ae ant F ee atin: nti he * . elena ty av THE PHILOSOPHICAL MAGAZINE: COMPREHENDING THE VARIOUS BRANCHES OF SCIENCE, THE LIBERAL AND FINE ARTS, GEOLOGY, AGRICULTURE, MANUFACTURES AND COMMERCE. rer E, BY ALEXANDER TILLOCA, M.R.LA. F.S.A. EpiIn. anp Perts, &c. ora as ae ee es eee ae eae anor See t Nec aranearum sane textus ideo melior -quia ex se fila gignunt, nec noster vitior quia ex alienis libamus ut apes,” Just. Lips. Monit, Polit, lib. i. cap. t. ae VOL. XXXIX. For JANUARY, FEBRUARY, MARCH, APRIL, MAY, and JUNE, 1812. (on a ee LONDON: PRINTED BY RICHARD TAYLOR AND CO., SHOE LANE: And sold by Ricnarpsons; Capgct and Davies; Loncman, Hurst, Rees, Oxme, and Brown; VeRNox, Hoop, and SHarPe; Mur- BAY ; Hicutey ;SHerwoop and Co.; Haxpine; London: Consrasie and Co, Edinburgh: Brass and Reip, and Niven, Glasgow: & Girsert & Hopess, Dublin. AVS Mies Maks US x wets pea TE Ps, Ly & : Pe Aa | r. y A“ cy? Saree |. S,. ae) ©. oe os py Mir ; aes i ~ pares |
  • Ay eta if mat mp 5 , t rat £ 4 e : f : ; era? eo > a =, we < — etal : We % ; : a 4a) ’ , g y alt ain satan Sabi enn sein cen erg ey ar socnaactal essayeke ls bac Sack, wl CON TERS GF THE THIRTY-NINTH VOLUME. A SYNOPSIS of the principal Elements of Astronomy ; deduced from M. LapLace’s SRE du Systéme du ‘Monde .. .. Balt ene 3 An Account of the Great pacer nen Denudation .. 26 Description of a new Levelling-Staff .. +. «+ 35 On the Cause of audible Sound in vibrating Strings, Tuning- Forks, €c.; on the Use of Hawxtns’s Mouth Tuning - Forks; on Earl STANHoPE’s roe Steel Piano- Forte Strings, &c. entice 3 4 DS «se Mae: 8 On the Nomenclature of the New ads Mtsncdectts 39 General Method for determining the Orbits of Comets 40 A Case of Morlbus Pedicularis .. .. » 49 Reply to Dr. Kexry’s Letter on his eos Baia of an Error in the Nautical Almanac .. .«- «+. 51 A Reply to some Observations and Conclusions in a Paper just published, in the Second Volume of the Medico- Chirurgical Transactions, on the Nature of the Alkaline Matter contained in various dropsical Fluids, and in the Serum of the Blood .. «+: «+ «sa oe «- 64 On the Localities of certain Reliquia, or extraneous Fossils, found in Dérbyshire 4. «+ se oe e+ oe 81 Account of some remarkable Cases of Venereal Infection 90 Val, 39. No. 170, June 1812. * CONTENTS. Geological Observations, in Correction of and Addition te the Puper on the Great Derbyshire Denudation, and the Resort pn Dertystare, Seta | ee) aM | Desultory Olservations concerning certain vegetalle Mus- cicape Re et Tew) etse e's. Cpe ALOR Case of Injury ofchosees oa ngaheh ous 8 ay Communications from Mr, Autan and Mr. STANCLIFFE on Allan’s Dividing Instrument .. .. .. «. 119 An Answer to the Observations of Dr. PEARSON (see page | 64) on certain Statements respecting the alkaline Matter contained in dropsical Fluids, end in the Serum of the OME ie 9 a ees mi A Re sh 4a me) ee Description of the Diacatopiron .. «2 «2 «+ 127 Description of a Cavern near Chudleigh in Devonshire 161 On the different Qualities of Wines, and the Methods of preserving and ameliorating them 6. ww 165 An Apparatus for preventing the Accumulation of Air in Conduit Pipes, &c. Se. Ese cai sot coda mtae Memoir upon the Mordants emplo fied in the Art of Piper big as ain ie wh Sipe lamin ts eee An Account of the Stevens Oa is.) le Extracts from Mr. Joun Farey’s jirst Volume of Report to the Board of Agriculture, on Derbyshire 191, 253 On the Radiation of Cold .. ws ++. +e oe 208 A Sketch of the Natural History of the Cheshire Rocke SE ISITE a a Cpe ee nas RU eRe On the Nautical "Ephemeris *.. ew ee we 2S Substitute fora Repeating Watch .. .. .. «. 216 Description of an Improvement on La Borpa’s Reflecting De cos, Mad thn se aig © ae on wn eae ieee Description of an inclosed Grindstone, intended to prevent prejudicial Effects to the Persons eae in pointing DOME ea ce ee ee eas ee eee aes Oe Description of a Contrivance for conveying Steam from Boilers oe ce ee ee ee ee ee ee ee 264 \» eer ee CONTENTS. Geological Observations on the County of Antrim, and others in the North-east Part of Ireland, Sc. .. 266, 353 Experiments on the Strength of Men and Horses in moving Machines... See ee, es yet se aes A Rejoinder to a Paper published in the Philosophical Ma- gazine, by Dr. Marcst, on the Animal Fluids .. 289 Case of Hernia Umbilicalis, operated on with Success during Utero-gestation .. «. gray aR le UD Notice respecting the Geblogica? Stra ucture of the Vicinity of Dublin: with an Account of some tare Minerals found MAT Os, en hie spe ee CE ee RTD Biographical Sketch of the late Maxwe_t GARTHSHORE, DID FR. 9. 69 S.A, MN Ley be ee na aes Bee An Account of the Coal Measures or Strata, lately explored, on the Water of Brora, in the Valley S of Clyne, near the SE Coast of Sutherland in Scotland, extracted from Capt. Joun Henperson’s Agricultural Survey of the Cnr OF SATIRE ns: ic apis eek mela Cook. eon On Gypsum near Doncaster, and Nodules of Limestone, and of Pyrites containing Sea Shells, in the Coal-district near Bradford.in Yorkshire . +, 6+ +. .0», $52 Description of an improved Pump for raising the Water while Shafts or Pits are sinking .. Sta Web ro 4 Further Remarks on a Case of Injury of the Brain .. 367 A Metnod of abs the Variation of the Mariner’s PONE ra Sui capers Kea rik oie Aen a eee TEE TO On the Rev. Mr. aie ron’s EUHARMONIC ORGAN, and his “<< Essay on perfect Intonation,” for explaining fully the Principlés of Tuning, and of performing upon the same with perfect Harmonies, in almost every possible Variety meer sani Prastaes a k's) Nee ee Shee OTS A new Solution of two Fluxions proposed ly Simpson 383 Some Account of the Methods of laying the Foundations of — TOILE GO co, 00. tel 69?) an. ee ial) ea CONTENTS. Further Remarks on the Rev. Mr. Liston’s “‘ Essay on perfect Intonation,” &c. A tk 8 an ee Qn Vegetable Fae 165 we inn Dm ager oa oes Correction of an erroneous Statament in the Account of Mr. BAKEWELL’s Lectures, &c. A. ob Aa eo On the Effects produced by the Use of the Oxymuriates of Lime and Magnesia in Bleaching .. .. «2 429 Method of preparing a cheap and durable Stucco, or Plaster, for outside or inside Wallis’ .. 20: oe. 00 2» 430 Cases of Hernia. 6 ee. 420, a os 435 On the Culture and Ereivaton of ‘Hemp in Dersetifire, and on the Growth of Sea Cale .. .. «2 «2 437 On a gaseous Compound of carbonic Oxide and Chlorine 443 New Tables for finding the Deviation of a Star in North Polar Distance and Right Ascension .. .. «- 448 A Narrative of the Eruption of a Volcano in the Sea off the dstand of Si. NUChigl sie: oe we op ae) oo eee On the primitive Crystals of Carbonate of Lime, Bitter- marae IFON=Spar 8 ee ee be Mee ee Soe , Notices respecting New Books .. «+ «+ «+ 217, 458 Proceedjngs of Learned Societies 72,130, 219,311, 385, 459 Intelligence and Miscellaneous Articles 77, 152, 244, 321, 402, 474 Sst of Patents .0 eee A 7G, (156,38 Meteorological Table 80, 160, 248, 327, 328, 408, 481 THE THE PHILOSOPHICAL MAGAZINE. 1. A Synopsis of the principal Elements of Astronomy ; de« duced from M. Lartace’s Exposition du Systeme du Monde. Communicated by Francis Batty, Esq. Tue following paper possesses po further merit thar as being a faithful abstract of the principles and facts given by M. Laplace in his Faposition du Systeme du Monde. It is taken from the third edition of that work (1808), wherein the author has given the elements of the planets in a more correct manner than in either of the preceding edi- tions; and wherein he has revised and amended all his for- mer calculations by more recent and exact observations. The arrangement of the present memoir is somewhat new: but many persons have frequently found the want of a manual of this kind, where all the different facts, relative to astronomy, might be brought under their respective heads, without the necessity of turning to a variety of works for information. Much time is often lost in a re- search of that kind, which it is.the object of the present abstract to prevent. Tn the original work, the author has universally adopted the decimal division of the day, and of the quadrant. This method is here preserved in the Tables of the Elements of the Planets (page 6): but, in the subsequent parts, the common sexagesimal notation is adopted, as being more easily understood in this country. Some other facts, not mentioned by M. Laplace, are in- serted in this tract, in order to enlarge the view of the sub- ject: but these passages are always kept separate, by being inclosed within brackets. Vol. 39. No. 165. Jan. 1812. AQ The 4 A Synopsis of the principal The Sun. The Sun, which is the source of light and heat to our system, is the most considerable of all the heavenly bodies ; and governs all the planetary motions. eine «i Its diameter is 111°454 times the mean diameter of the Earth: whence its volwme is 1384472 times greater than that of the Earth: but its mass is only 337086 times greater, Whence we conclude that its density is z5'yx5, or about 4 that of our globe. Jt is surrounded by an aimosphere: and it 1s oftentimes covered with spots. Some of these spots have been ob- served so large as to exceed the Earth 4 or 5 times in mag- niiude. The observation of these spots shows that the Sun moves on its axis, which is nearly perpendicular to the ecliptic: and the duration of an entire sidereal rotation of the Sun is about 253 days. Whence we conclude that the Sun is flattened at the poles. The solar equator is inclined 7° 30’ to the plane of the ecliptic. . A body, which weighs one pound at the surface of the Earth, would, if removed to the surface of the Sun, weigh 27°933 pounds. And bodies would fall there with a velocity of 334°65 feet in the first second of time. The Sun, together with the planets, moves round the common centre of gravity of the system: whick centre is nearly in the centre of the Sun. This motion changes into epicycloids the ellipses of the planets and comets, which revolve round the Sun, The Sun appears to have a particular motion, which car- ries our system towards the constellation of Hercules. The apparent diameter of the Sun, as seen from the Earth, undergoes a periodical variation. 't is greatest when the Earth is in its perihelion; at which time it is 32’ 35”,6: and it is least when the Earth is in its aphelion; at which time itis 31’ 31’,0. Its mean apparent diameter is therefore 32’ 3”,3. His horizontal parallax is 83”. The greatest equation of his centre is 1° 55’ 27”,73 which diminishes at the rate of 16,9 in a century. The diurnal motion of the Sun from east to west, and his annual motion in the ecliptic, are optical deceptions; arisiny from the real motion of the Earth on its axis, and in its orbit, The | Elements of Astronomy: 5 ‘ The Planets. The number of planets belonging to our system is eleven. Six of thesé have been known and recognised from time immemorral': namely, Mercury, Venus, the Earth, Mars, Jupiter, and Saturn. But the remaining five, which are not visible to the naked eye, have lately been discovered by the help of the telescope; aid are therefore called telescopic planets: namely, a2 Uranus, discovered by Dr. Herschel, March 13, 1781. Ceresy re. OM) Piazai, .. Januaryib 180 Pallas, « ...6:..\e00% -', Ms Olbers, .:. March 98, 18092. MGs syiehhs #3 as . M. Harding, Septem. 1, 1803. Vesta. ..22....0. M.'Olbers, ... March .29;:1807; All these planets revolve round the Sun, as the centre of motion: and in performing their revolutions .they follow the fundamental laws of the planetary motion. so happily discovered by Kepler and which have been fully confirmed by subsequent observations. | These laws are, J. The orbit of each planet is an ellipse; of which the Sun occupies one of the foci. The extremity.of. the major axis of this ellipse, nearest the Sun, is called the perthelion: the opposite extremity of the same axis is called the aphelion. The line, which joins these two points, is called the line of the apsides. The ra- dius vector is an imaginary line drawn from the centre of the Sun to the centre of the planet, in any part of its orbit. The velocity of a planet in its orbit is always greatest at its perihelion. This velocity diminishes as the radius vector increases; till the planet arrives at its aphelion, when its notion is the slowest. It then increases, in an inverse manner, till the planet arrives again at its perihelion. II. The areas, described about the Sun by the radius vector of the planet, are proportional to the times employed in describing them. These laws are sufficient for determining the motion of the planets round the Sun: but it is necessary to know, for each of these planets, seven quantities; which are called the elements of their ellipticul motion. The first, five of these elements relate to the motion in_an ellipse :. the last two relate to the. position of the orbit 5 since the planets do not all move in the same plane. 1, The duration of a sidereal revolution of the planet. 2. Half the major axis of the orbit ; or the mean distance of the planet from the Sun 3. The eccentricity of the orbit; whence we deduce the greatest equation of the centre. * A3 4. The 6 A Synopsis of the principal 4, The mean longitude of the planet at a given epoch. 5. The longitude of the perihelion at a given epoch. 6. The longitude of the nodes at a given epoch, 7. The inclination of the orbit 10 the ecliptic. The following tables present all these elements for the first moment of the present century: namely, for that point of time at midnight which separates the 33st of December 1800, and the Ist of January 1801; mean time at Paris. {The observatory at Paris is in north Jatitude 48° 50’ 14”, and in longitude 9 21” east from Greenwich observatory.] 1. Duration of a Sidereal Revolution. days. days. Mereury.. 87°96925904 Ceres.... 1681°53Q00000 Wenus.... 224°70082399 Pallas... 1681°70QgO00000 Earth .... 365°25038350 Jupiter .. 4332°59030760 - Mars..... 686°97961860 Saturn .. 10758:96984000 Festa .... 1335°20500000 | Uranus ..30688°71268720 Juno..... 1590°99800000 2. Mean Distance from the Sun. Mercury.... °38709S81 Ceres....+. 2°7674060 Venus...... °7233323 Pallus .. .. °2'7675920 Farth ...... 10000000 Jupiter.... 5°2027911 Mars .....- 15236y35 Saturn .... 9°5387705 Vesta...... 2°3730000 | Uranus .... 19°1833050 Pip Tere eee 2607 1630 3. Ratio of the Eccentricity to half the Major Azis. Wenus...... °00685208 Pallas .. .. *24538400 Earth...... 01685318 Jupiter.. .. ‘04817840 Mars...... ‘0893!3400 Saturn.... °05616830 Vesta... «+++ ‘089322000 Uranus.. .. °*04667030 Juno.....«. °25494400 Mercury.... ‘20551494 | yi ER "07834860 4. Mean Longitude January 1, 1801. Mercury.... 182° 15647 Ceres...... 204° 16826 WEnUS. .. «o> 11° 93672 Pallas .. .. 280° 68580 Farth....-. 121928179 | Jupiter... .. 124°67781 Mats...... 71924145 | Saturn.. .. 150°38010 Festa..-... 207° 12990 Uranus .... 197° 54244 Juno...... 322° 79380 5. Mean Longitude of the Perihelion. Sercury osteo @@.,,82° 6256 Ceres. «0-200 162° 9565. We cate nes 142° 9077 Pallas .. ..+. 134° 7040 Avs Yeicie «6. >» 110° 5571 Jupiter...... ‘12°3813 FSR cc cesses 247 4030 Uranus.. ».2- 185° 9574 Mars ......«. 369° 3407 Saturn ...... 99° 0549 JUNO so. guvsce OO 2049 | 6. Inclie Elements of Astronomy. 7 6. Longitude of the ascending Node. Mercury ...... 51° 0651 Ceres ....2. 89° 9083 Mens ie, .' ssa *iog7? Pallas...... 191°7148 Earth ...:.... 0° 0000 Jupiter .. .. 109°3624 Maras. ...s. 053° S608 Saturn .. .. 124°3662 Vesta... .. 4.22. 114° 4630 Uranus .... 80°9488 Juno... '.. 0+». 190° 1228 7. Inclination of the Orbit to the Ecliptic. Mercury...... 7° 78058 | Ceres ...... 11° 80680 Venus........ 3° 76936 Pallas .. .. 38° 46540 Earth........ 0° 00000 | Jupiter.... 1° 46034 Moarainls 2. j.1. 7. . 2° 05663 Saturn... '.. 2° 77102 Vesta ........ 7° Q4010 | Uranus... .. 0° 85990 Juno ........ 14° 50860 , The examination of the first two tables here given will show us that the duration of the revolutions of the planets increases with their mean distance from the Sun. Whence Kepler discovered his third fundamental law: namely, III. The squares of the times of the revolutions of the - planets are to each other as the cubes of their mean distances. The ellipses, which the planets describe, however, are not unalterable. Their major axes appear to be always the ‘same: but their eccentricities, the positions of their peri- helion and nodes, together with the inclination of their orbits to the ecliptic, seem to vary in a course of years. These variations, being sensible only in’a series of ages, are called secular inequalities. There is no doubt of their ex- istence: but the modern observations not being sufficiently extensive, and the ancient not sufficiently exact, there still rests some degree of uncertainty as to their magnitude. The following table will show the inequalities that happen in a period of one hundred years, and are the values that appear to accord best with the present observations. SECULAR INEQUALITIES OF THE PLANETS. The sign — signifies a Diminution. \ In the In the In the In the Eccentricity. Perihelion. | Inclination, |Place of Nodes. Planets. a ee Mercury ‘000003 867 0° 180110) 0° GO5612|—0* 241441 fenus ..|—‘000062711 |—0* 082663] —0* 001405|—0* 577 Earth . ..|—'000041632| 0°364140) ........) wr ccenes Mars.... ‘000090176| 0° 488405|—0* 000447|— 0° 718665 000159350} 0° 204895}—0* 006978)— 0° 486904}. —'000312402| 0° 597860|—0* 004788/—0* 699525 — 000025072] 0°073809| 0° 000967|—1° 110481 upiter .. Saturn .. Uranus .. A4 There 8 A Synopsis of the principal There are also some inequalities which affect the elliptical motion of the planets.. That of the Earth is a little altered. But they are most sensible in Jupiter and Saturn: for it appears that the duration of their revolution round the Sun is subject to a periodical variation. Mercury. Mercury is the nearest planet to the Sun: its mean dis- tance being +387, that of the Earth being considered as unity. This makes his mean distance above 36 millions of miles. He performs his sidereal revolution in 874 235 15' 43",9 and his mean synodical revolution in about 116 days. The eccentricity of his orbit is +2055; half the major axis being taken equal to unity. His mean longitude, at the commencement of the pre- sent century, was in 5° 23° 56’ 27,0. The longitude of his perihelion was, at the same time, in 2 14° 21’ 46",9. The line of the apsides has a sidereal mo- tion, according to the order of the signs, equal to 9’ 43",6 in acentury. But, if referred to the ecliptic, this motion will (owing to the precession of the equinoctial points) be equal to 55',8 in a year; or to 1° 33’ 13",6 in a century. His orbit is inclined to the plane of the ecliptic in an angle of 7°0' 9",1: which angle Is subject to a small in- crease of about 18”,2 1m a century. His orbit, at the commencement of the present century, crossed the ecliptic in 1* 15° 57’ 30’,9: having a sidereal motion, to the westward every century, of 13'2",2. But, if referred to the ecliptic, the place of the modes will (on account of the precession of the equinoxes) fall more.to the eastward by 42”,3 in a year, or 1° 10’ 27”,8 ina century. The rotation on his axis is accomplished in 14 O° 5’ 28",3. But the inclination of its axis is not known. [The diameter of Mercury is about 3123 miles: which, compared with the Earth’s diameter considered as unity, is about °3944.] His mass, compared with that of the Sun considered as mnity, 18° ...1-7-,- (The proportion of dight and heat received from the Sun is about 6°68 timés greater than on our planet. ] As seen from the Earth, Mercury never appears at any great distance from the Sun; either in the morning or the evening. His elongation, or angular distance, varies from 16° 19’ to 28° 48’. His course sometimes appears retrograde. The mean arc, which it describes in this case, is about 13° 30’; and its Elements of Astronomy. 9 its mean duration is about 23 days: but there is great dif- ference in this respect. This retrogradation commences of finishes when he is about 18° distant from the Sun. Mercury changes his phases, like the Moon, according to his various positions with regard to the Earth and Sun: but this cannot be discovered without the aid of a telescope. His mean apparent diameter is 6”,9. {Mercury is sometimes seen to pass over the Sun’s disk: which can only happen when he is in his nodes, and when the Earth is in the same longitude. Consequently this phenomenon can take place only in the months of May or November. The first observation of this kind was made by Gassendi in November 1631: since which period they have heen frequent. The next appearance of this kind will be m November 1815.) Venus. Venus performs her sidereal revolution in 2244 16% 49% 11”,2: and her mean synodical revolution in about 584 days. Her mean distance from the Sun is -723; that of the Earth being considered as unity. This makes her mean di- stance nearly 68 millions of miles. The eccentricity of her orbit is ‘0069; half the major axis being considered as unity. She is the least eccentric of all the planets. Her mean longitude, at the commencement of the pre- sent century, was in O° 10° 44’ 35”,0. The longitude of her perihelion.was, at the same time, in 4° 8° 37'0",9. The line of her apsides has a sidereal mation, contrary to the order of the signs, of 4! 27,”8 ina century. But, if referred to the ecliptic, this motion will appear (on account of the precession of the equinoxes) to proceed according to the order of the signs at the rate of 47",4 in a year, or 1° 19! 2”,2 in a century, Her orbit is inclined to. the plane of the ecliptic in an angle of 3° 23’ 32",7: which angle decreases about 4’36 in a century. Her orbit, at the commencement of the present century, crossed the ecliptic in 2* 14° 52’ 38’,9. But the nodes have an apparent motion in longitnde of 31”,4 ina year, or 52 20",2 in a century. The rotation on her axis is performed in 235 21/ 7”,2: but the inclination of her axis is not known. ' [The diameter of Venus is 7702 miles: consequently she is nearly as large as the Earth.] Her 10 A Synopsis of the principal Her mass, compared with that of the Sun considered a$ unity, IS 45 . [The tp of light and heat, received by her from the Sun, is 1°91 times greater than on our planet. ] It. is surrounded by an atmosphere, the refractive powers of which differ very little from those of our atmosphere. As viewed from the Earth, Venus is the most brilliant of all:the planets; and may sometimes be seen with the naked eye, at noon day. She is known as the morning and even- ing star; and never recedes far from the Sun. Her elon- gation, or angular distance, varies from 45° to 48°, Her motion sometimes appears retrograde. The mean are, which she describes in such case, is about 16° 12’; and her mean duration is about 42 days. ‘This retrogradation com- mences, or finishes, when she is about 28° 49’ distant from the Sun. Venus changes her phases, like the Moon, according to her position with respect to the Sun and the Earth: which causes a very considerable difference in her brijlancy. Her mean apparent diameter is 17,0; her greatest ap- parent diameter 13 about 57”,3. [Venus is sometimes seen to pass over the Sun’s disk: which can happen only when she is in her nodes, and when the Earth is in the same longitude. Consequently it can take place only in the months of June or Decem- ber. Three of these transits have been already observed ; one in 1639, one in June 1761, arid one in June 1769. There will not be another till the 8th of December 1874.) The Earth. The Earth which we inhabit is also one of the planets that revolve about the Sun. It performs its sédereal revolu- tion in 365% 6% g’ 11”,5: but the time employed in going from one tropic to the other is only 3654 5> 48’ 52”,6, The tropical year is abovt 11”,2 shorter than it was at the time of Hipparchus. Its mean distance from the Sun is 23578 times its own semi-diameter: whence it is above 93 millions of miles di- stant from that luminary. If this mean distance be taken equal to unity, we shall have its distance at the perihelion equal to *98323; and its distance at the aphelion equal to 1°0168." , The-eccentrictty of its orbit is ‘0168: half the major axis being considered as unity. The major axis, therefore, will be to the minor axis of the orbit, in the proportion of } to "99439. Its Elements of Astronomy. n Its. mean longitude, at the commencement of the present century, was 3° 10° g’ 13”,0. Its velocity varies in different parts of its orbit. Like all the other planets, it is most rapid in its perihelion, and slowest in its aphelion. In the former point it describes an arc of 1° 1’ 9",9 in the course of a day; and in the latter point it describes an are of only 57’ 11”,5 in the same period. The mean velocity is 59’ .0’,7 each day. The mean longitude of its perihelion at the commences ment of the present century was 3° 9° 30’ 5”,0. But the line of the apsides has a direct sidereal motion of 19’ 40,8 in a century: which, being referred to the ecliptic, will give it a motion (according to the order of the signs) of 1’ 1',9 in a year, or 1° 43’ 10’,8 in acentury. A complete revolution round the line of the apsides is called the ano- malistic year; and is performed in 365° 65 14' 9”. The perihelion coincided with the vernal equinox about the year 4089 before-the Christian era. It coincided with the sum- mer solstice about the year 1250 after Christ: and will coincide with the autumnal equinox about the year 6483. A complete tropical revolution of the apsides is performed in 20931 years. The axis of the Earth is inclined to the plane of the ecliptic in an angle of 23° 27’ 57”,0: which angle is observed to decrease at the rate of 52”,1 in acentury. But this variation of the angle is confined within certain limits ; and cannot exceed 2° 42’, The annual intersection of the equator with the ecliptic is not always in the same point: but is retrograde, or con- trary to the order of the signs. Consequently the equinoxial points appear to move forward on the ecliptic: and whence this phenomenon is called the precession of the equinoxes. The quantity of this annual change is 50,1 ; or 1° 23’ 30” in a century. A complete revolution is performed in 25863 years, The sidereal day, or the time employed by the Earth in revolving on its axis, is always the same. Its diurnal rota- tion bas not varied, the hundredth part of a second, since the time of Hipparchus. If the mean astronomical, or eivil, day be taken equal to 24 hours, the duration of the sidereal day will be 23" 56’ 4”,1. The astronomical, or civil, day is constantly changing. This variation arises from two causes; 1. The unequal mo- tion of the Earth in its orbit; 2. The obliquity of that orbit to the plane of the equator. {The mean and apparent solar days are never equal, except when the Sun’s daily mo- tion iz A Synopsis of the principal tion in right ascension is 59’ 8”. » This is the case about April 16th, June 16th, September Ist, and December 25ths on these days the difference vanishes, or nearly so; It is at its greatest about November Ist, when it is 16’ 16] The astronomical year is divided into four parts, deter- “mined by the two equinoxes and the two solstices.... The interval between the vernal and autumnal equinoxes is (on account of the eccentricity of the Earth’s orbit, and its un equal velocity therein) near eight days longer than the in+ terval between the autumual and:vernal equinoxes. These intervals are, at present, nearly as follow : From the spring equinox to the el Hityr- . a «922145 diiee ie summer solstice.......... From the summer solstice to At 10% . ° 93 13 35 the autumnal equinox....« F; autumnal equinox to ues pais \ ..89 16 47 the winter solstice........ om the winter solstice to the tia) ate) ..89 149 Spring EQUINOX ..eseeeee mM. = 185,35 20 =178 1829 4h 6, Sl The nutation of the Earth’s axis is 19”,3. Light takes 6’ 13,3 to come from the Sun to the Earth. But in this interval the Earth has moved 20”,2 in its orbit. This motion of the Earth produces an optical illusion in the light which comes from the stars: and which Bradley calls the aberration of light. The figure of the Earth is that of an oblate spheroid: the axis of the poles being to the diameter of the equator as 331 to 332. The mean diameter of the Earth is about 7916 miles: its equatorial diameter is 7924 miles. As a necessary consequence from this circumstance, the degrees of latitude increase in length as we recede from the equator to the poles. But different meridians, under the same latitude, present different results. The general fact, however, is well ascertained. The density of the Earth is 3°9326 times greater than that of the Sun, and is to that of water as 11 to 2. Its mass, compared with that of the Sun considered as UNity, 13 sxgeee The centrifugal force is greater at the equator than at the poles: in consequence of which, bodies lose part of their weight by being taken towards the equator. If the gravity of a body at the equator be represented by unity, its gravity at the poles will be increased by -00569. A pendulum, therefore, which vibrates seconds in the higher latitudes, ~ Blements of Astronomy, 13 latitudes, must be shortened at the equator in order to rens der the oscillations isochronous. [A pendulum 39°197 inches long will swing seconds at the poles: but, in order that it may swing seconds at the equator, it must be re- duced to 39°097 inches. ]} The centrifugal force at the equator is nearly ~}th of gravity. Ifthe rotation of the Earth were 17 times more rapid, the centrifugal force would be equal to that of gra- vity: and bodies at the equator would not have any weight. A rare and elastic fluid surrounds the Earth, which is called the aimosphere. Neither the temperature nor density of this fluid is uniform; but diminishes in proportion to its djstance from the surface of the Earth, and 1s also. af- fected by other circumstances. If the density of the atmosphere were every where the same and its temperature at zero, and the height of the ba- rometer at 29°92196 inches, the height of the atmosphere would be 26067 feet; or 3°7 miles. The atmosphere is a heterogeneons substance. Out of 100 parts, 79 are azotic gas, and the remaining 21 are oxy- gen gas. This is found to be universally the case, in what- ever season or whatever climate the experiment be tried. This proportion is also found to exist in the highest points of the atmosphere that have been reached by means of balloons, A body projected horizontally to the distance of about 4°35 miles, if theré were no resistance in the atmosphere, would not fall again to the surface of the Earth, but would revolve round it as a satellite; the centrifugal force being then equal to its gravity. The rays of light do not move in a straight line through the atmosphere ; but are inflected continually towards the Earth: so that the stars appear more elevated on the hori- zon than they really are. We find, trom the most.accurate observations, that the refraction, which the atmosphere produces, is independent of its temperature, and proportional to its density. But, as the density varies according to the temperature; it is necessary to attend not only to thé state of the barometer, but also of the thermometer, The humidity of the air produces very little effect on its rcfractive powers, and may therefore be safely omitted. The temperature of the whole atmosphere being sup- posed at zero, its density will diminish in a geometrical progression, according to its distance from the surface of the Earth: and we find by experience that, the height of the 14 A Synopsis of the principal the barometer being 29°92 inches, the refraction at the ho-~ rizon is 39/ 54’,7. [t would be only 30’ 24”,1 if its den- sity diminished in arithmetical progression; and would be nothing at the surface. The horizontal refraction, which we observe about 35’ 6”,0, is a mean_ between these limits. When the apparent height of a star upon the horizon does not exceed eleven degrees, its sensible refraction de- ends only on the state of the barometer and thermometer in the place of observation ; and it is nearly proportional to the tangent of the apparent distance of the star from the zenith, diminished by 3: times the corresponding refraction at this distance, the thermometer being considered as at the freezing point and the barometer at 29°92 inches. It is from these principles that have been formed the Tables of Refraction, corresponding to the several variations in the scale of the thermometer and barometer. The action of the Sun and Moon has a considerable ef- fect on the water of the ocean, and produces the phzno- mena of the fides. The sea rises and falls twice in each interval of time comprised between the consecutive returns of the Moon to the same meridian. The mean imterval of these returns is 1% gb 50’ 28”,3 : consequently the mean interval between two following periods of high water is 12% 25’ 14,3. So that the retardation in the time of high water, from one day to another, is 50’ 28” in its mean state: and it is af- fected by all those causes which influence the Moon’s mo- tion. This retardation varies with the phases of the Moon. It is at its minimum towards the syzigies when the tides are at their maximum, and it is then only 38’ 57”,1. But, when the tides are at their minimum, or towards the qua- dratures, it is then the greatest possible; and amounts to y> 14’ 58”,8. The variation in the distances of the Sun and Moon from the Earth (and particularly the Moon) has an influence also on this retardation. Each minute in the increase or diminution of the apparent diameter of the Moon augments or diminishes this retardation 3’ 42,9 towards the syzigies ; but towards the quadratures the effect is three times less. The daily retardation of the tides varies likewise with the declination of the Sun and Moon. In the syzigies, at the time of the solstices, it is about 2’ 13”,9 greater than in its mean state: and it is diminished in the same propor- tion, at the time of the equinoxes. On the contrary, in the Elements of Astronomy. 15 the guadratures, at the time of the equinoxes, it exceeds its mean state by 7’ 49,2; and is in a similar manner dimi- nished by this quantity, at the time of the solstices, The height of the tides is also considerably influenced by all those causes which have been just mentioned ; and depends on the phases and position of the Moon in her or- bit. It is greatest when the Moon is in the syzigies ; and is diminished in the quadratures. The distance likewise of the Sun and Moon from the Earth, as well as their declina- tion, has a material effect upon the height of the tides. But the state of the tides is so modified by the nature and position of the coasts, the depth of the channel, the operation of the winds, and by other causes, that the above Jaws will not always be found to correspond with the actual state of the tides, particularly near the coast, or in rivers. It will however be found, from the mean of a number of observations, that the inequalities in the heights and in the intervals of the tides have various periods. Some are of half a day and a day; others are of half a month and a month; whilst others again are of half a year and a year: and some are the same as the times of the revolutions of the Junar nodes and apsides. The action of the Moon upon the waters of the ocean is triple that of the Sun. Mars. Mars is easily known in the heavens by his red and fiery appearance. He performs his sidereal revolution in 6864 23" 30’ 39”,0 or in 1°881 Julian years: and his mean syno- dical revolution in about 780 days, or in about 2°135 years. His mean distance from the Sun is 1°524; that of the Earth being considered as unity, This makes his mean distance above 142 millions of miles. The eccentricity of his orbit is 093: half the major axis being considered as unity. His mean longitude, at the commencement of the pre- sent century, was in 2° 4° 7' 2,3. The longitude of his perihelion was, at the same time, in 115 2° 94’ 93”,9: but the line of the apsides has an appa- rent motion, according to the order of the signs, of 1’ 5,9 in a year, or 1° 49' 52”,4 in a century. His orbit is zuclined to the plane of the ecliptic in an angle of 1° 51’ 3",5; which angle decreases about 1,4 in a century. , His orbit at the commencement of the present century crossed the ecliptic in 1° 18° 1! 28",05 but the place of the nodes 16 A Synopsis of the principal nodes has an apparent motion in longitude, according to the order of the signs, of 26”,8 ina year, or 44’ 41",5 ina century. The rotation on his axis is performed in 14 08 39! 21”,3: and his avis is inclined to the ecliptic in an angle of 59° 41’ 49",2. [His mean diameter is equal to 4398 miles: consequently he is rather more than half the size of our Earth.] His mass, compared with that of the Sun considered as unity, 18S sss4+as {The proportion of light and heat, received by him from the.Sun, is ‘43: that received by the Earth being considered as unity.] He has a very dense but moderate atmosphere: and he is not accompanicd by any satellite. As viewed from the Earth, the motion of Mars appears sometimes re¢érograde. The mean are which he describes - in this case is 16° 192’: and its mean duration is about 73 days. This retrogradation commences, or finishes, when the planet is not more than 136° 48’ from the Sun. Mars changes his phases somewhat in the same manner as the Moon does from her first to her third quarter, ac- cording to his various positions with respect to the Earth and the Sun: but, he never becomes cornicular, as the Moon does when near her conjunctions. ' His mean appa rent diameter is 9”,7: which augments in proportion as the planet approaches its opposition, when it’ is equal ta 29",2. His parallax is nearly double that of the Sun. A Jupiter. Jupiter is, next to Venus, the most brilliant of all the . planets: whom he sometimes however surpasses in bright~ ness. He performs his sidereal revolution in 43324 14% 18’ 41",03 or in 11°862 Julian years. But this period is subject to some inequalities. He performs his mean syno- dical revolution in about 399 days. His mean distance from the Sun is 5*203; that of the Earth being considered as unity. This makes his mean di- stance above 485 millions of miles. The eccentricity of his orbit is 04823 half the major axis being considered as unity. His mean longitude at the commencement of the present century was in 3° 22° 0’ 36”,1. 290 The longitude of his perihelion was, at the same time, in OF 11° 8’ 35"j1: but the line of the apsides has an ap- , parent Elements of Astronomy. 17 parent motion, according to the order of the signs, of 56",7 in a year, or 1° 34’ 33,8 in acentury. spent’ His orbit is inclined to the plane of the ecliptic in an angle of 1° 18’ 51”,5: which is observed to decrease nearly 22”,6 in a century. © His orbit, at the commencement of the present century, crossed the ecliptic in 3° 8° 25’ 34”,2. But the place of the nodes has an-apparent motion in longitude, according _ to the order of the signs, of 34”,3 in a year, or 57 12",4 in a century. The rotation on his axis is performed in 9" 55! 49",7: and his axis forms an angle of 86° 54’ 30’,0 with the plane of the ecliptic. [His mean diameter is equal to 91522 miles: consequently he is about 112 times as large as our Earth.] The axis of his poles is to his equatorial diameter as *9287 to 1, or as 13 to 14, His mass, compared with that of the Sun considered as unity, is 5;!;-g5: but his density is -909501. [The proportion of light and heat, received from the Sun, is ‘037: that received by the Earth being considered as unity. ] : He is surrounded by faint substances called zones or belts; which are supposed to be parts of his atmosphere. And he is accompanied by four satellites. A body, which weighs one pound at the equatorial sur- face of the Earth, would, if removed to the surface of Jupi- ter, weigh 2-281 pounds, As seen from the Earth, the motion of Jupiter appears sometimes to be retrograde. The mean are which he de- scribes in this case is about 9° 54’: and its mean duration is about 121 days. This retrogradation commences, or finishes, when the planet is not more distant than 115° 19’ from the Sun. His mean apparent equatorial diameter is 38"2: it is greatest when in opposition, at which time it is equal to 47,6. Saturn. Saturn performs his sidereal revolution in 107584 935 16’ 34”,25 or in 29°456 Julian years. But this period is subject to some inequalities. His mean‘synodical revolu- tion is performed in about 378 days. fis mean distance from the Sun is 9°539; that of the Earth being considered as unity. This makes his mean distance aboye 890 millions of miles, Vol. 39. No, 165. Jan, 1812, B The 18 A Synopsis of the principal The eccentricity of his orbit is 05625 half the major axis being taken as unity. His mean longitude at the commencement of the present oentury, was in 4* 15° 20’ 31,5. The longitude of his periielion was, at the same time, in 95 29° 8' 57”,9: but the line of the apsides has an apparent motion in longitude, according to the order of the signs, of 1’ 9’,5 in a year, or 1° 55'47”,1 in a century. His orbit is inclined to the plane of the ecliptic in an angle of 2° 29’ 38”,1: which is observed to decrease about 15”,5 in a century. His orbit, at the commencement of the present century, crossed the ecliptic in 3° 21° 55’ 46’,5: but the place of the odes has an apparent motion in longitude, according to the order of the signs, of 27,4 in a year, or 45° 43”,5 in a century. The rotation on his axis is performed in 10° 16’ 19”,2: {ard the axis is inclined in an angle of 58° 41’ to the plane of the ecliptic. } {His mean diameter is 76068 miles: consequently he ts nearly 10 times as large as our Earth.] ‘The axis of his poles is to his equatorial diameter as 11 to 12. His mass, compared with that of the Sun considered as unity, 18 ssg¢-s¢: [but his density is 08.) {The proportion of ight and heat received from the Sun is “00113 that received by the Earth being considered as unity.] Saturn is sometimes marked by zones or belts ; which are probably obscurations in his atmosphere. And he is accompanied by seven satellites. The most singular phenomenon, however, attending this planet, is the double img with which he is surrounded. This ring, which is very thin and broad, is inclined to the plane of the ecliptic in an angle of 31° 19’ 12",0; and revolves from west to east, in a period of 105 29'16",8, about an axis perpendicular to its plane and passing through the centre of the planet. The breadth of the ring is nearly equal to its distance from the surface of Saturn: that is, about + of the diameter of the planet. The surface of the ring 18 separated in the middle by a black concentric band, which divides it into éwo distinct rings. The edges of this ring, being very thin, sometimes disap- pear: and, as this edge will present itself to the Sun twice in each revolution of the planet, it is obvious that the dis- appearance Elements of Astronomy. 19 eppearance of the ring will occur about once in 15 years ; bot under circumstances oftentimes very different. [The zntersection of the ring and the ecliptic is in 5° 20° and 11° 20°: consequently, when Saturn is in either of those signs, his ring will be invisible to us. On the con- trary, when he is in 2° 20° or 8° 20°, we may see it to most advantage. ‘This was the case towards the end of, the year 1811. Regard, however, must be had to the position of the Earth.] As viewed from the Earth, the motion of Saturn some- times appears retrograde. The mean arc which he describes in this case is about 6° 18’: and its duration is nearly 139 days. This retrogradation commences, or finishes, when ihe planet is distant about 108° 54’ from the Sun. His mean apparent diameter is 17",6. , Telescopic Planets. Uranus was discovered by Dr. Herschel, March 13, 1781, who gave it the name of the Georgium.Sidus. It performs its sidereal revolution in 30688¢ 17" 6’ 16”,2; or in about 84 Julian years: and it is probably situated at the confines of the planetary system. Its distance trom the Sun is upwards of 1800 millions of miles: and its apparent diameter is scarcely 3”,9. Its mass compared with that of the Sun considered as unity, Is ~>toy- Six satellites accompany this planet; which move in orbits nearly perpendicular to the plane of the ecliptic. The elements of the four remaining telescopic planets are not yet ascertained with sufficient precision. Satellites. The number of satellites in our system, at present known, is eighteen: namely, the Moon which revolves round the Earth; four that belong to Jupiter, seven to Saturn, and six to Uranus. The Moon is the only one visible to the naked eye. They all move round their primary planets, as their cen- tre, by the same law sas those primary ones move round the Sun: namely, I. The orbit of each satellite is an ellipse, of which the primary planet occupies one of the foci. Il. The areas, described about the primary planet, by the radius vector of the satellite, are proportional to the times employed in describing them. Be III, The 20 A Synopsis of the principal IT!. The squares of the times of the revolutions of the sa- iellites, round their respective primary planets, are to each other as ihe cubes of their mean distances from the, primary. Afoon. The motions of the Moon are exceedingly eccentric and irregular, She performs her mean sidereal revolution in 27275 43' 11",5.. But this period is variable: and a com- parison of the modern observations with the ancient proves incontestably an acceleration in her mean motion. Her mean tropical revolution is 2747" 43’ 4",7: and her mean synodical revolution is 29° 125 44’ 2'.8, Her mean distance from the Earth is 29°982175 times the diameter of the terrestrial equator ; or above 237 thou- sand miles. The eccentricity of her orbit is 0548553; the mean dis- tance from the Earth being taken equal to unity. But this eccentricity is variable iu each revolution. Her mean longitude, at the commencement of the pre- sent century, was in 35 21° 36’ 42”,1. Her velocity varies in different parts of her orbit. She is swiftest in her perigee (or point nearest the Earth) ; and slowest when in her apogee (or point furthest from the Earth). Her meandiurnal velocity is equal to 13° 10'34”,9, or about 13 times greater than that of the Sun. The greatest equation of her centre is 6° 17’ 54",5. The mean longitude of her perthelion was, at the com- mencement of the present century, in 8° 26° 6’ 5”,1: but the line of the apsides bas a motion, according to the order of the signs. The period of a sidereal revolution of the apsides is 32324 13> 56’ 16”,8, or nearly 9 years. The pe- riod of a tropical revolution of the apsides is but 32314 115 24' §”,6. But these periods are not uniform: for they have a secular irregularity, and are retarded whilst the motion of the Moon itself is accelerated. The period of an anzomalistic revolution of the Moon is 274 138 18’ 37",4. Her orbit is inclined to the plane of the ecliptic in an angle of 5° g’: but this inclination is variable. The greatest inequality, which sometimes extends to 8’ 47”,1, is pro- portional to the co-sine of the angle on which the inequality ip the motion of the nodes depends. . Her orbit, at the commencement of the present century, crossed the ecliptic in O° 15° 55’ 26’,3: but the place of her modes is variable. They havea retrograde motion, and make Elements of Astronomy. 21 make a sidereal revolution in 67934 10> 6’ 30”,0; or in about 18°6 Julian years. This variation, however, is subject to many inequalitues: of which, the greatest is proportional to the sine of double the distance of the Moon from the Sun; and extends to 1° 37’ 45",0 at its maximum. ,, 3069 Al 58" y= BM. | 832 490 1 oy"? 95 206° 4i/ € meee = pt 29 58! 43" — i= yt By woke for the epoch, thes instant of the mean obser- vation, 7. 2. the 19th of November, at 8* 29’ 44”, we have t= — 5, = 29,1! = 0, 1 a By 6; which gives 3B = —5'44",33 | dy = — 5° 39/ 59”,0 dp’ = — 3’ 3", 0 iy’ = — 2 31’ 12,0 eT A Ae Ee dy” = — |° 48! 35”,667 op’= — 1! 5,53 oy" = — 1° 16’ 46,0 A = 15/ 457,4 623’ = 10",4 8%’ = . 8! 31,267 88" = 107,945 | Oy'= 5’ 18",278 BB = — 2,733 | Oy = — 397,260 3’ = 0”,0681 | ‘ OB =a 0 254G 1) gti 1”,3766 The formula (p) will therefore give for the geocentric longitude of the comet, according to the small number x of days reckoned from the epoch, 306° 51’ 26” — 153”,46.% + 107,54.27, and the formula (7) will give for the expression ofits latitude, 39° 14° 487 — 7855”,16.z + 53544 .2%, from which we extract a =. 300 4196", % = — 0,0432501, b = 0,345366, ; § = 39° 14’ 48”, d h = — 2,913844, 1 = 17,54354. ad. We at General Method for determining ad: We shall determine by the astronomical tables the longitude of the earth seen from the sun at the instant which we have chosen for our epoch: let A be the longi- tude, R the corresponding distance from the earth to the sun, and & the distance which answers to the longi- tude 90° + A, of the earth: we shall form the four equa- tions , 7 = —— + 2Rr.cos (4—a) + R*,..(1) cos*0 R.sin(4—a) fl 1 bx y= 2 gosh ee ® a ree F 7 a?.sin §.cos 6 = eo —— nd y= x.{ .tang @ + Dh + Dh t R.sin 6 cos 6 i 1 «» (3) + eS aca «COs (4d —z). {r= a his \ iy o=y +a. + { yotang 6 a cane i + 2y. { (R’=1)-005 (4—a) — sates 1 4+(4) eee | + 2ax. { (R’—1).sin(4—a) + R 1 2 Tesh SE ea ee J Tn order to draw from these equations the values of the three unknown quantities x, y, and r, we shall begin by considering if, abstraction being made of the sign, 0 is greater or Jess than 7; in the former case we shall make use of the equations (1), (2) and (4); we-shall form a first hypothesis for 2, by supposing it, for instance, equal to unity; and we shall extract from it by means of the equations (1) and (2), the values of r and y; we shall af- terwards substitute these values in the equation (4), and if the remains are null, it will be a proof that the value of x has been well chosen; but if the remains are negative, we shall increase the value of x, and diminish it if the remains are positive. We shall also have by means of a small num- ber of trials, the true values of x, y, and r; but as these unknown quantities may be susceptible of several values, we must choose that which satisfies precisely or nearly ta the equation (3). : In the second case, 7. e. if we have 1 7 b, we shall make use of the equations (1), (3) and (4), and then it will be the equation (2) which will serve as the verification. Having the Orbits of Comets. 43 Having thus the values of x, y, and r, we shall form the quantity = a {y + hx.tang ot+ Ry.cos (A—a) +2 { (R’—1).cos (d—a)<= A + Rax.sin(A~a) + R.(R’—1). The perihelion distance D of the comet will be Ce ae ah a4 the cosine of the anomaly v of the comet will be given by the equation D ; cos? Fu = 2 from which we shall conclude, by the table of the move- ment of the comets, the time consumed in traversing the angle v*. In order to have the instant of the passage by the perihelion, we must add this time to the epoch, if P is negative, and subtract it if P is positive, because in the for- mer case the comet approaches the perihelion, and in the second case it remoyes from it. With respect to the second comet of 1781, the epoch being fixed as above, on the 19th November, at g 29/ 44”, we have at this epoch SA San 7287 ahh R = 0,987248, R’ = 0,988820, the equations (1), (2), (3) and (4) become thus r? = 1,667387.x7 — 0,7106137.x” + 0,974653 ...(1) 48 y = — 11,0665 + — + 3,9927.x...(2) 0,03931687 y = 5,771014.2 + ———,— — 0,04086053... .(3) 0 = y* + 0,00187057. x. +[0,8169372.y—3,691334'"]*—1,8320446.y...(4). + 0,0324357." + 1,026006 — —. * Call, as above, D the perihelion distance of the comet, U its anomaly, t.e.the angle formed by its vector radius with the axis of the parabola which it describes, lastly t, the time passed since the perihelion passage. This bemg done, according to the laws of parabolic motion, the time ¢ and the anomaly U are united together by the following ties: ner (1) et = 2 { 08 + } tang3 § ut 5 in which = is the demi-circumference, or 3,14159265, and T’ the duration of the sidereal revolution of the earth, or 365 days 256383. U being given, it is easy to calculate ¢ by this formula. But if ¢ is given, the search for the tang 7 U requires the resolution of these equations of the 3d degree. In or- der to avoid this difficulty, astronomers have formed a table of valuesof ¢ in a a in which D will be equal to unity, and from this table when once calculated, we may extract the values of U; ¢being known. This is what we call a table of the motion of comets. We may supply the place of this table by resolving the equation (1) by some trials, As 46 General Method for determining As we have in this particular case 77 J, we must employ the equations (i), (3), and (4). These three equations give x = 0,39107, y = 2,258355, r = 0,9755798. These values satisfy the equation (2) as much as we can expect of an equation which cannot be very exact on ac- count of the littke movement of the comet in longitude. By substituting them in the expression of P, we find P = — 0,185628. The negative sign of P makes known that the comet has not yet attained its perihelion. We aftewards find the perihelion distance D = 059583509, and the anomaly » of the comet, equal to 15° 16’ 24”, which answers to 10 days 40334: from which it follows that the perihelion passage took place on the 29th of November at 18" 10’ 34”, mean time at Paris. Having thus obtained nearly the pe- rihelion distance and the instant of the passage of the comet by this point, we may correct them by the following me- thod, which has the advantage of being independent of an intimate knowledge of the other elements of the orbit. Exact Determination of the Elements of the Orbit, when we know pretty nearly the Perihelion Distance and the Instant of the Passage of the Comet by this Point. 3. We shall select three observations removed from the comet: by afterwardssetting out from the perihelion distance, and from the instant of the passage by this point, deter- mined by what precedes, we shall easily calculate the three anomalies of the comet, and the three vector radii corre- sponding to the instants of the three observations ; let v, v” and v” be these anomalies, those which precede the passage of the comet by the perihelion being necessarily supposed to be negative: further let 7, 7’, 7” be the correspondin vector radii of the comet, v —v and v” —v will be the angles comprehended between 7 and 7’ and between 7 and 1’; let U be the first of these angles and U’ the second. Let us also call a, a’, a’, the three geocentric longitudes observed of the comet; 4, 4’, 6”,its three geocentric latitudes, the southern latitudes being supposed to be negative: C, C’, C’, the three corresponding longitudes of the sun ; R, R’, R’, its three distances from the earth; 6, 6’, 6", the three heliocentric longitudes of the comet; 7, a’, a”, its three heliocentric latitudes. This being done, We will imagine the letter S at the centre of the sun, the letter T at the centre of the earth, the letter C at the more ‘ 0 © the Orbits of Comets. 47 of the comet, and the letter C’ at its projection in the plane of the ecliptic; we shall have the angle STC’, on taking the difference of the geocentric longitudes of the sun and the comet; by afterwards adding the logarithm of the co- sine of this angle with that of the cosine of the geocen- tric latitude § of the comet, we shall have the logarithm of the cosine of the, angle STC; we shall therefore know in the triangle STC, the side ST or R, the side SC or r, and the angle STC; we shall thus have by rectilinear trigono- metry the angle CST; we shall afterwards have the helio- centric latitude @ of the comet by means of the equation sin @ sin CST sin CTS The angle TSC’ is the side of a spherical rectangular triangle, the hypothenuse of which is the angle 7'SC, and one of the sides of which is the angle a; from thence we shall easily extract the angle T'SC’, and consequently the heliocentric longitude 6 of the comet. We shall have in the same manner a’, 6’, a” and 6”, and the values of 6, 6’, 6” will show whether the motion of the comet be direct or retrograde. If we conceive the two arcs of latitude a and a’ united at the pole of the ecliptic, they will there form an angle equal to 6’—8; and in the spherical triangle formed by this angle, and by the sides 90°—a@ and 90°—a’, the side opposite to the angle 6’—f will be the angle at the sun comprehended between the two vector radii r and 7’. We shall easily determine it by the known analogies of spheri- eal trigonometry, or by the following formula: cos V = cos (6’—f).cos w.cos a + sin a@.sin a’, in which V represents this angle. By calling Y’ in a similar manner the angle formed by the two vector radii r and r”, we shall have cos V' = cos (6"—f).cos w. cos w”—sin @.sin a”, Now if the perihelion distance and the instant of the passage of the comet by this point were exactly determined, we shall have sine = ERY YN 1 aie Oia but as that will almost never happen, we shall suppose m=U—V;n=U'— VP’, We shal] here observe that the calculation of the tri- angle STC, gives for the angle CST, two different values, viz. CST and 180°; 2dly, STC—CST. We shali thus have two different values for each of the quantities 6, a, B', az’, 8", a’. Most frequently the nature of the motion, of 48 General Method for determining of the comet will make known the value of CST, of which we ought to make use, particularly if these two angles are very different; for then one of them will place the comet further than the other from the earth, and it will be easy to ascertain by the apparent motion of the comet, at the instant of the observation, which of the two ought to be preferred. In a great number of cases, one of them will be negative, and must consequently be rejected; but if any uncertainty remains on this head, we might always determine the true values of 6, 6’, 6”, by observing to take for B and 6’, the two angles which render V very little dif- ferent from U, and to take for 6 and 6” the two angles which render /’ very little different from U’. We shall afterwards form a second hypothesis, in which, by preserving the same |instant of perihelion passage with the above, we shail vary the perihelion distance ky a small quantity, for example, by the fiftieth part of its value, and we shall find out in this hypothesis the values of U—V, and of U’—V'; thus, m= U—V,n—U'— v'; finally, we shall form’a third hypothesis, in which, by pre- serving the same perihelion distance as in the first, we shall vary by half a day, or a whole day (more or less) the instant of the perihelion passage. We shall find out in this new hypothesis, the values of U—V and of U’—/’; thus, m= U— Vi, n'= U'— Vv’; this being done, if we call « the number by which we ought to multiply the supposed variation in the perihelion distance in order to have the true one, and ¢ the number by which we ought to multiply the supposed variation in the instant of the perihelion passage in order to have the true instant, we shall have the two equations, u(m—m') + t (m—m") =m, u(n—n') +#t(n—n") =n, from which we shall extract wu and 7; and consequently the perihelion distance corrected and the true instant of the passage of the comet by this point. The foregoing correction supposes that these elements determined by the first approximation, are sufficiently exact to treat as infinitely small their differences from the true: but if the second approximation did not still appear suffi- cient, we might have recourse to a third by operating on the elements already corrected, as has been done upon the first: we must only take care to make them undergo smaller variations. But in most eases this third approxi- mation A Case of Morbus Pedicularis. 