata are also common, chiefly Ophiocomide. Echinide,
Sipunculide, and Holothuriade occur more rarely, at least to the dredge, as
the oval tentacles of the latter are frequently brought up. This bank is
most interesting, as it bears a close resemblance to the Turbot Bank of the
Belfast Dredging Committee, many of the shells being identical; and one
remarkable coral, as yet only found in the north seas of Ireland, has been
detected in it by Mr. E. Waller (Sphenotrochus Wrightii). I have traced it
nearly the whole way across districts 2 and 3, though in some parts its
breadth is narrowed to a few yards; and it bears a constant relation to
Bank 2, which in district 3 is called the “ Back.”
4, Shanganagh Bank, a shingly, muddy, sand oyster-bed, formed from the
influx of the river of the same name lying inside the Back in Killiney Bay.—
Here Lupagurus levis first occurred to me; Asterias rosea, two specimens :
Holothuriade are not uncommon ; Zoophytes and Polyzoa not uncommon.
Of Mollusca some rare species occur here.
5. Sorrento Bay.—This consists of dense gravelly sand. Here living
Molluses are rare ; Nucula radiata occurs in some number, and very fine ;
and Annelids are not uncommon ; Crustacea, except Hyade, are rare.
6. Dalkey Sound.—This district requires almost a special description
for itself, though not half a mile long, and barely a quarter of a mile broad,
and the depth of water in no place, according to the Chart, exceeding at
lowest spring tides 12 fathoms; yet species of every group are met with in
it, which are ordinarily reputed to be deep-sea species. I have taken in it,
and in it only, Ophidion imberbe, Pirimela denticulata, Hyas coarctatus,
Inachus dorynchus, Ebalia Pennantii, and ynany other species which else-
where have only occurred to me in 20-fathom water. In fact, the only spe-
cies wanting here are those for which I would propose the name of broad
sea species, such as Spatangus purpureus, Lupagurus levis, Inachus Dor-
settensis, and Crangon Alimanni, none of which have ever occurred plenti-
fully except outside the “ Back.” I defer a full description of this district
until my final report, which I hope to present to the Association at their
next meeting.
7, The Cnook, a bank about seven miles from land in an easterly
direction.—This consists of fine sand and large shells: Zoophytes are very
common ; Oysters and Scollops also abound. Here I met several species of
mo
=
DUBLIN BAY DREDGING COMMITTEE. 29
Crustacea, which are rare elsewhere,—Lupagurus levis, Inachus Dorsettensis,
Pinnotheres pisum, Tetromatus Bellianus, &c. The bank is not easy of
attainment, as it requires smooth water for its proper working, and the past
season in Dublin has been a succession of easterly and westerly gales.
From all these grounds a number of species have been obtained ; of these,
the Annelida and Zoophytes are yet undetermined, but the author hopes to
put in a list of them at the next meeting of the Association. Of other
groups, the following number of species have been determined :—Fishes, 10,
one, Ophidion imberbe, new to Ireland: Mollusca, 188, exclusive of Polyzoa ;
of these none are new to Ireland: Crustacea, 7); of these 5 are hitherto un-
recorded in Ireland, 8 new to the east coast: Arachnida, 2: Echinodermata,
$0, one, Asterias rosea, new to Dublin, &c. Spouges are omitted for the
present. In the present immature condition of these researches, it were pre-
mature to attempt any general conclusions; but the results as yet obtained
go strongly to confirm an opinion advanced by the author some years since,
regarding the absence of southern types on the Dublin coast, which occur
further north, and which led him to the adoption of an eastern Irish or
Dublin district, extending from Dundrum Bay to Carnsole Point. For the
identification of most of the species the writer is responsible, with the ex-
ception of the minute Molluscs; these Edward Waller, Esq., kindly took in
hand—frequent recurrence of his initials in the accompanying list will show
with what success. Great quantities of the fine sand obtained in these
researches is yet unworked, so that it is probable that ere our next report
other species may be added to those here given.
To complete the work, the Committee would ask that the Committee may
be appointed, with the addition of Edward Waller, Esq., as follows :—Pro-
fessor J. R. Kinahan, Dublin; Dr. W. Carte; Professor J. Reay Greene; Dr.
E. P. Wright, and Edward Waller, Esq.; and that a further sum, not exceed-
ing £15, be placed at their disposal for this purpose, to enable them to
COMPLETE this investigation.
List of Species obtained in Kingstown and Killiney Bays, and a few from
Baldoyle.
Saxicava rugosa, living, very common.
Psammobia Ferroensis, single valves, not
arctica, living, not uncommon.
common.
Spheenia Binghami, living, one specimen :
Dalkey Sound.
Mya truncata, dead, not uncommon.
arenaria, living, young specimens.
Corbula nucleus, living, not common ; dead
yalyes, very common.
Lyonsia Norvegica, living, rare.
Thracia phaseolina, living, rare, double
valves.
— villosiuscula, not rare.
—— distorta, living, rare.
on pretenue, dead, single valves
only. ;
Solen marginatus, dead, single valves only,
—— siliqua, living, in Killiney Bay.
— ensis, living, in IGlliney Bay.
pellucidus, living, in some numbers, in
Killiney Bay.
Solecurtus candidus, single valves without
epidermis: Shell Bank.
——— coarctatus, a pair of valves: Dalkey
Sound,
tellinella, very common.
Tellina crassa, very common.
— incarnata, dead, single valves only.
—— tenuis, living, rare.
—— fabula, dead, single valves.
solidula, rare, living.
—— donacina.
pygmeza, very rare, living.
Syndosmya alba, common.
Serobicularia piperata, one dead specimen,
on Shell Bank.
Mactra solida, rare, living here.
—— subtruncata, one single valve.
—— elliptica, very common.
—— stultorum, rare here.
Lutraria elliptica, dead, shells only.
Tapes decussata, uncommon.
pullastra, not uncommon.
virginea, very common.
Venus casina, uncommon.
striatula, rare here.
——- fasciata, common.
30 REPORT—1860.
Venus ovata, common.
Artemis exoleta, common.
lincta, not uncommon.
Lucinopsis undata, rare.
Cyprina Islandica, common, dead; not
common, living here.
Circe minima, E. W., very rare.
Astarte sulcata, uncommon.
triangularis, EH. W., not uncommon.
Cardium echinatum, not uncommon, dead ;
living small, rare.
edule, rare here.
— pygmzum, uncommon.
—— Norvegicum, not uncommon.
—— nodosum, very common.
—— fasciatum, common.
Lucina borealis, common.
flexuosa, Killiney Bay, rare.
spinifera, one single valve.
Montacuta bidentata, H.W.
substriata, on Spat. purpureus,
Kellia suborbicularis, rare.
rubra, E. W.
Lepton nitidum, BH. W.
squamosum, single valves, rare.
Mytilus edulis, common.
Modiola Modiolus, common.
Crenella discors, common.
marmorata, uncommon.
Nucula nucleus, very common.
— nitida, common.
radiata, not uncommon, but local.
Leda caudata, rare, living.
Pectunculus glycimeris, living, rare and
small; dead, large and uncommon.
Lima Loscombii, rare.
Pecten varius, rare.
pusio, rare.
—— tigrinus, not rare.
maximus, not rare.
opercularis, very common.
Ostrea edulis, very common.
Anomia ephippium.
patelliformis.
— striata.
Chiton fascicularis, rare.
—— marmoreus, rare.
asellus, very common; other species
et undetermined,
Patella vulgata.
—— pellucida.
athletica,
Acmza virginea, common; Dalkey Sound.
testudinalis,
Dentalium entalis, uncommon.
tarentinum, dead, only fragments, rare,
Pileopsis Hungaricus, rare here.
Fissurella reticulata, uncommon.
Emarginula reticulata, uncommon,
Trochus zizyphinus.
granulatus.
Montagui,
—— tumidus.
— umnbilicatus.
cinerarius.
—— millegranus.
Trochus magus, broken.
helicinus.
—— pusillus, H.W,
Phasianella pullus.
Adeorbis subcarinata.
Littorina littorea.
rudis.
littoralis.
Lacuna vincta.
crassior, Shanganagh.
Rissoa Beanii, H.W., one fragment.
uly.
— costata.
parva.
labiosa.
—— punctura, E. W.
inconspicua, E. W.
semistriata, HE. W.
soluta, one specimen,
vitrea.
striata.
striatula, E. W.
Skenea divisa, E. W.
planorbis.
Turritella communis.
Cecum glabrum, EH. W..
Aporrhais pes-pelecani,
Cerithium.
adyersum, E. W.
Scalaria Turtonis, broken.
communis.
Eulima polita, B. W.
distorta, EH. W.
bilineata, E. W.
Chemnitzia fulyocincta: Shell Bank.
elegantissima, E. W.
indistincta, H. W.
Odostomia eulimoides.
insculpta, E. W.
—— interstincta, E. W.
spiralis, E. W.
decussata.
Natica monilifera.
nitida.
sordida.
Velutina levigata.
Murex erinaceus.
Purpura lapillus.
Nassa reticulata.
incrassata, rare.
—— pygmea.
Buccinum undatum.
Fusus antiquus,
Islandicus.
propinquus.
Trophon Barvicensis,
—— muricatus,
clathratus,
Mangelia turricula,
—— rufa,
septangularis.
— linearis.
—— nebula.
—— costata.
Cyprza Europa.
Cylichna cylindracea.
A
DUBLIN BAY DREDGING COMMITTEE.
Cylichna truncata, E. W.
Amphisphyra Hyalina.
Tornatella fasciata.
Akera bullata.
Scaphander lignarius.
Philine aperta.
Aplysia hybrida.
Pleurobranchus membranaceus.
-—— plunula.
Eolis papillosa.
Tritonia Hombergii.
Doto coronata.
Pholas dactylus.
crispata.
Aplidium fallax.
Botryllus polycyclus.
Ascidia mentula.
— virginea.
Molgula tubulosa.
Cynthia aggregata.
Hledone cirrhosus.
Rossia macrosoma.
Stenorhynchus phalangium.
Inachus Dorsettensis.
dorynchus.
Hyas araneus.
= coarctatus.
Eurynome aspera.
Cancer pagurus,
Pilumnus hirtellus,
Pirimela denticulata.
Carcinus mzenas.
Portunus puber.
arcuatus.
—— depurator.
— holsatus.
—— pusillus.
Pinnotheres pisum.
PEbalia Pennantii.
Atelecyclus heterodon.
Corystes Cassivelaunus.
Pinnotheres pisum.
Eupagurus Streblonyx.
—— Prideauxii,
— Cuanensis.
— Ulidianus.
—— Thompsonii.
Porcellana longicornis.
platycheles.
Galathea squamifera.
— strigosa.
—— Andrewsii.
—— nexa.
— dispersa.
Palinurus vulgaris.
Homarus vulgaris.
Crangon vulgaris.
— fasciatus.
— sculptus.
— Allmanni.
— bispinosus.
Nika edulis,
Detailed notes on the species will accompany the final Report.
Hippolyte yarians.
—— Cranchii.
—— Thompsonii.
—— pusiola.
Yarrellii.
Pandalus annulicornis.
leptorhynchus.
Palzemon serratus.
— squilla.
varians.
Athanas nitescens.
Lysianassa longicornis.
Anonyx denticulatus.
Ampelisca typicus.
Urothoe marinus.
elegans.
Iphimedia obesa.
Eblane.
Acanthonotus testudo.
Dexamine spinosa,
Gammarus locusta.
— fluviatilis.
palmatus.
—— Othonis.
longimanus.
Amphithoe rubricata,
—— littorina.
Podocerus falcatus.
variegatus.
Corophium longicorne.
Chelura terebrans.
Hyperia Galba.
Caprella tuberculata.
Comatula rosacea.
Ophiura texturata.
—— albida.
Ophiocoma neglecta.
Ballii.
bellis.
rosula.
minuta.
Uraster glacialis.
—— rubens.
— violacea.
hispida.
Cribella oculata.
rosea.
Solaster papposa.
Asterias aurantiaca,
Echinus sphera.
— Miliaris.
Echinocyamus pusillus,
Spatan urpureus.
ee hiaee cordatus.
Cucumaria fusiformis,
Hyndmanni.
Thyone papillosa.
Synapta inherens,
Syrinx Harveii.
granulosus.
Sipunculus Bernhardus.
Priapulus caudatus.
31
32 REPORT—1860.
Report on the Excavations in Dura Den.
By the Rev. Joan ANDERSON, D.D., F.G.S.
In reporting on the operations and researches in Dura Den during the
summer of 1860, the Committee laid open several large sections of super-
incumbent boulder clay and of the underlying yellow sandstone, but were
unsuccessful in obtaining any of the Pamphractean or Pterichthyan forms
sought after. None of the workmen engaged in the excavations in 1837,
when these organisms were found in great numbers, were living in the di-
strict ; and the Committee, proceeding on the information of others, failed to
detect the precise fossiliferous bed in question. Their labours brought them,
however, to a point which cannot be far distant from these crustacean trea-
sures, and they are hopeful that, on resuming their researches, they shall
meet with the desired success. They proceeded to other sections of the rock,
in the bottom of the ravine, and there they were richly rewarded with an
abundance of the fossil remains of fishes, chiefly of the genus Holoptychius
and other Celacanths.
The yellow sandstone deposit, as described in the ‘Course of Creation’
in former papers of Dr. Anderson, consists of an alternating series of grits,
shales, marls, and fine-grained sandstone, of various shades of colour. The
fossil fishes are confined to one particular bed, which, when laid open, easily
splits up, the organic materials determining the point of separation, and
exhibiting often on a single flag from fifty to a hundred closely-packed and
well-defined figures with scales, fins, and cranial plates quite entire. On the
present occasion your Committee were surrounded by an intelligent group of
lovers of the science, male and female, from Edinburgh, St. Andrews, Forfar,
Dundee, and Cupar, and succeeded, after a few hours’ labour, in displaying to
their eager gaze some of the largest and most beautiful specimens of these
older denizens of our seas.
It will not be necessary to describe in detail any of the well-known forms
and characteristics of Holoptychius, the most abundant of the genera found in
this deposit. But having submitted some of the most perfect of the spe-
cimens to Professor Huxley, and as he thereby was enabled to detect some
new particulars connected with the structure and figure of the genus, it will
not be deemed out of place to give an abstract of his interesting descrip-
tion, contained at length in Dr. Anderson’s ‘ Monograph of Dura Den*.’
“Tn studying,” says Professor Huxley, “ the new forms of Devonian fish
which have been described, I found it desirable to obtain a more definite
conception than was deducible from extant materials, of the characters of
Holoptychius. To this end I examined a considerable number of specimens
of Holoptychius Andersoni, contained partly in the collection of the British
Museum, partly in that of the Museum of Practical Geology, and I have
arrived at the following conclusions. Holoptychius Andersoni has very nearly
the proportions of a carp, but its body is thicker and its snout is more rounded
from side to side. ‘The greatest depth of the body is in front of its middle ;
the length of the whole body is to that of the head nearly as five to one.
The orbit is nearly circular, about one-fourth the length of the head. The
cranial bones all exhibit a peculiar granular structure. The two parietals
occupy a large extent of the upper wall of the cranium, and have the form
of pentagons with their elongated bases turned inwards and applied to one
another. The occipital region is covered by three bones, one median, and
two lateral; the lateral bones having radiating striz on the posterior halves
* Dura Den; A Monograph of the Yellow Sandstone and its remarkable Fossil Remains.
By the Rey. J. Anderson, D.D., F.G.S, Edinburgh: Thomas Constable and Co.
ON THE EXCAVATIONS IN DURA DEN. 33
of their outer surfaces. The operculum is a broad bone, larger behind,
where it is convex, than in front, where it is concave, and much longerthan
it is deep.
_ “The rami of the lower jaw are stout and strong, and form a very broad,
almost semicircular arch. The characters of the scales are well known.
The fins are lobate, and the dorsal fin is small and triangular. Sir Philip
Egerton, in a valuable memoir recently read before the Geological Society,
_expresses his belief that Holoptychius has two dorsal fins. I am very loath
to controvert the opinion of so experienced and skilful an observer, the more
particularly as specimens of Holoptychius with perfect tails are very rare,
but one or two complete examples I have seen, leave no room in my mind
for any other conclusion than that stated above.”
Numerous perfect specimens of this remarkable fish have been obtained
in our recent excavations, which show the lobate character of the fins as de-
scribed by the learned Professor, as well as the unity of the dorsal organ.
The entire form of the body of Holoptychius is likewise beautifully deve-
loped in some of the specimens, where the caudal end appears gradually
tapering toa point, and not at all dent up as represented in all former de-
scriptions ; while the ventral lobe of the caudal fin, though rather shorter than
the dorsal lobe, has nearly the same depth, and not in the ordinary sense
of the heterocercal structure.
In the course of our explorations we also succeeded in obtaining several
perfect specimens of two new and hitherto undescribed genera of Ceelacanths,
namely, Glyptolemus Kinnairdii and Phaneropleuron Andersont.
The specific distinction of Glyptolemus Kinnairdit was proposed and
adopted at the Meeting of the London Geological Society in honour of
Lord Kinnaird, whose zeal in promoting the interests of geology is only
equalled by his enlightened endeavours to advance the interests of anything
connected with our social and industrial well-being as a statesman. The
generic term of Glyptolemus was suggested on account of the marked
sculpture of the jugular plates in one of the specimens. As described in the
“Monograph” of Dura Den, the scales and fins likewise form strongly
marked characteristics of this new genus.
The scales are rhomboidal, and have an average short diameter of one-
sixth of an inch. Twenty-four series are visible, and diverge from the me-
dian line in the ordinary way ; they are larger on the anterior part of the
ventral surface than on the posterior part, and at the side of the body than
on the belly. They are pitted and ridged almost as in Glyptopomus, although
somewhat thinner and less bony than in that fish. There are two dorsal fins
which are situated very far back, the anterior edge of the root of the first
being nine inches distant from the end of the snout in one of the specimens : it
is remarkably slender, and of a semi-oval outline. The second dorsal fin is
considerably larger than the first, being two inches on its longest axis, and
its breadth about an inch in depth. The entire length of the body, in several
of the specimens, varies from a foot and a half to nearly two feet.
The other new genus discovered in the course of our explorations is the
Phaneropleuron Andersoni, and from some very imperfect fragments named
by Professor Agassiz as a Glypticus, but without describing or defining the
genus. The generic appellation, now bestowed by Professor Huxley, ex-
presses the most striking character of the fish—the curious development and
obtrusiveness of its ribs, arising from their complete ossification as well as
_ the thinness of the scales. The affinity of Phaneropleuron with the typical
ceelacanths is indicated not only by its singular tail, but by its persistent
ohh by its lobate pectoral and ventral fins, and by its well-ossified
0. D
34 REPORT—1860.
superior and inferior vertebral elements. The scales remind one of Holo-
ptychius, but are much thinner and differently sculptured. ‘The fins are more
nearly of the structure of this genus in theirgeneral facies, though they differ in
details. They are lobate in the lateral pairs, a character now regarded by one
of our most eminent ichthyologic authorities, Sir Philip Egerton, as belonging
to the entire family of Ccelacanths, and which Agassiz has also described
in his elaborate account of the Glyptolepis of Clashbennie in the ‘ Poissons
Fossiles.’
This locality, so richly stored with these and other forms of fossil remains,
has now contributed largely to our stock of paleontological knowledge.
Should the researches be continued, your Committee are sanguine, not only
in the recovery of the long-lost bed of the disputed Pamphractus, but like-
wise of new genera and new species still sealed up in the yellow sandstone
museum of Dura Den*. Trilobites of a small type, Productz and Spirifers,
are very numerous in the carboniferous shales of Ladeddie, which are in
immediate superposition and stretch along the southern opening of the Den.
About three miles to the eastward, in the irenstone deposits of Denbre
and Mount Melville, large jaws, teeth, bones, and scales of the genus
Rhizodus are in the greatest abundance and the most beautiful preservation.
Thus the geologist may here study successively the upper beds of the Old
Red Sandstone, the Mountain Limestone, Ironstone shales, and the Coal-mea-
sures on the most northern limits of the Carboniferous system. Trap-rocks
everywhere penetrate the series of sedimentary deposits, indurating the sand-
stone, fusing the limestone, roasting the coal, and exhibiting proofs of those
destructive agencies and deleterious impregnations by which the fishes of
Dura Den were suddenly overtaken, silted up, and preserved in such num-
bers and perfect forms in their stony matrix.
Report on the Experimental Plots in the Botanical Garden of the
Royal Agricultural College, Cirencester. By James BuckMAN,
F.L.S., F.S.A., F.G.S. &c., Professor of Botany and Geology, Royal
Agricultural College.
In presenting our Report for 1860, it will be necessary to remark, that on
account of the peculiarities of the season, particularly its latetiess, and the
fact of the unusual period of the Oxford Meeting, the Report before the
Section at Oxford was made verbally, permission having been obtained to
make a more full and written report when the experiments had attained to
something like completion. It was reported before the Section that 200
plots were in operation, which were classified as follows :—
Plots
Agricultural Plants........ Ss ortsticnt one OO
Medical PiiGs. ieee as sre te weet es Se
Psculent Vepetaples 2s"... c.p2c05 00 os 20
Grasses, old and new plots............ -- 60
Miscellaneous Plants <2 2.2... 20s>.: 22. 40
Total 200
Of these, at the Oxford Meeting it was reported that more than half were
either new seeds only just germinated, while for the others they had made
* See Reports of the British Association for 1858 and 1859.
ON THE GROWTH OF PLANTS. 35
so little progress, that we almost despaired of any substantial results under
such untoward circumstances. Still, however, we now offer remarks upon
some of the more striking experiments, which it may be said are so far com-
plete up to November.
GRASSES.
Sorghum saccharatum (Holcus saccharatus), Chinese Sugar-cane-—The
fine summer of 1859 enabled us to grow this plant to a height of as much
as 7 feet, as also to perfect its saccharine matter, at least in a very high
degree. This success, which was pretty general all over England, had caused
very flattering encomiums to be passed on the merits of this plant for agricul-
tural purposes, especially as a green soiling food. The total failure, however,
of our experiments for this season is not only instructive as to the great
diversity of seasons, but should also teach us caution in recommending the
extensive adoption of any new plant in our uncertain climate from only a
single year’s growth. Our best plants did not attain 6 inches, and indeed our
failure this year was more signal than our success the previous one.
fgilops ovata.— Although our specimens are far later in coming to matu-
rily than in any former season, yet the results are more striking than we have
before observed. Even at the time of our writing (November), little of our
crop for 1860 has ripened; but the spikes are longer than usual, whilst the
stalks (culms) are taller; and added to this is the important result of a show
of more and larger grain, of the shape of the wheat grain, so that we have
searcely a doubt left as to this being the parent of the cereal or corn wheat.
Again, as another evidence of the results and effects of cultivation, we have
the crop of this year affected with all the epiphytical fungi to which wheat
is liable, and the more so the more it is manured.
Gyneria argentea, Pampas Grass.—-Our specimens, one of which flowered
most beautifully last year, are all dead, so that however highly this plant
may be recommended for naturalization in other parts of England, where the
climate is milder, we cannot think it will ever be safe to trust to it on the
“Stony Cotteswolds.”
Of British Grasses, we have to report that we have had in operation during
the present season as many as sixty plots; several of these are only our usual
common English species, many of which are condemned to be resown on
account of their inevitable admixture. Among the experiments of interest,
we have to report the complete production of Festuca elatior from a plot of
F, loliacea, in which the changes were as follows :—
2nd year.— Festuca loliacea the rule, with exceptional cases of F’. pratensis.
3rd year.—Festuca pratensis the rule, with exceptional cases of £’. elatior.
4th year.—F. elatior increased.
5th year, 1860.—Festuca elatior has complete possession.
In reference to this, it will be remembered that we noted in a former
Report the occurrence of F. elatior in Earl Bathurst's Park, which we then
conjectured had been derived from the sowing of the seed of FP. pratensis.
This year we have further to remark that here the e/atior form is the rule,
and scarcely a vestige of the F. pratensis remains ; and very coarse and un-
sightly it is as a glade in a park.
We have now performed this experiment twice with the same result, and
our views seem confirmed by the accidental case just referred to; we have
then no doubt that the three forms just adverted to are but varieties of a
single species ; and we have much pleasure in observing that our views in
this and other cases of alike kind, derived from actual experiment, and
reported upon to the Association in 1847, should be confirmed by the
D2
36 REPORT—1860.
Specific Botanist as thus: under the head of ‘Meadow Fescue, Festuca
elatior,’ see Bentham’s ‘ Handbook of the British Flora,’ p.602, we have the
following :—
“a. Spiked Meadow Fescue (fF. loliacea, Eng. Bot. t. 1821). Spikelets
almost sessile, in a simple spike. Grows with the common form, always
passing gradually into it.
“b. Common Meadow Fescue (F. pratensis, Eng. Bot. t. 1592). Panicle
slightly branched but close. In meadows and pastures.
“ce. Tall Meadow Fescue (F.elutior, Eng. Bot. t. 1593 ; & arundinacea,
Bab. Man.). A taller, often reed-like plant, with broader leaves, the panicle
more branched and spreading. On banks of rivers, and in wet places, espe-
cially near the sea.”
Now, though well aware that these views are not generally shared by col-
lecting botanists, we are yearly more and more persuaded that even greater
innovations than now contended for y.ill be admitted; and we cannot help
expressing pride and pleasure that we should for the last fourteen years
have been conducting a series of experiments, many of which practically
prove the truth of several of the theoretical views, with regard to what has
been termed the “lumping” of species, of the author of the Handbook ;
and we cannot here omit expressing our best thanks to the British Association
for their assistance in prosecuting these interesting inquiries.
Poa ( Glyceria) aquatica.—Our plot with this experiment still continues
to exhibit 27 its entire space, without the slightest intermiaxture, the induced
form we have before reported upon, which indeed is so different from the
original grass, that at a first glance most observers would pronounce it to be
large examples of Poa trivialis ; the differences, however, in all parts are as
great between our induced form and that grass, as exists on comparing the
induced form with the Poa aquatica. There can be no doubt that in
this case the cultivation of the seed of a water grass in an upland situation
has led to great changes, not, as has been supposed, brought about by cross-
breeding or hybridizing, but the seed of the P. aquatica has at once been
changed in the growth of the plants that came up from it ; and it now remains
to see if the change be a permanent one, to which end we hope to be able
to sow a plot of the seed of the induced grass next spring; but in the mean-
time it may be well to remark, that although it has frequently seeded, yet
that the bed is still free both from innovations from seedlings of its own kind,
as also from those of other species.
Poa (Glyceria) fluitans.—At the same time that the plot was sown with
the seed of P. aquatica, another plot was occupied with seeds of the Poa
Jluitans ; and we should remark that in both cases the seeds were drilled, and
the drills remain intact to the present hour. Now the result is, that both
plots were indistinguishable at the first time of flowering, and have so re-
mained to the present hour; and with reference to the last form, it may be
well to point out that, having been favoured by Messrs. Sutton of Reading
with specimens of the collection of grasses which they keep in cultivation, a
bundle marked ‘‘ Glyceria fluitans” is identical with our induced forms from
both P. aquatica and P. fluitans.
Poa aquatica and P. fluitans.—We offer no explanation of these; being
wellacquaiuted with these two species, we can truly say that our induced form
is widely different ; nor is it at all identical with any other British species. It
is, however, still a matter of regret that we have not been able to procure
ripe seed of these species from the district, as, so far as we can discover, none
of the P. aquatica at least has ripened in the district. It may be well to
mention, that even this shyness in the ripening of the seed of this now so
i
ON THE GROWTH OF PLANTS. 37
emphatically a water grass, is not without value as affording something like
evidence that this species is perhaps after all out of place, and this may
point to the fact that our induced form is the right one; at all events, it quite
determines the fact that the name Glyceria is inapplicable, as it is a decided
Poa in cultivation.
Crop PLANTs.
Pastinaca sativa, Parsnip.—Our ennobled examples of these were con-
sidered so perfect, that it was thought advisable to consign the whole of the
seed of 1859 to the Messrs. Sutton of Reading, as new varieties of any cul-
tivated crop plant is always desirable, and more especially when, as in the
present case, the new form has been directly derived, not from a variety, but
from the original wild stock. In reference to the continued success of this
experiment, Mr. Sutton reports in a letter of October 17th of this year as
follows :—
“ The Student Parsnip in our trial ground is the nicest shape of any, more
free from fibres, and as large as the ‘ hollow crown,’ which is a good medium
size. The flavour seems to be very nice.”
This is the more important, as of late this useful garden esculent has much
fallen into disuse, its want of flavour being the assigned cause.
We must not omit to remark, that one of the most malformed specimens
of parsnip, and also a highly digitated Swedish Turnip, were set aside for
seeding, with a view to sowing next spring in the same kind of plots, as there
seems reason to expect that such degenerate forms could only beget a
degenerate progeny : with a view then to ascertain how far this degeneracy,
or otherwise, may proceed, we first took careful portraits of the seeded roots,
the seed of which is now put by for experiment. :
Brassica oleracea—Having gathered some seeds of this wild cabbage
from Llandudno, N. Wales, in August 1859, we sowed it in the summer of
the present year in our private garden, from whence we removed some plants
for a plot in our College garden. These, and our own examples, are already
highly curious, as showing the tendency to run into so many of the cabbage
varieties, e. g. long petioles ; the types known as “kale, greens,” &c., both
with broad, more or less undivided leaves, and with a tendency to deep lobes
and divisions. Others with short petioles, offer the true cabbage type; while
these even now show tendencies for the production of sorts, as flat heads,
sugar-loaf, green, red, and white varieties. These of course are what one
would expect, but still it is curious to mark its progress.
In speaking of the Brassica family, we cannot help expressing our conyic-
tion of the justice of including the genus Stnapis with Brassica ; for just as
our experiments incline us to the opinion that all our so-called species of
this genus are after all only derivatives, so we believe that the Charlock
Sinapis arvensis, L. is also an agrarian form of Brassica. Upon this, however,
we want the experiments of a lifetime; still these would be replete with
interest, and more especially as we find cabbage, rape, turnips, radishes,
and mustard almost wholly attendant upon cultivation, and that not only
with us, but in every variation of climate. How wild the thickets of Sinapis
nigra, some 6 feet high, look on the banks of the Ohio! and yet we have the
authority of Beck in favour of its introduction from Europe ; and so we have
evidence of the crops in India being smothered with wild rapes, which our
experiments show are principally Judbless varieties of the turnip.
Mangel Wurzel——The inquiry connected with the growth of this crop
is one which may be considered of interest in a physiological as well as an
agricultural point of view, and hence we give its results in this place.
38 REPORT—1860.
It is tolerably well known that this valuable crop was introduced into
cultivation with the hope that it would yield a valuable supply of food in the
shape of leaves, whilst at the same time it was supposed to be capable of
fully developing its growth of roots, the leaves then being employed for
summer and autumn food, whilst the roots were to be stored for winter use;
however, we were early struck with the fact, that using the leaves to any
extent, would prejudice the crop of the roots, and we therefore twice before
the last year instituted experiments upon this matter with a result that may
be generally stated as follows.
The Mangel Wurzel, stripped of its outer leaves from two to three times
during their period of growth, do not produce half the weight of root of those
left intact.
And herein we thought that we had established the law, that as long as a
leaf of Mangel was sufficiently sound to be useful as food for any animal, so
long was it of use in aiding the proper development of the plant; but this
statement has been controverted by the result of some experiments made at
the Albert Agricultural Model Farm, Ireland, where it is stated that the
result of taking the enormous quantity of 5 tons of leaves from the acre of a
growing Mangel crop, was to increase the weight of roots at the rate of nearly
54 tons. Now, under these circumstances we determined upon repeating the
experiments upon a larger variety of Mangels this year.
Ist. A set of experiments made with nine sorts of Mangel Wurzel planted
with burnt ashes, duly thinned and tended as usual; the plots being 24
yards square.
2nd. Nine plots of the same sorts transplanted.
The outer leaves of all these plots were taken off on the two following
dates, September 4 and September 21.
On the 12th of November the whole crops topped and tailed, consisting of
twenty-four roots to each bed, half of which had been stripped of their outer
leaves; thus twelve roots each, stripped and unstripped, gave the following
results for both the untransplanted and the transplanted plots :—
Untransplanted Plots. / Transplanted Plots.
Names. Entire. |Stripped. | Entire. |Transplanted.
lbs. oz. | Ibs. oz. lbs. oz. Ibs. 02+
J. Elvethan .0......cececcessccvcsessesese 8°10 at ea 14°10 5°10
DopVellow, Globe; .c.testecsec enessvarcses peta D° 2) |: Seale ela 6:14
Be med Glove 087. e lites eset 8 2 CAD OB Vis 3
4. New Olive-shaped Red Globe...... 11:13 7°60) 44 12° 4 5: 6
5. New Olive-shaped Yellow Globe 16°13 12.33 seo 11°14 7°10
6. Sutton’s New Orange Globe ...... 9-5 312.) 6 10° 2 5: 3
7. Improved Long Yellow .........++. 19: 0 Ol | 7.) 1910 We.
1 8. New Long White ......ceccccecssecee es aoe 7 8 8 12°11 7 6
Of SH VSMC ions zetcieen a deed sass cosas 16°15 So @) | 9 15°13 611
OtB eee ppcxsostteeee meee Boner os 114°10 63° 3 121: 4 63° 6
Here then we take these results from so many sorts as conclusive evidence
upon this point, only remarking that, in all probability, had the season been
one of an ordinary kind, the discrepancy would have been even greater, as
this year the tendency of growth has been in favour of leaf development.
The same experiments were tried with Kohl Rabbi, and withthe like results ;
and it should be mentioned, with regard to all of them, that the seed was
obtained from the Messrs. Sutton of Reading, and that it was true to sort.
ON THE GROWTH OF PLANTS. 39
It s not a little remarkable that in both the Mangel and Kohl Rabbi the
results have been greater in the transplanted than in the untransplanted plots,
the former yielding a larger crop; this too has probably been favoured by
the moist season, but as it is a subject of great farming interest, we shall
renew our experiments upon this matter.
Dipsacus fullonum et sylvestris.—Our plot of this year fully confirmed our
view of last year, as to the specific identity of these two forms of this plant;
for without being able to assert that we had decided D. fullonum from the
seeds of D. sylvestris, or the opposite, yet the specimens glided soimperceptibly
into either form, that, distinct as are decided examples, we were much puzzled
in deciding as to the paternity of some of our specimens.
To quote from English Botany, 2nd edition: ‘“ Hudson mentions this plant
as growing about hedges. Inthe clothing countries, where it is cultivated
for use, it may escape from the fields. There is much doubt concerning the
value of its specific difference from the D. sylvestris.”
Bentham is of the same opinion, so that our experiments in this only lay
claim to a simple and practical method of confirming these views. Our
notion at the same time is that it would be exceedingly difficult to find a
wild example of the true D. fullonum ; that is, one which from its hard re-
flexed bracts would be worth anything for fulling purposes. We have hunted
long in the districts where the economic form of the Teasel is grown, and we
have always been of opinion that where its seed has been scattered and allowed
to grow wild, it lost its stiff hooked characters ; and, to say the least, even the
best of them merged into D. sylvestris ; the fullonum being indeed a difficult
plant to keep perfect, unless under constant change of seed and soil.
WEEDS, &c.
Thistles have formed the subject of several experiments during the past
year, which will be referred to under the following names :—Carduus
arvensis, C. acaulis, vars., C. tuberosus.
Carduus arvensis.—Our experiments upon the growth of this plant were
undertaken in order to explain their method of reproduction, as it had been
disputed by the farmer that thistles were produced from seed.
On September 2nd, 1859, were sown ten seeds which had been collected
a few days previously ; by the 21st of the month these had all come up, and
some began to show the secondary leaves, as in Diagram, fig. 1. By the time
the prickly foliage became manifest, the cold weather had set in and all the
plants apparently died. However, in February 1860 we noticed a bud just
emerging through the soil, which induced us to take up a couple of the speci-
mens and make drawings of them, of which copies will be seen at 2a and 2b.
Here then at a and 6 are buds by which the continuance of the plant is
secured, the buds a, 6 forming whilst 5, b are sending up leaves for the second
year, so that by June the plants had advanced to the condition of fig. 3, in
which, while a strong shoot is progressing above ground, a most extraordinary
rhizomation is taking place below fig. 3, fully explaining how in the next
season we may meet with a thicket of Thistles derived from a single plant.
Here then it is obvious that the conclusions with respect to the Thistle not
seeding, were the result of the small and inconspicuous plant which it makes
the first year, and this apparently «lying, confirmed this view ; however, we
see from this experiment that thistle seed is as fecundate as that of other
plants, and as we have counted as many as 150 seeds from a single head of
flowers, and as we may haye an average of ten heads of flowers to a single
flowering stem, the eight tertiary buds at fig. 3 a, a may each represent a
40 REPORT—1860.
flowering head in the following season, which would thus give us the following
sum as the seeding capabilities of a single Thistle plant, namely—
150 x 10 x 8= 12000.
These figures then will account for the “ Plague of Thistles” which one
sometimes hears of, and points out most forcibly the importance of not
allowing these plants to perfect their seed, and hence waste places and
neglected waysides should carefully be watched in this respect ; but as this
cannot adequately be done without compulsory enactments, it is interesting
to find that some of our colonies have already instituted state laws with
reference to this subject, and during the last Session of Parliament an attempt
was made to get an act applicable for this object for Ireland. The destroying
of such thickets of Thistles as we have described has ever been an object of
interest with the farmer; and it is not a little curious to remark that the
operations connected therewith have so much been regulated by rhyming
directions, as follows :—
‘ Thistles cut in April,
Come up in a little while;
If in May,
They grow the next day;
If in June,
They ’Il grow again soon ;
If in July,
They ’ll hardly die;
If in August,
Die they must.”
These words, uncouth as they are, are still meant to express some important
facts in the natural history of the plant. It may be observed that, with the
preparation we have described of underground buds, there can be no wonder
at the quick reappearance of the plant on early cutting ; at the same time,
if we consider that the whole of the aboveground parts of the plants
would naturally die at the first approach of cold, we may conclude that the
decree of
“Tf cut in August,
Die they must ”’
is more apparent than real. For while the tertiary buds are advancing to
flower, they are also active in providing a still newer growth of rhizomata and
buds to perpetuate the continuance of the plant; and hence we have no hesi-
tation in saying that never can this thistle be destroyed by late cutting off its
aboveground stems. However, even at this time much good may be done
in keeping down the reproduction of the plant; for by the August mowing
seeding is prevented, though even for this object we should prefer an earlier
cutting, as one head of flowers usually ripens at a time, and not all at once.
Carduus acaulis—We last year reported upon our experiments with the
true acauline form and the slightly cauline examples of this species ; we have
now to remark that the acauline examples maintain their normal condition,
whilst the cauline ones, from being only about 3 inches high when selected
for the experiment, have this year advanced to a complete thicket of stems
nearly a yard high, some of which have as many as a dozen heads of flowers,
and is a very showy and handsome plant.
Carduus tuberosus.—The specimens originally discovered by us at Ave-
bury Druidical Circle have now advanced to immense masses, both as regards
their summer development of flowers and their tuberous rootstocks; the
flowers are above 3 feet high, much branched and very showy, very different
from the single, or at most two-headed flower-stems of the ‘ English Flora,’
pl. 2562, which, however, is a faithful representation of the plant we trans«
ported to our garden. The tubers with us are as large as those of Dahlias.
ON THE GROWTH OF PLANTS. 41
We should remark that this year we have a number of seedling plants which
have come up wildly in different parts of our experimental garden, which we
shall be curious to know if they become like their parents. With us it seeds
so enorniously, that it can hardly fail to be a matter of interest as to how this
plant, originally noticed as from Great Ridge between Boyton House and
Fonthill, Wilts, should have been for so many ycars lost to our flora, whilst its
present natural habitat on artificial earthworks, though truly ancient enough,
would seem to point to its having been introduced to its present locality.
Diagram showing the mode of Growth of Carduus arvensis.
}
f \ 77 Feb. 17, 1860. }
mee ee
3rd nat. size.
Fig. 1. Seedling of the first year.
Fig. 2. a & b. The position of the seedling plants in spring sending up secondary buds J, d.
Fig. 3. The secondary shoot advanced to a large plant, while the rhizome extends and ter-
tiary buds a, a are prepared for the following year.
Bentham, in his description of the position of this plant, has the following
remarks :—
“Tn moist, rich meadows, and marshy, open woods, in western and south-
central Europe, extending eastwards to Transylvania.”
Its position at Avebury is so very different from this, that we cannot for-
bear to describe it. Avebury Circles (of stones) are placed on an elevated
plain of chalk, around which are elevated mounds or earthworks, the whole
‘surrounded by a broad deep vallum, which is at all times perfectly dry, and it
42 ‘“REPORT—1860.
is on the driest and most exposed part of the mounds that the plant occurs.
Its change from such a poor position to our garden, which though only un-
manured forest marble-clay, is yet moist and stiff, will doubtless account for
its wonderful growth.
Cuscuta epilinum.—Our last year’s report on experiments in the growth
of this Dodder excited so much attention, that we determined upon following
out some additional ones in the present season, to which end we sowed two
plots with flax-seed, as follows :—
Plot 1. Flax-seed perfectly pure—The result was a very fine crop, per-
fectly clean.
Plot 2. Dirty Flax-seed with some seeds of Cuscuta epilinum infermixed.—
This was scarcely half a crop, and the fine specimens of Dodder bearing
down the partial crop, is at once an evidence of the mischief this parasite
can do to the crop in question, as also of the perfect ease with which we can
grow it ; so also how easy to prevent its presence in the flax-crop if we take
care to sow pure seed.
As regards the Clover Dodder, though this pest is yearly becoming more
and more prevalent, yet this season has been especially bad for ripening its
seed, and we are still in want of seed for special experiments upon it.
Seeds of Orobanche minor have been collected this year with a view to a
series of experiments upon it, as the Broomrape, like the Dodder, is yearly
becoming more and more troublesome; and it would seem that Clovers are
liable to attacks from both forms of the parasite, and in all probability of
more than a single species of either; for, as regards Broomrape, we have col-
lected the two forms O. minor and O. elatior from different Clover crops ; we
still want to know whether the Cuscuta europea and C. Trifolit are specific-
ally distinct.
Myosotis —We last year reported upon some curious changes wrought in
the cultivation of M. sylvatica, in which we gave it as an opinion that the
M. palustris of authors was subject to great variations, giving rise to annual
as well as perennial forms, the former introducing us to the M. sylvatica and
others, as offsprings of M. palustris. Our present stock still bears out this
view, as we have as derivatives from MW. sylvatica a still decreasing flowered
form and annual and perennial conditions of our varieties.
This year we introduced into the garden the very bright blue Forget-me-
not of our ditches ; this in cultivation (the same plant) has become the small
flowered light blue form which we take to be the M. repens of Don, as de-
scribed by Mr. Babington.
While upon this subject we must not omit to mention that, having been
favoured with a packet of seed from the eminent firm of J. Carter and Co. of
Holborn, under the name of Myosotis azurea major, we were much inter-
ested in observing what kind of bedding plant it might make, particularly as
in the Seed Catalogue for February 1860 we find the following remarks
appended to the Myosotis species :—
** Forget-me-not. These beautiful flowers are too well known to need
recommendation : will grow around fountains, over damp rockeries, or in any
moist situation. MM. azorica and azurea major are the finest.”
Of course, from this announcement we expected something rather choice ;
but our disappointment may be guessed when we found the result to be a
very poor small light-coloured variety of MZ. palustris.
Now, we are far from blaming the Messrs. Carter for this, as it will at once
be seen that this was an induced form, and no one can at all answer for its
permanency ; aud it may be that our position or some new circumstances of
cultivation induced the change from an expected fine flower to a very insig-
BALLOON COMMITTEE. 43
nificant one. Still this affords another curious instance of the effects of cul-
tivation upon this genus, which seem to tell us that we must not be too posi-
tive in the specific distinctions adopted by authors for these plants.
The effects of the season of 1860 have been remarkable in several particu-
lars; we would, however, only refer to a few plants under experiment.
Dioscorea Batatas, Potato Yam.—Smaller than ever; cannot be at all de-
pended upon, even to make its seed in the Cotteswold district.
The Cabbage tribe sadly cut up with us, but the Brussels Sprout was found
to be the most hardy of any kind.
Gyneria argentea.—Killed entirely, both in the College and our own
private garden.
Sorghum saccharatum.—Scarcely attained 6 inches in height against 7 feet
of the previous year.
Zea Mays.—Indian corn not 2 feet high, and died as soon as flowered.
Roots of all kinds smaller than usual.
Potatoes small in quantity and much diseased.
Fruits have not attained their usual size, have not ripened, and are
flavourless.
Forest trees have made little wood, and their new shoots are not ripened.
Garden flowers made little growth, shabby both in leaves and flowers.
Plants perfected for less seed than usual.
Cirencester, November, 1860.
Report of the Committee requested “to report to the Meeting at
Oxford as to the Scientific Objects to be sought for by continuing
the Balloon Ascents formerly undertaken to great Altitudes.” By
the Rev. Ropert Waker, M.A., F.R.S., Reader in Experimental
Philosophy in the University of Oxford.
{wn presenting their Report, the Committee would observe at the outset that
the main object for which the former Committee (in 1858) was appointed
remains yet unaccomplished ; and this is the verification of that remarkable
result derived from the observations of Mr. Welsh in his four ascents in
1852, viz. “the sudden arrest of the decrease in the temperature of the
atmosphere at an elevation varying on different days, and this to such an
extent, that for the space of 2000 or 3000 feet the temperature remains nearly
constant or even increases to a small amount.” It is obviously important to
determine whether this arrest represents the normal condition of the atmo-
sphere at all seasons of the year. The ascents of Mr. Welsh were made
between the 17th of August and the 10th of November. The question
remains, whether this “arrest ” would be observed before the summer solstice
as well as after, and whether there were any variations at different seasons.
The changes in the temperature of the dew-point, consequent upon this in-
terruption in the law of decrease of temperature, would extend our know-
ledge of the condition of the atmosphere at such altitudes. To accomplish
thus much would not require ascents to very great altitudes, although there
are many objects to be attained by ascending as high as possible. The
liberal offers that have been made by Mr. Coxwell and Mr. Langley, of New-
castle, would enable observations to be made at a very moderate cost, and
Mr. Langley appears fully competent to accomplish the task. There are
also many other observations which may be made in balloon ascents which
44 . REPORT—1860.
may prove of very great value. Prof. W. Thomson is anxious that obser-
vations should be made on the electrical condition of the atmosphere. He
has described in the article on the Electricity of the Atmosphere in Nichol’s
‘Cyclopedia,’ a portable electrometer, and also a mode of collecting electricity
by that which he styles the water-dropping system, which would, in his
opinion, be easily applicable. The observations might be carried on, first,
by ascending to very moderate heights, and then going as high as possible.
Dr. Lloyd desires that observations should be made for “the determination
of the decrease of the earth’s magnetic force with the distance from the sur-
face.” The failure of Gay-Lussac to detect any sensible change ought not
to deter future observers. His methods were wholly inadequate; but Dr.
Lloyd is of opinion that if attention be confined to the determination of the
total force or its vertical component (instead of the horizontal), it would be
easy to arrive at satisfactory conclusions. Sir David Brewster suggests that
further information may be obtained as to the polarization of the atmosphere
and the height of the neutral point. And, lastly, Dr. Edward Smith and
Prof. Sharpey are desirous that experiments should be made as to “the
quantitative determination of the products of respiration at different high
elevations.” Dr. Smith has, as it is well known, been for the last two or
three years engaged in experimental inquiries on inspiration, and he is so
satisfied of the value and importance of the investigation, that he is not only
willing, but desirous to make the requisite experiments himself. Dr. Smith
has furnished directions as to the points to be observed and the mode of ob-
servation.
Report of Committee appointed to prepare a Self-Recording Atmo-
spheric Electrometer for Kew, and Portable Apparatus for observing
Atmospheric Electricity. By Professor W. Tuomson, F.R.S.
Your Committee, acting according to your instructions, applied to the Royal
Society for £100 out of the Government grant for scientific investigation, to
be applied to the above-mentioned objects. This application was acceded
to, and the construction of the apparatus was proceeded with. The progress
was necessarily slow, in consequence of the numerous experiments required
to find convenient plans for the different instruments and arrangements to
be made. An improved portable electrometer was first completed, and is
now in a form which it is confidently hoped will be found convenient for
general use by travellers, and for electrical observation from balloons. A
house electrometer, on a similar plan, but of greater sensibility and accuracy,
was also constructed. Three instruments of this kind have been made, one
of which (imperfect, but sufficiently convenient and exact for ordinary work)
‘is now in constant use for atmospheric observation in the laboratory of the
Natural Philosophy Class in the University of Glasgow. The two others are
considerably improved, and promise great ease, accuracy, and sensibility
for’ atmospheric observation, and for a large variety of electrometric re-
searches. Many trials of the water-dropping collector, described at the last
Meeting of the Association, were also made, and convenient practical forms -
of the different parts of the apparatus have been planned and executed. A
reflecting electrometer was last completed, in a working form, and, along
with a water-dropping collector and one of the improved common house
electrometers, was deposited at Kew onthe 19thof May. A piece of clock-
EXPERIMENTS UPON WROUGHT-IRON GIRDERS. 45
work, supplied by the Kew Committee, completes the apparatus required
- for establishing the self-recording system, with the exception of the merely
photographic part. It is hoped that this will be completed, under the
direction of Mr. Stewart, and the observations of atmospheric electricity com-
menced, in little more than a month from the present time. In the mean
time preparations for observing the solar eclipse, and the construction of
magnetic instruments for the Dutch Government, necessarily occupy the staff
of the Observatory, to the exclusion of other undertakings. It is intended
that the remaining one of the ordinary house electrometers, with a water-
dropping collector, and the portable electrometer referred to above, will be
used during the summer months for observation of atmospheric electricity in
the Island of Arran. Your Committee were desirous of supplying portable
apparatus to Prof. Everett, of Windsor, Nova Scotia, and to Mr. Sandiman,
of the Colonial Observatory of Demerara, for the observation of atmospheric
electricity in those localities; but it is not known whether the money which
has been granted will suffice, after the expenses yet to be incurred in esta-
blishing the apparatus at Kew shall have been defrayed. In conclusion, it is
recommended to you for your consideration by your Committee, whether
you will not immediately take steps to secure careful and extensive obser-
vations in this most important and hitherto imperfectly investigated branch
of meteorological science. For this purpose it is suggested,—1. that, if
possible, funds should be provided to supply competent observers in different
parts of the world with the apparatus necessary for making precise and com-
parable observations in absolute measure; and 2. that before the con-
clusion of the present summer a commencement of electrical observation
from balloons should be made.
Experiments to determine the Effect of Vibratory Action and long-
continued Changes of Load upon Wrouyht-iron Girders. By
WivuiaM Fairsairn, Ksq., LL.D., F.R.S.
AMONGST engineers opinions are still much divided upon the question, whe-
ther the continuous changes of load which many wrought-iron constructions
undergo, has any permanent effect upon their ultimate powers of resistance ;
that is, whether a beam or other construction subjected to a perpetual change
of load, would suffer such an alteration in the structure of the iron or the
tenacity of the joints, that it would in time break with a much less force than
its original breaking weight. But few facts are known, and few experiments
have been made bearing on the solution of this question. We know that in
some cases wrought iron subjected to continuous vibration assumes a crystal-
line structure, and is then deteriorated in its cohesive powers ; but we are yet
very ignorant of the causes of this change, and of the precise conditions
under which it occurs.
A few experiments were made by the Commission appointed to inquire
into the application of iron to railway structures, to ascertain the effect of
changes of load upon homogeneous bars of wrought and cast iron. They
found with cast iron that no bar would stand 4000 impacts, bending them
through one-half of their ultimate deflection, but that sound bars would
46 REPORT—1!860.
sustain at least 4000 impacts, bending them through one-third of their ulti-
mate statical deflection. They ascertained also, that when the load was
placed upon the bars without impact, if the deflection did not exceed one-
third of the ultimate deflection, the bar was not weakened ; but that if the
deflection amounted to one-half the ultimate deflection, the bars were broken
with not more than 900 changes of load. With wrought iron bars they
found no perceptible effect from 10,000 changes of load, when the deflections
were produced by a weight equal to half the statical breaking weight.
These experiments are interesting so far as they go, but they are very in-
complete as regards wrought iron. For wrought-iron bars they were not
continued long enough, nor do they apply to those larger constructions in
which the homogeneous bar is replaced by riveted plates. The influence
of change of load on riveted constructions possesses a special importance,
from its bearing on the question of the proper proportion of strength in
plate and tubular bridges. Do these constructions gradually become weak-
ened from the continual passage of trains? and is it requisite to make allow-
ance for such a deterioration by increased sectional area of material] in their
original construction? These questions I have sought to solve by the fol-
lowing experiments.
As the load is brought upon bridges in a gradual manner, the apparatus
is designed to imitate as far as possible this condition. A riveted beam is
fixed on brickwork supports, 20 feet apart. Beneath this is placed a lever
grasping the lower web of the beam, and fastened upon a pivot at the ful-
crum. At the other extremity it carries the scale and weights. This lever
is lifted clear of the beam, and again lowered upon it by means of a connect-
ing rod attached to one of the arms of a spur-wheel placed at a considerable
distance overhead. In this way any required part of the breaking weight
can be lifted off and replaced upon the beam alternately by the revolution of
the spur-wheel. The apparatus is worked night and day by a water-wheel,
and the number of changes of load is registered by a counter.
The girder subjected to vibration in these experiments is a plate girder of
20 feet clear span, and of the following dimensions :—
Sq. in.
Area of top: 1 plate, 4in.x}in......,.. Sine. | 200
2 2 angle-irons, 2X2X 79; ........ 2°30
—— 4°30
Area of bottom: 1 plate, 4 in.x1tin........... 1°00
35 2 angle-irons, 2x2x73...... 14
—— 340
Web, 1 plate 155% 4.2.5. sb ds shi. cate eees 1:90
Total sectional area .............0005 ; 8°60
Depth, s,i006 9 ts02 06 Steaebesiniaswcls 16 ins
Weight : ~ab.)5.52 pase peep sass oiss)) TD eowk 3.qns;
Breaking weight (calculated) Ba sipn. aipisy emai
This beam having been loaded with 6643 lbs., equivalent to one-fourth of
the ultimate breaking weight, the experiment commenced.
EXPERIMENTS UPON WROUGHT-IRON GIRDERS. 47
Tas e I.—Experiment on Wrought-iron Beam with a changing load
equivalent to one-fourth of the breaking weight.
Date, Number of Deflection
1860. changes of load. | produced by load. Remarks.
March 21 0 0°17
» 22 10,540 0-18
i 7 craints O16 Strap loose and failing to lift
; SB Oe bille. eh wile 5 5 é
26 46,100 0-16 the weigt:
‘ania 57,790 0°17
eSB 72,440 0-17
oe 85,960 0°17
25.30 97,420 0°17
ey on 112,810 0°17
April 2 144,350 0°16
‘ae 165,710 0:18
ee 202,890 0°17
o10 235,811 0°17
ee 268,328 0°17
oe | | 281,210 0-17
3 («17 321,015 0°17
3° «20 343,880 0°17 Strap broken.
pH rg 390,430 017
#428 408,264 0-16
io. 28 417,940 0°16
May 1 449,280 0°16
a. Se 468,600 0°16
ee 489,769 0'16
ae 512,181 0-16
Bald 536,355 0°16
ue 560,529 0°16
5 14 596,790 0°16
As the beam had now undergone above half a million changes of load,
that is, it had worked continuously for two months, night and day, at the
rate of about eight changes per minute, and as it had undergone no visible
alteration, the load was increased from one-fourth to two-sevenths of the
statical breaking weight, and the experiment proceeded with till the number
of changes of load reached a million.
Tasxe IJ.—Experiment on the same Beam with a load equivalent to two-
sevenths of the breaking weight, or nearly 33 tons.
Date, Number of Deflection
1860. changes of load. in inches. Remarks.
May 14 0 0-22 In this Table the number of
i elo 12,623 0°22 changes of load are counted
me ay 36,417 0°22 from 0, although the beam had —
, 19 53,770 0°21 j already undergone 596,790
a 22 85,820 0°22 changes, as shown in the pre-
» 26 128,300 0°22 ceding Table.
» 29 161,500 0°22
» 31 177,000 0-22
June 4 194,500 0°21
mt fF 217,300 0°21
e 9 236,460 0-21
s 12 264,220 0-21
» 16 292,600 0°22
m. 20 403,210 0:23 The beam had now suffered a
million changes of load.
48 REPORT—1860.
TaBLeE IJI.—Experiment on the same Beam with a load equivalent to
two-fifths of the breaking weight.
Date, Number of Deflection
1860. changes of load. in inches. Remarks,
June 2
7 0
Sy 2S 5175
The beam broke after 5175 changes with aload equivalent to two-fifths of
the breaking weight, although with lesser weights it had appeared uninjured.
Summary of Results.
Ratio of load | Number of | Total number aes
Table. | to breaking | changes with | of changes of een me Remarks.
weight. each load. load.
16 1:40 596,790 596,790 0-17
10F 1:34 403,210 1,000,000 0:22
III. 1:2°5 5,175 1,005,175 0:35 Broke.
Since these experiments were made the beam has been repaired, and has
made 1,500,000 additional changes with a load equivalent to one-fourth of the
breaking weight without giving way. It would appear, therefore, that with a
load of this magnitude the structure undergoes no deterioration in its molecular
structure ; and provided a sufficient margin of strength is given, say from five
to six times the working load, there is every reason to believe, from the results
of the above experiments, that girders composed of good material and of
sound workmanship are indestructible so far as regards mere vibratory action.
As the experiments on this important subject are still in progress, we hope
to bring the subject more in detail before the Association at its next Meeting.
A Catalogue ¢f Meteorites and Fireballs, from a.p. 2 to A.D. 1860.
By R. P. Gree, Esq., F.G.S.
1. Turs Catalogue is intended partly as a sequel to the Reports on Lumi-
nous Meteors, now continued for a series of years in the volumes of the British
Association Reports, and partly as a continuation, in a corrected and extended
form, of a Catalogue of Meteorites published by the author, in two papers
on the same subject, in the Numbers of the Philosophical Magazine and
Journal of Science for November and December 1854.
2. The following works and periodicals have been consulted, viz—Thom-
son's Meteorology, 1849; Transactions of the Royal Society ; Nicholson's
Journal of Natural Philosophy ; Thomson’s Annals of Philosophy ; London,
Edinburgh, and Dublin Philosophical Magazine; Brewster's Encyclopedia,
article “ Meteorite ;” Annual Register; Journal of the Asiatic Society of
Bengal; British Association Reports; Proceedings of the Royal Irish
Academy ; Spurgeon’s Annals of Electricity ; New Edinburgh Philosophical
Journal ; Partsch’s, Shepard’s, and Reichenbach’s Catalogues of Meteorites ;
R. Wolf’s, Chladni’s, Boguslawski’s, Quetelet’s, Baumhauer's, and Coulvier-
Gravier’s Catalogues ; Dr. Clark’s Thesis on Iron Meteoric Masses ; Poggen-
dorff’s Annalen; Annales de Chimie et de Physique; Comptes Rendus; Trans-
actions of the Imperial Academy of Arts and Sciences of Vienna, 1859-60,
papers by W. Haidinger; Transactions of the Royal Academy of Brussels ;
Quarterly Journals of the Natural History Society of Zurich, 1856; Die
Feuermeteore insbesondere die Meteoriten, &c., von Dr. Otto Buchner of
CATALOGUE OF METEORITES AND FIREBALLS, 49
Giessen, 1859; Lithologia meteorica del Profesor Joaquin Balcells, Barce-
lona, 1854; Report on Meteorites, by Prof. Shepard; Reports of the Smith-
sonian Institution, United States; Silliman’s American Journal ; as well as
various private notices and public journals. I have likewise to acknowledge
the kind assistance and valuable information received from Herr P. A. Kessel-
meyer, Dr. Buchner, Herr W. von Haidinger, and Professor Heis.
3. The few abbreviations used in this Catalogue speak for themselves, and
hardly need explanation. Where weights of meteorites are stated, it is gene-
rally intended to denominate lbs. Troy, English, though sometimes the Vienna
or Prussian pound has unavoidably been given. Tables of analysis are added
at the end of the catalogues. Genuine cases of stone- or iron-falls and de-
tonating meteors, are marked with an asterisk (*), and in the Tables count
for 1; doubtful cases are marked in the Catalogue with a (?), and count as 4
in the Tables.
The numbers in some of the Tables, it will be found, do not quite agree
with those in the corresponding Tables given in the Report on Luminous
Meteors, in the Volume of the British Association Reports for 1860, owing
to the circumstance that when that Report was presented at the Oxford Meet-
ing the present Catalogue was not then quite completed.
4. A few remarks are added to the Tables, which do not eall for much
comment in this place, as they have mostly already been alluded to in the
aforesaid Report. With regard to the November period for shooting stars,
E. C. Herrick, of the United States, considers it to be advancing into the
year; in A.p. 1202, it occurred about the 26th October; in 1366 on October
30th ; so that the motion of the node of the zone or ring which furnishes
these shooting stars, is at the rate of 3 or 4 days a century ; the period itself
being a recurrent one probably of about 33 years. (See Silliman’s Journal,
No. 91, p. 137, for January 1861.)
5. In the Catalogue itself great care has been taken in separating the dif-
ferent kinds of fireballs and aérolites; hitherto this has not been done with
sufficient care, and large meteors have not unfrequently been called aérolitic,
when not even any detonation has been reported; examples of this not
unfrequently occur in the catalogues of Baumhauer, Kamtz, and Arago.
Dr. Buchner of Giessen, and P. A. Kesse!meyer of Frankfort-on-Maine, will,
I understand, shortly bring out catalogues of aérolitic falls, where details
in matters concerning original authorities and geographical distribution, &c.
will be given very fully.
In the Tables at the end of this Catalogue, Class A includes only cases
where stones or irons have really fallen; Class B, meteors accompanied by
detonation ; Class C, first-class meteors mot accompanied by detonation ; this
class includes all fireballs given in the catalogues up to the year 1820; after
that time, only the most remarkable ones, as in consequence of the subsequent
greatly increased number of observations from about that time, it is evident
the described fireballs would probably be of smaller size than for older ob-
servations ; Class D includes all fireballs mentioned in the catalogues and
supplements, large or small, where no detonation was reported, and of course
includes the C class. The Tables are so cunstructed, that a glance will suffice
to show the results as regards numbers and dates, and the proportion which
one class bears to another; some of them will be found to be not without
some interest.
Note—— Wherever the words “ Stone-fall” or “ Irou-fall” occur, it may be
understood, as a rule, that such phenomenon was also accompanied by a
detonating fireball, or at least by a detonation.
1860. E
REPORT—1860.
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REPORT
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CATALOGUE OF METEORITES AND FIREBALLS. 119
REMARKS.
1. While there appear to be eight yearly maximum and minimum aérolitic
periods for the years generally, there are likewise some indications of other
periods for some of the months taken separately.
Some months may have major or longer periods of maximum, as Novem-
ber, which perhaps has one of about 70 years (though for the sporadic
showers, according to Herrick, one of 33 years, in which case the numbers
of shooting stars should now be again on the increase, so as to culminate in
1866). January has also probably a long or irregular period, as regards
classes A and B. Of late years the numbers for December and January
have evidently been on the increase, and especially as regards the former
month, and this as regards all classes ; and the eighth to the seventeenth days
appears to embrace a time favourable to a considerable increase over the
average for the month. Tables I., II., II., and IV. §
2. The proportionate numbers of each class appear to have varied at dif-
ferent times for the different months. Table VIII.
3. There appear to be aérolitic and meteor epochs both distinct from and
common to each other. A proximate attempt has been made to show some
of these in Table V.; perhaps some of these are more apparent than real;
but the subject is worth consideration.
4. While the aérolitic class, A and B, in its total is under the average for
August, which is the principal and most constant month for an abundance of
sporadic meteors, it is over the average for November, likewise a month
noted for an abundant display of meteors and shooting stars ; and while there
is an increase over the average of detonating meteors (though not of recorded
Stone-falls), from the 9th to the 13th of November, i. e. precisely during the
regular periodical appearance, it is uota little singular that the August aéro-
litie period, if it may be so called, precedes by several days the usual period
of greatest abundance of the shooting stars ; one being August 4 to 7, both
inclusive, and the other August 9 to 12. See Table III.
5. The decided preponderance of aérolitic phenomena, alluded to in the
Report as occurring in the afternoon, as compared with the forenoon, will
be seen clearly given in Table IX.
6. As regards the observed direction of aérolitic and first-class meteors,
there would seem not to be any very great tendency one way or the other ;
it would have been natural to have expected a much more decided leaning to
a Westerly direction. The sudden change from an Easterly direction in Sep-
tember and October (about the time of the autumnal equinox), toa Westerly
direction in November, is remarkable, and calls for especial notice.
7. The considerable increase of aérolitic falls and meteors for the months
of June and July over those of December and January has been previously
alluded to in the Report itself. That more detonating meteors in proportion
to Stone-falls should be recorded during the winter months than during the
summer months, is precisely what might have been expected, and the reverse
holds equally good. Tables VI. and VII.
8. Taking the entire year, there is a much greater tendency towards equality
of distribution in the aérolitic class than is the case with sporadic shooting stars
and the smaller meteors; indeed, were it not for the excess in November (an
excess common to every class apparently), the numbers of the former (Aand
B) would be about equal for the first as for the second half of the year.
120 REPORT—1860.
CORRIGENDA ET ADDENDA.
Page 53, line 22 from top: for “1596” read 1596.x.
Page 59, line 18 from top: for “ Sarthé” read Sarthe.
Page 62, 1804. Apr. 15. Geneva. fireball: add, s.to N.; also, followed by a train of smaller
balls.
Page 64, line 18 from top: for “ Aug. 10” read early part of Aug.
Page 64, line 12 from bottom : for “ Iron-fail” read Stone-fall.
Page 65, line 7 from bottom: fireball at Gottingen; add, followed by many smaller balls.
Page 67, top line: for “1819. June 13. Jonsac’”’ read and add, 1819.x June 13. Jonsac,
Charente, &c. &e.
Page 70, line 5 from top: Gorlitz; fireball; add aérolitic ?.
Page 71, line 11 from bottom: replace the (x) before May 12, by a (?).
Page 71, line 12 from bottom: insert the (x) before May 19. Ekaterinosloff, &c.
Page 72, line 6 from top: read February 27 or February 16.
Page 72, line 11 from bottom of Notes: for “‘ Summer co.’’ read Sumner co.
Page 73, line 3 fron top: add Vouillé near “ Poitiers.”
Page 74, line 21 from top: for ‘ Okaninak ” read Okaninah.
Page 82, line 6 from top: for ‘‘ Nuremberg ” read Nurenberg.
Page 92, after line 5 from top: insert, Apr. 12. Berne. Fireball.
Page 94, line 10 from top : for “ Columb ” read Columbus.
Page 96, after line 16 from bottom: insert 1860.x Feb. 2. Alessandria, Piedmont. A stone-
fall, Also omitted in the Tables.
Report on the Theory of Numbers.—Part Il. By H. J. SrepnHen
Smitu, M.A., F.R.S., Savilian Professor of Geometry, Oxford.
39. Residues of the Higher Powers. Researches of Jacobi.—The principles
which have sufficed for the determination of the laws of reciprocity affecting
quadratic, cubic, biquadratic, and sextic residues, are found to be inadequate
when we come to residues of the 5th, 7th, or higher powers. This was early
observed by Jacobi, when, after his investigations of the eubie and biqua-
dratic theorems, he turned his attention to residues of the 5th, 8th, and 12th
powers*. It was evident, from a comparison of the cubic and biquadratic
theories, that in the investigation of the laws of reciprocity the ordinary
prime numbers of arithmetic must be replaced by certain factors of those
prime numbers composed of roots of unity ; and Jacobi, in the note just re-
ferred to, has indicated very clearly the nature of those factors in the case
of the 5th, 8th, and 12th powers respectively. He ascertained that the two
complex factors composed of 5th roots of unity into which every prime
number of the form 5z+1 is resoluble by virtue of Theorem LV. of art. 30
of this Report, are not prime numbers, i. e. are each capable of decomposi-
tion into the product of two similar complex numbers; so that every (real)
prime number of the form 5x+1 is to be regarded as the product of four
conjugate complex factors ; and these factors are precisely the complex primes
which we have to consider in the theory of ‘quintic residues, in the place of
the real primes they divide. ‘To this we may add that primes of the forms
5n+2 continue primes in the complex theory; while those of the form 52—1
resolve themselves into éwo complex prime factors. Thus
7=7; 1l=(2+a)(2+0°)(2+a*)\(2+a'); 13=13;
19=(4—3(a+a*))(4—3(a?+2°)); 29=(5—(a+a'))(5—(a?+a°)) ;
31=(2—2a)(2—2°)(2—a*)(2—a'), &e.,
* See a note communicated by him to the Berlin Academy on May 16, 1839, in the
‘Monatsberichte’ for that year, or in Crelle, vol. xix. p. 314, or Liouville, vol. viii. p. 268,
in which, however, he implies that he had not as yet obtained a definitive result; nor does
he seem at any subsequent period to have succeeded in completing this investigation.
q
ON THE THEORY OF NUMBERS. 121
where @ is an imaginary 5th root of unity. Precisely similar remarks apply
to the theories of residues of 8th and 12th powers,—real primes of the forms
8u+1, 12”+1, resclving themselves into four factors composed of Sth and
12th roots of unity respectively. By considerations similar to those pre-
viously employed by him in the case of biquadratic and cubic residues,
Jacobi succeeded in demonstrating (thorgh he has not enunciated) the for-
mul of reciprocity affecting those powers for the particular case in which
one of the two primes compared is a real number. But it would seem that
he never obtained the law of reciprocity for the general case of any two
complex primes; and indeed, for a reason which will afterwards appear, it
was hardly possible that he should do so, so long as he confined himself to
the consideration of those complex numbers which present themselves in the
theory of the division of the circle. No less unsuccessful were the efforts of
Eisenstein to obtain the formule relating to 8th powers, by an extension of
the elliptical properties employed by him in his later proofs of the biqua-
dratic theorem *. It does not appear that any subsequent writer has occu-
pied himself with these special theories ; while, on the other hand, the theory
of complex numbers composed with roots of unity of which the exponent is
any prime, has been the subject of an important series of investigations by
MM. Dirichlet and Kummer, and has led the latter eminent mathematician
to the discovery and demonstration of the law of reciprocity, which holds for
all powers of which the exponent is a prime number not included in a cer-
tain exceptional class.
40. Necessity for the Introduction of Ideal Primes.—The fundamental pro-
position of ordinary arithmetic, that if two numbers have each of them no
common divisor with a third number, their product has no common divisor
with that third number, is, as we have seen, applicable to complex num-
bers formed with 3rd or 4th roots of unity, because it is demonstrable that
Euclid’s theory of the greatest common divisor is applicable in each of those
cases. With complex numbers of higher orders this is no longer the case ;
and it is accordingly found that the arithmetical consequences of Euclid’s
process, which are of so much importance in the simpler cases, cease to exist
in the general theory. In particular, the elementary theorem, that a number
can be decomposed into prime factors in one way only, ceases to exist for
complex numbers composed of 23rd + or higher roots of unity—if, at least
(in the case of complex as of real numbers), we understand by a prime fac-
tor, a factor which cannot itself be decomposed into simpler factors}. It
appears, therefore, that in the higher complex theories, a number is not
necessarily a prime number simply because it cannot be resolved into com-
plex factors. But by the introduction of a new arithmetical conception—
that of ideal prime factors—M. Kummer has shown that the analogy with
the arithmetic of common numbers is completely restored. Some prelimi-
nary observations are, however, necessary to explain clearly in what this con-
ception consists.
* See M. Kummer, “ Ucber die Allgemeinen Reciprocitiatsgesetze,” p. 27, in the Memoirs
of the Berlin Academy for 1859.
ft For complex numbers composed with 5th or 7th roots of unity, the theorem still exists ;
for 23 and higher primes it certainly fails; whether ‘it exists or not for 11, 13, 17, and 19,
has not been definitely stated by M. Kummer (see below, Art. 50).
~ “Maxime dolendum videtur” (so said M. Kummer in 1844) “quod hee numerorum
realium virtus, ut in factores primos dissolvi possint, qui pro eodem numero semper iidem
sint, non eadem est numerorum complexorum, que si esset, tota hiec doctrina, que magnis
adhue difficultatibus premitur, facile absolvi et ad finem perduci posset.” (See his Disserta-
tion in Liouville’s Journal, vol. xii. p. 202.) In the following year he was already able to
withdraw this expression of regret.
122 REPORT—1860.
41. Elementary Definitions relating to Complex Numbers.—Let ) be a prime
a
2 ark :
number, and @ a root of the equation 2a =0; then any expression of the
form
F(a)=a,+a,a+4,0°+....+a,_,0*-” were en
in which a@,, a,, @,,.+--+@,_., denote real integers, is called a complex inte-
gral number. To this form every rational and integral function of @ can
always be reduced; and it follows, from the irreducibility of the equation
nal “ :
ae tages that the same complex number cannot be expressed in this
reduced form in two different ways. The zorm otf F(a) is the real integer
obtained by forming the product of all the A—1 values of F(a), so that
N.F(a)=N.F(a*)=... =N. F(a*—!)=F(a). F(a). F(a")... F(a*-!).
The operations of addition, subtraction and multiplication present no pecu-
liarity in the case of these complex numbers; by the introduction of the
norm, the division of one complex number by another is reduced to the case
in which the divisor is a real integer. Thus
fa) _flayE()E(a’)-...F(@) |
F(a) N.F(a) ;
and f(a) is said to be divisible by F(a) when every coefficient in the pro-
duct f(a)F(a*)F(a’)...F(a*—!), developed and reduced to the form (A),
is divisible by N. F(a). When f(a) is not divisible by F(a), it is not, in
general, possible to render the norm of the remainder less than the norm of
the divisor; and it is owing to this circumstance that the common rule for
finding the greatest common divisor is not generally applicable to complex
numbers. If, in the expression (A), we consider the numbers a,, @,.--@,—2
as indeterminates, the norm is a certain homogeneous function of order \—1,
and of A—1 indeterminates; so that the inquiry whether a given real number
is or is not resoluble into the product of \—1 conjugate complex factors, is
identical with the inquiry whether it is or is not capable of representation by
a certain homogeneous form, which is, in fact, the resultant of the two forms
O44 77+ 4,07 Sy 4 +°:° +Gy2y?—*,
and age 9 oo aR! i al ah tin
The problem is considered in the former aspect by M. Kummer, in the latter
by Dirichlet. The methods of Dirichlet appear to have been of extreme
generality, and are as applicable to complex numbers, composed with the
powers of a root of any irreducible equation having integral coefficients, as
to the complex numbers which we have to consider here. Nevertheless, in
the outline of this theory which we propose to give, we prefer to follow the
course taken by M. Kummer: for Dirichlet’s results have been indicated
by him, for the most part, only in a very summary manner *; nor is it in any
case difficult to assign to them their proper place in M. Kummer’s theory ;
while, on the other hand, it would, perhaps, be impossible to express ade-
quately, in any other form than that which M. Kummer has adopted, the
numerous and important results (including the law of reciprocity itself) con-
* See his notes in the Monatsberichte of the Berlin Academy for 1841, Oct. 11, p. 280;
1842, April 14, p. 93; and 1846, March 30; also a letter to M. Liouville, in Liouville’s
Journal, vol. v. p. 72; a note in the Comptes Rendus of the Paris Academy for 1840,
vol. x. p. 286; and another in the Monatsberichte for 1847, April 15, p. 139,
ON THE THEORY OF NUMBERS, 123
tained in the elaborate series of memoirs which he has devoted to this sub-
ject *.
42. Complex Units——A complex unit is a complex number of which the
norm is unity. If \=3, there is only a finite number [six] of units included
in the formula +a". But for all higher values of X, the number of units is
infinite. Nevertheless it is always possible to assign a system of »—1 units
(putting, for brevity, 3(A—1)=,) such that ad/ units are included in the
formula tatu ....u ts"; in which w,, t@,, Ws)+++%,—1 are the assigned
units, and f, 7,, 2,,..-2,—1, are real (positive or negative) integral numbers.
A system of units, capable of thus representing all units whatsoever, is called
a fundamental system. The existence, for every value of A, of fundamental
* The following is a list of M. Kummer’s memoirs on complex numbers :—
1, De numeris complexis qui radicibus unitatis et numeris realibus constant, Breslau,
1844. This is an academical dissertation, addressed by the University of Breslau to that of
Konigsberg, on the tercentenary anniversary of the latter. It has been inserted by M. Liou-
ville in his Journal, vol. xii. p. 185.
2. Ueber die Divisoren gewisser Formen der Zahlen, welche aus der Theorie der Kreis-
theilung entstehen.—Crelle, vol. xxx. p. 107.
3. Zur Theorie der Complexen Zahlen, in the Monatsberichte for March 1845, or in
Crelle, vol. xxxv. p. 319.
4. Ueber die Zerlegung der aus Wurzeln der Einheit gebildeten complexen Zahlen in ihre
Primfactoren.—Creille, vol. xxxv. p. 327. The date is Sept. 1846.
5. A note addressed to M. Liouville (April 28, 1847), in Liouville’s Journal, vol. xii. p. 136.
6. Bestimmung der Anzahl nicht zquivalenter Klassen fiir die aus Aten Wurzeln der Ein-
heit gebildeten complexen Zahlen, und die idealen Factoren derselben.—Crelle, vol. xl. p. 93.
7. Zwei besondere Untersuchungen iiber die Classen-Anzahl, und iiber die Einheiten der
aus Aten Wurzeln der Einheit gebildeten complexen Zahlen.—Crelle, vol. x1. p- 117. (See
also the Monatsberichte of the Berlin Academy for 1847, Oct. 14, p. 305.)
8. Allgemeiner Beweis des Fermat’schen Satzes, dass die Gleichung 2*+-y%=7zA unlésbar
ist, fiir alle diejenigen Potenz-Exponenten A, welche ungerade Primzahlen sind, und in den
Zahlern der ersten 3(\—3) Bernouillischen Zahlen als Factoren nicht vorkommen.—Crelle,
vol. xl. p.131. (See also the Monatsberichte for 1847, April 15, p.132.) This and the two
preceding memoirs are dated June 1849.
9. Recherches sur les Nombres Complexes.—Liouville, vol. xvi. p. 377. This memoir
contains a very full résumé of the whole theory, and may be read by any one acquainted
with the elements of the theory of numbers.
10. A note in the Monatsberichte of the Berlin Academy for May 27,1850, p. 154, which
contains the first enunciation of the law of reciprocity.
11. Ueber die Erganzungssitze zu den Allgemeinen Reciprocitatsgesetzen.—Crelle, vol. xliv.
p- 93 (Nov. 30, 1851), and vol. lvi. p. 270 (Dec. 1858).
12, A note on the irregularity of determinants, in the Berlin Monatsberichte for 1853,
March 14, p. 194,
13, Ueber eine besondere Art aus complexen Einheiten gebildeter Ausdriicke.—Crelle,
vol. l. p. 212 (Aug, 31, 1854).
14. Ueber die den Gaussischen Perioden der Kreistheilung entsprechenden Congruenz-
wurzeln.—Crelle, vol. liii. p. 142 (June 5, 1856).
15. Einige Satze tiber die aus den Wurzeln der Gleichung aA =1 gebildeten complexen
Zahlen fiir den Fall, dass die Klassenzahl durch A theilbar ist, nebst Anwendung derselben
auf einen weiteren Beweis des letzten Fermat’schen Lehrsatzes.—Memoirs of the Berlin
Academy for 1857, p.41. An abstract of this memoir will be found in the Monatsberichte
for 1857, May 4, p. 275.
16. Theorie der Idealen Primfactoren der complexen Zahlen, welche aus den Wurzeln
der Gleichung w”=1 gebildet sind, wenn n eine zusammengesetzte Zahl ist.—Memoirs of the
Berlin Academy for 1856, p. 1.
17. Ueber die Allgemeinen Reciprocitatsgesetze unter den Resten und Nicht-Resten der
Potenzen, deren Grad eine Primzahl ist—Memoirs of the Berlin Academy for 1859, p. 20.
Tt was read on Feb. 18, 1858, and May 5, 1859. An abstract will be found in the Monats-
berichte of the former year.
A memoir by M. Kronecker (De unitatibus complexis, Berlin, 1845; it is his inaugural dis-
sertation on taking his doctorate) connects itself naturally with the earlier memoirs of the
preceding series. :
124 REPORT—1860.
systems of »—1 units may be established by means of a general proposition
due to Dirichlet and relating to any irreducible equation having unity for
its first coefficient, and all its coefficients integral. If, in such an equation,
R be the number of real, and 2I of imaginary roots, there always exist
systems of R+I—1 fundamental units, by means of which all other units
can be expressed; or, in other words, the indeterminate equation “Norm
=1” is always resoluble in an infinite number of ways, and all its solutions
can be expressed by means of R+I—1 fundamental solutions*. The demon-
stration of the actuai existence, in every case, of these systems of fundamental
units (a theorem which is, as Jacobi has said+, “un des plus importants,
mais aussi un des plus épineux de la science des nombres”) is of essential im-
portance in the theory of complex numbers, and has the same relation to
that theory which the solution of the Pellian equation 2*—Dy’=1 has to
the theory of quadratic forms of determinant D. It may be observed, how-
ever, that in the case which we have to consider here, that of the equation
a
= 7 =o the existence of fundamental systems of »—1 units has been
a=
demonstrated independently of Dirichlet’s general theory by MM. Kro-
necker and Kummerf.
If A=5, a+a-! is the only fundamental unit; so that every unit is in-
cluded in the formula
ta*(a+a-1)”.
If \=7, the complex units are included in the formula
ta* (atta) (a? +a),
But for higher primes the actual calculation of a system of fundamental units
involves great labour; and a method practically available for the purpose
has not yet been given. It is remarkable that every unit can be rendered
real (i. e. a function of the binary sums or periods a'+a—", &c.) by multi-
plying it by a properly assumed power of a. We shall therefore suppose, in
* To enunciate Dirichlet’s theorem with precision, let f(v)=0 be the proposed equation ;
let 1, @g)+.. a» be its roots, and y(a,), (#,),..- P(#n) a system of n conjugate units. If
the analytical modulus of every one of the quantities Y(«;), W(a2),...W(#,) be unity, the
system of units is an isolated or singular system. The number of singular systems (if any
such exist) is always finite, whence it is easy to infer that the units they comprise are
simply roots of unity. For if ~(«) be a singular unit, its powers are evidently also singular
units, and therefore cannot be all different from one another; 7. e. /(«) is a root of unity.
If f(x) be of an uneven order, there are no singular units; if f(a) be of an even order, —1
is a singular unit; and if /(a)=0 have any real roots, it is the only singular unit; whereas
if all the roots of f(a#)=0 be imaginary, other singular units may in special cases exist.
A
tae
nO =0 has 2(A—1) singular units included in the formula +e*, Ad-
mitting this definition of singular units, we may enunciate Dirichlet’s theorem as follows :—
a system of A units [A=I+R—1], e,(a), eo(),...ex(@), composed with any root #, can
always be assigned such that every unit composed with the same root can be represented
(and in one way only) by the formula
w .€y(a)"1. €5(a)"2, @,(c)"3.... en()"A,
where 7, 7%)... 7, are positive or negative integral numbers and w is unity, or some one of
the singular units composed with a.
The principles on which the demonstration of this theorem depends are very briefly indi-
cated in the notes presented by Dirichlet to the Berlin Academy in 1841, 1842, and 1846.
+ Crelle’s Journal, vol. xl. p. 312.
{ See Kronecker, De unitatibus complexis, pars altera; and Kummer, in Liouville’s Jour-
nal, vol. xvi. p. 383.
Thus the equation
ea. ee
ON THE THEORY OF NUMBERS. 125
what follows, that the units of which we speak have been thus reduced to a
real form.
For all values of d greater than 5, the nuinber of systems of fundamental
units is infinite. For if w,, w,,...%¢,—1 still represent a system of fundamental
units, it is evident that the system E,, E,, ... E,—1, defined by the equations
1,1 1,2 (1, #—1)
E, = us , vee X UT gp
(1), (2,2) (2, w—1)
FE, =u, us a nsie.e Boe aes Me en CA
Ewa) ae Se tea BS). |
is also a fundamental system, if the indices (1, 1), &c. be integral numbers,
and if the determinant 2+(1, 1)(2,2)....(—1, p—1) be equal to unity.
And conversely, every system of fundamental units will be represented by
the equations (A.), if in them we assign to the indices (1, 1), (2, 2), &e.
all systems of integral values in succession consistent with the condition
Z+(1,1)(2,2)(3, 3).--(u—I, p—1)=+£1; so that a single system of fun-
damental units represents to us all possible systems.
We shall also have occasion to allude to independent systems of units. A
system of p—1 units, w,, w,,..U%,—1, is said to be independent when it is
impossible to satisfy the equation
ur ur ur at wee =1,
whatever integral values are assigned to the indices 7,, %,, 2) +++ My—1>
The equations (A.) will represent all possible systems of independent units,
if we suppose that in them the indices (1,1), (2,2), (3,3)... receive all
positive and negative integral values, subject only to the condition that the
determinant A=3+(1, 1) (2,2).--(#—1, »—1) must not vanish. Every
system of fundamental units is also independent; but not conversely. Every
unit can be represented as a product of the powers of the units of an inde-
pendent system ; but if the system be not also fundamental, the indices of the
powers are not in general integral, but are fractions having denominators
which divide A. Lastly, if ¢,(a), ¢,(a@),...- ¢u-1(@) be a system of inde-
pendent units, the logarithmic determinant
L.e¢,(@), L.¢,(a), aoe iewr Cr enc) A
L.¢,(a@”), PC aP ay | ts sree ee Oe (ae Yop
L. e(at~*), L. e(a”~*), Sey, Slee ema. )s
in which y denotes a primitive root of X, is different from zero; and con-
versely, if the determinant be different from zero, the system of units is inde-
pendent. For all systems of fundamental units, the absolute value of the
logarithmic determinant is the same; for any other independent system, its
value is A times that least value. The quantities denoted by the symbols
L.c,(a), L.e,(a), &c., are the arithmetical logarithms of the real units ¢,(«),
&c., taken positively.
43. Gauss’s Equations of the Periods——In Gauss’s theory of the division
of the circle, it is shown that if X be a prime number, and if ef=A—1, the e
periods of f roots cach, that is the quantities ,, 7,. 7, +++. 7,_,, defined by
the equations
126 REPORT—1860.
0 , _2 ay
iy ed! + av +a? E = evatoiets seal °
Et vet ~2e+1 (f—Ve+1
Beutcee! . ce aatew cteebes +a!
~e—1 ~Ze—1 3e—1 fe—1
Ne-=a ta? +a’ + eee tar
(y still denoting a primitive root of \), are the roots of an irreducible equa-
tion of order e having integral coefficients, which we shall symbolize by
F(y)=y°+ Ay '+A,y° 7+... A, ytA,=0
(see Disq. Arith. art. 346). This equation is of the kind called Abelian;
that is to say, each of the e periods is a rational function of any other, in
such a manner that we may establish the equations »,=9(»,), 7,=0(n,)s
7;=9(n,), «+++ 25=¢(ne-1); Where it is to be observed that the coefficients
of the function ¢ are not in general integral. The determination of the
coefficients of the equation F(y)=0 may be effected, for any given prime A,
and any given divisor e of A—1, by methods which, however tedious, present
no theoretical difficulty. Every rational and integral function of the periods
can be reduced to the form a,y,+a,n,+4,n,+ --+a,_,n,_;. If we com-
bine the equation 1+ 7,+7,+7,+..--+7e-1=0 with the e—2 equations,
by which 75, 79, -+-+ 5 | are expressed in that linear form, we may elimi-
nate 7,, 7) +++ %e—1, and shall thus obtain an equation of order e, satisfied by
No te. the equation of the periods, or F(y)=0. This is the method proposed
by Gauss (Disq. Arith. art. 346) ; M. Kummer, instead, forms the system of
equations
m7 == n, f+ (0,0), +(0, 1)n, +(0,2)n.+ --- +(0,e—1)ne-1,
mm, =2,f+(1,0)n, + 1)n,+C1,2)n,+ ---+C1,e—1)ne-1,
oN =n, f+ (2, 0)n,+(2, 1)n, +(2, 2)n.+ eee (2, e—1)me-1,
~ . . . 7 . . . . . . . . . . .
Ne =Ne-1f + (e—1, 0)n, +(e—1, 1)y, +(e—1,2)n,+ eee +(e— 15 e—1)ne-1,
and eliminates 7,, 7,5 --.e—1 from them. The symbol (4, /) represents the
number of solutions of the congruence y¥+*==1+y*+t*, mod A, w and y
denoting any two terms of a complete system of residues for the modulus f;
nx is zero for all values of k, excepting that 2,=1, if f be even, and m,=1,
if f be uneven*. The systems of equations corresponding to the particular
cases e=3, e=4, have been given by Gauss, who has succeeded in expressing
the values of the coefficients (2, 2) in each of those cases by means of num-
bers depending on the representation of \ by certain simple quadratic forms ;
and has employed these expressions to demonstrate the criterion already men-
tioned in this Report for the biquadratic character of the number2+. A
third method has been given by M. Libri{: he establishes the formula
ANL=M + n(1 +e.) + 0,(1 ben.) + +++ nea(1 Heres);
in which N; represents the number of solutions of the congruence
* Liouville’s Journal, vol. xvi. p. 404.
+ Disq. Arith. art. 358, and Theor. Res. Big. arts. 14—22.
+ See the memoir “‘ Sur la Théorie des Nombres,” in his ‘ Mémoires de Mathématique et
de Physique,’ pp. 121,122. The notation of the memoir has been altered in the text. See
also M. Lebesgue, in Liouville’s Journal, vol. ii. p. 287, and vol, iii. p. 113.
ON THE THEORY OF NUMBERS. 127
1+ai+apg+...+a,=0, mod A*.
If S,, S,, S,... denote the sums of the powers of the roots of the equation
F(y)=0, this formula may be written thus, —
k.k—-1 :
ANL=\* + 8, +heS,+——g— &S, + woe Ses,
or, solving for S,, S,,...,
#8.4:=2 Ne—AN at “ns oo ~(-)N, —(r=1)*.
From this equation, when the values of N,, N,, &c., have been determined,
S,, S,,... may be calculated, and thence by known methods the values of
the coefficients of the equation F(y)=0. Lastly, M. Lebesgue has shown
that, if we denote by o, the number of ways in which numbers divisible by
d can be formed by adding together & terms of the series y°, y',. . -yA-2, sub-
ject to the condition that no two powers of y be added the indices of which
are congruous for the modulus e, the function (A—1)F(y) assumes the form
ALY —o, y+ ony* "— «2. +(—1)° oe] —(y—S)'t-
But the practical application of any of these methods is very laborious
when X is a large number, chiefly on account of the determinations which
they all require of the numbers of solutions of which certain congruences are
pobre mie es a ons
susceptible. For e=2 the equation is vty. o, or, putting
r=2y+1, r°—(—1)"A=0. The cubic and biquadratic equations corre-
sponding to the cases e=3 and e=4 are also known from Gauss’s investiga-
tions. The results assume the simplest forms if we put r=ey+1. We then
have
(1) e=3, 4A=M?+27N?, M=1, mod 3; 7°—3Ar—AM=0.
(2) e=4; A=A’°+B’*; A=I1, mod 4; e=(—1)%
[7°+(1—2e)A]?—4A (r—A)?=0f.
Though these determinations are not required in M. Kummer’s theory, we
have nevertheless given them here, in order to facilitate arithmetical verifi-
cations of his results. The forms of the period-equations for the case r=8
and e=12 can (it may be added) be elicited from the results given by Jacobi
in his note on the division of the circle (Crelle, vol. xxx. pp. 167, 168.).
44. The Period-Equations considered as Congruences.—An arithmetical
property of the equation F(y)=O0, which renders it of fundamental import-
ance in the theory of complex numbers, is expressed in the following theorem.
“If g be a prime number satisfying the congruence gf=1, mod \, the
congruence F(y)=0, mod q, is completely resoluble, 7. e. it is possible to
establish an indeterminate congruence of the form
F(y)=(y—%) (y—u,) «+» (y—ue-1), mod g,
* In this congruence 2}, 2»,... x; are & terms (the same or different) of a complete system
of residues for the modulus ) ; and in counting the number of solutions, two solutions are to
be considered as different in which the same places are not occupied by the same numbers.
A simpler formula for S;,,, may be obtained by considering 2, 2g, ... 2, to represent terms
of a system of residues prime to A, and denoting by ey, the number of solutions of M. Libri’s
congruence on this hypothesis. We thus find 8z+1=Ayx— f* (Liouville, vol. iii. p. 116).
+ Liouville, vol. iii. p. 119. ‘
= M. Lebesgue, Comptes Rendus, vol. li. p.9. Gauss has not exhibited this last equation
in its explicit form. See Theor. Res. Big. 2. ¢.
123 REPORT—1860.
Ups Uyy ++ + Ue—1 Aenoting integral numbers, congruous or incongruous, mod q*.”
: : : ee
A particular case of this theorem, relating to the equation ae =0
(which may of course be regarded as the equation of the A—1 periods, con-
sisting each of a single root), is due to Euler, and is included in his theory
of the Residues of Powers; for it follows from that theory (see art. 12 of this
Report), that the binomial congruence x\—1=0 (and therefore also the
x—
congruence =0, mod g) is completely resoluble for every prime of
the form mA+1.
A remarkable relation subsists between the periods 7,, 7, «++ me—1 Of the
equation F(y)=0, and the roots 2,, 0,, Uz +++ Ue—1 of the conyruence F(y)=0,
mod g. This relation is expressed in the following theorem :—
«“ Every equation which subsists between any two functions of the periods,
will subsist as a congruence for the modulus g when we substitute for the
periods the roots of the congruence F'(y)==0 taken in a certain order.”
It is immaterial which root of the congruence we take to correspond to any
given root of the equation. But when this correspondence has once been esta-
blished in a single case, we must attend to the sequence which exists among
the roots of the congruence corresponding to the sequence of the periods.
When w,, u,, ... %e—1 are all incongruous, their order of sequence is deter-
mined by the congruences
U,= (4), U=O(uU,), «++. U=G(Me-1), mod g,
which correspond to the equations
=I)» m= GCM)» +++ + Mo = HCMe=1)»
and which are always significant, although the coefficients of @ are frac-
tional, because it may be proved that their denominators are prime to the
modulus g. When w,, %;+++%e—1 are not all incongruous [an exceptional
case which implies that g divides the discriminant of F(y)], a precisely simi-
lar relation subsists, though it cannot be fixed in the same manner, and though
the number of incongruous solutions of the congruence is not equal to the
number of the periods. (See a paper by M. Kummer in Crelle’s Journal,
* This theorem was first given by Schoenemann (Crelle, vol. xix. p. 306); his demonstra-
tion, however, supposes that g =e,—a limitation to which the theorem itself is not subject.
The following proof is, with a slight modification, that given by M. Kummer (Crelle, vol. xxx.
p- 107, or Liouville, vol. xvi. p. 403). From the indeterminate congruence of Lagrange (see
art. 10 of this Report)
x(a—1) (w7—2)....(v—g+1) =a! —2, mod g,
it follows that
(y—nx) (Y—g—1) (Y= MK—2) «+ YM IFAD SY 14)" — (Yn)
=y! — ng! — (ym) =" —y, mod g,
observing that ,.4=n,41naq» and that, if Ind g be divisible by e (or, which is the same
thing, if g satisfy the congruence gf=1, mod X), np41nd g=7%- Multiplying together the
e congruences obtained by giving to & the e values of which it is susceptible in the formula
(y—nx) Y—2¢-1) YE 2) + (Y= Me) Sy" —y, mod g,
we find
F(y) F(y—1) F(y—2) «-- Fy—gt )=(y?—-)*, mod g;
whence, by a principle to which we shall have occasion to refer subsequently (see Art. 69), it
appears that F(y) is congruous for the modulus g to a product of the form
(y—uy) (y=) + (Y—Ue_)-
ee
ON THE THEORY OF NUMBERS. 129
vol. liii. p. 142, in which he has established this fundamental proposition on
a satisfactory basis.)
45. Conditions for the Divisibility of the Norm of a Complex Number by
a Real Prime*.—Instead of the complex number
S(a)=a,+a, a+a,a’+.... +a), a\-%,
let us now, for a moment, consider the complex number
W(n)=e, NAC, M1 NaH +002 +Ce—1 Ne—1y
which, with its conjugates
Yin) =e, me, No lg Ng oe ee +Ce—1 No»
b(n.) =e, M+¢, 1; +¢, 14 oe Sie +¢e_1 Ny
eerste reoeeeeesere ee eoee sess ve vese
W(ne-1) =e, Ne—1 +, No +e, Nees Ce} Ne—2
is a function of the periods only, and is therefore a specialized form of the
general complex number f(a); and let ¢ still denote a real prime, satisfying
the congruence gf=1, mod d. By means of the relation subsisting between
the equation-roots 7, 7,, -+ e—1, and the congruence-roots %,, %,) ++ We—1y
M. Kummer has demonstrated the two following theorems :—
(i.) “The necessary and sufficient condition that (7) should be divisible
by q (z.e. that the coefficients ¢,, c,,...¢e—, should be all separately divi-
sible by q) is that the e congruences
W(u,) =e,u, +e, u,+0,U,+ .+++ +ee—1 M1 =0, mod g,
Yu) =e,u, +e,u,te,u,t..0.+¢c-1u%, ==0, mod q
W(Ue-1) =6, Ue-1 +6, Uy +e, U,+ . 60. +c] Ue~2 =0, mod qd
should be simultaneously satisfied.”
(ii.) “The necessary and sufficient condition that the norm of (7), taken
with respect to the periods, z.e. the number (n,) p(n,)..+- W(ne-1), should
be divisible by g, is that one of the e congruences
Y(u,) =0, W(w,) =0,...+++b(we-1) =0, mod q,
should be satisfied.”
These results may be extended to any complex number f(a), by first
reducing it to the form
S(a)=, (n,) +a y, (n)) +a" p, (n.)+ vee fall Wye (1).
This is always possible; for, since the f roots which compose any one
period, ¢. g. 4,, are the roots of an equation y(a)=0 of order f, the coeffi-
cients of which are complex integers involving the periods only}, we may
simply divide f(a) by x(a), and the remainder will give us the expression
of f(a) in the required form. Further, let g now denote a prime apper-
taining to the exponent f (not merely satisfying the congruence gf =1, mod A,
but also satisfying no congruence of lower index and of the same form).
The two preceding theorems are then replaced by the two following, which
are analogous to them, and include them.
* The outline of the theory of complex numbers contained in this and the subsequent
articles is chiefly derived from M. Kummer’s mémoire in Liouville, vol. xvi. p. 411.
T Disq. Arith. art. 348.
60. K
130 REPORT— 1860.
(i.) “The necessary and sufficient condition that f(a) should be divisible
by q, is that the congruences
(ux) =0, w, (ux) =0, aint (ux~)=0, mod g,
should be simultaneously satisfied for every value of k.”
(ii.) “ And the condition that the norm of f(a) should be divisible by 9,
is that the same congruences should be satisfied for some one value of k.”
When the congruences W, (wz )=0, Ww, (wr) =0, ... - by-1(&e) =0, mod g,
are simultaneously satisfied, f(a) is said to be congruous to zero (mod q), for
the substitution n,=u; These f congruences may be replaced by a single
congruence in either of two different ways. Thus, if we denote by F(y,) the
complex number involving the periods only which we obtain by multiplying
together the f complex numbers
FA FU FO Dy sss fet eel
it may be proved that the single congruence F (w,)==0, mod q, is precisely
equivalent to the f congruences
W,(uz)=0, W,(uz)=0,.... bei (ux) =0.
Or, again, if we denote by ¥(»,) a complex number congruous to zero for
every one of the substitutions 7,=,, 7,>=U. +--+ 4)>=Ue—1, but not con-
gruous to zero for the substitution 7,=u, (such complex numbers, involving
the periods only, can in every case be assigned) *, it is readily seen that the
same f congruences are comprehended in the single formula
W (ne-x) f (a) =0, mod g.
The utility of this latter mode of expressing the f congruences will appear in
the sequel: the formula F(az-)=0, mod q, is of importance, because it
supplies an immediate demonstration of the important proposition, that “if
a product of two factors be congruous to zero for the substitution 7,=wz,
one or other of the factors must be congruous to zero for that substitution.”
46. Definition of Ideal Prime Factors.—To develope the consequences of
the preceding theorems, let us consider a prime number gq appertaining to
the exponent f; and let us first suppose that it is capable of being expressed
as the norm (taken with respect to the periods) of a complex number (7),
which contains the periods of f terms only; so that
q=(n) Cm) + +++ (me-1)-
If the substitution of uw, in W render Y(w,)=0, mod g, we may distinguish
the e factors of g by means of the substitutions which respectively render
them congruous to zero; so that, for example, U(x) is the factor apper-
taining to the substitution n, =.
We thus obtain the theorem that if f(a) be congruous to zero, mod g, for
any substitution »,=w,, f(a) is divisible by the factor of g appertaining to
that substitution. For if Y(,) be that factor of g,
S(@) _ fle)Y(n Vn)» bne-1) ,
Wn) q ;
but f(a) d(n,) W(n,) «++ (ner) is congruous to zero, mod q, for every one of —
the substitutions y,=w,, 4,=U,, ++» 7,=Ue—-1; it is consequently divisible
by q; i.e. f(a) is divisible by U(m,). A useful particular case of this theo-
rem is that wz—7,=0, mod Y(n,), if Y(w,)=0, mod q.
* Crelle, vol. lili, p. 145. The number W(7) of this memoir possesses the property in
question.
ON THE THEORY OF NUMBERS. 131
Again, it may be shown that these complex factors of g are primes in the
most proper sense of the word: 2.e., first, that they are incapable of reso-
lution into any two complex factors, unless one of those factors be a complex
unit; and secondly, that if any one of them divide the product of two factors,
it necessarily divides one or other of the two factors separately. That W(n,)
possesses the first property is evident, because its norm is a real prime, and
that it possesses the second is a consequence of the last theorem of Art. 4.5.
For if W(,) divide f,(a) xf,(«), either f(a) or f(a), by virtue of that theo-
rem, is congruous to zero (mod q) for the substitution »,=«,; that is to say,
either f(a) or f,(a) is divisible by 1(»,).
ow, if every prime g which appertains to the exponent f were actually
eapable of resolution into e complex factors composed of the e periods of
Ff roots, these factors would represent to us all the true primes to be con-
sidered in the theory of the residues of Ath powers. And for values of J infe-
rior to 11, perhaps to 23, this is, in fact, the case. But for higher values of
X, the real primes appertaining to the exponent f divide themselves into two
different groups, according as they are or are not susceptible of resolution
into e conjugate factors. Let, then, g represent any prime appertaining to the
exponent f, whether susceptible or not of this resolution, and let f(a) still
denote a complex number which is rendered congruous to zero by the sub-
stitution n,=w,; f(a) is said by M. Kummer to contain the ideal factor of q
appertaining to the substitution n,=u,. ‘This definition is admissible, because
it is verified, as we have just seen, when ¢ is actually resoluble into e con-
jugate factors; and its introduction is justified, as M. Kummer observes, by
its utility. To obtain a definition of the multiplicity of an ideal factor, we
may employ a complex number ¥(7) possessing the property indicated in
the last article. If of the two congruences
C¥(n)]” f(a)=0, mod q”,
[¥(n.)]"**f(a)=0, mod g”*+},
the former be satisfied, and the latter not, f(a) is said to contain 7 times
precisely the ideal factor of g which appertains to the substitution »,=w,.
47. Elementary Theorems relating to Ideal Factors—The following pro-
positions are partly restatements (in conformity with the definitions now
intreduced) of results to which we have already referred, and partly simple
corollaries from them. They will serve to show that the elementary proper-
ties of ordinary integers may now be transferred to complex numbers.
(1.) A complex number is divisible by g when it contains all the ideal
factors of g. If it contain all of those factors 2 times, but not all of them
n+1 times, it is divisible by g”, but not by g”*!.
(2.) The norm of a complex number is divisible by g when the complex
number contains one of the ideal factors of g. If (counting multiple factors)
it contain, in all, of the ideal factors of g, the norm is divisible by g’/, but
by no higher power of g (f denoting the exponent to which g appertains).
(3.) A product of two or more factors contains the same ideal divisors as
its factors taken together.
(4.) The necessary and sufficient condition that one complex number
should be divisible by another is, that the dividend should contain all the
_ ideal factors of the divisor at least as often as the divisor.
(5.) Two complex numbers which contain the same ideal factors are
identical, or else differ only by a unit factor.
(6.) Every complex number contains a finite number of ideal prime fac-
tors. These ideal prime factors (as well as the multiplicity of each of them)
are perfectly determinate.
K 2
132 REPORT—1860.
The prime number ) is the only real prime excluded from the preceding
considerations. Since \=(1—a)(1—a’)..-.(1—a—}), it appears that the
norm of 1—a is a real prime, and therefore 1—a cannot be resolved into
the product of two factors, except one of them be a unit. Again, because
the necessary and sufficient condition for the divisibility of a complex number
by 1—a is that the sum of the coefficients of the complex number should
be congruous to zero for the modulus \, and because the sum of the coeffi-
cients of a product of complex numbers is congruous, for the modulus A, to
the product of the sums of the coefficients of the factors, it appears that if
the norm of a complex number is divisible by A, the complex number is itself
divisible by 1—a; and also that if the product of two complex numbers be
divisible by 1—a, one or other of the factors separately must be divisible by
1—a. Hence 1—a is a true complex prime, and is the only prime factor of
A; in fact, A=(1—a)(l—a’)... (1—ad—!)=e(a)(L—a)\-}, if e(a) denote
. the complex unit
1—a®? 1—a’° 1—ad-}
ta 12 l—a
The theorems which have preceded enable us to give a definition of the
norm of an ideal complex number. If the ideal number contain the factor
1—a m times, and if it besides contain &, k',k',...- prime factors of the
primes g, q', g",.... appertaining to the exponents f, f', f", -... respectively,
we are to understand by its norm, the positive integral number
AM GS glES qMEF" 6.05
a definition which, by virtue of the second proposition of this article, is
exact in the case of an actually existing number.
It will be observed that the number of actual or ideal prime factors (com-
pound of Xth roots of unity) into which a given real prime can be decom-
posed, depends exclusively on the exponent to which the prime appertains
for the modulus A. If the exponent is f, the number of ideal factors is
aa =e. Thus, if g be a primitive root of \, g continues a prime in the
A-1
complex theory ; if it be a primitive root of the congruence x 7 =I, mod A,
it is only resoluble into two conjugate prime factors. This dependence of
the number of ideal prime factors of a given prime upon the exponent to
which it appertains is a remarkable instance of an intimate and simple con-
nexion between two properties of the same prime number, which appear at
first sight to have no immediate connexion with one another.
It may be convenient to remark that the word Ideal is sometimes used so
as to include, and sometimes so as to exclude, actually existent complex
numbers; but it is not apprehended that any confusion can arise from this
ambiguity, which it is not worth while to remove at the expense of intro-
ducing a new technical term.
48. Classification of Ideal Numbers——An ideal number (using the term
in its restricted sense) is incapable of being exhibited in an isolated form —
as a complex integer; as far as has yet appeared, it has no quantitative —
existence ; and the assertion that a given complex number contains an ideal
factor, is only a convenient mode of expressing a certain set of congruential
conditions which are satisfied by the coefficients of the complex number.
Nevertheless we may, without fear of error, represent ideal numbers by the
same symbols, f(a), F(a), ¢(a@)..., which we have employed to denote
actually existing complex numbers, if we are only careful to remember that
these symbols, when the numbers which they represent are ideal, admit of
ON THE THEORY OF NUMBERS. 133
combination by multiplication or division, but not by addition or subtraction.
Thus f(a) x f(a), f(«)+f,(«), [f(«)]”; are significant symbols, and their
interpretation is contained in what has preceded; but we have no general
interpretation of a combination such as f(@)+f,(«), or S(«)—f(«)*. This
symbolic representation of ideal numbers is very convenient, and tends to
abbreviate many demonstrations.
Every ideal number is a divisor of an actual number, and, indeed, of an
infinite number of actual numbers. Also, if the ideal number ¢(a) be a
divisor of the actual number F(a), the quotient ¢,(a)=F(a) +¢(«) is always
ideal; for if ¢,(a) were an actual number, ¢(a), which is the quotient of
F(a) divided by 9,(a), ought also to be an actual number, It appears,
therefore, that there exists an infinite number of different ideal multipliers,
which all render actual the same ideal number. It has, however, been shown
by M. Kummer that a finite number of ideal multipliers are sufficient to
render actual all ideal numbers whatever; so that it is possible (and that in
an infinite number of different ways) to assign a system of ideal multipliers,
such that every ideal number is rendered actual by one of them, and one only.
Ideal numbers are thus distributed into a certain finite number of classes,—
a class comprehending those numbers which are rendered actual by the same
multiplier; and this distribution into classes is independent of the particular
system of multipliers by which it is effected, inasmuch as it is found that if
two ideal numbers be rendered actual by the same multiplier, every other
multiplier which renders one of them actual will also render the other actual.
Ideal numbers which belong to the same class are said to be egutvalent; so
that two ideal numbers, which are each of them equivalent to a third, are
equivalent to one another. We may regard actual numbers (which need
no ideal multiplier) as forming the first or principal class in the distribution,
and, consequently, as all equivalent to one another. If f(a) be equivalent to
S(a@), and g(a) to ¢,(a), f(a) x g(a) is equivalent to f(a) x $,(a),—a result
which is expressed by saying that “equivalent ideal numbers multiplied by
equivalent numbers, give equivalent products;” and the class of the product
is said to be the class compounded of the classes of the factors.
49. Representation of Ideal Numbers as the roots of Actual Numbers.—
An important conclusion is deducible from the theorem that the number of
classes of ideal numbers is finite. Let f(a) be any ideal number; and let us
consider the series of ideal numbers f(a), f(a)’, /(@)’,... These numbers
cannot all belong to different classes; we can therefore find two different
powers of f(a), for example [/(a)]” and [f(«)]”*”, which are equivalent
to one another. But the equivalence of these numbers implies that [/(a@) ]”
is equivalent to the actual number+1; ¢. e. that [/(«)]” is itself an actual
number. We may therefore enunciate the theorem, “ Every ideal number,
raised to a certain power, becomes an actual number.”
The index of this power is the same for all ideal numbers of the same class,
but may be different for different classes. By reasoning precisely similar
to that employed by Euler in his 2nd proof of Fermat’s Theoremf, it may
be proved that the index of the first term in the serics f(a), [/(«)]’,
[/(@)]°..-, which is an actual number, is either equal to the whole number
of classes, or to a submultiple of that number. This least index is said to be
the exponent to which the class of ideal numbers containing f(a) appertains.
* These symbols are, however, interpretable when f(a) and f,(a) belong to the same
i ome ©) ae. is ae Xf, («) be both actual, f(«) +f, («) is the ideal quo-
ent obtained by dividing 9 («) xf («)+¢@(«) xf, (a) by 9 (a).
Tt See art. 10 of this Report, ‘ tye
134 REPORT—1860.
It would seem that for certain values of the prime A, there exist classes of
ideal numbers appertaining to the exponent H, if H denote the number of
classes of ideal numbers*. Such classes (when they exist) possess a property
similar to that of the primitive roots of prime numbers ; 2. é., by compounding
such a class continually with itself we obtain all possible classes, just as by
continually multiplying a primitive root by itself we obtain all residues
prime to the prime of which it is a primitive root. It has, however, been
ascertained by M. Kummer that these primitive classes do not in all cases,
or even in general, exist.
The theorem of this article enables us to express ideal numbers as roots
of actually existing complex numbers. ‘Thus, if g be a prime appertaining
to the exponent f for the modulus X, and resoluble into the product of e con-
jugate ideal factors ¢(n,), 9(7,), $(7,),+++$(ne_,), these ideal numbers, which
will not in general belong to the same class, will nevertheless appertain to
the same exponent h; so that [o(n,) 1", Co(m,)1’; ..- will all be actual num-
bers. The power g” is therefore resoluble into the product of e actually
existing complex factors. If we effect this resolution, and represent the
factors of g” by &(n,), ®(n,)...., the ideal numbers $(1,); ¢(7,);++++ may be
represented by the formule
1 1
(1) = [&(m,)]* o(1,) = [(,) 1" gs9)2)
50. The Number of Classes of Ideal Numbers.—The number of classes of
ideal numbers was first determined by Dirichlet. He effected this determi-
nation by methods which he had previously introduced into the higher
arithmetic, and which had already led him to a demonstration of the cele-
brated theorem, that every arithmetical progression, the terms of which are
prime to their common difference, contains an infinite number of prime
numbers, and to the determination of the number of non-equivalent classes
of quadratic forms of a given determinant t. Dirichlet’s investigation of the
problem which we are here considering has never been published; but that
since given by M. Kummer is probably in all essential 1espects the same, as
it reposes on an extension of the principles developed in Dirichlet’s earlier
memoirs. Our limits compel us to omit the details of M. Kummer’s analysis ;
the final result, however, is, that if H denote the number of non-equivalent
2 x a In this formula P is a quantity
1 f i ae (7) ea
classes of ideal numbers, H @ay=i* A
defined by the equations
P=9(8) 9(B°) o(8°).+.g(B*),
0(BY=1+-y,B+ yf? + 738? + «+ +, ,
* See on this subject M. Kummer’s note “on the Irregularity of Determinants” in the
Monatsberichte of the Berlin Academy for 1853, p. 194. M. Kummer’s investigation,
however, is restricted to classes containing ideal numbers f(a) such that f(a)xf («*) is
an actual number.
+ See his memoirs on Arithmetical Progressions, in the Transactions of the Berlin Academy
for the years 1837 (p. 45) and 1841 (p. 141), or in Liouville, vol. iv. p. 393, ix. p. 255. The
first of these papers relates to progressions of real integers, the second to progressions of
complex numbers of the form a+27. In the memoir “ Recherches sur diverses applications
de V’analyse infinitésimale 4 la Théorie des Nombres” (Crelle, vol. xix. p. 24, xxi. pp. 1,
& 134), Dirichlet has applied his method to quadratic forms having real and integral co-
efficients; and in a subsequent memoir (Crelle, vol. xxiv. p. 291), he has extended this ap-
plication to quadratic forms, of which the coefficients are complex numbers containing 7.
See also Crelle, vol. xviii. p. 259, xxi. p. 98 (or the Monatsberichte for 1840, p. 49), xxii. p.
375 (Monatsberichte for 1841, p. 190). Weshall have occasion, in a later part of this Report,
to give an abstract of the contents of this invaluable series of memoirs.
ae
Be ——~ 7 eemeneii te eerie
ed
ON THE THEORY OF NUMBERS. 135
B representing a primitive root of the equation B\"'=1, y a primitive root
of the congruence y~'=1, mod X, and y,, y,) ys)++- the least positive resi-
dues of y, y’, y*,-.. for the modulus A; A is the logarithmic determinant
(see art. 42 of this Report) of any system of »—1 fundamental units, and
D the logarithmic determinant of a particular system of independent but not
fundamental units, e(a), e(a”), e av Satan an , defined by the equation
y q
sin ine 2ik
BfGee)G—e) Gwe
e(a)= (la) (Ima) + jaan hire 7. 7 = eae
sin rae
so that
L.c(a), Lee(a"), Lee(ai*), +. Lee(at +) |
L.e(a”), L.e(a”), L.e(a), aterae Leal
D=| 1 .e(a”), L.e(a”), L.e(a%), .... L.e(a”)
L.e(a?” ), L.e(a), L.e(a””),...- Lee (a),
Each of the two factors and 2 of which the value of H is com-
Ee
(2\)#-} ”
posed, is separately an integral number. That z is integral isa consequence
of the relation which exists between the logarithmic determinant of a system
of fundamental units, and that of any system of independent units; that P is
divisible by (20)*—* may be rendered evident from the nature of the ex-
pression P itself*. The factor a taken by itself, represents the number of
classes that contain ideal numbers composed with the periods of two terms
ata, a?+a-*,.... only; or, which is the same thing, it represents the
number of classes each of which contains the reciprocal f(a@~") of every ideal
number f(@) comprehended in it; aye? on the other hand, is the number
of classes of those ideal numbers which become actual by multiplication
with their own reciprocals+. The actual calculation of the factor 2 is ex-
tremely laborious, as it requires the preliminary investigation of a system of
fundamental units. For the cases \=5, \=7, the trigonometrical units e(a),
e(a"), e(a””)... ave themselves a fundamental system, so that in these two
P
(2A)a~
presents somewhat less difficulty ; and M. Kummer (though not without great
labour) has assigned its value for all primes inferior to 100. For the
primes 3, 5, 7, 11, 13, 17, 19, that value is unity; for 23 it is 3, and then
increases with extraordinary rapidity; so that for 97 it already amounts to
411322823001 =3457 x 118982593. The asymptotic law of this increase
is expressed by the formula
cases D=A, and Rae The computation of the first factor
* See the investigation in the next article.
+ See the note already cited, “‘ on the Irregularity of Determinants,” in the Monatsberichte
for 1853, p. 195.
136 REPORT—1860.
Lim [ Lipis pom |=
CN aa
when ) increases * without limit. It will be seen that the number of classes
of ideal numbers for A=3, A=5, A=7, is unity; 7.¢., for those values of A
every complex prime is actual. In the absence of any determination of a
system of fundamental units for A=11, A=13, A=17, and A=19, it is not
possible to say whether this is or is not the case for these values also. But
from and after the limit \=93, the value of the factor indicates
P
a
that a complex number is not necessarily a complex prime because it is
irresoluble into factors.
51. Criterion of the Divisibility of H by }.—The number of classes of
ideal numbers, which we have symbolized by H, is not in general divisible
by A; but in certain cases it may happen that it is so. The quotient 2 is
never divisible by \, except when the other factor is also divisible
lg
2h)e-}
by X. And it has been found by M. Kummer that the necessary and sufficient
condition for the divisibility of by \ is that the numerator of one of
BR
Gry
the first ~—1 fractions of Bernoulli should be divisible by A. The investi-
gation of this singular criterion depends on a transformation of the function
¢(() which enters into the expression of P. If we represent the product
(yB—1) ¢(B)=(rn-2—-1) + (y- B+ Cyn) P? + 000 + VY,
Ya—2)3*—*, in which every coefficient is divisible by A, by
ALB, +B,B-+0,8+ ...B,_ 9°], or X43)
(bm denoting the quotient a or I as ee if I represent the greatest
integer contained in the fraction before which it is placed), we obtain by
multiplication the equality
(7° +1) P=d*h (B) 4B"). (BX);
or, since y"+1 is divisible by X, and may be supposed not divisible by \°+,
Se= HOME) HOM),
C denoting a coefficient prime to. The congruence =0, mod A,
P.
(2A )R-}
is therefore equivalent to the congruence
¥(B) (6°) .... (B*—*) =0, mod d,
which may, in its turn, be replaced by the following,
Vy) Hy’). b(y*-?) =0, mod 2.
For, if there be an equation which, considered as a congruence for a given
modulus A, is completely resoluble for that modulus, any symmetrical function -
of the roots of the congruence is congruous, for the modulus X, to the cor-
responding function of the roots of the equation. The function J(() (3°)
* Liouville, vol. xvi. p. 473. The formula is given without demonstration.
t For y¥+1 and (y+-A)#-F1 are both of them divisible by \; but only one of them can
be divisible by 2, since their difference is not- divisible by 2. We can therefore, without
changing Yo 7, +++ Y,—g) determine y in accordance with the supposition in the text.
ON THE THEORY OF NUMBERS. 137
pete), which is a symmetric function of f, /’, ... 2, the roots of
the equation z*+1=0, is therefore congruous to f(y) p(y") --+- d(y*-?),
which is the same function of y, y’, y’,-.. y*~?, the roots of the congruence
gt+1==0, mod A. Hence the necessary and sufficient condition for the
Meeabiity of —*
i
Qi by \ is that one of the » congruences included in the
formula
Uae) ==0, mod Ny w= 1,9, 3 ..- fh -nublemths wiis., (A)
should be satisfied. Now y~@"-» Wy”) sbiy ee rewvar) A eaYa 0
+... +d, 57°%—)3 01, observing that y,5 y, Y2++-Ya-2 are the numbers
1, 2, 3,...N—1, taken in a certain order, and introducing the values of
b,, b,, by eee
z=r—1
yr On-Di (yn!) = gon-1 TY” mod 2.
z=] r
This last expression may be further transformed as follows. If f(x) denote
22
any function of x, and F(a)= 2 f(x), we have the identical equation
21
z=vA-1 a z=y—1 r
BT ees F (1M )=@—-1) FO)
s=1 r z=1 Y
y and 2 being any two numbers prime to one another. To verify
this equation, we may construct a system of unit points in a plane;
then the right-hand member is the sum of the values of f(a) for all unit
points in the interior of the parallelogram (0, 0), (A; 0), (A; y), (0; y);
while the two terms of the left-hand member represent similar sums for
the two triangles into which the parallelogram is divided by its diagonal
ye—hy=0. Writing then in this identity a°”~* for f(x), and employing
=F
the symbol F,,_, (x) to represent the sum 2 2”, or rather the function
x=1
My 20 a gy PMV ea
—4+i2 ike ee aa a) by ie eae Ee eras
oe 1.an—9.0.9. Tl. 2n—4.4 Ot
+(—1) Be. Il.2n—1 2
ei aie
1T.2.11.2n—2 ”
in which B, B,... B, are the fractions of Bernoulli, and which, when x is
an integral number, coincides with that sum, we find
x=)A—-—1 z=y—1 ‘
Bars, 2 Fea | W#l=G- ri @~))-
x=1 X= Laster
But F,,_; (A—1)=Fhs_i (A)—\2"-1 is evidently divisible by ; so that
x=r—1 z=y—1
> gn + >» anes [| = 0, mod X.
x=] 2=1 Y
The congruences (a) may therefore be replaced by the congruences
«x=y-—1
D2) \ peas [P| = (), mod A, which may be written in the simpler form
z=] Y
138 REPORT—1860.
z=y—1 i
>» Bays (-;)=o moda,
z=] v4
2r I (y—1)A
uf Y
are congruous (mod 2) to the fiactions—25 >) ett Rs taken in a cer-
PY Y
us
tain order. But, by a curious property of the function F,,-»» demonstrated
for the first time by M. Kummer,
if we observe that (A being prime to y) the numbers J 5 I
Y
7B Bape (—2) (LD Ba (=D.
r=] oF + 2nyn-1
The condition for the divisibility of H by X is therefore that one of the p
congruences included in the formula B, (y2”"—1) =O, mod 4, should be satis-
fied. The last of these congruences, or B, (y?—1)=0, is never satisfied ;
for it is easily proved that the denominator of B, contains \ as a factor,
while y2*—1=(y"+1) (y#—1), though divisible by A, is not divisible by \?.
And since, if n<p, y2”—1 is prime to d, that factor may be omitted in the
remaining .—] congruences ; so that the condition at which we have arrived
coincides with that enunciated at the commencement of this article.
We have exhibited M. Kummer’s analysis of this problem with more ful-
ness of detail than might seem warranted by the nature of this Report, not
only on account of its elegance, but also because it exemplifies transforma-
tions and processes which are of frequent occurrence in arithmetical inves-
tigation *.
52. “ Exceptional” Primes.—A prime number X, which, like 37, 59, and
A—3
67 in the first hundred, divides the numerator of one of the first frac-
tions of Bernoulli, and which consequently divides the number of classes of
ideal numbers composed with Ath roots of unity, is termed by M. Kummer
an exceptional prime. Such primes have to be excluded from the enunciation
of several important propositions ; and their theory presents difficulties which
have not yet been overcome. Thus the following propositions are true for all
primes other than the exceptional primes, but are not true for the exceptional
primes.
(1.) The exponent to which any class of ideal numbers appertains (see
art. 49) is prime to X.
(2.) The index of the lowest power of any unit which can be expressed
as a product of zntegral powers of the trigonometric units is prime to. For
that index is a divisor of " (see art. 42).
(3.) Every complex unit which is congruous to a real integer for the
modulus A is a perfect Ath power. (Whether X be an exceptional prime or
not, the Ath power of any complex number is congruous, for the modulus A,
to a real integer, viz. to the sum of the coefficients of the complex number.)
* In Liouville, vol. i. (New Series) p. 396, M. Kronecker has given a very simple demon~
stration of the congruence
2ndop (y2n—1) = (y2n—1) [1294-224 . + (N—1)2n], mod 3,
which, combined with another easily demonstrated formula, viz.,
12n4-22n +. (A—1)2n =(—1)n—1BnX, mod 2 [n <p],
leads immediately to the theorem of M. Kummer.
ON THE THEORY OF NUMBERS. 139
(4.) If f(@) denote any (actual) complex number prime to d (é. e. not
divisible by 1—a), a complex unit e (a) can always be assigned, such that
the product F (a)=e(a) f(a) shall satisfy the two congruences
F («) F(#—!) = [F(1)]’, moda,
F («) =F (1), mod (1—<)’.
A complex number satisfying these two congruential conditions is called a
primary complex number; the product of two primary numbers is there-
fore itself primary. This definition, in the particular case A=3, includes
the primary numbers of art. 37, taken either positively or negatively.
53. Fermat's Theorem for Complex Primes.—Let (a) be an actual or
ideal complex prime, and let N=N. ¢ (a) represent its norm. A system of
N actual numbers can always be assigned such that every complex number
shall be congruous to one and only to one of them for the modulus ¢ (a).
These N numbers may be said therefore to form a complete system of
residues for the modulus ¢ (a); and by omitting the term divisible by 9 («),
we obtain a system of N—1 residues prime to ¢ (a).
Let g be a prime appertaining to the exponent f, so that N=@/, and let
@ (a) or #, (no) be the prime factor of g which appertains to the substitution
no=U ; the formula
ata,a+a,a°+...+ar14f-], (A)
will represent a complete system of residues for the modulus ¢, (7), if we
assign to the coefficients dp, @,, a, .... the values 0, 1,2,...qg—1, in succession,
For if f (@)=wWo(n0) +a, (mo) +--+... a/-! be-1 (m0) be any complex num-
ber, f(a) is congruous for the modulus 9, (0) to Wo (%,) + api (um) +.-+af—!
1 (uo), because up—no = 0, mod , (n,); that is, f(@) is congruous to one
of the complex numbers included in (A); nor can any two numbers ay+
a,a+a,07+..+4 af, af! and 6) + 6,a+6,0°+... +b: af! included
in that formula be congruous to one another ; for the congruence (ao>—bo) +
a (a,—b,)+a*(a,—b,) + ... + af! (ap-1—b y_1) =0, mod ¢, (no), involves,
by M. Kummer’s theory (see art. 45), the coexistence of the f congruences
ao—bo =0, mod g; a,—b,=0, mod g; ..-a_1—b¢_1 =0, mod gq; ¢. e. the
identity of the complex numbers a+ aa,+a*a,+...a¢/—laz_1, and bp +ab,+
@ b.+..+af/—1bz_;. It is worth while to notice that, if g be a prime ap-
pertaining to the exponent 1, for the modulus A, @. e. if g be of the linear form
m\+1, the real numbers 0, 1, 2, 3...g—1 will represent the terms of a
complete system of residues for the modulus g(a); but if (@) be a factor
of a prime appertaining to any higher exponent than unity, a complete system
will contain complex as well as real integral residues.
By applying the principle (see art. 10) that a system of residues prime
to the modulus, multiplied by a residue prime to the modulus, produces
a system of residues prime to the modulus, we obtain the theorem, which
here replaces Fermat’s Theorem, that if ~(a) be any actual number prime
to » («), [y (@)]N-1=1, mod g(«). If we combine with this theorem the
principle of Lagrange (cited in art. 11) which is valid for complex no less
than for real prime modules, we may extend, mutatis mutandis, to the general
complex theory the elementary propositions relating to the Residues of
Powers, Primitive Roots, and Indices, which, as we have seen, exist in the
ease of complex primes formed with cubic or biquadratic roots of unity. In
fact, these propositions are of a character of even greater generality, and may
be extended, not only to complex numbers formed with roots of unity whose
index is a composite number, but also to all complex numbers formed with
the roots of equations having integral coefficients, as soon as the prime fac-
tors of those complex numbers are properly defined.
140 REPORT—1860.
54. M. Kummer’s Law of Reciprocity —We can now enunciate M. Kum-
mer’s law of reciprocity. It appears, from the last article, or it may be
proved immediately by dividing the N—1 residues of ¢(a@) into \ groups
N-1
of terms, after the following scheme,
(0) Fig Tay ose) Fy
eae
(1) AN Oy + +++ OTN,
A
(2) PaO Lin» oats. 8 Fag si
net PND
(A—1) a\—ly,, a\—}, eeee ON
A
and proceeding as in art. 33 of this Report, that if ~(@) be any actual com-
N-1
plex number prime to ¢(@), Y(a) * is congruous for the modulus ¢(@) to
a certain power a@* of a. This power of a may be denoted by the symbol
tees “4 so that we have the congruence [v(a)] * = [HS], =*
J -
mod ¢(a@). The symbol ee roaen we may term the Atic character
of Y (a) with regard to ¢(@), is evidently of the same nature as the corre-
sponding symbols with which we have already met in the quadratic, cubic,
and biquadratic theories, and admits of an extension of meaning similar to
that of which they are susceptible. Availing himself of this symbol, M.
Kummer has expressed his law of reciprocity by the formula eis
Y(ay
ACOMEN
aon ,¢(@) and {(«) denoting real or ideal primes. But, to interpret
%) 1»
this equation rightly, it is important to attend to the following observations.
(1.) When (¢) and ¢ («) are both actual numbers, the formula supposes
that they are both primary prime numbers. The prime 1—g is therefore
excluded.
(2.) The definition that we have given of the symbol [$3] becomes
N
unmeaning when ¢(@) is ideal, because no signification can be assigned to
an ideal number which presents itself, not as a modulus or divisor, but as a
residue. Let, therefore, i denote the index of the lowest power of ¢ (a)
which is an actual number; 2. e., let 2 be the exponent to which the class of
@ (a) appertains; and let [¢ (@) ]” represent the actually existing primary
complex number which contains the factor ¢(«) # times, but contains no
¢ (a)
¢ (a)
: : ; @ (a)* ;
tion a perfectly definite meaning. Let then kre ] =a"; we may define
A
other prime factor; then the symbol [ | has by the preceding defini-
A
h
the value of the symbol oe) by means of the equation Bal =
y v(a)Ja > 2 ¥(@)
h
o (4) =a’, which, ¢f h be prime to , always gives a determinate value
¥(«)
ae
ON THE THEORY OF NUMBERS. 141
a for [$ Ss , k being defined by the congruence AA ==h', modi. For the
symbol [§ 3
however to the condition that [¢(#)]” is primary.
It will be seen, therefore, that the exceptional primes of art. 52 are ex«
cluded from M. Kummer’s law of reciprocity, for a twofold reason :—first,
because if \ be one of those numbers, the definition of a primary number is
not in general applicable; and secondly, because, on the same supposition,
] so defined, the law of reciprocity still subsists, subject
the symbol 2) may become unmeaning.
“ion ad j
55. The Theorems complementary to M. Kummer’s Law of Reciprocity.—
The prime 1—a, and its conjugate primes, as well as the complex units,
are excluded from the law of reciprocity; but complementary theorems by
which the Atic characters of these numbers may be determined have been
given by M. Kummer. For a simple unit a*, we have the formula
k jie
On) =a* *® , With regard to A, which is the norm of 1—a, it may be
A
observed that if ¢ («) be a prime factor of a real prime g appertaining, for
‘the modulus A, to any exponent f different from unity, z.e¢. if g be not of the
linear form m\+1, the character of every real integer, and therefore of A,
a
with respect to ¢ (a) is+1, because, iff> 1, q = ! 5. divisible byg—1. But
whatever be the linear form of g, the characteristic of X or x (A) (for so we
x
@ («) Ja
shall for brevity term the index of « in the equation =at), is de-
termined by the congruence
x)= t Da, mod A,
LS o
D, being the value (for v=0) of the differential coefficient ee
Moo v\h
if @(a@) be an actually existent number, or of yee? if it be ideal.
To obtain the characteristics of the units, M. Kummer considers the system
of independent units
E, (a), E, (a), eeeee Ey-1 (a),
defined by the formula
—2k —4k =2(u—1)k
—] Y
7 Y
Ex (a)=e(a)e(a”) e (at) ane ne (es
in which e(a) represents tae trigonometrical unit of art. 50, and y is the
sale primitive root of A which occurs in the expression of e(«). We have
then, for x [E* (q”)] and x (l—a*), the formule
n k 2k B, 2
x CEx (2@")] = (—1)" (y*"—1) ah D,-2%, mod X,
PRB N—I hk?
and x(i—at)=— >, gNoT iB pf
ht Bd-3
—B, Du fre ee (= 1° oS Ba
142 REPORT—1860.
N representing the norm of ¢ (a), B,, B,...B,-1 the fractions of Bernoulli,
and D,,, the value of the differential coefficient
dm log ¢ (ea (or d™ log Le (e”)}" ) for v=0.
dvu™ hdv™
These formule do not in general hold for the exceptional prime numbers ),
which divide the numerator of one of the first »—1 fractions of Bernoulli.
This is evident from the occurrence in them of the coefficients D,,, which if
¢ (2) be ideal, and / be divisible by \, may acquire denominators divisible
by A, thus rendering the congruences nugatory. It is sufficient to have
determined the characteristics of the particular system of units E, (a), E, (a),
---E,_, («), because, as that system is independent, every other unit e (a)
is included in the formula
e(a)=E, (a)™ E, (a)™ «6... Ey—1 (@)™«-1;
so that x [e(a)] may be found from the congruence
k=
x Le («)] =s my x [Ex (a) ], mod A,
which cannot become unmeaning, except in the case of the exceptional
primes, because if D! be the logarithmic determinant of the system of units
E, (@), E, (a), 1. Ei: (a),D and A retaining the meanings assigned ng them
in art. 50, it may be shown that D is prime to X, and therefore 2 => xis
also prime to ); 7. e.,the denominators of the fractions m,,72,,...™,—1 are prime
to A (see art. 42). But M. Kummer has also given a formula which assigns
directly the characteristic of any unit e (a) whatsoever. If Ax denote the
value of the differential coefficient ance eS). for v=0, we have
Vv
k=p—1
x le(a)i] =4,Sol+3 Au, Dy_ay» mod *.
k=
56. We have already observed (see art. 39) that it is impossible to deduce
a proof of the highest laws of reciprocity from the formule which pre-
sent themselves in the theory of the division of the circle. It is true (as we
shall presently see) that the formule IV. and V. of art. 30 determine the
decomposition of the real prime p (supposed to be of the form 4+ 1) into its
A—1 complex prime factors ; but it will be perceived that these complex fac-
tors occur, not isolated, but combined ina particular manner. From equation
IV. of the article cited we infer that p= (a) w (a); let then y (a)=f (a,)
FS (a) «+ +f (Gy) 5 %,)&,.+%, being « different roots (of which no two are re-
i
ciprocals) of the equation ~ 14; so that f(a,), f(a), --~f(@,) are one-
p q 4=1
half of the complex primes of which p is composed ; if e(a@) be any real
unit, satisfying the equation e(a)=e (a), it is plain that e(a,)’e(a,)’...
e(a,)” =1, or p(a)= te(a,) f(a,) Xe(a,) f(a) --. XE (a) f(a.)- The
consideration, therefore, of the number (a) cannot supply us with any de-
termination of the Atic character of f(@,) which will not equally apply to
Sf (a,)xe(a,). But for all values of \ greater than 3, the number of real
complex units is, as we have seen, infinite; and the character of any com-
plex prime f(a) with respect to any other complex prime evidently changes
* The formule of this article are taken from M. Kummer’s second memoir on the com-
plementary theorems (Crelle, vol. lvi. p. 270).
—_" = + =
“a
ON THE THEORY OF NUMBERS. 143
when f(a) is multiplied by a unit of which the Atic character is not unity.
The inapplicability of the formule of art. 30 to any general demonstration of
the law of reciprocity is thus apparent. The only equation of reciprocity
that has been elicited from them is the following :—
el (22) x.. ; (22?) =(t) x(t.) x.. x5 x
in which ¢ (@) is a complex prime factor of a prime number p of the form
m\+1, and q,, J.,+++-Ge are the e conjugate factors of a prime number g
appertaining to the exponent f for the modulus X. This equation, which, if
we adopt the generalized meaning of the symbol of reciprocity, may be writ-
ten more briefly thus, (e%) =( q ) , was first obtained by Eisenstein,
q Ja \o(@)/r
who inferred it from M. Kummer’s investigation of the ideal prime divisors
of (a) (see a note addressed by Eisenstein to Jacobi, and communicated
by Jacobi to the Berlin Academy, in the Monatsberichte for 1850, May 30,
p- 189). In a later memoir (Crelle’s Journal, vol. xxxix. p. 351), Eisenstein
proposes an ingenious method—reposing, however, on an undemonstrated
principle—for the discovery of the higher laws of reciprocity ; but it would
seem that the application of this method failed to lead him to any definite
result ; and it is unquestionably to M. Kummer alone that we are indebted
for the enunciation as well as for the demonstration of the theorem.
57. M. Kummer appears to have waited until he had developed the theory
of complex numbers with a certain approximation to completeness, before
proceeding to apply the principles he had discovered to the purpose which
he had in view throughout, the investigation of the law of reciprocity. He
succeeded in discovering the law which we have enunciated, in the year
1847, and, after verifying it by calculated tables of some extent, he commu-
nicated it to Dirichlet and Jacobi in January 1848, and subsequently, in
1850, to the Berlin Academy, in a note which also contained the demonstra-
tion of the complementary theorems relating to the units, and the prime
divisors of X. From the analogy of the cubic theorem, it was natural to
conjecture that the law of reciprocity would assume the simple form
(2) =) for primes p, and p, reduced, by multiplication with proper
anf A JA
complex units, to a form satisfying certain congruential conditions. But
to determine properly these conditions, 2. e. to assign the true definition
of a primary complex prime, was no doubt the principal difficulty that M.
Kummer had to overcome in the discovery of his theorem. If \=3, the
single congruence f («)==f(1), mod (1—a)’, sufficiently characterizes a
primary number; and since, whatever prime be represented by X, that con-
gruence is satisfied by one, and one only, of the numbers included in the
formula a* f (a), it was probable that it ought to form one of the con-
gruential conditions included in the definition of a primary complex prime.
In determining the second condition, M. Kummer appears to have been
guided by a method which depends on the arithmetical properties of
the logarithmic expansion of a complex number. If we develope log £2)
I(@)—fQ) f(a) th
in ascending powers of ~—2_“ \-/ and represent by L\*/ the finite num-
oe fa) feos vinnie
ber of terms which remain in this expansion after rejecting those which are
congruous to zero for the modulus A, we are led, after some transformations,
to the congruence
144 REPORT—1860.
Ufo = D, X, (@)+D, X, (a) +... +Dy—2 X,~2 (a), mod A,
s=A—2
where X; (a) represents the function = —-y~* a’, and Dy, denotes, as in
i
__ , Glog fe)
art. 55, the differential coefficient EeRT In this congruence the first
coefficient alone is altered when f(«) is multiplied by a simple unit ; and only
the even coefficients are altered when f(a) is multiplied by a real unit. Now
D, is rendered congruous to zero by the condition f(@) =f (1), mod (1—«)’;
and M. Kummer has shown that, by multiplying f(a) by a properly chosen
real unit, D,, D,,...D,—3 may be similarly made to disappear, so that we
obtain
-u = D, X,(a)+D, X,(a@)+ ...-+Da—2 Xa_2(a), mod d,
a congruence which is proved to involve the second congruence of condition
satisfied by a primary number, 2. e. f(a) f(a—!) =f(1)’, mod A*.
58. The methods to which M. Kummer at first had recourse in order to
obtain a demonstration of his theorem, consisted in extensions of the theory
of the division of the circle. By such extensions he demonstrated the com-
plementary theorems, and even a particular case of the law of reciprocity
itself—that in which the two complex primes compared are conjugate. But,
after repeated efforts, he found himself compelled to abandon these methods,
and to seek elsewhere for more fertile principles. ‘I turned my attention,”
he says, ‘to Gauss’s second demonstration of the law of quadratic recipro-
city, which depends on the theory of quadratic forms. Though the method
of this demonstration had never been extended to any other than quadratic
residues, yet its principles appeared to me to be characterized by such
generality as led me to hope that they might be successfully applied to
residues of higher powers ; and in this expectation I was not disappointed f.”
M. Kummer’s demonstration of the law of reciprocity was communicated
to the Academy of Berlin in the year 1858, ten years after the date of his
first discovery of it. An outline of the demonstration is contained in the
Monatsberichte for that year; and it is exhibited with great clearness and
fulness of detail in a memoir published in the Berlin Transactions for
1859, which contains what is for the present the latest result of science on
a problem which, if we date from the first enunciation of the quadratic
theorem by Euler, has been studied by so many eminent geometers for
nearly a century. It would, however, be impossible, without exceeding the
limits within which this Report is confined, to give an account of its contents,
which should be intelligible to persons not already familiar with the subject
to which it refers. Taken by itself the demonstration of the theorem is, indeed,
sufficiently simple; but it is based on a long series of preliminary researches
relating to the complex numbers that can be formed with the roots of the
equation w\=D («), in which D (@) itself denotes a complex number com-
posed of Ath roots of unity. To those researches, and to the demonstration
of the law of reciprocity founded on them, we shall again very briefly refer,
when we come to speak of the corresponding investigations in the theory of
quadratic forms, an acquaintance with which is essential to a comprehension
of the method adopted by M. Kummer in his memoir. We may add that
M. Kummer has intimated that he has already obtained two other demon-
* Crelle, vol. xliy. p. 130-140. tT See the Berlin Transactions for 1859, p 29.
ON THE THEORY OF NUMBERS. 145
strations of his law of reciprocity, which, though they also depend on the
eonsideration of complex numbers containing w, yet do not require the same
complicated preliminary considerations.
59. Complex Numbers composed of Roots of Unity, of which the Index is
not a Prime.—In a special memoir (see the list in art. 41, note, No. 16),
M. Kummer has considered the theory of complex numbers composed with
a root of the equation w"=1, in which ” denotes a composite number. The
primitive roots of this equation are the roots of an irreducible equation of the
form
Fis)— isis aor sees 9
Tl (w?—1) 0 (w?%P—1)....
Py» Po Py» +--+ denoting the different prime divisors of x*. If W (x) be the
number of numbers less than 2 and prime to it, F (w) is of the order p(n),
and every complex number containing w can be reduced (and that in one way
only) to the form f (w)=a) +4, +a, 0°+.... +4) ,0¥-1, The
numbers conjugate to f'(w) are the J (~) numbers obtained by writing in
succession for w the p (7) primitive roots of w*=1; and the norm of f (w
is the real and positive integer produced by multiplying together the w (n
conjugates: If g be a prime number not dividing z, the sum
Bp=w* + wht + wh? + ....,
in which the series of terms is to be continued until it begins to repeat itself,
is termed a period. The ~ periods w,, w,,...@, remain unchanged if for w
we write w%, wi’, etc. Hence, if g appertain to the exponent ¢ for the modu-
lus 7 (i. e. if g satisfy the congruence g‘ = 1, mod m, but no congruence of a
lower order and similar form), the number of different numbers conjugate to
?
a given complex number containing the periods only is at most a For
brevity, a complex number containing the periods only—for example, the
number
Cote, BW, +0, D+ 10+. + ln Dy
may be symbolized by f(@,), so that
S (@)=%+e, WebC,Wapb voce Hey Dnke
If 1,7, 7,,...are a set fhe) numbers prime to and such that the quo-
tient of no two of them (considered as a congruential fraction+) is congruous
for the modulus x to any power of g, the numbers conjugate to f (a) may be
na
* The irreducibility of the equation % = =0 when x is a prime was first established by
et
Gauss (Disq. Arith. art. 341). Tor other and simpler demonstrations of the same theorem,
see the memoirs of MM. Kronecker (Crelle, xxix. p. 280, and Liouville, 2nd series, vol. i.
p. 399), Schoenemann (Crelle, vol. xxxi. p, 323, vol. xxxii. p. 100, & vol. xl. p- 188), Eisenstein
(Crelle, vol.xxxix. p. 166), and Serret (Liouville, vol.xv.p.296). The principles on which these
demonstrations depend suffice to establish the irreducibility of the equation =
gP —]
but they fail, as M. Kronecker has observed, to furnish the corresponding demonstration
when 2, as in the text, is a product of powers of different primes. This demonstration was
first given by M. Kronecker (Liouville, vol. xix. p. 177), who has been followed by M. De-
dekind (Crelle, vol. liv. p. 27), and by M. Arndt (id. lvi. p. 178).
+ For the definition of a congruential fraction see art. 14.
1860.
146 REPORT—1860.
represented by f (a,), f (@,); f (@,.) --+.+ The periods are the roots of
certain irreducible equations, each of which is completely resoluble when
considered as a congruence for the modulus g; and the roots w,, w#,,+.+ of the
congruences are connected with the roots a, @,,...of the equations, by a
relation precisely similar to that enunciated in art. 44. ‘This relation M.
Kummer has established by introducing certain conjugate complex numbers*
Y (w,), ¥ (w,), ¥ (@. ),»++- involving the periods only, not themselves divi-
sible by g, but each satisfying the x congruences included in the formula
Y (@,) (Sir—Uj,.) =0, mod g,
=y heh oo owe
From these congruences it is easy to infer that, if f (@,, @2)++++@nr) =O
be any identical relation subsisting for the periods, a similar relation
SF (Uys Uap oo Un) =0, mod q, will subsist for the numbers %,, %,)+++Un; for
we find
WY (wy) f (Bry Bary ++ = V (G,) f (uy U2. ), mod g,
i. @.f (Uy) Uy) +++) =0, mod g. Another important property of the complex
number ¥ (@,) is that it is congruous to zero, med gq, for every one of the sub-
stitutions 7, =U,, 7, =Ur,, DW, =Ur,, --. except the first: thus the congruences
WY (uy,) =0, VY (u,.) =0 are satisfied, ... but not ¥ (w,)=0, modg. If,
then, f (w) be any complex number satisfying the congruence W (a,)" f(w)
=0, mod g”, but not the congruence V (a,)”"+! f (w)=0, mod g”*1, f (w)
is said to contain m times precisely the ideal factor of g corresponding to
* These complex numbers are defined as follows (see the memoir cited at the com-
mencement of this article, sect. 3, and that in Crelle, vol. liii. p. 142) :—Let wy, be a period
satisfying the irreducible equation ¢ (w;,.)=0, and let a,, a,,... be the incongruous roots of
¢ (y) =0, mod g, 4,, 5,,... the remaining terms of a complete system of residues, mod g, so
that ¢ (b,), 9 (5.),-+-- are prime tog. Since w,/ = w;,,, mod 9, and wyy=wz, We have,
by Lagrange’s indeterminate congruence (see art. 10 of this Report)
(@,—-4,) (7-4)... (@E—3,) (W7,—D,) .... == 0, mod g,
or, since w,—3, divides ¢ (4,) etc.,
(51) p (Oy) +++» (yz, —a)) (WE—Ay) .-. = 0, mod G5
i. e. (wy —4) (@,—a,)+--.==0, mod gq. We may now consider the x series of factors
Sy iH SL CS i Ed
corresponding to the m values of & [the numbers a,, a,,...are of course the same for two
periods which satisfy the same irreducible equation, but not in general the same for any —
two periods], and, retaining among these factors only those which are different, we may
take for ¥ (w,) the complex number formed by combining as many of them as possible, in
such a manner as to give a product which is not divisible by g, but which is rendered divi-
sible by g by the accession of any one factor not already contained in it. It is evident that
W (w,) cannot contain all the factors w;,—a,, @j,—4,,---+ 5 let us then denote by wa—u a
factor which is not contained in W (w,); we thus obtain the relation
Y (w,) (w,—u,) =0, mod g,
or, changing the primitive root w into w”,
WY (a,) (w,7.—Uz,) = 0, mod 7.
The conjugates of Y (w,) are all complex numbers formed according to the same law as
Y (w,) itself; and, besides Y (w,) and its conjugates, no other complex number can be formed
according to that law. Also the number w, which corresponds to a given period w;, is ab-
solutely determined as soon as we have selected the multiplier Y (w,); for if two of the
factors w1,—d,, Wy,—4,,... were absent from ¥ (a,) we should have V (w,) (w,—a,)=0,
¥ (w,) (w,—4,) =0, mod g; and thence (a,—a,) Y (w,) =0, mod g, contrary to the hy-
pothesis that a, and a, are incongruous, and that V (w,) is not divisible by g. The corre-
spondence of the numbers w,, v,,.-.+U,, With the periods w,, @5,;-.-+@p, can thus be fixed
in ag many ways as there are numbers conjugate to YW (w,), @ ¢. in nd ) different ways.
ON THE THEORY OF NUMBERS. 147
the substitution a,-=w;. Since it can be shown that the numbers conjugate
to ¥ (a,) are all different from one another, it follows from the definition,
that the quotient —— represents the number of conjugate ideal prime fac-
tors contained in the real prime g, appertaining to the exponent ¢. If g bea
divisor of 2, the definition of its ideal factors requires a certain modification,
which we cannot here particularize. (See sect. 6 of M. Kummer’s Memoir.)
The two definitions, corresponding to the cases of g prime to , andga
divisor of 2, enable us, when taken together, to transfer to the general case
when z is composite, the elementary theorems already shown to exist when
m is prime (see art. 47). We may add that it is easy to prove, in the general
as in the special case (see art. 48), that the number of classes of ideal num-
bers is finite.
60. Application to the Theory of the Division of the Circle-—We cannot
quit the subject of complex numbers without mentioning certain important
investigations in which they have been successfully employed. The first
relates to the problem of the division of the circle. In this problem the
s=p—2
resolvent function of Lagrange = 627 (see art. 30) is, as is well
s=0
known, of primary importance. Retaining, with a slight modification, the
notation of art. 30, and still representing by \ a prime divisor of p—1, and
tee
z ==0, let us consider the function F (a, x),
by a root of the equation
which is a particular case of the resolvent, and let us represent the quotient
pate) F (a! x) by ¥z (@). We thus find
F (att, x)
LE @ 2) =v, (a) ¥, (a)... te s(a)F(aa), - . . (A)
and in particular, observing that F (a, x) F (a\—!, a)=p,
Bite. esrb (a ab. (a) .0.-Yr-a(h)y fn 6 et ew (2)
a result which is in accordance with the known theorem that [F (a, x) ]* is
independent of 2 and is an integral function of « only. The resolution of
the auxiliary equation of order \, the roots of which are the ) periods of
p—1 eP—l
=X
roots of the equation 7 =0, depends solely on the determination
“e—
of the complex numbers v, («), w, (~),..-.Wa—2(@). For when these com-
plex numbers are known, we may equate F (a, a) to any Ath root of the ex-
pression pw, (~) UJ, (%).-. Ya_2 (a); from the value of F (a, a), thus obtained,
those of F(a’, 2), F(a’, a)....may be inferred by means of equation (1);
and, lastly, from the values of F (1, x), F(a, 2), ... F (a4, 2), the values of
the periods themselves are deducible by the solution of a system of linear
equations. To determine the numbers w, («), ,(«),... M. Kummer assigns
the ideal prime factors of which they are composed, employing for this pur-
pose the results cited in art. 30. The equation yz (a) i. (a—-!)=p shows
that Y% (a) contains precisely 1 (p—1) ideal prime divisors of p, and no other
complex prime. To distinguish the prime factors of p contained in yy (a)
from those contained in uz (a#-!) M. Kummer avails himself of the congruence
V. of art. 30, viz.,
Il (m+n)
mod p.
Tlm.fin’ P
Vino
et. \!= eo, and w=y”, mod p, so that wu, u°,...w\—! are the roots of
PAs
148 - REPORT—1860.
_— = 0, mod p; also, to adapt the formule of art. 30 to our present pur-
pose, let @-"' =a, m=), n=h)N'; it will result from these substitutions, that
We (u-") =0, mod p, if & and h satisfy the inequality [A] + [4A] >A, where
[A] and [RA] are positive numbers less than \, and congruous, mod A, to h
and kh respectively. If we represent by f(a) the ideal prime factor of p
which appertains to the substitution «=u, this may be expressed by saying
that vz(«) contains the factor f(a—"), if [i 4 Hi >, the symbols Hi
and [FZ] denoting the least positive numbers satisfying the congruences
L
hx =1, mod X, and Ae=h, mod X. Assigning, therefore, to the number
every positive value less than \ compatible with this condition, we may write
te (a)= tar f(a-"),
+a’ being a simple unit which may be determined by the congruence
vz (a) = —1, mod 1—a)**: it is not necessary to add a real complex unit,
for a reason which has already appeared (see art. 56, supra). From the
expression for ¥z («) a still simpler formula for F (a, x) may be obtained,
viz. m=h—] [=
Lee rae Hy. LL ira
n=
61. Application to the Last Theorem of Fermat.—The second investigation
to which we shall advert relates to the celebrated proposition known as the
«“ Last Theorem of Fermat,” viz. that the equation 2” +y” =z” is irresoluble,
in integral numbers, for all values of x greater than 2}. As Fermat himself
* The numbers ;(«) are primary according to M. Kummer’s definition (art. 52); for
F (a, x) F (ak, x)
¥, (2) = F (e+, 2) = at, the summation extending to every pair of values of
?
y, and y, that satisfy the congruence y”!+-y/2=1, mod p, in which y represents the same
primitive root of p that occurs in the expression F(#, xv). Hence ~z(1)=p—2= —1,
mod X, and yz («) vz (2!) =p=1=[¥; (1)]*, moddA. Also ¥, («)—¥;, (1) is divisible
by (l—«)?; for ¥%(L)=2 (y, +4y,)=3 (1 +4) (p—1) (p—2), observing that y, and y,
each receive all the values 1, 2,...y—2 in succession. We have, therefore, the con-
gruence ¥',, (1) ==0, mod X, from which it follows (see a note on the next article) that
VY, (~) =, (1), mod (l—«)?, or yy, («) = —1, mod (1—<)?, as in the text.
+ Liouville, vol. xvi. p. 448. _M. Kummer has also extended his solution of this problem
to the case in which x is any divisor of p—1. See the memoir quoted in the last article,
sect. 11.
t Fermat’s enunciation of this celebrated theorem is contained in the first of the MS. notes
placed by him on the margin of his copy of Bachet’s edition of Diophantus. It would seem
that this copy is now lost; but in the year 1670 an edition of Bachet’s Diophantus was pub-
lished at Toulouse, by Samuel de Fermat (the son of the great geometer), in which these
notes are preserved (Diophanti Alexandrini Arithmeticorum libri sex, et de Numeris Mult-
angulis liber unus, cum commentariis C. G. Bacheti V. C. et observationibus D. P. de Fermat
senatoris Tolosani. Tolos 1670), ‘The theorems contained in them are, with a few excep-
tions, enunciated without proof; and it may be inferred from the preface of S. Fermat, that
he found no demonstration of thera among his father’s papers. Nevertheless, in the case of
several of these propositions, we have the assertion of Fermat himself, that he was in posses-
sion of their demonstration; and although, when we consider the imperfect state of analysis
in his time, it is surprising that he should have succeeded in creating methods which sub-
sequent inathematicians have failed to rediscover, yet there is no ground for the suspicion
that he was guilty of an untruth, or that he mistook an apparent for a real proof. In fact
these suspicions are refuted, not only by the reputation for honour and veracity which he
enjoyed among his contemporaries, and by the evidence of singular clearness of insight
which his extant writings supply, but also by the facts of the case itself. It would be inex-
ie poy
ON THE THEORY OF NUMBERS. 149
has left us a proof of the impossibility of this equation in the case of n=4,
by a method which Euler has extended to the case of m=3, we may suppose,
without loss of generality, that 2 is an uneven prime ) greater than 3, and we
plicable, if his conclusions reposed on induction only, that he should never have adopted an
erroneous generalization ; and yet, with the exception of the “ Last Theorem” (the demon-
stration of which, after two centuries, is still incomplete), every proposition of Fermat’s has
been verified by the labours of his successors. There is, indeed, one other exception to this
statement; but it is an exception which proves the rule. In the letter to Sir Kenelm Digby
which concludes the ‘Commercium Epistolicum, etc.’ edited by Wallis (Oxford, 1658),
Fermat enuntiates the proposition that the numbers contained in the formula 22”41 are all
primes, acknowledging, however, that, though convinced of its truth, he had not succeeded
in obtaining its demonstration. This letter, which is undated, was written in 1658; but it
appears, from a letter of Fermat's to M. de * * *, dated October 18, 1640, that even at that
earlier date he was acquainted with the proposition, and had convinced himself of its truth
(D. Petri de Fermat Varia Opera Mathematica, Tolose, 1679, p. 162). It was, however,
subsequently observed by Euler that 22°-+1=4294967297 =641 x 6700417, i.e. that the
undemonstrated proposition is untrue (Op. Arith. collecta, vol. i. p. 356). The error, if it is
an error, is a fortunate one for Fermat; it exemplifies his candour and veracity, and it shows
that he did not mistake inductive probability for rigorous demonstration :—‘ Mais je vous
adyoue tout net,” are his words in the letter last referred to, ‘‘ (car par advance je vous ad-
vertis que comme je ne suis pas capable de m’attribuer plus que je ne scay, je dis avec meme
franchise ce que je ne say pas) que je n’ay peu encore démonstrer l’exclusion de tous divi-
seurs en cette belle proposition que je vous avois enyoyée, et que vous m’avez confermée
touchant les nombres 3, 5, 17, 257, 6553, &c. Car bien que je reduise l’exclusion a la
pluspart des nombres, et que j’aye méme des raisons probables pour le reste, je n’ay peu
encore démonstrer nécessairement la vérité de cette proposition, de laquelle pourtant je ne
doute non plus & cette heure que je faisois auparavant. Si vous en avez la preuve assurée,
yous m’obligerez de me la communiquer: car aprés cela rien ne m’arrestera en ces matiéres.”
The “ Last Theorem” is enunciated by Fermat as follows :—
“Cubum autem in duos cubos, aut quadrato-quadratum in duos quadrato-quadratos, et
generaliter nullam in infinitum ultra quadratum potestatem in duos ejusdem nominis fas est
dividere ; cujus rei demonstrationem mirabilem sane detexi. Hanc marginis exiguitas non
caperet.” (Fermat’s Diophantus, p. 51.)
Fermat has also asserted that neither the sum (ébid. p. 258) nor the difference (ibid. p.338)
of two biquadrates can be a square. Each of these propositions comprehends the theorem
that the sum of two biqnadrates cannot be a biquadrate; and of the second, we possess
a yery remarkable demonstration by Fermat himself (#éd. p. 338; and compare Euler,
Elémens d’Algébre, vol. ii. sect. 13; Legendre, Théorie des Nombres, vol.ii. p.1). The
essential part of this demonstration consists in showing that, from any supposed solution
of the Diophantine equation 24—y4=a square, another solution may be deduced in which
the values of the indeterminates are not equal to zero, and yet are absolutely less than in
the proposed solution, from which it immediately follows that the Diophantine equation
is impossible. This method has been successfully employed by Euler (/oc. cit.) to demon-
strate several negative Diophantine propositions, and in particular the theorem that the sum
of two cubes cannot be acube. The only arithmetical principles (not included in the first
elements of the science) which are employed by Euler and Fermat in their applications of
this method, relate to certain simple properties of the quadratic forms x?+y?, 2?+2y?,
a°+3y?; and as these principles seem inadequate to overcome the difficulties presented by
the equation z”-+7"+2"=0, when x is > 4, it is probable that Fermat’s “ demonstratio
mirabilis sane” of the general theorem was entirely different from that which he has inci-
dentally given of the particular case.
The impossibility of the equation 2”+y”+2"=0 for n=5 was first demonstrated by Le-
gendre (Mémoires de l’Académie des Sciences, 1823, vol. vi. p. 1, or Théorie des Nombres,
vol. ii. p. 361. See also an earlier paper by Lejeune Dirichlet, Crelle, vol. iii. p. 354, with
the addition at p. 368, and a later one by M. Lebesgue, Liouville, vol. viii. p. 49) ; for n=14,
by Dirichlet (Crelle, vol. ix. p. 390); and for n=7, by M. Lamé (Mémoires des Savans
Etrangers, vol. viii. p. 421, or Liouville, vol. v. p. 295. See also the Comptes Rendus, vol. ix.
'p- 359, and a paper by M. Lebesgue, Liouville, vol. v. pp. 276 & 348). But the methods
employed in these researches are specially adapted to the particular exponents considered,
and do not seem likely to supply a general demonstration. The proof in Barlow’s Theory of
Numbers, pp. 160-169, is erroneous, as it reposes (see p. 168) on an elementary proposition
(cor. 2, p. 20) which is untrue. A memoir by M. Kummer on the equation 24+4y4=2*,
in which complex numbers are not employed, and in which no single case of the theorem is
150 REPORT—!1860.
may write the equation in the symmetrical form rrity*t2*—0, The impos-
sibility of solving this equation has been demonstrated by M. Kummer, first,
for all values of X not included among the exceptional primes* ; and secondly,
for all exceptional primes which satisfy the three following conditions :—
(1.) That the first factor of H, though divisible by A, is not divisible by
d? (see art. 50).
(2.) That a complex modulus can be assigned, for which a certain definite
complex unit is not congruous to a perfect Ath power.
(3.) That B,, is not divisible by d*, B, representing that Bernoullian
number [xk p—1] which is divisible by \+.
Three numbers below 100, viz. 37, 59, 67, are, as we have seen, excep-
tional primes. But it has been ascertained by M. Kummer that the three
conditions just given are satisfied in the case of each of those numbers; so
that the impossibility of Fermat’s equation has been demonstrated for all
values of the exponent up to 100. Indeed, it would probably be difficult to
find an exceptional prime not satisfying the three conditions, and conse-
quently excluded from M. Kummer’s demonstration.
We must confine ourselves here to an indication of the principles on which
the demonstration rests in the case of the non-exceptional primes f.
demonstrated (Crelle, vol. xvii. p. 203), is nevertheless of great interest for the number of
auxiliary propositions contained init. Of the same character are the notes by MM. Lebesgue
and Liouville, in Liouville’s Journal, vol. vy. pp. 184 & 360, and a few theorems given with-
out demonstration by Abel, Guvres, vol. ii. p. 264.
In the year 1847, M. Lamé presented to the Academy at Paris a memoir containing a
general demonstration of Fermat’s Theorem, based on the properties of complex numbers
(Comptes Rendus, vol. xxiv. p. 310; Lionville, vol. xii. pp. 137 & 172). It was, however,
observed by M. Liouville (Comptes Rendus, vol. xxiv. p. 315), that this demonstration is
defective, as it assumes, without proof, the proposition that a complex number can be repre-
sented, and in one way only, as the product of powers of complex primes—a proposition
which, as we have seen, is untrue, unless we admit ideal as well as actual complex primes.
The discussion on M. Lamé’s memoir attracted Cauchy’s attention to Fermat’s Theorem; and
the 24th and 25th volumes of the Comptes Rendus contain several communications from
him on the subject of complex numbers [or polynémes radicaux, as he has preferred to term
them]. In the earlier papers of this series, Cauchy attempts to prove a proposition which,
as we have already observed (see art. 41), is untrue for complex numbers considered gene-
rally, viz. that the norm of the remainder in the division of one complex number by another
can be rendered less than the norm of the divisor (see Comptes Rendus, vol. xxiv. pp. 517,
633 & 661). Llsewhere (iid. p. 579) he assumes the proposition as a hypothesis, and
deduces from it conclusions which are erroneous (pp. 581, 582). But at p. 1029 he recognizes
and demonstrates its inaccuracy. The results at which he arrives in his subsequent papers
on the same subject are, for the most part, comprehended in M. Kummer’s general theory
(Comptes Rendus, vol. xxv. pp. 37, 46, 93, 132, 177). In one place, however (p. 181), he
enunciates, though without demonstrating, the following important result :—
“Tf the equation a+ y+2=0 be resoluble, 2, y, z denoting integral numbers prime to
A, the sum
fake Sees e-em et +(e
is divisible by \.”
(Compare M. Kummer’s memoir in the Berlin Transactions for 1857, p. 64.)
The investigation of the Last Theorem of Fermat has been twice proposed as a prize-
question by the Academy of Paris—first at some time previous to 1823 (see Legendre’s
memoir already cited, in vol. vi. of the Mémoires de l’Académie des Sciences, p. 2), and again
in 1850 (Comptes Rendus, vol. xxx. p. 263): at neither time was the prize adjudged to any
of the memoirs received. On the last occasion, after several postponements of the date
originally fixed for the award, the prize was ultimately, in 1857 (id. vol. xliv. p. 158), con-
ferred on M. Kummer, who had not been a competitor, for his researches on complex num-
bers.
* Liouville, vol. xvi. p. 488, or Crelle, vol. xl. p. 131.
+ See the memoir No. 15 in the list of art. 41.
‘£ When A is not an exceptional prime, the equation v\+y\+z2*=0 is irresoluble not only
OO
ON THE THEORY OF NUMBERS, 151
We may suppose that \ is greater than 3, and that no two of the numbers
2, y, z admit any common divisor. And first, let none of them be divisible
ak—
by 1—a, « still representing a root of the equation =0. Since for x
we may write a’ a, we may assume that 2, y, z are of the form
x=a+(1—«a)’ X,
y=b+(1—«)’ Y,
z=c+(1—«a)’Z,
a, b, c denoting integral numbers prime to A, which evidently satisfy the con-
gruence a+6+c=0, mod. The equation a\+y*-+2*=0 may then be
written thus
(way) (a+a2y) (w@ta%y)....(atary)=—2",
No two of the factors of which the left hand member is composed can have
any common divisor; each of them is therefore the product of a perfect Ath
power by a unit; so that we may write, r+a°y=a?e(a)v*, e(a) denoting
areal unit. Since wv’ is an actual number, it follows (remembering that ) is
not an exceptional prime) that v is also actual ; hence v* is congruous, mod A,
to a certain integral number m. Eliminating m x e(a@) between the two con-
gruences x+a°y==ma’e(a), and +a “y=ma °e(a), mod Xd, we find
a °(ata’y)—a°(x+a *y)=0, mod AX. For the modulus (1—«) this
congruence is identically satisfied*. That it should be satisfied, mod (1—«)’,
we must have the relation (@+)p==ds, mod X; whence, putting
b
—— =k, mod d,
a+b
we have p=s, mod X. Substituting this value for p, we find that the con-
gruence
a" (e@tacy)—ak (a+a-*y)—0
is identically satisfied, mod (1—«)’*; but in order that it should be satisfied,
mod (1—a)*, we have the condition
s°b(2k—1) (R—1)—3s(k—1 .y"+ha")=0, mod A,
where 2 and y' are the values (for~=1) of the second derived functions
of # and y with respect to a. This conditional congruence must be satisfied
for every value of s; either therefore k==1, mod A, or 2R=1, mod. The
supposition A==1 is inadmissible; for it implies that a==0, mod A, contrary
to the hypothesis. Hence we must have 2k=1, and a=, or, by parity of
reasoning, a=b=c, mod Xr. But alsoa+b+c=0, mod A, whence we again
infer the inadmissible conclusion a==b==c=0, mod X.
in ordinary integral numbers, but also in any complex integers composed of Ath roots of
unity. The demonstration does not possess the same generality when A is an exceptional
prime satisfying the three conditions cited in the text. In this case M. Kummer has only
shown that the equation #\+-y*+-z\=0 is irresoluble when we suppose that 2, y, z are
ordinary integral numbers prime to X, or else complex numbers containing the binary periods
a+a—!, one of which has a common divisor with i.
* Since is divisible by (1—2)"—?, and since 9(«)=9 (1)-+(@-1) ¢'()+@-I2£O
+...,it is readily seen that, if-<X—1, the conditions for the divisibility of ¢(«) by
(1—«)” are ¢(1)=0, ¢'(1)=0,..... ¢°-)(1)==0, mod A.
Le REPORT—1860.
Secondly, let one of the numbers a, y, z (for example, z) be divisible by
1—a; it will be convenient to consider the equation in the generalized form
a +y*=E(a)(1—a)y™2%- 2.2 26
in which a, y, and z are all prime to 1—a@, and E(a) is any unit. We may
assume that the values of # and y are of the form
x=a+(1—a)’X,
y=b+(1—a)’Y,
a and 6 being prime to X, but satisfying the relation a+5==0, mod 2.
In the first place, m must be greater than]. For since v4 =a, and yA’ =B,
mod (1 —a)*+1, if a*+y* be divisible by (1—a)*, a*+0' is divisible by A’, and
therefore x+y by (l—a)‘*". Again, each of the factors x+ay, x+a7y,
...a+a—1y is divisible once, and once only, by l—a; whence it follows
that x+y is divisible by (1—a)”—**", and that no two of the d factors of
a\+y* have any other common divisor than 1—a. Hence the A factors
Rak6 s/o e+ay atar—ly
(l—a)ma—r>+’ et ee eee
are relatively prime, and may be represented by expressions of the form
2 (a) $e" e (2) o> Ch eR Oe €x-1 (a) pa-1 *
e, (a), €, (a), ... representing units, and ¢,\, ¢,°,.... Ath powers prime to
1—a. Eliminating x and y from the three equations
aty =e,(a)(1—a)™—**19,%,
ata" y=e,(a)(1—2) 4,
+ Gs y=es (a) (1—a) os’
we obtain a result of the form
gr +e (a) o\=E, (a) (1—ay™™*6., . «+ (2)
e(a@) and E,(a) denoting two units. But, as in the former case, it may
be shown that r* and os* are congruous, mod X, to real integers, and
(1—a)""~?*=0, mod d, because m>1. Hence (a) is also congruous to
a real integer for the modulus X, and _is therefore a perfect Ath power by a
property of every non-exceptional prime (see art. 52). The equation (2)
therefore assumes the form Te
x +yA=E, (a) 2 (1—ayer—a,
If, therefore, the proposed equation (1) be possible, it will follow, by suc-
cessive applications of this reduction, that the equation
x +y\=E (a) (1—a)* <*
is also possible. But this equation has been shown to be impossible; the
equation (1) is therefore also impossible.
62. Application to the Theory of Numerical Equations.—In the Monats-
berichte for June 20, 1853 (see also the Monatsberichte for 1856, p. 203),
M. Kronecker has enunciated the following theorem :—
“The roots of any Abelian equation, the coefficients of which are integral
numbers, are rational functions of roots of unity.” The demonstration of
this theorem (Monatsberichte for 1853, p- 371-873) depends ona compa-
heey
ON THE THEORY OF NUMBERS, 153
rison of a certain form, of which the resolvent function of any Abelian
equation is susceptible, with M. Kummer’s expression for the resolvent func-
tion in the case of the equation of the division of the circle (see art. 60).