49 mation will be useless, particularly if, in the first, we use four or five well selected observations. We may also, in the correction of the first elements, make use of the second differences in the following manner. Instead of calculating the values ef U, U’, Vand V’ in the three hypotheses, we shall calculate them in five hypo- theses, viz. 1. With the elements found by the first ap- proximation. 2. By varying the perihelion distance by a very small quantity. 3. By varying it by dcuble this small quantity. 4. By preserving the same perihelion distance as in the first hypothesis, and varying by a small interval the instant of the perihelion passage. 5. By vary- ing the same instant double this interval. Let m, m’, m’, mm", m'” be the values of U—V 3; 1, n', n", n'”, n'” the values of U'—V’: then in order to determine the values of w and z, we shall form the two equations, (42' —3m —m").u-+ (m" —9m' +m) .u? + (4m! —3m—m'").t + (m!"" —2m'" +m) .t7+ 2m=0, (4n'—3n—n").u + (n"”— 2n' + 1).u* + (4n!”"—3n—n"").£ + (n'” —2n'"+n).2+2n=0. The values of uw and of ¢ which satisfy these equations will be more precise than the foregoing. Although in most cases this overmuch precision is useless, it is nevertheless indispensable in forming these equations, at all times when the terms depending on the second differences may be of the same order with those which depend on the first dif- ferences ; which will happen, for instance, when in one of the observations the vector radius of the comet will be al- most perpendicular to the visual ray from the earth to the comet. [To be continued. ] VII. A Case of Morbus Pedicularis. Communicated by Joun ANDREE, Esq. Surgeon. A. R. esq. 35 years of age, of a very healthy and strong constitution, had for some years past, particularly when heated by good living and in warm rooms, been often trou- bled with a prickly itching on the surface of the body, armpits and thighs. In the summer of last year, on coming out of a warm bath at Brighton, he discovered an insect on his thigh. This circumstance induced him to suspect that the itch- ing he had so long been troubled with, might have been caused by insects. From that time until he applied to me Vol. 39. No, 165. Jan. 1812. D on 50 A Case of Morlus Pedicularis. on December 7, 1811, he had daily combed. out from the armpits, body and thighs, from twelve to between twenty and thirty living insects; and some he picked out of the ‘skin, as they had firmly attached themselves thereto ; seeming to have partly burrowed into the skin. -He was induced to use a small-toothed comb, from being remark- ‘ably hairy on the body, thighs, and armpits. J prescribed flores sulpburis intérnally, for him to take as much as his bowels would bear without operating more than once or twice daily ; and to use externally a lotion composed of a strong solution of hydrargyrus muriatus. On the 10th, “when I visited him, | had the satisfaction to find the re- medies had produced a good effect, the itching having abated, and the number of insects daily combed out dimi- nished to about balf the former number. __ By persevering in the use of these remedies to the end of the month, he was free from the disorder. On a minute examination of the insect, it appeared to be nearest in resemblance to the pediculus inguinalis; being a smaller and more delicately formed insect than that which infects the head. ‘s ; It is to be remarked, that this gentleman, who is very cleanly in his person, putting on clean linen every day, does not remember ever having lice in his head, nor on the groins. In the course of a practice of 30. years, I have not met with a similar case: and on looking into several authors find it mentioned in such terms as to induce me to believe it to be very uncommon, as few cases of the disease are re- Jated. ; “¢ Ulyssis Aldrovandi de animalibus insectis liber quintus. Aristotel. duo tantum pediculorum genera nata_ fuere; primum grandius hominibus valde familiare a capite orti, et toto corpore errans. Alterum ferum vocavit, durius eo, quod magna ex parte provenit, et corpori detrahi difficilius : hoc communi omnium prolatissimorum medicorum judi- cio, i]ud est quod plactulas nonnulli et plattas, Ttali plat- tolas et piattones a Jatitudine corporis dicunt. Galli mor- piones, Arabes gardan,”” &c. / The same author mentions one instance of the disorder ending fatally: ‘* Pherecydem Syrum pediculari morbo in- teriisse ;”? and adds, ** Oui morbum patitur primum ve- luti scabiei cujusdam pruritu allectus, corpus scalpit, vo- luptate simul et dolore perceptis *: deinde exorientibus pe- * These symptoms were exactly similar to those of this case. diculis Reply to Dr. Kelly’s Letter.. 51 diculis simul effluente sanie, morbi acerbitate, ac dolore percitus, unguibus corpus lacerat,” &c. The same author, among many instances of this disease being fatal, mentions that the English king Edmond died of the pedicular disease. Sauvage, (Nosologia methodica. Ordo septimus, CJassis X. Phthiriasis pedicularis. La maladie pédiculaire.) _ after describing the disease, adds, ‘‘ Phthiriasis olim inter morbos poenales habebatur, quo extinctos ferunt plurimos. Vide Schenkium, Camerarium, Plempium,”’ &c. and makes a second species, “ Phthiriasis interna: Vermine interne: Phthiriasis funesta.’’ In this species the insects issued from the eyes, ears, anus, urethra, and from the orifice made in venesection. This case terminated fatally. In conclusion, I would remark that, on touching one of these insects with oil, it was nearly dead in a few minutes : which circumstance would induce me to fecommend the trial ‘of such an application for this disease. Hatton Garden, Jan. 16, 1812. Joun ANDREE. VIII. Reply to Dr: Ketty’s Letter (see our last Number) on his supposed Discovery of an Error in the Nautical Almanac. By Mr. Firmincer, late Assistant Astro- nomer at the Royal Observatory, Greenwich. To Mr. Tilloch. Sir, I SHOULD imagine it is generally understood by the readers of your valuable Journal, that whatever papers ap- pear in that work without signature, or reference to other authors, are either the composition, of the editor, from in- formation received by him, or drawn up by. persons imme- diately under his inspection. With this natural impression on my mind I viewed the article in your Magazine for October, entitled, « On the Error discovered in the Nautical Almanac of 1812 ly Dr. Ketty,” and conceived you had received the information it contains either from the Doctor himself, or from some other of your correspondents to whom > he might have communicated it, and that, when it appeared before the public, the article with respect to its general tenor must be considered as your own. ' Knowing that this sup- posed discovery was no discovery at all, but that the Nau- tical Almanac of 1812 actually appeared in ‘the shape in which its learned author intended it, I was induced to send you an account of such facts as I believed would clearly show the truth of what I have advanced; and I considered I was at liberty so to do, under the form in which your D2 article 52 Reply to Dr. Kelly’s Letter on his supposed ' article appeared, without being thought to have reflected on the character or writings of the supposed discoverer, or indeed on any one else except the editor, whom T wished to correct not only in what regards the notice respecting the Nautical Almanac, but in that which it takes of the French astronomers in their conduct from copying the ephemeris of the Nautical Almanac into their Connoissance des Tems. Arecent communication has informed me, and must also many others of your readers, that what we take to be written by the editor, may in fact be the production of some other person, who chooses to consider himself of- fended at any animadversions on his subject, however in- accurate his statements may appear, without declaring such subject to be his own, till after the animadversions had been published. This circumstance we have now witnessed in the conduct of Dr. Kelly, who has thought proper to de- clare in your last number, that the article above alluded to was his own production; and the reason he gives for the omission of his signature is, that it has been considered as a plain, honest, and unassuming statement, that required neither voucher or signature,” a criterion by which your readers will be enabled in future to distinguish whether the articles they read are the production of the editor, or of a correspondent, to whom they may in some parts allude. — Whatever may be the opinion of the readers of the Phi- losophical Magazine, respecting the tenor of the article in question, I much doubt whetber they will entertain two opinions respecting Dr. Kelly’s last communication; they will, Iam induced to conclude, consider it as. a happy display of egotism, and an unwarrantable abuse of persons who neither knew, nor could be supposed to know, when they were animadverting on articles which appeared in the Phi- losophical Magazine without signature, that they were ac- tually animadverting on Dr. Kelly’s productions; at least I can so speak for myself. But with whatever impressions I wrote my former article, those under which I write this will certainly not be easily mistaken; and since I have been considered by Dr. Kelly as imprudent,’ I shall take the li- berty of freely discussing the merits of his statements. Dr. Kelly says, that ‘* neither was the statement dictated in terms likely to give offence, and yet it hus called forth two letters in animadversion, which are not of the most gen- éle tone or texture, and I shall therefore consider them as a kind of partnership production.”’ I do not know bow fara man may venture to publish his opinions when founded on the wild delusions of his imagination, so as to keep pa the < Discavery of an Error in the Nautical Almanac. 53 the proper boundary of prudence: but certainly in the pre- sent case Dr. Kelly is most completely mistaken ; for I can confidently affirm, that Mr. Groombridge knew no more of what I had written on the subject before it appeared in print, than did Dr. Kelly himself. But as the Doctor bas allowed mea right, I shall take an opportunity of occa- sionally referring to Mr. Groombridge’s letter, not only be- cause it has been considered a partnership production; but also because, from our long and intimate acquaintance, we have had frequent opportunities of communicating our thoughts on astronomical subjects. Jt was in one of these communications that Mr. Groombridge noticed to me the discrepancy in the quantity of the obliquity of the ecliptic as contained in the Nautical Almanac of 1812, from those of other years ; and my remarks upon it were, that the uncer- tainty arising from the observations of the Greenwich qua- drauit were such, as to render the quantity of that datum doubtful to many seconds. In confirmation of this state- ment, J shall once more call the attention of your readers to the paper which I published im the Philosophical Magazine of December 1810; and although J noticed this paper in my remarks upon the subject in question, I have good rea- son to believe Dr. Kelly has not given himself the trouble to read it; or, if he has read it, he has not thought proper to notice it, probably in consequence of its militating against his own supposed discovery. I shall therefore copy so much as relates to the present occasion, which runs thus: ‘ 10’ 31”; this hypothesis will give on! =F AS VSI) 2! SOW! VB" s we shall extract from these values the two following equas tions, “3102.u— 1899.¢= 1069, 1760.%— 617.t= 1016, which gives w = 0,881406, f = 0,910400: hence we conclude the true perihelion distance = 0,9609951, and the true instant of perihelion passage, the 29th of No- vember at 12" 49’ 46" mean time at Paris. In order to ascertain if these elements are very accurate, ave may calculate the corresponding values of m and n, and see if they are null or very small: now we shall find that in tlre present case these values amount only to a small number of seconds ; for the corrected elemepts give, for in- stance, for the first and last observation, v= — 60°56 37", ) /*y"=" 29° TO" 22", a = 10' 334, a@’= 279 11’ 56", c= Wg MO e” = 346° 38’ 53's from which we extract U7) ==' 907159507, 77 = 19091163", and consequently m= — 41. These elements: bieling very accurate, we shall extract from them by means of the for- mule (e) and (e’) the position 7 of the ascending node, and the inclination ef the orbit, and we shall find Place of the ascending node = FT 129 bate Inclination of the orbit = = 27° 19" 4”, In order to determine the place of the perihelion, we shall observe that &’—7= 269° 15’ 58", from which we extract 269° 20’ 50", for the distance from the comet to its node, reckoned on the orbit, at the instant of the third observa- tion: on adding to this distance the anomaly v" which the comet has traversed by a retrograde motion since its peri- helion passage, we shall have 298° 40! 19”, for the distance from the perihelion, reckoned on the orbit, to its ascending F4 node : 88 General Method for delermining node: by adding afterwards to this distance the longitude of this node, we shall have for the position of the perihe- lion’ on the orbit, 376° 3’.7", or more simply still 16° 3’ 7”. By collecting all these elements, therefore, we shall have for the true elements of the orbit of the second comet of 178), ; Perihelion distance.... 0,9609951. 20th Nov. 1781. Mean time at Paris of Ped 12h aot a6” perihelion ....eseees 5 Place of the perihelion of the orbit.. 16° 3” 7”. Place of the ascending node....... 77° 22’ 55”. Inclination of the orbit.........+. 27° 12! 4". The motion of the comet is retrograde. The supposition of the parabolic motion of the comets is not rigorous; it is even infinitely little probable, consider- ing the infinite number of cases which give an elliptic or hyperbolic motion, relative to those which determine the parabolic motion: A comet moved either in a parabolic or hyperbolic orbit will only Ke visible once ; we may sup- pose, therefore, with probability, that comets which de- scribe these curves, if some of them exist, have long ago disappeared, so that nowadays we only observe those which, being moved in re-entering orbits, are incessantly brought back to intervals more or less large, in the regions adjoining the sun. If they have been observed with pre- cision, and the visible are of their orbits be considerable, we may determine with tolerable accuracy, by the following method, the time of their revolution. For this purpose let us suppose that we have four excel- lent observations which embrace nearly the whole visible part of the orbit; and that we have already determined by the foregoing article, the parabola which nearly satisfies these observations. Let v, v’, v’, v'”, be the anomalies cor- responding to these observations; 7,757", 7°", the corre- sponding vector radii; take also v—v=U, vr —v=U', v"—v=U". This being done, we shall calculate by the foregoing ar- ticle, with the parabola which nearly represents these obser- vations, the values of U, U’, U", and those of V, V’, V'"; take therefore . U—V=m, U' —-Vt=m,U" —/" =m". We shall afterwards vary by a very small quantity the perihelion distance in this parabola; take then U.—V = ni — F'n" —V" = 0". We shall afterwards form a third hypothesis, in which, by preserving the same perihelion distance as in the first, we the Orbits of Comets. 89 we shall vary by a very small quantity the instant of the perihelion passage; take in this hypothesis, O-— V=), UV ='p5°U" =" =". This being done, with the perihelion distance and the instant of the passage of the comet by this point, found in the first hypothesis, we shall calculate the angle v and the vector radius r, in the supposition of a very eccentric el- lipsis ; so that by calling e the relation of the eccentricity of this ellipsis to its half great axis, the difference 1—e is equal to a very small quantity, for instance to 34. In order to have the angle v, in this supposition, it will be sufficient to add to the anomaly v, calculated in the para- bola, a small angle, the sine of which is . vs (1 —e).tang £ v. (4 —3.cos* Lu—6.cos* Zn) ; The new anomaly v being thus known, we shall substi- tute it in the equation fjs (i= ~ tang? $v) which is the expression of the vector radius in a very ec- centric ellipsis: by this means we shall have the corre- sponding veetor radius r. We shall calculate in the same way v’, rs v", Ps 0”, 7”; from which we shall extract U, U', U", V, V', V"; i this case take U—V=4, U!—Pi—q, Uts b=. Finally, let us call 2 the number by which we ought to multiply the supposed variation in the perihelion distance, in order to have the true one; ¢ the number by which we ought to multiply the supposed variation in the instant of the perihelion passage; and § the number by which we ought to. multiply the value supposed for 1—e; we shail form the three equations u.(n—m) +-t.(p—m)+2.(q—m)+m=0, u.(n'—m!') + t.(p'—m') + o.(g'—m’) + m= 0, u.(n"—m") + t.(p"—m") + o.(q'—m") + m’=0. We shall have, by means of these equations, the values of uw, ¢ and 0, from which we shall extract the true perihe- lion distance, the true instant of the passage by this point, - and the true value of 1—e. Let D be the perihelion di- stance, and a the semi great axis; we shall have a = smack from which it is easy to conclude, that the time of the re- volution of the comet will be equal to the number of sidereal. years expressed by ah ~. We shall have ‘as in page (1—-e)# 85; go Remarkable Cases of Venereal Infection. 85, the inclination of the orbit and the positions of the ascending node. and of the perihelion. _ When the arc observed of the orbit of a comet is con- siderable, and particularly when it extends beyond 90° of anomaly, where the ellipticity begins to become perceptible; it will be desirable that we should have four observations made with all the precision which we ought to expect from modern astronomy, taking care to verity the position of the stars to which we refer the motion ofthe comet. Whatever may be the precision with which we strive to make these observations, they will always leave some un- certainty as to the time of the revolution of comets: the most accurate method for determining it, is to compare the observations of a comet in two consecutive appearances : the resemblance of the elements of the two parabolic orbits determined by these observations, will make known the identity of the comet, and we shall have, by the difference of the instants of the perihelion passage, the time of its re- volution and its grand axis. It was thus that the period of the comet observed in 1531, 1667, 1682, and 1759, was determined; a period which 1s a Jittle unequal, on account of the attraction of the planets, as M. Clairaut has shown, by subjecting to analysis the perturbations experienced by this comet from Jupiter and Saturn, = = = = —=—S—S> KIV. Account of some remarkable Cases of Venereal Infection. To Mr. Tilloch. Sir, Padi me to communicate some medical facts which lately occurred in my practice; and as there is not any sufferer upon whom the circumstances can reflect dis- honour, or whose delicacy can suffer by the relation, an insertica of the entire matter in your imstructive Magagine may convey original information to professional men, and will oblige Your obedient servant, Rozert Heaty, M.B. On the 23d of July 1830, I was requested by a respectable friend to see his wife, who complained of great and general debility, loss of appetite, with violent pain of the head. She was nursing. The child seemed very healthy. She said she was attacked with hemorrhoids about three weeks after her lying-in, whith ason the itth of May 1810. She had had small glandular swellings in her groins, which had sub- sided ; Remarkable Cases of Venereal Infection. 91 sided; had taken no medicine. About ‘the esth, reddish spots appeared on her arms, ‘and? small tumours scattered ever her thighs, which disabled her from walking. She complained of profuse perspiration on her breast, particu- larly at night, 1 directed the warm bath with alteratives. August 7th. Notwithstanding the treatment, the sym- ptoms became much aggravated ; the reddish spots had spread upon her face. I requested my friend to confess whether he had not contracted the venereal disease; to which he answered in the most solemn manner in the negative. On the 14th I required a consultation, and met one of the most eminent physicians in Dublin. | After examining the patient, he mentioned our suspicion to the mother of the lady, that the disease was venereal. It was deemed advisable to bave a surgeon in consultation, and that we should meet the following day. In the evening I visited a patient convalescent from fever, from whom 1 heard that a Mrs. M. was dangerously ill, not only from a disease which she had contracted at the time of her lyimg-in, but also from avery sore mouth. On inquiry, it appeared that she was attended in her accouchement by the same gentleman who attended my patient. On the 15th we mets; and that consultation removed every doubt of the nature of the disease; and as she did not receive it from her husband, 1 suggested to the medical gentlemen that the accoucheur might have conveyed the infection by his hand, Tiat mode was deemed possible, though not very probable; and our opinion to that effect was communicated to the accoucheur, 18th. All that train of misery incident to supposed con- nubial infidelity, aggravated by the sufferings of a loathsome disease, must have been the fate of my patient, if she and her husband had not had proper mutual confidence and a friendly reliance on my farther investigation. I met Mrs. M.’s brother, with whom. | was acqnainted; and anxious to vindicate the character of my patient, | told him my su- spicion of his sister’s disease; and asked him, whether I could with propriety mention my suspicion of the disease to Mr. ivi. He answered in the afirmative, and introduced me to Mr. M. I related to that gentleman the situation of my patient, and requesied to know the disease his wife was labouring under, and the time of ber delivery. He said she lay-in. on the 92d of May 1810, that the accoucheur was treating ber at present for cancer in the womb, or a liver complaint, Isubmitied my opinion that it was the yenereal discase, and also that she might have been infected at 92 Remarkable Cases of Venereal Infection. at the time of her delivery, the accoucheur conveying the infection by his hand. He added, he suspected her dis~ ease to be venereal, and had mentioned. that suspicion to his wife frequently.. I was introduced to the lady; and after examining her, I became more confident in my opinion (as there were buboes in her groins). l-advised Mr. M. to have a conversation with the accoucheur, as to the nature of the disease. In consequence of this, he (Mr.M.). called.a consultation of the same medical gentlemen, with the ac- coucheur, who met onthe igth. The surgeon before the consultation called me out of the room, and communicated what the accoucheur bad informed him of that morning; namely, that he had contracted the venereal disease in his finger in the course of his practice, and had conveyed this disease in that manner. | I]t was deemed advisable, and even indispensable, for the accoucheur to confess that he was the cause of this severe ailment to those ladies; which he com- plied with by letter, not only to these ladies, but to others who had been diseased in like manner. Meaning to view the subject merely as.an instructive medical report, suf- fice it to say, that upon a full and legal investigation, it was deposed on oath by a medical gentleman, in behalf of the accoucheur, that he had contracted the disease in the course of his practice, about two years previous to the preceding unfortunate event; that he had undergone a complete course of mercury, and used even a larger quantity than is usual, and that he conceived himself incapable of communicating the disease ; that previous.to that gentleman’s attending my patient, a window sash had fallen on his finger, which produced a sore; that this sore became a venereal one, and infected. the ladies before he was aware of its real nature, The child of the first lady was weaned on the 15th; after- wards spoon fed, and continued healthy. The other child was transferred about the 19th to a sound. healthy nurse. In a month a rash, appeared on the bead of the child, which in a little time spread over the body, and remained ano- malous for a month, but afterwards became-distinctly sy- philitic, and) which yielded to the influence of mercury.) Sinee the occurrence of the above, I was called to attend a lady, who after exposure to,cold complained of acute pain of the right side, shooting to the scapula, causing difficult and impeded: respiration 5 cough and thirst urgent, want of appetite, tongue foul and blackish, pulse quick. She never was confined by sickness,.or stood in need of medicine. Married four months. These febrile pulmonary symptoms yielded ina week. After three weeks, I was again requested, to Geological Observations in Yorkshire, Derbyshire, Sc. 93 to see this lady. She now complained of sore throat’ with difficult deglutition. On inspection, there appeared slight inflammation of the tonsils extending to the palate, which ° continued stationary about a fortnight, without’ any other symptom of disease; when, during the use of the warm bath and gentle diaphoretics, venereal blotches on the fore- head and nodes on the shin bones arose. It appeared on investigation, that the lady had contracted the disease from her husband, who had had the disorder previous to his marriage, and who'had been apparently though not radi- cally cured. Relating this case to an eminent surgeon, he mentioned that a patient of his, a lady, who had con- tracted the venereal disease in her accouchernent from the above mentioned accoucheur, bad no other symptom but what first showed itself in the throat. "No. 1, Clarendon Steet, Dublin, Feb. 1, 1812. XV. Geological Observations, in Correction of and Addition to the Puper on the Great Derbyshire Denudation, in our last, and the Report on Derbyshire, &c. ; relating prin- cipally to Coal:méasures near to the Chalk Strata; the Course of the 3d and 4th Grit Rocks and Crowstone through Yorkshire, and the Termination of its Coal-field Northward: the Limits of the Yellow Lime Rock, and the Existence of Red Marl, Gypsum Beds, Strontian, &c. between its Rocks, ec. Se. By Mr. Joun Farry Sen. To Mr. Tilloch. Sir, W wen the paper which you have done me the ho- nour to copy from the Philosophical Transactions, into yotr last Number, p. 26, was sent to Sir Joseph Banks: but two or three sheets of my Derbyshire Report had been printed : since which period, by the many comparisons of my travelling and other notes and mineral maps, during the prinung of that volume, from the letters ad com- nlunications of my friends, and two journeys which J made into Yorkshire since the Report was published, some new Jights have been thrown on the north-eastern part of the great Derbyshire Denudation, the particulars of which I ~ aim anxious to submit without delay to your geological readers, im the hope, that some of them will be able and disposed freely to communicate new facts, and verifications or corrections of those which I have already, or am now about to mention, in order, that the remaining difficulties, with 94 Mr. Farey’s Geological Observations with regard tothe stratification of this important part of England, may be cleared up. When I said (p. 27 and 28 of your last Number) that ani uninterrupted series. of basset-edges of strata, dipping to the SE, and ranging in continuity from SW to NE in certain undulating lines conformable to the surface, “ from one sea to the other,” had been traced by Mr. Smith, and shown on his manuscript maps, | spoke from an imperfect recollection of some parts of his maps; and had forgot some difficulties which he once mentioned having expe- rienced, in tracing the strata across the flat country around York : at which time also, he was in the habits of meti- tioning the oalite or ova-formed limestone of the Bath series and of Portland island in Dorsetshire, as belonging to the same stratum; and as the Jate Rey. Mr. Michel also con- sidered them, as I have mentioned, p. 103, of your 36th volume, and vol. 1. p. 113, of my Derbyshire Report, but which now appears to be incorrect; and that the oalite of St. Alban’s-Head and Portland-Is!e on the south coast, is the same with that of Calne in Wilts, Aylesbury im Bucks ; and New-Malton, Helmsley, Kirby-Moorside, Pickering, and Filey head SE of Scarborough, in Yorkshire, and is situate within 100 yards (perhaps, and composed _princi- pally of chalk-marl) of the bottom of the chalk, greatly above the Bath-freestone *; and it seems, that beaded the disappearance of the upper of these important Oalites (the Aylesbury Limestone) under Alluvial Clay, from Stewkley in Bucks, through all Bedfordshire, (see that article in the Edinburgh Encyclopzedia,) and Cambridgeshire also, per- haps, till its first exit from the Island near Hunstanton- cliff in Norfolk, it makes no appearance, or where the lower Chalk again enters the Island nearW ainfleet in Lincolnshire, or for some distance after the bottom edge of the Chalk emerges {rom the Fens near Walton, as we proceed north- westward ; yet, in the hills near Dalby, Langton, &c. I saw’ thickness enough of strata basseting, to account for this Limestone Rock, that I had not time to search for minutely, or to inquire what had been proved underground, in sink- ing wells or otherwise, when I was in that county in 1807, * Do more than these éwo parts of the British series of strata produce ova- formed limestones ? a question Lask of your correspondents, from having seen a very flat Echinus filled with oalite (like those of the Bath strata) said to be brought from Linton-Swinden in Threshfield, ten miles N. of Skipton in Yorkshire? The large botryoidal Pisolithus at Boiling-hil! one mile S. of the mouth of the Wear in Durham, and in other situations, do not appear te compose regular strata, } believe, as the small pisolites do. Mr. Michel’s “very fine white sand,” vol. xxxvi. p. 104, seems to be that dug at the foot of the red marl range, on Markham-Moor, by the great North Road. i in. Yorkshire; Derbyshire, Gc. . 92 nor can I hear any thing more of the appearance of ‘this Oalite, near to Market-Raisin E, Caiston, W, Brigg E, crossing, the Humber NW _ of Barton, near Market- Weighton W, and near Pocklington, where J suppose to be its range, and on which points I solicit the assistance of your readers and correspondents, The first or outer-raised tract shown in the map and mentioned p. 30, of your last Number, I now suppose to have a north-eastern corner extended to near Leavening, between Acklam and Burythorpe, near to the edge of the Chalk! ; the eastern boundary fault, afier passing W_ of Bawtry and Thorne, as there mentioned, probably proceed- ing near Snaith, W of Howden, E of Aughton, W of Pocklington, W_ of Garraby-street Inn on the York and Bridlington Road (being here very near to the Chalk), near Acklam ; and after turning, nearly at right angles near Leavening, the same probably proceeds near Crambe S, Sheriff-Hutton S, Stillington S, Easingwold, Thirsk SW, to near the Swale River about Ainderby-Steeple, where 1 Suppose it to turn again at rather more than a right angle, pass NW of Northallerton, NW of Stokesley, near Ormsby, Wilton, and Kirkleatham, and enter the German Ocean near or on the SE of Redcar, near the mouth of the Tees: instead of this fault turning westward up the course of the Wharf River, as I conjectured a year ago (p. 80), before having seer the Country, as will be further noticed presently. By this prodigious eastern fault, it has lexpect happened, that the magnesian or Yellow Lime Rock (with perhaps Coal-measures above it in some places, Report i. 182) oc- cupies the surface under the Gravel, Peat, Sc. on its west side (p. 31) from vear Nottingham, to. somewhere near Pocklington* ; but on its eastern or/outer side, are Red: Marl strata, * And westward thence to near Wetherby, and even to Boroughbridge, probably, since in all the large part of this outer-raised tract, to the west of the line where Gravel is seea covering the Yéllow Lime, viz. from the E of Radford, near Nottingham, by Bobber’s Mill, Cinder hill S$, Basford NW, Bulweil E, Hucknal-Torkard E, Papplewick W, Anrfesley Park SE, S, and 5W, the Town W, Annesley-Woodhouse W, Kirkby 1 mile E, Sutton J mile E, Mansfield Town E, Mansfield: Woodhouse E, Market-Warsop W, Nether Langwith E, Cresswell E, (in Derbyshire), Belph E, Shireoaks E, (in Notts.) Gateford W, Carlton, Oldcoats W, Harworth W, Tickhill E, fin Yorkshire), Wadworth E, Uovetsall 'W, Doncaster W, Arksey E, Ows- ton, Sutton, Mawkhouse, Norton, Walden-Stubbs, Womersley, Gridling. Stabs EF, Knottingley E, Birkin, Hillam, Monk-Fryston, Soath-Milford E, Sherburn I’, Barlston E, Towton E, Tadcaster; and thence perhaps, W of Healaugh, b of Bilton, E of Kirk-Hammerton and Green-Haminerton, § af 1 the 96 Mr. Farey’s Geological Observations strata, containing accidental beds of Gypsum, at Newark and Hawton near it; at Tuxford, and Laxton, Askham and East-Markham near it ; at South and North Wheatley ; near Thorne, Crowle, &c. ; beds of ‘blue Marl-storie also occur in it, at Hookerton, Kirklington, Maplebeck, Sutton or Trent, &c. White Sand in West Markhani, as already men= tioned, &c.; and these Red Marl strata, abut against the fault on its E side, to somewhere NW of Howden* 3 when’ the Blue Lias strata of Long-Bennington, Coddington, and thence E of the Trent to Burton.on Stratherf succeed, and which strata soon after are lost under Peat’and'Gravel, and. I suppose, abut on the fault, NNW of Howden: ‘after these, other strata higher in the series, range ‘and’ abit in like manner, under Gravel probably, and’ then ‘the Bath Freestone ranges, along which the Roman* Road proceeds from Stamford E of Grantham, Ancaster, Lincoln, Spittal; the Yore River and of Boroughbridge, and E of Ripon, whichis as far N as my information of the eastern edge of the Yellow Lime (covered by Gravel) extends; crossing over therefore E to Sessay, and following the great fault above described, near Easingwold, S of Stillington, S of Sheriff Hutton, S of Crambe; turning then § along the vale of the Derwent to Butter- Crambe, and then SE te join the fault gain somewhere W of Pocklington, and thenée following the fault already described to Nottingham, all the large intervening space, including almost all the vale of York and Sher- wood Forest, has as Lam told, an entire surface of Gravel, Peat or other ex- traneous matters (according to my definition of each, Derbyshire Report i. p. 181), that prevent the regular or undisturbed stratification from being seen ; a circumstance which 1 particularly request assi:tance upou from your readers, who know or may happen to travel anywhere within this tract, and particularly that they would state, what the two remarkable Hills W of Selby, called Hambleton Hough and Brayton Barfe are composed of? since they can hardly be formed of alluvia? * In the north-east angle of the great fault, a piece of these same mea- sures secnis to remain on the surface, and produces a hail-pluster or Gypsum Quarry near to the Derwent, SW of Westow: and whrich Gypsum and Red Mart are probably in their proper relative situation to the Lias } strata, that might be found in Leppington aud Bugthorpe (alsu within the angle of the fault), as I judge, from the Pentacrinus or five-rayed Encrinus there found), (as mentioned Philosophical Transactions, No.112) especially if it be true, that this curious animal remain, is found in the British series; on/y i Lias sirata 2; on which question I particularly wish the assistance of your readers; for if they have also a place much higher in the series, it.may otherwise explain this part, and the appearance also of these fossils in the banks of the Swale at ‘Topcliffe (and perhaps at Allerton Maulleverer?) which bas induced Mr. Smith to conclude, that the Lias strata are there to be found? and us upper- measures to the Red Marland Gypsum, said to be found near Thirsk ?: and as all the suppositions that can be made on so new a subject of investigation, ought to havea candid examination, are there any local beds of Red Marl and Gypsum, much higher in the British series than the Bath Freestone? that might account for the Gypsum near Westow, aud perhaps at Bilton, Green Hammercon and 8 miles E of inaresborcugh, in the tanks of the Nidd near those places; W of Thirsk, and in Lazenby near the mouth of the Tees, &c, instead of the explanation that [intend to offer herein, regarding all but the first and last of the above-mentioned occurrences of Gypsum ? Wintringham, os to in Yorkshire, Derbyshire, @c. 97 Wintringham, and there it disappears under the waters of the Humber, and afterwards under the Peat and Gravel (as 1 understand) but proceeds beneath these until they ‘abut against the great eastern fault, somewhere SW of Pock- lington, and are no where afterwards seen northward in Great Britain, | believe*? The Sand, Limestone and gray Slate of Colly.Weston, the Barnack Rag-stone and Clay, the Bedford Limestone and Clay, and the great Clunch Clay, (Derby Report’i. 113), the Woburn Sands and Clays, &c. above it, and the Aylesbury or upper Oalite Limestone, all in like manner range successively to the Eastward, and are I believe, cut off obliquely and abut on this fault (perhaps under Gravel and Peat) W and NW of Pocklington: the Chaik-marl being perhaps the only stratum beneath the Chalk, that preserves its connection past the corner of the ouler or easternmost raised tract of strata (p: 2Q,of your last number), and after basseting at Birdsal (under Tottern- hoe Stone), occupies the space between the Chalk, east and south of it, near Settrington, Thorpe-Basset, Wiutringham, West Heselton,:Sierburn, Potter’s Brompton, Ganton, Folkton, Hunmanby, and the S end of Filey Bay: and the Oalite which ‘it overlies on the west and north &c. sides, near Langton, North-Grimstone, Settrington, Nor- ton, Old Malton, Amotherby, Barton, Stonegrave-Ness, Nunnington, Haram, Nawton, Webburn, Sinnington, Wrelton, Aislaby, Pickering, Thornton, Wilton, Ebbers- ton, Snainton, Brompton S, West-Ayton S, Scamer, Cayton, Lebberton, and Filey S. * Two circumstances seem to conspire, to prevent the tracing of the Malton or upper Oalite Limestone tar south of that town, viz. the low and flat alluvial surface of the country and the corner of the large lifted and denudated tract that-] have mentioned above, and | am not acquainted with any place where this Rock is conspicuously displayed $ of this, in Yorkshire, or im Lincolnshire, as mentioned above: north ‘of ‘the corner of this lifted tract, this Rock forms quite’a feature of the country, forming the surface in a large tract of very high and at present barren and heathy moors, principally, that stretch out to within seven miles of North- allerton s which extraordinary stretch of strata near the top of the British series, so far to the west, seems occasioned by a trough, or natural depression of the strata rather, per« haps, than to tilts by faults, which may be traced fromthe * Does Scotland produce any strata of ova-formed Limestone? Vol. 39. No. 166, Feb. 1812. G yale 98 Mr. Farey’s Geological Observations vale of the Hall River near Great Driffield, NW, near to West-Lutton, Wintringham, Kirby-Misperion, Helmsley, Old-Byland, and Over-Stilton, to the great fault perhaps, somewhere N of Northallerton; and which occasions the London Clay series to advance beyond Kendall, the Chalk beyond Wintringham on each side, the Chalk-marl almost to Helmsley, the Aylesbury Limestone to Keebeck, and the under strata of Coal-measures and Alum-shale near to Osmotherley at least; the dip being obliquely towards this line, itself declining eastward, but unequally in different parts; alow part of this trough, seeming to occasion the running of the Derwent W from near Filey to meet other streams coming eastward, on the N of Malton. The upper edge of this Limestone stratum has been men- ‘tioned, in speaking of the Chalk Marl; its lower edge and cline of its extent on the surface may be traced, near Wes- tow Crambe, Bulmer, Terrington, Dalby, Bransby N, Owston, Coxwold E, (with -detached hummocks at the Towns of Crake and Coxwold); then turning NE and E, owing to the deep and large excavation of the Rye River and some of its south branches (which has exposed the Coal-measures on Grimstone-moor E of Yearesley) N of Newboro’ Park, NE of Yearesley, SE of Shackleton, by Hovingham, crossing the Rye NE of this, by Stone- grave, S of Oswaldkirk (having inclosed a Limestone cap or hummock at Colton, and NW of it), Ampleforth, Oldstead, Kilburn S, Sutton under Whitsuncliff E, Thirlby, Boltby, Kirby-Knowle NE, (the town standing on a de- tached hummock), Cowsby, (Keebeck standing on a de- tached hummock), Arden-Hall N, Hawnby SW, S, and SE, Carleton 14 mile N, Skiplam N, Gillamoor N, Hutton in the hole S, Lestingham S, Cropton SW, S, and SE, New- ton N, Saltersgate or Half-way house S and SE, Lilla-cross S, Braxey W, Everly SW and S, (with » detached hum- mock E), Falsgrave S, Oliver’s Mount ?, Wheatcroft W, Osgodby, and Gristhorpe N, where it shows its under strata on the shore of the German Ocean: such are the results of my observations and inquiries, respecting the Locality of this interesting Oalite Rock, on which I shall be thank- ful to receive any corrections or additional particulars, from the kindness of your Readers, particularly such as can enu- - merate the extraneous fossils found in particular spots. From near Gristhorpe and Filey above mentioned, the measures that succeed these, below in the series, (with se- veral local peculiarities of dip, that I must reserve for -- other ‘in Yorkshire, Derbyshire, &c. ; 99 “other opportunity) occupy the coast in succession to near Marsk, and where the great eastern fault that has been men- ‘tioned abve, seems at once to cut off and conceal from the ‘sight, all the strata (that have been mentioned p. 96 and 97 above), between these and the Red Marl with Gypsum beds, of which there are said to be large quantities near to the Tees, N of Lazenby in Kirkleatham: whether these Red Marl strata occupy all the north-west side of the great “fault that I have supposed and mentioned, turn its W corner and proceed on the W side of Thirsk, where I have ‘been told that Gypsum is dug, as before hinted, T am un- able to say, any more than whether, the magnesian Lime- stone, that is described in Mr. John Bailey’s excellent Report oi Durham County, as overlying the great Newcastle Coal-series from near Sunderland to near Piersbridge on the Tees) is an immediate under-measure to the Red Marl, that I have been speaking of ? and whether it be the same with the Nottingham, Derby and Yorkshire magnesian or Yellow-lime Rock? and whether these actually connect, by way of Knaresborough, Ripon, Bedale, E of Richmond, Bee. as [ have been told “by some is the case? are questions on which IT am exceedingly desirous of accurate information 3 and would take the present opportunity of mentioning, that the lower or calcareous part of the Newcastle series, as de- scribed by Mr. Bailey, and by Mr. Westgarth Forster (see his * Section of the Strata’’) seem, in the blending of Grit- stone, Shale, Coal-seams, &c. with the Limestones pro- ducing Mineral Veins, to differ so essentially from the lower, or indeed any part, of the Derbyshire series, us to be with the utmost difficulty referred to the same part of the general-serics, as hinted in the note, p. 80, of your last number. Wiiether, in case of the identity of the magnesian Lime Rocks and their under Coal-measures in Derby and Dur- ham being established, the great fault that enters the island near Hartley i in Northumberland (see the Map afhxed to the ** Picture of Newcastle,””) by turning more southward, after * re-entering that County N. of Ebchester, may range across Durham. and the North Riding of Yorkshire, to connect perhaps with the great zigzag ‘fault of my Derbyshire Re- port and p. 32 of your last number, (on which | have more to say herein), and thereby entirely cut off and disconnect the upper and lower parts of what Mr. Forster has joined together as one series, perhaps about the 244th fathom o. his Section, being the place where Mr. W. Miller’s engraved G2 Section 100 Mr. Farey’s Geological Observations Section begins (and proceeds downwards further even than Mr. Forster’s), and by this means, make the Coa/ and the Lead districts of Northumberland, Durham, and York- shire to have no immediate or kuown relation to each other in the series, I am unable to say at present: but certainly this is one of several suppositions that ought to be fully tried, by an actual survey, before admitting the identity of such very different series of strata as compose the Lead districts of Derbyshire, and the Counties above mentioned. But [ return to the measures in Yorkshire, E of the great eastern Fault, that basset from under the Oalite Limestone, and occupy a space more or less wide on the SW and N sides of that limestone tract, from near Westow on the SSW of Malton, by Spittal-bridge, Sheriff-Hutton, Cox- wold, Thirsk, Northallerton, Stokesley, Gisborough, Marsk, Danby, Lyth, Whitby, Goadland, Cloughton, Scarborough, &c. &c. and have to mention that I find these, after a care- ful examination of the Country about Lyth (on which T in- tend to say more at a future opportunity) to be Coal-mea- sures, and consider them not less remarkable as occurring ina much higher part of the British series, than had hi- therto been supposed to contain any vegetal impressions or other true indications of Coal*, than as containing nu- * Candour and truth require, that I should here recall some too confident and hasty expressions, on what I had been led to think a true position, viz. that no distinct small vegetal impressions like those of the Coal-measures, were to be found in the British Series above the Lias and Red Marl, as I have said in the article}Coal, and some others in Dr. Rees’s Cyclopxdia, and in Dr. Dickson’s Agricultural Magazine, vol. i. p. 116, and vol. ii. p. 30, the latrer in answer to a defender of the disastrous scheme of sinking for Goals at Bexhill in Sussex; and it is somewhat singular, that the call or challenge which I therein gave (p.31) to produce a single specimen of such im- pressions found at Bexhill, or in any upper part of the series of strata, has not had the effect of obtaining cither public or private information of such an instance, until I saw the strata in the north of Yorkshire, above alluded to in July last. I now however think it highly probable, that the strata around Battel, and eastward of it in Sussex, belong to these Coal-measures (though I saw no vegetal impressions there) and that the appearances of thin seam of Coal seen N of Court-lodge in Mountfield, E of Mountfield, at Darvel-furnace near Robertsbridge, Silver-hill near Salehurst, &c. which Lheard of in 1806, but referred to imperfect accounts of //uvd-Coal or bitu- minated Wood in the Pipe Clay stratum (below the Chalk, and not above it, as I now understand the Clay of Purbeck to be): but without much altering my opinion oi the improbability of discovering even one useful seam of Coal at Bexhill, or in any other part of Sussex. I further think, that the appear- ances of Coals that have been mentioned at Brill N of ‘Thame, Southcote near Leizhton Buzzard, in Stone-lane, between Leighton aiid Woburn in Bedfordshire, near Bolingbroke in Lincolnshire, and in numerous other places, ju the range of the Clunch Clay, are to be referred to these Coal-measures, instead of bituminated Wood or Clay, as Mr. Smith and myself used to “think; a conjecture of which coincidence of the Clunch-Clay and the Alum Shale, 1 offered at p. 259, of your 35th vclume. aii merous in Yorkshire, Derbyshire, &c. 101 merous species and vast numbers of animal remains mixed with its vegetal remains, and as containing but one seam of Coals, and that a thin one, rarely amounting to 9 inches thick, and never exceeding 18 inches, as I believe, after a pretty extensive inquiry; though there is often a partial Jayer of wood-coal a good deal below it. The account of Mr. Edward Martin’s South- Wales Mi- neral-basin has, Tobserve, been by a mistake in the note in the Philosophical Transactions, and p. 28 of your last num- ber, referred to the volume for 1808 instead of 1806. From all that I had read or heard, respecting the northern termination of the valuable Coal- field of the West Riding of Yorkshire, some distance N of Bradford, Leeds, &c. and hearing bow much wider this fieid was Ww and NE (irom Halifax to Fryston-Hall near Ferrybridge) at no great di- stance before its termination, than it is anywhere S of this in Derbyshire: I rather too hastily (as it now appears) con- cluded, that the zigzag fault (Derby Report 1. p. 168, and p. 32 of your last number) was diminishing northward in Yorkshire, or the rise becoming less on iis W side, and that it would soon terminate, so as to admit a complete and more extensive series of Coal: -measures basseting, in regular succession, about the parallels of Leeds and Wakefield than I had seen, as hinted p. 176 of my Report: and that in consequence there must have been a fault, unconnected with this zigzag fault, that ranged E and W about the course of the Wharf River, &c. (p, 30 of your last num- ber), against which the several Grit-stene Roeks and Coal- shales abutted, nearly at night angles: on examining the country about Wakefield and Leeds and NE of itlast August, I find‘ however these facts to be very materially different, and that the zigzag fault continues northward of Dinning- ton (where it is shown in the Map in your last number) to increase and acta stil] more important part in the structure of the country, than it has done south of this; its route probably being, near to Hooton-Roberts, Clayton, Feather- sfone, Castleford, Church-Garforth, Barwick in Fimets Thbtner, Bardsea Ww, East- Keswick W, Sicklinghall, &ce. 5 and perhaps, if the V eltow Lime continues much farther northward? it may continue to follow its western edge un- til almost arrived at the Tees, and then diverge from it west- ward to let out the Newe astle Coal- field, as has been already hinted, page 99. Those three remarkable and characteristic strata, taken in connection, the coarse 3d Grit Rock of Freestone, the G 3 thick 102 Mr, Farcy's Geological Observations thick 3d Coal-shale upon it, containing Crowstone, Ganister or Galhiard, and the 4th Rock on this, of excellent gray Slate and paving-stone,.were left off in nty Survey for the Derbyshire Report, at Penistone (Yorks.), and.a little NW of it, ranging then almost NW, and proceeding, as I rightly conjecture d, for Huddersfield and Ealand on the Calder (Report i. 164), and from the recollection that I had of the range of the strata at Halifax, since I was at school there with the late Mr. Robert Pallman in 1783, I was nota little surprised, on visiting Woodhouse and Headingly NW of Leeds, in company with my very valuable F riend (acquired entirely through a ‘correspondence on these subjects in your Magazine) Mr. Smithson, in August last, to observe there these three strata with all their usual characteristics and some others, ranging about ENE and dipping southward, making direct for the edge of the Yellow Lime, and against which and the zigzag fault, I satisfied myself by numerous inquiries, that they actually abut near Thorner, the 4th Ruck being there clevated, on the SW of the Town, to the levei of the Yellow Lime on its E side! ; and that all the numerous upper strata to these, had made a ‘like but Jess extensive turn eastward, and had disappeared or basseted northward, instead of abutting in that direction against a fault, as supposed. he ranve of the 4th Rock, as an fades. to all the rest, may he, from Penistone by May -Thorn, Brake-hole, Al montbury, Huddersfield E, yell Ealand, Southowram, Bank-top, Thornton, ‘Afiertaug Heaton, Eccleshill i in Idle, Stanningley, Bramley village (the famovs quarries at the Fall by the Leeds and Liverpool Canal, bemg in the 3d Rock), Deadingly 5, Woodhouse N, Chapel- - Allerton, Rounday S of Shiadw ale and Thorner. The 3d Rock, I believe, abuts on the Yeliow Lime and zigzag Fault between Thorner and Bardsea, at a still higher level ! and it seems probable, that this southern dip continues, until the 2d and ist Grit Rocks and 1st Coal-shale and the Limestone-shalé are brought round to abut on the zigzag fault, near to the edge of the Yellow Lime: but still it seems, that a branch from the zigzag fault must range westward, not far beyond the Wharf River perhaps, anx T near Otley, Keighley, &c. (as mentioned p, 30 of your last number), as otherwise, if the dip continued, the Mineral Limestones and alternating Toadstones of the Derbyshire series must basset, N of Otley or W of Ripley, of w hich I never heard the probability ; ; but the Limestones aad other strata there seem, as far as | have heard, to answer nearly to the lower part of Mr. Westgarth Forster’s in Yorkshire, Derbyshire, Se. 103 Forster’s series, as already hinted p. 100: unless indeed, they can be referred to anomalous beds in the Limestone Shale? like other remarkable ones that are mentioned in the Der- by Report i. p. 228, &c, In the preface to my Derbyshire Report p. xiv. T have mentioned the Red Marl strata containing Gypsum beds, that had been said to cover or lie on the top of the Yel- low Lime Rock at Fairburn N of Pontefract in Yorkshire, and the importance oftascertaining (as I have no where yet been able to de) What is the regular or proper covering stratum to this Lime Rock? made it among the most in- teresting objects of my visit to Mr. Smithson, to go with him and view these Gypsum quarries; but before I men- tion my observations at Fairburn, it will be proper here to give a more exact account of the Western edge of the lower part of the Yellow Lime Rock (where it is seen covering the Coal-measures) to the north of the Anstons in York- shire, than is to be found at page 156 of my Report, and which, from what I have seen and been informed, 1s as fol- lows, viz. North-Anston, Dinnington SW, Laughton-en- le-Morthen W, Slade-Hooton, High-Hooton, Maltby 5, E, and N, Clifton W, Conisborough SE and E, Cadehy S and W, Melton SW, Barnborough NE, Hickleton, Hutton- Pagnell, Moorhouse E, Stubs-Hall, North-Elmsall W, Upton NW, Went-Bridge, (very probably with some detached hummocks to the W) East-Hardwick, Darring- ton W, Pontefract E, Glass-Houghton E, Fryston-Hall S, Ferrybridge W, Brotherton SW, Fairburn SW, Newton- Abberth S, Kippax SW, (with two curious detached hum- mocks SW) West-Garforth, Moor-Garforth, Barwick in Elmet E and NE, Potterton SW, Kid-hall, Thorner Church, East-Rigton W and N, (witha small and a large hummock north of this between East- Keswick and Colling- ham), Compton NW, (where my maternal Grandfather lived), Wattlesike, Linton S, Weod-hall N, Sicklinghall E, Spofforth E and NE, Plumpton Hall SW, High-Har- rowgate NE, Knaresborough W, &c.* After ascending with Mr. S. the edge of the Limestone at Newton-Abberth, in our way to Fairburn, I was soon after * In the Rev. William Atkinson’s collection at Boston, near Thc rp-Arch, I saw some turbinated and scallop shells in dark-gray Limestone from Allerton- Mauleverer, that may perhaps belong to the blue beds in the lower part of the lower Yellow Lime Rock (unless they belong to the Liasas before hinted) Report i. 157 ; and the Coals which G. B. Greenough, Esq. observed working at Arkendile NW of this, last summer, may be those called the Bilborough Coal, Reporti. 