It thus involves considerations relating to ideal numbers.
Two propositions of a more special character, and closely connected with
one another, have also been given by M. Kronecker (Crelle, vol. liii. p. 173).
Their demonstration is immediately deducible from the principles of Dirich-
let’s theory of complex units :—
‘<Tf unity be the analytical modulus of every root of an equation, of which
the first coefficient is unity and all the coefficients are integral numbers, the
roots of the equation are roots of unity.”
“Tf all the roots of an equation (having its first coefficient unity and all
its coefficients integral) be real and inferior in absolute magnitude to 2, so
that they can be represented by expressions of the form 2 cos a, 2 cos f,
2 cos y,....the arcs a, 2, y are commensurable with the complete circum-
ference.”
In the following proposition M. Kronecker has extended a theorem of
M. Kummer’s (art. 42) relating to complex units composed with roots of
unity of which the index is a prime, to complex units composed with any
roots of unity (Crelle, vol. liii. p. 176) :—
« Every complex unit composed with the roots of the equation w=1, can
be rendered real by multiplication with a 4th root of unity. If 2 be even,
a 2nth root will always suffice; and if m be a power of a prime, an nth root
will suffice.”
The demonstration of this proposition is also deducible from Dirichlet’s
principles.
63. Tables of Complex Primes——In M. Kummer’s earliest memoir on
complex numbers (Liouville, vol. xii. p. 206) he has given a table of the
complex factors, composed of \th roots of unity, which are contained in real
primes of the form m\ +1 inferior to 1000, A representing one of the primes
5, 7,11, 13, 17, 19, 23. This memoir was written before M. Kummer had
considered the complex factors of primes of linear forms other than mA+1,
and before he had introduced the conception of ideal numbers. The com-
plex prime factors of real primes of those other linear forms are, therefore,
not exhibited in the Table; and the five numbers of the form 23m+1, 47,
139, 277, 461, 967, each of which contains 22 ideal factors composed of 23rd
roots of unity, are represented as products of 11 actual factors (each of
which contains two reciprocal ideal factors). The tentative methods by
which the complex factors were discovered are explained in sect. 9 of the
memoir cited. Since the full development of M. Kummer’s theory, Dr.
Reuschle has undertaken to complete and extend the Table. He has already
given tables containing the complex prime factors of all real primes less than
1000, composed of 5th, 7th, 11th, 13th, 17th, 23rd, and 29th roots of unity,
together with the complete solution of the congruences corresponding to the
equations of the periods (see the Monatsberichte for 1859, pp. 488 and
694, and for 1860, pp. 150 and 714). For 5, 7, 11, 13, 17, the complex
primes are exhibited in a primary form; for 19, 23, and 29 they are exhibited
in a form which satisfies the condition f(a) = f(1), mod (I—«)?, but not
the condition f (2) f(a-!)=[f (1)}?, mod \. The ideal factors Dr.
Reuschle represents by their lowest actual powers; for 23 this power is the
cube, for 29 it is the square; for 11, 13, 17, 19, as well as for 5 and 7, all
complex prime factors of real primes less than 1000 are actual. It appears
from the Table (and it has indeed been proved by M. Kummer), that 29 is
an “ irregular determinant” (see art. 49, note) ; for the number of classes is
154 REPORT—1860.
8, while the square of every ideal number (occurring as a factor of a real
prime inferior to 1000) is actual. The methods employed by Dr. Reuschle
in the caiculation of his tables have not yet been published by him. In
some instances, as M. Kummer has observed, they have not led him to the
simplest possible forms of the ideal primes.
A particular investigation relating to the ideal factors of 4:7, composed of
23rd roots of unity, has been given by Mr. Cayley (Crelle, vol. lv. p. 192,
and lvi. p. 186).
64. The investigations relating to Laws of Reciprocity, which have so long
occupied us in this report, have introduced us to considerations apparently
so remote from the theory of the residues of powers of integral numbers, that
it requires a certain effort to bear in mind their connexion with that theory.
It will be remembered that the complex numbers to which our attention has
been directed are not of that general kind to which we have referred in art. 41,
but are exclusively those which are composed of roots of unity. The theory
of complex numbers, in the widest sense of that term, does indeed present to
us an important generalization of the theory of the residues of powers; for
the theorem of Fermat (see art. 53) subsists alike for every species of com-
plex numbers. But the complex numbers of Gauss, of Jacobi, and of M.
Kummer force themselves upon our consideration, not because their proper-
ties are generalizations of the properties of ordinary integers, but because
certain of the properties of integral numbers can only be explained by a
reference to them. The law of quadratic reciprocity does not, as we have
seen, necessarily require for its demonstration any considerations other than
those relating to ordinary integers ; the real prime numbers of arithmetic are
here the ultimate elements that enter into the problem. But when we come
to binomial congruences of higher orders, we find that the true elements of
the question are no longer real primes, but certain complex factors, composed
of roots of unity, which are, or may be conceived to be, contained in real
primes. For we find that the law which expresses the mutual relation (with
respect to the particular kind of congruences considered) of two of these
complex factors is a primary and simple one; while the corresponding rela-
tions between the real primes themselves are composite and derivative, and, in
consequence, complicated. It thus becomes indispensable, for the investiga-
tion of the properties of real numbers, to construct an arithmetic of complex
integers ; and this is what has been accomplished by the researches, of which
an account has been given in the preceding articles.
The higher laws of reciprocity (like that of quadratic residues) may be
considered as furnishing a criterion for the resolubility or irresolubility of
binomial congruences ; and this, though not the only application of which they
are susceptible, is that which most naturally suggests itself. When the bi-
nomial congruence is cubic or biquadratic, it is easy to resolve the real prime
modulus into factors of the form a+ dp, or a+ bi (arts. 37 and 24), and equally
easy to determine the value of the critical symbol of reciprocity by a uni-
form and elementary process (see art. 36). For these, therefore, as well as
for quadratic congruences, the criterion deducible from the laws of recipro-
city is all that can be desired. But for binomial congruences of higher
orders this criterion is not a satisfactory one, because of the difficulty of
obtaining the resolution of a real prime into its complex factors, and also
because of the impossibility of determining the value of the critical symbol
by the conversion of an ordinary fraction into a continued fraction.
The only known criterion applicable to such congruences is the following,
_the demonstration of which is deducible from the elements of the theory of
the residues of powers:—Let x”==A, mod p, represent the proposed con-
ee ee
———-. , —_
—
ON THE THEORY OF NUMBERS. 155
gruence ; it will be resoluble or irresoluble according as the index of A is or
is not divisible by d, the greatest common divisor of x and p—1, i.e. according
as the exponent to which A appertains is or is not a divisor of er (see
arts. 14 and 15).
65. Solution of Binomial Congruences.—We now come to the problem of
the actual solution of binomial congruences—a subject upon which our
knowledge is confined within very narrow limits.
When a table of indices for the prime p has been constructed, the resolu-
tion of every binomial congruence, if it be resoluble, or, if not, the demon-
stration of its irresolubility, is implicitly contained in it. But to use a table
of indices for the solution of a binomial congruence is, as we have already
observed in a similar case (art. 16), to solve a problem by means of a recorded
solution of it. When the congruence a”==A, mod 7, is resoluble, its solu-
tion may always be made to depend on that of a congruence of the form
x’==a, mod p, where d is the greatest common divisor of x and p—1, and
where aA‘, mod p, and ns==d, mod p—1. We may therefore suppose
that, in the congruence a”==A, mod p, n is a divisor of p—1. This con-
gruence (if resoluble at all) will have as many roots as it has dimensions; if
— be any one of them, and 1, 0,, 6,,--.@n_, be the roots of the congruence
x"==1, mod p, the roots of a*“==A, mod p, will be £, £0,, £0,,...£0n-1; so that
the complete resolution of the congruence a”= A, mod p, requires, first, the
determination of a single root of that congruence itself, and, secondly, the com-
plete resolution of the congruence #”==1, mod p. With regard to the first of
these requisites, in the important case in which the exponent ¢ to which A
appertains is prime to 7, a value of x satisfying the congruence a"= A, mod p,
can be determined by a direct method (Disq. Arith. arts. 66, 67). For, in
this case, it will always happen that one value of z is a certain power A* of
A, where & is determined by the congruence kn=1, mod ¢. Nor is it
necessary, in order to determine #, to know the exponent ¢ to which A
appertains; it is sufficient to have ascertained that it is prime to m; for, if
we resolve p—1 into two factors prime to one another, and such that one of
them is divisible by m and contains no prime not contained in n, the other
will be divisible by ¢, and may be employed as modulus instead of ¢ in the
congruence kn==1, mod¢. When this method is inapplicable, we can only
investigate a root of the congruence #”==A, mod p-(where A is different
from 1), by tentative processes, which, however, admit of certain abbreviations
(Disq. Arith. arts. 67,68). The work of Poinsot (Réflexions sur la Théorie
des Nombres, cap. iv. p. 60) contains a very full and elegant exposition of
the theory of binomial congruences; but neither he nor any other writer
subsequent to Gauss has been able to add any other direct method to that
which we have just mentioned.
66. Solution of the Congruence x"=1, mod p.—When a single root of the
congruence x”= A is known, we may, as we have seen, complete its resolu-
tion by obtaining all the roots of the congruence a”=1, mod p. The methods
of Gauss, Lagrange, and Abel for the solution of the binomial equation
x"—]=0 are in a certain sense applicable to binomial congruences of this
special form. It is evident, from a comparison of several passages in the Dis-
quisitiones Arithmetic *, that Gauss himself contemplated this arithmetical
application of his theory of the division of the circle, and that he intended to
include it in the 8th section of his work, which, however, has never been
given to the world. In fact, the method of Abel+ which comprehends that
* See Disq. Arith. arts. 61, 73, and especially art. 335.
T See Abel’s memoir, “‘ Sur une classe particulicre d’équations résolubles algébriquement,””
156 REPORT—1860.
of Gauss, and which gives the solution of any Abelian equation, is equally
applicable to any Abelian congruence; zt. e. to any completely resoluble con-
gruence of order m, the m roots of which (considered with regard to the
prime modulus p) may be represented by the series of terms
7, $(7)s g(r) +++. g9™—"(r),
the symbol ¢ denoting a given rational [fractional or integral] function.
And as we can always express the roots of an Abelian equation by radicals
(i. e. by the roots of equations of two terms), so also the solution of an Abelian
congruence depends ultimately on the solution of binomial congruences.
When, for any prime modulus, an Abelian equation admits of being con-
sidered as an Abelian congruence, so precise is the correspondence of the
equation and the congruence, that (as Poinsot has observed in a memoir
in which he has occupied himself with the comparative analysis of the equa-
tion «*=1, and the congruence z”==1, mod p*) we may consider the ana-
lytical expression of the roots of the equation as also containing an expression
of the roots of the congruence ; and by giving a congruential interpretation T
to the radical signs which occur in that expression, we may elicit from it the
actual values of the roots of the congruence. An example taken from
Poinsot’s memoir will render this intelligiblef. The six roots of the equation
we
= Sty are comprised in the formula
x—1
SLEW Eg 8 yo lh, Lid ee
alt Nats 7 av —7 +321 Bir ii 5Vai-5V a | ;
where the signs + and — are to be successively attributed to W —7, and
where the product of the two cube roots is + Vor Sa according
to the sign attributed to Va Considering the equation as a congruence
with regard to the modulus 43, and observing that
V —7= +6, mod 43, ¥21= +8, mod 43,
we obtain in the first place
‘Ov Ba yeet ey fh aad
— atsv 16 +58 mod 43,
Th. WA eS OL cee
and gata s/22t gv —2 mod 43,
the product of the two cube roots being congruous to +6 in the first formula,
and to —6 in the second; and finally, observing that
4/16 21, — 3, —18, mod 43,
ee: 14, — 2, —12, mod 43,
4/22 =—15, — 4, 19, mod 43,
2/ —2 =+ 9, —20, +11, mod 43,
sect. 3 (Guvres, vol.i. p. 114, or Crelle, vol. iv. p. 131), and M. Serret’s Algebre Supérieure,
26th and 27th lessons.
* “Sur l’Application de l’Algébre 4 la Théorie des Nombres,’’ Mémoires de l’Académie
des Sciences, vol. iv. p. 99. 1s
+ Gauss employs the symbol \// A, mod g, to denote a root of the congruence a" =A, mod p,
just as he employs the symbol = mod p, to denote the root of the congruence Av=B,
|
ll tl il
mod p. The congruential radical .’/ X, mod p, has of course as many values as the con-
gruence x"= A, mod 2, has solutions; if that congruence be irresoluble, the symbol is im-
possible.
t See the memoir cited above, p. 125,
bank
ON THE THEORY OF NUMBERS. 157
and attending to the limitation to which the cube roots are subject,
x= —8, +11, +21, or, —2,+4, +16; mod 43.
Thus the complete solution of a congruence of the sixth order is obtained by
means of binomial congruences of the second and third orders only.
An essential limitation to the usefulness of this method arises from the cir-
cumstance that it does not always (or even in general) happen that (as in
the example just given) each surd entering into the expression of the root
becomes separately rational. For that expression may itself acquire a rational
value, while certain surds contained in it continue irrational, precisely as, in
the irreducible case of cubic equations, a real quantity is represented by an
imaginary formula. To illustrate this point by an example, let us consider
7
v1 9 with respect to the modulus 29{ Here in
the same congruence
the expression
—1+¥—7 1 £74 Svan | 4 5e"[ 7-3 7-3 |
pa Sel 7g tt va +5? 7-3 —7-5v a1 |,
where p denotes a cube root of unity, we have, putting V —7= +14, and
p=,
2=— + : [eva|'+5 [-5vai] » =F=1, mod 29,
the irrational cube roots disappearing of themselves. Again, putting
p= 3 (1+ “=3),
we find
w=71tiv—3(5v a )=14(5V—7)"
=74(7)'=7416=-—6 or —9,
where every radical becomes rational of itself. Similarly taking the values
¥—7=—14, p=5(—1 +¥.—3), we find z=—5 or —13. But lastly,
putting V —7=—14, p=1, we find
r=12+ SC+7 V2)43(14—7 V2).
To rationalize this expression, we have to observe that 147 9, relatively
to the modulus 29, is the cube of a complex number of similar form ; in fact,
we have (14+7V2)=(5+11¥2)*, mod 29, whence x=—4. To elicit,
therefore, the value of this root from the irrational formula, we are obliged to
solve the cubic congruence x°=14+7 V2, which, although of lower dimen-
sions than the proposed congruence, is probably less easy to solve tentatively,
because 29 has 297—1=840 residues of the form a+b¥2, and only 29—1
=28 ordinary integral residues; so that practically the method fails. Theo-
retically, however, the relation between the analytical expression of the
equation-rocts and the values of the congruence-roots is of considerable
importance, and the subject would certainly repay a closer examination
than it has yet received. We may add that, if m be a divisor of p—1l,
t Ibid. p. 132.
158 REPORT— 1860.
the complete solution of an Abelian congruence of order m requires only
two things,—lIst, the complete solution of the congruence 2m — ] =0O,
mod p, and, 2ndly, the determination of a single root of a certain con-
gruence of the form #”—a==0, mod p, in which a is an ordinary integer;
a’ —]
so that in this case (which is that of the congruence ; =0, mod 43)
we obtain a real, and not only an apparent reduction of the proposed con-
gruence*.
It should also be observed that the primitive roots of the equation
ar—] : : ‘ achsayy
=0 furnish, when rationalized, the primitive roots of the congruence
a2—
“— =0,mod p. This, the only direct method that has ever been suggested
x
for the determination of a primitive root, appears to be the same as that
referred to by Gauss in the Disq. Arith. (art. 73).
Poinsot expresses the conviction that this method of rationalization is
applicable to any congruence corresponding to an equation, the roots of
which can be expressed by radicals+. With regard to equations of the
second, third, and fourth orders this is certainly true. If, for example, the
biquadratic equation F, (z)=0O be completely resoluble when considered as
a congruence for the modulus p, so that F, (x)= (a—a,) (w—a,) (wx—a,)
(x—a,), mod p, it is plain that the four roots of F(#)=0, and the four
numbers @, @,, @,, a, may be obtained by substituting, in the general formula
which expresses the root of any biquadratic equation as an irrational function
of its coefficients, the values of the coefficients of the functions F (a) and
(x—a,) (w—a,) (x—a,) (w—a,) respectively. But these two sets of coeffi-
cients differ only by multiples of p; 7. e. the values of a,, a,, a,, a, can be
deduced from the expressions of the roots of F (v)=0 by adding multiples
of p to the numbers which enter into those expressions. But this reasoning
ceases to be applicable to equations of an order higher than the fourth,
because no general formula exists representing the roots of an equation of
the fifth or any higher order. If, therefore, F(x)=0 be an equation of the
mth order, the roots of which can be expressed by a radical formula, and
which is also completely resoluble when considered as a congruence for the
modulus p, so that F(a)=(a—a,) (w—a,)...(a@—ad,), mod p, it will not
necessarily follow that the formula which gives the roots of F(z)=0 is also
capable (when we add multiples of p to the numbers contained in it) of
giving the roots of (vw—a,)(xw—a,)...(a—an)=0, 7. e. the roots of the con-
gruence F(2)==0, mod p; and thus the principle enunciated by M. Poinsot
is, it would seem, not rigorously demonstrated.
67. Cubie and Biquadratic Congruences.—The reduction of cubie con-
gruences to binomial ones has been treated of by Cauchy (Exercices des
Mathématiques, vol. iv. p. 279), and more completely by M. Oltramare
(Crelle, vol. xlv. p. 314). Some cases of biquadratic congruences are also
considered by Cauchy in the memoir cited, p. 286. The following criteria
for the resolubility or irresolubility of cubic congruences include the results
obtained by M. Oltramare, /. c., and appear sufficiently simple to deserve
insertion here :—
Let the given cubic congruence be
* This will be at once evident, if we observe that when the congruence #”=1, mod p,
is completely resoluble, its roots may be employed to replace, in Abel’s method, the roots of
the equation 7”™—1=0.
+ See the memoir cited above, p. 107, and M. Libri, Mémoires de Mathématique et Phy-
sique, p. 63.
a
ON THE THEORY OF NUMBERS. 159
a0?+360°+3c0+d=0, mod p,
p denoting a prime greater than 3, which does not divide the discriminant of
the congruence; 7. e., the number
D= — a d+ 6abed—4ac?—4.db? +36’ e’;
and in connexion with the congruence consider the allied system of functions *
U=(a, b, c,d) (a, )*,
H=(ace—0", > (ad—be), bd—c’) (2, y)’,
®=(—a’ d+3abe— 26°, —abd+2ac?+b’ ec, acd—2b? d+ be’,
ad*—3bed+ 2c’) (a, y)’,
which are connected by the equation
+ Duw’?=—4H';
let also w and ¢ denote the values of U and © corresponding to any given
values of x and y, which do not render H=0, mod p. Then, if (GP )=-1
P
the congruence has always one and only one real root; if (=)= +1, it has
P
fy =e
either three real roots, or none: viz., if a) = +1], it has three;
3
if (ete) p, or =p, it has none. The interpretation of the
P
eubic symbol of reciprocity will present no difficulty if we observe that ¥ —D,
mod p, is a real integer if p=3n-+1, z.e. if (=)=» and that, if p=3n—1,
el ir (> )=-1. we have V—D="—8x WID=(p—p")W ID, mod p,
so that ¥ —D, mod p, is a complex integer involving p. It will however be
observed that the application of the criterion requires in either case the solu-
tion of a quadratic congruence, 7*==—D, mod p, or r°=+1D, mod p.
Similar, but of course less simple, criteria for the resolubility or irresolu-
bility of biquadratic congruences may be deduced from the known formule
for the solution of biquadratic equations.
68. Quadratie Congruences—Indirect Methods of Solution—The general
form of a quadratic congruence is az*+2bx2+c=0, mod P;—p denoting an
‘uneven prime modulus, and a a number prime to p. It may be immediately
reduced to the binomial form 7*=D, mod p, by putting r=axz+6, D=0?
—ac,mod p. ‘The number of its solutions is 2, 0, or 1, according as D is a
quadratic residue or non-residue of p, or is divisible by p, and is therefore
in every case expressed by the formula 1+(— ).
If p=4n+3, and ~)=1, the congruence 7*— D==0, mod 9, is satisfied
by 7=D"*), and r=—D”*, and is in fact resoluble by the direct method
of art.65. But no direct method, applicable to the case when p=4n+1,
is at present known. Two tentative methods are proposed in the sixth sec-
tion of the Disquisitiones Arithmetic. They are both applicable to con-
gruences with composite as well as with prime modules. This circumstance
* See a note by Mr. Cayley in Crelle’s Journal, vol. 1. p. 285.
yo
160 REPORT—1860.
is important, because, when the modulus is a very great number, we may not
be able to tell whether it is prime or composite, and, if composite, what the
primes are of which it is composed, although, when the prime divisors of a
composite modulus are known, it is simplest first to solve the congruence for
each of them separately, and afterwards (by a method to which we shall
hereafter refer) to deduce from these solutions the solution for the given
composite modulus. To apply the first of Gauss’s methods, the congruence
is written in the form 77> =D-+ Py, P denoting the modulus. If in the formula
V=D+Py we substitute for y in succession all integral values which satisfy
the inequality —Pay<iP-Z. and select those values of V which are per-
fect squares, their roots (taken positively and negatively) will give us all the
solutions of the congruence. We should thus have I¢P or 1+I}P trials to
make, I denoting the greatest integer contained in the fraction before which it
is placed. If, however, we take any number E, greater than 2, and prime to
P (it is simplest to take for E a prime, or power of a prime), of which the
quadratic non-residues are @, 0, c,..., and then determine the values of a, 3, y,
... in the congruences a==D-+aP, mod E, 5=D+£P, mod E, &c., we shall
find that every value of y contained in one of the linear forms mE+a,
mE+/, &c., gives rise to a value of V which is a quadratic non-residue of
E, and which cannot, therefore, be a perfect square ; so that we may at once
exclude these values of y from the series of numbers to be tried. A second
excludent E! may then be taken, and by its aid another set of linear forms
may be determined, such that no value of y contained in them can satisfy
the congruence. Thus the number of trials may be diminished as far as
we please. The application of this method is still further facilitated by the
circumstance that it is not necessary actually to solve the congruences
a=D-+aP, mod E, ... but only the single congruence D+ Py=0, mod E
(Disq. Arith. art. 322). Gauss’s second method depends on the theory of
quadratic forms; it supposes that the congruence is written in the form
7?+D=0, mod P. By a tentative process (abbreviated, as in the first
method, by the use of excludents) Gauss obtains all possible prime representa-
tions of P by the quadratic forms of determinant —D; whence the com-
plete solution of the congruence r+ D=0, mod P, is immediately deduced.
This method involves the construction of a complete system of quadratic
forms of determinant —D, or, if the prime factors of D be known, of one
genus of forms of that system; it becomes therefore more difficult of appli-
cation as D increases, whereas the first method is not affected by the increase
of D. The second method, however, especially recommends itself when P is
a very great number; in fact, if we do not employ any excludent, the number
of trials required by the first method varies (approximately, and when P is
a great number) as P, whereas, on the same supposition, the number of trials
required by the second method varies as VDx VP.
M. Desmarest (in his Théorie des Nombres) has proposed a method less
scientific in its character than those of Gauss, but sometimes easily applicable
in practice. He has shown that if the congruence 7+ D==0, mod P, be re-
soluble, we can always satisfy the equation mP=2*+ Dy* with a value of
>
m inferior to i+; and of y not superior to 8. The demonstration of this
theorem is not very satisfactory, and the number of trials that it still leaves
is very great, viz. 3 Gr + s),
The application of Gauss’s second method is rendered somewhat more uni-
hi
|
|
ed
ys
ON THE THEORY OF NUMBERS. 161
form, and at the same time the necessity for constructing a system of qua-
dratic forms of determinant —D is avoided by the following modification of
it:—By a known property of quadratic forms, whenever the congruence
r’ +D=0, mod P, is resoluble, the equation mP=a°+ Dy’ is resoluble for
some value of m < 2/2. By assigning, therefore, to m all values in suc-
cession which are inferior to that limit, and which satisfy the condition
(5) = (5) and then obtaining (by Gauss’s method) all prime representa-
U
tions of the resulting products by the form x?+-Dy’, we shall have r=+
ff
r=+ oie .-.. mod P, 2’, y', x", y'! etc. denoting the different pairs of values
of x and y in the equation mP=2?+ Dy’.
69. General Theory of Congruences.—We may infer from several passages
in the Disquisitiones Arithmetice, that Gauss intended to give a general
theory of congruences of every order in the 8th section of his work, and
that, at the time of its publication, he was already in possession of the prin-
cipal theorems relating to the subject*. These theorems were, however,
first given by Evariste Galois, in a note published in the Bulletin de Férus-
sac for June, 1830 (vol. xiii. p. 438), and reprinted in Liouville’s Journal,
vol. xi. p.398. An account of Galois’s method (completed and extended in
some respects) will be found in M. Serret’s Cours d’Algébre Supérieure,
Jecon25. The theory has also been independently investigated by M. Schoe-
nemann, who seems to have been unacquainted with the earlier researches of
Galois (see Crelle’s Journal, vol. xxxi. p. 269, and vol. xxxii. p. 93). In
several of Cauchy’s arithmetical memoirs (see in particular Exercices de
Mathématiques, vol. i. p. 160, vol. iv. p. 217; Comptes Rendus, vol. xxiv.
p- 1117; Exercices d’Analyse et de Physique Mathématique, vol. iv. p. 87)
we find observations and theorems relating to it. Lastly, in a memoir in
Crelle’s Journal (vol. liv. p. 1) M. Dedekind has given (with important
accessions) an excellent and lucid résumé of the results obtained by his pre-
decessors.
In the following account of the principles of this theory, the functional
symbols F, ¢, ,... will represent (as in general throughout this Report)
rational and integral functions having integral coefficients; we shall use p
to denote a prime modulus, and @ an absolutely indeterminate quantity. As
we shall have to consider the functions F(x), f(x), (a), ete., only in relation
to the modulus p, we shall consider two functions F, (x) and F, (2), which
differ only by multiples of p, as identical, and we shall represent their identity
by the congruence F, (v)=F, (x), mod p, which is equivalent to an identical
equation of the form F,(2)=F,(«)+p)(x). The designation “modular
function,” which has been introduced by Cauchy (Comptes Rendus, vol. xxiv.
p- 1118) will serve (though, perhaps, not in itself very appropriate) to indicate
that the function to which it is applied is thus considered in relation to a
* See Disq. Arith. art. 11 and 43.
t Galois was born October 26, 1811, and lost his life in a duel, May 30, 1832. He was
consequently eighteen at the time of the publication of the note referred to in the text. His
mathematical works are collected in Liouville’s Journal, vol. xi. p. 381. Obscure and frag-
mentary as some of these papers are, they nevertheless evince an extraordinary genius, un-
paralleled, perhaps, for its early maturity, except by that of Pascal. It is impossible to read
without emotion the letter in which, on the day before his death and in anticipation of it,
Galois endeavours to rescue from oblivion the unfinished researches which haye given him a
place for ever in the history of mathematical science.
1860. M
162 REPORT—1860.
prime modulus. Since in any modular function we may omit those terms
the coefficients of which are multiples of p, we shall always suppose that
the coefficient of the highest power of z in the function is prime to p.
If F(w)=f, (x) xf, (w), mod p, f, (w) and f, (#) are each of them said to
be divisors of F(x) for the modulus p, or, more briefly, modular divisors of
F(x), or even simply divisors of F(a) when no ambiguity can arise from this
elliptical mode of expression. If a be a function of order zero, i. e. an integral
number prime to p, @ is a divisor, for the modulus p, of every other modular
function; so that we may consider the p—1 terms @,, @,, @,; -.. @p—1, of a
system of residues prime to p, as the units of this theory, and, in any set of
p—1 associated functions
a E(z), a, F(@)p26e. apa EC),
we nay distinguish that one as primary in which the highest coefficient is
congruous to unity (mod p).
If F(#) be a function which is divisible (mod p) by no other function
(except the units and its own associates), F(x) is said to be a prime or irre-
ducible function for the modulus p. And it is a fundamental proposition in
this theory, that every modular function can be expressed in one way, and
one way only, as the product of a unit by the powers of primary irreducible
modular functions. The demonstration of this theorem depends (precisely
as in the case of ordinary integral numbers) on Euclid’s process for finding
the greatest common divisor, which, it is easy to show, is applicable to the
modular functions we are considering here. For, if o, (a) and , (a) be two
such functions [the degree of ¢,(#) being not higher than that of @, (x)],
we can always form the series of congruences
$:() = (x) $.(@) +7 $4(x), mod p,
$2(@)=9.(#) $,(@) +7, 9,(@), mod p,
Ce et eC eC De Mie Dc Sa YS OR RSM Je Sea eer Tt CT
in which 7,, 7, ... denote integral numbers, g,(“), g,(#),-.. modular func-
tions, and ¢,(«), ¢,(v),-... primary modular functions, the orders of which
are successively lower and lower, until we arrive at a congruence
px (2) =k (2) ort (@) +7 or42(w), mod p,
in which 7,==0, med p. The function $741 (7) is then the greatest common
divisor (mod p) of the given functions ¢, (w) and @, (a); and, in particular,
if 441 (@) be of order zero, those two functions are relatively prime. We
may add that, if R be the Resultant of ¢,(#) and ¢,(«), the necessary and
sufficient condition that these functions should have a common modular
divisor of an order higher than zero is contained in the congruence R=0,
mod p*—a theorem exactly corresponding to an important algebraical pro-
position. From the nature of the process by which the greatest common
divisor is determined, we may infer the fundamental proposition enunciated
above, by precisely the same reasoning which establishes the corresponding
theorem in common arithmetic. Similarly, we may obtain the solution of
the following useful problem :—“ Given two relatively prime modular func-
tions A,, and A,, of the orders m and m, to find two other functions, of the
orders m—1 and m—1 respectively, which satisfy the congruence
A ke : Gat An Rene 1 ls mod Pp
* See Cauchy, Exercices de Mathématiques, vol. i. p. 160, or M. Libri, Mémoires de Mathé-
matique et de Physique, pp. 73, 74. But a proof of this proposition is really contained in
Lagrange’s Additions to Euler’s Algebra (sect. 4).
re
ON THE THEORY OF NUMBERS. 163
The assertion that f(«) is a divisor of F(x), for the modulus p is for
brevity expressed by the congruential formula
F(«)=0, mod [p, f(#)],
which represents an equation of the form
F(x)=p9 (a) + f(#) 9 (2).
Similarly the congruence F,(#)=F,(x), mod [p, f(x)], is equivalent to
the equation
P(e) =F) + po@) +f) Y @),-
If f(x) be a function of order m, it is evident that any given function is
congruous, for the compound modulus [p, f (x)] to one, and one only, of
the p™ functions contained in the formula @,+a,¢7+ ...+@m-12™—}, in
which a,, a,,...@m_—, may have any values from zero to p—1 inclusive.
These p™ functions, therefore, represent a complete system of residues for
the modulus [p, f'(2)].
A congruence F(X)=0, mod [p, f(z) ], is said to be solved when a func-
tional value is assigned to X which renders the left-hand member divisible
by f(«) for the modulus p; and the number of solutions of the congruence
is the number of functional values (incongruous mod [p, f(#)]) which ma
be attributed to X. The coefficients of the powers of X in the function F(X
may be integral numbers or functions of x. The linear congruence AX=B,
mod [p,f(«)], in which A and B denote two modular functions, is, in
particular, always resoluble when A is prime to f(a), mod p, and admits, in
that case, of only one solution.
We shall now suppose that the function f(2) in the compound modulus
Lp, f(«)] is irreducible for the modulus p,—a supposition which involves the
consequence that, if a product of two factors be congruous to zero for the
modulus Cp, f(«)], one, at least, of those factors is separately congruous to
zero for the same modulus. We thus obtain the principle (cf. art. 11) that
no congruence can have more solutions, for an irreducible compound modu-
lus, than it has dimensions. For, if X==£, mod [p, f(x)], satisfy the con-
gruence F,, (X)=0, mod [p, f(x)], we find
Bn (X) == Fn (X)— Fn (2) = (X—£) Fn (X), mod [p, f(x)];
Fm—1 (X) denoting a new function of order m—1, whence it follows that if
the principle be true for a congruence of m—1 dimensions, it is also true for
one of m dimensions ; 2. e. it is true universally.
70. Extension of Fermat's Theorem.—Let 6 denote any one of the p™—1
residues of the modulus [p, f(x)] which are prime to f(x); it may be
shown, by a proof exactly similar to Dirichlet’s proof of Fermat’s theorem,
that
Ge =1==1), mod [p, f(#)].........-.2.+- (A)
This result, which is evidently an extension of Fermat’s theorem, involves
several important consequences.
It implies, in the first place, the existence of a theory of residues of powers
of modular functions, with respect to a compound modulus, precisely similar
to the theory of the residues of the powers of integral numbers with regard
to a common prime modulus. A single example (taken from M. Dedekind’s
memoir) will suffice to show the exact correspondence of the two theories.
The modular function 6 is or is not a quadratic residue of f(«), for the
modulus p, according as it is or is not possible to satisfy the quadratic con-
gruence X*==0, mod [p, f(w)]. In the former case @ satisfies the congruence
M2
164 REPORT—1860.
o3(p™-1) =], mod [p, f(x)]; in the latter, 04(?"-D==—1, mod [p, f()].
And, further, if 6, and 0, be two primary irreducible modular functions of
the orders m and x respectively, and if we use the symbols lel and [F| to
1
denote the positive or negative units which satisfy the congruences 63‘?"—))
x= [zi]. mod (p, @,), and he hp [z| , mod (2, 0,), respectively, these
2
1
two symbols are connected by the law of reciprocity [F| =(—1)”" Fe] ‘
2 1
But the equation (A) admits also of an immediate application to the theory
of ordinary congruences with a simple prime modulus.
In that equation let us assign to @ the particular value x ; we conclude that
the function #?”—1—1, is divisible for the modulus p by f(«), @.e. by every
irreducible modular function of order m. Further, if d be a divisor of m,
gP™—1—] is algebraically divisible by avP’—1 —]; whence it appears that
gvP™—1_] is divisible, for the modulus p, by every function of which the
order is a divisor of m. But it is easily shown that 2?”—!—1 is not divisible
(mod p) by any other modular function, and that it cannot contain any
multiple modular factors. Hence we have the indeterminate congruence
vp™-1_] =I f(x), mod p, ......... sen hi
in which f(x) denotes any primary and irreducible function, the order of
which is a divisor of m, and the sign of multiplication [I extends to every
value of f(x). This theorem, again, is a generalization of Lagrange’s inde-
terminate congruence (art.10). We may infer from it that, when m is >1,
the number of primary functions of order m, which are irreducible for the
modulus 7, is
m an py alee
= [Pm 2p" + ph qa — Spi gas + ste >
Gy» J «++ denoting the different prime divisors of m. As this expression is
always different from zero, it follows that there exist functions of any given
order, which are irreducible for the modulus p.
A congruence F(a#)==0, mod p, may be considered resolved when we
have expressed its left-hand member as a product of irreducible modular
factors. The linear factors (if any) then give the real solutions; the factors
of higher orders may be supposed to represent imaginary solutions. We have
already observed that even when all the modular factors of F(«) are linear,
we possess no general and direct method by which they can be assigned ; it
is hardly necessary to add that the problem of the direct determination of
modular factors of higher orders than the first, presents even greater diffi-
culties. Nevertheless the congruence (B) enables us to advance one step
toward the decomposition of F(2) into its irreducible factors ; for, by means
of it, we can separate those divisors of F(«) which are of the same order,
not, indeed, from one another, but from all its other divisors. We may first
of all suppose that F(#) is cleared of its multiple factors, which may be
done, as in algebra, by investigating the greatest common divisor of F()
and I'(x) for the modulus p. The greatest common divisor (mod p) of
F(x) and 2?-!—] will then give us the product of all the linear modular
factors of F(x); let F(a) be divided (mod p) by that product, and let the
quotient be F\(#); the greatest common divisor (mod py) of F,(x) and
gP*—1—] will give us the product of the irreducible quadratic factors of F(x) ;
ON THE THEORY OF NUMBERS. 165
and by continuing this process, we shall obtain the partial resolution of F(x)
to which we have referred.
71. Imaginary Solutions of a Congruence.—We have said that the non-
linear modular factors of F(«)==0, mod p, may be considered to represent
imaginary solutions. These imaginary solutions can be actually exhibited,
if we allow ourselves to assign to # certain complex values. The following
proposition, which shows in what manner this may be effected, is due to
Galois :-—
“If f(#) represent an irreducible modular function of order m, the con-
gruence
F(6)=0, mod [p, f(x)],
is completely resoluble when F(a) is an irreducible modular function of
order m, or of any order the index of which is a divisor of m.”
To establish this theorem, write 0 for 2 in equation (B); we find 62"-!—1
==II F(@), mod p, the sign of multiplication II extending to every irreducible
modular function having m or a divisor of m for the index of its order.
But the congruence 6?”—!==1, mod [p, f(x)], admits of as many roots as
it has dimensions; therefore also every divisor of 9?”—1— 1, and, in particular,
the function F(@) considered as a congruence for the same compound modu-
lus, admits of as many roots as it has dimensions.
Let the order of the congruence F(0)=0, mod [p, f(«)], be 6, and let
any one of its roots be represented by 7; it may be shown that all its roots
are represented by the terms of the series r, 7?, 7?°,... 77°}, For, if
F(r)=0, mod [p, f(x)], we have also F (r?)=[F(r)]?=0, mod [p,f()],
and similarly F(7?*)==[F (r)]”°=0, mod p; so that 7, 7?, 77’, ... 7?°—} are
all roots of F(@)==0, mod [p, f(#)]. it remains to show that these 6 func-
tions are all incongruous, mod [p, f(x)]. If possible let rp*+*' = ppt",
mod [p, f(x)], & and k' being less than 6; we have, raising each side of this
6—k' b+k 6 ° ee
congruence to the power pé—"", rP°*"==rP", mod [p, f(x) ], i.e. rP*=r, or
rP*—1==1, mod [p, f(x)], observing that rr°=r, mod Lp, f(x) ], because
rP’-1__] is divisible by F(r) for the modulus p- We conclude, therefore,
that 7 is a root, mod [p, f(«)], of some irreducible modular divisor of the
function 6?*—1—], i. e. of some irreducible function of an order lower than 6;
because & is less than 6; r is therefore a root, mod [p, f(x) ], of two different
irreducible modular functions, which is impossible.
If, therefore, we suppose x to represent, not an indeterminate quantity,
but a root of the equation f(2)=0, we may enunciate Galois’ theorem as
follows :—
“Every irreducible congruence of order m is completely resoluble in com-
plex numbers composed with roots of any equation which is irreducible for
the modulus p, and which has m or a multiple of m for the index of its order.
“ And all its roots may be expressed as the powers of any one of them.”
72. Congruences having Powers of Primes for their Modules.—It remains
for us to advert to the theory of congruences wiih composite modules—a sub-
ject to which (if we except the case of binomial congruences) it would seem
that the attention of arithmeticians has not been much directed. We shall
suppose, first, that the modulus is a power of a prime number.
The theorem of Lagrange (art. 11), and the more general proposition of
art. 69, in which it is (as we have seen) included, cannot be extended to
congruences having powers of primes for their modules.
Let the proposed congruence be F (a) =0, mod p™; and let us suppose
(what is here a restriction in the generality of the problem) that the coeffi.
166 REPORT—1860.
cient of the highest power of x in F(x) is prime to p, or, which comes to the
same thing, that it is unity. Let F(a#)=PXQxR...mod p,—P,Q,R,
.-. being powers of different irreducible modular functions. 1t may then be
shown that F (7)=P’x Q'x R’..., mod p”, where P’, Q’, R',... are fune-
tions of the same order as P, Q, R,..., respectively congruous to them for
the modulus p, and deducible from them by the solution of linear congru-
ences only. We have thus the theorem that F (x), considered with respect
to the modulus p”, can always be resolved in one way and in one way only,
into a product of modular functions, each of which is relatively prime (for the
modulus p) to all the rest, and is congruous (for the same modulus p) to a
power of an irreducible function. We may therefore replace the congruence
F (x) =0, mod p”, by the congruences P!==0, mod p”, Q’==0, mod p™,
R'=0, mod p”,... But no general investigation appears to have been given
of the peculiarities that may be presented by a congruence of the form
P! =0, mod p”, in the case in which P is a power of an irreducible function
(mod p), and not itself such a function—a supposition which implies that the
discriminant of F (x) is divisible by p. If, however, P be itself an irreduci-
ble function, the congruence P! =0, mod pm, gives us one and only one solu-
tion of the given congruence if P be linear, or, if P be not linear, it may be
considered as representing as many imaginary solutions as it has dimensions.
In particular, if we consider the case in which all the divisors P, Q, R,...
are linear, we obtain the theorem :—
«« Every congruence which considered with respect to the modulus p has
as many icongruous solutions as it has dimensions, is also completely reso-
luble for the modulus p”, having as many roots as it has dimensions, and no
more.”
If «=a,, mod p, be a solution of the congruence F (x) =0, mod p, and
if that congruence have no other root congruous to a,, the corresponding
solution z =a m, mod p”, of the congruence F (2) ==0, mod p”, may be ob-
tained by the solution of linear congruences only—a proposition which is in-
cluded in a preceding and more general observation. The process is as
follows :—If, in the equation
F (a, +Ap)=F(a,) + Ap (a,) +2 F(a.) +00
we determine # by the congruence oF (a,)+kF'(a,)=0, mod p, (which is
always possible because the hypothesis that (a—a,)* is not a divisor of
F (x), mod p, implies that F’(a,) is not divisible by p*), and then put a,==
a,+hp, mod p’*, we have F (a,)==0, mod p*. Similarly, from the expansion
F (a,+kp*)=F (a,) +hp? F' (a,)+..-;
a value of & may be deduced which satisfies the congruence F (a,+kp*) =0,
or F(a,)==0, mod p*; and so on continually until we arrive at a congruence
of the form F(am)=0, mod p™. But when F(z) is divisible (ior the
modulus p) by (a—a)’ or a higher power of a—a, the congruence F(«)=0,
mod p”, is either irresoluble or has a plurality of roots incongruous for the
modulus p”, but all congruous to a@ for tle modulus p. Thus the congruence
(«—a)’+kp(«x—b)=0, mod p’, is irresoluble, unless a==6, mod p; whereas
if that condition be satisfied, it admits of p incongruous solutions, comprised
in the formula z=a+pp, mod p’, p=0, 1, 2, 3,..p—1].
* If F (x) =(x—a,) $ (x), mod p, where ¢ (a,) is not divisible by py, we have F’ (x) =
» («)+(a—a,) ¢' (x), mod p, or F’ (a,) = ¢ (a), mod p.
ON THE THEORY OF NUMBERS. 167
73. Binomial Congruences having a Power of a Prime for their Modulus.—
If M be any number, and Y(M) represent the number of terms in a system
of residues prime to M, it will follow (from a principle to which we have
already frequently referred : see arts. 10, 26, 53, 70) that every residue of that
system satisfies the congruence a¥(™) ==], mod M,—a proposition which is
well known as Euler’s generalization of Fermat's theorem*. In particular,
when M=p”, we have x?”~'(p-1)==1, mod p™. This congruence has,
consequently, precisely as many roots as it has dimensions—a property which
is also possessed by every congruence of the form «¢=1, mod p™, d denoting
a divisor of p"—!(p—1). This has been established by Gauss in the 3rd
section of the Disquisitiones Arithmetice, by a particular and somewhat
tedious method+. The simpler and more general demonstration which he
intended to give in the 8th section}, was perhaps in principle identical with
the following ; we exclude the case p=2, to which indeed the theorem itself
is inapplicable :—
Let d=dp", 6 representing a divisor of p—1, and m being < m—1; and let
us form the indeterminate congruence
x'—] ==(x—a,) (w—a,)....(%—az), mod p™—”,
which is always possible, because #°—1 ==0, mod p, has 6 incongruous roots.
It is readily seen that, if A and B represent two numbers prime to p, and if
A==B, mod p’, A”*==B?", mod p*+s; and conversely, if A?°=B?*, mod prts,
A=B, mod p"§. By applying this principle it may be shown that
xp” —] = (xP"—a,P”) (xP”—a,p") .... (av"—azP"), mod p™.
For if we divide a»"—1 by 2?"—a,”, the remainder is a,”"—1. But,
because a,5== 1, mod p”—, a,6p” ==1, mod p”; i. e.a?”—a,P” divides v?"—]
for the modulus p”. Similarly «2'»”—1 is divisible (mod p™) by 2"—a,P"
ete. ; and since all these divisors are relatively prime for the modulus p, x5?" —1
is divisible (mod p”) by their product ; 7. e.,
at" —] == (aP"—a,?”) (aP”—a,p) ... (a? —a,?”), mod p™.
We have thus effected the resolution of «*»”—1 into factors relatively prime,
each of which is congruous (mod p) to a power of an irreducible function ;
since evidently (7?”—a?”") == («—a)?”", mod p. To investigate the solutions
of x’»"— 1 ==0, mod p”, we have therefore only to consider separately the
8 congruences included in the formula «?”==a?", mod pm. But each of
these congruences (by virtue of the principle already referred to) admits
precisely p” solutions, viz. the p” numbers (incongruous mod p”) which are
congruous toa, mod p”—”. The whole number of solutions of a'»”—1 =0,
mod p™, is therefore equal to the index dp” of the congruence. It further
appears that the complete solution of the binomial congruence a?”—1 =0,
may be obtained by a direct method, when the complete solution of the
simpler congruence «'—|1==0, mod p, has been found. For we may first
-* Euler, Comment. Arith. vol. i. p. 284.
t Disquisitiones Arithmeticz, arts. 84—88. See also Poinsot, Reflexions sur la Théorie
des Nombres, cap. iv. art. 6.
} Disquisitiones Arithmeticz, art. 84.
§ If A=B, mod pr, but not mod pr+1, we have A=B-+Apr, where & is prime to p-
Hence A?* =(B+kp")P°=BPs>47BP%—! ptr LK ere K denoting a coefficient divisible
by p; or AP°=B?*, mod p**”, but not mod p **”*", because £B?*—! is prime to p. This
result implies the principle enunciated in the text.
168 REPORT— 1860.
(by the method given in the last article) deduce the complete solution of
x'—1==0, mod p™~”, from that of «7—1==0, mod p; and then the roots of
zx'p” —]==0, mod p™, can be written down at once.
74. Primitive Roots of the Powers of a Prime.—All\ the elementary pro-
perties of the residues of powers, considered with regard to a modulus which
is a power of a prime number, may be deduced from the theorem just proved.
In particular, the demonstration of the existence and number of primitive
roots (art. 12) is applicable here also; so that we have the theorem :—
“There are p—2 (p—1) (p—1) residues prime to p”, the successive
powers of any one of which represent all residues prime to p™.” These
residues are of course the primitive roots of p”.
If y be a primitive root of p, of the p numbers included in the formula
y+hp (mod p’), p—1 precisely will be primitive roots of p*. For y+Ap
is a primitive root of p* unless (y+/p)P—! =1, mod p’; and the congruence
xzp—1==], mod p’, has always one, and only one, root congruous to y for the
modulus p. But every primitive root of p* is a primitive root of p*, and of
every higher power of p, as may be shown by an application of the princi-
ple proved in a note to the last article, or, again, by observing that every
primitive root of p”+! is necessarily congruous, for the modulus p™, to some
primitive root of p™, and that there are p times as many primitive roots of
p™t) as of pm. (See Jacobi’s Canon Arithmeticus, Introduction, p. xxxiii ;
also a problem proposed by Abel in Crelle’s Journal, vol. iii. p. 12, with
Jacobi’s answer, ibid. p. 211.)
75. Case when the Modulus is a Power of 2.—The powers of the even
prime 2 are excepted from the demonstrations of the two last articles—in
fact, if m > 3,2™ has no primitive roots. Gauss, however, has shown (Disq.
Arith. arts. 90, 91) that the successive powers of any number of the form
8n +3 represent, for the modulus 2”, all numbers of either of the forms 82+3
or 82+1; similarly all numbers of the forms 8%+5 and 8x+1 are repre-
sented by successive powers of any number of the form 8z+5. If, there-
fore, we denote by y any number of either of the two forms 82 +3 or 82+5,
we may represent all uneven numbers less than 2” by the formula (—1)*y8,
in which a is to receive the values O and 1, and f the values 1, 2,5,....g™-2,
A double system of indices may thus be used to replace the simple system
supplied by a primitive root when such roots exist.
Tables of indices for the powers of 2, and of uneven primes inferior to
1000, have been appended by Jacobi to his Canon Arithmeticus.
76. Composite Modules.—-No general theory has been given of the repre-
sentation of rational and integral functions of an indeterminate quantity as
products of modular functions with regard to a composite modulus divisible
by more than one prime. Aud it is possible that no advantage would be
gained by considering the theory of congruences with composite modules
from this general point of view. A few isolated theorems relating to par-
ticular cases have, however, been given by Cauchy (Comptes Rendus,
vol. xxv. p. 26, 1847). Of these the following may serve as a specimen :—
“If the congruence I («)==0, mod M, admit as many roots as it has
dimensions, and if, besides, the differences of these roots be all relatively
prime to M, we have the indeterminate congruence
F (v)=h (a—1,) (a@—r,) (w—r,) ...(e—r,,), mod M,
k denoting the coefficient of the highest power of # in F (w).”
But if, instead of considering the modular decomposition of the function
F (x), we confine ourselves to the determination of the real solutions of the
ON THE THEORY OF NUMBERS. 169
congruence F (2) =0, mod M, it is always sufficient to consider the con-
gruences
F(x)=0, mod A, F(«)=0, mod B, F(x)==0, mod C, ete., .... (A)
where AX BxC..=M, and A, B, C,.. denote powers of different primes.
For if «=a, mod A, «= 6, mod B, X =e, mod C, denote any solutions of
the first, second, third ... of those congruences respectively, it is evident that,
if X be a number satisfying the congruences X =a, mod A, X =), mod B,
X==c, mod C (and such a number can always be assigned), we shall have
F(X) =0 for each of the modules A, B, C,.. separately, and therefore for
the modulus M; and further, if the congruences (A) admit respectively
a, 2, y, +. incongruous solutions, the congruence F(«)==0, mod M, will
admit axfxXy...inall; for we can combine any solution of F(x)=0,
mod A, with any solution of F(«)=0, mod B, and so on*.
77. Binomial Congruences with Composite Modules —The investigation of
the real solutions of binomial congruences depends (in the manner just stated)
on the investigation of the real solutions of similar congruences the modules
of which are the powers of primes. With regard to the relations by which
these real solutions are connected with one another, little of importance has
been added to the few observations on this subject in the Disquisitiones
Arithmetice (art. 92). If the modulus M=p* g’ re... »P> 4 7, «+» repre-
senting different primes, the congruence «¥(™) = 1, mod M, possesses no
primitive roots; for if m be the least common multiple of p*—! (p—1),
q’— (q—1), r°-! (r—1),...., 2 will be less than and a divisor of J (M).
But evidently, if x be any residue prime to M, the congruence «»—] =O
will be satisfied separately for the modules p+, g°, r¢,.., and therefore for the
modulus M ; 7. e., no residue exists, the first ~(M) powers of which are incon-
gruous, mod M. If, however, M=2p* this conclusion does not hold, since
the least common multiple of ~ (2) and (p”) is W (2p™) itself; and we
find accordingly that every uneven primitive root of p™ is a primitive root of
2p™. When, as is sometimes the case, it is convenient to employ indices to
designate the residues prime to a given composite modulus, we must empley
(as in the case of a power of 2) a system of multiple indices. To take the
most general case, let M=2?° p g? r¢ ..; let wu be any number of either of the
forms 8x+3 or 8n+5, and P, Q, R,... primitive roots of Pe Covina VEX
spectively. Then, if x be any given number prime to M, it will always be
possible to find a set of integral numbers en, wn», &ns Sn, Yn ++ » Satisfying the
conditions
(—1)*" wen==n, mod 2°; O< , <2, 0 <n < 29%,
p*r =n, mod p*; o< an <p" (p—1),
Qa =n, mod g?; 0<Pn <q -'(q—1),
R”=n, mod r*; o= An < re! (r--1);
and these numbers form a system of indices by which the residue of m for
each of the modules 29, Ee en Noes os (and consequently for the modulus M)
* “Tnfra [i. e, in the 8th section] congruentias quascumque secundum modulum e pluribus
primis compositum, ad congruentias quarum modulus est primus aut primi potestas reducere
fusius docebimus’”’ (Disq. Arith. art. 92). It is difficult to see why Gauss should haye ae
ployed the word “ fusius” if his investigation extended no further than the elementary
observations referred to in the text. Nevertheless it is remarkable that Gauss in the 3rd
section of the Disq. Arith. sometimes speaks of demonstrations as obscure, which are of
extreme simplicity when compared with one in the 4th and several in the 5th section (see in
particular arts. 53, 55, 56).
170 REPORT—1860.
is completely determined. (See Dirichlet’s memoir on the Arithmetical Pro-
gression, sect. 7, in the Berlin Memoirs for 1837.)
78. Primitive Roots of the Powers of Complex Primes.—Dirichlet has
shown * that, in the theory of complex numbers of the form a+ 07, the powers
of primes of the second species (see art. 25) have primitive roots; in fact, if
a+bi be such a prime, and N (a+i)=a*+b°=p, every primitive root of
p™ is a primitive root of (a+4-b7)™. On the other hand, if g be a real prime
of the form 42+3, 9” has no primitive roots in the complex theory. For in
general, if M be any complex modulus, and M=a* lf cy ..., a, b, ce, .. being
different complex primes, and if A=N (a), B=N (6), C=N (e), ete. the
number of terms in a system of residues prime to M, is A*~' (A—1) B®"
(B—-1) C’"' (C—1).... And if we denote this number by w (M), every
residue prime to M will satisfy the congruence
av¥(M) = 1, mod M,
which here corresponds to Euler’s extension of Fermat's theorem. If M=g™,
2m—2, 2
this congruence becomes #7 (¢ —1)==1, mod g”; but it is easily shown
that every residue prime to g™ satisfies the congruence «¥”" “—1) =],
mod q”™; 7. e., g” has no primitive roots, because the exponent g”—! (q’—1)
is a divisor of, and less than, g2"—-1)(q’—1). Nevertheless two numbers y
and y', can always be assigned, of which one appertains to the exponent g™—!
(q’—1) and the other to the exponent g”—!, and which are such that no
power of either of them can become congruous to a power of the other,
mod g”, without becoming congruous to unity; from which it will appear
that every residue prime to g” may be represented by the formula y* y', if we
give to ~ all values from 0 to (q’—1) g™—! —1 inclusive, and to y all values
from 0 to g™—!—1 inclusive.
The corresponding investigations for other complex numbers besides those
of the form a+0i have not been given.
We here conclude our account of the Theory of Congruences. The
further continuation of this Report will be occupied with the Theories of
Quadratic and other Homogeneous Forms.
Additions to Part I.
Art. 16. Legendre’s investigation of the law of reciprocity (as presented in
the ‘ Théorie des Nombres,’ vol. i. p. 230, or in the ‘ Essai,’ ed. 2, p. 198) is
invalid only because it assumes, without a satisfactory proof, that if a be
a given prime of the form 42+1, a prime 0 of the form 4%+3 can always
be assigned, satisfying the equation ; =—1]. M. Kummer (in the Memoirs
of the Academy of Berlin for 1859, pp. 19, 20) says that this postulate is
easily deducible from the theorem demonstrated by Dirichlet, that every
arithmetical progression, the terms of which have no common divisor, con-
tains prime numbers. It would follow from this, that the demonstration of
Legendre (which depends on a very elegant criterion for the resolubility or
irresolubility of equations of the form aa*+dy’?+cz*=0) must be regarded
as rigorously exact (see, however, the “ Additamenta” to arts. 151, 296, 297
of the Disq. Arith.). In the introduction to the memoir to which we have
just referred, the reader will find some valuable observations by M. Kummer
on the principal investigations relating to laws of reciprocity.
* See sect. 20f the memoir, Untersuchungen iiber die Thecrie der complexen Zahlen, in
the Berlin Memoirs for 1841.
ON THE THEORY OF NUMBERS. 171
Art. 20. Dirichlet’s demonstration of the formule (A) and (A’) first
appeared in Crelle’s Journal, vol. xvii. p. 57. Some observations in this
paper on a supposed proof of the same formule by M. Libri (Crelle, vol. ix.
p- 187) were inserted by M. Liouville in his Journal, vol. iii. p. 3, and gave
rise to a controversy (in the Comptes Rendus, vol. x.) between MM. Liouville
and Libri. The concluding paragraphs of Dirichlet’s paper contain the appli-
cation of the formule (A) and (A’) to the law of reciprocity (Gauss’s fourth
demonstration ).
Art. 22. From a general theorem of M. Kummer’s (see arts. 43, 44 of this
—s
Report), it appears that the congruence r*==(—1) * ), mod q, is or is not
A-1
resoluble, according as q? =+ 1, or ==—1, mod A,—a result which implies
the theorem of quadratic reciprocity. This very simple demonstration (which
is, however, only a transformation of Gauss’s sixth) appears first to have
occurred to M. Liouville (see a note by M. Lebesgue in the Comptes Rendus,
vol. li. pp. 12, 13).
Art. 24. A note of Dirichlet’s, in Crelle, vol. lvii. p. 187, contains an ele-
mentary demonstration of Gauss’s criterion for the biquadratic character of
2. From the equation p=a’*+0’, we have (a+6)* =2ad, mod p, and hence
(a+6)eP-0) == 24(P—1) at(P—)) h4(P—1) = (Qf )4(P—) at(P—), or, which is the
same thing,
()=en'? (2), hairs Tle Ap (A)
But (2)=(&)=» because p==6’, mod a; and = (45 , or, ob-
p a
ye
serving that 29=(a+6)’+(a—b)’,
a+b 2 ta es) iy "
Sal few a eee — fi(p-l) +hab
( P )= =) ( ) 8 ja >
since f*+1==0, mod p. Substituting these values in the equation (A), we
find 23(p—1) = 24>, mod p, which is in fact Gauss’s criterion.
Art. 25. In the second definition of a primary number, for “6 is uneven,”
read “6 is even.” Although this definition has been adopted by Dirichlet in
his memoir in Crelle’s Journal, vol. xxiv. (see p. 301), yet, in the memoir
“Untersuchungen tiber die complexen Zahlen” (see the Berlin Memoirs for
1841), sect. 1, he has preferred to follow Gauss.
Art. 36. In the algorithm given in the text, the remainders p,, p,... are all
uneven ; and the computation of the value of the symbol Po) is thus rendered
4
independent of the formula (iii) of art. 28. The algorithm given by Eisen-
stein is, however, preferable, although the rule to which it leads cannot be
expressed with the same conciseness, because the continued fraction equi-
valent to 2° terminates more rapidly when the remainders are the least
ia
possible, and not necessarily uneven.
Art. 37. In the definition of a primary number, for “@==+1,” read
“a=—1.” But, for the purposes of the theory of cubic residues, it is
simpler to consider the two numbers +(a+4p) as both alike primary (see
arts. 52 and 57).
Art. 38. Jacobi’s two theorems cannot properly be said to involve the
172 REPORT—1860.
cubic law of reciprocity. If (2 =1, it will follow from those theorems that
of 3
o a | (2) = or p*, they do not determine whether (2: =p,
3 2 1/3
or ps It is remarkable that these theorems, “forma genuina qua inventa
sunt,” may be obtained by applying the criteria for the resolubility or irreso-
lubility of cubic congruences (art.67) to the congruence r°—3Ar—\AM =0,
mod g (art. 43), which, by virtue of M. Kummer’s theorem (art. 44), is re-
soluble or irresoluble according as g is or is not a cubic residue of i.
On the Performance of Steam-Vessels, the Functions of the Screw, and
the Relations of its Diameter and Pitch to the Form of the Vessel.
By Vice-Admiral Moorsom.
(A communication ordered to be printed among the Reports.)
In this the fourth paper which I now lay before the British Association, it
may be desirable to recapitulate the points I have brought into issue, and for
the determination of which, data, only to be obtained by experiments, are
still wanting, viz.—
1. There is no agreed method by which the resistance of a ship may be
calculated under given conditions of wind and sea.
2. The known methods are empirical, approximate only, and imply smooth
water and no wind.
3. The relations in which power and speed stand to form and to size are
comparatively unknown.
4, The relations in which the direct and resultant thrust stand to each
other in any given screw, and how affected by the resistance of the ship, are
undetermined.
In order to resolve these questions, specific experiments are needed, and
none have yet been attempted in such manner as to lead to any satisfactory
result.
The Steam Ship Performance Committee of the British Association have
pressed upon successive First Lords of the Admiralty, the great value to the
public service which must ensue if the following measures were taken, viz.—
1. To determine, by specific experiment, the resistance, under given con-
ditions, of certain vessels, as types; and, at the same time, to measure the
thrust of the screw.
2. To record the trials of the Queen’s ships, so that the performance in
smooth water may be compared with the performance at sea, both being re-
corded in a tabular form, comprising particulars, to indicate the characteris-
tics of the vessel, of the engine, of the screw, and of the boiler.
Hitherto nothing has come of these representations.
In the paper read last year at Aberdeen, I showed, in the case of Lord
Dufferin’s yacht ‘Erminia,’ how the absence of admitted laws of resistance
interfered with the adjustment of her screw, and how, therefore, as a matter
of precaution, a screw was provided capable of a thrust beyond what the
vessel required.
1 also showed, in the case of the Duke of Sutherland’s yacht ‘ Undine,’ how
her screw, from being too near the surface of the water, lost a large portion
of the ¢hrust due to its size and proportions. In other words, a screw capa-
ble of giving out a resultant thrust in sea water of 5022 lbs., at a speed of
ON THE PERFORMANCE OF STEAM-VESSELS. 173
vessel of 9:26 knots an hour, did actually give out only 3805 lbs. ‘That is to
say, the effect produced was the same as if that screw had worked in a
fluid whose weight was about 48 Ibs. per cubic foot instead of 64 lbs.
Tam now about to exhibit some other examples from among Her Majesty’s
ships of war.
The questions now before us are—
1. The resistance of the hull below the water-line in passing through the
water, and of the upper works, masts, rigging, &c., passing through the air,
the weather being calm, and the water smooth.
2. The relation in which the thrust of the screw stands to this resistance.
[The Admiral here gave certain results from the ‘ Marlborough,’ the ‘ Re-
nown, and the ‘Diadem,’ and proposed that a specific issue should be tried
by means of the ‘ Diadem.’]
What would I not give, he observed, for some well-conducted experiments
to determine this beautiful problem of the laws which govern the action of
the screw in sea-water! It is a problem not only interesting to science, but
fraught with valuable results in the economical and efficient application of
the screw propeller.
After commenting on the performances of the U. S. corvette ‘ Niagara,’ the
Admiral observed, I have no means of forming a very definite opinion as to
how she will séay under low sail in a sea-way, how she will wear, how scud
in a following sea, or how stand up under her sails, or whether her statical
stability be too much or too little, or how the fore and after bodies are
balanced. These are points to be determined, not by the mere opinion of
seamen—-for a sailor will vaunt the qualities of his ship even as a lover the
charms of his mistress—but by careful records of performances in smooth
water and at sea, and a comparison of such performances with calculated
results from drawings beforehand. Let a return of such things be annually
laid before the House of Commons—we shall then know whether we are get-
ting money’s worth for our money; and also we should receive all the benefits
of public criticism towards improvement. We should not then allow defects
to be stereotyped, till chronic blemishes are turned into beauties, or, if not
so, then defended as things that cannot be remedied.
I have now completed the task which four years ago I imposed on myself.
Beginning with simple elementary principles, and ending with minute prac-
tical details, I have, as I conceive, shown the process by which the improve-
ment of steam-ships must be carried on.
More than one hundred years ago scientific men, able mathematicians,
showed the physical laws on which naval architecture must rest. A succes-
sion of able men have shown how those laws affect various forms of floating
bodies. Experiments have been made with models to determine the value
of the resistance practically. With the exception of some experiments of
Mr. Scott Russell, I am not aware that any have been made with vessels ap-
proaching the size of ships to determine the relations of resistance to power,
whether wind or steam.
Ships have been improved, and modifications of form have been arrived at
by along painstaking tentative process. The rules so reached for sailing ships
have been superseded by steam, and we are still following the same tedious
process, in order to establish new rules for the application of steam power.
I think the history of naval architecture shows that it is not an abstract
science, and that its progress must depend on the close observation and cor-
rect record of facts; on the careful collating, and scientific comparing of such
facts, with a view to the induction of general laws. Now, is there any where
such observing, recording, collating, and comparing? and still more, is there
such inducting process ?
174 REPORT—1860.
I can find no such thing anywhere in such shape that the public can judge
it by its fruits.
We are now in full career of a competition of expenditure, and England
has no reason to flinch from such an encounter, unless her people should tire
of paying a premium of insurance upon a contingent event that never may
happen ; and if it should happen without our being insured, might not cost
as much as the aggregate premiums. ‘Tire they will, sooner or later, but
they are more likely to continue to pay in faith and hope, if they had some
confidence that their money is not being spent unnecessarily.
There is now building at Blackwall the ‘ Warrior,’ a ship to be cased with
44-inch plates of iron, whose length at water-line is 380 feet, breadth 58 feet,
intended draught of water (mean) 255 feet, area of section 1190 square feet,
and displacement about 8992 tons, and she is to have engines of 1250 nomi-
nal horse-power.
Is there any experience respecting the qualities and performance of such
a ship? Anything to guide us in reasoning from the known to the unknown ?
Do the performances of the ‘ Diadem,’ ‘Mersey,’ and ‘Orlando,’ inspire
confidence? Where are the preliminary experiments ?
Before any contract was entered into for the construction of the Britannia
Bridge, a course of experiments was ordered by the Directors, which cost not
far short of £7000, and it was well expended. It saved money, and perhaps
prevented failure. This ship must cost not less than £400,000, and may cost
a good deal more when ready for sea. But there is another of similar, and two
others building, of smaller size. What security is there for their success ?
The conditions which such a ship as the ‘ Warrior’ must fulfil in order to
justify her cost are deserving of some examination. The formidable nature
of her armament, as well as her supposed impregnability to shot, will natu-
rally lead other vessels to avoid an encounter. She must therefore be of
greater speed than other ships of war. To secure this, it is essential that
her draught of water should be the smallest that is compatible both with
stability and steadiness of motion, and that she should not be deeper than the
designer intended. ‘To ensure steadiness it is necessary, among other things,
that in rolling, the solids, emerged and immersed, should find their axis in
the longitudinal axis of the ship. To admit of accurate aim with the guns,
her movement in rolling should be slow and not deep. Every seaman knows
how few ships unite these requisites.
It is not quite safe to speculate on the ‘ Warrior's’ speed; nevertheless I
will venture on an estimate, such as I have stated in the case of the ‘ Great
Eastern,’ whose smooth-water speed I will now assume to be 152 knots, as
before estimated, with 7732 horse-power, when her draught of water is 23
feet, her area of section, say 1650 square feet, and her displacement about
18,588 tons. The speed of the ‘ Warrior’ in smooth water ought not to be
less than 16 knots, in order that she may force to action unwilling enemies
whose speed inay be 13 to 14 knots.
The question I propose is the power to secure a smooth-water speed of
16 knots.
Reducing the ‘ Great Eastern’ to the size of the ‘ Warrior,’ and applying
the corrections for the difference of speed of 3 knot, and for their respective
coefficients cf specific resistance °0564 and ‘07277, the horse-power for 16
knots is 7543.
Raising the ‘ Niagara’ to the size of the ‘ Warrior,’ and applying the cor-
rections for the difference of speed between 10°9 and 16 knots, and for their
respective coefficients of specific resistance ‘0797 and ‘07277, the horse-power
to give the ‘ Warrior’ a smooth-water speed of 16 knots is 7867, being an
excess over the estimate from the ‘Great Eastern’ of 324 horse-power.
ON THE EFFECTS OF LONG-CONTINUED HEAT. 175
If the power required for the ‘ Warrior’ be calculated by adaptation from
the ‘ Mersey’ and the ‘ Diadem,’ it would be 8380 horse-power and 8287 re-
spectively ; from which this inference flows :—that unless the mistakes made
in the fore and after sections of the ‘Mersey’ and ‘Diadem’ are rectified in the
‘Warrior,’ she will require above 8000 horse-power for a speed of 16 knots,
notwithstanding her greater size and increased ratio of length to breadth.
Before investing more than a million and a half of money in an experiment,
commercial men would have probably employed a few thousand pounds in
some sort of test as to the conditions of success. Perhaps such test may have
been resorted to and kept secret for reasons of public policy. Perhaps it is
intended that the ‘ Warrior's’ speed should not be greater than that which is
due to five times her nominal horse-power, which could not exceed 152 knots
with 6250 horse-power, under the most favourable conditions, and may be
much less.
The British Association, by becoming the medium of collecting facts and
presenting them to the public, has done good service; but that service ought
not to rest there. Collectively, the Association may be able to do little more.
It can only act by affording public opinion a means of expression. But indi-
vidual members may do much. Towards such opinion I am doing my part.
I ask, in the cause of science, what is the system under which the Queen’s
ships are designed and their steam power apportioned ; the organization by
which their construction and fitting for sea are carried on; the supervision
exercised over their proceedings at sea, in the examination of returns of per-
formance and of expenditure ?
During part of 1858 and 1859, two committees appointed by the Admi-
ralty collected evidence and made reports on the Dock Yards and on steam
machinery. I have read both reports with some attention. They are not
conclusive, but they are entitled to respect. I have also read the replies and
objections of the Government officers. There is a clear issue between them
on some of the most essential principles of effective economical management,
and on the application of science.
A Royal Commission has been appointed to inquire into the system of
control and management in the Dock Yards. This is so far good, but it
does not go far enough. It does not comprise the steam machinery reported
on by Admiral Ramsay’s Committee, and it cannot enter upon the questions
Ihave just enumerated. Yet the efficiency of the fleet depends quite as
much upon the adaptation of the machinery to the ship, and of the ship to
the use she is to be put to, as it does upon the manner in which she is built.
The Commission ought to be enlarged both in objects and in number of
members. It consists of five members only.
Report on the Effects of long-continued Heat, illustrative of Geological
Phenomena. By the Rev. W. Vernon Harcourt, F.B.S., F.G.S.
Tue chief occupation of those who during the present century have
employed themselves in investigating the history of the earth, has been to
develope the succession of its strata. In following this pursuit, they have
found their best guide in the study of its organic antiquities, and have not
been led, for the most part, to very precise views of the physical and chemi-
cal changes which it has undergone.
Yet there are questions in Geology to which no answer can be given with-
out an accurate examination into these. In regard, for example, to the
176 REPORT—1860.
chronology of the earth, the observation of organic remains alone can never
supply reliable data for reasoning. If we should attempt to draw inferences
from biological analogies, and measure the duration of beds by the growth of
imbedded skeletons, we should be stopped by the probability that the first
species of every series were successively created in a state of full-grown
maturity*, and by the intrinsic weakness of all comparisons instituted non
part materia.
Neither can any precarious mechanical analogies render the inquiry more
definite, or give a logical value to our conclusions. We are not entitled
to presume that the forces which have operated on the earth’s crust have
always been the same. Were we to compare the beds of modern seas and
lakes with the ancient strata, and assume proportionable periods for their
accumulation, we must assume also that chemical and mechanical forces
were never in a state of higher intensity, that water was never more rapidly
evaporated, that greater torrents, fluid or gaseous, never flushed the lakes and
seas, and that more frequent elevations and depressions never gave scope for
quicker successions of animal life. To gain any real insight into these ob-
scure pages of ancient history, we must have recourse to a strict induction
of physical and chemical facts, and thence learn the probable course, and
causes, of the wonderful series of changes which geology unfolds.
I am not aware that any full and connected statement has been published
of the facts which have been contributed by physical observations, and
chemical experiment, towards elucidating the conditions of those changes,
and propose therefore to preface the account which I have to give of experi-
ments designed to throw light upon them, with a sketch of the progress of
science in that department.
Forty years have elapsed since the author of the ‘Mécanique Céleste’
drew attention to the fact that multiplied observations in deep mines, wells,
and springs, had proved the existence of a temperature in the interior of the
earth increasing with the depth. He remarked that, by comparing exact
observations of the increase with the theory of heat, the epoch might be
determined at which the gradually cooling globe had been first transported
into space ; he stated the mean increase, collected from actual data, to be a
centesimal degree for every 32+ metres, and added that this is an element
of high importance to geology. ‘ Not only,” he said, ‘‘does it indicate a very
great heat at the earth’s surface in remote times, but if we compare it with
the theory of heat, we see that at the present moment the temperature of
the earth is excessive at the depth of a million of metres, and above all at
the centre; so that all that part of the globe is probably in a state of fusion,
and would be reduced into vapour, but for the superincumbent beds, the
* To suppose otherwise with regard to animals which take care of their young would be
absurd; and hence it is probable also that this is the general system of creation. The most
remarkable fact which modern geology has disclosed is the continual succession of newly-
created species. It has been attempted to account for thes2 according to known laws of pro-
geniture, by supposing numerous non-apparent links of transitional existence to fill up the
gaps in the chain of derivation by which one species is presumed to have descended from
another. But this is only twisting a rope of sand; conjectural interpolations cannot give
coherence to a set of chains which are destitute of all evidence of continuity one with
another, and between which, as far as our experience goes, Nature has interposed a prin-
ciple of disconnexion.
In using the word creation, we acknowledge an agenf, and own our ignorance of the
agency, with regard to which, in this case, we only know that it is systematic ; for we see
successive species accommodated to successive conditions of existence.
+ M. Babinet (Tremblements de Terre, 1856), taking M. Waiferdin’s measurement from
artesian borings, which gave 31 metres for ]° C. as the most exact, remarks, that the tem-
perature at the depth of 3 kilometres must be above the heat of boiling water, and at that
of 60 kilometres, about 2000° C., sufficing for the fusion of lava, basalt, trachyte, and
porphyry.
ON THE EFFECTS OF LONG-CONTINUED HEAT. 177
pressure of which, at those great depths, is immense.” ‘ These considera-
tions,” he further added, “ will explain a great number of geological phe-
nomena ;” and he instanced those of hot springs, which he accounted for on
the supposition that rain-water in channels communicating from super-
ficial reservoirs with the interior of the earth, thence rises again, heated,
to the surface.
Fourier, at the same time, expounded the methods by which, after extended
observation of the internal temperature, and further experiments on the
conduction of heat, he conceived that mathematic analysis might determine
the epoch at which the process of cooling began, concluding in the mean-
while from facts already known,—Ist, that no sensible diminution of tem-
perature has taken place during the period of historical chronology ; 2ndly,
that at a former era the temperature underwent great and rapid changes.
Thus was a train of graduated causes, physical and chemical, introduced
into Geology on the foundation of inductive reasoning, which is capable of
resolving some of the chief difficulties of the science in our comparison of
the present with the past.
When, for instance, we read in the organic contents of the strata the
history of a period when the climate was apparently uniform in all parts of
the earth, and learn from the imbedded plants that the temperature of Arctic
lands was once equal to that of warm latitudes at the present day, to account
for these circumstances, we need no longer bewilder ourselves with hypo-
theses ; we have a vera causa in the knowledge that the earth has passed
through a state in which its temperature was due, not so much to a sun then
veiled in clouds, as to a heat penetrating equally in all directions from the
centre to the circumference of the globe.
When, again, we contemplate a mountain range, and view the abrupt pre-
cipices of some alpine chain, with its enormous masses of rock uplifted to
- the clouds, and descending as many miles into the bosom of the sea, and
when we compare such abnormal labours of nature with the petty risings
of the earth’s surface in the existing state of things, we have a vera causa
for that disparity, in the knowledge that there was a time when the eruptive
forces of the seething mass within were greater, and when a weaker crust
underwent vaster disturbances.
Or if we examine the general structure of the strata, and see the same stra-
tum contemporancously solidified over large portions of the earth’s circum-
ference, and then observe the absence of consolidation in the actual opera-
tions of nature, whether under the pressure of deep seas, or elsewhere,
except in a few foci of igneous action, we have here also a vera causa
of the difference, in the ancient prevalence of that high temperature which
the laboratory of nature and art shows to be the most capable of lapidifying
stony materials.
Descending into the details of mineralogy, we find the same departure
from the present order of nature in the constitution of minerals; and in the
sequence of chemical effects of heat increasing with the age of the stratum,
we see a real cause for the distinction.
Thus, for example, to begin with the upper beds; the chemist knows that
solutions of carbonate of lime, at the ordinary temperature, deposit crystals
with the common form of calcareous spar, but near the boiling-point of
water with that of drragonite. Now in the mineralogical collection of the
Yorkshire Philosophical Society is a specimen of this mineral investing
calcite, from the chalk cliffs of Beachy Head ; and if any one will examine the
caves of calcareous grit on the Yorkshire coast, he will find them in some
aie like those of volcanic rocks, or the mouths of hot springs, with
. N
178 REPORT—1860.
Arragonite*. Here then we have proof of a certain modicum of heat existing
in boiling-springs now extinct, which once pervaded these strata; for had the
heat of the water which left this deposit been much more, or less, than about
212° F., no such crystals could have been formed. Not far from the same
locality, in a thin seam of the cornbrash Oolite, I have found nodules en-
closing small Crustacea, the interior of which was filled with crystalline
blende. No other trace of zinc is to be seen in the country aroundt. The
same singular phenomenon may be observed in the neighbouring Lias-shale,
where the chambers of the Ammonites frequently contain blendet. This is
not a phenomenon peculiar to the district ; it illustrates the general con-
dition of the-earth after these shells were deposited, and is best accounted
for by the vera causa of an elevated temperature ; it indicates that the fumes
of zine, or one of its volatile combinations, must have penetrated the strata,
taking the form of blende in the chambers of the Ammonite, and having
been sealed up in these, escaped decomposition.
The same account is applicable to the dissemination of carbonate and sul-
phide of lead and copper in the Permian and Triassic strata, and of the
particles of metallic copper in the mountain limestone ; as well as to the de-
posits of calamine in the hollows of that rock, on the conditions of which de-
posits light is thrown by an experiment of Delanoue, who found that no pre-
cipitate of carbonate of zinc is produced by limestone at the common tempera-
ture, but that it is perfectly thrown down from a warm solution of its salts.
And here also it is worthy of remark, that in the experiments of Forch-
hammer to illustrate the formation of dolomitic strata, when a solution of
carbonate of lime was mixed with sea-water at a boiling heat, the compound
formed contained only 18 per cent. of carbonate of magnesia, but that the
proportion of magnesia increased with an increase of temperature; in the
experiments of Favre and Marignac, the composition of equal atoms, which
is that of many natural beds of magnesian limestone, was attained by raising
the heat to 392° F., and the pressure to 15 atmospheres; and in those of
Morlot a mixture of sulphate of magnesia and calcareous spar was com-
pletely converted, in the same circumstances, into a double salt of carbonate
of lime and magnesia, with sulphate of lime.
The probable history of all the caleareous and magnesian strata, with
their interstratified cherts and flints, and interspersed chalcedonie fossils, is
that they are products of submarine so/fataras, whence issued successively,
in basins variously extended, gases and springs capable of dissolving pre-
existent beds, which caused alternate depositions .of silica and carbonated
earths, and intermitting from time to time, allowed intervals for the succession
of organic and animated beings.
The manner in which materials are furnished for extensive sedimentary
deposits by processes of disintegration dependent on subterraneous ema-
nations, has been observed by Bunsen in the solfataras of Iceland. He
describes the palagonitic rocks, formerly erupted there, as undergoing con-
* Dr. Murray informs me that this Arragonite is found in a little bay within six miles of
Scarborough, in the seams and crevices of the upper calcareous grit. He describes it as
fibrous, compact, or imperfectly mammillated, wanting the oblique cleayage of calcite,
scratching Iceland spar, and flying into powder in the flame of a taper. Mr. Procter having
at my request taken the specific gravity of a fibrous specimen, finds it 3, and confirms Dr.
Murray’s description of the other characters of this mineral.
+ The only peculiarity is that a basaltic dike traverses the district at a distance of a few
miles from the site of the fossils.
t The Lias fossils sometimes also contain galena. Blum describes a bivalve from a fer-
ruginous oolitic rock near Semur, the shells of which consist entirely of crystalline lamin
of specular iron; and a cardinia from the lower lias, according to Bischof, likewise consists
of the same mineral, which we know elsewhere as a result of volcanic action.
Le
ON THE EFFECTS OF LONG-CONTINUED HEAT. 179
version by these means “ into alternate and irregularly penetrating beds of
white ferruginous, and coloured ferruginous, fumerole clay, the deposits
being disclosed to a considerable depth, and exhibiting in the clearest man-
ner the phenomena of alternating colours.” ‘‘ One is astonished,” he re-
marks, “ at observing the great similarity between the external phenomena
of these metamorphic deposits of clay still in the act of being formed, and
certain structures of the Keuwper formation. Thousands of years hence the
geologist who explores these regions when the last traces of the now active
fumeroles have vanished, and the clay formations have become consolidated
into marl-like rocks by the silica with which they are saturated, may suppose,
from the differently stratified petrographic and chemical character of these
beds, that he is looking at fletz strata formed by deposition from water.”
*« At the surface, especially, where the deposition is favoured by slow eva-
poration, innumerable crystals of gypsum, often an inch in diameter, may
frequently be observed loosely surrounded by an argillaceous mass. At the
mountain ledge of the Namarféyall, and at Krisuvik, this gypsum is found
to penetrate the argillaceous masses in connected strata and floor-like depo-
sits, which not unfrequently project as small rocks where the lower soil has
been carried away by the action of the water. These deposits are sometimes
sparry, corresponding in their exterior very perfectly with the strata of gyp-
sum so frequently met with in the marl and clay formations of the Tras.”
The great disturbances and fractures, the trappean rocks, and the frag-
ments of porphyritic conglomerates, at. the bases of these formations, tend to
confirm the opinion of Bunsen, that they have had a metamorphic origin, an
origin very probably common to other beds, whether consisting of marl, shale,
or sand. All the sand-beds now forming are due to the disintegration and
detritus of ancient sandstones, a process, which continued through a great
lapse of time, has but coated some portions of the sea-side with unconsoli-
dated sand. In the soundings of the Atlantic depths, the microscope, according
to Maury, has failed to detect a single particle of sand or gravel. For the
origin and consolidation of the inferior grits and shales we must look to ac-
tions, mechanical and chemical, more potent than those which the present
tranquil course of nature presents. In examining the carboniferous sand-
stones of the Blue Mountains in New South Wales, with their shales and coal-
beds, more than 12,000 feet in thickness, Darwin was ‘“‘surprised at obser-
ving, that though they were evidently of mechanical origin, all the grains of
quartz in some specimens were so perfectly crystallized that they evidently
had not in their present form been aggregated in a preceding rock;” and
he quotes Wm. Smith as having long since made the same remark on the
millstone grit of England. If any one, in fact, will observe with a lens the
surfaces of the quartz pebbles included in that grit, he will find on most of
them numerous wnabraded facets, which bear evidence of a quartz-crystalline
action having pervaded the rock whilst its consolidation was going on.
There can be no better proof of widely-spread chemical action due to
heat than the frequent presence of crystallized silica in every part of the
stratified rocks.
The deeper we descend in the strata, the more plentiful are the veins and
beds of guartz, and the more manifest the signs of metamorphic action.
Von Buch was the first to explain, on the principle of metamorphism,
the change of calcareous rocks, in contact with pyroxenic porphyries, into
dolomites ; and in 1835 the same principle was extended by Fournet to
the metallization of rocks by contact with quartziferous porphyries, and to
their felspathication and silicification by the contact of granite. “Since
the theory of a central fire,” he observed, “has been confirmed by modern
researches, all the great questions in the history of the globe appear suscep-
N2
180 REPORT—1860.
tible of a simple solution, and it is astonishing that chemists have not yet
carried their views in this direction. From the moment that we consider the
terrestrial globe as a mass of which the different parts have successively
undergone the action of fire, we must also conceive, as a necessary conse-
quence, a series of chemical phenomena, such as calcination, fusion, cemen-
tation, &c.,” meaning by this latter term, the mutual molecular inter-
penetration of bodies in contiguity, a process of which I shall presently have
to offer a remarkable example.
There was one mineralogical chemist, however, of high eminence, who had
long before carried his views in the direction desired by Fournet. In 1823,
Mitscherlich, having examined the forms, and analysed the ingredients, of
forty crystalline products of furnaces *, to which Berthier had contributed
several parallel results of experimental processes, pronounced them identical
with various native minerals, and in particular with peridot, pyroxene, and
mica. In the artificial mica, however, he found Lime, of which granitic
mica scarcely contains a trace; and this led him to speculate on the cause
of the chief chemical distinction between the granite and trap formations,
consisting in the absence of calcareous and magnesian silicates from the
former. Supposing, he argued, that the primary rocks were formed at that
stage of the earth’s refrigeration when 4ths of its water were in a state of
vapour, the pressure on every part of its surface, computed according to
Laplace’s calculation of the mean depth of the sea, would be 225 atmo-
spheres + ; but under such a weight the affinity of lime for silica would cease ;
hence the crystals of uncombined silica in Carrara marble.
The surmise has since been brought into evidence by an experiment of
Petzholdt, in which pulverized quartz, heated to whiteness with an equal
weight of carbonate of lime in an open vessel, was found to form a silicate
with the lime, but produced no combination when heated in a strong, close
vessel of iron.
The crystallization of the primary rocks was supposed by the early Plutonic
theorists to be due to slow cooling ; but this principle alone does not satisfy
the phenomena. The crystalline structure of granite is seen, for example in
Glen Tilt, at Shap Fell}, and elsewhere, to be equally uniform in its partial
irruptions into the superior strata, as where it appears to be the foundation
stone of the earth's crust; it has crystallized in its accustomed manner, where
it has penetrated fissures of the upper beds in plates as thin as the leaves of
a book and threads as fine as a hair, and even where it is involved in the in-
vaded stratum so that no junction with any vein can be observed. How
could it have been thus injected in a state of fusion, unless of the most liquid
kind? and how could the heat of such liquidity, in a material of which the
fusing-point is so high, be otherwise than rapidly cooled down?
Furthermore, the quartz which forms su large a constituent of granite,
has always the specific gravity of crystalline silica, which exceeds that of any
other species of silica. But Deville and others have shown that fusion
* Annales de Chimie, tom. xxiv. p. 258, 1824. Mitscherlich sur la production artificielle
des minéraux crystallisés—“j’ai trouvé, 4 Fahlun, du silicate et bisilicate de protoxide de
fer, 2 Garpenberg, du mica et du pyroxene, les mémes figures crystallines, et tous les autres
caractéres des minéraux correspondans, le bisilicate de protoxide de fer et de chaux, de
magnésie et de chaux, les trisilicates de chaux, de chanx et de manganése, le fer oxidé (fer-
rosoferricum), le protoxide de cuivre, le deutoxide de cuivre, ]’oxide de zinc, les sulfures
de fer, de zine, de plomb, l’arsénieure de nickel, &c. &c., et beaucoup d’autres substances
en cristaux bien prononcées.
t In Mitscherlich’s Mémoire, as printed in the ‘Annales de Chimie et de Physique,’
tome xxiv. pp. 372, 373, the atmospheres are stated as 2250, deduced from a mean depth of
sea, 96,000 feet, with a cipher too much, that is, in both cases.
¢ I understand from Mr. Marshall that the ramified granite of Shap Fell is similarly
crystallized with the rest of the rock, but finer grained.
ON THE EFFECTS OF LONG-CONTINUED HEAT. 181
lowers this specific gravity to a constant amount, and that fused silica does
not recover its density in cooling. Crystalline granite, as Delesse has shown,
passes by fusion from the density of 2°62 to that of 2°32, and Egyptian
porphyry from 2°76 to 2°48. .
Again, the felspar in granite is encrusted by the quartz, the most fusible
by the least fusible material, contrary to all experience of crystallization
either from solution or fusion.
Lastly, all the minerals of which granite is composed have been artificially
produced, and their production has in every instance taken place at tempera-
tures far below that of the fusing-point of that rock. ‘The first specimens
of artificial felspar analysed by Karsten, and measured by Mitscherlich,
were found in the lining of a copper furnace amongst a sublimate of zinc.
Mitscherlich tried to obtain the like by fusing several pounds of native felspar
in a porcelain furnace, and subjecting the mass to a process of slow cooling,
but without success*. In the Mulden sinelting works, Cotta observed the
walls of the furnace traversed, in the joints of its masonry, and in the cracks
which it had undergone, by beautiful metallic veins, the sides exhibiting the
_phenomena of impregnation and alteration as in the boundary walls of
natural veins, and the ores consisting of galena, blende, iron and copper
pyrites, purple copper, Fahl ore, native copper, &c. In like manner pyro-
morphite (Pb’ P+4+4 Pb Cl), in well-formed six-sided prisms from the iron
furnace at Asbach, was found attached to the stones of the masonry. There
can be no doubt but that Karsten’s crystals of felspar, like these, were
formed by gaseous sublimation; and an analogous process would account
for the felspar observed by Haidinger in a basaltic cavity, under the form
of Laumonite, and by Bischof in a porphyritic bed, in which a Trilobite
also was found.
A new view of the production of minerals has been opened by Ebelmen,
who obtained the most refractory crystals of the granitic rocks, such as
spinel, emerald, cymophane, and corundum, by segregation in the interior
of a fused mass. They were formed at a heat far below that which would
fuse either those crystals or granite, by means of the evaporation of a fusible
and volatile medium. Gaudin also, on the same principle using a similar
alkaline solvent, and substituting sulphuric for boracic and carbonic acids
as the volatile ingredient, obtained the ruby.
To the same category may be referred an experiment by Precht, who
having added to a transparently fused frit, weighing 14 ewt., a considerable
quantity of felspar, found, after cooling, that a large portion of this mineral
had separated itself in foliated masses, and in several distinct crystals.
The most important light, however, on this subject, especially in relation to
metamorphic phenomena, is from the experiments cf Daubrée on the reaction
of gaseous compounds upon various earthy bases. Conveying the chlorides
of tin and titanium over lime at heats varying from 572° to 1652° Fahr.,
he produced crystals of tinstone and brookite; by variations of the same
principle, at heats not exceeding redness, he obtained all the following mine-
rals :—wollastonite, staurolite, peridote, disthene, willemite, idocrase, garnet,
phenakite, emerald, euclase, corundum, zircon, periclase, spinel, augite, di-
opside, gahnite, franklinite, hematite, felspar, and tourmaline in hexagonal
prisms imbedded within crystals of guartz. The process was of this descrip-
tion :—Chloride of aluminium, passed over lime at a red heat, produced
corundum; chloride of siliciwm, passed in like manner over seven equiva-
Jents of potash or soda and one of alumina, produced the different species
of felspar : the latter named gas, decomposed by lime at the same heat, or
* Mr. Marshall fused a large mass of granite, and cooling it slowly obtained no crystals.
182 REPORT—1860.
by magnesia, alumina, or glucina, gave erystallized quartz in the usual form
of the pyramidal hexagon, passing below into a silicate of the associated
bases. ‘“ The most remarkable part,” as Daubrée has remarked, “ connected
with these reactions, in a chemical, and especially a geological point of view,
is that the silicium and the silicates thus produced have an extreme tendency
to crystallize, and that the crystallization takes place at a temperature far
below their points of fusion.” “* The manner,” he adds, “in which quartz and
the silicates are connected with the granite rocks has long been a difficulty
in all the hypotheses on the formation of the rocks called primitive. Now
we find, in our experiments, that guartz crystallizes at the same time with,
or even later than, the silicates at a temperature scarcely exceeding a cherry-
red heat, and consequently infinitely below its point of fusion.”
M. Daubrée disclaims the supposition that those rocks themselves were
formed after the formula of his experiments. Nevertheless, considering
the probability that formations at higher temperatures, now obliterated, may
have preceded that of the granitic rocks, observing the uniform erystalliza-
tion of granite in the tenuity of its ramifications, as well as in mass, and
perceiving that Daubrée by his process has reproduced almost all the granitic
minerals, and among them not only the felspar, but the crystalline quartz
of granite,—it must be admitted that such a theory is worth attention.
Durocher has added to Daubrée’s researches two capital experiments, of
direct geological application, in obtaining the sulphides of the mineral veins
by the reaction of sulphuretted hydrogen on the chlorides of the metals in a
state of vapour, and in having effected the metamorphism of limestone into
dolomite in an atmosphere of the vapour of chloride of magnesium.
A theory of sublimation, however, may admit of many modifications,
and may be combined with the principle of segregation illustrated in the
experiments of Ebelmen. Deville and Caron, having fused bone phosphate
at a red heat in excess of chloride and fluoride of calcium, found that lime
apatite crystallized out in cooling, and was easily separated by washing from
the soluble salts. In like manner, with different bases and different chlorides,
they obtained the numerous varieties of apatite and wagnerite. And they
observed further, that all these minerals became volatile at a slightly elevated
temperature in the vapour of the chloride amidst which they were formed.
Senarmont, pursuing another course, had applied a heat somewhat ex-
ceeding 662° Fahr. toan aqueous solution of hydrochlorate of alumina, con-
fined in a close tube, and thus decomposing it into its volatile and solid
ingredients, obtained corundum, distinctly crystallized and mixed with
diaspore, the same substance under a different form, and with different
chemical properties, thus repeating in a remarkable manner that process by
which the same minerals are found in nature similarly intermingled. He
also succeeded in eliminating crystals of quartz from hydrate of silica by
dissolving the hydrate in water charged with carbonic acid, and gradually
raising the temperature of the tube which contained it to a heat of from
400° to 500° Fahr., and by analogous methods he obtained carbonates and
sulphides identical with native minerals. In some of these experiments the
process was so varied as to show that the separation of the anhydrous cry-
stals was due to the gradual withdrawal of the dissolving gas. The hydrated ©
sesquioxide of iron, also heated in water of the temperature of 360° Fahr.,
was dehydrated, becoming magnetic. In an experiment by Wéhler, on the
contrary, apophyllite dissolved in water at the same temperature, returned —
on cooling to its original form, retaining its water of crystallization. To this
class of discovery Daubrée has likewise added some valuable facts, having —
obtained regular crystals of quartz, by decomposing, with the vapour of —
water alone, the interior of a glass tube subjected to a low red heat ; at the
¥
2
ON THE EFFECTS OF LONG-CONTINUED HEAT. 183
same time silicates were formed, hydrated or anhydrous, according to the
degree of heat; when fragments of obsidian were inserted, crystals of
Rhyacolite appeared ; and the silicated water of Plombiére being substituted
for plain water, and kaolin for obsidian, crystals of diopside insinuated
themselves into the silicated substance of the tube, and the kaolin was
changed into a substance possessing felspathic characters.
All these experiments are adverse to the idea that the primary rocks have
undergone fusion. The best natural criterion, perhaps, of the temperature
at which they were formed, was afforded by the discovery, in 1828, of a
method of manufacturing wltramarine, based on Vauquelin’s identification
of a furnace-product with the Lapis lazuli found in granite and in primitive
limestone. In some specimens which I possess of the latter rock, this
beautiful mineral may be seen enamelling with minute specks, and with
perfect distinctness, within and without, all the plates of the calcareous
erystals, which are here and there interspersed with small crystals of sulphate
of lime. The heat at which the artificial ultramarine is made is that of red-
ness. A lower temperature will not suffice to produce the colour, and a
higher destroys it.
We can now better understand how Hunterite, a white felspathic mineral
containing 11°6 per cent. of water, can have been formed where it is found ;
a hydrated silicate of alumina in the bosom of molten granite is an anomaly
for which high pressure would scarcely account; but if the rock was at the
temperature only of a low red heat, the formation of this mineral, and of
the hydrated micas, will no longer appear a marvel.
Other notices of ancient degrees of heat have been observed in the
strata. In a cavity within a quartz crystal from Dauphiné, Davy founda
viscous inflammable fluid in small quantity, in a perfect vacuum*. In the
cavities of other quartz crystals he found water and rarefied air. Sorby,
having determined the amount of rarefaction in one such from a bed of
mica-slate, in which he detected many others, calculated the temperature of
the crystal at the time of its formation to have been 320° Fahr. In one case
Davy found evidence of pressure which had condensed the elastic fluid in a
erystal of quartz, and Brewster observed the like in crystals of topaz.
From a general review of the researches now detailed, the following infer-
ences may be drawn :—
1. That all the consolidated strata, viewed chemically, bear marks of sub-
jection to an action of heat agreeable to the theory of the earth’s refrigera-
tion, in direct proportion to the age of their deposit ; and that they show that
action most explicitly in the presence, throughout, but more abundantly as
the series descends, of that peculiar form of silica which is chemically repro-
duced by the action of heated volatile matter.
2. That the igneous minerals were formed by molecular aggregation, at a
heat not exceeding, perhaps, that of an ordinary fire, either as a residuum
from the expiration of fusible and volatile materials, or more generally as a
deposit from volatile forms of matter.
As there are two classes of eruptive rocks, the guartzose and unquartzose,
so there are two classes of emanation which accompany them, and deposit
earthy minerals, differing for each class, in the neighbouring strata. They
generally mantle round the rock, and but seldom penetrate it; as if it had
rather made room for them to rise, than as if they made part of its substance.
Yet they bear a resemblance to the character of the rock which they follow.
Thus the erystallized owide of silicon is the characteristic ingredient of granite
* Rose quartz from granite, and cornelian from trap, are coloured by a carburet of hydro-
gen; crystals of graphite also have been found in quartz; but as carbonic acid must have
existed before plants could grow, these facts are no proofs of antecedent organic structure.
184 REPORT—1860.
rocks; and the earthy minerals imbedded in the metamorphic strata around
such rocks resemble quartz in being simple crystallized oxides,—innumerable
gems, for instance, of the crystallized oxide of alumina—vast masses of the
same, many tons in weight, in the form of emery, encysted in limestone
which has been metamorphosed by rocks of granitic character,—still greater
masses of crystalline sesquiowide of iron in similar relation to those rocks,—
crystalline peroxide of tin shot through them into the strata above.
In the eruptive rocks which followed the guartzose, these minerals, with
almost all the quartz, died out, and were succeeded by others of a more
complex nature appropriate to the porphyritic, trachytic, basaltic, and lavie
eruptions. Yet all these, as well as the granitic, are attended by similar
metalliferous veins, which grow very weak in the latest, but still show, at least
as far as the eruption of the more ancient lavas*, a continued communica-
tion with a common reservoir deeper seated than any of them.
Davy saw the lava of Vesuvius issuing, as if forced up by elastic fluids,
perfectly liquid, and nearly white-hot, its surface in violent agitation, with
large bubbles rising from it, which emitted clouds of white smoke, consisting
of common salt in great excess, much chloride of iron, and some sulphate of
lime, accompanied with aqueous vapour, and with hydrochloric and sul-
phurous acids. It contains also realgar and sulphide of copper, due pro-
bably to the reaction of sulphuretted hydrogen on the chloride of the metal.
In the early time of these eruptive emanations, when they escaped at
many points with little interruption, the land rose only to low levels above
the waters. As the crust of the earth grew more solid and weighty, and
the vent was confined to fewer lines of shrinkage, the elastic elements of
disturbance upheaved the incumbent beds with greater power, and the
* Though the presence of quartz in lava has been denied, the following account of its
coexistence with schorl in that of the valley of Maria in Lipari by Spallanzani shows that it
does exist in ancient, perhaps basaitic, lavas, and strikingly illustrates the theory of its sub-
limation, as here advanced. ‘‘ Among the lavas partly decomposed we find pumices and
enamels containing felspars and scales of black schorls, and certain curious and beautiful
objects, which derive their origin, in my opinion, from filtration. The lava is white and friable
to a certain depth, of a petrosiliceous base, full of small cells and cavities, within which these
objects make their appearance :—Tirst, minute crystals of schorl ; from the inside of these
cells project very slender schorls, sometimes resembling minute chestnut bristles, sometimes
a bunch, a plume, or a fan, to be ascribed to filtration after the hardening of the lava, since
though it is common to find schorls in lavas, they are found incorporated within them, not
detached as in this case. The second filtration has produced small guartzose crystals, and
the manner of their distribution in prodigious numbers renders them a very singular phe-
nomenon among volcanic objects. Wherever the lava is scabrous, wherever it has folds,
sinuosities, cavities, or fissures, it is full of these crystallizations. The larger crystals extend
to 34 lines, the greater part about 4a line. They consist of a hexagonal prism, infixed
by the base into the lava, and terminated by a similar pyramid. Three crystals, among those
I examined, were terminated by two pyramids, the prism being attached to the lava by a
few points, and the prisms projecting out. The most regular are in small cavities, but not
a few are on the surface of the lava. The Java, embellished with these, forms immense
rocks and vast elevations hanging over the sea, which, whenever they are broken to a certain
depth, are found to contain these crystals, with capillary schorls, not very numerous. I have
in my possession a group of needle-formed crystals from Mont St. Gothard, within which
are seven small prisms of black striated schorl. The same may be observed in these minute
crystals. One of these was perforated from side to side by a needle of schorl, the two ends
of which projected out. The tormation of these capillary schorls must have preceded that
of the quartzose crystals; otherwise it is impossible to conceive how the former should have
penetrated the substance of the latter. In remelting the lava in a furnace, the quartz
crystals remained perfectly unaltered.”
Spallanzani also states, that in this lava are garnets and chrysolites more refractory in the
fire than the matrix ; and he adds that since Dolomieu’s visit to the adjoining stoves, when
the whole ground on which they stood was saturated with hot vapours issuing everywhere
from small openings an inch or two in diameter, at the time of his own visit these were
reduced to one, exhaling some sulphur and encrusted with soft pyrites.
—
iT RWS
ON THE EFFECTS OF LONG-CONTINUED HEAT. 185
mountain chains culminated to their utmost height. In the progress of re-
frigeration the compressing and imprisoned forces became nearly balanced,
and the residual predominance of the latter produces the phenomena of
existing earthquakes and volcanoes.
In the earlier periods, unmutilated skeletons, undisplaced scales, entire
ink-bags, and florescent fronds, indicate conditions of nature which would
now be called unnatural, a history of sudden death and speedy embalment,
common, not to individuals only, but to generations and species. The pre-
servation, in exquisite casts, of the most delicate organizations indicates a
speedy but a tranquil entombment, which it would be difficult to refer
to any other agency than that of gaseous emanation through the waters
in which the plants and animals existed. Alcyonia and sponges, looking
like recent specimens preserved in the places where they grew, point to a
process of silicification, chiefly anhydrous, which anticipated decomposition.
In the decreasing activity of internal heat and insalubrious emanations, we
see the advancement of the physical and chemical conditions essential or
advantageous to /ife; and with the progress of such conditions, favourable to
the development of higher and higher forms of organization, we find a perfect
correspondence in the natural history of organized fossils, and the increasing
tones of the “ Diapason, closing full in Man.”
From the theory of heat and the facts of geology, combined with physio-
logical considerations, we learn that there was a definite era, in which the
earth first became capable of supporting vegetable and animal life ; and we
may account for the late appearance of man, by observing that there were no
conditions adapted to the well-being and progress of human nature, till this
state of things had yielded to a healthy atmosphere, a moderate heat,
differentiated zones of life, stable forces, and a stationary standing ground.
{In the rudimental ages of the earth we behold an ever-changing scene of
new and fitful conditions passing in rapid succession. Through all the stages
of its existence previous to the present uniformity, so favourable to the
exercise of reason and the freedom of will and action, we see force gradually
subsiding, and the time allowed to life expanded into a wider liberality. Our
ideas of its duration, as compared with indefinite ages, are equally limited with
our view of its magnitude, in comparison with space or matter ; we can find in
geological data no chronology but that of priority; the fossil records even of
its unconsolidated beds have not yet supplied us with the key of the cypher
which should connect geology with human history. If ever we come to know
the age of the primary rocks, or of the protozoic strata, it can only be by
combining physical data with the experimental reproduction of granite, and
a knowledge of the heat which the lowest organisms can bear, and live.
Since Hall first applied chemistry to the service of geology, few attempts
have been made in this country to pursue the path which he opened. In
1833 the British Association entrusted to a commission, consisting of Prof.
Sedgwick, Dr Daubeny, the late Dr. Turner,and myself, the task of illustrating
geological phenomena by experiments which it was hoped might have thrown
light on some of the subjects discussed in this Report. Disappointed of the
greater part of the fruit of these experiments, I yet believe that the few
results which I now lay on the table of the Section will not prove devoid of
interest, especially as evidence of the low temperature at which bodies scarcely
reputed volatile are capable of being sublimed.
The iron furnaces of Yorkshire having been selected as furnishing the
best field for these experiments, it fell to my lot to conduct them. Every
facility was afforded me by the zeal and liberality of the proprietors and
managers of two furnaces, one of which at Elsicar, belonging to the late Earl
_ Fitzwilliam, and managed by Mr. H. Hartop, worked for a period of five
186 REPORT—1860.
years; the other at Low Moor, belonging to Messrs. Wickham and Hardy, pro-
longed its unintermitting blast for fifteen years. The materials fur the experi-
ments, in addition to those which I was myself able to supply, were provided
partly by a grant from the Association, partly by an extensive donation of
minerals and fossils from the stores of the Yorkshire Philosophical Society.
Professor Phillips also, who was then in charge of that Society’s Museum, lent
me his valuable assistance.
The object kept in view, in devising experiments of so long a duration, was
to subject the greatest possible variety of materials to the greatest possible
variety of conditions, such as it might be presumed had formed, or altered,
rocks, minerals, and mineralized organic remains.
These were arranged in numerous crucibles, upright and inverted, and
within two strong tripartite boxes of deal bound with iron thongs; one
of these was stored with large blocks and copious powders of granite, basalt,
limestone, grit, and shale, with whole and pounded minerals of every kind,
hydrates and anhydrates, the ingredients of a great variety of minerals com-
pounded in proper proportions, all the different salts and elements calculated
to react upon them, with almost every metal adapted to form veins or to re-
gister heat ; the other contained organic substances, fossil and recent plants,
shells, corals, reptiles, and bones, disposed in clay, sand, chalk, marble, gypsum,
fluor, sulphates, muriates and other salts of soda and potash which might dis-
engage volatile elements by their mutual action, to react on fixed constituents.
At the Elsicar furnace I was allowed, whilst it was being built, to insert
crucibles in the back of the masonry in immediate contiguity with the body
of melted iron. At Low Moor it was agreed to place boxes filled with cruci-
bles and materials under the bottom stone, before the furnace was built.
This stone, consisting of millstone grit, 15 inches thick, though it gradually
wears hollow in the centre, retains the iron fused upon it usually for fourteen
or fifteen years, without being materially impaired. In its crevices are often
found the beautiful cubic crystals of nitrocyanide of titanium, first brought
into notice by Dr. Buckland.
In this situation the temperature to which the contents of the boxes would
be exposed could not be exactly foreseen. It was presumed that in the centre
it would be near to the melting-point of cast iron. It will be seen by refer-
ence to Plates IV. and V., which give a section and plan of the furnace, that
the boxes did not occupy the whole space beneath the bottom stone. It oc-
curred to me therefore, when these had been placed in position on a bed of
sand, covered with the same material, and built up with fire brick, to deposit
round them in asimilar bed of sand, and enclose in like manner within walls
of brick, lumps of various metals, and of granite, sandstone, fossiliferous
shale, and limestone. From these supplementary experiments are derived
the most interesting of the results which I have to describe.
For when at the expiration of fifteen years the furnace was blown out, I
found nothing left of the boxes but the iron straps with which they were
bound, in a state of oxidation ; a few crucibles and portions of crucibles only
had survived the general wreck of their contents ; granites, basalts, limestone,
choice minerals, measured pieces, weighed powders and compositions, had
disappeared ; all the exactness with which Professor Phillips had arranged for
identifying the altered substances by their position and by comparison with
reserved specimens, was lost labour.
Nor did I find the deposits in the Elsicar furnace, at the end of five years,
to have fared any better. From all these carefully devised experiments I can
produce but two worthy of notice. One of them exhibits the conversion of
river sand into sandstone, with a vacuity in its axis left by the volatilization
of arecent plant, The stone has considerable tenacity, and came out of the
.
a
a
ON THE EFFECTS OF LONG-CONTINUED HEAT. 187
erucible, with no adhesion to its sides, a perfect cast; no salt had been added
to it, nor is any separable from it by boiling. The close cohesion of the
grains of sand by the action of heat may have been facilitated by the inter-
mixture of some impurities, referable to oxide of iron, and possibly to felspar.
The only vestige of the plant is a skin of silica on the surface of the place
which it occupied in the interior of the sand, coating the vacancy, but not
furnishing an impression from which the character of the plant can be re-
covered. ‘The stone showed signs of splitting from shrinkage in an oblique,
or nearly vertical direction, a tendency which might probably have been more
conspicuous had the experiment been on a larger scale.
The other specimen is a translucent mineral of a pure blwe colour. This
colour it does not lose when heated red-hot in the outer flame of a candle.
Melted into a bead with carbonate of soda, it passes into a pure opake white ;
the same also with a small proportion of borax; when the proportion of the
borax is increased, the bead is transparent and colourless; dissolved in
hydrochloric acid, the mineral loses its colour. The solution contains much
sulphate of lime, and some silica and alumina, whether potash also, or soda, I
have not determined ; tested with prussiate of potash, it shows no trace of
copper; and none, or scarcely any, of iron. This substance therefore belongs
to the class of minerals of which Lapis lazuli and Haiiyne are varieties. It has
been formed irregularly under a thin crust of sand to which it adheres, is ini-
bedded in sulphate, sulphide, and carbonate of lime, and accompanied with
erystallized fluoride of lime. Whether this fluoride is a recomposition, or
part only of the original mixture from which the blue mineral has been
derived, I cannot say. The erucible certainly contained pounded fluor, and
a sulphate, which underwent decomposition, and partially decomposed the
fluoric crystals.
But the objects to which I have alluded as possessing a new and unexpected
interest, are the metals above mentioned as having been supplementarily
placed, outside the boxes, under the bottom stone of the Low Moor furnace.
The specimens consisted, originally, of pieces, of which chromographie plates
have been appended to this Report, cut from a bar of zine, a block of tin,
a pig of /ead, and a plate of tile-copper. They occupied, severally, the places
marked in the accompanying ground plan of the furnace, 1, 2, 3, 4, as
numbered at the time of the deposit. It will be seen that none of these
pieces have undergone fusion, that of which the melting-point is lowest (the
block tin) preserving perfectly its dimensions, the exact shape into which it
was cut, and the sharp edges of the cutting. ‘The external coat of the
tin, to the depth of from 1th to ith of an inch, is converted into deutoxide,
crystalline, transparent, and of the same specific gravity as the native ore;
between this and the metal, intervenes in some parts a space, which, with
the striation of the metallic surface, indicates that a portion of the substance
has been dissipated.
Of the bar-zinc, more than half has been changed, though it preserves its
original form, into a mass of crystalline oxide, interspersed with globules of
the metal, burrowed in all directions with drusy cells and cavities, and
showing extensive sublimation into the indurated sand which envelopes it.
The nature of the sublimation is manifested by a number of prismatic spicula
of metallic zine, about 4th of an inch long, standing within the cavities.
But that which is chiefly remarkable is the tile-copper, in respect both to
the temperature at which it has been volatilized, and the combination and
interpenetration which its molecules, in a volatile state, have effected with its
nearest neighbour, the dead. I have caused a drawing to be made of these
specimens in their relative positions, as they lay in proximity to, but not
touching, each other, having a portion of sand interposed.
188 REPORT—1860.
It will be seen that a very considerable portion of the copper plate has
been dissipated, that the surface has been sweated down, and in some parts
the whole substance has evaporated away. Bright crystals of red oxide of
copper line the wasted surface, which is also covered above with a coat,
ith of an inch thick, of mixed crystalline oxides of copper and lead; and
in the hollow which the dissipation of the metal has left between it and the
indurated sand, is a sublimate consisting of fine twisted coherent threads of
metallic copper, like those met with in mines and slags. Where nearest to
the lead, it has so intermixed its exhalations with those proceeding from
that metal as to have spread over the upper leaden surface a coating of green
crystals, consisting of a double oxide of copper and lead. Beneath, and round
the lead, at its contact with the sand (which below has penetrated its sub-
stance without altering its form), runs a pink skin, marking the path of the
red oxide of copper. I cut the lump of lead in half, and found it not only
traversed in the middle by a seam of mixed oxide, but, what was still more
remarkable, dotted with spots of metallic copper, which had found their way
to the very centre of the mass, and even reached the opposite side.
That it was the metal in this case, as in that of the zinc, which became
volatile, and was subsequently deposited in the form of specks and filaments
of copper in some places, and combining with oxygen, as a crystallized oxide
in others, cannot be doubted. To attribute these effects to thermal electricity
would not be consistent with the facts; for there was here no contact, and no
circuit. The penetration of the lead by the molecules of copper may be
called Cementation, and be supposed to be due to capillary attraction of pores
distended by heat acting on the volatile particles.
But the surprising part of the result is, that the sublimation of copper by
heat should have taken place at so low a temperature. These four metals, in
close proximity, and all acted upon in the same manner, were their own
mutual thermometers. It was impossible that the heat to which the copper
plate, as a whole, had been subject could have been higher than the melting-
point of the unfused lead and tin. I can attribute this unexpected fact to
no other cause than the continual and protracted passage of hot currents of
air and vapour, mingled perhaps with carbonaceous gas from the neigh-
bouring wooden boxes*; and it seems probable that if the central portion
of the bottom stone had withstood to the end the action of the furnace, or
if the buried boxes had been protected with a vault of brick, more light
might have been thrown on the transfer of molecules at moderate tempera-
tures by similar effects produced on other materials.
I owe an apology for having delayed this Report much longer than I
should have done, had the bulk of the experiments been attended with better
success. I have been reminded of them by the design of a member of the
Association to institute some of a similar character with the added conditions
of pressure and steam. Whoever should now undertake such experiments
would conduct them on the vantage ground of the later researches which I
have here noticed, and might obtain results of high interest to geological and
chemical science. It may be doubted whether heat protracted through many
years, or even extraordinary pressure, may be essential elements of such
results. The unintermitted presence of volatile materials, for a considerable
time, passing over and dwelling among those of greater fixity at temperatures
mounting up to a red heat, may be the only needful condition; and if a fur-
* Tf I am right in believing that an oolitic Echinus, Pecten, and Coral, and an Ammonite
from the Lias, which I recovered from the furnace, are those marked in the Plan with the
Nos. 8, 9, 10, then, as these were reduced to alkalinity, though without change of form or
markings, it would follow that the carbonic acid under the same circumstances separates
from lime at an equally low temperature of the mass, under the partial action of hot currents.
ON THE EFFECTS OF LONG-CONTINUED HEAT. 189
nace were appropriated to this object, it is not difficult to conceive a con-
struction and application of it which would fulfil such a requirement.
If any one could succeed in effecting the synthesis of pseuwdomorphic
crystals, or of granites and porphyries, he would certainly perform a great
service to chemical geology. In the first of these subjects of experiment
success is scarcely to be looked for, except in the metamorphic action of
heated volatile agents. It is possible that granite also, and porphyry, might
be formed by a process of volatilization ; or they might perhaps be produced
as a residual igneous crystallization out of a mass, of which the flux had been
removed from the denser substances by sublimation, solution, or pressure.
It should appear that the production of marble is also a problem still un-
determined. Rose has expressed an opinion, founded on his own ex-
periments, that the solid substance which Sir J. Hall obtained, by igniting
chalk under a pressure that prevented the extrication of the carbonic gas,
cannot have been marble. Possibly the presence of an excess of the acid
may be an additional requisite to the production of a perfect specimen.
Since this Report was drawn up, I have seen a memoir by M. Daubrée*
which contains a very able and complete exposition of the progress of
geological chemistry. His observations on the deposit of zeolitic crystals
and other minerals discovered in the interstices of the old Roman brick-
work and concrete at Plombiéres}, which have undergone the action of sili-
cated waters springing from the earth at a temperature not, now at least,
exceeding 158° F., seem to have solved the problem of the deposit of such
erystals and minerals in the vesicles of basaltic rocks, and to have proved
them to be due to aqueous infiltration whilst the rock was still hot.
His views on the formation of another class of minerals, and the origin of
the granitic and other early rocks, seem to be not equally satisfactory. To
these he has been led by his own late experiments on the effect of aqueous
vapour in decomposing obsidian and glass. He propounds, with the difftidence,
however, which belongs to a hypothetical speculation, a theory to the
following effect—that in a primeval state of the earth, when the heat now
known to exist in its interior extended to the surface, as that surface cooled.
down to a certain point, the red-hot obsidian, or silicated glass, of its first
coat was decomposed by water condensed from a state of vapour, under
great pressure, at a red heat; thus the quartziferous rocks were formed, at
first as a plastic sponge, and when the water had evaporated as granite, the
schist and slates immediately superincumbent upon it being the residuary
product of the mother-waters.
But this speculation is open to grave objections. What principle of
solidification, it may be asked, capable of compacting graaite, is included
in a process of disintegration? What has become of the silicates involved
in it, to which we might look for such solidification, but whieh are absent
from granite? The mother-waters which it supposes are incapable of dif-
fusing the peculiar minerals encysted in the proximity of granitic rocks
even to the distance of thousands of feet. No less unaccountable would be
the absence of all the zeolitic and opaline substances that might have been
expected. Everything tends to show that whatever the power of this process
may be, it must be confined, at least, to the lavas, basalts, and trachytes.
That heated water has been so universal a solvent as M. Daubrée supposes,
is rendered very improbable by a circumstance noticed by Cagniard de
Latour in his celebrated experiments on vapour highly heated and com-
* Etudes et expériences synthétiques sur le métamorphisme et sur la formation des roches
erystallines, 1860.
T The presence of fluorine in the apophyllite of Plombiéres is remarkable, the more be-
cause Vauquelin analysed the waters with the express object of detecting this constituent,
and denied its supposed existence in them.
190 REPORT—1860,
pressed. In one of these, the addition of a crystal or two of chlorate of
potash to water at the temperature of 648° F., proved sufficient to prevent
any action of the aqueous vapour on the glass ; so easily was it saturated by
the presence of a more soluble material.
Neither is it at all probable that any stratum which can be supposed to have
preceded granite under extraordinary conditions of heat and pressure, can
have resembled in any degree obsidian or glass) M. Daubrée takes the
vapour expansion of the ocean over the globe as equivalent to a pressure
of 250 atmospheres, somewhat exceeding Mitscherlich’s supposition before
quoted. On this pressure Mitscherlich, as has been said, sagaciously re-
marked, that it would probably materially modify the chemical affinities
of bodies, and prevent the formation of silicate of lime. His anticipation has
been experimentally verified; and an equally remarkable instance of the
same principle has been lately observed by Mr. Gore, who has found, on
immersing some fifty substances in carbonic acid liquefied by pressure, that
in that state it is chemically inert, to such a degree as not to dissolve oxygen
salts. In these cases it should seem that pressure favours homogeneous, or
simple, at the expense of heterogeneous, or complex, attractions ; and there is
all the less reason for admitting M. Daubrée’s supposition, that obsidian,
or any vitreous silicates, preceded the granitic rocks.
We may carry these ideas further ; we may extend our speculations from
the heat and weight of a vaporized sea to the gaseous system of Laplace, and
the ultimate atoms of Newton. ‘Then, as the heat by degrees radiated into
space, and as the repulsive force yielded to the forces of attraction, the
first compounds would be of the simplest order,—water, and hydrochloric
acid,—the chlorides of potassium, sodium, silicon, and aluminium, the oxides
of magnesium and calcium, with others of a like class. Here we have both
the materials of the sea, and of the primary crust of the earth; and at the
same time all the power of consolidation which free crystalline force and
enormous pressure can give to materials indisposed by that pressure to enter
into complicated combination.
In contemplating the origin of granite, it is not, however, competent to
us to regard it as a fundamental rock only, since it preserves the same
erystalline character under various conditions of heat and pressure. But
we must remember that the gaseous theory which we are imagining implies
a residue, in an internal gasometer, of similar primary compounds confined
in a highly heated, condensed, and elastic state at no great distance under
our feet, from the sudden or gradual evolution of which it is not difficult
to conceive that all the eruptive rocks and veins, and many of the pheno-
mena of consolidation in the sedimentary strata, may be accounted for.
Every rock of eruption, and every mineral vein, which has shot up into the
strata, indicates such an origin. The porphyries, trachytes, basalts, and lavas
are essentially chemical and erystalline compounds. They differ from the quart-
ziferous rocks only in this, that the chief part of the siliceous ingredients which
characterize the latter having been antecedently used up, the greater fusi-
bility of the former has more or less obliterated their crystalline structure.
In these speculations it matters not from what source we suppose the
heat of the earth to have been derived. Perhaps, a law of gravity, together
with the other forces of attraction, imposed on the ultimate particles of
matter, may account for all the heat which is, or has been inthe world. In
any case, the most probable inductive conclusion from our knowledge of
the earth’s heat, and the phenomena of eruption, with the light thrown on
the production of minerals by Daubrée’s first sertes of experiments, and
those of Durocher, appears to be, that mineral veins and eruptive rocks
are the result of gaseous combinations and reactions. As regards mineral
——
43>
ee oe ee ee ee ee
> De a eran nei
ON THE EFFECTS OF LONG-CONTINUED HEAT. 191
veins, this, I believe, is the opinion of most observers. But we see the same
metamorphic effects which are produced by them, equally produced by the
presence of any eruptive rock. If a stratum of limestone be invaded, and a
portion of it included in the invading substance, that portion is not unfre-
quently impregnated with magnesia and converted into dolomite, equally by
a mineral vein or a granitic rock.
The advantages which this theory possesses over any that have yet pre-
sented themselves, are that it accounts for all the following phenomena :—
1. The characteristic structures of granite, and of gneiss and mica-slate,—
which may be compared to the deposits of graphite in gas-retorts, solid
where the carburetted gas aggregates its decomposed molecules of carbon in
confinement, but faliated and quasi-stratified, where the gas chances to escape
through cracks in the retort into the more open chamber of brick-work ;—
2. The perfect uniformity of crystalline texture in granite, whether deep or
superficial, in thin veins or solid masses, showing that neither great pressure
nor slow cooliug have been essential conditions of its crystallization ;—
3. The wide diffusion of zones or atmospheres round the eruptive, and
especially the granitic rocks, of mineral substances, and metamorphic effects,
a phenomenon which, together with that of the filling up of mineral veins
from below, is not accounted for by any other theory ;—
4. The metalliferous and quartziferous impregnations of the sedimentary
strata.
If, with Cordier, we divide the eruptive rocks into the guartzose (which
correspond to the granites and earliest porphyries) ; and the wnquartzose,
comprehending the fe/spathic (which correspond to the later porphyries and
trachytes) ; with the pyroxenic (which correspond to the basalts and lavas) ;
and if we consider all these as originating from gases, accompanied by
aqueous vapour,—then the phenomena show the amount of such vapour
present in the guartzose formations to have been almost infinitesimal,
whilst that which attended some parts of the pyrowxenic formations was con-
siderable. As regards the sedimentary siliciterous rocks, they show, in the
semiopaline, semiquartzose composition of the siliceous beds, the action of
anhydrous gas, aided by aqueous vapour. Aqueous vapour acts on silicates
only at a heat approaching redness, and conveys no silica. Chloride of silicon
would carry silica, and would diffuse it at a much lower heat, since it boils
at a temperature below 140° F.
Connected with the preceding speculations the following remarks may
deserve attention. There is a singular resemblance of mineral and erystal-
line constitution between the pyrozenic rocks and meteoric stones,—a re-
semblance, in fact, so close as to indicate a similar mode of production out
of the same materials. The late optico-chemical discoveries of Bunsen and
Kirchhoff have shown, with a great degree of probability, that molecules of
tron, nickel, and magnesium abound in the solar atmosphere; should the
progress of those discoveries add silicon to this list, we have here again the
chief materials, both of meteorolites and of pyroxenic rocks. In any ease,
whether we suppose the meteorite to have been contemporaneous with the
earth, or to be ejected from the moon, or emitted from the sun, our thoughts
are led back to a time when the whole solar system consisted of the same
ultimate atoms, and are confirmed in the opinion that the meteorites and the
fundamental rocks of the earth have undergone similar processes of mole-
cular and erystalline combination, the vitreous coat of the meteorite, and the
vitreous character of the later lavas, being due also to the same causes :—
Ist, to the fusibility of the material; 2ndly, toa more intense heat generated
by a nearer proximity to an oxidating atmosphere; 3rdly, to a more rapid
rate of cvoling.
192 REPORT—1860.
What our views, however, of the original constitution of matter may be,
is a point of less consequence than what are the conclusions in geology to
which we are conducted by observation and experiment. The general con-
clusions to be drawn from the foregoing researches seem to be these :—
That no theory of the earth consists with the phenomena, which does not
take into account a heat of the surface once amounting to redness ;—that
the most prominent chemical and crystalline compounds which laid the base-
ment of the earth’s crust, and continued to penetrate it, as far as into the
tertiary strata, have disappeared in the present eruptive system ;—that the
nature, force, and progress of the past conditions of the earth cannot be
measured by its existing conditions ;—that to deduce accurate inferences in
the sciences of observation, the attention requires to be directed less to gene-
ral analogies than to specific and essential distinctions.
EXPLANATION OF PLATES.
PLATES IV. & V.
Section, and Plan, of the furnace in which the deposits lay for 15 years, the number
of each deposit, external to the boxes, being marked on the plan.
PLATE VI.
Fig. 1 (Plan No.4). Tile copper 5 in. X 2} in. X 3 in, coated with laminz of dark,
red, crystallized oxide of copper, alternating with white and yellow crystallized prot-
oxide of lead, and with a pink intermixture of crystallized oxides of copper and lead
covered with sand indurated, but not vitrified, by protoxide of lead.
a. Twisted filaments of metallic copper. 6. Crystals of red oxide.
bb. Lamine of crystallized red oxide of copper alternating with protoxide of
lead, and mixture of oxides of lead and copper.
c. Particles of metallic copper. ec. Golden metalline spot.
Fig. 2 (Plan No. 3). Pig lead, 4} in. x 3} in. X 2} in, View of upper surface, show-
ing green and yellow double oxides of lead and copper, with spots of metallic copper.
d. Cavity from which lead has sublimed.
e. Spots of metallic copper.
f. Double oxides of lead and copper.
PLATE VII.
Fig. 3 (Plan No. 3). Pig lead, vertical section, showing exterior and interior
seams of mixed oxides of lead and copper, green, yellow, and red, with spots of me-
tallic copper.
g. Red oxide of copper between lead and indurated sand.
h. Spots of metallic copper in the interior of the lead.
i. Oxide of copper and lead. kk, Lead hardened by disseminated oxide.
Fig. 4 (Plan No.4). Enlarged section of part of fig. 1, showing threads of metallic
copper.
Nie. 5 (Plan No.4). Part of fig. 1; enlarged view of pink mixture of crystallized
oxides of copper and lead, with spots and threads of metallic copper.
PLATE VIII.
Fig. 6 (Plan No, 2), Block tin, 3 in. X 2 in. X 1 in., with a coat of transparent cry-
stallized deutoxide from } in. to 4inch thick,
1. Striated surface of metal beneath oxide.
m. Crystals of deutoxide, transparent and colourless. :
Fig. 7 (Plan No. 1). Zine bar, in indurated sand, fractured, showing a surface
partly metallic, partly crystalline.
n. Spiculz of sublimed metal. o. Seam of metal.
Fig. 8 (Plan No.1). Showing cavernous face of oxide of zinc with crystals of do.
p. Cupped hollows set with crystals of oxide of zinc, out of which globules of
metal have sublimed.
Bottem Stone 16 inches thack
Dara Tar i ie TO 7
aq7ia wae en a ores |
D ‘
a od s nt th
ara yin Me,
REFERENCES.
cies Iron rests upon the bottom Stone in the space < feet 4inches in the Section
and the blast 1s introduced at the small Grclein D° The rigures tronv 1 te 23 on
the Ground Plan represent the order and situation of the Deposits made in the cavity
“on the outside of the Boxes. Lhe black tines in the centre of the Ground Plan repre -
"sent the two Boxes whose two sides meet exactly tn the centre of the Furnace.
e letters GR.B.C.D, agree with those marked on the Bocces.
N° L. Zine bar. 2. Coral tn Coral Rag, Tie how Moor Pig Trow.
; 2 Block Tin. ih = Jo. Lecten in Malton Oolite. 18. Septarium.
" 4 3. Lig lead. plates Al. Coral, recent . 19. Flagstone :
4. Tile Copper.| -7-8. LR. halk, 20. Granite .
5. Lit Shale trom Black Ironstone. 13. N° 11,395. 2L. dnamonite trv Lias .
6. Black Ball Zronstone. 4. Whale Vertebrx. 2%. Basalt.
7. Jet. Ls Blue linestone with Shells, 23. Granite Yorks Streets
8. Echirats in Malton Ovlite. 16. Magnesian Lanesterve .
ia
l
f
Ground Plan of the furnace .
Opening where the Blast is introduced
Bottom Stone L6 tnehes thick.
Ts
Front Arch where the
Furnace ts worked.
ae ra
Ss Pe Fas
2. ee ae
+e at »
oe
> . +
Oe tes :
» 2 Aw wick j ba 3° “ae.
Bf Foe es *
; Cr ee “
7" RIOTS om
* "y 2 e Pas ©
(Plan V°4 :
(Plan V?3.)
Fig 4&
Plan Ni 4)
hig 3
(Plan
Fig. 7.
(Plan N71)
fig. 6.
(Plan ¥* 2)
Fig. 8.
(Plan N’1)
ON STEAM-SHIP PERFORMANCE. 193
Second Report of the Committee on Steam-ship Performance.
CONTENTS,
Report. ’
Appendix No. I.—Table 1. Table showing the results of performances at sea and on
the measured mile, of 17 vessels of the Royal Navy, of 22 vessels in the Merchant
Service, and of two vessels of the United States Navy, together with the particulars
of their machinery.
Table 2. Return of the results of performances of 49 vessels in the service of the
Messageries Impériales of France during the year 1858.
Appendix No. II.—Table 1. Quarterly returns of the speed and consumption of coal
of the London and North-Western Company’s express and cargo boats, under
regulated conditions of time, pressure, and expansion; from January 1 to De-
cember 31, 1859.
Table 2. Half-yearly verifications of consumption of coal of the above vessels,
from January 1 to December 31, 1859.
Appendix No. ITI.—No. 1. Form of Log-book used by the Royal Mail Company.
No. 2. Form of Log-book used by the Pacific Steam Navigation Company.
No. 3. Form of Engineer’s log used by the Peninsular and Oriental Company,
No. 4. The Admiralty Form for recording the trial performances of Her Majesty's
steam-vessels.
No. 5. Board of Trade Form of Surveyor’s Return of Capabilities.
Appendix No. IV.—Table 1. Showing the ratio between the indicated horse-power
and the grate, the tube, the other heating, and total heating surfaces; also, between
the grate and heating surfaces, and between the indicated horse-power and the coal
consumed,
Appendix No. V. Letter from Mr. Archbold, Engineer-in-Chief, United States Navy.
Description of the hull, engines, and boilers of the United States Steam Sloop
‘Wyoming’.
Table 1. Return of performance of the ‘ Wyoming’ under steam alone.
Table 2. Return of performance of the ‘Wyoming’ under steam and sail combined.
Table showing the trial performances of the steam-vessels ‘Lima’ and ‘ Bogota’
when fitted with single cylinder engines, and after being refitted with double
cylinder engines. Also the sea performances of the same vessels under both these
conditions of machinery and on the same sea service.
Report.
Ar the Meeting of the British Association, held in Aberdeen in September,
1859, this Committee was re-appointed in these terms :—
“That the following Members be requested to act as a Committee to con-
tinue the inquiry into the performance of steam-yessels, to embody the facts
in the form now reported to the Association, and to report proceedings to
the next meeting.
“That the attention of the Committee be also directed to the obtaining of
information respecting the performance of vessels under sail, with a view to
comparing the results of the two powers of wind and steam, in order to their
most effective and economical combination.
“That the sum of £150 be placed at the disposal of the Committee for
these purposes.”
The following gentlemen were nominated to serve on the Committee :—
Vice-Admiral Moorsom. William Smith, C.E.
The Marquis of Stafford, M.P. J. E. M¢Connell, C.E.
The Earl of Caithness. Charles Atherton, C.E.
The Lord Dufferin. Professor Rankine, LL.D.
William Fairbairn, F.R.S. J. R. Napier, C.E.
J. Seott Russell, F.R.S. Richard Roberts, C.E.
Admiral Paris, C.B. Henry Wright, Hon. See.
The Hon. Capt. Egerton, R.N.
1860. o
194 REFORT—1860.
Your Committee, having re-elected Admiral Moorsom to be their Chair-
man, beg leave to present the following Report :—
They have held monthly meetings, with intermediate meetings of sub-
Committees appointed to carry out in detail matters referred to them by the
General Committee. The Committee regret that they were deprived of the
services of one of their members, Mr. Charles Atherton, at an early stage of
the present inquiry, his public duties preventing his attending.
They have been assisted by Corresponding Members ; noblemen and gentle-
men, who, not being members of your Association, were not, by its rules,
eligible as members of your Committee. Some of them, however, being
owners of steam yachts, and others intimately acquainted with all matters
relating to steam shipping, their cooperation was considered very essential,
as introducing to the Committee gentlemen, not only capable of dealing with
the subjects of this inquiry, but who also had it in their power to place in
the hands of the Committee, materials, which, it is confidently hoped, will
eventually lead to a correct and scientific knowledge of the laws governing
economic Steam-Ship Performance.
The Corresponding Members so elected were :—
Lord Clarence Paget, M.P., C.B., &e. | Capt. William Moorsom, R.N. (since
Lord Alfred Paget, M.P. deceased).
Lord John Hay, M.P. Mr. John Elder.
The Hon. L. Agar Ellis, M.P. Mr. David Rowan.
The Earl of Gifford, M.P. Mr. J. E. Churchward.
The Marquis of Hartington, M.P. Mr. Thomas Steele.
Viscount Hill.
It will be within the recollection of the Association that the labours of this
Committee last year were almost exclusively devoted to explaining to the
various shipping companies and others with whom they were in correspond-
ence, the objects proposed, and suggesting such forms as, if accurately filled
in, would accomplish the purposes contemplated by the British Association.
Log-books were prepared, and copies furnished to the leading Steam Packet
Companies.
At their first meeting the Committee took into consideration the manner
in which the grant of money placed at their disposal by the Association could
be most judiciously applied, and after mature consideration it was unani-
mously resolved :—
“That to procure information from shipbuilders and engineers, it is found
to be indispensable to hold personal intercourse with them, without which
little progress is likely to be made.”
The Honorary Secretary was accordingly deputed to wait upon the prin-
cipal Shipbuilders, Engineers, and Steam Shipping Companies in London
and its vicinity, to explain the objects of the Committee, and to solicit their
cooperation by furnishing the Committee with authenticated returns of the
sea performances of vessels, as well as of their trial trips.
In this your Committee are happy to report that they have succeeded. All
to whom application was made expressed concurrence in the objects of your
Committee, and their willingness to render every information in their power.
The great difficulty was to make a suitable selection of vessels as examples
of ordinary performance in the mercantile navy. Press of business, and
perhaps want of thoroughly understanding the aims of the Committee, induced
them to throw the whole labour of making these returns upon the Committee.
The log-books for a number of years, and any documents the Committee
desired to see, were freely placed at their service; but the time required to
ON STEAM-SHIP PERFORMANCE. 195
wade through the masses of logs, together with the fact of the Association
_ meeting this year nearly three months earlier than usual, rendered it imprac-
_ ticable for more than a limited amount of work to be got through. It was
therefore determined to make a selection of certain vessels, and to endeavour,
as far as possible, to render complete the record of a few.
Your Committee at the same time communicated with the Admiralty, with
a view of instituting a similar comparison between the trial trips and ordinary
performances of Her Majesty's vessels at sea.
They much regret that they have not been able to obtain the latter. The
Lords Commissioners, however, very courteously entrusted the Committee
with the original returns of Her Majesty’s vessels during the years 1857,
1858, and 1859, as furnished by the officers who conducted such trials, with
permission to copy and make any use they thought fit of the information
they contained. Diagrams of the engines taken on the trials during the year
1859 were also furnished. '
Your Committee must remark with regard to these trial performances, that
they do not appear to be instituted with any other view than as a trial of the
working of the engines, excepting in a few instances, when experiments have
been made to test the merits of certain screws. In very numerous cases, the
officer distinctly reports that the boiler power is insufficient. The speed
may or may not be taken at the convenience of the officers, but in no case
: : any note taken of the economical efficiency of the engines with regard to
uel.
As your Committee are restricted to a record of facts, it is out of place
__ here to suggest changes in the mode of conducting the trials of Her Majesty’s
_ ships. The Committee would, however, fail in their duty if they did not avail
themselves of this occasion to repeat their conviction, as expressed in their
last Report,—“ That it would tend to the advancement of science, the im-
provement of both vessels and engines, and to the great advantage of Her
Majesty’s service, if the trials of the Queen’s ships were conducted ona more
comprehensive plan, directed to definite objects of practical utility on a
scientific basis, and recorded in a uniform manner.”
In addition to the vessels of the British Royal and Mercantile Navies, your
Committee have great pleasure in being enabled to lay before the British
Association a return of forty-nine vessels in the service of the Messageries
_ Impériales of France, obligingly furnished by a member of the Committee,
Admiral Paris, and recorded in the form used by that Company ; also, of
__ two vessels belonging to the United States Navy, the particulars of which
have been extracted from the second volume of Mr. Isherwood’s recent
__ publication, entitled “ Engineering Precedents.” They have been introduced
_ into the Tables (see Appendix, Table I.).
While this Report was preparing, the Committee were gratified by receiv-
ing from Mr. Archbold, Engineer-in-Chief, United States Navy, two sets of
tabulated returns of performance of the United States steam sloop of war
_* Wyoming,’ under steam alone, and under steam and sail.
___These returns are of peculiar value, as comprising particulars in a form
which the Committee believe has never yet been published. Along with the
_ data afforded by Mr. Isherwood’s book, they give the area of sail spread and
_ the force of wind by notation, together with other particulars, useful for
_ caleulations of results and for comparisons.
_ These Tables are contained in the Appendix, with Mr. Archbold’s letter,
and a description of the hull, engines, and boilers of the ‘ Wyoming.’
The returns furnished by the British Admiralty embrace 216 vessels and
_ $53 trials, with about 900 diagrams. For the same reason as above stated, in
o2
— ere CU
—————————
‘©
os ee agen fd Pe
paneer
Or ot ales)
a
196 REPORT—1860.
case of merchant vessels your Committee were obliged to make a selection,
and to endeavour, for the purposes of the present Report, to obtain a complete
record of a few, in the form suggested by the Committee. With this view,
application was again made to the Admiralty, asking for the additional parti-
culars not embraced in the returns of trial performances already furnished,
and stating that their Lordships were, of course, aware that the particulars
given in those documents were of comparatively small value without others
of the vessels, their engines, screws, and boilers. The Committee added
that they were in possession of such full particulars from both companies and
private firms, and they trusted also to be favoured with similar information
from the Admiralty. To this communication, the Lords Commissioners re-
plied that they regretted they could not at present supply the information
desired; but they would be glad to receive a copy of the reports obtained
from companies and private firms. Your Committee thereupon constructed a
Table embracing the particulars of merchant vessels (Appendix I., Table 1),
and also a blank table filled in with the names of Her Majesty’s vessels,
selected as before mentioned, and containing the results of the test trials
already given, and furwarded them to the Admiralty, begging that they
might be favoured with the return of the table of the ships of war with the
blanks filled in, adding, that if pressure of public business should prevent
that being done, your Committee would send a person to copy the particulars
on receiving the sanction of the Lords Commissioners to such a course.
As a measure of precaution in case of failure on the part of the Admiralty
to send the promised particulars in time for printing, your Committee ob-
tained returns of the machinery of these vessels by application to the manu-
facturers, personally and by letter. They avail themselves of this opportunity
to thank Messrs. Boulton and Watt, Maudslay Sons and Field, and John
Penn and Sons, for having so fully and so promptly responded to the call.
They are, therefore, now enabled to lay before the Association a table com-
prising the results of the trials furnished by the Admiralty, together with the
particulars of engines, &c., furnished by the manufacturers: the figures in
Clarendon type (see Appendix I. Table 1) denote the Admiralty returns,
Your Committee regret that there are some particulars of the trials still
wanting, as, for example, the evaporation of water and the consumption of
fuel; but they believe that hitherto those items have not been recorded, It
is earnestly hoped, now that public attention has been called to the subject,
that a more exact and careful account may be taken, both on the measured
mile and on ordinary service at sea.
In compiling the Table of merchant vessels, a similar course has been
adopted, viz. of gathering from the best sources the various details necessary
to complete the Table. The Companies to which the vessels belonged, gave
every information in their possession, not only of the vessels themselves, but
also of their actual sea performances, and placed at the disposal of the Com-
mittee the sea logs for every voyage, with permission to make such extracts
as they deemed proper. For any additional information, they were referred
to the constructors of the engines and vessels. Your Committee cannot
speak in too high terms of the constant readiness to give information,
although at considerable inconvenience to themselves, which the various
Companies and private firms have invariably shown. They feel assured that,
had time permitted, and if the requisite labour could be devoted to it, the
whole shipping community would willingly contribute their quota of statistics :
all that is wanted is uniformity of arrangement, and that a form similar to the
one proposed by the Committee be generally adopted.
The thanks of the British Association are especially due to the Royal
ON STEAM-SHIP PERFORMANCE, 197
Mail Steam Packet Company, to the Pacific Steam Navigation Company, to
the London and North-Western Railway Company, to Messrs. Inglis Bro-
thers, Messrs. Randolph and Elder, Messrs. Caird and Co., Messrs. R. Na-
pier and Sons, and to Captain Walker, of the Board of Trade.
Captain Walker very obligingly placed at the service of the Committee
some of the books in which the vessels registered and surveyed by the Board
of Trade are recorded, and your Committee are in possession of copies of the
entries of 51 vessels, varying from 600 to 2000 tons register and upwards,
registered in the ports of London, Liverpool, Southampton, and Glasgow,
during 1858. These have formed a very useful guide in leading to a selec-
tion of vessels from which to obtain the particulars requisite for comparison.
Your Committee have been in communication also with the French and
American ambassadors, with a view to obtaining the statistics of perform-
ance of their respective navies ; and, after referring the matter to their home
Governments, the Committee have received the assurance of their willingness
to cooperate.
Your Committee, being precluded by the terms of their appointment from
discussing theories, or attempting to deduce laws, have, nevertheless, thought
it not inconsistent to prepare a table of ratios based on the indicated horse-
power, and showing the ratio between that element, as developed on the
measured mile, and the grate, the tube, and other heating surfaces of the
boilers producing it; also, between the grate and heating surfaces, and be-
tween the indicated horse-power and the coal consumed. The Committee
regret that this important item, the coal, is not more frequently recorded,
very few private trials making any note of it; and in no instance brought
under the notice of the Committee, have the Admiralty officers made known
this element, so necessary for ascertaining the efficiency of the boilers (for
Table of Ratios, see Appendix IV. Table 1).
The following is a general summary of the result of the Committce's
labours during the past session. They have obtained :—
1. Returns of 353 trials by 216 of Her Majesty’s vessels of war during the
years 1857, 1858, and 1859, with about 900 (898) diagrams taken during
the trials in 1859; also notes, by the officers conducting the trials, of
observed facts.
Of these trials, fifty-eight made by seventeen of the vessels, have been
selected by way of illustration, with the particulars of machinery obtained from
the makers, and arranged in a tabular form. (See Table 1, Appendix 1)
The names of the vessels are the ‘ Diadem,’ ‘ Doris,’ ‘ Mersey,’ ‘ Marlborough,’
‘Orlando,’ ‘Renown,’ ‘ Algerine,’ ‘Bullfinch,’ ‘Centaur,’ « Flying Fish,’
‘ Hydra,’ ‘Industry,’ ‘ James Watt,’ « Leven,’ ‘ Lee,’ « Slaney,’ and ‘ Virago.’
This Table also comprises the two American vessels, ‘ Niagara’ and ‘ Massa-
chusetts,’ together with the British vessel ‘ Rattler,’ introduced for compari-
son.
2. Returns of 68 merchant vessels.
Four diagrams taken during trials of the ‘ Atrato.’
Scale of displacement of the ‘ Atrato.’
Lines of ditto.
Eight diagrams of the ‘Shannon’ taken during trials.
Twenty-two of these vessels have been selected and tabulated. (See Ap-
pendix I. Table 1.) Their names are— Anglia,’ ‘Cambria,’ ¢ Scotia,’ ¢ Tele-
graph,’ ‘ Mersey,’ ‘ Paramatta,’ ‘Shannon,’ ‘ Tasmanian,’ ‘ Oneida,’ ¢ Atrato,’
‘La Plata,’ ‘Lima,’ ‘San Carlos,’ ‘ Valparaiso,’ ‘ Bogota,’ ‘ Callao,’ Guaya-
quil,’ ‘ Undine,’ ‘ Erminia,’ ‘ Admiral,’ ‘ Emerald,’ and ‘John Penn.
The returns of the first four, belonging to the London and North-Western
198 REPORT—1860.
Railway Company, are the mean of a number of trips on actual service be-
tween Holyhead and Kingstown. ‘The returns of the ‘ Erminia,’ ‘Admiral,’
‘Emerald,’ and ‘John Penn,’ are measured mile performances only ; but the
remaining 12 vessels, with the exception of the ‘ Undine, show their sea
performances over distances of about 6000 consecutive nautical miles each,
in addition to the performances on the measured mile.
3. Return of the results of performance of 49 vessels in the service of the
Messageries Impériales of France, recorded in the form used by that Com-
pany. ‘The whole of these vessels are given in the Appendix. (Appendix I.
Table 2.)
4. Quarterly returns of the speed and consumption of coal of the London
and North-Western Company’s express and cargo boats, under regulated con-
ditions of time, pressure, and expansion, from January 1st to December 31st,
1859—presented by Admiral Moorsom. (Appendix II. Table 1.)
Half-yearly verifications of the consumption of coal of the above vessels,
from January 1st to December 31st, 1859, (Appendix II. Table 2.)
5. Forms of log-book used by the Royal Mail Company (Appendix III.
No. 1), by the Pacific Steam Navigation Company (No.2), by the Peninsular
and Oriental Mail Company (No.3), the Admiralty form for recording trials
of Her Majesty’s vessels (No. 4), and the Board of Trade form of return of
capabilities (No. 5).
6. Table showing the ratio between the indicated horse-power and the
grate, the tube, the other heating and total heating surfaces; also, between
the grate and heating surfaces, and between the indicated horse-power and
coal consumed. (Appendix IV.)
From the above list, it will be readily conceived that the time of the Com-
mittee has been fully occupied, as the task of copying and condensing from
log-books is one involving a large amount of labour. Your Committee have
not therefore, as yet, been enabled to conduct experiments on the plan
recommended in their first Report presented to the Association in Aberdeen.
They have, however, kept that branch of their inquiry in view; and through
the courtesy of Mr. A. P. How, of Mark Lane, and of Messrs. Tylor and
Sons, of Warwick Lane, they have been presented with apparatus of the
value of about £60, consisting of salinometers, and an engine counter and
clock; they have also at their disposal, for use whenever required, a superior
dynamometer, and a compound stop-watch, and are now prepared to pro-
ceed with experiments, should the Association see fit to renew their powers,
and the consent of the Government be obtained.
The Committee regret that they have not been able to collect any such
information respecting the performance, under sail alone, of steam-vessels,
as was contemplated by the Association, “with a view to comparing the
results of the two powers of wind and steam, in order to their most effective
and economical combination.”
They must, however, draw attention to the synopsis given by Mr, Isher-
wood, of the steam-log of the ‘ Niagara, in which her performances, “ under
steam alone,” “under steam and fore-and-aft sails,” and “‘ under steam and
square sails combined,” are set forth in such manner that those conversant
with the subject will be enabled, without much difficulty, to assign its approxi-
mate value to the power of the sails alone.
In Mr. Archbold’s Table of the performance of the ‘ Wyoming,’ the addi-
tional particulars of the force of the wind by notation, the area of sail set,
and the indicated horse-power, which are not always stated in Mr. Isher-
wood’s synopsis, afford the means of tolerably accurate comparison.
It is a duty the Committee owe to themselves, to express thus publicly
ON STEAM-SHIP PERFORMANCE. 199
their sense of the services rendered to the Association by Mr. Henry Wright,
their Honorary Secretary, whose untiring energy, indefatigable labours, judg-
ment, and discretion, have enabled them to lay this information before the
meeting.
To Mr. Smith, a member of the Committee, their acknowledgements are
due, as well for the use of a room in his offices, as for several sources of
information opened to them by his influence.
The Marquis of Stafford, by placing a room in his house at the disposal
of the Committee for occasional meetings, has contributed materially to the
personal convenience of the members.
Of the grant of £150 voted by the Council of the Association, to defray
the expenses of printing, postage, collecting information, &c., £124 3s. 10d.
has been expended, viz.—
o's fe
Peprniuog last year’s Report ....... ...0--00cesncces Beware) oot
SenmrIMinn present Report. ... 52). -saa- sees ecco recess (8 14.0
To stationery and miscellaneous printing = GU Gt Mieedeecltn..0 5) RG Dee D
EMUMINEIE sic ne, 2 50S iv Mete sae amo satel v olple ey ia bide She whee a ‘iain abe
To sundry expenses, ‘including cab hire and railway fares, incurred 812 6
by the Honorary Secretary whilst collecting information .... 812 6
Votal expenditure 55.5% Vit. Fae. he's £124 3 10
Balance of grant remaining unexpended....£25 16 2
It was originally intended to institute inquiries, not only in London and its
vicinity, but also in Glasgow, Liverpool, Hull, Bristol, Southampton, New-
eastle-on-Tyne, &c., and for this purpose it would have been necessary to
defray the expenses of an agent to conduct the inquiry; but the shortness
of the session, together with the extended field which London presents, ren-
dered that course impracticable.
Your Committee feel, that a beginning having thus been made towards the
means of a scientific investigation of the performance of ships under differ-
ing conditions at sea and in smooth water, it would ill become the British
Association for the Advancement of Science to drop the question, although
expense as well as trouble is involved in its successful pursuit.
They recommend the reappointment of a Committee, with a renewal of
the grant, and with power to remunerate a clerk for such services as cannot
be undertaken by any of its members.
On behalf of the Committee,
C. R. Moorsom, Vice-Admiral,
19 Salisbury Street, Strand, London, Chairman.
June 13th, 1860.
WNote.—Since the above Report was written, and whilst in the press, infor-
mation was forwarded to the Committee which has enabled them to compile the
Table given in the Supplementary Appendix, showing very interesting com-
parative results of two vessels, the ‘Lima’ and ‘ Bogota,’ when fitted with
different systems of machinery. The Table shows the results of perform-
ances on trial of these vessels when fitted with single-cylinder engines, and
also at sea on a voyage of upwards of 6000 miles; also their performances
when fitted with double-cylinder engines.
ERRATA.—Larce TABLE—APPENDIX I.
‘ Atrato’ on trial, Stokes Bay, Jan. 22, 1857, omit Indicated Horse power 1128°42.
Ditto, ditto, Mar. 4, 1857, for Indicated Horse power 1198°22°
yead 2396°44,
200
Appenp1x I.—TAsBLE
Name of vessel.
Guirinal ...........
Seer +2 ane
Méandre
eee eeweneeee
sere eeeee
QOBITIS 5 i052 ateuien oat
Bosphore ........-
Hellespont ........
Qronteecsssed.<.2
Philippe Auguste
Merovée
Cheliff
Aventin ..........+.
Leonidas ..........+
Tage ¥
Tancréde
Télémaque
Amsterdam
Périclés
se eeereeeee
Totals
see eeeene
Nominal horse-power.
REPORT—1860.
2.
revolutions.
Mean number of reyolu-
tions by counter.
Corresponding number of
| 24
| 27-5] 2
h num-
Nominal power realized
ber of revolutions obtained.
corresponding wit
Total distance run.
Hours
Under
weigh.
Under
steam.
h
841
2211
805
2781
2677
1686
1822
2359
2269
6106
3244
4320
6870
218
63808
5795
5393
5370
2668
890
1174
5512
5454
1223
6129
5104
63874
284945
5815
2793
1967
1911
3108
2537
3514
1862
2018
525 2
2107
1671
1485
2168
2320
1969
2285
1924
1017
1424
2162
2543
2528 20
1904
116152 30| 92733
2370 1893
m m
25| 1462 15
2077 50
2556 15)
2622 15
2786 10
30
40
1400 40
25
25
55
45
50
36
2125 55)
Results of Performances of the Steam-ships in
Mean pressure of steam.
Mean cut-off.
ee ee
Mean vacuum in condenser.
0°65 | 0:50
ots
nae
Notz.—Metre = 3:2809 feet = 393702 inches
}
<3
1,935,570
2,180,496
543,000
2,268,404
1,704,550
1,414,570
1,259,626
1,350,790
3-46) 0°33} 2,081,867 | 1099
0, = 220549 Ibs, Avoirdupois,
Consumption of coal.
| 2
= a3 = ? 3 Pet 3 u
¢| 8 Total g | Fe '|eul es
Ble e | £8 leelas
A Sie ewes lee
= [2 |ERg*
K kilo. kilo. | kilo.| kilo
- 1483 465 | 40) 48
2 1390 432 | 3-7| 46
: 1533 450 | 41) 48
; 1248 384 | 3:4] 3-4
Fi 14380 411 | 3:8} 3-9
52 1675 416 | 45) 44
3 1586 462 | 4:9) 5-4
: 1529 414 | 47} 5-0
. 1605 489 | 45
“6% 1547 477 | 51
> 1644 495 | 5-4
“62 1130 345 | 4:7
Y 1222 369 | 50
2 1268 423 | 53
E 1215 336 | 5:0
a 3,336,095 | 1191 387 | 4:9
: 1,983,785 | 1008 318 | 4:2
1:33} 1,906,803 997 800 | 41
q 2,950,203 949 3809 | 4:7
9} 2,470,000 | 972 315 | 48
bd} 3,692,912 | 1051 348 | 5:2
47
372 | 49
348 | 46
366 | 59
372 | 46
St SUB HS G2 DH HH HS CHS OUT HS HS OT OT UH CUT Ou
HK ROMTROTATWHHAAAR WK MARSHESAS
348 | 4:3
339 | 5-4
354 | 5:6
806 | 4-2
300 | 4-2
309 | 5-4
303 | 5:3
288 | 48) 5-0
306 | 5:4) 53
836 | 53) 57
821 | 51] 5-1
279 | S51} 55
267 | 54) 5:2
279 | 5-7) 59
246 | +7) 48
303 | 43] 53
383 | 47) 5-9
270 | 49} 59
212 | 5:0} 5:7
282 | 3:9} 49
330 | 5:3} 55
261 | 47} 55
5:2] 5:2
358 | 48) 5:1
ON STEAM-SHIP PERFORMANCE.
201
the Service of the “ Messageries Impériales” of France during the year 1858.
Consumption of
oil and tallow. 3
B= |
s
pele
n
° 5 Zz
Fe a) oO
Total. 3 Py
uo
= a s
i]
o oO
5 & S
Ay
kilo kilo knots
. (184943 |10°521
3774 | 0-214) 9:21
Mean speed estimated.
8:81
9°30
9°82
peed
of nine knots,
Consumption of fuel per
mi
le reduced to the s
oo He Be
ict
78
352
iS)
Go 09
—
02 GO
303
329
bo
=I
or
291
SSSs
2 8 6
© He O>
Co poe
Nol &)
=
35
287
246
296
300
348
458
402
359
381
450
429
298
311
308
332
275
269
282
275
277
354
297
224
232
224
499
586
293
401
359
445
287
211
16782
342
Distance run with 1000
kilogrammes of coal at the
speed of nine knots.
métres,
13,517
14,684
15,766
16,939
17,729
18,311
16,878
20,181
14,181
13,741
14,025
18,843
18,299
13,096
14,096
15,592
19,341
22,547
18,713
18,472
15,962
12,673
13,804
15,484
14,575
12,338
12,945
18,639
17,820
15,494
16,715
20,165
20,595
19,668
20,160
14,723
15,667
18,652
24,802
23,856
24,781
11,120
9,469
18,985
13,851
15,460
12,465
19,318
26,208
|
31,295
16,945
202 REPORT—1860.
Appenpix IT.—Taste 1. Chester and Holyhead Railway—Steam-boat
Express and Cargo Boats, under regulated conditions of Time,
Passages.
No. Average Agius
of rate of jweight
Vessel. Date. trips ed | “pn
run, miles. |valves.
5 1859. hm h h lbs
Eupress: 1 Jan. to 31 March ...| 73 | 8 24%) 4 0 | 449 | 13-40 | 1
reek 1 April to 30 June ...| 47] 7 380] 420 | 4 37 | 1364 | 15
eg ta hota & 1 July to 30 Sept. ...} nil.
1 Oct. to 31 Dee. ...... 36| 526| 424 | 449 | 13:08 | 15
1 Jan. to 381 March ...} nil.
Carebtia 1 April to 30 June ...| 836 | 5 29] 417 | 431 | 18:95 | 15
a sr 1 July to 30 Sept. ...|75| 516] 413 | 427 | 1415 | 15
1 Oct. to 31 Dec....... 44| 555| 421 | 441 | 1845 | 16
1 Jan. to 31 March ...| 81 | 7 28%} 4 6 | 445 | 1326 | 15
ate 1 April to 30 June ...| 34] 6 48] 416 | 440 | 1350 | 15
ware ards 1 July to 30 Sept. ...| nil.
1 Oct. to 31 Dec....... 41| 615] 420 | 449 | 1308 | 15
1 Jan. to 31 March ...| nil.
1 April to 30 June ...| 37] 5 0} 4 7 | 430 | 1403 | 10
Telegraph ...... 1 July to 30 Sept. .../83| 6 7] 411 | 4 40 | 1350 | 10
1 Oct. to 31 Dee. ...... 40| 6 O| 427 | 458 | 1268 | 10
Sarge: 1 Jan. to 31 March ...| 77| 917 | 5 40 | 6 44 | 1039 | 15
hee 1 April to 30 June ...| 76 | 9 27] 5 44 | 6 28 | 1083 | 15
oir ae a 1 July to 30 Sept. ...| 63 | 8 33] 545 | 635 | 1063 | 15
1 Oct. to 81 Dec....... 77|1215| 540 | 6 47 | 10:31 | 15
1 Jan. to 81 March ...| 26} 1115] 615 | 755 | 884 | 12
1 April to 30 June ...| 87 | 9 25 | 555 | 6 22 | 10-41 | 12
sors 1 July to 30 Sept. ..... 75 | 12 45| 6 0 | 727 | 939 | 12
1 Oct. to 31 Dec. ...... 49|1335| 635 | 816] 846 | 12
1 Jan. to 31 March ...| 71]10 O0| 715 |] 8 3 848 } 10
1 April to 30 June ..| 7{| 8 5| 7 O | 728 | 9:37 | 10
bess! 1 July to 30 Sept. .../ 28/1115 | 6 O | 6 57 | 1007 | 10
1 Oct. to 31 Dec....... $9). 11-15'-615 | 738 (1937) 18
1 Jan. to 31 March ...| 56113 5| 545 | 656 | 1009 | 12
1 April to 30 June ...| 65 | 735| 530 | 6 14 | 11-23 | 12
1 July to 30 Sept. ...| 75 | 730| 520 | 6 7 | 11-44 | 12
1 Oct. to 31 Dee. ...... 91 | .8 20} 5 20 | 6 30 | 10-76 | 12
ON STEAM-SHIP PERFORMANCE, 203
Department.—A Return of the Speed and Consumption of Coal of the
Pressure, and Expansion, for the undermentioned Period.
Coals consumed.
Average
Proportion of Per trip Per hour Per hour
pressure] steam in cylinder. | including | including | exclusive of Remarks.
aE getting up raising raising
steam and | steam, bank- | steam, bank-
while lying ing fires, ing fires,
at Holyhead. &e, &e,
Ibs. tons cwt. Ibs. |tons cwt. lbs. |tons ewt, Ibs.
ir) iS a 121112 | 213 47) 2 30| * Heavy gale, W.N.W.
bo b
13 | f¢and none | 111714 | 211 40| 119 28| — Based engines.
123 | 18andnone | 1210 3 | 211 101} 119 79
133 26 11-15 37 | 212 11] 119 80
133 2s 12 211 | 214 33} 2 1 50
133 ze 138 17 66 | 219 28) 2 6 45
12 coe 13 138 59 | 217 65) 2 5 63) * Heavy gale, W.N.W.
19,|} “fzond2e | 12 998 | 215100; 2 3 98| Based engines,
103 18 1813 71 | 216 90} 2 4 71
HEPER fecetezs000...-: 12 17 60 | 217 15) 2 4 35
10 none Ther e | an A O82 oe lO
93 none 1418 25 | 219 41) 2 6 65
7s of) ISelswU 2S SS |p els ais
7 a 13 13 54 | 2 2 32|/ 114 12
7s 38 1415 96 | 2 4101} 116 78
7s a8 1413823 | 2 4 23) 116 O
103 none Sell64 | 11s 7 17 98
RENN fr cers << :-+-5s-- 8) 895621) ll 618) 4k
11 none GolD 28 \eil eT rAO 17 39
103 none Cha) ZU de ale ste) 17 88
9 none Qre2r dey ale 2ae72 isi alg
TUM Niece so. .00e. 102 6£.| tit) 16) V. 6 i
8 none 9: Te24-| 1 8+ 36) 1 3983
| 83 none 11 221 |} 1 9 48] 1 4 95] Norg.—Orders are given
to the vessels, in gales and
10 | 2nd grade ll 724/112 86] 1 4 45/heavy head sea, to ease
10 | land2 grade | 10 861 | 113 51} 1 5 10) the engines, which occa-
10 | land2 grade | 10 11 20 | 114 54} 1 5 _ 6/sionally increases the ave-
93 | land2 grade | 11 1812 | 115 39) 1 6 103) rage passage.
and full speed
204 REPORT—1860.
Appenpix IJ].—Tarie 2. Chester and Holyhead Railway—Steam-boat
Department.—Chester and Holybead Steam-boats’ Consumption of Coal
for the Six Months ending 30th June, 1859.
Total as shown
b
Num- Average mm, y
Th th Total f
Name of vessel. pees . = i pe i oe oe the sitar pair rasta
coal on board.
1859. tons ewt. Ibs. tons cwt. lbs. tons cwt. Ib.
Anglia. ies cose roma oF li iy df] 147315 78] 1458 8 0
Cambri March 31.
sao a June 30 ... 11 15 37 493 11100| 426 4 0
Bookin 2a. ho. pone 1313 591) 1532 11 47] 1575 13 0
March 31.
Telegraph ....... June 30 ... 12 17 60 476 8 92| 49812 0
Hibernia ......... pores 13 13 b4f| 210918 23] 2104 19 0
Hercules «........ Earring Sil Gfl) 533 18 94.) 585 15. 0
Ocean seve son a nie? Wi eoraie “0 | p28 Th
Sea Nymph...... Pet. ce Mgowar tls eae ee
8137 0 31] 8202 3 0
AprenpDIx II.—Tasre 3. Chester and Holyhead Railway—Steam-boat
Department.—Chester and Holyhead Steam- boats’ Consumption of
Coal for the Six Months ending 3lst December, 1859.
1859 tons ewt, lbs. tons cwt. Ibs. tons ewt, Ib.
Anglia ...sses.- {res | 36 | 1210 3 | 450 0108| 44917 0
Cambria ......... Pept 30 | Te aay eat |) Wsle1l eeyaaieg 1000
Sle RO {esr | 41 | 131371 | 56018111] 568 6 0
Telegraph ......\{ Dees | fo | 1413 25¢| 170811 60] 1688 3 0
Hibernia ......... {RPr sy? | 8 | i213 a3 f| 206015 91) 2074 16
Hercules .......-. SPE EO ee ty 1087 12> be | ames aes
Dcomtee ee {ree re dE
Sea Nymph...... ort a ie ta ie + |; 1852 1b 1d iaeeeceee
9820 14 27] 9823
205
ON STEAM-SHIP PERFORMANCE,
*‘sUTeTOY
— |—_—$———$ |
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————
soouisug ys —SSCSCSCSCSSSSOSOOOOSOCOCOSSCOSSSSO:~C~CS TATU QUITTING,
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“euUBUe 0} youd pure OsteredeA 07 vueneg woz osvoA v OF
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206
2
ON STEAM-SHIP PERFORMANCE. 207
Aprrnpvix JII—Tasrez 3. Peninsular and Oriental Company's Engineer’s
Log.
|
aoe: 2
4 o 2 2m 3
i) 1 eH u = H Cay Se fe)
q m ns a a 3 sv rc) o.|9
3! 2 a] a a see I are es ‘dd _Joslofl/e. n
dial & | 23] 8 |E5] & |3s/84)/ 88/238] a8] =
B/Si/o; ® ee S| SB Sa |Gopeang let | as (0) =
Date. o|e v 3B 10'S as} °o © | ssh hy bservations.
O} ey a 2 S) 2S a = ee ad (eo Us = |
Hels] 6 | os] ss] © l|eS| oe] 89] BE) BS] 3
Bao Af SiS (ier | Se are |) Smee acy el eae
o| 3 ya | = 8 & z O°} 90] &
a) eB |g Bere patie oie
o Ea iS)
AppENDIx II].—Taste 4.
Yard.
Report of trial of Her Majesty’s steam vessel
Date
TIRE TIRES coc etic ccs sa ccece cece catesecececsavastevevedess
REED Mee, Sync detache cakes eIdeehecd sa havadeasd divas
Draught of water... { “Aft
_ Number of revolutions of the engines ...............6.:00000
BreRSHeR OU Mateby VALVE. .......c6ssccsccsesececeesseccacessensons
MURR TE CONCENSCES « oi.cc5sascdedet odetaceLobadscencoetcdecass
merower-as shown by indicator .............cccsssccsccseneseteeees
o
SRMES DEE C res tate apd svdcdocs tee. fa cbs deehewsesecasetuedaneds
Indicator cards and tracings are attached to this Report.
Remarks as to the performance of the engines, boilers, &c.
Revolutions of aie 7
No. of runs. exigines per minute. time. pore Mean speeds. peed
Min. | Sec.
| | EE
Knots mean
| of means.
[Note—Appendix III. No. 5 carried to bottom of Tables opposite page 216.
-
208 REPORT—1860.
ApprenDIx IV.—Tasce showing the Ratios between the indicated Horse-
indicated Horse-power ;
Name of vessel.
VESSELS OF THE Unitep States Navy.
Niagara (screw) Performance in smooth water
Place and nature of performance.
Ordinary actual performance at sea under
also, between the grate and heating sur-
Statute miles.
$i. | Voasinenniesnabuas esas <ch’s cdadbaasnwe neve’
steam alone.s.sc.<cscs-cccespaees eee eee
Sic \ weadacemerpenne ens haces ieiadeshoweveceen Ditto ditto, steam and square sail combined|11°51
Ay. A avasgestpasenes seadatensersesdaesbadenseds Ditto ditto, steam and fore-and-aft sails...| 8°55
ry) apbboseacastagcdo pce conenerecn et Conds Mean of the above sea performance......... 9°75
Massachusetts (Screw) ....ssseceecsersereesees Performance in smooth water ............00+
ary i, WRI Gabor cnoatco. cote boscodoceantiqanc Ordinary performance at sea under steam
BIONE ...,.0%.se0cceekeasists's deus sepanctnceoeee tet
Sey Neha ciueaectat entre tears ieene asec Ditto ditto, steam and sail combined ......
Be CORR ees Necacemmconeamnedsas sent Mean of the above sea performances ......
VessEts or THE Roysn Navy.
attler (screw ))i.ss-cccsossteccese<teonsvenosu0 On trial, Thames, Sept. 5, 1844 ............
ST lo rets tenia scae caece cat van chimtenatlenwes Ditto ditto Jan. 1845 ctasseecnaceen
Fy) be casduenececcietedea teres d-cussauacecedensd Ditto ditto Sept..5, 1851 .o.....0.0.2
Sate WE cnet OM rcahnaek Glan de tenceetakeousasedes Ditto ditto Sept. 5, USS] « Stegivessask
PiNdeMN(SCLEW)|.sece0— cavsmastesaseeaseeeesa4 .|Ditto, Stokes Bay, Oct. 20, 1857 ............
sh RAPIER EOE Corer Tee Mercreconcne ey ‘|Ditto ditto Oct. D1 ie hee
Reh ME MsiewCecscssaesageteceteuncuesevepeeess as eae (Ditto ditto Nov 757.45 ee
ay VL besiae canhapacscerages cece nants tentberst Ditto ditto Dee? 1, ae
Phe Heaton eet coccr er scl Oaeae Ditto ditto Jansd 1858. ose
gy was thversh Scents oss wetese neotauee ease eS Ditto ditto April 16, 1858
WOVIS (CREW)... scrsnocsvecderspate ce tesecteer se Ditto, Stokes Bay, May 27, 1859............
3» (with common screw)...........+2+00++ Ditto ditto April : 21, 49, ecnuranaceel
y, (common ser#w increased to 20) ...|Ditto ditto May 5,— 3, ieescnerete
» (Ditto, with two foremost corners
CUE NSED)) Paes oa de eee ep eee ede set Ditto ditto May 9, %,,. Weeseteue
», (Ditto, with four corners cut off) .../Ditto ditto May 23, 5; sectesstacee
yy (TEENS RCKEW)!.;... accesses anesedee Ditto ditto May 25, 5, saeeetee
» (Ditto ditto) ..|Ditto ditto May 27, 4, ss.sseerees 14 130 12-266}
» (Ditto ditto) Ditto ditto dune $3, 5, sitvscateae 14:006 |12°15
Marlborough (screw) ...sccsccecceeseeneeeees Ditto, Stokes Bay, June 1, 1859 ............ 12-94
Bi es Soest ee ae Ditto ditto June 2, 4, sserseeveeee 12-92
_ (with half-boiler power) ...|Ditto ditto DUNE D, 59 cevbecnanare 10-62
A Ds 2 ae ee a ee Ditto ditto May 28, <5; <cbvecsweeee 12-24
Mersey (Screw) <cte.0s<soecessacscosevevavouses Ditto, Stokes Bay, March 23, 1859 ......... 15-31
(Renown: (screw) Sccseveecaceetvotneatwercas ies Ditto, Stokes Bay, April 19, 1858 ......... 12-902 |11-2 ©
Pe Pree SAM nS test ishicerd: notice Ditto, between Sheerness and Nore, Oc-
LODER Og Ope ssacees «+. cosets suze saaceaneorsee 12-533 {10-88
$50. | levesaswaies tc kocia ee gate eee OR ERT CEE Reon Ditto, between Sheerness and Sunk Light, 5
October S07 feac.s.ccer.ceceoscne saeealeee 12-533 |10-838
j5: .. cemvarapiebean semnebercevoubpans emt netors Ditto, between Sheerness and Swim Middle, |
October, SO: TBAT. wins sisecgacacsnnceneumens 14-573 |12-65
Oy. hesdaccutegabanecereeccesescenetmeetmenee es Ditto, down the Swim, October 30, 1837 ..