166, and those of Parlington near Abberford, and several other intermediate places, G4 conducted 104 Mr. Farey’s Geological Observations conducted to the north of the Road, and of Fairburn old Limestone Quarries, and in the midst of a common-field, the general surface of which is Limestone with many shal- Jow quarries in it made by the Farmers ; we ascended a de- tached hummock of perhaps four or five acres extent and 40 or 50 feet high, in the SE side. of which the Gypsum is dug, in a great number of thin regular beds in red marl, nowise materially different from all the Gypsum quarries that I had previously seen in this mal, except perhaps that the beds of Gypsum are more numerous and thinner than usual: standing on the top of this interesting hammock (which has been dug over for Gypsum) with Mr. 5S. I re- marked to him, that here were certainly undisturbed strata upon the Limestone Rock that we had ascended from the Coal-measures, and that the green hills in the inclosures to the north, showed marks of the ancient diggings of Gyp- sum or Marl in their sides, and doubtless were similarly constructed to that on which we stood: but observing, that the Limestone hill about five or six furlongs to the east of us, on which the village of Fairburn stands and the great North Road passes north of it, was much higher than the Limestone field that surrounded us, or than this hummock, T remarked, that either a fault must range between us and that hill, and had raised that so materially (previous to the denudation that had left these singular hummocks), or, that there were two Limestone Rocks, on the upper of which Fairburn stood, and Newton on the lower, and that these Marl hummocks were the remains of a stratum between these Rocks. We lost no time in reaching Fairburn to verify, if possible, one or other of these suppositions, and soon found on inquiry, that several of the Wells in the village had been sunk through Limestone into similar Marl with Gypsum beds: a more decisive proof however immediately offered itself, in a Tunnel that Mr. George Althas had about two years beforedriven under the Village and Turnpike Road, at 54 feet deep, for conducting a rail-way branch from the Air Navigation, into the deep Limestone quarries N of the Road, which Tunnel passed along this Marl and Gypsum stratum: in examining of which in its place:at bottom of the quarry, | was then and since able to detect several errors that [ had fallen into when on my Derbyshire Survey, and examined patches of loamy Sand and marly substances on. the planes of Yellow Lime, in different places, and which, from having seen or heard no instance of such basseting, or having a regular place between the Limestone Rocks, and owing chietly to the vicinity or admixture of the Sherwood- Forest in Yorkshire, Derbyshire, Gc. 105 Forest Gravel near or in the top of such patches, T con- cluded all such to be, and have described them as a/luvia, and have in consequence, omitted to observe or notice, a most important feature of the Yellow Limestone Rock, or Rocks rather, that of their having strata of Red Mar] (sometimes holding Gypsum and other substances), ochry ciay, loamy or founders’ sand, &c. interposed between them, of very variable appearance and thickness, but sometimes capable of forming a feature in the Country, as we have seen to the NW of Fairburn in Yorkshire. I will therefore here mention the places in order, beginning S, near which I suppose that the upper Yellow Lime Rock ends, and these anomalous beds basset, with remarks, as I go aloug, of the probable errors in my Derbyshire Report, in considering them as alluvia, &c. I am doubtful whether the Forest Gravel admits of seeing the upper Yellow Lime Rock, anywhere south of Mansfield in Nottinghamshire, (and probably the Red Clay on the Limestone at the south end of that town, of which bricks are made, may belong to these anomalous Beds? and so may the lower and regular part of the large patch of Founders’ or casting Sand, Report i. 464, Brick-earth, &c. extending to the Brick-kilns SE of Skegby, Report i. 452, that I have considered as alluvia in my Report, owing to the quartz pebbles scattered on its surface), but it probably _ appears at Mansfield-woodhouse, Warksop Park in Derby- shire, Shirebrook, Over-Langwith, Langwith Lane, Walley- Wood, (west of this, about 14 mile E of Bolsover, a hummock of Founders’ Sand and red Brick-earth occurs, W of the Tampike Road, Derb. Rep. 1. 135, 463 and 452), Walley village, Bonbuck E (Notts.), Crag-Mill, (west of these; Founders’ Sand at Frithwood-Farm, and on Elmton Com- mon, Report 1. 464 and 137), Whitwell E, (Redhill, of loamy saud with quartz on it, Report i. 142), Steetley, Shireoaks Park in Notts. Wood-mill, Yorkshire, (Sand and Brick- earth in Thorpe-Salvin, by the Chesterfield Canal, Report i, 141 and 452), Gilding Wells, Letwell, Roch-Abbey FE, Braithwell (the Fullers’ Earth at Raddle-Pits, Report i. 465, probably belongs to the anomalous beds of the Mar!), Ed- lington, Brodworth E, (Sand and Loam near Redhouse on the York Road, and Founders’ Sand near Hutton Pagnell), Wentbridge W, (reddish Clay in the north Hill, in the York Road), Greave-Park SW, (Clay on a remarkable small Com- mon by the York Road, SE of Pontefract, called the Devil’s sowling-Green), Knottingly E, (bere J am informed, that in cutting a canal near the Air River, Red Marl and Gypsum were 106 Mr. Farey’s Geological Olseruations in Yorkshire, Se, were found ; to the W, also, Founders’ Sand is got at Glassy Houghton and Wereldon or Weldale), Brotherton, Fairburn (Red Marl and Gypsum SW and W, as above mentioned), Ledston E, Micklefield, Abberford, Potterton E, (here and at Whinclose one mile N, near Bramley Park, a white Clay is found, with Galliard or Crowstone-like beds init, and a white tender Grit-stone or Sand at Bramley-moor Quarry, and at the SE corner of Bramley-Park; a patch of Clay on the Limestone SE of East-Rigton, belong also I expect to the anomalous beds between these Rocks), Bramham 13 mile E, (a very heavy and curious sparry bed about two feet thick, on the Limestone under Mr. Joseph Bovill’s Farm, at the NE end of Bramham Town, belongs perhaps to the anomalies of these Marl beds), Toulson (on thebanks of the Wharf River about a mile below Thorpe-Arch, beds of Red Marl and some Gypsum layers appear, and this Marl seems to make a red clay surface on the Lime, N of Thorp-Arch), Bilton (here Gypsum is found, see Mr. James Sowerby’s British Mineralogy, Tab. 234), Tockwith, Kirk-Hammer- ton, Green-Hammerton (at the latter place Gypsum is dug, as I am informed, and between them the Gypsum anil Sul. phate of Strontian is found, I believe, and in this stratum, that Mr. James Sowerby has figured and described in the last number of his “ British Mineralogy,” Tab. 444, though said by its diseoverer to be had from the banks of the Nidd ear Knaresborough, which is § miles off, A more particular survey of the western side of the Yel- low Lime district, would I] doubt not, discover many other curious and anomalous substances, that might be referred to the beds between the upper and lower Rocks of that series. The establishing of local Geological Societies, such as [ have recommended p. 217, and others of my Derby-~ shive Report, would prove of the most essential service in promoting and methodising the several inquiries which I have herein suggested, and many others net less important, that will occur to all those who apply seriously to the in- vestigation of the facts of the Terrestrial Stratification, a pursuit in which utility will be found eminently united with the highest species of gratification. I am, sir, Your obliged and very humble servant, Upper Crown-Street, Westininster, JOHN Farry Sen. February 9, 1812, Mineral Surveyor. AVI. De- [ 107. J XVI. Desultory Observations concerning certain vegetalle Muscicape. By Professor Barton, of Philadelphia. Communicated by the Author. A FEW years ago, I accidentally discovered that the flowers. of the Asclepias syriaca of Linnzus*, like the flowers of the Apocynum androsemifolium, are endowed with the faculty of catching and retaining flies and various other kinds of insects. I have given some account of this dis- covery in the Transactions of the American Philosophical Society tT. In the course of the present year (1811) I have ascer- tained that the beautiful Asclepias curassavica is also a Mu- scipula, or rather a Muscicapa. My observations were made on a small and by no means vigorous plant of this species, which I had raised from seed. These observations con- vince me that this Asclepias, in its native climate, or any where else when adult and vigorous, must be a powerful and even wseful fly-catcher. It often so completely retains insects, even pretty large house-flies, that they are wholly incapable of disengaging themselves, but perish upon the flowers. Others, hardly more fortunate, escape with the loss of their proboscis, or some of their limbs, Few, per- haps, escape entirely uninjured.—The mechanism by which Asclepias curassavica catches flies, is nearly the same as that by which they are caught in Asclepias syriaca B. As the genus Aseclepias consists of a considerable number of species, and as all the species are so similarly constructed that there is no good reason to doubt that they are all en- dued with the power of catching insects, it is easy to per- ceive what an immense havoc these plants must make of animal life, especially in many parts of the United States, where some of the species.of Asclepias are so numerous that they cover hundreds of acres of ground, in close con- nexion, especially along the banks of our rivers, in ihe sandy fields, &c. In the short paper entitled “ Memorandum concerning a new Vegetable Muscipula,” which is inserted in the Trans- actions of the American Philosophical Society, and to which * Asclepias syriaca fp. of Michaux. 4 Vol. vi. part i. No. xvi. p. 79—82, Mr. Sonnini has given the credit of this little discovery to an English naturalist of my name. ‘The respectable French naturalist, speaking of the Asclepias syriaca, says, “‘ Une propriété curieuse de ces mémes fleurs, dont la découverte récente est due au Docteur Barton, de Londres, c’est qu’elles attrapent les mouches qnis’y posent at- tirées par le suc mielleux qu’elles contiennent.”-—“ Plus de soixante mouches furent prises ..... sous les yeux del’ observateur Anglais, &c.”"—Juurnal de Physique, &e. tom, lxvi, p. 219. I have 108 Observations concerning I have already referred, I have, I fear, fallen into an error concerning the Nerium Oleander, or common Rosebay. My words are these: ‘ It has long been known that this is a poisonous plant. But I do not know that any per- son than myself has observed that this fine vegetable proves very destructive to the common house-flics. These insects visit the Oleander, 11 order to drink the fluid secreted in the tube of its flowers. The liquor soon intoxicates them, and very few of those which have gained admittance into the blossom ever return from it. So great is the number of flies destroyed in the course of one season by a single Oleander, that I have often thought it would be worth our while to pay more atiention, than we yet do, to the cul- tivation of this vegetable ; as, independently of its beauty, it is so weil calculated to lessen the numbers of a most common and troublesome insect.” Subsegnent and more cautious inquiries have convinced me, that although the nectareous fluid of the Oleander may prove deleterious to flies, yet that the greater number of the insects which are observed dead or dying, in the flowers of this plant, have been entrapped by the irritability of the genitalia; by a mechanism, at least, as truly irvitable as that by which insccts are detained in the flowers of the dif- ferent species of Asclepias, of Apocynum, and other similar plants. In the course of my inquiries and labours concerning the indigenous plants of the United States, I have had the additional satisfaction of remarking, that one of our Grasses is also a Muscicapa, or at least a catcher of small insects of various kinds. And, so far as L know, it is the only erass, hitherto discovered, that is entitled to the name of a Muscicapa. The grass to which J allude is the Leersta lenticularis of the late Mr. A. Michaux*®. This plant is a native of the marshy grounds of the Illinois country, of Virginia, North Carolina. &ce. I do not know that it has been found in Pennsylvania. The glume or corolla consists of two valves, a character which belongs to all the spectes of the genus Leersia. In the Leersia which is the subject of my observations, the glume ts of an orbicular form, inclin- ing to Jenticular, and is much larger than in any of the other American species that are known to me, or than it * Leersia (Jenticularis) panicula ramulis subsolitariis, ramillis secundariis imbricatim spicifloris: glumis lenticulari-orbiculatis, conspicue ciliatis, ma~ susculis—Flura Bercuts- dnicricana, &c. tom.1, p. 39. 1s certain vegetable. Muscicape. 109 is in the Leersia oryzvides of Europe and America. The edges of the valyes are very distinctly ciliated, or furnished with a number of fine teeth or delicate spinules. It is this ciliate structure that enables the plant to per- form the business of a Muscicapa. When a small insect, such as a spider or a minute fly, insinuates itself between the valves (probably in pursuit of a honeyed fluid), the valves close upon it, the spinules enfolding each other; thus re- taining the insect, which, I presume, as seldom escapes as the insect that has been caught by the valvalar structure at the ends of the leaves of Dionea Muscipula. In the Leersia oryxoides of Swartz and Michaux (Leersia virginica of Willdenow), which is called in the United States * Cut-grass” and ‘* Sickle-grass,” the structure of the glume is very similar to that which L have just described. In particular we observe the ciliated structure, though it is less conspicuous than it is in the Leersia lenticularis, No doubt, the former as well as the latter of these grasses is entitled to the appellation of a Muscicapa. But {have not yet observed insects between the valves of the Leersia virginica. I may hereafter inquire more. particularly into the subject. In Georgia and in Florida there grows a beautiful, shrub to which the inhabitants have given the name of ‘ Fly- catcher.” This shrub is the Befaria paniculata of Mi- chaux*, The inhabitants collect branches of it, when it is in flower, and hang them up in their rooms, and find the flowers of very great use to them in ridding them of flies: hence its name, which I have mentioned, and the only one, so far as I-can learn, by which it is recognised in its native country. Tam not sufficiently acquainted with this piant to say, with certainty, by what power it is that it catches, entan- gles, or destroys the flies; whether by a contractile or irri- table property, residing in some of the parts or organs of the flowers; whether by the glutinous quality which be- longs to the flowers; or whether by a deleterious quality belonging to the nectar of the flower... I may, however, observe in this place, that the Befaria is one of the vegeta- bles from which. the bees in the countries of Florida, &e, arc thought to procure a narcotic or deleterious honey, Sull L suspeer that the muscipulating faculty of this plant wil be found to be owing to a peculiar mechanism; that * Befaria (yonieulata) ramis hispidissimis; foliis ovali-lanceolatis, glabris. pauiculs subaphylla, mukifiora, glutivoss,— Fiera, &c, tam. i. p. 280. tab, 26. is, 110 Observations eoncerning is, to an irritable power residing in the flowers. But this point remains to be determined by better observations. I have never yet had an opportunity of examining the Befaria in a living state. I might here give a long list of vegetables, such as dif- ferent species of Rhododendron, Kalmia, Robinia, Silene, Lythrum, which by virtue of the viscosity upon different parts of their flowers, &c. entangle and destroy small in- sects. But my business in this imperfect essay is not with Muscicape of this kind. Yet a more critical inquiry into the use of this viscous matter, in the vegetable ceconomy, by which millions of insects are destroyed in our gardens, green-houses, woods, &c. might deserve the attention of physiologists. In regard to the Sarracenia, 'as J design to make their bis- tory, botanical, physiological and medical, the subject of a distinct memoir, I shall content myself at present by offer- ing a few detached facts and observations concerning these plants. It is well known that all the species of this singular genus (and I think at least seven species have heen dis~ covered in North America) are inhabitants of the water, or of wet situations. All the species are furnished with tu- bular or hollow leaves (ascidia), which in the more aduli plants are seldom found without a considerable number of insects dead or living in them. Ido not mean, however, to insinuate that these insects owe their presence in the Sarracenieé to any thing like an zrritable property residing in any part of the plants. Indeed, I have not discovered any vestige of peculiar irritability in the constitution of the Sarracenia. But I think it sufficiently evident that nature has taken some pains (if it be ever allowable to use such language in speaking of the works and operations of Na- ture) to solicit insects into the ascidia of the species of this genus. Thus, the flowers of the Sarracenia flava "(the yellow Trumpet-leaf or Side-saddle-flower of the people of the United States) have a most offensive, cadaverous or carrion- like odour. This odour, to speak more properly, seems to reside principally, if not entirely, in the broad peltated stigma of the plant. I think it probable that it is, 2 part at least, this odour, which is so potent and diffusible that it is sometimes perceived at a considerable distance from the plant, in a warm and rather confined atmosphere; that it is partly this odour, which serves to solicit various kinds of insects about the plant, many of which before they can reach certain vegetable Muscicape. 11a reach the stigma are necessarily entrapped in the ascidia. But I know not what may be the final intention of Nature in giving the peculiar odour which I have mentioned to the stigma of Sarracenia flava and some other species of the genus. Those philosophers* who imagine that there are some plants which cannot be impregnated without the aid of insects, may perhaps fancy that they have discovered Nature’s ulterior object in the present instance. Indeed, T confess myself at a loss to conceive how, in some of the species of Sarracenia, the pollen or fecundating in- fluence of the stamens can reach the wpper surface of the stigma. See in my Elements of Botany, and in other works, the figure of Sarracenia purpurea.—And I presume, that it is certainly upon the upper surface of the stigma of these plants’ that the pollen, or at least its fovilia, must be applied, in order to enlarge and render fertile the embrya seeds. In the Sarraceni@, the aid of insects in giving fer- tility to the germen or ovarium may possibly be necessary. I think it cannot be much less necessary (if at all less ne- cessary) in Sarracenia purpurea, than it is said by Mr. Will- denow, Dr. J. E. Smith, and other respectable botanists, to bein Aristolochia Clematitis.—See Willdenow’s Principles of Botany and of Vegetable Physiology, English translation, pages 316—318. Edinburgh, 1805f. But although I believe in the doctrine of the sexes of plants as a general doctrine, Iam compelled by many facts and considerationg to doubt whether the impregnation of any vegetable is necessarily dependent upon insectile aidf. On this curious subject I shall offer something more specific in my “ Memoirs on the Origin and Progress of our Knowledge concerning the Sexes of Vegetables.’’ . But there is still a much more considerable and obvious * Linnzus, Sprengel, Willdenow, Smith. + See also Dr. Smith’s Introduction to Botany, &c. page 337, &c. London 1807. This botanist not only reposes confidence in Willdenow’s theory of the insectile impregnation of Aristolochia Clematitis, but he thinks it pro- bable that “for waut of some insect adupted to the same purpose in its own country, the American Aristolochia Sipho, though it flowers plentifully, never forms fruit ” in the British gardens. However it may bein Aristolechia Cle- matiis, 1 am persuaded that insects are not necessary agents in the impreg- nation of the germ of Aristolochia Sipho, or “ Dutchman’s-Pipe,” as it is called in Pennsylvania. Iam well acquainted with this plant, and cannot perceive from the structure and disposition of its genitalia any obstacle to the appli- cation of the pollen to the femaleorgan. Certainly, there is much less difi- culty in conceiving how impregnation is effected in this Aristolochia, than in hundreds of other plants, concerning the impregnation of which no ditii- culties have ever occurred in the minds of botanists. ‘The dichogamic plants can be in no other way fecundated than by in- sects.” —Wlldenow. cause 312 Observations concerning cause of the collections of insects which are so frequently observed in the ascidia of the Sarracenie@., These ascidia, in some if not in all the species of the genus, appear to possess a kind of glandular function, like the true nectaries of a yreat many plants. A honeyed fluid is secreted or de- posited on the inner surface of the hollow leaves near their faux or opening; and it is this fluid which allures great numbers of the msects, which they are found’to contain, into the ascidia. . , I was entirely unacqnainted with this curious ceconomy in the ascidia of the Sarracenie when | published the first edition of my Elements of Botany; and even when I printed ihe Appendix (in vol. 1.) to the second edition of this work. The fact will not be deemed uninteresting by the cultivators of vegetable physiology, since it somewhat enlarges our views of the uses of the ascidia, and may assist us in making a better disposition of these parts among the glands, or glandular-like organs, of vegetables. I have little doubt, moreover, that a more accurate examination of the genera of Nepenthes, Aquarium, and similar plants, of which the number is not inconsiderable, will render it certaim that a honeyed fluid deposited about the opening of the ascidia of these remarkable plants, is in them, as in the Sarracenia, the principal eause of the deposits of insects which the tu- bular leaves are so generally found to contain. Let me add, that in the American plants, of which I have been speaking, the honeyed fluid may often be very distinctly seen; though sometimes, especially in the warmer weather, it is only to be discovered by the éaste. Many uisects, as well as some other anima!s, are found in the ascidia of the Sarracenia, Nepenthes, &c. which do not appear, to have been solicited thither either by the ca- daverous odour of the flowers, or by the honeyed fluid about the opening of the tubular structure. In the Sarracenia we find species and sometimes large species of gryllus, or grasshoppers, of gyrinus, &c. And Rumphius, speaking of Nepenthes distillatoria, informs us that ‘* various little © worms and Insects crawl into the orifice and die in the tube, except a certain small squilla or shrimp, with a protuberan& back, sometimes met with, which lives there.” Smith’s Introduction, &c. pages 197, 198. | Dr. Sunith has * no doubt, thai this shrimp feeds on the other insects and worms, and that the same purposes are answered in this instance as in the Sarracenie.’’ It is certain, that a remarkable instinct directs some species of insects to visit the ascidia of diferent species of Surracenia, certain vegetable Muscicape. 113 Sarracenia, principally, if not entirely, for the purpose of depositing their eggs or larve in them. We often see some of the Jarger species of Musca and Talanus sitting upon the edges of the openings of the ascidia of Sarracenia flava and Sarracenia purpurea. We soon find that they do not come here, as do the majority of insects, for the purpose of sipping the honeyed fluid from the ascidial glands.» The mother-insect, carefully poising herself upon the brim of the ascidium, emits from her uterus into the tube one or more larve, which immediately betake themselves to the lower part, where meeting with abundance of good food, they rapidly increase in size and in strength. I must give to Dr. Smith the credit of having preceded me in making, or at least in recording, an observation nearly allied tothe one which I have just detailed.“ An insect of the Sphex or Ichneumon kind,” as far as be could learn from the description communicated to him, ‘* in the Botanic Gar- den at Liverpool,” ‘* was seen by one of the yvardeners to drag several large flies to the Sarracenia adunca, and, with some difficulty forcing them under the Jid or cover of its leaf, to deposit them in the tubular part; which was half filled with water. All the leaves, on being examined, were found: crammed with dead or drowning flies.” ** The Sarracenia purpurea,” adds Dr. Smith, ‘*is usually observed to be stored with putrefying insects, whose scent is perceptible as we pass the plant in a garden.’ This I have not ob- served: and perhaps the odour spoken of may be that exhaled from the flowers, or genitalia, of the plant. ‘* Pro- bably (the learned English botanist goes on to observe) the air evolved by these dead flies may be beneficial to vegeta- tion, and, as far as the plant is concerned, its curious con- struction may be designed to entrap them, while the wa- ter* is provided to tempt as well as to retain them. The Sphex or Ichneumon, an insect of prey, stores them up un- questionably for the food of itself or its progeny, probably depositing its eggs in their carcases, as others of the same tribe lay their eggs in various caterpillars, which they some- times bury afterwards in the ground. Thus a double purpose is answered; nor is it the least curious circum- stance of the whole, that an European insect should find out an American plant in a hot-house, in order to fulfil that purpose.” * It is evident, from what has already been said, that it is not the water in, but the honey about and upon, the ascidia,which tempts the greater number of insects to visit these tubes, in the different species of Surracenias Neither is it the water that retains them. Vol. 39. No. 166. Fel. 1812. H T feel 114 Observations concerning I feel much obliged to Dr. Smith for leading me, by the preceding observations, to pay a more critical attention than I might otherwise have done to the ceconomy of the Sar- vacenice and other ascidial piants. Hitherto, however, 1 have not observed any species of Sphex, or of Ichnewmon, engaged in the singular business which he has mentioned. And although I do not doubt that the gardener’s statement is in the main correct, yet I incline to think that the sup- posed Sphex, or Ichnewmon, was an insect of some other ta- mily. Future observations will, | hope, enable me to de- termine this point entirely to my satisfaction, Although [ have no doubt that | ants may derive much of their nutriment and strength fics. the elements of de- composed animal bodies, just as i suppose that innume- rable species of animals are nourished by inorganic matter ; and although it is possible that the air evolved by the dead insects in the ascidia of the Sarracenie and other similar plants may contribute somewhat to the vegetation of these plants, yet I cannot suppose that the final intention of Nature in furnishing plants with ascidial leaves is to lay up a store of nutritious aliment for the plant. So far as the species of Sarracenia are concerned in this view of the subject, I hardly know avy plants to. which such storehouses as we are speaking of would be less ne- cessary. For they live in the midst or upon the margin of marshes, where animal matters of various kinds are con- tinually putrefying, and where of course the plants are al- most constantly surrounded by an atmosphere of azotic and hydrogen gases. ' Again, the wonderful Dion@a Muscipula, the extremities of whose leaves entrap, and frequently retain for a consi- derable time, various small species of insects, resides only in marshy grounds, not much unlike those just mentioned, In this plant, it appears to me to be still more difficult to give a plausible guess about the intention of Nature in constructing these vegetable Muscicape, than in regard to the Sarracenia. : If, however, we were acquainted with only the last-men- tioned vegetables, with Nependies aud with Diove@a, as the only plants, I say, endued with the power, however different the means, of catching or entrapping insects, we might, perhaps, with some degree of reason imagine that this fa- culty is, somehow or other, subservient to the business of ~ vegetable nutrition. But never can this idea be extended, with even the faintest shado of a good theory, to those truly irritable Aluscicapee, Apocynum androsemifolium, Asclepias certain vegetable Muscicupe. 