-|14:573 [12°65 —
oven
ON STEAM-SHIP PERFORMANCE. 209
power and the Grate, the Tube, the other heating and total heating surfaces and the
faces, and between the indicated Horse-power.and the Coal consumed.
. ic} fe} o * 5
>) . Pr ene ap o obo fet tH
Horse-power. og ee [es] 38 | ac oo S as | os Sy g.
= -— Ps oF CE 62 "39 EPPS BSeé aa cs] as
=0 se BO Rie) eee (ea as @H be ge. 3o.D
sa 22 |Hal Ba aon | $3 2a ne 2° esh on
—<———— a. Sem 57 st ago and On a2 [me] ae) oH
32 So ag a? CE we oe HO mod Sd e go
: Be | ge |os| $2 | 888 |a88| S2 | $8 |) BES) SBS] Se
Be d Ba | £3 |sa| 4 (S25 /8e3'| $3 | S21 888] Fee] Fe
3 g So | Sg | ho! =o leek loot] H8 | oS | sea] Saez] Ss
S] d ox S [es] SB ogo] °30| Sm 29 a= HHS ot
g 5 23 2.8 | os a cosa | ofa = °° on asa @¥
EI eq jase ios | 29 |S 28 gS | 88/48 eS aO
4 A es a8 BS) $3 ae a ‘S @n 3 2) cd Sa
a A | a4) al | & i é ma | § =
: | Ibs. | Ibs. | Ibs.
1955-09 | 700 858 | 2-793 | -247| 6-556) 2-192) 8:748 85°386| 334) 3-529
879-28 | 700 796 | 1-256 | 55414577 | 4873 19-451 |35°336| 334) 4-617 |41-813| 9.058
77365 | 700 “905 | 1-105 | -625 16-567 | 5-538 22-107 \35°336| -334) 4-904 42-743 8-716
837-31 | 700 *836 | 1:196 | -57815°308 | 5°117 |20-426 |35°336| 334) 4-987 |42-156) 8-452
824-48 | 700 849 | 1:178 | -587\15-546 | 5-197 |20-744 |35°336 |- -334| 4-790 |42-269| 8-597
(240-74 50° oe axe toll
% (|10-280 10-281 |28:448) ... | 4-029
—-168°81 30: oat w. =| 514 ie 14-661 |14:661 |28-448} ... | 4-401
149-61 ae ioe ... |°988) | & | |16:543 |16:543 |28-448|) ... | 4-491
16254 set bars .» | 585) ) & \115:227 115-227 28-448} .., | 4-429
428 200 467 | 2-140
436°7 200 “458 | 2-184
499-2 200 “401 | 2-496
519-2 200 385 | 2596
2324-42 | 800 344 | 2-906 | -234) 5-131) +991} 6-122 26-16 193
2325:96 | 800 *343 | 2°907 | 234) 5°035| +987) 6-022 |26:16 193
2663-60 | 800 300 | 3°330 |-204) 4:478| +865 | 5°343 |26-16 193
2587-50 | 800 *309 | 3°234 |-210) 4609) +894) 5:503 |26-16 193
2685:04 | 800 “298 | 3°356 | -203) 4441} -858)| 5-299 |26:16 193
2979 800 268 | 3°724 |-183| 4:004| +773) 4:777 |26-16 193
3091 800 "259 |3°864 |-176| x we | 4659 [26-47
2921-2 800 278 | 3-652 |-186| ... we. | 4:929 |26°47
(2788-4 800 287 | 3486 |-195) ... ... | 5°164 |26°47
2884-4 800 | -278 |3-606 |-189| ... ... | 4:992 |26-47
2920-32 | 800 | -274 |3-650 |-186| ... we | 4:931 126-47
2825-6 800 *283 |3-532 |-192| ... ... | 5-096 |26-47
3091-1 800 | -259 |3-864 |-176) ... ... | 4658 |26-47
3009'03 | 800 | -266 |3-761 |-188| ... ... | 4:786 |26-47
3022 800 265 |3°778 | :180| 3:947| -762)| 4:709 |26:16 193 |
3054-26 | 800 *262 | 3°818 |-178) 3-905] +754) 4-659 26-16 193
1722-08 | S00 ‘A465 | 2-153 | 316) 6°926| 1-338} 8-264 |26-16 193
273894 | 800 292 | 3-424 |-199| 4-355 | +841 | 5-196 26-16 193
4044 1000 247 | 4-044 | -168) 3:702| +736! 4-438 |26-40 198
3183 800 | -251|3:979 |-171| « | ... | 4524 126-47
2864-75 | 800 | -280 |3:581 |-1901 ... | ... | 5-027 26-47
2759-95 | 800 | -290 |3-450 |-197/ ... | ... | 5-218 26-47
2837:36 | 800 282 | 3-547 |-192! ... we | 5'075 26-47
2793 800 286 | 3491 |-195) ... vee | 91156 (26°47
ao Particulars of the tube-surface were not furnished by the manufacturers of the engines.
o0U. P
on
210 REPORT—1860.
TABLE (continued).
Speed.
Name of vessel, Place and nature of performance. z
F | 2
= S
3 |
s
m2
Renown (screw) .......csscssccueeeneeseeeeees On trial, Stokes Bay, March 15, 1858 ...... 13-167 |11-43
» (with half-boiler power) ......... Ditto. ditto ©) March 16-5 ers... 10°535 | 9:145
Ditto ditto, “April Oy syn eseseceee 13-611 |11°815
Ditto, Plymouth, August 22, 1859 ......... 14-97 {13-000
Ditto, outside Breakwater, Oct. 7, 1859 ...\15°16 |13°160
PANTERING (RCYOW): scccsesqessctaatiabiescoses eve: Ditto, Stokes Bay, April 9, 1858 ............ 10-71 | 9300
MVE NGCFEW)! ipessshvusdrasspasengroseyesoue ++ Ditto, Stokes Bay, April 29, 1858 ......... 10:68 | 9:270
Hee: (SCLOW)). i.>ssbcatancnsdosesscaseeaeay sens’ Ditto, Stokes Bay, April 13, 1858 ......... 10:68 | 9:270
Ditto, Stokes Bay, April 28, 1858 ......... 10:77 | 9:350
Ditto, Stokes Bey: June 20,1858: 2s..4.- 13°52 |11:736
..|Ditto ditto. dune!S0/-9) 3) eeeee = 12-48 |10°794
Ditto ditto July 2, ee ree 12-70 {11-025
Ditto ditto July 6, i Abetesees 12°56 {10-908
Ditto ditto July 8, bye ete 12-71 |11:038
Ditto veiaitho) J uly l Die ss. eset cece 13°29 {11-536
Ditto in Basin (Keyham), Mar. 28, 1859
Ditto outside Breakwater (Keyham) May4,
PBB: ova. <i} sbaes hs s0ueaeay aay eeeoe © ees area
Ditto in Basin (Keyham), Sept. 6, 1858 ..
Ditto outside Breakwater, Sept. 18, 1859...
Ditto in Basin (Keyham), Sept. 1, 1859 ..
Ditto between Sheerness and Sunk Light,
March’23;, 1858 vcsiv.s. theth.t8-s-ereaeeee 11:60 |10:068
Ditto outside Breakwater (Keyham), No-
wember’'S, 1858) Sii.csi.ccisesses.erethncwens
Gentanri(paddle)| .. .s:2.5.6ssc.+ee-.¢eegreeoee Ditto in Basin (Keyham), July 1B, 1859/7. Mers-0
Sy | DRE a esi sutiwascipeeadecssumesenenmedest Ditto outside Breakwater, Oct. 22, ,, Ae
Tuidustrys (screw), <siens+:capsbaresrssbenepeoee Ditto Long Reach, Jan. 12, 1858 ......... 8-41 | 7:300
Fire Waibocrencaddonanicode 1 nos en isg sa: Ditto Lower Hope, Aug. 24, 1858 ......... 10:50 | 9-120
Bulfinch (screw) .......sceccccsesssssereeeres Ditto, Lower Hope, March 5, 1856......... 10:13 | 8800
= (Griffith’s propeller, with in-
clined blades) ........ srarsecess Ditto ditto June 24, 1857 ......... 9-71 | £423
: (Ditto ditto ditto) ...|Ditto ditto dune 26, “,,. 1 sieae 9:36 | €-121)
3 | (Lowe's propeller) .naee eee Ditto ditto Sept. 10, |, ae 8:57 | 7-442
. (Ditto Gitto)) ....0s-steeeeeuens Ditto ditto March 20, 1858). ce: 9:83 | 8534
+ (Medwin’s propeller) ............ Ditto, Stokes Bay, July 8, 1859 9: 8-073
+ (Ditto reduced)............00es-05- Ditto ditto March 2, 1859... 7-249
» (Philp’s propeller) ..........00... Ditto ditto Julyl, ,, 7-989
» > ( (Ditto Ydilte): 7... Aes Ditto ditto Sept.27, ,, 7612
eS (Hirsch’s propeller)..........:.... Ditto ditto Oct.13, , 8-015
» (Ditto GILLO) sh seetepevenssse se Ditto ditto Feb.24, ,, 6843
ON STEAM-SHIP PERFORMANCE.
TABLE (continued).
211
Horse-power.
fa | 3
3s 4
“|
| z
2754-64 | 800 .
1429 800
31826 | 800
3617 1000
3992 1000
2939 80
299°5 80
303-6 80
299-8 80
1166 350
1090-88 | 350
1089-60 | 350
1266-9 | 350
1174-88 | 350
1019-68 | 350
1195 600
1436 600
258 300
408-6 | 300
480 300
453124) 220
394 220
1122 540
954 540
2616 80
317-4 80
283 60
24062 | 60
21650 | 60
222-67 | 60
241-48 | 60
196-82 | 60
223-90 | 60
220-13 | 60
211-62 | 60
24060 | 60
199-68 | 60
_ Ratio of nominal to
indicated horse-power.
ea)
fre =)
o_
Ratio of indicated to
nominal horge-power.
3443
1-786
3978
3617
3992
3674
3744
3791
3748
3:33]
3117
3113
3619
3357
2999
1-992
2°393
860
1-362
1-600
2-059
1-791
2-078
1-767
3:270
3968
4717
4010
3608
3711
4-025
3280
3731
3669
3527
4-010
3328
rate-surface to
d
horse power.
Ratio of
indicate
pod
oO
io?)
&
s
: 8 fa | 83
& 9 18se/] se
qT “4 Oo 3 v
#2 | ces | SEE
SS |Sey|see
Hg |ask| see
ed |stn| gee
IE Pe a e a
5:240
10:077
4°525
* 5:02)
eh 4:549
4:627| -476| 5:103
4:°541| +467] 5:008
4:479| -461| 4-941
4533) -467| 5-003
4-819} 1:089| 5-909
5:152| 1-165] 6316
5:157 | 1:165| 6°323
4-436 | 1:002| 5:439
4-783 | 1:081| 5-864
5 867 | 1-209) 6-579
6:587 | 1-889} 8-477
5°482 | 1:572| 7-054
8-981
none | $442) 5-442
none | 6:259| 6°259
3°863 | 5°117| 8-981
4-544} 6-018 |10°563
4556) °906| 5-463
3°755| +746} 4:502
x 3'943
4:638
5155
5-012
4-621
5-620
4-984
5-069
5:274
4-638
5:589
Ratio of heating surface
to grate-surface,
18-13
18-13
33°59
33:59
33°82
23°82
32°631
32°631
32631
\32°631
32°631
32-631
32°63]
32-631
32631
32°631
32'631
&
Ratio of other heatin
surface to tube-surface.
103
103
103
103
226
+226
226
226
"226
°226
286
286
1-324
1-324
198
198
* Particulars of the tube-surface were not furnished by the manufacturers of the engines.
rhour |
1 cy
a | ag
BS Tex
ke | Ses
aU ng E
PSL) 8: 2,
sae =r
B23) £238
eg | eee
6.4 S44
Ser RO
49 3g
Ss] |E
o
|
|
PQ
Water evaporated per.
hour per Ib. of fuel.
REPORT—1860,
TABLE (continued).
Name of vessel:
Mercnant VEssELs.
cAmaelia (Paddle) sie wacece. se omence vei mane
Cambria (paddle)
Sconia | (pAddle)| veep tacstesaersess same hees toe!
eee eee eee ry
Tasmanian (screw)
Onn e nee nent enter eeaeee
TUTOR e meee eee e ent a ee eeenenes
Oneida (screw)
Callao (paddle)
Lima (paddle)
Ue eee ee ee eee ee re
OORT e eee e meee nese eeeeeeenees
Valparaiso (paddle)
Bogota (Paddle) i ccsevescsksccsesscgasernars seek
San Carlos (screw)
CO er Cee eri
Guayaquil (screw).......sssccccsssssseseeeaeees
Erminia (screw)
eee eee ee eee eee eee
John Penn (paddle).....5.....0...sesvereaceee
Speed,
Place and nature of performance, g
Fe
z
| a
m
|
‘Mean of six special trips on ordinary
| service between Holyhead and Kings-
town, 29th September to 3rd October,
1B D4: ss xs deckvasacgihes aca, eae ee 14:93
Ditto ditto, 22nd to 26th May, 1856 ,..|14-07
Ditto ditto, 17th to 21st May, 1855 ...|15-68
Ditto of two trips, 29th May, 1855 ......... 15-24
On trial, Stokes Bay, March 13, 1854...... 15°86
Ditto ditto January 22, 1857...) ...
Ditto ditto March 4, 1857 ...... .
Ditto, Stokes Bay, April 21, 1859 ......... 15:31
Ditto, Stokes Bay, June 7, 1859 ............ 16:08
Ditto, Frith of Clyde, July 8, 1859......... 16:01
Ditto, Stokes Bay, August 1, ,, ........ 16-60
Ditto, Stokes Bay, June 15, 1858............ 16:42
Ditto, Stokes Bay, July 27, 1858............ 14:86
Ditto, Glasgow to Liverpool, Oct. 22, 1858.| 14-86
Ditto, Liverpool to Kingstown, May 20,
1859
Ditto in the Clyde, Sept. 16, 1859
eee eee eee eee ee eee eee eee eee rer)
Ditto, Glasgow to Liverpool, Sept, 22, 1859.
Ditto in the Mersey, February 20, 1860...
22,
Ditto, Glasgow to Liverpool, March
1860
FOR enna reenter eee n ween eee eeeeeteeseseesees
Measured mile, Greenhithe, July 6, 1858..
Holyhead to Mull of Cantyre, July 29, 30,
TSO8s.Sasngeks eeonhiee sa guase Ceawat aoe cee
Run in Lochs Ness and Lochy, Oct. 26,
27, 28, 1858
Dede meee e eee e eee eameereeereenes
eee eenee
Ditto in Stokes Bay, Oct. 12, 1858
Ditto, Lower Hope, Feb. 6, 1860............
13°82
14:40
13°54
13°82
10-67
11-49
9-48
ON STEAM-SHIP PERFORMANCE. 213
TABLE (continued).
= OV. ~ A q is ta
Horse-power. 2 3 28 /a8 £ 5 = ~ co E £8 8 3 3 $s
35 | SE [ses] 35 ge | ae ae oS reg iierey Eth, |) reise o
Be | de ($21 $2 | S8olsae) 82 | #8 | eee} ses] Bs
<3 = Fe | &$ |e2| 23 |Seh|set| 2 | $2 | es2) Ree] 84
2 & Ge be 5 Seay te pales a3 So BOS] Fad aaa}
3 | os og | he] AE |eoklwseok| 8 5 ao) sag o 6,
S B | £3 | g8 [38] Se | cae] ces] 3&1 $2188 | sek] ae
3.2 $ S28 Sa eae ‘Be Cs Sse | 5 2° =
4 a ae Fe g EE se lé 2 | g2 3 as 3 & |e4 a
|
Ibs.
816-07 | 330°52| -405 | 2-469 |-196) 4-769} -558) 5-827 |27-17 117| 6-837
995-35 | 392°10| -394 | 2-538 | -166) 5-544] -452| 5-996 136-17 ‘081 | 5:787
93418 | 379:92| :407 | 2:458 |-199| 4:943] +627] 5-571 |27-98 *127| 6-679
| 1165-98 | 448 384 | 2:603 | +142) 6:3382| 1-377 | 7-368 |51-68 164) 6-69)
ase 800 ee Soya iliecoe| iene noe w. (47-91 | 1-106
coe ee eaten Poet tes Rec ... |47-91 | 1-106
| 2396-44 | 800 3834 | 2-995 | 217) 3°346| 3-703} 7-049 |47-91 | 1-106 | 3-739
1088 250 230 | 4°352 |-163) 4-044] +925) 4-960 |30-39 228
2940 764 *260 | 3848 | -202) 4-998} +872) 5-871 |29-05 174
{29285 | 774 264 |3°783 | -193) 5-042| 1-259] 6-302 |82-55 249
3790 774 ‘204 | 4897 | +149) 3-896| -973| 4-869 |32°55 249
‘| 2800 550 "196 | 5-091 | -182| 3:768| +537] 4-306 |23-6414| +142] 3-000
FE 1912 450 1235 |4:249 | 222) 4:789| +795 | 5-584 |25-17 166 | 3-514
11050 320 805 | 3:281 | +133) 1-904) 1-142] 3-047 |22-85 600 | 2-133
| 1160 320 276 | 3°625 |-117| 1-465} 1-293} 2-758 |23-53 eee | 2615
800 320 “400 | 2500 |-162) none | ... | 3-000 |18-46 -.. | 3080
{1100 320 *291 |3:438 |-127|) 1-318} 1-091] 2 909 |22-85 “600 | 2-036
500 120 “240 | 4:167 |-152| none} ... | 4:400/28-94 wee | 25852
| 600 120 ‘200 |5-000 |-123) ... | ... | 3666/2973 | ... | 1-866
157:09 | 50 | -318 | 3-142 | -287| 4-697/ 1-311! 6-009 |20:90 | -279
15877 | 50 | -315 | 3-175 |-284) 4-648| 1-297) 5-945 20-90 | -279
160-84 | 50 | 311 |3-217 |-281) 4-588} 1-281! 5-869 20:90 | -279
5459 | 30 | 550 / 1-819] ... | 8172! 1-702} 9:875|38:174| 208
798 | 150 | -188 |5-320|-162, ... | ... | 4-229
214 REPORT—1860.
AppENDIx V.—Letter from Mr. Archbold, Engineer-in-Chief, U. S. Navy.
Office of Eugineer-in-Chief,
Washington, D.C., May 12th, 1860.
Srr,—I have the honour to transmit herewith, an abstract of the perform-
ance of the U. S. Steam-sloop ‘ Wyoming,’ under steam alone, and under
steam and sail, on the passage from Philadelphia to Valparaiso, Chili, col-
lated from the logs of the engineer department of the ship.
Iam unable to give you any account of her performances under sail alone,
as in these logs no note of the sail is made when not under steam, and the
ship’s logs are not sent to the Navy Department until the end of the cruise.
No trial of the ship was made in smooth water uninfluenced by sea from
which any data of value can be obtained. We do not try our ships at the
measured mile, the guarantees required of the contractors of the machinery
being on performances at sea, and for an extended length of time. The re-
sults for each day, as shown by the abstracts, are not assumed to be strictly
correct, as the data from which they are calculated are taken from the ordi-
nary observations of the engine-room, subject to errors and inaccuracies
unavoidable when the observers are so many, on duty for so short a time,
and when attention is necessarily engrossed for the greater portion of the
time in the care of the machinery. But as the errors are as likely to be on
the one side of the truth as the other, the average and means will not be far
from correct.
Indicator diagrams were not found in the logs for each day, which will
account for the omissions in some of the columns, and there was but one set
taken during each twenty-four hours. The horse-power for the day was cal-
culated from these diagrams, correcting for the average revolutions for the
day ; and the horse-power for those days during which no diagrams were
taken, is calculated from those taken on days when the circumstances of wind
and sea were as nearly similar as could be found. The force of wind is
expressed in our logs by numbers, as follows :—O, for calm; 1, light air;
2, light breeze; 3, gentle breeze; 4, moderate breeze; 5, fresh topgallant
breeze ; 6, strong single-reefed topsail breeze; 7, moderate gale, or double-
reefed topsails; 8, fresh gale, or three-reefed topsails; 9, strong gale, or
close-reefed topsails and reefed courses; 10, heavy gale, or close-reefed
maintopsails and reefed trysails; 11, storm trysails, or storm staysails; 12,
hurricane, or when no sail would stand.
In the column headed “ cut-off,” the figures indicate the distance in inches
the steam followed the piston.
The apparent discrepancy in the consumption of coal for the days between
October 25 and 31 inclusive, and some of the columns of which the coal
was the dividend, arises from the distilling apparatus having been in use,
making fresh water for ship’s use; the amount of fuel due to the water
freshened having been deducted before dividing. It should be remarked, in
justice to our system of surface condensing, that the vacuum shown by these
abstracts is not so good by from 10 to 12 per cent. as has been obtained by
the same engines on former occasions, or by condensers of the same class in
other ships.
I trust you will find in the abstracts everything necessary to the object
you have in view, and you may depend upon the truthfulness of the result
as nearly as they could be obtained from the data we have before us. We
have, in common with your Association, felt the want of systematized
authentic information upon steam-ship performance, and should feel obliged
by the receipt of any facts in relation to any of your modern vessels of war,
ON STEAM-SHIP PERFORMANCE. 215
which the plan you have organized has developed; in return for which we
shall be happy to render further service if desired.
I have the honour to be, Sir,
Your obedient Servant,
SAMUEL ARCHBOLD,
Engineer-in- Chief, U.S. Navy.
Vice-Admiral C. R. Moorsom,
Chairman of the Committee on Steam-ship Performance, British Association.
Description and dimensions of the Hull, Engines, and
Boilers of United States Sloop ‘Wyoming.’
Hutt.
ft. in.
Cpe SARA RACE AS ace crcocrortr rere ere rec 232 9
Length SUE APE SUCCAS sector cre tsecodethsad acnsseccasaascmessicos | 209+” 9
Length between perpendiculars. spadsoer Saco ebeacesoaneos IOsgNe 198 6
Length of keel from back al of forward stern post...... 158 O
Width of beam, moulded.. dageaactteteccdtincstgenatedeg Oe Oe
Width of beam, extreme . LA SR ean OP ree Oa ie Ta |
Depth of hold . Seen clessinaieecaedudelich caslecwss tans tceren 5 Het PU
Space allotted to ‘machinery GonIGr ORO CONC OGL ANC. acc EAL COLOO ei meeN) eats:
Draft of water (loaded) forward..........cssecssesesscesecees Pes
Mreatmrot Water (lORdEd) Ait... eo... ecscecscveccsscsnsecenscess 13 4
Area of immersed midship section ..........cscseesereeees sq- 391 O
tons.
SUEMREE GP as oh Pus o8 ti chavo escieek Vdeleedowsetay anleiaidtides Wipe aTE
RIEL fee Ws cance ics aces oo soon cree ara icenessemedb ard gaens 997
err ebele Of CHANCE 65.1. 266 66s és ccs caccensstesecsenendac 17 ao
EMPIHIIEC OL (OXI 65 255.05. ca0cenacwecdins dcoacupugntebaddestas. 1a? 30!
ENGINES.
Two in number, horizontal, with double piston rods, and direct-acting ;
slide valves, and independent cut-off valves, and situated 76 feet 6 inches from
serew. One surface condenser common to both engines, containing 3000
square feet of tube-surface.
Cylinder, not jacketed, diameter............... 4 2
Cylinder, stroke of piston .....ccscceeceeeeeeese 2 6
The air-pump (one to each engine) is worked directly from the cross-head,
and consequently has the same stroke as the steam-piston. Its piston is a
barrel plunger, packed by a gland in the centre of the pump. The foot
valves of vulcanized rubber are situated beneath the plunger, and the deli-
veries above it.
ft. in.
Capacity of air-pump, one revolution............ eubic 3 3
Area of foot valves, one end .............s000066. 8G: 179 5
Area of delivery valves, one end .............5. 8q-» 270 O
There is also a cold water circulating pump to each engine of the same
dimensions as the air-pump.
BoILers.
Three boilers, with vertical water space tubes over the furnaces. Shells of
916 REPORT—1860.
iron, tubes of brass, placed two on one side of the ship (of which one con-
sists of a single furnace and is used as an auxiliary or “ donkey,” and to sup-
ply the deficiency of fresh water caused by leakage, &c.) and one on the
other side, facing each other, with a fire-room fore and aft between them.
ff.
n.
Length of boiler ......ccscseseeseeteeseeeeeasesee see eesunncenseeeseaes 94 9
Breadth, including fire-roomj.e,. 2ssssesksgas es. aue~= ase aetee Eee 29 0
Depth, ecclnsive Of BLEAMAATUM *. cate seme seosuds ose ceeen ease eee 107 2
Depth, inclusive of steam drum 10 ft. diameter.................- 14 @2
Fire-room, length) se. ccc case gecemens sos coals eieeslee ag ries eee eee ee 24 9
Fire-room, Width oo, sect ose ctele ieusiecuiscecea uenowsisacteas stesseceeee 8 6
Heating surface in all eariee se Beuekccsuee ser sceceoncs tithe ER EEaee sq.7890 O |
Tubes, malength ..).52,ccesencesnsasaot uss geeiieplosaace Seen meme 2 74
Tubes, pecans GiaMeter | sicscccsscsesosetecescs snes coe eeReeeenere Oe
Tubes; WP BUmver. <5... Yeh s scenes ones acs etecncss cpeacanaae 4.230
FURNACES.
ft. in
Breadth, except “donkey,” which is 2 ft. Gin. .....ccsesee see eee 3°0
Length .. Se eRe wreeioisrae bd bicision § oie selene Selenisealedce sa he aaa eee 5 10
Area of all grates . - es ae 242 O
Smoke-pipe, one telescopic, height w whieh’ up "(above grate) . 52 O
MAMELSL coe ech se alebere ces one cc caamicncc ances icin cah\sin'ae eae carey sae eee 6 10
ADGA, see cnaions sewieiaiaeesiesis pps seg pens aie petals anew
Least area between tubes in all boilers seresconsnonceveseecnsncsee SMe . GU Go
tons.
Weight of Dotlers (1.00... senasevssevesceves esnsnusseenes ouesvenunawee 74°75
Weight of water in Hellehen eco er O 41°37
ft. “in
Cubic contents of water space........:..sceccesssocrecseececoccecees 1484 0
Cubic contents of steam space....,.... Slate athacete Mee 1318 O
Contents of combustion Shambers ‘each farnace. soe acetate 6183 O
Distance of fire-bars from top of furnace ........cceeceeeeeeee ees 2 30
Distance of fire-bars from ash-pit . ......0c0000cassecuiceseressusvsce 1 4
PROPELLER, one true screw of brass.
ft. in.
INumberofsblades' ..,. sssececrecoeccss cocesteleanatiownine osloctiveonten eee 4 0
Diameter on SCLEW . ccaccecanecrmesetcese eee cies se ese won ceckeearneee Vas ’
WD AINeleriOl DOSS sc. csc cc sanaecor ientes teeta ce crcless souls cciumseanteee cee 1 93 @
Length .. sisindleve eS O0-4a TTR EEE Ee 2 6
Projected ar area aL ‘tight ‘angles alee axis. as <eevee BQaue e436
Total weight of machinery, spars, &e., with ‘water j in | boilers cease UD LIS oe,
Carries 235 tons Anthracite coal.
The coal used was Blackheath Anthracite of the hardest variety. Its
analysis, as given by Professor Johnson, is—carbon, 92°12; water, hydrogen,
and yolatile matter, 4°83 ; ashes, &c., 3°05. Specific gravity 1°477.
Avrenpix V.—Tase 1. Performance of Un\\ted States Steam Sloop ‘ Wyoming’ under Steam alone. [ To face p. 216.
Engin Boilers Ersporation
a
Wator-por.b,
||
4
|
|
ibe
1461] 20-4
1 » {1o99| 15a
107 t
Ww 2 130-36 | 10°82 | 49
bY H 3106-66 erin
10 1 NM
106 1 1s
83 1 21 119
72 | 14 965) 13-7 919
x 85 1, (1049) 21
3 + (100015 | $50 [190-4 161-84
a A 118:5| 0481] 7
7 2 liso5 1335 |
i | 864 [146-2/116-96
7 ‘ 7Al |199-7|111-76 5
138) 20 i iF 161-4 |122-66 he
641) 17/8 aa | it 1, [2000 14-2 |1716 3 \195:88 |11-64 | i ‘
17 | 8002 wh | 86 | 69-4) 23-09),..| 1066) 18:46) 86 a /1244 a
Appenpix V.—Taate 2. Performance of United} tates Steam Sloop ‘ Wyoming’ under Steam and Sail.
m 7 Eng | Boilers. |
g 3 gl, | 5 | =
4 ; g § | a|é : i ae | | :
: t j | sl alti (iat | m | ite (iba ibs ibe Be
8 152 2 | 73 11:35 | 7|1195 | aus | 30 918] 4077 | J | | All plain
8 M4 107 | 84 97311 lesan ell in 3] GS [9588 | \ea20 | eee | 3
198 MW 5 A eet lor 661 | 2467 | 8 :
5 i at 8303) 1265 [107 | 807/455 All plain, 9 hrs. 6150
152 0 en ih Joo? | 832 | 7-05/2083 |28 |246 |10 Fore & aft, 15.
155 8 allot fan 5 150° | 267 |203 | 95 | 33
12 73 | lomt |fo 264 | 331 95 | All plain
15 9 fe fc] er 175 |13 166 3:66 | Sib and staysails
log 8 o fon don 161 | 100-9 | 8147/2558 6 | Foro and aft
\s 7 152 ean [Non 139-2 | 830 | 902-96 3 | B44
15 7 » |o 1166 | 811 2602 | 39-68)
7 7 Ral asia fi 99-9 | 759 /448 |
70405 {Lh 66 Me oerrelliy 900 1087 | 768 485 Square
86 (508 [167 7 oi erase ican 8 | 986 93-3 a ||
| gj'w ay 7 8 wel il] cael eer sige | M1 Fore and aft. 6150,
0 55 1 a5 RS fae | on] ae || Be 11000 Wl | 19-3 | 836) 1763 5°67 ” |
05 6 | i 821488 8 who | ow | 4 ¥ [10 8588/1969 | 1004 | 947) 2118 538 All plain, 9705)
6 | Smooth. | 8/8 4005 |178 Vd j252 |10}171-7 | 5636 4 {787 2 [15352 ) 2102 | 1803 [lod | 455-1 | 8-92 | a9; Fors and aft. /6150
| | | 2017] 64 \377|7 893] 87 | 75 [2487)...| | 30 1328 $29) 28072 3-698 209 | 8-806 ‘|
Avvenpix W.—Tanr
5. (Brought from page 207.) Surveyors’ Return of Capabilities required by the $21st section of the Act 17 & 18 Vic. cap. 104.
(Issued by the Marine Department of the Board of Trade in pursuance of the Merchant Shipping Act, 1854 Port of
| | val What gana coald | wo of
Mama of spy ia | | Weight bunks carry, A required Namo and
Mis lu. Hike it, | Dimensions | Particulars of engines Doilers por inch, aire
regpuary, | | | No
= Whe | Tangth {Forward (Kingine-room — When mado |Description {Diameter of cylinder —_|When mado _|No. | |
| |Where | Broadth Aft (Register Whore Nominal 11, P. — |Longth of stroko \Where Description ] | }
=a i ] |Depih Gross By whom Paddle or scrow {Revolutions por minuto {By whom (Thickness | |
= — | ‘ch == aT ‘a 1 | may) | | a |
SuprLementary Arrenpix- See note
Tabfe showing the Trial Performance of the Steam-vessels ‘Lima’ and ‘ Bogota’ when fitted with Single Cylin
Also the sea performances of the same vessels under both these q
=
at end of Report, page 199.
der Engines, and after being refitted with Double Cylinder Engines.
onditions of machinery and on the same sea service.
=orsaango adler Gal
Force and direction of Average
- | i
runs
aioe ee scearaiog
practice
gy im Sa. . Knot note
L a I ¥ Randolph and Elder's On trial betw Northerly MW 6 270,000 1160 1350 12-00
p . i return 8, Iffsoo 38 [fresh breeze 786 0 Total 825
: } is steaming 632158
Lima Greenock to Liverpool 1851 | 1200
aance between Panama and Valparaiso, and return 5 to March 9, 7 806 1272 0 |
| Not
Bog w nd Liverpool Wwpt. 22, 1859 la 46 Abeam. |Varinble Short a 15 16 | ascertained. 1100 (Dist.|180)
between Panama and Valparaiso, and return ...{Dco. 31, 1859, toFol—. 91, 1860 750 20 | 0]
. Ls (On trial from Green Liverpool Jon. 1852 ea 1 '
Fitted gle cylinder engines pitta | 1300 123
Sea performance between Panama and Valparaiso, and return. ..,|Oct. 6 to Nov 734 3 | 1337 6 80
Enginos
aos iiss ee : 2 Condenser. | Air-pump. Piston Pregeore
rr feteam
rr | ind or deseripti Total = of eanic uum Preasurs z
x Breas al Poewant| Aft | tral | ter of hat sort u t + Tart] Kind of | Cubl Kind of Cubi ek ot poe x | teen den cylinder. | racaun
wheel | Paarsion ylindlers | stroke, |linders.| 4 sir-pomp. | cone engine | In fe
a ie hin | in C17] Peat | ace ee ; SS
SE 30 | ¥ | 12 | Peathering. } 40 (Patent 4 uble 4 Common. | Short slide and grid- ) 90 u 2s 21 32
ailistatlis | oral | cylinder . | | _ iron, area 24 by 6. | : -. ‘Z
26) % Ordina! 16 Side lover. 2ordinary,| 80 Ordinary | Hicks’s valves, short | 16 12} au
i = | par oa ae ” ” ” ” | cack. s | slide, 30 by rt a
ww 0 | 302 20} 1410) 260) 86) 31 4 12 | Feathering | 4.0 | f Patent double 50 4 |Common.} 250 | { Common | | Exhaust. short slide |
r 11 113 }12 ©: » | 86 5 <4 oylindor. Two52 fe me li single- steam gridiron, 90 { 37 23 33
86 3 | 9 rdinar e je 7 ake noting. } | aren 24 by 6, |
3 34 Ordinary.| 11 | Side love 73 | 60| 2 ordinary] 80 | Ordinary. | [ Hicks’s short slide, } 4
4 fall Wi i i ud ” cach » IL d0bys i Fe
Boilers
Dimensions of boilers | | Dimensions of | Cut :
Pr 4 | ee Apel mrightott| sceakemeerer | Uweakers || Doe wbiacon- | Distance | Distanor | Actual Tube Tes
ear | athe | w = man | Mageestnsnt | emmerrsnd | ffamtct, | fcr’ | min, fAtceary “he Namter and. | Load on | iio a Bate
ys oh. | . heating surtac oe IE bert f] Aangth. | Diameter.| Material | ofchimmyn | “Talee | Shue |
Z scape 7 = | . - | mn | cals jor an mab fe a "nh. im "Te ma VT: a sts = ———
26 ubular super 2 2 Total 100)|/& R 1600 6 ete Ld 5 | x a
1435 heated to 400° | i 2 5 \{ Tabs 1700 |) 480 o}as6 50 8 | 6 oO | 1,5 |
" Fi «|| Boilers 60} || W. . 2000 |} Tabe | 25 5 1, 5/diam. | 25 | 3024 | Purnishod b :
)\ 1] Other 1500 | » lon = Sy [aie i te fs Furnished by Mesers. Randolph, Elder, and Co :
4 | Tubular M0} 110 | 110 |ftotl 150)) 68.8. 1450 |19,7 bya] {Grate 252)) a | | | eal from log book of atic Beazs Navigation Company
5 50 |12, 7 by 3 { Grate 0 2 23 ‘ ‘ = goer |
iy No » || Boilers 80} | | WR. 2520 2 Hae: aBOuiH ‘ae alt ae ate | " 160 | 6 Oo 2 diam 16 | 6720 _ Consumption of coal por indic. horse-powor per hour =5:169 Ibs
2 : ee Bale iaie/ | eran eee Fleet) eee | | high. 870384 Extracted from log-book of Pacific Steam Navigation Cow pany
583 7 ” 5 =, oile liw.k2 Taube 2000 a |{2 0 |g 0 60 288 | 6 0 leo 6 2,
| (Boilers 60} | | W. R. 2000 » (ome itoof{te#oo Hao llta) 4 | ; }1.6°0" diam.) 26 | 2240 |Rurnished by Messrs. Randolph, Elder, and Co
‘ Tabular 10} 110 | 10 |r 150) l/c 1450 | 19, 7 bya | {Ome | | } | | wt 2279'S |Extracted from log-book of Pacific Steam Navigation Company
se) i eee » || Boilers #0}||W.n 2520 | ||,” hoaeneaaa PA TS Peet Re ee | Wdinm.| 16 | 6720 |e tion of coul per indic. h
| } || Other 1600 * aa) as: Hs 5 ‘ ; 3 72 onsurmption of coal per indice. horse-power por hour 60 Ibs
Jon 4/ long 3694 (Extracted from log-book of Paciflo Steam Nev featon Conia
vf
Hor ig PP
pes
|
‘est Vidiparion
oe
Press is Vahpursion, wd rota
locoe to Vrrent
to Valpuras, wd rears
E he Léverpest,
Se Saree ieee lane
fo ser vm
Lo he. Vises
Menesend Mile, Gresnhvito..
Maas of Caney
Mone 20, 8 ,
‘Aye 3 0 Ape 1, yd
Saty 0180
Fely 2 to wi, tas
One 8, 21, 3m, At
O28, tha
140 rats sti
here 10)
G28 onary
t
3 hears steaming
mig, BUOY with sale set
30) hurare stenting
Shonre
10
1A bets 44 min.
1 directly abesd d
; :
row 6 530, ine
to, light wind and fine
fo 56, light winds & fine
Variabh
Miderate
mtb ensterly Not
setae
Seat Wrens
ary tight
Northerly, fresh broexe
dateroas weather
| Light abend fir altern'y
| steam
Favours
Strip
Vortly fav
Linof,
i
Milerale
Moerate
With
Flatt
fariable
TA) berars 90 rai,
At boone
736 hore 46 win, Light head wind ded
U6 boars 9 ic,
208 boars Vb wi, | Laight bead wind,
6 min M5 ane.
Variable
Vb, with and opninst
With and againiot
With and against
5 bones 15 main, { ebb fs
a es Hill water
OT aninseneesiseminrsiinttie tiaras @ DOE
es,
| Flea 0
Doe
adverse ak
Smooth
|
| Moderate
|
Smooth
Moalerate
ie no
hort ea se
Light Nad sen
Heaxy 1 hours
Calo
Nonoatls
| (3 tone 9
0 | Upehoue$ |
[iste 1 6 |
1100
100 11.0.
70 00
18 10.0
70 0.0
ih 00
om 10.0
9 00
1K 00.
Table showing the Results of Performance on the Measured Mile of Seventeen Vessels of the Royal Navy
BRITISH ASSOCIATION. —COMMITTER 01 STEAMS
and in additiotheit 8% Per
of Twenty-two Vessels in the Merchant Servic
Wf
c
ml) T ib) PL In. hi
sim iF r Fis Pem|rcm| im | ‘
a | a | | | |
| 1 aso low 2 Jraft) | § Horizontal Condensie| 72
wi 70546 4 4 | UDinet Acting |
i TIES) ao , a |
| Teast |ene Dinet Acting Condensi] 245
4} oc Ditto ait ‘
1] 4 Pet iis dit
wea | 104 10 0 | 39 | wh
we7 | 107 |
| Pe
1133 |
ital |
784 |
betty :
12003 Titto j
| Trunk e | to
ira
0 0 ‘ | | su} Horizontal ma jo
| 25) 0 a) | Moraontat e fi
| Tht :
Thilo
i} | | | Ditto
r 0 » 6 | ‘Trunk fo
am 310 Dit
04 TH Traak e | io
ti ase :
r - Thito
i ; Taito
s Dit
: Tht
Tht
nes is | ite
: ‘ Horizontal 1
5 | trunk w|i
eh 7
Ditto
: Dilla
f mit
Thitta
Tit
| Kl
| ’ Ditto
i} | |
N ? o 24 |Com-l20 60 Oj Direet-seing Si oo
} 2]
inf HI 33 | mou. | Tht 00
| linea
i Ne
| | a10« a o| » 3 | | | Dit 24
109088 t o| 2» : | Dit
2s 1 |
1086 no | x0 0 | m2 H
12009 10903 | 200 | m9 H
17 038 ) ) 1 |
1483 4 2 2 ; i : |
11436 ( 12 10 312 13 2|3915|'3 0 len| 1a ee |
B10 tah jour | | |
10068 t1 O12 2 | | 1 50
‘ cs) W615 4 Levolgsci|cxs| ~ | tf lever ;
, 1) B15 3 pe ofS cits o| |
7a” 9 lk 9 1 0 6 | 110 Js 0c Wes: | rh “pS
719 2 23 2 7 161 330 {eau | | =
11 , 3102 4 70/4 0| 30 lens] ao | 2 | 2 [3 0
146 5 bz 8 170/% 0/3 0 ley 4 2 | al
200 135 0 30 a o|8 4 6 0 oli4 fae %} 2 | 1)o19 Y | | Horizon s jl 6
| 930 | 195 0 a ¢ 8 aj7 0 o;14aiag N 8\o18 4 | Ditto 1
j m0 om | iso | a Bal7u coleolraise| of 2] slow a | j= ||| pie ;
Ish 0 ro} 710/84 eolaolral|sa Puech ania 3) | | | | 5 aria: wie
m8 vio | iso | mo 710)8 4| boleoli sla Hlhera\ Rel eee: | || Bis
| |
| my | Nut am | otf a he 2 | Lis 2s .
| sons rain § ahs a} | | : Pras il mae
337 | Dy | 13 013 3 fas : Thtto
rd Hy A She | : 4 Duta :
| | :
| 5 Wok) 18710 | 20 fiseas] 9 0 | ea | | pee 00 2] Dooble patent cylinder... 49, (*
| v0. 5 wor | ar 0 | 20 2 feng) $108 | so | | asp 29 10.0 0) 6 10] siteteer 7h
osyia| os 103 | 102 7 | 27 0 Iieaag| 8.10 | 080 | et fo 00 06 0] Doodle Patent Cylinder | 52 1
049 wn | oa | oa 2 leap] 0 8 | 8 fo » | 6 6 Sito Lever mi
1" if | te sho 0 | ea [6 hs 00 05 0] Ditto 06
| a Peath.| ” Ditto
wot | aya cr ee a Z
| | 1035 | dane | sits ian |19'20 | ast0 | 8 actus] = [33] Date
| | | | ayo leheeh [97 10.0 0 5 '
| le vm | O| ae aloo cal nimi it 10 0 Side Love 108
| ww | 904 Jaouso las | 123m | ssa 6 | m0 0 | gq 20 6] 120 | mi ; Oscillating »
| a | Iss | elias
| 5} 5 Doable Cylinder yt
izFoo | | heal he 5) 16 Ditto ny
} | Jou o} 4 a} 16 si
mas | 1076 | | ho Jono} to 15 fara Sai he | 2
=, | Mio olbo 1 | Ditto pe!
| | 5 6 0}/S armed 6 ib oO | ¥
2 | 5 10 | 1 j arto} aso | 3 0 | 510] & O7/Sareld & I | Jom | | Trunk Inverted cylinders u
ee | | wire 4m. | 0 740 1 10} rio} a] av [610] & spore) ene og | js} | Direct-acting hed
: afar | 28 [510] 2.0 [soma tooo y | | vetiesl Sa
} 4 | 22 | 0 1x0) ||| e06. 0\ll aa We Peel oo here le oo | Vere trunk gare
40 | | oa | cl | fear el | "
| 00 andalph and. Ekler's
| Patent double cylinder
ju1o 1 10| 10 Ditto dite
soe Dilla ditto
hy {tn t0 | 1220 Tito ditto
{tt 10 | 1230
Me Ditto ditto,
anal THito ditto...
ene Ditto ito
Ditto
100 | ob om 0
wo om bnito (ne
TUITE) quae L ur
Dit
1108 | ine v0 | 105 0 Ditto
00,140} tine oof Lnverte, at an angle of a
enon a0 Dito atte | a
W377 vor Ditto
ure wa
Ga ‘ Thigh prema ya.
7 ba
‘Doable Cylinder .....
mt a6 neo
[GH ASSOCIATION COMMITTEE 07 STEAMSHIP PERFORMANCE
Sea Performances over upwards of 6000 Miles; and of Ts
Vessels of the United States Navy; together with the Particulars of their Machinery.
Me
== ———— ; DOILENS
- ———— ee ~ 7 Ll Di = = > = T * 1 hom F |
= , E )a| | a §s S.
3 f= aise t Oivnlenn | cana Frnt tack | Brook 0 ? r i i =
‘ : ts fave} a |e { 3 4 | { ‘ safe {a t ‘
. : 1) E [its | ahs - U0) I i
$ § 43 fara | 3] pie at 100 | 3 1 D: Di t|
r a : #100) 5 1 Date Ditto ed from Tih ee
i : s v0] vo] wc iva ‘ (c 7 ast ot | eed :
% , |
2 = | F ) Bxtratted from the A Table of
0 J Hae Sew
ot ‘ " 21h, 4. 20) o|t 1 »| si200 | 19900 00 |e ‘ c A 7
"i | i \ a| 0 ¢ 3} 1 Jno) 6
21 : 4 ‘ , t | Ne 11 as | a 3} Dat 1
: ot | to i a Dit Ditto
‘ nae ‘ 6 | a8|2a| p a
: a4 alo « i I 20
| som F rn ‘
5 } ‘ 2 | 3\ 0 a | 5) ou mit tt Ey
| er 2 : f 13 a aos r 77" iawn] 90
: : P
oli ' Int 1 4
== ‘ Dit
. 2 4 | s ( x 4 f f Two, 7) 1
~ 3 i i J
= a 0 sa) y | oft ae fills eal tesa ree Stabe. 1088 ‘4 om ta | 30
oh 0| a0] 2
D0 ; ‘ iy rr 2 wi} 8 One, 7°77
1
1
3 I I 20
u ( ‘ wr|s o|2 Tron. | One 29” diam, | 09
Tits 1 H ita mt ty
i z s
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LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA. 217
Interim Report on the Gauging of Water by Triangular Notches.
4 2 Donegal Square West, Belfast,
; 23rd June, 1869.
__ Dear Srr,—-With reference to the experiments on the gauging of water
by its flow in triangular notches, authorized by the General Committee at
Abeideen, I have to report, for the information of the Association, that, as
they have to be carried on in the open air in a field adjacent to a waterfall
at several miles distance from home, and as they require the formation of
ponds and the construction of measuring tanks, sluices, &e., and involve
careful and repeated observations continued often through whole days, fine
summer weather free from both rain and wind is almost quite essential, and
winter weather is peculiarly unsuitable. For these reasons, and on account .
of my duties at Queen’s College here, I could not enter on the construction
of the experimental works until the close of the College Session, which
_ occurred only on the 9th inst. I have now, however, got the principal parts
of the works constructed, and have got preliminary trials made, but I have
found it impossible to have the final experiments ready for the very early
Meeting of the Association which occurs in the present year. For these
experiments a grant of £10 was placed at my disposal ; and in order to meet
the costs already incurred, of which some, from the nature of the case, are at
present uncertain, I now apply to the Treasurer for the whole amount of the
grant, for which I shall account at next year’s Meeting, giving at that meet-
ing my report on the experiments now in progress.
I am, dear Sir, yours faithfully,
James THomson.
To John Phillips, Esq., LL.D., F.RS.,
Assistant General Secretary, British Association.
List of the British Marine Invertebrate Fauna.
ts [For the Dredging Committee of the British Association. ]
bs NOTICE.
)
Tue following lists have been prepared in conformity with the desire of the
Committee of the Natural History Section of the British Association for the
Advancement of Science, which, at my suggestion, recommended the appoint-
ment of a general Dredging Committee, with a liberal grant of money for
the carrying out of its objects.
_ It is intended to place these lists in the hands of the local Dredging Com-
‘Mittees and naturalists engaged in researches in the most important districts
of the coasts of Great Britain and Ireland, with a request that they may be
returned, with notes on the conditions under which each species of the par-
ticular district has been found, and memoranda of such additional species as
may be obtained. By this means it is hoped to collect local lists of great
nterest, and materials for a more complete catalogue of the Invertebrate
Fauna of the British Seas. In the preparation of the present lists, I have
Deen assisted by Dr. Baird and Mr. S. Woodward and other members of the
Dredging Committee. The catalogue of Mollusca is taken from the work
f Messrs. Forbes and Hanley; that of Crustacea has been obligingly fur-
nished by Mr. Spence Bate; of Radiata by Mr. Stuart, of the Royal College
218 REPORT—1860.
of Surgeons; of Sponges by Dr. Bowerbank; of Rhizopoda by Messrs.
Rupert Jones and Parker; and to Dr. J. E. Gray I am indebted for permis-
sion to extract the list of Annelida from an unpublished work by the late
Dr. Johnston, of Berwick-upon-‘weed.
ROBERT McANDREW.
Isleworth House, Feb. 10, 1860.
*,* The nomenclature and arrangement are taken (with a few slight modifications)
from the “British Mollusca” of Messrs. Forbes and Hanley.
+t The species marked with an asterisk have been recorded as British since the time
when Mr. Barrett prepared the following list.
Octopus, Cuvier.
vulgaris, Lam.
Eledone, Leach.
octopodia, Penn.
Rossia, Owen.
Owenii, Bail.
macrosoma, Delle Chiaje.
Sepiola, Leach.
Rondeletii, Leach.
Murex, Linneus.
erinaceus, Linn.
corallinus, Scacchi.
Trophon, Montfort.
clathratus, Linn.
muricatus, Mont.
Barvicensis, Johnston.
Fusus, Lamarck.
gracilis, Da Costa.
propinquus, Alder.
Berniciensis, King.
Dalei, J. Sowerby.
fusiformis, Broderip.
antiquus, Linn.
Norvegicus, Chemn.
Turtoni, Bean.
Buccinum, Linneus.
undatum, Linn.
Humphresianum, Bennett.
Nassa, Lamarck.
reticulata, Linn.
pygmexa, Lamarck.
incrassata, Miiller.
Purpura, Lamarck.
lapillus, Linn.
Columbella, Zam.
nana, Lovén.
Mangelia, Leach.
attenuata, Mont.
costata, Pennant.
brachystoma, Philippi.
*Ginnaniana, Philippi.
gracilis, Mont.
Leufroyi, Michaud.
linearis, Mont.
nebula, Mont.
purpurea, Mont.
rufa, Mont.
CEPHALOPODA.
Atlantica, D’ Orbigny.
Ommastrephes, D’ Orbigny.
sagittatus, Lam.
todarus, Delle Chiaje.
Eblanz, Ball.
Loligo, Lamarck.
vulgaris, Lam.? (Forbesi,
Stp. De
GASTEROPODA.
Order PROSOBRANCHIATA.
septangularis, Mont.
striolata, Scacchi.
teres, Forbes.
Trevelliana, Turton.
turricula, Mont.
Lachesis, P7sso.
minima, Mont.
Marginella, Lamarck.
levis, Donovan.
Ovula, Lamarck.
atula, Pennant.
? acuminata, Bruguiére.
Cyprexa, Linneus.
Europea, Mont.
Natica, Lamarck.
monilifera, Lamarck.
nitida, Donovan.
sordida, Philippi.
Montagui, Forbes.
helicoides, Johnston.
pusilla, Say.
Kingii, Forbes.
Lamellaria, Montagu.
perspicua, Linn.
tentaculata, Mont.
Velutina, Fleming.
flexilis, Mont.
levigata, Linn.
? Otina, Gray.
otis, Turton.
Trichotropis, Broderip.
borealis, Brod.
*Triton, Lamarch.
cutaceus, Lam.
nodiferus, Lan.
Cerithiopsis, Forbes & Hanley.
*Naiadis, Woodw.
*nivea, Jeffr.
media, Linn.
marmore, Verany (media,
var.).
Sepia, Lenneus.
officinalis, Linn.
elegans, B/.
biserialis, De Montfort.
*pulchella, Jeffr.
tubercularis, Mont.
Odostomia, Fleming.
acuta, Jeffreys.
alba, Jeffreys.
conoidea, Brocchi.
conspicua, A/der.
cylindrica, Alder.
decussata, Monz.
dolioliformis, Jeffreys.
dubia, Jeffreys.
eulimoides, Hanley.
excavata, Philippi.
glabrata, Mih/feldt.
Gulsonx, Clark.
insculpta, Mont.
interstincta, Mont.
minuta, Jeffreys.
nitida, Alder.
obliqua, Alder.
pallida, Mont.
plicata, Mont.
rissoides, Hanley.
spiralis, Mont.
striolata, Alder.
truncatula, Jeffreys.
unidentata, Mont.
Warrenii, Thompson.
*Lukisii, Jeff.
Eulimella, Forbes.
acicula, Philippi.
affinis, Philippz.
clavula, Lovén.
Scillx, Scacchi.
Chemnitzia, D’ Orbigny.
clathrata, Jeffreys.
elegantissima, Mont.
fenestrata, Jeffreys.
——
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA. 219
formosa, Jeffreys.
fulvocineta, Thomps.
Mt indistincta, Mont.
rufa, Philipp?.
rufescens, Forbes,
scalaris, Philippi.
eximia, Jeffreys,
Eulima, Risso.
ome Linn.
istorta, Deshayes.
subulata, Donovan.
bilineata, Alder.
*stenostoma, Hanley.
Stylina, Mleming.
Turtoni, Broderip.
Cerithium, Bruguiére.
metula, Lovén.
reticulatum, Da Costa.
| adversum, Mont.
| *niveum, Jeff.
Aporrhais, A/drovandus.
pes-carbonis, Brongniart.
pes-pelecani, Linn.
- Turritella, Lamarck.
communis, isso.
Aclis, Lovén.
ascaris, Turton.
supranitida, 8. Wood.
2? unica, Mont.
nitidissima, Monzé.
_ Ceeum, Fleming.
trachea, Moni.
glabrum, Mont.
Scalaria, Lamarch.
Turtoni, Turton.
communis, Lamarch.
clathratula, Monz.
Greenlandica, Chemnitz.
Trevelyana, Leach.
Skenea, Fleming.
? costulata, Miiller.
? nevis, Philippi.
Eemorbia, Fabr.
? nitidissima, Adams.
? rota, Forbes.
Truncatella, Risso.
Montagui, Lowe.
Jetfreysia, Alder.
opalina, Jeffreys.
diaphana, Alder.
globularis, Jeffreys.
Rissoa, Frémenville.
*Alderi, Jeffr.
abyssicola, Forbes.
anatina, Drap.
Beanii, Hanley.
calathus, Forbes.
cingillus, Mont.
_—
Tornatella, Lamarck.
fasciata, Linn.
ulla, Lamarck.
hydatis, Linn.
Cranchii, Leach.
costata, ddams.
costulata, Risso.
crenulata, Michaud.
fulgida, Adams.
inconspicua, Alder.
labiosa, Mont.
lactea, Michaud.
littorea, Delle Chiaje.
muriatica, Lam.
parva, Da Costa.
proxima, Alder.
pulcherrima, Jeffreys.
punctura, Mont.
rubra, Adams.
rufilabrum, Adder.
sculpta, Philippi.
semistriata, Mont.
soluta, Philippi.
striata, Mont.
striatula, Mont.
ulvee, Pennant.
ventrosa, Mont.
vitrea, Mont.
Zetlandica, Mont.
Assiminea, Leach.
Grayana, Leach.
Lacuna, Turton.
crassior, Mont.
vincta, Mont.
puteolus, Turton.
pallidula, Da Costa.
Litorina, Férussac.
fabalis, Turton.
litoralis, Zinn.
litorea, Linn.
neritoides, Linn.
tenebrosa, Mont.
palliata, Say.
patula, affray.
rudis, Donovan.
saxatilis, Johnston.
Adeorbis, S. Wood.
subcarinata, Montz.
divisa, Meming.
Trochus, Linn.
alabastrum, Beck.
cinerarius, Linn.
conulus, Linn.
exiguus, Pulteney.
granulatus, Born.
crassus, Pulteney (lineatus,
Da Costa).
magus, Linn.
miliegranus, Philippi.
Montagui, Gray.
striatus, Linn.
tumidus, Mon¢.
umbilicatus, Mond.
Akera, Miiller.
bullata, Linn.
Cylichna, Lovén.
cylindracea, Pennant.
conulus, Desh.
lineatus, Da Costa.
zizyphinus, Linn.
Margarita, Leach.
undulata, Sowerby.
helicina, Fabr.
pusilla, Jeffreys.
Cutleriana, Clark.
Phasianella, Lamarck.
pullus, Linn.
Tanthina, Lamarck.
exigua, Lamarck.
communis, Lamarck.
pallida, Harvey.
Scissurella, D’ Orbigny.
crispata, Fleming.
Haliotis, Linn.
tuberculata, Linn.
Emarginula, Lamarck.
reticulata, J. Sow.
rosea, Bell.
crassa, J. Sow.
Puncturella, Lowe.
Noachina, Linn.
Fissurella, Lamarck.
reticulata, Donovan.
Pileopsis, Lamarck.
Hungaricus, Linn.
Calyptrea, Lamarck.
Sinensis, Linn.
Acmea, Eschscholéz.
testudinalis, Miiller.
virginea, Miiller.
Patella, Linneus.
vulgata, Linn.
athletica, Bean.
pellucida, Linn.
levis, Pennant.
Pilidium, Forbes.
fulvum, Miiller.
zxopies Forbes (Lepeta,
ancyloide, Forbes.
Dentalium, Linneus.
entale, Linn.
Tarentinum, Lam.
Chiton, Linneus.
fascicularis, Linn.
discrepans, Brown.
Hanleyi, Bean.
ruber, Linn.
cinereus, Linn.
albus, Linn.
asellus, Chemmn.
cancellatus, Sow.
levis, Pennant.
marmoreus, O, Fabr.
Order OPISTHOBRANCHIATA.
*Lajonkaireana, Basterot.
mamillata, Philippi.
nitidula, Zovén.
obtusa, Mon.
strigella, Lovén.
920 REPORT—1860.
Bullxa, Lemarck.
aperta, Linn.
quadrata, S. Wood.
scabra, Miiller.
catena, Mont.
punctata, Clark.
pruinosa, Clark.
Order NUDIBRANCHIATA.
(From the Monograph of Messrs. Alder and Hancock, 1856.)
truncata, Adams.
umbilicata, Mont.
Amphisphyra, Lovén.
hyalina, Turton.
Scaphander, Mon¢fort.
lignarius, Linn.
Aplysia, Gmelin.
hybrida, Sow.
Pleurobranchus, Cuvier.
plumula, Mont.
membranaceus, Mont.
Diphyllidia, Cuvier.
tineata, Otto,
Doris, Linn. elegans, Leuck.. nana, A. & H.
tuberculata, Cuv. Leachii, A. & H. stipata, 4. & H.
flammea, A. f° H. aspersa, 4. & H. angulata, 4. & H.
Zetlandica, 4. & H. ineequalis, Forbes. inornata, A. & A.
millegrana, A. § H. pulchella, 4. & H. concinna, A. § H.
Johnstoni, A. & H. quadricornis, Mont. olivacea, 4. & H.
planata, 4. ¢ H. Tritonia, Cuvier. aurantiaca, 4. & H.
coccinea, Forbes. Hombergii, Cuv. pustulata, 4. & H. ~
repanda, A. g H.
aspera, A. & H.
proxima, 4. 4 H.
muricata, Miill.
Ulidiana, Thomps.
diaphana, 4. f H.
oblonga, 4. ¢ H.
bilamellata, LZ.
depressa, 4. f H.
inconspicua, 4. § H.
pusilla, 4, & ZH.
sparsa, A. § H.
pilosa, Mil.
subquadrata, A. & H.
Goniodoris, Forbes.
nodosa, Mont.
castanea, A. & H.
Triopa, Johnston.
claviger, Mill.
ABgirus, Loven.
unctilucens, D’ Orb.
Thecacera, Fleming.
pennigera, Mont.
virescens, A. f H.
capitata, A. & H.
Polycera, Cuvier.
quadrilineata, Mudd.
ocellata, A. & H.
Lessonii, D’ Ord.
Ancula, Lovén.
cristata, Alder.
Idalia, Leuckart.
Hyalea, Lamarck.
trispinosa, Lesweur.
alba, A. & H.
plebeia, Johnston.
lineata, A. & H.
Scylleea, Linn.
pelagica, Linn.
Lomanotus, Verany.
marmoratus, 4. & H.
flavidus, A. & H.
Dendronotus, A. & H.
arborescens, Miill.
Doto, Oken.
fragilis, Forbes.
pinnatifida, Mont.
coronata, Miill.
JHolis, Cuvier.
papillosa, Linn.
glauca, A. & H.
Alderi, Cocks.
coronata, Forbes.
Drummondi, Thomps,
punctata, A. §& ZH.
elegans, 4. & H.
rufibranchialis, Johnst.
lineata, Lov.
smaragdina, A. & H.
gracilis, A. & H.
pellucida, 4. & H.
Landsburgii, A. &
alba, A. & H.
carnea, 4. & H.
glaucoides, 4. & H.
Peachii, A. & H.
PTEROPODA.
HI.
Flemingii, Forbes.
Jeffreysii, Forbes.
MacAndrei, Forves.
Couchii, Cocks.
ameena, 4. & H.
Northumbrica, 4. & H.
arenicola, Forbes.
Glottensis, A. & H.
viridis, Forbes.
purpurascens, lem.
cingulata, A. & H.
vittata, 4. & H.
cerulea, Mont.
picta, 4. & H.
tricolor, Forbes.
amethystina, 4. & H.
Farrani, 4. §& H.
exigua, 4. § H.
despecta, Johnst.
Embletonia, 4. & H.
pulchra, 4. & H.
minuta, J. & G.
pallida, 4. & H.
Fiona, A. & H.
nobilis, A. & H.
Hermza, Lovén.
bifida, Mont.
dendritica, 4. & H,
Alderia, Allman.
modesta, Lovén.
Proctonotus, A. & H.
mucroniferus, 4. & H.
Antiopa, 4. §& H.
cristata, Del. Ch.
hyalina, 4. & H.
Spirialis, Lydoux & Soulcyet. Clio, Miiller.
borealis, Zinn.
LAMELLIBRANCHIATA.
Pecten, O. F. Miller.
*aratus, Gmelin.
Danicus, Chemnitz.
maximus, Z777.
niveus, Macgillivray.
opercularis, Linn.
usio, Pennant.
similis, Laskey.
tigrinus, Miller.
varius, linn.
striatus, Miiller.
furtivus, Lovén.
Lima, Bruguiere.
hians, Gmelin.
Loscombii, Sowerby.
subauriculata, Mont.
Ostrea, Linneus.
edulis, Linn.
Anomia, Linneus.
aculeata, Miiller.
ephippium, Linn.
striata, Lovén.
patelliformis, Linn.
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA, 221
Avicula, Bruguiére.
Tarentina, Lam,
Pinna, Linneus.
_ pectinata, Linn.
Mytilus, Linneus,
edulis, Linn.
Modiola, Lamarck.
barbata, Linn.
modiolus, Linn.
*ovalis, G. B. Sdy.
phaseolina, Philippi.
tulipa, Lam.
Crenella, Brown.
costulata, isso,
decussata, Mont.
discors, Linn.
nigra, Gray.
marmorata, Forbes.
_ rhombea, Berkeley.
Area, Linneus.
lactea, Linn.
*nodulosa, Miiller.
raridentata, S. Wood.
_ tetragona, Poli.
Pectunculus, Lamarck.
__ glycimeris, Linn.
- Nucula, Lamarck.
decussata, Sow.
nitida, Sow.
nucleus, Linn.
radiata, Hanley.
tenuis, Afont.
Leda, Schumacher.
caudata, Don.
emea, Miinster.
Baiiam, Linneus.
aculeatum, Linz.
echinatum, Linn.
edule, Linn.
fasciatum, Mont.
nodosum, Zurton.
Norvegicum, Speng.
*papillosum, Poli.
pygmzxum, Don.
rusticum, Linn.
Suecicum, Reeve.
meina, Bruguiére.
borealis, Linn.
divaricata, Linn.
ferruginosa, Forbes,
flexuosa, Mont.
leucoma, Zurton.
spinifera, Mont.
iplodonta, Bronn.
— rotundata, Mont.
Kellia, Turton.
suborbicularis, Monz.
rubra, Mont.
Purtonia, Hanley.
‘minuta, O. Fabr.
ontacuta, Turton.
bidentata, Mont.
ferruginosa, Mont.
substriata, Mont.
epton, Turton.
Clarkiw, Clark,
“
nitidum, Turton.
squamosum, Mont.
*suleatulum, Jeff?.
Galeomma, Twrton.
Turtoni, Sow.
Cyprina, Lamarck.
Islandica, Linn.
Circe, Schumacher.
minima, Mont.
Astarte, Sowerby.
arctica, Gray.
compressa, Mont.
crebricostata, Forbes.
elliptica, Brown.
suleata, Da Costa.
triangularis, Mont.
Tsocardia, Lamarck.
cor, Linn.
Venus, Linneus,
casina, Linn.
fasciata, Don.
ovata, Pennant.
striatula, Don.
verrucosa, Linn.
Cytherea, Lamarck.
chione, Linn.
Artemis, Poli.
exoleta, Linn.
lineta, Puld.
Lucinopsis, Forbes.
undata, Penn.
Tapes, Miihifeldt.
aurea, Gmelin.
decussata, Linz.
pullastra, Wood.
virginea, Linn.
Venerupis, Lamarck.
irus, Linn.
Petricola, Lamarck.
lithophaga, Retzius.
Mactra, Linneus.
elliptica, Brown.
helvacea, Chemnitz.
solida, Linn.
stultorum, Zinn.
subtruneata, Da Costa,
truncata, Mont.
Lutraria, Lamarck.
elliptica, Linn.
oblonga, Chemn.
Tellina, Linneus.
balaustina, Linn.
crassa, Penn.
donacina, Linn.
fabula, Gronov.
incarnata, Linn.
proxima, Brown.
pygmexa, Philippi.
solidula, Pul¢.
tenuis, Da Cosfa.
Gastrana, Sch. (Diodonta, F.
&§ ZZ).
fragilis, Linn.
Psammobia, Lamarck.
costulata, Turt.
Ferroensis, Chemn.
tellinella, Lam.
vespertina, Chemn,
Syndosmya, Recluz.
alba, Wood.
intermedia, Thomps,
prismatica, Mont.
tenuis, Mont.
Serobicularia, Schumacher.
piperata, Gmelin.
Ervilia, Turton.
castanea, Mont.
Donax, Linneus.
anatinus, Lam.
politus, Poli,
Solen, Linneus.
ensis, Linn.
marginatus, Plt.
pellucidus, Penn.
siliqua, Linn.
Ceratisolen, Forbes.
legumen, Linn.
Solecurtus, Blainville.
candidus, Renieri.
coarctatus, Gmelin.
Mya, Linneus.
arenaria, Linn.
truncata, Linn.
Corbula, Bruguiére,
nucleus, Lam.
ovata, Forbes.
rosea, Brown.
Sphenia, Zurton.
Binghami, Turton.
Newra, Gray.
abbreviata, Lorbes,
costellata, Desh.
cuspidata, Olivi.
Poromya, Forbes (=Thetis,
Sby.).
granulata, Myst.
Panopxa, Menard dela Groye.
Norvegica, Speng,
Saxicava, Bellevue,”
arctica, Linn.
*fragilis, Nys¢.
rugosa, Linn.
Cochlodesma, Leach (=Peri-
ploma, Sch.).
preetenue, Pult.
Thracia, Leach.
convexa, Wood.
distorta, Mont.
phaseolina, Zam.
pubescens, Pu/¢.
villosiuscula, Macgill.
Lyonsia, Turton.
Norvegica, Chemn.
Pandora, Bruguiére.
obtusa, Leach.
rostrata, Lan.
Gastrocheena, Spengler.
modiolina, Lam.
Pholas, Linneus.
candida, Linz.
crispata, Linn.
dactylus, Linn.
222
parva, Penn.
striata, Linn.
Pholadidea, Turton.
lamellata, Turton.
papyracea, Solander.
Crania, Retzius.
anomala, Miiller.
Rhynchonella, Fischer.
psittacea, Chemn.
Aplidium, Savigny.
ficus, Linn.
fallax, Johnst.
nutans, Johnst.
Sidnyum, Savigny.
turbinatum, Savig.
Polyclinum, Savigny.
aurantium, M.-Edw.
Amouroucium, M.-Edw.
proliferum, M.-Hdw.
Nordmanni, M.-Edw.
Argus, M.-Edw.
Leptoclinum, M.-Hdw.
maculosum, M.-Hdw.
asperum, M.-Hdw.
aureum, M.-Hdw.
gelatinosum, M.-EHdw.
Listerianum, M.-Edw.
punctatum, Forbes.
Distoma, Gaertner.
rubrum, Savig.
variolosum, Gaertner.
Botryllus, Gaertner.
Schlosseri, Pallas.
polycyclus, Savig.
gemmeus, Savig.
violaceus, M.-Hdw.
smaragdus, M.-Edw.
virescens, 4. & H.
bivittatus, M.-Edw.
Stenorhynchus, Lamarck.
phalangium, Pennant.
tenuirostris, Leach.
Achzeus, Leach.
Cranchii, Leach.
Inachus, Fabr.
Dorsettensis, Penn.
dorhynchus, Leach.
leptochirus, Leach.
Pisa, Leach (Arctopsis, Lam.).
tetraodon, Leach.
Gibbsii, Leach (lanata, Lam.)
Hyas, Leach.
araneus, Fabr.
coarctatus, Leach,
Maia, Lam.
squinado, Herbst.
Eurynome, Leach.
aspera, Leach.
Xantho, Leach.
florida, Leach.
rivulosa, Hdw.
REPORT—1860.
Xylophaga, Turton.
dorsalis, Turton.
Teredo, ddanson.
bipennata, Turton.
malleolus, Turton.
BRACHIOPODA.
Terebratula, Bruguiére.
caput serpentis, Linn.
cranium, Miller.
capsula, Jeffreys.
TUNICATA.
rubens, 4. & H.
castaneus, 4. & H.
Botrylloides, M.-Hdw.
Leachu, Savig.
ramulosa, A. & H.
albicans, M.-Hdw.
radiata, 4. & H.
rotifera, M.-Hdw.
rubra, M.-Edw.
Clavelina, Savigny.
lepadiformis, O. F'. Miiller.
Perophora, Wiegmann.
Listeri, Wiegm.
Syntethys, Forbes & Goodsir.
Hebridicus, F. & G,
Ascidia, Baster.
intestinalis, Linn.
eanina, O. F. Miill.
venosa, O. F. Mull.
mentula, O. F. Mill.
arachnoidea, E. Forbes.
scabra, O. F'. Miill.
virginea, O. F. Miill.
parallelogramma, O. F.
Mill.
prunun, Miil.?
orbicularis, Mi7.
depressa, 4. & H.
aspersa, Miill.
vitrea, Van Beneden.
CRUSTACEA.
BRACHYURA,
tuberculata, Couch.
Cancer, Linn.
pagurus, Linn.
Pilumnus, Leach.
hirtellus, Leach.
Pirimela, Leach.
denticulata, Mont.
Carcinus, Leach.
meenas, Linn.
Portumnus, Leach.
variegatus, Leach (latipes,
Penn.).
Portunus, Leach.
puber, Linn.
corrugatus, Leach,
arcuatus, Leach.
depurator, Leach.
marmoreus, Leach.
holsatus, abr.
pusillus, Leach.
longipes, Risso.
plicatus, Risso.
megotara, Hanley.
navalis, Linn.
Norvegica, Speng.
palmulata, Lam.
Argiope, Deslongchamps.
cistellula, Searles Wood.
*decollata, Chemn.
conchilega, O. F. Mill.
echinata, Linn.
sordida, 4. & H.
albida, A. & H.
elliptica, 4. & H.
pellucida, A. & Z.
Molgwia, #. Forbes.
oculata, L. Forbes.
arenosa, A. & H.
Cynthia, Savigny.
microcosmus, Savig.
claudicans, Savig.
tuberosa, Macgillivray.
quadrangularis, Z. Forbes.
informis, £. Forbes.
tessellata, 2. Forbes.
limacina, Z. Forbes.
morus, £. Forbes.
rustica, Linn.
grossularia, Van Beneden.
ampulla, Brug.
mamillaris, Pallas.
ageregata, Rathke.
coriacea, A. & H.
Pelonaia, Forbes & Goodsir.
corrugata, Forbes & Hanl.
glabra, Forbes & Hani.
Salpa, Chamisso.
runcinata, Cham.
Appendicularia, Chamisso, sp.
carcinoides, Kin.
Polybius, Leach.
Henslowii, Leach.
Pinnotheres, Lazr,
pisum, Penn.
veterum, Bose.
Gonoplax, Leach.
angulata, Leach.
Planes, Leach.
Linnezana, Leach.
Ebalia, Leach.
Pennantii(tuberosa, Penn.).
Bryerii, Leach (tumefacta, —
Mont.).
Cranchii, Leach.
Atelecyclus, Leach.
heterodon, Leach (septem-
dentatus, Mont.).
Corystes, Leach.
Cassivelaunus, Leach.
Thia, Leach.
polita, Leach.
—e ee
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA.
Dromia, Hdw.
vulgaris, Edw.
_ Lithodes, Latr.
Maia, Leach.
Pagurus, Fabr.
Bernhardus, Linn.
Prideauxii, Leach.
Cuanensis, Thonvpson.
Ulidianus, Thompson.
Scyllarus, Fabr.
arctus, Linn.
Palinurus, Fabr.
Homarus, Linn.
Callianassa, Leach.
subterranea, Leach,
Gebia, Leach.
stellata, Mont.
deltura, Leach.
Axius, Leach.
stirhynchus, Leach,
Calocaris, Bell.
Macandrex, Bell.
_ Astacus, Fadr.
gammarus (Z.) (marinus,
7 Fabr.; vulgaris, Ldw.).
Nephrops, Leach,
S WN orvegicus, Linn.
— Crangon, Fabr.
; vulgaris, abr.
fasciatus, Pzsso.
spinosus, Leach.
sculptus, Bed/,
_ Mysis, Lat.
chameleon, V. Thompson.
vulgaris, V. Thompson.
Griffithsie, Beil.
Lamorne, Couch.
productus, Gosse.
Oberon, Couch.
Thysanopoda, Edw.
Couchii, Bell.
Macromysis, White(Themisto,
Goodsir, Bell).
longispinosus, Goodsir.
brevispinosus, Goodsir,
ynthilia, Whzte (Cynthia,
V. Thomps., Beil).
Orchestia, Leach.
littorea, Mont.
_Deshayesii, Savig.
Mediterranea, Costa (levis,
S. Bate; littorea, var.,
_ White).
Allorchestes, Dana.
Nilssonii, Kréyer (Danai,
‘Spence Bate).
imbricatus, Spence Bate.
ANOMOURA,
Hyndmanni, Thompson.
levis, Thompson.
Forbesii, Bell.
Thompsoni, Bell.
fasciatus, Bell.
Dillwynii, Spence Bate.
Porcellana, Lamarck.
platycheles, Penn.
longicornis, Penn.
MACROURA.
trispinosus, Hai/stone.
bispinosus, Westw., Kina-
han.
Allmanni, Kin.
Pattersonii, Kin.
Alpheus, Fabr.
ruber, Hdw.
affinis, Guise.
Autonomea, Risso.
Olivii, Risso,
Nika, Risso.
edulis, Risso.
Couchii, Bell.
Athanas, Leach.
nitescens, Mont., Leach.
Hippolyte, Leach.
spinus, Sowerby.
varians, Leach.
Cranchii, Leach.
Thompsoni, Bell.
Prideauxiana, Leach.
Gordoni, Spence Bate.
fascigera, Gosse.
STOMAPODA.
Flemingii, Goodsir,
Cuma, Edwards.
scorpioides, Mont.
unguiculata, Spence Bate.
Vaunthomsonia, Spence Bate.
Edwardsii, Kréyer.
cristata, Spence Bate.
Diastylis, Say (Alauna, Good-
sir, Bell).
Rathkii, Kr. (vostrata,
Goodsir, Bell).
Eudora, Spence Bate.
truncatula, Spence Bate.
AMPHIPODA NORMALIA.
Nicea, Nicolet (Galanthis,
Spence Bate).
Lubbockiana, Spence Bate.
Montagua, Spence Bate.
monoculoides, Montagu
(Lyphis monoculoides,
White, Gossc).
marina, Spence Bate.
Alderii, Spence Bate.
pollexiana, Spence Bate.
Danaia, Spence Bate.
dubia, Spence Bate.
223
Galathea, Faér.
squamifera, Leach.
dispersa, Spence Bate.
strigosa, Fabr.
nexa, Hmb.
Andrewsii, Kinahan.
Munida, Leach.
Bamfica, Penn. (Rondeletii,
Bell),
Grayana, Thompson.
Mitchelli, Thompson.
Whitei, Thompson.
Yarrellii, Thompson.
Barleei, Spence Bate.
pandaliformis, Beil.
pusiola, Kroyer.
Pandalus, Leach.
Jeffreysii, Spence Bate,
Kinahan.
annulicornis, Leach.
leptorhynchus, Kin.
Palzemon, Fabr.
serratus, Penn.
squilla, Fabr.
Leachii, Bell.
varians, Leach.
Pasipheea, Savigny.
sivado, Risso.
Pensxus, Fabr.
caramote, Risso.
Tphithoé, Spence Bate (Halia,
Spence Bate, White).
trispinosa, Goodsir,
Bodotria, Goodsir.
arenosa, Goodsir,
Cyrianassa, Spence Bate (Ve-
nilia, Spence Bate, White).
gracilis, Spence Bate.
longicornis, Spence Bate.
Squilla, Fabr.
Desmarestii, Risso.
mantis, Rondelet.
Phyllosoma, Leach.
Cranchii, Leach,
Lysianassa, M.-Edw,
Coste, M.-Edw.
Audouiniana, Spence Bate.
longicornis, Lucas (Chau-
sica, Sp. B., not M.-F.).
Atlantica, Edw. (marina,
Spence Bate).
Callisoma, Hope (Scopelo-
cheirus, Spence Bate).
crenata, Spence Bate.
Anonyx, Kréyer.
Edwardsii, Kréyer,
224
Edwardsii, Kréyer.
minutus, Krdyer.
Holbolli, Kréyer.
ampulla, Kréyer.
denticulatus, Spence Bate.
longipes, Spence Bate.
obesus, Spence Bate.
longicornis, Spence Bate.
Opis, Kréyer.
typica, Kréyer.
Ampelisca, Kréyer (Tetro-
matus, Spence Bate).
Gaimardii, Kréyer (typica,
Spence Bate).
Belliana, Spence Bate.
Westwoodilla (Westwoodia,
Spence Bate).
cxcula, Spence Bate.
hyalina, Spence Bate.
Monoculodes, Stimpson.
carinatus, Spence Bate.
Kréyera, Spence Bate.
arenaria, Spence Bate.
Phoxus, Kréyer.
simplex, Sp. Bate (Kvéyeri,
Spence Bate, not Stimp-
son).
plumosus, HoJdéll.
Holbolli, Kréy.
Suleator, Spence Bate.
arenarius, Spence Bate.
Urothoé, Dana.
marinus, Spence Bate (Sul-
cator marinus).
Bairdii, Spence Bate.
medius, Spence Bate.
elegans, Spence Bate.
Grayia, Spence Bate.
imbricata, Spence Bate.
Liljeborgia, Spence Bate.
pallida, Spence Bate.
Phiedra, Spence Bate.
antiqua, Spence Bate.
Kinahani, Spence Bate.
Tsxa, M.-Edwards.
Montagui, M.-Edw.
Iphimedia, Rathke.
Lestrigonus, Guérin.
Fabricii, M.-Edw.
REPORT—1860.
obesa, Rathke.
Eblanxe, Spence Bate.
Otus, Spence Bate.
carinatus, Spence Bate.
Acanthonotus, Owen.
testudo, Montagu.
Dexamine, Leach.
Loughrinii, Spence Bate.
spinosa, Mont.
Eusirus, Kréyer. ‘
Edwardi, Spence Bate.
Helvetix, Spence Bate.
Atylus, Leach.
bispinosus, Spence Bate.
Huxleyanus, Spence Bate.
Gordonianus, Spence Bate.
Pherusa, Leach.
cirrus, Spence Bate.
fucicola, Edw.
Calliope, Leach.
Leachii, Spence Bate.
Lembos, Spence Bate.
Cambriensis, Spence Bate.
versiculatus, Spence Bate.
Websterii, Spence Bate.
Danmoniensis, Spence Bate.
Adra, Kroy. (=Lalaria, Ni-
colet).
gracilis, Spence Bate.
Eurystheus, Spence Bate.
tridentatus, Spence Bate.
tuberculosus, Spence Bate.
Gammarella, Spence Bate.
brevicaudata, M.-Edw. (=
G. orchestiformis, Spence
Bate).
Crangonyx, Spence Bate.
subterranea, Spence Bate.
Amathia, Iathke.
Sabinii, Leach.
Gammarus, Fabr.
locusta, abr.
fluviatilis, Rese.
gracilis, Rathke.
camptolops, Leach.
marinus, Leach.
laminatus, Johnston.
AMPHIPODA HYPERINA.
Phronima, Lar.
sedentaria, Fors.
longimanus, Leach. ;
palmatus, Mont. (insequi-
manus, Spence Bate).
grossimanus, Mont.
maculatus, Johnston.
Bathyporeia. Lindstrém
(Thersites, Spence Bate).
pilosa, Lindstrom.
pelagica, Spence Bate.
Robertsoni, Spence Bate.
Leucothoé, Leach, not Kroyer.
articulosa, Mont.
furina, Savig. (procera, Sp.
Bate).
Pleonexes, Spence Bate.
gammaroides, Spence Bate.
Amphithoé, Leach.
rubricata, Mont.
littorina, Spence Bate.
? obtusata, Leach.
? dubia, Johnston.
Sunamphithoé, Spence Bate.
hamulus, Spence Bate.
conformata, Spence Bate.
Podocerus, Leach.
faleatus, Mont.
yariegatus, Leach.
pulchellus, Leach.
Jassa ?, Leach.
pelagica, Leach.
Siphonecetus, Kréyer.
Whitei, Gosse.
Erichthonius, M.-Edw,
difformis, M.-Edw.
Cyrtophium, Dana.
Darwinii, Spence Bate.
Corophium, Latreille.
longicorne, Fabr.
Chelura, Philippi.
terebrans, Phil.
Hyperia, Latreille.
Galba, Mont. (Latreillii,
Edw.=Metoechus medu- —
sarum, Latr.).
oblivia, Kréy.
Typhis, Risso.
nolens, Johnston.
AMPHIPODA ABERRANTIA. (Lxmopipopa of Latreille.)
Dulichia, Kréyer.
porrecta, Spence Bate.
falcata, Spence Bate.
Proto, Leach.
pedata, Leach.
Goodsirii, Spence Bate.
Protella, Dana.
longispina, Kréyer.
Caprella, Lamarck.
linearis, Lar.
Pennantii, Leach.
tuberculosa, Goodsir.
lobata, Miiller.
acuminifera, M.-Edw.
Cyamus, Lafreille,
ceti, Linn.
ovalis, Roussel.
gracilis, Roussel.
Thompsoni, Grosse,
ISOPODA ABERRANTIA. (Anisopopa of Dana.)
Arcturus, Zar. (Astacilla,
Johnston; Leachia, John-
ston.)
longicornis, Sow,
intermedius, Goodsir,
gracilis, Goodsir.
Anthura, Leach.
gracilis, Mond,
cylindricus, Mon¢.
Tanais, 1f.-Edw.
Dulongii, Aud.
hirticaudatus, Spence Bate.
ee
LIST OF THE
Apseudes, Leach.
talpa, Mont.
Anceus, Risso.
mavyillaris, Mont.
rapax, M.-Edw.
Praniza, Leach.
ceruleata, Mont.
Munna, Kréver.
Kroyeri, Goodsir.
Whiteana, Spence Bate.
Jzra, Leach.
albifrons, Leach.
Oniscoda, Lazreille.
maculosa, Leach.
Deshayesii, Lucas.
Limnoria, Leach.
lignorum, fathke (tere-
brans, Leach).
Idotea, Fabr.
pelagica, Leach.
tricuspidata, Desm.
emarginata, Fabr.
linearis, Lazr.
Order I. PHYLLOPODA.
Nebalia, Leach.
bipes, O. Fabr.
Artemia, Leach.
salina, Linz.
Order II. CLADOCERA.
Eyadne, Lovén.
Nordmanni, Lovén.
Order IIT. OSTRACODA.
Fam, I. Cytheride.
_ COythere, Miller.
flavida, Miill.
reniformis, Baird.
albo-maculata, Baird.
alba, Baird.
yariabilis, Baird.
aurantia, Baird.
' nigrescens, Baird.
Minna, Baird.
angustata, Minster.
acuta, Baird.
pellucida, Baird.
impressa, Baird.
fusca?, Johnston.
Edwardii, Spence Bate.
Liriope, Kréyer.
balani, Spence Bate.
Tone, Mont.
thoracica, Mont.
ISOPODA (NORMALIA).
acuminata, Leach.
appendiculata, Risso.
Ligia, Fabr.
oceanica, Jinn.
Sphzroma, Latr.
serratum, abr.
rugicauda, Leach.
Hookeri, Leach.
Cymodocea, Leach.
truncata, Leach.
emarginata, Leach.
Montagui, Leach.
rubra, Leach.
viridis, Leach.
Nerzea, Leach.
bidentata, Adams.
ENTOMOSTRACA.
quadridentata, Baird.
conyexa, Baird.
Cythereis, Rupert Jones,
Whitei, Baird.
Jonesii, Baird.
antiquata, Baird.
Fam. II. Cypridinide.
Cypridina, M.-Hdw.
Macandrei, Baird.
Brenda, Baird.
Marix, Baird.
interpuncta, Baird,
Order ITV. COPEPODA.
Fam. I. Cyclopide.
Canthocamptus, Westwood.
Strémii, Baird.
furcatus, Baird.
minuticornis, Mill.
Arpacticus, M.-Edw.
chelifer, Miil?.
nobilis, Baird.
Alteutha, Baird.
depressa, Baird.
BRITISH MARINE INVERTEBRATE FAUNA. 225
Bopyras, Latr.
squillarum, Laz.
hippolytes, Kréyer.
Phryxus, Rathke.
hippolytes, Rathke.
paguri, Reathke.
Campecopea, Leach.
hirsuta, Mont.
Cranchii, Leach.
Cirolana, Leach.
Cranchii, Leach.
Eurydice, Leach.
pulchra, Leach.
fea, Leach.
bicarinata, Leach.
tridens, Leach.
Conilera, Leach.
cylindracea, Mont.
Rocinela, Leach.
Danmoniensis, Leach.
monophthalma, Johnston.
Fam, II. Diaptomidz.
Temora, Baird.
Finmarchica, Gunner.
Calanus.
euchzta, Lubbock.
Anglicus, Lubbock.
Anomalocera, Templeton.
Patersonii, Templeton.
Fam. III. Cetochilide.
Cetochilus, Vauzéme.
septentrionalis, Goodsir.
Pontella, Dana.
Wollastoni, Lubbock.
Pontellina, Dana.
brevicornis, Lubbock.
Peltidium, Philippi.
purpureum ?, Phil.
Coryceus, Dana.
Anglicus, Lubbock.
Fam. IV. Monstrillide.
Monstrilla, Dana.
Anglica, Lubbock.
On what ani-
On what ani-
Bpeaics, mals found. decree mals found.
Order V. Miilleri, Zeach.............../various fishes.
SIPHONOSTOMA. centrodonti, Baird ......... sea bream.
ey minutus, Oto holibut.
Fam. I. Caligide. curtus, Miil/. ray.
Caligus, Miiller. |Lepeophtheirus, Nordmann.
diaphanus, Nordm. ......... various fishes. Stromii, Baird. ........... on salmon.
rapax, M.-Edw. .......1.05. various fishes. pectoralis, Mill. .......s000 yarious fishes.
1860. Q
226
Species.
Nordmanni, M.-Edw. ......
hippoglossi, Kréy. .........
obscurus, Baird
Thompsoni, Baird
Chalimus, Burmeister.
scombri, Burvit..........2.+.
Trebius, Kroyer.
caudatus, Kréy. ............
Fam. II. Pandaride.
Dinemoura, Lafreille.
alata; M-BOUEY. .....ccrsnes=
lamnzx, Johnst............000.
Fam. III. Cecropide.
Pandarus, Leach.
bicolor, Leach
Cecrops, Leach.
Latreillei, Leach
Lemargus, Kroyer.
muricatus, K7réy. ............
Fam. IV. Anthosomide.
Anthosoma, Leach.
Smithii, Leach ...............
Fam. V. Ergasilide.
Nicothoé, M.-Edwards.
astaci, M.-Edw.
ee eee
Fam. I. Balanide.
Balanus (Lister).
tintinnabulum, Linn.
spongicola, Brown.
perforatus, Bruguiére.
Amphitrite, Darwin.
eburneus, dug. Gould.
improyisus, Darwin.
porcatus, Da Costa.
crenatus, Bruguiére.
balanoides, Linz.
Hameri, Ascanius.
Acasta, Leach.
spongites, Poli.
Order PODOSOMATA.
Fam. I. Pycnogonide.
Pycnogonum, Fabricius.
littorale, Strozm.
Phoxichilus, Latreille.
spinosus, Mont.
REPORT—1860.
On what ani-
On what ani-
mals found. Species. mals found.
sun-fish. Fam. VI.
holibut. Chondracanthide.
brill. Chondracanthus, De Za Roche.
turbot. Zei, De la Roche ............ gills of dory.
Lernentoma, De Blainville.
on mackerel. cornuta, Miill. ...........0... gills of sole.
SeeliMae,, ...ccsscseesseeee gills of gurnard.
on skate. lophii, Johnst. ...1.1....080 pouches of an-
Lerneopoda, De Blainville. gler.
elongata, Grant ............ shark.
harie. Galen Troy. ..... Jee shark.
Br hake AalMIONEA TY, checidoeceeanee salmon,
‘Fam. VII. Anchorellide.
'Anchorella, Cuvier.
on shark. uncinata, Mill. .........5.. on the cod.
TUPOSH, MOY. ..use.seeeee ee on the cod.
on sun-fish.
Fam. VIII. Lerneide.
on sun-fish, |Lernea, L.
Pranchialts, Ji cic..3rces ae gills of cod.
Lerneonema, M.-Edwards.
Beate, SOY. oo... sce corks on the sprat.
on shark. Baird, SGiernc acceso cteees herring.
encrasicoli, Twrt. ............ sprat.
on gills of lobster
CIRRIPEDIA.
Pyrgoma, Leach.
Anglicum, G. B. Shy.
Xenobalanus, Sfeenstrup.
globicipitis, Steenstrup.
Chthamalus, Ranzani.
stellatus, Poli. _
Verruca, Schumacher.
Strémia, O. Miiller.
Alcippe, Hancock.
lampas, Hancock.
Fam. II. Lepadide.
Lepas, Linn.
anatifera, Linn.
Hillii, Leach.
ARACHNIDA. -
Fam. Il. Nymphonide.
Phoxichilidium, M.-Edwards.
coccineum, Joknst.
globosum.
olivaceum.
Pallene, Johnston.
brevirostris, Johnst.
ANNELIDA.
anserifera, Linn.
pectinata, Spengler.
fascicularis, Ellis § Solander.
Conchoderma, OZfers.
aurita, Linn.
virgata, Spengler.
Alepas, Sander-Rang.
parasita, Sander-Rang.
Anelasma, Darwin.
squalicola, Lovén.
Sealpellum, Leach.
vulgare, Leach.
Pollicipes, Leach.
cornucopia, Leach.
Nymphon, Fabricius.
gracile, Leach.
grossipes, O. Fabr.
femoratum, Leach.
pictum.
giganteum, Johnst.
*,* The following list of British Marine Worms is copied, by favour of Dr. J. E. Gray,
from an unpublished Catalogue by the late Dr. Johnston.
Order I. TURBELLARIA.
Fam. I. Planoceride.
Leptoplana, Ehrenberg.
subauriculata, Johnston.
tremellaris, Miiller.
flexilis, Dalyell. -
atomata, Miiller.
ellipsis, Dalyell.
Eurylepta, Ehrenberg.
cornuta, Miiller.
Dalyellii, Johnston.
.
*
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA.
sanguinolenta, Quatrefages.
vittata, Montagu.
Planocera, Blainville.
folium, Gruée.
Fam. II. Planariade.
Planaria, Miiller.
ulvee, Oersted.
affinis, Oersted.
alba, Dalyell.
variegata, Dalyell.
? gracilis, Dalyell.
? falcata, Dalyell.
Fam. III. Dalyellide.
Typhloplana, Ehrenberg.
flustree, Dalyell.
Convoluta, Oersted.
paradoxa, Oersted.
Doubtful species of this fam.
Planoides fusca, Dalyell.
Planaria hirudo, Johnston.
Astemma, Oersted.
rufifrons, Johnston.
filiformis, Johnston.
Cephalotrix, Oersted.
lineatus, Dalyell.
flustra:, Dalyell.
Tetrastemma, Khrenberg.
varicolor, Oersted.
variegatum, Dalyell.
alge, Dalyell.
Borlasia, Johnston.
olivacea, Johnston.
octoculata, Johnston.
purpurea, Johnston.
Gesserensis, Miiller.
striata, Rathke.
Ommatoplea, Ehrenberg.
gracilis, Johnston.
rosea, Miiller.
alba, Thompson.
melanocephala, Johnston.
pulchra, Johnston.
Stylus, Johnston.
viridis, Dalyell.
purpureus, Dalyell.
fragilis, Dalyell.
fasciatus, Dalyell.
Lineus, 7. W. Simmons,
longissimus, Simmons,
gracilis, Goodsir.
lineatus, Johnston.
murenoides, D. Chiaje.
fasciatus, Johnston.
_ viridis, Dalyell.
_ albus, Dalyell.
eckelia, Leuckart.
annulata, Montagu.
tenia, Dalyell.
Serpentaria, H. D. S. Goodsir.
fragilis, Goodsir.
fusca, Dalyell.
Order II.
BDELLOMORPHA.
Fam. I.
Malacobdellide.
Malacobdella, Blainville.
grossa, Miiller.
Valenciennxi, Blanchard,
anceps, Dalyell.
Order III. BDELLIDEA.
Fam. I. Branchelliade.
Branchellion, Savigny.
torpedinis, Savigny.
Fam. II. Piscicolide,
Pontobdella, Leach.
muricata, Linn.
verrucata, Grube.
areolata, Leach.
levis, Blainville.
littoralis, Johnston.
campanulata, Dalyell.
Order IV. SCOLICES.
Fam. I. Lumbricide.
Senuris, Hoffmeister.
lineata, Miiller.
Clitellio, Savigny.
arenarius, Miiller.
Valla, Johnston.
ciliata, Miiller.
Order V. GYMNOCOPA.
Fam. I. Tomopteride.
Tomopteris, Eschscholtz.
onisciformis, Grube.
Order VI. CHAATOPODA.
Fam. I. Aphroditide.
Aphrodita, Leach.
aculeata, Linn.
borealis, Johnston.
hystrix, Savigny.
Lepidonotus, Leach.
squamatus, Linn.
clava, Montagu.
impar, Johnston.
pharebratus, Johnston.
cirratus, Fabr.
semisculptus, Leach.
pellucidus, Dyster.
imbricatus, Linn.
Species not defined.
Aphrodita squamata, Dal-
yell.
lepidota, Pallas. |
minuta,. Pennant.
annulata, Pennant. 'e
velox, Dalyell.
Lepidonotus floccosus ?,
Dalyell.
Polynoé semisquamosa,
Williams,
227
Polynoé, Oersted.
scolopendrina, Savigny.
Pholoé, Johnston.
inornata, Johnston.
eximia, Dyster.
Sigalion, dud. § M.-Edwards.
boa, Johnston.
Fam. II.
Amphinomenide.
Euphrosyne, Savigny.
foliosa, dud. §& M.-Edwards.
borealis, Oersted.
Fam. III. Euniceidee.
Eunice, Aud. § M.-Edwards,
Norvegica, Linn.
annulicornis, Brit. Mus.
antennata, Savigny.
Harassii, dud. & M.-Edw.
sanguinea, Montagu.
margaritacea, Williams.
Northia, Johnston.
tubicola, Miiller.
conchylega, Sars.
Lycidice, Savigny.
Ninetta, dud. § M.-Edw.
rufa, Gosse.
Lumbrineris, Blainville.
tricolor, Leach.
Fam. IV. Nereide.
Nereis, Cuvier.
brevimana, Johnston.
pelagica, Linn.
diversicolor, Miiller.
cerulea, Linn.
fimbriata, Miiller.
imbecillis, Grube. -
Dumerilii, dud. § M.-Edw.
pulsatoria, Montagu.
Nereilepas, Oersted.
fucata, Savigny.
Heteronereis, Oersted.
lobulata, Savigny.
renalis, Johnston.
longissima, Johnston.
margaritacea, Johnston.
Fam. V. Nephthyide.
Nephthys, Cuvier.
cxca, Fabr.
longisetosa, Oersted.
Hombergii, Cuv. ? ?
Fam. VI. Phyllodoceide.
Phyllodoce, Cuvier.
lamelligera, Turton.
bilineata, Johnston.
maculata, Linn.
viridis, Linn.
ellipsis, Dalyell.
Griffithsii, Johnston.
cordifolia, Dyster.
Psamathe, Johnston.
punctata, Miiller.
Q2
228
Fam. VIT. Glyceridz.
Glycera, Savigny.
mitis, Johnston.
dubia, Blainville.
capitata, Oecrsted.
nigripes, Johnston.
Goniada, Aud. & M.-Edwards.
maculata, Oersted.
Fam. VIII. Syllide.
Syllis, Savigny.
armillaris, Miller.
cornuta, H. Rathke.
prolifera, Miiller.
? monoceros, Dalyell.
Gattiola, Johnston.
spectabilis, Johnston.
Myrianida, M.-Hdw.
pinnigera, Montagu.
Toida, Johnston.
macrophthalma, Johnston.
Fam. IX. Amytideide.
Amytidea, Grube.
maculosa(Nereis), Montagu
Fam, X. Ariciade.
Nerine, Johnston.
vulgaris, Johnston.
coniocephala, Johnston.
Doubtful species.
Nerine contorta (Nereis),
Dalyell.
Spio, Turton.
filicornis, Miiller.
seticornis, Zurton.
crenaticornis, Montagu.
Leucodore, Johnston.
ciliatus, Johnston.
Ephesia, Rathke.
gracilis, Rathke.
Spherodorum, Oersted.
peripatus, Johnst.
Cirratulus, Lamarck.
tentaculatus, Mont.
borealis, Lamk.
Dodecaceria, Oersted.
concharum, Oersted.
Fam. XI. Opheliade.
Ophelia, Savigny.
acuminata, Oersted.
Ammotrypane, Rathke.
limacina, Rathhe.
Travisia, Johnston.
Forbesii, Johnst.
Eumenia, Oers¢ed.
crassa, Oecrsted.
Fam. XII.
Siphonostomide.
Siphonostoma, Cuvier.
uncinata, dud. & M.-Edw.
Trophonia, Cuvier.
plumosa, Miiller.
REPORT—1860.
Fam. XIII. Telethusidez.
Arenicola, Savigny.
piscatorum, Lamk.
branchialis, Aud. §&M.-Edw.
ecaudata, Johnst.
Fam. XIV. Maldaniade.
Clymene, Savigny.
borealis, Dalyell.
Fam. XV. Terebellide.
Terebella, Montagu.
conchilega, Pallas.
littoralis. Dalyell.
cirrata, Mont.
nebulosa, Mont.
gigantea, Mont.
constrictor, Mont.
venustula, Mont.
tuberculata, Dalyell.
textrix, Dalyell.
maculata, Dalyell.
Venusia, Johnston.
punctata, Johnst.
Terebellides, Sars.
Streemii, Sars.
Pectinaria, Lamarck.
Belgica, Pallas.
granulata, Linn.
Fam. XVI. Sabellariade.
Sabellaria, Zamarck.
Anglica, Ellis,
crassissima, Lamk.
lumbricalis, Mont.
Fam. XVII. Serpulide.
Arippasa, Johnston.
infundibulum, Mont.
Sabella, Savigny.
pavonina, Savigny.
penicillus, Linn.
vesiculosa, Mont.
bombyx, Dalyell.
Savignii, Johnst.
volutacornis, Mont.
Doubtful species,
Sabella unispira, Sav.
rosea (Amphitrite)» Sow.
luna (Amphitrite), Dal.
curta (Amphitrite), Mut.
Protula, Risso.
protensa, Philippi.
Dysteri, Hualey.
Serpula, Linneus.
vermicularis, Ellis.
intricata, Linn.
reversa, Mont.
Berkeleyi, Johnst.
conica, fem.
armata, Jem.
Dysteri, Johnst.
Ditrupa, Berkeley.
subulata, Deshayes.
Filograna, Berkeley.
implexa, Berk.
Othonia, Johnston.
Fabricii, Johnst.
Fam. XVIII.
Campontiade.
Campontia, Johnston.
eruciformis, Johnst.
Fam. XIX. ? Meade.
Mea, Johnston.
mirabilis, Johnst.
Fam. XX. ? Sipunculide.
Syrinx, Bohadsch.
nudus, Linn.
papillosus, Thomps.
Harveii, Forbes.
Sipunculus, Linneus.
Bernhardus, Forbes.
Macrorhynchopterus, Rondel.
Johnstoni, Forbes.
saccatus, Flem.
tenuicinctus, M‘ Coy.
Forbesii, MM‘ Coy.
granulosus, M‘Coy.
Pallasii, Forbes.
Fam. XXI. Priapulide.
Priapulus, Lamarck,
caudatus, Wem.
Fam. XXII.
Thalassemide.
Thalassema, Cuvier.
Neptuni, Gaértner.
Echiurus, Cuvier.
oxyurus, Pall.
Species inquirende.
Nereis, Cuvier.
iricolor, Mont.
margarita, Mont.
lineata, Mont.
maculosa, Mont.
rufa, Penn.
mollis, Linn.
octentaculata, Mont.
punctata, Eneycl. Méth.
noctiluca, Linn.
pinnigera, Mont.
Aphrodita, Leach.
annulata, Penn.
minuta, Penn.
Spio, Turton.
seticornis, Twrt.
crenaticornis, Mont.
calcarea, Templeton.
Branchiarius, Mont.
quadrangularis, Mont.
Diplotis, Mont.
hyalina, Mont.
Derris, Adams.
sanguinea, Adams.
—
|
.
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA.
229
ENTOZOA.
*,* From Dr. Baird’s British Museum Catalogue; and Dr. Bellingham’s List of Irish
Entozoa, in the ‘ Annals
of Natural History,’ 1844.
In what ani-
Species. mals found.
Order NEMATOIDEA.
Fam. Filariade.
Filaria, Miiller.
? marina, Linn. ............ shad and cod.
inflexo-caudata, Siebold ...|porpoise.
Apiaceae eee cals hace antes o's + red gurnard and
Trichosoma, Rudolphi. mullet.
gracilis, Bellingh............- hake.
Spiroptera, Rudolpht.
BU earac asa tan ove sesebeos 00: skate.
Fam. Ascaride.
Ascaris, Linneus.
osculata, Rud. ........0.0008- seal, [ny.
Cyt P77) Ae eee viviparous blen-
TIPIGA, PUA. ...0scosrcereesee: lophius.
capsularia, Rud. ............ cod, &e.
COMATIS, RUA. os cieaesescree ss flounder, &c.
byatay Bud. ccs. es sce eee- cod, &e.
constricta, Rud. ......6..65. sea-scorpion, Xe.
rotundata, Rud. ............! skate.
GREE OGHE Me acjs vobaa case's 0 herring.
angulata, Rud.............6+ lophius.
tenuissima, Zeder............ whiting.
BUCCISA RUC cam siccsoies sees lump-fish.
Fam. Sclerostomidz.
Cucullanus, Miller.
minutus, Rud. ...........08- flounder.
heterochrous, Rud. ......... flounder.
foveolatus, Lam. ........... plaice and dab.
Stenurus, Dujardin.
inflexus, Rud. (part.) ...... porpoise.
Prosthecosacter, Diesing.
inflexus, Rud. ........0.0.+4 porpoise.
convolutus, Kuhn ......... porpoise.
Order TREMATODA.
Fam. Onchobothriadz.
Octobothrium, Leuckart.
lanceolatum, Leuck.......... shad.
Fam. Capsalide.
Capsala, Bosc.
GCoccinea, CWV. ..cocseccdseees sun-fish.
elongata, Nitzsch............. sturgeon.
Fam. Distomide.
Monostoma, Zeder.
filicolle, Rud. ..........0.... sea bream.
trigonocephalum, Rud. ...|turtle.
Distoma, Retzius.
appendiculatum, Rud. ...'shad, &c.
hispidum, Viborg ......... sturgeon.
megastomum, Fwd. ....:....'smooth shark.
microcephalum, Baird .../spinous shark.
¢ In what ani-
Species. mals found.
tumidulum, Rud............. pipe-fish.
fulvums Rud. .;Sei se skate.
Varietm ....cib.cccuseeeeene salmon,
gibbosum ?, Rud...........+. haddock.
rufo-viride, Rud. ............ conger-eel.
reflemuamn ?'25.cdecks «et seeenee eyclopterus.
OXCISUM, UA. yose.cs.ckeeees mackerel.
seabrum, Zeder .........04. whiting.
contortum, Rud. ............ sun-fish,
nigro-flavum, Fwd. ......... sun-fish,
Hirudinella, Garsin.
clavata, Menzies ............ Bonito.
Order
ACANTHOCEPHALA.
Fam. Echinorhynchide.
Echinorhynchus, Miller.
proteus, Westrwmb ......... flounder.
ACUS a JIU) Godies aye sven tence cod, &e.
gibbosus, Rud. ...........0065 herring.
strumosus, Rud. ............ seal,
Order CESTOIDEA.
Fam. Rhynchobothride.
||Rhynchobothrium, Blainville.
corollatum, Aézldg.......... smooth shark,
Tetrarhynchus, Rudolphi.
megacephalus, Rud.......... spotted dog-fish.
BOMAUSWIITUMs «0. t.c0snaccen salmon.
GROSSUS; HUG, wcnncc>.cdecet: salmon.
rugosus, Baird............0- salmon.
Tetrabothriorhynchus, Dies.
barbatus, Linn. ..........5. lemon sole.
Fam. Teeniade.
Bothriocephalus, Rudolphi.
fragilis, Aad: t22 0s an sp-scenee shad.
proboscideus, Bartsch. ...... salmon, &e.
punctatus, Rud. ............ turbot, &e.
tumidulus, Rud. ............ ray.
microcephalus, Rud. ...... sun-fish.
coronatus, Rud. ............ skate.
corollatus, Rud. ...........- dog-fish,
paleaceus, Rud. ............ dog-fish.
Fam. Scolecide.
Scolex, Miiller.
polymorphus, Rud.......... turbot, &c.
Order CYSTICA.
Fam. Cysticide.
Anthocephalus, Rudolphi.
elongatus, Rud. ............ isun-fish.
granulosus?, Rud. ......... whiting, &c.
paradoxus, Drum. ......... turbot.
230
Order CRINOIDEA.
Comatula, Lamarck.
rosacea, Link.
Celtica, Barrett.
Sarsii, Diiben § Koren,
Order OPHIUROIDEA.
Fam. Ophiuride.
Ophiura, Lamarck.
texturata, Lamk.
albida, Forbes.
Ophiocoma, Agassiz.
neglecta, Johnst.
punctata, Forbes.
filiformis, Miiller.
securigera, D. & K.
bellis, Link.
brachiata, Mont.
Ballii, Thonups.
Goodsiri, Forbes.
granulata, Link.
rosula, Link,
minuta, Fortes.
Subfam. Euryalide.
Astrophyton, Link.
scutatum, Link.
*Asteronyx, Miill. & Troschel.
Loveni, M. & T.
Order ASTEROIDEA.
Fam. Asteriade.
Uraster, Agassiz.
glacialis, Linn.
rubens, Linn.
violacea, Miiller.
hispida, Penn.
rosea, Miiller.
Echinaster, Miiller §- Troschel.
oculatus, Penn.
Solaster, Forbes.
endeca, Linn.
papposa, Linn.
REPORT—1860.
Palmipes, Link.
membranaceus, Refz.
Asterina, Nardo.
gibbosa, Penn.
Goniaster, Agassiz.
Templetoni, 7omps.
equestris, Gmelin.
Abbensis, Forbes.
Asterias, Linneus.
aurantiaca, Linn.
Luidia, Forbes.
fragilissima, Forbes.
Savignii, Audouwin.
Order ECHINOIDEA.
Fam. Cidaride.
Cidaris, Leske.
papillata, Leske.
Echinus, Linneus.
sphera, Miiller.
Flemingii, Ball.
miliaris, Leske.
lividus, Lamk.
melo, Lamk.
Norvegicus, D. & K.
neglectus, Lamk.
Fam. Clypeasteride.
Echinocyamus, Leske.
pusillus, Miller.
Echinarachnius, Leske.
placenta, Gmelin.
Fam. Spatangide.
Spatangus, Klein.
purpureus, Miller.
Brissus, Klein.
lyrifer, Forbes.
Amphidotus, Agassiz.
cordatus, Penn.
roseus, Yorbes.
gibbosus, Barrett.
POLYZOA.
Class ECHINODERMATA.
Order HOLOTHUROIDEA.
Fam. Pentactide.
Cucumaria, Cuvier.
frondosa, Gunner.
? fucicola, Forbes & Goodsir.
pentactes, Miiller.
? Montagui, Flem.
? Neillii, Flem.
? dissimilis, Flem. t
fusiformis, Forbes & Goodsir.
Hyndmanni, Thomps.
Ocnus, Forbes (=Cucuma-
ria ?).
brunneus, Forbes.
lacteus, Forbes & Goodsir.
Psolinus, Forbes.
brevis, Forbes & Goodsir.
Fam. Thyonide.
Thyone, Oken.
fusus, Mill.
Abildg.)
raphanus, Diiben § Koren.
communis, F. & G. (Thy-
onidium, D. ¢ K.)
Portlockii, Forbes.
Drummondii, Thomps.
pellucida, Vahl (Cucuma-
ria hyalina, F.). j
Aolothuria, Linn.
nigra, Couch.
intestinalis.
tubulosa, Linn.
Fam. Psolide.
Psolus, Oken.
phantopus, Linn.
Forbesii.
(papillosa,
Fam. Synaptide.
Synapta, Esch.
inherens, Mill.
digitata, Mont.
*,* Classified as in the British Museum Catalogue by Mr. George Busk.
Order I.
INFUNDIBULATA.
Suborder I. Cheilostomata.
Fam. II. Salicornariade.
Salicornaria, Cuvier.
farciminoides, Johnst.
Johnstoni, Busk.
sinuosa, Hassall.
Onchopora, Busk.
borealis, Busk.
Fam. ITI. Cellulariade.
Cellularia, Pallas.
Peachii, Bus.
cuspidata, Bush.
Menipea, Lamourouzx.
ternata, Ellis & Soland.
Scrupocellaria, Van Beneden.
scrupea, Bush.
scruposa, Linn.
Canda, Lamouroux.
reptans, Pall.
Fam. IV. Scrupariade.
Scruparia, Oken.
chelata, Linn.
clavata, Hincks.
Salpingia, Coppin.
Hassallii, Coppin.
Hippothoa, Lamourouc.
catenularia, Jameson.
divaricata, Lam,
FEtea, Lamourouc.
anguina, Linn.
truncata, Landsb.
recta, Hincks.
Beania, Johnston.
mirabilis, Johnst.
Fam. VI. Gemellariadez.
Gemellaria, Savigny.
_loricata, hand *
Notamia, Fleming.
bursaria, Linn.
‘
F
+4
x
Z
f
# linearis, Hassall.
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA.
Fam. VII. Cabereade.
Caberea, Lamourouzx.
Hookeri, Ftem.
Boryi, Aud.
Fam. VIII. Bicellariade.
Bicellaria, De Blainville.
ciliata, Linn.
Alderi, Bush.
Bugula, Oken.
neritina, Linn.
flabellata, J. V. Thomps.
avicularia, Pall.
plumosa, Pall.
Murrayana, Bean.
turbinata, Alder.
fastigiata, Fabr.
Fam. IX. Flustrade.
Flustra, Linn.
foliacea, Linn.
papyracea, Hillis.
truncata, Linn.
Barleei, Bush.
Carbasea, Gray.
papyrea, Pall.
Fam. X.
Membraniporide.
Membranipora, De Blainville.
membranacea, Linn.
pilosa, Pall.
coriacea, Esper.
lineata, Linn.
Flemingii, Bush.
Rosselii, Audouin.
Lacroixii, Savigny.
monostachys, Bush.
hexagona, Bush.
Pouilletii, Audouin.
spinifera, Johnst.
craticula, Alder.
unicornis, Fem.
imbellis, Hincks.
Lepralia, Johnston.
Brongniartii, Aud.
Landsboroviui, Johnst.
reticulata, Macgillivray.
auriculata, Hassall.
concinna, Bush.
verrucosa, er.
violacea, ate
spinifera, Johnst.
trispinosa, Johnst.
coccinea, Abildg.
ciliata, Pall.
Gattye, Landsb.
_ Hyndmanni, Johnst.
yariolosa, Johnst.
hitida, Fabr.
_ annulata, Fabr.
bispinosa, Johns¢.
Peachii, Johnst.
yentricosa, Hassall.
melolontha, Landsb.
innominata, Couch.
punctata, Hassall.
figularis, Johnst.
pertusa, sper.
Pallasiana.
labrosa, Busk.
simplex, Johnst. .
Malusii, Aud.
granifera, Johnst.
hyalina, Linn.
ansata, Johnst.
unicornis, F/em.
ringens, Bush.
fissa, Bush.
Cecilii, Audouin.
Barleei, Bush.
canthariformis, Bush.
umbonata, Bush.
discoidea, Bush.
bella, Bush.
monodon, Bush.
alba, Hincks.
eximia, Hincks,
Woodiana, Busk.
Alysidota, Bush.
Alderi, Busk.
Fam. XI. Celleporide.
Cellepora, Fabr.
pumicosa, Linn.
Hassallii, Johnst.
vitrina, Couch.
ramulosa, Linn.
Skenei, Hillis & Soland.
tubigera, Bush.
armata, Hincks.
avicularis, Hincks.
Fam. XII. Escharide.
Eschara, Ray.
foliacea, Ellis & Soland.
cervicornis, Soland.
cribraria, Johnst.
Retepora, Lamarck.
cellulosa, Linn.
Beaniana, King.
Suborder IT. Cyclostomata.
Fam. I. Tubuliporide.
Tubulipora, Lamarck.
patina, Zinn.
hispida, Flem.
penicillata, Johnst.
truncata, Jameson.
lobulata, Hassall.
phalangea, Couch.
flabellaris, Fabr.
serpens, Linn.
hyalina, Couch.
Diastopora, Lamourouz.
obelia, Flem.
Idmonea, Lamourouz.
Atlantica, Forbes.
Pustulipora, De Blainville.
proboscidea, M.-Edw.
231
deflexa, Couch.
Orcadensis, Busk.
Alecto, Lamourouc.
granulata, M.-EHdw.
major, Johnst.
dilatans, Johnst.
incurvata, Hincks.
Fam. II. Crisiade.
Crisia, Lamouroux.
eburnea, Linn.
denticulata, Lamk.
aculeata, Hassall.
geniculata, 1.-Edw.
Crisidia, M.- Edwards.
cornuta, Zinn.
setacea, Couch.
Suborder III. Ctenostomata.
Fam. I. Aleyonidiadz.
Alcyonidium, Lamourouz.
gelatinosum, Pallas.
hirsutum, FVem.
parasiticum, Fem.
mamillatum, Alder.
albidum, Alder.
hexagonum, Hincks.
Cycloum, Hass.
papillosum, Hass.
Sarcochitum, Hass.
polyoum, Johnst.
Fam. IT. Vesiculariade.
Amathia, Lamourous.
lendigera, Linn.
Vesicularia, Thompson.
spinosa, Linn.
Valkeria, Fleming.
cuscuta, lis,
uva, Linn.
pustulosa, Johnst.
Mimosella, Hincks,
gracilis, Hincks.
Avenella, Dalyell.
fusca, Dalyell.
Notella, Gosse.
stipata, Gosse.
Bowerbankia, Farre.
imbricata, Johnst.
Farrella, Ehrenberg.
repens, Johnst.
elongata.
gigantea. "
pedienlisie, Alder.
ilatata, Hincks.
Anguinella, Van Beneden.
palmata, V. Ben.
Buskia, Alder.
nitens, Alder.
Fam. III. Pedicellinidz.
Pedicellina, Sars.
echinata, Sars.
Belgica.
gracilis.
232
REPORT—1860.
Subkingdom Ca@LenTerRata.
Class HYDROZOA.
*,* This list is compiled from Dr. Johnston’s “ British Zoophytes ” (2nd edit.), Forbes’s
‘“‘ British Naked-eyed Medusz,” and the works of Mr. Alder, Prof. Allman, Mr. Cobbold,
Mr. Gosse, Professor Greene, Rey. Thomas Hincks, Professor Huxley, Dr. T. Strethill
Wright, &c.
Order CORYNIDZ.
Fam. I. Coryniade.
Clava, Gmelin.
multicornis, Johnston (re-
pens, 7. 8. Wright; dis-
creta, Allman).
cornea, T. S. Wright.
membranacea, T. 8. Wright.
Vorticlava, Alder.
humilis, Alder.
Lar, Gosse.
Sabellarum, Gosse.
Hydractinia, Van Beneden
(Podocoryna, Sars).
echinata, Flem.
carnea, Sars.
Mpyriothela, Sars.
arctica, Sars.
Clavatella, Hincks.
prolifera, Hincks.
Coryne, Gaértner.
pusilla, Zhr.
Sarsii, Lovén (decipiens,
Dujardin).
ramosa, Ehr. (Listerii, Van
Beneden).
sessilis, Gosse.
gravata, T. S. Wright.
eximia, Allman.
implexa, TZ. S. Wright
(Tubularia implexa,
Alder; ?C. Briareus,
Allman).
Cerberus, Gosse.
stauridia, Dujardin.
[Should be referred to
the next genus. ]
Stauridia, T. S. Wright.
producta, T. S. Wright.
Trichydra, T. S. Wright.
pudica, T. S. Wright.
Fam. IJ. Tubulariade.
Eudendrium, Ehrenberg.
ramosum, Linn.
rameum, Pail.
capillare, Alder.
arbuscula, 7. S. Wright.
Atractylis, T. 8. Wright.
ramosa, Van Beneden.
repens, 7. S. Wright.
sessilis, T. S. Wright.
Dicoryne, Allman.
conferta, Alder (Eudend.
confertum, Alder).
Garveia, T. S. Wright.
nutans, 7. S. Wright. _
Bimeria, 7. S. Wright.
yestita (Manicella fusca,
Allman).
Tubularia, Linneus.
indivisa, Linn.
Dumortierii, Van Beneden.
larynx, Ellis.
gracilis, Harvey.
Corymorpha, Sars.
nutans, Sars.
nana, Alder.
Order SERTULARID®.
Fam. I. Sertulariade.
Halecium, Oken.
halecinum, Eilis.
Beanii, Johnst.
muricatum, Ellis & Soland.
labrosum, -A/der.
tenellum, Hincks.
Sertularia, Linneus.
polyzonias, Linn.
tricuspidata, Alder.
tenella, Alder.
Gayi, Lame.
rugosa, Ellis.
rosacea, Linn.
pumila, Linn.
gracilis, Hassall.
Eyansii, Ellis & Soland.
nigra, Pallas.
pinnata, Pallas.
alata, Hincks.
pinaster, Ellis & Soland.
Margareta, Hassall.
fallax, Johnst.
tamarisca, Linn.
abietina, Linn.
filicula, Ellis & Soland.
operculata, Linn.
argentea, Ellis & Soland.
cupressina, Linn.
fusca. Johnst.
Thuiaria, Fleming.
thuia, Linn.
articulata, Pallas.
Antennularia, Lamarck.
antennina, Linn.
ramosa, Lame.
Plumularia, Lamarck.
falcata, Linn.
cristata, Lamk.
pennatula, Ellis & Soland.
myriophyllum, Linn.
tubulifera, Hincks.
pinnata, Linn.
setacea, Ellis.
Catherina, Johnst.
echinulata, Lamk.
similis, Hincks.
frutescens, Ellis & Soland.
halecioides, Alder.
obliqua, Saunders (Lao-
medea obliqua, Johnst.).
Fam. IT.
_ Campanulariade.
Laomedea, Lamourouz.
dichotoma, Linn.
longissima, Pallas.
geniculata, Linn.
flexuosa, Hincks.
Lovéni, Ad/man.
gelatinosa, Pallas.
angulata, Hincks.
neglecta, Alder.
pulchella, Wyville Thomson.
lacerata, Johnst.
tenuis, Allman.
acuminata, Alder.
Campanularia, Lamarck.
yolubilis, Linn.
Jobnstoni, Alder.
Hincksii, Alder.
raridentata, Alder.
integra, Macgillivray.
caliculata, Hincks.
verticillata, Linn.
[intertexta, Couch—a very
doubtful species. |
Calicella, Hincks.
dumosa, Flem.
gracilluma, Alder.
parvula, Hincks.
syringa, Linn.
fastigiata, Alder.
humilis, Hincks.
Reticularia, Wyville Thomson.
serpens, Hassall.
Grammaria, Stimpson.
ramosa, A/der.
Coppinia, Hass. [The position
of this genus is doubtful.]
arcta, Dalyell.
Order CALYCOPHORID JE.
Fam. Diphyde.
Diphyes, Cuvier.
appendiculata, Eschscholtz.
Order PHYSOPHORID#.
Fam. I. Stephanomiade.
(?) Halistemma, Huxley.
rubrum, Vogt.
—_——
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA,
Fam. II. Physaliadz.
Physalia, Lamarck.
pelagica, Eschscholtz.
Velella, Lamarck.
spirans, Forsk.
Order MEDUSID.
Fam. I. Willsiade.
Willsia, Forbes.
stellata, Forbes.
Fam. II. Oceanidz.
Turris, Lesson.
digitalis, O. F. Miiller.
neglecta, Lesson.
constricta, Patterson.
Saphenia, Eschscholtz.
dinema, Péron.
Titania, Gosse.
Oceania, Péron.
octona, Flem.
episcopalis, Forbes,
turrita, Forbes.
globulosa, Forbes.
duealis, Forbes & Goodsir,
pusilla, Gosse.
Fam. III. Ai’quoreade.
Stomobrachium, Brand.
octocostatum, Sars.
Polyxenia, Eschscholtz.
Alderi, Forbes.
/&quorea, Péron.
_ Forskalii, Forbes.
Forbesiana, Gosse.
vitrina, Gosse.
formosa, Greene.
sp., Greene.
Fam. IV. Circeade.
Circe, Mertens.
rosea, Forbes.
Fam. V. Geryoniade.
- Geryonia, Péron.
appendiculata, Fordes,
Geryonopsis, Fordes.
delicatula, Forbes,
Tiaropsis, Agassiz.
Patterson, Greene.
Thaumantias, Hschscholéz.
pilosella, Forbes.
quadrata, Forbes.
aéronautica, Forbes,
octona, Forbes.
maculata, Forbes,
melanops, Forbes.
globosa, Forbes.
convexa, Forbes.
gibbosa, Forbes.
lineata, Forbes.
pileata, Forbes.
Sarnica, Forbes.
Thompsoni, Forbes.
hemispherica, O.F'. Miiller.
inconspicua, Forbes,
punctata, Forbes.
lucifera, Forbes,
Buskiana, Gosse.
corynetes, Grosse.
undulata, Forbes & Goodsir,
confluens, Forbes 4 Goodsir.
achroa, Cobbold.
neglecta, Greene.
typica, Greene.
Slabberia, Forbes.
halterata, Forbes.
catenata, Forbes & Goodsir.
Fam. VI. Sarsiade.
Plancia, Forbes & Goodsir.
gracilis, Forbes & Goodsir.
Goodsirea, Strethili Wright.
mirabilis, S. Wright.
Sarsia, Lesson.
tubulosa, Sars.
pulchella, Forbes.
gemmifera, Forbes,
prolifera, Forbes,
Hippocrene, Mertens.
Britannica, Forbes.
nigritella, Forbes.
233
crucifera, Forbes & Goodsir’
simplex, Forbes & Goodsir:
dinema, Greene.
Lizzia, Forbes.
octopunctata, Sars.
blondina, Forbes,
sp., Claparéde.
Modeeria, Forbes.
formosa, Forbes,
Diplonema, Greene.
Islandica, Greene.
Euphysa, Forbes.
aurata, Forbes.
Steenstrupia, Forbes,
rubra, Forbes,
flaveola, Forbes,
Owenii, Greene.
Order LUCERNARIDA.
Fam. I. Lucernariade.
Lucernaria, Miiller.
auricula, Fabr.
campanulata, Lame,
fascicularis, Fem.
Depastrum, Gosse.
stellifrons, Gosse,
Carduella, Allman.
cyathiformis, Sars,
Fam. IT. Pelagide.
Aurelia, Péron.
aurita, O. F. Miiller.
campanula, O. Fabricius,
Cyanea, Péron.
capillata, Linn.
Lamarckii, Péron.
Pelagia, Péron et Lesueur.
cyanella, Péron e¢ Lesueur,
Chrysaora, Péron.
hysoscella, Linn.
Fam. III. Rhizostomide.
Cassiopeia, Péron.
lunulata, Fem.
Rhizostoma, Cuvier.
ima, Eschscholtz, pyramidata, Forbes & Good- pulmo, Gel.
Bairdii, Johnst. sir.
Class ACTINOZOA.
*x* The list of Zoantharia is taken from Goase’a “ Actinologia.”’ ‘.
Order ZOANTHARIA,
Fam. I. Actiniade.
inolobia, Blainville.
dianthus, Blainv.
agartia, Gosse,
llis, Elvis,
t Miniata, Gosse.
__Yosea, Grosse.
_ ornata, Holdsworth.
ichthystoma, Gosse.
Nivea, Gosse.
_ sphyrodeta, Gosse,
pallida, Holdsworth,
ite
pura, Alder.
coccinea, Miill.
troglodytes, Johnst,
viduata, Miid/.
parasitica, Johnst.
chrysosplenium, Cocks,
Adamsia, Forbes.
palliata, Forbes,
Phellia, Gosse.
murocincta, Gosse.
gausapata, Gosse.
picta, Gosse.
Brodricii, Gosse,
Gregoria, Gosse.
fenestrata, Gosse.
Aiptasia, Cocks.
Couchii, Cocks,
Anthea, Gaértner.
cereus, Hilis,
Actinia, Linn.
mesembryanthemum, Evlis,
Bolocera, Johnst.
Tuedix, Johnst.
eques, Gosse.
Bunodes, Gosse.
gemmacea, Hilis,
thallia, Gosse.
234
Ballii, Cocks.
coronata, Gosse.
Tealia, Gosse.
digitata, Mill.
tuberculata, Cocks.
crassicornis, Miill.
Hormathia, Gosse.
margarita, Gosse.
Stomphia, Gosse.
Churchix, Gosse.
Ilyanthus, Forbes.
Scoticus, Forbes.
Mitchellii, Gosse.
Peachia, Gosse.
hastata, Gosse.
undata, Gosse.
triphylla, Gosse.
cylindrica, Reid.
Halcampa, Gosse.
chrysanthemum, Peach.
microps, Gosse.
Edwardsia, Quatrefages.
callimorpha, Gosse.
carnea, Gosse.
Beautempsii, Quatref.
Arachnactis, Sars.
albida, Sars.
Cerianthus, J. Haime.
Lloydii, Gosse.
vermicularis, Forbes.
Capnea, Forbes.
sanguinea, Forbes,
Aureliania, Gosse.
angusta, Gosse.
heterocera, Thomps.
Corynactis, Al/man.
viridis, Allman.
*,* This list of British Foraminifera is taken from Prof. Williamson's “Recent
Foraminifera of Great Britain,” published by the Ray Society.
Proteonina, Williamson.
fusifornis, W2lliamson.
pseudospiralis, W2ldéamson.
Orbulina, D' Orbigny.
universa, D’ Orb.
Lagena, «Walker.
vulgaris, Williamson.
var. clavata.
yar. perlucida.
yar. semistriata.
yar. striata.
yar. interrupta.
var. gracilis.
yar. substriata.
Entosolenia, Hhrenberg.
globosa, Walker.
yar. lineata.
costata, Williamson.
marginata, Walker.
yar. lucida.
REPORT—1860.
Fam. II. Zoanthidee.
Zoanthus, Cuvier.
Couchii, Johnst.
sulcatus, (Gosse.
Alderi, Gosse.
Fam. III.
Caryophylleade.
Cyathina, Ehrenberg.
Smithii, Fem.
Paracyathus, M.-Edwards
Tamilianus, Gosse.
Thulensis, Gosse.
pteropus, Gosse.
Desmophyllum, Ehrenberg.
Stokesii, M.-Edwards.
Sphenotrochus, M.-Edwards.
Macandrewanus, M.-Edw.
Wrightii, Gosse.
Ulocyathus, Sars.
arcticus, Sars.
Oculina, Lamarck.
prolifera, Linn.
Hoplangia, Gosse.
Durotrix, Gosse.
Balanophyllia, Wood.
regia, Grosse.
Order ALCYONARIA.
Fam. I. Pennatulade.
Pennatula, Linneus.
phosphorea, Linn.
Virgularia, Lamarck.
mirabilis, Linn.
Payonaria, Cuvier.
quadrangularis, Pail.
Subkingdom Protozoa.
FORAMINIFERA.
var. ornata.
yar. lagenoides.
var. quadrata.
squamosa, Mont.
yar. scalariformis.
yar. catenulata.
var. hexagona.
Lingulina, D’ Orbigny.
carinata, D’ Orb.
Nodosaria, Lamarck.
radicula, Linn.
pyrula, D’ Ord.
Dentalina, D’ Orbigny.
subarcuata, Mont.
var. Jugosa.
legumen, Linn.
var. linearis.
Frondicularia, Defrance.
spathulata, W2lzamson.
Archiaciana, D’ Ord,
Fam. II. Aleyonide.
Alecyonium, Linneus.
digitatum, Linn.
glomeratum.
Sarcodictyon, Forbes.
catenata, Forbes.
agglomerata.
Fam. III. Gorgoniade.
Gorgonia, Linneus.
verrucosa, Linn.
pinnata, Linn.
anceps, Ellis.
Primnoa, Lamarck.
lepadifera, Linn.
Order CTENOPHORA.
Fam. I. Cydippide.
Cydippe, Esch.
pileus, Miill.
Flemingii, Forbes.
infundibulum, Mill.
lagena, Forbes.
pomiformis, Paterson.
Fam. II. Calymnide.
Bolina, Paterson.
Hibernica, Paterson,
Fam. III. Beroide.
Beroé, Miiller.
cucumis, Fabr.
fulgens, Flem.
borealis, Less.
Alcinoé, Cu.
rotunda.
Smithii.
Cristellaria, Lamarck.
calear, Linn.
var. rotifera.
yar. oblonga.
subarcuatula, Walker.
var. costata.
Nonionina, D’ Orbigny.
Barleeana, Williamson.
crassula, Walker.
Jeffreysii, Williamson.
elegans, Williamson. —
Nummulina, D’ Orbigny.
planulata, Lam.
Polystomella, Lamarck,
crispa, Linn.
umbilicatula, Walker.
var. incerta.
Peneroplis, Montfort.
planatus, Ficht. & Moll.
Patellina, Williamson.
did h
LIST OF THE BRITISH MARINE INVERTEBRATE FAUNA.
_ corrugata, Williamson.
Rotalina, D’ Orbigny.
Beccarii, Linn,
inflata, Mont.
turgida, Williamson.
oblonga, Williamson.
concamerata, Mont.
nitida, Williamson.
mamilla, Williamson.
ochracea, Williamson.
fusca, Williamson.
Sicbizerins, D Orbigny.
bulloides, D’ Ord.
Planorbulina, D Orbigny.
3 vulgaris, D’ Ord.
‘Truncatulina, D’ Orbigny.
lobatula, Walker.
apo D Orbigny.
pupoides, D’ Ord.
var. marginata.
var. spinulosa.
var. fusiformis.
var. compressa.
-
.
Tethya, Lamarck.
cranium, Johnst. (not Mill.)
lyncurium, Johnst.
eodia, Lamarck.
Zetlandica, Johnst.
‘Pachymatisma, Bowerbank.
Johnstonia, Bowb. (Hali-
' chondria, Johnst.)
Halichondria, Fleming.
panicea, Johnst.
coalita, Johnst.
- coccinea, Bowh. MS.
glabra, Bowb. MS.
inconspicua, Bowb. MS.
caduca, Bowb. MS.
distorta, Bowb. MS.
Dickiei, Bowb. MS.
Batei, Bowb. MS.
_ lingua, Bowd. MS.
-corrugata, Bowd. MS.
ulata, Bowb. MS.
hompsoni, Bowb. MS.
plumosa, Johnst.
1; - eniacidon, Bowerbank
(Halichondria, Johnst.).
4 ii MS.
Halina,
var. convoluta.
elegantissima, D’ Orb.
scabra?, Williamson.
Uvigerina, D’ Orbigny.
pygmza, D’ Orb.
angulosa, Williamson.
Cassidulina, D’ Orbigny.
levigata, D’ Ord.
obtusa, Williamson.
Polymorphina, D’ Orbigny.
lactea, Walker.
var. acuminata.
. oblonga.
. fistulosa.
. concava.
var. communis.
myristiformis, Williamson.
Textularia, Defrance.
cuneiformis, D’ Orb,
var. conica.
variabilis, Williamson.
yar. spathulata.
var. difformis.
rs
albescens, Johnst.
caruncula, Bowb. MS.
Alderi, Bowb. MS.
perlevis, Johnst.
aurea, Johnst.
pachyderma, Bowd. MS.
crustula, Bowb. MS
sanguinea, Johnst.
armatura, Bowb. MS.
floreum, Bowb. MS.
earnosa, Bowb. MS.
viridans, Bowh. MS.
sulphurea, Bowb. MS.
clavigera, Bowb. MS.
subclavata, Bowb. MS.
lactea, Bowb. MS.
Dujardinii (Halisarca),
Johnst.
celata, Johnst.
Bowerbank (Hali-
chondria, Johmnst.).
suberea (Halichondria),
Johnst.
ficus, Johnst.
carnosa, Johnst.
Bucklandi, Bowb. MS.
Isodictya, Bowerbank (Hali-
chondria, Johnst.).
Peachii, Bowb. MS.
rosea, Bowb. MS.
permollis, Bowb. MS.
indistincta, Bowb. MS.
indefinita, Bowb. MS.
Macandrewii, Bows. MS.
dichotoma, Bowd. MS.
cinerea, Johnst.
ramusculus, Bowb. MS.
sunulo, Bowb. MS.
mammeata, Bowb, MS.
235
var. levigata.
Biloculina, D’ F Orbigny.
ringens, D’ Orb,
var. carinata.
Spiroloculina, D’ Orbigny.
depressa, D’ Orb.
var. rotundata.
var. cymbium.
Miliolina, Williamson.
trigonula, Lamk.
seminulum, Linn.
var. oblonga.
var. disciformis.
bicornis, Walker.
var. elegans.
var. angulata.
Vertebralina, D’ Orhigny.
striata, D' Orb.
Spirillina, Ehrenberg.
foliacea, Philippi.
perforata, Schultze.
arenacea, Williamson.
margaritifera, Williamson.
sy LIST OF BRITISH SPONGES.
fucorum, Johnst.
Alderi, Bowd. MS.
Normani, Bowd. MS.
lobata, Johnst.
Barleei, Bowb. MS.
gracilis, Bowb. MS.
Gregorii, Bowb. MS.
Beanii, Bowb. MS.
clava, Bowb. MS.
infundibuliformis, Johnst.
Desmacidon, Bowerbank(Ha-
lichondria, Johnst.).
zegagropila, Johnst.
fruticosa, Johnst.
Raphyrus, Bowerbank.
Griffithsii, Bowb. MS.
Dictyocylindrus, Bowerbank
(Halichondria, Jolnst.).
stuposus, Johnst.
Howsei, Bowb. MS.
ramosus, Johnst.
aculeatus, Bowb. MS.
ventilabrum, Bows. MS.
fascicularis, Bowd. MS.
rugosus, Bowd. MS.
Haliclona, Bowerbank (Hali-
chondria, Johnst.).
palmata, Johnst.
Montagui, Johnst.
pygmza, Bowb.
seriata, Johnst.
simulans, Johnst.
columbe, Johnst.
gracilenta, Bowb. MS.
Microciona, Bowerbank, MS.
atro-sanguinea, Bowd, MS.
armata, Bowb. MS.
earnosa, Bowb. MS.
ambigua, Bowb, MS.
2936 REPORT—1860.
levis, Bows. MS. brevis, Bowb. MS. ciliata, Johnst.
spinulenta, Bow: MS. robusta, Bowb. MS. ensata, Bowb. MS.
Hymeraphia, Bowerhank,MS. Halicnemia, Bowerbank, MS. tessellata, Bowd. MS.
vermiculata, Bows. MS. patera, Bowb. MS. Leuconia, Bowerbank (Gran-
stellifera, Bowb. MS. Phakellia, Bowb. MS. (Hali- tia, Johnst.).
clavata, Bowb. MS. chondria, Johnst.). nivea, Johnst.
Hymedesmia,Bowerbank,MS. _ ventilabrum, Johnst. fistulosa, Johnst.
Zetlandica, Bowb. MS. Dysidea, Johnston. Leucosolenia, Bowerbank,
Halyphysema, Bowerbank, fragilis, Johnst. MS. (Grantia, Johnst.).
MS. Spongia, Linneus, botryoides, Johnst.
Tumanowiczii, Bowd. MS. pulchella, Johnst. coriacea, Johnst.
Euplectella, Owen. limbata, Johnst. lacunosa, Johnst.
mammillaris (Halichon- Grantia, Fleming. contorta, Bowb. MS.
dria), Johnst, compressa, Johnst.
ess
_ >
NOTICES AND ABSTRACTS
OF
MISCELLANEOUS COMMUNICATIONS TO THE SECTIONS,
MATHEMATICS AND PHYSICS.
MATHEMATICS.
Address by the Rev. Prof. Price, 4.A., F.R.S., President of the Section.
GENTLEMEN,—A custom has prevailed at our Meetings for some years for the Pre-
sident of each Section to make a short address at the opening. The object of it I
take to be twofold; first, to explain to new members the nature of the business which
we have to transact; and, secondly, to suggest to all the course of rocedure, and
the distribution of subject most convenient for the conduct of our business, The
area of scientific research which this Section covers is very large, larger perhaps
than that of any other; and its subjects vary so much, that while to some of
those who frequent this room certain papers may appear dull, yet to others they
will be full of interest. There are many and very good reasons why these subjects
should be grouped. Some of them possess, probably in the highest degree attain-
able by the human intellect, the characteristics of perfect and necessary science ;
while others are at present little more than a conglomeration of observations, made
indeed with infinite skill and perseverance, and of the greatest value ; capable
probably in time of greater perfection, nay, perhaps, of most perfect forms, but as
yet in their infancy, scarcely indicating the process by which that maturity will
e arrived at, and containing hardly the barest outline of their ultimate laws, We
have indeed sciences intermediate to these two extremes, in which some of the laws
are already capable of mathematical expression, and from which results have been
derived, and still many phenomena are as yet not brought within their comprehen-
sion. But as all subjects which we regard in this Section are of one type, so are
they rightly combined; and it will be, I venture to think, an evil day for natural
Imowledge, when we cease to regard the forms of the sciences of space, number,
and motion, as those to which all others ought to assimilate themselves.
Now first of all in our Section stand Mathematics, both pure and applied. These,
indeed, require very heavy and arduous study, inasmuch as they have peculiar
nomenclature, language, and processes, and thus it is only to the few generally who
have made them their particular study that they offer great interest. Mathematics
have also now become so large in their grasp and so curious in their details, that I
am, I am sure, only expressing the opinions of most analysts when I say that the
whole of a man’s life is not sufficient for more than one branch of it. Indeed,
and we are proud to say so, some members of this Association are devoting whole
lives, and intellects too of the highest order, to the advancement of our knowledge
in a particular direction. Take, for instance, the theory of homogeneous forms:
in the history of science the names of Boole, Cayley, Sylvester will always be
recorded, and in scientific treatises their labours will find a place. Or take again
the theory of elliptic functions, or the calculus of probabilities ; the difficulties of
these subjects require the utmost tension of the human mind, and even then they
transcend its limits. To many of the usual attendants on this Section, these and
__ kindred subjects may be dry and uninteresting. Well, if they are so to any of you,
_ I must beg you to bear with us for a short time; these things have a deep and
1860.
2 REPORT—1860.
significant meaning; and be assured too that they are not uninteresting to all; to
many they give the purest pleasure; and I must ask you not to grudge them that
during the few pale on the higher mathematics which we shall probably have.
In passing, too, [ would remind you that very frequently our knowledge of natural
phenomena depends on certain integrals, the properties of which can only be
studied with a profound knowledge of the higher mathematics; and thus the pro-
gress of one branch of knowledge depends on another, and is frequently stopped by
our ignorance of that.
_ To most of us, probably, the questions of applied mathematics will have greater
interest; we are more familiar with the laws of nature, the mathematical interpre-
tation of which, mixed mathematics, as they are called, take cognizance of ; we
most eagerly catch at the results of those laws. Consider the Newtonian law of
gravitation in its most general form; in its highest development in the lunar and
planetary theories, a dry mathematical paper will thin our room; an astronomical
paper will often fill it; and now too, perhaps, more than heretofore; for our
interest in the subject has been keenly aroused of late. The lunar disturbances
have been, as you know, calculated with greater precision, and new results have
been arrived at, which exhibit certain discrepancies relatively to the old. I
need do no more than allude to what has lately taken place at our own Royal
Astronomical Society and at the French Academy; and express a hope that we
shall have some communication on this subject from those who are here present, and
are so well qualified to give it. Mathematicians, however, have been startled by
an announcement that “ what is commonly called mathematical evidence is not so
certain as many persons imagine; and that it ultimately depends on moral evidence ;”
and moreover we are told that the “results of long and complicated mathematical
calculations are not more than probably true.” This we can hardly believe; it
takes us quite by surprise, and we hope for further light; if, however, we must
wait for light, we must wait patiently; let us not forestal a conclusion which many
of us venture to think is as yet, not to say more, unproved; let us wait for the
new lunar theories, which are as yet unpublished, and for the new lunar tables,
which are the results of these theories. I am told, however, already that Baron
Plana has corrected his calculations, and that he finds the results arrived at by
Delaunay and Adams to be in accordance with his amended formule. These new
lunar calculations have taken us by surprise; but again I would say let us wait,
“magna est veritas et preevalebit.”
_ We are desirous, so far as is possible consistently with the convenience of con-
tributors, to take the papers on mathematical subjects on the early days of our
meeting ; and we shall es glad therefore if members who have papers on these sub-
jects will announce them to the Secretaries without delay. And before I proceed
further, we have a debt to pay, due by the cultivators of these branches of science,
to those who have lately contributed reports on particular parts of our science to
the British Association ;—to Mr. Cayley for his report on the present state of
Theoretical Dynamics, and to Mr. Smith for the first part of his report on the
Theory of Numbers. It is only they who have had to go through the existing
literature in any one problem, say the Lagrangian equations, or the theory of the
motion of a material system, that can form an adequate value of such papers as
those I refer to: the literature is catalogued, indexed, and analysed; we know
thereby all that has been done up to a certain point, and in our subsequent inves-
tigations our commencement starts from the close of other men’s labours. We
are hereby prevented from travelling over other men’s ground; and we avoid that
most unsatisfactory plagiarism of them, “qui nostra ante nos dixerunt.” Vast and
various are the benefits of our Association ; but I am inclined to consider as one of
the greatest, the series of valuable reports which our published volumes contain ;
and those last reports to which I have referred, for their learning, their deep re-
search, their comprehensive views of the theories explained in them, will maintain
the character shared by their predecessors. While we lament the loss of Dr. Pea-
cock and others, to whom we owe the very able reports contained in the early
volumes of our proceedings, we are proud to have worthy successors in our present
talented contributors.
We propose, next in order, to take those papers which treat of subjects within the
grasp of mathematical symbols, at least partially, if not wholly; those whose laws
iN cio
an
es
TRANSACTIONS OF THE SECTIONS. 3
are sufficiently general for functional symbols, and from particular forms of which
by mathematical processes other truths may be derived. Such are the subjects of
Light, Heat, Sound, Electricity, Magnetism ; we propose to take these subjects in
the latter days of this week, and the first day of next. We shall, of course, con-
sult the conyenience of contributors; but it will tend, we think, to the orderly
arrangement of our business if this order can be adopted. Vast indeed in their
subjects are these sciences; and as discoveries are being daily made in them,
we have a right to expect some interesting communications, either in the way
of mathematical deduction from received laws, or as mathematical explana-
tions of observed phenomena, or as simple experiments. I cannot help observing
here the advantage of combining these sciences in the same Section with pure
mathematics ; it seems to indicate that the laws of all are to be brought to the
same test,—to the never-failing, to the unerring accuracy of measurement and num-
ber ; we show hereby the character of the knowledge we are in search of ; not for-
tuitous observation, but precise laws. The mind will wander in its imagination ;
there is, indeed, no boundary to it; once, however, bring it back to the severe test
of number and weight and measurement, and the discovery or the observation
becomes valuable for its precision ; it thus leads to general laws, and sound mathe-
matical reasoning derives from them the results they are pregnant with.
And, finally, we come to the facts of meteorology and its kindred subjects, man
of which are scarcely yet brought within any law at all; analogies have been traced,
and concurrent events have been indicated in many cases; little, however, has been
done: towards a satisfactory proof of a connexion between cause and effect. It is
true that curves are traced, which purport to exhibit these effects; and they do so
most graphically ; but, as mathematicians say, these curves are traced only by points,
and the law is not known, or, in other words, we do not know the equation of the
curve; so long as this is the case, our knowledge lacks precision. ‘These papers,
howeyer, are frequently valuable, because they supply us with accurately observed
_ facts, which will doubtless hereafter be brought within a law. This, however, I
_ Suppose at present to be the state of the case; but we must not despise the lesser
light because we have not the greater. I cannot pass over this class of papers (papers
: of observed facts) without alluding to the loss which we all feel in the death of the
late able Professor of Geometry, Professor Baden Powell. For some years past
_has he continued his reports on the meteors or falling stars, or whatever you call
_ them ; this year we have his last report, which, indeed, he has not lived to finish,
_ but has been placed in the hands of Mr. Glaisher, and completed by him. In
some of these subjects we shall, I hope, obtain large accessions to our fre lodee.
__ Some few years ago I remember reading a complaint made by an eminent philo-
Sopher on the decay of mathematical knowledge in Great Britain, and especially in
“that of physico-mathematical knowledge. It is not my duty to make invidious
distinctions ; but I am sure I am repeating the now common opinion of foreigners
when I tell you that that complaint was made in quite the infancy of some of
our older philosophers, and before the days of Cayley, Sylvester, Boole, Mac-
“eullagh, Stokes, W. Thomson, and Adams. To this revival of science amongst
us, doubtless, many causes have contributed ; and I believe that the periodical Yneet-
‘ngs of this Association have done good service towards that revival; we have
“hereby become acquainted with others who are engaged in the same pursuits as our-
Selves, and stores of knowledge are communicated. Let us, however, bear in mind
that our Association is formed for the advancement of science, and that we do not
meet to hear of old things again in the old form; our motto is “progress.” Old
things we do not discard, for they may be put before us in new forms: but we meet
especially to promote the advance of the boundaries of natural knowledge, and we ask
our members and others to lay before us the results of their investigations. And not
mly in the papers which shall be read, but also in the elucidation of any difficulties
which authors may favour us with, and in the discussions which it is my duty to
nyite you to take upon these papers, will additions to our knowledge be made;
and many remarks will, I venture to think, be made pregnant with matter for
oughtful meditation hereafter. In all these discussions difference of opinion
will doubtless arise ; but I am sure that a spirit of friendly and mutual concession
l prevail ; and that in our search after truth we shall gladly and readily attribute
0 those who differ from us the same pure motives which we claim to ourselves,
|*
t
4: REPORT—1860.
On some Solutions of the Problem of Tactions of Apollonius of Perga by
means of Modern Geometry. By Dr. BRENNEcKE, of Posen.
The author suggested a new solution, depending on a remarkable property of the
centres of similitude of three given circles; e. g. a circle described around an exter-
nal centre of similitude, with a radius equal to the geometrical proportional of its
potential distances from the two circles, intersects all homogeneously touching circles
orthogonally (around an internal centre all heterogeneously touching circles). Such
a circle is called a potential circle. To get the two circles which touch the three
given circles simultaneously internally or externally, take two external centres of
similitude, draw the two potential circles, find their radical axis, which will contain
the centre of similitude of the two circles which cut the three given circles in the
same time externally or internally. By combining the three external centres of
similitude, you find three potential circles and three radical axes, which all three
coincide. Having found this straight line, which contains the centres, it is easy to
find the centres themselves by introducing a fourth circle, the reHected mirror-image
as it were of any of the three given circles, by means of the found radical axis, and
finding out the two circles which touch the two symmetrical circles and any one of
the three given circles. Dr. Brennecke has treated the subject at large in a book
which has just now been published at Berlin, ‘ Die Bertthrungsaufgabe fur Kreis und
Kugel,’ Th. Chr. Fr. Enslin, 1860, 8vo, illustrated by eighty-four diagrams, in which
all information will be found concerning the most renowned problem of geometry,
concerning the problem of tactions of three given circles or four given spheres.
On a New General Method for establishing the Theory of Conic Sections.
By the Rev. James Boorn, LL.D., F.RS.
On the Relations between Hyperconic Sections and Elliptic Integrals.
By the Rev. James Bootu, LL.D)., ERS.
In this communication the author extended the analogies that the Continental and
English geometers had established between elliptic integrals of the third order under
the circular form, and the arcs of spherical conic sections, to the corresponding rela-
tions between elliptic integrals of the third order and logarithmic form to the arcs of
carves described in the surface of a paraboloid.
On Curves of the Fourth Order having Three Double Points.
By A. Cayrey, PRS.
The paper is a short notice only of researches which the author is engaged in
with reference to curves of the fourth order having three double points. A curve
of the kind in question is derived from a conic by the well-known transformation of
substituting for the original trilinear coordinates their reciprocals ; and the species of
the curve of the fourth order depends on the pesition of the conic with respect to the
fundamental triangle.
Cn the Trisection of an Angle. By Parnricx Copy.
Sx a aan 5
On the Roots of Substitutions. By the Rev. T. P. Kirkman, A.M, PRS.
To determine the number of roots of a given degree, of a substitution @ made with
n letters, and of the rth order. A substitution @ which has not two circular factors —
of the same order, has no roots which are not found among the series
of its powers, ~apellegt et
A substitution which has two or more circular factors of the same order, will have
roots of an order superior to its own, and therefore not among its power. |
Thus the substitution of the 3rd order made with 9 elements,
__ 231564897
~~ 123456789"
has 1 square root of the 3rd order, 9 square roots of the 6th order, 9 fourth roots
of the 6th order, 18 cubic roots of the 9th order, and 18 sixth roots of the 9th
TRANSACTIONS OF THE SECTIONS. is)
order. These roots can be enumerated by a simple general method for @ of any
order, made with 7 letters.
The fundamental theorem is the following :—
If n=Aa+Bb+Cc+......, the number of different groups of the order K, which
is the least common multiple of ABC... ., of the form
Os Oo nerc Osa,
whereé hasa circular factors of the order A, d of the order B, &c.,is (wmu=1.2.3...2),
TN
,
Rx A“B’C’..aanbaec...
Rx being the number of integers, unity included, which are !ess than K and prime
to it.
The partition n=9=3.3=Aa
gives WOO ee 5.4
Rs 33. 73 phar
groups, 166 ly ed Hy eerreei t0(G)
j2
of the third order, which is that of 6 and of 6°.
The partition
n=9=6.14+3.1=Aa+Bb
gives TO
fic pra Pacer ee ttn ta
groups, 1p’... $’, eit Ss Lee att arTs On wh eh teh CED)
of the 6th order. Every group (H) contains a group (G), namely,
1 2 ht
and ¢ of the 6th order is the square root of ¢? of the 3rd order, and the fourth root
of * of the 3rd order. Also #” of the 6th order is the square root of ¢*, and the
fourth root of d.
The number of groups (H) being nine times that of the group (G), the group 166°
will be comprised in nine different groups (H) ; that is, @ has nine square roots of
the 6th order, and nine fourth roots of the same order.
The partition
n=9=9.1=<Aa
gives OG
‘ Ro 9 Cee Die a bled
> groups, lyy? eee Vv’, . 28 @ e968, On Viewed te 8 eS le (J)
of the 9th order. This comprises the group (G),
f Wy
where y’ has the cube roots p y' w" of the 9th order, and the sixth roots py? p’ 1p"
of thesame order. ‘There are six times as many groups (J) as groups (G). Therefore
106?
will be found in six groups (J), and either 6 or 6? has 18 cube roots, and 18 sixth
roots all of the 9th order.
Inthe same manner it is easily proved that the substitution of the 2nd order(n=8),
g'— 34127856
12345678
which has four circular factors of the 2nd order, has twelve square roots all of the
4th order. These form with unity and 6’ the two groups following,
12345678 12345678
34127856 34127856
58763214 23418567
76581432 41236785
23416785 78561234
41238567 56783412
87652143 85674123
65874321 67852341
6 ; REPORT—1860.
which are of the form (IV.) discovered by Mr. Cayley (Phil. Mag. vol. viii. 1859,
p- 34), who there first enumerated the forms of groups of eight.
Two such groups can be completed with unity, and any one of the
78
ee] Oh Ae
R,. 4°. 7 2
substitutions of the form 6’,
It is easy to form groups of Mr. Cayley’s form (II.) ; e. g.,
12345678
34127856
23416785
41238567
56781234
78563412
67852341
85674123
which is-one of the grouped. groups whose general theory I have handled in a memoir
which will shortly see the light.
On a new Proof of Pascal's Theorem. By the Rev. T. Rennison, M.A.
On Systems of Indeterminate Linear Equations.
By O. J. Stepnen Suits, .A., Fellow of Balliol College, Oxford.
The object of this communication was to point out the connexion which exists
between particular solutions of indeterminate linear equations, and their most gene-
ral solution. The principle upon which this connexion depends may be explained in
a very particular case. Let the sytem of indeterminate equations reduce itself to the
single equation
Ag By z=, 1 gcrdip s gutgialaiia als a ietais aia seal)
in which we may suppose A, B, C to have no commun divisor; let also a, 6, c and
a', b', c’ be two different solutions of that equation in integral numbers; then, if the
three numbers
be'—0'c,. eai—op', 0 abl—alb =... x). 2» oases erets (2)
admit of %o0 common divisor, the complete solution of the indeterminate equation is
contained in the formule
x=at+a'u,
ies OL te wots a tea mia igas's Cgasphasletia en)
z=ct+c'u,
in which ¢ and wu are absolutely indeterminate integral numbers; but if the condi-
tion (2) be not satisfied, the formule (3) will not represent all, but only some of the
solutions of the equation (1). If, therefore, by any method, as for example that of
Kuler, we have arrived at formule of the type of the formule (3), which demonstra-
bly contain the complete solution of the indeterminate equation, we may be certain
that the three numbers analogous to the numbers (2) admit of no common divisor.
Thus, by applying Euler’s method of solution, which is explained in most books of
algebra, to the indeterminate equation Aw+ By+Cz=0, we obtain the solution of a
celebrated problem, first considered by Gauss in the ‘ Disquisitiones Arithmetice,’
of which the following is the enunciation.
“Given 3 numbers A, B, C, to find six others,
a, b,c,
such that eli 0
A=be'—b'c, B=ca'—ac', C=ab'—a'b.”
Other methods more symmetrical, and perhaps not more tedious than that of Euler, —
were also suggested in this paper for the treatment of indeterminate equations, and
for the resolution of an important class of arithmetical problems which depend on
those equations in the manner just explained.
ee
be eet
TRANSACTIONS OF THE SECTIONS. 7
On a Generalization of Poncelot’s Theorems for the Linear Representation
of Quadratic Radicals. By Professor Sytvester, M.A., F.RS.
The author explained the application of Poncelet’s theorems, to practical ques-
tions of mechanics in the case of forces acting in a single plane as in the theory of
bridges.
He next referred to the mode of extension of this theorem, suggested by Poncelet,
applicabie to the case of forces in space, and pointed out its insufficiency, and, ina
certain sense, its incorrectness,
The essential preliminary question to be resolved in the first instance (after which
the matter became one of easy calculation), was shown to be that of cutting off by
a plane the smallest possible segment of a sphere that should contain the whole of a
given set of points lying on the sphere’s surface. Some years ago Prof. Sylvester
had proposed in the ‘ Quarterly Mathematical Journal,’ without any suspicion of
its haying any practical applications, the following question :—* Given a set of points
in a plane to draw the smallest possible circle that should contain them all.” By a
singular coincidence, Professor Pierce, of Cambridge University, U.S., had studied
this question and obtained a complete solution of it, which he had communicated to
the author during the present meeting of the British Association. A slight con-
sideration served to show that precisely the same solution as Professor Pierce had
found for the problem of points in a plane was applicable with a merely nominal
change to the sphere also; and thus the solution of a question set almost in sport
was found to supply an essential link for the complete development of a method of
considerable importance in practical mechanics. The author stated that it would
be easy to draw up tables of the values of the constants appearing in the linear
function, representing the resultant of three forces at right angles to one another,
for the principal cases likely to occur in practice, the values of these constants
depending solely upon the condition of relative magnitude to which the component
forces are supposed to be subjected,
Licut, Heat.
On the Influence of very small Apertures on Telescopic Vision.
By Sir Davin Brewster, A.M, F.RS.
[The manuscript of this paper has been lost. |
On some Optical Illusions connected with the Inversion of: Perspective.
By Sir Davin Brewster, K.H., F.RS.
The term “Inversion of Perspective” has been applied to a class of optical
illusions, well known and easily explained, in which depressions are turned into
eleyations, and eleyations into depressions. One of the most remarkable cases of
this kind, which has not yet been explained, presented itself to the late Lady
Georgiana Wolf, and has been recorded by her husband Dr. Wolf. When she was
riding on a sand-beach in Egypt, all the footprints of horses appeared as elevations,
in place of depressions, in the sand, No particulars are mentioned, in reference to
the place of the sun, or the nature of the surrounding objects, to enable us to form
any conjecture respecting the cause of this phenomenon. Having often tried to see
this illusion, I was some time ago so fortunate as not only to observe it myself, but
to show it to others. In walking along the west sands of St. Andrews, the foot-
prints, both of men and of horses, appeared as elevations, In a short time they
sank into depressions, and subsequently rose into elevations. The sun was at this
time not very far from the horizon, on the right hand ; and on the left there were
large waves of the sea breaking into very bright foam. The only explanation which
occurred to me was, that the illusion appeared when the observer supposed that
the footprints were illuminated with the fight of the breakers, and not by the sun,
-Haying, however, more recently observed the phenomenon, when the sun was yery
high on the right, and the breakers on the left very distant, and consequently yery
8 REPORT—1860.
faint, I could not consider the preceding éxplanation as well-founded. Upon
attending to the circumstances under which they were now seen, I observed that
the human footprints were all covered with dry sand that had been blown into them,
so that they were much brighter than the surrounding sand, and than the dark side
of the impression next the sun; and hence it is probable that they appeared to be
nearer the eye than the dark sandin which they were formed, and consequently eleva-
tions. After repeated examinations of them, I found the footprints appeared as
elevations as far as the eye could see them; and they were equally visible with one
or both eyes. But whenever the eye rested for a little while on the nearest foot-
print, it resumed its natural concayity.
I have observed other illusions of this kind, which are more easily explained,
though they differ from any hitherto described. In the Church of Saint Agostino
in Rome, there is above cach arch a painted festoon suspended on two short pil-
lars; but instead of appearing in relief, as the painter intended, by shading the one
side of them, they appeared concave, like an intaglio. In other positions in the
church they rose into relief. Upon a subsequent visit to the church, I found that
the festoon, or suspended wreath, was concave when it was illuminated, or rather
when the observer saw that it was illuminated, by a window beneath it, and in re-
lief when the eye saw that it was illuminated by a window above it, the object
being similarly iluminated in both cases. In the common cases of inverted per-
spective, the eye is deceived by looking at the inversion of the shadow in the
cameo or intaglio itself; but in the present case the eye is deceived by perceiving
that the body painted, supposed to be in relief, is illuminated by a light either above
or below it.
An optical illusion of a different kind presented itself to me in the Church of
Santa Giustina at Padua. Upon entering the church we see three cupolas. The
one beneath which we stood appeared very shallow; the next appeared much
deeper, and the third deeper still. They were all, however, of the same depth, as
we ascertained by placing ourselves under each in succession, and observing that it
was always the shallowest.
On Microscopie Vision, and a New Form of Microscope.
By Sir Davin Brewster, KE, TRS.
Io studying the influence of aperture on the images of bodies as formed in the
camera, by lenses or mirrors, it occurred to me that in microscopic vision it might
exercise a still more injurious influence. Opticians have recently exerted their
skill in producing achromatic object-glasses for the microscope with large angles
of aperture. In 1848 the late distinguished optician, Mr. Andrew Ross, asserted
“that 185° was the largest angular pencil that could be passed through a micro-
scopic object-glass,” and yet in 1855 he had increased it to 170°! while some
observers speak of angular apertures of 175°. In considering the influence of aper-
ture, we shall suppose that an achromatic object-glass with an angle of aperture
of 170° is optically perfect, representing every object without colour and without
spherical aberration. When the microscopic object is a cube, we shall see five of
its faces ; and when it isa sphere or a cylinder, we shall see nine-tenths or more of its
circumference. How then does it happen that large apertures exhibit objects which
are not seen when small apertures with the same focal length are employed ?
This superiority is particularly shown with test-ohjects marked with grooves or
ridges, and obliquely illuminated. The marginal part of the lens will enlarge the
grooves and ridges, and they will thus be rendered visible, not because they are
seen more distinctly, but because they are expanded by the combination of their in-
coincident images. Hence we have an explanation of the fact—well known to all
who use the microscope,—that objects are seen more distinctly with object-glasses
of small angular aperture. In the one case we have, with the same magnifying
power, not only an enlarged and indistinct image of objects, but a false representa-
tion of them, from which their true structure cannot be discovered; while in the
other we have a smaller and distinct image, and a more correct representation of
the object:
But these are not the only objections to large angular apertures and short focal
lengths. 1. In the first place, it is extremely difficult to illuminate objects when
pw’ Os See ee ae eee
TRANSACTIONS OF THE SECTIONS. 9
so close to the object-glass. 2. There is a great loss of light, from its oblique in-
cidence on the surtace of the first lens. 3. The surface of glass,—with the most
perfect polish,—must be covered with minute pores, produced by the attrition of
the polishing powder ; and light, falling upon the sides of these pores with extreme
obliquity, must not only suffer diffraction, but be refracted less perfectly than when
incident at a less angle. 4. When the object is almost in contact with the anterior
lens, the microscope is wholly unfit for researches in which mechanical or che-
mical operations are required, and also for the examination of objects enclosed in
minerals or other transparent bodies. 5. In object-glasses now in use, the rays
of light must pass through a great thickness of glass of doubtful homogeneity. It
is a question yet to be solved whether or not a substance can be truly transparent,
--in which the elements are not united in definite proportion,—in which the sub-
stances combined have very different refractive and dispersive powers; and in
which the particles are so loosely united that they separate from one another, as in
the various kinds of decomposition to which glass is liable.
If the best microscopes are affected by these sources of error, every exertion
should be made to diminish or remoye them. 1. The first step, we conceive, is
to abandon large angular apertures, and to use object-glasses of moderate focal
length, effecting at the eye-glass any additional magnifying power that may be re-
quired. 2. In order to obtain a better illumination, either by light incident verti-
cally or obliquely, a new form of the microscope would be advantageous. In place of
directing the microscope to the object itself, placed as it now is almost touching
the object-glass, let it be directed to an image of the object, formed by the thinnest
achromatic lens, of such a focal length that the object may be an inch or more ~
from the lens, and its image equal to, or greater, or less than the object. In this
way the observer will be able to illuminate the object, whether opake or trans-
parent, and may subject it to any experiments he may desire to make upon it. It
may thus be studied without a covering of glass, and when its parts are developed
by immersion in a fluid. 3. The sources of error arising from the want of perfect
polish and perfect homogeneity of the glass of which the lenses are composed, are,
to some extent, hypothetical; but there are reasons for believing,—and these
reasons corroborated by facts,—that a body whose ingredients are united by fusion,
and kept in a state of constraint from which they are striving to get free, cannot
possess that homogeneity of structure, or that perfection of polish, which will allow
the rays of light to be refracted and transmitted without injurious modifications. If
glass is to be used for the lenses of microscopes, long and careful annealing should
be adopted, and the polishing process should be continued long after it appears
perfect to the optician. We believe, however, that the time is not distant when trans=
parent minerals, in which their elements are united in definite proportions, will be
substituted for glass. Diamond, topaz, and rock-crystal are those which appear
best suited for lenses. The white topaz of New Holland is particularly fitted for
optical purposes, as its double refraction may be removed by cutting it in plates
perpendicular to one of its optical axes. In rock-crystal the structure is, generally
speaking, less perfect along the axis of double refraction than in any other direc~
tion, but this imperfection does not exist in topaz.
On the decomposed Glass found at Nineveh and other places.
By Sir Davin Brewster, K.H., PRS.
The different kinds of glass which are in common use, consist of sand or silex
combined by fusion with earths or alkalies, or metals which either act as fluxes, or
communicate different colours or different degrees of lustre or refractive power to
the combination.
In quartz or rock-crystal, which is pure silex, and in other regularly crystallized
bodies, the molecules or atoms unite in virtue of regular laws, the pole of one atom
uniting with the pole of another. Such substances, therefore, do not decompose
under the ordinary action of the elements. The lens of Rock- Crystal, for example,
found by Mr. Layard at Nineveh, is as sound as it was many thousand years ago
when in the form of a crystal.
* In the case of glass, however, the silex has been melted and forced into union
10 REPORT—1860.
with other bodies to which it has no natural affinity; and therefore its atoms,
which have their similar poles lying in every possible direction, have a constant
tendency to recover their crystalline position as when in a state of silex. For the
same reason, the earths, alkalies and metals, with which the atoms of silex have
been constrained by fusion to enter into union, all tend to resume their crystalline
position and separate themselves from the silex.
Owing to the manner in which melted glass is cooled and annealed, whether it
is made by flashing or blowing, or moulding, the cohesion of its parts is not the
same throughout the mass; and consequently its particles are held together with
different degrees of force, varying in relation to points, lines, and surfaces. An
atom of the flux, or other ingredient, may be less firmly united to an atom of silex
in one place than in another, depending on the degree of heat by which they were
combined, or upon the relative positions of the poles of the atoms themselves when
combined. There are some remarkable cases where flint-glass without any rude
exposure to the elements has become opake, and I haye seen specimens in which
the disintegration had commenced a few years after it was made. In general, how-
ever, the process is very slow, excepting in stables, where the prevalence of am-
monia hastens the decomposition and produces all the beautiful colours of the
soap-bubble. It is, however, from among the ruins of ancient buildings that glass
is found in all the stages of decomposition ; and there is perhaps no material body
that ceases to exist with such grace and beauty, when it surrenders itself to time
and not to disease.
In damp localities, where acids and alkalies prevail in the soil, the glass rots as
it were by a process which, owing to the opacity of the rotten part, it is difficult to
study. it may be broken between the fingers of an infant; and we often find in the
middle of the fragment a plate of the original glass which has not yielded to the
process of decay.
~ In dry localities, where Roman, Greek, and Assyrian glass has been found, the
process of decomposition is exceedingly interesting, and its results singularly beau-
tiful, At one or more points in the surface of the glass the decomposition begins.
It extends round that point in spherical surfaces so that the first film is a minute
hemispherical cup of exceeding thinness. Film after film is formed in a similar
manner, till perhaps twenty or thirty are crowded into the 50th of an inch. They
now resemble the section of a pearl or of an onion, and as the films are still glass,
the colours of thin plates are seen when we look down through their edges which
form the surface of the glass. These thin edges, however, being exposed to the
elements, suffer decomposition. The particles of silex and the other ingredients
now readily separate, and the decomposition goes on downwards in films parallel
to the surface of the glass, the crystals of silex in one specimen forming a white
ring, and the other ingredients rings of a different colour. (See the Figure.)
Such is the process round one point, but the decomposition commences at many
points, and generally these points lie in lines, so that the circles of decomposition
meet one another and form sinuous lines. When there are only two points, these
eircles, when they meet, swround the two points of decomposition like the rings
round two knots of wood; and in like manner, when there are many points, and
these points near each other, the curves of decomposition unite as already mentioned,
and form sinuous lines. When the decomposition is uniform and the little hemi-
spheres have nearly the same depth, we can separate the upper film from the one
below it, the convexities of the one falling into the concavities of the other.
This general description was illustrated by drawings on the table, all of which
were executed by Miss Mary King, of Ballylin, now the Hon, Mrs. Ward.
But beautiful and correct as these drawings are, they convey a very imperfect
idea of the brilliant colours and singular forms which characterize glass in a parti-
cular stage of its decomposition, and of the optical phenomena which it exhibits in
common and polarized light,
When the decomposition has gone regularly on round a single point, and there
is no other change, a division of the glass into a number of hemispherical films
within one another takes place, the group of films exhibiting in the microscope cir-
cular cavities, which under different circumstances become elliptical and polygonal.
In salt water the decomposition of glass goes on more rapidly, as I haye found in
—s
TRANSACTIONS OF THE SECTIONS. 11
examining one of the bottles brought up in the wreck of the ‘ Royal George ;’ and the
same effect may be produced by a quicker process. M. Brame*, of Paris, having
seen a notice of the decomposed glass from Nineveh which I read at the Association
some years ago, succeeded in producing, in a very short time, regular and irregular
circles of decomposition, in the centre of which there was always a small cavity or
nucleus, This effect was obtained by immersing fragments of thick glass in a
mixture of fluoride of calcium and concentrated sulphuric acid, or by exposing
them to the action of the vapour of fluorhydrique acid.
Such are some of the general phenomena of decomposed glass when seen by light
reflected from its exposed surfaces ; but when we separate the films and examine
them in the microscope, either by common or polarized light, a series of phenomena
are seen of the most beautiful kind,—so various and so singular that it would be a
vain attempt to describe them. A general idea of them, however, may be obtained
from the drawings, and from a description of three varieties of these films.
I. The first of these varieties has rough surfaces,—the roughness arising from
an almost infinite number of hemispherical cavities on one side of the film, and
hemispherical convewities on the other side. When these cavities are separated by
flat portions of the film, they are perfectly circular; but when they are crowded
together, they are irregularly polygonal, the sides of the polygons forming a sort of
network, the cavities or convexities forming the meshes of the net.
The convex and concave surfaces are not rough but specular, and reflect and
transmit white light, exhibiting none of the colours of thin plates.
In polarized light, each of the cavities, whether circular or polygonal, act as
negative uniaxal crystals, exhibiting by the interference of the refracted and trans-
mitted pencils the black cross, and the white of the first order in Newton’s scale,
rising sometimes to yellow or falling to the palest blue, or disappearing altogether,
according to the number or curvature of the films which compose it.
Il. The second variety of these films has perfectly specular surfaces, in conse-
quence of having almost no cavities. They exhibit in common light, and in a very
beautiful manner, the colours of thin plates, the transmitted being complementary to
the reflected light. This variety is exceedingly rare. In a specimen on the table
the reflected light is blue and the transmitted yellow. In some of the fragments a
few insulated circular cavities with the black cross occur, the tints which surround
it being modified by the general tint of the film.
lil. The third variety of decomposed glass consists of films containing cavities of
all sizes and forms, from the 30th of an inch to such a size that they are hardly
visible by the microscope, giving to the film which they compose a sort of stippled
appearance, or an imperfectly specular surface.
These cavities or combinations of hemispherical films are circular, elliptical, or
irregularly polygonal. The colours which they reflect and transmitare complementary,
and the tints and rings which in polarized light surround the black cross are curiously
modified by the general tint of the fragment, and the curvature of its component
films,—the black cross itself varying its shape with the form of the cavities. “When
the cavities are flat, the black cross disappears as in thin slices of uniaxal crystals ;
but the tints reappear, rising to higher orders by inclining the plate.
The cavities are often arranged in sinuous curves, and encroach upon one another,
so that the polarized tints appear only at the margin of the line which they form.
They frequently run in perfectly straight lines, and when they are very small and
invisible as cavities, their margins form in polarized light brilliant lines, which are
often grouped in bands like the stripes in a ribbon. Sometimes they are only a few
thousands of an inch in diameter, and might be used as micrometers in the micro-
scope, every trace of the cavities which form them having disappeared. These lines
of polarized light all disappear when they lie in the plane of polarization of the
incident light, or perpendicular to that plane.
Tn some specimens a decomposition has taken place on several points of the con-
yex or concave surfaces of the cavities, so as to form new cavities ; and each of these
minute cavities, often ten or twelve in number, exhibit the black cross with its tints,
but disfiguring, of course, those of the cavity upon which they have encroached.
In the three varieties of decomposed glass which I have described, the films are
* Comptes Rendus, &c., Noy, 2, 1852.
12 REPORT—1860.
pure glass,—deriving their colour from the individual films of which they are com~-
posed. This is obvious from the fact of their becoming colourless by a sufficient
inclination of the plates, and also by the introduction of a drop of water or alcohol.
When the fluid has evaporated, the films recover their original colour; and though
a film of fluid has separated each of the almost infinitesimal layers of the glass, yet
they adhere as firmly as ever after the fluid has evaporated. If an oil or balsam is
introduced, it passes slowly and unequally between the layers, so that the retreating
colour is bounded by a spectrum of the various tints which the film combines.
But though the films themselves are glass, yet I have often found between them
beautiful circular crystals of sélex, which are finely seen in polarized light, and exhi-
bit many of the regular and irregular forms which I have represented in a paper on
Circular Crystals lately published in the ‘ Transactions of the Royal Society of Edin-
burgh.’ They are sometimes dendritic, and assume, round the ‘black cross, foliated
shapes like the leaves of plants. At other times, but very rarely, they occur in
circular groups,—related to a crystal of silex in their centre. One of these groups
is so remarkable as to merit particular notice. Around a minute speck of silex
there is formed, at a considerable distance from it, a circular band of equally minute
crystalline specks, and at a greater distance a second circular band concentric with
the first, and consisting of still smaller siliceous particles, hardly visible im the mi-
croscope. By what atomic force, or by what other cause, the central crystal has
laced its attendant crystals in regular circles around it, remains to be discovered. I
ave already described a similar phenomenon, as produced during the formation of
circular crystals under constraint, and when crystallizing freely ; but I am not aware
that any other person has either seen the phenomenon or attempted to explain it.
The films of decomposed glass, as I haye long ago shown, absorb definite rays of
the spectrum like coloured media. They change, in the most distinct manner, the
colours of different parts of the spectrum, and frequently insulate bands of purely
white light, in or near its most luminous division.
[The drawings referred to in this commnnication were laid before the Section, and
some of the specimens of decomposed gluss were exhibited in the Museum in the course
of the evening.]
On his own Perception of Colours. By J. H. Gravstone, Ph.D., PRS.
The author described himself as in an intermediate position between those who
have a normal vision of colours, and those who are termed ‘‘colour-blind.”” These
latter are usually unacquainted with the sensations of either red or green, and it
becomes a desideratum to have good observations on those who are capable of acting
somewhat as interpreters between them, and those who perceive every colour. By
means of Chevreul’s chromatic circles and scales, Maxwell’s colour-top, coloured
beads, &c., the author was able to determine the following points in respect to his
own vision. He sees red, in all probability, like other people, but it requires a larger
quantity of the colour to give the sensation than is usually the case; hence a purple
appears to him more blue, and an orange more yellow, than to the generality of
observers. He is perfectly sensible of green, or rather of two distinct greens, the
one yellowish, the other bluish ; but between them there lies a particular shade of
green, to which his eyes are insensible as acolour. This modifies his perception of
many greens that approximate to what is to him invisible. ‘The shade occurs in
nature on the back of the leaf of the variegated holly, and it may be produced in Max-
well’s top by certain combinations of the coloured disc; the simplest being
94°5 Brunswick Green (Blue Shade) + 5°5 Ultramarine =94 Black-+ 6 White.
He finds that this shade, though invisible to him as green, is yet capable of neu-
tralizing red when viewed simultaneously, but it does not neutralize so much red
with him as with observers of o1dinary vision.
While able perfectly to distinguish between red and green, the contrast does not
readily catch his eye, especially at a distance; in fact, he is somewhat short-sighted
in respect to these colours. He has reason to believe that, in his case, there has
been a gradual improvement in his actual perception of colours, independently of his
greater knowledge of them, though this is in opposition to the general experience of
eS ee a
TRANSACTIONS OF THE SECTIONS. 13
those whose vision is in any way abnormal, and no other stance was known to the
late Prof. George Wilson, whose book is the standard one on the subject of colour-
blindness.
On the Chromatic Properties of the Electric Light of Mercury.
By J. H. Guapsrone, PA.D., F.RS.
While examining the brilliant electric light produced in an interrupted current of
mercury in the apparatus contrived by Professor Way, the author was struck by the
strange manner in which it modified the apparent colours of surrounding objects,
and especially with the ghastly purple and green hues which it imparted to the faces
and hands of the spectators. This led him to an investigation of the subject, and a
prismatic analysis of the light itself. Chevreul’s ‘cercles chromatiques ” showed
yellow, green, and blue distinctly, but very little red, while the violet became remark-
ably luminous. The modifications of colour in many bodies of known composition
were then related, as for instance the green sulphate of iron which appeared colour-
less, and the scarlet iodide of mercury which assumed a brownish metallic appear-
ance. Substances capable of fluorescing exhibited that phenomenon with remark-
able beauty. On analysing this light by means of a refractive goniometer, the author
found it to consist of a great number of separate rays, and not to present in any
part a continuous band of light. This was exhibited by means of a diagram in
coloured chalks on black paper, by the side of a solar prismatic spectrum. The
position of the different rays had been measured, and their relative intensity deter-
mined. There are red and orange rays, but they are of the most feeble intensity ;
some yellow rays of great brilliancy; two bright green rays; one blue ray of great
luminosity ; and a number of violet rays. One of these latter is situated far beyond
the limits of the visible solar spectrum, in fact at about Becquerel’s line N, and was
bright to the eye, although it had passed through several pieces of glass—a medium
that does not easily transmit the extra-violet rays. Its colour appeared to differ
considerably according to its intensity, but might be described generally as a red-
violet. The prismatic analysis explained fully the changes that red substances un-
dergo when exposed to it—sometimes to brown, and at other times to purple, green,
or whatever other colour in addition to red is principally reflected by them: it also
explained all the other chromatic phenomena. Professor Wheatstone in 1835 de-
scribed the spectrum of the electric light of mercury as containing seven definite rays ;
and Angstrom has recently given a drawing of the lines that coincides closely with
the observations of the author on the more luminous rays, and shows that the Swedish
physicist had not seen the extra violet lines. From his figures also it appears that
the air is excluded from the luminous cone of mercurial vapour in Way’s apparatus.
On a New Instrument for determining the Plane of Polarization.
By the Rev. Professor JELLErT.
Professor Jellett described to the Section a new analysing prism, by which the
plane of polarization of polarized light may be determined with great precision.
This instrument consists of a long prism of cale-spar, which is reduced to the form
of a right prism by grinding off its ends, and sliced lengthwise by a plane nearly
but not quite perpendicular to its principal plane. he parts into which the prism
is thus divided are joined in reversed positions, and a diaphragm with a circular
opening is placed at each end. The light which passes through both diaphragms
produces a circular field divided by a diametral slit into two parts, in which the
planes of polarization are slightly inclined to one another. If then light which has
been previously plane polarized be transmitted, it will be extinguished in the two parts
of the field of view in positions which lie close together, and the light will become
uniform in a position midway between these. This position determines the plane in
which the incident light was polarized, with a precision much greater than has been
otherwise attained. Professor Jellett stated that the different observations did not
differ from one another by an angle greater than a minute, and that the instrument
was equally applicable to the case of homogeneous light,
14 i REPORT—1860.
Note on the Caustics produced by Reflexion.
By L. L. Linvexor, Professor at Helsingfors.
There are, no doubt, few branches of mathematical physics that have been more
often discussed than the reflexion and refraction of light, and the theory of these
phenomena has consequently been gradually reduced to the greatest simplicity. The
whole doctrine of catoptrics and dioptrics may indeed be said to be implicitly con-
tained in the elegant principle successively developed by Dupin, Quetelet, and Gor-
gonne, namely, that a system of rays that can be cut orthogonally by a particular sur-
face, preserves this property after any number of reflexions and refractions. Never-
theless, it appears to me that the theory of caustics has been somewhat neglected.
Not but what there are many interesting researches on this subject that have been
conducted with abundance of care, but because these, for the most part, refer to cer-
tain very restricted cases, as for example, to reflecting surfaces of a particular kind.
In examining from a somewhat more general point of view the theory of caustics
produced by reflexion, I have arrived at certain results, which appear to me to be
sufficiently curious to deserve a short notice.
I suppose the reflecting surface to be of any kind whatever, and that it is illumi-
nated by a bundle of parallel rays. Suppose, now, that two of these rays impinge on
the surface at two points A and A! infinitely near each other. Unless certain par-
ticular conditions are fulfilled, the corresponding reflected rays will not be in the same
plane. In order, therefore, that the two rays may meet after reflexion so as to form
a point in a caustic, the points A and A! must be related in a certain manner. Now
it will be found that, starting from any point A, there will always be two different
directions in which the consecutive reflected rays intersect, and by following these
directions from point to point, certain curves will be traced on the surface, which play
an important part in the theory of caustics, and which may be called catoptrical lines.
These lines bear some analogy to the lines of greatest and least curvature, with which
they sometimes coincide. Their form and situation depend not only on the nature of
the surface, but also on the direction of the incident rays. Each point of the surface is
the intersection of two catoptrical lines, which possess the remarkable property that
their projections on the plane perpendicular to the incident rays, cut each other at
right angles. ‘To each catoptrical line there is a correspouding caustic formed by the
rays reflected from the catoptric, and these caustic lines themselves form a caustic
surface, which in general consists of two sheets, corresponding to the two systems
of catoptrical lines.
Let a, y, and z be the coordinates of any point in the reflecting surface, and let the
axis of z be parallel to the incident rays. Calling, as usual, the partial differential
coefficients of s with respect to a and y of the first order p and gq, those of the second
r, s, and #, we have for the catoptrical lines the simple equation
dp . dy=dq .dr,
dy CY Retain
Wy Saati ia,
which may be put in the form
since dp=rdx+sdy, dg=sda-+ tdy.
The quantities p, g, 7, s, and ¢ being all expressible in terms of x and y by means of
the equation to the reflecting surface, the two values of =~ derived from the above
a
equation can also be expressed in terms of w andy. If this differential equation can
be integrated, the resulting relation between 2 and y, together with the equation to
the surface, determine the catoptrical lines.
The point &, n, and ¢ of the caustic corresponding to x, y, z of the reflecting sur-
face, is determined by the following equations :—
dy
t—s—
sor ae tea ¢ 2s dz
2p 2g pte] 2@=rt)’
Eliminating x, y, z by means of these three equations and that of the given surfaces,
we obviously get the equation to the caustic surface ; and eliminating the same quan-
TRANSACTIONS OF THE SECTIONS. ‘15
‘tities between the same three equations, and the two equations of any catoptrical line,
we get the equations to the corresponding caustic line.
As to the application of this theory it offers no difficulty. On directing my
aig fon more particularly to surfaces of the second order, I obtained the following
results :—
(1) In the case of a sphere illuminated by parallel rays, the first system of catop-
trical lines consists of great circles passing through the same point, the second of small
citcles cutting the former at right angles. The equation to the caustic surface that
corresponds to the first system is
[4 +7?+0)—a* P= 2708 (E+7°),
a being the radius of the sphere, while the second system has for its caustic a straight
line passing through the centre of the sphere.
(2) If the reflecting surface be an ellipsoid or a hyperboloid, either of one or of
two sheets, and the incident rays are parallel to one of the axes, the projections of the
catoptrical lines on the plane of the other axes are either ellipses or hyperbolas, whose
foci coincide with those of the section of the surface by the same plane.
(3) In the case of an elliptic paraboloid illuminated by rays parallel to its axis,
the catoptrical lines form parabolas whose planes are parallel to one or the other of
the principal sections of the surface. The caustic surface is reduced to two parabolas
lying in the planes of the principal sections, and having the axis of the paraboloid for
their common axis, but situated in opposite directions. ‘That which lies in the plane
of the greatest of the principal sections is turned in the same way as the paraboloid,
that lying in the perpendicular plane is turned in the opposite direction. Each of
these parabolas has the same focus as the principal section to which it is perpendicu-
lar, and a parameter equal to the difference of the parameters of the principal sections.
Lastly, each of these caustic lines is perpendicular to the corresponding system of
catoptrical lines.
(4) In the case of a hyperbolic paraboloid illuminated by rays parallel to its axis,
the catoptrical lines also form two systems of parabolas in planes parallel to the planes
of the principal sections, and the caustic is again reduced to two parabolas situated in
the same two planes, and turned in opposite directions, each having a parameter
equal to the sum of the parameters of the two principal sections.
There would be no difficulty in applying the above formule to surfaces of revolu-
tion, to cylindrical conical developable surfaces, &c., but the preceding will suffice to
give an idea of the results that may be deduced in certain cases.
On the Results of Bernoulli's Theory of Gases as applied to their Internal
Friction, their Diffusion, and their Conductivity for Heat. By Professor
Maxwe tt, F.R.S.E.
_ The substance of this paper is to be found in the ‘ Philosophical Magazine’ for
January and July 1860. Assuming that the elasticity of gases can be accounted
for by the impact of their particles against the sides of the containing vessel, the
laws of motion of an immense number of very small elastic particles impinging on
each other, are deduced from mathematical principles; and it is shown,—1st, that
_the velocities of the particles vary from 0 to o, but that the number at any instant
having velocities between given limits follows a law similar in its expression to
that of the distribution of errors according to the theory of the ‘‘ Method of least
“squares.’’ 2nd. That the relative velocities of particles of two different systems are
‘distributed according to a similar law, and that the mean relative velocity is the
‘Square root of the sum of the squares of the two mean velocities. 3rd. That
‘the pressure is one-third of the density multiplied by the mean square of the
‘Velocity. 4th. That the mean vis viva of a particle is the same in each of two
Ryaterns in contact, and that temperature may be represented by the vis viva of a
‘Particle, so that at equal temperatures and pressures, equal volumes of different
gases must contain equal numbers of particles. 5th. That when layers of gas have
a motion of sliding over each other, particles will be projected from one layer into
another, and thus tend to resist the sliding motion. The amcunt of this will depend
on the average distance described by a particle between successive collisions. From
the coefficient of friction in air, as given by Professor Stokes, it would appear that
16 REPORT—1860.
this distance is a inch; the mean velocity being 1505 feet per second, so that
each particle makes 8,077,200,000 collisions per second. 6th. That diffusion of gases
is due partly to the agitation of the particles tending to mix them, and partly to the
existence of opposing currents of the two gases through each other. From experi-
ments of Graham on the diffusion of olefiant gas into air, the value of the distance
described by a particle between successive collisions is found to be =m of an
inch, agreeing with the value derived from friction as closely as rough experiments
of this kind will permit. 7th. That conduction of heat consists in the propagation of
the motion of agitation from one part of the system to another, and may be calcu-
lated when we know the nature of the motion. Taking sonaaa of an inch as a pro-
bable value of the distance that a particle moves between successive collisions, it ap-
pears that the quantity of heat transmitted through a stratum of air by conduction
would be aa of that transmnitted by a stratum of copper of equal thick-
ness, the difference of the temperatures of the two sides being the same in both
cases. This shows that the observed low conductivity of air is no objection to the
theory, but a result of it. 8th. That if the collisions produce rotation of the parti-
cles at all, the vis viva of rotation will be equal to that of translation. This relation
would make the ratio of specific heat at constant pressure to that at constant volume
to be 1°33, whereas we know that for air it is 1°408. This result of the dynamical
theory, being at variance with experiment, overturns the whole hypothesis, however
satisfactory the other results may be.
On an Instrument for Exhibiting any Mixture of the Colours of the
Spectrum. By Professor Maxwe tt, F.R.S.L.
This instrument consists of a box about 40 inches long by 11 broad and 4 deep.
Light is admitted at one end through a system of three slits, of which the position
and breadth can be altered and accurately measured. This light, near the other end
of the box, falls on two prisms in succession, and then on a concave mirror, which
reflects it back through the prisms, so as to increase the dispersion of colours. The
light then falis on a plane mirror inclined 45° to the axis of the instrument, and is
reflected on a screen in which is a narrow slit. On this screen are formed three pure
spectra, the position and intensity of each depending on the position and breadth of
the slit through which the light was admitted. The portions of these spectra which
fall on the slit in the screen pass through, and are viewed by the eve placed close
behind it. A colour compounded of these three portions of three different spectra
is seen illuminating the prisms, and can be compared with white reflected light seen
past the edge of the prisms, ‘The advantage of the instrument over that described
to the Association in 1859 is, that by the principle of reflexion the rays return in the
same tube, so as not to require two limbs forming an awkward angle; while at the
same time, by doubling the dispersion, the necessary length of the instrument is
diminished. By means of this instrument many observations of colours have been
taken. Some of these by a colour-blind person are published in the ‘ Philosophical
‘lransactions ’ for 1860.
Further Researches regarding the Laws of Chromatic Dispersion.
By Munco Ponron.
In this paper the author has revised, and improved in its details, his method of
expressing the refractive index of a medium as a function of the wave-length.
He employs A to denote the ratio of any particular wave-length referred to that
of the fixed line B as unity. The numerical values of the wave-lengths of the lines
C, D, E, F, G, H are given, as calculated from Fraunhofer’s measures.
The author’s formula for expressing the refractive index (1) as a function of d is
x”
a
TRANSACTIONS OF THE SECTIONS. 17
-where » must be found by the method of trial and error for each medium in parti-
cular, and e*, a» are certain known functions of and of the observed indices.
Thus the formula contains three arbitrary constants, which must be determined
from the results of observation.
When these constants are properly determined for any medium, the formula, even
in the case of the most highly dispersive media which have been observed, is found
to represent very accurately the observations, the utmost error being only a few units
in the fourth place of decimals.
Experiments and Conclusions on Binocular Vision.
By Professor Witt1aM B. Rocers, Boston, U.S.
The following experiments, intended to test the theory of the successive com-
bination of corresponding points in stereoscopic vision, are I believe in part new,
and are in part modified repetitions of experiments already described by Professor
Wheatstone and Professor Dove.
1. Let two slightly inclined luminous lines, formed by narrow slits in a strip of
black card-board, be combined into a perspective line, either with or without a
stereoscope. Looking at this for a few seconds, so as to induce the reverse ocular
spectrum, and then directing the eyes towards the opposite wall of the apartment,
a single spectrum will be observed having the attitude and relief of the original
binocular resultant.
As a strong illumination of the lines is necessary to bring out the full effect, the
card-board should be held between the eyes and some brilliantly white surface, as
the globe of a solar lamp or a strongly illuminated cloud, care being taken to pre-
vent the entrance of extraneous light.
2. Using the same arrangement, let the luminous lines be regarded ¢n succession
each by the corresponding eye, the ether eye being shaded so that no direct bino-
cular combination can be formed. On looking towards the wall, it will be seen that
the two subjective images unite to form a single spectral line, having the same relief as
of the lines had been directly combined by simultaneous vision, either with or without
a stereoscope.
While the perspective image continues distinctly visible, let either eye be closed,
the other being still directed towards the wall.’ The image will instantly lose
its relief and take its position on the plane of the wall as an inclined line, corre-
sponding to the subjective image in the eye that has remained open. When
the subjective impressions have been sufficiently strong, it is easy to alternate
these etlects, by projecting first the picture proper to the right eye, then that of
the left, on the plane of the wall, with their respective contrary inclinations; and
_ then looking with both eyes, we see the resultant image start forth in its perspec-
tive attitude.
d It is hardly necessary to say that to obtain these effects satisfactorily the lines
_ should be very strongly illuminated, and the observer should have some practice in
experiments on subjective vision. Under these conditions I have found the results
to be perfectly certain and uniform.
In these experiments, according to the theory of Sir David Brewster, the result-
ant spectrum, instead of being a single line in a perspective position, ought to pre-
sent the form of two lines inclined or crossing, situated in the plane of the wall
without projection or relief. The conditions of the experiments are such as te
exclude all opportunity of a shifting of the image on the retina, and such shifting is
obviously essential to the successive combination of pairs of points required by the
theory in the production of perspective effect.
In reference to the first experiment, it might perhaps be maintained that, as the
perspectiveness of the original resultant on which the eyes were converged formed
part of the direct perception in first combining the lines, it would be likely through
association to be included also in the spectral or subjective perception. But this
consideration, which at best appears to me of little weight, is entirely inapplicable
to the conditions of the second experiment. For here the eyes are in the first
place impressed in succession with their respective images, and are not allowed to
see the resultant ; and yet when they are together directed to the wall, the percep-
tion of the single perspective resultant is at once originated.
1860. 2
Y
'
‘
18 REFORT—1860.
3. Without resorting to these troublesome efforts of subjective vision, the fol-
lowing experiment furnishes, as I think, conclusive proof that pictures successively
eae on the respective eyes are sufficient for the stereoscopic effect.
et an opake screen be made to vibrate or revolve somewhat rapidly between
the eyes and the twin pictures ofa stereoscopic drawing, so as alternately to expose
and cover each, while it completely excludes the simultaneous vision of any parts
of the two. The stereoscopic relief will be as apparent in these conditions as when the
moving screen is withdrawn. Here at each moment the actual impression in the
one eye and the retained impression in the other, form the elements of the per-
spective resultant perceived.
{t seems clearly inferrible from these experiments, that the perception of the
resultant in its proper relief does not require that each pair of corresponding points
should be combined by directing the optic axes to them pair by pair in succession,
as has been maintained. Nor is it necessary for the singleness of the resultant
perception, that the images of corresponding points of the object should fall on
what are called corresponding points of the retin. The condition of single vision
in such cases seems to be simply this, that the pictures in the two eyes shall be such
and so placed as to be identical with the pictures which the real object would form if
placed at a given distance and in a given attitude before the eyes.
4, I have of late years frequently repeated Dove’s experiments with instantaneous
illumination, leading, as is well known, to similar conclusions. In these I have found
it most convenient to use the momentary bright flash of the Leyden bottle, con-
nected with the Ruhmkorff coil according to Grove’s plan. With a powerful
coil of Ritchie’s construction, and a brass disc 8 inches in diameter having the usual
concentric striation, I am able, even with a single flash, to see the luminous line in
perspective, and by a quick succession of flashes, I can have it as steadily before
me as if illuminated by the sun.
A twin-drawing of a simple geometrical solid, placed in the stereoscope, and
illuminated by the same means, appears single and in just relief in all cases where
the flashes recur at short intervals, and very frequently presents the same appear-
ance even with a single momentary light.
To be assured that the effect was not due to the recollection of a previous stereo-
scopic impression, I have caused slides to be introduced, of which the form could
not be thus anticipated, and still have had no difficulty in describing the perspec-
tive resultant as exhibited by the instantaneous illumination.
5. On the inability of the eyes to determine which retina is impressed.—Let a
small disc of white paper be fastened on a slip of black pasteboard of the size
of a stereoscopic slide, and let this be so placed in the instrument as to bring the
disc centrally in front of one of the glasses, the person who is to view it being kept
in ignorance of the position of the spot. On looking into the instrument he will
think he sees it with both eyes equally, and, without resorting to the expedient of
closing his eyes alternately, will be entirely unable to determine whether the spot is
before his right eye or his left eye. The spot appears to be placed in the mesial or
binocular direction, and in the same position as that of the resultant image of two
such discs, presented severally to the two eyes.
It may be concluded from this that the mere retinal impression on either eye is
unaccompanied by any conscious reference to the special surface impressed, and that
the visual perception belongs to that part of the optical apparatus near or within
the brain, which belongs in common to both eyes.
This experiment is moreover interesting from its bearing on the law of visible
direction. It shows that the sense of direction is just as truly normal to the central
part of the retina that has received no light from the object, as to the part of the
other retina upon which the white spot has been actually painted by the rays. In
truth it is normal to neither, but is felt to be in the middle line between the two,
that is, in the binocular direction. This experiment therefore contradicts the law,
which assumes that the direction in which an object appears is always in the normal
to the point of the retina impressed.
TRANSACTIONS OF THE SECTIONS, 19
Régulateur Automatique de Lumiére Electrique. By M. Serr.
To form the electric arch of light, it is first necessary to bring the charcoal points
into contact, then gently to separate them by degrees, as they glow, afterwards to
cause them to approach constantly, as they are wasted by use, carefully avoiding
bringing them into contact. In order to keep the point of illumination fixed in space,
each charcoal point must simultaneously approach the other, and that in the pro-
portion in which each is wasted by use. In fine, for rendering the electric light
useful, all these conditions must be self-produced with the utmost regularity, with-
out any intervention of the human hand, that is to say, in a manner completely
automatic; and this was the object the regulator was invented for. In a simple
and easy manner, this apparatus, which may be compared to an extremely sensible
balance, is composed of two mechanisms connected the one with the other, and yet
independent ; when one acts the other is in repose, and reciprocally. One of these
consists of an oscillating system,—the chief feature of the regulator destined to pro-
duce the separation of the charcoal points, and also to determine their re-approach.
The other mechanism, composed of wheel-work, has for its object to ensure the re-
approach of the charcoal points in the proportion of their waste by use. The two
port-carbons which carry the charcoal pieces are placed vertically one above the
other. The superior is in connexion with the wheel-work, and is the positive elec-
trode of the battery; the inferior depends as well on the wheel-work as on the
oscillating system, and is the negative electrode. The superior port-carbon, by its
weight, causes the inferior to ascend. The oscillating system forms a parallelogram,
of which the angles are jointed, one of the vertical sides of which is suspended bya
spring, and carries at its lower part a soft iron armature, placed over a horizontal
electro-magnet. When the apparatus is in repose, the charcoals are in contact ; on
the contrary, they separate when the circuit is completed and the voltaic arc ap-
pears. As the wasting by use of the charcoals increases the length of the voltaic arc,
the armature increases its distance from the electro-magnet, become less powerful,
and the charcoals re-approach by a quantity frequently less than the one-hundredth
of a millimetre; but according as they re-approach, the electro-magnet recovers its
original power, the armature is attracted anew, and the charcoals stop until a new
wasting gives rise to a new re-approach followed by a new stoppage, and so on in
succession. In consequence of its extreme sensibility, it will work either with a
voltaic pile or an electro-magnetic machine.
On some Recent Extensions of Prevost’s Theory of Exchanges.
By Barrour Stewart, M.A.
On Rings seen in viewing a Light through Fibrous Specimens of Cale-
spar. By G. Jounstone Stoney, M.A, F.R.A.S. Sc.
The author mentioned that Sir David Brewster had drawn the attention of the
Association, at the York meeting, to the beautiful display of four rings which may
be seen on looking at a luminous point through fibrous specimens of calc-spar.
In the present communication the forms of the rings were traced asa consequence
of Huygen’s construction, and the points where rings vanish, or where irises pass
into one another, were determined. The state of polarization was also examined, and
the positions, in which two of the rings, which are faint, will be most conspicuous.
The author drew particular attention to the great range of brightness of these faint
rings, and to the circumstances attending the disappearance of one of them, in con-
Sequence of a curious case of impossible reflexion, as offering peculiar facilities for
testing rival hypotheses.
On Thin Films of Decomposed Glass found near Oxford.
By R. Tuomas.
The films were observed on bottles of the form called magnums, which had been
lying in the Cherwell above a century. The films formed by decomposition on the
QF
20 REPORT—1860.
surface were easily detached, and submitted to observation. The reflected and trans-
mitted tints were complementary to each other when held perpendicularly; they
varied when the position was changed and the path of the rays became oblique. By
examination under the microscope the films were found to be composed of a series of
still thinner films, several of which were required for manifesting colours by trans-
mitted light. In some cases as many as sixteen of these thinner laminz were counted.
The colour is brightened in proportion to the number of lamine. When two films
overlap, the tint produced is the mixture of the two—yellow and blue, for instance,
producing green. In general the layers are flat and the colour uniform, but some-
times undulated over bubbles, and then the colour is varied. Some specimens with
a few bubbles show a difference of colour at the bubble with common light, and with
polarized light the black cross and complementary colours appear.
Ecvectricity, MAaGnertismM.
On certain Results of Observations in the Observatory of His Highness the
Rajah of Travancore. By Joun ALLAN Broun, F.RS.
The following were noticed by the author. lst. With regard to the mode in
which the diurnal law of magnetic declination varies from place to place, and the
probable position and epoch of the line of least diurnal variation near the equinoxes.
For this object two stations were chosen—one near the magnetic equator, 90 miles
north of Trevandrum, the other about 40 miles south at Cape Comorin, where con-
tinuous hourly observations were made during several months about the periods of
the equinoxes. The most marked of the conclusions arrived at from these observa-
tions were, that the minimum diurnal variation near the March equinox occurred
earlier in the year at Trevandrum than at Shertally 90 miles north, and on the mag-
netic equator ; that the law presented marked differences at the two places, near the
epoch of minimum variation; and that the difference of the variations at the two
stations occurred almost whoily between midnight, sunrise, and noon, the difference
between noon, sunset, and midnight being comparatively small.
2nd. Projected observations were exhibited in proof of the results communicated
by the author to the Leeds Meeting of the Association, that the daily mean inten-
sity of the earth’s magnetism increases as a whole or diminishes as a whole; so that
if at any point on the earth’s surface the daily mean intensity increases, it will be
found that it increases similarly at all other places in proportion to the absolute in-
tensity at each place, allowance being made in cases of great disturbance to the
greater value of disturbances in high latitudes.
3rd. Projected observations were also exhibited, showing that the mean daily
easterly declination of the north end of a magnet followed on the whole the same
law of variation in both hemispheres, differing from the diurnal variation, where the
north end moves east in the southern hemisphere, while it moves west in the north-
ern hemisphere.
4th. The author had investigated the laws of the diurnal variation of the baro-
meter within the tropics. He had endeavoured to determine whether the chain of the
Indian Ghats had any influence on the great atmospheric semidiurnal wave moving
westward. Hourly observations had been made for a month in 1857, at a station
on the eastern base of the Ghats, on the highest peak in Travancore, on the western
base (all within a few miles), and at Trevandrum 20 miles distant, near the sea shore.
Similar observations had been made in 1858, at four stations on the western face of
the Agastier Malley, differing by 1500 to 1700 feet from each other in height, in
correspondence with the Trevandrum Observatory. In these observations the greatest
care was taken to have the best instruments, the times of observations were pre-
cisely simultaneous, and instruments of all kinds were observed likely to give results
related to the question examined : fifteen observers were employed, and the observa-
tions continued hourly during a month. From these observations, it appears that
—_——
TRANSACTIONS OF THE SECTIONS. 21
the semidiurnal law of atmospheric pressure is the same at all heights up to 6200
feet (on a sharp peak), from 9 p.m. to 9 a.m., both as regards epoch and range. The
day variation (9 a.m. to 9 p.m.) is greatest for the lowest station, depending evidently
on the temperature. The author connected these facts with the hypothesis proposed
by Dr. Lamont and himself, that the semidiurnal variation is due to the inducing
electrical action of the sun on our earth and its atmosphere.
These and several other results, at present only partly worked out, would be pub-
lished soon in detail. The printing of the observations made in the observatory of
His Highness the Rajah of Travancore was proceeding as rapidly at Trevandrum as
could be expected in Jndia, and the first sheets were in the author’s hands.
On the Diurnal Variations of the Magnetic Declination at the Magnetic
Equator, and the Decennial Period. By Joun ALLAN Broun, F.R.S.
Solar-diurnal Variation.—The author stated that the observations made at the
intertropical observatories had shown the fact that the law of solar-diurnal variation
was opposite, or nearly opposite, at two seasons of the year; this result was made
generally known to the scientific world by General Sabine, in his discussion of the
St. Helena Observations. St. Helena, however, is too far from the magnetic equator
to show the change from one law to the other, otherwise than as a shifting move-
ment of the maxima and minima, which seem to slide in the course of a month or
two from one position to the other; the whole range of the variation being consider-
able at all seasons. Mr. Broun offered to the Section the results of five years’
observations made at the Trevandrum Observatory, about 90 miles south of the
magnetic equator, which showed perfectly the mode of variation of the diurnal law.
In the months of December, January, and February, the minimum of easterly de-
clination occurs at 7; A.m., in the months from April to September, the mazimum
occurs at exactly the same time. In the months of March and October a period of
indifference is attained, when the variation becomes nearly zero, or the variation is
a series of maxima and minima at different hours, and the range or total angular
movement is reduced to about thirty seconds (0'5) when the mean of a few days
is taken. The epochs at which this change takes place are neither those of the sun’s
crossing the equator nor the zenith, and the epoch seems to vary from year to year.
The March epoch is not distant from the vernal equinox, but the other occurs nearly
a month later than the autumnal equinox. So far is the second epoch for the change
from one law to the other from tliat of the sun’s crossing the zenith or equator, that
August and September are the months of greatest diurnal range.
Although Trevandrum is in 83° north latitude, it has a magnetic dip of 23° south;
but the diurnal variations affect the character of the northern hemisphere more than
that of the southern hemisphere,—the mean range for the months from May to
September being nearly three minutes (3’), while for the months of December and
January the range is only about two minutes (2’).
Mr. Broun was the first to point out that the diurnal law at any place might be
represented by the superposition of two variations, one resembling that peculiar to
high north latitudes, the other resembling that peculiar to high south,—the northern
part being always in excess in high magnetic north latitudes, and in excess for places
in low magnetic north latitudes only for the sun north of a given line. It is evident
that we may, by descending towards the magnetic equator, reach a station where for
a given position of the sun the two variations will be equal or nearly equal, in which
case for that position of the sun the complete extinction of the diurnal law may be
expected ; this occurs approximately at Trevandrum.
- When the diurnal range is examined with reference to the decennial period, it is
found that the mean range had a minimum in the year 1856, the exact epoch of
minimum being, perhaps, about January of that year; but when the ranges for
given months are considered, some curious differences from the law are discovered.
The yearly mean of monthly mean ranges, with the mean ranges for the months of
March and October, are as follows :—
22 REPORT—1860.
Yearly Mean. March. October.
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It will be perceived from this Table that the range for the month of March has
gone on increasing from 1854 till 1858, the range for the latter year being more than
double that for the former ; that while the minimum for the whole year occurred in
1856, that for March occurred in 1854, or before that year. In the case of the
month of October, the ranges differ little, that for 1854 being the greatest, and that
for 1857 the least. It is conceived by the author that this curious variation in
March and October is connected with a shift in the epoch of minimum diurnal
variation. If this epoch happen near the middle of the month, the range for the
mean of the month will be least; if it happen earlier or later, the greater range of the
preceding or succeeding periods will preponderate in the monthly mean. Should this
be the cause of the variation of range for March and October, it would follow that
the two superposed variations which produce the total variation may change their
relative values from year to year for a given place and for a given position of the sun.
Lunar-diurnal Variation.—This variation, which was first remarked by M. Kreil,
and afterwards, though quite independently, by the author, has since been discussed
by General Sabine. The latter gentleman has made it a subject of inquiry, first,
whether the lunar-diurnal variation within the tropics obeyed different laws for the
moon north and south of the equator, like the solar-diurnal law; and 2nd, whether
the decennial period could be perceived in the former as it is in the latter. His con-
clusions in both cases have been in the negative. Mr. Broun has discussed five
years’ observations at Trevandrum, from which he arrives at the following results.
lst. That the lunar-diurnal law varies with the moon’s declination, but not to
the extent of inverting the law. In all cases there are two maxima of easterly de-
clination near the superior and inferior transits, and two minima for the moon near
the horizon. If we consider the period about the solstice of December, we shall find
that the greatest maximum occurs at the inferior transit for the moon furthest north,
and at the superior transit for the moon furthest south. ‘The greatest minimum is
near moonrise for the moon on the equator going north, and near moonset for the
moon on the equator going south, while the minima are equal for the moon furthest
north and furthest south. The epochs also vary slightly.
2nd. The lunar-diurnal law, which remains nearly constant as regards epochs for
all positions of the moon at any given season of the year, is the inverse in June of
what it is in December ; so that, for the sun furthest north, the lunar-diurnal Jaw has
its maximum where for the sun furthest south it has its minima, the latter occurring
near the epochs of transit in June and July. In this way the Junar-diurnal law de-
ee on the position of the sun relatively to the ecliptic, and not (or little) on that of
the moon.
The range of the lunar-diurnal variation is greatest near perihelion, which is just
the reverse of the solar-diurnal law ; this appears to depend on the moon’s greater
proximity to the sun as the cause of its magnetic action. The range is least near
the epochs of the equinoxes, as for the solar-diurnal law.
The cause of the great differences found by General Sabine in the laws for dif-
ferent places in the same hemisphere, is attributed by the author partly to the com-
bination of laws which vary considerably at the same place for different seasons.
The author also pointed out that General Sabine’s failure to discover the decennial
period in the lunar-diurnal variation may be due to the fact that, before he com-
menced his discussion, he had first cut out all the disturbances beyond a certain
limit, so that a greater proportion were rejected in the years of greatest disturbance.
The decennial law is one affecting the regular diurnal variations, chiefly, through the
disturbance; so that if the latter be omitted the effect should not appear (or appear
but slightly) in the former. The projected observations were exhibited to the Section.
TRANSACTIONS OF THE SECTIONS. 23
On a New Induction Dip-Circle. By Joun ALLAN Broun, F.R.S.
The idea of determining the earth’s magnetic intensity by its inducing action on
soft iron was employed by Dr. Lloyd for the purpose of obtaining the magnetic in-
clination. A soft iron bar being placed vertically, so that the induced magnetism of
one end should act on a freely suspended magnet, the deflection thus produced was
observed, and considered proportional to the vertical component of the earth’s mag-
netic intensity ; the bar was then placed horizontal, and, the same end acting, the
deflection was observed, which was in the same way considered proportional to the
horizontal component : were there no sources of error, the inclination might be
determined from these two angles. The iron bars employed always possess or
acquire a certain amount of induced magnetism, the effect of which is eliminated by
inverting the bar for the different deflections ; there are, however, still two sources
of error which remain. The most important is that due to the different actions of the
different parts of the bar in the vertical and horizontal positions. If the whole mag-
netism were accumulated in one point at the acting end of the bar, this source of
error would not have existed; but as the magnetism is distributed over the whole
length, that part whose action is equal on both ends of the suspended magnet when
the bar is in the vertical position, becomes greater on one end of the magnet than
the other when the bar is in the horizontal position. It was probably for this rea-
son that Dr. Lloyd’s method has never been put into practice.
Last year, while observing with Dr. Lamont’s theodolite magnetometer, Mr. Broun
employed a method for the determination of the absolute magnetic inclination, to
which it is believed there can be no objection in low magnetic latitudes, and which,
with the modifications proposed, may probably be used in all latitudes.
In Dr. Lamont’s apparatus the variations of magnetic dip from place to place are
determined by means of two soft iron bars clamped to a horizontal ring, the ring
surrounding a freely suspended magnet, one bar vertically above the ring, the other
vertically below it. By a series of observations of the deflections produced by the
bars in different positions, inverted and exchanged from side to side, the effect of per-
manent magnetism is eliminated, and the deflection due to the earth’s force is
obtained ; the sine of this angle, multiplied by a constant, gives the dip for each place;
the constant, however, requires the aid of the usual dip apparatus for its determina-
tion, It is evident, however, that if we can incline the bars moving in the plane of
the magnetic meridian till the observed deflection be zero (should there be no per-
manent magnetism), and observe the angle through which the bars have been moved
from the vertical, this angle will evidently be that of the magnetic inclination, for
the bar will have been moved into the direction at right angles to that of the total
force. This method, as thus stated, requires the determination of the vertical posi-
tion of the bars ; and itis supposed that there is no permanent magnetism : as far as
the latter supposition is concerned, the error is eliminated by reversing the bars; in
order to render the determination of the vertical position unnecessary, it is only re-
quired to observe the angular inclination of the bars, which (for each position)
diminishes the deflection by an amount equal to the mean deflection previously ob-
tained. It will be observed that for low latitudes, where the bars are moved little
from the vertical, the objection applying to Dr. Lloyd’s method exists to so small a
degree as to be negligible.
This method, which Mr. Broun employed in Sndia, is, however, liable to error in
high magnetic latitudes ; and the following is proposed for use in all positions. A
small magnet, 2 inches long, is suspended by a silk fibre as with the usual declination
Magnet; a small mirror attached to the magnet allows the determination of the
magnetic meridian by means of a telescope having a prism near the wire at the eye-
piece, as in Dr. Lamont’s apparatus. When the wire coincides with its image re-
flected by the mirror (no disturbing cause being near), the magnet is in the magnetic
meridian. A vertical circle in the magnetic meridian parallel to the magnet, and
3 inches distant, centre to centre, has a soft iron bar clamped to the alidade, so that
the acting pole of the bar is opposite the centre of the circle and the middle of the
Magnet. The reading of the circle is first obtained for the bar vertical: the ver-
ticality of the axis of the bar may he determined in different manners; the best,
24 F REPORT—1860.
perhaps, is to have the bar hollow, and to employ reflexion of a cross wire from a
surface of mercury. ‘The bar is then moved in the magnetic meridian from the ver-
tical position till the deflection of the magnet is zero; if the permanent magnetism
acts with the induced magnetism, the movement of the bar will he greater than the
inclination by a given angle; in turning the bar in the opposite direction (So as to
invert it), the angle from the vertical will be less by the same amount.
Since in the position at right angles to the magnetic force the induced magnetism
is zero, the objection applying to Dr. Lloyd’s method does not exist ; there is, how-
ever, still a source of error remaining that applies to both: as the magnetic inclina-
tion increases, the position at right angles to the force can only be attained by moving
the bar nearer and nearer to the horizontal, and as it approaches the horizontal, a
certain amount of magnetism is induced in the bar by the small suspended magnet.
Different methods have been imagined by the author to destroy or balance this
action; but the best method he thinks will be to make observations with the bar at
two different distances. ‘The magnetism induced by the small magnet in the bar
may be represented by a weak magnet, whose force will vary inversely as the cube of
the distance: as the action of this weak magnet will also vary inversely as the cube
of the distance, the effect may be determined and eliminated by observations at two
or more distances.
Any error of the observation for the vertical position of the bar due to the non-
coincidence of the axis of magnetism and of figure may be eliminated by turning the
bar on its vertical axis of figure through 180°.
The author remarked that the error due to the inducing action of the small
suspended magnet might be rendered as small as we please, by employing a modi-
fication of the method used by him in India. If the total deflection due to the bar
vertical (direct and inverted) be determined, and we then observe the change of de-
flection due to a given angular movement of the bar from the vertical, we may com-
pute the movement necessary to render the deflection zero: the angular movement
may be taken of such magnitude as to render the effect of the inducing action negli-
gible. This modification requires, however, the determination of the angles of
deflection, and therefore is far from the simplicity of the first method. The author
pcinted out, that, since when the bar is at right angles to the direction of the total
force any small movement of the bar will produce induced magnetism in proportion.
to the size of the small angle of movement, this position is that best fitted to give
the true position of the magnetic meridian with the least error of inclination.
The author coneluded by stating that he had learned since his return to Europe
that Dr. Lamont had also proposed a method differing from that of Dr. Lloyd. Dr.
Lamont employed an astatic needle, and turned the bars into different azimuths by
movement on a vertical axis, so as to produce different amounts of induced magnet-
ism without changing the position of the bars relatively to the vertical. ‘This
method, Dr. Lamont informed the author, had failed on account of the bars receiving
different amounts of permanent magnetism in changing from azimuth to azimuth.
This difficulty does not exist in Mr. Broun’s method, as the bar is always kept in the
meridian, and is always brought to the position where the inducing action is zero.
On Magnetic Rocks in South India. By Jouxn Avan Broun, £.R.S.
The Moocoonoomalley is a granite hill rising about 800 feet above the sea, 5 miles
south-east of Trevandrum, and about 35 miles north-west of Cape Comorin. General
Cullen, the late British Minister at Travancore, had observed several anomalies in the
magnetic dip in ascending this hill. The dip near Trevandrum and about the base
of the hill was from 2° 30’ to 2° 40’ S.; on the top he found the dip to be from
5° 52’ to 11° 23’ in different years, in which he probably slightly varied the position
of observation.
In December 1855 I examined the rock masses constituting the hill. The plain
around the base is formed of a stratified rock known to Indian geologists by the
name of laterite. The first rocks in the ascent are dark syenites, containing a con-
siderable proportion of hornblende (in some cases the appearance is more like a
greenstone) ; towards the middle of the ascent light-grey syenites become common,
Paes “(elem i ts ee
TRANSACTIONS OF THE SECTIONS, 25
and at the top the rocks are pegmatites or granites. I first examined a small frag-
ment of the rock presented to me by General Cullen, of a greyish-red tint, composed
chiefly of felspar and quartz with particles of magnetic iron ore disseminated ; these
particles were of about ;; to 34 inch in diameter, and without any regular form or
smooth face (as far as my examination went), when a magnet was presented to one
of these particles, detached from the specimen, it showed its polarity by tumbling
over, if the homonymous pole was at first nearest the magnet. The specimen
alluded to was about 5 inches long, 23 inches broad, and 12 inch thick, tapering
and thinning off to one end (A). On presenting the different extremities to a freely
suspended magnet (the declination magnet of the Trevandrum Observatory), the
following results were obtained :—
Se. div,
Specimen away. Declination reading................ 0°00
End A presented......... ais ous] dieiola alates aysTalers\inictalst voles aL se
bigs re nieile) 0061 0jn aje «, 2 ciaie) ssw 6is/e'S ie ea/sielas e'sb'es “fo be
SideC ,, WiatwyaYeheielesieveleyaieieketsWereiiveketeler aie Wes CCR ICY eal tas Wf
aD eee aalaininls feipibisuate ehafelevalajainieiel ais eisitir leieliicie) ain: €S
where the negative sign signifies repulsion of the north end of the magnet, and
the positive sign attraction of the same pole. The changes of magnetic declination
occurring during the experiments were observed by another instrument, and have
been subducted. As the line of the magnetic axis of the specimen was evidently
towards the direction of its greatest length, the northern end being towards A and C,
it was desired to determine whether the same relation would hold true for any
fragment ; for this purpose, two ends of the specimen were knocked off, leaving a
fragment in the middle with a distance of a (towards A) to 6 (towards B) of nearly
2 inches, while the breadth from C to D was nearly 3 inches; so that the longest
dimension was now nearly at right angles to that of the whole specimen. The cen-
tral fragment being placed at the same distance from the suspended magnet as in the
previous experiment, the following were the results :—
, Sc. div.
Fragment away. Declination reading...........«+++. 0°00
Binal as PreSenbed ore mie oso siahals;o)s-opcfeie) ovo) ajaicia/sje cicie’ heres: efeie = O79
” 6 5 aie) e\agalelio.a alae ei bls\'eelclepatel's ¥aterp ales aiateeie sletek aL
Side C = siat slat blaletel steel Yelatarciaverd al viciovetelechamiaecsrd Ory
5) D 3 so MaaNetele itciet allan. a/ah etotayatial eypeyeigce’ ‘epajape\ stale MCE LE
The ends and sides show the same polarities as in the whole specimen, but with
the north end of the magnetic axis turned more to the side D, for which the deflec-
tion has increased. Upon presenting the small fragment constituting the end A of
the specimen, the results were as follows :—
: : Sc. div.
Fragment away. Declination reading................ 0°00
NGRASPLESENEEM 5 S40\ejsi0, 0/6 2:512t0. ears foinisiants szaoiefoys, sy e{e ate, —-OsSO
Prac! = Rieke lal aefausieualal ¢ o¥e,a-a/oinis (ai c¥ 6, desta tela sie tern, 0°30
SideC ,, selvinis[eletiois)olate'e\a| ois cial) esiecn eG) sitethec ian Oo LA ©
aD ee Bia ole cies sewccsicscswecsvenccceesue - O14
Here it will be observed that the broken fragments of the specimen acted exactly as
the broken parts of a magnet ; thus the end a in the central fragment gave a repul-
sive effect of 0°79 scale divisions, while the end a’, the opposite face of the fracture,
gave an attractive action of 0°36.
Several questions of interest presented themselves in connexion with these rocks.
Whether the hill as a whole would give results similar to those obtained from this
specimen? Whether the lines of magnetic force in it had any relation to the lines
of crystallization, or to those of the earth’s poles? Whether any particular direction
was most favoured? or whether the magnetic axes vary from spot to spot, and the
magneticules, possessing their present magnetism when tossed up in the liquid mass,
had their positions determined by chance?
On the 11th of December, 1855, I visited the hill, making observations with a 6-inch
26 REPORT— 1860.
dip-circle by Robinson ; the following differential results were obtained without
reversing the poles of needle :—
Oo 7
10th December, 1855, 65 a.m. Base of Bill oy. 88 crc ccee econ 70 (9)
Top of hill. Circle 43 feet above rock A 3 34
oF, Circle 4 foot FF 1 6
8» to 10 a.m. ae Circle 42 feet be B 130
e Circle 4 foot fy, 1475
Noon. Base of hill over laterite............ 1 50
4" pM. Trevandrum Observatory ..,....... oo
The bearing of the Trevandrum Observatory was observed approximately by a
hand compass at the stations Aand B. At 43 feet above the rock the error was small ;
but when placed on the rock A, the declination was found 10° west, while on B
(9 feet W.N.W. of A) it was 35° east, the true declination over laterite being about
3° east.
The pegmatite and granite on the top of the hill seemed to form kinds of dykes
running parallel to each other nearly north and south, and crossed by lines nearly at
right angles to the direction, so as to form large blocks, between which the decaying
rock has allowed the accumulation of soil to some depth. Blocks of about 9 inches
diameter were cut out of the rock at A and B, having previously marked the direc-
tion of the true north and south upon the upper surface, which was nearly horizontal.
With these specimens I made the following observations. A specimen was placed
with its centre at about 2 feet from the centre of the freely suspended magnet, and
in the line at right angles to the direction of the magnet ; the points of the compass
marked on the upper surface, when the specimen was in situ, were successively pre-
sented to the centre of the magnet, and the scale readings of the instrument were
observed. The direction of the plane of greatest force being found, the specimen was
inclined at different angles to the horizontal, till the direction of the line of greatest
force was determined.
Specimen A: elliptic cylinder, axes 93 inches and 8 inches, average height about
5 inches; a granite containing a small quantity of hornblende, colour reddish grey ;
from about 1 foot west of the position A for the dip observation. The numbers fol-
lowing are in scale divisions, each equal 15" nearly :—
N. deflection ........ +21°4. S. deflection... .... —17°8
ININ:ES 5 Ss oes feet a LOPE SIS W oka ee cco —17°3
NEES PO aac ese! lbs “Have een, —15°3
E. ry Su erevete'e -+o8s W. en bt atelaetets . — 2:3
S.E. os Oe ee 193% ON Ws ay bere areata +14°5
SiS Be yp ss altec eas — 15745 CIN Weiss Pe eaG ee -. +19°9
S of lGae nse FeRe RING Wig sivaclaveinte « +21°4
The direction of the plane containing the magnetic axis is in this case nearly
north and south. On raising the point S. presented to the magnet, it was found
that the north end of the magnetic axis dipped from 10° to 20° below the south
horizon ; the exact position could not be determined, from the difficulty of keeping the
centre of the specimen always at the same distance from the magnet. The result
agrees with the fact that the dip observed on A was diminished, since the rock mag-
net having here its south end uppermost, would necessarily attract the north end of
the dipping needle.
Specimen B: cylinder 10 inches diameter, 9 inches deep; upper surface red and
weathered, interior bluish grey; contains besides the bluish felspar and quartz a
large quantity of hornblende. The observations for B were made only for the north
end of the axis.
INGING We defection’: toc sie ccuviane © tou —36°4
N. + aieleteyeteivia nidte'sretetele — 38°8
TS iy eget Re Sere ae —44:0
N.N.E. ar ie want recto Tense ats —42°4
N.E. US MMR Ate cnetere eater oh eee. —36°0
‘
TRANSACTIONS OF THE SECTIONS. 27
The north end of the magnetic axis was here evidently nearly in the direction
N. by E.3 E. Upon raising this point of the stone, presented to the centre of the
magnet, the deflection diminished ; on lowering it, the deflection increased to 10°; su
that the north end of the axis here inclined 10° above the horizon to N. by E. 3 E.
This result also agrees with the increase of dip found at B.
- In a third specimen examined, which was weakly magnetic, the north end of the
axis made an angle of 80° above the N.W. by W. point of the horizon.
From these results it is evident that though the direction of the magnetic axis
may not vary much in small specimens, it does so in parts of the rock separated by
a few feet only from each other; and it appears probable that it may be considerable
for smaller distances than those under experiment. Neither do the directions of the
axis seem to have any relation to the lines of crystallization.
Another question was examined by me, namely, whether the magnetic intensity of
the rock varied with the temperature. For this question I chose a specimen of
about 6 inches long by 4 broad and 3 thick, taken from near the middle of the ascent
of the hill. The observations were made in the same manner as for the temperature
coefficient of a magnet. The specimen was placed in a wooden trough, into which
water of different temperatures was poured: the deflections of the declination mag-
net by the specimen at different temperatures were noted ; the variations of declina-
tion during the experiments were eliminated by means of another instrument. The
results are contained in the following Table :—
Scale reading
Be VER | comer ot | ene | tania ot
hm ; Se. div.
Dec. 20. 19 Ze war eae +88° 1:07
A ee eee ea
52 | Stone away 81°82
The result is that the magnetic rock, like a steel magnet, loses force by an increase
of temperature ; and, using the notation employed for steel magnets, the temperature
coefficient is approximately
g=0'000214,
nearly the value obtained for steel magnets used in the British and Colonial Obser-
vatories.
The following may be considered as the conclusions at which I have arrived :—
Ist. The rock fragments have determinate magnetic axes.
2nd. Broken fragments resemble broken magnets, showing opposite polarities at
the two surfaces of fracture.
3rd. The magnetic axis varies from place to place within small distances.
4th. The action of the whole hill on magnets freely suspended at moderate di-
stances is nearly imperceptible; the opposite directions of the magnetic axis in the
rocks rendering the total action nearly zero.
5th. As in some cases the north end of the magnetic axis was found to the south-
ward (as with specimen B), we cannot suppose that the magnetism of the small
magnets has been due to the inducing action of the earth in their present position or
since the rock mass became solid.
6th. The directions of the magnetic axis have no relation to the lines of division
of the rock masses.
7th. The magnetic force of the rock masses varies with temperature like that of
steel magnets.
On a Magnetic Survey of the West Coast of India.
By Joun ALLAN Broun, F.R.S.
This survey was undertaken at the expense of His Highness the Rajah of Travan-
28 : REPORT— 1860.
core, for the purpose, in the first instance, of determining the exact position of the mag-
netic equator (which passes through his territory) and the variations of intensity about
the line of no inclination. This part of the survey was performed with considerable
care, stations being chosen along the line of coast, at distances of from 10 to 15 miles,
generally far from the chain of the Ghats, and in a flat country, covered in many
places by backwaters or lagoons. The instrument employed was the excellent theo-
dolite magnetometer of Dr. Lamont. The results were, that the magnetic south in-
clination, instead of diminishing regularly from Cape Comorin northwards to the line
of no dip, diminished through a space of 30 miles, increased through a similar space,
and again diminished in the most capricious manner. The same irregularities were
observed north of the estimated position of the equator. Some irregularities had
been already observed by Mr. Caldecott, Mr. Taylor, and General Cullen; but the
author had confirmed his results by observations at many different stations, and had
come to the conclusion that a belt of disturbance for this element existed near the
line of no dip. This disturbance could not be attributed to the influence of hills or
of rocks, as no ground of greater elevation than 30 to 40 feet existed within several
miles of those stations showing the greatest irregularities, no rocks were reached by
borings of 30 to 50 feet deep, and none appeared upon the surface above the sandy
soil near these stations.
The survey was extended by the author on his way to Europe by observations at
stations further north than those in Travancore, as Kodungalur, Kalikut, Mangalur,
Goa, Rutnagherri, Bombay, and Aden. From this and the first part of the survey,
the author found that the horizontal intensity was nearly the same from Cape
Comorin to Bombay, showing, as the author conceived, that the lines of equal inten-
sity followed (somewhat like the isothermal lines) the line of the Indian coast. This
result agrees with that obtained by the Messrs. von Schlagintweit, whose previous
observations indicate a great bend of the isodynamic lines from the Himalayas and
towards Cape Comorin. The whole question, the author conceived, required careful
examination by means of observations at more numerous stations, as the theory of
the causes of the earth’s magnetic intensity, and the arrangement of the magnetic
lines, were evidently involved in results which differed so much from what had been
found elsewhere, especially from the results obtained by Dr. Lamont from his admi-
rable magnetic survey of the greater part of the European Continent.
On the Velocity of Earthquake Shocks in the Laterite of India.
By Joun ALLAN Brown, F.R.S. (See GEoioey.)
On a Mode of correcting the Errors of the Compass in Iron Ships.
By A. Crarke, New South Wales.
On Electrical Force. By Sir W. Snow Harris, F.RS.
The author adverted to the assumed existence in nature of an electric fluid or
fluids, an idea entertained by philosophers from the earliest periods of the history of
electricity. Many thought that all bodies expire or inhale this fluid. In modern
times less ambiguous views have been resorted to, and the doctrine of an electric
fluid or fluids has been employed principally as aiding to link the phenomena into
an intelligible and connected chain. The author thinks the time is fast approaching
when it may be found desirable to abandon all idea of electrical fluids as the agency
concerned in the development of electrical force, and treat this species of force as
Newton did gravity, without any care as to its occult quality. For although it may
be convenient and perhaps useful to employ analogical expressions in interpreting
the phenomena and to facilitate description, as when we speak of the quantity of
electric matter, of its tension, density, or thickness of stratum, &c., yet it must
ever be remembered that, in using this figurative language, it is force and the laws
of force with which we are dealing, and not with electrical fluids or other assump-
tions as to its occult nature or quality.
———._ ose. |.) =
a
TRANSACTIONS OF THE SECTIONS. 29
The author proceeded to say that the foundation of all exact science is number,
weight, and measure ; and that, as observed by an eminent writer, no branch of phy-
sical knowledge could be held as being out of its infancy which did not in some way
or the other frame its theory, or correct its practice with reference to these elements.
He here described and explained the nature of a series of very beautiful instruments,
by which the quantity of the electrical agency, its attractive force, its explosive
power, and the effects produced, could be accurately measured. Having thus en-
deavoured to bring the unknown agency we term electricity under the dominion of
number, weight, and measure, the leading characteristics of electricity as a force
were next brought under consideration. And first, we observe electrical power
exhibits itself under two forms, usually termed vitreous and resinous electricity, or
positive and negative electricity. These have been usually considered as arising
out of two distinct and separate fluids, or of a single elementary fluid in a greater or
less state of condensation. They are, however, one and the same force, and have
the same relation to each other as the forces of compression and extension in the
case of a bent bow or spring. We cannot have one without the other; and as in
the latter instance we should gain but little by assuming the existence of elastic
fluid or fluids as the source of elasticity, so in the case of electrical force we may as
well look at once upon positive and negative electricity as elementary facts of which
we have no adequate explanation.
Secondly, we observe that whatever be the nature of electricity as a physical
agency, it cannot exert itself equally in all directions at the same moment. In the
case of gravity, the sun does not attract the earth with less force because it is
exerting its gravitating power on the other planets. Such is not the case in the
development of electrical force. The author here introduced a striking experiment
in illustration of this; showing that a delicate electroscope, attracted toward an
electrified circular plate placed vertically, became less forcibly drawn toward the
plate from a distance when a second body was brought to share in the action. This
is the result of a third characteristic of electrical force, termed electrical induction
or influence, the laws and operation of which were now further explained and illus-
trated. It is solely upon this species of electrical action, apparently of a sympa-
thetic kind, operating at a distance, probably by propagation through the intervening
medium, that electrical attractive force altogether depends: without it no exertion
of power is possible. In electrical force bodies are first rendered attractable before
they become attracted, and for the regular and full exertion of the attraction, both
the bodies must be susceptible of unlimited electrical change. When this is the case
the development of force is easily traced ; and the force will be found to vary as the
square of the quantity of electricity in operation directly, aud as the squares of the
distances inversely : of this some striking and very interesting experimental illustra-
tions were given through the instrumentality of the electrical balance, delicately set
up with complete means of adjustment for distance and force; and it was with re-
markable precision the beam descended when under the influence of two attracting
surfaces ; the quantity of electricity and the weights being given, the force of in-
duction, upon which the resulting force depends, varies in the simple inverse ratio of
the distance between the attracting surfaces, and depends, first, upon the direct in-
fluence of the electrified surfaces, secondly, upon a reflected induction thrown back
upon the excited body. The total force is in a compound ratio of these forces, and
it is in this way we obtain a force in the inverse duplicate ratio of the distances. If
from any cause either or both of the previous elementary actions be interfered with,
then we have no longer this law ; so that any law of electrical force is possible, as
found in the experiments of many eminent philosophers of past days—Muschenbroek,
Brook, Taylor, Whiston, Martin, and others. The author thinks that the results of
the experiments of these eminent men have been called unjustly in question; every
result they arrived at is producible by careful manipulation.
The author now brought under consideration the question of electrical force be-
tween spheres, one charged with electricity, the other neutral and in a free state.
This question had been often elaborately treated, and had been hitherto considered
a physico-mathematical question of great intricacy. An analysis of the elements of
this question was here entered upon. Upon the proved facts that the force varies
with the quantity of electricity and is in the duplicate inverse ratio of the distance,
30 REPORT—1860.
two points may be found within the opposed hemispheres in which we may con-
ceive the whole force to be collected, and to be the same as if proceeding from every
point of the opposed hemispheres. These points approach the surface, and become
the touching points when the spheres touch ; as the spheres separate they approach
the centre, and reach the centre when the distance is infinite. If we call a the
distance between the points of contact, and r=the radius of sphere, we have,
putting F=the total attractive force, F « ; and calling the points of centre
1
a(a+ 2r)
of force=gq q’, we have distance q q’=the tangent from either of the touching points
to the opposite sphere; or if distance ¢ q'=D, we have Fz pt a 5°
Several very remarkable experiments were now adduced in evidence of the truth of
these formule. Spheres of variable diameters were put in opposition in the balance,
the quantity of electricity measured, and weights placed in the scale-pan, as deter-
mined by calculation; the distances being regulated accordingly, the scale beam
bowed in obedience to the given law of force with extreme and wonderful exactitude :
the experiments elicited much commendation.
The author thinks that every observed operation of electrical action is reducible
to simple and elementary laws free of complication, and may be investigated and ex-
pressed by an easy mathematical analysis and forms of expression. He thinks that
all the laws of nature are of the most simple kind, and only involve a simple rela-
tion of cause and effect; if we double the cause we double the effect. To suppose
an effect to be as the square or cube of its cause, is to suppose the effect to depend
partly on the cause and partly on nothing. There is probably, taken as a simple
elementary law, no such a law in nature as that of a force being in the inverse
duplicate ratio of the distance. Take, for example, the case of gravity as central
force, and assumed to be a species of emanation from a centre, it is true that
at twice the distance we have only one-fourth the force ; but this is because the areas
of the concave spherical surfaces, which we may imagine the emanation to fall upon
at these distances, are to each other as 1:4; so that in any one point of the outer
sphere there is only one-fourth the agency upon which the force depends, conse-
quently only one-fourth the attraction; but this is a simple relation of cause and
effect. Taking light as an emanation from a centre, the same result ensues. If
there be only one-fourth the quantity of the emanation in any point, we can only
have one-fourth the light, and thus light or gravity may be said to be in the inverse
duplicate ratio of the distance.
On the different Motions of Electric Fluid. By the Rev. T. Rankin.
The author, from several very striking and vividly-described thunder-storms and
their permanent effects, concludes that sometimes the electric fluid moves downward,
sometimes upward, and sometimes horizontally. On one occasion, some years since,
about two o’clock, on a night on which it had thundered almost incessantly, a loud
whizzing sound was heard to pass over the rectory-house, which he judged to be an
aérolite; a tree in the direction it had passed was struck; and from the nature of the
injury inflicted, the conclusion was drawn that the motion of either the aérolite or
of the electric fluid had been nearly horizontal.
On the Phenomena of Electrical Vacuum Tubes, in a letter to Mr. Gassiot.
By Professor W. B. Rocers, Boston, U.S.
I send you, by my brother, a printed abstract of remarks made some months ago
on the phencmena of the vacuum tubes, and a hypothesis as to the condition and
cause of the stratifications.
You will see that, with the aid of Mr. Ritchie and our skilful photographer, Mr. ~
Black, I have been experimenting on the actinism of these electrical discharges.
_ In some more recent trials I have obtained beautiful photographs of the stratifica-
tion, of which I send youa specimen, The tube, as you will see, is a straight one, of
se a oe
eS
TRANSACTIONS OF THE SECTIONS.
31
uniform calibre. It is about 15 inches long, by $ inch diameter, and is marked
by Geissler as containing phos. hydrogen. As you have
perhaps observed, it gives the strata with extraordinary di-
stinctness ; and after the action has been continued a little
while, the strata near the blank end arrange themselves in
pairs, consisting each of a bluish and a more reddish layer,
separated by a blank interval from the next, as seen very
plainly in the photograph.
By a steady, rapid motion of the ratchet-wheel of Mr.
Ritchie’s coil, it was easy to keep the strata almost perfectly
stationary. The picture was obtained with eighteen turns of
the wheel, each giving twelve sparks. With six turns a
tolerably clear picture was secured.
You see that the unilluminated space at one end made no
impression, and that the intervals between the strata are also
as devoid of actinic as they are of luminous rays.
The picture of the winding tube, with bulbs, shows how
superior is the actinism of the faint blue light of the negative
end compared with the brighter and less refrangible rays of
the opposite bulb.
The third photograph was
produced by the two slender
Geissler tubes, containing re-
spectively N and CO,. The
former was placed below the
latter as they were presented
before the camera, and the
current was sent through them
in succession. To the eye the
intense whitest light of the
voit
cai ies
CO, tube was more dazzling than the crimson colour-
ing of the other. Yet you will observe the picture
made by the latter is far the stronger of the two, as
indeed might have been expected from its more re-
frangible illumination,
This photograph was produced with half a turn of
the wheel, that is, six successive flashes of the light.
I am unable to state the aggregate time of exposure to
the rays, as I have not yet ascertained the duration of
a flash. This I hope, with Mr. Ritchie’s aid, to ac-
complish at an early day. But if we assume the time
to be as much as tenfold the duration of the electric
spark, as measured by Wheatstone, we should have
less than saath of a second for the entire time which
the light required for producing this intensely clear picture. I believe that.a single
flash would suffice, but I have not yet made the trial.
32 REPORT—1860.
General Abstract of the Results of Messrs. de Schlagintweit’s Magnetic Sur-
vey of India, with three Charts. By M. H. von ScHLacintwEIt.
M. Hermann de Schlagintweit gave a general report on the results obtained
during MM. de Schlagintweit’s magnetic survey of India and High Asia, from 1854
to 1857.
He presented three charts, showing the lines of equal declination, dip, and inten-
sity, from Ceylon up to Turkistén. Also the details of their observations as con-
tained in the first volume of their work, ‘ Results of a Scientific Mission to India
and High Asia,’ undertaken by order of the Hon. East India Company, was laid
upon the table.
The magnetic results were preceded by a communication of those latitudes and
longitudes, particularly to the north of the Himalayas, which were either new as to
localities or found to differ from previous determinations.
For the construction of their charts, they most carefully compared also the previous
observations ; such as, for the intensity in Northern India, Taylor’s and Caldecott’s,
and particularly those recently made by Mr. Broun; for the declination along the
coasts, the determination of the Indian Navy; but Capt. Elliot, their predecessor,
having died before he could extend his survey from the Indian Archipelago to India,
and the only detailed observations in the outer Himalaya (General Boileau’s, at
Simla) being destroyed in the last mutiny, their observations must be considered as
made in a territory novel for this branch of science; and a great part of them was
besides made under circumstances so difficult, that unhappily one of the three
brothers was killed in Turkist&n.
The following results are particularly to be mentioned :—
I. Declination.—1. A zone of too little easterly declination, of considerable ex-
tent, was found inAssam. 2. In the north-western part of India the declination was
found to vary more rapidly than in the surrounding territories. 3. In the region of
the Kuerluen the declination was found more easterly than given by the approximate
form of the isogonic lines as provisionally laid down till now for these regions.
Il. The Dip.—This was found, of the three elements, the most regular in its
general forms; though local deviations are not unfrequent, they are small and very
limited.
III. Total Intensity.—Two unexpected results presented themselves:—1l. A de-
cided inflection of the isodynamic lines in the central and southern parts of India,
2. A zone of depression all along the outer ranges and the base of the Himalaya.
In reference to the first, M. de Schlagintweit pointed out, as particularly import-
ant, that the very careful observations of Mr. Broun all along the western coast of
India, made quite independent of, and subsequent to, their own, perfectly coincided
with the lines based on their observations.
The magnetic influence of a large surface of soil exposed to the physical action of
a tropical insulation, and the non-existence of such an influence in the rainy and
much more clouded regions of the outer Himalayas, were named as perhaps not un-
connected with this phenomenon, so particularly characteristic in India.
Outline of the Principles and Practice involved in dealing with the Elec-
trical Conditions of Submarine Electric Telegraphs. By M. Werner
and C.W. SteMENs.
The authors, who have had very extensive experience in dealing with submarine
and other electric telegraphs, state that the failures of the more extensive submarine
lines commence generally by a gradual decrease of insulation. The cause of this
failure has been found, in repairing these lines, to consist in a disintegration of the
gutta percha by the electrolytical action of the currents employed in working the
line in such places where the insulating covering was much below the average thick-
ness, owing to excentricities, cavities, &c. In other places, where the gutta percha
had been of uniform and sufficient thickness, not the slightest destruction took place ;
but it might be laid down as an axiom, that “so long as there are any thin places
b
v
é
‘s
7
d
>
TRANSACTIONS OF THE SECTIONS. aa
allowed to remain in the gutta percha coverings of a submarine conductor, so long will
their insulation fail by slow degrees.”
Great improvements have of late been effected, which may be estimated by the
fact that the covering of the Rangoon and Singapore cable, now in process of manu-
facture, insulates ten times better if reduced to the same thickness of coating than
the covering of the Red Sea and India cable did before it was laid; and these
marked improvements are due to the greater care used by the Gutta Percha Com-
pany, assisted by stringent electrical tests which the authors are charged by the
British Government to apply.
The chief characteristic of these tests is, that the conductivity of both the con-
ducting wires and the surrounding coating, which is regarded in the light of an in-
ferior conductor, is expressed in numerical units, capable of direct comparison. The
unit of resistance adopted is that of a column of mercury, 1 metre in length and of
One square millimetre sectional area, taken at the freezing-point of water (as de-
scribed by Werner Siemens in Poggendorft’s ‘ Annalen,’ vol. cx.). In expressing
the degrees of conductivity of both the wire and the insulating medium in definite
units of resistance, not only the advantage of a more accurate comparison between
the results of different indication is obtained, but subsequently, when the separate
coils are united together to a single cable, it affords an admirable means of judging
its electrical condition in comparing the total resistances of both the conductor and
insulating medium with the sum of the resistance previously obtained in testing each
coil separately ; but the principal advantage derived from this system of measuring,
consists in the facilities it affords in determining the position of a fault in a cable
while it is being Jaid and after submersion. In carrying this system into practice,
MM. Siemens constructed coils of definite resistance variable from 1 to 50,000 units
of resistance.
The cables to be tested are placed for twenty-four hours in water regulated to
75° F.; they are then removed into the testing tank of the same temperature, which
is hermetically closed, and hydraulic pressure of at least 600 lbs. per square inch
applied, in order to force the water into the cavities or fissures that may present
themselves.
It is a remarkable fact, which is also borne out by observation upon cables in
process of submersion, that the application of hydrostatic pressure sensibly decreases
the conductivity of gutta percha; which, however, increases again slightly beyond
the former rate when the pressure is relieved.
For a full description of the methods of testing employed, we must refer our
readers to the paper itself.
The authors give a description of a new instrument by means of which they test
the inductive capacity of cables, which has also to be accurately ascertained for the
purpose of detecting faults; and have affixed a Table containing many satisfactory
results, and proving the correctness of a formula for calculating the specific induc-
tion of cables, which was obtained by Professor Thomson and M. Werner Siemens
by different scientific deductions.
The specific inductive capacity of all gutta percha is shown to be nearly the same,
and to be entirely independent of the specific conductivity of the gutta percha ; while
India-rubber and Wray’s mixture are far inferior in specific inductive capacity, being
equal to 0'7 and0°8 respectively, gutta percha being taken = 1.
In this way the cable is examined repeatedly at the earliest stages of its manu-
_ facture, in lengths of one knot, during the joining and covering of the cable, and
finally during the paying out.
The paper next gives a full description of the electrical tests to be applied during
the paying out, and numerous formule by means of which faults in the cable are
ascertained under various circumstances. By these means Messrs. Siemens were
_ enabled to determine with great accuracy faults in the Indian cable, both during the
“paying out and afterwards, which enabled the contractors, Messrs. Newall and Co.,
_ to effect the necessary repairs with a certainty which could not formerly be obtained.
_ Respecting the prospects of success of new lines of submarine cables, the paper
_ States that, owing to the great care used, the conductor of the Rangoon and Singa-
pore cable is fully ten times more perfectly insulated than the best cable hitherto
submerged ; and that it may confidently be expected that the result in practice will
1860. 3
4
34 REPORT—1860.
also greatly exceed that of previous experience; still the insulating material em-
ployed remains the same, and is therefore liable to be affected by the same causes of
failure.
The frequent failure of gutta percha has given rise lately to several projects of
substituting India-rubber and its compounds for the same, which, owing to the
higher insulating properties and lesser inductive capacity of India-rubber, and
above all, owing to its greater homogeneity and resisting power to effects of heat,
give promise of valuable results in making electric telegraphs less liable to failure,
The chief difficulty consisted hitherto in working India-rubber in such a way as to
obtain uniform and perfect coatings upon the conductor without injury to the con-
ductor itself. The authors have endeavoured to remove this difficulty in construct-
ing a covering machine, which they brought before Section G of the Association.
They conclude,—‘ We do not wish, however, to rest upon our individual efforts
for the further development of this important new branch of applied science. Our
object in writing this communication has been to show that, although submarine
electric telegraphs have often failed, the experience gained has not been lost; and
that in bringing the present stock of knowledge to bear upon the subject more com-
plete success may be ensured.”
ASTRONOMY.
On the Forms of certain Lunar Craters indicative of the Operation of a
peculiar degrading Force. By W. R. Birt, F.RAS.
There are on the surface of our satellite three well-marked classes of lunar craters,
those that are more or less complete in the outlines of the mountainous rings by
which they are surrounded, having in many cases a somewhat deep interior, and
appearing as excavations on the surface of the moon. Cleomedes, Geminus, and
others in their neighbourhood are examples. We have also among the perfectly
surrounded craters those that have their rings somewhat considerably elevated above
the general level of the lunar surface. Tycho may be cited as the most perfect
instance of the raised craters. Both these kinds agree in a very important particu-
lar; the surrounding ring (whatever may be the varying altitudes of different peaks,
or however certain portions may rise higher than others) is in this class complete ;
there is no evidence of the operation of the peculiar degrading force, to which | shall
presently allude—certainly not to any very great extent—in breaking down any por-
tion of the surrounding annulus.
A second class of lunar crater consists of those that, having the surrounding ring
complete, do not exhibit the depth of such craters above specified, or the gradual rising
from the general surface as seen so distinctly in Tycho; they stand out as it were
above those portions of the surfaces of the moon where they occur—generally the
Maria—as if the smooth undulating plains had come quite up to the rings which rise
abruptly from them. Most of these craters have smooth level interiors; and there
are instances of the first class situated in rugged mountainous districts possessing
also a smooth interior. Plato may be quoted as an example. Many instances of
this class occur in which the ring is but slightly raised above the interior and exte-
rior surfaces.
The third class, to which I am particularly desirous of referring, consists of such |
craters as having apparently at some previous period of their history possessed a
perfect ring; 2 degrading force, not such as may have produced the terraces and
ravines which we notice in Copernicus, but something of a different character, has —
invaded them from without, breaking down certain portions of the annulus, and ~
leaving only a portion of the walls standing: these craters mostly occur on the bor- —
ders-of the Maria; and it is not a little significant that the broken portions are in-
variably, so far as my observations extend, on the side next the Maria, the parts of
the annuli opposite the Maria being more or less in their earlier state.
The two undermentioned craters appear to be interesting examples of this class—
Fracastorius, situated on the border of the Mare Nectaris, and Hippalus on the
——
TRANSACTIONS OF THE SECTIONS, 35
border cf the Mare Humorum. The ring of Fracastorius is so much broken down
towards the Mare Nectaris as to give the crater the appearance of a small bay, un-
less viewed under a suitable illumination—a very early one—when the edge of the
crater towards the Mare is seen as a series of low points or peaks casting very short
shadows. The floor of the interior appears to be somewhat different from the sur-
face of the Mare, and seems to be slightly depressed below its level. The crater
Hippalus is highly interesting; seen under a very early illumination: the western
half of the floor is rngged, having a number of hillocks scattered over it and two
minute craters ; the eastern half is smooth, very like in appearance to the surfaces of
the Maria; but the most remarkable feature is the line separating the crater from
the Mare, just as though the Mare had come up to and swept away half the ring of
the crater and a portion of its floor, the two extremities of the semicircular range of
mountains being very distinct, especially the north-eastern, which terminates ab-
ruptly ; not the vestige of a shadow is observed between the two, the light passing
between them unobstructedly.
On the Possibility of Studying the Earth's Internal Structure from Pheno-
mena observed at its Surface. By Professor Hennessy, F.R.S.
This the author showed to follow as a result from the comparison of the level
surface, usually called the earth’s surface by astronomers and mathematicians, with
the geological surface which would be presented if the earth were stripped of its
fluid coating. He had made several comparisons of the arcs of meridian measured
in different countries, and had been thus led to the conclusion that the surfaces in
question were not only dissimilar, but that the former derived many of the irregular.
ities which it is known to present from the influence of the obvious irregularities of
the latter. In the absence of precise knowledge of the true figure of the surface of
the solidified crust of the earth, as well as of the assumed level surface perpendicular
to gravity, theory was necessarily somewhat in advance of observation upon this
particular question. At present the number of unknown quantities involved in
an inquiry as to the earth’s internal structure was greater than the number of condi-
tions ; but by knowing the true surface, and adopting the results of established
physical and hydrostatical laws relative to the supposed internal fluid mass*, we
should be able to form as many equations as we have unknown quantities, and thus
ultimately obtain a solution.
On some Recorded Observations of the Planet Venus in the Seventh Century
before Christ. By the Rev. Epwarp Hincxs, D.D., of Killyleagh,
Ireland.
There is a tablet of baked clay in the British Museum, the inscription on which,
if I interpret it aright, contains a series of observations of the planet Venus, and a
series of predictions grounded on the observations. The latter are of no value; but
the former may in great measure, if not altogether, determine the law by which the
Assyrio- Babylonian lunar year was regulated in respect to its intercalary months.
The knowledge of this law, again, will either establish or disprove the view which I
have Jong entertained, and repeatedly expressed, that the era of Nabonassar was
an astronomical, and not a political one; and I may add, it is not impossible that it
may furnish a test of the genuineness of the works attributed to Quthami and other
_ supposed ancient Babylonian writers. For these reasons I am desirous that the
observations which I suppose to be recorded should be submitted to astronomers.
I now offer two, which will suffice to test the correctness of my interpretation of the
records. If any astronomer will take the trouble to calculate whether what is here
stated to have happened would have actually happened, and will communicate the
result to me, I will, if he desire it, communicate to him other records of observations,
as to the interpretation of which I feel less confidence than I do as to these. I observe
_ that the Babylonian months are expressed by monograms, for which I substitute
_ Hebrew names of months. The Babylonian day began at noon; and that day in
_ the evening of which the new moon was first seen was considered to be the first day
of the month. I suppose, but am not very confident, that the year of the first obser-
-* See Reports for 1859, Trans, Sect. p. 5. :
3%
06 ae REPORT—1860,
vation was —685. The month of Thamuz would begin in the spring. The second
observation was some years later. ‘‘ On the 25th of Thamuz, Venus ceased to appear
in the west, was unseen for seven days, and on the 2nd of Ab was seen in the east.”
“On the 26th of Eiul, Venus ceased to appear in the west, was unseen for eleven
days, and on the 7th of the second Elul was seen in the east.’”? This being an em-
bolismatic year, the day last mentioned was necessarily its 184th day, and was 200
days before the first day of the new year. If, then, this day can be determined from
what is recorded of Venus, the commencement of two Babylonian years out of a
cycle of eight will be determined. The foregoing had been communicated to the
Royal Astronomical Society, but is not yet published. Dr. Hincks now added his
conviction, that by combining those observations with that of the equinox, recorded
on another tablet, a translation of which was given by him in the Transactions of
the Royal Irish Academy, the determination of the year in which any of those obser-
vations took place would determine the commencement of every Babylonian year.
The Babylonians were acquainted with the approximate equality of eight tropical
years, five synodic revolutions of Venus, and ninety-nine synodic revolutions of the
moon. The first observation, if in the seventh century before Christ (which is pro-
bable, though not quite certain—later than this it could not be), must have been
in a year of the form —685 = 87.
On the brilliant Eruption on the Sun's Surface, 1st September 1859.
By R. Hoveson, F.R.A.S.
While observing a group of solar spots on the Ist of September, I was suddenly
surprised at the appearance of a very brilliant star of light, much brighter than the
sun’s surface, most dazzling tothe protected eye, illuminating with its light the
upper edges of the adjacent spots, not unlike in effect the edging of the clouds at
sunset: the rays extended in all directions, and the centre might be compared to the
dazzling brilliancy of the bright star « Lyre, when seen in a large telescope
with a low power. It lasted five minutes, and disappeared instantaneously
about 11525" a.m. Telescope used an equatorial refractor, 6} inches aperture,
carried by clockwork. Power single convex lens 100, with pale neutral tint sun-
glass. The whole aperture was used with a diagonal reflector. The phenomenon
was of too short a duration to admit of a micrometrical drawing, but an eye-sketch
was taken from which the enlarged diagram was made.
The only other observer was Mr. Carrington at the Red dill Observatory, but a
drawing was made of the spot by the Rev. William Howlett of Hurst Green, at
noon, within half an hour of the occurrence. From a photograph taken at Kew
the previous day, the size (length) of the entire group appears to have been about
2 minutes 8 seconds, or say 60,000 miles.
' The magnetic instruments at Kew and Greenwich were simultaneously disturbed
at the same instant to a considerable extent.
Prospectus of the Hartwell Variable Star Atlas, with six Specimen Proofs.
By Joun Let, LL.D.
The work announced is to form one of a series of quarto volumes, of which
Admiral Smyth’s well-known ‘ A‘des Hartwelliane’ and ‘ Speculum Hartwellianum’
may be regarded as the commencement. It is to comprise maps of the vicinity of
all stars of established variability, —at the present moment 102 in number. The
light ratio or magnitude scale employed was explained, and six specimen proofs ex-
hibited to the meeting. The scale of projection is unusually large and clear; 3
inches to one degree, to avoid crowding and confusion. After dwelling at some
length upon the unsatisfactory state of our knowledge of the variable stars, and
making allusion to the most recent researches and discoveries, especially to those of
Professor Argelander, Sir John Herschel, Mr. Hind, and Mr. Pogson, and to the
annual ephemeris of the variable stars published by the last named astronomer for
four years past, Dr. Lee remarked,—
“A variable star usually remains unchanged for several nights, sometimes even
for weeks, when either at maximum or minimum; and yet, owing to the difficulty
of estimating absolute magnitudes correctly, and still more to the prevalence of haze
TRANSACTIONS OF THE SECTIONS. iA
and other uncertain atmospheric fluctuations, the most practised eye would fail to
fix at all satisfactorily, either the time or amount of greatest or least brilliancy. By
comparing the variable with neighbouring stars, which are of course similarly affected
by atmospheric influences, most of this uncertainty is however avoided; and by
careful consideration of the rapidity of increase and of decrease, the time of maximum
or minimum is very closely and easily limited. In order to make such comparisons,
it is requisite to know the absolute magnitudes of the stars of reference pretty cor-
rectly. A convenient number of stars in each map will therefore have the magni-
tudes annexed in plain figures, omitting the decimal points to prevent their being
mistaken for faint stars; and it is to render this aid to future observers of variable
stars that the ‘ Hartwell Atlas’ is now being constructed.”
On the Physical Constitution of Comets.
By Professor B. Prerce, of Cambridge, United States.
On the Dynamic Condition of Saturn’s Rings.
By Professor B. Pierce, of Cambridge, United States.
On the Motion of a Pendulum in a Vertical Plane when the point of suspen-
sion moves uniformly on a circumference in the same Plane. By Professor
B, Pierce, of Cambridge, United States.
METEOROLOGY.
On a Plan for Systematic Observations of Temperature in Mountain
Countries. By Joun Bari, MRLA.
Several members of the Alpine Club have agreed to unite in a plan of systematic
observations of temperature in the Alps, and such other mountain countries as they
may visit. It is possible that the plan of combined action may eventually be
extended to other objects, but for the present it embraces only such observations as
may be made with thermometers. As the intention of the present paper is merely
to invite the suggestions, and if possible the cooperation, of members of the Physical
Section, it seems unnecessary to state in detail the arrangements which are proposed ;
and it will be sufficient to indicate generally the points to which it is believed that
the observations about to be commenced may most usefully be directed.
Ist. The condition of the upper parts of high mountains in regard to temperature
is most imperfectly known. It may not be possible to learn much by direct con-
tinued observations, but it is thought that by means of self-registering instruments
we may add considerably to the little which is now known. It is proposed to place
such instruments, and especially minimum thermometers, on as many of the higher
peaks of the Alps as possible, and to register their indications in succeeding seasons.
The chief practical difficulty in carrying out this branch-of the proposed plan is to
find positions at great heights that are free from winter snow. It will be necessary
to select vertical or nearly vertical rocks in order to attach the instruments thereto,
and these are not always to be found very near to the highest summits of great
mountains.
2nd. It is a matter of much interest, but of considerable difficulty, to obtain
measures of the effect of the lower strata of the atmosphere upon the radiant heat of
the sun. The general opinion of mountain travellers is adverse to the use of the
actinometer in any of the forms in which that instrument has yet been devised, and
the same may be said in regard to other instruments proposed for the same purpose,
The objections to observations with the black bulb thermometers are obvious and
well known, but it is thought that observations made on a uniform plan, and with
instruments of exactly the same dimensions and construction, would give compara-
tive measures which would have some positive value, If it should be possible to
obtain series of such observations made at two stations very different in elevation,
and exactly simultaneous, they could scarcely fail to give valuable results.
3rd. We are very ignorant at present as to the mode in which disturbances of
38 REPORT—1860.
temperature are propagated from one place to another in mountain countries. Con-
siderable variations of temperature are not unfrequent, and sometimes occur very
rapidly, usually if not always in connexion with changes of wind ; but we know very
little of the way in which a disturbance of this kind is transmitted eitker in the
horizontal or the vertical direction. It is conceived that a network of observations
made by a considerable number of observers scattered over a district, such as Swit-
zerland and Piedmont, would lead to some increase of our knowledge in this respect.
4th. Observations on the temperature of the surface and upper layers of the soil
have a considerable bearing on many questions connected with the distribution of
plants. One difficulty in investigating these questions arises from the difficulty of
comparing observations not made upon a uniform plan. It is thought that the
adoption of uniform instruments, and a plan of observations previously agreed upon
by all the members of the party, will much increase the value of their results. All
the instruments used in these observations are exactly of uniform construction, and
made by Mr. Casella with the utmost practicable regard to lightness and convenience.
Each instrument is numbered for purposes of future reference.
On Atmospheric Waves. By W.R. Birt, F.R.A.S.
The object of this communication is rather elucidatory than otherwise. It is now
twelve years since I had the honour to lay before this Association the last of my
reports on the subject. During the interval it has doubtless occupied the attention
of other minds, and some degree of misconception may have arisen which may call
for some elucidatory remarks on my part, especially as the series of reports in our
annual volumes has been referred to on the Continent, as establishing a priority of
investigation into these phenomena on the part of the British Association for the
Advancement of Science.
It is now several years since Professor Dove announced as his conviction that the
equilibrium of the atmosphere was maintained in the extra-tropical zones, more by
parallel than superposed currents, that these currents had a shifting transverse or
lateral motion, and in consequence, so to speak, they advanced “‘sideways.” I am
not aware that Professor Dove connected these shifting parallel currents with baro-
metric phenomena, although he did with thermometric. In the course of my inves-
tigations into those phenomena termed atmospheric waves, I ascertained, by carefully
discussing the records of the wind for the greater portion of November 1842, that
not only such parallel compensating currents existed as stated by the Professor, but
that during the period under inquiry, a similar system of parallel and compensating
winds were blowing and moving at right angles to them. The arrangement of these
cross winds was N.E.—S.W. and N.W.—S.E. I also found that these winds were
intimately connected with barometric pressure, so that when the barometric curve
Was projected and presented the wave form, the mind was led to group under the
general term ‘‘ atmospheric wave,” at least ¢wo if not three distinct classes of phe-
nomena. First, the winds succeeding one another, as we know they do with more or
less regularity. Second, the pressure, a more or less continuous fall of the barometer
generally succeeding a gradual and continuous rise: both these phenomena are
capable of being represented by curves, the rising barometer mostly coinciding with
the decreasing force of wind, and the falling barometer with its increase, so that a
rising and falling curve will with more or less fidelity represent the passage over a
station or a tract of country of the two compensating currents of Dove. It is not
the mere rise and fall of the barometer, as such, that constitutes an atmospheric
wave; the barometric curve itself is doubtless the complex result of two or more
distinct variations of pressure connected with variations of wind as above. When
these are disentangled, the mind is able to grasp the onward march of the two par-
allel winds, accompanied by their respective pressures; so that true waves of press-
ure really, I apprehend, sweep over a country; and applying the wave nomenclature,
low pressures have been characterized as troughs and high pressures as crests.
As illustrative of these remarks, I beg to exhibit on this occasion the most com-
plete instance of opposite pressures that has come under my notice ; it is the opposite
barometric curves at Alten and Lougan during the early part of November 1842: the
curves will be found on page 39, ‘ Report,’ 1848. Iam indebted to Dr. Lee for the
observations furnishing the curve at Alten.
;
:
‘
=e ere
TRANSACTIONS OF THE SECTIONS. 39
Observations on the Meteorological Phenomena of the Vernal Equinoctial
Week. By M. Du Boutay.
The author has been engaged for the long period of thirty years in endeavouring
to ascertain whether there could be traced in the winds or weather prevailing about
the equinox, in any given locality, a counexion with, or resemblance to, the winds
and weather generally prevailing during the ensuing summer in the same locality,
He infers from his observations that such is the case, and that the probable character
of the summer in England may be predicated about the 25th of March, by noting
the weather in the equinoctial week then just ended. He gave examples in support
of his views.
On the Effect of a Rapid Current of Air. By R. Dowven.
On British Storms, illustrated with Diagrams and Charts.
By Admiral FirzRoy, F.R.S.
It is well known that no year passes in which the British islands are not visited by
storms, and that they vary in degree of force from what seamen call a gale to a
hurricane irresistible in violence. Only of late years, however, has it been supposed,
and but recently proved, that nearly all, if not indeed the whole, of these remarkable
tempests, by which a very notable amount of injury has been done, have been so
much alike in character, and have been preceded by such similar warnings, as to
warrant our reasoning inductively from the well-ascertained facts, and thence inferring
laws. Every one looks back to some extraordinary storm as exceeding all others in
his lifetime; but a tempest that is severely felt in one part of the country is not
always extensive, but usually the reverse,—more or less limited in area, varying in
range, direction, and force. It would be tedious to advert to some of even the most
devastating tempests in much detail, therefore I propose to take three only as types,
and glance summarily over their most marked features, hoping that the diagrams
suspended around or lying on the table will supply enough additional facts. The
first storm to which I would ask attention in passing is that so well and so fully
described by De Foe, in 1703. He calls it (page 11) ‘‘ the greatest, the longest in
duration, the widest in extent of all the tempests and storms that history gives any
account of since the beginning of time... . . Our barometers,” he continues, “ in-
formed us that the night would be very tempestuous; the mercury sank lower than
ever I had observed it on any occasion” (page 25) ; it fell to 28°47 (page 30). This
storm began at south and veered through the west towards north, round to the scuth,
and then continued between south-west and north-west, with more or less strength,
for a whole week! Very remarkable it is that not only did De Foe suppose this
storm began near the southern coast of North America, but that it traversed England,
France, and the Baltic, to lose itself in the Arctic regions. He recurs afterwards
to its shifting from south-west to north-west, and coming from the west like other
storms in the south of England, but does not advert to any corresponding north-
easterly wind, nor had he evidently any idea of a rotatory or circulating atmospheric
current. Probably accounts from the north of England were much less attainable
then ; but it is noted that the north of England escaped the violence of that storm.
I cannot now take more from De Foe, but venture to say that his graphic accounts
of many storms, and the more comprehensive views of Dampier, are well worth the
notice of even scientific meteorologists. To Franklin, Capper, Redfield, Reid, and
Dove, besides other authorities, seamen may well be grateful; for their works, and
those compiled from them, are facts and inferences at present trusted because demon-
strated to be indisputably true.
It is now necessary that other storms should be noticed, and in a much more
precise manner ; but two alone will probably suffice as types. The ‘Royal Charter’
gale, so recent in our recollection, so remarkable in its features, and so complete in its
illustrations, I may say, from the fact of its having been noted at so many parts of
our coast, and because the storm passed over the middle of the country, is one of
the easiest to deal with which has occurred for some length of time. I would
therefore ask for a few minutes’ attention to this particular instance. There are
four diagrams among those on the wall which refer particularly to the 25th and the
40 REPORT—1860.
26th of October last. Referring to the charts and the diagrams, it will be seen that
the lowest barometer and a corresponding or simultaneous /ull prevailed over ten,
fifteen, or twenty miles successively in the direction I have pointed out. But at the
time that this comparative lull existed, there was around this central space what by
some is called a vortex, but can hardly be appropriately termed a vortex, because
there was no central disturbance : there were only variable winds or calm for a short
time in the middle of this space, which was about ten or fifteen miles across. ‘The
wind obtained a maximum velocity of from sixty to one hundred miles an hour, ata
distance of twenty to fifty miles from this comparatively quiet space, and in suc-
cessive meteoric eddyings crossed England towards the north-north-east, the wind
blowing from all points of the compass around the lull, so that while at Anglesea
the storm came from the north-north-east, in the Straits of Dover it was from the
south-west; on the east coast it was easterly ; in the Irish Channel it was northerly,
and on the coast of Ireland it was from the north-west. The charts show that there
was a similar circulation, or cyclonic commotion, going or passing northwards from
the 25th to the 27th, being two complete days from the time of its first appearance
in (what is called) ‘the chops of the Channel,” while outside of this circulation the
wind became less and less violent; and it is very remarkable that, even so near
as on the west coast of Ireland, they had fine weather, with light winds, while in the
British Channel it blew a northerly and westerly gale. At Galway and at Limerick
on that occasion there were light winds only, I repeat, while over England the wind
was passing in a tempest, blowing from all parts of the compass around a central
similar “lull.’”’ The next storm that occurred was similar in its features, though it
came from aslightly different direction. This storm was on the Ist and 2nd of No-
vember, and its character was in all respects like that just described, now usually
called the “Charter Gale.’? It came more from the westward, passed across the
north of Ireland, the Isle of Man, the north of England, and then went off across
the North Sea towards Denmark. Further than that distance facts have not yet
been gathered; but, no doubt, in the course of a few months they will be.
The general effect of these storms fell unequally on our islands, and less inland than
on the coasts. Lord Wrottesley has shown, by the observations made at his Observa-
tory in Staffordshire, that the wind is diminished or checked by its passages over
land; and looking to the mountain ranges of Wales and Scotland, rising 2000, 3000,
or 4000 feet above the level of the sea, we see they must have great power to alter the
direction, and probably the velocity of wind, independently of the alterations caused
by the changes of temperature. The very remarkable similarities of this storm of the
1st and 2nd of November and that of the 25th and 26th of October, the series of storms
investigated by Dr. Lloyd during ten years, and the investigations of Mr. William
Stevenson in Berwickshire, require especial notice on this occasion. There is no
discrepancy between the results of the ten years’ investigations published by Dr. Lloyd
in the Transactions of the Irish Academy, the three years’ investigations published
by Mr. W. Stevenson, and all the investigations which have been brought together
during the last four years. They all tell the same story. Dr. Lloyd only found in
ten years one instance even of a partial storm which differed; namely, one storm
that came from the north in the first instance. Storms from the south-west are
followed by sudden and dangerous storms from the north and east ; and these storms
from the north and east do much damage on our coasts. Upon tracing the facts, it
is proved that the storms which come from the west and south come on gradually,
but that storms from the north and east begin suddenly, and often with extraordinary
force. The barometer, with these north-eastern storms, does not give so much warn-
ing upon this coast, because it ranges higher than with the wind from the opposite
quarter. But though the barometer does not give much indication of a north-east
storm, the thermometer does; and the known average temperature of every week in
the year affords the means at once, from the temperature being much above or below
the mean of the time of the year, of showing whether the wind will be northerly or
southerly (thanks to Mr. Glaisher’s Greenwich observations).
Now to revert to a few of the signs which preceded the ‘Charter gale.’ Fora
few days before that storm came on, the thermometer was exceedingly low in a
great part of the country; there were north winds in some places, and a good deal
of snow; but nothing else extraordinary. There had been a great deal of exceed-
ingly dry and hot weather previously. These facts, of course, require consider-
TRANSACTIONS OF THE SECTIONS. 41
ation, but not now. I may just mention, that over our islands, and especially in
the north of Ireland, at that time, on the 22nd and 23rd of October, barometers
were very low. Many days preceding the ‘Charter storm,’ an extraordinary clear-
ness in the atmosphere was noticed in the north of Ireland—the mountains of
Scotland were never seen so prominently as they were in the few days preceding
those on which the great storm took place. Every one is aware that last summer
was remarkable for its warmth: it was exceedingly dry and hot. All over the
world, not only in the Arctic, but in the Antarctic regions, in Australia, South
America, in the West Indies, Bermudas, and elsewhere, auroras and meteors were
more or less prevalent, and they were more remarkable in their features and appear-
ances than had been noticed for many years. There was also an extraordinary dis-
turbance of the current along the telegraph wires. They were so disturbed at times,
that it was evident there were great electric or magnetic storms in the atmosphere
which could be traced to no apparent cause. Lord Wrottesley, in his Address, adverted
to some extraordinary facts respecting various circulating substances apparently
absorbed by the sun. Perhaps these electric disturbances were connected with the
peculiar action of the sun upon our atmosphere. Electrical wires above ground, as
well as submarine wires, were unusually disturbed, and these disturbances were
followed within two or three days hy great commotions in the atmosphere, or by
some remarkable change.
I will now refer to another subject—the question of areas or lines of barometric
pressure. Professor Espy, of the United States, contends for a long line from north
to south, or from one direction straight to another, and not only Espy but also
some among our own countrymen. The principal object of making these sections,
as it were soundings, of the atmosphere, shown in the diagrams, was to prove
whether lines of pressure, or whether areas of pressure prevailed; and I think,
when they are all closely looked into, they go to prove that while the atmosphere
in the British islands varied in its pressure from time to time, such variation was
not on a particular line, but extended over a large area. Before I leave this part of
the subject, I may say, as some of the remarkable exceptions to the force of these
particular storms, that at some places there was little or no wind; the barometer
fell much, but there was no storm, for the wind circulating around these districts
did not affect them, while at other places the storm was tremendous. It has been
often asked whether the ship that was lost—the ‘ Royal Charter ’"—might have been
saved ; and I will give an instance of what another ship did which took ordinary pre-
cautions on that night. Whether the ‘ Royal Charter’ did take the right course it
is not for me to say, but I hold in my hand the details of another kind of manage-
ment within ten miles of the ‘ Royal Charter’ that night. The commander of this
vessel, a sailing-ship and not a steam-ship (the ‘Royal Charter’ had the double advan-
tage), was guided by the instructions laid down by Capt. Maury, who has treated
the subject of winds in a practical manner, and has brought together a large amount
of useful information; and although, as I am aware, he occasionally theorises when
he has not facts enough for philosophy, as a practical man he has been guided by
plain principles, intelligible to seamen generally. Unquestionably, Maury has
brought together a great deal of valuable information, and made it generally avail-
able. The following paper has come into my hands within the last few days very
opportunely :-—
_ “ Having had many threatenings of bad weather for several days past, I began to
apply your views as to storms; and not having much sea-room, I considered them
more closely. For three or four days before the 26th of October, we had very
squally weather, with frequent sharp flashes of lightning from east to north-east.
During the night of the 24th, I stood to the northward, and till noon of the 25th,
with the wind strong from east-north-east. At noon I tacked, thinking that if the
gale should come on, I might take the off-shore tack in the night, and have the
vortex of the gale to the south-eastward. I stood on, therefore, till half-past five p.m.,
and then wore ship under short sail, when ina line with Holyhead and Bardsey,
about ten miles or so distant from Holyhead, as near as I could judge, being thick
and dark. At eight p.m., gale increasing, I took in close-reefed main topsail, and
fore topmast stay-sail, having nothing then set but the main spencer and a small
storm-mizen. It blew a complete West-India hurricane, but I drove off-shore, and
I thought the force of the storm did not increase. I now think, from what other
42 REPORT—1860.
ships suffered which were to the northward of me at the same time, that further
from me it blew harder. I did not suffer any damage whatever more than usual in
ordinary blows; only a little chafe and some spray. The lightning alluded to above
was very unnatural in its appearance, being of such a sharp flashing glare, without
leaving off. Unless looking at the exact place of its flash, you could not tell from
where the light actually came.
(Signed) ‘‘ Witur1am J. Jouns, Commanding the Ship.’?
** William Cumming, U.S.”
These two instances are important; one of a ship managed in accordance with
instructions published for seamen, being saved, while the other, which adopted a
different course, was lost. ‘There is one special instance on which not only private
but public interests were at stake, and where the ship to which I allude was seriously
injured. There wasone of Her Majesty’s ships, a 90-gun ship, fitted up with steam-
engine and other appliances, in the Atlantic, in the early part of October last. That
ship had very bad weather near the edge of the Gulf-stream. A succession of circling
storms occurred, and in every instance the ship was managed in direct opposition
to the known laws of storms, was considerably damaged, and obliged to return.
Now, that is a fact which ought not to have occurred in the British Navy at the
present day. It might have been that there was some reason for such usually in-
correct proceeding in one instance; but that there should have been any reason in
three successive instances is more than we can conceive: any one can estimate the
amount vf expense caused by a ship so brought back to England from her destination,
The simple rule of seamanship is when facing the wind the centre of the storm will be to
the right or on the right hand, therefore you should go to the left. In the southern
hemisphere the centre is on the left hand, and you must go to the right. supposing
that sea-room and circumstances enable you to choose. But these simple results
are the consequence of very great consideration on the part of scientific persons,—
particularly Sir W. Reid, Redfield, Capper, Espy, Dr. Lloyd, and others,—especially
those in India, who have done so much, viz. Piddington and Thom. In this
country no one has effected more than Sir W. Reid, who collected together all that
had been done for many years, and published in a clear manner the results of his
accumulated investigations. A very remarkable storm has been lately traced by
Mr. Rowell, of Oxford, and his description published within the last few days. This
storm occurred near Calne in Wiltshire, cutting through fields and trees, and in one
place actually lifted a broad-wheeled waggon from the road over a hedge into the neat
field! The violence of the wind was confined to a limited line. The downward and
onward pressure of the wind was so great in that locality, that it acquired such
elasticity as to lift opposing weights and carry them on. I have known such things
myself. I have known the wind lift a boat into the air and shake it to pieces. We
have all heard of houses being unroofed, of trees torn up by the force of the wind ;
but this is the first time I have heard of a heavy waggon being lifted up and hurled
over a hedge.
I will only venture to make one or two observations in reference to the theory
of these subjects. Dove, in his work, shows how currents of wind, parallel cur-
rents, as he calls them, co-exist. A great polar current coming from the north
and east is passing in one direction, while a current from the tropical regions is
going in the other direction, nearly opposite; but to follow the theoretical consider-
ations of how these great currents move from the Arctic regions towards the tropics
and return to the Arctic regions, is a subject too large for the present limited time.
Dove has shown most clearly in his work (which is translated into English), that
circulation of the atmosphere in great polar and equatorial or tropical currents, pre-
vail not only in our hemisphere, but everywhere. I can bear witness that his
reasonings and particular views can be corroborated in every part of the world.
The British Association has made application to Her Majesty’s Government to
authorize arrangements for communicating warning of storms from one part of the
country to the other; and, in conclusion, I will read the details of that arrange-
ment which promises to he so beneficial. Arrangements have been authorized
by the Board of Trade (under a minute from the President, dated June 6), in conse-
quence of which a daily and mutual interchange of certain limited meteorological
information will be transmitted between London and Paris, the results of five
——
TRANSACTIONS OF THE SECTIONS. 43
subsidiary communications to the central stations of Paris and London. Authority
being thus given to collect and communicate, by the telegraph, particular meteoro-
logical intelligence, a commencement may be made on the Ist of September, as the
plan proposed is simple, and the machinery is ready. Once a day, at about nine
A.M., barometer and thermometer heights, state of weather, and direction of wind
will be telegraphed to London, from the most distant ends of our longest wires,—
namely, Aberdeen, Berwick, Hull, Yarmouth, Dover, Portsmouth, Jersey, Plymouth,
Penzance, Cork, Galway, Londonderry, and Greenock. Facts sent thus from five of
these places, will be put into one telegram, and sent to Paris immediately, when a
corresponding communication will be made from the southward Atlantic coasts.
When threatening signs are not apparent, no further notice will be transmitted to
or from London on taat day, respecting weather. But when indications are such
as to warrant some cautionary signal at a certain part of, or along all our coasts,
the words ‘‘ Caution,—North” (or ‘‘South’’) will be sent to some of the thirteen
places specified, or to all of them, on the receipt of which a cone (or triangle) will
be hoisted at a staff (point up for north, down for south), indicating the side whence
wind may be expected. ‘This signal will be repeated along part of the coast by the
Coast Guard, at such of their stations as may be authorized (at most of their stations
flagstaffs are visible to coasters). Danger will be implied by a drum (or square), a
cone, and perhaps, in addition, very great danger by a cone, a drum, and a second
cone. [Thecones and drums may be made with hoops and black canvas, to collapse,
without top or bottom. They will be the same in shape from all points of view,
and unlike any other signal, such as a time-ball, used ordinarily.] As the Coast
Guard extends all along the frequented parts of our shores, and as the telegraph
companies are liberally willing to have instruments and signals placed at their ex-
treme stations, in charge of and used by their officials, only the necessary materials
and instructions will be required, all of which are ready or in progress. By vigilance
at the central station, and by taking great care to avoid signalling too frequently,
much may be done towards diminishing the losses of life on our increasingly crowded
coasts. Property alone may be duly insured, but every wise precaution for the safety
of life should, of course, be used. As an auxiliary measure, a concise Manual of
Instructions for the Barometer will be circulated among maritime communities ;
who, though they may have frequent access to ‘‘ weather-glasses ” of various kinds,
do not generally know how to use them most advantageously. The following details
may be useful, as well as interesting, to those who wish to investigate these subjects
and examine the diagrams more critically :—The probable limits of error of the
barometric curves on the synoptic sheets, 21st of October —2nd of November 1859.
The observations at the regular observatories, such as Greenwich, Oxford, Cam-
bridge, Highfield House, Kew, &c., have had all corrections applied, and have been
reduced to sea-level, and the temperature of 32°. The returns from members of the
British and Scottish Meteorological Societies (nearly ninety in number) have nearly
all been corrected for the exact height above sea-level, all within a few feet. The
corrections due to instrumental errors and reduction to 32° have (in most cases I
believe) been applied by the observers. The Continental observations have been
collected partly from the Dutch papers and partly from the ‘ Moniteur.’ Those from
the former have been reduced to 32°, and, it may be presumed, have also beet cor-
rected for instrumental errors. The heights of some stations are known ; the cor-
rections due to those heights have been applied, and others are known to be little, if
at all, above the sea-level. Any error in laying down a curve from such data can
scaicely exceed two or three hundredths of an inch. The observations obtained
from the ‘ Moniteur’ itis assumed are givendulycorrected. The heightsot the stations
of ordinary observers are known for the most part pretty nearly, and corrections for
such heights have been applied to the returns. Other corrections have only been
applied in a few cases—observations sometimes recorded only to the nearest tenth, not
being deemed worthy of any further correction. Those returns, however, of which
the barometrical observations are evidently erroneous (from comparison with other
more reliable neighbouring and contemporaneous obsevations), have been rejected
altogether. On the whole, we may safely assume that even these observations,
as laid down, are less than a tenth inerror. The heights of the lantern above the
sea-level and of the tower, from the base to the vane, being known, the probable
height of the barometer can be ascertained, The proper correction for the height
44 REPORT—1860.
thus estimated has been applied, and all returns suspected of being erroneous
rejected.
On the Similarity of the Lunar Curves of Minimum Temperature at Green-
wich and Utrecht in the Year 1859. By J. Park Harrison, M.A.
The author showed that, on the mean of twelve lunations, in 1859 the greatest
amount of cold displayed itself at both the above-named stations between full and
new moon: the difference between the mean minimum temperatures of the first and
second halves of the lunation at Greenwich being 2°°4; at Utrecht 2°°0. There were
two minima for night temperature both at Greenwich and Utrecht; they followed on
full moon and last quarter. The least amount of cold was at first quarter. The
difference between the minimum temperatures at first quarter and shortly after last
quarter, on a mean of twelve observations taken at both stations, was nearly 7°. The
difference in the means of the mean temperature of the day for forty-three years for
the two periods of fourteen days, at the former place had been previously found to
be 1° 1.
Mr. Harrison expressed increased conviction that effects so contrary to expectation
must be due to the presence or absence of cloud, or to its height above the earth,—
to whatever cause this phenomenon may ultimately be assigned.
On the Principles of Meteorology. By Professor Hennessy, F.R.S.
The author contended that the principal object of meteorology was the prediction of
the weather within certain probable limits. The great complication of atmospherical
phenomena, and the influence of remote causes of disturbance, would undoubtedly
render this extremely difficult. Although the atmosphere is itself one of the best
examples of an unorganized body to which we could refer, yet its complicated and
fluctuating phenomena suggest to us the mode in which such phenomena should be
investigated. Any success could be expected only by treating the atmosphere very
nearly as an organized body, and studying its abnormal conditions with the same
continuity and generality of observation as is usually employed in physiology. Ob-
servations made at stated hours have been found by themselves rarely capable of
affording means to foretell the future conditions of the weather for even short
periods of time. A careful study of the appearances of the sky, such as has been
so long familiar to mariners and others interested in the conditions of our atmo-
sphere, would, when made by men well prepared with preliminary knowledge of
the principles of physical science, throw far more light upon the chief object of our
search. Mr. Hennessy illustrated this remark by referring to some such observations
which he had made during the month of June. Although he had at first consi-
derable scepticism as to the possibility of obtaining correct results from the continuous
photographical registration of atmospherical conditions, Mr. Hennessy was satisfied,
from what he had witnessed during 1856 in the Radcliffe Observatory, that such a
system was not only possible, but that it sometimes disclosed important changes
which would have escaped the method of observation at stated hours. He instanced
the connexion between the phenomena of thunder-storms and sudden barometric
depressions, as pointed out by the late Radcliffe Observer at the Glasgow Meeting,
and the connexion between days of great solar irradiation and minute vertical
atmospheric currents, as pointed out by himself*. He concluded by pointing out
the manner in which, from the increasing knowledge we possess of the influence of
the ocean upon climate, the greater stability of its currents, compared to those of the
atmosphere, may under the peculiar conditions of the British islands enable us to
foresee many important changes within comparatively extended periods of timef.
On Antarctic Expeditions. By Captain Maury, U.S. Navy.
Observatory, Washington, 20th May, 1860.
My pear Lorp Wrorrestry,—I hope the time is not far distant when circum-
stances will be more auspicious than at present they seem; for, as soon as there appears
* Report for 1858, Trans. Sect. p. 36.
+ Report for 1859, Trans. Sect. p. 50. Proceedings of the Royal Society, vol. ix, p, 324.
Atlantis, yol. i. p. 396. Philosophical Magazine, April 1846, and October 1858, ;
—
TRANSACTIONS OF THE SECTIONS. 45
the least chance of success, I shall urge the sending from this country an exploring
expedition to the eight millions of unknown square miles about the South Pole. I
hope that my letter to you upon the subject was sufficiently clear to satisfy your
mind, and conclusive to enlist your influence with Her Majesty’s Government and
the English people in the cause of Antarctic exploration. It is an enterprise in which
the British nation may well take the lead, for it is nearer to them than to the rest of the
world. There is Melbourne, your great commercial mart, that is already, in amount
of shipping, a rival of Liverpool. It is within less than two weeks’ run by steamer
from the borders of this unknown region. So, you observe that these eight millions
of unknown square miles lie at your door, and the responsibility of permitting them
so to lie longer will lie there too, ‘You go; we'll come.” An expedition might
be sent from Australia with little or no risk. Two propellers, or even two vessels
with auxiliary steam-power, might be sent out, so as to spend our three winter
months in looking for a suitable point along the Antarctic Continent to serve as a
point of departure for over-land, or over-ice parties. Having found one or more
such places, vessels, properly equipped for land and ice and boat expeditions, might
be sent the next season, there to remain, seeking to penetrate the barrier, whether
of mountain or of ice, or both, until the next season, when they might be relieved by
a fresh party, or return home to compare notes, and be governed accordingly. You
know the barometer at all those places which have a rainy and a dry season, stands
highest in the dry, lowest in the wet. Now, I do not find any indications that the
Antarctic barometer has months of high range: it is low all the year. Therefore—
if | be right in ascribing the apparent tenuity of the air there to the heat that is
liberated during the condensation of vapour, from the heavy precipitation that is con-
stantly taking place along the sea front of those “ barriers ””—we should be correct
in inferring that the difference in temperature between the Antarctic summer and
winter is not very marked. If, in a case like this, we might be permitted to indulge
the imagination, we might fancy the “‘ barrier” to be a circular range of mountains,
and that beyond these lies the great Antarctic basin. Beyond this range, as beyond
the Andes, we may fancy a rainless region, as in Peru,—a region of clear skies and
mild climates. Though the air in passing this range might be reduced below the
utmost degree of Arctic cold, yet being robbed of its vapour, it would receive as
sensible the latent heat thereof. Passing off to the Polar slope of these mountains,
this air then would be dry air; descending into the valleys, and coming under the
barometric pressure at the surface, it would be warm air. Leslie has explained how,
by bringing the attenuated air down from the snow-line, even of the tropics,-and
subjecting it to the barometric weight of the superincumbent mass, we may raise its
temperature to intertropical heat by the mere pressure. In like manner, this Ant-
arctic air, though cold and rare while crossing the “ barrier,” yet receiving heat
from its vapours as they are condensed, passing over into the valleys beyond, and
being again subjected to normal pressure, may become warm. We have abundant
illustrations of the modifying influences upon climate which winds exercise after
having passed mountains and precipitated their vapour. The winds which drop the
waters of the Columbia river, &c. on the western slopes of the Rocky Mountains,
make a warm climate about their base on this side, so much so that we find in Pied-
mont Nebraska the lizards and reptiles of Northern Texas. Indeed, trappers tell me
that the Upper Missouri is open in fall long after the Lower is frozen up, and in
spring long before—several weeks—the ice in the more southern parts has broken
up. The eastern slopes of Patagonia afford even a more striking illustration of
climates being tempered by winds that descend from the mountains, bearing with them
the heat that their vapour has set free. Thus you observe, that an exploring party
after passing the barrier might, as they approach the pole, find the Antarctic climate
to grow milder instead of colder. It would be rash in the present state of our in-
formation to assert that such is the case ; but that such may be the case should not
be ignored by the projectors and leaders of any new expedition to those regions,
The existence of an open seain the Arctic ocean has, with a great degree of proba-
bility, been theoretically established. But the circumstances, as strong as they are,
which favour the existence of an open water there, are not so strong and direct as
are the proofs and indications of a mild polar climate in the Antarctic regions. I
have examined the immense library of log-books here for the lines of Antarctic ice-
46 REPORT—1860.
drift. There appear to be two, both setting to the north-east, one passing by the
Falkland Islands, the other having its northern terminus in the regions about the
Cape of Good Hope. Further south, icebergs are found all around; but in these
lines of drift they are found nearest the equator. The space between the Falkland
drift and the Good Hope drift is an unfrequented part of the ocean. It may there-
fore be one broad drift, the edges of which only I have pointed out, The most active
currents from the south do not run with this ice. Humboldt’s current is the most
active, but it does not get its icebergs as far north as they come by these lines.
This circumstance has suggested the conjecture that one part of the Antarctic Con-
tinent must be peculiarly well situated for the formation of glaciers and the launching
of icebergs. These lines of drift point to such a place. The facts stated in my
former letter will, I trust, when considered in connexion with these views, impress
you with the importance of the subject. So, trusting, and hoping that you will join
with me in the cry, ‘ Ho for the South Pole!”
On the Climates of the Antarctic Regions, as indicated by Observations upon
the Height of the Barometer and Direction of the Winds at Sea. By
Captain Maury, U.S. Navy.
In the course of my labours connected with the wind and current charts, I had
caused to be grouped 1,213,933 observations upon the direction of the wind at sea.
Each one of these observations embraces a period «of eight hours, and aims to give
the prevailing direction of the wind during that time. Thus each individual of my
group is, in fact, itself the mean of many. ‘The result of the whole is presented
diazrametrically in Plate I., in which the mean direction of the wind in each belt,
and for the four quarters, is represented by the arrows correctly, both as to mean
direction and average duration.
From the labours of Lieut. Andrau and his colleagues at the Meteorological In-
stitute of the Netherlands *, I obtained 83,332 observations upon the barometer be-
tween the parallels of 50° N, and 36° S, at sea. This fine series was enriched by the
observations at Greenwich, St. Petersburg, and Hobart Town on shore, and by Dr.
Kane, Sir James Clark Ross, and Lieut. Wilkes at sea, du:ing their Arctic and Ant-
arctic explorations. From these the barometric profile of the atmosphere (Plate I.)
was constructed.
The barometric observations on shore were not found in all cases to accord with
those at sea. Moreover, those of Wilkes and Ross were the means of observations
for only a few days.
Our ‘ Marine Magazine,’ as the precious store of abstract logs may be called, con-
tained many more, and which, by their great numbers, and in consequence of their
having been made at all seasons of the year, would afford better mean results. In
extension of Andrau’s series, I therefore added 6915, between the parallels of 40°
and 60° south, from the log-books of this office. These, Andrau’s, and Dr. Kane’s
in the ice, form the elements of the Barometric Curve, Plate II.
Proceeding upon the supposition that, with regard to the general movements and
the mean status of the atmosphere, we should have at sea the rule, on land the ex-
ceptions, I commenced to group these observations for discussion.
As the North Indian Ocean, the China and West India seas, where the monsoons
blow, are known to present exceptional cases to the general movements of the winds
at sea, the observations for them were excluded from the general summing up.
Thus premising, the winds were taken from the pilot charts and grouped in belts
5° of latitude broad. As a rule, the vessels that are cooperating with us seldom go
on the Polar side of 60° north or south; for our fleet of observers consists for the
most part of merchantmen, whom the channels of trade do not carry beyond these
parallels; consequently the observations of the winds were arranged in 24 belts
(12 on each side of the Equator) ; all the observations between the Equator and
5° north, for example, being in one belt; and so on for every 5° of latitude.
Now, considering that the general movements of the atmosphere, as exhibited by
* Maandelijksche Zeilaanwijzingen van Java naar Het Kanaal. Als Uitkomsten Weten-
schap en Ervaring Aangaande Winden en zeestroomingen in sommige Gedeelten van den
Oceaan Uitgegeven Dour Het Koninklijk Nederlandsch Meteorologische Instituut. Utrecht,
1859.
TRANSACTIONS OF THE SECTIONS. 47
the winds at sea, are to and fro between the Equator and the Poles, all these obser-
vations were arranged in two groups for each belt, and classed either as winds with
northing, or as winds with southing, in them, as per Table, showing the average
annual duration in days of winds.
Winds with Northing, and Winds with Southing in them.
Northern Hemisphere. Southern Hemisphere.
Belts. No. of | Northing. | Southing. | Excess in days. || No, of | Northing. | Southing. | Excess in days.
observa-|——— |__| ——__—_— ] obs erva-, ——__, —_______}—_______—_
tions. Days, Days, North. | South. || tions. Days. Days. | North. | South.
Between
0° & 5° | 67,829 79 268 w= | 189° || 72,945 83 269 .. | 186
5&10 | 36,841 158 183 stele 25 || 54,648 72 283 Pregclten |
10 & 15 | 27,339) 278 73 | 205 43,817 82 275 Sep 193
15 & 20 | 33,103} 273 9] 182 46,604 9] 266 aoe 175
20 & 25 |44,527| 246 106 | 140 66,395} 128 227 ve 99
25 & 30 | 68,777) 185 163 22 66,635 147 208 rae 61
30 &35 | 62,514) 155 195 “ah 40 || 76,254; 150 204 ies 54
35 & 40 | 41,233) 173 179 a 6 107231) 178 178 0 0
40 & 45 | 33,252) 163 186 oe 23 || 63,669) 202 155 47
45 & 50 | 29,461 164 189 aaa 25 || 29,132) 209 148 61
50 &55 |41,570) 148 203 oas 55 || 14,286) 208 151 57
55 & 60 [17,874 142 213 308 71 =|13,617} 224 132 92
6 Ey SPLIT LE AE eS
{t thus appears that we have, as we already well knew, in each hemisphere a
medial belt—a barometric ridge in the air—from which the prevailing direction of the
wind on one side is towards the Equator, and from the other towards the Pole. In
the southern hemisphere this ridge is sharp, being included between the parallels of
35° and 40°; in the northern hemisphere, however, it seems to be less sharply de-
fined, for the debateable ground, or helt, within which neither wind appears to have
a very marked ascendency as to prevalence, extends from lat. 25° to 50° N.
Proceeding from these belts towards the Equator, equatorial-bound winds become
more and more prevalent ; or if we proceed towards the Pole, the polar-bound winds
become more and more prevalent, — thus indicating the existence both near the
Equator and in the polar regions of a permanent degree of aérial rarefaction suf-
ficient to produce an indraught from a medial line or belt towards each.
To ascertain the degree of rarefaction about the Poles, as far as the observations on
the barometer at sea would indicate a result, the Barometric Curve (Plate Il.) was
constructed from the data expressed in this Table, showing
The Mean Height of the Barometer.
No. of ob-|/ ratitude. |Barometer,| No- of ob-
servations,|| servations.
a
Oto 5N/ 29-915 | 5114 || Oto $s.| 29-940 | 3692
5 to 10 ,,| 29922 | 5343 || 5to10,,| 29-981 | 3924
10 to 15 ,,| 29964 | 4496 ||10t015 ,| 30-028 | 4156
15 to 20 ,,| 30-018 | 3592 ||15 to 20 ,.| 30060 | 4248
20 to 25 ,,| 30081 | 3816 |/20 to 25 ,,/ 30-102 | 4536
25 to 30 ,,| 30149 | 4392 || 25 to 30 .,| 30.095 | 4780
30 to 35 ,,| 30-210 | 4989 ||30to 36 .,| 30052 | 6970
35 to 40 ,,| 30124 | 5103 || 40 to 43 || 29-88 1703
40 to 45 ,,| 30-077 | 5899 || 43 to 45 || 29-78 1130
45 to 50 ,,| 30060 | 8282 || 45 to 48 ,,| 29°63 1174
78° 37’ ,,| 29:759 |Dr. Kanel| 48 to 50 ,,| 29°62 672
50 to 53 ,,| 29-48 665
53 to 55 ,,| 29°36 475
563 ,,| 29:29 1126
| Latitude. (Barometer.
It would seem from this curve, which by its regularity shows the observations at
48 REPORT—1860.
sea to be remarkably accordant, that the atmosphere is much more attenuated in
austral than in boreal regions; and that the high barometer, with the light airs
and baffling winds of the tropical calm belts, is the dividing atmospherical ridge, so
to speak, between the low barometer about the Pole on one side and near the Equator
on the other; and that the position of this ridge is determined by the degree of
polar in contrast with the degree of equatorial rarefaction. The trade-winds rushing
in on one side, and the counter trades on the other—as the polar-bound winds may
be called—supply the indraught for these places of attenuated air and low baro-
meter.
It thus appears that the equatorial calm belt is a sort of thermal adjustment be-
tween the calms of Cancer and Capricorn; which in turn are in adjustment to the
dynamical power of the ascending columns of air in the equatorial and polar calm
laces.
The low barometer off Cape Horn has long attracted the attention of navigators.
The low barometer in other longitudes south caused Wilkes, Ross, and others, to
remark upon the diminished pressure in high southern latitudes, and upon the ap-
parent inequality in the distribution of the atmosphere north and south of the
Equator.
The barometric observations between 40° and- 60° South, and which are quoted
in the preceding Table, were collected in three groups—first, from the logs between
the Cape of Good Hope and Australia, next from Australia to 80° West, and then
about Cape Horn. The result showed that a low barometer is not peculiar to Cape
Horn regions, but that it is general and circumferential in austral latitudes, dimi-
nishing rapidly as we approach the Pole.
The great extent of the austral water surface, with the vapour with which it
keeps the “ brave west winds” of these regions loaded, and the heat which with the
condensation of these vapours is liberated there, suggests the cause of this low
barometer.
If it be the vapour and the liberation of its latent heat that cause the permanent
expulsion from Antarctic regions of so much of the atmosphere as this curve and
these observations indicate, then should we not follow the argument up, and infer
that the extreme cold of the Antarctic climate is by no means so seyere as that of the
north?
The unexplored regions of the south embrace an area of more than eight million
square miles, or about one-sixth of the whole extent of the dry land surface that is
contained on our planet.
Since the attempts to penetrate those unknown regions, steam has been intro-
duced upon the ocean, and the modern explorer has at his command a power which
enables him to defy wind and tide. Hygiene on board ship has been so improved,
that the sailor may now keep the sea for almost an indefinite period of time. The
invention, the discoveries, and the improvements of the age, place in our hands the
means of fitting out Antarctic expeditions, and of endowing them with powers that
would have made any previous expedition there doubly effective.
Under these circumstances, would it not be areproach upon the Christian nations,
and especially upon those great governments who have agreed to unite ina common
plan of physical research at sea, if so large a portion of the earth’s surface were
permitted to remain unexplored ?
Plate III. shows the furthest reach of Antarctic exploration. The tracks of Ant-
arctic explorers, from Cook down to the present day, go to make up these limits.
It is not the object of this paper to elaborate the views suggested by the observations
offered with this paper; but rather to present the observations themselves, with
such explanation as seemed necessary to enable others to understand them.
If I have succeeded in doing this, all who will take the trouble to study them will
find them very suggestive. M. F. Maury.
Observatory, Washington, 11th May, 1860.
On the Cause of the Descent of Glaciers. By the Rev. Henry Mose tey,
F-.R.S., Canon of Bristol, Inst. Imp. Se. Paris Corresp.
The fact of the descent of a body, when placed upon an inclined plane, due to the
Plate 1.
1 : 420 inch —1 month
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3.
OG
TRANSACTIONS OF THE SECTIONS. 49
variations in its temperature, first observed in the descent of the lead which covers
the south side of the choir of Bristol Cathedral, and communicated by me to the
Royal Society in the year 1855, I have since confirmed by the following experi-
ment. I fixed a deal board, 9 feet long and 5 inches broad, to the south side of my
house, so as to form an inclined plane, and upon it placed a sheet of lead, turning
its edges down over the edges of the board, and taking care that it should not bind
upon it, but be free to move with no other obstruction than that which arose from
its friction. The inclination of the board was 18° 32’, the thickness of the lead was
one-eighth of an inch, and its weight 28 lbs. The lower end of the board was
brought opposite to an upper window, and a “ vernier’’ was constructed which
could be read from within, and by which the position of the lead upon the board
could be determined to the 100th of aninch. I began to measure the descent of the
lead on the 16th of February, 1858, and recorded it every morning between seven
and eight o’clock, and every evening between six and seven until the 28th of June.
The lead had descended between the 16th of February and the 30th of April (a
period of seventy-four days) 10°61 inches, being an average daily descent of °1433
inch. On the 4th of May it was drawn up the board again to its first position.
Between that date and the 28th of June (a period of fifty-five days) it had descended
11°97 inches, being an average daily descent of -2176 inch. Its descent was far
from uniform, being on some days scarcely (if at all) perceptible, and on others
amounting to nearly half aninch. The average daily descents in successive months
from February to June were in
inch.
ODRUALY (¢: &graiejs-e-eroleln's 10; thele.0\ i clale eisiaielefeyelsi sien “LOOOO
IVEAECH si avn, s\exaheieisre(sYeisiwioie, ele 'aloereaiciefeialre ini sen etF SOOG
SNSUILesracele sie cecelm inate elmtoisrshate tole slvisieterstots aieieteintesll Otley.
Rg dg arecayale Cues wcbsa a Genre clas “emia Soke es HEL
pUAATD Gis «quo bs alada Feb ated evale: oxaieyerairass rola! ale. aro: oftttasat abs tere to ea ee
Every variation in the temperature of the lead contributed to its descent. The
extreme temperatures of the day and the night could not therefore determine its
daily motion ; for with the same extremes of day and night temperature, there may
be great differences in the number and amount of the intervening variations of tem-
perature. It is the effect of these daily variations of temperature, up and down, by
which the descent of the lead totalizes. Although, therefore, we are to look for the
influence of the extremes of day and night temperature upon the daily descent, we
are also to look for that of the variations between each two extremes. I accordingly
remarked that it was on days when a thermometer in the sun varied its height
rapidly and often, that the lead descended most. On the contrary, when the sky
was open and the heat advanced and receded uniformly, the descent was less, although
the difference of the extreme temperatures might be greater. It was least of all
when there was continuous rain. During the night the descent of the lead was
often imperceptible. I have explained the descent of the lead in a paper published
in the ‘ Proceedings of the Royal Society’ for April 1855.
If we suppose the sheet of lead to become ice, and its dimensions to be incfeased
20,000 times, and if for the board on which it rests we substitute a mountain side lying
at a slope of 183°, we shall have a glacier 14 mile broad, 200 feet deep and 34 miles
long, and which in no other respect than as it regards its length will be an exaggera-
tion. By converting the lead into ice, its physical properties will, however, have been
in some important particulars changed. It will have become twice as dilatable as lead
is, that is, it will dilate twice as much by a given variation of temperature when un-
opposed as lead does*. It will have become a more elastic substance than lead is, that
is, it will be capable of overcoming a greater force opposed to its dilatation under a
given change of temperature. It will have lost its ductility and have become friable,
that is, its parts will have become more liable to separation from one another and
its mass to disintegration. But, together with the last-mentioned quality, it will
have acquired the property (called regelation) of easily, and under a moderate press-
ure, returning from a state of disintegration to one of solidity; which qualities of
* See the experiments of Schumacher at Pultowa, as detailed in the paper of W. Struve,
“ Sur la dilatation de la Glace,” Mém. de l’Académie de St. Pétersbourg, ser. 6. tom. iv. 1848.
1860. 4:
50 REPORT—1860.
friability and regelation have been shown by the experiments of Professor Tyndall
to be sufficient (the requisite force ‘‘a tergo’’ being supposed) to account for its
crushing its way through contractions in its channel, and reconstructing itself at the
bottom of ice-cataracts. Now such a glacier, if it be supposed penetrable to external
heat as lead is, could not but descend as lead does. In its descent portions of it
would be thrust forward and compressed, and others would be dragged behind and
crevassed. The melting of the lower part of such a glacier would favour its descent
as compared with the lead whose mass remains unchanged. All these conditions
might, however, be influenced by variations in the form of its channel and the incli-
nation of its bed. Its motion would be like that of a snail clinging, but descending.
The whole question, however, depends upon the penetrability of the glacier to
external heat. On this point we have the high authority of Professor Forbes,
founded on three series of observations on the motions of the Mer de Glace and the
Glaciers des Bossons and des Bois. Of these observations, made in the summers of
1842 and 1844, he has recorded the results in his ‘Travels in Savoy’ (2nd ed.
p. 141), and in his recent work entitled ‘On the Theory of Glaciers’ (p. 131) ; and
he has compared them with the mean daily temperatures of the air as recorded at
Geneva and the Great St. Bernard. He has, moreover, represented the relation
between the average daily motions of these glaciers, and the average daily tempera-
tures of the air at the corresponding periods by means of diagrams, which it is im-
possible to look at, however cursorily, without being struck with the fact (not to be
better expressed than in the words of Mr. Forbes himself), that they establish a
“close relation between the mean temperature of any portion of the year, and the
velocity of the glacier corresponding to it*.’’ Moreover, it is not only on the sur-
face of the glacier that this relation may be considered to have been observed. The
glacier moves with different velocities at different depths; but all are related to its
surface motion, so that the influence of variations of temperature, if felt on its sur-
face, must penetrate throughout its depth. Being dilatable as lead is (but in a
higher degree), and being thus shown to be sensible to variations of temperature
throughout its mass, it cannot but descend as lead under the like circumstances does.
Every variation of temperature, however slight, cannot but produce a corresponding
descent, and such small variations, often enough repeated, might produce a descent,
however great, even although at each change the glacier returned to the same tem-
perature. The oscillation of the heat backwards and forwards is all that is required.
For the purpose of this argument, the fact that a relation exists between the motion
of a glacier and the external temperature is all that is required. It is not necessary
to enter on a discussion of the causes out of which that relation arises.
On Meteorological Observations for 1859, made at Huggate, Yorkshire, East
hiding. By the Rev. T. Rankin.
This communication was in continuation of similar observations and general
remarks furnished, by the same author, to the Association for upwards of twenty
years. ;
On Thermo-barometers, compared with Barometers at great Heights.
By M. R. de ScuitacintWEIr.
M. Robert de Schlagintweit communicated some of the results which he had de-
duced from comparisons of the boiling-point with direct barometric readings. These
observations, taken by his brothers and himself during their journeys in India, the
Himalaya, &c., at various heights and different periods, were chiefly made to test by
direct experiments the correctness of the tables of the boiling-point of water corre-
sponding to barometric pressure, of which the latest and the most detailed ones are
those of Magnus, Regnault, and Moritz.
Direct observations had been previously made in India, particularly by Colonel
Sykes-; in America, Mr. Wisse made such experiments up to 14,000 feet; in High —
Asia, Messrs. de Schlagintweit had occasion to carry on such observations up to
heights exceeding 18,600 feet.
A resulting Table of comparison was presented, an examination of which showed
* Forbes, Theory of Glaciers, p. 130.
3
7
TRANSACTIONS OF THE SECTIONS, 51
that, for all practical purposes, the tables quoted above are quite accurate enough,
though for great heights, they contain an error; the correction to be applied is
small, and additive. The instruments with which Messrs. de Schlagintweit made
their observations, were expressly made for the purpose; they ranged from 100° Cels.
to 78° Cels., but had a length of 1 foot 9 inches, so that it was possible to divide
each degree into fifty parts directly. M. de Schlagintweit drew attention to the
accuracy of the results obtainable by these delicate thermo-barometers, which, as
far as his experience goes, he considered to be quite comparable to the barometer, if
used with all the necessary precautions, though for daily variations the barometer
is preferable on account of the greater facility of reading. The circumstance that
the thermo-barometer is much less liable to get out of order, makes it a most valu-
able instrument for travellers.
Messrs. de Schlagintweit’s Comparison of Boiling-pomts.
Simultaneous baro-
metric readings.
Thermos! '
Name of the place of Wearand Dates barometer Millims. bd Fg
observation, readings, es reduced to C. degrees.
C. degrees. sah oiling |"
8 point,
C. degrees,
Group I.—100° to 96°: Correction —0°-09 of the Thermo-barometer*.
oO ° °
RAMU rete evisccnnr sce s TSG PAP Messen asa 97-99 7046 97:90 | —0:09
BORGEDDE NG ccs -cict eset is ozsnes 1855, Sept. 12 ......... 96°84 675°7 96-75 | —0:09
AARON Es racs 7a cers ve oes 1855, Sept. 12 ......... 96:73 6735 96:66 | —0:07
RORAMMACH 0... scec cee escere es 1855, Sept. 15 ......... 95°85 652°9 95:81 | —0-04
PORAMATD 50. sis sce ececaeces 1855, Sept. 16 ......... 95°85 651-7 95:76 | —0:09
Group II.—95:99 to 94: Correction — 0°10 of the Thermo-barometer.
EHOSIMALH .......csscersre- 1855, Sept. 9 iiveses-sn 94:06 610°4 93:99 | —0:07
BEMOUKESEL,......0.00050004- 1855, Sept.8 .......<-.-« 93:99 | 6082 | 93:39 | —010
MHOSIMAtH so... se... 1855, Sept. 9 ............ 93°98 607-0 93°84 | —0:14
Gaurikind) <3.6.6..6..c8is0s 1855, Sept. 24 ......... 93:78 | 6033 | 93°67 | —O-11
IGBNTIKUNA). S60. 05.s..ce.. 1855, Sept. 23 ......... 93:73 | 601-2 | 93:58 | —O-15
Garand .........06.00c00- 1855, Sept. 19 ......... 93°64 601:0 93°57 | —0:07
RUIUTALN Maio nis ceis's «a sis'eic'enels 1855, Sept. 29) .:.....-: 93:13 5873 92:95 | —0-18
BAM Abs aca ncdstshcsevosecens. 1856, April 12 ......... 93-00 585°7 92:88 | —0-12
Trichugi Narain............ 1855, Sept. 24 ......... 92:96 585-2 92°86 | —0:10
Group III.—93:99 to 92: Correction—0°11 of the Thermo-barometer.
IMIMASAUTA ......0650.000000- 1855, Sept. 28 ......... 90:76 | 537-9 | 9062 | —0-14
Badrinath ..........0s00000 1855, Sept. 7 ....ss00000 90:20 5275 90:10 | —0:10
PSBOTINAE « cass0 00 55<e0 ste. 1855, Sept. 5 ......0..05 90:18 526°6 90:06 | —0-12
PSAUTINALN 4... 20000200s00e ees 1855, Sept. 6 ...........- 90°12 5256 90:01 | —O11
Mangu Pass «............... 1855, Sept. 26 ......... 89°87 520-0 89:73 | —014
“UN Baghageiocssdancteasa-ade 1855, Aug. 28..........-. 89°85 519-1 89:69 | —0-16
Group IV.—91:99 to 90: Correction—0°'12 of the Thermo-barometer.
sdarnath ..2...sasreseeivs- 1855, Sept. 20 .. ...... 88°68 498°] 88:61 | —0:07
BEPOENALL ev cxddcvyis wae 1855, Sept. 20 ......... 88-67 497°8 88:59 | —0-08
METI 5, ovocnesecesposie 1855, June 11............ 87:66 | 477:2 87:49 | —017
REPU ors cise): pap ciaaan'en 1855, June 14,........... 86:70 | 459°6 86:53 | —017
CUETO ASRS nse VSa5), Ulva worse scores: 84:72 4259 84:58 | —014
Group V.—89-99 to 81: Correction —0°13 of the Thermo-barometer.
PPUGAMIN: wiciciaesaesvees 1856, Aug. 16.........45 83-02 | 397-7 | 82:85 | —0-17
PEMTEPASS: 5.)..csicdseevaernee 1855; July lOve. wrens 82-20 385°5 82:07 | —0-13
HOMME ASS a scicsscsisesnee’ USS5 Alu yi Dy agave sores - 82°16 385°5 82:07 | —009
Jbi Gamin Pass............ 1855, Aug. 18............ 81:56 | 375°6 81-42 | —0-14
* The corrections of the thermo-barometer, given at the different groups, are values
obtained by fundamental determinations. These determinations will be given in detail in
yol. ii. of Messrs. de Schlagintweit’s ‘ India and High Asia,’ 1861.
—
4%
59 REPORT—1860.
On Practical Experience of the Law of Storms in each Quarter of the Gilobe.
By Captain W. Parker Snow.
From practical experience in several parts of the globe, Captain Snow confirmed
the soundness of the theory of the Law of Storms brought forward by Admiral
FitzRoy. In one place, well known to the Admiral, viz. the tempestuous seas about
Cape Horn, he, Capt. Snow, had cruised for two years without the smallest damage
to his vessel, and this owing to the attention he ever paid to those laws of nature
in connexion with wind movements.
On another occasion, off the coast of Australia, he preserved his little ship, by
similar attention, in a terrific gale, when at the same time several other vessels were
wrecked. He well remembered how his chief officer derided the idea of any storm
theory being true, and, when referred to Reid and other stormists, said he had never
heard of them, and did not believe in what they might say. But that same night
the mate was convinced when the gale took the turn predicted by the captain.
One more occasion Capt. Snow would refer to. Hewas coming home as passen-
ger in asailing ship ; it was in the end of 1856. Within a few days’ sail from England
a cyclone came down upon them. Clearly it was passing ahead, and Capt. Snow
advised his brother captain to adopt those measures which prudence then suggested,
and allow the centre to go by. After some argument this was done; but, to con-
vince the master of the ship, Capt. Snow said that the correctness of his view of the
case then, would be proved by the direction of the wind at that time in the South of
England, which should be opposite to what they had it. Four days afterwards they
took a pilot, and ascertained it to have been exactly so.
Nore.—The above is merely the substance of remarks made when Admiral FitzRoy read
his paper. They form the outline of what was read on a following day, by Captain Snow,
when he entered upon details.
Results of an Investigation into the Phenomena of English Thunder-storms
during the years 1857-59. By G. J. Symons. .
This paper contained an analysis of 1889 observations made in various parts of
England during the three years ending December 31st, 1859.
The average number of days on which thunder-storms occurred at one or more
stations was 121, the number of days in each month being—
JAMUANY? ier ot ele SiApril Jeeee. «oe 2i July). ete clove LS) \Octobercernent nO
February....:. 2|May.......+. 18} August...... 14} November..... 6
March........ 6|June.........-20|September... | 12|December,<.... 5
The effect of thunder-storms on the various meteorological instruments was exa-
. mined and described, special attention being drawn to those sudden oscillations of the
barometer which occur during the height of a storm, and which have been found by
_ Mr. Eaton, of Little Bridy, to be contemporaneous with tidal disturbances. The
shape, colour, and disruptive force of lightning were also treated in detail, the
| frequency with which it assumes a globular form being proved by the number of
' eases in which it is so described: the determination of colour was not perfectly
' satisfactory; the returns taken generally show that forked lightning is usually blue,
sheet lightning being, on the contrary, white. Mr Symons, however, supposes that
the colour may vary with the distance of the discharge from the observer, with the
density of the air through which it passes, and with the existence or non-existence of
other sources of illumination; but the subject is quite open to investigation: the
disruptive force was shown to be often equal to a dead weight of 500 tons.
The advantage of employing the gutters and rain-water pipes of private houses —
as lightning conductors, by establishing perfect communication with the earth, and
at the same time carrying a short rod from the gutter up the side of the chimneys, —
was discussed ; the author’s opinion being that, although far from a perfect arrange- —
ment, it would determine the discharge to the outside of the house rather than
inside, its most frequent course; and from its trifling cost it seems more adapted for
general use than the expensive forms hitherto employed.
TRANSACTIONS OF THE SECTIONS. 53
Notes on Atmospheric Electricity.
By Professor Witttam Tuomson, LL.D., F.R.S,
Two water-dropping collectors for atmospheric electricity were prepared, and
placed, one at a window of the Natural Philosophy Lecture-room, and the other at
a window of the College Tower of the University of Glasgow. A divided ring-
electrometer was used at the last-mentioned station; an electrometer adapted for
absolute measurement, nearly in the form now constructed as an ordinary house elec-
trometer, was used in the lecture-room. Four students of the Natural Philosophy
Class, Messrs. Lorimer, Lyon, M‘Kerrow, and Wilson, after having persevered in
preliminary experiments and arrangements, from the month of November, devoted
themselves with much ardour and constancy during February, March, and April to
the work of observation. During periods of observation, at various times of day,
early and late, measurements were completed and recorded every quarter-minute
or every half-minute; the continual variations of the phenomenon rendering soli-
tary observations almost nugatory. During several hours each day simultaneous
observation was carried on on this plan at the two stations. A comparison of the
results manifested often great discordance, and never complete agreement. It was
thus ascertained that electrification of the air, if not of solid particles in the air
(which have no claim to exclusive consideration in this respect), between the two
stations and round them, at distances from them not very great in comparison with
their mutual distance, was largely operative in the observed phenomena. It was
generally found that after the indications had been negative for some time at both
stations, the transition to positive took place earlier by several minutes at the
tower station (upper) than at the lecture-room (lower). Sometimes during several
minutes, preceded and followed by positive indications, there were negative indica-
tions at the lower, while there were only positive at the upper. In these cases the
circumambient air must have contained negative (or resinous) electricity. A hori-
zontal stratum of air several hundred feet thick overhead, if containing as much
positive electricity per cubic foot as there must have been of negative per cubic foot
of the air about the College buildings on those occasions, would produce electrical
manifestations at the earth’s surface similar in character and amount to those ordi-
narily observed during fair weather.
Beccaria has remarked on the rare occurrence of negative atmospheric indications
during fair weather, of which he can only record six during a period of fifteen years
of very persevering observation by himself and the Prior Ceca. On some, if not
all of those occasions, there was a squally and variable wind, changing about rapidly
between N.E. and N.W. On several days of unbroken fair weather in April and
May of the present year the atmospheric indication was negative during short periods,
and on each occasion there was a sudden change of wind, generally from N.E. to
N.W., W., or S.W. For instance, on the 3rd of May, after a warm, sunny, and very
dry day, with a gentle N.E. breeze and slight easterly haze in the air, I found about
8°30 p.m. the expected positive atmospheric indication. After dark (nearly an hour
later) it was so calm that I was able to carry an unprotected candle into the open
air and make an observation with my portable electrometer. To my surprise I
found a somewhat strong negative indication, which I observed for several minutes,
Although there was no sensible wind in the locality where I stood*, I perceived by
the line of smoke from a high chimney at some distance that there was a decided
breeze from W. or S.W. A little later a gentle S.W. wind set in all round, and
with the aid of a lantern I found strong positive indications, which continued as long
as I observed. During all this time the sky was cloudy, or nearly so. That re-
versed electric indications should often be observed about the time of a change of
wind, may be explained with a considerable degree of probability, thus :—
The lower air up to some height above the earth must in general be more or less
electrified with the same kind of electricity as that of the earth’s surface, since this
reaches a high degree of intensity on every tree-top and vegetable fibre, and must
therefore cause always more or less of the phenomenon, which becomes conspicuous
as the “‘ light of Castor and Pollux,’’ known to the ancients, or the “fire of St.
Elmo” described by modern sailors in the Mediterranean, and which consists of a
* About six miles south of Glasgow
54 REPORT—1 860.
flow of electricity of the kind possessed by the earth into the air. Hence, in fair
weather the lower air must be negative, although the atmospheric potential, even close
to the earth’s surface, is still generally positive. But if a considerable area of this
lower stratum is carried upwards into a column over any locality by wind blowing
inwards from different directions, its effect may for a time predominate, and give rise
to a negative potential in the air and a positive electrification of the earth’s surface.
If this explanation is correct, a whirlwind (such as is often experienced on a small
scale in hot weather) must diminish, and may reverse the ordinary positive indication.
Since the beginning of the present month I have had two or three opportunities of
observing electrical indications, with my portable electrometer, during day thunder-
storms. I commenced the observation on each occasion after having heard thunder,
and I perceived frequent impulses on the needle which caused it to vibrate, indicating
sudden changes of electric potential at the place where I stood. I could connect the
larger of these impulses with thunder heard some time later, with about the same de-
gree of certainty as the brighter flashes of lightning during a thunder-storm by night
are usually recognized as distinctly connected with distinct peals of thunder. By
counting time I estimated the distance of the discharge, not nearer on any occasion
than about four or five miles. There were besides many smaller impulses, and most
frequently I observed several of these between one of the larger and the thunder with
which I connected it. The frequency of these smaller disturbances, which sometimes
kept the needle in a constant state of flickering, often prevented me from identifying
the thunder in connexion with any particular one of the impulses I had observed.
They demonstrated countless discharges, smaller or more distant than those that gave
rise to audible thunder. On none of these occasions have I seen any lightning.
The absolute potential at the position of the burning match was sometimes positive
and sometimes negative ; and the sudden change demonstrated by the impulses on
the needle were, so far as I could judge, as often augmentations of positive or dimi-
nutions of negative, as diminutions of positive or augmentations of negative. This
afternoon, for instance (Thursday, June 28), I heard several peals of thunder, and I
found the usual abrupt changes indicated by the electrometer. For several minutes
the absolute potential was small positive with two or three abrupt changes to some-
what strong positive, falling back to weak positive, and gathering again to a discharge.
This was precisely what the same instrument would have shown anywhere within a
few yards of an electrical machine turned slowly so as to cause a slow succession of
sparks from its prime conductor to a conductor connected with the earth.
I have repeatedly observed the electric potential in the neighbourhood of a loco-
motive engine, at work ona railway, sometimes by holding the portable electrometer
out of a window of one of the carriages of a train, sometimes by using it while stand-
ing on the engine itself, and sometimes while standing on the ground beside the line.
I have thus obtained consistent results, to the effect that the steam from the funnel
was always negative, and the steam from the safety-valve always positive. I have
observed extremely strong effects of each class from carriages even far removed from
the engine. I have found strong negative indications in the air after an engine had
disappeared round a curve, and its cloud of steam had dissolved out of sight.
In almost every part of a large manufactory, with steam-pipes passing through
them for various heating purposes, I have found decided indications of positive elec-
tricity. In most of these localities there was some slight escape of high pressure
steam, which appeared to be the origin of the positive indications.
These phenomena seem in accordance with Faraday’s observations on the electricity
of steam, which showed high pressure steam escaping into the air to be in general.
positive, but that it was negative when it carried globules of oil along with it.
Note on the Dispersion of the Planes of Polarization of the Coloured Rays
produced by the Action of Magnetism. By M. Vervet, Paris.
The researches in which I have been for some years engaged upon the magnetic
relations of the plane of polarization, discovered as we all know by Mr. Faraday,
have naturally led me to examine how these relations vary with the nature, or, using
theoretical language, with the length of the undulation, of the light. The experi-
mental method which I have employed is the general method introduced into science
TRANSACTIONS OF THE SECTIONS. 55
by MM. Fizeau and Foucault, which consists in decomposing the white light after
it has traversed the apparatus in which it-has suffered a certain modification ; and
in examining how this modification varies from one extremity to the other of the
spectrum thus obtained, selecting especially, for the numerical measure of the rela-
tive effect, the seven principal rays which Fraunhofer has defined, and the length
of those undulations he has determined. As the exact determination of the position
of a plane of polarization requires that the light shall have a certain intensity, I have
been obliged to confine myself to measuring the relations of beams which correspond
with five rays, C, D, E, F and G.
As in my previous researches, in order to operate upon certain bodies well de-
fined and easily reproduced, I have always experimented upon liquids, contained in
tubes closed at their extremities by transparent plates ; placing these tubes in the
interior of a strong electro-magnetic coil, and so arranged that their two ends shall
sufficiently pass the edges of the coil, to obviate the necessity of taking into account
the action which the transparent plates themselves might exercise on polarized light.
But under these conditions the employment of a powerful current was rendered ab-
solutely necessary by the feebleness of the phenomena; and the nature of the experi-
ments requiring that each liquid should remain for a long time under observation,
an elevation of temperature was produced which easily reached 50° or 60° Centigrade,
and which produced a contraction of the rotations observed, which it was very diffi-
cult to correct.
The only way of avoiding this source of error, was to place the tube containing the
liquid in an annular collar continually traversed by a stream of cold water within
the electro-magnetic coil,—a considerable complication to the apparatus.
The coil which I employed was not less than 45 centimetres in length, 15 centi-
metres in internal, and 30 centimetres in external diameter. It contained more than
80 kilogrammes of copper wire 2°25 millimetres in diameter, and was set in action
by a Bunsen’s battery of twenty or thirty elements.
I have not yet quite finished my experiments, but I am now in a position to esta-
blish one result, which does not appear to me to be unworthy of being communi-
cated to the Association. M. Wiedemann, in a note published in 1851, believed that
he might deduce from a small series of experiments, that if one submitted to the
action of magnetism a substance capable of itself of turning the plane of polarization,
such as the spirit of turpentine or essential oil of lemon, the rotation proper to the
substance and the magnetic rotation were proportional to one another through all
the colours of the spectrum. In order to submit toa decisive proof this law, which
would be, were it true, of immense theoretical importance, I have just examined an
extreme case, that of tartaric acid. We know that solutions of this acid induce in
the planes of polarization rotations which do not increase from the red to the violet,
as in ordinary cases, but which present in the interior of the spectrum a maximum
whose exact position varies with the strength of the solution. Were the relations
admitted by M. Wiedemann correct, the magnetic rotations of tartaric acid should
present the same anomaly. My experiments have, however, proved, on the contrary,
that the magnetic rotations in different solutions of this acid always increase from
the red to the violet. There is no essential relation between the two orders of phe-
nomena, as there is no analogy between their causes.
On the other hand, my experiments show how the two phenomena may have ap-=
peared in some cases proportional. They show, in fact, that in all cases the mag-
netic rotations of the plane of polarization increase very rapidly from the red to the
violet, but that the product of the rotations by the square of the length of the un-
dulations, increase very slowly between the same limits; and one recognizes in this
announcement, that which experiment has long ago demonstrated in most of the
natural rotatory powers.
Results of Self-registering Hygrometers. By E. Vivian, M.A., Torquay.
Mr. Vivian reported to this Section a series of observations made with his new
self-registering hygrometers, which were first exhibited before the Association at its
Cheltenham meeting. One is a combination of the ordinary wet and dry bulb and
the differential thermometers, registering the maximum and minimnm, or range during
56 REPORT—1860.
any period ; the other, by the continuous precipitation of the vapour from alcohol, re-
cords the mean amount of difference between the wet and dry bulbs. The curves laid
down from these instruments varied very greatly from that of the ordinary observa-
tions at 9 a.m. The instruments are very simple, and not capable of derangement.
Curves were also exhibited showing the character of the climate of Torquay during
a long series of years, from observations periodicaily communicated to the Registrar-
General. The comparison with the average of other places in England showed the
climate of South Devon to be very much more equable, both in regard to temperature
and humidity. The summers are as much cooler as the winters are more mild.
The fall of rain is rather greater, but the number of wet days is less. Other curves
exhibited the degree of confidence to be placed in the barometer in prognosticating
changes in the weather, and the influence of the moon, which was only discoverable
in the more disturbed state of the atmosphere at the times of the spring tides.
Results of Ten Years’ Meteorological Observations at Stonyhurst.
By the Rev. A. WELD.
Stonyhurst College is situated in the county of Lancashire, in lat. 53° 50’ 40" N.,
and long. 9° 52’ W. It stands at an elevation of 380 feet in the S,E. vicinity of
Longridge Fell, which rises upon elevated broken undulations from the bed of the
Ribble to 1140 feet. In the centre of the garden, which commands a wide extent
of country, was chosen the site for the observatory, having on all sides generally a
free and distant horizon. The observatory contains a 5-foot equatorial, a meridian
circle 23 feet diameter, a transit instrument, two transit clocks, and a considerable
meteorological apparatus. The report opens with an historical sketch of the origin
of the Meteorological Observations in 1847. The instruments have been compared
with standards by Mr. Glaisher, of the Royal Observatory, Greenwich. The report
extends over ten years, from the beginning of 1848 to the end of 1857. ‘The chief
instruments recorded have been the barometer; the dry and wet bulb; the highest
and lowest readings of the thermometer in the shade; the highest of a thermometer
with a blackened bulb exposed to the sun’s rays, and the lowest of a thermometer
exposed upon grass ; the direction and estimated force of the wind, and the amount
of cloud at the time of each observation; the daily and monthly fall of rain and
snow; amount of evaporation from an exposed surface of water; the general cir-
cumstances observed to attend Aurora Borealis and thunder-storms ; and a general
description of the state of the weather and appearance of the sky. ‘The observations
were recorded at 9 a.m., 1 P.M., 3 P.M., and 9 Pp. M., local time, which have been
made, almost without exception, throughout. The report describes at length the
methods used in recording and reducing the observations. Then follow the tables
and very carefully executed curves and diagrams, with explanatory notes interspersed.
GENERAL PHysIcs.
Physics as a Branch of the Science of Motion.
By J. §. Stuart Gienniz, MA.
In order that the great aim of modern science may be accomplished, and
mechanical principles be rigorously applied to physical and chemical phenomena,
it seems clear that physical and chemical forces must be conceived in the same
Way as mechanical forces. Therefore, as the general condition of the development
of a mechanical force, and, consequently, of a mechanical motion, is a difference of
pressures, and as a mechanical motion is in the direction of least pressure, a phy-
sical or chemical force must be similarly conceived as a difference of pressures, and
attractions and affinities explained as motions in the direction of least resistance :
and as the cause of an ordinary mechanical motion is no supernatural or unrelated
entity or agent, but simply the condition or relation of difference among a set of
mutual pressures, so the causes of physical and chemical motions must he conceived,
not as agents, but as relations. But as (though an absolute force is inconceivable)
Re
TRANSACTIONS OF THE SECTIONS, 57
we may speak of a moving body as a mechanical force because it cannot come into
contact, be brought into relation with another body without there being thus a dif-
ference of the previously existing polar pressures on that body, and hence a motion
or change of motion; so we may speak of heat, electricity, &c. as forces, because
bodies in such states of molecular motion or tension cause a motion of other bodies,
or of their molecules. And these forces are thus conceived, not as absolutely exist-
ing agents acting on matter, but as conditions of matter.
It is evident that this idea of force, by which all particular forces become one (by
being referred to the same general conception of a difference of pressure), postulates
a plenum. But this will prebably be now generally granted. If, then, there is a
pleaum, we may conceive the influence which every part of matter exerts on every
other, as acting not “ at.a distance,’ but through other intermediate matter, form-
ing lines of pressure. Hence we may conceive a body or molecule as a centre of
pressure, and see whether, retaining the usual mechanical conception of “ pressure”
as “‘ a balanced force,” or ‘‘ virtual momentum,” such influence, or, more definitely,
physical and chemical phenomena, become mechanically explicable.
A molecule, therefore, or body, an aggregate of molecules, is conceived as a centre
of lines of pressure ; the lengths and curves of these lines are determined by the rela-
tive pressure of the lines they raeet; and lines from greater, are made up of similar
lines from lesser molecules, and so on ad infinitum. In speaking of a molecule or
body as such a centre of pressure, we may, for convenience sake, call it an atom.
In chemistry, the term equivalent will be used exclusively, and not as more or less
synonymous with atom, which I have thus ventured to appropriate for a new con-
ception.
edkid*or mutually determining centres of lines of pressure, may also be defined
and mathematically considered as mutually determining elastic systems with centres
of resistance.
But these fundamental conceptions of centres of lines of pressure, or centrally
resisting elastic systems, are not hypotheses, but convenient forms of the general
conception of the parts of matter as mutually repelling.
If, in a system of such atoms, the centres, whether molecules or suns, are all of
equal mass, and at equal distances, the mutual repulsions of their lines will be equal
in all directions ; there will be no difference of pressure, no moving force will be
developed, and the conditions of equilibrium are satisfied. But it was shown that
if there are in such a system differences in the masses of the resisting centres, or
in their relative positions, the law of universal attraction, or approach of these
centres, whether, in any particular case, equal or unequal, would follow as a me-
chanical consequence of the deflection of the mutually opposing lines.
But such centres may differ not only in mass, but intension. Tension is conceived
as a state of unstable equilibrium, in which a (molecular) atomic centre, having been
moved towards the next atom in any plane, rests in a position in which the pressure
of its lines is increased in that direction, and correspondingly, of course, diminished
in the opposite. Such is the general mechanical conception of polarity proposed in
this theory.
The phenomena caused by bodies in a state of static electricity are deduced from
the conception of outward or inward tension in a closed curve.
In dynamically electrified bodies the tension is conceived as longitudinal, and the
poles as the ends towards and from which the molecules have been moved. A mag~
net is conceived as a body in which the molecules are in a permanent state of trans-
verse tension ; and hence, evidently, as in Ampére’s theory, the analogy (except as
to power on iron core) between a helix and a magnet.
Induction is the necessary mechanical effect on adjacent bodies of electricity or
Magnetism as above conceived. The character of that effect depends on the rela-
tive conditions of the tension of the acting body, and of the mechanical resistance
due to the molecular motion or aggregation of the bodies acted on.
The various motions in the presence of electric or magnetic bodies are explicable
as differential effects of (electric or magnetic) conduction,
It is proposed to apply this general theory to the undulatory theory of light and
heat, with the hope that the difficulties therein at present encountered may be hereby
overcome,
58 : REPORT—1860.
As to chemistry, it may be briefly noted that its phenomena seem capable of being
brought within the science of motion by deductions from the general conceptions of
a body as a system of moving molecules (specific heat), which, the motion at every
point being equal in intensity, is in a state of dynamic equilibrium; and of the
formation of compounds, as the formation of new states of dynamic equilibrium.
A General Law of Rotation applied to the Planets.
By J. 8. Stuart Guienniz, M.A.
The author directed attention to a table of elements which seemed to point to a
general law for the angular velocity of rotation of the planets ; though, of the many
formule calculated, none had as yet given perfect accuracy.
But these tables gave a new law connecting the angular velocities of revolution
with the distances.
He referred the nullity of effect on the planets of the resisting medium which
shortens the periods of Encke’s comet to a neutralization deduced from a hydrody-
namical theorem.
SounpD.
On the Velocity of the Sound of Thunder.
By the Rev. 8S. Earnsuaw, IA.
The object of this paper was stated by its author to be, to solicit the attention of
observers to certain phenomena which seem to indicate that the velocity of the
sound of thunder is sometimes much greater than that of ordinary sound. He had
himself noticed a case where the sound followed close upon the flash of lightning,
though judging from the distance of the point struck (more than a mile) from him,
the interval between the flash and the sound should have been upwards of five seconds.
He stated also that Professor Montigny of Antwerp had communicated to him accounts
of similar instances noticed by himself and M. Raucoux, curé of Temploux. One in
particular was very remarkable. Ona certain night last autumn, Professor Montigny
observed the lightning strike a farm at such a distance from him, that, according to
the received velocity of sound, more than fifteen seconds ought to have elapsed before
he heard the report, whereas it reached him in two seconds. This was confirmed
to him the next day by the curé of Temploux, who being at nearly the same distance
from the farm, heard the crack of the thunder in what he judged to be certainly not
more than two seconds from the descent of the electric fluid. The difference in this
case is so great between theory and observation, that errors of estimation of the time
cannot possibly account for it. The two observers were more than 4000 métres
apart. The author stated, that although there were in these instances such discre-
pancy between them and the received theory, he had communicated investigations to
the ‘Philosophical Magazine’ with which they were in perfect agreement, But,
nevertheless, he hoped that some of the members of the Association would turn their
attention to these phenomena, in order that it might be definitely settled, whether
his theoretical deductions are, or are not, supported and confirmed by undoubted
facts.
On the Triplicity of Sound. By the Rev. 8. Earnsuaw, M.A.
The fundamental idea of this paper is the hypothesis of finite intervals. Setting
out from this, the author shows that the most simple elements of wave-motion are
defined by the equation = +a, x being the displacement of an aérial particle at
any time ¢. If the radius of molecular action extend over a large number of parti-
cles, the method pursued by the author gives the velocity of ordinary sound 1130
feet. He also shows that the velocity of a thunder-clap must of necessity be greater’
than that of ordinary sounds. There are two essentially distinct types of wave-
motion, corresponding to the two signs with which k° is affected in the above
equation ; the upper sign belongs to the thunder type, and the lower to-ordinary’
payers
TRANSACTIONS OF THE SECTIONS. 59
musical sounds: and it is shown that for a given value of k there are three different
velocities of wave transmission, viz. one corresponding to the upper sign, and two to
the lower sign. This is what the author means by the triplicity of sound. The
papers on this subject will be found printed at length in the ‘ Philosophical Maga-
zine’ for June, July, and September.
INSTRUMENTS.
Description of an Instrument for Measuring Actual Distances.
By Parrick ADIE.
The telemeter consists of two telescopes so arranged in two concentric tubes, that
the rays formed by two object-glasses, at or near the extremities of the tubes, are by
means of reflectors brought together into one eyepiece in the middle of the tubes ;
thus both telescopes are simultaneously pointed at the same object, one being move-
able, and their relative angle taken from a scale and vernier, and this by reference
to a table on the instrument gives the distance of the object looked at. The author
has obtained measures to 5 yards in 500, and 20 in 1000 with a base of only 18 inches,
The length of the arm and power of the telescopes being equal to such minute accu-
racy, this promises to supply the link wanting to make the long range in gunnery use-
ful. Its power is such, that with the 18-inch base, the one described, we can read to
5 yards in 500, or 20 in 1000, and it may be used up to 4 or 5 miles with effect.
Description of a New Reflecting Instrument for Angular Measurement.
By Patrick ADIE.
The instrument is a sextant or circle which the author proposed to name the bino-
cular reflector. It consists of two telescopes, also so arranged as to work with one
eyepiece, one telescope being directed to each of the objects whose angular distance
is sought ; one of these is fixed below the limb, the other above it; and the rays are
passed from the lower into the upper, by means of a reflector sending them at right
angles through the centre of the instrument, which is hollow; these rays entering
the upper telescope, are by means of a second reflector passed along with those of
the other half which is open into the eyepiece. The point of this instrument is, that
it gives the whole instead of half degrees as in Hadley’s principle, thus reducing the
size of the instrument one-half, and the cost nearly in like degree; it will also be
much less subject to disarrangement, and can measure any angle up to 180°.
- Ona Pile with Sulphate of Lead. By M. E. BecquereE-.
The pile of M. Edmond Becquerel is composed of an exterior receiver of zinc of
an annular shape, and of a cylinder composed as follows, A cylinder of lead of 29
centimetres (9} inches) long and about half a centimetre (,2,ths of an inch) diameter,
is placed in the inside of a mould 13 centimetres (4°6 inches) in height, and 9 centi-
metres is filled (2} inches) in diameter, with a paste of sulphate of lead pulverized,
and 400 grammes water saturated with marine salt at 25° of the areometer, {being
129 to 139 cubic centimetres. The mixture of these should be made very quickly.
After the sulphate of lead has acquired a sufficient consistence, we remove it from the
mould, and we cover it round with a bed of plaster of half a centimetre in thick-
ness. ‘This pile is charged with water rendered saline with common (sea) salt about
ath saturated. Its electromotive force is equal to the half of that of sulphate of
copper, and its resistance to conduction is equivalent to 100 metres of red copper
wire of a millimetre diameter. It has the advantage of being very simple, and of
not requiring anything to keep it in action; it is put into action by a single liquid,
and does not need a porous vessel. It possesses much constancy, and does not cease
to act until the sulphate of lead is entirely reduced to the metallic state. M. Bec-
querel had one in action composed of ten pairs, of which the circuit remained com=-:
pletely closed for three months. :
:
60 REPORT—1860,
On an Atmotic Ship. By the Hon. W. Bann, New South Wales.
The proposal in this case was to employ a light keel and ship-formed body buoyed
up by an elongated balloon, and two heavy weights guided by a rope slung from
stem to stern, to alter the centre of gravity of the machine and direct its motion
upwards or downwards at pleasure. To cause it to move onwards in any assigned
direction, large but light and strong vanes were to be driven round, acting like the
screw propeller of a ship.