115 Asclepias syriaca, Asclepias curassavica, Nerium Oleander, and many others, whose flowers entrap insects or the parts of insects. For, in these plants, the whole quantity of ani- mal matter applied to and retained by the plants, in their most vigorous state, is a mere atom in comparison of the volume ot living vegetable matter to be nourished. More- ever, the animal matter is applied only to the flowers, which no one imagines to be essentially concerned in nourishing the plant; to the femporary organs, and not to those which may be called permanent, the leaves or ascidia. In making these observations, I have not an eye to the theories or speculations of any particular author. I must confess, however, that 1 once imagined that Dionzea Mus- cipula itself does receive a part of its nourishment from the insects which it entraps. And Mr. Roth, if J do not mis- take, has endeavoured to show that the species of Drosera, so common in the bogs of Europe, &c. are, in some mea- sure, indebted for their growth and nourishment to the in- sects which they entangle and retain. IT have not seen the arguments by which the respectable botanist just men- tioned supports his hypothesis. I must not take my leave of the Sarracenie without ob- serving, that the ascidia of some (perhaps all) of the species of the genus furnish us with still another beautiful example of what the ingenious author of ** The Studies of Nature” would call the “ harmonies” of the vegetable and animal kingdoms. For, omitting, at present, all further speculations about the intention of Nature in giving to the species of this genus ascidial leaves, and a capacity of entrapping great numbers of insects, it is a fact, that these leaves be- come repositories of the food of various species of birds. It is not uncommon, in the native soils of someof the species of Sarracenia, to see great numbers of birds, especially some Muscicape, or Flycatchers, and other Passeres, assembling about these plants, and, by means of their bills, slitting the ascidia in order to get at their favourite food*. This weil ee ascertained * Linnzus tells us that the hollow leaf of Sarracenia purpurea is a reservoir of water for thirsty little birds, ‘ Folium S. purpurez in Spec, Pl. deserip- tum, aquam prebet sitientibus aviculis.” Prlectiones in Ordines Naturales Plantarum, Edit. Giseke, p.316. Hamburgi 1792. ‘This is doubtless a mis« take. ‘The birds supposed to be sipping water from the ascidium of Sarra- cenia were, I suppose, engaged in the very different business of eating the insects which the reservoir contained. None but a bird with a very long bill would be able to take the water from the tube. Is it likely, moreover, that any bird should be driven to the necessity of satisfying its thirst from the reservoir of a plant which always grows in wet places, and frequently in waters of a foot or more in depth? for Sarracenia purpurea is sometimes secn growing in our cypress swamps, its roots, like those of a Lemyg or an i Utvicu- 116 Observations concerning certain vegetable Muscicape. ascertained fact will not be deemed incurious in a history of the genus Sarracenia; nor unimportant in a history of the instincts and intelligence of the great class of birds. We know much less of the structure and ceconomy of the different species of the genus Nepenthes, and of the only species of the genus Aquarium that has yet been discovered, than we do of the structure and ceconomy of the species of Sarracenia. But it is highly probable, that the ascidia of both Nepenthes and Aquarium* will be found. by future ‘botanists and naturalists to serve the same purpose, with respect to birds, as do the Sarracenia variolaris and other species of the genus in America. The large ventricose ascidia of Sarracenia purpurea are employed as cups, for holding and conveying water, by the reapers and mowers in some parts of the United States, particularly, 1 think, in New Jersey, where the plant is called ‘* Water Brash.” tie ali After proceeding thus far, it was originally my intention to have offered some speculations of my own concerning the final object of Nature in constructing VeGETABLEMUs- CICAP#, and especially those which I have ventured to call irritable Muscicape. But the present essay has already been extended to too great a length. My intended specu- Jations may possibly form the subject of a future commu- nication. In the meanwhile, these ‘* Desultory Observa- tions” may perhaps contribute to the amusement of some of my brother naturalists, both in Europe and in America. Tf they shall produce this effect, my principal object in lay- ing them before the public, in their present crude and irre- gular state, will have been accomplished. BenJAMIN SmitTH Barton, M.D. Philadelphia, Septen.ber 3, 1811. Utricularia, being suspended in the water and totally detached from the earth. Ifit be true, as is asserted, that the Trochi/us Colulvis. or common Humming-Bird, is sometimes seen about the ascidia of the Sarrucenice, we seem safe in conjectrring, that this beautiful bird visirs these tubes for the double purpose of sipping the honeyed fluid and of eating the insects.@l have elsewhere shown that insects constitute a part, and pérhaps a considerable part, of the food of this Trachtlus.—See the Philadelphia Medical and Physical Journal, vol. i. part 1. art. xxiv. : * Ido not know whether this singular plant (Aquarium sitiens of Lesche- nault), belonging to the natural order of Succulentee, has yet been publicly figured or described by any botanist. I have seen a drawing of the plant, which is a native of Australasia, in the possession of Mr. Leschenauit, when {had the pleasure of knowing this intelligent botanist, and of inspecting a part of his rich collection of plants, &c. in Philadelphia, in 1807. The Aquarium grows in a moist but firm soil. Its radicel leaves are hollowed, and are in shape somewhat like a water-pot. Each pot is about an inch long, and is capable of containing a good deal of water. XVII. Case Cuz] XVII. Case of Injury of the Head, To Mr, Tilloch. Srr, Drererent Numbers of your Magazine having at times fallen in my way, and seeing that several medical cases were recorded; I thought | would send you the fol- lowing notes of a case which has lately come under my own observation, that, if you deemed fit, they may be in- serted in your widely circulating Magazine. From your humble servant, Joun Burne. —={s—— J.T. aged 36, for the last ten months has been a con- stable. About five months ago he was struck on the fore- head by a man he was endeavouring to secure. He felt very little inconvenience from the blow, and went about his em- ployment as usual. Jan. 3, 1812. He said he was very unwell, with a dull heavy pain ‘in the head, bnt he complained of nothing else ; his appetite was very good; his bowels pretty regular ; his eyesight very good, and he could walk about quite well. B Pulvens Rhet. Terebinthinee Chie aa 5]. M. Ft. pilule xxx, qua- rum duas his die sumat. KR Emplastrum Picis compositum Neucha. Jan. 7th, -he found limself much better; the pain was nearly gone, and he thought he should have no need to apply again. The above treatment continued. Jan. 17th. I have heard nothing of him since the 7th till this morning, when he sent to request that I would visjt him, for he was confined to his bed, and very dangerously ill. When I visited him (which was about noon), I was informed from his wife that he had continued to get much better till the 16th, when he was suddenly seized with pain in the head, giddiness, trembling ; lost his speech, and the use of his right arm. In this state I found him ;’ the light did not affect his eyes; he seemed very dull and stupid; his bowels were contined : RK Submuriatis Aydrargyri gr. vj. : Pulveris Rhei gr. x. M. Ft. pulvis statim sumendus ex Theriacd, K Emplastrum Lytte Neucha. Jan. 18th. Bowels have been purged ; has passed a very restless night: cannot speak; in other respects the samme: bis skin hot and dry. H 3 A Misturee 118 Case of Injury of the Head. KR Misture Camphore 3yvj. Liquoris Ammoniz Acetatis 31. Liquoris Antimonii tartarizati 3ij. M. Fiat mistura, cujus sumat cocblearia dno ampla quartis horis. Jan. 19th. No better; has passed a very restless night : cannot speak: right arm still insensible, and he has no power to move it. R Submuriatis Hydrargyri gr. }. Pulveris Antimonialis gr. 1). Nitratis Potasse gr. xv. M. Fiat pulvis quartis, horis sumendus ex Melle. R Emplastrum Lyttz largum toto capite. Jan. 20th. Somewhat better; can speak a few words, but very indistinctly: has had no sleep; the light during the whole time has produced no pain or inconvenience to his eyes: there is much stupor and dulness about him ; he complains of nothing, but shakes his head when he is asked how he does. The powders continued. Jan. 21st. Has had a little sleep ; can speak rather more distinct ; his right arm is sensible to the touch, and he can move it a very Jittle. The same treatment continued. Jan. 22d. His bowels are regularly open; has passed a better night ; moves his right arm rather more freely, and can take a little food. The powders continued, but not so often. Jan. 24th. Much better; can sit up in the bed and eat some meat; sleeps tolerably well, but has a troublesome tickling cough. The powders are discontinued. B Oxymellis Scillz. Syrupi Papaveris albi 4a 3]. M.Cochleare minimune urgenti tusse capiat. Jan. 30th. Cough relieved: has taken no other medicine 5 he is able to get up and walk about the room: appetite pretty good ; his right arm is more sensible, and he can move it much better; speaks more distinctly. I put a se- ton in the back part of the neck, and ordered him to take no medicine whatever. Feb. 12. The seton has discharged copiously, and he has found very great benefit from it; he sits up all day; can walk very wel]; has quite recovered the use of his arm: appetite very good ; sleeps very well, and can speak nearly as well as ever, and now wants nothing but strength ta en- able him to resume his former employment. Ts it not most probable that the above symptoms were occasioned by effusion causing compression in consequence of the blow, or by inflammation? The symptoms seemed to indicate the former more than the latter, Hatton Garden, Feb. 17, 1812. XVIII, Com- [ 119 J XVIII. Communications from Mr. Attan and Mr. Stan- CLIFFE on Allan’s Dividing Instrument. To Mr. Tilloch. Sir, I BEG leave to inform vou, that Mr. Stancliffe wrote his first opinion of my improvement on the mathematical Dividing Engine, after he went home from seeing the wooden model at the Society’s house, and before he saw the engine itself. As \ was surprised to see such an opinion inserted in the Society’s Transactions, after giving his ap- probation in so strong terms when before the Gentlemen of the Committee of Mechanics appointed by the Society of Arts to view the engine at my house on the 15th of De- cember 1810, I mentioned the circumstance to him, and told him of some observations in a certain obscure publica- tion ; in consequence of which he has thought proper to fa- your me with the enclosed paper. Mr. Stancliffe has for many years been justly celebrated for his extraordinary nicety in dividing, as well as for his extensive knowledge of the most useful imstruments in the mathematical line; and any ideas that he commits to paper on the subject of mechanism I consider to he worthy of notice ; and I hope you are of the same opinion. If so, I should be very bappy to see it published in the next Number of the Philosophical Magazine. I am, sir, with true respect, Your obedient servant, February 19, 1812. JaAmMES ALLAN. fCOPY.] To Mr. Allan. Srr,—I HAVE lately seen in the Retrospect (No. 30) of philosophical, mechanical, &c. discoveries, some very strange remarks in the observations on the improvement on the Dividing Engine made by you, which I am clearly of opinion must have had their foundation in prejudice or ex- treme ignorance, or perbaps'both. Here | shall not enter into any detail or vindication of what T said respecting my opinion before the Gentlemen of the Society of Arts, of the great perfection, | believed, and do still believe, that may be produced from your plan of racking or cutting the teeth of a circle for the purpose of dividing mathematical instruments. However, by way of explanation, I wilt! Ha slightly 120 On Allan’s Dividing Instrument. slightly touch on a few points as a.corroboration of my former opinion, When the wooden model of the wheel and ring was first .put into my hands at the Society’s house, I immediately saw the, great utility of the ring. [am still in the same opinion, that the principle, which is not attended with any great de- gree of difficulty in, formation, will be found to produce that accuracy which I think is not likely soon -to -be excelled. The great improvement which bas teen made in Jathes for turning large work would render that part of the operation - quite easy, even if it was carried to six feet or inore in dia- meter. A partial expansion at the time of racking, seems to ah one of the greatest objections that can be made to a large size, and the bad effects of that I believe might be overcome. To that extraordinary remark, in the Retrospect, saying, ‘* We can conceive cases in which the effect of the shifting would be to diminish the size of one or-more of the teeth each time below that of the rest, instead of equalizing them, and. finally, to cut some ad them away entirely,” I shall. make no reply. only, that it cannot take place without an error of at least one whole tooth, before the shifting of the ring. Any man that knows the principle of e 'd a wheelbarrow will see the absurdity of this remark in a moment. T hope it is mentioned in the Transactions of the Society of Arts, that when under the operation of racking or form- ing the teeth, the ring must, after being reversed. or moved 180° once or twice, which will produce correctly all the way round opposite teeth, although unequal in themselves, be shifted one quarter or 90° ; and then proceed with the racking and reversing as before, Which will in the end, I have no doubt, provided all the work and apparatus concerned is good, produce the number of equal. teeth required round a circle, for the purpose of dividing mathematical instruments probably not yet equalled. I have bad some experience in these things, which | hope will allow me ‘to speak with that confidence T do on this point. | The in- sirument alluded to in the Retrospect: is the first essay on the art of dividing by the rack and screw, brought forth by Dr. Hook in the year 1674, was merely a quadrant for the purpose of astronomy, with teeth cut with a screw all the way on the outer edge ; which was not into degrees. and minutes, but their true value was to be found afier- wards: therefore it was pat intended as a machine to divide. others * On Allan's Dividing Instrument. 1291 others with.) The plan was soon abandoned by the Doctor on account of its inaccuracy, As far as I was ever able to learn, I believe my old master, Hendly of York, was the first that ever made an engine to work all the way round by a screw, to divide with. It was about 13 inches diameter, and cut into 260 teeth or degrees. 1 have worked with it many a day, both in the dividing and cutting down way. Mr. Smeaton saw it in the year 1741, and he has told me since that he believed it was made ‘about two years before that time. Now 72 or 73 years, ¢ Now J] will on your plan, just in a few words, ron over the whole of the operation of making the teeth. All the apparatus being prepared and quite ready for the cutting part, J would first start on Ramsden’s plan by the dots, one half or nearly of the whole depth of the teeth. This done, the screw has now got a firm hold of the teeth, and plenty of room for correcting by the ring, before the finish, apy inequality that can exist in the complete circle. Having arrived at this point, I consider the work in a forward state, and the difficulty all over. So much accomplished, I would proceed no further on Ramsden’s plan, but wou!d have re- course to the correcting ring, proceed with the racking and shifting in the manner described above. Towards the last I would shift the ring every time it was once worked round by the screw cutter. By this moving the ring to half and to quarters alternately, all those errors will be perfectly corrected without much attention of the workman. The Retrospect says you have given no proof, but bold enconiums on the perfection of your instrument, and denies its self-evidence. I really do not know any Greater test’ that it can be put to than may be done by the ring, which is certainly a part of the machine. I am confident in my own mind, that with making some little change, the whole of this piece of business, I mean cutting or racking the teeth truly, might be accomplished to the greatest degree of exactness, without steady pins or ever lines (only a few pencil marks) by contact itself, which Mr. Smearon says, und seems to have proved, in the Philo- sephical ‘Transactions of the year 1785, is fifteen times nearer the truth than coincidence. Respecting your im- provement in the dividing engine, by what I have said above, yous will perceive thai [still Support my first opinion, that it is a great and important discovery ; and remain, sir, yours truly, Little Mary-le-Bone Street, Joun Sra NCLIEPR. Feb. 10; 1814, P.S.—I 122 On the alkaline Matier contained in dropsical Fluids P,S.—I must say this, that I think the Gentlemen of the Society of Aris, &c. are very unhandsomely treated by the critic to whom I have alluded, as if they exercised no judge- ment on whom, or for what, they bestow their honourable and bountiful rewards, XIX. An Answer io the Observatious of Dr. PEARSON (seé our last Number) on certain Statements respecting the alkaline Matter contained in dropsical Fluids, and in the Serum of the Blood. By Avex. Marcet, M.D. F.R.S. one of the Physicians to Guy’s Hospital. To Mr. Tiiloch. SIk, Aurnover I feel disinclined to engage in any public philosophical controversy, especially when the object is to vindicate statements, the truth of which any common. ob- server may easily ascertain by experiment ; yet, as there are some points in the above communication which do not place the question in its proper light, and might mislead those who have no opportunity of referring to the original documents, I have thought it necessary to offer in return a few observations. The state of the question is simply this: all chemists have for a long time agreed that the blood, and probably all the animal fluids, contain, together with various neutral salts, a certain portion of alkali not combined with any acid. This alkali bas generally been considered as being soda, although a few chemists had also noticed traces of potash in some of these fluids. Dr. Pear- son, on the contrary, in examining various kinds of animal substances, and especially of expectorated matter, was led to conclude that the whole of the uncombined alkali con- tained in the animal fluids, was potash ; and that they did not contain uncombined*® soda in any proportion what- ever. In analysing the fluids of dropsy, I was naturally led to Inquire into this question, and the results wbtained induced me to conclude, that the only uncombined alkali present in the bleod, or other animal fluids, was soda; and that the indications of potash, which by applying the test used by Dr. Pearson [ was able to detect in these fluids, were owing to the presence of that alkali in a state of Combination with the muriatic acid, The experiments I adduced in evidence were of two * By the expression uncomlined, 1 mean not combined with acid. kinds ; and in the Serum of the Blood. 193 kinds; some. jof. them showing, that the uncombined alkali was soda, .and..others, that, it. was not-potash. 2.4). )0 05 Portions of saline matter. being procured from, various animal fluids by evaporation, and, incineration, and brought by subsequent redissulution and evaporation to a crystalline state, crystals of determinate forms were obtained, some of which appeared to consist exclusively of subcarbonat of soda, some of muriat of soda, and others of muriat of potash; but none could be detected which appeared to contain any carbonat of potash. Other similar portions of the saline matter being treated with acetic acid, in order to bring any uncombined alkali present to the state of acetat; and alcohol being added with a view to separate these acetats, the residue of this alcoholic solution appeared to consist almost solely * of acetat of soda; whilst, on the other hand, potash was found in the residue left undissolved by the alcohol. In these various trials the presence of potash, in a state of combination, was proved by the tests of oxymuriat of platina and tartaric acid, both of which form precipitates with potash, and not with soda. The uncombined alkali, on the contrary, was shown nof to be potash by the last-mentioned tests failing to indicate the presence of that alkali; whilst, on the other hand, it was proved to be soda by the action of nitric acid, which, in combining with it, formed crystals of a rhomboidal instead of a prismatic figure. I shall not enter into the particulars of these operations, because they are minutely related in the communication which has given rise to this discussion ; but I shall now rapidly examine the principal objections which Dr. Pearson has made to the above conclusions. Dr. Pearson’s first ground of complaint is, that instead of showing his conclusions to have been erroneous, that is, I conceive, instead of following him step by step in his. inquiry, I have contented myself with exhibiting my own experiments and conclusions. But I beg to observe, that the object of my inquiry was not to repeat Dr, Pear- son’s experiments, but to examine dropsical fluids; and that, if in the course of my analysis I met with results which militated against his conclusions, it could not be reasonably expected, that in stating these results I should think it incumbent upon me to wade through his laborious * A trace of potash was detected in the alcoholic solution; but it must be remembered that alcohol, however rectified, will take up minute portions of muriat of potash, or indeed of almost any other soluble salt, researches 124 On the alkaline Afatter contained in dropsical Fluids researches' on the various forms of sputum or expectorated matter. I might indeed have abstained altogether from re+ ferring to, bis labours 3, but I thought it due to him, as a philosophical 3 inquirer ‘Tong known in the chemical world, to point out such similarities or discordances of results as occurred, in. our respective experiments; thus referring the matter,to the decision of physiologists, and showing that there was no wish, on my side, to overlaok the authority of former inquirers. In endeavouring to analyse the various objections brought forward by Dr. Pearson, [ am’so often ata loss to under- stand his meaning, and, I must add, so much embarrassed by the obscure and inaccurate manner in which he has stated some of my own proceedings, that it would be a task equally fruitless and Jaborious to follow his steps closely. I must, therefore, as much as possible, select those objections which are of a specific nature, and may be answered by an- appeal to experimental evidence. Suchr i is, for instance, tbe argument which he employs, no less than three times, (once in support of his own experiments, and twice with a view to invalidate my inferences,) on the effects of alcohol and acetic acid,—which argument is founded upon his belief that acetat of soda is mot soluble in alcohol, and that it is ~ wet a deliquescent salt; two palpable errors, which half a grain of this salt and a few drops of alcohol, with no other apparatus than a watch-glass, would have enabled him to rectify. But the objection which recurs most frequently, and that upon which the greatest stress is laid, is the minute- ness of the quantities of saline matter subjected to experi- ment. It would appear that Dr. Pearson questions whether a few grains of saline matter may be expected to yield re- sults similar to those which would be obtained from larger quantities ;. whether, for instance, the same inferences might be drawn from rhomboidal crystals of a minute size, as from similar crystals of larger dimensions ;—or, whether experiments tried upon an ounce or two of my dropsical fluids, may be brought into competition with those which he performed upon two or three pints of his ropy sputum ? Sueb a scepticism, I must own, I have myself never en- tertained. I have always thought, on the contrary, that the chemical properties which belonged to a particle of matter were exactly similar to those which would be found to be- long to a whole mountain of the same substance; that a rhomb of only one hundredth part of an inch might be characterized by its form as distinctly as one a hundred times . and in the Serum of the Blood. . 125 times larger *, But TI carry the point still further; for I go the length of believing, that many experiments of re- search may be wonderfully facilitated by analysing upon a smal] scale—that a great deal of convenience, of economy, and sometimes even of accuracy, may thus be gained; and that, in some instances, we even acquire new powers of in- guiry by operating upon small quantities f. hus, were it not for the assistance of minute microscepic observation, a great number of important facts which have enriched chemistry within the last twenty years, would in all probability have remained undiscovered ;. and this country might not have obtained that first rank in philoso- phical chemistry, to. which it has but lately been raised, and which it had long held in other departments of science. Is it necessary that I should specify particular instances ? Can any philosopher, attentive to the progress of analytical chemistry, overlook so many discoveries in which neither furnace, nor forge, nor subterraneous. laboratories, have been concerned—in whicb a watch glass, a blow-pipe,’and a few drops of chemical. re-agents, have been all the in- struments required? Were not, for iustance, the analyses of the Iceland springs by Dr. Black (the same eminent phi- losopher to whom Dr. Pearson appeals as an authority against microscopic observations) performed upon quanti- ties of saline matter of astonishing minuteness '—Surely Dr. Pearson cannot have forgotten that it was by the. accurate examination of only a few grains of matter, that the na- ture of no less than five kinds of urinary calculi has been ascertained, and their discrimination rendered easy and cer- tain—that the nature of diamond bas been established—that no less than four new metals have heen discovered in the crude ore of platina—that the similarity between ail the * Thus. I have no hesitation in maintaining that, unless it be proved that nitrat of potash may crystallize in rhombs, my conclusions respecting the particular point in question, would stand upon that evideuce alone; or that unless it be shown that carbonat of potash may erystallize in cubes, my inforence respecting the presence of muriat of potash stands uncontro- verted. With regard to my attempt at expressing centesimal parts of grains, which is, with some apparent reason, noticed s an instance of singular pre- tension to accuracy, 1 beg to observe, that I have never actually attempted to weigh smaller quantities than decimal parts of grains; and whenever smaller fractions have been expressed, they have arisen from a conversion of those numbers to some general standard. + 1 would also observe, whilst upon this subject, that there is a degree of neatness gained by reducing the scale of operations, which is ofteg incom- patible with processes conducted in the large way: thus, [ have never found it necessary, in analysing, to introduce amongst the enumeration of contents “a litle dirt,” as some old-school chemists have been in the habit of doing. f meteoric 326 On the alkaline. Matter contained in dropsical Fluids, _meteoricistones has been proved+that the identity’of the ‘chemical: agencies of’ electritity, whether ‘excited by’ the common niachine, or by the Voltate’ battery, has been demonstrated-that in’ a'neighbouring’ country the forma- tion of crystals has been explained upon systematic prin- cipies—that amongst us a new and wonderfully accurate in- strument of crystallography has been invented—and above all, that the metallic bases of alkalies, those extraordinary bodies which nature had hitherto concealed under an im- penetrable disguise, have at last been brought to light ! Let it be remembered as one of the most glorious circumstances of that discovery, that it was by examining mere atoms of these substances that their properties were first ascertained ; and that when, in consequence of subsequent improvements in the mode of obtaining these bodies, they were procured in larger quantities, and their general properties were re- examined, no error was discovered, and no important in- formation was added to that which had originally been gained from microscopic quantities. It is far from my intention, however, to contend, that, on some occasions, new and important facts may notbe brought to light by means of processes conducted upon an extensive scale, which would not admit of being reduced to a sinall compass. I only mean to assert, that such in- stances are comparatively but rare; and that no philippic against the examination of small objects—no appeal to old masters—no slight upon modern improvements, ought to deter chemical inquirers trom adopting methods which some of our contemporaries have employed with so much utility and success. ; Amongst other inaccuracies in the critique which has given rise to these remarks, my paper on dropsical fluids has been represented as being the joint work of Dr. Wol- Jaston and myself; for which supposition there was no other authority than a note in the paper in question, in which I acknowledged my obligations to Dr. Wollaston for the information and assistance which I bave on this and other occasions, derived from his kindness. I need not say how highly { should’ have been flattered by such an association ; but I think it due to him to state, not only that he had no share in the general inquiry, bat that be did not even see the paper in question previous to its publication. 