On an Improved Instrument for describing Spirals, invented by Henry
Johnson. By the Rev. J. Bootu, LL.D., F.RS.
Mr. Johnson’s instrument, which, looking to its practical use, he calls a volutor,
admits of several varieties, and may be briefly described as follows:—The form
which most clearly exemplifies the principle consists of a vertical axis resting on a
horizontal plane, and retained on it by a metal point to prevent slipping or lateral
motion. To this upright axis is attached one extremity of the horizontal arm or
bar. The vertical axis passes through the extremity of the horizontal arm, or a block
attached to the end of it, in such a way that the horizontal arm may revolve freely
round the vertical axis. The remote extremity of the horizontal bar is furnished
with a drum or pulley, over which a band or chain passes; one end of this band is
affixed to the centre upon a level with the pulley, and the other end of the chain or
band, after passing over the pulley at the outer end of the horizontal rod, returns
and is attached to a slide which carries a pencil ur marking instrument. The hori-
zontal bar is made to revolve, either by the hand directly applied to it, or by a string
wound round a drum attached to the block revolving on the vertical axis.
The chain or band is thus wound round the upright axis, while each succeeding
coil encloses the preceding one, and is supported by a small plane projecting from
the centre. The slide is drawn from the centre towards the drum at the other end
of the horizontal arm, and thus the curve is traced by the pencil or other point, pro-
gressively increasing its radius vector as the slide recedes from the axis. The addi-
tion of small tubes to slide down, when required, to the junction, with an opening
for the chain or band, will afford the means of varying the size of the axis, and con-
sequently the interval between the successive spirals of the curve. The intervals
between the spirals are determined by the size of the axis, and the thickness of the
band coiled round it. When each coil round the cylindrical axis rises above the
preceding one, without enclosing it, the spiral of Archimedes is described, as the
radius vector is increased each revolution by the circumference of the axis, neglecting
the inclination of the cord.
A cone may be conveniently used as a centre, and the band wound round it in lieu
of being wound in a flat coil; and the size of the centre may be enlarged, by wind-
ing the band one or more times round the cone before tracing the curve.
A number of pulleys are affixed to the slide and the block on the axis, and the
curve may be modified by passing the band over one or more of them.
As the vertical axis of the volutor, and the slide on the horizontal bar to which
motion is communicated, are connected by a cord or chain passing over a system of
pulleys, the length of cord which wraps round the vertical cylinder becomes 2 times
the radius of the spiral, n being the number of pulleys attached to the slide which
travels on the horizontal arm. Hence, by increasing m, we may diminish the mag-
nitude of the spirals described by the volutor *.
When, instead of the vertical cylinder round the axis, a grooved cone is sub-
stituted, the width of the whorls increases with each revolution of the radius vector
of the spiral ; and by substituting in succession a series of cones in the vertical axis,
each of a different pitch, we may obtain spirals where successive whorls shall widen
out in any given ratio.
Recent improvements in the volutor, as shown in the annexed drawing, include
arrangements for the vertical position of the pencil, as also for attaching the band to
the base of the cone when required, and for applying the set of pulleys to either end
of the horizontal bar.
* In fact, the cord wound round the axis, and the end of the slide which carries the
tracing point, are as power and weight in a system of mechanical pulleys.
TRANSACTIONS OF THE SECTIONS. 61
In addition to the spirals that are traced, when the band is wound first round the
apex of the cone descending to the base, by the pencil receding from the centre, on the
principle described; spirals may also be traced by the pencil approaching the centre
from the extremity of the radius vector, when the pulleys are attached to the pencil
end of the horizontal bar, and the band is wound round the grooved cone ascend-
ing from the base.
A A stand, with wheels moveable round the central point O.
B Horizontal bar, passing through the horizontal tube D on stand.
C Tracing pencil, pressed down by vertical spiral spring.
D Horizontal tube on stand.
E Set of pulleys on stand.
F* Set of pulleys screwed on to the end of the horizontal har.
G Band wound about the grooved cone at the centre, and passing over pulleys at F and ¥.
- H Handle attached to grooved cone, and held stationary with one hand; while the stand
carrying horizontal bar, &c., is moved by means of a winch handle attached to the top of a
steel axis rising through the cone and handle.
I The winch handle.
On the Means of increasing the Angle of Binocular Instruments, in order to
obtain a Stereoscopic Effect in proportion to their Magnifying Power.
By A. Curauvet, £.R.S.
In a paper on the stereoscope, which Mr. Claudet read before the Society of
Arts in the year 1852, alluding to the reduction of the stereoscopic effect produced
by opera glasses on account of their magnifying power, he stated that, in order to
redress that defect, it would be necessary to increase proportionately the angle of the
two perspectives. This he proposed to do by adapting to the object-glasses two sets
of retlecting prisms, which by a greater separation given to the two lines of perspec-
tives, would reflect on the optic axes images taken at a greater angle than the angle
of natural vision. Such was the instrument that Mr. Claudet submitted to the
British Association, to prove, as he has always endeavoured to demonstrate in various
memoirs, that the binocular angle of stereoscopic pictures must be in proportion to
the ultimate size of the pictures on the retina,—larger than the natural angle when the
images are magnified, and smaller when they are diminished; which, in fact, is
62 REPORT—1860.
nothing more than to give or restore to these images the natural angle at which the
objects are seen when we approach them or recede from them. For magnifying or
diminishing the size of objects is the same thing as approaching them or receding
from them, and in these cases the angles of perspectives cannot be thesame. Mr.
Claudet showed that, looking at the various rows of persons composing the audience,
with the large ends of the opera-glass, all the various rows appeared too close to
one another, that there was not between them the distance or space which separates
them when we look with the eyes alone; and he showed also that, with the small
end, the distance appeared considerably exaggerated. But applying the sets of
prisms to the opera-glass in order to increase the angle of the two perspectives, then
looking at the audience as before, it appeared that the various rows of persons had
between them the natural separation expected for the size of the image or for the re-
duction of the distance of the objects. By applying the two sets of prisms before
the eyes without the opera-glass, it was observed, as was to be expected, that the
stereoscopic effect was considerably exaggerated, because the binocular angle was in-
creased without magnifying the objects. But looking with the two sets of prisms
alone at distant objects, the exaggeration of perspective did not produce an unplea-
sant effect. It appeared as if we were looking at a small model of the objects
brought near the observer. By the same reason, stereoscopic pictures of distant
objects (avoiding to include in them near objects) can advantageously be taken at a
larger angle than the natural angle, in order to give them the relief of which they
are deprived as much when we look at them with the two eyes, as when we look
only with one eye; instead of being a defect, it seems that it is an improvement.
In fact, the stereoscope gives us really two eyes to bring out in relief the pictures of
distant objects.
On the Principles of the Solar Camera, By A. Ciauvet, F.R.S.
The solar camera, invented by Woodward, is one of the most important improve-
ments introduced in the art of photography since its discovery. By its means
small negatives may produce pictures magnified to any extent; a portrait taken on a
collodion plate not larger than a visiting card can be increased, in the greatest per-
fection, to the size of nature; views as small as those for the stereoscope can be also
considerably enlarged. This is an immense advantage, which is easily understood
when we consider how much quicker and in better proportion of perspective small
pictures are taken by the camera obscura, while the manipulation is so greatly sim-
plified. There is nothing new in the enlargement of photographic pictures. This
has been done long ago simply by attending to the law of conjugate foci; and every
photographer has always been enabled, with his common camera, to increase or
reduce the size of any image. For the enlargement, it was only necessary to place
the original very near the camera, and to increase in proportion the focal distance.
But the more the focal distance was increased, the more the intensity of light was
reduced; and a still greater loss of light arose from the necessity of diminishing the
aperture of the lens, in order to avoid the spherical aberration. Such conditions
rendered the operation so long that it became almost an impossibility to produce any
satisfactory results when the picture was to be considerably enlarged. For these
reasons, it naturally occurred, that if the negative, having its shadows perfectly
transparent and its lights quite black, was turned against the strong light of the sun,
its image at the focus of the camera would be so intense that the time of exposure
would be considerably reduced; so that, in order to employ the light of the sun,
and follow easily its position without having to move constantly the whole camera,
it was thought advisable to employ a moveable reflecting mirror sending the parallel
rays cf the sun on a vertical plano-convex lens, condensing those rays on the nega-
tive (placed before the object-glass and behind the condenser) somewhere in its
luminous cone. Many contrivances for this object were resorted to, but without
considering anything else than throwing the strongest light possible on the negative
to be copied. The constructors of these solar cameras never thought it very im-
portant to consider whether the focus of the condensing lens was better to fall before
or behind the front of the object-glass, provided the negative was placed in the lumi-
nous cone of the condenser. This want of attention has been the cause which has
made the solar camera a very imperfect instrument for copying negatives. The
i
TRANSACTIONS OF THE SECTIONS. 63
beautiful principle of Woodward’s apparatus consists in his having decided the ques-
tion of the position of the focus of the condenser, and in having placed it exactly on
the front lens of the camera obscura. As this principle had not yet been explained
when the invention was exhibited before the Photographic Societies of London and
Paris, and not even by the inventor himself in the specification of his patent,
Mr. Claudet has undertaken, in the interest of the photographic art, to bring the
subject before the British Association, and to demonstrate that the solar camera of
Woodward has solved the most difficult problem of the optics of photography, and
is capable of producing wonderful results. This problem consists in forming the
image of the negative to be copied only by the centre of the object-glass reduced to
the smallest aperture possible, without losing the least proportion of the light illus
minating the negative. The solar camera does not require any diaphragm to reduce
the aperture of the lens, because every one of the points of the negative are visible
only when they are defined on the image of the sun, and they are so exclusively for
the centre of the Jens, the only point which sees the sun; while the various points
of the negative, which from the marginal zone of the lens are defined against the
comparatively obscure parts of the sky surrounding the sun, are, as it were, invisible
to that zone; so that the image is produced only by the central rays, and not in the
least degree by any other points of the lens, which are subject to spherical aberration.
It is, in fact, a lens reduced to an aperture as small as is the image of the sun upon
its surface, without the necessity of any diaphragm, and admitting the whole light
of the sun after it has been condensed upon the various separate points of the nega-
tive. It is evident that from the centre of the lens the whole negative has for back-
ground the sun itself, and from the other points of the lens it has for background
only the sky surrounding the sun, which fortunately has no effect in the formation
of the image. Such is the essential principle of Woodward’s solar camera, which
did not exist in that instrument when the focus of the condenser was not on the
object-glass. This principle is truly marvellous ; but it must be observed, that the
solar camera, precisely on account of the excellence of this principle, requires the
greatest precision in its construction. For its delicate performances, it must be as
perfect as an astronomical instrument, which, in fact, it is. The reflecting mirror
should be plane, and with parallel surfaces, in order to reflect on the condenser an
image of the sun without deformation; and in order to keep the image always on
the very centre of the object-glass, the only condition for the exclusion of the oblique
rays, the minror should be capable, by its connexion with a heliostat, of following
the movements of the sun. The condenser itself should be achromatic, in order to
refract the image of the sun without dispersion, and to define more correctly the
lines of the negative; and a no less important condition for losing nothing of the
photogenic rays would be, to have the condenser formed with a glass perfectly
homogeneous and colourless. With such improvements, the solar camera will be-
come capable of producing results of the greatest beauty ; and, without any question,
its introduction into the photographer’s studio will mark a period of considerable
improvement in the art.
On a Reflecting Telescope for Celestial Photography, erecting at Hastings,
near New York. By Henry Draper, M.D.
In the summer of 1857, after the Dublin meeting of the British Association, a
party visited Lord Rosse’s telescope at Parsonstown. We were shown the ma-
chinery employed in its construction, and, as far as the weather permitted, its per-
formance.
That visit first led me to attempt constructing an instrument which should be
specially adapted for celestial photography, for which purpose the reflector possesses
such conspicuous advantages over any refractor.
Those who are familiar with photographic operations know well how important it
jis for the ensuring of uniform success, that the sensitive surfaces should always be
placed in similar circumstances as to position, and that position must afford every
facility for carrying on the necessary manipulations.
It appeared to me that a modification of a form of mounting, proposed some
time ago by Mr. Nasmyth, could be made to answer these requirements perfectly,
64 REPORT—1860.
and that a Newtonian reflector, sustained on hollow trunnions, through one of
which the rays from the small mirror could come, would permit of operations being
carried on upon a horizoptal table at the end of the trunnion with great ease. What-
ever might be the altitude or position of the object the photographic table would
always be horizontal.
As I proposed that the telescope should not be less than 12 feet in focal length,
an advantage would obviously arise from making the vertical axis of the framework
beneath its centre of gravity. The observatory in which it should be placed would
then require to be only one-half the diameter that would otherwise be demanded,
A 12-foot tube could be worked with its frame in a cylindrical space, 13 feet in dia-
meter and 13 feet in height.
I therefore cast a speculum of 15 inches in diameter and 2 inches in thickness.
The materials employed were Minnesota copper, regarded in America as the purest
commercial form of that metal, and Banca tin. Their proportions were those re-
commended by Lord Rosse. The cast was made in sand, 4 inches in thickness in
every direction from the speculum, which was permitted to remain for two days un-
opened, to ensure slow cooling. It proved to be perfectly successful. The machine
used for grinding and polishing it was that of Lord Rosse.
The tube of the telescope is of black walnut, bound externally by brass rings, and
strengthened interiorly by iron ones. The trunnions at the little mirror are of gua-
metal: they work on friction rollers of the same substance, supported on polished
steel axles.
- The telescope is moved in altitude, with the utmost facility, by the aid of counter-
poising levers, which act perfectly, whatever the position of the tube may be. The
pulleys through which these counterpoising levers work are also of gun-metai, sup-
ported on friction rollers, with polished steel axles. The motion, upon a vertical
axis, is accomplished by a cast-iron shaft, 2, feet in length and 3 inches in thick-
ness, working at one end on a hemispherical termination in gun-metal, and the other
sustained in a strong and ground cast-iron collar.
The observatory in which this instrument is being placed is situated on a hill,
400 feet above the level of the sea, at Hastings, about twenty miles north of New
York.
The edifice consists of a sunken chamber, excavated out of the solid rock. The
walls of this chamber are substantially built of stone, laid in hydraulic cement.
They are 9 feet high. On the top of these walls a lighter wooden edifice is raised,
sufficient to make the building of the required height. The revolving roof is metallic.
The ground plan is square, and 17 feet in the clear interiorly. As the frame of the
telescope only requires a cylindrical space of 13 feet, the corners of the building are
very available for the necessary photographic preparations.
On the top of the stone wall is placed a circular gallery running entirely around
the interior of the room, and enabling the operator to have access with great facility
to the photographic table and the eyepiece trunnion of the instrument. The in-
terior of the observatory is sheathed throughout with wood.
This partly underground construction has been adopted for the purpose of ensu-
ring a more complete invariability of the temperature of the mirror. A thorough
ventilation is, however, secured whenever desirable, the local position of the edifice
being such that the door of entrance is on the side of the hill at the level of the floor.
The wooden sheathing is for the purpose of avoiding deposition of moisture.
At the moment of writing this paper the building is unfinished, though rapidly
approaching completion. The various parts of the instrument and the photographic
arrangements are provided, and no difficulty is anticipated.
This is the first observatory that has been erected in America expressly for celes-
tial photography, and it is hoped that, considering the purity of the skies, it will
yield good results.
I expect also to derive considerable advantage from the method of darkening col-
lodion negatives by the aid of protochloride of palladium, described by me in a paper
read before the American Photographical Society, and which I think in this applica-
tion will permit of good proofs being taken by unprecedentedly short exposures,
_
——
y
TRANSACTIONS OF THE SECTIONS. 65
On an improved Form of Air Pump for Philosophical Experiments.
By W. Lavp.
On the Chromoscope. By Joun Smiru, M.A., Perth Academy.
The author sent a specimen of the cut-out card, by the rotation of which, in
strong light, as sunshine, he could produce various colours. There were also dia-
grams exhibited painted so as to represent the several colours and tints which the
author had succeeded in causing to appear. The chromoscope, he said, was not the
result of a happy accident, but was constructed to verify certain opinions which he
had long entertained as to the cause of colour; that it not only produced colour, but
explained the principle on which it was produced, and proved the necessity of intro-
ducing a negative term into the theory of colour—the purpose for which it was con-
structed. On the theory he said he would not enter, as he had explained it at the
Meeting at Aberdeen, when he also made some experiments before Section A.
The author’s object at present was to direct attention particularly to what he
considered a most remarkable phenomenon connected with these experiments, which
manifested itself in the change of colour which took place when the motion of the
figure was reversed. The simplest illustration given, was a semidisc divided into a
nuthber of concentric rings of equal breadth, each alternate ring being painted black
or cut out of the card, and tbe card fixed on the axle of the machine at a point,
exactly equal to half the breadth of one of the rings, from the centre of the disc.
When the card is made to rotate, each ring is thus divided into two equal sections,
and the section of a black ring is superposed, as it were, on a white, or a white on
a black when in motion; or in each revolution of the machine there is produced a
sensation of light and no light on the same spot of the retina. In this experiment
each contiguous ring has a different colour, one purple, the other a greenish yellow,
and each alternate ring has the same colour.
Reverse the motion, the rings which were purple will now be yellow, and vice
versd, those which were yellow will be purple.
There was another diagram giving an analysis of this; showing how all the rings
could be made of one colour, exhibiting discs wholly of purple rings, or wholly of
yellow rings.
He said that in these experiments, when the revolutions of the machine were more
than thirty-two in a second of time, all colour was lost to the eye; among other
reasons, demonstrating to the mind of the author, that the pulsations of light are
not so frequent as science represents them to be. He considered every revolution of
the machine equivalent to an effective pulsation of light; and that the usual experiment
of placing the prismatic colours on a wheel, and making them revolve, only proves the
inability of the eye to estimate such rapid vibrations, and not the composition of
white light, for the colour produced is a grey, not white, and so is the colour of his
cards when in such rapid motion.
To represent refracting substances, such as prisms or other transparent crystals
of any form, the author said it was necessary to make the cards revolve perpendi-
cularly, in order to produce the form of a solid. Several of these were shown to
the Section. A section of a ring produced the figure of a vase of a pink colour, with
a greenish centre. A semiring produced a vase of a different form and of various
colours, the brim being of a deep purple. A scroll composed of two semirings pro-
duced a strange compound figure, the predominant colour being a deep dark green.
Along these figures, in given conditions, there is a dark or a bright line, which he
said was the axis of motion, and might be considered as the line of no motion or of
no reflexion, ar of intermittent reflexion, according to the construction of the figure.
The card can be cut so as to represent both phases—the black and the coloured—in
the same figure.
The author in his paper said, ‘‘ Are not these phenomena very like those of
polarized light?’? only more astonishing, and more within the range of human
research, After looking at these experiments he always felt disposed to put the
question, ‘‘ What now is polarized light ?”
He also added that the horizontal and perpendicular experiments were constructed
on the same principle, and that the colours are the result of the same law.
1860. 5
66 REPORT—1860.
In concluding the author said, ‘‘ He was anxious that philosophers should become
acquainted with these experiments, as he considered that the ideas which they con-
veyed, and the facts which they revealed, must modify our views of some of the cog-
nate sciences ; and he was of opinion that they gave rise to a new theory of coloured
refraction, sut that he was unwilling to enter on the subject of refraction, until
scientific men were acquainted with the phenomena of the chromoscope.”
CHEMISTRY.
On Ozone. By Professor ANpreEws, M.D., F.R.S., MRLA.
On the Deodorization of Sewage. By Dr. Brirp.
On the Quantitative Estimation of the Peroxide of Hydrogen.
By Professor B. C. Bropiz, F.R.S.
On some Reactions of Zinc-Ethyl. By G. B. Bucxton, F.R.S.
Note on the Destruction of the Bitter Principle of Chyraitta by the Agency of
Caustic Alkali. By J. J. COLEMAN.
On some remarkable Relations existing between the Atomic Weights, Atomic
Volumes, and Properties of the Chemical Elements. By J. J. COLEMAN.
The author commenced by referring to the labours of Kopp, Schroeder, Joule, and
Herapath, respecting the atomic volumes of the non-gaseous elementary bodies.
The term atomic volume being defined as “indicating the space occupied or kept
free from the excess of other matter by the material atom itself together with its investing
sphere of heat,” particular attention was directed to a fact noticed some time ago by
Kopp, viz. that the atomic volumes of several elements correspond, so that they may
be arranged in groups. The author then proceeded to show that, in taking a group
of elements having equal or nearly equal atomic volumes, it would invariably be found
that the element possessing the least atomic weight would be the most chemically
active, the least reducible ; and, on the contrary, the element having the greatest
atomic weight would be found to be the most chemically inactive, the most reducible
member of the series. These important facts were demonstrated by quoting numerous
groups, Thus, amongst others, were brought forward the following, viz. :—
Atomic Atomic Atomic Atomic
weight. volume. weight. yolume,
Manganese.... 27°6 ....;. 44 |-, jSulphur .... 16 ...... 101
LUO OR ioe idoiad eae GOO 44 we Selenium.... 39° 25.535 101
1.2 Cobalt mere ~ 29 Sz ieee 44 Lead. ..<cc; 103°7. ck Seeeeulaet
| Nickel. 02.00) spent aa), | 0s A Silvet *.+teu) LOM, ei male 128
(Copper........ 82 ...... 44 Gold i i.3. 197) chem
Zine. . EO 13 Se eUoT Eusis nem OF, Chlorine .... 35°5 sseses 820
2, + Palladium apn cnes aareleis aD. 6.4 Bromine.... 80 ..4... 320
Platinum... sce Gomme eaa De Iodine .:.,4. 127 sacess 820
Molybdenum .. 46 ...... 66 Antimony .. 129 ie
Tungsten...... hs isle hs es 66 Bismuth ....< 213 wSigee re
Comparing together the members of the first group quoted, it was noticed that man-
ganese, having the least atomic weight, is the most chemically active, the most eager
in entering into combination with other elements,—iron, nickel, cobalt, and copper
following in due order; whilst the facility with which the respective metals are
jel 5 ae Tee we eee OO }stinony 32 sae ee
Se tf
TRANSACTIONS OF THE SECTIONS. 67
reduced is exactly the reverse—copper with the greatest atomic weight being the
most reducible, nickel and cobalt, iron and manganese following in order.
In group 2, zinc being the most active, the least reducible, and, on the contrary,
platinum the most inactive, the most reducible, another illustration of the law is
afforded,—the striking differences between the weight of the atoms finding its repre-
sentative in the equally striking differences between the properties of the respective
metals. Similar results are afforded by the study of other groups; thus in the
chromium, molybdenum, and tungsten group, chromium—the most active, the miost
difficult to reduce, the metal forming the largest number of combinations,—possesses
the least atomic weight of any member of the series, and precisely as the weight of
the atom increases, in molybdenum, and then in tungsten, does the chemical activity
decrease.
The group sulphur and selenium offers a pertinent illustration of the existence of
the law; selenium having an atomic weight 24 times greater than that of sulphur,
being to a corresponding extent the more reducible of the two.
Lead, gold, and silver afford another illustration of the universality of the law,
lead having the least atomic weight, being the most active, the least reducible, and
gold the greatest atomic weight, being the least active, the most reducible.
In the group chlorine, bromine, and iodine, the relation is very evident (the atomic
volume of chlorine being that of the liquid state), Phosphorus, antimony and
bismuth, and many other groups, when studied in a similar manner, confirm the
generality of the law, as applied to groups of elements having equal or nearly equal
atomic volumes.
These interesting results induced the author to extend the survey, and to institute
a careful examination into the general relations existing between the atomic weight,
atomic volumes, and properties of the whole of the elements. Considerable details
were entered into, the results arrived at being summed up as follows :—
1, That elements having a small atomic weight and a small atomic volume, such
as carbon, aluminium, sulphur, are difficult toreduce from their compounds, When
they are isolated, they are endowed with a certain degree of permanence; but the
limit of their resistibility is easily attained.
2. Elements with a small atomic weight and a large atomic volume, such as
potassium, sodium, phosphorus, are invariably active, and difficult to keep in an
isolated state.
3. Elements having a large atomic weight associated with a small atomic volume,
such as platinum, iridium, are characterized by their capability of resisting chemical
and physical agencies.
4, Elements possessing alarge atomic weight, associated with alarge atomic volume,
such as gold, bismuth, have considerable chemical activity; but the motion of the
atoms appears to be impeded by reason of their great weight.
From an accumulated amount of evidence of this nature, the author came to the
conclusion that the cohesive or attractive force of the chemical atom bears some
marked relation to (if it is not represented by) the actual weight of the atom, and
that it is to the repulsive forces associated with the atom that we must attribute the
variations in the relative volumes of the elements. The correctness of this conclusion
was further confiymed by reference to the atomic constitution of a numerous series of
compounds ; but prior to entering into details, reference was made to those elements
which possess the peculiar power of condensing upon their surfaces the molecules of
the surrounding medium.
Attention was called to the fact that elements or compounds possessing a small
atomic volume are invariably found to be endowed with this property, provided the
atomic weight is sufficiently high.
Thus carbon, an element remarkable for its power of effecting surface condensa-
tion, not only possesses a small atomic volume, but the smallest of any known element.
Again, the atomic volumes of zinc and platinum are equal, but their atomic weights
differ widely, that of zinc being 33 and of platinum 98 ; thus in this group of elements
we find that the one possessing the greatest power of inducing surface condensation
is the one endowed with the highest atomic weight. Other comparisons of a similat
character, and leading to a similar result, induced the author to believe that ‘“ surface
condensation is caused by the cohesive attraction of the solid exerted upon the sur+
vounding molecules of gas,” This idea was put forth some time since by Dr. Faraday,
: hanes 5x
68 REPORT—1860.
The author further extended it by supposing that the amount of the power of effect-
ing surface condensation is dependent upon, and corresponds with, the actual weight
of the atom, but that the repulsive force which keeps the atoms asunder, acting
in a contrary direction to the cohesive force, prevents that cohesive force from per-
ceptibly acting upon the molecules of the medium in which the atom is placed.
Resuming the consideration of the atomic constitution of compounds, particular
attention was directed to the fact that, in a series of compounds of one metal (oxide
for instance), it would be found that the compound possessing the most neutrality (the
least activity) would have the greatest atomic number. The term “ atomic number ’”’
was defined as ‘‘denoting the total number of elementary atoms capable of being
contained within the space which would be filled by a single atom, of hydrogen.”
The numbers brought forward by the author were quoted from Gmelin’s works; but,
as Gmelin’s atomic numbers denoted the number of compound atoms capable of being
contained within a given space, his (Gmelin’s) numbers were by the author multi-
plied by the total number of elementary atoms contained in an atom or equivalent of
the compound. Thus, taking equal budks of lead and oxide of lead, it will be found
that if the lead contains 1218 atoms, the oxide of lead will contain 1888 atoms, half
of them oxygen, and the other half lead atoms, The following, amongst other series,
were brought forward :—
Atomic number.
fCPromium. pees naciecs* DOE Hs .0i6 0,0 Ave.euevieia LACUVEs
Sesquioxide of chromium.. 8610 ............ Neutral.
Chromicideigunen acs este F200 ae aa idiee ue ea ACHIVES
1,
Manganese, .......++6+. 3220 ..00.4.ee0+6 Intermediate,
2 Protoxide of manganese .. 2948 ............ Most active.
* ‘) Peroxide of manganese.... 3777 ........+.+. Neutral.
Manganic acid ......... ?
TYOM (5 shaven side lara! sarawa MOS ORs.“ sbive a ssarente se deel OSGEaC Limes
3 Magnetic oxide......... 3486 ............ Intermediate.
* ‘)Sesquioxide............ 3715 .........+s- Most neutral.
errieacid pea aecinasiss anal?
Lead’. cine cuieasone vacees, L2LS epi leetiwe enn UV LOstiapinres
Oxide ditto ............ 1888 :
4. PEGE: © Sa Utiget e LLOBSI ee Re Intermediate.
Peroxide of lead ........ 2475 .cceeveecee. Mostineutral.
Mercury Perchloride,.... 878 .....0s.+.+. Most active,
5. 4 Ditto Protochloride ...... 975 ............ Intermediate.
Mercuryis:). sscccs carves L480 vspcavess cscs, east mctives
Thus in the first series quoted the compound endowed with the most inactivity, the
most neutrality, possesses also, of the three, the greatest atomic number, so that in the
union of two atoms of chromium with three atoms of oxygen in the production of this
compound, viz. the sesquioxide, considerable condensation must occur, Chromium
is chemically active in one direction, oxygen in another; and on bringing the two
together, the opposing forces appear to neutralize, and balance each other ; if the pro-
portion of oxygen is increased, if one atom of chromium is united with three of oxygen,
a compound is produced, not neutral, but endowed with great activity ; and connected
with that activity is the important fact, that its constituent atoms are wider apart
than the constituent atoms of the sesquioxide, the neutralmember of the series,
Examining the succeeding series in a similar manner, equally striking and interesting
results were obtained.
The paper concluded with the following remarks :—
To seek for an explanation of the phenomena we have been studying is a natural
impulse; that an explanation cannot be given without resorting to hypothesis is very
obvious ; but if an hypothesis can be advanced which will connect the facts together,
which will tend to enlarge our views upon the subject, and which will not be incom-
patible with well-known and established facts, surely that hypothesis, whatever it
may be, is worthy of our present attention. There is no need to imagine the existence
of any new force, any new agency; the whole of the phenomena can be satisfactorily
TRANSAOTIONS OF THE SECTIONS. 69
accounted for on the supposition that the force which gives chemical activity to the
atom is identical with the force which keeps the atom asunder, and that the cohesive
power of the atom is represented by its weight. ‘Thus potassium has a powerful
chemical force, an electro-positive force (if we are so pleased to name it), and that
force confers activity upon the atom, and by its self-repulsive nature keeps those atoms
widely asunder, Chlorine has an activity of quite an opposite character, an electro-
negative activity, and the self-repulsive nature of that force keeps its atoms widely
apart, But when the two elements are brought together, the activity of the one de-
stroys the activity of the other, the repulsive force of the one destroys that of the other ;
consequently the coliesive force (a force represented by the weight of the atom)
immediately comes into play, and its effects are manifested by the great condensation,
the permanent character of the resulting compound. The argument then is, that it
is chemical force or electrical attraction (for the two terms are by many considered as
synonymous) which determines the combination of atoms; but that, when combina-
tion actually occurs, the very force which occasions it is masked, neutralized, the
elements of the compound being merely held together by the cohesive force, which
corresponds with and depends upon the absolute weight of the atom.
In conclusion, the author reminded the members of the Section that the hypothesis
advanced should be considered separate and distinct from the numerous facts which
it had been his object to bring before their notice,
On a new Organic Compound containing Boron,
By Dr. FRANKLAND and B, Duppa.
The authors exhibited a new body obtained by the action of zinc-ethyl on boracie
ether, in which the whole of the oxygen in boracic acid is replaced by ethyl, B(CH,).
This boric triethide is a colourless, mobile liquid, spontaneously inflammable. ‘The
authors are engaged in investigating the corresponding reaction on the ethers of car-
bonic, oxalic, and silicic acids.
Chemical Notes. By Dr. GLavstonz, F.R.S.
The first of these notes referred to the gradual reduction of hydrate of cresyl into hy-
drate of phenyl and other compounds through the agency of chloride of calcium or zinc :
the second described a crystalline precipitate obtained by the addition of hydrofluoric
acid to molybdous chloride: the third showed by an analysis of the diffusate, that when
equivalent proportions of choride of sodium and nitrate of baryta are mixed together
in solution and diffused, four salts exist contemporaneously in the liquid; or in other
words, a portion of each acid combines with a portion of each base; thus affording an
additional evidence of the generality of the law of reciprocal decomposition,
On the Transmission of Electrolysis across Glass.
By W. R. Grove, Q.C., F.RS. Sc.
If glass, or an equally non-conducting substance, be interposed between electrodes
in an electrolyte, so that there be no liquid communication around the edges, it is
hardly necessary to say that, according to received opinions and experiments, no
current passes, and no electrolysis takes place. Mr. Grove was led by some theoretic
considerations to think that this rule might not be without an exception, and the follow-
ing experiment realized his view:—A Florence flask, well cleaned and dried, was
filled two-thirds full of distilled water, with a few drops of sulphuric acid added to it,
and placed in an outer vessel, containing similar acidulated water, and which reached
to the same height as the liquid in the interior. A platinum wire was passed through
a glass tube, one end of which was hermetically sealed to the platinum, so that a small
part of the wire projected beyond the tube. This tube passed through a cork fitted to
the flask, and the platinum point was dipped into the liquid within the flask, anda simi-
lar coated wire was dipped into the outer liquid, and the two wires connected with the
extremities of the secondary coil of a Ruhmkorff’s apparatus. Upon the latter being
excited by the battery, a stream of minute bubbles arose from both the platinum points,
proving that electrolysis took place notwithstanding the interposition of the glass. The
portions of the flask above the liquid, both outside and inside, were perfectly dry, so
70 REPORT—1860.
that there could have been no communication of the current over the surface of the
glass. This was further proved by removing the outer wire a short distance from the
liquid, when sparks passed nearly equal in length to those between wires from the ter-
minals. As the outer wire was further removed, keeping it near the flask, sparks
passed along the surface of the latter for a short distance; and as it was further re-
moved from the liquid, still being near the flask, they ceased, thus showing that there
was no passage of electricity over the upper and unwetted surface of the glass. With
unacidulated water no electrolysis was observed, nor when a battery of thirty cells
was used instead of Ruhmkorff’s coil. In the first experiment the evolution of gas
gradually diminished, and ceased in about twenty minutes, but recommenced on rever-
sing the current. Mr. Grove concluded that the electrolysis was effected by induction
across the thin glass of the Florence flask, and that its cessation indicated something
like a state of charge or polarization of the surface of the glass.
On the Oxidation of Potassium and Sodium. By A. Vernon Harcourt,
On the Composition of the Ash of Wheat grown under various circumstances.
By J. B. Lawes, F.R.S., and Dr. J. H. GitBerr.
On the Atomic Weight of Oxygen. By Prof. W. A. Mitier, M.D., F.RS.
In this paper the author pointed out some practical objections to Gerhardt’s pro-
posal for doubling the atomic number for oxygen.
~ It has been stated that one advantage which would be obtained by adopting the pro-
posal, would be that it would remove all inconsistency in the vapour volumes of all
compound bodies by representing them all as of equal volume.
The author commenced by showing that this assumed consistency was only imaginary,
inasmuch as such uniformity does not exist in nature. In addition to the differences
existing between the vapour volumes of the protoxide and deutoxide of nitrogen, similar
irregularities exist in the volume of chlorous acid, and of bisulphide of mercury and
some other bodies.
The practical objections, if a notation in harmony with this view were adopted, were,
he stated, of still greater weight, and might be summed up as follows :—
1. The ordinary notation is known to every one who has made the science of che-
mistry his study. 2. All the memoirs, with the exception of a few in later years, are
written in accordance with this system, and a change of notation would at once render
these memoirs less easily accessible and intelligible. 3. The new notation required
would not be in harmony with the language of chemistry, NO, for example, would be
called binoxide of nitrogen, but written as a protoxide. 4. The present system of
notation is capable of expressing all the later theories with perfect precision, while it
is applicable to the older views; but the new notation is not applicable to many of the
older views. By the ordinary notation, nitrate of potash, for instance, may be repre-
sented either as a compound of potash and nitric acid (KO, NO,), or as a combination
of potassium with nitrion (K, NO,), or as an aggregation of particles without indicating
any specific mode of combination (KNO,); whereas, in the new notation, unless its
principle is abandoned by doubling the formule, it is impossible that (KN Q,) should
be represented as formed of potash and nitric acid. It would therefore be a retro-
grade step thus to exclude from our notation the power of indicating the constitution
of a large class of compounds upon a view which has long been more or less prevalent.
5. Any extensive change of nomenclature or of notation, while the truth of the
theory upon which it rests is still under discussion, cannot but lead to serious incon-
venience. If such a practice were admitted, every new theory would be privileged to
introduce a new language, which, in a continually progressive science like chemistry,
would soon give way to an equally transitory successor. Chemistry, it must be re-
membered, is not merely a science: it is also an art, which has introduced its nomen-
clature and its notation into our manufactories, and, in some measure, even into daily
life; it is therefore specially necessary to beware of needless innovation. Any system
of notation, it must also be borne in mind, is a mere artificial contrivance to represent
to the mind certain changes or certain hypotheses ; and to argue for a system of nota~ ~
_—
TRANSACTIONS OF THE SECTIONS. 71
tion as though it were anything more, as has sometimes been done, shows a want of
true appreciation of its meaning.
The question to be considered is not simply, what is in the abstract the best mode
of notation, but what, considering all the circumstances of the science, possesses the
greatest advantage. ‘That system of notation which is consistent with itself, and
which lends itself most completely to the expression of the various theories and aspects
of the science which have been maintained,-or may be maintained, is therefore, philo-
sophically speaking, the best. And such grounds, it appeared to the author, exist
for continuing to use the system hitherto generally adopted.
The question of notation, it was observed, is entirely independent of Gerhardt’s
theory of the atomic constitution of the elements to which he proposes to apply it, for
even those who admit the truth of his hypothesis may still express it by the ordinary
mode of notation.
Remarks on the Volume Theory. By C. Mortrz von Bost.
It is endeavoured to show that the theory of volumes which separates gases from
other bodies must be untrue; that there is no generic difference, but a difference of
degree only between gases on the one hand, and solid and fluid substances on the
other; that therefore the three states of aggregation may be considered under the
Same aspect.
And it is suggested that one equal standard be introduced for the specific gravity
of gases and other substances ; and that the attention of mathematicians be drawn
to the numbers of equivalent weight and atomic volume (as obtained on using equal
standard), with the view to solve the question whether those numbers being inter-
preted as relative distances of equivalent masses, chemical processes can be accounted
for by the law of gravitation.
On a New Acetic Ether occurring in a Natural Resin.
By Warren De ra Rue, F.R.S., and Dr. Huco Miuer.
On the Isomers of Cumol.
By Warren De 1a Ruz, F.R.S., and Dr. Huco Miuuer.
On the Representation of Neutral Salts on the type of a Neutral Peroxide HO,
instead of a Basic Ovide H,O,. By Lyon Prayrair, Ph.D., F.R.S.
On the Analysis of some Connemara Minerals. By Tuomas H. Rowney,
Ph.D., F.CS., Prof. of Chemistry, Queen's College, Galway.
Connemara Andalusite——Occurs in right rhombic prisms, having apparently the
same regular measurement as the Tyrol mineral; it has a rhombic cleavage, rather
eminent but interrupted; lustre of cleavage planes rather high, and somewhat resinous ;
colour of fracture reddish purple ; the cross fracture is dull. Occurs in a vein of mica-
ceous schist associated with quartz and a silvery mica, apparently magnesian, Faces
of crystals slightly blistered.
Specific gravity 3-070.
BOA evi Veetenaae Tides tet ee GCOS
IMMUNE coal aniterinwenree us a3 case. COTS
Sexquioxide-of ifon c.40ds<sgasacce, 18
PMs Uncen ae Maendeauaece, 1°70
HEASNERIN vlensite aot yy scans sy) | 80
Traces of manganese ......... 95°33
see ”
Connemara Pyrosclerite.—Bluish green ; lustre somewhat waxy on the surface of a
fracture, translucent; bears a polish, but not very high, owing to its being rather soft ;
contains arborizations like those of moss-agate, generally of a brown and dark green
colour; readily reduced to powder, and is decomposed by strong acids without gela-
tinizing.
72 REPORT—1860.
Specific gravity 2-604.
Silica scree eee tine AS SOO R ED Ot . 3471
ATUMINGs 4 cscs sutsactieles siete clove = Weare of fe iis}
Magnesia fais sie)+ -,s)biieje> sfeyeltyorseleele 36°56
IWiatere cca Gre mee cpiatercieisls acfeute een terne 11°49 99°94
Connemara Garnet.—Occurs in rhombic dodecahedrons with bevelled edges; faces
of crystals have a metallic Justre, colour resembling bronze. The matrix appears to
consist of the same mineral mixed with epidote.
Specific gravity 3°585,
39°77
Sbtei Als doc seve Sen toto boe AAO
i\linitnzy. Bptiadigao aac oeopouepoe . 15°49
Sesquioxide of iron ........00+-000. 16°27
LU ido. CApOOR SOOSHOTOG cur oO. ». 20°98
VEL ORESIA boyy vuptc; afer) efecev els fol stalo' Ada ge cKO
Minnganese ters e's io. « aie ale > seseeee *48——100°05
Analysis of the Matrix.
Specific gravity 3°404.
Si ieeaa wacveys basen foieimverassbel svolovalsielerensienere tise am.
Alumina ........- stew sets's vlc clle > ve LOrok
Sesquioxide of iron ........: ..+.-. 1511
Gimie!. 2 sya leite. pe aseeenee Bteis islets state) eae
Magnesia ......... Secetiahice aiecenanicceone PL
Traces of manganese ..... wesc vets ——99°21
On the Composition of Jet. By Tuomas H. Rowney, Ph.D. F.CS.,
Prof. of Chemistry, Queen's College, Galway.
The following results were obtained by the analysis of two specimens of jet and of
a very pure coal, a portion of a fossil plant :—
Jet No. 1. Jet No. 2.
Specific gravity 1:2655 Specific gravity 1:1743
Coke. dates cha APE O! een cscs core atv aehe tliye 27°38
Volatile matter.. 58°81 Srscaas ae tele ; 72°62
100:00 100:00
Gaxbon, bi. bh.ccc ND GON sis oekaateeie hiesote choles 80:05
Hydrogen...... GZ erryaita = save taps fohrrasohe) sis 7°21
Nitrogen ..... aig dled tae eral sis rs. « usaeaeveves els 1-44
say pe diLAN- Cea tiaiiri es meee 2 10°50 ..
xygen
PASH tees s\a'0)5 810 23.0 iS MOA PP ete BS teteissa sys SOM.
100:00 100°00
On Waterproof and Unalterable Smatll-arm Cartridges.
Coal.
1:2860
71°65
28°35
100-00
82°70
5°42
1:77
imams UL
cles
100-00
By T. ScorFern.
On a New Form of Blowpipe for Laboratory Use.
By Dr. HerMANN SPRENGEL.
Mr, Symons exhibited some forms of Alkalimeters suggested by Mr. Wiers,
On Thiotherine, a Sulphuretted Product of Decomposition of Albuminous
Substances.
By Dr. Tuupicuum.
TRANSACTIONS OF THE SECTIONS. 73
On the Occurrence of Poisonous Metals in Cheese.
By Professor VoELCKER.
The author stated that he had detected both copper and zinc in cheese: in some
specimens copper, in others zinc, and in some both copper and zine were found. The
description of cheese in which these poisonous metals were found was double-Glou-
cester cheese. Skimmed-milk cheese, which was likewise examined for copper and
zine, did not contain any metallic impurity. Stilton, and other varieties of cheese,
have not as yet been examined; it must not therefore be inferred that cheese made
in other districts than Gloucestershire contains poisonous metals. Inquiry in the
dairy districts of Gloucestershire and Wiltshire has led to the discovery that in many
dairies in these counties sulphate of copper, and sometimes sulphate of zinc, are
employed in the making of cheese. The reasons for which these prejudicial salts are
added to the cheese are variously stated. Some persons added sulphate of zine with a
view of giving new cheese the taste of old; others employed sulphate of copper for
the purpose of preventing the heaving of cheese. Dr. Voelcker also stated that he
had found alum in Gloucester cheese, and mentioned that he had Jearnt that in some
dairies alum was employed to effect a more complete separation of the caseine from
the whey.
On the Causes of Fire in Turkey-red Stoves. By Dr. W. WALLACE.
GEOLOGY.
Notes on two newly discovered Ossifevous Caves in Sicily.
By Baron F. Anca.
Founp in the Grotta de Olivella, near Palermo. Molar of Eleph. Africanus (the
existing species), amidst bones and teeth of an extinct species of Hippopotamus, both
in a well-marked fossil state, and infiltrated with hydrate of iron.
Grotta de San Feodora, Molar of Eleph. Africanus, with abundant remains ; upper
and lower jaws of Jiyena crocuta, determined by M. Lartet.
Facts go to prove continuity of land between Sicily and the African continent, pro-
bably along the line of the Adventure Bank of Admiral Smyth, stretching between
Capo Bono, the promontory of Tunis and Marsala. The Admiral found only 75
fathoms sounding upon the bank; but a deep sea to the north and to the south.
Proofs of continuity with Sicily are found at Malta.
Details respecting a Nail found in Kingoodie Quarry, 1843.
By Sir Daviv Brewster, K.H., D.C.L., F.RS.
On the Stratigraphical Position of certain Species of Corals in the Lias.
By the Rev. P. B. Bropiz, IA., F.G.S.
The author first alluded to the exact position of a species of Coral found in the
Hippopodium bed near Cheltenham, and another locality near Evesham, where the
same form was equally abundant. Another and distinct genus, a Monilivaltia allied
to M. Stutchburyz, was procured in the same bed in Warwickshire, associated with
numerous other fossils, and a section of the pit was given, Other and distinct species
of Corallines, one of which frcm Gloucestershire belongs to the genus Cladophyliia,
were known to occur lower down in the ‘ Lima beds,’ the probable position of the fine
Isastrea Murchisoni, found occasionally in Worcestershire and Warwickshire. One
or more additional species have been met with in the bottom beds of the Warwickshire
Lias, which had not been previously observed so low down. The divisions of the
Lias, which seem to be characterized by the presence of Corals, are—1, the Hippo-
podium bed; 2, the Lima bed; 3, the White Lias; and 4, the Guinea bed. So that
it would appear that Corals are more numerous in the Lias than has been usually
supposed, and that they occupy certain zones in it, which future investigations may
show to be as well marked and distinctive as that of any other particular organisms.
74 REPORT—1860.
A few Corals have been recorded from the Upper Lias, but they are smaller and less
frequent than the above.
On the Velocity of Earthquake Shocks in the Laterite of India.
By Joun ALLAN Broun, F.RS.
Mr. Mallet’s interesting observations on the velocity of earthquake shocks had
drawn my attention to the subject ; and when earthquakes were remarked in Travan-
core, the part, South of India, where I resided, I endeavoured to add something to
our knowledge of the subject.
Four earthquakes were perceived in Travancore during the year 1856; that to
which I am about to allude was observed at the Trevandrum Observatory, August 22,
where the commencement of the shock was noted accurately by the Observatory
clock, at 4" 25™ 10° of Trevandrum mean time. The magnets in the magnetic
observatory were dancing up and down with sharp jerks, but without any change
of mean positions; a vessel containing water was wetted highest on the points to
W.N.W. and E.S.E. The vibration of the bifilar magnet was 3°0 scale divisions a
few minutes after the shock. On the 11th of the same month a shock had been
felt at Trevandrum, and I had addressed a circular to several persons in the district
for information as to the time, direction, and character of the shock: this circular
had drawn attention to the questions of interest in connexion with such shocks.
One gentleman at Quilon (thirty-seven miles N.W. of Trevandrum) was writing
an account of the former shock when the shock of August 22nd occurred. Four
gentlemen and one lady noted the time of the shock at Quilon; these times were
as follows :—Mr. D’Albed’yhll and Mr. Newas (same watch), 45 20"; Capt. Carr,
4h 95™; Mr. Stone, 4°19"; Mrs. Wilkins, 4" 16". A box chronometer by Dent
was sent by me to Quilon, for the purpose of comparing it with the different
watches or clocks used in the determination of the time of the shock: the rate of the
chronometer was +8 seconds, and the error was determined before and after the
comparisons, which were made August 27th. The following are the facts connected
wth the observations :—Mr. Newas had set his watch, on the 17th of August, to
6" 0” at sunrise; allowing for the height of the chain of Ghats where the sun rose,
I have computed that sunrise must have been about 3 minutes before six o’clock :
the watch had been allowed to run down after the shock, so that it could not be
compared with the chronometer. Supposing the watch without any marked rate,
the Trevandrum mean time of the shock was 4" 183™. Mr. Stone had set his watch
August 17, by the time of the Trevandrum Observatory (where a ball is dropped
daily at eleven o’clock). When compared with the chronometer, it had gained 3™ 35°
giving a daily rate of about +21°°5; so that on the 22nd the error of the watch
must have been about 1™ 47%, and the shock must have occurred about 4" 171™
Trevandrum mean time. This is by far the most important observation; the others
can be considered only as approximate determinations. Capt. Carr’s watch was
found fourteen minutes fast of Trevandrum time on the 27th; supposing the rate
zero, the time of shock was 4" 11”. Mrs. Wilkins’s clock had been compared with
the mess clock of the native regiment at Quilon, which was regulated by persons
proceeding from Trevandrum, with the Observatory time, and which was found
correct when compared with the chronometer. Mrs. Wilkins’s clock was three mi-
nutes slow of Trevandrum mean time, making the time of the clock 4" 19", The
four observations, therefore, corrected to Trevandrum mean time, gave—
hm hm
Mr. NewaS..eeseeeeeees 4 183 | Mrs. Wikins+.i..c..sc00 4005
Stones. ces geepreen a lee The mean gives.......... 4 16%
Capt. Catre..seeeeeeeee 4 11
There can be no doubt that Mr. Stone’s observation is the most trustworthy, as
his time depends on two comparisons with the Trevandrum Observatory, viz. on the
17th and 27th; and the deduced error for the middle of the interval (the 22nd) can-
not be far from the truth. Mr. Newas’s observation, which agrees with it within
about a minute, depends wholly on the observation for the sunrise ; it is so far con-
firmatory. Rejecting Capt. Carr’s observation, as differing too much from the others,
the mean of the remaining three is 4" 18}.
If we suppose the shock to have travelled in the direction from Quilon to Trevan-
TRANSACTIONS OF THE SECTIONS. 75
drum, which does not differ much from that indicated by the vessel of water, and
take the distance at thirty-seven miles, we obtain a velocity of propagation of 470
feet per second; and if we take the latest result at Quilon, or 4" 19™, we have still
a velocity of only 530 feet per second—-little more than three-fifths of that found.
by Mr. Mallet in wet sand. If we take the W.N.W. as the direction of propaga-
tion of the shock, or any other than that direct from Quilon, the velocity will of
course be diminished. It should be remarked that the laterite, which forms the
upper stratum (about 30 feet deep) between Quilon and Trevandrum, is a clayey
rock, in a semi-pasty condition of perhaps the lowest degree of elasticity ; and the
laterite reposes in some places on strata of sand and clays.
On the Course of the Thames from Lechlade to Windsor, as ruled by the
Geological Formations over which it passes. By the Rev. J. C. CLurTer-
Buck, M.A.
The tortuous course of the Thames between Lechlade and Windsor shows that
there must be some physical cause which obliges it to deviate from the straight line
it would naturally take to its outfall. This is found in the obstructions encountered
in its passage over or through the various strata, From Lechlade to Sandford the
river finds its bed in the Oxford clay; it then passes through a narrow gap in the
middle oolite to the Kimmeridge clay, holds its course on that clay, under the
escarpment of the Iron-sand in Nuneham Park, turns the escarpment at Culham,
passes to the Gault at Appleford, touches a ledge of the Iron-sand at Clifton Hamp-
den, returns to the Gault, enters the Greensand near its junction with the Thame
stream, passes to the Chalk, in which it finds its bed to the point,—which is the limit
proposed for consideration, The natural obstructions are found at the junction of the
different strata. The quantity of water flowing down the river, whether issuing in
perennial springs, or thrown from the surface in flood, is due to the geological condi-
tion of the district. The tributaries or feeders discharge more or less of perennial or
flood water, as they carry the water from permeable or impermeable strata. The
flooding of the district necessarily affects the sanitary condition of Oxford. The city
itself is placed on a bed of gravel, overlying the Oxford clay, the surface of which
undulates so that the water is stanked back in the gravel ; it was cutting through one
of these undulations, in carrying out the Jericho drainage, that deprived many wells
in Oxford of their water. As this bed of gravel extends beyond the limits of the city,
on the subsidence of the floods, the water filtrates through the gravel, and thus
noxious evaporation is diminished. Considerable accumulations have raised the bed
of the river in many places, evidence as to the date of which is found in antiquities
which have been discovered when constructing locks or weirs, or in dredging for gravel.
At Sandford, arms of the time of Charles I. have been found 8 feet below the river-
bed, relics of greater antiquity and at various depths have often been found in other
places, where the bed of the river has been raised, or, as in some cases, entirely
changed its course. The phenomenon of the formation of ice at the bottom of the
stream, when the temperature falls to 20 Fahr., and the transportation of stones from
the bottom by the ice rising to the surface, adds to the natural obstructions in the
stream, and hinders the passage of the flood-waters by which so much damage has
been done at various times in the neighbourhood of Oxford. The paper, which
entered into full details, was illustrated with a map, sections, and diagrams,
Photographs of a Paddle of Pliosaurus of great size, found at Kimmeridge, were
exhibited by Mr. R. Damon, of Weymouth. =
Remarks on the Elevation Theory of Volcanos.
By Professor Dauseny, M.D., F.R.S.
This paper was chiefly intended as a protest against the assumption of certain geo-
logists, that because it had been shown, more especially by Sir Charles Lyell in his
memoir published in the ‘ Philosophical Transactions’ for 1858, that sheets of compact
lava have been formed on steep inclines, it therefore followed, that all voleanic moun-
tains have been built up by a series of successive eruptions.
Not denying that this explanation may serve for the oldest, as it certainly does for
the more recent beds, which constitute such mountains as Etna and Vesuvius, the
76 REPORT—1860.
author contended that it is not applicable to the celebrated case of Jorullo, as described
by Humboldt, nor yet to the volcanic islands thrown up in deep water at various times
during the historical period.
He was also disposed to refer the four trachytic Puys near Clermont, in Auvergne,
as well as the still loftier Cones composed of the same material in the Andes, which
Humboldt describes, rather to the upheaval of a softened mass of rock, than to the
outburst of liquid lava.
He appealed also to the crater-lakes in the Eifel country and elsewhere, as furnish-
ing cases of upheaval, even where no lava had been ejected; and argued, that so long
as the idea of paroxysmal action continued to be entertained with reference to rocks
in general, it was probable that volcanic countries, above all others, would be subject
to such operations.
On the Mode of Flight of the Pterodactyles of the Coprolite Bed near Cam-
bridge. By the Rev. J. B. P. Dennis, F.G.S.
Coprolitic remains of Pterodactyle bone have afforded an opportunity of studying its
microscopic characters, and this had led to the present attempt to show from the ana-
logy of other flying animals, from the different modes of flight among birds, from the
apparent adjustment of the haversian canals thereunto, and the harmonious perfection
of the skeleton with the adaptation of the pectoral muscle to the same (so that even the
humeral process of its attachment has its marked characteristics), that these and other
analogies lead to the inference that considerable knowledge even of the mode of flight
of this extinct reptile may be obtained from the study of its microscopical bone struc-
ture. In elucidation of this subject, a brief account was given of the structure of the
wing-bones of a bird, and of the mode of flight of the Gull, a bird distinguished for
its elasticity and endurance on the wing, and in other respects very suitable for illus-
trating the subject.
A description was then given of fragments of Pterodactyle bone obtained by Mr.
Barrett from the coprolite bed, most of which were portions of wing-bones of very
thin texture. It was also shown that the Pterodactyle required not to be encumbered
with muscular legs, and thus the vastus was only sufficiently developed to enable the
animal to spring from the ground preparatory to flight (as the form of the femur also
seemed to indicate); also the biceps, semitendinosus, &c., or their analogues, did not
require any great development; while the gastrocnemius, as it would assist in the
spring, was probably on that account fairly represented. The pectoral muscle, follow-
ing the saurian type, must have been less voluminous than that of birds, flatter, with
its greatest development in front, and in position comparing somewhat with that
muscle in gulls and owls, birds of elastic but not rapid flight. The Pterodactyle was
also shown to agree more with birds than with bats, especially in its omoplate, while
the absence of a fercula implied no similar volume of muscle; the bones in like man-
ner were permeated by air, or if some were not, they were yet filled with a light fatty
substance or marrow to give additional strength to their light texture; and though the
natural weakness of its muscular powers was considerable in comparison with birds,
yet this was balanced by an extremely light framework, the weight of which predomi-
nated in front, where the muscular force was more directly antagonistic; and above all, the
admirable microscopic structure of its bone eminently conduced to its powers of flight,
Delicate in the extreme to the unassisted eye, when examined under the microscope,
the bone is found to contain numerous and large haversian canals in a very marked
degree, comparing in their arrangement with those seen in the wing-bones of gulls;
also lacunz well displayed, larger than those of a bird of flight, long and fusiform.
From this correspondence of the characters of the haversian canals, of which illustra-
tions were given, an inference seems capable of being drawn in reference to the flight
of these large Pterodactyles, which, if they did not possess the dash of the falcon or the
impetuosity of the wood-pigeon, yet sailed gracefully over primzeval seas with a lizht-
ness and buoyancy, as it would seem, analogous in some degree at least to the con-
spicuous grace of the gulls, which are the present ornament of our coasts. So in every
respect is seen the wisdom displayed in the adaptation of means, each inadequate
in itself, and the result is the production of one of the strangest anomalies, of
which, if we had not had the clearest testimony, the imagination would have failed to
picture,—a true Pterosaurian, in some respects perhaps more wonderful in its con-
struction than bats or even birds, and being as fully capable of flight as they, teaching
TRANSACTIONS OF THE SECTIONS. 77
us how great are the resources and how infinite the wisdom of Him who has done all
things well,
On the Corrugation of Strata in the Vicinity of Mountain Ranges.
By the Rev. J. Dineie.
This paper was in continuation of an attempt to determine the mechanical causes
of the formation of the earth’s crust, and to trace its progress. The author described
the varying forms of flexure, diminishing in intensity with their distance from the
igneous axis, which characterizes the strata in the neighbourhood of the mountain
chains; and showed how this form would arise from the action of the molten interior,
by referring to the result of experiments upon the action cf fluids under like condi-
tions. He expressed his obligations to Professor Rogers for the valuable information
which he had derived from a paper of his in the Edinburgh Transactions, but de-
murred to some of his hypotheses. Flexures at definite points must be produced by
repeated or continued pressures, and not by paroxysmal action. The latter chiefly
spends itself in earthquakes and volcanoes, which, upon the whole, can produce no
continuous change of form, ‘The two forces, however, seem to be intimately related
to each other; and if we suppose the one to be only the other in excess, we are
supplied with a simple explanation of the connexion between the corrugated moun~
tain chains and the lines of earthquakes and volcanoes.
As a corollary from the above views, it might be observed that they destroyed the
idea of any distinct theory of volcanoes of elevation or eruption, as the quantities of
elevated or ejected matter in the case of a fissure or a ruptured corrugation might be
in any proportion whatever to each other.
Remarks on the Ichthyolites of Farnell Road.
By Sir Purrip ve M. Grey Ecerton, Bart., F.R.S.
At the Meeting of the British Association last year at Aberdeen, I had an oppor-
tunity of examining several speciimens of the small fishes found in the Old Red Sand-
stone deposits of Farnell, and in the discussion which ensued upon the reading of
Mr. Mitchell's paper, I took occasion to remark upon their several characters. I then
stated that all the specimens I had seen belonged to the family Acanthodei, and the
great majority of them to the genus dcanthodes, representing, however, a new species
of the genus. I proposed inconsiderately to name this species 4. antiquus, a very
inappropriate title, inasmuch as two contemporaneous species were subsequently ex-
hibited by Mr. Peach. As, however, this name has not appeared in print, I propose
to cancel it, and substitute 4. Mitchelli, as the original or type-specimen is in the
possession of the Rev. Hugh Mitchell, of Craig. The other specimens I described as
constituting a new genus corresponding in many characters with Diplacanthus, but
differing in the shortness and position of the spines of the fins. I proposed for this
genus the name Brachyacanthus.
The specimens from the same locality recently received from Mr. Powrie are of the
same species as those examined at Aberdeen. I learn, however, in a letter received
from Mr, Powrie since I have examined his specimens, that he has in his possession
others comprising at least two’ very distinct species of Dipiacanthus, one remarkable
for its very strong anterior dorsal spine, and fragments belonging probably to other
species. Mr. Mitchell also writes that another locality has been found rich in remains
of Acanthodian and other fishes. Under these circumstances it would be premature to
enter into any detailed account of these interesting ichthyolites. As the materials, how-
ever, are sufticiently complete, I append a short description of Acanthodes Mitchelli.
The specimens I have examined vary in length from 2 to 23 inches. The one I
have selected for description attains nearly the latter dimensions. The greatest depth
of the trunk occurs in advance of the ventral fins, where it measures rather more than
half an inch, The head is small and elegantly sculptured. It measures about 1th of
the total length. ‘The outline of the body is very graceful. It is fusiform anteriorly,
and tapers gradually posterior to the insertion of the highly heterocerque tail. The
orbit is placed very forward, and is embraced by the remarkable bony plates described
by Romer as characteristic of the genus. ‘The peculiar structure of the gill-covers also
corresponds with that of other species of 4canthodes, The pectoral spines are long
and curved. The other fin-spines are slender and straight. The species differs from
all others of the same period in the ornament of the head-bones and the form of the
78 REPORT—1860.
body. It is distinguishable also from Acanthodes Peachi, a new species discovered
last year by Mr. Peach in the Caithness flags, by the form of the spines, the pectoral
spines in the latter being straight, and the dorsal and anal spines curved.
Photographs of Fishes, from Farnell in Fifeshire, were exhibited by Mr. W. Rocers,
of Montrose.
On a New Form of Ichthyolite discovered by Mr. Peach.
By Sir Pattie Ecerton, Bart., M.P., F.RS.
This fossil fish, discovered by Mr. Peach in the Caithness flagstones, is chiefly re-
markable for the structure of the fins. The dorsal and anal fins are supported upon
three interspinous bones in each organ, from which the fin-rays spread in tufts. A
similar structure prevails in the caudal fin, It is nearly allied to Dipterus, and pro-
bably belonged to the Ccelacanthoid family. The name Tristichopterus alatus has
reference to the peculiar structure characteristic of the genus.
On Circular Chains in the Savoy Alps.
By M. A. Favre, Professor at the Academy of Geneva.
The object of this memoir is to describe the peculiar structure of the mountain
chains in Savoy, on the left bank of the river Arve.
This region may be divided into several districts, which, in passing from Mont
Saléve to Mont Blanc, are as follows: (1) the Tertiary, (2) the Cretaceous, (3) the
Jurassic, and (4) the district of crystalline rocks. M. Favre treats of the second of
these, in which the mountain chains surmounted by precipitous peaks are composed in
great part of cretaceous rocks. This district is about 49 kilometres long from the
river Arve to the lake of Annecy, by 24 broad. The loftiest mountain attains the
height of 2760 metres above the sea-level, and there are several other summits be-
tween 2300 and 2400 metres high. The geological formations which constitute this
district are,—1. the Jurassic which occupy a very limited space; 2. the Neocomian;
3, the Urgonian, which forms enormous escarpments, and constitutes the crest of the
mountains; 4. the green sandstone; 5. the chalk; 6. the nummulite limestone ; fis
the alpine macigno, which at its base contains various marls with fish scales, and
above marls and sandstones associated with the Taviglianas freestone which is a
species of volcanic cinder.
One of the valleys of this district, that namely of Thones on Grand Bornant, is a
longitudinal valley ; the others are transverse valleys watered by rivers arranged almost
like the radii of a circle. This peculiarity in the direction of these rivers depends on
that of the mountain chains; for the rivers in general cut the chain perpendicularly
to their axes, and with the exception of Mont Charvin a la Pointe Percée, all the
mountain chains of this district, and especially those on the borders, are in the shape
of a quadrant, and lie in every direction that can be found in a quadrant. It is to
these chains that M. Favre has given the name of circular chains.
Mountain chains have long been remarked whose axes are more or less undulatory,
others separating from a common trunk like the branches of a tree; strata, moreover,
have been observed that rise to the surface of the ground in the form of the bottom
of a boat; and the opposite phenomenon has likewise been observed, that namely of a
mountain chain in the form of a vault or half cylinder sinking so as to disappear in
the plain; but M. Favre is of opinion that the fact to which he has called attention is
different from any of these, insomuch as it refers to entire chains, which are not only
curved, but curved to such a degree that their extremities are at right angles to each
other,
M. Favre concludes his essay by calling attention to the fact that the chains of the
Alps display the closest orographical resemblances to those of the Jura, which are
now well known. Although the displacement of the soil is much greater in the Alps
than in the Jura, in both are found groups either entire or broken, which in the latter
case disclose in their interior, one, two, or three of the strata below that which forms
their crest; in both are found combes, ravines, and valleys of the same form. M.
Favre believes that the identity of these forms leads to the conclusion that the eleva-
tion of the Alps and the Jura is due to causes of the same nature.
TRANSACTIONS OF THE SECTIONS. 79
On some Transformations of Iron Pyrites in connexion with Organic Remains.
By AvPuonse GAGEs.
I have to direct the attention of the Section to some facts regarding the transforma-
tion of iron pyrites connected with fossil graptolites from Tinnaglough, Co. Wexford.
These peculiar characteristic fossils of the Lower Silurian schists are found very
often transformed into rhombic iron pyrites.
This transformation into pyrites is now, since the observations of Pepys and others,
easily accounted for, and therefore I have not to dwell upon it.
Looking over some of those schists, we may observe the various transformations
the fossil has passed through until it entirely disappears from the schist.
I. Fossil] exhibiting some traces of organic matter, and not mineralized by pyrites.
II. The same fossil transformed into rhombic iron pyrites.
III, The transformation of the pyritic fossil into a corresponding fossil of aluminite.
1V. A mere cast of the fossil, or indication of one only remaining.
And lastly, in some neighbouring joints of the schist, a thin layer of sesquioxide of
iron, alum, or of aluminite generally accompanied by free sulphur.
Analogous phenomena may be observed in other fossils of the carboniferous form-
ation, and especially in the lower limestone shale near Drogheda.
One may observe in some points in which the fossil has been completely obliterated,
a thin mineral layer of aluminous compounds, varying more or less in their chemical
constitution.
These facts are very suggestive in this sense, that if the processes of mineralization
going on for ages have served to preserve many forms of organic beings, so also they
serve to destroy them.
We witness every day the destruction of a great number of pyritic fossils hy the
mere action of air, and their transformation into sulphates, and sometimes, according
to local circumstances, into sulphates and free sulphur. Whenever sulphur occurs
in deposits containing organic remains, we are induced to believe that it has been
formed in somewhat a similar way.
On Snow Crystals observed at Dresden. By Dr. GEIN1Tz.
On the Silurian Formation in the District of Wilsdruff. By Dr. GrtniTz.
The discovery of Graptolites in the Lydit and Phthanit, lately made in the district
of Wilsdruff, near the villages of Limbach, Lotzen, and Lampersdorf, a neighbour-
hood where the azoic and metamorphic clay-slates, sometimes with true chiastolith,
are predominant, now combines a considerable part of the most northern part of the
Saxon Erzgebirge with the Silurian. :
These black schists of Graptolites, with Monograpsus triangulatus, Harkness, Mon.
priodon, Bronn, Mon. Becki, Barrande, and Mon. nuntius, Barrande, are continued in
the schists of Graptolites on the northern slope of the Erzgebirge near Langenstriegis,
not far from Frankenberg, Ober-Cainsdorf near Zwickau, Ronneburg, Oelsnitz, Hein-
richsruhe near Schleiz, and various places of the district called Voigtland, where they
indicate the same geological horizon as in Bohemia, the upper part of the Lower
Silurian, or the base of the Upper Silurian of M. Barrande. All the species found
in Saxony are described in the author’s ‘ Monograph of Graptolites,’ Leipzig, 1852.
On the Metamorphic Rocks of the North of Ireland. By Rosert HarK-
yess, F.RS., F.G.S., Professor of Geology in Queen's College, Cork.
Almost the whole of the county of Donegal is occupied by rocks which appertain
to the metamorphic series, consisting of gneissose rocks associated with limestones
and quartz rocks. ‘The relation which these several rocks bear to each other, and to
the syenitic masses which in some cases are found accompanying them, is well exhi-
bited in the sections along the north side of Lough Foyle, from Malin Head to Inis-
howen Head. On the S.W. side of Malin Head a protrusion of syenite is seen, which
forms an axis in this portion of Ireland; and reposing on this axis there are found,
first and lowest, quartz-rocks, succeeded conformably, on the north side, by flaggy
gneiss; and on the southern side a like occurrence commonly takes place, In somé
80 REPORT—1860.
localities, on the southern side of this axis, limestone frequently intervenes between
the underlying quartz-rocks and the overlying gneissose strata; and the limestones,
scattered in small patches among the metamorphic rocks of the north of Ireland, oc-
cupy this position with reference to the rocks of this character. The arrangement of
these rocks in this part of Ireland, as regards position, is as follows: the lowest quartz-
rocks succeeded by limestones, which are not persistent, but upon which, when present,
great masses of chloritic gneiss are seen having usually a S.E, dip, often the result of
reversed flexures. ‘Through these rocks, which are the Irish representatives of the
strata of the Grampians, numerous trap dykes occur.
Notes on the Geology of Captain Palliser’s Expedition in British North
America. By Dr. HeEcror.
The following remarks are explanatory of a section commencing at Lake Winnipeg,
continued along the basin of the Saskatchewan River to the Rocky Mountains, and
from thence to Vancouyer’s Island. his section is only intended to represent the
more general results of this geological exploration, as a preliminary to the reports
which are in preparation.
The rocks east of Lake Winnipeg have been fully described by geologists. They
are a part of the so-called Laurentine chain, and consist of granite and metamorphic
rocks. On these lie Silurian limestones, cherty, and of magnesian character, with
corals and shells, easily referable to Silurian types. Above these Mr. Hind has found
Devonian strata, of which, however, I saw no trace farther south. The supposed line
of their outcrop is marked by salt springs.
The first well-defined strata in the Prairie country occur 150 miles west of Red
River, and are indurated olive shales, with ferruginous bands and traversed by veins
of clay ironstone, with a few small fossils, chiefly fish-scales, and a small, neat species
of nucula. They are a deep-water deposit.
At the elbow of the Saskatchewan River, the banks are formed of purple laminated
clays, with lines of Septaria of various sizes, These Septaria yield fossils, which are truly
cretaceous forms. ‘The most common are Baculites and Inocerami, These Septaria
clays are also deep-sea deposits. ‘hey are again met with on the north branch of
the Saskatchewan, 150 miles to north-west, and the course of this river is for some
distance determined by these soft beds. At the Snake Portage, in lat. 54° N., L
thought I observed them overlaid by thick grits and clays, which must be next de-
scribed; but of this junction I am not certain, and the dip is so slight that they may
be even underlaid by these grits.
The latter strata, in beds often 200 feet thick, form high ridges, which range north
and south, crossing both Saskatchewans, and also the Red Deer River, at the Nick
Hills. They form mainly two parallel ranges, and between them occur clays with
coal or lignite beds from 2 to 10 feet thick, and consistent in their strike from north-
west to south-east. This coal is used at Fort Edmonton, and burns pretty well.
Some vegetable impressions, like those of cypress and dicotyledonous leaves, are found
in the shale, but no other fossils.
As these coal-beds and shales occur in the river-beds, and at low levels compared
with the surrounding prairie, it is manifest that the surface-beds of which these are
composed, are of later age; but whether conformable with them or not, I am unable
to say.
To the south-east of the elbow of the Saskatchewan, at the base of the Coteau de
Prairies, and at a locality on the Souris River known as the Roche Percée, is a group
of marls, with limestone bands, containing so much iron as to weather of a bright ver-
milion colour, and ash-coloured arenaceous clays, with their bands of lignite and
silicified wood. Selenite crystals are abundant in these marls, often clustered in stel-
late forms. ‘They are mixed with bands of grit, from a few feet to 30 feet in thick-
ness; and these being generally of a soft nature, with indurated portions, weather out
in the most grotesque forms.
On the higher grounds traversed by Battle River, and again on Red Deer River,
where they are seen to rest on the great lignite group, are also beds of marl, lime-
stones with iron like those of the Roche Percée, beds of lignite and true brown coal,
with silicified trees, and abundance of fossils of an estuarine character. Among these
latter are oysters, a good deal like the Pacific species, Mytili, Cyprina, and other
TRANSACTIONS OF THE SECTIONS. 81
marine forms in some beds; and in others Paludina is the prevalent fossil. On the
very high grounds (such as the Ochéschis or Hand Hills and the Cyprees Hills), these
strata pass up into sands, gravel, and beds of coarse shingle, which, at the same level
(4000 feet above the sea), skirt the base of the Rocky Mountains, and there rest on
the edges of upturned strata of various ages,
All the strata which I have mentioned are covered with a mantle of drift, which
does not rise much above 3000 feet; but near Battle River there seems to be a group
of deposits which I have termed Tertiaries of the low grounds,
The strata composing the Rocky Mountains may be briefly described as follows :
—lIn crossing from the east, thirty or forty miles before entering the range, beds of
grits and shales are observed much disturbed, but obviously dipping to the east.
From a level of 4000 feet above the sea, the mountains rise as parallel ranges of cliffs
from 3000 to 4000 feet in height. The first five or six of these ranges are composed
of blue crystalline and earthy limestone in bold plications, including portions of the
same grits and clays that are seen along the eastern base. ‘This group of strata must
be several thousand feet in thickness, and contain fossils of Carboniferous age. To
the west, and forming the range which in general determines the water-shed, is an
immense thickness of quartzite and conglomerates, not much altered, and apparently
horizontal. A wide longitudinal valley marks the line between this formation and
the Jast mentioned, and is probably the site of a great fault.
On descending the western slope of the mountains, while in the bottom of the
valleys are vertical talcose slates, the higher parts of the mountains are composed of
the same strata which form the eastern ranges, until the great valley is reached,
which the Columbia and Kootanie rivers traverse, while their course is parallel to the
range.
West of this a belt of slates and semi-metamorphic rocks was crossed, followed by
granite with true metamorphic rocks containing serpentine and marble, which brings
us to Colville.
South and west of this plain commence the great superficial floes of basalt with
beds of tufa, which have emanated from the flanks of the Cascade range. The Cas-
cade range itself consists of syenite and slates, with volcanic rock of recent date.
The greater mass of Vancouver's Island is composed of the same metamorphic
strata as at Colville; but along both sides of the Gulf of Georgia, which separate it
from the mainland, and also forming the islands in that gulf, occur beds of grits and
coarse conglomerate, much disturbed and resting on volcanic rocks, and containing
the well-known deposits of coal and lignite as at Nanaimo and Bellingham Bay.
These coal-bearing grits at Nanaimo, I found to be overlaid by Septarian clays, such
as those I have found to the eastward of the Rocky Mountains, and containing the
same cretaceous fossils, comprising Baculites and Inocerami. These clays are ob-
served, again, to be covered by grits. Fossils were obtained at some distance below
the coal at the base of the whole group, which have not yet arrived in England for
examination, ‘They are, however, either lower cretaceous or oolitic forms.
Remarks on the Geology of New Zealand, illustrated by Geological Maps,
Drawings, and Photographs. By Prof. F. von HocustTerrer.
Some Observations upon the Geological Features of the Volcanic Island of
St. Paul, in the South Indian Ocean, illustrated by a Model in Relief of
the Island, made by Capt. Cybulz, of the Austrian Artillery. By Prof. F.
von HocusrEtrer.
On the Six-inch Maps of the Geological Survey.
By E. Hutt, B.A. BGS.
On the Blenheim Iron Ore ; and the Thickness of the Formations below the
Great Oolite at Stonesfield, Oxfordshire. By Epwarpv Hutt, B.A,
F.G.S.
The author described the position of this iron ore as occurring in the upper part of
the Marlstone or Middle Lias, along the valley of the Evenlode, near Charlbury ; its
1860. 6
82 REPORT—1860.
outcrop being traceable for some distance along both banks of the river. It is
identical in geological position with the Cleveland ore of Yorkshire, and similar in
its mineral character. ‘Che bed varies in thickness from 10 to 15 feet, and the ore is
capable of being worked to an unlimited extent by tunneling into the hilly side from
the outcrop. The fossils, which are local, consist of the usual Marlstone species, as
Rhynchonella tetrahedra, Terebratula punctata, &c.
Mineral Character.—At the outcrop, the iron-bed presents a rich ferruginous aspect ;
but when followed to some depth below the surface, the original colour is found to be
olive-green, and under the magnifying glass the stone appears oolitic. In this state
the ore is probably a carbonate and silicate of iron—the latter imparting a green
tinge. When exposed, it passes into a hydrated peroxide of iron. The remaining
constituents are carbonate of lime, 10 per cent. ; silica, 12 per cent.; alumina, 7°8 per
cent. Phosphoric acid is only present in minute quantity, viz. 0°55 percent. The
chief market for the ore is expected to be South Wales*.
Thickness of the Formations below the Great Oolite at Stonesfield.
For the purpose of ascertaining the depth of the iron-bed below the Stonesfield
slate, the Duke of Marlborough directed that one of the slate pits should be continued
downwards till the ore was reached. This has not been accomplished ; for on reach-
ing at a depth of 120 feet the Upper Lias Clay, the water flowed in so plentifully that
the men were drowned out. With the assistance of numerous sections near Fawler,
the deficiency in the series may be supplied; and the following are the results :—
Succession of Strata at Stonesfield.
feet.
Great Oouire. 1, Upper Zone.—White limestone, resting on caleareous shales
and marls (total thickness about) ............eceeseseevees itseadduwenl sascsttcae MOG
2. Lower Zone.—Sandy shales, flags, and shelly oolite, with a band of
“« Stonesfield slate” at 10 feet from the top ....... sh Debts cbecadee ss ocawub treet 80
Inrerton Oorire. Upper Ragstone (zone of Ammonites Parkinsoni).—Large-
grained, rubbly oolite, very fossiliferous, with Trigonia costata, Lima
gibbosa, Terebratula globata, Clypeus Plotii... ........4. cadedvdasaceeeeepeees 30
Urrer Lias Cray.—Blue laminated clay..........scccseseeseees Siiessaisvinteas inane sre
Martstone. 1. Zron-bed.—Massive ferruginous rock, with Rhynchonella tetra-
Peed, Cress bee ee Ee Perens re caaeaccsederssenobort e 10-15
2. Sands, with iron concretions atop .........6...000e: vateeaee PTT Ce ace
Lower Lirias Cray.—Thickness unknown.
Comparing the development of these formations with that which they attain in
Gloucestershire, the author showed that they all tended to decrease in thickness when
traced from the north-west towards the south-east of England, and contended that
these facts bore out the theory which he had on previous occasions endeavoured to
demonstrate, that all the secondary rocks of England undergo attenuation towards
the south-east. The following comparison had been arrived at from carefully mea-
sured sections :—
Comparative Sections.
Gloucestershire. Oxfordshire.
Maximum thickness. Minimum thickness.
feet. feet.
Fuller’s Earth ...... ae 40 0
Inferior Oolite ........ . 264 5
Sands... 20-50 0
Upper Lias Shale ... 380 6
Marlstone ..:...3.05.06-. 250 25
Wowerdviasie ccs scree --- 600 (nearly) g
The author considers it probable that under Oxford the Great Oolite is separated
* As this ore extends under the property of the Duke of Marlborough, theauthor has
named it the “ Blenheim iron-ore;” and for fuller details refers to his memoir, ‘‘The Geo-
logy of the Country round Woodstock,” Mem. Geol. Survey, 1857.
TRANSACTIONS OF THE SECTIONS. 83
from the Lower Lias by not more than 25 feet of strata, of which the Marlstone forms
the greater part.
Notes on some Points in Chemical G'eology.
By T. Sterry Hunt, F.L.S., of the Geological Survey of Canada.
Dolomites and Gypsum.—Mr. Sterry Hunt has shown, from the mode in whick dolo-
mites occur and from the phenomena presented by their associated fossils, that these
magnesian rocks cannot have been formed by the alteration of pure limestones, so that
the theories of Von Buch and Haidinger, proposed to explain their formation, are
really in nowise applicable. He has further shown, that in the famous experiment
suggested by Haidinger and performed by Von Morlot, who asserted that by the
action of sulphate of magnesia, in presence of water in an excess of carbonate of lime,
at 200° C. under pressure, there is formed sulphate of lime and a double carbonate of
lime and magnesia, the fact has been overlooked that in reality no double carbonate
is obtained, but only a mixture of anhydrous carbonate of magnesia with carbonate
of lime, and consequently not a dolomite, which is a chemical compound of the two.
In Marignac’s modification of Von Morlot’s experiment, where the chloride is sub-
stituted for the sulphate of magnesia, Mr. Hunt finds that a variable portion of this
double carbonate is really formed, and remains mingled with the excess of carbonate
of lime and anhydrous carbonate of magnesia, which is also a result of the reaction as
before. Charles Deville’s late experiments, in which fragments of limestone were im-
pregnated with magnesian solutions, and heated at the ordinary pressure, with forma-
tion of soluble lime-salts and magnesian carbonate, are but imperfect repetitions of
Von Morlot’s and Marignac’s processes, and none of these are applicable to the great
majority of cases in which pure and magnesian limestones are associated in such ways
as to show that they have been successively deposited from water, the latter sometimes
enclosing pebbles and fossils of pure carbonate of lime.
Mr. Hunt proceeds to show that, when mixtures of amorphous hydrated carbonate
of magnesia with carbonate of lime are heated under pressure to a temperature of
300° to 400° F., direct combination ensues, and dolomite is formed; and he gives
reasons for supposing that this combination may take place slowly at much lower
temperatures.
It was, however, necessary to find a source for the magnesian carbonate which had
formed these magnesian sediments, and here Mr. Hunt has signalized a remarkable
and hitherto undescribed reaction, by which carbonate of lime decomposes sulphate of
magnesia, not with the aid of heat and pressure as in Von Morlot’s experiment, but at
the ordinary temperature. When a solution of bicarbonate of lime is mingled with a
liquid containing sulphate of magnesia, a double decomposition takes place, and by
evaporation at temperatures between 90° and 180° F., the lime is deposited in the
form of gypsum, a very soluble bicarbonate of magnesia remaining dissolved, which
is precipitated by further evaporation, If we conceive the carbonate of lime to be
furnished by springs falling into a closed lake or basin, the carbonate of magnesia
would be precipitated in a state of mixture with carbonate of lime, thus giving the
elements of the dolomite which is always associated with stratified gypsum.
Mr. Hunt has further shown that, by the action of waters containing alkaline carbo-
nates upon sea-water, the lime is first precipitated, and at length there is formed a
solution of bicarbonate of magnesia. To this agency he ascribes the vast deposits of
magnesian rocks which exist independent of gypsum, and which sometimes contain
‘an excess of carbonate of magnesia over that required to form dolomites, or lime being
absent, are magnesites,
The part which carbonate of soda has played in giving rise to carbonates of lime and
magnesia must, according to Mr. Hunt, have been very important in former periods,
The source of this has been the decomposition of felspar, which, in being reduced to
‘clays, have lost the whole or a part of their soda in the form of silicate, which, converted
into carbonate by the carbonic acid of the atmosphere, is now represented by the sea~
‘salt of the ocean and the carbonates of lime and magnesia of the rocky strata. Clays
‘and argillites are unknown in the vast thickness of crystalline rocks which constitute
in Canada the Laurentian system, lying beneath the Lower Silurian series. In these
oldest rocks, the alumina exists in the form of felspar, in great part with a base of
‘soda; but in the Silurian rocks, when altered, aluminous silicates abound, such as
6*
84 REPORT—1860.
chlorite, epidote, and alumina-garnet, and in those strata where lime and magnesia
are absent, chloritoid Andalusite, staurotide, and kyanite. These minerals, which are
only formed in aluminous sediments that have lost their alkalies, become more and
more abundant on the newer strata.
‘The consideration of the composition of mineral springs, as Mr. Hunt has remarked,
shows that the solvent action of water removes from sediments chiefly soda, lime, and
magnesia, and with the concurrence of organic matter, oxide of iron, so that the more
permeable strata, and generally more siliceous, retain scarcely any other bases than
alumina and potash; the argillaceous and less permeable beds, on the contrary, retain
the whole of their bases. ‘The operation of processes continually going on in nature
therefore tends to divide the silico-argillaceous rocks into two classes, whose meta-
morphism and displacement will give rise, on the one hand, to granites and trachytes,
and on the other, to rocks made up of basic felspar and pyroxenes. :
The author regards all the so-called igneous rocks as altered and translated sedi-
ments, and distinguishes them by the name of exotic rocks, from the same sediments
altered in situ, which may be called indigenous plutonic rocks. He insists upon the
fact that the chemical composition and, for the most part, the lithological characters
of all the varieties of intrusive rocks may be found represented in metamorphosed sedi-
ments.
Mr. Hunt has called attention to the fact, that as long ago as 1834 Keferstein
advanced the opinion that all plutonic rocks are only altered sediments, and thus
anticipated in part Sir John Herschel’s theory of earthquakes and volcanic pheno-
mena, to which Mr. Hunt has given a wider extension, connecting it with Mr. Bab-
bage’s speculations on the result of the rising of the isothermal lines in the earth’s
crust, consequent upon the accumulation of sediments. ‘The first result of this heat
would, as Mr. Babbage has shown, produce expansion and elevation ; but when meta-
morphism takes place, the contraction attendant upon the conversion of the sediments
into the denser silicates, such as chloritoid pyroxene, garnet, epidote staurotide, and
chiastolite, must produce an effect directly opposite. In this way Mr. Hunt conceives
that while the earth’s nucleus may be a solid, although incandescent mass of anhydrous
silicates, we may suppose that the inferior strata, which are undergoing metamorphism
and igneo-aqueous fusion, agreeable to the views of Poulett Scrope, Herschel, Scheerer,
and Sorby, are contracting in such a manner, that we may possibly admit with Elie
de Beaumont a shrinking of the fluid mass beneath, which will explain the great plica-
tions of the earth’s crust, and thus reconcile this theory with the view of a solid
nucleus. At the same time he is inclined to refer the great movements of elevation
and subsidence, for the most part, to what Herschel has described as “ the disturbance
of the equilibrium of pressure” consequent upon the transfer of sediments, while the
yielding mass reposes upon a mass of matter partly solid and partly liquid.
These views will be found in the ‘ Reports of the Geological Survey of Canada for
1857 and 1858,’ where the experiments upon gypsum and magnesian rocks are given
in detail. Also in a memoir published in the ‘Quarterly Journal of the Geological
Society’ for Nov. 1859.
On the Igneous Rocks interstratified with the Carboniferous Limestones of the
Basin of Limerick. By J. Beetz Juxes, M.A., F.RS.
The author called attention to some of the lately published sheets of the ‘ Geological
Survey of Ireland,’ including this district, and stated that the ground had been sur-
veyed by Messrs. Kinahan, Foot, O’Nelly, and Wynne.
He gave a brief sketch of the physical structure of the country around Limerick,
and then proceeded to describe its igneous rocks. These are of two kinds, trap and
trappean ash. The trap varies greatly in texture and aspect, more perhaps than in
mineral composition, ‘The trappean ash (or tuff) is the result of the mechanical ero-
sion of the igneous rock, either during the time of its eruption or immediately after,
and before it was buried under other aqueous rocks, It consists of grains or frag-
ments of trappean material, varying from the finest powder to a coarse conglomerate,
with blocks several inches in diameter, and often contains large and small fragments
of limestone, and sometimes of other matters.
It is perfectly stratified, lying in regular beds, interstratified both with the limestone
TRANSACTIONS OF THE SECTIONS. 85
and with the trap, and blends, almost insensibly, sometimes into one, and sometimes
into the other rock.
In the centre of the district, about Ballybrood, is a small hill of the lower coal-mea-
sure shales, resting upon the upper limestone on one side, and on trap on the other.
This trap attains a thickness of 800 or 1000 feet, and is chiefly contemporaneous bedded
trap, but has some intrusive parts, which cut like dykes into the coal-measures. It rests
on a bed of ash, and at its eastern end, at Nicker Hill, near Pallas, the most curious
and complicated interstratifications of limestone, ash, and trap may be distinctly ob-
served.
Beneath this upper trap comes a regular band of upper limestone, 600 or 800 feet
thick, surrounding the trap and coal-measures on all sides, and forming an oval basin.
From underneath this another great belt of trap and ash crops out, forming a cor~
responding outer basin, the dimensions of which are about 12 miles from E. to W., and
6 miles from N. to S.
The lower limestone rises from underneath this, and undulates for some miles over
the adjacent country. Towards the N.W. some of these undulations are sufficiently
great to bring the upper limestone in again, underneath the present surface of the
ground, and with that large parts of the lower trap and ash. ‘here are thus formed
three considerable detached outlying basins of trap and ash, one round Cahernarry
and Roxborough, another about the eastern side of the city of Limerick, and a third
round Carrigagunnil. ‘There are also one or two small exhibitions of similar rocks
towards the north, apparently on a rather lower horizon.
The above igneous rocks are all bedded and interstratified with the limestones,
except in a few places, where they seem rather to occur as small intrusive dykes,
cutting through the other traps as well as the aqueous rocks.
In many places the bedded traps become quite vesicular and scoriaceous, the vesi-
cles being often filled with carbonate of lime and other minerals, and thus forming
an amygdaloid.
In some places these vesicular parts occur as irregular bands intermediate between
bands of solid, compact, or even crystalline trap, precisely resembling the figures given
by Sir C, Lyell of the junctions of different flows of lava on Mount Etna.
There are, however, six other detached masses of igneous rock, five on the south
and one on the north of the basin above spoken of, which are clearly intrusive masses
rising up through the limestone, and not now connected with any overlying contem-
poraneous sheets of trap. It is probable that these mark the sites of the volcanic foci
or funnels, through which some of’ the sheets of trap flowed to the then surface, such
sheets, with the upper limestone including them, having been long ago removed by
denudation. It is also probable that similar small detached foci or funnels lie still
concealed beneath the areas occupied by the contemporaneous traps and ashes.
One of these detached masses, called Knock Dirk (not the hill which is called merely
Dirk), is a true syenite, having crystalline particles of quartz mingled with felspar
and hornblende.
It is difficult to give any precise name to the rock comprising the other masses.
Some of the traps, both intrusive and contemporaneous, would be commonly called
felspar porphyry, others gréenstone, and others basalt. When the felspar porphyry
loses its distinct crystals of felpar, it might perhaps be called felstone. Felstone,
however, as understood by the author, means a rock composed of a trisilicated fel-
spar, mingled with an overplus of silica in a state of paste; and it seems diflicult to
suppose that silicated rocks proceeding in a molten condition through and over sucha
basic substance as the carboniferous limestone, should still contain any uncombined
silica, except in the heart of a large mass like Knock Dirk. It would seem, therefore,
advisable to apply some other name, such as aphanite, for instance, to the compact
felspathic rocks above spoken of. In the absence of precise chemical analysis, which
the author regretted that he had been unable hitherto to procure, it had seemed better
to speak of all the igneous rocks collectively under the vague but sufficiently intelligible
designation of trap.
Mr. Jukes also stated, that he was much struck with the very great resemblance
between these trappean ashes and some of the traps, and those which he recollected
to have observed in the volcanic islands in Torres Straits, where small detached yol-
canoes have broken through the coral reefs, and formed rudely conical accumulations
of stratified ashes containing lumps of coral limestone together with flows of horn-.
86 REPORT—1860.
blendic lava. It is probable that beneath the sea-level sheets of such lava and vol-
canic ash lie interstratified with the coral limestone. Certainly, if Torres Straits were
depressed, and these islands exposed to the breakers, horizontal beds of the ash and
voleanic conglomerates would be derived from them, and spread over the surface of the
coral reefs.
On the Tynedale Coal-field and the Whin-sill of Cumberland and Northumber-
land. By J. A. Knipe.
The author points out the interesting fact of the true Newcastle coal being worked,
and that most successfully, at a distance of about 40 miles west of the Great Northum-
berland and Durham coal-fields at the locality named. The history of this and an ad-
joining coal-field, called the Stublick, are both similar, viz. the stvata are thrown down
many hundred feet by the prolongation of the 90 Fathom Fault, which is well known
and may be well observed on the Northumberland coast at Cullercotes. The principal
shaft sunk on this outlying coal-field, on the line of railway from Haltwhistle to Ald-
stone Moor, is named the “ King Pit,’’ Midgeholm Colliery. The depth of the shaft
is 506 feet 6 inches; there are five workable seams of coal, the aggregate thickness
of which is 23 feet.
The Great Whin-sill, or interstratified trap, may be traced, more or less, for many
score miles in the counties of Cumberland and Northumberland, to its termination
on the coast of the German Ocean, at Dunstanburgh Castle. At Wall Town, situated
on the old Roman Road, north by west from Haltwhistle, a town and station on
the Newcastle and Carlisle Railway, about 23 miles, the Whin-sill assumes a very bold
bluff appearance, after emerging from the superincumbent limestone rock. In places
it has a columnar structure, but has now much of its mural appearance changed by
trees growing amongst the ruin and debris of the rocky structure; on the summit
there is still a very perfect portion left of the Roman wall. ‘The author described the
section through the limestone grit shales, ironstone, and Blenkinsop Mines to the King
Pit and Tynedale Fault.
On the Eruption in May 1860, of the Kotliigjé Volcano in Iceland.
By W. Lauper Linpsay, I.D., P.LS.
It may interest the Geological Section of the British Association to be informed
that an eruption has recently occurred of the Kétltigj4 voleano, Iceland, from a visit
to which island I have just returned, Had time permitted (which it does not) I in-
tended to have drawn up for the British Association a brief account of the chief phe-
nomena of the eruption in question, accompanied by drawings made on the 13th June
inst., and a map of the district, and preceded by a summary of the preceding erup-
tions of the same volcano, which are fourteen in number. I hope at greater leisure to
prepare such a notice for some of the journals,
Meanwhile I may concisely state that the volcdno in question is situated in the
south of Iceland, about twenty miles from the coast, near, but considerably to the east
of, the well-known Hekla, which has been quiescent since 1846. Kotltigj4 is part of a
range, fifteen to twenty miles long, of glacier-covered mountains or “ Jokuls,” which
include Eyafjalla, Myrdals and Godalands Jékuls; the average elevation above the
sea being between 4000 and 5000 feet. The eruption began on the 8th of May last;
it was preceded by earthquakes of a local character; the first indication of its advent
being a dark cloud hovering over the summit of the mountain. The usual chief ejecta
of K6tligj4, when in a state of eruption, are hot water, pumice, and ashes. On the
occasion of the last, or fifteenth eruption, in May last, the most noteworthy pheno-
menon was the enormous water-flocd sent forth, a flood which bore with it pieces of
ice so large that they were stranded in the sea (twenty miles distant) at a depth of 20
fathoms. ‘The flames which issued from the crater were on the 12th of May visible
in Reykjavik, the capital of Iceland, which is at least eighty miles distant; and on
the 16th smoke rose to the height of 24,000 feet, this column of smoke being also
visible in Reykjavik. I left Scotland for Iceland on the 8th of June inst., expecting to
find K6tliigja still giving forth its fire and pouring out its floods of water. On the 13th
we sailed close to the south coast of Iceland from Portland’s Hak westward, the wea-
ther being beautiful and our view of Myrdals-Jokul and the neighbouring Jékuls ex-
TRANSACTIONS OF THE SECTIONS. 87
cellent: but all was quiet; not a vestige of smoke even was to be seen. Touching
at the Westmanna Islands, we were informed that the Kétltigj4 eruption had ceased
a few days previously, having done comparatively little mischief to the farms in its
vicinity.
[Derails of the eruptions above referred to, as well as an account of the Geology
and Topography of K6tltigja, will be found in a paper by the author “On the Erup-
tion in May 1860, of the Kotltigj4 Volcano, Iceland ”—accompanied with a Map
“illustrative of the Physical Geography of that part of the South of Iceland in which
Kotliigj4 is situated "—in the ‘ Ndinburgh New Philosophical Journal’ for January
1861, p. 6, and pl. 2; and also in his “ Contributions to the Natural History of Vol-
canic Phenomena and Products in Iceland” in the ‘ Proceedings of the Royal Society
of Edinburgh’ for 17th December 1860.]—June 1860.
On some Reptilian Foot-prints from the New Red Sandstone, north of
Wolverhampton. By the Rev. W. Lister.
The object of this paper is simply to announce the discovery, in a fresh locality, of
foot-prints of the Labyrinthodon, Rhynchosaurus, and of another animal, or animals,
with which I am not acquainted. Hitherto, I believe, the remains of the Laby-
rinthodon have only been found in Warwickshire, and the north of Cheshire and its
neighbourhood ; and the Rhynchosaurus in the Grinsel quarry near Shrewsbury*. The
foot-prints now discovered have been met with in Staffordshire, in a quarry of the
New Red Sandstone, on the very borders of the Red Marl, at a place about six miles
north of Wolverhampton, in the parish of Brewood, on the road between “The
Stone House”’ and Somerford. “‘The Stone House,” which is given on the Ordnance
Map, is near to Chillington Avenue Gates, and within 200 yards of the quarry. The
bed in which the foot-prints occur is about 12 feet from the surface. One of the slabs
was so thickly covered with impressions, resembling those of the Rhynchosaurus, as
to make one feel that the animals which made them must have been very numerous
on the spot. These were smaller than most of the others, and I have a strong im-
pression that they were those of young animals, they were so uniform in size and
form. But unfortunately, the slab, whick was from 5 to 6 feet long by from 3 to 4
broad, was removed before I had an opportunity of re-examining it.
The ripple-mark is very beautifully preserved on some of the slabs, and so is also
the rain-drops; while in many cases the amount of sand deposited by each tide is
readily discovered by the thickness of its layers, which lie one on the other, and which,
by means of the ripple-mark, show also the direction in which the water flowed, or
the wind blew, at the time they were deposited. The deposits of two, three, and, in
some cases, of even four tides are easily seen.
Some of the foot-prints of the Labyrinthodon are 10 inches in length; those of the
Rhynchosaurus are from 1 to 2 inches.
On the Koh-i-Noor previous to its Cutting.
By the Rev. W. Mircuett and Prof. Tennant, F.G.S.
On the Contents of Three Square Yards of Triassic Drift.
By C. Moors, F.G.S.
The author stated that several years ago he suspected the presence of triassic rocks
in the neighbourhood of Frome, from accidentally finding a single block of stone on a
roadside heap of carboniferous limestone, containing fish remains of the former age;
but that for a long time he was unable to discover it in situ. More recently, when
examining some carboniferous limestone quarries near the above town, he observed
certain fissures which had subsequently been filled up by a drift of a later age. One
of these was about a foot in breadth at the top, but increased to 15 feet in breadth at
the base of the quarry, 30 feet below, at which point teeth and bones of triassic reptiles
* After the reading of the paper, it was stated by Mr. Hull of the Government Survey,
that impressions of the Labyrinthodon have been discovered in two or three other fresh
localities, but they haye not, as I understand, been published.—W. L. ;
88 REPORT—1860.
and fishes were found. Usually these infillings consisted of a material as dense as
the limestone itself, and from which any organic remains could only be extracted
with difficulty. In another part of the section he was fortunate enough to find a de-
posit consisting of a coarse friable sand, containing similar remains, In order that
this might receive a more careful examination than could be given to it ou the spot,
the whole of it, consisting of about 3 tons weight, was carted away to the residence
of the author, at Bath, a distance of twenty miles; all of which had passed under his
observation, with the following results:—The fish remains, which were the most
abundant, were first noticed. Some idea might be formed of their numbers when he
stated that of the genus dcrodus alone, including two species, he had extracted 45,000
teeth from the three square yards of earth under notice, and that they were even
more numerous than these numbers indicated, since he rejected all but the most
perfect examples. Teeth of the Saurichthys of several species were also abundant ;
and, next to them, teeth of the Hybodus, with occasional spines of the latter genus.
Seales of Gyrolepis and Lepidotus were also numerous, and teeth showing the pre-
sence of several other genera of fishes. With the above were found a number of
curious bodies, each of which was surmounted by a depressed, enamelled, thorn-like
spine or tooth, in some cases with points as sharp as that of a coarse needle; these
the author supposed to be spinous scales, belonging to several new species of fish,
allied to the Squaloraia, and that to the same genus were to be referred a number of
hair-like spines, with flattened fluted sides, found in the same deposit. There were
also present specimens, hitherto supposed to be teeth, and for which Agassiz had
created the genus Ctenoptychius, but which he was rather disposed to consider
(like those previously referred to) to be the outer scales of a fish allied to the Squa-
loraia. It was remarked that, as the drift must have been transported from some di-
stance, delicate organisms could scarcely have been expected; but, notwithstanding,
it contained some most minute fish-jaws and palates, of which the author had, either
perfect or otherwise, 130 examples. These were froin a quarter to the eighth of an
inch in length, and within this small compass he possessed specimens with from thirty
to forty teeth; and in one palate he had succeeded in reckoning as many as seventy-
four teeth in position; and there were spaces where sixteen more had disappeared, so
that in this tiny specimen there were ninety tecth! Of the order Reptilia there
were probably eight or nine genera, consisting of detached teeth, scutes, vertebra,
ribs, and articulated bones. Amongst these he had found the flat crushing teeth
of the Placodus ; a discovery of interest, for hitherto this reptile had only been found
in the muschelkalk of Germany,—a zone of rocks hitherto wanting in this country,
but which, in its Fauna, was represented by the above reptile. But by far the most
important remains in the deposit were indications of the existence of triassic mam-
malia. Two little teeth of the Microlestes had, some years before, been found in
Germany, and were the only traces of this high order in beds older than the Stonesfield
slate. The author’s minute researches had brought to light fifteen molar teeth, either
identical with, or allied to, the AZicrolestes, and also five incisor teeth, evidently be-
longing to more than one species. A very small double-fanged tooth, not unlike the
oolitic Spalacotherium, proved the presence of another genus and a fragment of a
tooth, consisting of a single fang, with a small portion of the crown attached, a third
genus, larger in size than the AZicrolestes. Three vertebrae, belonging to an animal
smaller than any existing mammal, had also been found. The author inferred that
if twenty-five teeth and vertebrae, belonging to three or four genera of Mammalia,
were to be found within the space occupied by three square yards of earth, that por-
tion of the globe which was then dry land, and from whence the material was in part
derived, was probably inhabited at this early period of its history by many genera of
Mammalia, znd would serve to encourage a hope that this family might yet be found
in beds of cven a more remote age.
Remarks on Fossil Fish from the North Staffordshire Coal Fields.
By Witt1am Mouynevx.
The author of this paper stated that little more than two years ago the fossil fish of
the coal-field in question comprised, so far as was then known, a list of eight genera
only, and those of a kind most commonly found in other home-representatives of the
system. J.ast year, at Aberdeen, he had the honour, in connexion with Mr. Garner,
TRANSACTIONS OF THE SECTIONS, 89
of exhibiting before this Section a collection of such remains, the generic number of
which amounted to upwards of twenty, including some new to science, and others of
a rare and interesting order. On the present occasion his principal object was to
draw attention to some specimens obtained since the period alluded to. One of
these, Ctenacan/hus hybodoides (Egerton), was in a perfect state of preservation.
Another specimen was a lower jaw of Rhizodus, whose long powerful teeth, arranged
in pairs, resembled in their curved points R. incurvus of the Ohio coal-field; but as
there appeared to be doubts of its specific identity, probably it would prove to be a
new species. There was also a fragment of a massive jaw of the same genus which
presented features of much interest to the ichthyologist.
Of the smaller ganoids exhibited, one represented a new genus, obtained from the
deep mine ironstone shale at Longton, at the pit where ironstone was first worked
for the purpose of manufacture in North Staffordshire. The specimen measured four
inches in length, but was scarcely one inch in its greatest depth immediately behind
the head ; the form being tapering and elegant. ‘The dorsal fin was placed but half
an inch before the bifurcating point of the caudal, and slightly in advance of the
anal fin, the rays being strong and articulated. The scales were rhomboidal in
form, and profusely ornamented with raised lines, which assumed the character of a
series of Gothic arches ranging from the centre of the scale. Some undescribed spe-
cimens of Paloniscus, with many large teeth of Placoid fish, were also exhibited.
__ The coal-field in question was found to be particularly rich in fish-remains ; and
although little more than two years had been actively devoted to the subject, the
generic list had during that time increased from eight to thirty-three in number, and
the author felt sanguine that it would ultimately prove quite as rich in species as the
Old Red of Scotland. These remains, it was stated, occur very irregularly ; some
beds of ironstone in the upper division of the measures contain considerably more
than others, but it was only in one instance, that of the new mine, that they were
found forming a stratum from one to three inches in thickness. Though anything like
perfect specimens were comparatively rare, the fine compact shales of the knowls
and deep mine ironstones had lately produced some well-preserved specimens of
Palzoniscus and Platysoma,
Notice of a Fossiliferous Deposit near Farnell, in Forfarshire, N. B.
By J.Pownrts. (Communicated by Sir R. Murcuison.)
This deposit, which is situated on the south-east bank of the Pow Burn, about half a
mile south-west of the Farnell Station of the Scottish North-Eastern Railway,
mostly consists of fine greyish argillaceous shales, the lower portion splitting into
laminz nearly as thin as writing-paper, and when first opened of a delicate cream-
colour; the upper beds are thicker, and vary from a cream-colour to dark grey: in
many places these are considerably stained by the infiltration of iron in solution.
The dip is, at an angle of about 12°, in a nearly north-west direction, the strike thus
following that of the Great Anticline which runs through Forfarshire, a little to the
south-east, in a direction of from north-east to south-west nearly.
This deposit rests conformably on a thick-bedded coarse dark red sandstone, and
varying from 4 to 6 or 7 feet in thickness, is overlaid by coarse broken shales, above
which is a considerable thickness of boulder clay and soil. Both from its position
and peculiar organic remains, it can at once be recognized as occupying the same
position in the Forfarshire formations as the Turin Hill and Carmyllie flagstones.
Cropping out on the banks of a small stream, it was first noticed as affording indications
of being fossiliferous by the Rev. Henry Brewster of Farnell, and pointed out by him
as such to the Rev. Hugh Mitchell, who first discovered that, besides Parca decipiens
and remains of Pteryyoli, &c., it contained small fishes in astate of wonderful preserva-
tion; these being, with the exception of Cephalaspis and afew veryimperfect ichthyolites,
the first fishes found in the Forfarshire sandstones: a paper was read, and a selection
of these exhibited by Mr. Mitchell at the Meeting of the British Association held at
Aberdeen last August (1859). Indisposition has prevented him continuing to aid in
these explorations.
The Earl of Southesk, on whose estates this deposit is situated, has lately most
liberally opened up this deposit, and placed the examination of its contents under the
90 REPORT—1860.
superintendence of Mr. Brewster and myself: already a considerable portion has
been carefully looked over, and has yielded to our researches some most interesting
remains: these lie scattered through the whole deposit, but in the upper and coarser
beds are for the most part both badly preserved and very fragmentary; in the lower
fissile portions they are more perfect, and the state of preservation is generally very
fine: no painting could equal the beautiful appearance some of the smaller fishes
exhibit when the little slab in which they have been entombed is first opened up, and
still damp. From the fragile nature of the matrix, great care is required in splitting
it up; and in afterwards fitting up the specimens for preservation they are exceedingly
apt to be destroyed.
The Parca decipiens is the most abundant organism found; finely sculptured frag-
ments of Plerygotus Anglicus and other Pterygoti are by no means uncommon ; and
one or two varieties of as yet unnamed Eurypteride have been found, and are now in the
collections of Mr. Brewster and Mr. Mitchell. But by far the most interesting feature
of this deposit is the comparative abundance of small-sized fishes not found elsewhere
in Forfarshire ; although Cephalaspis is frequently found in other localities along with
Plerygotus, as yet not a fragment of this fish has been disinterred. All the fishes I
have as yet examined, in a state of preservation sufficient for identification, belong to
the family Acanthodii, and, in so far as I am able to ascertain, to the genera Acanthodes
and Diplacanthus. Of the latter genus (Diplacanthus), two, if not more, very distinct
species have, up to this time, been found; unfortunately these are very rarely entire,
the deposit being a good deal fractured and faulted; although the largest of the
Diplacanthus yet found does not seem to have been over 6 inches in length, only one
nearly complete fish of that genus has as yet turned up; the other specimens show
merely portions of the body, tail, &c. Of Acanthodes, the fishes, being small, are
generally much more entire: of this genus I can only discern one species, and this,
although provisionally named at the Aberdeen Meeting ‘ Acanthodes antiquus,” in
no way differs, in so far as I can see, from the specimens of Acanthodes pusillus I have
been able to procure for comparison (these, however, have all been very imperfect),
further than the condition of the sediment in which they had been laid down, and
similar natural causes might readily explain. :
Although by no means prepared to assert the positive specific identity of the Far-
nell fishes with those of the same genera found in Cromarty, Morayshire, &c., yet their
general resemblance to these fishes found in our more northern deposits, in- my
opinion, strongly points to the probability of our Forfarshire flagstones belonging to an
epoch more nearly approximating in geological time to the fish-beds of the northern
counties than has as yet been generally thought likely.
Besides these, some very imperfect remains of fishes, evidently belonging to other
families, have been found; it is to be hoped that further explorations may throw some
additional light on the nature of these fragments (see p. 78).
Sir R. I. Murcutson exhibited the New Geological Map of the Vicinity of Oxford.
On the Geology of the Vicinity of Oxford.
By Professor Puriuies, M.A., F.RS.
On some New Facts in relation to the Section of the Cliff at Mundesley,
Norfolk. By Josery Prestwicu, F.R.S. Se.
The object of the author was to correct an opinion which prevailed regarding the
superposition of the freshwater depusit at Mundesley. In the interesting sections
of the Norfolk coast, given by Sir C. Lyell in the ‘ Philosophical Magazine ’ for May
1840, the freshwater beds of Mundesley are represented as intercalated in the Boulder
Clay. The wearing away of the cliff since that period has exposed a clearer section,
from which it appears to the author that there is no intercalation of the beds; but
that the freshwater beds overlie the Boulder Clay, and that they are newer than any
portion of the cliff except a bed of the gravel which passes over them. They lie in a
hollow worn through the upper beds and the Boulder Clay down to the sands beneath,
TRANSACTIONS OF THE SECTIONS. 91
and they are clearly separated from all these older beds by another and underlying bed
of gravel.
The author further noticed that the lower sands and gravels under the Boulder clay
contained a layer of marine shells in a perfect state of preservation, consisting of
Mytilus edulis (some with Balani attached) and Littorina littoralis, and traces of
others. Again, below this is a seam of dark clay containing freshwater shells, chiefly
the Pisidium amnicum, and a Unio, while a short distance lower is the well-known
Forest bed with its elephant and other mammalian remains. He concludes by call-
ing attention to the Mundesley deposit as being probably synchronous with the flint-
implement bearing deposit of Hoxne.
On Slickensides. By J. Price,
On the Chronological and Geographical Distribution of the Devonian Fos-
sils of Devon and Cornwall. By WiiLiaM PENGELLY, F.G.S.
The limestones, slates, and associated sandstones of North and South Devon and
Cornwall have, as is well known, caused much perplexity as to their real place in the
chronological series of the geologist. Thanks, however, to the labours of Professor
Sedgwick, Sir R. I. Murchison, Mr. Lonsdale and others, the problem is now gene-
rally admitted to be solved; the rocks in question are the equivalents of the Old Red
Sandstones of Scotland and elsewhere ; they belong to what is known as the Devonian
age of the world.
Some little difficulty, however, exists—or rather once existed—in the way of the
full and unqualified acceptance of this decision. The rocks of Devonshire are crowded
with the remains of invertebrate animals, especially sponges, corals, and shells;
whilst the supposed contemporary deposits of Scotland and the adjacent isles are so
rich in fossil fish, that, in the language of the late Hugh Miller, ‘‘ Orkney, were the
trade once opened up, could supply with ichthyolites, by the ton and the shipload,
the museums of the world*;” but the fossils characteristic of either of these districts
are not found in the other. Scotland does not yield the mollusks and zoophytes of
Devonshire, nor is there recorded in the Jatter district more than the faintest trace of
the ichthyolitic wealth of the North.
Though this fact may still have difficulties connected with it, they have ceased to
be chronological; for Sir R. I. Murchison tells us that ‘‘ The same fossil fishes, of
species well known in the middle and upper portions of the Old Red of Scotland, and
which in large tracts of Russia lie alone in sandstone, are in many other places found
intermixed, in the same bed, with those shells that characterize the group in its slaty
and calcareous form in Devonshire, the Rhenish country, and the Bouionnais,” ‘‘ The
fact of this intermixture completely puts an end to all dispute respecting the identifi-
cation of the central and upper masses of the Old Red of Scotland with the calcareous
deposits of Devonshire and the Eifel+.”
Professor Sedgwick has proposed the following threefold division of the Devonian
rocks of Devon and Cornwall :—
«The first and oldest of these groups may be conveniently called the Plymouth
group, using these words in an extended sense, so as to include all the limestones of
South Devon and the red sandstones superior to the Plymouth limestones. The
equivalent to this group in North Devon includes, I think, the Ilfracombe and Linton
limestones as well as the red sandstones of the north coast. i
«The second group includes the slates expanded from Dartmouth to the metamor-
phic group of Start Point and Bolt Head, and is, so far as I know, without fossils: it
may be called the Dartmouth group, and its equivalent in North Devon is found in
the slates of Morte Bay, which end with beds of purple and greenish sand-rock and
coarse greywacke. It ranges nearly east and west across the county. :
“The third group is not, I think, found in South Devon; but in North Devon it is
well-defined, commencing on a base-line of sandstone beds which range nearly east
and west from Baggy Point (on the western coast) to Marwood (which is a few miles
north of Barnstaple), and thence towards the eastern side of the county. This group
* Footprints of the Creator, p. 2. T Siluria, Third Edition, p. 382.
92 REPORT—1860.
is continued in ascending order to the slates on the north shore of Barnstaple Bay ;
but its very highest beds are seen on the south shore of the bay, dipping under the
base of the culm-measures.
“The equivalent of this third and highest Devonian group is found to the south of
the great culm-trough in a group, near the top of which appear the limestone bands
and fossiliferous slates of Petherwin. It may be called the Barnstaple or Petherwin
roup*.”
: Ponfesser Sedgwick recognizes the Plymouth group in the slates of Looe, Polperro,
and Fowey in Cornwall f.
Accepting, at least provisionally, these divisions, we have, when considered chro-
nologically as well as geographically, what, as a matter of convenience, may be called
five fossiliferous areas; namely, a deposit of the age of the Plymouth group in each of
the districts, South Devon, North Devon, and Cornwall; and one of the Barnstaple
age in each of the two latter. To avoid undesirable repetition, they will be spoken of
throughout this paper as Lower South Devon, Lower North Devon, Lower Cornwall,
Upper North Devon, and Upper Cornwall. ‘The terms ‘‘ Lower’’ and “‘ Upper”’ are
to be understood as applied relatively only to the rocks of Devon and Cornwall, and
not as embodying or implying any opinion respecting the co-ordination of these rocks
with deposits of the Devonian age elsewhere.
Had existing materials warranted it, it would have been desirable to have made a
farther division, namely, one having reference to the mineral character of the depo-
sits, as well as to time and place; for it is certain, as might have been expected, that,
in the same area, some fossils are peculiar to the argillaceous beds, and others are
found only in the calcareous strata; thus, for example, I learn from Mr. Godwin-
Austen that he has found the remarkable coral Pleurodictyum problematicum in the
slates, but not in the limestones, at Ogwell in South Devon. My own experience is
in harmony with this; the same fossil occurs in the slates at Torquay and, in great
abundance, at and near Looe in Cornwall; but not in limestone anywhere. At pre-
sent, however, it would be premature to attempt a division of this kind.
The object contemplated in the present paper is to give some account of the ancient
population of the five areas, especially with reference to their distribution, so far as it
was known when the Census was last taken.
Amongst the things which have recently drawn my attention to this subject may be
mentioned the following passage in the address of Professor Phillips as President of
the Geological! Society of London. ‘‘ Only a small proportion of the fossils of North
Devon occur in South Devonf.” And also the following statement by Professor
Haughton:—“I do not believe in the lapse of a long interval of time between the
Silurian and Carboniferous deposits, in fact in a Devonian period.
«« The same blending of corals bas been found in Ireland, the Bas Boulonnais, and
in Devonshire, where Silurian and Carboniferous forms are of common occurrence in
the same localities §.”
It should be remembered that the statement with which we have here to deal is that
the ‘blending of corals” (the word is not fossils) “of Silurian and Carboniferous
forms is of common occurrence in Devonshire.”
I have consulted such registers as I have been able to command, and have thrown
so much of their contents as bear on the questions before us into the following tabular
form, for which, of course, no higher value is claimed than attaches to the original
documents.
The materials have been in a great degree derived from Professor Morris’s ‘ Cata-
logue of Fossils.’
Every geologist must, of course, be aware of the numerous and elaborate Tables
which Professor Phillips has introduced in his ‘ Paleozoic Fossils of Devon and
Cornwall,’ when discussing subjects akin to those at present under consideration. In
the preparation of this paper the author has in no way made use of the valuable data
these Tables contain.
* Quarterly Journ. Geol. Soc. vol. viii. p. 3. t Ibid. p. 14.
t Quarterly Journ. Geol. Soc. vol. xvi. p. xl.
§ Voyage of the ‘ Fox’ in Arctic Seas, Appendix, No. IV. p. 387.
93
TRANSACTIONS OF THE SECTIONS.
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We learn from the three left-hand columns of figures headed “Totals” in the
94 REPORT—1860.
Table, that, taken together, the five areas have yielded 347 species of fossils belong-
ing to 97 genera and 49 families, of 9 classes of animals; namely, three classes of
the subkingdom Radiata, one of Articulata, and five of Mollusca; hence 15 of the
24 classes into which the existing animal kingdom is commonly divided are totally
unrepresented in the series, as is the entire vegetable kingdom also.
It is scarcely necessary to remark that the fossils of Devon and Cornwall do not
fully represent the organisms of the Devonian age, as six other classes—Pisces,
Pteropoda, Cirripedia, and Annelida amongst animals, and Cellulares and Monoco-
tyledones amongst plants—have been found in rocks of this age elsewhere; and of
these the last and first two have been met with in British localities.
The most important class numerically is Brachiopoda, to which 108 species belong ;
that is 31 per cent. of the entire series. The families and genera of Cephalopoda are
richer in species than those of any other class, averaging 16 for each family and 10
for each genus.
The most striking fact in this connexion, is the abundance of Brachiopoda and
Cephalopoda, and the paucity of Lamellibranchiate and Gasteropod species, as com-
pared with the numerical rank of the same classes in the existing British fauna; this
will, perhaps, be most strikingly exhibited by the following Table :—
Taste II.
Devonian Mol- Existing
lusca of Devon British
_and Cornwall. Mollusca.
BYYOZB4) (55, Gisscinee ieee bed 42 PE gies 72
Brachiopoda ......... pier NB iese th sis ag 15°5
Lamellibranchiata ...... 186 abs car 359°5
Gasteropoda......... Eat palidige a i ae 5215
Cephalopoda sig iiahsbacn? L828. SM Aeash ceed 315
1000 1000
which has been thus computed ; in the left-hand column the aggregate number of the
species of fossil Mollusca found in Devon and Cornwall has been put=1000, and the
numbers belonging to each class equated to this; the right-hand column has been
formed on the same principle, and is based on the data given by Forbes and Hanley
in their ‘ History of British Mollusca.’
It appears then that within existing British seas, the Lamellibranchiates are about
twenty-four times more numerous, specifically, than the Brachiopods, whilst within
what may be called the same area, the latter were to the former during the Devonian
period somewhat more than as 2 to 1; that is, they were then 50 times more abun-
dant than at present in comparison.with the other great class of Acephala. In like
manner it is seen that, relatively to the Gasteropoda, the Cephalopoda were, in this
early age of our planet, seventeen times more numerous than now. It may be added
that, within the district under notice, the registered species of Devonian Brachiopoda
and Cephalopoda absolutely, and in a high ratio, exceed those belonging to the same
classes within existing British seas.
The five columns of Table I. headed “ Peculiar to,” and distinguished from one
another by the initials of the five areas, show the number of fossil species which, so
far as England is concerned, are peculiar to each; from which it appears that 296
species are peculiar to one or other of them, leaving no more than 51 distributed
amongst them. Lower South Devon monopolizes no fewer than 19] species in this
way, whilst Lower North Devon is equally remarkable for its fossil poverty.
Five areas, taken two, three, four, and five together, are capable of being formed
into twenty-six different combinations. Not a single species is common to the
five areas, and only one, Cyathophyllum celticum, is found in each of four of them.
The well-known coral Favosites cervicornis is the only fossil found in each of the
three contemporary deposits of Lower North and South Devon and Cornwall. Of
two areas only, Upper North Devon and Upper Cornwall have the greatest number-—
fourteen—in common.*
_ * See in Table I. the ten columns headed “Common to,” and distinguished by combina-
tions of initials of two or more areas.
TRANSACTIONS OF THE SECTIONS. 95
It must be understood that any one of the ten columns just noticed shows, not the
total number of species common to the areas the initials of which stand at its head,
but simply the number at once common and restricted to them collectively; thus the
second of these columns, headed L. S. D., L.C., shows that five species are common
and restricted to Lower South Devon and Lower Cornwall; but in the third column
we find one species common to them and also to Lower North Devon, in the fourth
one common to them and to Upper North Devon, and in the eighth one found in each
of them and also in Upper North Devon and Upper Cornwall; hence there are eight
species common to the two areas instanced, five being restricted to them collectively
and three not. The same explanation applies to the other areas. Hence the total
number of species found in any area will be ascertained by adding the figures in all
the columns marked ‘“ Peculiar to”’ and ‘Common to” at the head of which the
initials of the area are found; thus, for example, a total of 47 species of Zoophyta
occurs in Lower South Devon, of which 40 are not found elsewhere in Devon and
Cornwall. Moreover, as the column marked “Species” shows that the two counties
have yielded a total of 49 species belonging to this class, it is evident that two of this
total number have not been met with in Lower South Devon. And so on for the
other classes and areas, as is shown in the five columns headed “Totals” and
distinguished by the initials of the areas.
Of the 347 species, 67 are met with in various parts of Continental Europe, and
7 in North America; 6 of the latter being included in the European 67, and one of
the 6 is also found in New South Wales; thus making a total of 68 common to Deyon
and Cornwall and to districts beyond the British Isles*.
Comparatively few of the Devonian fossils of the two counties appear to have been
derived from the Silurian fauna ; eight species only are referable to that earlier period+.
Amongst these are the three corals, Favosites fibrosa, Emmonsia hemispherica, and
Chonophyllum perfoliatum. The first has been found in Lower Silurian rocks at
Llandovery ; in the upper deposits of the same system in various parts of the typical
Silurian country, in eight counties of Ireland, in Russia, and in three North American
localities ; during the Devonian era it existed in several parts of Devonshire, in
France, and in Germany. The second, Emmonsia hemispherica, dates its origin
in Upper Silurian times, when it seems to have been confined to the area of modern
North America, ranging from the State of Ohio to Tennessee; having outlived the
Silurian period, it sent colonies to Spain and Britain and greatly extended its range
in America.
Chonophyllum perfoliatum differs from the two former in having always lived
within narrow geographical limits; it occurs in Upper Silurian beds at Wenlock, and
in Devonian in one quarry near Newton in Devonshire; but its appearance is not
recorded elsewhere.
The wide geographical range of the first two would seem to imply hardy plastic
constitutions, fitting them for distant travel, and existence under varied circumstances;
there is, therefore, nothing very surprising in their extended vertical range; it is,
perhaps, worthy of remark, that the second seems to have disappeared at the very
zenith of its widely extended power.
The very limited distribution, in space, of the last of the trio would scarcely suggest
the thought that such an organism would be likely to be capable of enduring physical
and thermal changes such as, there are reasons for believing, considerable lapses of
time have always introduced into any given area; changes probably similar to those
which an organism would experience in passing to a distant locality in any one and
the same period.
On the other hand, the well-known fossil coral Favosites Goldfussi occurs in Devo-
nian rocks in Devonshire, at Nehou and Visé in France, at Millar in Spain, in the
Oural, in the States of Ohio and Kentucky in North America, and in New South
Wales. It seems to have successfully struggled with the varying conditions of change
of place, and might have been expected to be equally capable of contending with
such as depend on lapses of time; nevertheless, the facts do not harmonise with such
* See in Table I. the columns headed Eu. (Continental Europe), Eu. Am. (Europe and
America), Am. (America), Eu. Am. Au. (Europe, America, and Australia). >
+ See in Table I. the column headed “ Silurian,”
96 REPORT— 1860.
inferences ; Chonophyllum perfoliatum formed part of the Silurian and Devonian
faunas, but was confined to the British area; Fuvosites Goldfussi was at home in
every part of the world, yet it commenced and terminated its career within the De-
vonian period.
The rocks of Devon and Cornwall have 58 species of fossils in common with
those of the Carboniferous group*, but no corals or sponges amongst them; so that
it cannot be said that “there is a blending of Silurian and Carboniferous corals in
Devonshire,” whatever there may be elsewhere; for though, as has been stated, three
Silurian corals have been found, not one referable to the Carboniferous fauna has
been exhumed there}.
The species which thus passed from the Devonian into the Carboniferous period are
found in the three principal fossiliferous deposits of Devon and Cornwall, as exhibited
in the following Table :—
Taste ITI.
Totals. | L,S.D.| U.N.D.} U.C.
iEehinodermatary, tie cieeis sis e poles 6 3 2 cv ee
Cristaceain, hychieelisasde cite 1 1 see sae
EVGzGWa sla agen eet gates tooo. 6 3 2 2
Brachiopudateeauiner sy creeks 24 15 9 7
Lamellibranchiata,..........08. 4 2 aoe 2
Gasteroportats isis cise eg nc 6 tei 10 6 3 3
Cephalopoda 3), Sivenca epic sees > ss 7 = 2 3
The populations of the three areas seem to have been thus composed :—
South Devon :—6 Silurians+220 new species (7. e. Lower Devonian)=a total of
226, of which 34 passed into the Carboniferous.
Barnstaple :—1 Silurian + 13 Lower Devonians + 64 new (Upper Devonians) = a
total of 78, of which 18 passed into the Carboniferous.
Petherwin :—1 Silurian + 15 Lower Devonians + 57 new (Upper Devonians) = a
total of 73, of which 18 passed over to the Carboniferous.
Of the ‘new forms” in the Barnstaple and Petherwin areas (64 and 57 respect«
ively) 14 are common, :
It is perhaps worthy of remark that the five areas have a smaller number of organic
forms in common—closely connected as they are both in time and space—than with
Devonian deposits in Continental Europe and elsewhere beyond the British Isles, or
with the Carboniferous rocks of Ireland and Central and Northern England.
Table I., to which attention has so frequently been directed, represents, so far as
is at present known, the absolute distribution of the fossils in the two counties in
which they occur ; but, for purposes of geological chronology, it is probably of greater
importance to ascertain their relative distribution; this is shown in Table 1V., which
has been calculated from Table I. thus : the total number of species in each class is
put=1000, and the figures in the other columns equated to this,
* See in Table I. the column headed “ Carboniferous.”
+ See ‘Monograph of British Fossil Corals,’ by Messrs. Edwards and Haime, pp. 150 and
212.
97
TRANSACTIONS OF THE SECTIONS.
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“TPMUIOD PUL MOAI] JO S]Isso] URrUoAaT a3 Jo ‘aovdg puv awry, ur ‘uorNqIystq sarmjagy oy Surmoyg “Ay atavy.
1860.
98 REPORT—1860.
Each area is marked by some class being relatively most abundant in it, as is ex-
hibited below, thus* :—
L. 8. D. L.N. D. L. C. U.N. D. U.C.
Zoophyta. | Bryozoa. | Amorphozoa. | Lamellibranchiata. | Cephalopada.
When ranged, in descending order, so as to show, relatively, the migration of their
species from the Devonian to the Carboniferous era, the classes stand thus: Bryozoa,
Echinodermata, Brachiopoda, Gasteropoda, Cephalopoda, Crustacea, Lamellibran-
chiatat.
The distribution of the genera is just as marked as that of the species; 92, out of
the total 97, are found in Lower South Devon, and of these 45 are, in Britain, pecu-
liar to it. Every genus of the classes Zoophyta and Brachiopoda occurs in it; the
genera thus limited, however, are usually poor; 33 of the 45 contain each but a
single Devonian species. The richest genus not found elsewhere is Acervularia, a
group of corals belonging to the great Palaeozoic family Cyathophyliide ; it contains
7 species, all peculiar to this area. One of the richest genera in the entire series
is Clymenia, belonging to the class Cephalopoda; of this genus 11 species are found
at South Petherwin, and not one is met with elsewhere in Britain. The genus Cyrto-
ceras, with the single exception of C. rusticum (probably a synonym for Orthoceras
arcuatum), is restricted to Lower South Devon, where it isrepresented by 12 species.
The chronological range of the Devonian genera of Devon and Cornwall is shown
below.
Tasre V.
pe eee Common to
Ses re
ees| 22
eB Aa oO ze Devonian, Cerponteriity Carboniferous,
2 fat Silurian, Silurian.’ Devonian.
Amorphoz0a ....-...++ 4 3 1 So ese
Zoophyta sse...cssessseee 20 10 5 3 2
Echinodermata ......... 6 2 50 3 1
Crustacea ....ersesessess 8 1 5 sie 2
Bryozoa......- scauacstece 7 0 ne 5 2
Brachiopoda............. 16 3 2 8 3
Lamellibranchiata...... 17 2 1 9 5
Gasteropoda. ..........4+ 14 2 aes 11 1
Cephalopoda ............ 5 1 2 2
a Se ees jee ee as
1f 07a ee 14 41 18
Some of the genera common to the Devonian and Carboniferous eras, are found
also in more recent deposits, and even in the existing fauna.
Such appear to be the prominent facts in connexion with the subjects under con-
sideration. What is their interpretation? This is a problem more easily proposed
than solved. Are we to believe that our knowledge of the geological record is too
imperfect to warrant any important generalizations? Do our museums fully repre-
sent the fossilized remains of bygone forms of life? Have all the extinct organisms
already in our possession been registered in the published lists? Is the record itself
so incomplete as to be altogether incapable of revealing to us the physical and organic
history of our planet? Are the notions of biologists respecting specific distinctions
sufficiently mature and uniform to warrant a reliance on their decisions? Some-
thing must doubtless be conceded on each of these points; still there cannot but be a
* See in Table IV. the columns headed “ Totals.”
+ See in Table IV. the column headed “ Carboniferous.”
TRANSACTIONS OF THE SECTIONS. 99
large outstanding amount of fact incapable of being thus explained away ; the problem
demands some other solution. Suppose it true that in some cases the organic dissi-
milarity, which has been described, was due to differences in the mineral character of
the ancient sea-bottoms; still when we have two areas like Lower South and North
Devon, consisting of contemporary, almost contiguous, and scarcely dissimilar depo-
sits, one rich and the other poor in the variety of its organic remains, having together
233 species yet no more than 8 in common, some other solution is obviously needed.
Was there a terrestrial barrier separating the two areas? Was that which is now
Central Devon occupied by dry land, which stretched far both east and west, while
the waves of the Devonian ocean rolled over the north and south of the county? All
the known physical facts are opposed to such a hypothesis. Moreover, 8 species
actually did migrate from one area to the other; eight proofs, then, that a passage did
exist, unless we suppose that both areas Were peopled from some more distant centre
or centres of dispersion.
It may be asked, were not these eight the remnants of an earlier (a Silurian) fauna?
forms of life whose localization had been determined by an earlier distribution of land
and water? Eight Silurian forms do make their appearance amongst the Devonians
of Devon and Cornwall; are not these the very eight thus common? Nowit so hap-
pens that they are not; in fact there is not a single Silurian form in the Lower North
Devon series. This hypothesis then fails. Shall we hold with Professor Phillips, that
“this unequal diffusion of definite forms of life may often be ascribed to eceanic cur-
rents*?” 1 cannot but think that fewer difficulties attach to this than to any other
hypothesis which has been proposed. It simply requires us to suppose that a per-
sistent oceanic stream, flowing through Central Devon, separated the contemporary
deposits of the north and south, and formed, by its thermal or other qualities, an all
but impenetrable barrier to the marine tribes.
Though, as we have seen, at least so far as Devonshire is concerned, the basis
entirely fails on which scepticism respecting the existence of a Devonian period has
been founded, namely, that ‘the blending of Silurian and Carboniferous corals is of
common occurrence,” yet if the word “ fossil” be substituted for “ coral,” a blending
of this kind certainly does occur, and doubiless the fact is not without a meaning.
Eight species from the older and 58 found in the more modern (a total of 66) meet
in Devon. Are they necessarily so many proofs that the rocks in which they were
inhumed are not Devonian? It must be borne in mind that there are 281 species
that are neither Silurian nor Carboniferous, but of an intermediate character. The
paleontological argument then stands thus: there are 66 witnesses supposed to
testify that the rocks are not Devonian, and 281 (upwards of 4 to 1) emphatically
declare that they are. But the adverse witnesses are by no means agreed amongst
themselves ; eight of them claim the rocks as Silurian, and fifty-eight as Carboniferous,
Is there no way of interpreting their evidence, but that of sacrificing the Devonian
system altogether? Are they not so many arguments in favour of the gradual pas-
sage of system into system? so many difficulties in the way of a belief in catastrophes?
by which I mean convulsions (or call it by any other name) which, from time to
time, shook the very life out of the world, causing a series of universal and synchro-
nous depopulations of our planet. May we not regard them as so many tints inter-
mediate, both in quality and in place, between the extreme bands of the rainbow,
uniting them into one beautifully graduated chromatic spectrum, so softly blending
as to render it impossible to define the exact place of lines of demarcation? which
perhaps have not, and never would have been supposed to have, a physical existence,
had not observers hastily generalized from the imperfect evidence obtained during
a period of colour blindness.
But if the Devonshire rocks were handed over to the Carboniferous system, we
should not be quit of the doctrine that some of the forms of one period have, at least’
in some instances, lived through it into the next; for the opponents of a Devonian
period not only admit this, but rest their case on the alleged fact that “ Silurian and-
Carboniferous forms are found blended together in Devonshire and elsewhere.” When,
nearly a quarter of a century ago, Mr. Lonsdale first suggested that the fossils of
South Devon, taken as a whole, exhibited a peculiar character intermediate to those
of the Silurian and Carboniferous groups, he was perfectly aware that amongst them
* Quarterly Journ. Geol. Soc. vol. xvi. p. xl.
Als
100 REPORT—1860.
were forms referable to each of these faunas, yet this did not deter him from making
the suggestion, even in the face of a physical difficulty connected with the culmiferous
beds of North Devon—subsequently removed by Prof. Sedgwick and Sir R. I, Mur-
chison.
And what has been the effect of the recent progress of discovery and nicer discri-
mination on this question? Has it increased or decreased the evidence in favour of
a Devonian period? In 1846 Sir H. De la Beche, discussing this subject, gave a
total of 190 species noticed in South Devon which he disposed of thus: 75 Carboni-
ferous forms, 10 Silurian, 8 common to Silurian and Carboniferous, and 97 peculiar
to Devonshire*. At present—confining ourselves also to South Devon—the lists give
a total of 226, of which 34 are Carboniferous, 6 Silurian, not one common to both,
and 186 peculiar to the district; or putting the totals at each period =1000, and
equating the separate numbers to this, the figures stand as in the following Table, and
show a decided advance Devonianward.
Taste VI.
1846. 1860.
Silurian..... BS Hate riebave ale eae 53 27
Carboniferous.......... Cnet siete 395 150
Silurian and Carboniferous ......... 42 0
Pecnlrarthe re cette tte Cae eee hee 510 823
1000 1000
Doubtless the fact that the Carboniferous forms so greatly outnumber the Silurian
has a meaning. Does not this greater organic affinity betoken a closer chronological
connexion with the more recent than the more ancient period? Is it not an intima-
tion that the lowest beds of Devonshire do not constitute the basement of the Devo-
nian system? That the county has an ample development of Upper and Middle, but
not of Lower Devonian rocks?” .
Hitherto we have accepted the hypothesis that the South Devon rocks are more
ancient than the Barnstaple and Petherwin groups, and that the two last are contem-
poraries. It may perhaps be well before concluding this paper to glance at the bear-
ings of the palzontological evidence at present before us on this point. Putting the
entire series of fossils found in each of the three districts =1000 and equating accord-
ingly, the numbers stand as below.
Tarte VII,
South Devon, | Petherwin. | Barnstaple.
Rihana: a<u-deranuueasnieee 27 14 13
Deyomianiisc sve fiers cueisia tee soatere 823 740 756
Carboniferous ,.........e0008 150 2416 231
1000 1000 1000
Whence it seems tolerably safe to infer that neither of the three deposits is Carboni-
ferous or Silurian, but intermediate, having a closer connexion with the former than
the latter period, and that South Devon is the most ancient of the three groups; but
the evidence is scarcely strong enough to carry any conclusion respecting the relative
age of the remaining two; so far as it goes, it amounts to no more than a suggestion
that Petherwin is rather more modern than Barnstaple. Be that as it may, the fossils
found common to South Devon and each of them must be regarded as contributions
* “Memoirs” of Geological Survey, vol. i. p. 96.
TRANSACTIONS OF THE SECTIONS. 101
from it to them; using the same notation as above, the figures stand—Lower Devo-
nians in Petherwin 205, in Barnstaple 167; and intimate a relative age the reverse of
that just suggested, so that the only thing proved is the insufficiency of the evidence
to decide the point; unless, indeed, it leaves us where it found us, accepting the
hypothesis that the two deposits are strictly of the same age.
The figures now produced, though they fairly represent our present knowledge, can
only be regarded as rough approximations. It is more than probable that whenever
the Census is taken again, it will be found necessary to make, perhaps extensive,
modifications in the Tables.
On some Phenomena of Metamorphism in Coal in the United States.
By Professor H. D. Rogers, LL.D., F.RS., F.GS., Glasgow.
On the Geology of the Neighbourhood of Cambridge and the Fossils of the
Upper Greensand. By the Rev. Professor S—epewick, F.R.S., F.G.S.
On three undescribed Bone-Caves near Tenby, Pembrokeshire.
By the Rev. Gitpert N. SMITH.
The first of these caves was discovered about twenty years ago in blasting a cliff
overhanging the sea at Caldy Island, for the purpose ofgtransporting the mountain
limestone of which it is composed to the opposite coast of Devonshire. It had no
external opening at that time: the side walls were vertical, or nearly so, the strata
standing perpendicular to the plane of the horizon, as they frequently do hereabouts.
The cave was formed by a stratum of considerable thickness, having disappeared at
that place for some eight or ten yards, being probably of softer materials than that
both above and below, supposing the mass to be restored to its natural horizontal posi-
tion; and this apparently by the action of the sea in earlier periods. Both the walls
and the roof have since been removed, so that now no cave exists there; but the floor,
still containing fragments of bone, is covered with the debris of the quarrymen’s
labours,
While the cave yet remained I obtained from it the usual osseous relics of the cave
mammals,—as bones of the Elephas primigenius, Rhinoceros, Sus Scrofa, Equus,
Cervus, Bos, Ursus, Hyena, Felis Tigris or Leo, Lupus, Canis Vulpes, and some
smaller Carnivora. Besides these bones, there were the remains of marine fauna—
abundance of dorsal spines of some species of ray probably: these varied in length
from I3 inch to 2 inches; and other portions of fish skeletons.
The larger bones showed the same marks of gnawing described in the ‘ Reliquiz
Diluvianz’ of buckland. Some of them exhibit down the edges impressions of the
teeth of a Rodent, probably a rat. The nearer these bones lay to the surface of the
red water-washed loam in which they were imbedded, the lighter they were, and more
nearly approaching in every respect the condition of exposed bones of recent existing
animals ; indeed many on the surface were sheep’s bones; but some on high ledges of
the cave were in the same ponderous state as those below, which is usually called
fossil. At this time geology had not so far progressed as to suggest the possibility
of human remains, which therefore, if present, were not observed.
The condition of the cave in general, and the situation of some of the bones in
particular, suggested nothing of the probability of this being a den of hyenas, by whom
the bones had been conveyed into its recesses. but quite the contrary. Hyzenas’ bones
lay about precisely in the same condition as the rest: the whole seemed to have been
forcibly driven into the cavern by the action of water; and some of the bones, par-
ticularly a large ulna, 103 inches in diameter, were wedged firmly into fissures, just
as pieces of drift wreck are observed to be on rocky coasts.
It is assumed in the ‘ Reliquiz Diluvianz’ that the presence of hyena’s dung in
these caves decides this point; but it should be remembered that the hyzna is a bone-
rather than a flesh-eating animal, and that consequently the coprolitic balls are exceed-
ingly hard, being composed almost entirely of phosphate of lime; and that they stand
the action of water almost, if not altogether, as well as the bones themselves. M
impression is that the whole were carried into the cave by water, and that the bones
102 / REPORT—1860.
were gnawed before they were deposited there. Moreover, if these Troglodyte follow
the habits of their congeners in this latitude at present, they will be found to seek
external, and even distant places for the purpose indicated. Badgers, for instance,
resort to the same place nightly; and the ground glitters with the elytra of beetles,
which at one time of the year constitute their principal food. It is an ill bird that
fouls its own nest. The cleanly habits of dogs, too, are well known.
A brief notice will suffice to mark the site of the second cave for future examination.
It is on the same coast-line, and about the same sea-level, but further to the eastward.
Like the former, its walls have been removed. The floor was covered with bones, which
were shovelled into the sea when it was first broken into by the quarrymen.
The particulars of the third cave will at this time be more interesting, perhaps,
because with some of the same remains of Carnivora mentioned aboye, flint-implements,
apparently of human workmanship, have been obtained.
This cave is situated on the main land, and has a large open entrance half-way up
the cliff, known to the inhabitants by the name of ‘the Hoyle.” I am not aware
that it was examined with a definite purpose till about twenty years ago, when Major,
afterwards Colonel, Jervis and Major Pugett exhumed two so-called flint celts, and one
of metal, which were sent toamuseumin London. Lately a more careful examination
has been made of the contents of the red loam which constitutes the floor of what may
be called the first chamber of the Jong winding passage of which this cave consists,
Teeth of the bear and hyzna were discovered in this deposit, together with a consider-
able accumulation of sheep, pigs, and other existing animals. Here also are fish-bones,
mixed with littoral shells like those of our present sea; among them may be named
Patella, Cardium, Purpura lapillus, Mytilus, Littorina littorea, and Natica monili-
fera. Most of these shells are found also in the raised beaches which appear at different
heights ail round the adjacent coasts.
Of the filling of these caves we have possibly some examples in the deep holes
which occur in water-courses, over mountain limestone, in the neighbourhood, and
which receive the mud and water after every glut of rain, for very many years, without
becoming choked or full; but something more in the nature of a flood would really
sometimes appear to be necessary to account for some of the phenomena.
On the Selection of a Peculiar Geological Habitat by some of the rarer
British Plants. By the Rev. W. 8. Symonps, M.A., F.G.S.
The Rev. Mr. Purchas, who is now engaged on the Botany of Herefordshire, has
divided the county of Hereford into twelve districts, and Mr. Symonds has been struck
by the apparent selection of a peculiar geological habitat by some of the rarer British
plants.
The Snowdonian plants appear to affect the bands of volcanic ash that are inter-
stratified with rocks of Snowdon.
Lychnis viscaria grows in four botanical districts out of five in Great Britain on
Greenstone; it grows on Stanner rocks, near Kington, with Scleranthus perennis.
Carex montana is only found on the carboniferous limestone. Lathyrus Aphaca, in
Worcestershire, affects the Keuper marls and sandstones.
Mr. Symonds asks his brother naturalists especially to observe the flora of isolated
trap rocks, and do him the favour of forwarding to him the result of their observation.
On the Geological System of the Central Sahara of Algeria.
By the Rev. H. B. Tristram, W.A., PLS. Sc.
The paper, of which a short summary is appended, was compiled from the notes
and observations made during a six months’ travel in the Sahara. The writer has no
pretensions to being a geologist, nor was geology the object of his wanderings.
But as so little is known respecting the characteristics of this portion of North
Africa, he has not hesitated to give the result of his observations, in the hope that
ae attention of more able and scientific naturalists may be directed to so interesting
a field,
On leaving the Atlas crest, and descending its southern slopes, we soon come upon
the secondary rocks, which are the prevailing formation of the whole country between
the Atlas and Laghouat. This district for about 400 miles due south is rocky,
TRANSACTIONS OF THE SECTIONS. 103
and with mountain-ranges running for the most part in parallel lines north-east and
south-west, The southern slopes of the Atlas chain rise from a depression which in
several parts, especially to the south of Tunis, is many feet below the level of the
Mediterranean. From this depression the Sahara is for the most part a system of end-
less terraces, some of which are only a few miles apart, while others are expanded into
plains of from 50 to 100 miles in width, and which, so far as my observations and the
information I could gather from native caravans and a trustworthy guide extended, in
an unbroken series to within three days’ journey of Timbuctoo, when the traveller will
probably find himself on the northern watershed of the valley of the Niger.
As we advance, on every stage is written the record of the retiring ocean, which
gradually, by the elevation of its southern shores, was driven back and back to the
northward, till the last long inlet from the Gulf of Cabes to Tuggurt was drained and
evaporated, leaving its traces in the salt plains, and occasional moisture of the Wed
BRhir and Chott el Melah—the ancient Lake Tritonis.
There are several singular exceptions to the course of the mountain-ranges above
mentioned, which are generally the local causes of the oases,
Thus at Laghouat we find several elliptical basins of diminishing size piled one on
another. The lowest and largest rests on the flat surface of the secondary rock, which
is the base of the whole system. Several great fissures, which pervade all these super-
imposed basins, allow the water to percolate. It then rests on the impermeable rock,
draining through a very thin stratum of gravel or sand into any depressions, whence
it is raised by artesian wells, and creates an oasis.
From the Sebaa Rous to Laghouat, all these ranges appear to belong to the lower
chalk formation. Limestone predominates, and forms the ridges of the Sahari, Senalba,
and Djellal mountains. It is of saccharoid structure, and of a variable colour, generally
greyish white. In many of the plains there is sandstone, sometimes hard, and at other
times so soft as to yield to the pressure of the fingers. This sandstone encloses nodules
of flint of various colours and semi-transparent. By disaggregation these become de-
tached from the softer medium in which they were imbedded. As the wind sweeps
the sand, they form shingly beaches of pebbles, many of them of a pretty chalcedony,
which is exported in some quantity to Paris.
The upper deposit of limestone is marked by regular beds of gypsum of vast extent,
which are found in every district of the Sahara, but never in the secondary formation
of the Atlas region.
South of Laghouat, the furthest French outpost, we came upon a shallow alluvial
deposit of the very latest tertiary and diluvian formation. Near the mountains this is
often composed of rolled pebbles in a limestone matrix. On the plains it is a white
calcareous rock, a sort of crust, very hard at the surface, but soft and friable below,
where it is mixed with green or grey clay, and epcloses many crystals of gypsum.
The diluvian formation may be traced more or less distinctly, I believe, between
all the ranges, even as far north as the Zahrez, near Djelfa.
I was particularly struck by the fact that several of my fossil shells from these super-
ficial deposits proved specifically identical with freshwater tertiary fossils from the
region of the Black Sea. May not further research perhaps reveal, that at no very
distant geologic epoch a vast chain of freshwater lakes, similar to those of North
America at the present day, extended from the plateaux of the western Sahara as far
as the neighbourhood of the Caspian?
The basin of the M’zab country further still to the south supplied me only with a
few fossils, apparently miocene.
In turning from the M’zab southwards to Waregla, and thence north-east towards
Tuggurt and the Gulf of Cabes, the geological system appears to be the same, but with
fewer distinct little basins, and with more extensive diluvial deposits.
As far as we could trace them, the basins are generally horizontal up to Biskra in
the north, and Gufza in the east, or very slightly inclined, consisting of alternating
beds of greensand (?), gypsum, and clay. These beds extend almost without inter-
ruption, or with very slight depressions, from latitude thirty-one degrees north to
thirty-five degrees north, and from longitude five degrees east to nine degrees east.
The most interesting portion of this district is the Wed R’hir, a long line of depres-
sion sloping from the Touareg desert, latitude thirty degrees north, and longitude five
degrecs east (circiter), with its surface occasionally moistened by salt lakes, but with-
104 REPORT—1860.
out any springs of fresh water, yet affording at intervals throughout its whole extent
a never-failing supply of sweet water, through artesian wells penetrating the upper
limestone. An immense population is supported by this Wed R’hir, which is for many
days’ journey one continuous line of oases, such as El Marier, ‘Tamerna, Tuggurt,
Temacin, and after a further interval, in which its traces are lost, it reappears in the
oases of N’Goussa and Waregla, and gradually is lost in the highlands of the south.
But it is probable that even here the subterranean course of the water can be traced,
and that the Touareg owe their means of subsistence to their knowledge of wells on
this line.
The Wed R’bir terminates in the Chott Melr’hir, a depression probably eighty feet
below the Mediterranean sea-level and the lowest point of the whole Sahara. This
basin extends eastwards to the Chott el Melah (Lake Tritonis), at a greater elevation,
but yet scarcely rising to the sea-level, from which it is separated by some thirty miles
of sand-hills and rocks.
Proceeding northwards of the Melr’hir, we rapidly lose all traces of the diluvial
deposits, and come upon the chalk, chalk-marl, and greensand in regular succession,
dipping generally southwards. The three southernmost ridges of the Mons Aures,
viz. the Djebel Checha, the Dj. Khaddou, and Dj. Amar, present us with these three
stages of the cretaceous group in order.
When we advance to the north of Biskra, the boundary between the Tell and the
eastern Sahara, the mountains are composed of masses of nummulite limestone, with
bands of gypsum and occasional interruptions of rock-salt, mixed with layers of marl.
One of these mountains of rock-salt has been described long since by Dr. Shaw—that
of El Outaia.
There are many salt deposits, sometimes masses of isolated rock-salt, perfectly pure,
of many hundred yards in circumference, as at Hadjera el Mehl (or Rochers de Sel),
more frequently in the form of layers or incrustations on the plains near the Chotts,
or beds of evaporated lakes. Some of the isolated rock-salt hills have been suggested
to have been eruptions of argillaceous mud, gypsum, and rock-salt across the secondary
and tertiary deposits.
In such a country as the Sahara, we cannot expect to find much mineral wealth,
beyond the salt, gypsum, and natron. There is a quarry of oxide of manganese in the
Djebel Trisgrarine, traces of lignite and carbonized trees at Ain el Ibel, and many hot
springs—some pure, others strongly impregnated with chlorine. The temperature of
one of these I found to be 125° Fahr., of others from 75° to 95° Fahr. in one of the
latter were swarms of a little fish, Cyprinodon dispar, also found in the warm springs
of Egypt.
On the Invertebrate Fauna of the Lower Oolites of Oxfordshire. By J. F.
Wuireaves, F.G.S., Honorary Member of the Ashmolean Society, Oxford.
Although the physical geology of the neighbourhood of Oxford is, with some ex-
ceptions, tolerably well understood, our knowledge of its paleontology, especially of
the invertebrate division of the animal kingdom, is very meagre and unsatisfactory.
The only exception I am aware of is a detailed list of the fossils of the Stonesfield
Slate, in a paper contributed by Prof. Phillips to the volume of ‘* Oxford Essays” for
1855, entitled “ The Neighbourhoed of Oxford and its Geology.”
The following brief sketch of the Invertebrata obtained from the Great Oolite,
Forest Marble, and Cornbrash during several years’ collecting, must be considered as
temporary only, nearly every day spent in practical investigation revealing fresh
species, only a very small area having been carefully explored, and even that small
area by no means so thoroughly as one could wish. Hence the few inductions that
I have, as it seems to me, /egetimately deduced from facts, must be considered as
approximate results only in the present state of our knowledge. ‘To Prof. Phillips's
list of the fossils of the Stonesfield Slate, I am enabled to add twenty-eight species of
Mollusca; these are,—
Ammonites Waterhousei, Mor. and Lye. Nerita hemisphxrica, Roemer.
Cerithium ? minuta, Sow.
Natica canalicnlata?, Mor. and Lyc. costulata, Deshayes.
Lulima communis, Mor.and Lye. (castsonly. rugosa, Mor. and Lyc.
TRANSACTIONS
Trochus spiratus, D’ Archiac.
Pecten retiferus, for. and Lyc.
personatus, Gold/uss.
Hinnites abjectus, P/il.
Placunopsis radians ?, Mor. and Lyc.
socialis, Mor. and Lyc.
Pteroperna pygmea, Koch and Dunker.
Gervillia aviculoides ?, Sow.
Modiola compressa, Portlock.
Cardium Stricklandi, Mor. and Lyc.
OF THE SECTIONS. 105
Opis lunulatus, Sow.
Astarte Wiltoni, Mor. and Lyc.
angulata, Mor. and Lyc.
—— squamula, D’ drch.
pumila, Sow.
Tancredia brevis, Mor. and Lye.
curtansata, Phillips.
Quenstedtia oblita, Mor. and Lye. (young.)
Corbula involuta, Goldf.
Pholas —— ?
We may add also, on the authority of Dr. Wright, two Echinoderms, viz. Clypeus
Plott, Klein, and Pseudodiadema Parkinsoni, Wright.
In deep cuttings on the Oxford, Worcester, and Wolverhampton Railway, between
the Handborough and Charlbury stations (especially in two sections nearly opposite
the village of Stonesfield), the lower zone of the Great Oolite is well exhibited. Near
the Kirtlington station on the Great Western Railway several fine sections exposing
the upper zone of the same formation may be studied with advantage: for detailed
descriptions of these beds see Hull’s Memoir on the Geology of the country round
Woodstock. Up tothe present date (June, 1860), the following is a list of the Inver-
tebrata procured from these localities,
From the lower zone in the railway cuttings nearly opposite Stonesfield :—
Isastreea explanata, M‘Coy.
— Montlivaltia trochoides ?, M.-Edw.
Acrosalenia hemicidaroides, Wr.
Echinobrissus Woodwardi, Wr.
— Griesbachii, Wr.
Clypeus Milleri, Wr.
— Rhynchonella concinna, Sow.
— obsoleta, Sow.
Terebratula globata ?, Sow.
maxillata, Sow.
Ostrea Sowerbyi, Mor. and Lyc. —
subrugulosa, Mor. and Lye. -
—— gregarea, Sow. —
acuminata, Sow. -
Placunopsis socialis, Mor. and Lye. -
Pecten lens, Sow.
vagans, Sow. «
Gervillia acuta, Sow. ~
new sp.
Perna rugosa, Mor. and Lye. -
Lima cardiiformis, Sow. —
duplicata, Sow. ~-
Modiola imbricata, Sow. ~*
Mytilus sublzevis, Sow. -
Arca emula, Phillips.
Macrodon Hirsonensis, D’4rch.
Trigonia Moretoni, Mor. and Lyc. ~
Cardium Buckmani, Mor. and Lye.
—— Stricklandi, Mor. and Lyc. —
Cypricardia Bathonica, D’ Orb. -
— nuculiformis, Roemer.
rostrata, Sow. (casts.) —
Astarte angulata, Mor. and Lyc. —
Cyprina Loweana, var., Mor. and Lyc. ~
Tancredia brevis, Mor. and Lyc. ~
new sp.
Nezra Ibbetsoni, Morris. —
Myacites dilatus ?, Phil.
Pholadomya ovulum, Mor. and Lyc. —
Heraulti, .4g. ;
Cylindrites angulatus ?, Mor. and Lyc.
Stomatia Buvignieri, Mor. and Lyc.
Monodonta Labadyei, D’ Archiac.
Trochus Ibbetsoni, Mor. and Lyc.
Nerita rugosa, Mor. and Lyc.
costulata, Desh.
— hemispherica, Roem.
Natica Michelini, D’ Arch.
Chemnitzia, new sp.
Nerinza Eudesii, Desi.
Voltzii, Dest.
From the upper zone, at the Kirtlington railway station and at Enslow Bridge.—By
far the larger portion of this assemblage was obtained from the beds marked G, in
Professor Phillips’s description of the secticn at the Kirtlington railway station. The
species marked with an asterisk were procured from the Enslow Bridge quarries.
Anabacia orbulites, Lame.
*Clypeus Plotii, Klein.
* Miulleri, Wright.
Acrosalenia hemicidarvides, Wr.
Diastopora diluviana, M.-Edwards.
Rhynchonella concinna, Sow.
Terebratula maxillata, Sow.
digona, Sow.
Placunopsis socialis, Mor. and Lye.
*Pecten arcuatus, Sow. *
annulatus, Sow. =
Pteroperna costatula, Desi. ~
— emarginata, Mor. and Lyc. ~
Gervillia acuta, Sow. -
— monotis, Desi. -
106 REPORT—1860.
Gervillia ovata, Sow.
crassicosta, Mor. and Lye.
Lima cardiiformis, Sow.
Pinna cuneata, Phillips.
Modiola imbricata, Sow.
Arca Prattii, Mor. and Lye.
zemula, Phillips. -
Cucullea >
Nucula Menkii, Roemer.
variabilis, Sow.
Limopsis ooliticus, D’ Archiac. -
Cardium subtrigonum, Mor. and Lye. ~
—— Stricklandi, Mor. and Lyc.
—— incertum, Phillivs (fide Lycet?).
new sp.
Lueina striatula, Buvign.
cardioides, D’ Archiac.
Sphera Madridi, Mor. and Lye.
Cypricardia rostrata, Sow.
~ Astarte squamula, D’ Archiac.
~ —— Wiltoni, Mor. and Lye.
-* extensa, Phillips.
_Cyprina Loweana, Mor. and Lye.
depressiuscula, Mor. and Lyc.
Tancredia, new sp.
Corbula inyoluta, Goldf. ~
new sp.
~ Nezra Ibbetsoni, Morris.
*Myacites Scarburgensis, Phillips.
calceiformis, Phillips.
*Pholadomya Heraulti, Agass. ~
* solitaria, Mor. and Lyc. ~
Actzonina oliveformis, Dunker.
bulimoides, Mor. and Lye.
parvula, Roemer.
*Cylindrites brevis, Mor. and Lye.
new sp.
Bulla, new sp.
Patella cingulata, Goldfuss.
Phasianella elegans, Mor. and Lye.
Leymeriei, D’ Archiac.
Monodonta Labadyei, D’ Archiae.
Trochus spiratus, var., D’ Archiae.
—— Ibbetsoni?, Mor. and Lye.
Nerita minuta, Sow.
Nerita hemispherica, Roemer.
Rissoina acuta, Sow.
new sp.
Chemnitzia, new sp.
Eulima communis, Mor. and Lye.
Natica intermedia, Mor. and Lye.
>
Ceritella rissoides, Bur.
unilineata, Sow.
Nerina Eudesii, Desi.
Voltzii, Des.
funiculus ?, Des/.
Cerithium, new sp.
Alaria trifida, Phillips.
levigata, Mor. and Lye.
*
— decurtatus, Phillips. *Ammonites subcontractus, Mor, and Lye.
Until the publication of the Monograph on the Mollusca of the Great Oolite (by
Messrs. Morris and Lycett), but little was known respecting the fossils of this forma-
tion. This monograph, too, was not so much an account of English Great Oolite
fossils in general, as of a particular assemblage, restricted for the most part to a
limited area around Minchinhampton. ‘The above lists of species appear to me
chiefly interesting as tending to remove the apparent isolation of the Minchinhampton
fauna. As in Gloucestershire, so in Oxfordshire, the Cephalopoda seem to be but
sparingly distributed in the Great Oolite ; and but few species of carnivorous Gaste-
ropods have yet been detected in the same formation near Oxford.
As compared with the same zone of life at Minchinhampton, the upper beds of the
Oxfordshire Great Oolite would seem apparently to have been deposited in seas of
greater depth and of more tranquillity, Bivalves are commonly found with the valves
united and the ligament preserved, and large reef-like masses of coral are not unfre-
quent. In Oxfordshire a large proportion of the Great Oolite fossils range upwards
into the Forest Marble and Cornbrash, and no inconsiderable series occur even as high
as the €oralline Ovlite. Five species have not previously been detected in this for-
mation, and eleven shells are quite new to science. From the Forest Marble at Islip
and Kidlington I have collected the following species :—
Placunopsis socialis, Mor. and Lyc. -
Gervillia acuta, Sow. -
Pteroperna costatula, Desi. ~
Lima cardiiformis, Sow. -
duplicata, Sow. «
Arca minuta, Sow. ~<
Nucula variabilis, Sow. -
Leda lacryma, Sow. ~-
Limopsis ooliticus, D’Arch. ~
Trigonia Moretoni, Mor. and Lye. ~
costata, Sow. -
Cardium Stricklandi, Mor. and Lye. ~
Cypricardia rostrata, Sow. —
Astarte interlineata, yc. <
Anabacia orbulites, Lame.
Cricopora straminea, Phillips.
Rhynchonella concinna, Sow.
Terebratula cardium, Lam.
var. bifurcata.
Ostrea Sowerbyi, Mor. and Lyc. ~
acuminata, Sow. :
Pecten rigidus, Sow. -
— annulatus, Sow. °
lens, Sow. =»
— arcuatus, Sow. «
—— personatus, Goldf.-
TRANSACTIONS OF THE SECTIONS. 107
—Astarte minima, Phil. Eulima communis, Mor. and Lye.
—— new sp. Rissoina duplicata, Sow.
—Cyprina Loweana, Mor. and Lyc. levis, Sow.
Corbis, new sp. new sp.
-Tancredia truncata, Lye. Nerita minuta, Sow.
Corbula inyoluta, Goldf. Brochus spiratus, D’ Arch.
— Macneilii, Morris. - Ibbetsoni, Mor. and Lyc.
—— new sp. Crossostoma discoideum, Mor. and Lyc.
—— new sp. Pagodus nodosa, Mor. and Lyc.
Pholadomya acuticosta, Sow. — Patella cingulata, Goldf.
Cerithium quadricinctum, Goldfuss. Emarginula scalaris, Sow.
Ceritella acuta, Mor. and Lye. Cylindrites acutus, Sow.
— longiscata, Buv. Actzonina Luidii, Mor.
The similarity between the fossils of this group and those of the Great Oolite is
very remarkable ; many Minchinhampton fossils occur in it which, as yet, I have been
unable to detect in the Great Oolite of this district. Teeth of fishes, which are so
abundant in the Wiltshire Forest Marble, appear to be somewhat rare in the same
beds in Oxfordshire. The Cornbrash at Islip and Kidlington has yielded the following
assemblage.
Cidaris Bradfordiensis, Wr. (plates and Lima impressa, Mor. and Lye.-
spines). Mytilus sublevis, Sow.
Pedina Smithii, Fordes. Modiola Sowerbyana, Bronn. -
Acrosalenia hemicidaroides, Wr. — compressa, Portlock. —
spinosa, Agassiz. —— bipartita?, Sow.
Stomechinus intermedius, Agassiz (with —— aspera, Sow.
spines attached). — imbricata, Sow. ~
Holectypus depressus, Leske. Lithodomus inclnsus, Phillips. -
Echinobrissus clunicularis, Lihwyd. Macrodon Hirsonensis, D' Archiac. —
Clypeus Plotii, Klein. Arca emula, Phillips.
Pygurus Michelini, Coteau. Nucula Menkii, Roemer. ~
—— variabilis, Sow. -
Anabacia orbulites, Lama. Leda mucronata, Sow. —
———— lacryma, Sow. -
Alecto dichotoma, Lama. Trigonia Moretoni, Mor. and Lye. ~
costata, Sow. ~-
Goldfussi, dg. - if
Cardium Buckmani, Mor. and Lyc. -
Stricklandi, Mor. and Lyc. —
subtrigonum, Mor. and Lyc. —
>
Peastopora diluviana, Milne-Edw.
Cricopora straminea, Phillips.
Rhynchonella Morieri, Dav.
concinna, Sow.
Terebratella hemisphzrica, Sow.
Terebratula cardium, Lamarck. Cypricardia rostrata, Sow. (casts). ~
: intermedia, Sow. Bathonica?, D’Oré. =
obovata, Sow. Cyprina Loweana, Mor. and Lyc. ~
Ostrea Sowerbyi, Mor. and Lyc. ~ Tsocardia minima, Sow. ~-
acuminata, Sow. - Corbula involuta, Goldf. -
costata, Sow. Macneilii, Morris.
Placunopsis socialis, Mor. and Lye. ~ new sp.
Pecten vagans, Sow. « Ceromya ——?
— hemicostatus, Mor. and Lyc. ~ Pholadomya lyrata?, Sow,
— arcuatus, Sow. « deltoidea, Sow.
lens, Sow. Myacites gibbosus, Sow.
annulatus, Sow. “ — decurtatus, Phillips. ~
— personatus, Goldfuss. ~ securiformis, Phillips.
Gervillia acuta, Sow. « Gresslya peregrina, Phillips. -
- ovata, Sow. - Patella cingulata, Goldfuss.
new sp. Trochus ?
Lima duplicata, Sow. ~ Monodonta, new sp.
gibbosa, Sow. ~~ Chemnitzia variabilis, Mor. and Lyc.
cardiiformis, Sow, < Actzonina Luidii, Morris.
A careful study of the fossils of the Oxfordshire Cornbrash appears to me by no
means favourable to that theory of Professor Buckman, that the Cornbrash assemblage
of fossils, on the whole, more strongly resembles the fauna of the Inferior than that of
the Great Oolite.
108 REPORT—1860.
Very few of the fossiis common to both the Cornbrash and Inferior Oolite are not
found in the intermediate formation ; and in the above list of Cornbrash fossils, a large
per-centage are well-known Great Oolite species. The great comparative rarity of
the Cephalopoda is also noticeable, both in the Cornbrash and Forest Marble; one
solitary, mutilated fragment of an ammonite in the Islip Cornbrash is the only
example of this class I have seen from these two formations during several years
active collecting.
On the Intermittent Springs of the Chalk and Oolite of the Neighbourhood of
Scarborough. By Captain Woovatt, M.A. F.G.S.
On the Avicula contorta Beds and Lower Lias in the South of England.
By Tuomas Waieut, M.D., F.R.S.E. and GS.
The black shales, with their interstratified sandstones and bone-beds which lie at
the base of the Lias, have by one class of observers been grouped with the Lias, by
others with the Trias; the author had made a series of observations on these beds,
where they are exposed at Westbury, Wainlode, and Aust, on the banks of the Severn;
and at Penarth and Watchet, on the shores of the Bristol Channel: in all these sec-
tions he had found several species of Conchifera, which are special to the beds, as
Avicula contorta, Portl., Pecten Valoniensis, Defr., Mytilus minutus, Goldf., Cardium
Rheticum, Mer., Lima precursor, Quenst., Neoschizodus posterus, Quenst., Cardium,
sp., Cypricardia, sp., Anomya, sp., with several other small bivalve shells which he
was unable to determine. He found the same beds at the base of the Lias in War-
wickshire and Worcestershire ; and they have recently been found in Staffordshive by
Mr. Howell, and several years ago were discovered by General Portlock in Ireland.
In Germany Quenstedt calls these beds Vorlaufer des Lias; they are the true repre-
sentatives of the Upper St. Cassian beds of German geologists, aud the Késsener-
schichten of the Tyrolese. Since they were first described by Von Buch thirty
years ago, they have formed the subject of many interesting observations by conti-
nental geologists, although up to this time it has not been settled whether they belong
to the Trias or to the Lias. ‘The Conchifera found in these beds in England are special
to them, and none of the species pass into the true Lias; whereas it has been asserted
by Sir Philip Egerton and Professor Agassiz that the species of fishes found in the
Bone-beds of England and Ireland are ‘I'riassic forms. Should this statement hold
good, the evidence for the triassic character of the Avicula contorta series will greatly
preponderate over their liassic affinities. M. Jules Martin, in an able memoir, ‘ Palé—
ontologie Stratigraphique de l’Infra-Lias du Département de la Céte-d’Or,’ has exa-
mined these beds in the departments of Cote d’Or, Rhone, Ardeche and Isére, and has
placed them all as Infra-lias. The absence of the Bone-bed from the French deposits,
although found in Luxembourg, is remarkable; and therefore the evidence afforded
by the fossil fishes is excluded from M. Martin’s estimate of the Paleontological afti-
nities of these Infra-Liassic deposits.
Dr. Wright divides the Lower Lias into six zones of life, each characterized by
certain species of mollusca which are special to it; these are—lIst, the zone of Am-
monites planorbis; 2nd, the zone of Ammonites Bucklandi; 3rd, the zone of Ammo-
nites Turneri; 4th, the zone.of Ammonites obtusus; Sth, the zone of Ammonites oxy~-
notus; and 6th, the zone of Ammonites raricostaius. Each of these zones was sepa-
rately described, its fauna enumerated, and the localities where it was developed
ointed out. ‘The Lower Lias in the South of England was compared with the Lower
Tage of Wurtemberg, and the correlations of that formation in both countries pointed
out.
TRANSACTIONS OF THE SECTIONS. 109
BOTANY AND ZOOLOGY, tnctupinc PHYSIOLOGY.
GENERAL.
On the Progress of Natural Science in the United States and Canada.
By Purie P. Carventer, B.A., Ph.D.
THe principal part of this communication was devoted to_an explanation of the
principles and working of the Smithsonian Institution at Washington, D.C. It
was founded “ for the increase and diffusion of knowledge among men,” and was
not restricted either by nation or “red tape.” It gives aid to students in prose-
cuting any branch of research ; carries on an extensive series of meteorological
observations over the North American Continent; directs the Natural History
observations of the various governmental Exploring Expeditions of the U.S. Govern-
ment; superintends an intricate system of exchanges of books and specimens
between individuals or Societies in Europe or America, in conjunction with the
Royal Society, and with special exemption from customs; and gives to the world
a large amount of original matter through the press. The entire Museum depart-
ment of the United States Government, till lately deposited at the Patent Office,
is now the property of the Smithsonian Institution, with authority to exchange
duplicates. The publications consist of three classes—(1) the “ Smithsonian Con-
tributions to Knowledge,” expensive works sold at cost price ; (2) the ‘Miscellane-
ous Collections” of pamphlets, which are freely distributed; and (3) an annual
yolume of Reports, &c. published at Government expense. In regulating exchanges,
whether of books or specimens, the directors do not require a guid pro quo, but
simply a friendly reciprocity ; their first desire being to make their materials useful
to science, wherever that can best be done*.
The Federal Government, as well as most of the Sovereign States, have published
Reports on Geology and other branches of science, many of which are of the highest
value. The ten quarto volumes on the ‘ Pacific Railroad,’ abounding in plates,
contain a complete réswmé of the Natural History of the great western deserts and
the Rocky Mountains, and may be purchased in Washington for about £5. The
State of Massachusetts is giving liberal aid to Professor Agassiz in forming a
magnificent museum at Cambridge University, which will be arranged geographi-
cally. There is already a vast amount of material accessible to students, and of
duplicates for exchanges. The State Museum at Albany is under the direction of
the Regents of the University of New York. They have a large number of dupli-
cate palxozoic fossils, available for exchange. The Academy of Natural Science of
Philadelphia, the Lyceum of New York, and the Natural History Society of Boston,
are well known by their publications. The Colleges of Yale, Amherst, and
Charleston, 8.C., have also dore good service to science. In Canada, the Geologi-
cal Survey under Sir W. Logan is not surpassed by any for admirable arrangement.
The Natural History Societies both of Montreal and of Toronto publish periodicals.
In M‘Gill College, Montreal, under Professor Dawson, and in the University of
Toronto, under Professor Hincks, the study of natural science is steadily increasing,
The importance of the magnetic observations at Toronto is well known; and a
system of recording meteorological information, at the public grammar schools of
Canada West, is now being organized in connexion with the Smithsonian Institu-
tion.
Remarks on the Final Causes of the Sexuality of Plants, with particular refer-
ence to Mr. Darwin’s Work ‘ On the Origin of Species by Natural Selec-
tion, By C.J. B.Dauseny, UD. LL.D., F.RS., Professor of Botany
in the University of Oxford.
Dr. Daubeny began by pointing out the identity between the two modes by which
the multiplication of plants is brought about, the very same properties being im-
parted to the bud or to the graft, as to the seed produced by the ordinary process
of fecundation; and a new individual being in either instance equally produced.
* All communications to the Smithsonian Institution should be addressed to ‘‘ Professor
Henry, Secretary of the Smithsonian Institution, Washington, D.C., U.S.A.”
110 REPORT—1860.
We are therefore led to speculate as to the final cause of the existence of sexual
organs, in plants, as well as in those lower animals which can be propagated by
cuttings.
Que use, no doubt, may be the dissemination of the species ; for many plants, if
propagated by buds alone, would bein a manner confined to asingle spot. Another
secondary use is the production of fruits which afford nourishment to animals. A
third may be to minister to the gratification of the senses of man by the beauty
of their forms and colours.
But as these ends are only answered in a small proportion of cases, we must
seek further for the uses of the organs in question; and hence the author suggested,
that they might have been provided, in order to prevent that uniformity in the
aspect of Nature which would have prevailed if plants had been multiplied exclu-
sively by buds.
It is well known that a bud is a mere counterpart of the stock from whence it
springs, so that we are always sure of obtaining the very same description of fruit
by merely grafting the bud or cutting of a pear or apple tree upon another plant of
the same species.
On the other hand, the seed never produces an individual exactly like the plant
from which it sprung, and hence by the union of the sexes in plants some variation
from the primitive type is sure to result.
~ Dr. Daubeny remarked, that if we adopt in any degree the views of Mr. Darwin
with respect to the origin of species by natural selection, the creation of sexual
organs in plants nlight be regarded as intended to promote this specific object.
Whilst, however, he gave his assent to the Darwinian hypothesis, as likely to aid us
in reducing the number of existing species, he wished not to be considered as advo-
cating it to the extent to which the author seems disposed to carry it. He rather
desired to recommend to Naturalists the necessity of further inquiries, in order
to fix the limits within which the doctrine proposed by Darwin may assist us in
distinguishing varieties from species.
Botany.
Dr. DAUBENY invited the Members to visit an experimental garden under his
superintendence in the neighbourhood of Oxford, in which he had been carrying on
some investigations connected with Agricultural Chemistry, the nature of which
he proposed to explain on the spot.
On a Plant Poisoning a Plant. By R. Downey.
On Abnormal Forms of Passiflora cerulea. By Dr. C. Dresser.
On the Morpholegical Laws in Plants. By Dr. C. Dresser.
On the supposed Germination of Mummy Wheat.
By the Rev. Professor Henstow, W.A., F.LS.
The author introduced his observations by reading a letter from Professor
Wartmann, of Geneva, who had recently found that seeds might be exposed to
a temperature of 198° below zero of Fahrenheit’s scale, without losing the power
of germination. Professor Henslow had himself exposed seeds to the tempe-
rature of boiling water, and they germinated. The question of how long seeds
would retain their vitality was one of great interest; and a Committee of this
Association had reported on the subject, but they had not succeeded in making
seeds grow which had been kept more than two centuries. He then showed that
experiments recorded on the growth of mummy wheat were not trustworthy;
and especially noticed the case which had been relied on so much, of the growth of
mummy wheat by Mr. Tupper from seeds supplied him by Sir Gardner Wilkinson.
He alluded to a sample of mummy wheat which he had carefully inspected grain
TRANSACTIONS OF THE SECTIONS. 111
by grain, and found among it two grains of a different variety from the rest ; these
were perfectly fresh, whereas the others were dark-coloured, with decided indica-
tions of decomposition and partial charring. Upon inquiry he was able to ascer-
tain that this sample was a portion of a large stock, which had been taken from a
catacomb some years previously, and had been exposed for sale in the jars of a
corn merchant at Cairo, There could be no doubt an accidental admixture of a
few recent grains left in the jars had taken place. In samples supplied by Sir G.
Wilkinson to the late Robert Brown for the purpose of experiment, the latter
had found in it a few grains of Indian corn! He thought it not at all improbable
that the samples he had examined, and those furnished by Sir G, Wilkinson, might
have formed portions of the same stock.
On the Distinctions of a Plant and an Animal, and on a Fourth Kingdom
of Nature*. By Joun Hoce, M.A, F.RS., PLS. &e.
The author stated the great difficulty he had long experienced when examining
some of the simpler living beings, in defining the characters of those primary
forms of life, whether they belone to the vegetable or animal kingdom; and he
considered that there may strictly be no distinction in nature between those king-
doms; and that life in the lowest animal, as well as in the simplest plant, may be
the same; still that it is necessary to draw a line of demarcation between them, for
the purpose of classifying the numerous creatures or organisms existing in the world.
Mr. J. Hoge then showed that he had, more than twenty years ago, demonstrated
that locomotion, although apparently spontaneous, was no distinction of animality.
Neither could the presence of iodine nor of starch be accounted a satisfactory test
of vegetability. So the four chemical elements, hydrogen, carbon, nitrogen, and
oxygen, have been regarded for the same objects, though without positive success ;
and even the green colouring matter, called “chromule,” or “ chlorophyll” (once
supposed to belong exclusively to vegetables), has been shown to be likewise pre-
sent in certain of the lower animals. But the author observed that the “two prin-
cipal characteristics of an animal are undoubtedly the muscular and nervous systems,
which do not exist in a plant, and which Prof. Owen has not included in his de+
finitions of a plant and an animal given in his new work on ‘ Paleontology,’ ”
Mr. J. Hoge then referred to Linnzeus’s arrangement of all natural bodies into
three kingdoms, and, after quoting his definitions of Lapides, Vegetabilia, and
Animalia, said that they must at this day be accounted as insufficient and too
concise; and, considering the great extension of science, both in Zoology and
Botany, which had taken place since the time of Linnzus, he attempted to enlarge
the definitions of those three divisions of natural bodies thus :—Minerals are bodies,
hard, aggregative, simple, or component, haying bulk, weight, and often regular
form; but inorganic, inanimate, indestructible by death, insentient, and illocomo-
tive. Vegetables are beings, organic, living, nourishable, stomachless, generative,
destructible by death, possessing some sensibility, sometimes motive, and some-
times locomotive in their young or seed state; but inanimate, insentient, immus-
cular, nerveless, and mostly fixed by their roots. Animals are beings, organic,
living, nourishable, having a stomach, generative, destructible by death, motive,
animate, sentient, muscular, nervous, and mostly spontaneously locomotive, but
sometimes fixed by their bases.
Further, as regards a fourth kingdom of Nature, the author having perused
Prof. Owen’s ‘ Paleontology,’ published this year, found that he had introduced
the “Kingdom Protozoa,” and placed it before the ‘‘ Kingdom Animalia.” He
roved that there were objections to the term “ Protozoa,” which was formed by a
foreign naturalist, and that it could not include those lower organisms, whose
nature partook more of plants (Phyta) than of animals (Zoa) without creating
errors; and since it appears tv many desirable to place those organic beings which
are of a doubtful nature in a fourth or an additional kingdom, he suggested one
under the title of the Primigenal Kingdom,—Regnum Primigenum continens
Protoctista, ¢. e. Protophyta et Protozca. This would comprise all the lower
creatures, or the primary organic beings—* Protoctista,” from mpdros, first, and
* This entire paper, with the coloured Diagram, is published in the ‘Edinburgh New
Philosophical Journal,’ yol. xii. (new series) for October 1860, pp. 216-225,
112 REPORT—1860.
krista, created beings—hoth Protophyta and Protozoa; and would also include
the Sponges or Amorphozoa of M. de Blainville, although Mr. J. Hogg thought
it better to substitute for the latter the name of Amorphoctista, derived from
apophos, formless, and xriora, creatwres or organisms. ; ‘
Some having compared the Vegetable and Animal Kingdoms to éwo pyramids,
which diverge from each other as they ascend, but are placed on a common base,
the author conceived that that base might fairly represent the Primigenal King-
dom, which embraces the lower or primary organisms of both the former, but
which are of a doubtful nature, and can, in some instances, only be considered as
haying become blended or mingled together.
An accompanying diagram was exhibited, which represented the two pyramids
springing from the same base: one, coloured yellow, denoted the Vegetable King-
dom; the other was tinged blue, and signified the Animal Kingdom; whilst the
base, common to both, was coloured ereen, which was intended to show by the
union of the two former colours the blending of the two natures of the lower
created beings comprised in the fourth, or Primigenal Kingdom. These pyramids,
with their base, stood on a foundation tinged brown, thereby signifying the earth
and the Mineral Kingdom.
On the Normal and Abnormal Variations from an assumed Type in Plants.
By M. 'T. Masters.
The paper was illustrated by a large number of recent and dried forms of mon-
strous plants and parts of plants.
In this paper there was an attempt to show that no definite limits could be
drawn between what are termed Variations and Monstrosities. Numerous instances
of extreme degrees of variation and of polymorphism in plants, apparently depend-
ent on external circumstances, were exhibited; among them two specimens of
Ficus stipularis, the one taken fromaplant grown against awall, the other from a plant
of the same species, and derived from the same original stock, but which had been
treated as a standard. The differences in habit, size, form and texture of the leaves
and other parts were such, that had the two specimens not been taken from the
same plant, it would have been difficult to believe that they could have belonged to
the same species. Allusion was made to the changes that naturally take place during
the growth of some plants, and to the fact that a condition which is unnatural in
one plant is the common condition in another. So also irregularity of growth, as
it is the constant condition in some plants, and for many other reasons, cannot be
considered an abnormal variation. On the other hand, Peloria, or a return to typical
regularity, can hardly be considered abnormal. Again, certain changes which are
physiologically abnormal are not so morphologically. ‘The paper concluded with a
review of the principal points of distinction between variations and malformations,
areyiew which showed that no arbitrary line could be drawn between them.
On the Structure of Fern Stems. By G. Octrvie, M.D.
The object of this communication was to determine the arrangement and rela-
tions of those tissues in Ferns commonly regarded as analogous to the vascular and
woody elements of the stems of the higher plants.
In the case of the former the correspondence may be admitted without much
hesitation, from the close resemblance of the vascular bundles of ferns to those of
endogenous stems ; the fasciculi in both being imbedded separately in the general
parenchyma, and each surrounded by a layer of soft cambium tissue. The peculi-
arities of the Fern consist in the polygonal form and ladder-like or scalariform
markings of its elongated cells or vessels, and in the disposition of the fasciculi, so
as to form, by their anastomosis, the reticulated wall of a hollow cylinder, imbedded
in the general parenchyma of the stem—an arrangement which is rarely departed
from in our British ferns, though in Pter’s aquilina we find in addition two broad
vascular bands in the central part of the stem, and in Osmunda and Hymenophyllum
we have the netted cylinder replaced by a central vascular cord, as in the Lycopo-
diacez. The correspondence of the hard tissues to the true stem-wood of the
higher plants is more open to objection, notwithstanding the occasional resemblance
in their minute structure, The so-called woody fibres of ferns are never, like those
TRANSACTIONS OF THE SECTIONS. 113
of the Phanerogamia, associated with the vessels in the same fasciculus or layer ;
nor are they ever surrounded by a stratum of cambium tissue ; but they are merely
indurated and transformed portions of the general parenchyma, and this even when,
as in some species, they form a sort of outer sheath to the fasciculi. Its great
variability is another point which assimilates this element rather to such sclero-
genous formations of the higher plants as nut-shells and other husky tissues, than
to the proper wood of their stems. In some it occurs only as a thin cortical coating
(Polypodium, Lastrea Filix-Mas, Asplenium Filic-Femina) ; in others it constitutes
the entire mass of the rhizome, except a thin sheath of soft tissue surrounding the
vascular bundles (Blechnwin, Osmunda, Hymenophyllum) ; while there are various
intermediate forms in which it occurs in the guise of isolated nodules or filaments
(Lastrea dilatata, L. oreopteris) of sheaths to the vascular bundles (Asplenium), or of
one or more longitudinal tracts (Allosorus, Pieris). [These variations were illus-
trated by magnitied sectional views of thirteen species, mostly British. ]
The true homologue of the stem-wood of the Phanerogamia is to be sought, it
haz been suggested, in a fibrous stratum which occurs in the fasciculi of some tree
ferns, immediately within the cambium layer; for though these fibres have nothing
of a woody character, and are mostly represented in our indigenous species only by
an outer series of small and imperfectly developed scalaritorm vessels, it is the
outer layer corresponding to them which is woody in the fasciculi of the endogenous
stem, and in all the cases its development seems to show that it arises from a
peculiar transformation of the cells of the cambium tissue.
ZOOLOGY.
On the Acclimatization of Animals, Birds, &c., in the United Kingdom.
By Frank T. Buckianp.
Remarks on the Respiration of the Nudibranchiate Mollusca. By CUTHBERT
Cottincwoop, M.B., F.L.S., §¢., Professor of Animal Physiology in
Queen’s College, Liverpool.
The author described and exhibited drawings of a remarkable immature form
of Z'riopa claviger, which had led to the observations he was about to make,
more especially on account of the entire absence of the branchial plumes. He
canvassed the various definitions given by authors of the term Nudibranchiata,
and showed that, although it might with accuracy be applied to the family Dori-
didee, the Molidide could not with propriety be called Nudibranchs, inasmuch as
their papille were neither anatomically nor morphologically to be regarded as
gills. These mollusks all respired by the whole surface of the body, more or less;
and the author suggested that in the Doridinz the appendages to the body were
supplementary to the branchial plumes; which, as a rule, were less developed in
them than in the true Dorids, which were without such appendages. The fact,
however, that there was no specialized apparatus for respiration in the A¥olidide,
coupled with many analogies which that family bore to animals much lower in
the scale of organization, seemed to separate them much more widely from the
Nudibranchiata proper than was generally allowed.
On the Nudibranchiate Mollusca of the Mersey and Dee. By CuTuBert
Cottinewooo, M.B., F.L.S., &c., Professor of Animal Physiology in
Queen's College, Liverpool.
The author dwelt particularly upon the richnes3 of the estuaries of these
rivers in this beautiful group, and especially referred to some very interesting
forms, such as Doris depressa, D. subquadrata, D. proxima, and Eohs Landsburgi,
E. concinna, &c., which were found in them. The most interesting of all, however,
was Antiopa hyalina, a yery local species, only found at Hilbre Island, in the Dee,
1860. 8
114 REPORT—1860.
where it was discovered by Mr. Byerley, and where the present writer had found it
in the same rock-pool, with its congener A. cristata. He submitted the following
Catalogue of the Nudibranchiata of the Mersey and Dee.
Doris tuberculata. Mersey and Dee; common.
Johnstoni, Mersey and Dee; once or twice.
proxima. Mersey and Dee; common (nowhere else).
— bilamellata. Mersey and Dee; abundant.
pilosa. Mersey and Dee; not uncommon.
— subquadrata. Dee; once (the second known specimen).
depressa. Dee; once.
Polycera Lessonii. Mersey; occasional.
ocellata. Mersey and Dee; occasional.
10. Ancula cristata. Mersey and Dee; common.
11, Tritonia Hombergii. Mersey and Dee; occasional.
plebeia. Mersey and Dee; occasional,
18, Dendronotus arborescens. Mersey and Dee; common.
14. Doto coronata. Mersey and Dee; very common.
15. Eolis papillosa. Mersey and Dee; common.
coronata. Mersey and Dee; common.
17. —— Drummondi. Mersey and Dee; very common.
18. —— rufibranchialis. Mersey and Dee; not uncommon.
Landsburgii.. Mersey and Dee; rare.
concinna. Mersey; common (the second known locality).
21. —— olivacea. Dee (once taken),
aurantiaca. Mersey and Dee; common.
picta, Mersey and Dee; not uncommon,
24, —_—exigua. Mersey; apparently rare.
: despecta. Mersey; common.
26. Embletonia pallida. Mersey (the only known locality); very rare.
27, Antiopa cristata. Dee; occasional.
28, —— hyalina, Dee (the only known locality); very rare.
$9: GON SD Sup CO LS ps
On Recurrent Animal Form, and its Significance in Systematic Zoology. By
Curusert Cotiincwoop, M.B., F.L.S., §c., Professor of Animal Phy-
siology in Queen’s College, Liverpool.
The object of this paper was to call attention to the frequent recurrence of similar
forms in widely-separated groups of the animal kingdom; similarities, therefore,
which were unaccompanied by homologies of internal structure. These analogies
of form had greatly influenced the progress of classification, by attracting the atten-
tion of systematizers, while as yet structural homologies were imperfectly under-
stood ; and, as a consequence, many groups of animals had been temporarily located
in a false position, such as bats and whales by the ancients, and the Polyzoa and
Foraminifera in more modern times. These resemblances in form were illustrated
generally by the classes of Vertebrata, and more especially by the various orders of
Mammalia,—the Invertebrata affording, however, many remarkable examples.
Since no principle of gradation of form would sufficiently account for these ana-
logies, the author had endeavoured to discover some other explanation, and had
come to the conclusion, that the fact of deviations from typical form being accom-
panied by modifications of typical habits, afforded the desired clue. Examples of
this were given, and the principle educed, that agreement of habit and economy in
widely separated groups is accompanied by similarity of form. This position was
argued through simple cases to the more complex, and the conclusion arrived at
that, where habits were known, the explanation sufficed; and it was only in the
case of animals of low organization and obscure or unknown habits, that any serious
difficulty arose in its application ; so that our appreciation of the rationale of their
similarity of form was in direct ratio to our knowledge of their habits and modes
of life. In conclusion, by a comparison of the Polyzoa with the Polyps, it was
TRANSACTIONS OF THE SECTIONS. 115
shown that the economy of both was nearly identical, although they possessed
scarcely anything in common except superficial characters; and this identity of
habit was regarded as the explanation of their remarkable similarity of form.
This it is published (as read before the Section) in the ‘ Annals of Natural
History, for August 1860; and still more at length in the volume of ‘ Proceedings
of the Liverpool Literary and Philosophical Society’ for the past Session.
Dr. DavBEny gave an account of some experiments he had performed on the
subject of Equivocal Generation. He described the apparatus he had employed,
and stated that, even after vegetable matter had been exposed to a temperature
exceeding 300° of Fahr., and had been subsequently brought into contact with
nothing but water carefully distilled, and with air that had been passed through
sulphuric acid, indications of organic life were discoverable in it.
r. Daubeny stated that Dr. Bowerbank and other gentlemen had examined the
flasks in which he had performed his experiments on Equivocal Generation. No
animal life was to be found, but a few filaments of fungi were visible. As the
latter might possibly have been derived from the cork and linseed-meal, as was
suggested by Dr. Bowerbank, he proposed to repeat the experiment under circum-
stances which would eliminate these sources of error,
——_
On the Intellectual Development of Europe, considered with reference to the
views of Mr. Darwin and others, that the Progression of Organisms is de-
termined by Law. By Professor Drarer, M.D., New York.
The object of this paper was to show that the advancement of Man in civilization
does not occur accidentally or in a fortuitous manner, but is determined by im-
mutable law.
The author introduced his subject by recalling proofs of the dominion of law in
the three great lines of the manifestation of life :—first, in the successive stages of
development of every individual from the earliest rudiment to maturity; second,
in the numberless organic forms now living contemporaneously with us, and con-
stituting the animal series; third, in the orderly appearance of that grand succes-
sion, which in the slow lapse of geological time has emerged, constituting the life
of the earth, showing therefore not only the evidences, but also proofs of the domi-
nion of law oyer the world of life.
In these three lines of life he maintained that the general principle is to differ-
entiate instinct from automatism, and then to differentiate intelligence from instinct,
In man himself three distinct instrumental nervous mechanisms exist, and three
distinct modes of life are perceptible, the automatic, the instinctive, the intelligent.
2 piey occur in an epochal order, from infancy through childhood to the more per-
ect state.
Such holding good for the individual, it was then affirmed that it is physiologi-
cally impossible to separate the individual from the race, and that what holds good
for the one holds good for the other too, and hence that man is the Archetype of
Society, and individual development the model of social progress, and that both are
under the control of immutable law; that a parallel exists between individual and
natural life in this, that the production, life, and death of an organic particle in the
_ person, answers to the production, life, and death of a person in the nation.
Turning from these purely physiological considerations to historical proof, and
selecting the only European nation which thus far has offered a complete and com-
pleted intellectual life, Professor Draper showed that the characteristics of Greek
mental development answer perfectly to those of individual life, presenting philo-
sophically five well-marked ages or periods, the first being closed by the opening
of Egypt to the Ionians ; the second, including the Ionian, Pythagorean, and Eleatic
et, was ended by the criticisms of the Sophists ; the third, embracing the
ocratic and Platonic, by the doubts of the Sceptics ; the fourth, ushered in by the
Macedonian expedition and adorned by the splendid achievements of the Alex-
andrian School, degenerated into Neoplatonism ; and imbecility in the fifth, to which
the hand of Rome put an end. From the solutions of the four great problems of
Greek philosophy, given in each of these five stages of its life, he showed that it is
3”
116 REPORT—1860.
possible to determine the law of the variation of Greek opinion, and to establish its
analogy with that of the variations of opinion in individual life.
Next, passing to the consideration of urope in the aggregate, Professor Draper
showed that it has already in part repeated these phases in its intellectual life.
Its first period closes with the spread of the power of Republican Rome, the second
with the foundation of Constantinople, the third with the Turkish invasion of
Europe ; we are living in the fourth. Detailed proofs of the correspondence of these
periods to those of Greek life, and through them to those of individual life, are
given in a work now printing on this subject by the author in America.
Having established this conclusion, Professor Draper next briefly alluded to many
collateral problems or inquiries. He showed that the advances of men are due to
external and not to interior influences, and that in this respect a nation is like a
seed, which can only develope when the conditions are favourable, and then onl
in a definite way; that the time for psychical change corresponds with that for
physical, and that a nation cannot advance except its material condition be touched,
this having been the case throughout all Europe, as is manifested by the diminution
of the blue-eyed races thereof; that all organisms, and even man, are dependent for
their characteristics, continuance, and life, on the physical conditions under which
they: live; that the existing apparent invariability presented by the world of
organization is the direct consequence of the physical equilibrium ; but that, if that
should suffer modification, in an instant the fanciful doctrine of the immutability
of species would be brought to its proper value. The organic world appears to be
in repose because natural influences have reached an equilibrium. A marble may
remain motionless for ever on a level table, but let the table be a little inclined,
and the marble will quickly run off, and so it is with organisms in the world. From
his work on Physiology, published in 1856, he gave his views in support of the
doctrine of the transmutation of species, the transitional forms of the animal and
also the human type, the production of new ethnical elements or nations, and the
laws of their origin, duration and death.
On some Specimens of Shells from the Liverpool Museum, originally from
the Pathological Collection formed by the late Mr. Gaskoin. By the Rev.
H. H. Hicerns, W.A., Rainhill, Liverpool.
The late Mr. Gaskoin had in his museum a series of specimens, collected for the
purpose of illustrating the pathology of the Mollusca, This series was in course of
formation in the year 1835, from which period, to the time of his decease, Mr.
Gaskoin devoted considerable attention to the selection, from various sources, of
specimens of shells in any wise remarkable for distorted growth, or for the repair
of injuries received during the life of the animal. Iam not aware that Mr. Gaskoin
published or left in manuscript any account of the result of his observations in this
department of Natural History. 1t is evident that in any case of abnormal growth a
second, and still more a third or a fourth, instance of the same kind may afford a
fair ground for a conclusion, which, if based upon a single instance only, would be
of little or no value. ‘he extensive character of the series was in this respect very
valuable. In the course of more than twenty years’ collecting, Mr. Gaskoin had
enriched his pathological cabinet, not only with a great variety of mended fractures
and distorted growths, but with many duplicates, sometimes of cases apparently
altogether exceptional, and likely to be unique. A select series of specimens was
then exhibited to the Section, and remarks were made upon them, which can
scarcely be presented intelligibly apart from the specimens themselves.
Notice of British Well Shrimps. By the Rev. A. R. Hocan, WA.
The author exhibited specimens of some remarkable additions not long since
made to our British Crustacea. They consisted of two species of Miphargus (Fon-
tanus and Kochianus), and the new genus Crangonyx, with its single species swb-
terrancus of Spence Bate. These species have been described and figured in the
volume of the ‘ Natural History Review and Quarterly Journal of Science’ for last
yea (1859). They are of great interest, as examples of a subterranean Fauna in
ngland, analogous to that long known on the Continent and in America, The
ea Or
a
TRANSACTIONS OF THE SECTIONS. 17
first established instance of the occurrence of Niphargiin England, was Mr. West-
wood's discovery at Maidenhead, Berkshire, of a well containing numbers of IV.
aquiler. They have more recently been obtained from Corsham and Warminster,
Wiltshire, and also from Ringwood, on the borders of the New lorest, Hampshire.
Crangonyx subterrancus has occurred at the two latter places, but not at the first
named, Miphargus fontanus is found at both Corsham and Ringwood, but with a
difference in the shape of the gnathopoda and posterior pleopoda, amounting to a pro-
bably distinct variety, if not species. The form of the gnathopoda, or hands, is
worthy of attention, being each armed with a moveable claw of large size, forming
a prehensile organ of great power. NV. fontanus is also possessed of small, yellow
eyes, which distinguish it in a very marked way from the allied species (of the
genus Gammarus) found on the Continent. Every member of the subterranean
Fauna hitherto found has been destitute of eyesight. The movements of Niphargi,
when kept in captivity, are interesting to observe; but Mr, Hogan states that ia
has found great difficulty in preserving them alive. The longest period during which
even the strongest specimens survived its capture was three wecks. ‘The average
temperature of the water in which Miphargus and Crangonya are found is about
50° Fahr., and they seem to propagate in recently-formed wells as freely as in old
ones. In no case have any species of this family been found, either in this country or
abroad, in open wells or other than artificial ones,—pumps, in fact. They are found
at all seasons of the year, but most abundantly towards the end of the autumn. The
largest size known among the English species (that of NV. fontanus) hardly exceeds
half an inch. Mr. Hogan hoped that more extended observations would be made
in Great Britain on this interesting family of Crustacea, as their economy and struc-
ture are as yet very imperfectly known, and an accurate examination would be sure
to reward the investigator with results at least as interesting as those already
obtained regarding their allies by Vontinental naturalists.
Mr. J. G. Jurrreys exhibited several specimens of the conmon whelk (Bucctnwm
undatum) having double opercula; in one instance, a second or supplementary
operculum being piled on the usual one ; and in the others, there being two separate
opercula, instead of one, in each whelk. He adverted briefly to the different kinds
of monstrosity which occur in animals and plants, and said he believed this to be
the first case of a similar monstrosity in the Mollusca. He observed that the
monstrosity under consideration appeared to be congenital, and not to have arisen
from an accidental loss of the original organ, because in some of the specimens both
opercula were cases of hypertrophy, and in the others of atrophy ; and he mentioned
that all the specimens came from the same place (Sandgate in Kent), showing a
repetition, and perhaps an hereditary transmission, of the same abnormal pheno-
‘nenon ; and he suggested that thus permanent varieties might in course of time
be formed, and constitute what some naturalists would call “ distinct species.” He
adduced in support of this view, the case of a reversed monstrosity of the common
garden snail (Helix aspersa), having been bred for many years in succession by the
late M. d‘Orbigny in his garden at Rochelle, as well as many instances of a
reversed form of almond whelk (Luss antiguus) having occurred in the same
localities on the coasts of England and Portugal, such bemg the normal form in
the crag.
On the British Teredines, or Ship-Woris.
By J. G. Jerrreys, PRS.
After observing that his researches had not been confined to the British Tere~
dines, but that he had recently had an opportunity of meeting all the French
naturalists who had published on the subject, as well as of studying all the access-
ible collections and books, he treated the matter first in a zoological point of
view, and gaye a short history of the genus Zeredo, from the time of Aristotle and
his pupil Theophrastus to the present time ; especially noticing the elaborate mono-
raph of Sellius, in 1733, on the Dutch ship-worm; the valuable paper of Sir
Hverard Home and his pupil Sir Benjamin Brodie, in 1806 ; and the physiological
essays of Quatrefages, in 1849,
118 REPORT—1860.
He showed that the Teredo undergoes a series of metamorphoses ; the eggs being
developed into a sub-larval form after their exclusion from the ovary, and remaining
in the mantle of the parent for some time. In its second phase (or that of proper
larve) the fry are furnished with a pair of close-fitting oval valves, resembling those
of a Cythere, as well as with cilia, a large foot, and distinct eyes, by means of which
it swims freely and with great rapidity, or creeps, and afterwards selects its fixed
habitation. The larval state continues for upwards of 100 hours, and during that
period the fry are capable of traversing long distances, and thus becoming spread
over comparatively wide areas. The metamorphosis is not, however (as Quatrefages
asserts), complete ; because the young shell, when fully developed, retains the larval
valves. He then discussed the different theories, as to the method by which the
Teredo perforates wood, giving a preference to that of Sellius and Quatrefages, which
may be termed the theory of “ suction,” aided by a constant maceration of the wood
by water, which is introduced into the tube by the siphons. This process, according
to Quatrefages, is effected by an organ which he calls the “ capuchon céphalique,” and
which is provided with two pairs of muscles of extraordinary strength. Mr. Jeffreys
was of opinion that the foot of the Teredo was the sole instrument of perforation.
He instanced, in illustration of this theory, the cases of the common limpet, as
well as of many bivalve mollusks, Echinus lividus, and numerous annelids, which
excayate rocks to a greater or less depth; and he cited the adage of “ Gutta cavat
lapidem non vi sed seepe cadendo,” in opposition to the mechanical theory. The
Teredo bores either in the direction of the grain or across it, according to the kind of
wood and the nature of the species ; the Teredo Norvegica usually taking the former
course: every kind of wood is indiscriminately attacked by it. The Teredines con-
stitute a peaceful, though not a social community; and they have never been known
to work into the tunnel of any neighbour. If they approach too near to each other,
and cannot find space enough in any direction to continue their operations, they en-
close the valves or anterior part of the body in a case, consisting of one or more hemi-
spherical layers of shelly matter. Sellius supposed that the Zeredo ate up the wood
which it excayated, and had no other food ; and, labouring under the idea that it
could no longer subsist after being thus voluntarily shut wp, he considered it to be
the pink of chivalry and honour, in preferring to commit suicide rather than infringe
on its neighbour. In this enclosed state the valves often become so much altered
in form, as well as in the relative proportion of their different parts, as not to be
easily recognizable as belonging to the same species ; and one species ( 7. divaricata)
was constituted from specimens of Z. Norvegica which had been so deformed. The
food of the Teredo consists of minute animalcula, which are brought within the
vortex of the inhalant siphon, and drawn into the stomach. The wood which has
been excavated also undergoes a kind of digestion during its passage outwards
through the long intestine. The animal has been proved by Laurent and other
observers to be capable of renewing its shelly tube, and of repairing it in any part.
It is stated by Quatrefages (and apparently with truth) that the sexes are separate,
impregnation being effected in a similar mode to that which takes place among
alm-trees and other dicecious plants. There appear to be only five or six males
in one hundred individuals. The Teredo perforates and inhabits sound wood only,
but an allied genus (Xylophaga) has been recently found to attack the submarine
telegraph cable between this country and Gibraltar at a depth of from sixty to
seventy fathoms, and to have made its way through a thick wrapper of cordage into
the gutta percha which covered the wire. The penetration was fortunately dis-
covered in time, and was not deep enough to reach the wire. He gave several
instances to show the rapidity of its perforating powers,—one of them haying been
supplied by Sir Leopold M‘Clintock while he was serving with the author’s brother
in the North Pacific.
Mr. Jeffreys traced the geographical distribution of the Teredines, and showed
that at least two species, which are now found living on our own shores, occurred in
the post-pleistocene period; and he inferred from the circumstance of one of these
species having been found in fossil drift wood, that conditions similar to the present
existed during that epoch. Some species inhabit fixed wood, and may be termed
ittoral,” while others are only found in floating wood, and appear to be “ pelagic.”
Each geographical district has its own “littoral” species, and the old notion of
he ship-worm (which Linnzus justly called “ Calamitas Navium”) haying been
TRANSACTIONS OF THE SECTIONS. 119
introduced into Europe from the Indies was contrary to fact as well as theory, be-
cause no “littoral” species belonging to tropical seas has ever been found living
in the northern hemisphere, or vice versd. 1t is true that some species have been
occasionally imported into this and other countries in ships’ bottoms, and that
others occur in wood which has been wafted thither by the Gulf and other oceanic
currents; but the former cases belong to littoral species, and never survive their
remoyal, while the latter may be said to be almost cosmopolite. Every species of
Teredo has its own peculiar tube, valves, and pair of “ pallets,” the latter serving the
office of opercula, and by their means the animal is able at will to close completely
the entrance or mouth of the tube, and thus prevent the intrusion of crustacean
and annelidan foes. The length of the tube is, of course, equal to that of the
animal, which is attached to it by strong muscles in the palletal ring, and varies
in the different species from three inches, or even less, to as many feet. The in-
ternal entrance or throat of the tube is also distinguishable in each species by its
— transverse laminz, and it has frequently a longitudinal siphonal ridge.
onstrosities occasionally occur in the valves and pallets; and in one instance the
pallet-stalk is double, showing a partial redundancy of organs, as exemplified by
the author with respect to the operculum of the common whelk. More than one
species often inhabit the same piece of wood; and want of sufficient care by natu-
ralists in extracting the valves with their proper tubes and pallets may account in a
great measure for the confusion which exists in public and private collections, and
which has thence found its way into systematic works. The Zeredines have many
natural enemies. In the South of Italy, and on the North African coast, they are
esteemed as human food. In Great Britain and Ireland, four species occur in fixed
wood, and eleven others in drift wood, the latter being occasional visitants. Of
these, no less than six have never yet been described, and two others are now, for the .
first time, noticed as British. The number of recorded exotic species only amounts
to six more, making a total of twenty-one ; but it is probable that, when the subject
has been more investigated, a considerable addition will be made to this number.
Mr. Jeffreys then explained the distribution of the littoral species on the shores of
Great Britain and Ireland, and produced a synoptical list with descriptions of the
new species. He believed all the Teredines were marine, except, possibly, Adanson’s
Senegal species, and one which had lately been found in the River Ganges, the
water of which is fresh for about eighteen hours out of the twenty-four, and brackish”
during the rest of the day; but as a well-known exception of the same kind occurs
in a genus of marine shells (47a), and the transition from fresh to brackish, and
thence to salt water, is very gradual, such exceptions should not be regarded with
suspicion or surprise. He concluded this part of the subject by exhibiting some
drawings and specimens, and acknowledging his obligations to Dr. Lukis and other
scientific friends.
He afterwards treated the subject in an economical point of view, and remarked
that, although the French Government had issued two commissions at different
times, and the Dutch Government had lately published the report of another com-
mission, which was appointed to inquire into the mode of preventing the ravages
of the Zeredo in the ships and harbours of those countries, our own Government
had done nothing. He alluded to the numerous and various remedies which had
been proposed, during the last two or three centuries from time to time, some of
which were very absurd; but he was of opinion, from a study of the creature’s
habits, that the most effectual preventive would be a siliceous or mineral composi-
tion, like that which has been proposed by Prof. Ansted for coating the decompusing
stones of our new Houses of Parliament, or simply a thick coat of tar or paint,
continually applied, which would not only destroy any adult ship-worms then
living in the wood, but prevent the ingress of the fry. The Zeredo never com-
mences perforation except in the larval state *.
A Committee of the Association was formed, at the suggestion of Mr. Jeffreys
to inquire and report as to the best mode of preventing the ravages of Teredo an
other animals in our ships and harbours.
* See also Papers by Mr. Jeffreys on this subject in the ‘Annals of Natural History’
for August and October 1860,
120 REPORT—1860.
Dr. LanxkesTer called attention to the completion of the first part of Mr. Black-
wall’s work on British Spiders,—a copy of which he placed on the table. The
work contains twelve coloured plates, and is one of the most complete monographs
hitherto published of the class of animals to which itis devoted. It forms the Ray
Society’s volume for 1859.
—_——
On the Statistics of the Herring Fishery. By Cuanrtes W. Peacu.
On Cydippe. By Joun Price, Chester.
I will only remind my fellow-naturalists that the Cydippe (which has been, like
everything else, retarded by this cold season) was pretty abundant in the Mersey
on the 16th of June, and may therefore be looked for confidently on the coast
henceforward.
In order to enjoy the sight of this most enchanting Oceanid, I advise them—
1. To provide tall glass jars, or, faute de mieux, the largest size of “sample bot-
tles,” que¢e transparent, and with large mouths. The last can be taken to the shore
in a frame like a cruet stand to hold several bottles, corked during carriage.
. 2. To catch the animals in some cup or ladle large enough to take up a gill of
water with them, to prevent damage. Best of all, ina 3 spherical ladle, with
tubular handle.
In either case, plunge it in a full inch in advance of the swimming Cydippe, to
save the trains, which easily break.
3. To keep them, when transferred to their permanent Jodging-jar, glass or
a Ppebyeas as cold as possible; and never (except when examining them) in a
ull light,
‘ 4, ‘lo watch minutely for the ova (grey specks smaller than “Noctilucee”) floating
near the surface; and ladle them out (say with a salt-spoon) as most interesting
microscopic objects before and after hatching.
5. To microscope, with a low power, Cydippes containing food ; easily known, as
they are transparent. And if you get the right kind of prawn, they will capture
and swallow them, but not shrimps.
6, If Beroes are to be had, and Cydippes are “as plenty as blackberries,” re-
member that the dutter are the natural food of the former, who will bolt as many
as five, one after the other.
7. By wniting the two last hints, my curious friends may see, by virtue of the
ts ara of both animals, two digestions going on ( for a short time) at once.
The Cydippe digests the prawn, whilst the Beroe digests the Cydippe. Qu. Inges-
tion ?, Digestion ?, Indigestion ?. :
8. To remember that a number of these creatures were kept in the “good old
times” for 13 weeks, without plants, and only changing the water occasionally ;
that these perished after all by mere accident, and that it is the pleasing duty of the
rising generation to keep them all the year round under the improved régime.
On the Aspergillum or Watering-pot Mollusk.
By Lovett Reeve, F.L.S., F.G.S.
The Aspergillum is a siphoned bivalve mollusk which ceases in an early stage of
its existence to live free, and while yet no more than the eighth of an inch in length,
sinks into the sand, or adheres to shell or stone, and directs its calcifying functions
to the formation of a comparatively large tubular sheath. Upwards the sheath
enlarges with the growth of the siphons for their special protection ; downwards
the animal closes in the sheath by a disc like the rose of a watering-pot, fissured and
erforated and bordered by a frill of small tubes.. The mantle of the animal, which
as been observed once, and only once, on the shores of the Red Sea, enlarges on
commencing its sheath growth, and a number of tentacles are emitted, each corre-
sponding with a perforation or tube of the disc. Frequent distortion is imparted to
the shell, more especially to the disc end of it, the scat of the mollusk, according to
the circumstances of its place of habitation ; and when adhering to shell or stone
the disc may be scarcely recognizable. Shells with the strength of growth even of
Spondylus, hecome distorted by their inability to contend against the outward press-
TRANSACTIONS OF THE SECTIONS. 121
ure of foreign bodies. Shells, therefore, of the delicate and comparatively fragile
growth of Aspergillum would be liable to extreme contortion. Asperyillum vagini-
ferum, inhabiting the shores of the Red Sea, sinks into the sand, as may be seen
by the particles of sand and shell débris that become agglutinated to the sheath, to
the depth of eight to twelve inches and more ; the sheath is comparatively straight
and symmetrical, and the protruding end becomes furbelowed. A season of rest
ensues, another effort is made to extend the sheath, but the calcifying functions
either have done their part, or are enfeebled. A little is added to the sheath, and
the end is again furbelowed ; and in some specimens the process has been as many
as eight times repeated.
In adherent species, only one of which, 4. Strangez, inhabiting the shores of
N.E. Australia, has been discovered, the disc is very much pressed in, Two speci-
mens only have been collected, one affixed to the inner cleft of a mussel hinge, and
one attached to stone. The peculiarity of this form of Aspergillum is that the
sheath is formed in a square, and being formed, not in sand, but free, is tortuous and
enveloped by a slight periostracum.
Dr. Gray has stated his opinion in a recent memoir in the ‘ Proceedings of the
Zoological Society,’ that the sheath of A. Stranget is an enlargement of the primi-
tive pair of valves, and that it differs in this respect from the rest of the Aspergila,
I incline to dissent from this opinion. Whether by a stretch of induction 1t be
regarded as an enlargement of the primitive valves, or not, the relation between
them [ hold to be the same in the sand-inhabiting species, as in the adherent species.
Dr. Gray also draws a distinction between species which have a wavy depression in
the sheath around the circumference of the valves, regarding the wavy depression
as a part of the valves, of which only the umbones are seen. My own view is that
at the time of the metamorphosis of the mollusk, the valves are not larger in any
species than are defined by the smaller outline. When it is considered that the
valves are discarded at this time, but not entirely, inasmuch as they are appropriated
as material for a nucleus from which to develope a sheath, it is only reasonable to
suppose that the new sheath matter would, in some species, obtain a wavy deposit
corresponding with the outline of the nucleus.
Remarks on the Geographical Distribution of recent Terrestrial Vertebrata.
By P. L. Scrater, M.A., Ph.D., See.ZS.
After enunciating the principles of the distribution of organic beings according to
certain laws, independent of the influences of climate and other external conditions,
and that of the “continuity ” of generic areas, which might, as a general rule, be
extended to all natural groups, small and large, the author proceeded to point out
what appeared to be the most natural primary divisions of the earth’s surface, as
deducible from a careful study of the distribution of the terrestrial vertebrates.
These were :—
}. The Palearctic Region, embracing Europe, Asia north of the Himalayas, and a
strip of Africa north of the Atlas.
2. The Athiopian Region, embracing Africa inclusive of Madagascar, and Arabia.
8. The Indian Region, including Southern continental Asia, Sumatra, Borneo,
Java, and other islands down to the Straits of Macassar.
4, The Australian Region, including New Guinea and adjoining islands, Australia,
New Zealand, and Pacitic Islands.
5. The Nearctic Region, including America down to the Southern limits of the
Mexican Table-land.
6. The Neotropical Region, including the rest of the New World and the West
India Islands.
These Regions were well characterized by their striking zoological peculiarities,
as shown by the preponderance of certain types and the absence of others in each ;
and by the fact that many of the families, more of the genera, and nearly all the
species found in each were as a general rule distinct, of which numerous examples
were given. These greater divisions of the earth’s surface or regions were subdi-
visible into lesser areas or provinces, characterized by being the abode of distinct
species, which in many cases represented one another in their different localities.
An inquiry into the meaning of these laws of geographical distribution was then
122 REPORT—1860.
entered upon, and the question asixed, whether it was possible in the present state
of our knowledge of the subject to arrive at any explanation of them. It was
remarked that the only hypothesis yet put forward which would explain these laws,
was that of “ genetic relationship ” between species or their descent from a common
ancestral form. It was an acknowledged fact that the best naturalists were at
issue as to the precise limits between representative species and local varieties.
It was generally allowed that the latter were descendants of a common progenitor,
and the reasons given for the belief in the case of “local varieties ” might be shown
to be equally applicable to “representative species.” Specific differences being once
granted to have originated from natural causes, it would be impossible to stop here,
and it must follow that greater divergences may have resulted from the operation
of similar agents acting through longer periods of time.
On some Peculiar Forms amongst the Micro-Lepidopterous Larve.
By H. T. Sratinron, FLAS.
It is well known that the normal form of a ci ne et larva is a cylinder, flat-
tened beneath, and slightly tapering and rounded at each end. To this, the typical
form of a Lepidopterous larva, we have abundant exceptions in most groups; thus
we have the woodlouse-shaped larvee amongst the butterflies, and again amongst
the Bombycina; and in the latter group we have also numerous instances of larvee
adorned with humps or large protuberances on several of the segments, and in some
of the Noctuze larvee we observe a protuberance on the eleventh segment.
The normal number of legs is sixteen, that is, six true legs and ten prolegs; but
two of the latter are wanting in some of the Bombycina and in some of the Noctuina,
and in the whole group of the Geometrina from four to six of the prolegs are
wanting.
In the group of the Torticina there are very few deviations from the typical form
of the larva; but amongst the Tineina we find many genera which give instances
of very considerable deviation from the regular cylindric form.
Among the most curious forms in this family, the larvee of the genus Phyllocnistis
may be mentioned; in these the hinder extremity is so drawn out that it reminds
us of the rat-tailed larvee amongst the Diptera, though the object of the prolonged
tail in the Phylloenistis larvee is very different. These larve are also perfectly
apodal, and the structure of the mouth is peculiar: the jaws of all other Lepido-
pterous larvee terminate in two sharp-pointed mandibles; the mandibles of a Phyl-
locnistis are perfectly blunt and rounded, like the points of lace-scissors. The
reason of this singular formation is pretty evident; the larve of the genera Coleo-
phora and Lithocolletis, which mine in the interior of leaves, feed on the parenchyma,
which they detach piece by piece by their sharp mandibles and swallow; but the
larvee of Phyllocnistis, though feeding beneath the cuticle of the leaf, do not eat the
parenchyma, and a leaf eaten by one of these larvee, if held up to the light, shows
no trace of the attacks of the larva. On what then do they subsist? The larvae
mine rather rapidly forwards beneath the cuticle, raising the cuticle from the epi-
dermis, and they apparently devour something which they find between the two,
which, as they do not seem to remove any solid matter of the leaf, must be of a
juicy nature. It is no doubt essential to the comfort of these larve that the cuticle
should not remain detached from the parenchyma in those parts of the leaf which
the larva has passed over, and accordingly we find that the cuticle again becomes
attached to the parenchyma immediately behind the larva, and that the cuticle
may be let down gradually and gently is, I believe, the cause of the prolonged
attenuated tail. The object of the blunt mandibles, in like manner, appears to be
to avoid any risk of the larva piercing the cuticle, which by letting in the external
air would probably be fatal to the existence of the larva, as these lary have to
move their jaws in constant juxtaposition to the cuticle, which, in the aspen tree
(which is frequented by the commonest species of the genus, P. sufiusella), is re-
markably thin;; it must be a great convenience to the larva that the structure of its
jaws is such that it can eat its fill without any danger of piercing the cuticle.
Sharp-pointed jaws are necessary to a larva which feeds on the harder parts of
leaves ; but to this, which only, as it were, sucks up the juice, sharp-pointed jaws
are quite unnecessary,
TRANSACTIONS OF THE SECTIONS. 123
If a leaf eaten by this larva be held to the light no symptoms of its operations
will be apparent; but if, instead of holding the leaf between us and the light, we
look down on it slantways, we shall perceive some slightly iridescent tracks, which
have very much the appearance as though a snail had been crawling across the leaf.
Another peculiarity of this larva is that it never moults; its skin is apparently
of so elastic a nature, that it grows with the larva; most larve cast their skins four
or five times in the course of their lives, but this larva never once undergoes that
operation. Besides this, it never sleeps; most larvee, after enjoying a hearty meal,
may be found inactive and inert, in a position which conveys to us precisely the
idea of sleep, but a Phyllocnistis larva never sleeps, it is always eating; from its
exclusion from the egg to its being full-fed, night or day, its jaws are perpetually
at work. This is not true only of the larva of Phyllocnistis, it occurs throughout
the extensive genus of Nepticula. I have had abundant opportunities of observing
these larvee at all hours of the day and night, and, unless they are ill or dying,
they are invariably eating. Their jaws have certainly solved the problem of per-
petual motion.
Ehrenberg expressed surprise that the Infusoria never sleep; and Owen, after
long watching the motions of the Polygastrica, concluded they were generally of
the nature of respiratory acts, and not attempts to obtain food orayvoid danger. He
adds, “ Very seldom can they be construed as voluntary, but seem rather to be
automatic; governed by the influence of stimuli, within or without the body, not
felt but reflected upon the contractile fibre; and therefore are motions which
never tire.”
But the motions of these small larve are certainly not automatic; you frequently
see the larva turning its head about from side to side of its mine, as though con-
sidering where it should eat a bit next, and immediately it has determined that
point it sets to work with a will, little indicative of involuntary action.
On the Effect of Temperature and Periodicity on the Development of
certain Lepidoptera. By Dr. VERLOREN, of Utrecht.
A Table was exhibited showing the period at which the pupe of the Sphing
Tigustri were hatched. From these tables it appeared that the great proportion of
the insects was produced in the middle of June, independent of the state of the
temperature of the season ; and it appeared that in cases where the development of
the insects had been retarded beyond the fixed period in one year, they appeared
only during the limited period in the succeeding year. The observations had been
extended through a number of years, and had enabled Dr. Verloren to establish
seyeral other interesting physiological facts connected with the species in question.
Mr. WEstwoop gave an account of an insect which, on account of its anomalous
character, had been referred to three different orders of the class Insecta, and which
forms the genus Acentropus of Curtis, the type being the Phryganea nivea of Oliver,
regarded as Trichopterous by Curtis, and as Neuropterous by Stephens: Mr. West-
wood had many years ago endeavoured to prove it to be Lepidopterous from a con-
sideration of the structure of the perfect insect alone. The transformations of the
ae having, however, been recently observed by Mr. Brown of Burton-upon-Trent,
the opinion of Mr. Westwood had been fully borne out, as was shown by a series of
highly magnified diagrams representing the details of the insect and its metamor-
phoses, contrasted with those of the orders Trichoptera, Lepidoptera, and Neuro-
ptera. The genus appears to be most nearly allied to the family Crambiz.
On Mummy Beetles. By J.O. Westwoon, M.A, F.L.S.
The object of this paper was to show that no change had taken place in the struc-
ture and habits of several species of insects during the period which had elapsed
since the embalment of the mummies buried in the pyramids of Egypt. A number
of species of such insects had been recorded by Latreille in the work upon Egypt
by M. Calliand; and Mr. Westwood exhibited species of the genera Necrodia and
Dermestes found within the bodies of mummies by Dr. Pettigrew, and which must
have found their way into such bodies during the process of embalment and before
124 REPORT—1860.
the final cere-cloths were applied. These insects were not specifically distinguish-
able from existing species, although of a somewhat paler colour.
On a Lepidopterous Parasite occurring on the Body of the Fulgora candelaria.
By J. O. Westwoopn, M.A. F.L.S.
After some general remarks on parasitism, the author gave a detailed account of
the occurrence of the larvee of a species of moth on the body of the firefly (Fulgora
candelaria), for which the name of Epipyrops anomala had been proposed by Mr.
Bowring, by whom the transformations of the insect had been observed in China.
Not only was the fact of the parasitism of the species as a Lepidopterous insect
extremely unusual, but also the circumstance that it was not upon the ligaments of
the body that the larva of this moth fed, but evidently upon the white waxy secre-
tion so common amongst the Fu/goride, with which their abdomens are enyeloped,
was quite anomalous, although wax-feeding habits were known to occur in the
larvee of the species of wax-moths. The insect in question appeared to belong to
the great family Bombycidz, and specimens were preserved in the British Museum
and Hopeian Collection at Oxford.
Notes on Tomopteris onisciformis. 2y Dr. E. Percevat Wricut, A.M.
Dub. Owon., F.L.S., Lecturer on Zoology, Dublin University.
In the summer of 1858, while investigating with Professor J. Reay Greene of
Cork, the marine zoology of the south-west coast of Ireland, I had an opportunity
of examining somewhat in detail the structure of that puzzling little annulose
animal, called Tomopteris onisciformis. ‘The tidal current sets in very strongly from
the Atlantic into the narrow entrance between Bere Island and the main land, and
carries along with it, in the summer season, whole fleets of oceanic swimming
creatures. ‘The number of naked-eyed Medusze and free Actinozoans is almost pass
belief to those who haye not witnessed similar phenomena. Various little bays
with hollow caverns line the sides of this channel, and in these the water lies very
still and quiet ; here, too, vast numbers of the ocean swimmers congregate, imparting
to the water almost a milky hue, which sometimes changes and presents an appear-
ance as if oil had been cast upon it, owing to the highly prismatic colouring of the
various Beroes, Aquoreas, Cydippes, Kc. A retired nook of this sort is a very
aradise to the marine explorer, and such were to us places of very frequent resort.
After a little practice, one’s eye got accustemed to the varied kinds of locomotion
that distinguished more or less each species, so that when I first perceived T
onisciformis swimming swiftly with its very peculiar wriggling movements, small as
it was, I perceived it to be something new; and afew seconds served to transfer it
to a glass collecting-jar. While the whole body was more or less employed, by
successive wrigglings, in locomotion, yet it was quite obvious that true locomotion
was assisted by the bipinnated series of paddle-shaped organs which are attached
at each side of the body. When compared with the graceful floating and umbrella
movements of an A%quorea, or the headlong paddle-wheel-like moyements of a
Beroe or a Cydippe, it could not be truthfully described as graceful ; nevertheless,
there was something about it very characteristic—something that even seemed to
point out its proper natural affinities. One of the little creatures lived in apparently
good health with me for about twelve hours, though incarcerated in a small glass
jar holding but ten ounces of water; and it would have probably lived longer, but
wanted its tail for examination, and the necessary compressicn of such an agile
and slippery creature between two pieces of thin glass hastened its end. ‘lhe
author then alluded to the papers by Dr. Carpenter, Messrs. Leuckart and Pagen-
stecher and others on this creature, and gave an outline of its anatomy, alluding to
the presence of cilia on the pharyngeal portion, to the peculiar structure of the
central portion of the antenna-lke organs, to the tail-like extremity, and the
presence therein of masses of Spermatozoa; and finally expressed his conviction
that there could be no doubt as to its being a complete creature, and that its tail
is not a zooid form, as hinted by Dr. Carpenter.
7
TRANSACTIONS OF THE SECTIONS. 125
PuysioLoey.
On the Ultimate Arrangement of Nerves in Muscular Tissue.
By Professor Beare, M.B., F.RLS.
On the Leptocephalide. By Professor V. Carus, Leipzig.
Dr. Kaup places the European species of this highly interesting family in four
generic groups,—Esunculus, Hyoprorus, Tilurus, and Leptocephalus. 1t strikes at
first, to find amongst the “ Apodal” fishes a form with well-developed ventral fins,
viz. Esunculus, similar to the rest only in its transparency, and in wanting the
generative organs, differing from them also in the distinctness of the dorsal and anal.
Among the rest there are two well-established genera, Ziduwrus with its hair-like
tail, and Leptocephalus. According to Dr. Kaup, Tilurus contains two species, tri-
chiurus and Rissoi, but both are probably the same, as Risso? is most likely founded
on a mutilated specimen. The chief character is taken from the tail here being
shorter; Dr. Kaup adds, however, himself, “ perhaps defective in the tail.”” The
species of the genus Leptocephalus are to be classed in two groups ; the type of the
first is Z. Morrisii, that of the other is Helmichthys diaphanus ot Ratinesque. The
former have the body compressed, the latter rounder, earth-wormlike body. Z. Mor-
risti and ZL. Spallanzanii differ only by the height of the former, upon which
argument one cannot lay much stress, as exact measurements of many individuals
give very considerable differences in the relative height and length of the whole
body, as well as of the head and the other parts. The species of the second group,
L. punctatus, diaphanus, Kollikert, Gegenbauri, Bibroni, and Yarrelli, are representa-
tives of at most two species, punctatus and diaphanus. The chief distinction is
taken from the relative position of the intestinal outlet. I did not find in two
specimens out of some dozens the same position of this orifice ; nor are the row of
black points, which characterize the Z. punctatus, always so well developed, that
they could be taken as a good character. However, the habits differ in some respect
from that of the rest. L. longirostris reminds of Hyoprorus ; the latter is probably
nothing but a further developed or an earlier form of the Z. longirostris, L. stenops,
and ZL. brevirostris : the two last Muropean species of Dr. Kaup’s Synopsis I know
only by his figures, but I am very much inclined to believe that they are to be
judged like the others.
Taking together the anatomical structure of the whole group, the absence of ge-
nerative organs, the structure of their skin, their skull, their vertebral column, taking
furthermore into consideration the variability of both the zoological characters and
the proportional measurements, I cannot but come to the conclusion that all these
fishes are nothing but /arval forms of others. The developed full-grown species to
which all of them, except the Lsunculus Costar, belong, are most likely among the
Ophidians, or other compressed forms (Cepola, and so on). Although Iam not yet
able to state with certainty what species or even genera are to be studied in their
development as giving Leptocephalideous larvee, yet I feel quite sure that the
family under consideration will ere long be erased from the Systema Nature, just
as the Ammoccetes has been excluded from the benefit of being reckoned a full-
erown member of the Animal family.
On the Value of “ Development” in Systematic Zoology and Animal
Morphology. By Professor V. Carus, Leipzig.
Although there may be some who will object to my bringing forward a topic of
general bearing, and who would prefer to have stated some special facts and details
new to science, yet I think that meetings of this kind afford the best opportunity
of clearing up, or at least recalling to mind, questions which we are all familiar with,
the true bearing of which, howeyer, we are very apt to lose sight of. Since Cuvier
laid the foundation-stone of our modern classification of animals, there has been
within the last thirty-three years much labour bestowed upon the mending his
system, and looking for new characters by which his classes and orders may be
either altered and arranged in a somewhat different manner, or still better founded.
However, we look up to him not only as the reformer of the classificatory branch of
126 : REPORT—-1860.
zoology, but moreover as the founder of the natural system and of the science of
comparative anatomy.
As I intend to inquire into the value of one of the most striking characters of
animals with regard to their classification, as well as to their typical organization, I
may. be allowed to state, first, what is meant by a Systema Animalium, or in other
words, what place the classification of animals takes among the branches of zoolo-
gical inquiry.
We are scarcely aware that we use the word system of animals in quite a differ-
ent sense from thatin which Linneeus used it, and which was intended even by Cuvier
when he arranged the animal kingdom anew according to its organization. Even
Cuvier compares the system to a great catalogue of animals, in which every single
one can easily be found and named. There is, however, one great feature stamped
upon all forms of organized beings, which, although implied and even indicated in
the system of Cuvier, yet has given to the system of animals quite another aspect,
—I mean the relationship between different animals. Cuvier, and some later natu-
ralists, and I may say some of the best, considered the system only as a servant to
true science. Classification, according to them, is nothing more than, as Stuart Mill
says, acontrivance for the best possible ordering of the ideas of objects in our minds,
and at most “for causing the ideas to accompany or succeed one another in such a
way as shall give us the greatest command over our knowledge already acquired.”
Although a classification worked out in the most perfect manner in this way must
also be one of the aims of our endeavours, yet I may say that our present classifi-
eatory inquiries go further. They start from the very fact that the oldest forms,
and for this reason the forms nearest to the original creation, do not represent any of
those groups of individuals which we are used to call species ; nor can all of them be
classed under the nowestablished genera, families, and orders, but only under the type
to which all succeeding species belong. And although we cannot give the direct ex-
erimental proof, yet we are bound by logicand by truths forced upon us from all other
ranches of natural history, to say that these oldest original forms are the primeval
forms of all living animals, which originated from them by continued generation
and by accommodation to external circumstances continually and progressively
changing*. Hereby the general bearing of the system of animals is totally changed.
We consider it not only as an arrangement of the animals in such a manner as
may help us best in gaining a general view of the animal world, and in placing
and finding certain forms of it; but we try to make it the faithful expression of
the state of our knowledge respecting the relation of all animals to each other.
Passing from the much spoken of differences between artificial and natural
systems, I may only state, that even that arrangement, which is mainly founded on
the internal structure of animals, is nothing more than a somewhat modified form
of artificial system, taking only one set of properties as basis of the classification.
However, it is the best form hitherto proposed, because it takes into consideration
more characters than any other arrangement, and leads us naturally forward in the
study of animal life. There is as yet one great chasm which seyers the classifi-
cation of minerals from that of animals. In the mineral world we are justified in
speaking of species, as the identity of physical and chemical properties grants us the
identity of all bodies endowed with these. In the animal world we have nothing
but individuals, and all sorts of groups are entirely and totally artificial. The law
of equal production of like from like through generations and generations, upon
which the notion of the species mainly is based, cannot be trusted to, as we have no
experience whatever that it holds good for the same animals under different circum-
stances.
Passing in review the leading characters upon which the different subkingdoms
of the animal world are founded, we perceive at once that they change almost in
every class. For although the general headings may be taken from the same system
of organs, yet the splitting of the classes and orders into minor divisions is de-
pendent on characters especially modified by these very classes and orders. And
even here our classification is not quite consistent. Amongst the lower classes of
animals, the comparatively simpler organization allows us to take the general form
of the bodies as a character to be relied upon, yet no person would be able to calla
* T first made the foregoing remarks in my ‘System of Animal Morphology,’ 1853,
Tntroduction.
TRANSACTIONS OF THE SECTIONS. 127
etenophorous medusa a radiated animal. Similar instances may be taken from the
higher divisions of the animal kingdom ; as they are known to all who are familiar
with our zoological system, I should go too far if I were to specify what a little
attention paid to different orders of animals will tellin a moment. The simple
result of carefully looking through the established classes and orders of animals, is
that there is only a relative weight to be laid upon the different groups of zoolo-
gical characters. It depends entirely upon the whole typical organization, and on
the correlation of parts as modified by that type. This correlation of parts, which
allows us to draw a conclusion from the nature of one organ as to the nature of
another, must naturally be changed by the physiological dignity of an organ, which
in different types is not always the same; and it will become uncertain whenever
the characters which we call specific are becoming indistinct themselves.
I thought it necessary to state first in few words, that there is a difference in the
value of zoological characters according to different classes, and I am of opinion
that the progress of zoology as science depends mainly on the determination of
this value in a sharper manner than it has been stated. I published some years
ago some general remarks on this subject in a small pamphlet which will scarcely
haye reached England. Since then my opinion has become still stronger, as I saw
that the progress, which zoology owes of late years especially to some eminent
British naturalists, was chiefly dependent on the circumstance that the point men-
tioned was, with or without purpose, taken into consideration.
The structure of animal bodies shows three different relations of complexity ; com-
mon to all three are these two points; first, that a structure, at first simple, becomes
more and more diversified ; secondly, that all the differences which appear one after
the other make their appearance on a basis fundamentally equal and in itself not
changing. They differ according to the difference of this substratum. In one case
there is one and the same body changing and becoming more and more complex ;
in the second case different members of one great fundamental type of organization
constitute a series of forms, some less, some more diversified ; in the third case the
very types themselves are to be regarded as members of one great series, showing
less and greater complexity. The practice of scientific inquiry has severed these
three different points of view into three different branches of science. The first is
the history of development, which may just as well be called the comparative
anatomy of the individual; the second is the comparative anatomy of the different
types ; the third is the general morphology of the animal kingdom. These are the
three different bearings which animals generally present to the zoologist with regard
to their structure. Now we must ask, what use can we make of them, and of the
first-mentioned especially ? As the zoologist has nothing before him but individuals,
it is no wonder that the comparative anatomy of these will throw much light on
their nature, their life, and their morphology. As long as it is kept in mind that
all the facts of the history of development have relation to the individual, and to
nothing else, so long nobody will object to the manner of inquiring, which is quite
properly called the genetic method.
All our zoological classification, however, tends toward the establishment of
larger groups and types, and here comparative anatomy has its place. It is very
significant, that in the Cuvierian system, which we all follow, its later alterations
being quite irrelevant to the grand truths upon which it is founded, there is no
use whatever made of the history of development, not even in one instance. It
has been said that the emendations of this system, and the whole progress of
systematic zoology, depend, if not chiefly, yet for a great part, on the employment
of the genetic method. On this I may he allowed to make the following remarks,
As comparative anatomy rests entirely on the knowledge of the structure of indivi-
duals, everything which throws light on the individual will also throw light on
comparative anatomy. But with regard to systematic zoology, we have not to
deal with larval forms and immature individuals, but only with such as are able
to propagate their individual, or if you like it better, specific form. We cannot,
of course, put aside all embryological data in our systematic endeavours. How-
ever, there is great danger in overrating the help they give us. A system based
on anatomy alone is an artificial one, however true it may be; but its value is
always great, and the more attention is paid to the physiological and biological
bearings of structural facts, the greater will this value be. A classification of
128 REPORT—1860.
animals from embryonic data, however, is still more artificial; it takes only one
small group of properties of the animals, and just a group which, by its being con-
fined exclusively to individuals, forbids by itself the taking account of other pro-
perties. There are so many striking examples of different development in animals
related as nearly as possible, that by these alone the exclusive use of embryology
a3 a basis for classification is defended. And if the fact of frogs developing with-
out the intermediate stages of tadpoles be true (and I have no reason to doubt it), we
have in one and the same species differences of development which would in other
classes suffice to establish urders. B, this very instance it is shown that embry-
ology also ha3 only a relative value as zoological character. Ournext inquiry ought
to be directed here, a3 well a3 in all other cases, towards the establishment of the
characteral standard of embryology. Nature herself assists us in the rightly
weighing of this character of animal bodies, as almost in all cases it serves only to
contirm and strengthen relations which have been found by other methods.
While there is scarcely any ditficulty in giving to embryology amongst the other
sets of properties its right place with regard to the classification of animals, there
is, I should not like to say difficulty, but some seemingly perplexing complexity of
phenomena and relations, when we are to make out the true bearing of embryology
on animal morphology. Here I have to answer two questions: How must we look
upon animal forms? and secondly, Are we allowed to explain analogous pheno-
mena by methods not correlate to each other? Animal morphology, as the science
of animal forms, has to explain these, that is to say, to bring them back to Jaws. A
law manifested on different forms cannot be that of cause and effect, but only one of
a constant repetition of the same phenomena under seemingly different conditions.
The object of animal morphology therefore will be to show the constancy with which
certain organs appear in certain groups of animals, and to showthat the relative posi-
tion of these organs is always one and the same in the larger and lesser groups. With
regard to the first part of these inquiries, there can be no doubt as to the utter failure
of embryology. Nothing buta simple anatomical investigation can tell us whether a
certain organ or system of organs is present in a certain division of the animal
kingdom or absent ; and respecting the second part of our morphological researches,
{ am equally inclined to doubt whether embryology gives us an insight into the
anatomical specialities of a somewhat more complex animal by anything else, but
by bringing before us certain forms which are not quite as complex as the animal
which we dissect. And here we need not take embryological data; we have before
us in every type of animals a whole series of more and more diversified forms, which
by themselves offer that same series of simpler forms which we find in the indi-
vidual, and even more clearly manifested, because an embryo is always endowed
with certain individual or specific peculiarities, which we cannot at present account
for at all. With respect to my second question, the embryologists say that two
organs which are developed in two different ways cannot be considered homologous.
Now, here I have to give a somewhat similar answer to that which I gave with
respect to the embryological classification. The homology of parts is determined
by the constant relative position of the organs in one andthe same type. An artery
which runs up along the mesial line of the cervical vertebree, is homologically dit.
ferent from an artery which runs along the jugular vein and the pneumogastric
nerve. The morphological relations of a certain class cannot be determined but by
comparing full-grown individuals, as all the organs do not work to the purpose of
these individuals before the development is finished. And in this respect I must
deny any influence of embryological researches on morphological questions. There
is, however, another set of questions frequently brought betcre the morphologist,
namely, whether two homologous organs are developed in the same way. It is
easily seen that their homology must have been determined beforehand. It is of
course of the greatest interest to know the differences of the development of the
same organ in different representatives of the same type. But they show nothing
more than the wonderful facility with which Nature arrives at the same results by
different ways. They give us additional proofs of that immense richness of means
with which the Creator of all animal bodies works out his plans,
On the Deglutition of Alimentary Fluids. By Professor Cornett, M.D.
TRANSACTIONS OF THE SECTIONS. 129
On the Formation of Sugar and Amyloid Substances in the Animal Economy.
By Dr. Roperr M*DonneE tt.
After briefly noticing the history of the discovery by Bernard and Hensen of the
matter named by the former “ glycogene,” the writer observed that the term now
very generally adopted to indicate this substance, viz. “ amyloid matter,” seemed in
the present state of our knowledge preferable, as it did not involve any theory con-
cerning the ultimate destination of the material in question. It was proposed to
embrace under the generic term amyloid substance, two varieties of the starch-like
material known to exist in the animal economy, viz. that of the first species, or the
amyloid substance of Bernard, a ternary compound isomeric with dried erape-
Sugar, convertible by contact with animal ferments into sugar capable of fermenting
on the addition of yeast—and that of the second species, or the amyloid substance of
Virchow, a material, which, although in histological characters analogous to cellulose
and starch, yet as met with in the prostate gland, spleen, choroid plexus, &c., has
not yet been shown to be capable of conversion into sugar undergoing fermentation,
and which cannot be considered free from the intimate admixture of azotized
matters.
Dr. M*Donnell discussed at considerable length the question as to whether the
liver is endowed with the function of converting its amyloid substance into sugar
during life and health, or whether some at least of this substance has not another
destination, viz. that of becoming nitrogenized, and thus being, so to speak, raised
from the class of ternary to that of quaternary compounds.
Admitting that this is one of the most delicate questions in physiology, and being
most unwilling to appear to dogmatize on the subject, the writer detailed a consider=
able number of experiments on blood drawn from the right side of the heart of
animals variously fed, which seem, on the whole, to support the view that trans-
eon into sugar is not the normal destination of the amyloid substance formed
in the liver,
An Experimental Inquiry into the Nature of Sleep.
Sy Arruur E. Durwam.
Contributions to the Theory of Cardiae Inhibition.
By Dr. Micuart Foster.
On certain Alterations in the Medulla Oblongata in cases of Paralysis.
By Rozert Garner, F.L.S.
Tn this paper it was shown, and the fact illustrated by specimens, that in old
paralytic cases the crus cerebri on the side of thecerebral lesion and the corresponding
anterior column below the pons, but only to the decussation, are both found much
atrophied, and this very frequently, though it has been almost entirely overlooked.
In such cases the corresponding olivary body retains its plumpness, and these
anglia, therefore, rather appertain to the columns to be seen on the floor of the
ourth ventricle, and to the posterior or tezumentary portion of the crura. This con-
nexion may be well seen by tearing down the hardened medulla oblongata through
the locus niger, when it will be found that below the pons the posterior torn
portion comes forwards and is firmly connected with the olives,
The author appreciates the remarks of Turck and Van der Kolk, and goes on to
notice how the olfactory and optic nerves are, in different animals, connected, some-
times with the cerebrum principally, in other cases with the cerebral ganglia, or in
others with the medulla oblongata; as they are subservient to the intellectual, the
animal, or to the locomotive, respiratory and automatic functions. Some remarks
on the origin of a few of the cerebral nerves in animals, and a denial that there is
any well-marked distinction of an upper and lower tract in the ganglionic cord of
such animals as the scorpion and scolopendra, as indeed was long ago shown in the
last animal by Mr. Lord, form the conclusion of the paper.
1860. g
130 REPORT—1860.
On the Structure of the Lepadide. By R. Garner, F.L.S.
In this paper the author bore testimony to the high regard for truth with which
Mr. Darwin has recorded his labours, in respect to these animals, though further
observation has modified some of his conclusions, and indeed is still wanted.
From finding fragments of shells, small pebbles, &c. in the cesophagus of the
Lepas anatifera, the author supposes that this part acts as a gizzard, comminutin
the food. With Poli he believes in the existence of a heart, situated on the back,
a little posterior to the base of the second pair of cirri: however, these observers
stand alone with respect to this point. The heart can only be seen in some speci-
mens, according to the state of the tissues, which vary much. It receives its
supply at the sides, and gives off vessels before and behind: other large and lon-
gitudinal vessels exist.
With respect to the canal running along the abdominal side of the peduncle,
and communicating with the body of the animal, on each side, behind the adductor
muscle, the author thinks that by means of it the cavity of the prosoma is distended
with fluid, thus acting as an antagonist to the adductor, parting a little the shelly
valves. The communicating opening lies betsveen the nerves and oviducts as they
course between the peduncle and the body.
Mr. Darwin thought that these oviducts conyeyed the ova from his ovaries, or
the salivary glands of Cuvier, into the peduncle, where ova are found sure enough.
But in some specimens, where they are distended with ova, the oviducts are easily
traced from the peduncle down into the body of the animal, making a sweep, and
apparently ending at the cavities and apertures called acoustic by Mr. Darwin, who
informs us that Krohn has also made out this point. The little membranous,
buskin-shaped follicle, found in this acoustic cavity, is sometimes wanting.
Cuvier did not often use the microscope, or he would haye soon discovered that
his so-called ovaries are, in reality, testes.
Little need he said, after Mr. Darwin, respecting the nervous system. The sub-
oral ganglion, besides being connected by a ring with the supra-oral ganglia, supplies
the salivary glands, the adductor muscle, the viscera, and the mantle by means of a
large anterior branch ; also it gives others to the mouth and first cirri, and is con-
nected of course with the chain of ganelia between the other cirri. From the
supra-oral pair of ganglia, which are in close apposition, two large nerves (anten-
nary of Mr. D.) go to the peduncle, and two minute twigs to the eye, described
exactly in the “ Lepadidie.” With respect to this eye Mr. Darwin observes, “in all
the genera the double eye is seated deep within the body ; it is attached by fibrous
tissue to the radiating muscles of the lowest part of the cesophagus, and lies actually
on the upper part of the stomach; consequenly a ray of light, to reach the eye, has
to pass through the exterior membrane and underlying corium connecting the two
scuta, and to penetrate deeply into the body.” This is not quite all; the little
organ is made perfect in its adaptation, by a small oval or lozenge-shaped trans-
parent spot in these coverings to admit the light, and exactly behind this spot the
eyelet may always be easily seen or found. In specimens of Conchoderma Hunteri,
parasitic on the carapax of a crab from Amoy, this visual organ is situated between
the mouth and the adductor.
The so-called proboscis appears to act as an ovipositor, and probably in the pre-
hension of the food. The ova are finally attached to the “ovigerous fraena” as
broad sheets, with the assistance of a cement, which sometimes glues them unna-
turally together. The fatty matter with which the mantle abounds appears to go
to their nutrition, and is apparently taken in at the roots of the frana. In this
mantle, in some species, the young animals are imbedded, and within its cavity
‘impregnation takes place.
The author’s specimens of Zepas came on shore last January at Kimmeridge,
attached in vast quantities to a beam of pine. Some were a foot and a half in
leneth; mostly simple, but others springing one from another. They are tenacious
of life, and appear to be generally cast on shore upon our coasts in rough winter
weather. The author has had large living Balani picked up in the Mersey, and
has Lepadidse attached to nuts of China, the small shells of a Sepia, and minute
ones on the shells of Zanthina and Spirula from the Gulf-weed,
TRANSACTIONS OF THE SECTIONS. 131
On Saccharine Fermentation within the Female Breast.
By Georce D. Giss, M.D., W.A., F.G.S.
After referring to Vogel’s discovery of vibriones in human milk, and the suspicion
he entertained that their origin was due to fermentation of the milk, but which was
denied by subsequent observers, the author proceeded to state that his own researches
into this question commenced in the latter part of 1854. At that time an infant seven
weeks old was brought to him in the most extreme state of emaciation, whosé
mother had the appearance of good health. The child, although but skin and bone,
was healthy and piump at birth, and was in no way diseased; it had plenty of its
mother’s milk, but never was satisfied, and seemed ravenous. The most profuse
diaphoresis and diuresis had worn it toa shadow. ‘The mother’s milk was found
to be rich in cream, neutral, sp. gr. 1032, and contained a large quantity of sugar.
Examined under the microscope upon the instant of withdrawal from the breast, it
revealed numbers of living animalcules, those known as the Vibrio baculus, but
which he proposed to change to Vibrio lactis as more appropriate. These he con-
sidered the result of fermentation of the saccharine element within the eland.
There was an absence of mammary congestion and heat, which are usually present
in such cases, but much general nervous excitement, which it was necessary to
control by proper treatment. The child was supplied with an abundance of: good
cow’s milk, and gradually weaned, after the lapse of some weeks, and ultimately
completely recovered. The mother’s condition also improved ; the milk continued
to be rich in cream and sugar for some time, varying in sp. er. from 1032 to 1035,
and always neutral; the animalcules remained for some weeks, and finally disap-
peared; and when drawn from the breast, the milk invariably turned sour much
sooner than other examples of cows or healthy human milk.
From 1854 to the present time the author has examined many hundred specimens
of human milk, chemically and microscopically, and has occasionally found twospecies
of animalcules to be present in the glands of those whose general health was dis-
ordered from various causes during lactation, or where the process of lactation was
unusually prolonged, or again, where the quantity of milk secreted was small and
insufficient to satisfy the wants of the infant. At early lactation also, where the
milk was good and plentiful, but with constitutional symptoms present as already
referred to, both species were found, but not in the same individual.
These creatures consisted, first, of the Vibrio lactis, resembling little rod or
minute hair-shaped bodies, similar to those found in some of the other fluids of the
body ; and secondly, of monads, which he has found to be far more frequent and com-
mon than vibriones, and which he proposed to call Monas lactis,
Both species were noticed at all periods of lactation, froma few days to upwards
of twelve months; the colour and specific gravity of the milk varied, but it was inva-
riably alkaline or neutral. The children were mostly skin and bone, resembling
little old men, and soon died of inanition unless other food than the mother’s milk
was supplied to them. It was not these little bodies that disagreed, but the healthy
properties of the milk for assimilation were destroyed, by constitutional causes in
the mother, which imparted as it were a galvanic shock through the agency of the
uterine nervous system, at the moment of its secretion, giving rise to fermentation
in the sugar alone, a substance the author believed the only one likely to produce
it within the breast. This process did not necessarily give rise to the formation of
lactic acid ; had it done so, it would have destroyed the animalcules ; moreover, in no
single instance was the milk ever found acid. ' He referred to some experiments of
Berthelot to show that fermentation of sugar could take place in alkaline fluids;
and the rapidity with which milk containing these animalcules is decomposed and
turns sour out of the breast, now generating a large quantity of lactic acid, the
author considered a strong proof of fermentation having previously commenced
within the breast.
He believed it very probable that the animalcules were generated from the sur-
face of the mucous membrane of the lactiferous tubes, by the fermentation of the
sugar at the moment of its secretion from the blood, and this in some cases explained
the large numbers present. The necessary connexion subsisting between the mam-
mary glands and uterine organs, explained the influence of the latter in producing
the heat and internal congestion of the former by reflex nervous agency, giving rise
to the conditions described, in which the vitality of the milk was much impaired,
*
132 REPORT—1860.
The author then briefly entered into the general question of treatment to be pur-
sued, both for the parent and child, under the circumstances detailed.
On Asiatic Cholera. By Sir CHARLES Gray.
A Word on Embryology, with reference to the mutual relations of the Sub-
kingdoms of Animals. By J. Rray Greene, B.A., Professor of Natural
History in the Queen’s College, Cork.
Tn a communication bearing the above title, the author endeavoured to explain
that any real improvements in the arrangement of the animal kingdom which have
been made since the time of Cuvier accorded well with the corresponding advances
of comparative embryology. Thus only, indeed, were they shown to be true; for
the method of gradations, whatever might be its value in suggesting affinities,
could not, of itself, be deemed sufficient to prove them ; while its exclusive employ-
ment had already, in too many cases, engendered errors, the further multiplication
of which could alone be kept in check by a continual appeal to the test of develop-
ment. From this point of view, the mutual relations of the five sub-kingdoms of
animals appear as in the accompanying analytical Table :—
THE ANIMAL KINGDOM.
The organism does not exhibit a A blastoderm is formed, which
division into true layers. divides into inner and outer
Subkingdom 1. PROTOZOA. layers.
The two layers of the blastoderm The blastodermal layers become
undergo no further funda- further differentiated. The
mental differentiation. There organism exhibits neural and
is no distinction into neural heemal regions.
and heemal regions.
Subkingdom 2. CAALENTERATA.
he hemal region is first deve- The neural region is first deve=
loped. There is no segmenta- loped.
tion of the blastoderm.
Subkingdom 8. MOLLUSCA.
SS ee
The blastoderm may become an- The blastoderm divides into so-
tero-posteriorly segmented, but matomes, A primitive groove,
there is no formation of pri- dorsal and visceral plates are
mitive groove, dorsal and vis- formed.
ceral plates*, Subkingdom 5, VERTEBRATA.
Subkingdom 4. ANNULOSA.
The generalizations here expressed may, to a certain extent, be regarded as cO-
rollaries from the well-known proposition of J. F. Meckel :—d. h. das hohere Thier in
seiner Entwickelung dem Wesentlichen nach die unter ihm stehenden, bleibenden
Stupen durchliuft, wodurch also die periodischen und Classenverscheidenheiten
auf einander zuriickgefiihrt werden}. Fora Vertebrate ovum, before segmentation,
differs but little, essentially, from an astomatous Protozoon. At a later stage,
when the division of the blastoderm into serous and mucous layers has just taken
place, it admits of easy comparison with the permanent forms of Celenterata, the
simpler organisms of this group being little more than double-walled sacs of peculiar
form, with one extremity open for the purpose of alimentation.
* This proposition is stated and commented on by Professor Huxley in his recent memoir
“On the Agamic Reproduction and Morphology of Aphis.” See especially § 5 of the same
paper, entitled ‘‘The Embryogeny of the Articulata, Mollusca, and Vertebrata compared”
(Linn. Trans. vol. xxii.).
ft System der yergleichenden Anatomie, Erster Theil, p. 396.
TRANSACTIONS OF THE SECTIONS. 133
Recent researches on the structure of the Infusoria show that some members of
that group, for example Vorticella, present a more or less obvious differentiation of
their primitively homogeneous tissue into imperfect layers. A mouth, also, is con-
stantly present. In these characters the higher Protozoa pre-indicate, as it were,
certain structural features which are seldom absent among the members of other
sub-kingdoms. So also do the more advanced Cclenterata, and especially the
Ctenophora, foreshadow, in a manner, the anatomical peculiarities of some of the
higher types.
All this may be admitted as true, without in any way neglecting the fundamental
distinction insisted on by Von Baer between the grade of development and the
type of organization.
t is to be observed with reference to the Annulosa, that the difficulty of enun-
ciating propositions which shall be equally applicable to the Articulata properly so
called (Arthropoda), and those lower annulose forms known collectively as Annuloida
or Vermes, is still so much felt, as to render it doubtful whether these two great
divisions should not be raised to the rank of separate subkingdoms. This, at
resent perhaps the most important question in systematic zoology, has already
ean answered in the affirmative by J. V. Carus, Gegenbaur, R. Leuckart, Siebold,
and Vogt.
The threo first-mentioned of these naturalists regard the Echinodermata as con-=
stituting a seventh subkingdom. Of the propriety of separating this group from
the Celenterata no doubt can any longer be entertained, although Prof, Milne-
Edwards and a few other zoologists of repute still continue to unite these widely
different forms under the oldname of Radiata. So long, however, as the arguments
brought forward by Prof. Huxley remain unanswered, the author can see no reason
to dissent from his conclusion, that the Echinodermata, while forming a distinctly
circumscribed class, are nevertheless connected by true affinities with the division
Annuloida.
On the Mode of Death by Aconite.
By Evwarp R. Harvey, M.A., B.M., Oxon.
Death by aconite has been attributed by different observers to its influence upon
each of the three vital organs, the heart, lungs, and brain. The following experiments
were made with a view of determining, if possible, the organ whose functions were
most directly interfered with by the poison. Fleming’s tincture was always used.
In experiment 1, two minims of the tincture were injected beneath the skin of a
dog. In 23 hours after injection the dog died. There had been no convulsions,
no loss of consciousness, no apparent loss of sight, no change in the pupils, and no
disturbance of the respiration: the two marked symptoms were vomiting and great
prostration. On examination after death, the veins of the neck were seen to be
enormously distended. The heart contained blood partially clotted in both auricles.
The other organs were healthy. In experiment 2. on a rabbit, the heart was the
organ first affected (its pulsations falling in 5 minutes from 140 in a minute to 100,
and soon becoming laboured and irregular) ; the breathing then became distressed,
and just before death there were convulsions. Post-mortem examination directly
after death :—The veins of the neck and brain were distended with blood. The heart
gave, when exposed, two very slight quiverings, not to be called contractions; all the
cavities contained blood. The other organs were healthy. In experiment 8,
similar symptoms during life and appearances after death were observed. Experi-
ment 4, The heart of a frog having been exposed by removal of a portion of the
sternum, the pulsations numbered 60 in a minute, and were forcible and irregular.
After three or four drops of the tincture had been let fall into the thoracic cavity,
the pulsations became very rapid, feeble, and irregular, and soon could no longer
be felt: the beating here ceased: 10 minutes after death the heart was again
pulsating, though much more feebly than in another frog killed by pithing. Ex-
net 5. A young rabbit was killed by aconite, and another young one by a
low behind the ears. In the animal killed by aconite, there was aslight fluttering
movement of the heart, but there were no regular contractions, and galvanism pro-
duced no effect whatever ; in the other rabbit, the heart was contracting regularly
after death ; and when all contraction had ceased, galvanism occasioned slight but
decided contractions, Experiment 6, Fiye minims of the tincture were injected
134 : REPORT—1860.
beneath the skin of a rabbit. In 40 minutes the pulse was intermittent, and
had fallen from 168 in a minute to 36. The temperature within the ears, which
at the time of injection was 97°, was 93°. The animal at this time was ex-
tremely weak, and unwilling to move; twenty minutes later it was more lively;
the pulse beat 60 in a minute, and the temperature within the ears was 96°.
The heart’s pulsation slowly and steadily increased, and the animal recovered.
Experiment 7. In a very young rabbit which received beneath the skin four
minims of the tincture, similar symptoms terminated in recovery. In the latter
case the temperature fell from 97° to 89°. In each case the only sign of cerebral
disturbance was an extreme weakness of the hind legs, which perhaps amounted
to temporary paralysis ; the breathing was never distressed, and but little hurried.
Loss of power of the heart and of the muscles generally, with a fall of temperature,
was the marked symptom, and the condition of the animals improved or deterio-
rated coincidently with the state of the heart. Experiments 8 and 9. In two
rabbits poisoned by aconite the heart and large veins were distended with blood.
In experiment 10, where there had been during life no symptoms of asphyxia, the
right side of the heart alone contained clots; a little liquid blood escaped from
both ventricles. This is the only evidence throughout the experiments of death
from asphyxia. With this exception, all the preceding experiments led to the
conclusion that aconite kills by its action upon the heart, and that the disorder of
the brain and lungs, when present, is due to the congestion consequent upon the
heart’s failure. To discover if the circulation was affected by the outward application
of the tincture to an inflamed part, a frog’s web was placed under the microscope,
and inflammation excited by a little mustard; the whole web was then moistened
with a few drops of the tincture; no effect whatever was observed for two hours
during which the web was under the microscope. It remained to be seen if the
poison acted directly upon the muscles or nerves. For this purpose experiments
were made upon frogs: galvanism was applied under various circumstances, and
though the experiments were not sufficiently numerous to decide the point, the
conclusion arrived at was, that aconite acts immediately upon the nerves, and
through them upon the muscles—the heart among the number—and that that organ
is the first of the vital organs whose function is interrupted. The latter experiment
will be repeated, as well as others which have been instituted on the antidotes of
aconite.
Several very careful analyses of the blood and urine of animals under aconite
were made, but beyond the increased quantity of urine, nothing worthy of parti-
cular comment was discovered.
On the Anatomy of Stenops Petto, Perodicticus Geoffroyi of Bennett.
By Professor Van per Hoeven.
. It is not for the first time that I make a communication on this species to the
British Association (see Report of the British Association for 1850, Trans. Sect.,
p: 125*). On a former occasion I proved that this species, first described, or rather
commemorated, at the beginning of the foregoing century, by Bosman, in his Dutch
work on the coast of Guinea, belongs to the group of the genus Stenops of Iliger
or Nycticebus of Geofivoy. I haye now the pleasure of bringing here to the meeting
a nearly complete anatomical monograph of this species. It was in the begin-
ning of 1857 that I received two well-preserved male specimens of the Potto, pre-
sented to me by a Surgeon in the service of the army of the Netherlands, then
residing at George d’Elmina. I placed them in the hands of a Candidate of
Medicine, F. A. W. van Campen, to procure him a good argument for his disserta-
tion. That able young man, who had devoted himself to the study of anatomy, died
* In the few lines inserted at that page the name Lemur Pollo occurs twice, but is a mis-
print for Lemur Potto. 1 avail myself of this opportunity to correct another fault, not of the
printer, but of myself. ‘The late excellent zoologist E. T. Bennett has not stated in his de-
scription of the Perodicticus (Proceedings of the Zoological Society, part 1, 1830, pp. 109, 110)
that the tarsus was elongated. For the words, ‘* The tarsal bones were of the same shape as
in Svenops, and the statement of Bennett, that the tarsus was elongated, is incorrect ” read
‘* The tarsal bones were of the same shape also in Stenops, and my former opinion, that the
tarsus was elongated, is incorrect,”
TRANSACTIONS OF THE SECTIONS. 135
before he could obtain his degrees. I received his notes and wrote after them the
Monograph, which was edited in 1859 by the Royal Academy of Sciences of the
Netherlands in its seventh volume (Ortleedkundig Ondersock yan der Potto van
Bosman door F. A. W. van Campen, Med. Cand. Uit zesse nagelasen aan
seekeningen byeen gebragt door J. van der Hoeven (Met due Platen Amsterdam,
Ato, 77 pp.). Except the female organs of generation, a species, scarcely known
thirty years ago, is now more completely investigated than many species of the
mammalia living in Europe. :
The little but very natural group of Mammalia called Lemuride, is one with
whose investigation I have been often and at different times engaged. It is well
known that zoologists have given the name of a hand to every extremity in which the
thumb is opposable to the other fingers. Some haye such only on the posterior ex-
tremities, as the opossum (Didelphis) of America and the Chiromys of Madagascar.
Those are called Pedimana, or hind-handed, Others haye this structure both in the
anterior and posterior extremities, as in the case in the greatest number of monkeys,
and in the lemurs (Quadrumana). Man is the only species of the order Bimana
where the opposable thumb exists on the anterior extremities only. Amongst the
Quadrumana the Lemuridx are distinguished by the nail of the second finger of the
hind feet, which is erected, compressed and sharp (of a subulate shape), while the
other fingers have flat nails. I found that in all the species the fourth finger, both
of the anterior and posterior feet, is the longest. In the apes, on the contrary, as in
most other mammals having five fingers, the third is the longest of all. To those
characters, sufficient perhaps for the systematic zoologist, we may add, after what
is known by the investigations of Cuvier, Fischer, Meckel, W. Vrolik, Burmeister,
A. Smith, Kingma and myself, several anatomical characters, as, for instance, that
the lower jaw is divided into two distinct lateral parts (as in many other mammals,
but neyer in the monkeys); that the orbit is notclosed by the interposition of the ala
magna ossissphenoidei between the malar and frontal bones, so that the fisswwa orbitalis
inferior is not distinct from the temporal fossa*; that there exists a flat, mem-
branaceous or aponeurotic tongue-shaped appendage beneath the tongue, terminated
in slender slips forming a pectinated tip; that the first pair of cerebral nerves is
represented by large corpora mammillaria, and that the uterus (in those of which
the anatomy is known) has two cornua, and not that pyriform shape which it
assumes in the monkeys and in woman.
The whole group is confined to the eastern hemisphere of our planet. The
greatest number of species lives only in Madagascar; some are found on the continent
of Africa in tropical regions; and some in East India, chiefly in the isles at the
south and east coast of Asia.
I distinguish the Zemurina into two groups. In the first there is only one nail of
the hinder feet erected and subulate; in the other, not only the second, but also the
third has that shape. To this second group belongs only the genus Tarsius, living
in Celebes, Borneo, and the Philippine Isles. It scems not to be proved that there
is more than one species of that genus. ‘The tarsus is very elongated,
To the first group belong all the other Zemurina. In those the superior inci-
sors are placed by two pairs, and a vacant space is left between them in the middle.
Some of those have the tarsal bones elongated like Zursiws; the calcaneum and
navicular bone forming two slender elongated bones placed near cach other like
the radius and ulna in our fore-arm. This genusis Ofolionus or Galago. In others
the tarsus is not elongated. Some have only two incisors in the lower jaw
(Lichanotus, Propithecus); others have four in both jaws. To this last subdivi-
sion belong the genus Lemur (stricto sensu) and Stenops. The first has a long tail,
the second a short, or only rudimental tail, or no tail at all. The last is the case
in the slender and small Ceylonese species (Stenops gracilis). All species of Stenops
have a short index to the fore-hand; i Stenops Potto there is an exaggeration of this
generic peculiarity, and the index has only two phalanges. The species is further
distinguished by the peculiarity that some spinous processes of the neck, covered
* In Tarsius the orbit appears to be closed behind, but the deviation from the other
Lemurid@ is more apparent than real; the great ala of the sphenoid bone is not concerned in
the formation of the hind wall of the orbit, but the malar bone is enlarged.
+ Propithecus seems to make an exception, but it ismore an apparent than arealone. See
Proceedings of the Zoological Society, 1832, p. 21.
136 REFORT—1860.
only by a thin corneous epiderm, pierce through the fur like prickles. They are
those of the fifth to the last cervical, and of the first two dorsal vertebree.
Observations on the Teredo navalis, and the Mischief caused by it in Holland.
By Professor vAN DER HoeEven.
It is well known that the Zeredo has been greatly destroying the piles which
were employed in the construction of the dykes of Holland in the beginning of the
preceding century, chiefly in the years from 1730 tol733. Since that period it is
scarcely recorded that any mischief has been produced by that bivalve till the year
1827, when in the province of Sealand it again became noxious. But it was chiefly
in the years 1858 and 1859 that the species increased very much, and the destruction
produced by it was the cause of a committee of members of the Royal Academy
of Science being formed, with the view of inquiring concerning the damages in
different localities, and as to the best means of protecting timber against their ravages.
I have the pleasure to place the Report of those gentlemen, published some weeks
before I left Leyden, in the hands of the gentleman who has given such an elaborate
dissertation on the Ship-worm to this meeting of the British Association. He will
I hope make known hereafter the chief contents to the English naturalist. From
the comparison of different records, it seems to result that the species, which it is
well known now was not imported from foreign and warmer seas, exists always on
our coasts, but that there are some periods of greater occurrence, produced as it
seems by high temperature of the year and by dry summers.
Different experiments have proved that some proposed means of preserving tim-
ber against the ship-worm are only useful for a short time, or even not useful at all ;
such are mixtures of fine fragments of broken glass and fat, different oil-paintings
and the like ; such is also the imbibition with different solutions of salts, sulphate
of copper, acetate of lead, and others. The best success, on the contrary, yet
obtained was by creosoting timber, a result also obtained in this country, as is
stated in the ‘Proceedings of the Institution of Civil Engineers.’ I think myself
fortunate in having the opportunity of placing the book I have brought with me in
the hands of a Member of this Association who has such a great knowledge of a
subject, to the elucidation of which, in a practical point of view, the Committee of
the Academy of Amsterdam has given its conscientious and laborious consider-
ation.
On the Development of Pyrosoma. By Professor Huxtey, F.R.S.
On the Nature of Death from the Administration of Anesthetics, especially
Chloroform and Ether, as observed in Hospitals. By Cuar.es Kipp, M.D.
The author haying collected and tabulated 109 deaths from chloroform, 22 from
ether, and 2 from amylene, believes himself to be in a position to offer some ex-
planation of these accidents.
Of these 133 deaths, 90 occurred in male patients, and 43, or less than half that
number, in females, though anesthetics have been largely used in midwifery practice,
Such occurrences are very rare in children.
From 250,000 to 300,000 operations of all kinds have been performed under the
influence of anesthetics, and chiefly of chloroform, and in some hundreds of severe
cases the patient has been more than an hour in a state of deep anesthesia. In all
these latter cases not a single well-attested instance is on record in which death
has taken place from simple stoppage of the functions of life, or narcotism of the
system by the chloroform. Fully 80 per cent. of all the deaths, and nearly all
those from chloroform, have occurred from trivial operations, from very small doses,
and suddenly before the anesthetic had produced its full effect. The author does
not contend that death cannot occur in the human subject from long-con-
tinued inhalation of chloroform, but only that it has not been observed to do so
in hospital practice. It seems probable that when anesthesia is once established in
a favourable surgical subject, respiratory action is diminished, and the breathing
for a definite interval proceeds on a diminished scale, almost as it does in the case
TRANSACTIONS OF THE SECTIONS. 137
of hybernating mammals. On the other hand, if respiration by fresh pungent
chloroform, vomited matter, &c., be disturbed, slight spasm of the glottis may
take place through the recurrent laryngeal nerves. This occurs occasionally in
strong and healthy, but nervous subjects, and especially in trivial cases; and the
occurrence of death in such instances from a few drops of chloroform is to be
attributed to this disturbance and stoppage of the respiratory muscles at the end
of the irritant or second stage—this being the dangerous point in administration of
chloroform. It may be considered almost as an established law, that patients suf-
fering under old disease and severe nervous irritation or neuralgic pain bear chlo-
roform best.
Dr, Kidd thinks that statistics for future use ought to be examined in two ways:
first inductively, and then by comparing the several groups of facts collected, and
deducing from them conclusions applicable to practice. Single “ positive instances ”
lead only to false conclusions. Though a single instance in a case of pure physical
science may be all that is requisite, as in the case of measurements of atomic ele-
ments, angles, &c., this is not the case in so complicated a matter as the one under
discussion, in which it is necessary to generalize, not from single facts, but from a
comparison of groups of facts.
In surgical practice under chloroform we have to fear, not so much deep insen-
sibility as the production, first, of apnea from muscular inaction, or spasm of the
Berta of the neck by irritation of the excito-motor respiratory apparatus. The
eaths from chloroform may be proved to be of an accidental character, and many
deaths during operations are charged to chloroform which would have occurred
equally before chloroform was used, and would then haye been put down to some
other cause. For instance, of 45 deaths recorded by Dr. Snow, 6 were attributable
to fright. Those which really follow chloroform commonly occur before the ope-
ration, and seldom or never as the result of a long tedious operation: of 85 deaths
which have been classified, 9 were cases of delirium tremens, and of the remainder
not one followed a capital operation.
The fact also that in 300,000 operations of all kinds chloroform has saved from
6 to 10 per cent. of lives, as held by Prof. Simpson and the author, also tends to
eer that the cause of death, at least in hospitals, is of an accidental character,
rom ageneral survey of the facts, the author finds that the deaths from chloroform
are all sudden, and many of the nature of “ fit.” Chloroform has a powerful irritant
action upon the pneumogastric nerve; and it is found that a similar irritation by
electricity causes vomiting and stops the action of the heart. Hence syncope may
possibly occur, if this irritation or (tetanoid ?) apnea of the respiratory muscles
and laryngeal nerves be reflected to the heart through the cardiac nerves of the same
pneumogastric trunk : this mode of death is most remarkable, for instance, under the
analogous agent—amylene. The general effect of the introduction of chloroform into
surgical practice has been good; and where it acts badly the author believes that
the cause may often be found in the tendency in patients themselves to defer sub-
mitting to an operation till too late. Upon a comparison of the present surgical
death-rate with that of 1846 immediately before the introduction of chloroform, it
appears 10 per cent. lower; and further, of the deaths which have taken place,
one-fourth have been in persons who have previously taken chloroform without ill
effect. Both these facts support the author’s view of the accidental nature of
death from chloroform.
The fact of death from chloroform occurring in slight operations and early in
the administration, has been remarked by all the chief observers, viz. MM. Robert
of Paris, Denonyilliers, Paget, Snow, and Brown-Séquard. The opinion that this
is due to disease of the heart is erroneous. In most fatal cases the heart has not
been found diseased. Thus in 4 cases in London hospitals, the post-mortem ex~
aminations of which were attended by the author, the heart-fibres were examined
and found healthy, though one of them (at Guy’s) was reported in the medical
Journals as a marked case of fatty heart. In 18 deaths reported in Journals which
presented some visible lesion, 8 only showed diseased heart. Again, in 24 deaths.
from ether, the cause appears to have been extreme hebitude, muscular relaxation
and exhaustion, and in some consequent hemorrhage following operations.
On the other hand, numerous patients known to have diseased hearts have taken
chloroform without any bad result, and in hundreds of animals death has been.
138 REPORT—1860.
observed to take place through the respiratory muscles first, the heart suffering as
a mere consequence. There have been probably 100 deaths from chloroform, and
twice as many patients saved from impending death by the proper use of restora-
tives, the chief of which is artificial respiration, which ‘ wakes up ” the respiratory
muscles. These restoratives have been directed so as,to excite the reflex and respi-
ratory system of nerves. Some patients have probably been lost by means used on
the theory of fatty or obstructed heart. Intoxication, delirium tremens, and hysteria
all contraindicate the use of chloroform; and it was also found during the Crimean
war, and more recently at three several seats of war in Italy, that nervous fright-
ened prisoners were particularly bad subjects for it. Any condition of violent
emotion (“exaltation of sensibility”) would appear to approach that state which
causes spasm of the glottis, trachelismus, Xc., while depressing emotion (fright ?)
may lead tosyncope. Dr. Snow does not seem to have noticed the effect of delirium
tremens; but in 85 fatal cases, collected by the author in the hospitals, 9 appear
due to it, or to intoxication ; the mischief is probably owing to the cerebral hemi-
spheres, medulla, and reflex system in the spinal cord being weakened by alcohol.
In 4 well-authenticated cases the heart was still beating after respiration had
ceased ; this is also very often seen in experiments on animals; and probably obser-
vation only is wanting to establish the more frequent occurrence of this phenc~
menon in man. In the author's opinion the heart is one of the very last organs
which is depressed by chloroform, and this fact it is which renders its use compa-
ratively safe. He fears rather the implication of the “respiratory tract.” The chief
conclusions at which Dr. Kidd arrives are as follows :—
1, Ether is little if at all superior to chloroform. In “ ether mixtures” the
ether is first inhaled pure. Ether causes the pulse to intermit, and is to be avoided
where we fear excessive hemorrhage or muscular relaxation ; but in dislocations
and in midwifery it has some points in its favour, but not in a mixture with chloro-
form. Ether, too, in a sick room may take fire, but chloroferm does not.
2. There is less reason to fear the effect of anesthetics in women and children
and in severe operations, than on robust men ; especially if given to the use of intoxi-
eating liquors, or when the operation is connected with tendinous parts, in which
cases syncope often follows when no chloroform is used.
3. Hospital experience tends to prove that chloroform is less dangerous in pro-
portion as the operation for which it is used is more severe. When once the pai-
pebral conjunctiva is insensible, there is a period of safety during which the respira-
tory action is diminished like that of hybernating mammals ; the heart remains unaf-
fected, but the pulse becomes larger. The many instances in which this has been
seen, seem to overpower isolated cases of death from diseased heart and chloroform,
and should encourage hopeful views on the use of anesthetics.
4. Idiosyncrasy has probably little or nothing to do with deaths from anesthetics,
if we omit habits of intoxication, hysteria, and tendency to “fits.” Thus re-
peated trials of chloroform (“ trials Cessai”) on a patient are a mistake, and nowise
affect the chance of his safety on any given occasion.
5. There are two, or perhaps three modes in which anesthetics may cause death,
and which require watching. (a) Ether may do so at some uncertain interval
of time during the first twenty-four hours after an operation. (8) Chloroform in-
stantly, by an action on the laryngeal-recurrent and double respiratory centre in the
neumogastric nerves. In half these cases, probably, as in apnea or asphyxia, the
fieart is still beating; and (y) in other cases by syncope (as a coincidence ?).
6. In several cases, e g. those of delirium tremens, the death probably occurs
because ordinary restoratives fail to act in consequence of the imperfect reflex ner-
vous system; but in cases of impending death, we are to have recourse to artificial
respiration by pressure (rather than the Marshall Hall plan), since this also acts
upon the engorging cavities of the heart; tracheotomy if we have reason to fear
spasm of the glottis or asphyxia; sudden dashing (not too long continued) of cold
water; fanning of fresh air on the face, &c.; but as the spasm may subside, we are
not to do too much at first. Acupuncture, quickly done, of the muscles of the neck
is recommended in order to irritate the spinal accessory and phrenic nerve, but not
the eighth pair; and “ Faradisation ” here also is most valuable.
7. Our experience of oxygen gas, common galvanism, &c. as restoratives is not
encouraging at present. Injection of port wine into the rectum is better, or the
iP.
nied
TRANSACTIONS OF THE SECTIONS, 139
transfusion of any simple saline fluid into the veins, as has been tried in the case
of animals poisoned with chloroform, and as in the analogous collapse of cholera.
On a Hydro-spirometer. Ly Dr. Lewis.
On the Development of Buccinum, By Joun Lussock, LR, PLS,
In the year 1851 MM. Koren and Danielssen published a memoir* on the
Development of the Eggs of Buccinum undatum and Purpura lapillus, in which
they gave an interesting account of the development of the young mollusks, and
especially excited the surprise of naturalists by certain statements regarding the
amalgamation of several eggs to form one embryo.
The two above-mentioned species produce peculiar capsules, each containing
several hundred eggs. The capsules of Purpwra are bottle-shaped, those of Buc-
cinum are like around cushion, and are attached to one another in clusters, and
fastened to rocks, shells, or sea-weeds. Often, however, they are detached and
thrown up on the shore, so that they are familiar to all those who ever walk along
the beach near high-water mark. The egg-capsules of Purpura are attached singly
to the rocks. It was already known that, although each capsule contained a great
number of eggs, only a small number of embryos, from fifteen to thirty, came to
maturity.
MM. Koren and Danielssen gave a very extraordinary account of the phenomenon,
According to them the eggs grouped themselves in masses, round which a common
skin was formed, and thus numerous ova combined to form one embryo. This
account of a process, so different from that with which we are familiar in other
animals, was not likely to pass long without either confirmation or opposition ; and
accordingly Dr. Carpentert, having studied the development of the eggs of Purpura
lapillus, disputed some of the statements made by MM. Koren and Danielssen, gave
a very different explanation of the whole phenomenon, and added the high authority
of Messrs. Busk and Huxley in confirmation of his view.
Dr, Carpenter had no opportunity of making any observations on the embryology
of Buccinum, but he convinced himself that the egg-capsules of Purpura lapillus
contain two sorts of bodies, namely true eggs and “ yolk-spheres,” which, however,
are at first undistinguishable from one another. After a while, however, “all the
egg like bodies in the capsule begin to show signs of cleavage. In the greater part
of them, the two segments produced by the first cleavage are equal, or nearly so;
and each of these again subdivides into other two, which are alike equal ;” after
which the division becomes irregular. These are the so-called “ yolk-spheres.”
Some few of the egg-like bodies, on the contrary, divide into two wnequal segments,
These are the true eggs, and each embryo takes its origin from one of these. The
embryo then developes rapidly in itself a central hollow or stomach, a wide ceso-
phagus, and two lobes covered with cilia. It then commences to swallow the yolk
matter around it, and this is the reason that the number of embryos is so much
smaller than that of the egg and yolk-spheres.
MM. Koren and Danielssen by no means gaye up their theory, but after repeat-
ing their observations, they reiterated their statements }, giving, however, it must
be confessed, figures much more nearly resembling those of Dr. Carpenter than the
ones contained in their first memoir.
Finally, Dr. Carpenter, in the ‘Annals and Magazine of Nat. Hist.’ for 1857, has
published some further remarks on the subject, and adds, in addition, the testimony
of Dr. Dyster to the truth of his assertions. This is the present state of the ques-
tion; and considering how common are the egg-capsules of Buccinum, it is remark-
able that no one has tested MM. Koren and ces wee’ statements in reference to
that genus.
The whole subject is one of great interest; and though I could not doubt the
truth of statements made from independent observations by four such excellent
authorities as Messrs. Carpenter, Bush, Huxley, and Dyster, yet MM. Koren and
* Bitrag til Pectinibranchiernes Udviklingshistoire. I have not seen the original work
but there is a translation of it in the Ann. des Sc. Nat. for 1852.
t Quarterly Journal of Microscopical Science, vol. iii. p. 17.
{ Fauna Littoralis Norvegiz, vol. ii,
140 REPORT—1860.
Danielssen, though wrong as to Purpura, might still be quite correct in the case of
Buccinum, and I was very anxious to repeat their observations. It could not be
denied that it was @ priori probable that what was true of Purpura, would also
apply to Buccinum. Still, if I had any bias, it was in favour of MM. Koren and
Danielssen. Many insects present us with a case in many respects parallel. In
Lepidoptera, Hymenoptera, Diptera, Neuroptera, and the Geodephagous beetles,
each ege is accompanied by several vitelligenous cells, or as we might call them in
the words of Dr, Carpenter, yolk-spheres. After a while the walls of the vitelli-
genous cells disappear, and the whole group unites to form an egg. Here we have
undoubtedly a certain similarity with that which, according to MM. Koren and
Danielssen, occurs in Purpura and Buccinum.
Buccinum undatum has been stated * to lay its eggs from the beginning of January
to the end of April. On our south coast of England, howeyer, it begins earlier, for
I found some fresh ones at Brighton last November. I was not then able to examine
them with much care, but in February last I received from My. Lloyd two packets
of egg-capsules, in which I have succeeded in tracing the development of the
embryos.
When I received them, the germinal yesicle had already disappeared, and the’
eges consisted of yelk-particles immersed in a viscid substance. According to
MAL. Koren and Danielssen, each egg is surrounded by a chorion and a vitelline
membrane, but I was as little able in the case of Buccinum, as Dr. Carpenter was in
that of Purpura, to discover any trace of these structures; and I think I can safely say,
from the appearance of the eggs, and from their behaviour when crushed, that they
were surrounded by no definite membrane. Many of the eggs, indeed, resembled
MM. Koren and Danielssen’s fig. 16 (Ann. des Se. Nat. 1852, vol. xviil.), in which
a thick outer membrane is apparently present ; but this arises, as will be presently
described, from a condensation of the yelk-particles leaving a clear border of the
viscid substance.
The presence of a vitellime membrane certainly seems to me improbable, but
about the so-called chorion Iam more doubtful. MM. Koren and Danielssen men-
tion (i. ¢. p. 258) that it early disappears, and this may haye already taken place
in my specimens as well as in those of Dr. Carpenter.
The eggs in my egg-capsules did not coalesce. They collected certainly in a heap,
but they remained quite separate from one another, and showed no tendency to unite.
Very few showed any trace of segmentation. In this respect my observations,
so far as they go, are quite in accordance with those of MM. Koren and Danielssen.
There is, however, always a certain amount of suspicion attached to negative evi-
dence, and it seems a priori very improbable that Purpura and Buceinum, which
agree so closely in most points connected with their embryology, should differ in
such an important matter.
Dr. Carpenter considers that the capsules of Purpura contain two sorts of egg-
like bodies, which, however, can be distinguished from one another only by their
modes of segmentation.
I was not able to perceive any difference in the eggs of Buccinum, except that in
some the yolk-granules were condensed, so as to leave a margin of the clear, glairy
substance; but it must be remembered that in each capsule only a very few eggs
undergo segmentation at one time; and the process appears to be altogether so
irregular, that my observations do not enable me to come to any satisfactory con-
clusion on this point. It would be desirable to investigate the formation of the
eggs in the ovary, both of Buecinum and Purpura, in order to determine whether
or no they are all originally alike, and if not, to determine the points of difference,
It would also be well worth while to ascertain the relation which the segmenta-
tion of the yolk bears to the development of the embryo.
It is so generally present throughout the animal, and apparently so universal in
the Mollusca, that strong evidence would be required to show that Buecinum forms
any exception to the general rule; and yet, as far as my observations went, the
process certainly seemed to be subject to considerable irregularities.
The whole subject of yolk-segmentation is one of great interest.
Among the Entozoa, it appears to occur in certain species of Strongylus, Ascaris,
Gordius, Mermis, and Echinorhynchus, and in Filaria, Filaroides, and Spherularia.
* Ann. des Sc, Nat. 7. c. p. 258,
‘
TRANSACTIONS OF THE SECTIONS. 141
Van Beneden asserts that it occurs in the Cestoids generally ; but this is denied
by Kolliker, as far as concerns Tenia and Bothriocephalus. There is a similar differ-
ence of opinion as regards Cucullanus elegans, in which species Siebold (misled,
according to Kolliker, by the large size of the two primary embryo cells) supposed
that there was a true segmentation. The figure given by Kolliker sufficiently
explains how such a mistake might have occurred*, Van Beneden also denies that
any segmentation occurs in Echinorhynchus, a difference of opinion which may have
arisen from different species having been examined, since, while segmentation has
been observed in Ascaris nigrovenosa, acuminata, succisa, osculata, labiata, brevi=
caudata, &c., it appears, according to Kolliker, to be absent in Ascaris dentata. It is
evident therefore that this species cannot be naturally included in the same genus
as the others, and that the two groups, however similar, are in reality very remote
from one another.
Oxyuris ambigua and Gyrodactylus have been also asserted to develope without
yolk-segmentation, though in the case of the latter there appears to be some doubt.
In the Annelids it has been observed in Polynoe, Exogone, Clepsine, Nephelis,
Protula, Hermella, &c., and is not known to be absent in any,
Ithas also been observed in the Tardigrada and in Lacinularia. Among the
Articulata, it has been noticed in Nicothoe by Van Beneden, in Diaptomus and
Cyclops by Claus (which I also can confirm). On the other hand, in Insects} and
Daphnia I have sought for it in vain, and it is unmentioned by Rathke and Heroldt
in their works on the development of Asellus, Oniscus, Astacus, and the spiders,
though in the two latter cases it may perhaps be represented by the dispersion and
reunion of the “ Keimscheibe.”
Among the Mollusca it has been described in Acteon, Aplysia, olidia, Dentalhium,
Doris, Limax, Limnea, Planorbis, Teredo, Tergipes, Tritonia, &e.
Among the Bryozoa it occurs in Aleyonella.
In Salpa it has been observed by Kolliker, while in Pyrosoma it would appear,
according to the recent researches of Huxley, to be impossible.
All this, however, is a digression, and I must return to my Buccinum.
The ege-capsules were sent to me on the 19th of February, at which date the eggs
in most of them were diffuse, though in some they had already begun to collect
together. At this time no embryos had appeared. On the 29th the eggs were
more closely compacted, and each capsule contained from five to twenty embryos.
The eggs now adhered together in a more or less compact mass, but showed
no tendency to amalgamate, and were very easily separable from one another by
the point of a needle, Imbedded in and about the mass were the embryos; the
smallest consisting apparently only of a clear substance, surrounding the almost
unaltered yolk, and having on one side an enormous orifice or mouth leading into
a central cavity. The more advanced embryos already showed traces of the ears
and the salivary glands, and began to swallow the other eggs whole. In spite of a
careful search, I never found any collections of eggs simply surrounded by a mem-
brane, as described by MM. Koren and Danielssen and figured, /.c. fig. 17. Embryos
containing more than three or four eggs always possessed the salivary glands and
auditory organs. Nevertheless, were Messrs. Koren and Danielssen’s theory correct,
such masses ought to be tolerably frequent.
Nevertheless, the young embryos were so voracious and swallowed so many other
eggs that they became greatly distended, and on a superficial view appeared some-
times as in MM. Koren and Danielssen’s fig. 17 (Ann. des Sc. Nat. 1852, pl. 5).
By turning these over, however, with a little care, the ciliated lobes could always
be discovered. At this period also the eggs sometimes adhered together so as to
form rounded masses; but in such cases they were quite separate, were surrounded
by no membrane, and were easily separable from one another. Nevertheless, if
masses such as those described and figured by MM. Koren and Danielssen
formed one stage in the normal development, it is very unlikely that I should
never have come across a single specimen in this stage.
Moreover, even in the smallest embryos we see already a broad cesophagus, and
* Van Beneden appears also to have fallen into the same error. See Mém. sur les Vers
Intestinaux, p. 275, 1858.
+ Leuckart supposed that he had found it in Diptera, but he was doubtless misled by the
vitelligenous cells.
142 REPORT—1860.
laree that a needle can easily be introduced into it. If, however, the in-
pwnage? be simply by imbibition through the skin, these would be of no use.
Moreover it is very common to see other eggs actually in the cesophagus of the
embryos in the act of being swallowed ; or we might almost say that an embryo is
seldom seen without an egg in its cesophagus. - In Purpura, according to Dr. Car-
penter, the yolk is swallowed particle by particle ; in Buecinum, on the contrary,
the ecos not having undergone any segmentation, are swallowed whole, and the
process of deglutition is therefore probably less rapid and more easily seen. The
presence of yolk matter in the cesophagus of Purpura may also be more plausibly
ascribed to accident than in Buceinwm, where, from the large size of the egg com-
pared to that of the embryo, it cannot take place without a considerable tension of
the i and the swallowing must therefore apparently be a work of some
ate tae ee suggests (Ann. des Se. Nat. J. c. p. 26) that the so-called eggs
are probably only “des spheres vitellines, dont l’envelope utriculiforme présenté
un peu plus de consistance que d’ordinaire, et que, par conséquent, Vagregat dont
nait le corps de Yembryon est le résultat du groupement des sphéres vitellines d un
seul ceuf, et non le produit de la reunion de plusieurs ceuts primitivement distincts.
Tt will be seen, however, from the preceding description, that iitoug M. Milne-
Edwards was fully justified in the scepticism with which he regarded the descrip-
tion given by MM. Koren and Danielssen, he was not equally happy in his
attempt to explain away the supposed anomaly.
L 2
Fig. 1. Embryo in outline, to show the mouth and digestive cavity.
Fig. 2. Young embryo in the act of swallowing an egg.
On the Influence of Systematized Exercise on the Expansion of the Chest.
By ArcuiBaLtp MacLaren.
Exercise is the most important agent in physical growth and development, inas-
much as it qualifies the condition, the action and the influence of all the others. This
importance is not always appreciated, because the effects of exercise on any part of
the body but the muscular system are imperfectly understood. All exercises may
be classed under two heads, Recreative and Educational. ‘The first of these em-
braces all our school games, sports and pastimes,—a most valuable list, but quite in-
sufficient to produce the perfect development of the body :—1st, because the parts
of the body chosen to execute the movements of the game are those which can
do them best, not those which need the exercise most ; 2nd, because it isa distinc-
tive feature in the bestand most ardently practised of them, that they give a large
share of employment to the lower half of the body, and but little (some not at all)
to the upper half; and 3rd, the little which they do give is almost monopolized by
the right side, The tendency of these exercises is therefore to develope the lower
half of the body to the exclusion of the upper. It must always be remembered that
while in developing a limb to its full power and perfect conformation, we do that
and nothing more ; in developing the trunk of the body, we do that and a great deal
TRANSACTIONS OF THE SECTIONS. 143
more, we directly aid in the development of all the organs which it contains, The
oint to be desired is the uniform and harmonious development of the entire body;
ecause the strength of a man is but equal to that of his weakest part, while the
natural tendency is to gauge and estimate the general strength by the power of
the strongest part. This equal development is to be obtained only from systema-
tized exercise, prepared upon a clear comprehension of what is required, and based.
upon a knowledge of the structure and ascertained functions of the parts of the
body to be employed, and of the laws which govern growth and development. The
inadequacy of recreative exercise to produce this development is fully borne out
by the frames of the youths who yearly arrive in this University from our public
schools. As the case now stands, every one who so arrives here does so with the
upper part of the body greatly in arrears. So distinctly is it in arrears, that an
average of 2 inches in girth of chest is obtainable in the very first term of his prac-
ticeinthe Gymnasium. This rate of increase is not sustained beyond the first term,
therefore it must be chiefly expansion of the cavity of the chest; and it must be
an arrears of expansion, otherwise it would be sustained, secing that the process
which produced it is increased and accelerated in the advancing courses of exercise.
The operations of systematized exercise are equally important and decided in other
directions, and especially in the rectification of abnormal spinal developments.
On the Artificial Production of Bone and Osseous Grafts.
By M. Outter.
M. Ollier exhibited some specimens illustrating the results of his experiments on
the production of bone, and summed up in the following propositions :—
1, When the periosteum is detached from a bone, one end remaining attached,
bone is formed in the direction of the periosteum, its form and size being deter-
mined by the size and position of the membrane.
2. After union has begun to take place between the periosteum and the soft parts,
the pedicel may be divided, but bone will still continue to form.
3. If the periosteum be removed altogether and inserted among the soft parts, it
will make an attachment, and bone will be developed.
4. If the inner surface of the periosteum be scraped off in part, no bone will form
on the portion so treated.
5. If the matter scraped from the inside of the periosteum be brought into con-
tact with soft parts, bone will be developed from the periosteal cells.
6. Ifa bone be taken out of its periosteal sheath, new bone will be produced ;
but if a segment of such sheath be removed, no bone forms in that space,
7. Ifa bone be removed entire with its periosteum and inserted into soft parts,
eo will take place, and new bone will be deposited from the periosteum on
the old.
8. If, in a piece of inserted bone, a part be deprived of periosteum, that part dies
or is absorbed. Thislatter process may take place by the denuded portion becoming
either encysted or ecciel, to suppuration; as a general rule, in animals that are
healthy, and live in the country, the process of encysting takes place; while in
feeble animals and those living in towns, suppuration is the ordinary result.
Experiments on Muscular Action from an Electrical point of view.
By Dr. C. B. Ravcwirr.
On the Process of Oxygenation in Animal Bodies.
By B. W. Ricuarpson, M.A., M.D.
So soon as the discovery of oxygen by Priestley became an established fact in
the world of science, inquiries were set on foot as to the influence of this substance
on animal bodies. The term by which it was long known, “vital air,” indicates
sufficiently the interest that was attached to it ina physiological point of view.
Priestley himself made various physiological experiments with oxygen, in which
line of research he was followed by Lavoisier, Beddoes, Sir Humphry Davy, Hill
and several other celebrities of the declining eighteenth, and rising nineteenth
century. From the researches of various experimentalists, it had been concluded
144 REPORT—1860.,
that the inhalation of oxygen in the pure state, by giving rise to a greater absorption
of the gas, sets up an increased oxygenation in the body,—hypercausis, and inflam-
matory conditions, general and local. This view, first promulgated by Dr. Beddoes,
and followed up by many contemporary writers, was probably the basis of the
chemical nomenclature of disease invented by Baumé, in which disorders were
divided into those of oxygenation, of calorification, hydrogenization, azotification,
and phosphorization, with remedies of the same names for their treatment,
A second conclusion as to the influence of oxygen on animals, intimated (also
from experiment) that oxygen, when inhaled in the pure form, is even less active
than as it exists diluted in common air; that, instead of increasing the combustion
of the body and its activity, it lessens these, and that animals exposed to it too long
die from coma attended with a steady and undiminishing exhaustion. The idea
that less oxygen is absorbed when the gas is breathed in the undiluted state was
supported by Davy: the statement that the gas destroys by narcotic exhaustion
was doubtfully suggested by Priestley, and openly by Broughton. For years this
view of the question has been the one most commonly taught in this country.
The last conclusion that had been drawn from experiment relative to the effects
of pure oxygen was, that it has no injurious influence on life. Lavoisier, in his later
a ie aie seems to have drawn this inference, and Regnault has greatly con-
rmed it.
In 1852, with these conflicting data before him, those of Regnault only excepted,
Dr. Richardson commenced an inquiry into the whole subject, which he had con-
tinued, with intermissions, to the present time. The author here narrated his earlier
experiments, from which he came to the conclusion that animals of active respiration,
as dogs, cats, and pigeons, on being subjected to a constant stream of freshly made
oxygen, become subject to inflammation, owing to the rapid destruction of the
tissues,—hypercausis. In further experiments, he found, however, that his rule was
not common to all animals; for rabbits and frogs were kept by him even for weeks
in oxygen without apparent injury. On the data, therefore, he gaye the following
as the first major proposition of his paper :—
The influence of pure oxygen, as an excitant, differs according to the animal ;
being most marked in animals of quick respiration and high temperature, and least
marked or nil in those of feeble respiration and lower temperature.
Up to 1856 the author had felt assured that oxygen, when it destroys life in the
‘actively breathing animals, does so by causing a too rapid oxidation of tissue and
the so-called inflammatory process ; and he believed that the symptoms of narcotism
and paralysis, named by Broughton, were due without doubt to one or other of
two possible errors, introduction of carbonic acid, or modifications of the air-pressure
exerted on the animal. In 1857 he began to suspect that his view was not strictly
correct; but he had no proof either one way or the other until the present year,
when a new observation opened a new phase of the question. Having made on one
occasion forty gallons of oxygen, and having, by the side of the reservoir containing
the oxygen, another reservoir of equal size filled with water, Dr. Richardson deter-
mined, in order to economise both labour and material, to collect the oxygen from
the supplying reservoir, after it had passed through the chamber containing the
animals. He arranged also to wash the oxygen in alkaline solution until it was
free of carbonic acid altogether, to pass it over sulphuric acid to remove any am-
monia, and finally to charge the second reservoir with it and to use it again,
sending it thus backwards and forwards from one reservoir to the other until it
was all used.
When the apparatus was complete, he placed four warm-blooded animals, a cat,
a dog, a pigeon, and a rabbit, with two frogs, in a large chamber, and at 11 o’clock
in the morning commenced the transference of the oxygen, passing it through the
chambers at the rate of 2000 cubic inches per hour. In six hours the whole of
the primitive oxygen, minus nearly 1000 cubic inches which had been lost in
respiration, was transferred into the second reservoir. The gas was now tested,
and having been found to give no reaction to lime-water, it was driven back
through the chamber and washed again thoroughly with potash, to he received
once more into the reservoir number one. As the first charge of oxygen was passing
through the chamber, there were exhibited no signsdifferent from those of excitement,
which had before been seen; but as the second charge passed through, all the
Aen
TRANSACTIONS OF THE SECTIONS. 145
animals became depressed and drowsy. After an interval of four houts, the current
was again changed, and the oxygen, purified most carefully of extraneous matter,
was a third time given to the animals. It now became more obvious that every
animal was under some peculiar depressing influence ; even the rabbit did not escape.
The symptoms were entirely different from those arising from carbonic acid. The
breathing was quick, but easy and tranquil. There was not the slightest approach
to convulsion. ‘The pigeon buried its head under its wing, and simply drooped and
slept. The four-footed animals sat with their four lees straight and their heads
between them, nodding as if in profound and pleasant sleep; they were aroused
with difficulty, and fell off again in an instant. ‘Then the fore-legs slowly gave way
forward, as if paralysed ; and, before the third charge of the oxygen was three parts
over, the pigeon was dead, and the kitten was so nearly dead that it was not easy
to detect its chest movement; the dog gaye no sign of sensibility, but breathed
softly ; the rabbit was fast asleep. ‘The frogs alone were unaffected.
At this crisis, a little air was pumped out of the chamber through lime-water ;
it gave less indication of carbonic acid than the common air which the experiment-
alist was breathing.
The animals were then removed, and a lighted taper was placed in the chamber.
The taper burnt with more brilliancy than in the air, but with a slight yellowness
of flame.
The animals were all nearly dead. The kitten died a few minutes after removal ;
the rabbit recovered in two hours; the dog seemed paralysed in the limbs for the
preaterpart of the day, but recovered. When the bodies of the pigeon and the kitten
were opened, there was found no indication of asphyxia. The lungs were inflated
and red; the heart contained blood on both sides, but the blood in each side was
of the same hue, neither being very dark; the brain was bloodless; the other organs
were natural. The appearances in the pigeon corresponded with these with the
most minute accuracy. ;
Dr. Richardson next narrated the histories of several other experiments, from
which he derived, apparently to demonstration, the following and second major
proposition :—Oxygen, when breathed over and over again, although freed entirely
from carbonic acid or other known products of respiration, loses its power of sup-
porting life ; the process of life ceasing, not from the introduction of a poison, but
as by a negation, or a withdrawal of some principle extant in the primitive oxygen,
which is essential to life.
The last section of the paper had reference to the influence of oxygen on muscular
irritability; and various experiments were again given. On them the author
founded the third major proposition.
Oxygen, while it is essential to muscular irritability and muscular power, exerts
its influence over muscle, not as a direct excitant of muscular contraction, but by
supplying to the muscle an agent or force by which the muscle is fitted for contrac-
tion on the application of an exciting cause.
The Action of Tea and Alcohols contrasted. By Kowarv Smitu, M.D.,
EL.B., F.RS., Assistant Physician to the Hospital for Consumption
and Diseases of the Chest, Brompton, §c.
In this paper the author stated the results of a series of original inquiries into
the influence of these two substances which appeared in the Philosophical Trans-
actions for 1859.
The general expression of the action of tea is, that it increases all vital actions,
and causes the elimination from the body of more material than it supplies.
It inereases the ease, frequency and depth of respiration, but does not much
affect pulsation.
It increases the action of the skin, as shown by the increase of perspiration; and
as in the conversion of fluid into vapour there is a thousand-fold increase in the
absorption of latent heat, perspiration must cool the body.
It wnereases, and does not disturb, nervous, mental and muscular action, and it
is not followed by reaction.
Small doses often repeated have fourfold the effect of a large dose.
1860. 10
146 REPORT—1860.
Large doses cause nausea and narcotism.
The addition of acids and fat, as cream, lessens its action on the skin and increases
pulsation.
The addition of an alkali, as soda, increases the action upon the skin and renders
it more soothing, but a caustic alkali destroys it.
Hence the author considers that it is inapplicable in the following conditions of
the system, viz. :—
In the absence of food (except when a large meal has been recently taken), and
therefore at breakfast, unless the system be replete with food, as from a late and
large supper, In the ill-fed, and in those of spare habit.
In prison or other dietaries, in which it is a duty not to allow the supply to ex-
ceed the real wants of the system, except in the cases in which the powers of
assimilation are defective, and then as tea, like other nitrogenous matters, has been
shown by the author to promote the assimilation of starchy food, it may prevent
the waste of undigested food.
When unusual muscular exertion is made, unless there be also an abundance of
food and the skin acting insufficiently.
In those who perspire too easily and profusely.
In low temperatures, except in connexion with abundance of fat, since then the
action of the skin should be reduced to a minimum.
In very early life, when all the vital actions are rapidly performed.
He considers also that it is more suited to the following states :—
Tn the after part of the day, when the powers of assimilation have been shown by
him to be enfeebled, and when food has accumulated in the body,
In old persons,
In hot climates, with lessened powers of assimilation; with excess of heat and
excess of food.
In those who usually transform food imperfectly.
In those who take too little exercise, and eat too much.
In conditions in which. gout is likely to occur.
In those who haye the skin inactive.
In all states in which there is excess of food, not, perhaps, in relation to the
wants of the system always, but in relation to the power to transform it, and
especially where there is excess of heat, as to soldiers on march exposed to the
eastern sun,
The author then compared these deductions from science with the actual instinct-
ive habits of mankind in different climates—the test to which all such inquiries
must be ultimately subjected—and showed that there is a most striking correspond-
ence, as, for example, the frequent use of tea alone by the sedentary, corpulent, fat
and starch-eating Chinese, and, with the addition of an acid, by the industrious poor
-and exposed classes in that country, and by all classes in the cold of Russia ; the
addition of milk or cream in our climate; our habit of taking food with tea when
we regard it as a meal, and of drinking it after dinner in hot weather when we
would perspire more freely ; the enjoyment of it by the poor, who live chiefly on
bread, which is imperfectly digested; and the large appetites of teatotallers.
__ Hence he was of opinion that tea had a more powerful action upon the body, both
for good and eyil, than has hitherto been understood, and believed it to demand
the regulation which attends the administration of a medicine; and especially
urged it to be supplied to soldiers in hot climates, to be drunk cold or hot in small
-doses during exposure to heat.
In reference to alcohols, the author showed that ales, wines, and spirits differ
in their action, not only because they contain varying amounts of alcohol, but have
other ingredients, as volatile oils and ethers, salts, gluten and sugar, and thence
each must always be discussed separately. He showed that neither the public nor
the medical profession substitute a given amount of alcohol and water for these
various substances, but admit that each substance has a special action, and that
even impurity and newness are held to be deteriorations in any member of the
a
same class. s
He showed that all alcohols lessen the action of the skin and increase the force
medicinal actions,
and frequency of the action of the heart, and that these are their true dietetic and 5
; TRANSACTIONS OF THE SECTIONS. 147
__ When the usual dose of a spirit or alcohol was taken duly diluted with water,
_ he had found, by numerous experiments, that the following sequence of pheno-
- mena took place :—
_ L Upon the heart, probably by the direct contact of the alcohol, and occurring
in 2 to 4 minutes,
2. Upon the brain, in from 3 to 7 minutes, as shown by the effect upon conscious-
ness, mental and sensual perceptions,
. 3. Upon the spinal cord, as shown by lessened tone, lessened power of controlling
and lessened desire to use the muscles, a sense of purring through the whole
system, and the sensation of heat and cold.
4, Upon the respiratory nervous tract.
5. Upon the secretory (sympathetic nervous) system.
The exhilaration of spirits, accompanied by sense of heat, swelling and redness of
the skin, occurred in the first stage, and continued about 30 minutes, and this was
gpanged for taciturnity, chilliness, and sense of miserable depression in the second
stage.
Alcohol usually increases the activity of the respiratory actions in a moderate
degree ; as did also whisky in many instances, and rum commonly, whilst brandy
and gin lessened them.
Beers he believed to act also by their sugar and gluten, and thus tend to pro-
mote the digestion of starchy food; but for this purpose only small quantities, as
by an ale-glass, should be taken ata time, so as to obtain this action apart from the
alcoholic action.
The author also appended a few remarks on the action of coffee, on account of
its parallel use with tea, and proved that whilst both agree in increasing vital
action, they differ in the important particular of their action upon the skin,
Coffee usually lessens the action of the skin, and thereby renders it dry and hot, at
the same time increasing the action of the heart, and, as a further consequence of
the former, increasing the action of the kidney, or failing that, inducing diarrhoea,
Hence it is applicable in conditions widely differing from those suited to the
use of tea.
Tn contrasting tea and coffee with alcohols, the author found only one analogy
with tea, viz. that of beers, since both tend to promote the digestion of starchy
food, and therefore both the teatotallers and the anti-teatotallers may be equally
right. There is no similarity whatever between the action of tea and alcohols ; but
both are in their essential actions opposed, whilst there is an important correspond-
ence in the action of alcohols and coffee. The use of tea in the arctic regions
must be associated with that of alcohols, or the substance having an equivalent
but less perceptible and more enduring action upon the skin, viz. fats, whilst rum
is less injurious to the sailor of all countries than brandy or gin would be, by its
special power of increasing the respiratory and other vital actions, When it is
conjoined with milk, it is the most perfect restorative known.
- The author did not regard any of these substances as true food, viz. substances
which by their own elements directly nourish the system, but haying the special
_ power of curtailing the power of assimilating other food. Hence, although there
may not be “more nutritive matter in a pint of beer than will lie upon a sixpence,”
there is a power whereby other food is made more useful to the system.
Pe ee se lel ,lrlC eee
eet tial thd Ven Ieee Bile ek
4 The Physiological Relations of the Colouring Matier of the Bile.
4 By J. L. W. Tuupicuum, M.D.
The author having convinced himself by experiment that the ordinary method of
purifying cholochrome (the colouring matter of bile) does not give a uniform
material, has sought for such a reaction as would give the rational composition of
this substance in order to establish its formula by metamorphoses. Such a reaction
he has obtained with nitrous acid, which, when passed in the gaseous state into
water, alcohol, or ether containing cholochrome in suspension in a finely divided
state, decomposes the latter with effervescence due to the evolution of nitrogen.
There remains in the vessel a new acid, viz. cholochromic acid, insoluble in water,
but soluble in alcohol, ether, and chloroform, and yery changeable on exposure to
air, It crystallizes in dark-red rhombic octohedra when its solution in chloroform
; 7 Lo
S 10
x
148 REPORT—1860.
is evaporated in a current of hydrogen or coal-gas, and the crystals much resemble
those of hematoidine. The hematoidine extracted by Valentiner and Briicke
from gall-stones and ox-bile has some resemblance to this new acid. From the
above reaction it is evident that cholochrome, like the other acids of the bile and like
hippuric acid, leucine and tyrosine, and many other substances connected with the
human economy in health and disease, is an amido-acid, i. e. an acid in which the
nitrogen is contained in the form of amide (NH?) ; this radical replacing one equi-
valent of hydrogen in the hypothetical acid, of which the cholochromic is the oxy-
acid, the radical (N H’) in the amido-acid being replaced by peroxide of hydrogen
(110?) in the oxyacid.
With nitric acid, cholochrome yields an amorphous yellow substance, little
soluble in water, nitro-cholochrome, a crystallizable acid easily soluble in alcohol,
perhaps nitrocholic acid ; and a colourless syrupy acid easily soluble in water, and
yielding a crystallized salt with ammonia, perhaps cholesteric acid or a homologue.
Chlorine transforms the brown matter, cholophaine, into the green cholochloine in
the space of a few minutes. The process of Heintz required several weeks for
effectine the same transformation. The continued influence of chlorine produces
the red cholochromic acid, which exists, however, only for a moment, being trans-
formed into white chlorocholic acid, little soluble in water, more soluble in alcohol.
These researches have been undertaken by Dr. Thudichum, partly with a view
of ascertaining the pathological process which gives rise to certain casts of the
biliary ducts, previously described by him in the ‘ British Medical Journal.’ He
believes it to resemble the putrefaction of bile in a stoppered bottle. If the process
is acute, it constitutes “ biliosity or biliousness;” if more chronic, it gives rise to
casts of the ducts and gall-stones; if it extend to the liver-cells, it constitutes ma-
lignant jaundice.
The author further intimates that, since the above reaction with nitrous acid is
now ascertained, the therapeutic eflects of nitric and nitro-hydrochloric acids in
various forms of jaundice, which are already recognized by many practitioners, are
deserving of further investigation and trial, His own experience is in favour of
these remedies,
GEOGRAPHY AND ETHNOLOGY.
Opening Address by the President, Sir Ropericx Impey Murcuison,
D.C.L., F.RS., V.PR.GS. & V.P.R.GS., Director-General of the
Geological Survey of the United Kingdom.
Durine the last two years only, the President of each Section of the British Asso- ,
ciation having usually opened the business of the Meeting by a short address, it fell
to my lot to offer a few words to the Geographers and Ethnologists who were as-
sembled at Lecds in 1858. I there expressed the satisfaction I felt in proposing, at
the Edinburgh Meeting in 1850, the formation of a separate Section for Geography
and Ethnology, to occupy the place left vacant by our Medical Associates who had
seceded to found an Association of their own. ;
Until that year Geography had been attached exclusively to the Geological Section,
in which it was almost submerged by the numerous memoirs of my brethren of the
rocks, whilst Ethnology, forming a Sub-Section, with difficulty obtained a proper
place of meeting. Now, however, both these sciences are, [ am happy to say, fully
represented, and I trust that the result of the coming week will show that the sub-
jects to be illustrated will attract so many members to our hall, as will prove that
Geography in its comprehensive sense is as popular in Oxford as it is in the metro-
polis.
Before I enter upon the consideration of any memoirs which may be laid before
us, let me allude to a few of the subjects of deep interest which have been illustrated
by British Geographers in various parts of the world in the two years which have
elapsed since I had the honour of last presiding over you.
In Africa, the earlier discoveries of that great traveller Livingstone have been fol-
TRANSACTIONS OF THE SECTIONS. 149
lowed by other researches of his companions and himself, which, as far as they go,
have completely realized his anticipation of detecting large elevated tracts, truly
Sanatoria as compared with those swampy and low regions near the coast, which
have impressed too generally on the minds of our countrymen the impossibility of
sustaining a life of exertion in any intertropical region of Africa. The opening out
of the Shire river, that grand affluent of the Zambesi, with the description of its banks
and contiguous lofty terraces and mountains, and the discovery of the healthfulness
of the tract, is most refreshing knowledge, the more so as it is accompanied by the
pleasing notice, that the slave trade is there unknown except by the rare passage of
a gang from other parts. Again, this portion of the country so teems with rich
vegetable products, including cotton, and herds of elephants, as to lead us to hope
that the spirit of profitable barter, which powerfully animates the natives, may lead
to their civilization, and thus prove the best means of eradicating the commerce in
human beings.
Whilst Livingstone was sailing to make his last venture, and to realize the promise
he had given to his faithful Macololo friends, that he would return to them, and
bring them kind words from the Queen of the people who love the black man, Cap-
tains Burton and Speke were returning from their glorious exploits in a more central
and northern region of South Africa, where they had discovered two great internal
lakes or freshwater seas, each of not less than 300 miles in length.
I may here notice, to the honour of our Government, and particularly to that of the
present Secretary of Foreign Affairs, that the undaunted Captain Speke, associated
with another officer of the Bengal army, Captain Grant, has received £2500 to enable
him to terminate his examination of the great Nyanza Lake, under the equator, and
we have reason to hope that he will find one of the chief feeders of the White Nile
flowing out from its northern extremity, and thus determine the long-sought pro-
blem of the chief source of that classic stream.
I also trust, that in the last and most arduous portion of his efforts in proceeding
northwards, he will be assisted through the cooperation of Her Majesty’s Consul at
Khartum on the Upper Nile in traversing the country immediately to the north of
the equator, where notraveller, ancient or modern, has ever penetrated, and which is
inhabited by wild and barbarous natives. After a residence of sixteen years in that
region, and having made many trading expeditions to the confines of this unknown
region, that bold and experienced man, Consul Petherick, is, I am persuaded, the
only European who can afford real assistance to Captains Speke and Grant; and
if by their united efforts the true source or sources of the Nile should be discovered,
Britain will have attained a distinction hitherto sought in vain from the days of the
Roman Empire.
During the week of our meeting, Mr. Petherick will bring before us his project,
which I trust you will support*, either for ascending the Nile to its source or
affording effective assistance to Captain Speke, without which it is much to be feared
that the gallant officer will never be able to traverse the savage tracts which intervene
between the Nyanza Lake and the highest part of the Nile yet visited by any
traveller.
If we turn to the Polar Circle, we see what individual British energy has been
able to elicit from the frozen North. There, indeed, notwithstanding many a well-
found expedition sent out to ascertain the fate of Franklin, all our efforts as a nation
had failed, when the energy and perseverance of a woman, backed only by a few
zealous and abiding friends, accomplished the glorious end of satisfying herself, and
of proving to her admiring country, that in sacrificing their lives, her heroic husband
and his brave companions had been the first discoverers of the North West Passage.
For her noble and devoted conduct in having persisted through so many years
to send out expeditions at her own cost, until she at length unravelled the fate of
the ‘Erebus’ and ‘Terror,’ the Royal Geographical Society of London has rightly
judged in awarding to Lady Franklin one of its Gold medals, whilst the other has
been appropriately given to that gallant and skilful officer Sir Leopold M‘Clintock,
who in the little yacht the ‘ Fox’ so thoroughly accomplished his arduous mission.
He not only ascertained the death of Franklin, and the subsequent abandonment of
'* A Subscription List in furtherance of this great object is opened, headed by Lord Ash-
burton and Sir Roderick Murchison,
150 REPORT—1860.
his ships, but also showed that the great navigator had discovered vast breadths of
Arctic lands and seas which were entirely unknown when he left our shores, and
had even remained so until the truth was revealed by the expedition of the ‘ Fox.’
The geographer who compares the map of the Arctic regions as laid down by
Parry and others up to the year 1845, when Franklin sailed, and marks on it all that
he is now known to have added in the two brief summers before he was beset, and
then inspects any one of the most recent maps, even up to the year 1858 inclusive,
and traces the discoveries made by M‘Clintock and his associates, Hobson, Young,
and Walker, will see what vast additions to geographical knowledge have been made
by the last expedition of Lady Franklin.
Such services are indeed worthy of the highest national reward, and I have, I am
happy to say, reason to know, that a monument in commemoration of the glorious
deeds of Franklin and of his having been the first to discover a North West Passage
will be erected, and also that the officers and crew of the ‘ Fox’ will receive that recom-
pense to which they are so justly entitled at the hands of their admiring countrymen.
Whilst on this subject, I may well express the satisfaction and pride I felt as the
President of this Section, when the officers of the British Association asked us, the
Geographers, to bring forward one of our distinguished men to deliver a lecture
on one of our manifold subjects, before the body of men of Science assembied
at Oxford. As this is the first occasion since our foundation on which geographical:
discovery has been considered to be of sufficient scientific importance to occupy the
attention of the whole meeting, I rejoice in the fact, and also in the knowledge that
Captain Sherard Osborn, so well known to us through his charming ‘ Arctic Stray”
Leaves,’ and other books, as well as by his laurels won in the Crimea and the Sea
of Azof, is to be the lecturer, and that he who is so experienced an ice-man is to
give us a sketch of the discoveries of Franklin, as laid open by the last researches of
Sir Leopold M‘Clintock. ;
And here I may well say, that every justice will be done to any subject connected
with the conditions of icy seas, including the proposed submarine telegraph by the
Faroe islands, Iceland and Greenland to Labrador ; for never at any of our former
meetings have I seen so many explorers met together who have rendered their names
eminent through Arctic and Antarctic discoveries. Under their observation the
paper which is to be brought before us by Captain Parker Snow of the Merchant
Marine, warmly urging a further search after the missing crews and scientific records
of the ‘Erebus’ and ‘ Terror’, will be ably scrutinized. The names of Admiral Sir
James Ross, Sir Edward Belcher, Captains Ommaney and Sherard Osborn, when
united with those of Sir J. Richardson and Dr. Rae, are truly guarantees that the
question will have so much light thrown upon it, as will either satisfy the public
that no additional important results as respects the lost expedition can be achieved,
or they will stimulate us to fresh exertions. For, though all the Arctic voyagers
with whom I have conversed are satisfied that there is now no longer the hope, which
I long cherished, of saving a human life, still every man of science must wish that
strenuous efforts should be made to recover, if practicable, some more of the many
scientific records of the lost expedition which may have been left in various places
around the spot where Franklin breathed his last.
In the vast possessions of British North America much additional knowledge has
been gained by the successful explorations of Palliser and his associates, Hector,
Blakiston, and Sullivan, not only as respects the great fertile prairies watered by the
Saskatchewan and its affluents, but also touching the practicability of traversing the
Rocky Mountains within our territories by passes lower than any which exist to
the south of the boundary of the United States.
At this stage of our inquiries it would be very hazardous to speculate on these
passes being rendered available for railroads ; the more so, as the wild region lying to
the west of the Rocky Mountains—i. e. between them and those parts of British
Columbia which are gold-bearing, and are beginning to be inhabited by civilized people -
—is as yet an unexplored woody region. We may hope, however, that such routes of
communication will be established as will connect the Red River settlements with
the prairies of the Saskatchewan, and these last with the rich auriferous tracts of-
British Columbia. And if the most northern lines be found too difficult for railway
communication, through the severity of the climate and physical obstacles, let us
_— oe
TRANSACTIONS OF THE SECTIONS. 151.
hope that by giving and taking ground in an amicable manner with our kinsmen of
the United States, we may be enabled by a more southern railroad to traverse the
prairies on either side of the neutral boundary, and then pass down the river Co-
Jumbia to Vancouver Island. By this operation the great Gulf of St. Lawrence and
Hudson’s Bay on the east, may eventually be placed in communication with the
noble roadsteads of Vancouver Island and the adjacent mainland on the Pacific. At
all events, Britain will doubtless not be slow in establishing communications between
the Atlantic and Pacific, first by the electric telegraph, next by ordinary roads, and
finally, it is to be hoped, in part at least, by railroads.
On these subjects we are to be favoured at this Meeting with a paper by Captain
Synge, in addition to the vivdé voce communications of Captain Palliser and his asso-
ciates.
Having not as yet had access to many of the papers which are to be communi-
cated to this Section, I can allude to a few more of themonly. In a Memoir on the
Geographical Distribution of Plants in Asia Minor and Armenia by my distinguished
friend M. Pierre de Tchihatcheff, you will find some remarkable results as flowing
from the long-continued researches of that ardent and successful traveller. After
accounting for the absence of some plants and the profusion of others in given
localities as dependent on climatal conditions (an example of which is, that the grape
there flourishes in one tract at the great height of nearly 6000 feet above the sea),
M. de Tchihatcheff brings out some striking statistical data, showing the vastly
greater abundance and variety of vegetation in Asia Minor compared with that of
any other country. He points out that the plants of five mountains only amount
in number to double the entire quantity of British plants, and concludes with an
eloquent regret that these classic regions, so blessed by the hand of the Creator, and
which in the earlier history of mankind were replete with highly civilized communi-
ties, should now, through misgovernment, be the scene of oppression and barbarity.
Another distinguished Russian geographer, M. N. Khanikoff, who has explored
large portions of Persia and the adjoining countries, will bring before us his maps
and descriptions of the mountainous tracts of the countries of the southern parts of
Central Asia, where the lofty mountains.ef Ararat, Demavend, and Savalan form the
chief elevations of the region to which we look as the cradle of our race.
But, to revert to subjects connected with Britain. In no portion of the surface of
the globe have we made such great and rapid advances as in Australia. Doubtless
much of this progress in settlement and civilization, particularly in Victoria, is due to
the discovery of those enormous masses of gold which are producing far and wide
such powerful effects. But looking to the work of purely geographical pioneers, I can
declare, that some of the most valuable and daring researches from the earliest days
to the present time have been completed, wholly irrespective of profits gained
through the attraction of the precious metal. The great discoveries of Sturt, Eyre,
and Leichhardt were made before the existence of gold was known; and even now,
when it is the most seductive of baits to entice the traveller, see what vast regions
the brothers Gregory have laid open in Northern, Eastern, and Western Australia
without the recompense of a single yellow nugget. Again, look to South Australia,
where gold is scarcely known, at least in any appreciable quantity, and see what its_
inhabitants have done in pushing far into the interior, simply to acquire fresh pas-
ture-lands. In contemplating these recent discoveries, we read with astonishment
of what one individual, Mr. M‘Dougall Stewart, has accomplished in so short a time,’
and of the privations he underwent to realize the existence of freshwater streams
and oases on the borders of the great interior saline desert.
Still more were we surprised when we learned that this great continent, the rivers
of which were so long considered to be useless, has had its one mighty stream, the
Murray, rendered navigable for 1800 miles. With its affluents, the Darling and
Murrimbidgee, this river may indeed be said to have been laid open for 2500 miles,
i. e. between many new towns which have sprung up in the interior and the sea—
and all this by the clearing away of the stems and stumps of trees, the result of ages
of decay.
There are now indeed in England some of the eminent men, whether governors,
statesmen, or explorers of this great colonial region, who will, I hope, before we’
atljourn, throw fresh light on these recent discoveries,
152 REFORT—1860.
Having presided for several years over the Royal Geographical Society, it has been
my duty to pass in review the progress made by the sons of Britain in different parts
of the world, and it has ever been to me a source of the sincerest gratification to
watch the rapid strides made by the colonists of Australia, and to observe how they
have carried with them all the energy of our race into the land of their adoption.
if I traced with deep interest the explorations of their boldest travellers through the
bush—and witnessed with delight the working out of that golden wealth, of which
perhaps, because I was a Highlander as well as a geologist, I had a sort of second
sight—or if I revelled in seeing their ports filled with ships, and abounding in com-
merce—not all these attributes have rejoiced me more than the knowledge | acquired,
that our Australian colonists are truly and sincerely attached to Britain and their
Sovereign.
As it is out of my power on the present occasion to advert to all the recent ad-
vances in ethnology, I will now only say, that, besides many communications from
other gentlemen, including Mr. Lockhart’s excellent notes on China, my eminent
and valued friend, Mr. John Craufurd, will give us two memoirs; the one, “On the
Relation of the Domesticated Animals to Civilization ;” the other, “‘ On the Aryan,
or Indo-Germanic Theory ;” each of which will, I doubt not, be worthy of the Pre-
sident of the Ethnological Society of London.
Let me, however, offer a few general observations on those sciences, to the culti-
vation of which the business of this Section is devoted. Geography, regarded only as
the description of the outlines of the earth, and the determination by astronomical
observations of the relative position of hills, rivers, valleys, and coasts, to be laid down
by the topographer on a map, is but the key-stone of that splendid science when
viewed in its most comprehensive bearings. For, of how much real value is it
deprived if not followed in its train by all the affiliated sciences which relate to the
phenomena of our,mother earth! How infinitely is the important basis of our
science enriched by the descriptions of the animals and plants which, living on the
surface of our planct, are distinguished by forms peculiar to each region—such dis-
tribution being coincident with relative differences of climate!
Again, as a weather-beaten geologist, 1 know full well, that the science which I
have most cultivated would be void of a foundation if it did not rest on the principles
of physical geography ; for much of the labour of the geologist consists in restoring,
not in imagination, but by a positive appeal to data registered on tablets of stone,
the former outlines of sea and earth at different successive periods, whilst he marks
the various oscillations of land and Avater as well as the necessary accompaniments
of grand meteorological changes.
If therefore the geographer is guided to the relative position of his localities by
the lights of astronomy, he also knows that accurate observation of all terrestrial
changes is of the highest value in enabling his ally the geologist to interpret and
read off the former conditions of the crust of the earth. Just as geography in its
present phase is necessarily connected with ethnology, so its earliest features as a
science can best be thoroughly comprehended by the geologist. His is the province to
bring to the mind’s eye various relations of land and water through the olden periods,
when most of our present continents were fermed bencath the sea; and to trace the
successive elevations and depressions which characterized epochs long anterior to
the existence of man. Even in those remote times when some lands were elevated
and others depressed, we have ascertained that the waters and the earth were occu-
pied by various animals which successively lived and died to be followed by other and
more highly organized races, until at length a being endowed with reason was created.
And when, having gone through all the long epochs of geological time, we ap-
proach the period when man appeared, how interesting is it to endeavour to unravel
the changes which our lands underwent from that recent geological date when the
British Isles formed part of the terra firma of Europe! ‘Then at a later period, how
inviting is it to mark the signs of the commixture of the rudest and earliest works of
man with the remains of animals, most of which are now extinct, yet mixed up with
others which have lived on to our own day!
Thus, whilst the geological geographer visits the banks of the Somme, and sees
such an assemblage of relics beneath great accumulations formed by water (as I have
recently witnessed myself), he is compelled to infer, that at the period when such a
TRANSACTIONS OF THE SECTIONS, 153
phenomenon was brought about, the waters which have now diminished to an ordi-
nary small river, rose in great inundations to the height of 100 feet and more above
the present stream, and swept over the slopes of the chalk on which the primeval
inhabitants were fashioning their rude flint instruments —when, as I would suggest,
they might have escaped to the adjacent hills, and saving themselves from the sweep-
ing flood, have left no traces of their bones in the silt, sand, or gravel.
This linking on of geology with human history and the works of primeval art
comes legitimately under our consideration, and here we have just as full right to
discuss and test this question as my dear friends the geologists, the more so as it
was to this connexion between geology and history that Lord Wrottesley has called
the attention of the Association in his Presidential Address.
Then, again, as we descend with the stream of time until we reach historical
records, the geographer next endeavours to throw light on the marches of the great
generals of antiquity and the sites of ancient cities; and then truly the geologist,
geographer, and ethnologist become united with the antiquary and historian. Taking
our recent British example of the discovery of the Uriconium of the Romans at
Wroxeter in Shropshire—where is the geographer who has looked at the mounds of
earth which till recently covered that ancient city, and is not convinced, that causes
arising from the combined destruction by man and natural decay, have produced the
mass of overlying matter on the shores of the Severn, which has hidden from our
vision one of the famous Roman towns of Britain ?
As I have delighted in tracing the sites of the battles of our great British chief
Caractacus*, and in unravelling the age of those Silurian rocks in which he made
the chief defences of his own kingdom, so I can now bring back to my imagination
how the legions of Ostorius may have been reinforced from that Uriconium, which
has just been disinterred from its earthy covering by the zealous labours of the
enlightened antiquary Wright, now a Secretary of this Section.
In this manner we see, that as our inquiries necessarily stimulate us on the one
hand to recede to the very earliest traces of man upon the globe, so, on the other,
we are led on into that department of Art and Archeology which connects the present
with the past, and are thus enabled to offer to the consideration of our associates
and auditors, subjects of prevailing and universal interest—subjects which will, I
doubt not, be handled with redoubled zest, now that we are again happily met
together for the third time in this very ancient seat of learning.
In conclusion, Ladies and Gentlemen, I have now only to congratulate you on the
recent rapid extension of geographical science throughout the enlightened classes of
our countrymen. Brought up with a profound reverence for the works of God, and
a due admiration of the fivest efforts of man, those sons of our gracious Sovereign
who are of sufficient age to profit by extensive travel, are already proving, that in
their spirit of adventure they are true Englishmen. The heir to the crown, after
rambles in our Scottish Highlands and travels on the continent, is about to quit this
his Alma Mater, and, to the great joy of our colonists, to visit North America, and
there rivet still more strongly the link which binds the loyal people of those pro-
vinces to the mother country ; whilst Prince Alfred, after cruizing in the Mediter-
ranean, is now sailing across the Southern Atlantic to Bahia, not without having
ascended on his way to the very summit of the Peak of Teneriffe. The willing co-
operation of the last and present President + of the Royal Geographical Society
demonstrates that our nobility are as much alive to the vast importance of our
subject as the middle classes of the community. On my own part, having laboured
zealously in diffusing geographical knowledge among my countrymen, I can truly say
that my gratification is now complete in seeing that this Section is second in popu-
larity and utility to no branch of the British Association.
On the Caravan Routes from the Russian Frontier to Khiva, Bokhara,
Kokhan, and Garkand, with suggestions Sor opening up a Trade between
Central Asia and India, By 'V. W. ArxKtyson.
* See the Preface to the ‘ Silurian System.’
t Earl de Grey and Ripon, and Lord Ashburton.
154 REPORT—1860.
On the Caravan Route from Yarkand to Mai-matchin, with a short account
of this Town, through which the Trade is carried on between Russia and
China. By T. W. AtKinson.
On the Manufacture of Stone Hatchets and other Implements by the Esqui-
maux, illustrated by Native Tools, Arrow-heads, §e. By Captain Sir
EI. Bencuer, NV.
Sir Edward commenced by setting forth his belief in the connexion of the north-
ern littoral tribes of Asia, America, and Greenland in habits, customs, and language,
differing less in this latter point than in our counties in England, Wales, or Scotland.
Comparing the American with tlie Asiatics, the Tchutchi, he found the latter more
experienced or accomplished in music, manufacturing their own violins, and per-
forming wonderfully, imitating @ la Paginini on one string the sounds of various
animals ; they were also good buffoons and actors as imitating the anctics of bears,
&c. But as regards the useful arts, or those calling for invention or energy in over-
coming difficulties, improving tools, weapons, &c., they were much inferior to the
Esquimaux of America, and certainly far below them in mental acquisitions. Sir
Edward then gave an interesting description of the habits and manners of the tribes
with which he lived in contact near Icy Cape. He obtained great influence over
them, and so long as he continued to teach them any new mode of working they
submitted to his direction. He had no doubt, if necessity had compelled him to re-
main there (as he was wrecked there), he might have existed and possibly become one
of their chiefs. This disposition on their part to associate with and be instructed
by white men, confirmed him in the notion he had entertained, that possibly one or
two of the crews of the ‘Erebus’ and ‘Terror’ might have escaped and be now
willingly living among them.
The principal object of the paper was to explain the stone implements found
among them, and similar to those of Celtic origin, as well as their mode of manu-
facturing them from a vein of chert at hand. Sir Edward saw them obtain the
chert from the stratum, work them into spear and arrow-heads, and there purchased
the articles as well as the tools employed which were explained in detail to the Meet-
ing. No hammer or blow is used in splintering off the conchoidal splinters to form
the serrated edges, but a tool of deer antler effects this by pressure on the faces alter-
nately. Sir Edward also observed that the same process is adopted by the Indians
of Mexican origin in California, by the natives of the Sandwich Islands, as well as
Tahiti, 2300 miles asunder. Other curiously wrought and interesting instruments, as
planes, drill bows, &c., were exhibited, all manifesting great skill and a higher degree
of mechanical ability than we could expect from an untutored race—indeed a race
taking the lead pre-eminently in meeting scientifically those wants occurring in savage
life. With reference to their ornamentation of their drill bows, &c., Sir Edward
maintained that they exhibited proofs of record, which Dr. Rae considered to be
wanting in the tribes encountered by him some degrees to the eastward. Steam,
and the mode of using it, to bend or straighten bows or arrows, was constantly em-
ployed by them; and Sir Edward concluded by expressing his conviction that these
people were in a condition to be rendered useful by civilization, and thus epen more
lucrative trade with the western and southern nations in the Pacific.
On the Aryan or Indo-Germanie Theory of Races.
By Joun Crawrourp, FAS.
The object of the writer of this paper is a refutation of the Aryan or Indo- Genial
theory, or that which supposes all the peoples from the eastern confines of Bengal
to the western shores of Spain and Britain to be of one andthe same race of man, on
the evidence of a fancied identity of language. A few of the main objections advanced
by the author may be stated. The theory supposes a people, whose language was the
Sanskrit, to have migrated at some unknown time, spreading east in one direction
and west in another, and to have performed these prodigious migrations, although an
agricultural people, or in other words, one of fixed habits. ~The theory makes men
aS ae ee Oe; ee
TRANSACTIONS OF THE SECTIONS. ‘ "455
who are black like the Hindus, brown like the Russians, and fair like the Standina-
vians, to be of one and the same race, insisting that the Greeks of Alexander and the
Englishmen of Clive had the same blood in their veins as the Hindus whom a hand-
ful of them vanquished. As to the supposed identity of race from the evidence of
language, the author considered it sufficiently disposed of by the notorious fact that
many of the languages of Hindustan spoken by people asserted to belong to the
Aryan stock, had no fundamental relation to the Sanskrit tongue of the supposed
Aryans. In Europe, the isolated Basque language was evidence to the same effect.
On the Influence of Domestic Animals on the Progress of Civilization (Bir ds).
By Joun Crawrurp, F.R.S.
The object of this paper, one of a series on the same subject, was to show the
effect of the domesticated animals in the civilization of man, and was confined to
birds. The author showed that out of the vast variety of the feathered creation, not
above nine or ten species had been domesticated, while there was a wide range in
the quality and amount of the domestication which even this small number had
attained. The origin of a few of the species only could be traced to particular
countries, as the common fowls to India and China, the turkey to Mexico, and the
gallinze to Africa. But he seemed to think that the first domesticated of the greater
number was common to several countries, as the grouse, pigeon, duck, to most
countries of Europe and Asia. The author further showed that the numbers of
birds domesticated by a people might be considered a measure of their relative civilis
zation. Thus savages possessed no domestic bird at all; barbarians very few, and
the most advanced only the whole number. Thus the savage tribes of America pos-
sessed none at all. The Mexicans possessed but one. The more advanced tribes of
the South Sea had one, the common fowl, while the Australians had none. The
Malayan nations were possessed of two, the common fowl and duck; the Persians
of these and the pigeon, and Hindus of the last three with the peacock ; and the
Chinese of five, the common fowl, the goose, the pigeon, and two species of pheasant,
It is the more civilized nations of Europe alone that possess the entire number,
On certain remarkable Deviations in the Stature of Europeans.
By R. Curt.
On the Existence of a true Plural of a Personal Pronoun in a living
European Language. By R. Curr.
On a Set of Relief Models of the Alps, §c.
By Captain Cysurz, Imperial Austrian Artillery.
The author desires to introduce to the notice of this Meeting a set of models, in-
tended to facilitate instruction in the manner of delineating the features of the ground
on topographical maps, and lately introduced into the technical schools of Austria.
It is the first aim of the author to lead the pupil, by means of these models, to a
correct understanding or appreciation of form, as the only way of producing a first-
rate topographical draftsman. Instead, therefore, of setting him to imitate drawings
from paper, his studies and copies will be made from models, and, at a more advanced
stage, from nature itself. These models represent, first, inclined planes or slopes,
separate, in combination, or intersecting each other. It is from these the pupil acquires
the first idea of the principle upon which depends a correct delineation of the ground..
Secondly, we have three models which represent the most characteristic and most
widely distributed features of the ground. Having acquired from the preceding a
thorough knowledge of fundamental principles, the pupil will proceed to delineate
upon paper the following models. ‘These represent, first, an undulating country ;
secondly, a plateau formation, with deeply-cut valleys; thirdly and fourthly, some
mountainous tracts. Contour lines have been laid down upon the whole of these
models with mathematical accuracy. The horizontal projection of some of the most
difficult sections has also been added, to illustrate the manner of filling up the con-
156 REPORT—1860.
tour lines and laying down auxiliary contours. It has not, however, been thought
advisable to do more, as otherwise the pupils would avail themselves of these facilities
to too great an extent. A small instrument for measuring the gradients, and a scale
showing the intensity of the shading (hachorres) for various degrees of acclivity, are
to be made use of in copying the models. ‘The author believes that the use of
models, judiciously selected, will engage the pupil’s uninterrupted attention ; he will
overcome mechanical difficulties with greater facility, and will not be so wearied as
by the tedious, but abortive, and, in reality, useless attempts to copy a topographical
drawing placed before him, ‘The author would add, that his models have been made
of galvanoplastic copper, and are therefore not so liable to breakage as plaster-of-
Paris models.
On the Arrangement of the Forts and Dwelling-places of the Ancient Irish.
By the Rev. Professor Graves, M.A.
On certain Ethnological Boulders and their probable Origin.
By the Rev. Epw. Hincxs, D.D.
The author began by observing that, if a geologist were to see a mass of stone
lying in a place where all the rocks around were of a totally different character, he
would not be satisfied till he had accounted for its being there; till he had found
whence it came, and at what period, and by what agency it was brought. He be-
lieved that like inquiries should be made, and might be answered, respecting ethno-
logical boulders ; by which he understood words ‘occurring in writings of remote
antiquity, which were of a totally different character from the words of which the
writings were mainly composed. He believed that it would be possible, by help of
these boulders, to trace the people to whose Janguage the words belonged, along the
line by which they must have travelled, forward to the point where their migration
terminated, and backward to that where it must have commenced. In the pre-
sent paper he proposed to do this in a particular case, the discussion of which
was peculiarly appropriate to the present meeting, as it related to that language, a
proficiency in which was the acknowledged glory of Oxford.
The language of the Assyrian inscriptions is of the family called Semitic, that is,
of the same family with Hebrew; and by the way it resembles this language in some
important particulars, such as having a Niphhal conjugation, more closely than it does
any other known language of that family. It is remarkable also that the copious
inscriptions which exist in this language were all written between the writing of the
earliest and the writing of the latest books of the Old Testament; so that it would
seem that no language could be expected to clear up what is obscure in these books
so well as the Assyrian.
In these Semitic inscriptions, however, numerous words are to be met with which
are evidently not Semitic. One class of such words was pointed out several years ago
by Sir Henry Rawlinson. They belonged to the language of Chaldea or Accad, which
was spoken to the south of Assyria, and which he pronounced to be an Hamitic
language, akin to the Egyptian.
In a paper read at the Dublin Meeting of the British Association in 1857, of which
a copious abstract is given, pp. 134-143 of the Report, Dr. Hincks took a very
different view of the matter. He maintained that this Accadian language represented
a sister language to that which is the common parent of all the Indo-European lan-
guages ; the common parent of these two, which he called the Japhetic language,
being a sister to the Egyptian language and to the common parent of all the Semitic
languages. He now aflirmed that the views contained in that paper (with which he
must, for brevity, assume that his hearers were acquainted) were fully confirmed by
his subsequent researches, and that he had met with nothing inconsistent with
them. The linguistic pedigree there laid down was so fully established by induction
from a number of verbal pedigrees that it needed no further confirmation. Still,
comparisons of Indo-European words with words of one of the languages above
named, which was not Indo-European, would be found useful, and that in three
ways :—
1, Such a comparison might establish the fact of a word having been in use in the
TRANSACTIONS OF THE SECTIONS. 157
original family from which the Indo-European races have sprung. This fact may be
inferred from the word being used by remote subfamilies ; but its being used by two
subfamilies (or even by a siagle one), and being also found in one of the languages
that are cognate to the original Indo-European, but not derived from it, is still
stronger evidence. Thus the word horse, which is peculiar to the Teutonic family, but
which is cognate to the Latin curro, ‘‘I go like a horse, 7. e. I run,” is shown to
have been in use in the original Indo-European family from its evident connexion
with the Accadian kurra. The original Indo-European root must have been kurs.
2. Such a comparison may determine the original form of an Indo-European root,
which varies in the different languages known to us; as it may also determine the
original Semitic form. For example, in p. 141, Report for 1857, the facts that the
original Indo-European form of the second numeral was iwi and the original Semitic
form thni, could only be established by a comparison of the different forms known to
exist with the Accadian mi, as explained in that paper. In treating of the words for
“lion,” No. 14, he was ignorant that the Assyrian word was libbu. Comparing
this with the Accadian /ig, he now thinks that the Semitic form must have been ligh,
and that this was also the Japhetic form. The Indo-European root would be ligw.
In Latin this would be declined lix, livis; and, as (s)nix, (s)nivis gives snow in
English, and snig, sneg in the Letto-Sclavonian languages, so /éwe in modern and
lew in older German correspond to lix; and lig might be the ancient Letto-Sclavo-
nian root, equivalent to these.
3. An etymological relation between Indo-European words may possibly be
established if both can be shown to correspond to the same word in a language
which is not Indo-European. ‘Thus, the relation between yAvkis and yAéaca is not
generally admitted by Greek lexicographers ; though if the words be written as they
would be in the Cadmean alphabet (see p. 142 of the former paper), yAok-Fes and
yox-1a, the resemblance is easily seen. But this relationship is established when
we find that ghlu is used in Egyptian both for “sweet” and for “tongue.” The
Latin dulcis, originally dlucvis, is cognate to these.
Enough, however, on the subject of the Accadian words occurring inthe Assyrian
inscriptions. They present no ethnological difficulty, as the people who spoke the
language to which they belonged lived close to Assyria. The case is the same with
the Semitic words which occur in the Egyptian inscriptions. He pointed out one in
1845; MID“ achariot;” used also for “ chariots ;’’ the Egyptians not generally
expressing the vowels, and thus writing the terminations eth and 6th alike. Mr.
Birch has since found another meaning, ‘‘ round bucklers,’’ which appears to be the
Arabic we pe These are Canaanitish words, expressing objects brought from
Canaan.