1 cannot refrain from noticing, amongst Dr. Pearson’s remarks, another kind of licence which appears to me still less warrantable. I allude to the practice of quoting in italics, or placing between inverted commas, words or phrases The Diacatoptron. 127 phrases which have not been used, and to seize upon them as a subject of ridicule. | This is the case with some pro- posed elegant changes, and with my supposed recommen- dation to transfer chemistry to the “ fire-side of the draw- ing-room :” expressions which I have not used, and yet upon which Dr, Pearson has thought proper to be extremely jocular. I have only further to add, that should Dr. Pearson again write upon the subject, I shall not easily be induced to re- sume the controversy. Iam sorryy therefore, to see it inti- mated at the conclusion of his paper that he proposes to continue his observations in your next Number; and as it appears that those intended remarks are meant as a return for the notice which I have taken of his papers, T regret the more that he should take so much trouble. For praise, when used as the vehicle of irony, is the worst kind of cen- sure. The discovery of truth ought to be the only object of philosophical discussion. There are, doubtless, many errors in my bumble attempts at chemical analysis; but unless Dr. Pearson points out those errors, or brings for- ward new facts connected with my inquiries, I confess that Thad much rather he would not again honour them with his notice. “ Quicquid id est, timeo Danaos et dona ferentes.” T remain, sir, &c. &c. Russel Square, Feb. 21, 1812. ALEX. MArRceErT. KX. Description of the Diacatoptron. Communicated vy Dr, Grpzes, of Bath. V anrous optical instruments have been applied to the purposes of drawing and copying, and have been carried to a great degree of perfection. The Camera obscura, the Delineator, and Camera lucida, have severally been justly: celel rated for the facility of tracing outlines, and the rules of perspective have been correctly illustrated by these re- presentations of natural objects on a plain surface, The great simplicity of the instrument now about to be described, may entitle it to rank among the most usettil of the kind, as, to the advantage of its simple structure and applicability without straining the eyes, it adds a deurce of truth not to be exceeded. Without the aid of additional reflecting surfaces, this instrument represents its objects as an ordinary mirror, at the same time that it allows suti- cient transmitted light to pass for the guidance of the hand behind it, Thus, by a very little management, both the hand ‘ oa 2 128 The Diacatoptron. hand directing the pencil, and the obje ect to be traced, may — be equally well defined and. clear. Aleta, advantage pos- sessed by this apparatus is, that very little light is lost, as is the case where many glasses intervene between the object and its representation, The application is.also immediately obvious to the most éareless observer. -Take a perfectly clear piece of glass, a foot, square, well po- lished and quite even, and parallel throughout ; ; place this in a trame (PI. UI. fig. 1.) about one inch and a balf wide, and one inch thick, and instead of wood at the bottom of the frame place a brass wire or narrow and thin plate which will bold the three sides together, and prevent the glass from falling out, as it must rest on the wire or plate, ‘hich should be fastened tight to the feet of the frame. The feet must be exactly at right angles with the frame, so that when the plate is placed upon aw eyen table, it will stand perpendicular. In the upper part of the frame at 4, make a long groove, in which insert the brass sight aa indh broad (fig. 7.) having the sinall eye-hole cz this is to be fastened at top by the screw d, which may be screwed up or loosened at pleasure. Divide the frame (fg. 5.) into two equal parts, beginning at the upper part from the groove J, to the bottom of the feet a, or of the brass wire. Divide again the lower part from eé into eight equal parts, and on each side of the’ frame bore holes, taking great care to place them exactly at the eight measured points, A board (fig. 6.) 1s called the table, of the Lrcpriiki of the frame, in which two. brass pins are fastened of such size that they may exactly pass into the holes to raise the table to different heights corresponding with. the holes in’ the frame ; otherwise you cannot magnify or diminish objects correctly according to the size you may wish to obtain. On the opposite side of the table are supports at each cor- ner, so placed that they may be conveniently pushed up or down. The supports pass through two holes in the table, and in each are eight sinall holes of the same size as those in the frame, so that by means of a brass wire under the table it may be kept fast in a horizontal position. The blind (fig. 2.) is made of a piece of woad, bevelled, one foot long, one inch and a half wide, and one aii in iiielee ness. A brass or iron rod is bent in such a manner as to form a square, and the wood serves as a support to it. This frame is then covered with writing paper, which should be of moderate thickness. When you make use of the apparatus, place the object 4 upon a flat table on a level with The Diacatoptron. 129 with the window ; on the right: hand) Jay some: blank; pa~ per, upon which a person may draw; and between the two place the Diacatoptron or transparentyreflecting plate of glass in its frame; place the blind & at right angles with the glass on the right hand, so that the drawing paper may Jie in the broken shade, and a person looking through the glass trom the left side will observe the object exactly de- signed upon the paper. If the figure isnot sufficiently distinct, you may darken the blind by hanging a paper upon it; if it should darken too much, you place ita little further from the glass. It is of much consequence that the proper degree of shade should be thrown upon the paper; for, if it is too dark, you will neither see distinctly the lines of the draw- ing which you copy, nor the point of your pencil: if, on the contrary, it is not sufhciently dark, you will work at random, and the representation will be faint. In copying after this manner you do not make use of any eye hole, becanse the eye is easily kept in the proper direction, as the drawing remains in its appropriate situation ; but in the following experiments, where the objects are diminished or magnified, whether a picture or prospects in perspec- tive, the eye hole must be always used, since it is necessary to look exactly and constantly at the same point of view. The diminishing of an object is effected by raising the height of the table. Since the object placed on the left side of the glass is always represented on the right side, although the surface of the table should not be of an uniform height, it will be found that, if you take a fixed point of view, the object will be diminished the nearer the reflected image approaches to ibis point, and will be magnified as the re- flected and transmitted image is made to recede from the eye. Or rather, the image will appear larger than the ob- ject when it is removed further from the fixed eye than the object itself, and vice versa. This may be seen clearer by fig. 5. The parallel lines 1, 2, 3, 4, 5, 6, 7, 8, represent the different heights of the table. If now the line # were to be diminished, it would be reduced + upon the table at 1, }at 2, 2 at 3, and at 4 t, 48 is shown by the lines of sight where the parallel lines intersect. ‘ Fig. 3. represents the Diacatoptron when the letter B is diminished +; the table with the paper is placed in the fourth hole, . Fig. 4. represents the magnifying of an object when the table is on the left side. _In both cases you must look at the object through the Vol. 39. No. 166. Fel, 1812. I eye 130 Royal Sociely. eye hole which is on the left. By this method of diminish- ing with the Diacatoptron, it is easy to take in prospects and objects in perspective. Make a board (fig. 8.) 24 feet long, and bore two holes six inches from one end of the board at the width of the Diacatoptron, so that the supports of the table may pass through and may be placed upright. | Fasten behind two perpendicular pieces of wood a; and also at the upper part two props which may pass into the holes of the table, into which the feet were before fixed, so that the table may be -ecured both at the top and bottom, and all shaking prevented. Bore holes in the board from c¢ to a, that you may place there the sight-piece e, which is either made of brass or wood, about six inches high, and bas at the top a round brass plate one inch in diameter, in which is the eye hole. When you make a trial of it, fix the paper fast on the table according to fig. 9. Place the Diacatoptron about six or eight inches from it, upon the board, and parallel with the table; the blind, (fig. 10.) which is made of wood, pasteboard, or paper, then covers the space between the Diacatoptron and the table, so that the opening g may be on the right hand: the sight-piece e is then so placed in one of the holes that you may have the desired power of diminishing, taking care that your head may not intervene between the object and the glass, and you may easily draw upon the perpendicular paper the objects diminished. In this way you may witb ease draw plants, and in short all objects, even academy figures, &c., and under circum- stances in which the Camera obscura could not be con- veniently employed. XXI. Proceedings of Learned Societies. ROYAL SOCIETY. Thursday Feb. 6. Tue Society again met, when a short paper by Dr. Wollaston was read on the primitive form of calcareous, bitter, and iron spar. The composition of these three kinds of spar being essentially different, although their primitive form bas hitherto been admitted to be the same, seemed to militate against the truth of the crystallogical : system. Haiiy himself having rather hastily allowed that the angle of the rhomboid of calcareous spar, magnesian spar, and iron spar, being 101° 27', formed an exception to the general principle that a difference of constituent ‘parts produced a difference of form, Dr. W. with his goniometer was induced to examine these spars with greater attention. The Royal Institution. 131 The angle in all of them he found some degrees more than M. Haily ; and also that each had a distinct measure, which in whole numbers may be stated at 105°, 106°, and 107°. Hence he was led to the very important conclusion, that a difference in constituent principles does in every case produce a difference of primitive form; that the exceptions to this general position are entirely owing to errors in our crystal- lographical operations, and that the crystallogical theory 1s move true to nature than even its author had supposed. Feb. 13. A paper by Mr. John Davy, communicated by his brother Mr. Dayy, was read. MM. Gay-Lussac* and Thenard and Mr. Murray have asserted that there is no ac+ tion between gaseous oxide of carbon and oxymuriatic gas or chlorine, when they are exposed to sunshine. Mr. John Davy states in this paper avery different result—that the two gases combine and become condensed to half their yolume, and form a peculiar new elastic fluid possessed of acid pro- perties. He gives an account of the nature ¢nd combina- tions of this substance, which neutralizes four times its vo- lume of-ammonia, and forms with it a peculiar salt; it is not disengaged from ammonia by acetous acid, nor by sulphureous acid, and.it is decomposed by the metals into gaseous oxide of carbon and chlorine, so that its constitu- tion is established both by analytical and synthetical ex- periments. Feb. 20. Another paper by Mr. John Davy was com- municated to the Suciety by Mr. Davy. It related to the combinations of certain metals with chlorine and oxygen, and contained some general views on the theory of definite proportions. The pure combinations of metals with chlorine resemble in many respecis oxides ; they are non-conductors of electricity, many of them are very yolatile, and they form muriates by decomposing water. Mr. John Davy describes two combinations of copper and chlorine, one containing twice as much chlorine as the other. Two of iron and chlorine, one containing balf as much as the other, And two of tin and chlorine, of which the second contains double as much chlorine as the first. Bismuth, antimony, arsenic, zinc, lead, he has been able to combine with chlorine in one proportion only. Between the oxygen in oxides and the chlorine in these combinations, the rate is as 7°5 to 33°6. Many of these combinations with chlorine combine with oils; and Libavius’s liquor, the compound of ghlorine and tin, inflames in acting upon oil of turpentine. As the oxides are soluble in acids, so likewise are these compounds im an acid that they cannot decompose. Corrosive subr jimate forms a particular salt, by combining with muriati¢ 12 acid, 132 . Royal Institution. acid, and there are other analogous substances. Mr. John Davy considered the whole tenour of these experiments as offering confirmations of the fact that oxymuriatic gas, or chlorine, has not yet been decompounded, and that it is 2 solvent and acidifying principle analogous to oxygen. ROYAL INSTITUTION. Mr. Davy’s Lectures on the Elements of Chemical Phitosophy. Mr. Davy delivered his second lecture on Saturday, Feb. the first. He offered somé general views concerning the different modifications of matter, and the active powers en- gaged in the production of the phenomena of nature and of art; he then directed the attention of his audience to heat, or calorific expansion. He considered its important and diversified agencies in the economy of things; and after bi : : ) 5 an elaborate discussion concerning the mechanical and che- mical hypotheses relative to the nature of heat, he concluded by defining the limits of our knowledge on the subject. The expansive energy, or power of repulsion producing heat; and attraction, which is cither gravitative, chemical, or electrical, being one of the active powers belonging to matter, which cannot be separated from it—matter itself may be considered as inert, and all the harmonious arrange- ments in the heavens and the earth may be regarded as flowing from one primary cause, which, as it is intelligent, says Mr. Davy, must be divine. The Professor entered into particular details relative to the effects of heat, its importance, and the laws of its ope- rations. The law of expansion is connected with the equali- zation of the temperature of the globe, the production of winds, and the preservation of animal and vegetable life. He particularly pointed out its application to the ventilation of mines, and the heating and ventilating of rooms. He exhibited a model, illustrating the: manner by which the House of Lords is ventilated and warmed, after a new plan proposed by himself. All the air deteriorated by respiration or combustion in the house, finds a ready exit by means of three copper pipes carried to the roof, and ultimately meeting in a single pipe; the circulation of the air is assisted by a furnace, and by means of ventilators below there is a constant supply of fresh air. Such a plan Mr. Davy con- ceives might be adopted in large drawing-rooms, or in crowded assemblies, with exeellent effect and at a trifling expense, The ee Royal Institution. 133 he formation of elastic fluids arising from the decompo- sition of yegetable and animal matters, proceeds very slowly under pressure: in illustrating this principle Mr. Davy re- ferred to the method lately adopted by M. Appert for pre- Serving meat or vegetables, which consists of enclosing them in close tin plate wast excluded from the contact of ar. Putrefaction cannot proceed unless aériform fluids escape. Mr. Davy conceives that this method may be im- proved by using stronger vessels, and compressing into them ‘a quantity of fixed air, which by its pressure and gm properties would prevent decomposition. in illustrating the effects of combustion, Mr. Davy no- ticed some recent experiments made by Count Rumford, who conceives that the light emitted is proportional to the heat of the flame, and that it may be greatly increased by bringing several parallel wicks near each other. A model of what the Count calls a polyflame light was exhibited. It had four wicks, and the Count states that a lamp of this kind, when properly constructed, will afford as much light as 50 wax candles. Mr. Davy concluded his lecture by explaining the phz- nomena of heat on the mechanical hypothesis of its heing a vibratory motion of the particles of bodies ; and accounted for latent heat, when solids are converted into fluids, by supposing that ‘the motion is employed to make the par- ticles revolve round their axis. He offered this view, merely for the parpose of coniparison with the idea of a specific fluid, the existence of which had often been too confidently advanced by some philosophers. On such a subject it was proper to doubt. The facts of science should be kept per- fectiy distinct from the hypothetical if shoe advanced to explain them. * The truly philosophical inquirer into nature,” says Mr. Davy, ** will not consider it as a disgrace that he is unable to explain every thing. He will feel that truth is more promoted by the minute and accurate examination of a few objects, than by any premature attempts to form grand and universal theories.” Mr. Davy delivered his 3d Lecture on Saturday, Feb. 8, (it was upon chemiéal attraction). After stating that the Most important phenomena of chemical change depend upon the operation of chemical atiraction, and on the agencies of heat, the Professor said it would be necessary to enter into a discussion of the Jaws of attraction, and to illustrate them by experiments. This discussion, he said, might appear minute and tedious; but it was essential, as the subject was the scaffolding by which the edifice of che- T3 niical 134 Royal Institution. mical philosophy was to be erected ; and it should therefor be constructed with care. Mr. Davy mentiotied that che- mical attraction was the power by which different bodies wnite with each other and form new and different substances; that some bodies possess no chemical attraction, and others exert it with different degrees of force; which he illustrated by experiments. He said, the law of combinatton, or the union by chemical attraction, applied to all the different ponde- rable forms of matter; fluids not only produce solid matter, but sometimes likewise gaseous matter; and gases aie condensed into fluids or solids: he instanced the comhi- nation of aquafortis, or nitric acid, with alcohol; also ole- fiant gas and chlorine; likewise sulphureous acid gas with -ammonia; and proved, that as their forms and properties were visibly changed, so likewise were their other sensible qualities. He next referred to his introductory lecture, in which he mentioned that bodies which attract each other unitein definite proportions. This law, said the Professor, is perhaps the most important of our science, and admits of elucidation by a number of experiments, He showed the ‘combinations of barytes and sulphuric acid, chlorine and hydrogen, hydrogen and oxygen; they always unite in definite proportions. Mr. Davy showed also some ex- periments on the combination of muriatic acid gas with ammonia. -This experiment, he said, was mentioned lately in a monthly publication, by Mr. Murray, to prove the presence of water in muriatic acid gas; but the Professor clearly proved, that the presence of water was owing to the hygrometric qualities of the salt, which, when exposed. to the atmosphere for an instant, absorbs Taner directly ; and he showed an experiment, in which, when muriatic gas and ammonia were combined. out of the atmosphere and heated, not an atom of water could be procured frem them. Nature acts by this fixed and immutable Jaw ; and her ar- rangements, said he, however diversified, follow a certain order ; the circumstances of crystallization and definite proportion form the alphabet by which ber chemical Jan- guage is to be deciphered; and it is not composed of nu- merous hieroglyphics, but of a few simple characters. Mr. Davy said, that when two bodies combine in more than one proportion, still their proportions are definite, that the second proportion is always a multiple or a divisor of the first; he instanced mercury, which combines with two proportions of oxygen, the second oxide contains double the quantity of oxygen of the first; also fluoric acid, which combines with ammonia in two proportions, viz. one in yolume, and two in volume; so that the first con- tains Royal Institution. 135 tains half as much alkali as the second: also Dr. Wollas- ton’s experiment of equal weights of carbonate of potash, one fused, the other in its common state; the one contain- ing exactly half as much gas as the other. He said it was in consequence of these abe N NE that whenever com- pounds decompose each other by double affinity or double attraction, there is always merely a new arrangement of their elements, and none of the substances are found either in excess or deficiency: he instanced the salr called nitrate of barytes, which, when mixed with an equal weight of that called sulphate of potash, the potash unites to the nitric acid, and the barytes to the sulphuric acid, and the results are neutral as before. Lt i is, said Mr. Davy, in consequence of this simple law, that whenever one body precipitates another from its solution, the same quantity of one always precipitates the same quantity of the other; and hence the different chemical elements may be expressed by numbers, and all their combinations be represented by the simple ad- dition. of those numbers. Some of those principles, said he, may appear abstruse; but if the proportions be consi-' dered as uniform parts, there can be no difficulty in under- standing the doctrine, On this part of the science, said the Professor, it is necessary to gain distinct ideas ; the doc- trines of chemical afhuity become the instruments for com- paring the results of our experiments, and their deviation from or coincidence with the law of proportion are the tests of their accuracy or imperfection. These doctrines, said he, are capable of being made the guides both to the practical and philosophical chemist; they teach the artist or manufacturer what proportions of substances are neces- sary for his combinations, and enable him to pursue new principles with precision and certainty. Mr. Davy delivered his fourth Lecture on Saturday Feb. 15th. He considered and illustrated the principles. of elec- trical science, as developed by the various combinations of haman ingenuity, and exhibited in the phenomena taking place in the external world. When resin, glass, &c. are rubbed by woollen, they first attract, and after contact repel, light substances. Bodies in such a state aie said to be electrical. This property was first observed in amber, called electron by the Greeks, from which the term electricity is derived. In the 16th century, the researches of Gilbert awakened the attention of philosophers. He considered electricity as exhibiting the attractive and repellent powers of matter, The sagacity of Newton pointed out these powers as pecu- liar forces. 14 Otto 136 Royal Institution. Otto de Guericke, Boyle, Hawkesbee, &c. observed that lainitosne appearances were exhibited by electrified bodies, and for a series of years these novel exhibitions served rather to amuse scientific men than to direct them io the funda- mental principles of electricity. The discevery of Franklin, that lightning depends on the electrical state of the atmosphere, gave a new impulse to this department of knowledge ; anJ the novel facts ob- served by Galvani led to the noble inventions of Volta: ‘* The discoveries to which they led,” says Mr. Davy, “have produced a new order and arrangement of facts, he have to a certain extent connected together mechanical and che- mical science, and exhibited new and unexpected proper- ties of material bodies.”’ The Professor said, that in treating of the subject he should offer views different from any that have been de- veloped by elementary writers on electricity ; but no apology was necessary, the progressive nature of science is one ‘of its noblest characters. As the facts of electricity have mul- tiplied, the theory is more capable of being simplified ; a number of effects formerly supposed to be insulated may be attributed to the same cause. Mr. Davy described the different modes in which elec- tricity is excited, by the contact of bodies, by friction, by heat and changes of their form; and this property seems to belong to all material substances. In the mineral kingdom there are several stones which exhibit electrical effects by being heated, as the tourmaline, boracite, &c. Dry vegetable SUbsteidoes and most crys- tallized bodies produce ‘these phenomena by friction, and the metals by contact." Thus zine made to touch mercury becomes positive, the mercury is negative. The case is the same with other metals, as gold and mercury, copper and mercury, &c. Even fluids and metals produce similar ef- fects, as in the case of liver of sulphur and copper. The electrical effects produced by the contact of different metals are Jess obvious than those connected with luminous appearances; but thev may be perceived by the sensations, or by the cffects produced on the limbs of cold-blooded animals recently deprived of life, as in the celebrated ex- periment of Galvani, who conceived that the effect was produced by a specific subtile Huid; bui the genius of Volta, said Mr. Davy, proved that it was electrical, and gave the demonstration af its principles in one of the noblest igven- tions ever produced by human sagacity. ** Very slight circumstances,” said the Professor, ‘ are sufficient to develop these important powers of matter, and they Se ee ee a Royal Institution. 