There were words, however, in the Assyrian inscriptions which Dr, Hincks be-
lieved to be Indo-European; and as no Indo-/uropean people had been hitherto
recognized as existing on the west of Assyria, their existence presents an ethnolo-
gical difficulty which the author seeks to explain in this paper.
The words in question were ligwindinas and ldsanan. The former occurs on a
great slab or altar in the north-west palace at Nimriid (B. M. Series, pl. 44, I. 17).
Every other word in the sentence is of known signification. ‘“ Z. alive I took cap-
tive.” From the context it must necessarily be the name of an animal, in the plural
number (being joined toa plural adjective) and in the accusative case (being governed
by a transitive verb). Every one who has the slightest knowledge of the grammar
of the Semitic languages must see that ligwindinas cannot be a Semitic accusative
plural; and every one that knows anything of the grammar of the Indo-European
languages must see that it is a regularly formed Indo-European accusative plural.
Taking it as Sanskrit or Zend, the nominative singular would be ligwind?; taking
it as Greek, it would be ligwindis or ligwindin. Whatever be the particular language
to which it belongs, and whatever be the meaning, its being Indo-European ought
uot to be questioned. The other word, /dsanan, has puzzled the interpreters of the
Assyrian inscriptions as much as any other word. It occurs in several contexts :
«king ldsanan’’ after ‘‘ king of Assyria” on Bellino’s cylinder, 1. 1; ‘ ruler of the
tribes /dsanan,” on the Tiglath Pileser cylinder (I. 29), “ wielder of the sceptre ldsa-
nan,” same cylinder (VI.56). ‘Assur the great lord has made me to possess (? yusad-
limanni ; the first radical may be 7, 0 or 4) the kingdom ldsanan,” Bellino’s cylinder,
158 REPORT—1860.
1.4. In all these contexts, a genitive of the name of a people who were not Assy-
rian seems required. Yet ldsanan is an impossible form for a Semitic genitive. The
word }W), “a language, i. e.a people speaking a language,”’ suggests itself at once;
but its genitive plural would be disandti. The idea that ldsanan should be resolved
into two words, the first being Jd, the negative particle, suggested itself also; but to
this also there were insuperable objections. Sanan is, no doubt, the theme of an
adjective; but when joined to a noun it must have a case ending. In the first con-
text the rules of grammar would require sannu, in the second sanndii, in the third
sanatii euph. for sanandi. In the fourth sarrut is in construction, and would require
a genitive after it, and not an adjective. The same might be said of kissat in the second
context. Besides, /é sanan would mean “ not fighting,’’ and would be the very last
title that a king of Assyria would apply to himself. The translation “‘ unchanging,”’
which has been suggested, would require Jd sanah, in place of Id sanan, if the case
ending were to be omitted, which, however, it could not be.- Whether, therefore,
ldsanan be regarded as one Assyrian word or as two, it presents insuperable diffi-
culties. These, however, disappear at once if it be considered as an Indo-European
word. It has all the appearance of an Indo-European genitive plural from a nomi-
native /dsas; and such a word is just what will suit all the contexts. Accordingly,
the recognition of ligwindinas as Indo-European led immediately to the recognition
of ldsanan as so too.
The next question to be considered is to what country the Indo-European people
who used these words belonged.
The account of the hunting expedition in which the Assyrian king took the lig-
windinas is preceded by that of his receiving tribute from the people on the coast of
Syria, beginning with the Tyrians and ending with the Arvadites. This renders it
probable that his hunting was on the west of Assyria; and indeed he states in the
Payement Inscriptions that he hunted on the banks of the Euphrates. Again, if the
word ldsanan signified a people, other than the Assyrians, over whom Tiglath Pileser
acquired dominion, they must have been to the west or north of Assyria; for he
mentions no conquests towards the south; and we know from the inscription of
Sennacherib at Bavian that he was defeated by his southern neighbours, his capital
taken, and his gods carried off by them. He could have had no dominion over the
Medians, or any neighbouring people that have been hitherto supposed to be Indo-
European.
This. leads to the inquiry whether the Egyptian or Assyrian inscriptions afford any
grounds for the supposition that an Indo-European population was located in Syria.
Fifteen years ago Dr. Hincks pronounced certain names published by Champollion
as those of the chiefs of the Khita, to be Indo-European. Four names terminating
with stro, as Champollion read the characters, were published by him, the former
part of the first name, which was that of the chief of the nation, being Khita, the
name of the nation. Dr. Hincks affirmed in 1845 that this name must be Indo-
European, and must mean ‘lord of Khita.’”’ He read the latter part of the name
swar, connecting it with kipios. M. de Rougé adopted this interpretation of the
name, but said that the second element in it was the Semitic sar; to which it was
replied that no Semitic compound could be formed as M. de Rougé supposed.
« Lord of Khita”’ would be Sar-Khitti, not Khita-sar, according to the mode of
arrangement of the elements of a compound name adopted by all Semitic people.
From the fact of these names being Indo-European, Dr. Hincks at first inferred that
the enemies of Rameses 11. were Scythians, as Champollion had supposed; but it
was subsequently proved that they lived within a short distance of Egypt; and their
capital Kadish, formerly read Atish, was identified with a place on the Orontes,
south of Emessa. They were, in short, the AKhattaya of the Assyrian inscriptions,
and the Hittites of the Old Testament; and their religion, as shown by the Egyptian
inscriptions, was clearly Canaanitish. How then could they have Indo-European
names?
Conceiving it to be certain that some of their chiefs had such names in the time of
Rameses II., Dr. Hincks reconciled this fact with the other by supposing that Indo-
Europeans had previously overrun their country, and acquired dominion over it;
but that they had adopted the religion and probably the language of the conquered
people; at any rate they had failed to impose upon them their own language. The
Kita had chiefs with Indo-European names, and doubtless of Indo-European race;
ee
acer
a
TRANSACTIONS OF THE SECTIONS. 159
just as the English in the twelfth century had Norman chiefs with Norman names;
but the great body of the people had in both instances remained unchanged.
There was thus evidence that a body of Indo-Europeans had conquered the coun-
try north of Mount Lebanon before the reign of Rameses II.; and on the other
hand, there was evidence that at the marriage of Amenholp III. the Egyptian empire
extended to Naharina or Mesopotamia. During this interval a peculiar form of
sun-worship was introduced into Egypt, and obtained a temporary superiority. That
this worship was of Aryan origin and that its introduction synchronized with the loss
of the foreign conquests of the Egyptians, are generally admitted by Egyptologists.
The middle of the reign of Amenholp III. must therefore have been about the time
when the Indo-European invasion in question took place; 7. e. according to Lepsius,
1506 u.c.; according to Bunsen, 1468; according to Dr. Hincks, about 1390.
Of the four proper names of Hittite chiefs which, according to Champollion,
ended in siro, three are supposed by Dr. Hincks to signify lords of different people ;
the fourth (Sopa-siro of Champollion) he reads Asp-iswar, ‘lord of the horse.”’ This
reading (which, as well as the worship of the sun which these Indo-Europeans prac-
tised, suggests their close connexion with Persia) is confirmed by the name of Kus-
taspi, king of Kummukh, or Commagene, who, along with Razin of Damascus
and Minikhimi of Samaria, paid homage to Tiglath Pileser II]. It would appear
that this Indo-European immigration took deeper root in uorthern than it did in
southern Syria. The name Kustaspi is evidently a compound, signifying, like that
of the father of Darius, ‘‘ having .. . . horses ;”’ the meaning of the participle wista
or kusta being uncertain. In Sanskrit and Zend such compounds require no suffix
at the end. Assuming that kusta signified “chosen,’’ kustaspa gen. kustaspahyd
would signify ‘‘ having a chosen horse, or chosen horses.’’ Here, however, a suffix
isadded. The name is kustaspi, which would have for its genitive kustaspinas. This
marked difference is an argument for the diversity of the Indo-Europeans of Syria
from the Persians, though they resembled them in their sun-worship and in using aspa
for ‘‘horse.’’ Another argument to the same effect is derived from the impossibility
of a Persian population making an incursion into Syria. Not only is the Semitic
population of Assyria interposed, but either Media or Elymais would have to be
traversed, in the latter of which the language was of a totally different character
from any Indo-European one; while in the former a dialect of Persian was used, in
which we know that aspa did not signify “a horse.”” In the Behistun inscription,
which was in this dialect, ‘horse”’ is expressed by asma, instead of by aspa, as at
Persepolis. See lines 86, 87 of the first column, where dasha and asma (in pure
Persian dasti and aspa) are translated in the Scythic, or rather Elymean version,
published by Mr. Norris, by the well-known Accadian words habba and kurra,
which are constantly used in the Assyrian inscriptions for ‘‘elephants”’ and “ horses.”
The true translation of the passage is this: ‘‘ I divided the army. A part I made to
be carried by elephants. The other part I made to swim with the horses.”
These considerations lead to the conclusion that the Indo-Europeans in Syria did
not come from Persia; but that the Persians and they formed part of the same body
of immigrants, which divided into two bodies inArmenia or the neighbouring country.
‘The next thing to be considered is the evidence which may exist of such a people
having been settled in northern Syria and the country to the north of it.
This evidence consists of proper names of men preserved in the Assyrian inscrip-
tions, which appear to be Indo-European compounds; and of names of districts
which end in a sibilant which disappears when the word is inflected, and which
must therefore be the sign of the Indo-European nominative singular ; also of names
of districts in the genitive singular, which also terminates in s.
A series of proper names of princes which all terminate alike is found in the Tiglath
Pileser cylinder; namely, Kaltantiru, Kiliantiru, and Sadiantiru. The fact of the
latter parts of the three names being the same, is strong presumptive evidence that
those names are Indo-European. ‘To determine their respective meanings is, how-
ever, the part of philology and not of ethnology. The name Kashkash, which oc-
curs in the Sallier Papyrus No. 3, as that of a country in alliance with the Khita, is
manifestly the Kaskaya of the Assyrian inscriptions; and the Muskaya of these last,
the 7W/ of the Hebrew Scriptures, is the Mushush of the Egyptian inscriptions, or,
as it should rather be written, the Muskusk ; for in ancient times the Egyptians, like
160 REPORT—1860.
the Assyrians, had no SH. They expressed that sound in foreign words by their
double letter SK. In both these instances the final sibilant, which is preserved in
the Egyptian, disappears in the Assyrian gentile adjective. Inthe name of Carche-
nish (Gargamusk of the Assyrian and Egyptian inscriptions) the case ending is pre-
served in Hebrew, Assyrian, and Egyptian. In Tarshish it is preserved in Hebrew,
but lost in Egyptian. This name has not been met with in the Assyrian inscrip-
tions; but the Greek form Tapo-ds shows that the second sibilant in the Hebrew word
is acase ending. In the Tiglath-Pileser inscription names of districts are always
expressed in the genitive, the character signifying ‘‘ country ”’ which precedes them,
being to be read as a noun in construction, mat. Some of these genitives are Assy-
rian, as Kummukhi, ‘‘ (the landof) Kummukh;”’ but others are to all appearance
Indo-European, as Ligrakhinas, Ammaus, Adaus, Skaraus. These last three have
a strong resemblance to the genitives of the Persian nouns in ush, such as Margaush,
Babilaush. The aw was pronounced as two syllables.
The next point investigated was the interpretation of the words of this language,
ligwindinas and Idsanan, and their connexion with like words in other languages.
The former word was supposed to be equivalent to Acovroeidets, and the latter to
Aady. It was observed that Aéwy was a secondary word for “lion,”’ the participle of
a verb, which was itself derived from the primitive word Nis, originally AceFs. The
words first introduced were nouns, from which verbs were derived. Thus mus,
mouse, expressed the idea to which the name was first assigned. It had been stated,
and assigned as a reason why the Sanskrit language ought to be acknowledged as
the parent of the European languages, that Sanskrit was the only language in which
the verb “to steal,’ from which mouse, ‘‘the stealer,’”? was derived, was known to
exist. It is very true that the Sanskrit noun signifying ‘a mouse” was derived
from a Sanskrit verb signifying “to steal ;’’ but this verb was itself derived from
a primary noun signifying ‘‘a mouse,’”’ which was preserved in Greek, Latin, and
Teutonic, though unknown in Sanskrit. As in English we say “‘ to ape a person,”
meaning ‘‘to do to him what an ape does,” 7. e. “to imitate him ;” so we might
say ‘‘to mouse a thing,” meaning ‘to do to it what a mouse does,” i, e. “to steal
it.” In Wilson’s Sanskrit dictionary four different forms of the verb ‘‘ he mouses it”
are given; but the roof, the primary noun mus, is not to be found in the language
at all. So much for this argument in favour of the antiquity of Sanskrit, as com-
pared with the European languages cognate to it! Whatever weight it has is in the
opposite direction.
Using the primary for the secondary Greek word for “ lion,” and the uncontracted
form, we should have AvoeSéas. In the Cadmean alphabet, in which ¢ was only
used as a semivowel, this would be written \eFoFevdéas ; and the word preserved in
the Assyrian inscriptions, if expressed in the same alphabet, would be deyFevdevas.
The other word ldsanan, expressed in this alphabet, would be Aagovor, or at least
might be so rendered; for, as long a expressed the sound of a in fall or in father,
the corresponding short a might have the sound of 0 in folly (which would be ex-
pressed by 0) as well as that of ain fat. So the Assyrian Aranta became ’Opdvrns
in Greek. In this same Cadmean alphabet, \aév would be Adadoy: the o being here
“ «iBSndov,”’ or deceptive ;—written, but not pronounced; as it was so late as the
time of Pindar.
The dropping of the sibilant between two vowels being admitted to have taken
place in a great number of instances (if not in every instance where it was originally
unaccompanied by a consonant or semivowel) by all Greek grammarians ; and the
wv of the genitive plural being also admitted by Bopp and others to have been
originally ovov and then oov (as pei¢@ was originally pei{ova and then pei{oa), there
is no difficulty whatever in deriving the second Greek word in classical use from that
preserved in the Assyrian inscriptions. The former of the two words, however,
requires some remarks.
In the first place, it is not generally admitted that -éas, from a nom. sing. -7s, has
sprung from évas. It is commonly supposed to be from evas. The point suggested
is, that the Ur-Griechisch word now discovered is evidence that this supposition is
not altogether correct. It is admitted that a compound adjective in -7s, the latter
element of which is a noun in -os -eos, such as dvo-jrevns, b1-erns, would have originally
formed its genitive in -écos. Such a word would correspond to a Sanskrit noun in
TRANSACTIONS OF THE SECTIONS. 161
ds, as dur-mands. But the question now raised is whether there may not be com-
pounds, the last element of which is a verbal root, or a primary noun from which
this is derived, to which the suffix.in was attached as implying possession; and
whether the in of such compounds has not become in the nominative -7s, -és; so that
these adjectival terminations are in some instances the equivalents of the Sanskrit
adjectival terminations 7,7. his is supposed by Dr. Hincks to have been the case
in such instances as pudo-erd-7s, d-hyd-ns, tTpt-np(er)-ns, &c.; the roots being 1d
(Fed), AaO and epes. ‘The original form of the suffix implying possession he supposed
to be ith, which was liable to pass both into ts and intoin. Thus, in the first person
plural of active verbs the original form meth, written -yer, -ped (retained in the pas-
sive, where we have in classical Greek -<8a), became pey and dialectically wes. Itis
this ¢h, written in the old alphabet r or 6, which is so apt to be dropped between
vowels, and at the end of a word, and which in the latter position, if not dropped,
must be changed into c or y. In reality, the root which is above written epes was
eped, ereth.
The addition of the suffix in, implying possession, to a compound, is unusual in
Sanskrit; but instances may be produced. One is, according to Bopp, dmndya-sdr-
iz. In Lithuanian, however, a suffix is generally added to the compound. It ap-
pears in the present languages as 7, which Bopp supposes to have been za, but which
may have been originally ix, The usual form ofa Lithuanian compound is did-burn-is,
rot-pon-is, tri-kamp-is; na-baga-s, without the suffix, is spoken of by Bopp as
exceptional.
This is one reason for supposing that the language to which these words belong
was of Lithuanian origin. The suffix in, which appears not only in ligwindinas, but
in the proper names nom. Kustaspi, gen. Ligrakhinas, may be connected with the
Lithuanian is and the Greek js, but is abhorrent to the genius of both the Sanskrit
and Zend languages.
The difference between Fevd and Fe.d seems also to require some observations.
The root is fed ; and according to the custom of the Indo-urcepean languages, and
especially of the eastern family, or families of them, a nasal may be introduced
between a short vowel and the consonant which follows it. The Greek ec and oF
were in the old Cadmean alphabet the representatives of the long vowels # and @%.
They are equivalent to iy and ww, ¢ and F being in that alphabet semivowels; and
these long vowels were substituted for « and o followed by a nasal, when that nasal
was omitted. It is worthy of notice, however, that in the inscription on a broken
obelisk in the British Museum, in the first column, where the king enumerates the
animals that he had taken or killed, or rather designed to do so (blanks for the
number being left before each name of an animal, which were never filled up), men-
tion is made in the twenty-third line of “ ligwidini’’ followed by the plural sign.
The omission of the nasal in the word, as here written, shows that it was not essen-
tial. ‘The plural sign after mi is here substituted for the Indo-European termination
nas. Possibly digwidini is intended for the nominative singular feminine ; or it may
be the nominative ligwidi with the Assyrian termination of the accusative plural.
The word wida is used in Old Prussian for ‘likeness ;”’ sta-wida and ka-wida
representing the Latin ¢alis and qualis. This is another indication of a connexion
between the languages to which these words belong, and the old Lithuanian.
A third indication of this is derived from the name /dsanan. As used in the
Assyrian inscriptions, it denoted the Indo-European tribes on the west of Assyria ;—
those who called themselves by this name. Exactly in the same way, the Egyptians
applied the name )3) to the Semitic tribes in whose language this word signified
“the peoples.”” Now this word /édsanan was originally /d/hanan; and while its
stern is the same as that of the name of the Lithuanian people, it has other affinities,
which are very remarkable. The Lydians, AvSoi, were evidently a branch of the
same people; notwithstanding the mythic derivation of their name given by Hero-
dotus. but their identity with the Lutan or Ludan of the Egyptian inscriptions is
equally certain, and still more important, as it shows us that fora considerable time
before they pushed their conquests to the neighbourhood of Egypt (viz. to Mount
Lebanon), they had been warring against them on their northern frontier, when
their empire extended to Mesopotamia.
The termination of this name requires some remarks. It may be the Semitic-
186°. 11
162 REPORT—1860.
plural ending, which the Egyptians borrowed from those tribes which intervened
between them and these Ludan; or it may be the accusative plural of the Indo-
European name. It may be well, however, to compare it with the termination of
another proper name, which occurs in the Sallier Papyrus No. 3, and which appears
to refer to the very same people. A name is found there, which Champollion read
Iwan and took for the Jonians. It has since been ascertained that the character
which Champollion read has for its value ari or ivi. The name therefore is driwan,
the Aryans or noble people, a title which the Indian and Persian branches of this
people which descended from the north applied to themselves, and which (it would
seem) the Syrian branch of the same people also used. The an at the end of these
two names is probably the same element; and the fact of its being preceded by w,
when not preceded by a consonant, suggests a third explanation of it. It may be the
suffix which appears in rdjan (nom. rdjd), Saiwewr, latron (nom. latro) and ahman
(nom. ahma), which suffix was probably the theme of the first numeral, denoting a
noun of unity. Thus Ariwan would be ’Apior, or ‘Ipiwy, from the latter of which it
is just possible that ”"Ioy may be derived.
Whatever may be thought of this last derivation, it seems clear that the Indo-
European glosses, found in the Assyrian inscriptions, are in the language of a people
which had separated, some centuries before the date of the earliest Assyrian inscrip-
tion, from the Aryans of Persia, and which had probably accompanied these in their
migration from the northern region which they originally inhabited; and that while
a portion of these western Aryans remained in Syria and the adjacent countries, the
main body of them proceeded westward through Asia Minor and across the Bospho-
rus or Hellespont, forming the Hellenic or Ionic people of the Greeks ; which mingled
with the Pelasgians (a more ancient Indo-European race akin to the Italian tribes),
and by their union formed the different dialects of Greek with which we are acquainted.
It is probable, but not so certain, that the language of the people from whom all these
Aryan tribes were derived, was Lithuanian in its oldest form.
A New Map of the Interior of the Northern Island of New Zealand, con-
structed during an Inland Journey in 1859. By Professor F. von Hocu-
sTETTER ( Vienna), Geologist of the Austrian Novara Expedition.
On the Antiquity of the Human Race. By Dr. J. Hunt.
On the Geographical Distribution and Trade in the Cinchona.
By V. Hurtavo.
The different species of the tree which yields the bark known in commerce as
Peruvian bark, and from which the sulphate of quinine is obtained, grow on the
slopes of the Andes, at a height which varies according to the latitude and the topo-
graphical situation of the mountains where this precious vegetable production has
been found. In New Grenada it grows on the central branch of the Cordillera,
which extends from the province of Paito, and separates the two valleys of the Cauca
and Magdalena, being most abundant in the districts of Pitay6 and Almaguer. It is
also found on the mountains above Finagamga, near Bogota. The Pitayo bark has
been the richest in quinine; and as in that locality the cuttings have been carried on
to the greatest extent, the article is nearly exhausted. The same may be said of the
Finagamga variety, which, although not so rich as the Pitay6, is prized on account
of its being of easier labour. The Almaguer bark, which at first was hardly saleable,
is now used to a great extent in Philadelphia and London, on account of the scarcity
of the two former species. The best bark is found on the Pitay6 mountain, at a
height of from 8000 to 11,000 feet above the level of thesea. ‘The tree grows among
the numerous species of Alpine vegetation which cover those mountains with thick
forests, either in clusters or scattered about. For that reason it varies in size. Like
all trees of a cold climate, it is of slow growth, and requires a great many years to
arrive at a good height. Some of them have been found so large as to yield forty
arrobas of green bark, which, when dried up, is reduced to about a third of its
weight. Others only produce about ten arrobas, As this tree is chiefly found in
TRANSACTIONS OF THE SECTIONS. 163
wild, cold, uninhabited mountains, constantly covered by clouds, there has been no
system in cutting, nor any study made to ascertain how long a spot should be left at
rest before undertaking new cuttings. It is known that the roots produce a great
many shoots after a tree is cut down, and that these require about fifty years to be-
come of a middling size. Young trees are also found growing from seeds, The
nature of the soil seems to determine the qualities of the alkalies contained in the
bark, quinine being most abundant in Pitayd, and cinchonine in Almaguer. But
rocky mountains and ravines are the spots where nature has placed this vegetable
species, The author is not aware that any bark trees have been found on the western
Cordillera, which separates the valley of Cauca from the Pacific coast, which ridge
never attains the elevation of perpetual snow in those latitudes. It only remains to
state, that the price of good sound Pitay6é bark, which had gone down in London to
1s. 8d. per pound, is now as high as 2s. 6d., and some very inferior lots have been
sold at 3s. The Almaguer sort, which was entirely neglected two years ago, is now
accepted by manufacturers at from 1s. to 1s. 4d, per pound. No mention is made
of the Bolivian bark, the most esteemed in commerce, as the author is not personally
acquainted with that trade.
On Alphabets, and especially the English ; and on a New Method of Mark-
ing the Sound of English Words, without change of Orthography. By the
Rev. Professor JARRETT, M.A.
On the Origin of the Arts, and the Influence of Race in their Development.
By R. Knox.
A brief Account of the Progress of the Works of the Isthmus of Suez Canal.
By D. A. Lance.
On the Jaczwings, a Population of the Thirteenth Century, on the Frontiers
of Prussia and Lithuania. By R. G. Laruam, M.D. F.R.S.
In the middle of the thirteenth century, the Jaczwings were a powerful nation,
between the Vistula, the Niemen, and the Upper Dnieper. At the present moment,
a small population, called by the neighbouring Lithuanians Jodwezhai, and distin-
guished by a dark complexion and certain peculiarities of dress and manners, is the
chief representative of the name. A few localities—(1) Jaévis Pol=Jaczving Land,
(2) Jatvis Stara= Old Jatvis, (3) Jatvis Nova=New Jatvis, (4) Mogilki-Jadzhvin-
gowski=Jacxving Graves, and (5, 6, 7) three villages named Jatvesk, complete the
fragments. The name, having come to us through Latin, Polish, German, Bohemian,
and Russian mediums, is hardly twice spelt alike, e. g. we have Jazuingi, Jasuingi,
Jacuingi, Jacwingi, Jaczwingi, Jatwingi in the German and Polish; Jatvyagi, Jatviazhi,
Jatviezie, &c., in the Russian. To these add Getwezeu, Getuinzete, and even Geta.
In speculating upon the ethnological affinities and the former extension of these
tribes, in the direction of both the Gothini and the Gothones of the classical writers,
this multiplicity of variations must be borne in mind. In respect to the immediate
affinities of the nation at the particular time under notice, the evidence is very decided
to their being members of the same family, and to their speaking the same language
with the Prussians (i.e. the occupants of East Prussia before the German Conquest),
the Lithuanians, the Samogitians, and the Letts. Their locality supports these
statements, as do the few words which have come to us from their language. Whe-
ther they were equally Lithuanic in blood, is another questiun. The few, but ia-
portant details of their history derive their interest (as do those of the Lithuanic
family altogether) from the peculiar character of the great religious contest which
they represent. With the Greek Christianity of Russia on the east, and the Papal
influences on the west, Lithuania and Finland were not only the last strongholds of
Paganism, but were acted upon as such in two directions. The resistance, however,
of the Lithuanians was most obstinate; and the most obstinate of the Lithuanians
were the Jaczwings. Their annihilation, too, was most complete. In 1264, a
great battle broke their power. In the fifteenth century not even the — of the
11
164 REPORT—1860.
Jaczwings remained. A more moderate notice simply says that the name of the Jacz-
wings was very rare and known to few. Conjointly with the special details of the
Jaczwings themselves, those of the populations with which they came in contact
should be studied—those of Russia and Poland, cut up into duchies; of Gallicia, a
powerful principality ; of Lithuania, a kingdom under Mindovy, vacillating both in
creed and politics; of North-Eastern Ger:nany under the Knights of the Teutonic
order; and, finally, of Volhynia occupied by Comanian Turks, and partly overrun by
Mongols. Details, however, of this kind are beyond the pale of the present notice,
which is chiefly made for the sake of drawing attention to the history of a nation—
the pre-eminently Pagan nation of Europe—once powerful, but now fragmentary,
the blood of which must still be found in more than one district where the language
is German, Lithuanic, Polish, or Russian.
On the latest Discoveries in South-Central Africa.
By Dr. D. LivincsTone.
The following letter from Dr. Livingstone was read to the Section :—
River Shiré, Nov. 4, 1859.
The River Shiré has its source in the green waters of the great Lake Nyassa (lat.
14° 23'S., long. 35° 30’ E.). It flows serenely on in a southerly direction, a fine
navigable stream, from 80 to 120 yards in breadth, expanding some 12 or 15 miles
from Nyassa into a beautiful lakelet, with a well-defined water horizon, and perhaps
5 or 6 miles wide; then narrowing again, it moves quietly on about 40 miles, till it
reaches Murchison’s Cataracts. After a turbulent course of 30 miles, it emerges
from the cataracts a peaceful river capable of carrying a large steamer through the
remaining 112 miles of its deep channel, and joins the Zambesi in iat. 17° 47'S.,
100 miles from the confluence of that river with the sea. The valley through which
the Shiré flows is from 10 to 12 miles broad at the southern extremity of Lake
Nyassa, but soon stretches out to 20 or 30 miles, and is bounded all the way on
both sides by ranges of hills, the eastern range being remarkably lofty. At Chihisas
(lat. 16° 2' 3S., 35° 1'E.), a few miles below the cataracts, the range of hills on the
left bank of the Shiré is not above 3 miles from the river, while the other range has
receded out of sight. If from Chihisas we proceed in a north-easterly path, a three
hours’ march places us on an elevation of upwards of 1000 feet. This is not far
from the level of the Upper Shiré valley (1200 feet), and appears to be its prolonga-
tion. Four hours’ additional travel, and we reach another plateau, 1000 feet higher,
and in a few hours more the highest plateau, 3000 feet above the level of the sea, is
attained, and we are on an extensive table-land, which, in these three distinct divi-
sions, extends to Zomba (lat. of southern end 15° 21’ S.). It is then broken; and ©
natives report that, north of Zomba, which is 20 miles in length from north to south,
there is but a narrow partition between Lakes Nyassa and Tamandua (Shirwa).
Three islands were visible on the west side of what we could see of Nyassa from its
southern end. The two ranges of hills stretch along its shores, and we could see
looming through the haze caused by burning grass all over the country the dim out-
lines of some lofty mountains behind the eastern hills. On the table-land are
numerous hills and some mountains, as Chicadgura, perhaps 5000 feet high, and
Zomba (which was ascended), from 7009 to 8000 feet in altitude. From this table-
land we can see, on the east of Lake Tamandua, the Milanje Mountains, apparently
higher than Zomba and Mount Clarendon, not unworthy of the noble name it bears.
All this region is remarkably well-watered; wonderfully numerous are the streams
and mountain rills of clear, cool, gushing water. Once we passed eight of them
and a strong spring in a single hour, and we were then at the end of the dry season.
Even Zomba has a river about 20 yards wide, flowing through a rich valley near its
summit. The hil! is well wooded also; trees, admirable for their height and the
amount of timber in them, abound along the banks of the streams. ‘Is this country
good for cattle?” the head man of the Makololo, whose business had been the
charge of cattle, was asked. “‘ Truly,” replied he ; “‘ don’t you see the abundance of
such and such grasses, which cattle love, and on which they grow fat?”” And yet
the people have only a few goats, and still fewer sheep. There are no wild animals
in the highlands, and but few birds; and with the exception of one place, where we
—
> tw
el PS? OL TS Oe ra
TRANSACTIONS OF THE SECTIONS. 165
saw some elephants, buffaloes, &c., there are none on the plains of the Upper Shiré,
but the birds, new and strange, are pretty numerous. In the upper part of the
Lower Shiré, in the highlands, and in the valley of the Upper Shiré, there is a
somewhat numerous population. The people generally live in villages and in hamlets
near them. Each village has its own chief, and the chiefs in a given territory have
a head chief, to whom they owe some sort of allegiance. The paramount chief of
one portion of the Upper Shiré is a woman, who lives two days’ journey from the
west side of the river, and possesses cattle. The chief has a good deal of authority ;
he can stop trade till he has sold his own things. One or two insisted on seeing
what their people got for the provisions sold to us. The women drop on their knees
when he passes them. Mongazi’s wife went down on her knees, when he handed
her our present to carry into the hut. One-evening a Makololo fired his musket
without leave, received a scolding, and had his powder taken from him. “If he
were my man,” said the chief, “I would fine him a fowl also.’’ The sites of their
villages are selected, for the most part, with judgment and good taste. Astream or
spring is near, and pleasant shade-trees grow in and around the place. Nearly
every village is surrounded by a thick high hedge of the poisonous Euphorbia.
During the greater part of the year the inhabitants could see an enemy through the
hedge, while he would find it a difficult matter to see them. By shooting their
already poisoned arrows through the tender branches, they get smeared with the
poisonous milky juice, and inflict most -painful if not fatal wounds. The constant
dripping of the juice from the bruised branches prevents the enemy from attempting
to force his way through the hedge, as it destroys the eyesight. The huts are larger,
stronger built, with higher and more graceful roofs than any we have seen on the
Zambesi. The Boabab (spreading place) is at one side of the village; the ground is
made smooth and level, and the banians, the favourite trees, throw a grateful shade
over it. Here the people meet to smoke tobacco and bang; to sing, dance, beat
drums, and drink beer. [In the Boabab of one small village we counted fourteen
drums of various sizes, all carefully arranged on dry grass.] Some useful work, too,
is performed in this place, as spinning, weaving, making baskets and fish-nets. On
entering a village, we proceeded at once to the Boabab, on which the Strangers’ hut
is built, and sat down. Large mats of split bamboo are politely brought to us to
recline on. Our guides tell some of the people who we are, how we have behaved
ourselves since they knew us, where we are going, and what our object is. This
word is carried to the chief. If a sensible man, he comes as soon as he hears of
our arrival; if timid or suspicious, he waits till he has thrown his dice, and given
his warriors, for whom he has sent in hot haste, time to assemble. When the chief
makes his appearance, his people begin to clap their hands, and continue clapping
until he sits down; then his councillors take their places beside him, with whom he
converses for a minute or so. Our guides sit down opposite them. A most novel
scene now transpires ; both parties, looking earnestly at each other, pronounce a word,
as ‘‘ Amhinatu” (our chief or father), then a clap of the hands from each one—
another word, two claps—a third word, three claps—and this time all touch the
ground with their closed hands. Next, all rise clapping—sit down again, and—clap,
clap, clap—allowing the sound gradually to dieaway. They keep time in this most
perfectly, the chief taking the lead. ‘The guides now tell the chief all they please,
and retire, clapping the hands gently, or with one hand on the breast; and his own
people do the same, when they pass the chief, in retiring. The customary presents
are exchanged, after a little conversation with the chief, and in a short time his
people bring provisions for sale. In some villages the people clapped with all their
might when they approved what the chief was saying to us. In others, the clapping
seems omitted in our case, though we could see it was kept with black strangers who
came into the village. The chief at the Lake, an old man, came to see us of his own
accord,—said he had heard that we had come, and sat down under a tree,—and he
came to invite us to take up our quarters with him. Many of the men are very
intelligent-looking, with high foreheads and well-shaped heads. ‘They show singular
taste in the astonishingly varied styles in which their hair is arranged. ‘Lheir
bead necklaces are really pretty specimens of work. Many have the upper and
middle as well as the lower part of the ear bored, and have from three to five rings
in each ear. The hole in the lobe of the ear is large enough to admit one’s finger,
166 REPORT—1860.
and some wear a piece of bamboo about an inch long init. Brass and iron bracelets,
elaborately figured, are seen; and some of the men sport from two to eight brass
rings on each finger, and even the thumbs are not spared. They wear copper, brass,
and iron rings on their legs and arms; many have their front teeth notched, and
some file them till they resemble the teeth of a saw. The upper lip ring of the
women gives them a revolting appearance; it is universally worn in the highlands.
A puncture is made high up in the lip, and it is gradually enlarged until the pelelé
can be inserted. Some are very large. One we measured caused the lip to project
two inches beyond the tip of the nose; when the lady smiled the contraction of the
muscles elevated it over the eyes. ‘‘ Why do the women wear these things?” the
venerable chief, Chinsurdi, was asked. Evidently surprised at such a stupid ques-
tion, he replied, ‘‘ For beauty! ‘They are the only beautiful things women have;
men have beards, women haye none. What kind of a person would she be without
the pelelé? She would not he a woman at all with a mouth like a man, but no
beard.”” One woman having a large tin pelelé with a bottom like a dish, refused to
sell it, because, she said, ker husband would beat her if she went home without it.
These rings are made of bamboo, of iron, or of tin. Their scanty clothing—the
prepared bark of trees, the skins of animals (chiefly goats), and a thick strong cotton
cloth—are all of native manufacture. They seem to be an industrious race. Iron
is dug out of the hills, and every village has one or two smelting houses; and from
their own native iron they make excellent hoes, axes, spears, knives, arrow-heads, &c,
They make, also, round baskets of various sizes, and earthen pots, which they orna-
ment with plumbago, said to be found in the Hill Country, though we could not
learn exactly where, nor in what quantities: the only specimen we obtained was not
pure, At every fishing village on the banks of the river Shiré men were busy spin-
ning buaze and making large fishing-nets from it; and from Chihisas to the Lake,
in every village almost, we saw men cleaning and spinning cotton, while others were
weaving it into strong cloth in looms of the simplest construction, all the processes
being excessively slow. This is a great cotton-growing country. The cotton is of
two kinds, ‘‘ Tonji manga,” or foreign cotton ; and ‘ Tonji cadji,”’ or native cotton.
The former is of good quality, with a staple from three-quarters to an inch in length.
It is perennial, requiring to be re-planted only once in three years, The native
cotton is planted every year in the highlands, is of short staple, and feels more like
wool than cotton. Every family appears to own a cotton patch, which is kept clear
of weeds and grass. We saw the foreign growing at the Lake and in yarious places
for 30 miles south of it, and about an equal number of miles below the cataracts on
the Lower Shiré. Although the native cotton requires to be planted annually in the
highlands, the people prefer it, because, they say, “‘it makes the stronger cloth.”
It was remarked to a number of intelligent natives near the Shiré lakelet, ‘‘ You
should plant plenty of cotton, and perhaps the English will come soon and buy it.”
** Surely the country is full of cotton,” said an elderly man, who was a trader and
travelled much. Our own observations convinced us of the truth of this statement.
Everywhere we saw it. Cotton patches of from 2 to 3 acres were seen abreast of
the cataracts during the first trip, when Lake Tamandua was discovered, though in
this journey, on a different route, none were observed of more than half an acre.
They usually contained about a quarter of an acre each. There are extensive tracts
on the level plains of both the Lower and Upper Shiré, where salt exudes from the
soil. Sea island cotton might grow well there, as on these the foreign cotton be-
comes longer in the staple. The cotton-growers here never have their crops cut off
by frosts. There are none. Both kinds of cotton require but little labour, none of
that severe and killing toil requisite in the United States, The people are great
cultivators of the soil, and it repays them well. All the inhabitants of a village,
men, women, and children, and dogs, turn out at times to labour in the fields. The
chief told us all his people were out hoeing, and we saw in other parts many busy
at work, Ifa new piece of ground is to be cultivated, the labourer grasps as much
of the tall dry grass as he conveniently can, ties it into a knot at the top, strikes his
hoe through the roots, detaching them from the ground with some earth still adhering,
which, with the knot, keeps the grass in a standing position. He proceeds in this
way over the field. When this work is finished, the field exhibits a harvest-like
appearance, being thickly dotted all over with these shocks, which are 3 feet high.
5 oe
TRANSACTIONS OF THE SECTIONS. 167
A short time before the rains several of these shocks are thrown together, the earth
scraped over them, and then the grass underneath is set on fire. The soil is thus
treated in a manner similar to that practised in modern times among ourselves on
some lands. When they wish to clear a piece of woodland, they proceed in precisely
the same way as the farmers in Canada and the Western States do,—cut the trees
down with their axes, and, leaving the stumps about 3 feet high standing, pile up the
logs and branches for burning. They grow lassaver in large quantities, preparing
ridges for it from 3 to 4 feet wide, and about a foot high. They also raise maize,
rice, two kinds of millet, beans, sugar-cane, sweet potatoes, yams, ground-nuts,
pumpkin, tobacco, and Indian hemp. Near Lake Nyassa we saw indigo 7 feet high.
Large quantities of beer are made, and they like it well. We found whole villages
on the spree, and saw the stupid type of drunkenness, the silly sort, the boisterous
talkative sort, and on cne occasion the almost up-to-the-fighting- point variety, when
a petty chief, with some of the people near, placed himself in front, exclaiming,
“TI stop this path; you must go back.’’ Had he not got out of the way with greater
speed than dignity, an incensed Makololo would have cured him of all desire to try
a similar exploit in future. It was remarked by the oldest traveller in the party
that he had not seen so much drunkenness during all the years he had spent in
Africa. The people, notwithstanding, attain to a great age. One is struck with the
large number of old grey-headed persons in the highlands. This seems to indicate
a healthy climate; for their long lives they are not in the least indebted to frequent
ablutions. ‘Why do you wash yourselves? our men never do,” said some women
at Chinsurdi to the Makololo. An old man told us he remembered having washed
himself once when a boy, but never repeated it; and from his appearance one could
hardly call the truth of his statement in question. A fellow who volunteered some
wild geographical information followed us about a dozen miles, and introduced us to
the chief Moena Moezi by saying, “‘ They have wandered ; they don’t know where
they are going.”” ‘‘Scold that man,” said a Makololo head to his factotum, wha
immediately commenced an extemporary scolding ; yet the singular geographer would
follow us, and we could not get quit of him till the Makololo threatened to take him
to the river and wash him. The castor-oil with which they lubricate themselves
and the dirt serve as additional clothing, and to wash themselves is like throwing
away the only upper garment they possess. They feel cold and uncomfortable after
awash. We observed several persons marked by the small-pox. On asking the
chief Mongazi—who was alittle tipsy, and disposed to be very gracious,-—if he knew
its origin, whether it had come to them from the sea, ‘‘ He did not know,”’ he said,
“but supposed it must have come to them from the English.”’ Like other Africans,
they are somewhat superstitious, A person accused of bewitching another and
causing his death, either volunteers or is compelled to drink the Maiori, or ordeal.
On our way to the lake a chief kindly led us past the next two villages, whose chiefs
had just been killed by drinking the Maiori. When a chief dies his people imagine
that they may plunder any stranger coming into their village. A chief, near Zomba,
at whose village we took breakfast on our way up, drank the Maiori before our
return, and vomiting, was therefore innocent. His people we found manifesting their
joy by singing, dancing, and beating drums. Even Chibisa, an intelligent and power-
ful chief, drank it once, and when insisting that all his numerous wars were just,
and that his enemies were always in the wrong, said to us, “‘ If you doubt my word,
I am ready to drink the Maiori.’”” On the evening of the day we reached Moena
Moezi, an alligator carried off his principal wife from the very spot where some of
us had washed but a few hours before. We learned on our return that he had sent
messengers to several villages, saying, “ He did not know whether we had put
medicine on the spot, but after we had been there his wife was carried off by an
alligator.’’ The first village refused to sell us food, would have nothing whatever
to do with us, and the chief of the next village, who happened to be reclining in the
Boabab, ran off, leaving his wooden pillow and mat behind. The women seldom
run away—baving more pluck perhaps than the men. When a person dies, the
Women commence the death-wail, and keep it up for two days, A few words are
chanted in a plaintive voice, ending by a prolonged note: a—a, or o—9, or ea, ea,
e—a. ‘The corpse is buried in the same hut in which he dies. It is then closed up
and allowed to fall into decay. We found one village in mourning, on the banks of
168 REPORT—1860.
the Upper Shiré. The chief’s father had died some time previous. They had not
washed themselves since, though washing is practised more or less on these plains;
and they would not wash until some friends at a distance, who possessed muskets,
had come and fired over the grave. The badge of mourning consists of narrow
strips of Palmyra leaf, tied round the head and arms, sometimes round head, neck,
breast, knees, ankles, arms, and wrists. They have the idea of a Supreme Being,
whom they name Pambé, and also of a future state. The chief Chinsurdi said they
all knew that they lived again after death. ‘‘ Sometimes the dead came back again,
—they appeared to them in dreams, but they never told them where they had gone
to.”’ This is an inviting field for benevolent enterprise. There are thousands needing
Christian instruction, and here are materials for lawful commerce, and a fine healthy
country, with none of the noxious insects with which Captains Burton and Speke
were tormented, and, with the single exception of 30 miles, water communication
all the way to England. Let but a market be opened for the purchase of their
cotton, and they can raise almost any amount of it, and the slave trade will speedily
be abolished.
On the Mountain Districts of China, and their Aboriginal Inhabitants.
By W. Locxuart.
Much of the empire of China with which we are best acquainted, consists of the
plains that lie near the mouths of the rivers, as they find their way to the sea-board,
and it is here that the important ports for our trade are situated. The interior of
the country is richly diversified ; the land rises considerably towards the hilly districts,
that slope from the chains of mountains that traverse all the western provinces and
spread themselves out through the central part of the country, being in fact the east-
ern spurs of the Kwan-lun and Himalaya ranges, that rise in Northern India to a
vast height, and gradually pass down through the north and south of Tibet towards
China. The Kwan-lun range passes into the northern and central provinces of
China, and the Himalaya into the southern and south-western provinces, while
the Tien-shan or Celestial Mountains and the Altai chain pass into Mongolia and
Mantchouria, commonly called Chinese Tartary.
In the mountainous regions of China the country is very beautiful, and combines
the varieties of scenery found in other similar districts ; many of these portions of the
empire are brought into communication with the sea coast, by means of the large
rivers that flow through all the rich and fertile central provinces, offering great
facility for the interchange of the various commodities of different parts of the em-
pire. These rivers form in fact the high roads of the country.
For purposes of communication in the mountain districts, and to facilitate the
transit of goods, many roads have been cut at great expense and with much labour
over the passes between the high ridges. The great road from Pekin to the south-
west through Shen-si to Sze-chuen, is by amountain route, whichrequired great ability
and skill to make passable; many years were spent in this work, and it is a monu-
ment of the patience and perseverance by which it was accomplished; by this road
merchants and officers constantly travel between the capital and the western frontier.
The road from Shan-si to Kan-suh is one of the most extensive works of the kind in
China. Besides these great trunk roads, there are several other mountain routes, by
which goods are carried from province to province across the mountains, one of
which may be mentioned, as the well-known Mei-ling pass between Kwang-tung
and Kiang-si; it is 24 miles long, and over it all the tea and silk that go to Canton
are carried on men’s shoulders. Much might be said regarding these mountain
roads of China, Lut it is impossible to enter on the subject here.
It is among these mountains and in the valleys they enclose, that many tribes of
people dwell who are probably the aborigines or natives of the land. The great
mass of the people who inhabit China are those who dwell in the cities and villages,
cultivating the land, following the pursuits of commerce, and acknowledging the
authority of one emperor; these may be considered to be the Chinese of the present
day; but in the islands of Formosa and Hainan, as well as in the western frontier,
dwell those native savage tribes, who acknowledge no submission to the Emperor of
China, dwell among their owr hills, and have ever maintained their independence.
SE ee
=
Ss va
Se PD ee TF Pe
“a
TRANSACTIONS OF THE SECTIONS. 169
The island of Formosa is divided from north to south by a chain of mountains
that cuts the island in two. On the western side live the Chinese, who passing
from the opposite coast of Fuh-kien, have gradually driven away the aborigines to the
eastern side ; some barter is kept up between these two parties, but they are generally
in a state of hostility, and constant vigilance is required on the part of the Chinese
to guard against the attacks of the natives, and this interferes very much with their
intercourse. The natives are governed by their own chiefs, who keep up a kind of
government. The occupations are tilling the ground, working in the mines in the
mountains, weaving coarse cloth, fishing, and washing the sand of certain districts
for gold.
The Aurelia Papyrifera, from the pith of which rice paper is made, grows in For-
mosa. These native tribes also inhabit the mountain districts of the island of Hai-
nan. The Chinese live on the eastern coast, where they have large fishing stations,
for the supply of Southern China with salt fish ; and the natives dwell by themselves
on the western side, and maintain their independence and separation from the in-
truders on their coast.
The mountainous regions of the Nan-ling and Mei-ling between Kwang-si and
Kwei- chau give lodgment to many clans of these aborigines, who are called Miau-
tsze, or “children of the soil,’’ which they no doubt are. It is singular that any of
these people should have maintained their independence so long and not been com-
pelled to submit to Chinese rule, surrounded as they are by the Chinese people.
This race presents so many physical points of difference to the Chinese, as to lead
me to infer that they are a more ancient people than the latter, and the aborigines
of Southern China. They are smaller in size and stature than the Chinese, have
shorter necks, and their features are more angular. The degree of civilization they
have obtained is much below that of the Chinese. It is not known what language
they speak, but the names given to the parts of the body and the common articles
about their boats, by some boatmen who visited Canton some years since, showed
that it was evidently not Chinese.
There are about forty tribes of these Miau-tsze scattered over the mountains of
Kwang-tung, Kwang si, Hu-nan, and Kwei-chau, speaking several dialects, and dif-
fering among theniselves in their customs, government, and dress. The Chinese
government keep troops at the foot of the mountains to restrain these tribes, who,
though often hostile, are on the whole inclined to live at peace, but resist every attempt
to penetrate into thcir fortresses. ‘The tribes are often at strife among themselves,
which becomes a source of safety to the Chinese, who are ill able to resist these hardy
mountaineers. It would appear that the race called the Chinese people, spreading
over the magnificent country they had found, drove back the Miau-tzse or ‘‘sons of
the soil,’ those on the coast taking refuge on the islands of Formosa and Hainan,
while those to the westward sought their homes among the mountains in their
neighbourhood ; and there they have remained a separate people, divided into various
tribes, ruled over by governors or chiefs of their own; the larger number of these
Miau-tsze have maintained their independence, but some have taken office in the
Imperial army, and have associated themselves with the Chinese. Various opinions
are entertained as to the religious doctrines of these Miau-tsze, who appear not to
be wholly idolaters; some of the tribes have a tradition of a Supreme God, who
created the world, but their knowledge is very indistinct and imperfect. The chief
source of information about these people is derived from a series of coloured draw-
ings ; one of the most perfect of such series that has been obtained was exhibited
in the Section; the drawings were evidently taken by some Chinese traveller who
visited the mountain tribes. Each drawing illustrates one of the tribes, and presents
a group of the people in sume characteristic occupation or amusement, and is accom-
panied by a short description of the tribe to which it refers.
These people are interesting from the fact that they must have a variety of ancient
customs among them, and also because they are the sons of freedom; and however
great may be the difference between us and them, they have a certain affinity with
us, and may some day bid us a hearty welcome to the Jand of their forefathers.
They are dispersed over the mountains cf Southern and Central China, and live in
a changeable state of relationship to the Chinese around them ; sometimes they fight
in open war, at others they rob and plunder, and sometimes they buy and sell.
170 REPORT—1860.
These Miau-tsze live to a great extent on the eastern slopes of the mountains,
whose western slopes, in South-Eastern Asia, are peopled by the numerous tribes of
Laos and Shans, and more particularly of the Karens, who are our tried and faithful
adherents in the territory of Burmah; and there are probably strong marks of simi-
larity of origin and identity of race between the Miau-tsze of China and the Karens
of Burmah and Pegu.
Journey in the Yoruba and Nupé Countries. By D. May, RN,
History of the Ante-Christian Settlement of the Jews in. China.
By Dr. Maccowan, U.S.
Critise in the Gulf of Pe-che-li and Leo-tung (China). By J. Mickie.
On the Formation of Oceanic Ice in the Arctic Regions.
By Captain Suerarp Ossory, #.N., F.R.G.S.
On the Course and Results of the British North American Exploring Expe-
dition, under his Command in the years 1857, 1858, 1859. By Captain J.
PALLISER.
The first part of this paper was occupied with a sketch of the course of the expedi-
tion, illustrated by a large map. — Starting from England in May 1857, the expedi-
tion reached Lake Superior by New York and the United States, from whence they
travelled in canoes to the Red River settlement, then with horses and carts across
the Plains to the north-west to Carlton, where the first winter was spent. During
that season Captain Palliser travelled back to the States on business, and Dr. Hector
reached as far west as the Rocky Mountains. In June 1858 the expedition resumed
its westward course, and in August reached the line of the Rocky Mountains. The
remaining two months before the winter set in was occupied in exploring the Moun-
tains, resulting in the discovery of four passes. ‘The second winter was spent at
Edmonton, where the expedition reassembled in October. Captain Blakiston returned
to England from this place. The winter of 1858-59 was spent in various explo-
rations into the Rocky Mountains with the purpose of learning their winter aspect,
The furthest of them reached almost to Mount Brown. In spring of 1859 M. Bourgeau
returned to England, his term of engagement having expired ; and the rest of the party,
accompanied by two English gentlemen, the late Captain Brisco and Mr. Mitchell,
proceeded through the Blackfoot country along the South Saskatchewan and bound-
ary line, till in August they again separated to explore the mountains; Captain
Palliser and Mr. Sullivan undertaking the west slope, and Dr. Hector to endeavour
to pass direct to the valley of Fraser River. The party again rejoined at Fort Colvile,
and from thence descended the Columbia river to the sea. A necessary delay at
Vancouver Island allowed of a visit to the coal mines at Nanaimo, and also to Fraser
River, after which the expedition returned to England by California, Panama, and
the West Indies, having been absent exactly three years.
The territory which has now been examined and mapped by this expedition ranges
from Lake Superior to the eastern shore of the lesser Okanagan Lake, and from the
boundary line to the watershed of the Arctic Ocean. This large belt of the continent
was explored in three seasons.
The first season was devoted to the examination of its south-eastern portion
between Lake Superior to the elbow of the south branch of the Saskatchewan, and
from the British boundary line or 49th parallel to Fort Carlton, in lat. 52° 52’ N.,
long. 106° 18’ W.
The second season was devoted to the examination of the territory between the
two Saskatchewans, to the exploration of the Rocky Mountains, and to the discoyery
of the passes available for horses in the British territory.
The third season commenced with a long journey from our winter quarters at Ed-
monton in lat. 53° 34’ N., long. 113° 20’ W., through the Blackfoot country to the
TRANSACTIONS OF THE SECTIONS. 171
most western point in the neighbourhood of the boundary line, previously reached
by the expedition from the eastward in 1857. A westward course was then resumed
along the country between the South Saskatchewan and the British boundary line,
thence once more across the Rocky Mountains. Finally, the connexion of a route
practicable for horses was effected the whole way from Red River settlement across
the continent to the Gulf of Georgia, entirely within British dominions.
This large belt of country embraces districts, some of which are valuable for the
purposes of the agriculturist, while others will for ever be comparatively useless,
The extent of surface drained by the Saskatchewan, and other tributaries to Lake
Winipeg, which we had an opportunity of examining, amounts in round numbers to
150,000 square miles. This region is bounded to the north by what is known as the
“ strong woods,” or the southern limit of the great circum-arctic zone of forest,
which occupies these latitudes in the northern hemisphere. This line, which is in-
dicated in the map, sweeps to the north-west from the shore of Lake Winipeg, and
reaches its most northernly limit about 54° 30’ N., and long. 109° W., from where
it again passes to south-west, meeting the Rocky Mountains in lat. 51° N., long,
115° W. Between this line of the “strong woods” and the northern limit of the
true prairie country there is a belt of land varying in width, which at one period
must have been covered by an extension of the northern forests, but which has been
gradually cleared by successive fires.
It is now a partially wooded country, abounding in lakes and rich natural pasturage,
in some parts rivalling the finest park scenery of our own country. Throughout
this region the climate seems to preserve the same character, although it passes
through very different latitudes, its form being doubtless determined by the curves
of the isothermal lines. Its superficial extent embraces about 65,000 square miles,
of which more than one-third may be considered as at once available for the pur-
poses of the agriculturist. Its elevation increases from 700 to 3500 feet as we ap-
proach the Rocky Mountains, consequently it is not equally adapted throughout to
the cultivation of any one crop; nevertheless at Fort Edmonton, which has an altitude
of 2000 feet, even wheat is sometimes cultivated with success.
The least valuable portion of the prairie country has an extent of about 80,000
square miles, and is that lyingvalong the South Saskatchewan, and southward from
thence to the boundary line, while its northern limit is known in the Indian languages
as ‘ the edge of the woods,” the original line of the woods before invaded by fire.
On tae western side of the Rocky Mountains, in the country which we examined,
there were but few spots at all fitted for the agriculturist, and these form isolated
patches in valleys separated by mountain ranges.
As the next result of our explorations, I shall briefly mention the different passes
through the Rocky Mountains which we explored, alluding to the chief advantages
and disadvantages of each.
The Kananaskis Pass and the British Kootanie Pass were examined by myself,
Of these I consider the Kananaskis Pass the preferable one, both on account of its
direct course through the mountains and its easier ascent.
The ascent to the height of land from the east is through a wide gently sloping
valley, and the immediate watershed is formed by a narrow ridge, which, if pierced by
a short tunnel, would reduce the summit level to about 4600 feet above the sea. The
descent to the west, into which Kananaskis Pass opens, is comparatively easy.
The British Kootanie Pass also opens out into the Kootanie River valley, but the
altitude here to be overcome is much greater, amounting to 6000 feet. ‘Chere are
likewise two ridges to be passed, which fact would form a very strong objection to
this pass.
The Vermilion Pass, which was traversed by Dr. Hector, presents on a whole the
greatest natural facilities for crossing the mountains without the aid of engineering
work, as the rise to the height of land is gradual from both sides, a feature which
seems to be peculiar tothis pass. It would thus be impossible to diminish its summit
level (which is less than 5000 feet), as is proposed in the case of Kananaskis Pass,
but on the other hand it would be the most suitable for the construction of an easy
waggon road.
This, like the other two passes I have mentioned, also strikes the Kootanie River
close to its source; but last summer Dr, Hector crossed the mountains by another
172 REPORT—1860.
pass from the head of the north branch of the Saskatchewan, directly to the Columbia
River, in the vicinity of the boat encampment.
Leaving this latter pass out of consideration for the present, as all of the others
open to the Kootanie River, it becomes necessary to consider the course by whch it
may be practicable to reach the coast of the Pacific without crossing to the south or
American side of the boundary line. It was with great difficulty for this purpose
even a partial examination of the country could be effected, owing to the rugged
valleys which intersect it in a direction parallel to the mountains, and which, though
not formidable themselves, are covered with such dense forest as to present obstacles
tothetraveller. Notwithstanding these difficulties, Mr. Sullivan succeeded in making
his way on the north side of the boundary line, and at the same time following a
system of transverse valleys, which might allow of the construction of a road with-
out much trouble from the mouth of Kananaskis Pass to the Columbia, above Fort
Colvile. From this point westward I myself ascertained that it would be possible
to reach the valley of the Okanagan, by which I believe the Americans have already
commenced to connect the waggon road of the Columbia with the upper country cf
the Frazer River. While pointing out the circumstances that seem to favour the
possibility of carrying a road.through British territory, from the Saskatchewan to
the Pacific, I wish to refrain from expressing any opinion as to the expediency of
undertaking at the present time a work which would involve a vast amount of labour
and a corresponding heavy expenditure. For how long a time in the year such a
road would remain open, is a question as yet unanswered, and which has a most
important bearing on the subject. In addition, the difficulty of direct communication
between Canada and the Saskatchewan country, as compared with the comparatively
easy route through the United States by St. Paul’s, renders it very unlikely that the
great work of constructing a road across the continent can be solely the result of
British enterprise.
Not the least important results of the expedition are the meteorological observa-
tions, which have been carefully conducted during the whole period of the explorations,
both in the winters and summers, whether we were stationary or travelling. I lay
stress upon this fact, as it affords materials for ascertaining the exact nature of the
climate, and means for a correct comparison between its nature and that of Canada.
The hourly magnetic observations were conducted by Lieutenant Blakiston, R.A.,
assisted by the other members of the expedition, during the winter of 1857-58.
These were not, however, carried on during the winter 1858-59, owing to the return
of Lieutenant Blakiston with the instruments; the magnetic declinations however were
attended to.
The astronomical observations and computations were placed in the hands of Mr. .
Sullivan, and the geographical position of the several salient points of the map are
determined principally by his lunars, the rates of chronometers being, of course, too .
unsteady to be depended on while travelling through so rough a country,
The large botanical collection of our botanist, M. Bourgeau, has already been sent
to Kew Gardens, where the specimens have been carefully arranged by himself under
the inspection of Dr. Hooker, who highly values them.
Dr. Hector’s specimens of fossils, &c. were from time to time transmitted to Sir
Roderick Murchison at the Jermyn Street Museum, but from the nature of the subject
much time must elapse before the results can be laid before Her Majesty’s Government.
In conclusion, I have great pleasure in bearing testimony to the unceasing zealand
energy of my companions, whose valuable assistance has been instrumentalin bringing
the expedition to so successful a termination, i
AppENDUM 1.—Remarks concerning the Climate of the Saskatchewan
District. By Dr. Hector.
The winter temperature is about 21° Fahr., ranging, however, in regular succes-
sions from high to low temperatures. In January 1858 it was as high as 40° above
zero for a few hours, accompanied by rain and high wind*. In that instance, how-
ever, between 4 p.m. and 9 P.M. it fell from +37° to —13,a difference of 50° in five
hours. The greatest depression of the thermometer in both years was about the 12th
* January 3rd, 1858, at Fort Edmonton.
TRANSACTIONS OF THE SECTIONS. 173
of February. Throughout the winter the snow falls in storms, which seldom last
more than two tothree days. The first fall generally occurs in the month of October,
but that always disappears again before the snows of November commence, which
are permanent for the winter. From the open country the snow evaporates very
rapidly, so that the prairies are never deeply covered ; but in the woods it accumulates
till spring. In some districts of the country more snow falls than in others; for
instance, at Fort Pitt, about 400 miles east of the mountains, there is generally 3 feet
to 4 feet of snow in spring, while close along the eastern base of the Rocky Mountains
it seldom exceeds 6 inches, and disappears very early. At Fort Edmonton the snow
always disappears fully a fortnight sooner than at Fort Pitt, although both places are
in the same latitude, but the former 3° further to the west.
The rivers generally freeze up about the 12th of November, and it is curious that the
Saskatchewan “ ¢akes,’’ as the local term has it, on the same day both at Edmonton
and Carlton, places distant from one another nearly 500 miles. In 1858 the ice
broke up on the 7th of April, but in 1859 not till the 26th of that month. But this
does not show the whole of the remarkable difference in those two seasons ; for in
the former the ice rotted away gradually, while in the latter it “‘gave”’ in a single
night from a sudden flood which followed the first warm weather.
A spring season hardly exists in the Saskatchewan, for in a few days everything
bursts into full verdure after the breaking up of winter. June is generally a wet
month; and much rain also falls during the first half of July, but atter that period
the summer is very dry. There is little or no thunder in the higher country, unlike
the Red River settlement, where for a certain season thunder-storms are of daily
occurrence.
The nature of the snow-line on the Rocky Mountains gives a clew to the climatal
arrangement of the country to the east. Although there are many of the mountains
in the eastern part of the range which exceed those to the west in altitude, only few
of their valleys are filled with glaciers. The great glaciers at the source of the north
branch of the Saskatchewan are fed from fields of ice and perpetual snow, that may
be considered as lying on the western slope of the range. The diminished altitude
of the snow-line towards the west is thus proved. The reasonis, that the prevailing
winds are from the west, and in rising to cross the mountains they are cooled, and
so deprived of their moisture, which ceases to be deposited after they pass over the
greatest altitude.
Concerning the Indians of the west side of the mountains, he stated that the tribes
are very numerous, and principally support themselves on fish. In most of the
tributaries of the Columbia the salmon swarm in such numbers as to taint the air at
a certain season of the year when their bodies are cast up on the banks. These fish-
eating Indians are of very low grade, as wherever Indians obtain their living easily
they invariably become debased. Thus the Indians to the east of the Rocky Moun-
tains, that dwell! in the strong woods, and live by the chase of animals, such as the
Moose-deer, which requires great skill and sagacity, are vastly superior to the Indians
of the plains, who, living on buffalo, with ease obtain abundance of food.
He adduced the case of the Sarcees, who belong to a tribe of M°Kenzie River
Indians, called the Chepeyans, who are perhaps the finest Indians on the continent ;
and yet these Sarcees, from havirg left their natural course of life some centuries
back, and taken to the plains, where they live among the Blackfoot tribes, have be-
come the worst Indians of the Saskatchewan. Their constitutions have become en-
feebled, as is shown by the prevalence of goitre among them, the whole tribe being
affected with this disease almost without exception, whereas it seldom or never occurs
among other Indians. The half-breeds who live in the Forts of the Upper Saskat-
chewan are very subject to goitre, the cause for which is very obscure.
ADDENDUM 2.—Remarks concerning the Tribes of Indians inhabiting the
Country examined by the Expedition. By Mr. Sutuivan.
Mr. S. pointed out that the northern portion was occupied by the Crees, which are
‘the most prominent tribe of the country, and best known to white men. The district
along the South Saskatchewan and towards the boundary line, he stated was inhabited
by a collection of allied tribes, all speaking nearly the same language, and known as
174 REPORT—1860.
the Blackfoot. This term comprises the Blackfoot proper, the Blood Indians,
Peagans, Gro Ventres, Sarcees, and several others. ‘The Sarcees, however, are really
very different Indians, and have their relations far to the north on M‘Kenzie River.
He next spoke concerning the languages of the tribes, of which he has prepared voca-
bularies, stating that that of the Crees is very perfect, having a very effective system
of grammar, which has been ably developed by the missionaries, who have also
invented a system of syllabic characters, by which the Indians soon learn to read
and write in their own language. These characters could also be applied to all the
other Indian languages he examined east of the mountains, excepting Sarcee, which is
too guttural.
He remarked that a very interesting, though small tribe, known as the Mountain
Stoneys, had been induced by the Wesleyan missionary to commence a little agricul-
ture. It does not amount to much, however, their principal crop being turnips,
which they generally pull and eat raw before they are nearly grown. Of the very
different habits of Indians which inhabit the woods from those of the plains, he men-
tioned in addition the curious circumstance, that in a camp of the former Indians
there is never any noise ; and even in conversation they talk almost at an inaudible
pitch, a habit derived from their stealthy habits in hunting; whereas a camp of Plain
Indians resembles a fair, as drums beating, whooping, and singing is continued all
day and all night.
On his proposed Journey from Khartum in Upper Egypt to meet Captain
Speke on or near the Lake Nyanza of Central Africa. By Consul
PETHERICK.
On the Formation of Icebergs and Ice Action, as observed in the Hudson's
Bay and Straits. By Dr. J. Rar.
The manner in which icebergs are generally formed is so well known that it would
be out of place to mention it here, but I have observed in Hudson’s Bay and Straits
these ice-islands formed in a mode different from that usually described.
Along these shores there are high and steep cliffs fronting the sca, and having deep
water at their base. Many of these cliffs face to the south-eastward. In the winter
falls of snow are frequent, and as almost every snow-storm is followed or accompanied
by a gale of northerly or north-westerly wind, the snow is blown over the cliff and
deposited in deep drifts at the cliff- foot on the ice, which is forced down by the weight.
As I have known a drift-bank of 20 or 30 feet formed by one gale of wind of as
many hours’ duration, it may be readily understood how in the course of a winter an
accumulation of snow to the depth of several hundred feet may be formed, extending
in a sloping direction to seaward thus :—
As soon as warm weather comes on in spring the surface snow is thawed; the
water percolates downwards until it reaches the snow, which is colder than the
freezing-point, and the whole is frozen into a solid mass of ice.
This process goes on to a greater or less extent according to the severity of the
season, the quantity of snow, and the amount of windy weather, until the snow-
formed ice attains great thickness and breaks off in large masses in the form of ice-
bergs.
In Hudson’s Bay the icebergs formed in this manner are small and scarcely de-
serving the name, but in the Straits they are large and lofty.
When passing through the Strait near to the north shore, J have seen some of
these lying close to the cliff from which they had become detached, and showing
projections and hollows corresponding to the form of the rocks from which they
had broken away.
I
:
TRANSACTIONS OF THE SECTIONS. 175
Whilst wintering at Repulse Bay on the Arctic circle in 1846-47 and 1853-54,
I had an opportunity of observing the manner in which boulders are taken up and
transported by ice.
In the early part of winter, when the sea-ice has attained considerable thickness,
it adheres at low water to any stones it may rest upon, and as the tide flows, raises
these from the ground. As the ice increases in thickness, these stones, some of them
3, 4, or 5 feet in diameter, are gradually imbedded in the ice, which attains a depth
of 8 feet or more.
In the spring the surface-ice wastes away by the combined action of thaw and
evaporation, whilst it is still acquiring fresh thickness underneath.
In the month of June, the boulders, which in the autumn were under the ice, now
appear on its surface, and may be floated off to great distances, when the ice is broken
up whilst still strong, by the action of winds and currents.
On the Aborigines of the Arctic and Sub-Arctie Regions of North America.
By Dr. Raz.
Remarks on some of the Races of India and High Asia (in connexion with
Casts exhibited). By Ropert von SCHLAGINTWEIT.
Mr. Robert de Schlagintweit gave a short sketch of the aboriginal tribes of Cen-
tral India, as also of the race inhabiting the country between the Karakorim and
Sayan Shan, which go by the name of the Turks. He also presented, in illustra-
tion of his remarks, some metal casts* of native faces taken from life. The tribes
composing the population of the mountain regions of Central India are the Kols,
the Gods, the Bils, and the Santals,
In physical conformation these people differ most distinctly from either Hindoos
or Mussulmans. In their religious observances also, and the habits of domestic life,
they have nothing in common with their neighbours. The language originally
spoken by them is now almost entirely lost, and it was only with great difficulty
that we could collect from old people any remains of their former idiom.
Though there exist many affinities amongst the four tribes above mentioned, yet
each preserves its peculiar and characteristic features. The complexion is remark-
ably dark, nearly approaching the colour of Negroes; the mouth is extremely large,
though the lips, which are scarcely ever parallel to each other, are not very fleshy ;
the nose is broad and flat, and the hair, which is generally shaved off or cut very
short, stands out stiff and straight. Though at first glance these tribes may show a
superficial resemblance to the African race, yet a closer examination will disclose
characteristic differences, especially with reference to the lower part of the head,
which is more prominent and considerably stronger with the Negroes. By some
ethnographers a remote affinity with Australian tribes has been pointed out; but
the likeness, on closer comparison, proves merely an apparent one.
The mountainous countries inhabited by the Kols, Bils, and Santals are, for the
greater part, covered with dense jungles, and at certain seasons of the year become
so unhealthy as to prove extremely dangerous for every one except the natives them-
selves,—a most remarkable instance of the fact, that some human tribes are capable
of living under conditions altogether fatal, or nearly so, to others.
Cultivation can only be carried on to a very limited extent; and the inhabitants
chiefly occupy themselves in cutting down trees, and in hunting the wild animals
with which their country abounds.
The clothing of this rude people is very scanty, consisting merely of a small piece
of unbleached cloth for the loins, and another piece of the same wound round the
temples, so as to leave a great part of the head exposed to the powerful rays of the
sun. They have no shoes, but sometimes wear a kind of sandal made of rough
wood, and shaped to the foot, with another small round covering of wood at its
upper end, to afford a hold for the toes.
Their sole weapons are axes, in the use of which they display considerable experts
* These casts are a selection from Messrs. de Schlagintweit’s collection of 275 heads,
published (1859) by T. A. Barkt at Leipzig.
176 REPORT—1860.
ness. For dwellings, they erect for themselves miserable huts constructed of bam-
boo and the leaves of various trees.
The contempt with which they are universally treated by their neighbours, the
Hindoos, has rendered them extremely shy and suspicious ; whenever I approached
one of their villages, they invariably left their huts and tried to conceal themselves
in the dense jungles of the neighbourhood. Though I had the necessary supply of
guides with me, yet their services in this respect were indispensable on many occa-
sions.
M. de Schlagintweit passed on to the Turks, a people particularly recommending
themselves to his notice, as presenting marked differences from all the tribes he had
had occasion to observe.
This remarkable race inhabits those parts of Central Asia which to the north of
Tibet are interposed between the Komakorinn, the Sayan Shan, and considerably to
the east of it. In many respects they show points of resemblance to the Mongols,
but nevertheless form a separate and distinct tribe, and may be considered as the
original stock from which the Turks in Europe have sprung. Even at the present
day the true Tarkish language holds its ground amongst them ; and though, on com-
parison with the kindred idiom used by the European Turks, there are many dialectic
deviations to be observed, yet it is evident that the Turks in Central Asia have pre-
served the purity of the original tongue, whilst the related race in Europe have
modified it with a considerable ailmixture of Persian and Arabic words.
Like their European brethren, the Asiatic Turks are fanatic Mussulmans, honest,
active, and hospitable, and far more civilized than their neighbours the Tibetans.
Their manners are characterized by the strictest observance of punctilious etiquette,
some of the ceremonies being so complicated as to raise up an almost impassable
barrier for all strangers.
The native dress is rather handsome and rich, varying according to the seasons.
For winter, or when travelling over the mountains, the Turk wears a Jong fur coat,
woollen trowsers, and a round fur cap. The stockings are of felt, and so long that
they can be drawn over the trowsers, when they are fastened by an ornamental
ribbon above the knee. So far, the dress, which we had to assume ourselves when
disguised, is very convenient; but the shoes are so thin as to offer but a slight
protection to the feet. The summer costume consists also of a coat and trowsers, a
light cap for the head, and boots reaching up to the knee worn without any stock-
ings.
Yarkand, their chief place, as also Kashgar, is one of the most important and
flourishing places of Central Asia. ‘The population is in general a wealthy one, and
live in good solid houses.
The inhabitants of the mountainous parts are mostly shepherds; the principal
occupation of those in the plains is trade, which they carry on with horses and
Bactrian camels along routes apparently impracticable for loaded animals. The
merchants travel as far south as Ladak and Pesham, and to the north find their way
to the shores of the Issikul lake. On the west they penetrate beyond the Russian
frontier ; but towards the east commercial intercourse is restricted by the large
desert, stretching along the eastern part of the Kuenluen.
It may here be mentioned, that the caravan route from Yarkand to Ladak leads
for more than fourteen days’ march over uninhabited mountain country, at an eleva-
tion of from 14,000 to 16,000 feet. Passes above 18,0U0 feet in height occur; and
the whole district is so bare and sterile, possessing so little vegetation, that the
traders are obliged to carry with them even the food for their animals.
By far the greater part of the trade between India and High Asia, including the
adjoining parts of Russia, is carried on by the Turks.
In conclusion we may remark that, besides our special geographical observations,
we had occasion to collect various specimens of manufacture, mostly from Turkish
and Tibeto-Indian parts; and we consider ourselves fortunate in being able to add
more than 207 specimens to the splendid general collection now accumulated, under
the energetic direction of Dr. Forbes Watson, within the walls of the India House
Museum.
er aS -..-~-~-~
.
TRANSACTIONS OF THE SECTIONS. 177
On the Tribes composing the Population of Morocco.
By Lieutenant Epvwarp ScuLaGintweIr.
This paper was read by Mr. Hermann Schlagintweit, who stated that his brother
Edward, First Lieutenant in the Bavarian Army, had joined the Spanish forces
during their iate campaign in Morocco. Subsequently he had made a second visit
to Morocco in furtherance of certain scientific purposes of his own, when he received
the most valuable assistance from the well-known British Resident in that country,
Mr. James Drummond Hay*.
The principal population of Morocco, the Moors, are a mixed race, deriving their
origin partly from the Berbers and partly from the Arabs. They form the most
numerous section of the inhabitants of the towns. Their complexion is compara-
tively fair, not unlike that of the inhabitants of Southern Europe, while the colour
of their hair is various, comprising both light and dark shades; the form of the face,
as well as of the figure in general, betrays a tendency to stoutness. With regard to
character, but little can be said in the way of praise. Like most Orientals, the
Moors are false and covetous, grovelling in the lowest servility before their superiors,
and full of arrogance and cruelty to those below them. This race took very little
part in the late war, while the following ones showed themselves as possessing much
greater energy, and capable, under proper guidance, of quitting themselves well in
active service.
The various tribes of the Berbers or Brabers must be considered as the original
inhabitants of this district. They were found already in possession of the country
on the arrival of the Romans, as appears from the geographical terminology used by
the latter in reference to these parts. The interesting work of “Al Hasem” of
Granada—better known under his name, when a Christian, of ‘‘ Leo Africanus,’”’—
shows, moreover, that during their conquests in North-western Africa (650-700
A.D.) the Arabs were frequentiy engaged in conflict with these primitive tribes.
Like the Fellahs in Egypt who have succeeded in preserving the ethnographical
type of the ancient inhabitants, so here also it occurs that, in spite of the many
changes in the dynasties of the country, the pure type of the Berbers is still repre-
sented by a considerable proportion of the population. They chiefly inhabit Mount
Atlas and its spurs, but have also extended themselves as far as Fez, Mekinéz, and
the towns along the sea-coast. ‘
In Morocco two principal tribes of the Berbers can be distinguished: the
Shlockhs, who are settled in villages and towns; and the Amazirgens, forming a
migratory and unsettled population.
The Kbilas (Kabiles) and the Shayvas in Algiers must also be considered as be=
longing to the Berber race. [n person they are thin, but sinewy; their hair brown,
occasionally reddish, and with those from the southern provinces rather dark.
Though in general character not unlike the Moors, they are a much more active
people, are good cultivators of the soil, and make hardy soldiers. One tribe in par-
ticular of the Berbers, the Hudnyas, have played an influential part at various
times in the military history of Morocco. Like the Ianichars, they formed a strong
and formidable guard, though often in opposition to the government; but were at
last disbanded and scattered throughout various cantonments of the country.
The Riffers inhabit the mountain ranges along the Mediterranean, which begin
at Tetuan and reach to Cape “Tres Forcas.’’ Confined as they are to their almost
inaccessible mountains, they form a distinct and well-marked race, their language
even differing considerably from the Arabic. There are six principal tribes into
which they are divided,—the Ghoniaras, Aksenayas, Bukone’a, Tems’manes, Gvelayas,
and Kebdanas. They are almost entirely independent of the Emperor of Morocco,
the small yearly tribute paid to him being offered rather to the head of their church
than to their Emperor. The greater part of them are robbers and pirates ; and, in-
deed, in the late war, when posted in the town of Tetuan for its defence, they
exercised their native calling with a zeal and cruelty which considerably accelerated
the surrender of the place.
The Sis race. These tribes approach the Negro type in respect of complexion
* During his stay in the country Mr. Edward Schlagintweit took many facial and cranial
_ casts, besides making numerous detailed measurements.
1860. 12
178 REPORT—1860.
and general proportions, but their character is better than that of the preceding
races. They are very active both in trade and agriculture, and evince great dexterity
in the manufacture and use of arms. Their dependence upon the Emperor is of the
same nature as that of the Riffers.
Geography of the North Atlantic Telegraph.
By Colonel Ta. P. SHAFFNER, of the United States.
The Route—Lands and Seas.—The route of the telegraph is from Scotland vid
Farée Isles, Iceland, Greenland, and Labrador, to Quebec, there connecting with
other lines to different parts of America.
The sea sections of the proposed telegraphic route are as well known to nautical
geographers, excepting, perhaps, the places sounded by the Telegraphic Expedition
last autumn (1859) between Labrador and Greenland, and between Greenland and
Iceland. The bottoms of those seas were found to be deep mud, and acable once laid
thereon will lie undisturbed for all time. Icebergs float, and there is no part of the
sea in which the cables will be laid where the bergs will reach the bottom. Arcfic
navigators, with whom the author has had the pleasure of conversing since his arrival
from the voyage of last autumn, agree that if the cable can be carried into deep
fiords on the respective coasts, there will be no danger of interruptions from icebergs.
The author has seen such fiords on the coasts of Labrador and Greenland, and
therefore regards the problem as solved.
The land sections are not of serious importance. A telegraph line can be con-
structed on land wherever the foot of man can be placed. Lines have been built
over hills and valleys where neither waggon nor beast could go, and these regions
were in the great Mississippi valley, a country having great variety of soil, surface,
and climate.
Farée Isles.—The cable wiil be landed at Thorshaven, the capital of the Farde
group, and from thence a few miles by land to Westerman’s haven. ‘The island is
hilly, the roads inferior; there is but little cultivation; pasturage good ; the people
intellectual; religion Lutheran ; it sends one member to the Danish Parliament; it
has a governor, sheriffs, and other officers of state: the climate is about the same as
Copenhagen, more mild than Stockholm, Quebec, Montreal, or Boston.
Icelund will be traversed by the line from Berufiord or Portland to Reikiavik.
The people are highly educated, and a considerable trade is carried on between them
and the Europeans. The French have some 120 vessels fishing on the south coast.
They have free trade with foreign countries, and all the fisheries are free. The in-
habitants are industrious and religious, and have their own local Parliament. The
country is partially cultivated, but much of the island is covered with lava. The
climate is moderate ; the ice never interrupting navigation on the south and west
coasts. There will be no difficulty whatever in running the telegraph across Iceland.
Labrador.—The cable will be landed in Hamilton Inlet, lat. 54°30’ N. The
line will then be run either to the Gulf or to the River St. Lawrence. This country
is rolling or hilly, and covered with timber, principally pine, spruce, and juniper.
The trees are large, many being 15 or 20 inches in diameter at the base. ‘There is
much grass where the country is open. Turnips,- potatoes, and other vegetables are
cultivated to a limited extent. The inhabitants are mostly Esquimaux. They are
civilized, under the teachings of the Moravian missionaries. ‘There is a station of
the Hudson’s Bay Company on Hamilton Inlet, about 50 miles from the sea, The
coast is hilly and barren. Fishermen from Newfoundland are scattered along the
coast, and many are employed in Hamilton Inlet. The cod and herring fisheries
are the most profitable. The country is not much settled. There will be difficulties
to be met in the construction of the line, and maintaining it across Labrador; but
these difficulties will not be so great as those which have been overcome in other
countries; for example, in Newfoundland, and the Southern and Western States of
America. The line across Newfoundland traverses marshy and uninhabited regions,
wholly unknown to the world until a few years ago, when it was explored for the —
telegraph.
Greenland.—The section of the route the least known is Greenland; and
-although that part of the country proposed to be traversed is not so cold as the
climate of St, Petersburgh, a city of some 700,000 inhabitants, yet-there prevails
TRANSACTIONS OF THE SECTIONS. 179
the most erroneous impressions in regard to the temperature of that interesting and
wonderful country. Whether it is a continent, or numerous islands extending to the
North Pole, is a problem yet to be solved. In the southern portion we find green
valleys, covered with grass and vegetation, surrounded with mountains towering into
the heavens ; and these in the morning are covered with white glittering snow, which
with the mid-day sun disappears, leaving exposed their blackened minarets and spires.
The scenery is grand and picturesque.
The coasts of Greenland are barren hills and mountains. Along the shore are
many islands. The fiords penetrate to the interior 10, 20, or 30 miles. Some of
these bring out ice, others do not. Into one of the fiords which are free of ice will
be carried the telegraph cable, as indicated inthe map. The water is very deep, and
no iceberg can reach the bottom, or go far up their meanderings to their heads.
They do not freeze, except in narrow places, where there is still water. A cable can
be easily laid from the sea into one of these fiords, and when brought to land it can
be well secured against native ice, as is the case at many places in America, and on
the belts and sound of the Baltic Sea.
The exact locality where the line is to cross Greenland has not been determined,
but it will be in the southern portion, not 60 miles north of Cape Farewell. The
particular kind of surface to be traversed—whether green valleys, or mountain ranges
—is not fully known, but in either case no insuperable difficulties can be foreseen.
What it is in the interior, or whether there be ice there or not, no one knows.
Col. S. found alluvial soil on the ice several miles distant from the sea, and it may
have been blown there from the interior. Some 12,000 deer are killed in the Holsten-
berg district every year. They disappear in winter, Whither do they go?
The ice travelled over by Colonel Shaffner was solid freshwater ice. The snow
falls in small quantities. On the plateau some considerable collections of water were
seen. There were many deep crevices. The thickness of the ice no one has been
able to determine. The author does not believe it entirely rests upon the earth, but
_ it forms bridges, and perhaps where he went it was 4000 feet above the level of the
sea; or perhaps there was a cavern beneath, 1000 feet between the ice and the earth,
exceeding in grandeur the great Mammoth Cave of America, with its 200 subterranean
avenues. This may seem most wonderful, but he had many reasons for believing
_ that it was possible. He had been in some of the caverns, and heard a waterfalt
resembling the rushing of a river over rocks. The bergs from the fiord blinks, he
noticed were clear and clean ice; no gravel or earth either in or on them, excepting
those that were near the shore. If the ice were upon the earth in the interior, we
might expect to find some earth in the bergs. He has seen boulders on bergs, but
they came from the glaciers of the north, or from the sides of the blinks crushing”
against the mountains as the ice moved from the interior. The inhabitants are Danes
and Esquimaux. The Julianahaab District is the most southern in Greenland, and
has about 2600 Esquimaux. They are all civilized, and mostly members of the
Lutheran Church. There are afew Moravians. The children are baptized, and at
fourteen years old confirmed. They have churches and schools, and they preach,
sing, and pray. In the principal churches they have organs and some fine paintings.
The town of Julianahaab has about 300 inhabitants. The people received the
yisit of the party last autumn with much joy. The houses were stone and frame,
and covered with slate. It is not cold enough for double windows. They had cows
and sheep. The Esquimaux lived in stone huts covered with earth, fully as com-
fortable as many log cabins that Colonel Shaffner has lived in when in the western
forests of America.
_ The Esquimaux are honest and good-hearted. They never steal unless on the
verge of starvation. The men treat their wives well. The children are never
whipped. Peace, love, and domestic happiness seem to be more common to them
than to the more civilized races. It will not be difficult to have a telegraph line
Maintained in Greenland, with the aid of such people; and, in fact, a telegraph
line can be constructed across the hills, the valleys, and the fiords of Greenland, and
_ it can be maintained thereafter with much more facility and certainty than has been
done across the plains of Russia, the mountains of Norway, the swamps of New-
foundland, the inundated lands of the Mississippi, the uninhabited forests of America,
or the Alpine ranges of Europe.
19*-
180 REPORT—1860.
On the Lost Polar Expedition and Possible Recovery of its Scientific
Documents. By Captain PARKER Snow.
Captain Parker Snow, in addressing the audience upon the subject of his paper,
stated that the great object he had in view was to keep before the public the fact
that we had not yet done all that might be done as regarded the lost polar expedi-
tion. Thuse who went out in that expedition ought, none of them, ever to be for-
gotten ; and it was our duty to persevere in ascertaining their real fate until posi-
tive evidence came forward concerning it. This evidence, he asserted, had not yet
been found; and he was prepared to show that more could be obtained if right mea-
sures were taken.
He then commenced his arguments by giving an analysis of Franklin’s instruc-
tions, and pointed out how certainly numerous scientific observations of great value
must have been made by the officers in that expedition. He enumerated the differ-
ent searching expeditions, and with much pleasure dwelt upon the exertions made
by the several leaders and subordinates engaged upon this work, many of whom he
named. He next pointed out Dr. Rae’s discuveries, and then those of the ‘ Fox’
under the present Sir Leopold M‘Clintock, doing full justice to one and all. After
this, he dissected the whole information that had been obtained by making the fol-
lowing remarks :—
« First of all,’’ said he, ‘‘ what do we know for a certainty concerning the lost
expedition? Why this: 105 persons landed at Point Victory in April 1848, and
Captain Crozier (one of their chiefs) said that he or they, or some of them, were going
to start on the 26th for Back’s Fish River. They do not say a word about being in
want of assistance, nor yet that they are suffering. They have abandoned their
ships and are going southward, even as Captain M‘Clure had intended to do with a
part of his crew.
“This is all we positively know from any written evidence. What else we know
is from other testimony. It is as follows :—Three skeletons—perhaps belonging to
the 105, perhaps not—have been found; also a boat. Forty of our countrymen
were seen by the natives in the spring of 1850 walking to the Fish River, where,
later in the year, it is said that some of them died. ‘Traces of others have been
found part of the way up the Fish River, and along the Boothian Isthmus, the coasts
of Boothia, and King William Island. Rumours of white men, going westward
along the coast of America, have been heard for several years past. To Cape War-
ren, the Peel River, the Fish River, and, about the Melville Peninsula, strange tales
attach great interest. These places have yet to be searched, and the mystery con-
nected with them examined.
“‘Such.is what we know. Now what is it we suppose? Briefly this:—From
April 1848 to the spring of 1850 is two years. Clearly the party must have been
wandering about during that interval. What so likely as that, in the summer of
1848, they found open water for their boats, and went away to the westward (or at
all events one party did), and tried to reach the Mackenzie or Peel River. Some may
have perished, some have gone another way than by the coast (possibly by a direct
channel yet undiscovered by us), and finally, being unsuccessful in their western
route, they return to the eastward for Fish River, and perhaps a few of them to-
wards Lancaster Sound, or the channels leading into Baffin Bay; in fact, to any
place, where a hope of relief, and where good hunting would be presented.
“This hypothesis would explain away the lapse of time, and account for only
forty being seen by the natives in 1850. It is further strengthened by other circum-
stances founded on negative facts.
“They did not take away any of the Fury Beach stores, though well known to
them as existing at only about 200 miles’ distance: they did not send information
of distress through the Esquimaux or Indians, as we now know could have been done,
even as Captain Collinson and Captain Maguire sent notices of relief: they did not
say a word about being starving or in want of immediate aid; and many other
things they did not do, which we should expect would have been done, in case of
great distress. Hence we may infer that in April 1848 they were not so badly off
as is supposed. Had they been so, why did they not visit the Fury Beach stores
and get relief? Those stores are even now in excellent order, as may be known from
Captain M‘Clintock’s published Journal. Yet we find them unused, at all events
TRANSACTIONS OF THE SECTIONS. 181
for any large supply, though it is possible they may have been visited by a few of
the lost party.
«Remarks have been made about the Franklin Expedition suffering from Goldner’s
provisions. But, independent of all other argument on this point, there is one fact to
be got over, before we can agree to such an idea ;—the ships wintered at the threshold
of their explorations, yet afterwards went onward into unknown regions instead of
returning, as wisdom would have dictated, on finding their stores defective!
“« Another fact to be well considered is, that close attention to all the information
obtained from the natives, leads to a belief that the actual ground where the whole
truth could be known has not yet beenexamined. The natives told Captain M‘Clin-
tock that the white people had gone to a place where there was plenty of salmon.
Now we know the lakes of South Boothia abound in salmon.
“* Again, the Esquimaux referred to parts known by certain names ; as, for instance,
Amitoke, Neitchillee, and Akkollee. ‘These parts, however, were not visited by our
late explorers, perhaps from not knowing where they were. But a careful reading
of the various Arctic Voyages of Parry, Ross, Simpson, and Back, would have
shown that the places named, all exist about the Boothian Isthmus southward; and
it is there, and in adjoining localities, we find all the plate and other articles in pos-
session of the natives.
“More argument could be brought forward; but it is enough to call attention to
one other important fact, viz. that Ross and his small crew, after being frozen in
for three years, managed to escape from a position almost identical with that of
Franklin’s ships, and then get home by way of Lancaster Sound.
“That we have no traces of the Franklin crews attempting the same thing is very
singular. We must therefore infer either that they were not in absolute distress,
or else that one party did visit Fury Beach without being able to leave a notice. Be
it as it may, assuredly the Expedition would never have abandoned their journals
and other documents, without first placing them in some sort of security. When
Ross escaped he carried even minerals with him! These with other things he had to
abandon ; but he deposited them in a secure place, and they were afterwards brought
home to England in a whaling ship sent expressly to the locality for them. Can we
suppose that the officers and crew of a national expedition like Franklin’s—and withal
a scientific one—would not take equal care to preserve the records of their labours ?
The question needs no answer. There can be little doubt about it in the minds of all
impartial persons; and it only requires a good summer search to know the truth.”
Captain Snow then brought forward evidence to show that life could be prolonged
in the arctic regions, and that the place was not so destitute as generally supposed.
Sir R. Murchison himself had given good reasons in support of this view; and
Lord Wrottesley, Baron von Humboldt, Sir Francis Beaufort and others had ex-
pressed something similar. The burial of the dead, too, was another thing not to be
forgotten. Three sailors were buried suitably on shore, therefore it is almost certain
Sir John Franklin would have been interred in like manner; and as the Esquimaux
are very. superstitious concerning the dead, it is possible important records can be
found near the locality where the illustrious chief is known to have died.
Other arguments were brought forward by Captain Snow, who stated that he had
a committee formed of well-known names to aid him in a renewed search he was
prepared to make in a small vessel of from 75 to 100 tons if sufficient means could
be raised. A brave American (Mr. Hall) was already on his way there to try and do
the work ; and it was for our credit and honour that another attempt should be made
by our own flag to complete that which comparatively could now be easily done.
On the Proposed Communication between the Atlantic and Pacific, via
British North America. By Captain M. H. Synce, R.E.
On the Geographical Distribution of Plants in Asia Minor.
By PuerrE DE TCHIHATCHEF,
On the Excavations on the Site of the Roman City of Uriconium at Wroxeter.
: By Tuomas Wricut, F.S.A.
182 REPORT—1860,
STATISTICAL SCIENCE.
Opening Address by Nassau W. Senior, M.A., President of the Section.
In 1856 the General Committee of the British Association decided that the Section
over which I have the honour to preside should be entitled “The Section of Econo-
mic Science and Statistics.”
I have looked through the papers which since that time have been commu-
nicated to us, and I have been struck by the unscientific character of many of them.
I use that word not dyslogistically but merely distinctivingly, merely as ex-
pressing that the writers had wandered from the domain of science into that of art.
* I need scarcely remind you that a Science is a statement of existing facts, an
Art a statement of the means by which future facts may be brought about or in-
fluenced. A Science deals in premises, an Art in conclusions. A Science aims
only at supplying materials for the memory and the judgment. It does not pre-
suppose ash purpose beyond the acquisition of knowledge. An Art is intended to
influence the will: it presupposes some object to be attained, and it points out
the easiest, the safest, or the most effectual conduct for that purpose.
The subjects to which the British Association has directed our attention are
Economic Science, and Statistics.
Economic Science, or, to use a more familiar name, “The Science of Political
Economy,” may be defined as “ The Science which states the laws regulating the:
production and distribution of wealth, so far as they depend on the action of the
uman mind.”
I say, “so far as they depend on the action of the human mind,” in order to
mark to which of the two great genera of sciences, the Material, or, as they are
usually called, the Physical, and the Mental, or, as they are frequently called, the
Moral, sciences, Political Economy belongs.
Unquestionably the political economist has much to do with matter. The
phenomena attending the production of material wealth occupy a great part of his
attention; and these depend mainly on the laws of matter. The efficacy of ma-
chinery, the diminishing productiveness, under certain circumstances, of successive
applications of capital to land, and the fecundity and longevity of the human
species, are all important premises in political economy, and are all laws of matter.
But the political economist dwells on them only with reference to the mental
phenomena which they serve to explain; he considers them as among the motives
to the accumulation of capital, as among the sources of rent, as among the regulators
of profit, and as among the causes which promote or retard the pressure of popula-
tion on subsistence.
If the main subject of his studies were the physical phenomena attending the
production of wealth, a system of political economy must contain a treatise on me-
chanics, on navigation, on agriculture, on chemistry—in fact, on the subjects of
almost all the physical sciences and arts, for there are few of those arts or sciences
which are not subservient to wealth. All these details, however, the political
economist avoids, or uses a few of them sparingly for the purpose of illustration.
He does not attempt to state the mechanical and chemical Jaws which enable the
steam-engine to perform its miracles—he passes them by as laws of matter; but
he explains, as fully as his knowledge will allow, the motives which induce the
mechanist to erect the steam-engine, and the labourer to work it. And these are
laws of mind. He leayes to the geologist to explain the laws of matter which
occasion the formation of coal, to the chemist to distinguish its component elements,
to the engineer to state the means by which it is extracted, and to the teachers of
many hundred different arts to point out the uses to which it may be applied.
What he reserves to himselfis, to explain the laws of mind under which the owner
of the soil allows his pastures to be laid waste, and the minerals which they cover
to be abstracted ; under which the capitalist employs, in sinking shafts and piercing
galleries, funds which might be devoted to his own immediate enjoyment ; under
which the miner encounters the toils and the dangers of his hazardous and laborious’
occupation; and the laws, also laws of mind, which decide in what proportions the
+4 tein) eed se
ae
—— eo
ere) Oe ee
TRANSACTIONS OF THE SECTIONS. 183
produce, or the value of the produce, is divided between the three classes by whose
concurrence it has been obtained.
When he uses as his premises, as he often must do, facts supplied by physical
science, he does not attempt to account for them ; he is satisfied with stating their
existence. If he has to prove it, he looks for his proofs, so far as he can, in the
human mind, Thus the economist need not explain why it is that labour cannot
be applied to a given extent of land to an indefinite amount with a proportionate
return. He has done enough when he has proved that such is the fact; and he proves
this by showing, on the principles of human nature, that, if it were otherwise, no
land except that which is most fertile, and best situated, would be cultivated. All
the technical terms, therefore, of political economy, represent either purely mental
ideas, such as demand, utility, value, and abstinence, or objects which, though some
of them may be material, are considered by the political economist so far only as
they are the results or the causes of certain affections of the human mind, such as
wealth, capital, rent, wages, and profits.
The subject matter of political economy is, I repeat, wealth. The political
economist, as such, has nothing to do with any of the other physical or moral.
sciences, or with any of the physical or moral arts, excepting so far as they affect the
production or distribution of wealth. Whether wealth be a good or an evil, whe-
ther it be conducive to human morality or to human happiness, that it be hoarded
or that it be consumed, that it be accumulated in masses, or that it be generally
diffused, are questions beyond his science. His business is to state what are the
effects on the production and distribution of wealth, or, to use a shorter expression,
the economic effects, of accumulation and of expenditure, of the different kinds of con-
sumption, and of the aggregation in a few hands, or the division among many, of the
things of which wealth consists. Whenever he gives a precept, whenever he ad-
vises his reader to do any thing, or to abstain from doing anything, he wanders
from science into art, generally into the art of morality, or the art of government.
The science of statistics is far wider as to its subject matter. It applies to all
phenomena which can be counted and recorded. It deals equally with matter and
with mind. Perhaps the most remarkable results of the statistician’s labours are
those which show that the human will obeys laws nearly as certain as those which
regulate matter.
here are countries in which we find year after year the same number of marriages
at the same ages and in the same proportion to the population, the same number
of children to a marriage, the same number of bankruptcies, and the same number
of crimes and suicides, committed at the same ages, and by each sex in permanent
proportions; in which the average height, the average weight, the average con-
sumption and production of commodities, and the average longevity, of men and of
women, continue for long periods unaltered.
There are others in which the number or the proportion of these events varies;
in which marriages, births, deaths, crimes, consumption and production, and even
the average stature are different at different periods. This uniformity, or these
differences, are detected by the statistician. His task is over when he has stated and
recorded them. It is the business of the legislator to draw from the figures of the
statistician, practical inferences. To ascertain the circumstances, moral, commercial,
or political, under which the tribute paid by his countrymen to insolvency, crime, .
sickmess and death, has been increased, has been diminished, or has remained
stationary—these circumstances will often appear to be under control, and by
watching the statistical results of every attempt to control them, he will ascertain
whether they we under control or not.
We have been told that a statesman “reads his history in a nation’s eyes.”
I should rather say that he reads it in a nation’s figures.
But it is not only to the statesman that statistics are useful, many of the most
important and most useful employments of capital depend onthem. Vital statistics
are the base of life insurance. They decide the value of annuities, of life estates,
and of reversions. Every man in the management of his property has to consult
them. The statistics of fires regulate fire insurance, those of wrecks regulate
marine insurance, Wherever the success or failure of an undertaking depends on
184 REPORT—1860.
the calculation of chances, and wherever the events subject to those chances have
been observed and recorded in numbers sufficient to afford an average, the prudence
or imprudence of the undertaking depends on that average. To give that average
is the business of the statistician. ‘To act on it is the business of the speculator. If
in London one house in two thousand were burnt down every year, nothing would
be gained or lost by insuring houses in London at a shilling per cent. per annum.
If one in a thousand were burnt down, such insurance would beruinous. If only one
in three thousand, it would be very profitable. But, I repeat that the observation,
the recording and the arranging facts, which is the science of statistics, and the
ascertaining, from observation and from consciousness, the general laws which
regulate men’s actions with respect to production and exchange, which is the
science of political economy, are distinct from the arts to which those sciences are
subservient. We cease to be scientific as soon as we advise or dissuade, or even
approve or censure.
I said, that I had been led into this train of thought by looking through the
papers which have been communicated to this Section since 1856. I find that we
received during that year ‘“ Suggestions on the education of the people.”
We had a paper, “On the general principles by which Reformatory Schools
ought to be regulated.” We had another, “On the importance of open and public
Competitive Examinations.”
In 1857 we had one on the prevention of crime ; one on the reasons for extending
limited liability to joint-stock banks; and one on the apprenticeship system in re-
spect to freedom of labour.
In 1858 we had one on the principle of open competition ; one on public service,
academic and teacher’s examinations; one on the importance of a colonial penny
os to the advancement of science and civilization ; and one on the race and
anguage of the gypsies.
If it be said that in all these papers, except indeed the very last, there was a
reference to statistical facts, or to economic principles, and that therefore they were
properly communicated to this Section, the answer is, that there is no province of
the great arts of legislation, of administration, of commerce, of war, indeed, of any
of the arts which deal with human feelings, in which frequent reference must not
be made to political economy, and occasional reference to statistics. There is
scarcely a moral art therefore of which we should not be able to take cognizance.
But I do not think that such an extension of our jurisdiction would be advi-
sable. I believe that in mental, as in manual arts, the division of labour is useful.
Within the strict limits of economic science and statistics a large field is open to us.
It appears to me that we shall do well, if, as far as may be practicable, without
much inconvenience, we confine ourselves within it, and deviate as little as we can
into the numerous arts to which those sciences afford principles.
On the True Principles of an Income Tax.
By the Rey. J. Bootu, LL.D., F.RS.
On Educational Help from the Government Grant to the destitute and neg-
lected children of Great Britain. By Mary CARPENTER.
The educational movement, as such, is of comparatively recent date in our
country. ‘The importance of popular education was not generally acknowledged in
England fifty years ago: but yet as early as in the sixteenth century there were
distinct efforts made to give instruction to the very poorest, as is proved by the King
Edward and many other endowed Charity Schools. These gradually became
employed by a higher class than the children for whom they were originally in-
tended, and a part of the population were uncared for. In 1781 Raikes began the
first Sunday school for outcast children; in 1800 Bell and Lancaster began day
schools, to give gratuitous instruction to the very lowest. Now the Sunday schools
no longer receive the vagrant children, and the Bell and Lancaster schools have
gradually merged into the National and British pay schools. A large class of the
people are instructed by these schools, but those who most need instruction are not
able to attend them.
“At the Educational Conference in 1857, H.R.H. Prince Albert stated that there’
Rs
TRANSACTIONS OF THE SECTIONS. 185
are 2,200,000 children in England and Wales not at school, whose absence cannot
be traced to any legitimate cause. If Government educational help is given to
any portion of the population, it ought, for the good of society, to be directed
efficiently towards these. From this uneducated mass spring the pauperism and
crime which are so great a national burden. Union Inspectors find the state of
degraded ignorance in which children usually come to the workhouse indicative
of the existence of a large portion of the population untouched by existing institutions;
in Liverpool, out of 19,386 persons apprehended in 9 months, only 3 per cent. could
read and write. Industrial and Ragged Schools alone have attempted distinctly to
act on this class. Wherever they have been well conducted and efficiently supported
they have completely effected the object intended, but many have failed from want
of teaching power. The children of this class, in addition to ordinary instruction,
must have much moral and industrial training, and schools capable of acting on
them must be adapted to their wants, and of a very different character from the
ordinary pay schools.
The Committee of Council on Education, in administering the Parliamentary
Grant, have adapted their regulations to the pay schools; in 1859, 6222 Certiti-
cated Teachers for them were partially paid, receiving £86,528 ; Assistants, £6244;
Pupil Teachers, £252,550; thus providing a good teaching power for 9555 schools.
No teaching power (except a gratuity to certified masters, who very seldom are
qualified for such schools) and no educational help is allowed to the schools for the
destitute and neglected children.
The importance of giving an efficient teaching power to the lowest and most
ignorant children was acknowledged by Parliament in 1849, when an annual grant of
£30,000 was made to teachers in union schools, with a much lower test than that
required for certificated masters. The Parliamentary Committee of Inquiry, in
1853, into the Condition of Criminal and Destitute Juveniles, reported the “ bene-
ficial effects produced on the most destitute classes” by the Ragged and Industrial
schools, and their need of help from the Educational Grant; that aid is still re-
one to carry out efficient action on the destitute and neglected children of
rreat Britain.
On the Economical Results of Military Drill in Popular Schools.
By Evwix Cuanvwicx, Esq., C.B.
On the Physiological as well as Psychological Limits to Mental Labour.
By Enwin Cuapwick, £sq., CB.
The business of education still requires for its successful prosecution, scientific ob-
servation, and the study of the subject to be operated upon—the human mind, Even
to empirical observation, it should have suggested itself that the mind has conditions
of growth which are required to be carefully noted, to adapt the amount of in-
struction intended to be given to the power of receiving it. It is a psychological law
that the capacity of attention grows with the body, and that at all stages of bodily
growth the capacity is increased by the skilful teacher's cultivation. Very young
children can only receive lessons of one or two minutes’ length. With increasing
growth and cultivation, their capacity of attention is increased to five minutes; then
to ten, and at from five to seven years of age, to fifteen minutes. With growth and
cultivation, by the tenth year a bright voluntary attention may be got to a lesson
of twenty minutes; at about twelve years of age to twenty-five minutes; and from
thence to fifteen years of age, about half an hour: that is to say, of lessons requiring
mental effort, as arithmetic, not carried beyond the point at which the mind is
fatigued, with the average of children and with good teaching. By very skilful
teachers and with very interesting lessons, the attention may be sustained for longer
eriods; but it is declared by observers that prolonged attention beyond average
imits is generally at the expense of succeeding lessons.
The preponderant testimony which I have received in the course of some inquiries
into educational subjects, is that with children of about the average age of ten, or
eleven, or a little more, the capacity of bright voluntary attention, which is the
only profitable attention, is exhausted by four varied lessons to subjects and exer-
cises requiring mental effort of half an hour each in the forenoon, even with inter-
186 REPORT—1860.
vals of relief. After the mid-day meal the capacity of voluntary attention is gene-
rally reduced by one-half, and not more than two half-hour lessons requiring mental
elfort can be given with profit.
The capacity of attention is found to be greater in cold weather than in hot, in
winter than in summer.
I collect that the good ventilation, lighting, and warming of a school-room will
augment the capacity of attention of the pupils by at least one-fifth, as compared
with that of the children taught in school-rooms of the common construction.
Talso collect, that the capacity of attention varies with bodily strength and
weakness, It is reported to me that school-boys, of nearly the same ages and con-
ditions, of the same school-rooms, and under the same tuition, being weighed, and
divided into two classes, the light and the heavy, the attainments, as denoted by
the number of marks obtained, were found to be the greatest with the heaviest,
that is to say, those of the greatest health and bodily strength.
These were chiefly of town-born children, of common habits. The robust
children of rural districts, of less cultivated habits of attention, are found to be
slower in receiving ideas; but with cultivation they are brought up to equal
capacities of attention, and to greater retentiveness of the matter taught, than the
common classes of town-born children.
There are differences in the capacities of attention in different races, or in the
habits of attention created previously to the school-period by parents of different
races. The teacher of a large school in Lancashire, who had acted as a school-
teacher in the southern counties, rated the capacity of attention of the native Lanca-
shire children as 5 to 4, as compared with those in Norfolk. In other instances the
differences were wider.
Experienced teachers have testified to me that they can and do exhaust the
capacity of attention, to lessons requiring mental effort, of the great average of
children attending the primary schools in England, in less than three hours of.
daily book instruction, namely, two hours in the morning, and one hour after the
mid-day meal.
Infants are kept in school, and the teacher is occupied in amusing and instruct=
ing them, for five or six hours, but the duration of mental effort in the aggregate
bears only a short proportion to the whole time during which they are kept
together. So in schools for children of more advanced ages. Even the smaller
amount of mental effort in infant schools is, however, subject to dangerous excess.
I am assured by a teacher in the first infant school established in Scotland, that he
did not know a pre-eminently sharp child who had in after life been mentally
distinguished.
In common schools, on the small scale, the children will frequently be not more
than one-half the time under actual tuition; and in schools deemed good, often
one-third of their time is wasted in changes of lessons, writing, and operations
which do not exercise, but rather impair the receptive faculty.
It may be stated generally that the psychological limit of the capacity of attention
and of profitable mental labour is about one-half the common school-time of
children, and that beyond that limit instruction is profitless,
This I establish in this way. Under the Factories Act, whilst much of the in-
struction is of an inferior character and effect, from the frustration of the provi-
sions of the original bill, there are now numerous voluntary schools, in which the
instruction is efficient. The limit of the time of instruction required by the statute
in these half-time schools for factory children is three hours of daily school teaching,
the common average being six in summer and five in winter. There are also
pauper district industrial schools, where the same hours, three daily, or eighteen
in the week, or the half-time instruction, are prescribed; which regulation is in”
some instances carried out on alternate days of school teaching and on alternate
days of industrial occupation. Throughout the country there are now mixed schools,
where the girls are employed a part of the day in needlework, and part of the day
in book instruction. Now I have received the testimony of school inspectors and”
of school teachers, that the girls fully equal in book attainments the boys who are.
occupied during the whole day in book instruction. The preponderant testimony is
that in the same schools, where the half-time factory pupils are instructed with the
full-time day scholars, the book attainments of the half-time scholars are fully equal
eee 7 aaa a — = SS
ee eee eee
TRANSACTIONS OF THE SECTIONS. 187
to those of the full-time scholars, 7. e. the three hours’ are as productive as the six
hours’ mental labour daily. The like results are obtained in the district pauper
schools. In one large establishment, containing about six hundred children, half
7 and half boys, the means of industrial occupation were gained for the girls
efore any were obtained for the boys. The girls were therefore put upon half-
time tuition, that is to say, their time of book instruction was reduced from thirty-
six hours to eighteen hours per week, given on the three alternate days of their
industrial occupation, the boys remaining at full school-time of thirty-six per week
—the teaching being the same, on the same system and by the same teachers, the
same school attendance in weeks and years, in both cases. On the periodical
examination of the school, surprise was expressed by the inspectors at finding how
much more alert mentally the girls were than the boys, and in advance in book attain-
ments. Subsequently industrial occupation was found for the boys, when their
time of book instruction was reduced from thirty-six hours a week to eighteen; and
after a while the boys were proved upon examination to have obtained their previous
relative position, which was in advance of the girls. The chief circumstances to
effect this result, as respects the boys, were the introduction of active bodily exer-
cises, the naval and the military drill, and the reduction of the duration of the
school teaching to within what appear to me to be the psychological limits of the
capacity of voluntary attention.
When book instruction is given under circumstances combining bodily with
mental exercises, not only are the book attainments of the half-time scholars proved
to be more than equal to those of the full-time scholars, but their aptitudes for
applying them are superior, and they are preferred by employers for their superior
alertness and efficiency.
In the common course of book instruction, and in the average of small but well-
managed long-time schools, children after leaving an infant school are occupied on
the average six years in learning to read and write and spell fairly, and in acquiring
proficiency in arithmetic up to decimal fractions. In the larger half-time schools,
with a subdivision of educational labour, the same elementary branches of instruc-
tion are taught better in three years, and at about half the annual expense for
superior educational power.
The general results stated, I have collected from the experience during a period of
from twelve to fifteen years of schools, comprising altogether between ten and twelve
thousand pupils. From such experience it appears that the general average school-
time is in excess full double of the psychological limits of the capacities of the
ayerage of children for lessons requiring mental effort.
_ LT haye not hitherto been enabled to carry my inquiries to any sufficient extent
for astatement of pees results, to the schools for children or youth of the
higher ages, but I believe it will be found that the school and collegiate require-
ments are everywhere more or less in excess of psychological limits. I gather that
the average study, continuous and mental labour, of successful prizemen at the uni-
yersities is from five hours and a half to little more than six hours of close mental
labour or exertion from day to day. An able Oxford examiner informs me, that if
he ever hears that some one is coming up for examination who has been reading
twelve or thirteen hours a day, he is accustomed to exclaim, “that man will be
lucked!” and during his experience of thirteen years a3 an examiner at Oxford,
e has never known an instance to the contrary. In respect to the mental labour
of adults, it is observed by Sir Benjamin Brodie in his ‘ Psychological Inquiries,’
“A man in a profession may be engaged in professional matters for twelve or
thirteen hours daily, and suffer no very great inconvenience beyond that which may.
be traced to bodily fatigue. The greater part of what he has to do (at least it is so.
after a certain amount of experience) is nearly the same as that which he has done
many times before, and becomes almost matter of course. He uses not only his
previous knowledge of facts, or his simple experience, but his previous thoughts,
and the conclusions at which he had arrived formerly; and it is only at intervals
that he is called upon to make any considerable mental exertion. But at every step
in the composition of his philosophical works Lord Bacon had to think, and no one
can be engaged in that which requires a sustained effort of thought for more than
a very limited portion of the twenty-four hours, &e.
r But great things are accomplished more frequently by moderate efforts persevered.
188 REPORT—1860.
in with intervals of relaxation during a very long period. I have been informed
that Cuvier was usually engaged for seven hours daily in his scientific researches ;
but these were not of a nature to require continuous thought. Sir Walter Scott,
if my recollection be accurate, describes himself as having devoted about six hours
daily to literary composition, and his mind was then in a state to enjoy some lighter
pursuits afterwards. After his misfortunes, however, he allowed himself no relaxa-
tion, and there can be little doubt that this over-exertion contributed as much as
the moral suffering which he endured to the production of the disease of the brain,
which ultimately caused his death. Sir David Wilkie found that he was exhausted,
if employed in his peculiar line of art for more than four or five hours daily; and
it is probable that it was to relieve himself from the effects of too great labour that
he turned to the easier occupation of portrait-painting. In fact, even among the
higher grades of mind there are but a few that are capable of sustained thought,
ete day after day, for a much longer period than this.”—P, 9-13.
Sir Benjamin Brodie has stated to me that he subsequently ascertained that in
the above passage he had rather exceeded the limits of the mental labour of Sir
Walter Scott, who, in a conversation on the topic, in the presence of Sir Charles
Lyell and Mr. Lockhart, had declared that he worked for three hours with pleasure,
but that beyond about four hours he worked with pain. Sir Benjamin states to me
that he is of opinion “that for young children three or four hours’ occupation in
school must be even more than sufficient, and that they will be found in the end to
have made greater progress, if their exertions are thus limited, than if they are
continued for a longer period.”
In large public establishments in which I have had an executive direction, I have
not found it practicable to sustain, on the average, for longer than six hours per
diem, from day to day, continuous and steady mental labour on the part of adults.
I find ground for the belief that as more and more of mental effort and skill is
required in the exercise of the manual arts, the hours of work must be more and
more reduced for the attainment of the best economical results without waste of
the bodily power.
The psychological limits to mental labour are governed by phystological limits,
which in the case of young children are first indicated by bodily pain experienced,
in continued sedentary constraint, from suppressed muscular activity, or from mus-
cular irritability. As respects children, the physiological case is put in the follow-
ing letter which I wrote to Professor Owen, and in his answer :—
“Dear OwEN,—Permit me to submit to you for your consideration and for my
instruction, some questions on topics of observation made from time to time offi-
cially on the common practice of popular education, whether, in the duration of
sedentary attention which its theory requires, it is not at variance with elementary
principles of physiology ?
“First, let me observe upon the very young of our species, their mobility at the
periods of growth, particularly in infancy,—their constant changes of bodily position,
when free to change,—their incessant desire for muscular exertion,—their changes,
short at first, longer as growth advances,—these changes being excited by quickly
varying objects of mental attention, and forming incessantly varying alternations of
exertion and repose, with manifestations of pleasure when allowed free scope for
them, of pain when long restrained. Now to what physiological conditions do
these alternations of exertion and repose subserve ?
“ When obstructed and subjected to constraints for long periods, and when pain
and mental irritation and resistance are excited amongst classes, are not the pain and
resistance to be taken as a remonstrance of nature against a violation of its laws ?
“The theory of the common practice of school instruction is of five and as much
as six hours’ quietude, and for intervals of three hours each, perfect muscular inac-
tivity and stillness of very young and growing children from seven to ten years old,
and during this constrained muscular inactivity, continuous mental attention and
labour.
“To ensure these conditions of continued bodily inactivity and prolonged mental
labour, the common office of the schoolmaster is everywhere a war for the repres-
sion of resistances and incipient rebellions. But are not these resistances excited
by nature itself? Are not dase cutting, whittling with knives, mischief, conditions
en wae =
| atte caine
ey ee
TRANSACTIONS OF THE SECTIONS, 189
of irritability, manifestations of excessive constraints against physiology? If the
condition of muscular inactivity were completely enforced, what does physiology
tell us may be expected from these restraints? I might ask you, indeed, whether
much of the insanitary conditions of our juvenile and very young populations are
not consequences following from them ?
“First, there is the proverbial pale-facedness of the young scholar, and a lower
bodily condition of those who are subject to the confinement of schools, even of the
best construction and ventilation, than of those who are free from them and at
large, at liberty to follow natural instincts.
“ When the weakly fail in health in a marked degree under the restraints of the
school, the remedy 1s restoration to natural freedom, which commonly leads to
improved health. I cannot but attribute to the lowering of the system and bodily
debility produced by this excessive school constraint (even where there is good ven-
tilation), and the consequent exposure to epidemic conditions and other passing
causes of disease, a large share of our juvenile mortality, especially between seven
and ten years of age, when the opportunities of retrieving the effects of the school
constraints by athletic exercises are less than at later periods.
“But the constraints of a school are accomplished most fully in girls’ schools, more
especially in boarding schools, where the sedentary application of young children
is extended to eight hours daily, and diseases are attendant upon them, which I
cannot help ascribing largely to violations of the laws of physiology. In Manchester,
with the increase of prosperity, an increased proportion of females have been sent
to boarding schools and high class schools with long hours; and I am assured
by Mr. Roberton, who is especially conversant with the diseases of females, that
the proportion of the mothers of the middle class who cannot suckle their own
children is increasing. He has shown me statistically that, with all the care be-
stowed upon females who have been so highly educated, the failures and deaths
in childbirth are full sevenfold greater than amongst females of a lower condition
in life, who have had less school restraint and sedentary application, and more
freedom and muscular development in childhood. Cases of spinal distortion, ner-
vous disorder, nervous mania, and hysteria, prevail peculiarly amongst the middle
and higher class of females, whose education has been of prolonged sedentary occu-
pation, even under the best sanitary conditions in other respects. As applied to
them, it is a proverbial observation that ‘ailing mothers make moaning children.’
A lady who was eminent as a boarding-school teacher, but who has retired from
business, has observed painful evidence of the injury done by the prolonged hours
of sedentary application which custom and the demands of parents require, and
she confirms the experience of the best half-time schools, that better instruction
might be given in shorter hours. I have received a body of evidence from able
teachers, that they can and do exhaust the capacity of attention to book instruction
in half the time for which sustained attention to such instruction and bodily in-
activity is demanded by custom.
“But what I seek is the sanction of your opinion, as to whether, if the laws of
physiology be duly consulted for providing a sound body for a sound mind, other
treatment is needed than that which prevails in schools, of requiring five or six
hours of sedentary occupation for children in the infantile stage, and seven or eight
for those in the juvenile stage? I appeal to you more particularly from the fact,
that in lectures and papers the teaching of physiology is insisted upon as an addi-
tional element of popular education, and an additional demand of time in those
schools, the whole condition and theory and attempted practice of which, though
not yet so recognized generally by professors of the science, appears to me to be a
large violation of it, and an offence against infantile nature.
“ Yours ever, &e.”
“My pEAR Cuapwicx,—I have perused and carefully considered every point in
the inquiry which you have addressed to me, and I concur completely with your
belief in the agreement with nature of the changes you recommend in the distribu-
tion and change of the periods devoted to school restraint and studies, and to bodily
exercise and relaxation.
“All the nutritive functions and actions of growth proceed more vigorously and
rapidly in childhood and youth than in mature life,—not merely as regards the
190 ; REPORT—1860.
solids and ordinary fluids, but also in the production of those imponderable and
interchangeable forces which haye sometimes been personified as ‘ nervous fluid,’
‘muscular force,’ &c. Using the latter term to exemplify my meaning, the excess of
nervous force is in the child most naturally and healthily reduced by its conversion
into muscular force ; and at very short intervals, during the active or waking period
of life, the child instinctively uses its muscles, and relieves the brain and nerves of
their accumulated force, which passes, by the intermediate contraction of the mus-
cular fibre, into ordinary force or motion, exemplified by the child’s own movements,
and by those of some object or other which has attracted its attention,
“The tissues of the growing organs, brain, muscles, &c., are at this period of
life too soft to bear a long continuance of their proper actions; their fibres have
not attained their mature tone and firmness; this is more especially the case with
the brain-fibre. The direct action of the brain, as in the mental application to learn-
ing, soon tires; if it be too long continued, the tissues are unhealthily affected ; the
due progress of growth, which should have resulted in a fibre fit for good and con-
tinuous labour at maturity, is interfered with; the child, as an intellectual instrument,
is to that extent spoiled by an error in the process by which that instrument was
sought to be improved.
“The same effect on the muscular system is exemplified in the racers that are
now trained to run, at 21 or 3 years’ old, for the grand prizes at Doncaster or Epsom.
The winner of the ‘ Derby’ never becomes an ‘ Eclipse’ or ‘ Flying Childers,’ because
the muscular system has been overwrought two or three years before it could have
arrived at its full development, which development is stopped by the premature
oyer-exertion.
“Tf the brain be not stimulated to work, but is allowed to rest; and if, at the
same time, the muscles be forbidden to act, there then arises, if this restraint be
too prolonged, an overcharged state of the nervous system. It is such a state as
we see exemplified in the caged quadruped of active habits, when it seeks to relieve
it by converting the nervous into the muscular force to the extent permitted by its
rison, either executing a succession of bounds against the prison-bars, like the agile
eopard, or stalking, like the lion, sullenly to and fro.
“Tf the active child be too long prevented from gratifying the instinctive impulse
to put in motion its limbs or body, the nervous system becomes overcharged, and
the relief may at last be got by violent emotions or acts, called ‘passion’ or ‘naughti-
ness,’ ending in the fit of crying and flood of tears,
“ But all these impediments to a healthy development of the nervous system
might be obviated by regulations, based on the system which you rightly advocate,
providing for more frequent alternations of labour and rest, of study and play, of
mental exertion and muscular exercise ; in other words, by briefer and more frequent
periods allotted to those phases of educational procedure, and modified to suit two
or three divisions of the scholars, according to age,
“The powers and workings of the human frame concerned in the complex acts
and influences, which you have asked me to explain physiologically, are amongst
the most recondite and difficult in our science. You will therefore comprehend
and excuse my short-comings in trying to fulfil your wish. But, on the main point,
T have no doubt that your aim is in close accordance with the nature of the delicate,
and, for good or evil, easily impressible organization of the child.
“ Believe me, ever truly yours,
* RICHARD OWEN,”
It is difficult to separate distinctly the evils arising from the excess of simple
bodily inactivity, from the results of the common insanitary conditions of schools—
bad ventilation, bad lighting, bad warming, and overcrowding. These, however,
are attended by epidemic and eruptive diseases, which ravage the infantile com-
munity, Simple constraint appears to be attended by eneryation and obstructed
functions, and thence maladies of another class. The preventive of these is the
occupation of children, with means of physical training, with systematized gym-
nastics, including swimming, and the naval and military drill. Where there have
been good approximations to the proper physiological as well as the psychological
conditions, as in the half-time industrial district schools, epidemic dossei have
been banished, and the rate of mortality reduced to one-third of that which prevails
—
a
TRANSACTIONS OF THE SECTIONS, 191
amongst the general community, and in England and Wales alone, where upward
of a quarter of a million of children are annually swept away from preventible
disease, which enervates those who survive. Four labourers, who have had the
advantage of this improved physical and mental training, are proved to be as effi-
cient as five or more of those who have not. I am prepared to show that by ad-
ministrative improvements in the application of the principles in question, double
the population may be physically and mentally trained well at the expense of
educating the existing numbers ill.
On Local Taxation for Local Purposes. By R. Dowven.
Dr. Whewell on the Method of Political Economy.
By Henry Fawcert, W.A.
On Co-operative Societies, their Social and Political Aspect.
By Henry Fawcett, M.A.
On the Province of the Statistician. By J. J. Fox.
On Sanitary Drainage of Towns. By J. Hircuman.
On the System of Taxation prevailing in the United States.
By E. Jarvis, Boston, U.S.
On Serfdom in Russia. By Dr. MicuEtsen.
On the Economical History and Statistics of the Herring. By J. M.
Mitcue ty, F.R.S.S.A., one of the Secretaries for Foreign Correspondence
- of the Society of Antiquaries of Scotland, &c.
_. The author said that he read this paper with the view of drawing public atten-
tion to the great national importance of the Herring F ishery on the British coasts;
and stated that the propriety of affording every encouragement and protection to
it has been already affirmed by this Association, in its roposing for one of its
objects “The improvement and extension of the British Fisheries ;” and the author,
im pointing out its importance, quoted the following extract from Baron Cuvier's
‘Natural History of Fishes,’ vol. xx. pp. 30, 31:—
“ Par son inépuisable fécondité le hareng est une de ces productions naturelles
dont l'emploi décide la destinée des empires. La graine du cafier, la feuille du thé,
les épices de la zone torride, le ver & soie, ont moins influé sur les richesses des
nations que le hareng de l’océan septentrional; le luxe ou le caprice demandent
les premiers, le besoin réclame le second. La péche de ce poisson fait partir
chaque année, des cdtes de France, de Hollande, des Iles Britanniques, des flottes
nombreuses pour aller chercher dans le sein d’une mer orageuse, la moisson
abondante et assurée que les légions innombrables présentent & la courageuse
activité de ces peuples. Les evandes politiques, les plus habiles économistes, ont
vu dans la péche du hareng la plus importante des expeditions maritimes; ils ]’ont
surnommées la grande péche. Elle forme des hommes robustes, des marins intré+
pides, des navigateurs expérimentés. L’industrie que s’empare des produits de ce
péche sait en faire l'objet d’un commerce, source des richesses inépuisables.”
Many Acts of Parliament for the purpose of encouraging the fishery, from an
early period downwards, had been passed by the Legislature; but, owing to the
want of the knowledge of the natural history and habitat of the herring, they
proved either injurious or abortive, although bolstered up with bounties and pre-
miums ; and the fishery would not have become of any importance had not a local
board of unpaid Commissioners been established, with efficient officers acquainted
with the localities, so that the fishery might be prosecuted with success at the
192 REPORT—1860.
properly ascertained seasons. The Board was established in 1808, and its beneficial
operations would be proved by the statistics of the progress of the fishery; and it
will be seen that this fishery became, and is now, one of the greatest and most
rosperous in the world, and is now only in danger from improper interference, if it
is not guarded and controlled by the influence and opinions of scientific and intelli-
gent men, such as are found at this Association.
To prove the great interest that is taken by other maritime nations in the Herring
Fishery, he stated that an interesting discussion took place at the French Academy
in 1855, on the question of the migration of the herring, with no satisfactory
results, from the want of the knowledge of facts: also, that the Government of
Norway had been occupied for several years past in legislating with the view of
promoting the Herring Fishery on the coasts of that country; and that in Sweden
an elaborate report had been prepared, by the authority of the Government of that
country, by one of the heads of the civil department, M. von Wright, with the
view of obtaining information as to the cause of the total disappearance of the vast
shoals of herrings that formerly visited the Swedish coasts; and that the Govern-
ment of Holland is anxiously occupied in obtaining information on the subject, and
has employed scientific men to investigate the subject of the visits of the feria
and to prepare reports. The results of these observations, made on board of forty-
five of the Dutch fishery busses, are given in a work published by the authority of
the Dutch Government, which has been thought of such importance that the
British Board of Trade has ordered a translation of it to be made and published for
general information ; and it is important that it should be known that this move-
ment of the Government of Holland is caused by the lately rapid declension of the
Dutch Fishery, and that Government, seeing the rapid progress of the British Fishery
on our coasts, has established a system of superintendence and regulation similar to
that so successfully promoted by the Fishery Board.
He said that there were many subjects for inquiry which do not properly belong
to our Fishery Board, the Commissioners of which and their officers have special
duties to perform under legislative enactments, and it may therefore be considered
as a reproach to this country, which gains so abundant a supply of food of the best
description, while at the same time securing a large force of useful mariners ready
to detnd our coasts, and in the day of peril to man our navy, that no efficient
efforts have yet been made to elucidate the natural history of the herring.
At the present time we seem to pay too little attention to the fostering of our
native industry; it is surely obvious that in encouraging the search for gold in our
colonies, we are losing, or sending away from our own country, some of the most
enterprising and industrious of our inhabitants, not easily to be replaced ; while by
encouraging the search for the golden treasures on our own coasts, as truly said by
the distinguished author, Cuvier, we create those men of so much yalue to a
maritime country—“ INTREPID AND ROBUST MARINERS,” besides adding every year
additional suPPLIEs OF FOOD and “INEXHAUSTIBLE RICHES.”
To prove the great advantage of the system of superintendence and inspection of
the Fishery Board and their officers, some statistics were given of the progress of the
Fishery : among others the following :—
When the Fishery Board was first established in 1808, the quantity of herrings
cured and salted in barrels was 99,185 barrels, while in 1855 the quantity cured
was 766,703 barrels; and adding the quantity sold fresh, 130,759 barrels, we find
the total quantity of herrings caught in that year was 897,462 barrels—yielding at
a moderate calculation the value of one million sterling, which may be safely taken
as the average annual value of the herrings fished on the coasts of Scotland, without
calculating the quantity caught at Yarmouth and other places on the English and
Trish coasts, which are principally sold fresh or smoked.
Before an efficient system of legislation and regulation was adopted in this
country, the demand from abroad was inconsiderable, but it has annually increased
since: for instance, in 1812 the quantity exported to the Continent was only 4720;
in 1815 it amounted to 35,891; in 1840 to 82,351; in 1845 to 143,754; in 1850 to
257,103; and in 1855 the quantity exported was 344,029. And to show how rapid
the progress has been in foreign markets of the sale of British herrings, he gave the
amount of the British, Dutch, Danish and Norwegian herrings imported into one of
the largest exporting towns in Prussia (Stettin) in successive years.
—
I
TRANSACTIONS OF THE SECTIONS. 193
In 1825 there was imported there—from
Great Britain. Holland. Denmark, Norway.
18,160 A295 1960 6,758
In 1845 81,189 2457 307 44,264
In 1850 = 116,53 508 470 12,567
and in 1855 the quantity of British herrings amounted to 160,572 barrels—about
nine times the quantity sent in 1825 to Stettin; and as the herrings are carefully
separated, assorted and packed into proper-sized barrels, cured under the eye of the
inspecting officers, the British herrmgs have become known, in consequence, as
a safe and staple article of commerce, and are imported into various other ports;
for instance, there were exported to the following ports in 1855—
sed Soa HQ gp Or iSnNEnes SOOD GS DIC . 14,417
PIE, FO ean ek fee tame natinie «has mte 59,204
Eipnpere’. fsck cerhutiace coe ee 26,774
aerate POF: Set eee hae ee ee 60,577
IreTnen 24 PL Se ee Soe ee es salen 6,754
Rotterdam, for the Rhine ......,.......5% 7,955
Chater Paris, NEU etree ta etal tsa 8,244
SLOG , Were hiked oer a Sofia PG SEA ies 160,572
Maleate artoteler VE P55 0 es bee 344,207
And it is interesting to know that at the fishery stations in Scotland there were
. employed in the year referred to, Fishing Boats 11,251, the tonnage being 77,794;
and the fishermen, coopers and others employed, amounted to 91,139, of which
91,189 people directly employed, 39,266 were fishermen. These statistics apply to
the Scottish coasts only, where the greatest shoals of herrings resort ; but there are
other places, as already stated, such as Yarmouth, where many of the fishermen are
occupied in fishing herrings in the usual seasons.
Tt is necessary that the truth should be known as to the progressive prosperity
and increase of the Herring Fishery, because there are some authors who are in-
clined to depreciate our national productions and progress; for instance, we find
McCulloch, in his ‘ Dictionary of Commerce,’ which is considered a text-book and
standard work by a certain class of readers, saying “the Dutch have uniformly
maintained their ascendency in the Herring Fishery since the earliest period,” and
that “ ours remains in a very unhealthy and feeble state.”
_ As already stated, the Dutch Herring Fishery is in a declining state, and instead
of 300 busses proceeding annually to the fishery, as was the case not many years
ago, the number has been gradually decreasing, and does not now exceed 60 busses ;
but on our coasts great prosperity is evident from the progress of the population,
the increase of towns ‘and villages, and from the comfortable state of the fishermen
and their families, and the great circulation of wealth that must exist by an annual
increase of one million sterling taken out of the sea on our own coasts.
The value of this great fishery should teach us the propriety of carefully fostering
and protecting it; and to enable us to do so efficiently, we must have some know-
ledge of the natural history and habits of the herring, as well as accurate statistcis.
He said he was prepared to prove that the herring was a native of the seas adjacent.
_ to the coast to which it resorted; and in conclusion, he said that to promote its
prosperity, or even to protect it, legislation was necessary, and power should be
given to prevent the disturbance of the spawn, and the indiscriminate destruction
_ of the young herring or fry. The fishery grounds during the proper season shonld
_ be attended by the proper number of ships of war, to prevent disputes and disturb-
ance among the fishermen, and to prevent the large fishing vessels from driftin
into the smaller ones. He recommended that the Fishery Board established in
Scotland, should be extended to England and Ireland, as calculated to increase the
rosperity of the fisheries and the number of fishermen and seamen suitable for
e€ navy.
_Betore concluding he produced a copy of a letter written by him to the Right.
Hon. the Lord Adyocate of Scotland, to prove that it is absolutely necessary for
1860. i
194 REPORT—1860.
the protection of the fishermen and the merchants that the system of inspection by
the Fishery Officers be continued to preserve order among the fishermen during the
fishing season, to prevent the fishermen using illegal nets, and to prevent the
fishermen being defrauded by illegal measures; and more particularly as the
merchant buys perhaps several thousand barrels at a time, that the necessity of
opening the barrels and seeing the herrings may be avoided; and the various onerous
duties of the officers he thus enumerates : —
“J, They are the police of the fishery, who maintain and have the power to en-
force order. Much fraud and disorder existed before the officers were appointed ;
at ae such cannot exist without being repressed. [This may be said to be the
only constabulary force paid out of the national funds in Scotland, and costs only
£14,000 per annum. The constabulary force in Ireland, paid out of the national
funds, costs £650,000 per annum. |
“2, They protect the fishermen in this way,—the measure or cran by which they
are paid for their fish must be of legal size and branded. Formerly it was often
made too large, and the fishermen were defrauded.
“3, They prevent the meshes or squares of the net from being made below the
proper size, which, if so made, would take the young and inferior herring.
“4, They see that the fishermen do not fish during the day and on Sunday.
In a paper I read at the Literary Institute the other day, I proved that three im-
portant fisheries were annihilated by this practice of fishing during the day.
“5, They prevent, as far as they are authorized by law, the destruction of the
fry and spawn, which would diminish or annihilate the herrings.
“6, They point out to the tyro fish-curer the mode of cure.
“7, They see where the fishing localities rise into importance, so that they can
point out where creeks may be improved, by forming fishing harbours and shelter
for the fishermen.
“8, They see that the herrings are cured within twenty-four hours after being
caught.
«9, They see that the different kinds of herrings are properly separated and
packed in different barrels.
“10. They see that they are properly gutted.
; “11. They see that a sufficient quantity of salt is put into the barrels with the
errings.
“12. They see that they are properly packed in the barrels.
“13. They see that they are, after ten days, properly filled up with a sufficiency
of herrings and pickle.
“14, They see that the barrels are of the proper legal size.
“15. They see that the barrels are of the requisite materials and strength, which
they formerly were not. °
é ‘ie They see that no branded barrel is used a second time to cover inferior
sh.
“17. And when all the requirements are attended to, they apply the brands to
the various descriptions of herrings as they have been assorted. There are several
brands applicable to the different kinds—the highest being the crown brand and the
word ‘full.’ The applying the crown brand isa proof of the officer having watched
the progress of the cure. It is, in short, the mere Finis coronut opus—the opus, or
work, has been going on since the herrings were fished, and the crown proves that
the herrings are merchantable; but the various operations require careful attention
during the whole year.”
On some suggested Schemes of Taxation, and the Difficulties of them.
By W. NewMarcu.
Hints on the best Plan of Cottage for Agricultural Labourers.
By Henry Joun Ker Porter, MRA.
The present condition of the dwellings of farm labourers requires, I believe, with
some exceptions, improvement no less than the abodes of the labouring classes in
larye towns. The drainage and ventilation are generally admitted to be imperfect ;
but the eyil of too much cold air is severely felt in some districts with which 1 am
TRANSACTIONS OF TIE SECTIONS. 195
acquainted ; I have found cottages built of what I have seen in New Zealand and
Australia, and there called “ wattle and dab” or wicker work, covered with untem-
pered mortar: these walls cannot keep out the piercing cold in winter; the frame-
worl: on which the roof rests frequently gives way, and the doors and windows can-
not be kept water-tight.
Ihave turned my attention towards their improvement. I haye had the large
heayy thatched roofs, where they are good, supported, while new brick walls
have replaced “the wattle and dab,” and new doors and;windows have been added.
I found this alteration cost from £10 to £12 each cottage, and the occupiers were
quite willing to have 5 per cent. on the outlay added to their rent.
With reference to new buildings, I have the pleasure to present to this Section
of the British Association the drawings of a cottage which I found from practical
experience to be the best suited to the labourer in rural districts. It combines the
advantages of at least three airy bed rooms, a lofty kitchen or living room, and an
apartment which may be turned either into a parlour or a bed room, where the
family is large ; or if neither of those apartments are required, it may form an outer
kitchen or scullery. A lean-to is added to the end of the house, which forms
a barn to hold the gleaning, the fuel, or other matters, without which no labourer’s
cottage can be kept neat and comfortable. Two peculiar features in the cottages I
have built I beg to refer to. Ventilation is secured by a4-inch square opening near
the ceiling in each apartment; this opening leads the foul air into a small flue of the
same size carried up to the gable of the house, and finding egress in a narrow open-
ing in the outer side of the wall. When the cottage is built of brick, this adds
nothing to the expense; when built of stone, it is only the additional cost of the
round tiles for forming the flues. Several of these flues may lead to the upper one,
which of course must be proportionably enlarged to carry off the increased quantity
of air. In Ireland I built twenty dwellings in a double row of houses, at one side
opening into a court yard, the other into the street of alarge market town. Fevers
prevailed in the following year, and several deaths occurred amongst the labouring
classes, and not one death amongst the 100 individuals occupying those houses.
I built two villages on the same estate, and the medical gentleman whose duty it
was to visit the labouring classes on that property, bore testimony to the value of
the system adopted for ventilation. The other peculiarity in these houses was the
mode in which the window-sashes were made, Hvery one acquainted with English
cottages of the last half-century, is aware of the misery and expense of lead lights,
neyer keeping out cold and always wanting repair. Metal has been substituted,
and these are often so imperfect that they fit badly and neither exclude wet
nor cold; it is the case in school-houses in the parish in which I reside, and there
was no expense spared in their erection. To avoid these difficulties, I adopted
wood for the outer part of the sash, the inner divisions being formed of 3 inch
hoop iron cut half through where they intersect, and thus forming one of the
strongest sashes possible, with the advantage of being able to add to or take from
the outer sides of the sash, to make them fit tightly ; they open on a pivot let into the
sash on each side, thus giving the whole size of the window, when necessary, for the
admission of fresh air. “I have made a very rude attempt at a model before breakfast
this morning, but it will serve to show the plan of forming the window with the
hoop iron. I have erected one such cottage in the county of Huntingdon, upon the
estate which is placed under my management as agent; and so many tenants have
requested 4wo houses each on their farms, that I am about to build several more,
the money being advanced by the Land Improvement Society, to be paid by instal-
ments in 31 years, thus giving the estates, the tenants, and the labourers the imme-
diate benefit of the improvement, while the proprietor of the estate, who is only
tenant for life, will not be obliged to expend so very large a sum, which might
have the effect of curtailing other improvements. The tenants in every case have
agreed to pay 5 per cent. increased rent for the outlay, and these rents will be paid
by labourers, who gladly settle down where they find constant employment and
comfortable and healthy dwellings.
On the Systems of Poor Law Medical Relief. By ¥. Purvy.
13*
196 REPORT—1860.
Notes on various Efforts to improve the Domiciliary Condition of the
Labouring Classes. By Henry Roserts, FSA.
It is only within the past fifteen or twenty years that much attention has been di-
rected to this subject, and considering its importance in regard to a very numerous
class of the community, I trust that a brief statement of facts, drawn from experience,
and tending to show by what means the object is most likely to be obtained, will not
be deemed foreign to the investigations of that branch of the British Association
which is devoted to Economic Science and Statistics.
That an undertaking which in its commencement may appear very easy should
in its progress encounter some unexpected difficulties, is of such common occur-
rence, that it would be almost an exceptional case were it otherwise in this
instance. But to be daunted by difficulties is foreign to the character of Britons, and
it should be so especially when the object aimed at is the benefit of our fellow-
creatures.
I assume that something of the actual domiciliary state of vast masses of our
fellow-subjects is known to most, though but few have sounded the depths of its
misery or of its degradation, and none can fully estimate its evil results. Whilst
on the Continent for the recovery of health, I have seen and heard it so often
referred to, that, when recommending the subject to the attention of influential
persons in different countries, I could not but think of those words, “ Physician,
heal thyself.”
The first associated efforts of a practical character were commenced in England,
shortly after the investigations made by Government authority into the state
of the poor, subsequent to the first outbreak of cholera in the metropolis. Two
societies were then formed by philanthropic individuals, with a view to work out
and to exhibit a practical remedy for the great social evils resulting from the con-
dition of the dwellings of the working classes,—a remedy which would commend
itself to extensive adoption, and be the means of stimulating the owners of existing
houses from self-interested motives, to improve and render them healthy abodes,
and afford the evidence of practical results in support of an appeal to the legisla-
ture for a somewhat unprecedented interference with private property.
The first established of these Societies, though the second to commence building,
which it did in 1845, is the Metropolitan Association for Improving the Dwellings
of the Industrious Classes. Up to the present time it has expended on its ten
distinct ranges of dwellings £89,613 14s. 10d., of which £71,528 2s. 6d, has been
laid out on six separate blocks of dwellings in different parts of the metropolis, which
accommodate 395 families ; the net return received from them, for the year ending
31st March last, after deducting all current expenses and repairs, amounted to
£2687 4s. 4d., being about 33 per cent. on the outlay. On two lodging houses
for single men,—one of them new, which has accommodation for 234, and the other
old, which provides for 128,—the return, owing to the want of sufficient occupants,
has been very unsatisfactory ; such indeed as to involve a considerable loss, which
proves that the buildings are’either too large, or in some way unadapted to the class
of men frequenting their neighbourhood.
It is worthy of observation that the same result has attended a similar lodging
house at Marseilles, built outside the town, for 150 men, too far from their daily
occupation, whilst many such houses elsewhere, on a smaller scale, accommodating
from 50 to 100 men, and near to their work, have fully succeeded; in some instances
they have been gradually increased, which is the case at Leeds and at Liverpool.
Of two adjoining houses, built on the Boulevard de Batignolles in Paris, to accom-
modate together 203 men, and having on the ground floor a restaurant and café,
one was closed two years since. In this instance, however, the failure is doubtless
in some degree attributable to defective management.
The second established Society in London, that for Improving the Condition of
the Labouring Classes, commenced its first building in 1844. It has constructed —
four distinct ranges of new buildings, which accommodate .97 families in separate —
dwellings, provide 94 rooms for single women, and lodgings for 104 single men, as
well as a public wash-house with baths. It has also renovated and fitted up, in —
three distinct localities, old houses which lodge 158 single men. These several
dwellings and lodging houses have all been im full occupation since 1851, Within
—————— ee Ul hl ee
TRANSACTIONS OF THE SECTIONS. 197
the past six years, three entire courts in different localities have been taken by
the same Society; and the condition of the houses, which were indescribably filthy,
and occupied by the lowest class of tenants, has been completely changed. The
number of rooms collectively contained in these courts is 275, and there is also a
single men’s lodging house with 40 beds. The total expenditure on these new
and old buildings, with the land, has been £43,631 17s. 3d.
The form in which the accounts of this Society are presented does not afford the
same facility for ascertaining the pecuniary return on the capital invested, as those
of the Metropolitan Associations do; and one of its undertakings,—that in Portpool
Lane, the Thankseiving Model Buildings, which was commenced in 1850 with
contributions received after the removal of the cholera,—was avowedly of so
experimental and mixed a character, that the pecuniary results are not a criterion
applicable to other cases, excepting as a caution against providing largely in one
building for single women. The average occupation of 64 rooms, which progressed
very slowly at the commencement, has not exceeded 50 to 52; and more stringent
regulations, with regard to the hours of closing, and more constant supervision
than in the men’s lodging houses, are proved to be indispensable. The public wash-
house and baths, though a boon to the neighbourhood, have not been remunerative.
The receipts and expenses of the different buildings during the year 1852, for
which I can personally speak to the management of this Society, having then acted
on its committee and as its honorary architect, were,—
Bagnigge Wells: self-contained houses and flats for 23 £ 8 ds
families, and rooms for 30 aged females. Outlay on} Receipts 875 7 7
land £1045, building £5025. Expenses 82 6 9
Net return 203 0 10
Streatham Street: houses for 54 families built on flats : r -
fire-proof, and with galleries. Outlay, ground rent panaiat Sea 5 ;
£50, building £8916 16s, Od. PP 2
; Net return 499 9 3
George Street: lodging house for 104 men, six stories .
high, including basement offices, and four floors of ssh os 7 ‘
dormitories. Outlay, land £1200, building £5226, P
Net return 812 5 2
Charles Street : lodging house for 84 men formed out of .
three old houses, ‘renovated and thrown into one. Bs — ae Hs 4
Outlay on repairs and furniture £1163 14s, 2d. P
Net return 184 15 2
King Street: lodging house for 22 men. An old house,
on the repairing and furnishing of which £135 was
expended.
Receipts 111.9 8
Expenses 73 13 11
Netretun 3715 9
The rents received from these houses have varied but slightly since they were
opened, up to the present time, and they are generally well-filled, the families chan-
ging but seldom. The cost of repairs is not included in the expenses which are
above stated ; they should be taken as averaging $ per cent. on new, and generally
from 1 to 2 per cent. on old buildings.
Calculating 4 per cent. interest on the cost of the land, the clear return on the out-
lay of £19,467 16s. Od. on the three first-named piles, which are new buildings, is
5; per cent., from which, deducting ~ per cent. for repairs, leaves 4} per cent. net.
It should, however, be observed, that the return from the Streatham Street family
houses is higher than from the other two, amounting to 5 per cent. net, and the
rents of the family houses were mostly fixed below those usually paid for similar
accommodation. The two lodging houses, which were old buildings and lease-
_ hold, yielded a return of about 17 per cent. ; and deducting 2 per cent. for repairs,
_ they gave a net return of 15 per cent.
The outlay in putting the three old courts into a good sanitary state, with suit-
198 REPORT—1860.
able fittings, including the lodging house, has been £7226 1s. 4d.; and the clear
return for the year ending 31st December 1858, was £203 14s. 3d., from which
deducting 14 per cent. for the expense of repairs, leaves about 1} per cent. net on
the outlay.
From these figures it would appear that whilst in the metropolis old buildings
may be renovated and fitted up for men’s lodging houses, with the prospect of at
least a fair remunerative return, although this has not been the case invariably,
the putting of old courts and blocks of dwelling houses for families into a good
sanitary condition, unless they are obtained at an unusually low price, is not likely
to yield a satisfactory return on the outlay, even taking 4 to 5 per cent. as the lowest
rate of interest which such investments should yield, after provision has been made
for repairs, and a sinking fund to pay off the capital, which there should be, espe-
cially in the case of leasehold property.
It is well also to notice that the actual benefit resulting from these efforts has
not been conferred to the extent which might be supposed, on those who were the
occupants of the courts, when they were taken by the Society, as a considerable
portion of them have been ejected, in order not only to reduce the number of occu-
pants to a due limit, but also to secure a more eligible set of tenants.
It may, however, be stated here, that a Society has for the past three years been
successfully in operation at Hastings, established mainly through the instrumenta-
lity of Dr. Greenhill, and called the Hastings Cottage Improvement Society, which
avowed “the fixed determination to spare no pains in securing the main object of
benefiting the tenants, and at the same time not to discourage the good cause by a
commercial failure.” With an expenditure to the present time of £9246 in pur-
chasing and putting old dwelling-houses into good condition, a dividend of 6 per
cent. has been paid.. Judging from what I have seen of the Society’s labours at an
early stage, it is simply that of putting the acquired property into the condition
which any kind-hearted considerate landlord would desire for his own tenants;
and this has been done with as little disturbance of the existing occupants as pos-
sible. The operations of this Society derive much advantage from the seg Ba
of two visitors, whose duty is to inspect the houses every fortnight. The forma-
tion of a reserve fund at the rate of 1 per cent. per annum, and also of a beneyo-
lent fund amongst the tenants, deserve notice.
The physical results obtained by the two Societies in the Metropolis have been
of a very marked character. For the four consecutive years 1850 to 1853, the
average number of deaths in all their houses was only 15-6 per 1000, as compared
with 27 to 28 per 1000 in the districts immediately around them, and of 26 per
1000 in the Metropolis generally, whilst there has been an almost entire freedom
from the special diseases to which the lower classes are more peculiarly subject,
not even excepting cholera. That such returns should not have been regularly
continued by the second named of these societies, is cause for regret. A very beneficial
influence has been exercised on the localities in which the houses are situated,
especially those occupied by families; and it may be confidently asserted that the
most sanguine expectations of their projectors have been realized in every respect,
excepting that of their financial returns, and the extent to which it was anticipated
that the example would be followed.
Had the returns generally proved more remunerative, doubtless a greater number
of similar houses would have been built; yet, although they are but a drop in the
bucket, when the extent and vast population of London is considered, they are not,
as compared with what has been done at Paris, encouraged by a large government
subvention, by any means as insignificant as might be inferred from a remark made
in the last number of the Quarterly Review, that “the wants of the displaced poor
have with us been utterly neglected.” It is too true that in the Metropolis of
Great Britain, as well as in that of France, the formation of new streets, and the
removing masses of miserable dens, has only increased the evil, by crowding yet more
those that remain. I can, however, after minutely examining all which had been
done or commenced in Paris two years ago, and ascertaining the additions since
made, confidently assert that Ingland, which took the lead in this effort of prac-
tical benevolence, has done much more through the unaided force of that motive,
than has been accomplished in France, with the stimulus of a government subyen-
tion of 10,000,000 francs.
OO ——— orrererree oe
TRANSACTIONS OF THE SECTIONS. 199
The number of improved dwellings for working people which have been con-
structed in London, either by local associations, or by individuals, following more
or less closely the plans of those built by the two societies before referred to, for-
bids their detailed notice ; they may be learnt from my paper on “ the Improvement
of the Dwellings of the Labouring Classes,” given in the Transactions of the
National Association for the promotion of Social Science for 1858. On this occa-
sion I shall only allude to such of them as especially illustrate the points which it
is the main object of this paper to prove.
At Shadwell, close to the line of the Blackwall Railway, a number of miserable
dwellings, tenanted by the lowest class of persons, came by inheritance into the
foo of a private gentleman, W. E. Hilliard, Esq. of Gray’s Inn: actuated
y the most philanthropic views, he decided on endeavouring to improve, not only
his own property, but also by example the immediate neighbourhood, and his
efforts have been crowned with signal success. The old dwellings have been
replaced by an entire street of considerable length ; on both sides of which houses
for accommodating in the whole 112 families have been built, on the general plan
of H.R.H. The Prince Consort’s Exhibition Model Houses 1851, with an open stair-
case, giving access to each pair of upper floor tenements. The twenty-eight blocks
of four houses cost £487 each ; and after allowing for ground rent and all charges,
I can state, on the authority of the owner, that “they continue to pay upwards of
six, in fact nearly seven per cent. asa net return on the investment; and what,” he
adds, “is perhaps of more consequence, they are almost constantly let, and are ap-
preciated by the tenants, who, as a rule, are pretty stationary, and not migratory,
as that class frequently are.
- “We have before us in this case, an outlay of nearly £14,000 on new buildings
which contain 448 rooms, kitchens or sculleries included, yielding from 6 to 7 per
cent., whilst we have seen that the cost of obtaining and putting into sanitary con-
dition three old courts, which contain 275 rooms, and a lodging house with 40 beds,
has been upwards of £7000; and in that instance the return on the outlay has been
1} per cent., after deducting 14 per cent. for repairs, but making no allowance for a
sinking fund.”
' The Strand Building Company, on their houses for 25 families in Eagle Court,
has last year paid a dividend of 4} per cent. to the shareholders.
The Victoria Lodging House for married soldiers, built by an association of officers
of the battalion of Guards, near the Vauxhall Bridge Road, and containing 54 tene-
ments or 112 rooms, was the first practical result of the interest manifested in this
object by H.R.H. The Prince Consort in connexion with the Great Exhibition.
I allude to it partly as showing how justly the late Duke of Wellington estimated
the probable effects of placing that small building in the barrack yard at Knights-
bridge, when, as Commander-in-chief, he objected to the situation lest it should
cause a feeling of dissatisfaction in the army, with the want of any accommodation
for married soldiers ; an evil which the Marquis of Anglesea told me His Grace
apprehended the country to be then unprepared to remedy. Since that time,
separate dwellings for the married non-commissioned officers and men of the regiment
stationed at Chatham garrison, as well as for the engineers, have been built; and
during the present session of Parliament £30,000 have been voted for married
soldiers’ quarters.
The Windsor Royal Society, established in 1852, has now £9000 invested in new
cottages and in two lodging houses, the net returns from which enable them to
pay a dividend of 4 per cent. to the shareholders. ata aets ?
_ At Liverpool, on a range of dwellings for 23 families, built in Upper Frederick
Street after the general plan of The Prince Consort’s Exhibition model-houses,
43 per cent. is realized. The Association at Brighton has also built one block of
six houses on the same plan, and they pay a fair return on the cost.
Not fewer than twenty societies for providing improved dwellings for the work-
ing classes have, to my knowledge, been established in various provincial towns in
England; and whilst their operations are, without exception, beneficial in regard to
the occupants, the pecuniary results have varied considerably. In such under-
takings, competent skill and watchful supervision are most important elements
of success. In order to show what may be done with sound judgment and care-
ful management, I instance one example, in addition to those already given; and
200 REPORT—1860.
as that is taken from Scotland, I may observe that the urgent necessity for such
efforts is as great in the two sister kingdoms as it is in England.
The Pilrig Model Buildings, near Leith Walk, Edinburgh, were commenced in
1850 ; they consist of forty-four dwellings in three blocks, with access on both sides,
the upper floor tenements being approached from the opposite side to that on which
the ground floor tenements are entered. The greatest economy, consistent with
fitness and durability, was maintained in the construction, so that the total cost of
the forty-four houses, including drains, &c., was only £4052 15s. 9d., being on an
average about £92 per house, with scarcely any extras. The rent of the whole is
£303 19s. Od., varying from £5 5s. per house up to £9 15s., one half of them not
exceeding £6 6s, per house. Higher rents might have been charged had not the
committee desired to benefit a class of persons who could not afford to pay more.
After deducting all expenses,—feu duty £22 14s, 10d. ; insurance £6 12s, 6d, ; rates
and taxes £13 11s. 23d. ; repairs £13 4s. 7d.; management £21 6s, 3d., and paying
a dividend of 5 per cent. (less income tax) amounting to £196 16s, 6d.,—a balance
of £30 15s. 1d. was last year added to the sinking fund, from which a expenses,
such as painting and papering, are defrayed. This fund now amounts to about £150.
Having had the opportunity of seeing these houses when returning from the
Aberdeen Meeting last year, I refer to them with pleasure, as in many respects
worthy of imitation, and am not surprised at hearing that the demand for them is
generally at least six times equal to the supply.
The facts given thus far, refer exclusively to buildings in towns: with regard to
country districts, in which there is an equal necessity for exertion, the number
of improved cottages built by landed proprietors, as well as by other large em-
ployers of working people, such as manufacturers, railway and other public com-
panies, owners of collieries, mines, quarries, &c., has within the past twelve years
been very considerable; and it is to the increased feeling of responsibility in this
respect, as well as to more enlarged views of their own interest on the part of
employers, that we must mainly look for the much needed improvement in the
domiciliary condition of our rural population, and of those whose industrial em-
ployments are remote from towns.
In thus saying I do not forget that in many places Benefit Building Societies
present a useful machinery for enabling the working classes to obtain improved
dwellings, and that much good may result from judicious advice given to their
members in the selection of such plans as will enable them to obtain a healthy
and convenient home. In many places on the Continent, societies haye, within
the past ten years, been formed by philanthropic persons to build suitable houses
for working people, and likewise to afford facilities which enable their occupiers,
by small periodical payments in addition to the rent, to become the owners of their
own dwellings; the parties who advance the money being satisfied with 4 per
cent. interest, and the security of a sinking fund to pay off the capital. Such
buildings act as a savings’ bank, promoting sobriety and habits of forethought.
The beneficial effects resulting from a diffusion of sanitary knowledge amongst
the working population generally, and the importance of their being led to under-
stand and feel how greatly they are personally interested in the possession of a
wholesome dwelling, ought on no account to be overlooked by those who seek to
promote this object. Great evils which have arisen out of the selfish system,
pursued in some close parishes, of pulling down cottages in order to obtain relief
from a burden which is thereby thrown on a neighbouring parish, loudly call for
legislative interference.
In regard to populous towns, and the metropolis more especially, the facts which
have been stated lead to the conclusion, that the evils of overcrowding which
result from a demolition of large masses of dwellings of the working classes, effected
for the carrying out of popes improvements, can only be prevented by a parlia-
mentary enforcement of the construction of suitable buildings in the place of
those destroyed. A standing order of the House of Lords for the investigation of
such cases exists, but it appears thus far to have been practically a dead letter.
Whilst the pressure consequent on these destructions is felt by all classes of the
working population within their influence, facts have been brought to light by
experience, which conclusively prove that no efforts of societies, or of individuals,
can remedy the existing state of wretchedness, which is a consequence of sanitary.
ey he eer pg,
Bie
TRANSACTIONS OF THE SECTIONS. 201
defects and of overcrowding in the lowest class of dwellings. Nothing can effect
this much-needed remedy, but the extension to all tenements in towns and thickly
populated neighbourhoods, which are let at low weekly rents, of such legislative
interference as is universally admitted to have been of the greatest benefit in the
case of common lodging houses. Within the limited jurisdiction of the Corporation
authorities in the City of London, such a power was conferred in 1851, and it is judi-
ciously exercised under the supervision of the Medical Officer of Health, to the great
benefit of the poor, and with a marked diminution in the returns of mortality,
which have fallen since that date from 25 to 23 in 1000.
In the case of all new buildings, proper drainage should be enforced by authority,
prior to their commencement; the want of it is a most fruitful source of sickness,
and consequent expense to the public.
In the preceding notes my aim has been to draw only such conclusions as are
fully supported by the facts adduced. I cannot, however, omit glancing at this
subject from one other point of view, and that the most important in which it can
be presented for consideration, its bearing on our fellow-creatures as moral and
accountable beings. The experience of a right rev. prelate, when formerly rector
of St. Giles-in-the-Fields, one of the most thickly-populated and poverty-struck
parishes in London, must give peculiar weight to the following words: “The
physical circumstances of the poor paralyse all the efforts of the clergyman, the
schoolmaster, the scripture reader, or the city missionary, for their spiritual or their
moral welfare. .... Every effort to create a spiritual tone of feeling is counteracted by
a set of physical circumstances which are incompatible with the exercise of common
morality. Talk of morality amongst people who herd, men, women and children
together, with no regard of age or sex, in one narrow confined apartment! You
might a talk of cleanliness in a sty, or of limpid purity in the contents of a
cesspoo
Our prisons are no longer hot beds of fever* and of moral contagion as they
formerly were: may it not be asked in this Association, whether, with the advance
of science, the reproach to which England is justly amenable on account of the
domiciliary state of our labouring population, ought not to be effaced ? and, whilst
self-interested motives might be urged on many, the divine command, “thou shalt
love thy neighbour as thyself,” lays a serious responsibility on all who have it in
their power to promote an object so indispensable to the well-being of our poorer
neighbours.
MECHANICAL SCIENCE.
Tue President, mm opening the business of the Section, took occasion to refer
to the great loss Mechanical Science had sustained, since: the last Meeting, in the
deaths of Brunel and Stephenson. He then made some brief remarks on the recent
progress of Mechanical Science, especially in the use of heat to produce motive
power.
On the Mechanical Effects of combining Suspension Chains and Girders, and
the Value of the Practical Application of this System (illustrated by a Mo-
del). By P. W. Bartow, F.R.S.
* At the black assizes held in Oxford in July 1577, the gaol fever spread from the prisoners
to the court, and within two days had killed tne judge, the sheriff, several justices of the peace,
most ofthe jury, as well as a great number of the audience, and afterwards spread amongst the
inhabitants of the town.
202 REPORT—1860,
of successful small ones, which had given satisfactory results in every way, except
that they had failed after a short time for want of strength. Mr. J. Lawrence, in
1855, rifled a 63-inch gun with three shallow broad grooves, like an Enfield, and
fired a lead and zinc bullet, like the Infield. At an elevation of 5°, the range was
2600 yards—150 more than Sir W. Armstrong’s; but the gun burst after about
50 rounds. Mr. Whitworth, after making some excellent small arms and nine-
ounders, tried a large gun with 4 inches bore, and sides 9 inches thick; but
it burst. He then tried another, 11 inches thick, and it too burst. He had, how-
ever, since made a stronger cannon, whose success was absolute proof that the one
thing wanting in the other was strength. Capt. Blakeley explained his own
method of obtaining strength, which consists simply of building up the gun in
concentric tubes, each compressing that within it. By this means the strain is
diffused throughout the whole thickness of the metal, and the inside is not unduly
strained, as in a hollow cylinder made in one piece. As the whole efficacy of the
system depended entirely on the careful adjustment of the size of the layers, Capt.
Blakeley said he was not astonished that Sir W. Armstrong had lately failed
utterly in his attempts to carry it out, because he did not put on the outer layers
and rings with any calculated degree of tension; “they were simply applied with
a sufficient difference of diameter to secure effectual shrinkage,” to quote his own
words at the Institution of Civil Engineers. To show that the late failure by Sir
W. Armstrong did not disprove his, Capt. Blakeley’s, theory, he quoted oficial
reports of a trial of a nine-pounder made by himself in 1855, which showed an
endurance sevenfold that of an izon service gun, and threefold that of a brass gun,
as well as of an 8-inch gun, from which bolts weighing 4 cwt. had been fired, and
of a 10-inch gun which had discharged bolts weighing 526 lbs. Mr. Whitworth’s
last new 80-pounder was another instance of the successful application of Capt.
Blakeley’s pr:nciple. To quote Mr. Whitworth’s own words,—“ It was made of
homogeneous iron. Upon a tube having an external taper of about one inch, a
series of hoops, each about 20 inches long, were forced by hydraulic pressure. Ex-
eriments had enabled him to determine accurately what amount of pressure each
oop would bear. All the hoops were put on with the greatest amount of pressure
they would withstand without being injured. A second series was forced over
those first fixed.” This gun was so made at Capt. Blakeley’s suggestion, except-
ing that the rings were put on too tight, which might prove a cause of weakness,
The method of rifling adopted by Capt. Blakeley cannot be made intelligible with--
out a diagram; but it may be described as a series of grooves of very shallow
depth, so arranged as to exert a maximum force in the direction of the rotation of
the bullet with a minimum force in a radial or bursting direction. Capt. Blakeley
exhibited in the court of the building in which the Section met, a 66-pounder,
constructed on his own plans, from which he had thrown shells to a distance of
2700 yards, with only 5° of elevation, which was stated to be a range 300 yards
greater than that of Sir W. Armstrong’s 80-pounder.
On a deep Sea Pressure Gauge, invented by Henry Johnson, Esq.
Read by the Rev. Dr. Bootu, F.R.S., §e.
In deep sounding the pressure is too intense to admit of measurement by the com-
pression of any highly elastic fluid in a small portable instrument. Water, however,
possesses a slight degree of elasticity, and an instrument recording the compression
of an isolated portion of water by the pressure of the sea, will show the compression
of the water at the depth to which it has been lowered.
Mr. Canton, who in 1761 communicated his observations to the Royal Society,
found in water, compressed under a glass receiver, by the pressure of an additional
atmosphere, a diminution in bulk equal to one part in 21,740; and in water placed
under a receiver a similar expansion when the air in the receiver was exhausted.
Mr. Perkins, more recently, found a diminution of bulk of “>ths in water under a
pressure of 1120 atmospheres. The theory of increased pressure at great depths is
corroborated by a very interesting experiment made by the distinguished voyager
Rear-Admiral Sir James Clark Ross, who lowered, to a great depth, a bottle fitted
with a tube, with a cork suspended so as to enter the tube, if, as anticipated, the
water in the bottle, condensed under heavy pressure, should expand upon the raising
of the bottle and the removal of the pressure. Upon the return of the bottle to the
a a
. cation of a pressure of 1000 lbs. to the square inch on
TRANSACTIONS OF THE SECTIONS, 203
surface, it was found that the cork had been forced some distance along the tube, and
the amount of compression and of subsequent expansion were thus roughly estimated.
The pressure gauge exhibited, may, in its present form, be considered as a small
hydraulic press ; of which the ram is forced into the
cylinder by the increasing pressure of the sea when
sinking, and expelled by the expansion of the water
in the cylinder when rising. It consists of a small
tube or cylinder having at one end a tap through
which water is admitted; the tap having in addition
to the opening admitting water, a smaller opening
for the escape of air. At the other end of the cylin-
der is a packing-box, through which a round bolt or
solid piston passes. A scale by the side of the pis-
ton contains the degrees of compression, and an
index at the further end of the scale is drawn along
the scale by the piston when forced by increasing
pressure into the cylinder, and secured by a spring
in its position, where it remains when the piston
is pushed back by expansion of water in the cylinder
to its former position. The scale and index are pro-
tected by a tube screwed on to the cylinder, and the
cylinder is protected from the risk of indentation by
an outer tube. In an experimental instrument the
packing-box has remained water-tight underthe appli-
the piston; so that the isolation may be considered
sufficiently perfect, as in actual use this pressure on
water in the cylinder would be counterbalanced by
the external pressure of the ocean. The packing-box
is just large enough to admit the packing, which con-
sists of vulcanized caoutchouc rings, stretched upon
the piston, and consequently adhering closely to it.
A moderate application of the packing-box screw
presses these rings against the packing-box, and a
perfect isolation of the water in the cylinder is thus
obtained. A slight Jubrication of the rings, by the
addition of a small quantity of lard between them,
renders the amount of friction attending the motion
of the piston very trifling.
In ascertaining the pressure of water, the amount A—Cylinder.
of friction overcome should be added to the com- p__Pp,
pression recorded by the index, to obtain the total ¢_Opening in Tap for admission
amount of pressure. Some portion of the diminu- of water.
tion of bulk will probably be cccazioned by variation D—Opening in Tap for escape of
of temperature, and which causes a greater variation air.
in bulk at high temperature. As 4000 parts of sea- E—Packing-box.
water at the temperature of 86° Fahrenheit, con- F—Packing-box Screw.
tracted to 3987 parts at the temperature of 65°, G—Piston. 4
being ;}3;5 parts for 21°; while from the tempera- 5 hes of Se Pace
ture of 65° to 35°, the diminution to 3977 parts ~ ceustenduder.
was only at the rate of ;1°; parts for 30°,—the expansion and contraction of the
cylinder by yariation of temperature counteract the variation of water to avery small
extent, being about ;;4,5th parts for 40° Fahrenheit.
' The experimental instrument indicates a compression of about one part in 20,000
per atmosphere (estimated at 15 lbs.) at the temperature of 60° Fahrenheit.
The experiments will be varied by the use of a glass bulb with a long stem, finely
graduated, with a stopper of vulcanized caoutchouc, and in the tube an elastic ring
which is pushed during compression by the stopper towards the bulb, and remains
to mark the degree of compression.
204 REPORT—1860.
On Road Locomotives. By the Earl of Caituness.
The author referred to what had hitherto been done in this direction, and the
importance of attention being given to the construction of them as feeders to the
Railway system. He described the arrangement adopted in one which he had had
built for his own use, and which was successful. The carriage was exhibited in
action, and made several trips in the street under his Lordship’s guidance. In the
discussion which took place, great stress was laid on the importance of Parliament
reducing the turnpike tolls in respect of such carriages, which, in reality, were in
no way injurious to the road,
On Water Meters. By Davin Cuavwicx, Assoc. Inst. C.E., Manchester.
After pointing out the defects in some of the water-meters at present in use, he
described the high-pressure piston water-meter of Messrs. Chadwick and Frost,
which obviated these defects, and secured the correct measurement of water at all
pressutes and velocities of discharge, without the use of tumbling-levers, springs,
or flexible diaphragms, by a more compact and simple arrangement than any other
piston meter; but, without a diagram, it would be impossible to make its con-
struction intelligible.
A New Mode of obtaining a Blast of very High Temperature in the
Manufacture of Iron. By E. Cowper.
The blast is obtained by an adaptation of the principle of Siemens’s regenerative
furnaces. A hot blast of a temperature of 1800° Fahrenheit can readily be obtained,
and this without the destruction of iron tubes—-the substance used in contact with
the air being the most refractory fire-brick. This mode of obtaining a blast was
in successful operation at Messrs. Cochran’s iron-works. The temperature of the
blast could be regulated to any required degree. The heat might be obtained with
far greater economy than by any method hitherto known.
The Cylindrical Spiral Boiler. By Joux Evver.
{A communication ordered to be printed entire in the Transactions of the Sections.]
The object of the construction of this boiler is to obtain a form with all the useful
properties of the simple cylindrical high-pressure boiler on shore adapted to steam-
ships.
The following advantages appear to be attained over the ordinary marine boiler,
namely :—
1. A form of boiler capable of carrying higher pressure, and presenting more
heating surface, and of a more effective description from a given weight of material.
2. A boiler capable of being easier cleaned and repaired in both water and fire
spaces.
Wes A boiler capable of producing superheated steam to any practical temperature.
4. A less average specific gravity of water whilst working at sea with the usual
amount of feed and blow-off, and a more perfect combustion chamber, and better
formation of flue surface.
5. The pressures being altogether internal, the boiler is not liable to collapse, a
danger lately ably demonstrated by Mr. Fairbairn ; and as the diameters of the various
cylinders are reduced to the minimum size for permitting the tradesmen to pass
through, clean and repair them, the boiler, when formed of ordinary thickness,
possesses enormous strength without stays.
6. The expense of the boiler per square foot of heating surface is about the same
as that of the ordinary boiler, and is capable of carrying five times the pressure..
The general construction_of this boiler is as shown in the accompanying plans,
and as follows :—
There are twenty-four round boilers or tubes, of not less than nineteen inches in
diameter, twenty-two of these forming, when bound together, a cylindrical vertical
shell; the twenty-third, a centre boiler concentric to that shell; and the twenty-
fourth, a spiral coil-boiler winding spirally round between the centre boiler and those
es a
TRANSACTIONS OF THE SECTIONS. 205
composing the circumference shell: these boilers contain the water, and the spaces
between them the fire.
The feed water passes first into the spiral compartment, or No. 24, and from it
into the centre compartment, or No. 23, and then into each in rotation, and blows
off at the last compartment, or No. 1, thus rendering the water in No. 24 nearly pure
sea-water, and gradually from compartment to compartment more dense, till it blows
off at No. 1 at the usual density, and thus makes the average specific gravity of the
water less than usual.
The twenty-two outside boilers are 24 feet long, 19 inches diameter, and 55; of an
inch thick; the bottom ends are conical for 3 feet, and kneed outwardly to give a
larger diameter of furnace, say 12 feet diameter. There is a furnace-door for every
alternate tube, or say, eleven furnace-doors, equally divided round the base of the
boiler, giving great facility to the firemen for doing their work efficiently. In firing
it is proposed to charge all the fresh coal round the circumference of the fire, in order
that the hydrogen of the coal may be consumed separately from the carbon; and as
the furnace has great altitude, the combustion will be completed in vertical flames
from the coals, and will thus prevent the carbonic acid gas, given out from the com-
bustion of the carbon, coming so much in contact with and preventing the com-
bustion of the hydrogen, as is usual in ordinary furnaces.
The centre compartment, or No, 23, is 30 feet long, 34 inches diameter, and 2 of
an inch thick, with 3 feet at the bottom and top, conically reduced to 18 inches
diameter, forming a man-hole door; the upper end of this vertical tube forms a
reservoir for the steam of the whole twenty-four compartments, and acts as a super-
heating apparatus, and may be carried up the funnel to the extent necessary to
superheat the steam to 400 degrees; the steam-pipe is taken from the top of this
boiler to the safety-valve chest, fastened on the front of the boiler low down, which
serves as a water-trap during the discharge from the safety-valve chest, the steam-
pipe to the engines being taken off the same pipe at a higher level than the escape
steam. The spiral compartment, or No. 24, is about 100 feet long, 34 inches
diameter, and 2 of an inch thick, made of best iron boiler plate ; the ends are conical
for 3 feet, formed into man-hole doors; this spiral boiler makes four or five con-
volutions close round the centre one, and is bound close to the circumferential
boilers by hollow stay-bolts, and fastened to the centre one at each end only ; in the
same manner the steam and water flow through the whole boiler by these hollow
stay-bolts or rivets, and complete the entire circulation of water and steam; the
whole of these twenty-four compartments or boilers terminate at the bottom, about
1 foot below the fire-grate, and are supported on six stanchions from the ash-pit
beneath, making a free passage for the air under the great bar; the circumferential
compartments or boilers terminate at the top 6 feet above the ship’s deck, and have
each a man-hole door forming the cover; the funnel is made conical at the bottom
to embrace the internal diameter of the boiler-shell and draw off the smoke in the
usual manner: this completes the whole boiler proper; but in order to prevent
radiation of heat, a thin outer casing of iron is made (9 inches) clear of the boiler all
round, terminating about 7 feet from the stoke-hole floor ; and above, at the level of the
galley or funnel-house, this casing is lined with felt and thin wood to keep the deck
and the adjacent parts cool, and retain the heat. The twenty-two straight cylindrical
boilers or compartments are constructed in the sides by four plates 24 feet long and
16 inches broad, rolled to a 93-inch radius curve at the iron works, leaving no plate
setting for the boiler maker of this description.
The plates of Loiler No. 24, or the spiral compartment, are delivered flat by the
iron-maker, and are bent to the spiral curve by one blow of a large spiral concave
block falling upon a counterpart convex one, prepared by the constructors of the
boiler. This operation has been found to simplify the making of this spiral cylin-
drical boiler to about the same amount as the straight cylindrical boilers. The
conical ends are bent in the same manner as the spiral plates,‘and the whole work of
plate bending is reduced as far as possible to machine work. The products of com-
bustion, after leaving the furnace, have to travel spirally upwards a distance of 100
feet, and must of necessity be continually rotating during that time, and prevent the
possibility of any portion passing off without being brought frequently in contact
with the heating surface of the boiler; and will therefore be cooled down to the
206 REPORT—1860.
minimum temperature compatible with a given amount of cooling surface, or the
greatest quantity of heat extracted from the products of combustion, before their
escape to the atmosphere. The soot forming usually inside of boilers will not be so
injurious in this arrangement, as it will fall down through the external crevices, and
also between the spiral and the centre boilers into the furnace below, and be thrown
overboard with the ashes.
This spiral coil and all the heating surfaces will keep more clear of flue dust than
usual, and will consequently be more efficient in that respect, as well as save the
usual trouble and loss by sponging experienced in the ordinary tubular boilers at sea.
Also as the products of combustion must pass off at the rate of at least 7 feet per second
in this as in the ordinary boilers, it will take upwards of 14 seconds from the time
it leaves the furnace till it arrives at the top of the boiler; whilst if the boiler were
of the ordinary tubular type, it would pass in about two seconds along the whole
heating surface of the boiler; the gas has therefore seven times more time to give
out its heat, and its revolving tendency will not admit of the same strata of gas
passing along the passages after it is cooled down, as is the case with the ordinary
boiler, but will bring the hot products of combustion usually occupying the centre
of the tubes of a tubular boiler in contact with the cooling surfaces, and reduce the
whole products of combustion to one temperature before entering the chimney.
In cleaning the salt or sludge out of these boilers, the man- and sludge-hole doors
are taken off the top and bottom (and the hose with fresh water may be played down
through from the top, and the refuse run out at the bottom). ‘lhe man in charge
can also pass down through the whole boiler, the dimensions necessary for this pur-
pose being made the minimum and maximum of the various compartments of the
boiler; and are specially constructed to maintain to the engines steam at much
higher pressure than usual, in order to admit of a much larger amount of expansion
to be developed by the engines, which are all on the double cylinder expansive prin-
ciple. The constructors are now making the boilers for three steam-ships on this
principle, two of which are for carrying Her Majesty’s mails on the Pacific between
Valparaiso and Panama (as described by the writer at the meeting of the British
Association at Leeds); and it has long been his desire to be able to construct boilers
for marine purposes without stays, and with no surface exposed to the collapsing
tendency, which in so many cases has been the cause of loss of life aboard of steam-
ships. The boilers now described have no large flat surfaces and no stays, the whole
tendency of the pressures being to inflate the boiler plates, and, if possible, to give
them a stronger form; the smallest diameter is large enough to give access to the
men in charge, and the largest diameter 34 inches and 3 thick,—dimensions that can
carry several hundred pounds pressure on the square inch before rupture could take
place. Such a form the writer adopts, with great satisfaction to himself, as a con-
structor sending machinery abroad, where the usual form of boiler gives him consi-
derable anxiety. In comparing the construction of this boiler with that of the
ordinary tubular one, in the latter angle-iron ribs and stays now compose a large
portion of the weight and expense; contribute no heating surfaces; and if one stay
breaks, which is not an uncommon occurrence, the next is placed in great danger ;
and if it gives way, the whole may follow in rotation, and a serious accident be the
result. In the former boiler, however, the plates may be reduced to a very small
amount of thickness by tear and wear before explosion could be expected.
Having thus described the objects of the spiral boiler, it may not be out of place
to give the following statement of the comparative evaporative power and temperatures
of the gases in the furnace and chimney of the spiral boiler, with three of the ordi-
nary types of boiler now in general use.
Fig. 1 is a vertical section of the cylindrical spiral boilers as fitted on board the
Pacific Royal Mail Company’s steam-ships ‘San Carlos’ and ‘ Guayaquil,’ by
Messrs. Randolph, Elder, &c. Fig. 2 is a sectional plan of the same, taken near the
level of the water-line in fig. 1. Fig. 3 is a vertical elevational view of the same—
the exterior casings which surround the circumferential vertical tubes (and which
are shown in figs. 1 and 2) being in this view removed.
It will be seen from these figures that there are in these boilers 21 tubes in all,
viz. 19 circumferential vertical tubes, 1 central and 1 spiral tube.
The three types experimented upon were, first, a common cylindrical land boiler
—) =" =
TRANSACTIONS OF THE SECTIONS. 207
(figs. 1, 2, and 3) 33 feet long, 5 feet Ginches diameter, with two round flues 19 inches
diameter through the centre ; this boiler had 40 feet of heating surface to the nominal
horse-power of the engine: the two flues contained 20 feet, and the shell 20 feet per
nominal horse-power ; the furnace was below the boiler at the fore-end, had a fire-grate
of 26 square feet; the fire passed underneath the boiler to the opposite end from the
furnace, and returned along the sides, and then passed back again through the flues
to the chimney. The temperature above the centre of the fire was found to be, upon
one occasion, 3200°; at the top of the bridge 1730°; the temperature of the gases
Fig. 1. ; Fig. 2.
58
— a = SS EE
=6\=—b2—s5s—B-— Ba
deel tee Bay
NESS
gradually reduced as they passed back the remaining length of 26 feet under the
boiler and along the side flues, till they entered the centre flues at 1163°, and left
them at about 800°. Thus the furnace containing a surfece of 2 feet per nominal
horse-power reduced the heat about 1500°; the shell of the boiler behind the furnace,
of about 18 feet per nominal horse-power, reduced the temperature about 600°; and
the flues containing a surface of 20 feet per nominal horse-power reduced the tem-
perature about 350°. The temperatures of the gases in the flues were found to be
about the same in the centre as at the top; but at the bottom of the flue the tempe-
ratures of the gases were at the fore-end rather less than at the top, but towards the
Fig. 4. Fig. 5.
_ back end the temperature of the bottom of the flues reduced gradually below the
temperature at the top to the extent of 300°. Upon another occasion the tempe-
rature over the centre of the fire was found to be 3610°; at the top of the bridge
1739°; and the different temperatures of the flues were as indicated in fiz. 1, where
the average temperatures of the flues at B‘=$26°, B’= 879°, B’= 937°, B'= 959°,
and at B’ = 981°. Thetemperatures at the top of the flues at C? = 982, at C' = 1034°,
at C?=1087. The temperatures at the bottom of the flues at A’= 571°, A? = 603°,
A? = 678°, At=764°, A°=822°. It would therefore appear that, notwithstanding
the large amount of surface in this boiler, the evaporative power is very inferior, as
208 REPORT—1860.
\
the amount of heat taken out of the gases per square foot of heating surface is very
small; and that the natural conclusion is that the gases pass along in straight lines,
and only the thin stratum in contact with the surface is cooled down. In the results
of the spiral boiler (fig. 6) three times the quantity of heating surface was found to
reduce six times the quantity of gas from the same temperature of 3200°, to a tem-
perature of 4800 instead of 800°, showing that a more complete turning over of the
gases is much wanted in our land boilers. The water evaporated per hour in the
land boiler referred to was found by meter to be 2000 lbs., and the coal, best
Glasgow quality, found to be 300 lbs. per hour; making about 62 lbs. of water per
pound of coal. During the measuring of the water evaporated by the meter, indicator
diagrams of the engine were taken with a view to cal-
culate the weights of steam by the ordinary method, and
the calculations were found to agree with the meter;
these calculations can be repeated and substantiated at
any time. The second type of boiler tested was that of
the ordinary steam-boat horizontal tubular boiler (fig.
4); the example chosen was one in a first-class ocean
steamer; the temperature of the furnace was found to
be 3200°, and the inside of the funnel about 1100°. The
heating surface of this boiler was 22 feet per nominal
horse-power, and the water evaporated about 83 lbs. per
pound of coal, according to the calculation from the
diagrams. The coal consumed was about 20 lbs. per
square foot of fire-grate, of the best Glasgow coal.
The next example taken was that of a first-class ver-
tical tubular boiler (fig. 5), on Mr. David Napier’s
principle, now universally selected on the Clyde for river
steamers. This boiler had a surface of about 22 feet
per nominal horse-power; the temperature of the fire
was found to be about 3300°, and in the funnel 1160°;
the weight of water evaporated was found by calculation to be 83 lbs. per pound of
coal consumed, and the weight of combustion about twenty pounds square foot of
fire-grate. In the spiral boiler (fig. 6) of the ‘San Carlos,’ ‘ Guayaquil,’ and ‘ Prinz
van Orange’ the boilers were found to give the following peculiar results :—first,
that even with Scotch coal there was no smoke emitted from the chimney, and no
carelessness on the part of the fireman seemed to occasion the formation of smoke ;
second, that the boilers showed a bright furnace, indicating first-class draught; the
temperature of the funnel was found to be 480°, whilst the fire was at its greatest
energy. ‘he heating surface was, in the case of the ‘San Carlos’ and ‘ Guayaquil,’
2200 square feet, the coal consumed 1400 lbs. per hour, and the water evaporated
11 Ibs. per pound of coal consumed; the fire-grate contained about 76 square feet,
and the rate of combustion about twenty pounds per square foot of fire-grate. The
heating surface of the boiler was 18 feet per, nominal horse-power ; the coal consumed
was Glasgow best steam coal. The stoke-hole was found to be remarkably cool,
and the boiler, which was loaded to 52 lbs. on the square inch steam pressure, and
tested to 150 lbs. on the square inch water pressure, was found to be perfectly tight.
In the case of the ‘ San Carlos,’ I may mention that that ship has now steamed about
20,000 miles, and the vessel has not been in any one port more than three days ;
during that time she has been consuming soft Chili coal for a considerable part of
her voyage, and the merits of the long flue show a decided advantage in this boiler
over the ordinary tubular boiler for the native bituminous coal of South America.
In order to give a more extended form of the comparative evaporative power of
various flues and tubular boilers, the writer begs to lay before this Association the
accompanying Table. It shows several proportions of heating surface and evapora-
tive powers of several ships that have come under his notice. He can certify the
accuracy of most of these particulars, except that shown in the last column, which
is taken from Professor Rankine’s report on the performance of the ‘Thetis.’ This
vessel has about six times more heating surface in her boilers in proportion to the
coal consumed, than any example the writer is aware of. The boiler is Craddock’s
patent boiler, though that inventor’s name appears rarely to be mentioned in con-
i TRANSACTIONS OF THE SECTIONS, 209
nexion with the said vessel. Efficient, however, as this boiler must be as an evapo-
rator, it cannot possibly accomplish the quantity shown in this Table.
The theoretical quantity of water capable of being heated from 90°, and evaporated
at, say 212°, with an infinite quantity of heating surface and a perfect fire, is some-
where about 133 lbs. per pound of coal; whilst from the diagrams represented in
Professor Rankine’s report of the ‘Thetis’ performance, 18 lbs. weight appear to
a be about the quantity of water per pound of coal. This calculation I have made
from the diagrams published, and any party interested may repeat the calculations.
The calculation is made as follows : the area of the large cylinder, as shown in the
diagram, is 1380 square inches, or 9°583 square feet. The four revolutions of piston
marked on the diagram 493, 52, 53, and 52 revolutions per minute, with a stroke of
23 feet, or say 258°12 feet per minute, gives 258°12 X 9°583 X 60=146433 cubic feet
per hour. And if we take the average pressure shown in the four diagrams at the
end of the piston stroke, supposing the barometer to be 14°5 lbs., we find the weight
of that steam to be about 44 cubic feet per pound: this number therefore, divided
by 44, gives the quantity of steam as 3300 pounds per hour; to this must be added
2'> for contents of ports and clearance, which makes 3465 pounds of steam.
This clearly gives the weight of the steam per hour given out of the cylinders
after the work is performed, to this therefore must be added the quantity of heat
that must have disappeared during the performance of the work; this, in the case
of the ‘Thetis,’ is about + of the entire heat; we must therefore add +, or say
3465-+693=4158 pounds of water must have been raised from a temperature of
about 100° and evaporated, or say 18 lbs. of water to the pound of coal said to be
consumed ; this result is about equal to 20 lbs of water evaporated at 212°, to the
pound of coal consumed; a quantity quite absurd.
Comparisons of certain Results obtained fram Certified Diagrams of Steamers ‘Elk,’ ‘ Earl of
Aberdeen,’ ‘ Valparaiso,’ ‘ Pride of Erin,’ ‘ Inka,’ ‘ Europa,’ ‘ Cambrian,’ and ‘ Thetis.’
areas
Tec’
oe OS a —-
t Elk. yo Velbig P ride cf Inka. | Europa.| Cambrian, Thetis.
Nominal H.P. ......... 250 380 320 | 400 | 80 648 472 80
Indicated ditto ......... 780 780 826 | 960 | 272 {1207 | 1072 226
Proportion of indicated
H.P. to nominal II.P. 3°28 2°05 2581; 2:4 | 3:8 1:863| 2°272 a 2°82
i. : ft F Two 52) | wo { |T'wo 28 ? ne 21
Diameter of Cylinder... 57in. | 7 Oin. { Two 90 | 72{ Two 48\ 7 20 775 One 42
L 5 ft. 6 in. 6ft. 5ft. |5ft.6in.| 3ft. 8ft. | 7ft. Gin. 2ft. Gin.
Number of Strokes per
MBTMITIUCE ........esseceseee 25 175 24 Ze ae 153 16 52 F
‘B oilers, Flue or Tubular} Tubular. Flue. Flue. | Flue, | Flue. | Flue. | Flue. ete rs fe
Area of Fire-grate...... 144ft. 190ft. | 130ft.| 252 50 314 247
2 ea of Heating Surface 4000 4300 2400 | 4400 | 480 | 7000 | 5400 About 4000
Coals consumed per hr.) 3360lbs. 3584 2520 | 4928 | 672 | 5100 | 4480 226
Quality of Coal .........|Glasgow best.|Newcastle.| Welsh. | Welsh. | Welsh. |Welsh.| Welsh. Good.
‘Steam evaporated per
Mlb. of Coal ............ 7354 6°87 774 | 7159] 81 ah 7509 |15 Ibs. about.
Estimate, water evapo-
EU isos assccce ves 81 74 8-6 79 9:0 8°5 8°3 18]bs.
Voal consumption per
indicated H.P.......... 4071 4:358 | 3:05 | 5°126] 2:47 | 4:2 4:17 1:018
fire-grate per nominal
MEE Etecieoscesesceee Coeceee 576 5) 406] *63 625] 484] 536
It therefore appears that in the report referred to, the indicated power of the said
diagrams may be correct, but the coals said to be consumed per indicated horse-
_ power per hour, namely 1°08, must be wrong ; and before a proper comparison could
be established between the merits of the ‘ Thetis’ ’ boiler and that of any other boiler,
a correct trial of the former would be necessary. In the mean time we have but to
1860. 14
210 REPORT—1860.
consider that the report of Professor Rankine was based upon one hour’s consumption
of say 230 lbs. of coal, and compare that with a mass of boiler, water and firebrick,
weighing 20 tons, at a temperature of say 300°, it is evident that the mass of heat in
proportion to the coal consumed is so great, that no conclusion should be made from
such an experiment; also, that when the quantity of coal said to be consumed, viz.
230 lbs., is compared with area of fire-grate, say 40 square feet, it is evident that
the result should not be depended upon, as no ordinary comparisons could be made
of the condition of the fires before and after the experiment. In conclusion, let me
ask of every party present to consider the trial trips of steam-ships and boilers in
their true lights, and before drawing any inferences from such short trials, make a
perusal of results obtained from sea voyages. The evaporative power and economy
of boilers is one of the most important subjects for this Society to consider. We
need only refer to the able Report drawn up by the Steam Shipping Committee of
the British Association, to show how mixed up the question of the relative efficiency
of the boiler and engines is generally considered. Indeed the American navy
returns form the only reports showing the evaporative power of the boilers in this
list, and the whole merit of a good evaporating boiler is often sacrificed to the cha-
racter of the engines. With regard to the ‘ Thetis,’ I would recommend any mistake
to be remedied as soon as possible, as there are many contracts, involving much
responsibility, formed in consequence of this report, that will lead to serious loss and
disappointment to the steam-shipping interest, and the engineering profession of this
country.
On the Density of Saturated Steam, and on the Law of Expansion of Super-
heated Steam. By WiivtAM Farrearry, LL.D., F.RS. §c.
This ee contained a continuation of the experiments detailed in a paper read
by My. Fairbairn at the Aberdeen Meeting, and which had been carried on in con-
junction with Mr. Tate. Experimental determinations had been obtained of the
density of steam fully confirming the anticipations of Mr. Thomson and Mr, Ran-
kine, that the vapour of water does not exactly obey the gaseous laws. They show
that the density of saturated steam is always greater than that given by the gaseous
laws, even for temperatures as low as 136° Fahr., and at pressures below that of the
atmosphere. The experiments at present extend over a range of temperature from
186° Fahr. to 292°, or from 2°6 to GO Ibs. pressure per square inch, The general
result obtained is expressed in the following formule, which closely agrees with the
experiments,
49513
v=25'62+ Pp— 7 6 8 ee iy ol) Sa erie (.)
49513
iP => ——_—_, — 0:72 ’ ‘ ‘ cece ‘ ’ . . , 2.
oe. Ce
where v is the specific volume or ratio of the volume of the steam to that of the
water which produced it, at the pressure P, expressed in inches of mercury.
On the subject of superheating steam, the experiments throw some light, which _
the author hopes to follow up by a special series of experiments. They show that
within a short distance of the maximum temperature of saturation the rate of ex-
pansion is variable, being higher than that of a perfect gas near the saturation point,
and rapidly decreasing, till at a point at no great distance above the temperature of
saturation it becomes sensibly identical with that of a perfect gas,
On an Atmospheric Washing Machine. By Joun Fisuer.
The action of this machine was derived from streams of air forced through the
water from below. The author in his paper observed, that for effectual use the water
must never be of a higher temperature than 140° of Fahrenheit. It was stated
that machines on this principle, driven by steam-power, had been for some time
ast in successful overation for cleansing the soiled laces at Messrs, Fishers’ manu-
actory at Nottingham,
TRANSACTIONS OF THE SECTIONS. 211
On Giffard’s Injector for Feeding Boilers. By WitttaM Froupe.
In this instrument a jet of steam taken from the boiler and issuing from a pro-
perly tapered orifice, is met by and enveloped in a regulated supply of water, either
cold or of limited temperature.
The column formed by the combination of water and steam is made to impinge
on the aperture of a similarly tapered orifice, of rather smaller area, connected with
the feed-pipe; and penetrating this orifice, it flows in a continuous stream into the
boiler.
The rationale seems to be as follows :—were it possible to condense such a jet of
steam by a simple abstraction of temperature, it would collapse into a jet of water
having only ;5;th of its previous sectional area, its particles, however, retaining
the same weight and velocity, and therefore the same momentum for each unit of
time which they had possessed as steam. And since the momentum of a jet is the
exact dynamic equivalent of the pressure which produces it, this water-jet would
possess a momentum equal to that of a jet of equal diameter taken from a boiler
having 1700 times the pressure of that from which itself had issued as steam, and
wouid be capable of penetrating a boiler having a pressure enlarged almost in the
same proportion.
In the injector the water which is added condenses the steam and becomes incor-
porated with it, forming a compound jet which possesses for each unit of time the
same momentum which the jet of steam possessed. And if the supply of water be
duly regulated, the sectional area of the compound jet may be precisely adapted to
the orifice of the feed-pipe.
Now were that orifice equal in area to the steam-jet orifice, and were a jet of
water allowed to issue from it under the same pressure which discharged the steam,
the water-jet would have the same momentum for each unit of time as the
steam-jet had, and therefore as the compound jet derived from it; and the two
would precisely neutralize one another when brought into opposition. If, however,
the steam-jet orifice be the larger of the two, then the jet derived from it, if reduced
by condensation to the diameter of the smaller, will be the stronger in the same
proportion, since it will possess the momentum due to the larger area of pressure ;
it will therefore drive back the water which is striving to escape from the feed-pipe,
and will pass as a continuous stream into the boiler.
The water supply is considered to be correctly adjusted when the passage takes
place without an overflow of steam or water; but the test is deceptive; for an over-
flow of steam merely implies that the supply of water is barely sufficient to condense
the steam into a jet as small in section as the feed-pipe orifice ; an overflow of water
merely implies that though the steam is fully condensed, the supply of water has
enlarged the compound jet to a section exceeding that of the feed-pipe orifice.
In reality the operation should be brought as near as possible to the latter limit ;
for though it will indeed seem to be proceeding quietly and properly in all the inter-
mediate stages, it will be found that the compound jet, when not so enlarged as to
fill the feed-pipe orifice, possessing its full momentum in a smaller section, will have
energy enough to take up with it and carry into the boiler a considerable quantity of
air, wasting thus not only its own power, but in a high degree that of the engine
also, when it is a condensing one, since it encumbers the air-pump with extra duty.
On a Process for covering Submarine Wires with India-rubber
for Telegraphic purposes. By WavteR Hatt.
The author exhibited a model of his machine, which effected the object by wind-
ing strips of rubber, and moistening the same with naphtha during the process of
covering ; the wire thus formed being covered with a thread of vulcanized India-
rubber, and the whole afterwards subjected to a temperature of 140°. The wires
thus covered were protected with a plaited covering of hempen cord, into which
longitudinal steel wires were introduced for the purpose of giving strength,
Suggestions relative to Inland Navigation.
By Professor Hennessy, F.R.S,
The fact that the forces operating in canal and river navigation are so different
14.*
912 REPORT—1860.
from those of sea navigation, shows that a totally different construction may be
adopted for the vessels employed. The short heavy barges with clumsily rounded
bows and broad sterns should be entirely abandoned. Boats of very great length,
compared to their breadth cf beam, may be used for canals with considerable economy
of power in proportion to the cargo. The highest perfection of lines may thus be
attained so as to secure the smallest amount of resistance to motion, and the least
disturbing effect to the canal banks. For this object also a selection might be made
among the varieties of the screw propeller, which would obviate any lateral disturb-
ance of the water and drive it backwards rather than sideways. In some cases the
above suggestion as to the shape of boats could not be realized without lengthening
locks, and wherever these are numerous, jointed vessels, like those proposed for the
Indian rivers, might be employed. The loss of water in passing locks would be the
same as fora train of entirely separate boats, while the resistance to propulsion
would be considerably less. Steam-propelled boats thus constructed would proba-
bly realize the twofold result of economy in power and increase of speed to the
highest limit advisable for traffic in heavy goods.
On the Longitudinal Stress of the Plaie Girder. By Catcorr REILty.
On Suggestions for an Electro-Magnetic Railway Break.
By Dr. B. W. Ricuarpson.
On the Character and Comparative Value of Gutta Percha and India-
rubber employed as Insulators for Subaqueous Telegraphic Wires. By
S. W. Sitver.
After pointing out some of the mistakes prevalent on the subject of the insula-
ting properties of india-rubber, a comparison was made by the writer between the
relative advantages and the insulating power of india-rubber and gutta percha
respectively. Insulation in the case of a submarine cable depends upon two causes
or properties of the bodies used:—1. The specific non-conducting power of the
substance ; 2. its impermeability, by which the original insulating conditions may
be maintained. The insulating power of gutta percha is very high; but, in the
case of a submarine telegraph cable, its porosity renders it a very imperfect insulator
in practice. India-rubber, with lower specific insulating properties (as would
appear from experiments made in dry air), is, nevertheless, practically a far more
efficient insulator, by reason of its complete impermeability, while in addition it
ossesses a lower inductive capacity. It was pointed out that impermeability is as
important a question as specific non-conductility in an insulator of such cables; and
that even if a substance could be found insulating perfectly in dry air, it still might
in practice be of questionable utility for submarine lines, owing to its porosity, as
was the case with gutta percha. There was now no difliculty in covering wires
with india-rubber.
On Improvements in Iron Ship-building. By W. Simons.
Diagonal Beams.—Each range of beams is placed in the reverse diagonal direction
to the range of beams, above or below it, so that collectively the vessel’s beams con-
stitute a complete system of horizontal diagonal trussing.
Fore and aft along the middle of each range of beams are riveted strong iron
clamps; and along the centre of the ’tween decks are secured in long lengths along
the inside of the frames, strong, angle, back-to-back iron clamps. For these beams,
various degrees of obliquity may be adopted; but the angle chosen by the author (re-
presented in a plan which was exhibited) will probably best answer the combined
purpose of a beam and diagonal truss.
It is a well-known fact that the beams, as at present placed, do not prevent the
straining of a vessel, but merely form a connexion between the vessel’s sides and a
framework to support the deck. ;
The hatchways and mast partners are framed in the usual manner, and the masts
are wedged on both the upper and lower decks,
ae
TRANSACTIONS OF THE SECTIONS. 913
The decks may be laid also diagonally in a reverse direction to the beams, and may
be edge-bolted throughout and made of hard wood.
This system of decks, by which the objectional butts are entirely avoided, is
more particularly adapted for 4 or 5-decked battle-ships, where the strain from the
weight of the guns and action of propeller is found to strain and twist them so
much.
Iron Waterways are formed in the following manner. Every iron beam is made with
a vertical projection on its upper edge at both ends; this projection is about 7 inches
deep and 20 to 40 inches broad, according to the tonnage of the vessel. On the
upper edge of these projections are riveted double-angle iron. On the front or bosom
of these projections is riveted, in long lengths along the beams, heavy angle-iron,
say 6+5. Over this are then placed the plates which form the waterway ; these are
rounded over on their inside edge, which is riveted to the heavy angle-iron inside ;
the top of the plate is double riveted down to the double angle-iron on each beam
end: the outer edge is riveted to the angle-iron along the sheer strake, where it is
securely iron-caulked.
Round any angle-iron frames necessary to project through the waterway is fitted
exactly a doubling piece, which is securely caulked round the frame.
The usual iron stringer and wood water-ways are thus superseded, and this iron
water-way, it is submitted, forms a serviceable and complete box gunwale.
The beam-end projections form also stronger and improved knee fastenings, par-
ticularly to the upper part of the beam, where hitherto in iron vessels such a knee
has not yet been adopted, although considered essential in timber vessels.
In fact, for the convenience of stowage and passengers’ berths, the knee or the
under side of all iron beams on this principle might be dispensed with. Of course,
this waterway can be adopted with either diagonal beams or common beams.
Plating diagonally with two thicknesses of plate, each in the reverse diagonal
direction to the other, or with one thickness in combination with frames arranged in
the reverse diagonal direction.
In the former case, both thicknesses of plating will be riveted together, and the
butts arranged to make shifts with cach other; by this mode of construction the
present vertical frames become unnecessary, and even the keel not essential. In
place of these are substituted, in long lengths, internal longitudinal stringers,
clamps and keelsons, about 5 feet asunder; these would have the advantage over the
present internal longitudinal fastenings, of being fitted and secured directly to the
skin of the fabric through which they may be fastened every 3 inches; by this
system it is not requisite that the plate butts be more securely riveted than the rest
of the external skin, as it will be evident that such a vessel could not break asunder
at the butts or vertical joints like a postage-stamp, as was described in the case of
many late wrecks of iron ships constructed on the present mode.
Timber vessels of 2000 tons have been planked on. this principle with complet
success.
Keelsons made in the following manner have greater strength as a backbone, and the
necessary rigidity to receive the thrust of diagonai central hold stanchions or trusses.
Every floor, or alternate floor, is made to project up in the middle in the form of a
square. Round these projections are fixed angle-iron, to which the upper and side
plates of the keelson are secured in the form of abox. Bilge and sister keelsons may
be also formed on the same principle.
The keelson required by Lloyds for their highest classed iron vessel, has only four
rivets to secure it to the top of each floor ; consequently, when by accident the strength
_of the bottom is tested, these rivets of course break, leaving the strength of the floors
and keelson as a backbone untested, while with the above improved keelson, the
floors are so well fastencd to the keelson, that they must break before the keelson
will yield.
Diagonal Central Hold Stanchions or Trusses.—in place of the common vertical
hold and ’tween-deck pillars or stanchions in two lengths at present in use in wood
and iron vessels, most of which are made portable, and intended merely for the sup-
port of the deck, the inventor forms, from stem to stern, a range of diagonal trussing
in bars of one length, the joint object of which is to strengthen he fabric and sup-
port the deck,
914 REPORT—1860.
These trusses are placed to cross each other in a reverse diagonal direction, so as
to resist either a tensional or compressive strain; they are made of 5 X 2 flat iron, are
securely riveted above to every second or fourth upper deck-beam, and below, a butt
on, and are secured to the upper side of the keelson. They are riveted together at
their points of intersection, and where they cross the line of the old beams, a double
central back-to-back 7 X 6 angle-iron clamp is riveted to every truss and beam. If
desired, a similar angle-iron clamp may be riveted along at the junction of their
upper extremities with deck beams.
The angle of these stanchions is about 60°, that being found best suited to the
convenience of the hatch arrangement. The hatchways and masts can easily be left
clear.
It is submitted, these stanchions form a central range of diagonal trussing at a
part of a vessel requiring support, and which hitherto has not had such; they will be
of great service in connecting together two strong frameworks, namely a vessel’s
bottom, and her upper deck platform. The writer also places the diagonal stanchion
in athwartship direction; this he has found reduces vibration in steamers, besides
clearing the screw-shaft. On these principles of construction, the writer’s firm have
nearly completed at Glasgow a 900-ton iron Indiaman, named ‘The R. Mackenzie ;’
and he is glad to state that the result of such practice has more than realized the
expectation formed from the theory; and respecting the element of expense, he finds
that such a vessel costs £2000 less than a Thames or Mersey-built timber ship of
the same size and class.
Plate Butt Frames.—In an iron vessel plated in the common manner, the writer
uses butt-frames. In the place of the usual mode of securing the vertical joints of
the external plating on an iron internal strop between the frames, they are secured
upon a frame in the following manner. There is bent round the exterior of every
alternate angle-iron frame, a long continuous plate of some breadth and thickness,
as the ordinary butt-strop ; this plate is punched before being fixed to the frame ; the
plate-butts or vertical joints are then arranged to be riveted only on this continuous
butt-frame.
If longer outside plating be desired, every third frame may be constructed as a
butt-frame.
If preferred, the continuous butt-strop may be placed between the frames, in one
length, from keel to gunwale.
By either of these modes of securing the butts of common plates, no short butt-
strops are required, and it is evident that a vessel having her butts or vertical joints
so secured, is greatly increased in point of strength, and that there is little or no
liability to break asunder at those points,
Ceiling.—For the purpose of increasing the strength of iron vessels, the ceiling
from the bilge keelson up to the gunwale is made of angle-iron or flat iron in one
Jength placed diagonally and from 12 in. to 10 ft. apart, tailing from the centre of
the vessel to the extremities. The port side of a ship being reverse to the starboard
side, these diagonal ceiling bars are riveted to the reverse angle-iron of every frame,
and their extremities secured to the gunwale angle-iron and bilge keelson.
These iron ceiling side trusses, in conjunction with my centrai range of stanchion
trussing, yield great strength without occupying space, and both can be adopted
with advantage in timber vessels and in battle-ships. If preferred, these diagonal
ceiling bars may be of wood in iron vessels.
Tron Masts.—The writer plates iron masts and spars diagonally from top to bottom,
the plates winding round the entire length and riveted together. He also forms an
iron mast of diagonal spiral lattice-work riveted together at their points of inter-
section.
If desired, such a mast may be stayed transversely in its interior throughout. The
writer also fixes winches to iron masts, with their spindles through the sides of the
mast, the aperture required for such spindles being compensated by an internal
doubling plate.
War Ships.—Between the seams of the external planks of wood battle-ships
exposed to shot, the writer inserts iron or steel plates, in thickness from 1 to 2 inches,
and in breadth the entire thickness of the planks to which they are secured ; these
being in long lengths, are bolted vertically to the planks above and below them, and
TRANSACTIONS OF THE SECTIONS. 215
besides increasing the strength of the vessel, will form a resistance to shot or shell :
they may be placed from 6 or 8 inches asunder.
In wood battle-ships, he also fastens along the interior sides of their gun decks,
vertical iron plates, from 1} to 23 inches thick, close secured and bolted through the
side. Such are for the purpose of resisting the shot after it has spent its force in
penetrating the external wood side.
For the same purpose, he places fore and aft along the interior of the gun decks
of wood battle-ships, angled metal shields, the apex of each being in the centre line
of the gun ports, and bolted there through the side of the ship: where the upper and
lower edges of these shield plates join the beams above and below, they are strongly
bolted to the beams and to each other.
In an iron battle-ship or ram, he builds the side of the hull above water and plates
it with 2 or 23-inch thick iron or steel. Outside of this he timbers, planks, fastens,
and caulks the wood side of a battle-ship, not for the purpose of strength, but for a
resisting medium, in which a common ball may spend its force before coming into
contact with the internal angle- plated shields, which it is submitted will then turn
aside the ball from penetrating into the interior.
These angled shields answer also for beam knees, the weight and cost of which
may be dispensed with.
It is submitted, that owing to such angled shields, the reduced thickness of shield
plates protected by the timber side, the diagonal arrangements of four tiers of beams,
and the central diagonal trussings, an iron battle ram so constructed would have less
displacement, greater strength, more buoyancy, greater speed, and be more credit-
able to the engineering science of this country than those now building at an expense
of 11 million, the designs of which were not thrown open to public competition,
although the Exhibition building, St. George’s Hall, and some of the first engineer-
ing structures in England, are the result of such a course.
A Novel Means to lessen the frightful Loss of Life round our exposed
Coasts by rendering the Element itself an Inert Barrier against the Power
of the Sea; also a Permanent Deep-water Harbour of Refuge by Artifi-
cial Bars. By Admiral Taytor.
On Street Railways as used in the United States, illustrated by a Model of a
Tramway and Car, or Omnibus capable of conveying sixty persons. By
G. F. Train, of Boston, U.S.A.
In America such a car is drawn by a pair of horses. The tramway is laid in
the centre of the street, and the rail is so shallow that it offers no obstruction
whatever to carriages crossing it. In wide streets two such tracks are laid down,
one for the going and the other for the returning traffic. Mr. T. stated that in the
cities of America the system was in constant use, and was now an absolute neces-
sity there. He saw no difficulty in carrying out the system in our English
towns or in London. Where there were inclines, an extra horse would be used ;
and where a street was not wide enough for two tracks, he would put down asingle
track there, and bring the trafic back by a line laid in a parallel street. He had
received a concession to bring out his system in Birkenhead, and he hoped by
September to be able to show itin operation there. All he required was leave from
the authorities in any town to lay down his trams and run his carriages.
On a Mode of covering Wires with India-rubber.
By Messrs. WERNER and C. W. SIEMENS.
The authors exhibited a very ingenious machine for accomplishing this object.
These gentlemen use no solvent or heat whatever, but take advantage of the pro-
perty which india-rubber possesses of forming a perfect junction when newly-cut
surfaces are brought together under pressure. The core or wire, with the ribbon
of rubber applied to it longitudinally, is pushed into an orifice, which serves as a
guide to carry them into the machine, so that the superfluous rubber is cut off by
what may be termed a revolving pair of scissors, formed by a disc of steel with a
sharp edge revolving excentrically against a stationary plate, and immediately, by
216 REPORT—1860.
means of two grooved wheels, the edges are pressed together, and thus the wire
becomes encased in a perfect tube of india-rubber. As many additional tubes as
may be desired can be then ee on. The machine is also applicable to the coat-
ing of wires with what is known as Wray’s Compound, with yulcanized India-
rubber and other compound substances containing India-rubber.
APPENDIX.
PuHysIoLoey.
On the Deglutition of Alimentary Fluids.
By Professor J. H. Consett, M.D.
In this paper the author describes two distinct forms of deglutition ; that while the
alimentary bolus is propelled with rapidity over the epiglottis, fluids can flow in
two streams, one at each side of the epiglottis and of the aryteno-epiglottic folds,
without the danger incidental to its passage over the central aperture of the larynx.
He believes that such occurs in the newly-born infant and mammal during suction ;
it can take place in the sipping of fluids, swallowing of the saliva, and even during
drinking in a continuous Speake. Ordinary drinking is accomplished by gentle
muscular movements, which should not be confounded with the gulping of fluids.
In gulping, the fluid is rapidly and forcibly propelled backwards through the
isthmus of the fauces, each gulp requiring a separate act of deglutition; such act
much resembles the deglutition of solids. The author contends that when the infant
or mammal seizing and retaining the nipple, sucks in the fiuid in an almost con-
tinuous stream, the process of respiration is not totally interrupted, as should
occur if the fluid absolutely passed in the middle line over the epiglottis; it is
argued that the salivary secretion is swallowed safely during sleep ; fluid carefully
introduced into the mouth of persons in a state of insensibility, passes into the
pharynx; fluid poured gently into the mouth of a patient whose head rests upon
one side, flows backwards by a gentle act of deglutition, which is chiefly performed
in this instance by the muscles of the corresponding side; fluids cannot be shaped
like solid food into a definite form ; alimentary drinks must be subject, in their course,
to the laws which regulate the passage of fluids in other cases; the root of the
tongue being narrow and the organ convex on its upper surface, fluids must naturally
have a tendency to flow from the middle line to either side ; during the mastication
of solid aliment, the juices expressed by the action of the teeth and pressure of the
tongue, rapidly escape backwards, so that the bulk of the mass is considerably
diminished before the deglutition of the solid part is attempted; during inflam-
matory affections of the tonsillitic glands, the swallowing of fluids is attended with
difficulty, while a moderately sized portion of solid aliment, which proceeds in
the middle line, may be transmitted with comparative facility; when a single
gland is much inflamed, deglutition is chiefly performed at the opposite side.
In experiments made by the author on the dead body, fluid poured upon the
dorsum of the tongue passes backwards into the pharynx in two streams, through the
grooved channels situated at each side of the epiglottis and aryteno-epiglottic folds.
From all these considerations, it is inferred that in the living body, during the
deglutition of fluids, the uvula falls forward upon the tongue in front of the epi-
glottis; thus both uvula and epiglottis afford protection to the respiratory apparatus.
The fluid is divided by the uvula into two currents, which descend at each side
of the root cf the tongue, under the half arches of the palate, as water flows under
the arches of a bridge; and such is the principal use of the uvula. The anato-
mical arrangements in the human body are perfectly adequate for the transmission
of fluid in this safe manner. The anatomy of the porpoise, in which the larynx
rises for several inches above the level of the tongue, affords a strong confirmation of
this view, which is further sustained by instances in which the epiglottis has been
destroyed, wounds of the throat, &c. The distinctness of the two forms of deglu-
tition is also indicated by the fact that the mouth may be filled with food, and yet
drink can be swallowed without displacement of the solid aliment; the newly-born
infant can perform suction in a perfect manner; on the other hand, the power of
swallowing solid focd is gradually acquired, and the organs of deglutition are trained
by successive steps to the safe performance of this process,
‘= =?
INDEX I.
TO
REPORTS ON THE STATE OF SCIENCE.
OBJECTS and rules of the Association,
XVil.
Places and times of mecting, with names
of officers from commencement, xx.
Treasurer’s account, xxiv.
Members of Council from commence-
ment, Xxv.
Officers and Council for 1860-61, xxviii.
Officers of Sectional Committees, xxix.
Corresponding Members, xxx.
Report of Council to Gexeral Committee
at Oxford, xxx.
Report of Kew Committee, xxxi.
Report of Parliamentary Committee, xliv.
Recommendations adopted by the Ge-
neral Committee at Oxford :—involv-
ng grants of money, xlv; applications
for reports and researches, xlvi; ap-
plications to Government or public
Institutions, xlvill; communications to
be printed entire among the Reports,
xviii.
Synopsis of grants of money appropriated
to scientific objects, xlvii.
General statement of sums paid on ac-
countof grants for scientific purposes, 1.
Extracts from resolutions cf the General
Committee, liv.
Arrangement of General Mectings, liv.
Address by the Right Hon. the Lord
Wrottesley, ly.
Actinozoa, British, list of, compiled by
Rh. M° Andrew, 233 :—Zoantharia, 233 ;
Aleyonaria, Ctenophora, 234.
Aérolites and bolides, catalogue of, by
R. P. Greg, 50.
Agricultural College (Royal), Cirencester,
Prof. Buckman on the growth of plants
in the Botanical Garden of the, 34.
Anderson (Rey. Dr.), report on the exca-
vations in Dura Den, 32.
Annelida, British marine, list of, compiled
by R. M°Andrew, 226 :—Turbellaria,
227 ; Bdellomorpha, Bdellidea, Scolices,
Gymnocopa, Chectopoda, 227.
Arachnida, British marine, list of, com-
piled by R. M*Andrew, 226.
Atherton (Charles), report on steam-ship
performance, 193.
Atmospheric electricity, Prof. W.Thomson
on an electrometer for observing, 44,
Balloon ascents to great altitudes, report
on the scientific objects to be sought
for by, 43.
Botanical Garden of the Royal Agricul-
tural College, Cirencester, report on
the experimental plots in the, by Prof.
Buckman, 34.
Brachiopoda, British, list of, compiled
by R. M*Andrew, 222.
Brewster (Sir D.), report on the scientific
objects to be sought for by continuing
balloon ascents, 43.
Bridges, experiments on the effect of
vibratory action and long-continued
changes of load upon wrought-iron
girders of, by W, Fairbairn, 45.
Buckman (Prof. J.), report on the expe-
rimental plots in the Botanical Garden
of the Royal Agricultural College, Ci-
rencester, 34.
Caithness (the Earl of), report on steam-
ship performance, 193.
Cephalopoda, British, list of, compiled by
R. M°Andrew, 218.
Ccelenterata, British marine, list of, com-
piled by R, M*Andrew, 232.
218
Congruences, the period-equations con-
sidered as, 127.
— , binomial, solution of, 155.
, 2 =1, mod gp, 155.
—, cubic and biquadratie, 158.
> quadratic,—indirect methods of
solution, 159.
, general theory of, 161.
, extension of Fermat’s theorem, 163.
——, imaginary solutions of a, 165.
——, having powers of primes for their
modulus, 165.
, binomial, having a power of a prime
for their modulus, 167.
Crop plants, experiments made at the
Agricultural College, Cirencester, on
the growth of, 37.
Crustacea, British, list of compiled by
R. M‘Andrew, 222 :—Brachyura, 222 ;
Anomoura, Stomapoda, Amphipoda
Normalia, 223; Amphipoda Aber-
rantia (Lemodipoda), Isopoda Aber-
rantia (Anisopoda), 224 ; Isopoda(Nor-
malia), Entomostraca, 225 ; Cirripedia,
226,
Devonian fish, new forms of, 32.
Dredging Dublin Bay, Prof. Kinahan’s
report on, 27.
Dublin Bay, Prof. Kinahan’s report on
dredging, 27.
Dufferin (Lord), report on steam-ship
performance, 193.
Dura Den, report on the excavations in
the yellow sandstones of, by the Rev.
Dr. Anderson, Prof. Ramsay, Prof.
Nicol, and D. Page, 32.
Earth, researches on the physical and
chemical changes of the, 175.
Echinodermata, British, list of, compiled
by R. M*Andrew, 230 :—Crinoiea,
Ophiuroidea, Asteroidea, Echinoidea,
Holothuroidea, 230.
Egerton (Hon. Capt.), report on steam-
ship performance, 193.
Electricity, atmospheric, Prof. W. Thom-
son on portable apparatus for observ-
ing, 44.
Electrometer, atmospheric, self-recording,
report on the construction of a, by
Prof. W. Thomson, 44.
, portable, for atmospheric observa-
tion, by Prof. W. Thomson, 44.
Entozoa, British marine, list of, compiled
by R. M°Andrew, 229 :—Nematoidea,
Trematoda, Acanthocephala, Cestoidea,
Cystica, 229.
Fairbairn (W.), experiments to determine
REPORT—1860.
the effect of vibratory action and long-
continued changes ofload upon wrought-
iron girders, 45; report on steam-ship
performance, 193.
Fauna, British marine invertebrate, list
of, by R. M°Andrew, 217.
Fireballs and meteorites, catalogue of, by
R. P. Greg, 48.
Fish, fossil, in the yellow sandstone of
Dura Den, 32.
Flax plant, on the growth of the, 42.
Foraminifera, British marine, list of, com-
piled by R. McAndrew, 234.
Forbes (Prof. J. D.), report on the scien-
tific objects to be sought for by con-
tinuing balloon ascents, 43.
Fossil remains in the Dura Den yellow
sandstone, 32.
Gasteropoda Prosobranchiata, British,
Het of, compiled by R. M*Andrew,
18.
—— Opisthobranchiata, British, list of,
compiled by R. M*Andrew, 219.
— Nudibranchiata, British, list of,
compiled by R. M*Andrew, 220.
Gauging of water by triangular notches,
Boe report on the, by J. Thomson,
Geological phenomena, on the effects of
long-continued heat, illustrative of,
175.
Girders, wrought-iron, experiments on,
by W. Fairbairn, 45.
Gladstone (Dr. J. H.), report on observa-
tions of luminous meteors, 1.
Glaisher (James), report on observations
of luminous meteors, 1.
Grasses, experiments made at the Agri-
cultural College, Cirencester, on the
growth of, 35.
Greg (R. P.), report on observations of
luminous meteors, 1, 22; catalogue of
meteorites and fireballs from A.D. 2 to
A.D. 1860, 48.
Harcourt (Rev. W. Vernon), report on
the effects of long-continued heat,
illustrative of geological phenomena,
175.
Heat, long continued, Rev. W. V. Tiar-
court’s report on the effects of, illus-
trative of geological phenomena, 175.
Holoptychius, fossil, some new particu-
lars on the structure and figure of the
genus, 32.
Hydrozoa, British marine, list of, com-
piled by R. M*Andrew, 232:—Cory-
nide, Sertularide, Calycophoride,
Physophoride, 232; Medusidz, Lucer-
naridz, 233.
4
INDEX I.
Invertebrate fauna, British marine, list
of the, by R. M°Andrew, 217.
Killmey Bay, shells obtained in, 29.
Kinahan (Prof.), report on dredging in
Dublin Bay, 27.
Kingstown Bay, shells obtained in, 29.
Lloyd (Rev. Dr. H.), report on the scien-
tific objects to be sought for by con-
tinuing balloon ascents, 43.
Lowe (E. J.), report on observations of
luminous meteors, |.
Marine invertebrate fauna, British, list
of, by R. M°Andrew, 217.
M‘Andrew (Robert), list of the British
marine invertebrate fauna, 217.
M°Connell (J. E.), report on steam-ship
performance, 193.
Messageries Impériales of France, table of
results of performances of steam-ships
in the service of, 200.
Meteor, very remarkable, observations of
aj. 12;
Meteorites and fireballs, catalogue of, by
R. P. Greg, 48.
Meteors, luminous, report on observa-
tions of, by J. Glaisher, Dr. Gladstone,
R. P. Greg, and E. J. Lowe, 1.
——, luminosity of, from solar reflexion,
15; onthe luminous trains left by, 15;
on the motion of the tail of, 17 ; on the
duration of, 17 ; on the hypothesis that
the intensity of the light of, is caused
by the oxygen in the atmosphere, 18;
list of 168 bolides observed from 1841
to 1853, 19; results of the most re-
markable as regards their general ob-
served direction, 21.
Mollusca, British, list of, compiled by R.
McAndrew, 218.
Moorsom (Vice-Admiral) on the perform-
ance of Steam-vessels, the functions
of the screw, and the relations of its
diameter and pitch to the form of the
vessel, 172.
, chairman of the committee on steam
ship performance, second report, 193.
Napier (J. R.), report on steam-ship per-
formance, 193.
Naval architecture, Admiral Moorsom
on, 172.
Nicol (Prof. J.),report on the excavations
in Dura Den, 32.
Numbers, Prof. Smith’s report on the
theory of, 120; residues of the higher
powers, researches of Jacobi, 120; neces-
sity for the introduction of ideal primes,
219
121; elementary definitions relating to
complex numbers, 122; complex units,
123; Gauss’s equations of the periods,
125; the period-equations considered
as congruences, 127; conditions for
the divisibility of the norm of a com-
plex number by a real prime, 129;
elementary theorems relating to ideal
factors, 131; classification of ideal num-
bers, 132; representation of ideal num-
bers as the roots of actual numbers,
133; the number of classes of ideal
numbers, 134; criterion of the divisi-
bility of H by A, 136; “exceptional ”
primes, 138; Fermat’s theorem for
complex primes, 139; M. Kummer’s
law of reciprocity, 140; the theorems
complementary to M. Kummer’s law
of reciprocity, 141 ; complex numbers
composed of roots of unity, of which
the index is not a prime, 145; appli-
cation to the theory of the division of
the circle, 147; application to the last
theorem of Fermat, 148; application
to the theory of numerical equations,
152; tables of complex primes, 153 ;
solution of binomial congruences, 155 ;
solution of the congruence «*=1,
mod p, 155; cubic and biquadratic
congruences, 158; quadratic congru-
ences—indirect methods of solution,
159; general theory of congruences,
161; extension of Fermat’s theorem,
163; imaginary solutions of a congru-
ence, 165; congruences having powers
of primes for their modules, 165; bi-
nomial congruences having a power of
a prime for their modulus, 167 ; primi-
tive roots of the powers of a prime,
168; case when the modulus is a power
of 2,168; composite modulus, 168 ;
binomial congruences with composite
modulus, 169; primitive roots of the
powers of complex primes, 170; addi-
tions to Part I., 170.
Page (D.), report on the excavations in
Dura Den, 32.
Paris (Admiral), report on steam-ship
performance, 193.
Plants, Professor Buckman’s report on
the growth of, in the Botanical Garden
of the Royal Agricultural College,
Cirencester, 34.
Polyzoa, British marine, list of, compiled
sae M°Andrew, 230:—Infundibulata,
230.
Porifera, British marine, list of, compiled
by R. M°Andrew, 235.
Protozoa, British marine, list of, compiled
by R. M°Andrew, 234.
220
Pteropoda, British, list of, compiled by
R. M°Andrew, 220,
Railways, experiments on cast and
wrought-iron girders, by W. Fairbairn,
45.
Ramsay (Prof. A. C.), report on the ex-
cayations in Dura Den, 32.
Rankine (Prof.), report on steam-ship
performance, 193.
Roberts (Richard), report on steam-ship
performance, 193.
Russell (J. Scott), report on steam-ship
performance, 193.
Sabine (General), report on the scientific
objects to be sought for by continuing
balloon ascents, 43.
Sharpey (Dr.), report on the scientific
objects to be sought for by continuing
balloon ascents, 43.
Shells, list of species obtained in Kings-
town and Killiney Bays, 29.
Ships. iron-cased, remarks on, by Admi-
ral Moorsom, 174.
Ships, steam, Admiral Moorsom on the
performance of, the functions of the
screw, andthe relations of its diameter
and pitch to the form of the vessel,
172.
Shootng-stars, on, 1.
Smith (Prof. H. J. S.), report on the
theory of numbers, Part IT., 120.
Smith (Wm.), report on steam-ship per-
formance, 193.
REPORT—1860.
Sponges, British marine, list of, compiled
by R. M°Andrew, 235.
Stafford (Marquis of), report on steam-
ship performance, 193,
Steam-ship performance, second report
of the committee on, 193.
Steam-vessels, Admiral Moorsom on the
performance of, the functions of the
screw, and the relations of its diameter
and pitch to the form of the vessel,
172.
Sykes (Colonel), report on the scientific
objects to be sought for by continuing
balloon ascents, 43,
Thomson (James), interim report on the
gauging of water by triangular notches,
21
Thomson (Prof. W.), report on the scien-
tific objects to be sought for by con-
tinuing balloon ascents, 43; report on
the construction of a self-recording
atmospheric electrometer for Kew Ob-
servatory, and portable apparatus for
observing atmospheric electricity, 44.
Walker (Rev. Prof.), report on the scien-
tific objects to be sought for by con-
tinuing balloon ascents, 43.
Weeds, experiments made at the Agri-
cultural College, Cirencester, on the
growth of, 39.
Wright (Henry), Hon. Secretary of the
committee on steam-ship perform-
ance, second report, 193,
INDEX IT.
221
INDEX II.
TO
MISCELLANEOUS COMMUNICATIONS TO THE
SECTIONS.
AccaptaNn language, Dr. Hincks on
the, 156.
Aconite, E. R. Harvey on the mode of
death by, 133.
Adie (P.), description of an instrument
for measuring actual distances, 59 ; de-
scription of a new reflecting instrument
for angular measurement, 59.
Africa, South-Central, Dr. Livingstone’s
discoveries in, 164.
Agricultural labourers, H. J. Ker Porter
on the best plan of cottage for, 194;
H. Roberts on, 196.
Air-pump, improved form of, W. Ladd
on an, 65.
Alcohols and tea, the action of, contrasted,
by Dr. E. Smith, 145.
Algeria, Rev. H. B. Tristram on the geo-
logical system of the central Sahara
of, 102.
Alimentary fluids, on the deglutition of,
216.
, J. Ball on systematic observations
of temperature in the, 37.
, Capt. Cybultz on a set of relief
models of the, 155.
Alps, Savoy, Prof, Favre on circular
chains in the, 78.
America, British North, Dr. Hector on
the geology of Captain Palliser’s expe-
dition in, 80.
American, British North, exploring expe-
dition, Capt. J. Palliser on the course
and results of, 170.
Anesthetics, Dr. C. Kidd on the nature
of death from the administration of,
136.
Anca (Baron F.) on two newly disco-
vered ossiferous caves in Sicily, 73.
Andalusite, Connemara, analysis of, by
Prof. Rowney, 71.
Andrews (Prof.) on ozone, 66.
Angular measurement, P. Adie on anew
reflecting instrument for, 59.
Animals, domestic, J. Crawfurd on their
influence on the progress of civiliza-
tion, 155,
Animal and a plant, J, Hogg on the di-~
stinctions of an, 111,
Animalcules in human milk, G, D. Gibb
on, 131.
Antarctic expeditions, Capt. Maury on, 44,
Antarctic regions, Capt. Maury on the
climates of the, 46,
Aryan or Indo-Germanic theory of races,
J. Crawfurd on the, 154.
Assyrian inscriptions, Dr. Hincks on the
language of the, 156.
Asia, Central, R. von Schlagintweit on
the aboriginal tribes of, 176.
Aspergillum, or watering-pot Mollusk, L.
Reeve on the, 120,
Assyrio-Babylonian
Hincks on the, 35.
Atkinson (T, W.) on the caravan routes
from the Russian frontier to Khiva,
Bokhara, Kokhan, and Yarkand, 153
on the caravan route from Yarkand to
Mai-Matchin, 154.
Atlantic (North) telegraph, geography of
the, by Col. Schaffner, 178.
Atmospheric electricity, Prof. W. Thom-
son on, 53.
Atmospheric waves, W. R. Birt on, 38.
Atmotic ship, Hon. W. Bland on an, 60.
Atomic weight of oxygen, Prof. W. A.
Miller on the, 70.
Atomic weights, atomic volumes, and
properties of the chemical elements,
J.J. Coleman on some remarkable re-
lations existing between the, 66.
Avicula contorta beds and lower lias in
the S. of England, Dr. T. Wright on
the, 108.
lunar year, Dr,
Ball (John) on a plan for systematic
observations of temperature in moun-
tain countries, 37.
Barlow (P. W.) on the mechanical effects
of combining suspension chains and
girders, 201.
Barometer, J. A. Broun on the laws of
the diurnal variation of the, within the
tropics, 20,
.
b]
222
Barometers, M. R. von Schlagintweit on
thermo-barometers compared with, at
great heights, 50.
Barometric pressure, Admiral FitzRoy on
the areas or lines of, 41.
Barometric readings, M. R. von Schlagint-
weit on some results deduced from com-
parisons of the boiling-point with, 50,
Beale (Prof.) on the ultimate arrangement
of nerves in muscular tissue, 125.
Becquerel (E.) on a pile with sulphate of
lead, 59.
Beetles, mummy, J. O. Westwood on, 123.
Belcher (Capt. Sir E.) on the manufacture
of stone-hatchets, &c. by the Esqui-
maux, 154.
Berbers or Brabers of Morocco, E. Schla-
gintweit on the, 177.
Bernoulli’s theory of gases as applied to
their internal friction, their diffusion,
and their conductivity for heat, on the
results of, 15.
Bile, Dr, Thudichum on the physiological
relations of the colouring matter of the,
147.
Binocular instruments, A. Claudet on the
means of increasing the angle of, 61.
Bird (Dr.) on the deodorization of sewage,
66.
Birt (W. R.) on the forms of certain lunar
craters indicative of the operation of a
peculiar degrading force, 34; on atmo-
spheric waves, 38.
Blackwall’s (J.) work on British spiders,
notice of, 120,
Blakeley (Capt.) on rifled cannon, 201.
Bland (The Hon. W.) on an atmotic ship,
60.
Blast of very high temperature, E. Cow-
per on a new mode of obtaining a, 204.
Blenheim iron ore, E. Hull on the, 81.
Boats for inland navigation, Prof. Hen-
nessy on, 212.
Boiler, cylindrical spiral, J. Elder on the,
204.
Boilers, W. Froude on Giffard’s injector
for feeding, 211.
Bone and osseous grafts, M. Ollier on the
artificial production of, 143.
Bone-caves near Tenby, Rev. G. N.
Smith on three undescribed, 101.
Booth (Rev. Dr.) on the relations be-
tween hyperconic sections and elliptic
integrals, 4; on a new general method
for establishing the theory of conic sec-
tions, 4; on an improved instrument
for describing spirals, 60; on the true
principles of an income tax, 184; ona
deep sea pressure gauge invented by
Mr. H. Johnson, 202.
REPORT—1860.
Boric triethide, a new organic compound,
Dr. Frankland and B. Duppa on, 69.
Boron, Dr. Frankland on a new organic
compound containing, 69.
Bose (C. Moritz Von), remarks on the
volume theory, 71.
Brennecke (Dr.) on some solutions of the
problem of tactions of Apollonius of
Perga by modern geometry, 4.
Brewster (Sir David) on some optical il-
lusions connected with the inversion of
perspective, 7; on the influence of
very small apertures on telescopic vision,
7; on microscopic vision, and a new
form of microscope, §; on the decom-
posed glass found at Nineveh and other
places, 9; on a nail found in Kingoodie
quarry, 73.
British coasts, J. M. Mitchell on the im-
portance of the herring fishery on the,
191,
British Islands, Admiral FitzRoy on the
storms of the, 39.
Brodie (Prof. B. C.) on the quantitative
estimation of the peroxide of hydrogen,
66.
Brodie (Rev. P. B.) on the stratigraphical
position of certain species of corals in
the lias, 73.
Broun (John Allan) on results of obser-
vations in the Observatory of His High-
ness the Rajah of Travancore, 20;
on the diurnal variations of the mag-
netic declination at the magnetic equa-
tor, and the decennial period, 21; on
a new induction dip-circle, 23 ; on mag-
netic rocks in South India, 24; on a
magnetic survey of the west coast of
India, 27; on the velocity of earth-
quake shocks in the laterite of India, 74.
Buccinum, J. Lubbock on the develop-
ment of, 139.
Buckland (Frank T.) on the acclimatiza-
tion of animals, birds, &c., 113.
Buckton (G. B.) on some reactions of
zinc-ethyl, 66.
Caithness flagstones, Sir P, de M, G.
Egerton on a new form of ichthyolite
discovered by W. Peach in the, 78.
Caithness (Earl of) on road locomotives,
204.
Cale-spar, on rings seen in viewing a light
through fibrous specimens of, 19.
Cambridge, Rev. J. B. P. Dennis on the
mode of flight of the Pterodactyles of —
the coprolite bed near, 76.
Camera, solar, A. Claudet on the prin-
ciples of the, 62.
Canada, short notice of the progress of
INDEX II.
natural science in, by P, P. Carpenter,
109.
Cannon, rifled, Capt. Blakeley on, 201.
Carpenter (Mary) on educational help
from the Government grant to the de-
stitute and neglected children of Great
Britain, 184.
Carpenter (P. P.) on the progress of na-
tural science in the United States and
Canada, 109.
Carus (Prof. V.) on the value of “ deve-
lopment” in systematic zoology and
animal morphology, 125; on the Lep-
tocephalidz, 125.
Caustics produced by reflexion, Prof.
Lindelof on the, 14.
Cayley (.4.) on curves of the fourth order
haying three double points, 4.
Chadwick (David) on water meters, 204,
Chadwick (Edwin) on the physiological
as well as psychological limits to mental
labour, 185; on the economical results
of military drill in popular schools,
185.
Cheese, Prof, Voelcker on poisonous me-
tals in, 73.
Chemical elements, J. J. Coleman on
some remarkable relations existing
between the atomic weights, atomic
volumes, and properties of the, 66.
Chemical geology, I. S. Hunt on some
points in, 83.
Chest, A. MacLaren on tie influence of
exercise on the expansion of the, 142.
China, W. Lockhart on the mountain
districts of, and their aboriginal in-
habitants, 168.
Chloride of calcium, gradual reduction of
hydrate of cresyl into hydrate of phenyl
and other compounds through the
agency of, Dr. Gladstone on, 69.
Chloride of sodium and nitrate of baryta,
when equivalent proportions of, are
mixed together in solution and diffused,
four salts exist contemporaneously in
the liquid, Dr. Gladstone on, 69.
Chloroferm, Dr. C. Kidd on the nature of
death from, 136.
Chromatic dispersion, M. Ponton on the
laws of, 16.
Chromatic properties of the electric light
of mereury, Dr. J. H. Gladstone on
the, 13.
Chromoscope, J. Smith on the, 65.
Cinchona, V. Hurtado on the geographi-
cal distribution and trade in the, 162.
Civilization, on the influence of domestic
animals on the progress of, 155.
Classification, Prof. V. Carus on the value
of development in, 125.
223
Clarke (A.) on a mode of correcting the
errors of the compass in iron ships, 28.
Claudet (A.) on the means of increasing
the angle of binocular instruments, to
obtain a stereoscopic effect in propor-
tion to their magnifying power, 61 ; on
the principles of the solar camera, 62.
Classification of animals, J. R. Greene on
embryology in reference to the, 152.
Climates of the antarctic regions, Captain
Maury on the, 46.
Clutterbuck (Rev. J. C.) on the course of
the Thames from Lechlade to Windsor,
as ruled by the geological formations
over which it passes, 75.
Coal-field, Tynedale, on the, 86.
Coal-fields, North Staffordshire, W.
Molyneux on fossil fish from the, 88.
Cody (Patrick) on the trisection of an
angle, 4.
Coleman (J. J.) on some remarkable re-
lations existing between the atomic
weights, atomic volumes, and proper-
ties of the chemical elements, 66; on
the destruction of the bitter principle
of chyraitta by the agency of caustic
alkali, 66.
Collingwood (Prof. Cuthbert) on the re-
spiration of the nudibranchiate mol-
lusea, 113; on the nudibranchiate mol-
lusea of the Mersey and the Dee, 113;
on recurrent animal form, and its sig-
nificance in systematic zoology, 114,
Colour-blindness, Dr, J, H. Gladstone on,
12.
Colour, J. Smith on the chromoscope, to
verify certain opinions as to the cause
of, 65.
Colouring matter of the bile, Dr, Thudi-
chum on the physiological relations of
the, 147.
Colours, Dr. Gladstone on his own per-
ception of, 12.
Colours of the spectrum, Prof. Maxwell
on an instrument for exhibiting any
mixture of the, 16.
Connemara, Prof. Rowney on the analysis
of some minerals of, 71.
Coprolite bed near Cambridge, Rey. J. B.
P. Dennis on the pterodactyles of the,
76.
Corals in the lias, Rev. P. B. Brodie on
the stratigraphical position of certain
species of, 73.
Corbett (Prof. J. H.) on the deglutition of
alimentary fluids, 216,
Cornwall and Devon, W. Pengelly on the
chronological and geographical distri-
bution of the Devonian fossils of, 91,
Cottage. for agricultural labourers, H.
224
J. K. Porter on the best plan of, 194 ;
H. Roberts on, 196.
Cowper (E.) on a new mode of obtaining
a blast of very high temperature in the
manufacture of iron, 204.
Crawfurd (John) on the influence of
domestic animals on the progress of
civilization, 155; on the Aryan or
Indo-Germanic theory of races, 154.
Crustacea, British well shrimps, new,
Rev. A. R. Hogan on, 116.
Cull (R.) on certain remarkable deviations
in the stature of Europeans, 155; on
the existence of a true plurafof a per-
sonal pronoun in a living European
language, 155,
Cumberland and Northumberland, J. A.
Knipe on the Tynedale coal-field and
the whin-sill of, 86.
Curves of the fourth order, having three
double points, A. Cayley on, 4.
Cybulz (Captain) on a set of relief models
of the Alps, &c., 155.
Cydippe, J. Price on, 120.
Daubeny (Dr.) on the elevation theory
of volcanos, 75; on the final causes of
the sexuality of plants, in reference to
Mr. Darwin’s ‘Theory, 109; experi-
ments on equivocal generation, 115.
Death by aconite, on the mode of, 133;
from the administration of anesthetics,
on the nature of, 136.
Deglutition of alimentary fluids, Prof. J.
H. Corbett on the, 216.
De la Rue (Warren) on a new acetic
ether occurring in a natural resin, 71;
on the isomers of cumol!, 71.
Dennis (Rev. J. B. P.) on the mode of
flight of the Pterodactyles of the copro-
lite bed near Cambridge, 76.
Devon and Cornwall, W. Pengelly on the
chronological and geographical distri-
bution of the Devonian fossils of, 91.
Devon, South, E. Vivian on the climate
of, 56.
Devonian fossils of Devon and Cornwall,
W. Pengelly on the chronological and
geographical distribution of the, 91.
Dingle (Rev. J.) onthe corrugation of strata
in the vicinity of mountain ranges, 77.
Dip-circle, induction, new, J. A. Broun
on a, 23.
Dispersion, chromatic, M. Ponton on the
laws of, 16.
Distances, P. Adie on an instrument for
measuring, 59.
Dolomites and gypsum, T. S. Hunt on, 83.
Donegal, north of, Prof. Harkness on the
metamorphic rocks of, 79,
REPORT—1860.
Dowden (R.) on the effect of a rapid cur-
rent of air, 39; on a plant poisoning a
plant, 110; on local taxation for local
p poses, 191.
Draper (Dr. H.) on a reflecting telescope
for celestial photography, erecting at
Hastings, near New York, 63; on the
intellectual development of Europe,
considered with reference to the views
of Mr, Darwin and others, 115.
Dresser (Dr. C.) on the morphological
laws in plants, 110; on abnormal forms
of Passiflora czerulea, 110.
Drift, triassic, from the neighbourhood of
Frome, C. Moore on the contents of, 87.
Du Boulay (M.) on the meteorological
phenomena of the vernal equinoctial
week, 39.
Duppa (B.) on a new organic compound
containing boron, 69.
Durham (Arthur E.) on the nature of
sleep, 129.
Earnshaw (Rev. S.) on the velocity of
the sound of thunder, 58; on the tri-
plicity of sound, 58.
Earth’s crust, Rev. J. Dingle on the for-
mation of the, 77.
internal structure, Prof. Hennessy
on studying the, from phenomena ob-
served at its surface, 35.
Earthquake shocks, in the laterite of In-
dia, J. A. Broun on the velocity of, 74.
Earthquakes and volcanic phenomena, T.
S. Hunt on the theory of, 84.
Education of the destitute and neglected
children of Great Britain, Mary Car-
penter on help from the Government
grant for the, 184,
, E, Chadwick on the physiological
as well as psychological limits to mental
labour, 185,
Egerton (Sir P. de M, G.) on the ichthy-
olites of Farnell Road, Forfarshire, 77;
on a new form of ichthyolite discovered
by Mr. Peach, 78.
Eggs of Buccinum, on the development
of, 139,
Elder (John) on the cylindrical spiral
boiler, 204,
Electric fluid, Rev, T. Rankin on the dif-
ferent motions of, 30.
light, M. Serrin on an automatic
regulator for, 19,
light of mercury, Dr. J. H. Gladstone
on the chromatic properties of the, 13.
telegraphs, submarine, C. W. Sie-
mens and M, Werner on the principles
and practice involved in dealing with
the electrical conditions of, 32,
OO a
INDEX Ii.
Electrical foree, Sir W. S. Harris on, 28.
indications during day thunder-
storms, Prof. W. Thomson on, 54.
vacuum tubes, Prof. W. B. Rogers
on the phenomena of, 30.
Electricity, atmospheric, Prof. W. Thom-
son on, 53
Electro-magnetic railway break, on an,
212,
Electrolysis across glass, W. R. Grove on
the transmission of, 69.
Embryology, J. R. Greene on, with refer-
ence tc the mutual relations of the sub-
kingdoms of animals, 132,
Equations, indeterminate linear, Prof. H.
J. S. Smith on systems of, 6.
Equinoctial week, vernal, M. Du Boulay
on the meteorological phenomena of
the, 39. :
Esquimaux, on the habits and manners of,
and on their manufacture of stone-
hatchets, 154.
Ether, Dr. C. Kidd on the nature of death
from, 136.
Ethnological boulders and their probable
origin, Rey. Dr. Hincks on, 156.
Ethnology, R. von Schlagintweit on some
of the Aborigines of India and High
Asia, 175.
Exercise, A. Maclaren on its influence in
physical growth and development, 142.
Eyes, Prof. W.B. Rogers on their in-
ability to determine which retina. is
impressed, 18.
Fairbairn (William) on the density of
saturated steam, and on the law of ex-
pansion of superheated steam, 210.
Farnell, Forfarshire, J. Powrie on a fos-
siliferous deposit near, 89.
Farnell Road, Forfarshire, Sir P. de M. G.
Egerton on the ichthyolites of, 77.
Faroé Isles, some remarks on the, by Col.
Schaffner, 178.
Fauna, invertebrate, of the lower oolites
of Oxfordshire, J. F. Whiteaves on the,
104,
Favre (Prof. A.) on circular chains in
the Savoy Alps, 78.
Fawcett (Henry) on the method of poli-
tical economy by Dr. Whewell, 191;
on cooperative societies, their social and
political aspect, 191.
Fern stems, Dr, G. Ogilvie on the struc-
ture of, 112.
Fish, fossil, from the N. Staffordshire coal-
fields, W. Molyneux on the, 88.
, remains of, in the triassic drift in
the neighbourhood of Frome, C, Moore
on, 87,
1860.
225
Fishes found in the old red sandstone de-
posits of Farnell, Forfarshire, Sir P. de
M. G, Egerton on, 77, 89.
Fisher (John) on an atmospheric wash-
ing machine, 210.
Fishery, herring, J. M. Mitchell on the
importance of the, 191,
FitzRoy (Admiral) on British storms, 39.
Fluids, alimentary, on the deglutition of,
216.
Forfarshire, Sir P. de M. G, Egezton on
the ichthyolites of Farnell, 77; J.
Powrie on a fossilferous deposit near
Farnell, 89.
Formosa, island of, W. Lockhart on the,
169,
Fossil remains in two newly-discovered
caves in Sicily, Baron Anca on, 73.
Fossil fish, from the North Staffordshire
coal fields, W. Molyneux on the, 88.
fishes, of the old red sandstone of
Farhell, Forfarshire, Sir P. de M, G.
Egerton, 79, 89.
Fossiliferous deposit near Farnell, in For-
farshire, J. Powrie on a, 89.
Fossils, British North American, Dr. Hec-
tor on, 80. :
, Devonian, of Devon and Cornwall,
W. Pengelly on the chronological and
geographical distribution of the, 91.
of the lower oolites of Oxfordshire,
J. F. Whiteaves on the, 104.
of the triassic drift in the neigh-
bourhood of Frome, C. Moore on, 87.
Foster (Dr. M.) on the theory of cardiac
inhibition, 129.
Fox (J. J.) on the province of the statis-
tician, 191.
Frankland (Dr.) on a new organic com-
pound containing boron, 69.
Freshwater deposit at Mundesley, J.
Prestwich on the, 90.
Frome, C. Moore on the fossils of the
triassic drift in theneighbourhood of, 87.
Froude (William) on Giffard’s injector for
feeding boilers, 211.
Fulgora candelaria, J. O. Westwood on a
lepidopterous parasite on the, 124,
Gages (Alphonse) on some transforma-
tions of iron pyrites in connexion with
organic remains, 79.
Galvanic battery with sulphate of lead,
M. E. Becquerel on a, 59.
Ganoids, notice of one representing a new
genus, by W. Molyneux, 89.
Garner (Robert) on certain alterations in
the medulla oblongata in cases of pa-
ralysis, 129; on the structure of the
Lepadide, 130,
15
226
Garnet, Connemara, analysis of, by Prof.
Rowney, 71.
Gaskoin’s (Mr.) pathological collection of
shells, 116.
Gases, Bernoulli’s theory of, as applied
to their internal friction, their diffusion,
and their conductivity for heat, Prof.
Maxwell on the results of, I5.
, ©. M. von Bose on the theory of
volumes which separates them from
other bodies, 71.
Gauge, deep-sea pressure, Rev. Dr. Booth
on a, 202.
Geinitz (Dr.) on snow crystals, 79 ; on the
Silurian formation in the district of
Wilsdruff, 79.
Generation, equivocal, experiments on, by
Dr. Daubeny, 115.
Geology, chemical, T. S. Hunt on some
points in, 83.
Gerhardt’s proposal for doubling the
atomic number for oxygen, some prac-
tical objections to, by Prof. W. A. Mil-
ler, 70.
Gibb (Dr. G. D.) on saccharine fermen-
tation within the female breast, 131.
Giffard’s injector for feeding boilers, W.
Froude on, 211.
Gilbert (Dr. J. H), on the composition
of the ash of wheat, 70.
Glaciers, Canon Moseley on the cause of
the descent of, 48.
Gladstone (Dr. J. H.) on his own percep-
tion of colours, 12; on the chromatic
properties of the electric light of mer-
cury, 13 ; chemical notes, 69.
Glass, decomposed, R. Thomas on thin
films of, 19.
, decomposed, found at Nineveh, Sir
D. Brewster on, 9.
Glennie (J. S.S.) on physics as a branch
of the science of motion, 56; on a ge-
neral law of rotation applied to the
planets, 58.
Graptolites, A. Gages on the transform-
ation of iron pyrites connected with, 79.
—— in the Lydit and Phthanit, discovery
of, in the district of Wilsdruff, Saxony,
Dr. Geinitz on, 79.
Graves (Rev. Prof.) on the arrangement
of the forts and dwelling-places of the
ancient Irish, 156.
Gray (Sir Charles) on Asiatic cholera,
132.
Greene (Prof. J. R.) on embryology, with
reference to the mutual relations of the
subkingdoms of animals, 132,
Greenland, some remarks on, by Col.
Schaffner, 178.
Greenwich and Utrecht, J. Park Harrison
REPORT—1860.
on the similarity of the lunar curves of
minimum temperature at, 44.
Grove (W.R.) on the transmission of
electrolysis across glass, 69.
Gutta percha and india-rubber, as insu-
lators for subaqueous telegraphic wires,
W. Silver on, 212.
Habitat of plants influenced by nature of
strata, Rev. W.S. Symonds on the, 102.
Hall (Walter) on a process for covering
submarine wires with india-rubber,
211.
Harcourt (A. Vernon) on the oxidation
of potassium and sodium, 70.
Harkness (R.) on the metamorphic rocks
of the north of Ireland, 79.
Harris (Sir W. 8.) on electrical force, 28.
Harrison (J. Park) on the similarity of
the lunar curves of minimum tempera-
ture at Greenwich and Utrecht, 44.
Hartwell variable star atlas, 36.
Harvey (Edward R.) on the mode of death
by aconite, 133.
Hatchets, stone, of the Esquimaux, Sir
E. Belcher on, 154.
Heat, Prof. Maxwell on the results of
Bernoulli’s theory of gases as applied
to their internal friction, their diffusion,
and their conductivity for, 15.
Hector (Dr.) on the geology of Captain
Palliser’s expedition in British North
America, 80; on the climate of the
‘ Saskatchewan district in British North
America, 172.
Hennessy (Prof.) on studying the earth’s
internal structure from phenomena ob-
served at its surface, 35; on the prin-
ciples of meteorology, 44; suggestions
relative to inland navigation, 211.
Henslow (Rev. Prof.) on the supposed
germination of mummy wheat, 110.
Herring, J. M. Mitchell on the economi-
cal history and statistics of the, 191.
Higgins (Rev. H. H.) on some spe-
cimens of shells from the Liverpool
Museum, 116.
Hincks (Rev. Dr.) on recorded obserya-
tions of the planet Venus in the seventh
century before Christ, 35; on certain
ethnological boulders and their probable
origin, 156.
Hitchman (J.) on sanitary drainage of
towns, 191.
Hochstetter (Prof. von) on the geological
features of the volcanic island of St.
Paul, in the South Indian ocean, 81; on ~
the geology of New Zealand, 81; ona
new map of the interior of the Northern
Island of New Zealand, 162.
INDEX II.
Hodgson (R.) on a brilliant eruption on
the sun’s surface, 36.
Hogan (Rev. A. R.) on British well
shrimps, 116.
Hogg (John) on the distinctions of a plant
and an animal, and ona fourth king-
dom of nature, 111.
Houses for the labouring classes, on, 194,
196.
Hudson’s Bay and Straits, Dr. J. Rae on
the formation of icebergs and ice action
in the, 174.
Hull (Edward) on the Blenheim iron ore,
and the thickness of the formations be-
low the great oolite at Stonesfield, Ox-
fordshire, 81; on the six-inch maps of
the Geological Survey, 81.
Hunt (Dr. J.) on the antiquity of the hu-
man race, 162.
Hunt (T. Sterry) on some points in che-
mical geology, 83.
Hurtado (V.) on the geographical distri-
bution and trade in the Cinchona, 162.
Huxley (Prof.) on the development of
Pyrosoma, 136.
Hydrate of cresyl, gradual reduction of,
into hydrate of phenyl and other com-
pounds through the agency of chloride
of calcium or zinc, Dr. Gladstone on, 69.
of phenyl, gradual reduction of
' hydrate of cresyl into, through the
agency of chloride of calcium or zinc,
Dr. Gladstone on, 69.
Hygrometers, self-registering, E. Vivian
on results of, 55.
Hyperconic sections and elliptic integrals,
Rev. Dr. Booth on the relations be-
tween, 4.
Icebergs and ice action, Dr. J. Rae on the
formation of, in the Hudson’s Bay and
Straits, 174.
. Iceland, W. Lauder Lindsay on the erup-
tion in May 1860 of the KGtliigja vol-
cano in, 86.
» Some remarks on, by Col. Schaff-
ner, 178.
Ichthyolite, on a new form of, discovered
by Mr. Peach, 78.
Ichthyolites of Farnell Road, Forfarshire,
Sir P. de M. G, Egerton on the, 77.
India, Central, R. von Schlagintweit on
the aboriginal tribes of, 175.
, South, J. A. Broun on magnetic
rocks in, 24.
, J. A. Broun on the velocity of
earthquake shocks in the laterite of, 74.
and High Asia, general abstract of
the results of Messrs. de Schlagintweit’s
magnetic survey of, 32.
227
India, West Coast of, J. A. Broun on a
magnetic survey of the, 27.
Indians, Mr. Sullivan on the tribes of, in-
habiting the country explored by the
British North American expedition in
the years 1857-1859, 173.
India-rubber, Messrs. Werner and Sie-
mens on a mode of covering wires
with, 215.
India-rubber and gutta percha as insu-
lators for subaqueous telegraphic wires,
W. Silver on, 212.
Indo-European languages, Dr. Hincks on
the, 156.
Indo-Germanic theory of races, J. Craw-
furd on the, 154.
Integrals, elliptic, and hyperconic sec-
tions, Rev. Dr. Booth on the relations
between, 4.
Interference of light, phenomena pro-
duced by decomposed glass found at
Nineveh, Sir D. Brewster on, 9; at
Oxford, by R. Thomas, 19.
Invertebrate fauna of the lower oolites of
Oxfordshire, J. F. Whiteaves on the,
104.
Ireland, North of, Prof. Harkness on the
metamorphic rocks of the, 79.
Iron, E. Cowper on a new mode of ob-
taining a blast of very high tempera-
ture in the manufacture of, 204,
Iron ore, Blenheim, E. Hull on the, 81.
Jaczwings, a population of the 13th cen-
tury, Dr. R. G, Latham on the, 163.
Jarrett (Rev. Prof.) on alphabets, 163.
Jarvis (E.) on the system of taxation pre-
vailing in the United States, 191.
_ Jaundice, Dr. Thudichum on nitric and
nitro-hydrochloric acids in, 148.
Jeffreys (J. G.) on the British teredines,
or ship-worms, 117; on specimens of
the common whelk having double oper-
cula, 117.
Jellett (Rev. Prof.) on a new instrument
for determining the plane of polariza-
tion, 13.
Jet, Prof. Rowney on the composition of,
72,
Johnson’s (Henry) improved instrument
for describing spirals, 60; deep sea
pressure gauge, 202.
Jukes (J. Beete) on the igneous rocks
interstratified with the carboniferous
limestones of the basin of Limerick,
84,
Kidd (Dr. Charles) on the nature of death
from the administration of anesthetics,
especially chloroform and ether, 136,
[5>*
228
Kimmeridge, paddle of pliosaurus of great
size found at, Mr. R. Damon on a, 75.
Kirkman (Rev. T. P.) on ‘the roots of
substitutions, 4.
Knipe (J. A.) on the Tynedale coal-field
and the Whin-sill of Cumberland and
Northumberland, 86.
Knox (R.) on the origin of the arts, 163.
Labouring classes, H. Roberts on various
efforts to improve the domiciliary con-
dition of the, 196.
Labrador, some remarks on, by Col.
Schaffner, 178.
Labyrinthodon, Rey. W. Lister on foot-
prints of the, from the new red sand-
stone north of Wolverhampton, 87.
Tadd (W.) on an improved form of air-
pump for philosophical experiments, 65.
Lange (D. A.) on the progress of the
Isthmus of Suez Canal, 163.
Latham (Dr. R. G.) on the Jaczwings,
163,
Lawes (J. B.) on the composition of the
ash of wheat, 70.
Lee (Dr.John), prospectus of the Hartwell
variable star atlas, 36.
Lemuridz, Prof. Van der Hoeven on the
anatomy of the, 135.
Lenses, diamond, topaz, and rock-crystal,
best suited for, Sir D. Brewster on, 8.
Lepadide, R. Garner on the structure of
the, 130.
Lepidoptera, Dr. Verloren on the effect of
temperature and periodicity on the de-
velopment of, 123,
Lepidopterous larvz, micro-, H. T. Stain-
ton on some peculiar forms amongst
the, 122.
parasite on the body of the firefly,
J. O. Westwood on a, 124.
Leptocephalide, Prof. V. Carus on the,
125.
Lewis (Dr.) on a hydro-spirometer, 139.
Lias, Rev. P. B. Brodie, on the stratigra-
phical position of certain species of
corals in the, 73.
Lias, lower, in the south of England, Dr.
T. Wright on the, 108.
Light, electric, M. Serrin on an automatic
regulator for, 19.
Lightning conductors, G. J. Symons on
employing the gutters and rain-water
pipes of private houses as, 52.
Limerick, J. B. Jukes on the igneous rocks
interstratified with the carboniferous
limestones of the basin of, 84.
Limestones, carboniferous, of the basin of
Limerick, J. B. Jukes on the igneous
rocks interstratified with the, 84,
REPORT—1860.
Lindelof (Prof.) on the caustics produced
by reflexion, 14.
Lindsay (Dr. W. L.) on the eruption in
May 1860, of the Kétltigj& volcano in
Iceland, 86.
Lister (Rev. W.) on reptilian foot-prints
from the new red sandstone, north
of Wolverhampton, 87.
Liverpool Museum, on some specimens of
shells from the, 116.
Livingstone (Dr.) on the discoveries in
South Central Africa, 164.
Lockhart (W.) on the mountain districts
of China and their aboriginal inhabit-
ants, 168.
Locomotives, road, Earl of Caithness on,
204,
Lubbock (John) on the development of
Buccinum, 139.
Lunar craters, W. R. Birt on the forms of,
34. &
Lunar curves of minimum temperature at
Greenwich and Utrecht, on the simi-
larity of the, 44.
Macgowan (Dr.), on of the ante-chris-
tian settlement of the Jews in China,
170.
Machine atmospheric, for washing, J.
Fisher on an, 210.
MacLaren (Archibald) on the influence
of systematized exercise on the expan-
sion of the chest, 142.
Magnesian rocks, ‘I’. S. Hunt on, 83.
Magnetic declination, J, A. Broun on the
mode in which the diurnal law of,
varies from place to place, and the
probable position and epoch of the line
of least diurnal variation near the
equinoxes, 20,
— declination, J. A. Broun on the
diurnal variations of the, at the mag-
netic equator, and the decennial period,
21,
equator, J. A. Broun on the
diurnal variations of the magnetic decli-
nation at the, 21.
rocks in South India, J. A. Broun
on, 24.
survey of the west coast of India,
J. A. Broun on a, 27.
survey of India, Messrs. de Schla-
gintweit’s general abstract of the re-
sults of, 32, ;
Magnetic-induction dip-circle, new, J. A.
Broun on, 23.
Magnetism of the earth, the daily mean
intensity of the, increases as a whole
or diminishes as a whole, J, A, Broun
on, 20,
INDEX II.
Mammalia, triassic, C. Moore on remains
of, in the drift in the neighbourhood of
Frome, 88.
Man, J. Crawfurd on the Aryan or Indo-
Germanic theory of the races of, 154,
Maps, topographical, Capt. Cybulz on
models to facilitate instruction in deli-
neating the features of the ground on,
155.
Masters (M. T.) on the normal and ab-
normal variations from an assumed type
in plants, 112.
Maury (Captain) on antarctic expeditions,
44; on the climates of the antarctic
regions, 46.
Maxwell (Prof.) on the results of Ber-
noulli’s theory of gases as applied to
their internal friction, their diffusion,
and their conductivity for heat, 15; on
aninstrument for exhibiting any mixture
of the colours of the spectrum, 16.
May (D.), journey in the Yoruba and
Nupé countries, 170.
M*Donnell (Dr. Robert) on the formation
of sugar and amyloid substances in the
animal economy, 129.
Measuring actual distances, P. Adie on
an instrument for, 59.
Measurement, angular, P. Adie on a new
reflecting instrument for, 59.
Mechanics, Prof. Sylvester on the appli-
cation of Poncelet’s theorems for the
linear representation of quadratic radi-
cals to practical questions of, 7.
Medulla oblongata, R. Garner on altera-
tions in the, in cases of paralysis, 129.
Mental labour, E. Chadwick on the phy-
siological as well as psychological limits
to, 185.
Mercury, electric light of, Dr. J. H.
Gladstone on the chromatic properties
of the, 13.
Mersey and Dee, Prof. Collingwood on the
nudibranchiate mollusca of the, 113.
Meteorological observations at Stony-
hurst, results of, 56.
—— phenomena of the equinoctial week,
_ M. Du Boulay on the, 39.
Meteorology, Prof. Hennessy on the prin-
ciples of, 44.
Michelsen (Dr.) on serfdom in Russia,
191,
Mickie (J.), cruise in the Gulf of Pe-che-li
. and Leo-tung, China, 170.
Microscope, new form of, Sir D. Brewster
on a, 8.
Milk, human, G. D. Gibb on living ani-
~ malcules in, 131.
_ Miller (Prof. W. A.) on the atomic weight
of oxygen, 70.
229
Mitchell (J. M.) on the economical history
and statistics of the herring, 191.
Mitchell (Rev. W.) on the Koh-i-Noor
previous to its cutting, 87.
Mollusca, Nudibranchiate, Prof. Colling-
wood on the respiration of the, 113;
of the Mersey and Dee, 118,
Mollusca, on the Aspergillum, or water-
ing pot, 120.
Molyneux (William) on fossil fish from
the North Staffordshire coal-fields, 88.
Moon, W. R. Birt on the forms of certain
lunar craters in the, 34,
Moore (C.) on the contents of three square
yards of triassic drift, 87.
Morocco, E. Schlagintweit on the tribes
composing the population of, 177.
Morphology, animal, Prof. V. Carus on the
value of development in, 125.
Moseley (Rev. Canon) on the cause of the
descent of glaciers, 48,
Motion, science of, J. S. S. Glennie on
physics as a branch of the, 56.
Mountain countries, J. Bell on a plan for
systematic observations of temperature
in, 37.
Mountain ranges, Rev. J. Dingle on the
corrugation of strata in the vicinity of,
Moors of Morocco, a mixed race, E. Schla-
gintweit on the, 177.
Miller (Dr. Hugo) on the isomers of cu-
mol, 71; on a new acetic ether occur-
ring in a natural resin, 71.
Mundesley, Norfolk, the cliff at, J. Prest-
wich on some new facts in relation to,
90.
Murchison (Sir R. I.), his address as Pre-
sident of Section E, 148.
Navigation, inland, suggestions relative to,
by Prof. Hennessy, 211.
Newmarch (W.) on some schemes of
taxation and the difficulties of them,
194,
Nineveh, Sir D. Brewster on the decom-
posed glass found at, 9.
Northumberland- and Cumberland, J. A.
Knipe on the Tynedale coal-field and
the whin-sill of, 86.
Observatory, Travancore, J. A. Broun on
results of observations in the, 20.
Ogilvie (Dr. G.) on the structure of fern
stems, 112.
Ollier (M.) on the artificial production of
bone and osseous grafts, 143.
Oolite, great, at Stonesfield, Oxfordshire,
E. Hull on the thickness of the form~
ations below the, 81.
230
REPORT—1860.
Oolites, lower, of Oxfordshire, J. F.| Pierce (Prof. B.) on the dynamic con-
Whiteaves on the invertebrate fauna of
the, 104.
Optical illusions connected with inversion
of perspective, Sir D. Brewster on, 7.
Organic remains, A. Gages on some trans-
formations of iron pyrites in connexion
with, 79.
Osborn (Captain Sherard) on the forma-
tion of oceanic ice in the arctic regions,
170.
Ossiferouscavesin Sicily, newlydiscovered,
Baron Anca on, 738.
Owen (Prof.), letter to Mr. E. Chadwick
on the physiological limits to mental
labour, 189.
Oxford, notice of the new geological map
of the vicinity of, by Sir R. Murchison,
90.
Oxfordshire, J. F. Whiteaves on the inver-
tebrate fauna of the lower oolites of,
104.
Oxygen, Prof. W. A, Miller on the atomic
weight of, 70.
Oxygenation in animal bodies, Dr. W. B.
Richardson on the process of, 143.
Palliser (Capt.), on the course and results
of the British North American Explor-
ing Expedition, 170.
Paper, rice-, from the pith of the Aurelia
papyrifera, W. Lockhart on, 169.
Paralysis, R. Garner on alterations in the
medulla oblongata in cases of, 129.
Peach (C. W.), anew form of ichthyolite
discovered by, 78; on the statistics of
the herring fishery, 120.
Pembrokeshire, Rev. G. N. Smith on three
undescribed bone caves near Tenby,
101,
Pengelly (William) on the chronological
and geographical distribution of the
Devonian fossils of Devon and Corn-
wall, 91.
Perspective, inversion of, Sir D, Brewster
on some optical illusions connected with
the, 7.
Peruvian bark, the places where the tree
grows which yields the, 162.
Petherick (Consul) on his proposed jour-
ney from Khartum in Upper Egypt to
meet Capt. Speke on’or near the lake
Nyanza of Central Africa, 174.
Phillips (Prof.) on the geology of the
vicinity of Oxford, 90.
Photography, celestial, H. Draper on a
reflecting telescope for, erecting at
Hastings near New York, 63.
Physics as a branch of the science of mo-
tion, J. S.S. Glennie on, 56.
dition of Saturn’s rings, 37; on the
motion of a pendulum in a vertical
plane when the point of suspension
moves uniformly on a circumference in
the same plane, 37; on the physical
constitution of comets, 37.
Pile with sulphate of lead, M.E. Becquerel
on a, 59.
Placodus, teeth of the, discovered in the
triassic drift, in the neighbourhood of
Frome, by C. Moore, 88.
Pliosaurus, a paddlo of, found at Kim-
meridge, 75.
Planets, J. S. S. Glennie on a general law
of rotation applied to the, 58.
Plant and an animal, J. Hogg on the dis-
tinctions of a, 111. ~
Plants, British, Rev. W.S. Symonds on
the selection of a peculiar geological
habitat by some, 102.
, on the morphological laws in, 110.
, M. T. Masters on the normal and
abnormal variations from an assumed
type in, 112.
, on the final causes of the sexuality
of, in reference to Mr. Darwin’s theory,
109.
Playfair (Dr, Lyon) on the representation
of neutral salts, 71.
Poisoning, E. R. Harvey on the mode of
death by aconite, 138.
Polar expedition (Franklin’s), Capt. Snow
on the, and the possible recovery of its
scientific documents, 180.
Polarization, plane of, Prof. Jellett on a
new instrument for determining the,
13.
. M. Verdet on the dispersion of the
planes of, of the coloured rays produced
by the action of magnetism, 54,
Poncelet’s theorems for the linear repre-
sentation of quadratic radicals, Prof.
Sylvester on a generalization of, 7.
Ponton (M.) on the laws of chromatic
dispersion, 16.
Porter (H. J. Ker) on the best plan of
cottage for agricultural labourers, 194.
Powrie (J.) on a fossiliferous deposit near
Farnell, in Forfarshire, 89.
Prestwich (Joseph) on some new facts in
relation to the section of the cliff at
Mundesley, Norfolk, 90.
Price (J.) on Cydippe, 120; on slicken-
sides, 91.
Price (Rev. Prof.), address as President
of Section A, 1. 3
Pterodactyles of the Coprolite bed near —
Cambridge, Rev. J. P. B. Dennis on
the mode of flight of the, 76. ;
INDEX II.
Purdy (F.) on the systems of poor-law
medical relief, 195.
Pyrites, iron, A. Gages on some transfor-
mations of, in connexion with organic
remains, 79.
Pyrosclerite, Connemara, analysis of by
Prof, Rowney, 71.
Quadratic radicals, Prof. Sylvester on a
generalization of Poncelet’s theorems
for the linear representation of, 7.
Quinine, V. Hurtado on the barks from
which it is obtained, 162.
Radcliffe (Dr. C. B.) on muscular action
from an electrical point of view, 148.
Rae (Dr. J.) on the formation of icebergs
and ice action in the Hudson’s bay and
straits, 174; on the aborigines of the
arctic and sub-arctic regions of N. Ame-
rica, 175.
Railways, street, as used in the United
States, G, F. Train on, 215.
Rankin (Rev. T.) on the different motions
of electric fluid, 30; on meteorological
observations made at Huggate, 50.
Reflexion, Prof. Lindiléf on the caustics
produced by, 14.
Reeve (Lovell) on the Aspergillum or
watering-pot mollusk, 120.
Reilly (Calcott) on the longitudinal stress
of the plate-girder, 212.
Rennison (Rev. T.) on a new proof of
Pascal’s theorem, 6.
Respiration, B. W. Richardson on the
process of, 143.
Rhynchosaurus, Rev. W. Lister on foot-
prints of the, in the new red sandstone
north of Wolverhampton, 87.
Richardson (Dr. B. W.) on the process of
oxygenation in animal bodies, 143 ; on
an electro-magnetic railway break, 212.
Riffers of Morocco, E. Schlagintweit on
the, 177.
Rings seen in viewing a light through
fibrous specimens of calc-spar, on, 19.
Road locomotives, Earl of Caithness on,
204.
Roberts (Henry) on various efforts to
improve the domiciliary condition of
the labouring classes, 196.
Rocks, igneous, T. S. Hunt on, 84.
3 Magnesian, T. S. Hunt on, 83.
—, plutonic, T. S. Hunt on, 84.
, Magnetic, in South India, 24.
Rocks, metamorphic, of the N. of Ire-
land, Prof. Hennessy on the, 79.
gneous, interstratified with the car-
boniferous limestones of the basin of
Limerick, J. B. Jukes onthe, 84.
231
Rocky Mountains, British North America,
Dr. Hector on the strata composing the,
81.
—— Mountains, Capt. J. Palliser on
explorations in the, 170.
Rogers (Prof. H. D.) on some phenomena
of metamorphism in coal in the United
States, 101.
Rogers (Prof. W. B.), experiments and
conclusions on binocular vision, 17;
on the phenomena of electrical vacuum
tubes, 30.
Rotation, J.S.S.Glennie on a general
law of, applied to the planets, 58.
Roots of substitutions, Rev. T. Kirkman
on the, 4.
Rowney (Prof. T. H.) on the analysis of
some Connemara minerals, 71; on the
composition of jet, 72.
Saccharine fermentation within the female
breast, on, 131.
Sahara, central, of Algeria, Rev. H. B.
Tristram on the geological system of
the, 102. “
Sandstone, new red, north of Wolver-
hampton, Rev. W. Lister on some foot-
prints of the Labyrinthodon, Rhyncho-
saurus, &c. in the, 87.
, old red, of Farnell, Forfarshire,
Sir P. de M. G. Egerton on the fishes
found in the, 77.
Saskatchewan territory, British North
America, examination of, by Capt, Pal-
liser, 170.
, Dr. Hector on the climate of the,
172.
Schlagintweit (Lieut. Edward) on the
tribes composing the population of
Morocco, 177.
Schlagintweit (H. von), general abstract
of the results of Messrs. de Schlagint-
weit’s magnetic survey of India, 32.
Schlagintweit (Robert von) on thermo-
barometers, compared with barometers
at great heights, 50; on some of the
races of India and High Asia, 175.
Schools, educational, E, Chadwick on the
physiological as well as psychological
limits to mental labour, 185.
Sclater (P. L.) on the geographical distri-
bution of recent terrestrial vertebrata,
121.
Scoffern (T.) on waterproof and unalter-
able small-arm cartridges, 72.
Sea pressure gauge, deep, on a, 202.
Sedgwick (Rev. Prof.) on the geology of
the neighbourhood of Cambridge and
the fossils of the upper greensand,
101.
232 REPORT—1860.
Semitic inscriptions, Dr. Hincks on, 156.
Senior (N. W.), address as President of
Section F., 182.
Serrin (M.), régulateur automatique de
lumiére électrique, 19.
Shaffner (Colonel Tal. P.), on the geo-
graphy of the North Atlantic telegraph,
178
Shells, pathological collection of, Rev. H.
H. Higgins on a, 116.
Ship, atmotic, Hon. W. Bland on an, 60.
Ship-building, iron, W. Simons on im-
provements in, 212.
Ship-worms, J. G. Jeffreys on the British,
117.
Shiré river and valley, and inhabitants, in
South-Central Africa, Dr. Livingstone
on the, 164.
Sicily, Baron Ancaon two newly dis-
covered ossiferous caves in, 73.
Siemens (C. W.) and M. Werner, outline
of the principles and practice involved
in dealing with the electric conditions
of submarine electric telegraphs, 32.
Silurian formation in the district of
Wilsdruff, Saxony, Dr. Geinitz on the,
19.
— schists, Lower, A. Gages on the
transformation of iron pyrites connected
with fossil graptolitesfrom Tinnaglough,
Co. Wexford, 79.
Silver (S. W.) on gutta percha and india-
rubber as insulators for subaqueous tele-
graphic wires, 212.
Simons (W.) on improvements in iron
ship-building, 212.
Smith (Dr. Edward) on the action of tea
and alcohols, 145.
Smith (Prof. H. J. S.) on systems of in-
determinate linear equations, 6.
Smith (John) on the chromoscope, 65.
Smith (Rey. G. N.) on three undescribed
bone-caves near Tenby, 101.
Smithsonian Institution, P. P. Carpenter
on the principles and working of the,
109
Snow (Capt. W. Parker) on the lost Polar
expedition and the possible recovery of
its scientific documents, 180.
Sound, Rey. S, Earnshaw on the triplicity
of, 58.
Sound of thunder, Rev. S. Earnshaw on
the velocity of the, 58.
Species, Prof. Draper on the intellectual
development of Europe, considered with
reference to the views of Mr. Darwin
and others on, 115.
Spectrum, colours of the, Prof. Maxwell
on an instrument for exhibiting any
mixture of the, 16,
Spiders (British), notice of Mr. Black-
wall’s work on, 120.
Spirals, on an improved instrument for
describing, 690.
Sprengel (Dr. Hermann) on a new form
of blowpipe for laboratory use, 72.
Staffordshire (North) coal fields, W. Mo-
lyneux on fossil fish from the, 88.
Stainton (H. T.) on some peculiar forms
amongst the micro-lepidopterous larve,
122,
Stars, variable, prospectus of the Hartwell
atlas of, 36.
Statistics, address by N. W. Senior at
Oxford, 182.
Steam, saturated, W. Fairbairn on the
density of, 210.
Steam-ships, cylindrical spiral _ boiler
adapted to, by John Elder, 204.
Steam, superheated, W. Fairbairn on the
law of expansion of, 210.
Stenops Potto, Prof. Van der Hoeven on
the anatomy of, 134.
Stereoscopes, A. Claudet on the means of
‘ increasing the angle of, to obtain an
effect in proportion to their magnifying
power, 61.
Stewart (Balfour) on some recent exten-
sions of Prevost’stheory ofexchanges,19.
Stonesfield, Oxfordshire, E. Hull on the
thickness of the fermations below the
great oolite at, 81.
Stonestield slate, J. F. Whiteaves on the
fossils of the, 104.
Stone hatchets, Sir E. Belcher on their
manufacture by the Esquimaux, 154.
Stoney (G. J.) on rings seen in viewing
a light through fibrous specimens of
cale-spar, 19.
Stonyhurst, results of ten years’ meteo-
rological observations at, 56.
Storms, British, Admiral FitzRoy on, 39.
, arrangements for communicating
warning of, from one part of the country
to the other, 42.
Storms, Captain W. Parker Snow on
practical experience of Admiral Fitz-
Noy’s law of storms in each quarter of
the globe, 52.
Strata, Rev. J. Dingle on the corruga-
tion of, in the vicinity of mountain
ranges, 77.
Substitutions, Rev. T. P. Kirkman on the
roots of, 4.
Sugar and amyloid substances, Dr. R.
M°Donnell on the formation of, in the
animal economy, 129.
Sullivan (Mr.) on the tribes of Indians
inhabiting the country explored by the
British N, American expedition, 173.
INDEX II,
Sun’s, surface, R. Hodgson on a brilliant
eruption on the, 36.
Siis tribes of Morocco, E. Schlagintweit
on the, 177.
Sylvester (Prof.) on a generalization of
Poncelet’s theorems for the linear repre-
sentation of quadratic radicals, 7.
Symons (G, J.), results of an investiga-
tion into the phenomena of English
thunder-storms, 52.
Symonds (Rev. W. S.) on the selection
of a peculiar geological habitat by some
of the rarer British plants, 102.
Synge (Capt. M. H.) on the proposed com-
munication between the Atlantic and
Pacific, vid British North America, 181.
Tactions of Apollonius of Perga, Dr.
Brennecke on some solutions of the
problem. of, by modern geometry, 4.
Taylor (Admiral) on means to lessen
the loss of life round our coasts; also a
permanent deep-water harbour of
refuge by artificial bars, 215.
Tchihatchef (Pierre de) on the geogra-
phical distribution of plants in Asia
Minor, 181.
Tea and alcohols, their action contrasted,
by Dr. E. Smith, 145, :
Telegraph, North Atlantic, Col. Schaffner
on the geography of the, 178.
Telegraphic wires, S. W. Silver on gutta
percha and india-rubber as insulators
for, 212.
Telegraphic wires, Messrs. Werner and
C. W. Siemens on a mode of covering
with india-rubber, 215.
Telegraphic wires, submarine, W. Hall
on a process for covering with india-
rubber, 211.
Telegraphs, electric submarine, M. Wer-
ner and C, W. Siemens on the princi-
ples and practice involved in dealing
with the electrical conditions of, 32.
Telemeter, P. Adie on an instrument for
measuring actual distances, 59.
Telescope, reflecting, for celestial photo-
graphy, H. Draper on a, 63.
Temperature, minimum, at Greenwich
and Utrecht, J. Park Harrison on the
similarity of the lunar curves of, 44,
Temperature in mountain countries, J.
Ball on a plan for systematic observa-
tions of, 37.
Tenby, Rev. G. N. Smith on three un-
described bone-caves near, 101.
Tennant (Prof.) on the Koh-i-Noor pre-
vious to its cutting, 87.
Teredines, British, J. G. Jeffreys on the,
117.
233
Teredo navalis, Prof. Van der Hoeven on
the, 136.
Thames from Lechlade to Windsor, Rev.
J. C. Clutterbuck on the course of the,
as ruled by the geological formations
over which it passes, 75,
Thermo-barometers compared with baro-
meters at great heights, R. von Schla-~ °
gintweit on, 50.
Thomas (R.) on thin films of decomposed
glass found near Oxford, 19.
Thomson (Prof. W.) on atmospheric elec-
tricity, 53.
Thudichum (Dr.) on thiotherine, 72; on
the physiological relations of the co-
louring matter of the bile, 147.
Thunder, Rev. S. Earnshaw on the velo-
city of the sound of, 58.
Thunder-storms, English, G. J. Symons
on results of an investigation into the
phenomena of, 52,
Tomopteris onisciformis, notes on, by Dr,
E. P. Wright, 124.
Topaz, white, of New Holland, particu-
larly fitted for optical purposes, Sir D.
Brewster on, 8.
Train (G, F.) on street railways as used
in the United States, 215.
Travancore, observatory of, J. A. Broun
on certain results of observations in
the, 20.
Triassic drift, C. Moore on the contents
of three square yards of, from the
neighbourhood of Frome, 87,
Tristram (Rev, H. B.) on the geological
system of the central Sahara of Algeria,
102.
Turks in Central Asia, R. von Schlagint-
weit on the, 176.
Tynedale coal-field, J. A. Knipeon the, 86.
United States, P. P. Carpenter on the
progress of natural scienve in the, 109;
on street railways as used in the, 215.
Utrecht and Greenwich, J. Park Harrison
on the similarity of the lunar curves of
minimum temperature at, 44.
Vacuum tubes, electrical, Prof. W. B.
Rogers on the phenomena of, 30,
Van der Hoeven (Prof.) on the anatomy
of Stenops Potto, 134; on the Teredo
navalis, 136.
Vancouver's Island, geology of, Dr. Hec-
tor on the, 81.
Venus, planet, on some recorded observa-
tions of the, in the seventh century be-
fore Christ, 35.
Verdet (M.) on the dispersion of the
planes of polarization of the coloured
934
rays produced by the action of mag-
netism, 54.
Verloren (Dr.) on the effect of tempera-
ture and periodicity on the develop-
ment of certain lepidoptera, 123.
Vertebrata, terrestrial, P. L. Sclater on
the geographical distribution of, 121.
Vision, binocular, experiments and con-
clusions on, by Prof. W. B. Rogers, 17.
Vivian (E.), results of his new self-regis-
tering hygrometers, 55.
Voelcker (Prof.) on poisonous metals in
cheese, 73.
Volcano (the Kotligja) in Iceland, W.
L. Lindsay on an irruption of, 86.
Volcanos, Dr. Daubeny on the elevation
theory of, 75.
Volume theory, C. M. von Bose on the, 71.
Volutor, Rev. Dr. Booth on an improved
instrument for describing spirals, 60.
Wallace (Dr. W.) on the causes of fire
in Turkey-red stoves, 73.
Washing machine, atmospheric, by J.
Parker, 210.
Washington, Smithsonian Institution at,
P. P. Carpenter on the principles and
working of the, 109.
Water, D. Chadwick on a meter for the
correct measurement of, 204,
Water-meters, D. Chadwick on, 204.
Weeds, exposed to a temperature of 198°
below zero of Fahrenheit’s scale not
losing the power of germination, Prof.
Wartmann on, 110.
Weld (Rev. A.), results of ten years’ me-
teorological observations at Stonyhurst,
56.
Werner and Siemens (Messrs.), outline
of the principles and practice involved
in dealing with the electrical conditions
of submarine electric telegraphs, 32 ;
REPORT—1860.
on a mode of covering wires with india-
rubber, 215.
Westwood (J. O.) on mummy beetles,
123 ; on a lepidopterous parasite on the
body of the Fulgora candelaria, 124.
Wexford, iron pyrites connected with fos-
sil graptolites from Tinnaglough in the
county of, A. Gages on, 79.
Wheat, mummy, Prof. Henslow on the
supposed germination of, -110.
Whelk, common (Buccinum undatum), on
specimens having double opercula, 117.
Whin-sill of Cumberland and Northum-
berland, J. A. Knipe on the, 86.
Whiteaves (J. F.) on the invertebrate
fauna of the lower oolites of Oxfordshire,
104.
Wiers’s (Mr.) alkalimeters, 72.
Wilsdruff, Saxony, Dr. Geinitz on the
Silurian formation in the district of, 79.
Wolverhampton, Rev. W. Lister on rep-
tilian foot-prints in the new red sand-
stone north of, 87.
Woodall (Captain) on the intermittent
springs of the chalk and oolite of the
neighbourhood of Scarborough, 108.
Woodward’s solar camera, A. Claudet on,
62.
Wright (Dr. E. P.) on Tomopteris onisci-
formis, 124.
Wright (Dr. Thomas) on the Avicula con-
torta beds and lower lias in the south
of England, 108.
Wright (T.) on the excavations on the
site of the Roman city of Uriconium at
Wroxeter, 181.
Zoology, systematic, Prof. Collingwood
on recurrent animal. form, 114; Prof.
V. Carus on the value of development
in, 125.
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PROCEEDINGS orf THE FIRST ann SECOND MEETINGS, at York
and Oxford, 1831 and 1832, Published at 13s. 6d.
Contents :—Prof. Airy, on the Progress of Astronomy ;—J. W. Lubbock, on the Tides;
—Prof. Forbes, on the Present State of Meteorology ;—Prof. Powell, on the Present State
of the Science of Radiant Heat ;—Prof. Cumming, on Thermo-Electricity ;—Sir D. Brewster,
on the Progress of Optics ;—Rev. W. Whewell, on the Present State of Mineralogy ;—Rev.
W. D. Conybeare, on the Recent Progress and Present State of Geology ;—Dr, Prichard's
Review of Philological and Physical Researches.
Together with Papers on Mathematics, Optics, Acoustics, Magnetism, Electricity, Chemistry,
Meteorology, Geography, Geology, Zoology, Anatomy, Physiology, Botany, and the Arts;
and an Exposition of the Objects and Plan of the Association, &c.
PROCEEDINGS or tue THIRD MEETING, at Cambridge, 1833,
Published at 12s.
ConTENTS :—Proceedings of the Meeting ;—John ‘Taylor, on Mineral Veins ;—Dr.
Lindley, on the Philosophy of Botany ;—Dr. Henry, on the Physiology of the Nervous Sy-
stem ;—P. Barlow, on the Strength of Materials ;—S. H. Christie, on the Magnetism of the
Earth ;—Rev. J. Challis, on the Analytical Theory of Hydrostatics and Hydrodynamics;—
G. Rennie, on Hydraulics as a Branch of Engineering, Part I. ;—Rev. G. Peacock, on vercaa
Branches of Analysis.
Together with papers on Mathematics and Physics, Philosophical Instruments and Mecha-
nical Arts, Natural History, Anatomy, Physiology, and History of Science.
236
PROCEEDINGS or tue FOURTH MEETING, at Edinburgh, 1834,
Published at 15s.
Contents :—H. G. Rogers, on the Geology of North America;—Dr. C. Henry, on the
Laws of Contagion ;—Prof. Clark, on Animal Physiology ;—Rev. L. Jenyns, on Zoology ;—
Rev. J. Challis, on Capillary Attraction ;—Prof. Lloyd, on Physical Optics;—G. Rennie, on
Hydraulics, Part II.
Together with the Transactions of the Sections, and Recommendations of the Association
and its Committees.
PROCEEDINGS or tue FIFTH MEETING, at Dublin, 1835, Pub-
lished at 13s. 6d.
ConTENTS :—Rev. W. Whewell, on the Recent Progress and Present Condition of the
Mathematical Theories of Electricity, Magnetism, and Heat;— A. Quetelet, Apercu de
l’Etat actuel des Sciences Mathématiques chez les Belges ;—Capt. E. Sabine, on the Phe-
nomena of Terrestrial Magnetism.
Together with the Transactions of the Sections, Prof. Sir W. Hamilton’s Address, and Re-
commendations of the Association and its Committees.
PROCEEDINGS or tHE SIXTH MEETING, at Bristol, 1836, Pub-
lished at 12s.
ConTENTS :—Prof. Daubeny, on the Present State of our Knowledge with respect to Mine-
ral and Thermal Waters ;—Major E, Sabine, on the Direction and Intensity of the Terrestrial
Magnetic Force in Scotland ;—J. Richardson, on North American Zoology ;—Rev. J. Challis,
on the Mathematical Theory of Fluids ;—J. T. Mackay, a Comparative View of the more
remarkable Plants which characterize the neighbourhood of Dublin and Edinburgh, and the
South-west of Scotland, &c.;—J. T. Mackay, Comparative Geographical Notices of the
more remarkable Plants which characterize Scotland and Ireland ;—Report of the London Sub-
Committee of the Medical Section on the Motions and Sounds of the Heart ;—Second Report
of the Dublin Sub-Committee on the Motions and Sounds of the Heart ;—Report of the Dublin
Committee on the Pathology of the Brain and Nervous System;
of the Recent Discussions of Observations of the Tides ;—Rev. B. Powell, on determining the
Refractive Indices for the Standard Rays of the Solar Spectrum in various media;—Dr. Hodgkin,
on the Communication between the Arteries and Absorbents ;—Prof. Phillips, Report of Experi-
ments on Subterranean Temperature ;—Prof. Hamilton, on the Validity of a Method recenily
proposed by G. B. Jerrard, for Transforming and Resolving Equations of Elevated Degrees.
Together with the Transactions of the Sections, Prof. Daubeny’s Address, and Recommen-
dations of the Association and its Committees.
PROCEEDINGS or true SEVENTH MEETING, at Liverpool, 1837,
Published at 16s. 6d.
ConTENTS :—Major E. Sabine, on the Variations of the Magnetic Intensity observed at dif-
ferent points of the Earth’s Surface ;—Rev. W. Taylor, on the various modes of Printing for
the Use of the Blind ;—J. W. Lubbock, on the Discussions of Observations of the Tides ;—
Prof, T. Thomson, on the Difference between the Composition of Cast Iron produced by the
Cold and Hot Blast ;—Rev. T. R. Robinson, on the Determination of the Constant of Nutation
by the Greenwich Observations ;—R. W. Fox, Experiments on the Electricity of Metallic
Veins, and the Temperature of Mines ;—Provisional Report of the Committee of the Medical
Section of the British Association, appointed to investigate the Composition of Secretions, and
the Organs producing them ;—Dr. G. O. Rees, Report from the Committee for inquiring into
the Analysis of the Glands, &c. of the Human Body ;—Second Report of the London Sub-Com-
mittee of the British Association Medical Section, on the Motions and Sounds of the Heart ;—
Prof. Johnston, on the Present State of our Knowledge in regard to Dimorphous Bodies ;—
Lt.-Col. Sykes, on the Statistics of the Four Collectorates of Dukhun, under the British Go-
vernment ;—E. Hodgkinson, on the relative Strength and other Mechanical Properties of Iron
obtained from the Hot and Cold Blast ;—W. Fairbairn, on the Strength and other Properties
of Iron obtained from the Hot and Cold Blast;—Sir J. Robison, and J. S. Russell, Report of
the Committee on Waves ;—Note by Major Sabine, being an Appendix to his Report on the
Variations of the Magnetic Intensity observed at. different Points of the Earth’s Surface ;—
J. Yates, on the Growth of Plants under Glass, and without any free communication with the
outward Air, on the Plan of Mr. N. J. Ward, of London,
Together with the Transactions of the Sections, Prof. Traill’s Address and Recommenda-
tions of the Association and its Committees.
Eien! WA).
etry.
———EEE————— ee
237
PROCEEDINGS or toe EIGHTH MEETING, at Newcastle, 1838,
Published at 15s.
ConTENTS :—Rev. W. Whewell, Account of a Level Line, measured from the Bristol Chan-
nel to the English Channel, by Mr. Bunt;—Report on the Discussions of Tides, prepared
under the direction of the Rev. W. Whewell;—W. S. Harris, Account of the Progress and
State of the Meteorological Observations at Plymouth ;—Major LE. Sabine, on the Magnetic
Isoclinal and Isodynamic Lines in the British Islands ;—D. Lardner, LL.D., on the Determi-
nation of the Mean Numerical Values of Railway Constants ;—R. Mallet, First Report upon
Experiments upon the Action of Sea and River Water upon Cast and Wrought Iron ;—R.
Mallet, on the Action of a Heat of 212° Fahr., when long continued, on Inorganic and Organic
Substances.
Together with the Transactions of the Sections, Mr. Murchison’s Addresa, and Recommen-
dations of the Association and its Committees.
PROCEEDINGS or tue NINTH MEETING, at Birmingham, 1839,
Published at 13s. 6d.
ConTEnTs :—Rev. B. Powell, Report on the Present State of our Knowledge of Refractive
Indices, for the Standard Rays of the Solar Spectrum in different media ;—Report on the Ap-
plication of the Sum assigned for Tide Calculatiocs to Rev. W. Whewell, in a Letter from T. G.
Bunt, Esq. ;—H. L. Pattinson, on some Galvanic Experiments to determine the Existence or
Non-Existence of Electrical Currents among Stratified Rocks, particularly those of the Moun-
tain Limestone formation, constituting the Lead Measures of Alton Moor ;—Sir D. Brewster,
Reports respecting the two series of Hourly Meteorological Observations kept in Scotland ;—
Report on the subject of a series of Resolutions adopted by the British Association at their
Meeting in August 1838, at Newcastle ;—R. Owen, Report on British Fossil Reptiles ;—E.
Forbes, Report on the Distribution of Pulmoniferous Mollusca in the British Isles ;—W. S.
Harris, Third Report on the Progress of the Hourly Meteorological Register at Plymouth
Dockyard.
Together with the Transactions of the Sections, Rev. W. Vernon Harcourt’s Address, and
Recommendations of the Association and its Committees.
PROCEEDINGS or tue TENTH MEETING, at Glasgow, 1840,
Published at 15s.
ConTENTs :—Rev. B. Powell, Report on the recent Progress of discovery relative to Radiant
Heat, supplementary to a former Report on the same subject inserted in the first volume of the
Reports of the British Association for the Advancement of Science ;—J. D. Forbes, Supple-
mentary Report on Meteorology ;—W. S. Harris, Report on Prof. Whewell’s Anemometer,
now in operation at Plymouth ;—Report on ‘‘ The Motion and Sounds of the Heart,” by the
London Committee of the British Association, for 1839-40 ;—Prof. Schénbein, an Account of
Researches in Electro-Chemistry ;—R. Mallet, Second Report upon the Action of Air and
Water, whether fresh or salt, clear or foul, and at various temperatures, upon Cast Iron,
Wrought Iron and Steel ;—R. W. Fox, Report on some Observations on Subterranean Tem-
' perature ;—A. F. Osler, Report on the Observations recorded during the years 1837, 1838, 1839
and 1840, by the Self-registering Anemometer erected at the Philosophical Institution, Bir-
mingham ;—Sir D. Brewster, Report respecting the two Series of Hourly Meteorological Ob-
servations kept at Inverness and Kingussie, from Nov. Ist, 1838 to Nov. 1st, 1839 ;—W.
Thompson, Report on the Fauna of Ireland: Div. Vertebrata ;—C. J. B. Williams, M.D.,
Report of Experiments on the Physiology of the Lungs and Air-Tubes ;—Rev. J. S. Henslow,
Report of the Committee on the Preservation of Animal and Vegetable Substances.
Together with the Transactions of the Sections, Mr. Murchison and Major E. Sabine’s
Address, and Recommendations of the Association and its Committees.
PROCEEDINGS or tHze ELEVENTH MEETING, at Plymouth,
1841, Published at 13s. 6d.
ConTEnTs :—Rev. P. Kelland, on the Present state of our Theoretical and Experimental
Knowledge of the Laws of Conduction of Heat ;—G. L. Roupell, M. D., Report on Poisons ;—
T. G. Bunt, Report on Discussions of Bristol Tides, under the direction of the Rev. W. Whewell;
—D. Ross, Report on the Discussions of Leith Tide Observations, under the direction of the
Rev. W. Whewell ;—W. S. Harris, upon the working of Whewell’s Anemometer at Plymouth
during the past year ;—Report of a Committee appointed for the purpose of superintend-
ing the scientific co-operation of the British Association in the System of Simultaneous Obser-
vations in Terrestrial Magnetism and Meteorology ;—Reports of Committees appointed to pro-
‘vide Meteorological Instruments for the use of M, Agassiz and Mr. M‘Cord ;—Report of a Com-
238
mittee to superintend the reduction of Meteorological Observations;—Report of a Com-
mittee for revising the Nomenclature of the Stars ;—Report of a Committee for obtaining In-
struments and Registers to record Shocks and Earthquakes in Scotland and Ireland ;—Report of
a Committee on the Preservation of Vegetative Powers in Seeds ;—Dr. Hodgkin, on Inquiries
into the Races of Man ;—Report of the Committee appointed to report how far the Desiderata
in our knowledge of the Condition of the Upper Strata of the Atmosphere may be supplied by
means of Ascents in Balloons or otherwise, to ascertain the probable expense of such Experi-
ments, and to draw up Directions for Observers in such circumstances ;—R. Owen, Report
on British Fossil Reptiles ;—Reports on the Determination of the Mean Value of Railway
Constants ;--D. Lardner, LL.D., Second and concluding Report on the Determination of the
Mean Value of Railway Constants ;—-E. Woods, Report on Railway Constants ;—Report of a
Committee on the Construction of a Constant Indicator for Steam-Engines.
_ Together with the Transactions of the Sections, Prof. Whewell’s Address, and Recommen-
dations of the Association and its Committees.
PROCEEDINGS or toe TWELFTH MEETING, at Manchester,
1842, Published at 10s. 6d.
ConTENTs :—Report of the Committee,appointed to conduct the co-operation‘of the British
Association in the System of Simultaneous Magnetical and Meteorological Observations ;—
J. Richardson, M.D., Report on the present State of the Ichthyology of New Zealand ;—
W. S. Harris, Report on the Progress of Meteorological Observations at Plymouth ;—Second
Report of a Committee appointed to make Experiments on the Growth and Vitality of Seeds;
—C. Vignoles, Report of the Committee on Railway Sections ;—Report of the Committee
for the Preservation of Animal and Vegetable Substances ;—Lyon Playfair, M.D., Abstract
of Prof. Licbig’s Report on Organic Chemistry applied to Physiology and Pathology ;—
R. Owen, Report on the British Fossil Mammalia, Part I.;—R. Hunt, Researches on the
Influence of Light on the Germination of Seeds and the Growth of Plants ;—L. Agassiz, Report
on the Fossil Fishes of the Devonian System or Old Red Sandstone ;—W. Fairbairn, Ap-
pendix to a Report on the Strength and other Properties of Cast Iron obtained from the Hot
and Cold Blast ;—D. Milne, Report of the Committee for Registering Shocks of Earthquakes
in Great Britain ;—Report of a Committee on the construction of a Constant Indicator for
Steam-Engines, and for the determination of the Velocity of the Piston of the Self-acting En-
gine at different periods of the Stroke ;—J. S. Russell, Report of a Committee on the Form of
Ships ;—Report of a Committee appointed “to consider of the Rules by which the Nomencla-
ture of Zoology may be established on a uniform and permanent basis ;’’—Report of a Com-
mittee on the Vital Statistics of large Towns in Scotland ;—Provisional Reports, and Notices
of Progress in special Researches entrusted to Committees and Individuals.
Together with the Transactions of the Sections, Lord Francis Egerton’s Address, and Re-
commendations of the Association and its Committees.
PROCEEDINGS or tue THIRTEENTH MEETING, at Cork,
1843, Published at 12s.
CoNnTENTS:—Robert Mallet, Third Report upon the Action of Air and Water, whether
fresh or salt, clear or foul, and at Various Temperatures, upon Cast Iron, Wrought Iron, and
Steel;—Report of the Committee appointed to conduct the co-operation of the British As-
sociation in the System of Simultaneous Magnetical and Meteorological Observations ;—Sir
J. F. W. Herschel, Bart., Report of the Committee appointed for the Reduction of Meteoro-
logical Obseryations;—Report of the Committee appointed for Experiments on Steam-
Engines ;—Report of the Committee appointed to continue their Experiments on the Vitality
of Seeds ;—J. S. Russell, Report of a Series of Observations on the Tides of the Frith of
Forth and the East Coast of Scotland ;—J. S. Russell, Notice of a Report of the Committee
on the Form of Ships;—J. Blake, Report on the Physiological Action of Medicines;—Report
of the Committee on Zoological Nomenclature ;—Report of the Committee for Registering
the Shocks of Earthquakes, and making such Meteorological Observations as may appear to
them desirable ;—Report of the Committee for conducting Experiments with Captive Balloons;
—Prof. Wheatstone, Appendix to the Report ;—Report of the Committee for the Translation
and Publication of Foreign Scientific Memoirs ;—C. W. Peach on the Habits of the Marine
Testacea ;—E, Forbes, Report on the Mollusca and Radiata of the AZgean Sea, and on their
distribution, considered as bearing on Geology ;—L. Agassiz, Synoptical Table of British
Fossil Fishes, arranged in the order of the Geological Formations ;—R. Owen, Report on the
British Fossil Mammalia, Part II. ;—E. W. Binney, Report on the excavation made at the
junction of the Lower New Red Sandstone with the Coal Measures at Collyhurst i—W.
LL’
239
Thompson, Report on the Fauna of Ireland: Diy. ZJnvertebrata ;—Provisional Reports, and
Notices of Progress in Special Researches entrusted to Committees and Individuals.
Together with the Transactions of the Sections, Earl of Rosse’s Address, and Recommen-
dations of the Association and its Committees.
PROCEEDINGS or true FOURTEENTH MEETING, at York, 1844,
Published at £1.
ConTENTS :—W. B. Carpenter, on the Microscopic Structure of Shells ;—J. Alder and A*
Hancock, Report on the British Nudibranchiate Mollusca ;—R. Hunt, Researches on the
Influence of Light on the Germination of Seeds and the Growth of Plants ;—Report of a
Committee appointed by the British Association in 1840, for revising the Nomenclature of the
Stars ;—Lt.-Col. Sabine, on the Meteorology of Toronto in Canada ;—J. Blackwall, Report
on some recent researches into the Structure, Functions, and Ciconomy of the Araneidea,
made in Great Britain ;—Earl of Rosse, on the Construction of large Reflecting Telescopes ;
—Rev. W. Y. Harcourt, Report on a Gas-furnace for Experiments on Vitrifaction and other
Applications of High Heat in the Laboratory ;—Report of the Committee for Registering
Earthquake Shocks in Scotland ;—Report of a Committee for Experiments on Steam-Engines;
—Report of the Committee to investigate the Varieties of the Human Race ;—Fourth Report
of a Committee appointed to continue their Experiments on the Vitality of Seeds ;—W. Fair-
bairn, on the Consumption of Fuel and the Prevention of Smoke ;—F. Ronalds, Report con-
cerning the Observatory of the British Association at Kew ;—Sixth Report of the Committee
appointed to conduct the Co-operation of the British Association in the System of Simulta-
neous Magnetical and Meteorological Observations ;—Prof. Forchhammer on the influence
of Fucoidal Plants upon the Formations of the Earth, on Metamorphism in general, and par-
ticularly the Metamorphosis of the Scandinavian Alum Slate ;—H. E. Strickland, Report on
the recent Progress and Present State of Ornithology ;—T. Oldham, Report of Committee
appointed to conduct Observations on Subterranean Temperature in Ireland ;—Prof. Owen,
Report on the Extinct Mammals of Australia, with descriptions of certain Fossils indicative
of the former existence in that continent of large Marsupial Representatives of the Order
Pachydermata ;—W. S. Harris, Report on the working of Whewell and Osler’s Anemometers
at Plymouth, for the years 1841, 1842, 1843 ;—W. R. Birt, Report on Atmospheric Waves;
—L. Agassiz, Rapport sur les Poissons Fossiles de l’Argile de Londres, with translation ;—J.
S. Russell, Report on Waves ;—Provisional Reports, and Notices of Progress in Special Re-
searches entrusted to Committees and Individuals.
Together with the Transactions of the Sections, Dean of Ely’s Address, and Recommenda-
tions of the Association and its Committees.
PROCEEDINGS or tut FIFTEENTH MEETING, at Cambridge,
1845, Published at 12s.
ConTENTS :—Seventh Report of a Committee appointed to conduct the Co-operation of the
British Association in the System of Simultaneous Magnetical and Meteorological Observa-
tions ;—Lt.-Col. Sabine, on some points in the Meteorology of Bombay ;—J. Blake, Report
on the Physiological Actions of Medicines ;—Dr. Von Boguslawski, on the Comet of 1843;
—R. Hunt, Report on the Actinograph ;—Prof. Schénbein, on Ozone ;—Prof, Erman, on
the Influence of Friction upon Thermo-Electricity;—Baron Senftenberg, on the Self-
Registering Meteorological Instruments employed in the Observatory at Senftenberg ;—
W.R. Birt, Second Report on Atmospheric Waves ;—G. R. Porter, on the Progress and Pre-
' sent Extent of Savings’ Banks in the United Kingdom ;—Prof. Bunsen and Dr. Playfair,
Report on the Gases evolved from Iron Furnaces, with reference to the Theory of Smelting
of Iron ;—Dr. Richardson, Report on the Ichthyology of the Seas of China and Japan ;—
Report of the Committee on the Registration of Periodical Phenomena of Animals and Vege-
tables ;—Fifth Report of the Committee on the Vitality of Seeds ;—Appendix, &c.
Together with the Transactions of the Sections, Sir J. F. W. Herschel’s Address, and Re-
commendations of the Association and its Committees.
PROCEEDINGS or tHe SIXTEENTH MEETING, at Southampton,
1846, Published at 15s. ’
ConTENTS:—G. G. Stokes, Report on Recent Researches in Hydrodynamics ;—Sixth
Report of the Committee on the Vitality of Seeds ;—Dr. Schunck on the Colouring Matters of
Madder ;—J. Blake, on the Physiological Action of Medicines;—R. Hunt, Report on the Ac-
tinograph ;—R. Hunt, Notices on the Influence of Light on the Growth of Plants ;—R. L.
Ellis, on the Recent Progress of Analysis ;—Prof. Forchhammer, on Comparative Analytical
240
Researches on Sea Water;—A. Erman, on the Calculation of the Gaussian Constants for
1829;—G. R. Porter, on the Progress, present Amount, and probable future Condition of the
Iron Manufacture in Great Britain ;—W. R. Birt, Third Report on Atmospheric Waves ;—
Prof. Owen, Report on the Archetype and Homologies of the Vertebrate Skeleton ;—
J. Phillips, on Anemometry ;—J. Percy, M.D., Report on the Crystalline Flags ;—Addenda
to Mr. Birt’s Report on Atmospheric Waves.
Together with the Transactions of the Sections, Sir R. I. Murchison’s Address, and Re-
commendations of the Association and its Committees,
PROCEEDINGS or tue SEVENTEENTH MEETING, at Oxford,
1847, Published at 18s.
ConTENTS :—Prof. Langberg, on the Specific Gravity of Sulphuric Acid at different de-
grees of dilution, and on the relation which exists between the Development of Heat and the
coincident contraction of Volume in Sulphuric Acid when mixed with Water ;—R. Hunt,
Researches on the Influence of the Solar Rays on the Growth of Plants ;—R. Mallet, on
the Facts of Earthquake Phenomena ;—Prof. Nilsson, on the Primitive Inhabitants of Scan-
dinavia ;—-W. Hopkins, Report on the Geological Theories of Elevation and Earthquakes;
—Dr. W. B. Carpenter, Report on the Microscopic Structure of Shells ;—Rev. W. Whewell and
Sir James C. Ross, Report upon the Recommendation of an Expedition for the purpose of
completing our knowledge of the Tides ;—Dr. Schunck, on Colouring Matters ;—Seventh Re-
port of the Committee on the Vitality of Seeds;—J. Glynn, on the Turbine or Horizental
Water-Wheel of France and Germany ;—Dr. R. G. Latham, on the present state and recent
progress of Ethnographical Philology ;—Dr. J. C. Prichard, on the various methods of Research
which contribute to the Advancement of Ethnology, and of the relations of that Science to
other branches of Knowledge ;—Dr. C. C. J. Bunsen, on the results of the recent Egyptian
researches in reference to Asiatic and African Ethnology, and the Classificatiof¥ of Languages ;
—Dr. C. Meyer, on the Importance of the Study of the Celtic Language as exhibited by the
Modern Celtic Dialects still extant ;—Dr. Max Miiller, on the Relation of the Bengali to the
Arian and Aboriginal Languages of India;—W. R. Birt, Fourth Report on Atmospheric
Waves ;—Prof. W. H. Dove, Temperature Tables, with Introductory Remarks by Lieut.-Col.
E. Sabine ;—A. Erman and H. Petersen, Third Report on the Calculation of the Gaussian Con-
stants for 1829.
Together with the Transactions of the Sections, Sir Robert Harry Inglis’s Address, and
Recommendations of the Association and its Committees.
PROCEEDINGS or tHe EIGHTEENTH MEETING, at Swansea,
1848, Published at 9s.
ConTENTs :—Rev. Prof. Powell, A Catalogue of Observations of Luminous Meteors ;—
J. Glynn on Water-pressure Engines ;—R. A. Smith, on the Air and Water of Towns ;—Eighth
Report of Committee on the Growth and Vitality of Seeds ;—W. R. Birt, Fifth Report on At-
mospheric Waves ;—E. Schunck, on Colouring Matters ;—J. P. Budd, on the advantageous use
made of the gaseous escape from the Blast Furnaces at the Ystalyfera Iron Works;—R. Hunt,
Report of progress in the investigation of the Action of Carbonic Acid on the Growth of
Plants allied to those of the Coal Formations ;—Prof. H. W. Dove, Supplement to the Tem-
perature Tables printed in the Report of the British Association for 1847 ;—Remarks by Prof.
Dove on his recently constructed Maps of the Monthly Isothermal Lines of the Globe, and on
some of the principal Conclusions in regard to Climatology deducible from them; with anin- ©
troductory Notice by Lt.-Col. E. Sabine ;—Dr. Daubeny, on the progress of the investigation
on the Influence of Carbonic Acid on the Growth of Ferns ;—J. Phillips, Notice of further
progress in Anemometrical Researches ;—Mr. Mallet’s Letter to the Assistant-General Secre-
tary ;—-A. Erman, Second Report on the Gaussian Constants ;—Report of a Committee
relative to the expediency of recommending the continuance of the Toronto Magnetical and
Meteorological Observatory until December 1850.
Together with the Transactions of the Sections, the Marquis_of Northampton’s Address,
and Recommendations of the Association and its Committees.
PROCEEDINGS or tut NINETEENTH MEETING, at Birmingham,
1849, Published at 10s.
ConTENTS :—Rev. Prof. Powell, A Catalogue of Observations of Luminous Meteors ;—Earl
of Rosse, Notice of Nebulz lately observed in the Six-feet Reflector ;—Prof. Daubeny, on the
Influence of Carbonic Acid Gas on the health of Plants, especially of those allied to the Fossil
Remains found in the Coal Formation ;—Dr. Andrews, Report on the Heat of Combination ;
—Report of the Committee on the Registration of the Periodic Phenomena of Plants and
————— eC
PS OCT OSA IGEN.»
241
Animals ;—Ninth Report of Committee on Experiments on the Growth and Vitality of Seéds ;
—F. Ronalds, Report concerning the Observatory of the British Association at Kew, from
Aug. 9, 1848 to Sept. 12, 1849 ;—i. Mallet, Report on the Experimental Inquiry on Railway
Bar Corrosion ;—W. R. Birt, Report on the Discussion of the Electrical Observations at Kew.
Together with the Transactions of the Sections, the Rev. T. R. Robinson’s Address, and
Recommendations of the Association and its Committees,
PROCEEDINGS or rue TWENTIETH MEETING, at Edinburgh,
1850, Published at 15s.
ConTEnTs :—R. Mallet, First Report on the Facts of Earthquake Phenomena ;—Rev. Prof.
Powell, on Observations of Luminous Meteors;—Dr. T. Williams, on the Structure and
History of the British Annelida;—T. C. Hunt, Results of Meteorological Observations taken
at St. Michael’s from the Ist of January, 1840, to the 31st of December, 1849;—R. Hunt, on
the present State of our Knowledge of the Chemical Action of the Solar Radiations ;—Tenth
Report of Committee on Experiments on the Growth and Vitality of Seeds ;—Major-Gen.
Briggs, Report on the Aboriginal Tribes of India;—F. Ronalds, Report concerning the Ob-
servatory of the British Association at Kew ;—E. Forbes, Report on the Investigation of British
Marine Zoology by means of the Dredge ;—R. MacAndrew, Notes on the Distribution and
Range in depth of Mollusca and other Marine Animals, observed on the coasts of Spain, Por-
tugal, Barbary, Malta, and Southern Italy in 1849 ;—Prof. Allman, on the Present State of
our Knowledge of the Freshwater Polyzoa ;—Registration of the Periodical Phenomena of
Plants and Animals ;—Suggestions to Astronomers for the Observation of the Total Eclipse
of the Sun on July 28, 1851.
Together with the Transactions of the Sections, Sir David Brewster’s Address, and Recom~
mendations of the Association and its Committees.
PROCEEDINGS or tue TWENTY-FIRST MEETING, at Ipswich,
1851, Published at 16s. 6d.
CoNTENTS :—Rey. Prof. Powell, on Observations of Luminous Meteors ;—Eleventh Re-
port of Committee on Experiments on the Growth and Vitality of Seeds ;—Dr. J. Drew, on
the Climate of Southampton ;—Dr. R. A. Smith, on the Air and Water of Towns: Action of
Porous Strata, Water and Organic Matter ;—Report of the Committee appointed to consider
the probable Effects in an Giconomical and Physical Point of View of the Destruction of Tro-
pical Forests ;—A. Henfrey, on the Reproduction and supposed Existence of Sexual Organs
in the Higher Cryptogamous Plants;—Dr. Daubeny, on the Nomenclature of Organic Com-
pounds ;—Rey. Dr. Donaldson, on two unsolved Problems in Indo-German Philology ;—=
Dr. T. Williams, Report on the British Annelida;—R. Mallet, Second Report on the Facts of
Earthquake Phenomena ;—Letter from Prof. Henry to Col. Sabine, on the System of Meteoro-
logical Observations proposed to be established in the United States ;—Col. Sabine, Report
on the Kew Magnetographs ;—J. Welsh, Report on the Performance of his three Magneto-
graphs during the Experimental Trial at the Kew Observatory ;—-F. Ronalds, Report concern-
ing the Observatory of the British Association at Kew, from September 12, 1850, to July 31,
1851 ;—Ordnance Survey of Scotland.
Together with the Transactions of the Sections, Prof. Airy’s Address, and Recom-
mendations of the Association and its Committees.
PROCEEDINGS or raz TWENTY-SECOND MEETING, at Belfast,
1852, Published at 15s.
ConTENTs :—R. Mallet, Third Report on the Facts of Earthquake Phenomena ;—Twelfth
Report of Committee on Experiments on the Growth and Vitality of Seeds;—Rev. Prof.
Powell, Report on Observations of Luminous Meteors, 1851-52 ;—Dr. Gladstone, on the In-
fluence of the Solar Radiations on the Vital Powers of Plants;—A Manual of Ethnological
Inquiry ;—Col. Sykes, Mean Temperature of the Day, and Monthly Fall of Rain at 127 Sta-~
tions under the Bengal Presidency ;—Prof. J. D. Forbes, on Experiments on the Laws of the
Conduction of Heat;—R. Hunt, on the Chemical Action of the Solar Radiations ;—Dr. Hodges,
_ on the Composition and Giconomy of the Flax Plant ;—W. Thompson, on the Freshwater
_ Fishes of Ulster; —W. Thompson, Supplementary Report on the Fauna of Ireland;—W. Wills,
onthe Meteorology of Birmingham ;—J. Thomson, on the Vortex-Water-Wheel ;—J. B. Lawes
and Dr. Gilbert, on the Composition of Foods in relation to Respiration and the Feeding of
Animals.
Together with the Transactions of the Sections, Colonel Sabine’s Address, and Recom-
mendations of the Association and its Committees.
1860. 16
242
PROCEEDINGS or tue TWENTY-THIRD MEETING, at Hull,
1853, Published at 10s. 6d.
Contents :—Rev. Prof. Powell, Report on Observations of Luminous Meteors, 1852-53;
—James Oldham, on the Physical Features of the Humber ;—James Oldham, on the Rise,
Progress, and Present Position of Steam Navigation in Hull ;—William Fairbairn, Experi-
mental Researches to determine the Strength of Locomotive Boilers, and the causes which
lead to Explosion ;—J. J. Sylvester, Provisional Report on the Theory of Determinants ;—
Professor Hodges, M.D., Report on the Gases evolved in Steeping Flax, and on the Composition
and Economy of the Flax Plant ;—Thirteenth Report of Committee on Experiments on the
Growth and Vitality of Seeds ;—Robert Hunt, on the Chemical Action of the Solar Radiations;
—John P. Bell, M.D., Observations on the Character and Measurements of Degradation of the
Yorkshire Coast; First Report of Committee on the Physical Character of the Moon’s Sur-
face, as compared with that of the Earth;—R. Mallet, Provisional Report on Earthquake
Wave-Transits; and on Seismometrical Instruments ;—William Fairbairn, on the Mechanical
Properties of Metals as derived from repeated Meltings, exhibiting the maximum point of
strength and the causes of deterioration ;—Robert Mallet, Third Report on the Facts of Harth-
quake Phenomena (continued).
Together with the Transactions of the Sections, Mr. Hopkins’s Address, and Recommenda-
tions of the Association and its Committees.
PROCEEDINGS ofr tue TWENTY-FOURTH MEETING, at Liver-
pool, 1854, Published at 18s.
ConTENTS:—R. Mallet, Third Report on the Facts of Earthquake Phenomena (continued) ;
—Major-General Chesney, on the Construction and General Use of Efficient Life-Boats;—Rev.
Prof. Powell, Third Report on the present State of our Knowledge of Radiant Heat ;—Colonel
Sabine, on some of the results obtained at the British Colonial Magnetic Observatories ;—
Colonel Portlock, Report of the Committee on Earthquakes, with their proceedings respecting
Seismometers ;—Dr. Gladstone, on the influence of the Solar Radiations on the Vital Powers
of Plants, Part 2;—Rev. Prof. Powell, Report on Observations of Luminous Meteors, 1853-54 ;
—Second Report of the Committee on the Physical Character of the Moon’s Surface ;—W. G.
Armstrong, on the Application of Water-Pressure Machinery ;—J. B. Lawes and Dr. Gilbert,
on the Equivalency of Starch and Sugar in Food ;—Archibald Smith, on the Deviations of the
Compass in Wooden and Iron Ships ;—Fourteenth Report of Committee on Experiments on
the Growth and Vitality of Seeds.
Together with the Transactions of the Sections, the Earl of Harrowby’s Address, and Re-
commendations of the Association and its Committees,
PROCEEDINGS or tot TWENTY-FIFTH MEETING, at Glasgow,
1855, Published at 15s.
ConTENTS :—T. Dobson, Report on the Relation between Explosions in Coal-Mines and
Revolving Storms;—Dr. Gladstone, on the Influence of the Solar Radiations on the Vital Powers
of Plants growing under different Atmospheric Conditions, Part 3 ;—C. Spence Bate, on the
British Edriophthalma ;—J. F. Bateman, on the present state of our knowledge on the Supply
of Water to Towns ;—Fifteenth Report of Committee on Experiments on the, Growth and
Vitality of Seeds ;—Rev. Prof. Powell, Report on Observations of Luminous Meteors, 1854—55 ;
—Report of Committee appointed to inquire into the best means of ascertaining those pro-
perties of Metals and effects of various modes of treating them which are of importance to the
durability and efficiency of Artillery ;—Rev. Prof. Henslow, Report on Typical Objects in
Natural History ;—A. Follett Osler, Account of the Self-Registering Anemometer and Rain- —
Gauge at the Liverpool Observatory ;—Provisional Reports.
Together with the Transactions of the Sections, the Duke of Argyll’s Address, and Recom-
mendations of the Association and its Committees.
PROCEEDINGS or tHe TWENTY-SIXTH MEETING, at Chel-
tenham, 1856, Published at 18s.
ConTENTs ;—Report from the Committee appointed to investigate and report upon the —
effects produced upon the Channels of the Mersey by the alterations which within the last
fifty years have been made in its Banks;—J. Thomson, Interim Report on progress in Re-
searches on the Measurement of Water by Weir Boards ;—Dredging Report, Frith of Clyde,
1856 ;=—Rev. B. Powell, Report on Observations of Luminous Meteors, 1855-1856 ;—Prof.
Bunsen and Dr. H. E. Roscoe, Photochemical Researches ;—Rev. James Booth, on the Trigo-
243
nometry of the Parabola, and the Geometrical Origin of Logarithms ;—R. MacAndrew, Report
on the Marine Testaceous Mollusca of the North-east Atlantic and Neighbouring Seas, and
the physical conditions affecting their development ;—P. P. Carpenter, Report on the present
state of our knowledge with regard to the Mollusca of the West Coast of North America ;-—
T. C. Eyton, Abstract of First Report on the Oyster Beds and Oysters of the British Shores ;
——Prof. Phillips, Report on Cleavage and Foliation in Rocks, and on the Theoretical Expla-
nations of these Phenomena: Part I. ;--Dr. T. Wright on the Stratigraphical Distribution of
the Oolitic Echinodermata ;—W. Fairbairn, on the Tensile Strength of Wrought Iron at various
Temperatures ;——C. Atherton, on Mercantile Steam Transport Economy ;—J. S. Bowerbank, on
the Vital Powers of the Spongiadz;——Report of a Committee upon the Experiments conducted
at Stormontfield, near Perth, for the artificial propagation of Salmon ;—Provisional Report on
the Measurement of Ships for Tonnage ;—On Typical Forms of Minerals, Plants and Animals
for Museums ;—J. Thomson, Interim Report on Progress in Researches on the Measure-
ment of Water by Weir Boards;--R. Mallet, on Observations with the Seismometer ;—A.
Cayley, on the Progress of Theoretical Dynamics ;—Report of a Committee appointed to con-
sider the formation of a Catalogue of Philosophical Memoirs.
Together with the Transactions of the Sections, Dr. Daubeny’s Address, and Recom-
mendations of the Association and its Committees.
PROCEEDINGS or tut TWENTY-SEVENTH MEETING, at Dub-
lin, 1857, Published at 15s.
Conrents :—A. Cayley, Report on the Recent Progress of Theoretical Dynamics ;—Six-
teenth and final Report of Committee on Experiments on the Growth and Vitality of Seeds ;
—James Oldham, C.E., continuation of Report on Steam Navigation at Hull;—Report of a
Committee on the Defects of the present methods of Measuring and Registering the Tonnage
of Shipping, as also of Marine Engine-Power, and to frame more perfect rules, in order that
a correct and uniform principle may be adopted to estimate the Actual Carrying Capabilities
and Working-Power of Steam Ships;—Robert Were Fox, Report on the Temperature of
some Deep Mines in Cornwall;—Dr. G. Plarr, De quelques Transformations de la Somme
— & tlt Bil+15¢|+1
0 yéltiytl+et|+1
est exprimable par une combinasion de factorielles, la notation atl+1 désignant le produit des
t facteurs a (a+1) (a+2) &c....(a+¢—1);—G. Dickie, M.D., Report on the Marine Zoology
of Strangford Lough, County Down, and corresponding part of the Irish Channel ;—Charles
Atherton, Suggestions for Statistical Inquiry into the extent to which Mercantile Steam Trans-
port Economy is affected by the Constructive Type of Shipping, as respects the Proportions of
Length, Breadth, and Depth ;—J. 8. Bowerbank, Further Report on the Vitality of the Spon-
giadez ;—John P. Hodges, M.D., on Flax ;—Major-General Sabine, Report of the Committee
on the Magnetic Survey of Great Britain ;—Rev. Baden Powell, Report on Observations of
Luminous Meteors, 1856-57 ;—C. Vignoles, C.E., on the Adaptation of Suspension Bridges to
sustain the passage of Railway Trains ;—Professor W. A. Miller, M.D., on Electro-Chemistry ;
—John Simpson, R.N., Results of Thermometrical Observations made at the ‘ Plover’s’
Wintering-place, Point Barrow, latitude 71° 21’ N., long. 156° 17’ W., in 1852—54 ;—Charles
James Hargrave, LL.D., on the Algebraic Couple ; and on the Equivalents of Indeterminate
Expressions;—Thomas Grubb, Report on the Improvement of Telescope and Equatorial
Mountings ;—Professér James Buckman, Report on the Experimental Plots in the Botanical
Garden of the Royal Agricultural College at Cirencester ;—William Fairbairn on the Resistance
of Tubes to Collapse ;—George C. Hyndman, Report of the Proceedings of the Belfast Dredging
Committee ;—Peter W. Barlow, on the Mechanical Effect of combining Girders and Suspen-
sion Chains, and a Comparison of the Weight of Metal in Ordinary and Suspension Girders,
to produce equal deflections with a given load ;—J. Park Harrison, M.A., Evidences of Lunar
Influence on Temperature ;—Report on the Animal and Vegetable Products imported into
Liverpool from the year 1851 to 1855 (inclusive) ;—Andrew Henderson, Report on the Sta-
tistics of Life-boats and Fishing-boats on the Coasts of the United Kingdom.
Together with the Transactions of the Sections, Rev. H. Lloyd’s Address, and Recommen-
dations of the Association and its Committees.
, a étant entier négatif, et de quelques cas dans lesquels cette somme
PROCEEDINGS or tue TWENTY-EIGHTH MEETING, at Leeds,
September 1858, Published at 20s.
Conrents:—R. Mallet, Fourth Report upon the Facts and Theory of Earthquake Phe-
nomena ;— Rev. Prof. Powell, Report on Observations of Luminous Meteors, 1857-58 ;—R. H.
Meade, on some Points in the Anatomy of the Araneidea, or true Spiders, especially on the
16*
244
internal structure of their Spinning Organs ;—W. Fairbairn, Report of the Committee on the
Patent Laws ;—S. Eddy, on the ]uead Mining Districts of Yorkshire ;—W. Fairbairn, on the
Collapse of Glass Globes and Cylinders ;—Dr. E. Perceval Wright and Prof. J. Reay Greene,
Report on the Marine Fauna of the South and West Coasts of Ireland ;—Prof. J. Thomson, on
Experiments on the Measurement of Water by Triangular Notches in Weir Boards ;—Major-
General Sabine, Report of the Committee on the Magnetic Survey of Great Britain ;—Michael
Connal and William Keddie, Report on Animal, Vegetable, and Mineral Substances imported
from Foreign Countries into the Clyde (including the Ports of Glasgow, Greenock, and Port
Glasgow) in the years 1853, 1854, 1855, 1856, and 1857 ; Report of the Committee on Ship-
ping Statistics;—Rev. H. Lloyd, D.D., Notice of the Instruments employed in the Mag-
netic Survey of Ireland, with some of the Results;—Prof. J. R. Kinahan, Report of Dublin
Dredging Committee, appointed 1857-58 ;—Prof. J. R. Kinahan, Report on Crustacea of Dub-
lin District ;—Andrew Henderson, on River Steamers, their Form, Construction, and Fittings,
with reference to the necessity for improving the present means of Shallow-Water Navigation
on the Rivers of British India;—George C. Hyndman, Report of the Belfast Dredging Com-
mittee ;—Appendix to Mr. Vignoles’ paper ‘‘ On the Adaptation of Suspension Bridges to sus-
tain the passage of Railway Trains ;’’—Report of the Joint Committee of the Royal Society and
the British Association, for procuring a continuance of the Magnetic and Meteorological Ob-
servatories;—R. Beckley, Description of a Self-recording Anemometer.
Together with the Transactions of the Sections, Prof. Owen’s Address, and Recommenda-
tions of the Association and its Committees.
PROCEEDINGS or tur TWENTY-NINTH MEETING, at Aberdeen,
September 1859, Published at 15s.
Contents :—George C. Foster, Preliminary Report on the Recent Progress and Present
State of Organic Chemistry ;—Professor Buckman, Report on the Growth of Plants in the
Garden of the Royal Agricultural College, Cirencester ;—Dr. A. Voelcker, Report on Field
Experiments and Laboratory Researches on the Constituents of Manures essential to cultivated
Crops ;—A. Thomson, Esq. of Banchory, Report on the Aberdeen Industrial Feeding Schools ;
—On the Upper Silurians of Lesmahago, Lanarkshire ;—Alphonse Gages, Report on the Re-
sults obtamed by the Mechanico-Chemical Examination of Rocks and Minerals ;—William
Fairbairn, Experiments to determine the Efficiency of Continuous and Self-acting Breaks for
Railway Trains ;—Professor J. R. Kinahan, Report of Dublin Bay Dredging Committee for
1858-59 ;—Rev. Baden Powell, Report on Observations of Luminous Meteors for 1858-59 ;
—Professor Owen, Report on a Series of Skulls of various Tribes of Mankind inhabiting
Nepal, collected, and presented to the British Museum, by Bryan H. Hodgson, Esgq., late Re-
sident in Nepal, &c. &c. ;—Messrs. Maskelyne, Hadow, Hardwich, and Llewelyn, Report on
the Present State of our Knowledge regarding the Photographic Image ;—G. C. Hyndman,
Report of the Belfast Dredging Committee for 1859 ;—James Oldham, Continuation of Report
of the Progress of Steam Navigation at Hull;—Charles Atherton, Mercantile Steam Trans-
port Economy as affected by the Consumption of Coals ;—Warren de la Rue, Report on the
present state of Celestial Photography in England ;—Professor Owen, on the Orders of Fossil
and Recent Reptilia, and their Distribution in Time ;—Balfour Stewart, on some Results of the
Magnetic Survey of Scotland in the years 1857 and 1858, undertaken, at the request of the
British Association, by the late John Welsh, Esq., F.R.S.;—W. Fairbairn, The Patent Laws:
Report of Committee on the Patent Laws;—J. Park Harrison, Lunar Influence on the Tem-
perature of the Air;—Balfour Stewart, an Account of the Construction.of the Self-recording
Magnetographs at present in operation at the Kew Observatory of the British Association ;—
Prof. H. J. Stephen Smith, Report on the Theory of Numbers: Part I.;—Report of the
Committee on Steam-ship performance ;—Report of the Proceedings of the Balloon Committee
of the British Association appointed at the Meeting at Leeds ;—Prof. William K. Sullivan,
Preliminary Report on the Solubility of Salts at Temperatures above 100° Cent., and on the
Mutual Action of Salts in Solution.
Together with the Transactions of the Sections, Prince Albert’s Address, and Recommenda-
tions of the Association and its Committees.
PE et ee
List of those Members of the British Association for the Advancement
of Science, to whom Copies of this Volume [for 1860] are supplied
gratuitously, in conformity with the Regulations adopted by the General
Committee.
[See pp. xvii & xvin.]
HONORARY MEMBER.
HIS ROYAL HIGHNESS THE PRINCE CONSORT,
LIFE MEMBERS.
Adair, Colonel Robert A. Shafto, F.R.S.,
7 Audley Square, London.
Adams, John Couch, M.A., D.C.L.,
F.R.S., F.R.A.S., Lowndsean Professor
of Astronomy and Geometry in the
University of Cambridge; Pembroke
College, Cambridge.
Adie, Patrick, 16 Sussex Place, South
Kensington, London.
Ainsworth,Thomas,The Flosh, Egremont,
Cumberland.
Aldam, William, Frickley Hall near Don-
caster.
Allen, William J. C., Secretary to the
Royal Belfast Academical Institution ;
8 Wellington Place, Belfast.
Allis, Thomas, F,L.S., Osbaldwick Hall
near York.
Ambler, Henry, Watkinson Hall, Oven-
den near Halifax.
Amery, John, F.S.A.,
- Stourbridge.
Anderson, William (Yr.), Glentarkie, Fife.
Andrews, Thos., M.D., F.R.S., M.R.1.A.,
Vice-President of, and Professor of
Chemistry in, Queen’s College, Belfast.
Ansted, David Thomas, M.A., F.R.S.,
F.G.S., Lecturer on Geology at the
Royal East India Military College, Ad-
discombe; Athenzum Club, and Bon
Air, St. Martin, Guernsey.
Appold, John George, F.R.S., 23 Wilson
Street, Finsbury Square, London.
Archer, T. C., Professor of Botany in
Queen’s College, Liverpool; Higher
Tranmere, Cheshire.
Armstrong, Sir William George, C.B.,
F.R.S., Elswick Engine Works, New-
castle-upon-Tyne.
Arthur, Rev. William, M.A., 26 Campden
Grove, Kensington, London.
Ashburton, William Bingham Baring,
Lord, M.A., F.R.S., Bath House, Pic-
cadilly, London, and The Grange,
Hants.
Park House,
Ashton, Thomas, M.D., 81 Mosley St.,
Manchester.
Ashworth, Edmund, Egerton Hall,Turton
near Bolton.
Atkinson, John Hastings, 14 East Parade,
Leeds.
Atkinson, Joseph B., Cotham, Bristol.
Atkinson, J. R. W., 38 Acacia Road,
Regent’s Park, London.
Atkinson, Richard, jun.,31 College Green,
Dublin.
Auldjo, John, F.R.S.
Austin, Rev. William E. Craufurd, M.A.,
New College, Oxford.
Ayrton, W. §., F.S.A., Allerton Hill,
Leeds.
Babbage, Charles, M.A., F.R.S., 1 Dorset
Street, Manchester Square, London.
Babington, Charles Cardale, M.A.,F.R.S.,
Professor of Botany in the University
of Cambridge; St. John’s College,
Cambridge, (Local Treasurer).
Backhouse, John Church, Blackwell,
Darlington.
Baddeley, Captain Frederick H., R.E.,
Ceylon. :
Bain, Richard, Gwennap near Truro.
Bainbridge, Robert Walton, Middleton
House near Barnard Castle, Durham.
Baines, Edward, Headingley Lodge,
Leeds.
Baines, Samuel, Victoria Mills, Brig-
house, Yorkshire.
Baker, Henry Granville, Bellevue, Hors-
forth near Leeds.
Baker, Johu, Dodge Hill, Stockport.
Baker, William, 63 Gloucester Place,
Hyde Park, London.
Baldwin, The Hon. Robert, H.M. Attor-
ney-General, Spadina, Co. York, Upper
Canada.
Balfour, John Hutton, M.D., Professor of
Botany in the University of Edinburgh,
F.R.S. L. & E., F.L.S.; Edinburgh.
[It is requested that any inaccuracy in the Names and Residences of the Members may be communicated to
Messrs, Taylor and Francis, Printers, Red Lion Court, Fleet Street, London.]
246
Ball, John, M.R.I.A., F.L.S., 18 Park
Street, Westminster.
Ball, William, Rydall, Ambleside, West-
moreland.
Barbour, Robert, Portland Street, Man-
chester.
Barclay, J.Gurney, Walthamstow, Essex.
Barclay, Robert, Leyton, Essex.
Barker, Rev. Arthur Alcock, Rector of
East Bridgeford, Nottinghamshire.
Barnes, Thomas, M.D.,F.R.S.E., Carlisle.
Barnett, Richard, M.R.C.S., 11 Victoria
Square, Reading.
Bartholomew, Charles, Rotherham.
Bartholomew, William Hamond, 5 Grove
Terrace, Leeds.
Barton, John, Bank of Ireland, Dublin.
Barwick, John Marshall, Albion Street,
Leeds.
Bashforth, Rey. Francis, B.D., Minting
near Horncastle, Lincolnshire.
Bateman, Joseph, LL.D., F.R.A.S., J.P.
for Middlesex, &c., 24 Bedford Place,
Kensington, London.
Bayldon, John, Horbury near Wakefield.
Bayley, George, 2 Cowper’s Court, Corn-
hill, London.
Beale, Lionel S., M.B., F.R.S., Professor
of Physiology and of General Morbid
Anatomy in King’s College, London ;
61 Grosvenor Street, London.
Beamish, Richard, F.R.S., 2 Suffolk
Square, Cheltenham.
Beatson, William, Rotherham.
Beaufort, William Morris, India.
Beck, Joseph, 6 Coleman Street, London.
Beckett, William, Kirkstall Grange, Leeds.
Belcher, Captain Sir Edward, R.N.,
F.R.A.S.
Bell, Matthew P., 245 St. Vincent Street,
Glasgow.
Bennoch, Francis, The Knoll, Blackheath,
Kent.
Bergin, Thomas Francis, M.R.I.A., 49
Westland Row, Dublin.
Berryman, William Richard, 6 Tamar
Terrace, Stoke, Devonport.
Bickerdike, Rev. John, M.A., Leeds.
Binyon, Thomas, St. Ann’s Square, Man-
chester.
Bird, William, 9 South Castle Street, Li-
verpool.
Birks, Rev. Thomas Rawson, Kelshall
Rectory, Royston.
Birley, Richard, Sedgley,
Manchester.
Birt, W. Radcliff, F.R.A.S., lla, Wel-
lington Street, Victoria Park, London.
Prestwich,
Terrace, Glasgow.
MEMBERS TO WHOM
Blackwall, John, F.L.S., Hendre House
near Llanrwst, Denbighshire.
Blackwell, Thomas Evans, F.G.S., Mon-
treal.
Blake, Henry Wollaston, F.R.S., 8 Devon-
shire Place, Portland Place, London.
Blake, William, Bishop’s Hull, Taunton.
Blakiston, Peyton, M.D., F.R.S., St.
Leonard’s-on-Sea.
Bland, Rev. Miles, D.D., F.R.S., 5 Royal
Crescent, Ramsgate.
Blythe, William, Holland “Bank, Church
near Accrington.
Bohn, Henry G., F.R.G.S., York Street,
Covent Garden, London.
Boileau, Sir John Peter, Bart., F.R.S.,
20 Upper Brook Street, London; and
Ketteringham Hall, Norfolk.
Bond, Walter M., The Argory, Moy,
Ireland.
Bossey, Francis, M.D., 4 Broadwater
Road, Worthing.
Bowerbank, James Scott, LL.D., F.R.S.,
3 Highbury Grove, London.
Bowlby, Miss F, E., 27 Lansdown Cres-
cent, Cheltenham.
Brady, Antonio, Maryland Point, Essex.
Brady, Cheyne, M.R.I.A., 54 Upper
Leeson Street, Dublin.
Brakenridge, John, Bretton Lodge,
Wakefield.
Brebner, James, 20 Albyn Place,Aberdeen.
Brett, John Watkins, 2 Hanover Square,
London.
Briggs, Major-General John, F.R.S., 2
Tenterden Street, London.
Brodie, Sir Benjamin Collins, Bart.,
D.C.L., President of the Royal Society ;
Broome Park, Betchworth, Surrey.
Brooke, Charles, B.A,, F.R,S., 16 Fitzroy
Square, London.
Brooks, Samuel, King Street, Manchester.
Brooks, Thomas, (Messrs. Butterworth
~ and Brooks,) Manchester.
Broun, John Allan, F.R.S., Astronomer
“to His Highness the Rajah of Tra-
vancore ; Observatory, Trevandrum,
India.
Brown, Samuel, F.S.S., The Elms, Lark-
hall Rise, Clapham, London.
Brown, Thomas, Ebbw Vale Iron Works,
Abergavenny.
Brown, William, 3 Maitland Park Villas,
Haverstock Hill, London.
Bruce, Alexander John, Kilmarnock.
Buck, George Watson, Rae: Isle of
Man.
5 Buckman, James, F.L.S., F.G. Si Profes-
Blackie, W. G., Ph.D., F.R.G.S., 10 Kew |
sor of Natural History in the Royal
Agricultural College, Cirencester.
Ge
BOOKS ARE SUPPLIED GRATIS.
Buckton, G. Bowdler, F.R.S., 55 Queen’s
Gardens, Hyde Park, London.
Budd, James Palmer, Ystalyfera Iron
Works, Swansea.
Buller, Sir Antony, Pound near Tavistock,
Devon.
Burd, John, jun., Mount Sion, Radcliffe,
Manchester. 4
Busk, George, F'.R.S., Sec. L.S., 15 Har-
ley Street, Cavendish Square, London.
Butlery, Alexander W., Monkland Iron
and Steel Company, Cardarroch near
Airdrie.
Caine, Rev. William, M.A., Greenheys,
Manchester.
Caird, James T., Greenock.
Campbell, Dugald, F.C.S.,7 Quality Court,
Chancery Lane, London.
Campbell, Sir James, Glasgow.
Campbell, William, 34 Candlerigg Street,
Glasgow.
Carew, William Henry Pole, Antony
House near Devonport.
Carpenter, Philip Pearsall, B.A., Ph.D.,
Cairo Street, Warrington.
Carr, William, Blackheath.
Cartmell, Rev. James, B,D., F.G.S.,
Master of Christ’s College, Cambridge.
Cassels, Rev. Andrew, M.A., Batley Vi-
carage near Leeds.
Chadwick, Charles, M.D., 35 Park Square,
Leeds.
Challis, Rev. James, M.A., F.R.S., Plu-
mian Professor of Astronomy in the
University of Cambridge ; Observatory,
Cambridge.
Chambers, Robert, F.R.S.E., F.G.S.,
1 Doune Terrace, Edinburgh.
Champney, Henry Nelson, St. Paul’s
Square, York.
Chanter, John, 2 Arnold Terrace, Bow
Road, Bromley.
Cheetham, David, Staleybridge, Man-
chester.
Chesney, Major-General Francis Rawdon,
R.A.,'D.C.L., F.R.S., Ballyardle, Kil-
keel, Co. Down, Ireland.
Chevallier, Rev. Temple, B.D., F.R.A.S.,
Professor of Mathematics and Astro-
nomy in the University of Durham.
Chichester, Ashhurst Turner Gilbert,D.D.,
Lord Bishop of, 31 Queen Anne Street,
Cavendish Square, London, and The
Palace, Chichester.
Chiswell, Thomas.
Christie, Samuel Hunter, M.A., F.R.S.,
Ailsa Villas, St. Margaret’s, Twick-
enham,
24:7
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Phys., 38 Broad Street, Oxford.
Gages, Alphonse, Museum of Irish In-
dustry, Dublin.
Gassiot, John P., F.R.S., Clapham Com-
mon, London.
Gerard, Henry, 13 Rumford Place, Liver-
pool,
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Gibson, Thomas F., 124 Westbourne
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Grant, Robert, M.A., F.R.A.S., Professor
of Astronomy in the University of
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Greene, Professor J. Reay, M.R.I.A.,
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Greenwood, William, Stones, Todmorden,
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Greg, Robert Philips, F.G.S., (Local
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Gregor, Walter, Macduff, Banff.
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Hay, Sir Andrew Leith, Bart., Rannes,
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Hennessy, Henry, F.R.S., M.R.L.A.,
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Hervey, The Rey. Lord Arthur, Ickworth,
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tenham.
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mon, London.
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Hunt, James, Ph.D., F.S.A., Hon. Sec.
Ethnol. Soc.; Ore House; Hastings.
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hurst ; 18 Bessborough Gardens, Pim-
lico, London.
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bledon Park, Surrey.
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Kinahan, G. Henry, Geological Survey
of Ireland, 51 Stephen’s Green, Dublin.
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Latham, R. G., M.D., F.R.S., Greenford,
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Leslie, William, M.P., Warthill, Aber-
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Printed by Taylor and Francis, Red Lion Court, Fleet Street.
a2 :”:—C Oe ee
ELST OF PGA TES.
PLATES 1., II., III.
Illustrative of Captain Maury’s paper on the Climate of the Antarctic
Regions, as indicated by observations upon the height of the Barometer,
and direction of the Winds at Sea.
PLATES IV. to VIII.
Illustrative of the Rev. W. Vernon Harcourt’s Report on the Effects of long-
continued Heat, illustrative of Geological Phenomena.
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