137 they must he continually in operation in external nature; their grandeur and sublimity are exhibited in the thunder storm; and iu their more tranquil agencies they minister to the order of the terrestrial systeni, and perform slowly and silently important functions in the economy of things.” Electricity, by influence or induction, is different for different substances; and the phenomena of electricity, by influence, exhibit the difference between conductors, \im- perfect conductors, and non-conductors. It is also on the printiple of induction, combined in some cases with that of primary excitation, that the powers of the instruments for accumulating electricity depend, as in the Leyden jar and Voitaic apparatus. Mr. Davy exhibited the powers of the Voltaic instru- ment by some brilliant experiments; medals were fused upon the surface of water and oil of turpentine, and burnt in contact with them. He stated that the maximum of heat was at the positive electrical surface ; and he exhibited an experiment in which, though the most brilliant light was at the negative surface, yet the ignition was infinitely greater at the positive. ? The Professor pointed out the analogy between the Vol- taic battery and the organs of the torpedo and gymnotus. ‘© These mean animals,’”’ said he, * in the bosom of the waters, are found armed with the power that ‘produces lightning and thunder. The more the resources of art are extended, the more analogies to them are found in nature, which offers, as it were, the archetypes of even our happiest and most extraordinary invention.” In speaking of lightning, the Professor said, that rods intended to preserve buildings from its effects should be at Jeast half an inch thick, and coated at top and bottom with platina, to prevent the effects of the weather. They should also terminate, if possible, in a moist stratum of earth. In considering the applications of electrical science to explain natural phenomena, Mr. Davy said, that the brilli- ant and astonishing discoveries made known in this science in the middle of last century, attracted the attention of speculative as well as of experimental philosophers 3 and at- tempts were made to explain all the great and extraordinary phenomena of nature by electrical agencies. ** New prin- ciples,” said he, when first discovered, are always extend- ed too far; the imagination, like the eye, is dazzled by no- vel and brilliant lights, and time is required before objects are seen in their true relations or proper colours.” The natural appearances which may with probability be attributed to, or supposed to be connected with, electrical ‘ effects, 138 Royal Institution. effects, Mr. Davy considers, are water-spouts, some earth- quakes, the Juminous phenomena in storms, and the au- rora borealis or northern lights. Lightning and the thun- der-bolt, said he, were regarded by the ancients as the terrible instruments of the divine vengeance of heaven. The moderns, in developing their causes, have not only disarmed them of their powers, but have removed much of the superstitious fears which they occasioned, and have shown their uses in the ceconomy of things. In the system of nature the obvious effect is often the least important, and that which seems evil, when distinctly considered, is found only to exalt the good and render it more impressive. Poets have given malevolent spirits to direct the storm, and have made it an instrument of vengeance and destruction 3 the philusopher, on the contrary, finds it guided by the ministrations of wisdom, goodness, and intelligence. Mr. Davy’s fifth lecture was delivered on Saturday, Fe- bruary 22d. He illustrated the laws of electricity by the great Voltaic battery, consisting of two thousand double plates of copper and zinc, of four inches square. He show- ed the identity of Voltaic and common electricity, and ex- hibited the decomposing agencies of the battery in a series of beautiful and impressive experiments, many of which were ofa novel kind. © The identity of Voltaic and common electricity is de- monstrated by the spark, the eflects produced on the in- struments employed for exhibiting electrical phenomena, as electrometers, the electrical battery, and on the organs of sensation. When bodies are similarly electrified by Vol- taic as by common electricity, they repel each other; but when dissimilarly, they attract each other. The electrical battery-was charged, and produced a spark by a single con- tact from the Voltaic instrument. The more the powers of the Voltaic battery are investigated, the more correct the original views of Volta appear concerning the identity of Voltaic and common electricity. Mr. Davy could not avoid reprobating the use of the terms Galvanic batteries and Gulvanie electricity. Galvani was only the accidental discoverer of an important fact. Volta ascertained the true cause of the phenomena, and the merit of correct views and of sagacity peculiarly belongs to him, ‘* Where the names of men are to be connected with science,’”’ says Mr. Davy, ‘* truth should be rigorously attended to. Almost the only reward offered in these times to scienufic excel- lence, is fame; and philosophical men should award it with the same justice to the living as to the dead.” Mr. Davy distinguished the chemical agencies of the battery Royal Institution, 139 battery into two kinds—into decompositions by ignition, and polar decompositions. The former are exhibited when compound gases, fluids, or solids are submitted to the aency of the fire excited by electricity. The latter, when alkaline, earthy, or metallic combinations in a fluid staie, or moistened with water, are acted on by the battery. Mr. Davy illustrated these different decompositions by appro- priate experiments. Sulphurated hydrogen and olefiant gas were decomposed in glass globes by the contact of char- coal. These experiments were novel and impressive,—es- pecially that on sulphurated hydrogen gas, the sulphur was precipitated in the form of a dense white cloud. Mr. Davy decomposed soluble and insoluble compounds, as nitre, sulphate of barytes, &c. and in all decompositions he found that alkalies, metals, metallic oxides, and hy- drogen, were uniformly attracted by the negative surface, and repelled by the positive surface ; and that acids, oxy- gen, and chlorine were uniformly attracted by the positive and repelled by the negative surface. It was in conse- quence of the discovery of this law of decomposition, that Mr. Davy decompounded the fixed alkalies, the earths, &c. Mr. Davy explained the transfer or passage of an acid through intervening alkali, or vice versa. Jn such cases the usual operation of chemical affinity appears to be suspended or destroyed by the agencies of Voltaic electricity. Mr. Davy pointed out the application of the chemical polar agencies of electricity, to obtain alkali from the decompo- sition of neutral salts. “ In illustrating the fusing powers of the battery, the Pro- fessor stated, that the German philosophers were said to have converted charcoal into a substance analogous to diamond, by a powerful combination. The only effect which he had been able to witness in trials of this kind, was, that the charcoal became harder at the points of contact. He ex- hibited an experiment in which very fine points of charcoal were electrized in chlorine gas, but there appeared to be no indications of fusion. Electrical decompositions and combinations, there is an reason to believe, are constantly taking place in the osom of the earth and on its surface ; and many of those phenomena, says Mr. Davy, which are attributed by con- tending theorists, cither to the effects of water or fire, may possibly be owing to more refined agencies operating in the course of ages, and producing effects scarcely perceptible in the short period allotted to human observation. The surface of the globe must be influenced by the elec trical changes which occur in the atmosphere, and they may 140 Geological Society. may act an important part in the formation and renovation of soils. To some, says Mr. Davy, these circumstances may ap- pear too minute to be dwelt upon—but nothing which marks intelligence in the ceconomy of Nature, he said, should be passed over without notice. We recognise, with feelings ot pleasure, the combinations of ingenuity in hu- man inventions ; and surely the grand arrangements of Na- ture are worthy of our contemplation ; and if we can feel sentiments of respect and obligation to the contrivers of ar- tificial machinery, limited in purpose, feeble in effect, we cannot refuse the higher tribute of gratitude and devotion to the Author of the mechanism of the universe, where the scheme is designed by infinite wisdom and goodness, and executed by infinite power. Mr. Davy stated, that the chemical attractions of bodies are nearly related to their electrical polarities ; the chemical agents which act most powerfully on each other, produce the most striking electrical phenomena. The powers of all Vol- taic combinations appear to be, in some measure, propor- tional to the chemical attractions of the acting bodies. Mr. Davy stated, that he had been misunderstood rela- tive to the ideas he formerly advanced concerning electrical - and chemical attractions. He did not say that chemical at- tractions were produced by electrical attractions, or vice versa. He conceived that they may be different exhibitions of the same powers of matter, in one case acting upon par- ticles, and in the other upon masses. He wished, however, not to attach much importance to this or any other hypo- thetical notion. Hypothesis, he said, should always be in- duction from experiments, and should be regarded as dan- gerous and unprofitable when it does not lead to new ex- periments. GEOLOGICAL SOCIETY. The annual general meeting of this Society was held on the 7th of February, when the following gentlemen were elected as Officers and Council for the ensuing year. OFFICERS. President. George Bellas Greenough, Esq. M.P. F.R.S. Vice Presidents. William Babington, M.D. F.R.S. Sir Abraham Hume, Bart. M.P. F.R. and L.S. Sir John St. Aubyn, Bart. M.P. F.R.A, and LS. Robert Ferguson, Esq. F.R.S. Treasurers. ee EOeerleercerorrr— Geological Society. 14} Treasurers. William Uaseldine Pepys, Esq. F.R.S. Samuel Solly, Esq. Secretaries. Leonard Horner, Esq. Arthur Aikin, Esq. Foreign Secretary. James Lewis, Count de Bournon, F.R. and L.S. COUNCIL. The Council consists of the Officers of the Society, and of twelve other Ordinary Members. The Ordinary Members for the present year are Alexander Apsley, Esq. James Franck, M.D. The Hon. Henry Grey Ben- | James Laird, M.D. net, M.P. Alexander Marcet, M.D. The Rev. E. J. Burrow. iS kteeys John George Children, Esq. | William Phillips, Esq. F.R. and L.S. Henry Warburton, Esq. Samuel Davis, Esq. F.R.S. [tebe Sir Henry Englefield, Bart. | Samuel Woods, Esq. F.R. and L.S. | Feb. 2ist, 1812. An extract of a letter from Mr. J. R. Jones of Holywell to the President was read, giving an account of a specimen, presented by him to the Society, of supposed native lead, found in a bed of gravel in the neighbourhood of Holywell. An extract of a letter communicated’ by the Hon. Henry Grey Bennet, member of the Geol. Society, was read, de- scribing a submarine voleano which made its appearance on Feb. ist, 1811, off the Island of St. Michael’s in the Azores. The reading of a paper by W. Phillips, Esq. member of the Geol. Society, entitled “ A description of the oxide of tun the production of Cornwall; of the primitive crystal and its modifications, including an attempt to ascertain with precision the admeasurements of its angles mechani- cally, by means of the reflecting goniometer of Dr. Woi- Jaston: to which is added, a series of its crystalline forms and varicties,” was commenced. The native oxide of tin appears to have been found in almost every district of Cornwall, and in the opinion of Mr. Phillips is by no means peculiar to the primitive rocks of that country. Particular crystalline modifications of this substance characterize particular veins. Alluvial depositions of tin of considerable extent and depth have been found in several parts of Cornwall, which appears 142 London Philosophical Society. ; appears to be the only part of Europe in which this metal occurs under these circumstances. The peculiar variety called wood tin has hitherto only been met with in these beds, or stream-works as they are termed in the country ; and these have also furnished the only specimens of gold hitherto found in Cornwall. Among the specimens of tin in the collection of Mr, Philips, it amay be observed occurring in granite, in mica slate, and in ‘other varieties of schist, accompanied by chlorite, tourmaline, calcareous spar, schicfer spar, topaz, calcedony, quartz, fluor spar, and clorophane; yellow cop- per ore, blende, arsenical pyrites, and wolfram. The following Donations were received : Statistical Accounts of the Counties of Cork and Antrim. From the right honourable the Dublin Society. Exotic Mineralogy, Nos. ¥ to 6. From James ‘Sowerby, Esq. the Svat Member of the Geological Society. ° Histoire Naturelle de la France Méridionale, par M.1’ Abbé Giraud Soulavie, 6 vols. Svo. From Dr. Laird, Mem- * berof G.S. Specimens from Northumberland. From the Hon. Henry Grey Bennet, Member of G.S. Specimens from Ireland. From G. B. Greenough, Esq. President of G. S. LONDON PHILOSOPHICAL SOCIETY. The objects of this Society are, according to its Prospec-’ tus, ** those of every man who loves improvement :—to foster genius, to eradicate unphilosophic prejudice, to increase the knowledge of nature, and most, of man ; to destroy, as miuch as possible, that false demuigen of words which has been justly reprobated by Locke and Bacon as the origin of sophistry and misconception ; but, above all, to remove that barrier erected by pedantry against universal knowledge, which has introduced an esprit de corps into philosophy, and rendered it «the territory of a sect rather than the pro- vince of the world.” The means which they adopt to effect these desirable pur- poses are, principally by the production of lectures in every department of philosophy, excepting theology and poli-’ tics; and by a rigorous ea ata examination, in which Truth is the solitary object of devotion, and the inductive system of Bacon the portal to her shrine. This principle. of responsibility imposed on the lecturer we believe to be perfectly original ; and the good resulting from it must-be £on- London Philosophical Society. 143 considerable ; because, while it fosters the vigorous growth of original talent, it lops away the puny excrescences of plagiarism, and the decayed branches of false and unwar- rantable hypothesis. The attention of the Society has, for this month, been chiefly directed to a-brief course of lectures on the Pyra- mids, by Mr. Clarkson, as a prelude to a regular attempt at illustrating the hieroglyphical language. The first object of Mr. C. is to establish the point, that the Pyramids in question were not sepulchres, but temples dedicated to the mysteries of! Solar Fire; and we think he. has succeeded. Indeed, be has brought together such a mass of evidence from every possible source, from Arabian manuscript, Coptic tradition, Hindoo analogy, Greek re- cord, various etymology, and logical deduction; he has condensed such an intense corradiation of proof, as we feel assured will searcely fail, on perusal, to produce a simul- taneous conviction. It is impossible for us to follow him through all the various channels of his research ; it is suf- ficient to say, that part of his lectures was occupied with proving that the Pyramids were not sepulchres, and the re- mainder in arguing that the passages of those singular buildings were devoted to the mysteries of Fire. In pur-. suing the first of these divisions, he rests his conclusions on the following facts:—That the form of the Pyramids was sacred and mysterious; and this he proved by the pyra- midal stones sacrea to the Sun, to Hermes, to the Paphian Venus, and, in modern times, to Bramha. He proceeds from this to trace the connection of this form with the geometrical philosophy of the Egyptians, which descended from them to the Platonists and Pythago- reans; and he imagines it scarcely probable, that a nation imbued with such a veneration for this form as the Egyp- tians were, would have consecrated it to the purpose of shel- tering the body of a single monarch at an enormous ex- pense. If this building were intended to neutralize the che- mnical properties of Nature in this body, as Napoleon was informed, he inquires, how it came that the builders left a hole of a foot in diameter, which perforates the wall of the second pyramid to the central room? If this body was that of Cheops, as it has been affirmed, how was it that Cheops, who despised the theology of the Egyptians, should’spend a whole life in building a mausoleum which belied his own atheistical notions, and confessed his fears to be under the influence of the priests whom he despised? As to the Sar- cophagus, he remarks, that six circumstances mark that it was never intended for atomb. If it could neither be intro- duced 144 London Philosophical Society. duced by the common entrance passage, nor, by the well, how was the body to be deposited within it? Would the attendants convey it in their arms? This was impossible, for a single man can scarcely penetrate one department of the passages—or would they drag it by cords? This was ab-. surd to suppose, when the Egyptian veneration for the dead was called to mind :—and supposing this true, what was the use of so many passages so curiously contrived? Was it to increase the magnificence of the burial ? This could not be; for the passages are in general only three feet and a half high, and only one of them leads to the upper room. Was it for the attendants, who, according to Maillet’s theory, were buried alive with the dead monarch? This was ridicu- lous, for they were confined to a single room :—and for what parpose the two rooms, the five galleries, the platforms, and the well?. And if the niche in the lower room were de- dicated to the mummy of the queen, how came it that the unalterable laws of the Egyptian priests were violated at the same time, and in the same building? How came it that the body in the sarcophagus was placed horizontally, but the body in the queen’s chamber perpendicularly ? The six circumstances, from whence he infers his conclusion, are therefore, 1st, that it was impracticable to bury the body with any the least degree of decency in the sarcophagus ; ed, that the form was not likely to be given to the human body, being half the width of the length; 3d, that it was customary for the Egyptians to hollow the internal cavity of their real sarcophagi in the human shape, and this is not so formed ; 4th, that it was a custom of the Egyptians to decorate them with hieroglyphics, and this is not so adorned 5 stb, that it was likewise a custom of the Egyptians, de- pending upon invariable laws, to place them upright against awall, and this is not so placed :—it may be said, that it has been moved; but itis fixed, and the attempt to dig for trea- sure beneath it, of which the testimonials still remain, proves that it retains its original position ; and 6th, that the sarcophagus consists of two exact cubes ; and this circum- stance, combined with its mystic situation, which is pre- cisely that of one of the foci of an ellipse, supposing an ellipse inscribed on the rectangle ef the floor, substantiates clearly the fact, that its purposes were mysterious. ‘To what purposes then, asked Mr. C. was it applied? to those of lustration, similar to the same vases in Hindostan? We have Tanks of this description, adds Mr. C., in the British Museum, and no one ever imagined that they were in- tended for sepulchres. He then proceeds with a just and sensible argument, drawn from the pyramidal Temples of India. — J Sa eS ee ee London Philosophical Society. 145 India. These temples, as he observes, bear the same exter- nal character, have similar intersal passages, and yet no one ever imagined that these temples were mausoleums. Why then do we induce a different conclusion where the premises are the same? He pursues this argument by producing an extract from a Brahmin tradition, (the Maka Calpa,) which asserts that a Hindoo conqueror was the founder of the Pyramids, that the Sarcophagus was devoted to the myste- ries of the Egyptian Isis, and that the well communicates with immense subterraneous regions,—a circumstance sup- ported by another extract from an Arabian manuséript. We agree, however, with Mr. C. that although it is ex- tremely probable that there was a legitimate entrance to the pyramid of Cheops; yet that, if it rested on the mere Cop- tic tradition recorded in the manuscript described, it would by no means be worthy of implicit credence. We give him credit for sacrificing speculation on this and on other occa- sions to prudence; and we think he has acted wisely in abstaining from the question, when the Pyramid was built? though it is settled by the manuscript at 300 years before the Deluge. With regard to his etymological definition, though we entertain no greater respect for it than Mr. C. considered as affording illustration, we think that the Hebrew word Py- vamido, the revelation of Perfection, or the Bull, is 4 much less strained analogy than Booremiih, the cave of Death. It is curious, however, that the Coptic word Meed, which corresponds with the Greek Mathos, the Jewish M/i- do, signifies in Shanscrit a college of priests, and, when combined with the foregoing part of the word, implies that Fire was the object of their devotion. To proceed: If it be proved that the Pyramids were not sepulchres, there appéars to be no alternative but admitting that they were Sabean temples. But Mr. Clarkson is not satisfied with this position, singly considered, and has therefore entered into a variety of evidence to prove that the passages afforded the original model of initiatory ca- verns. After detailing at some Jength the exoteric and esoteric rites of the ancient nations with a degree of erudi- tion which does him credit, he proceeds to adapt the de- scription of these rites to the peculiar form of the pyramidal recesses. We copy this adaptation, because we consider it extremely ingenious; and though we are ready to admit that it bears a character of abstract speculation, we think, as he has established his main point, that the details de- Vol. 39. No. 166. Feb, 1812. K pending 146 London Philosophical Society. pending on that point may be allowed a little clothing from a clasical imagination. “© It is sufficient for me to observe, on the admission of the foregoing premises, that the room situated in the exact centre of the Pyramid of Cheops, as the Sun is situated in the centre of that starry system ofi which the Pyramid is a symbol, must have been devoted to Osiris. Next, that the situation of the Sarcophagus, exactly placed on one of the foci of an ellipse, and formed of two exact cubes, both of which circumstances were symbols of the same meaning, was dedicatedto the birth of Horus, or Light, one of the gemini who sprung from the egg of Chagas. Now the Gemini were like the Cherubim, the two visible apparitions of the Triune Principle; for, according to Pausanias, the number of the Dioscuri originally corresponded with the Cabiri. And here f cannot but remark, that, according to the Pythagoreans, in two minds, that is, [sis and Osiris, was contained the» great generating Fountain of souls, and that Light and Life sprung from their mystical marriage. Now the Demiurgic principles of nature were represented by cubic stones. “Hence the cubic temple of Mecea, hence the cubic stone of Bubaste. The temple of Solomon was indeed built upon a similar model; it consisted of three exact cubes, two of which were visible, but one invisible, * For myself | have no doubt, although L may not be able to express my ideas so strongly as I feel them, that the Sarcophagus in question was devoted to the higher myste- ries, We know that the Mosaic Tabernacle v was formed upon a similar model ; and that it contained, according to the Rabbins, the Sephy roth, that is, the Spheres or the Sidereal Gates, and the great Decad of the Law written on two stones. Now we are informed by Plutarch and Apuleius, that a Chest containing a golden Ark was used in the my series of Osiris. We learn from Svnesius, that these Arks, according to the priests, contal: ned the Spheres ; those Spheres w hich were sometimes represented by semicircles, and sometimes by cubes ; those Spheres, of which the Dioscuri, the Sephy- roth, the Cherul; im, (and even Proserpine, the object of Eleusinian initiation,) were alike the symbols. We are told, moreover, by Suidas and Eusebins, that Arks were devoted to the mysteries cf Fire, and that they were consi- dered sacred, as well as the triangular form, to the great triple Deity of Eleusinian as well as Eevptian initiation, Bacchus, Proserpine, and Ceres. But tliat nothing may be wanting to ideniuly these Arks withthe triangular ee the London Philosophical Society. 147 the chamber of Osiris-Bacchus, and the Sarcophagus it- self, Pausanias informs us that the Image of Bacchus was found in a Chest which was said to be the gift of Vulcan— that Vulcan of whom the Pyramid was a symbol—that Chest of which the Sarcophagus was a model—that Bacchus to whom the central room was certainly devoted. Finally, to complete the evidence, for it is impossible to turn with- out finding so many proofs as can scarcely be condensed into two Lectures, we hear from Plutarch, that on the third day after Osiris had been deposited in his Ark, during which time he was supposed to have descended into Hades, (the lower hemisphere of the astronomers,) they opened it, and brought forth a Heifer to the people as the Deity restored to life. Now the famous manuscript of Denon represents the exact point of time. The Sarcophagus on which the Heifer rises, is evidently the mystical tomb of Osiris, from the prostrate figure on the side and the triune symbol above ; and it certainly agrees with the figure of the pyramidal Ark. i shall add, by way of corollary to this evidence, that the Hebrew word Pyramido signifies a revelation of the Heifer, ‘as well as of Perfection, or of Fire. «¢ To proceed : The under room, still"bearing the name of the Queen’s chamber, was devoted to the mysteries of Isis 5 for that goddess bore the name of the Queen among the Egyptians. (Diodorus Siculus.) With regard to the niche in this room, it was probably devoted to a statue of Isis Multi- mammiaj or the same triformed goddess exhibited at Eleu- sis. Maillet pretends that the mummy of'a dead queen was deposited here. But I put it to the candour of antiquarians, whether, if I had stated that in the very same monument, and almost at the same time, the Egyptians, so tenacious as they were of invariable customs, so tenacious indeed that, even while they knew as much of the principles of statuary as the Greeks, they sacrificed the truth of proportion and of nature to the standard of monastic prescription,—that these priests should in one instance deposit the body horizontally, and in another perpendicularly, they would not have con- ceived it an insult on their understandings ? . ‘*To return from this digression, however, it must have been in the two first passages that the Aspirant was ter- rified and bewildered by the flickering lights, the groans, ihe cries, and the howlings of dogs. It was there, possibly, that a hundred terrible shadows, disgorged from the mouth of the well or from the grotto beneath, surrounded him with indescribable terrors. Aud here, were I desired to account for the holes in the central room, one of which extends . K 2 the 148 * London Philosophical Society. the outward wall, and the other to the foundations of the Pyramids, I should answer, with very little hesitation, that they were devoted to secret communication, and most likely to inform the assembled priests of the exact moment when the initiate entered the north angle, or thé well. I consider this as a much more satisfactory and plain state- ment than that of Savary, who contends that one of them was intended to convey food to the visionary personages he here confined; for, according to his own. hypothesis, it was scarcely possible to ascend the external wall ; and it is not very probable that a set of priests, tenacious to a refinement of their secrets, should have suffered a basket of provisions to be dangling trom a height of two hundred feet—a mere realization of Mother Bunch’s Tales. But it is the constant feature of a forced hypo- thesis, that some little difficulty is perpetually starting which requires a correcting or a pruning hand. For myself, though I. feel conscious that my powers of research are infinitely inferior to those who have preceded me, yet satis- fied that I have yielded every thing to fact, and nothing to imagination, I am persuaded, that every candid and unpre- judiced mind will submit to the weight of evidence I have ‘adduced, and particularly to that harmony of feature which pervades and characterizes the system which I have endea- youred to erect with comparatively feeble powers, but with unremitting patience of investigation. Even the narrow communication between the first and second gallery, which has confounded and perplexed the opposite theorists, and certainly put them to their last shifts of explanation, is to me a matter of triumph and of aid. For [ have only to read the ordinary descriptions of travellers, and the cause of it is apparent. We are compelled, they all concur, to strip ourselves at this point, and to crawl upon our bellies like serpents ;—and behold two accredited steps of ancient initiation : for it is notorious that these actions, rendered necessary by the skill of the architect, are symbolical rites, representing at once the fall of man, and his willingness to return to his original simplicity and purity. Indeed, if the analogy were not so sirong as it is, we are not deficient in evidence, drawn from the cave of Trophonius, St. Patrick, &e. which were built upon a similar model, that the narrow- ness of the passage was intended to impress a feeling of : ‘terror on the mystic votary. Proceeding, therefore, by the ‘ same analogical clue, the concession seems as It were ex- ‘ acted from us, that the five platforms-and five galleries were the inferior gates of the great Sidereal Ladder which led London Philosophical Society. , 14g led the initiate to the central Sanctorum of Osiris. The Coptic manuscript says, that there were images of the Stars and the Sun and Moon within—but the arrangement of the ‘passage speaks for itself. I baye before proved that the Sephyroth, with its own gates, was an Egyptian mystery. It remains to observe, that all the ancient temples of which we have record, were built upon an astronomical principle. Of this, the temples of Mecca, of Solomon, of Elephanta, are proofs. Navy, there were pyramidal temples in Chaldea aud Mexico, which were erected on the very principle of the Sidereal Ladder and the Sephyroth. There is nothing, there- fore, overstrained in seeking for it in the Py ‘raids of Eeypt, expressly dedicated io the Universal System. It ~ must be recollecied, however, that the Sidereal Ladder was not always uniformly represented. It was not in the two instances before us; one consisted of concentric circles, the other of steps. We know that the Jewish Sephy roth was sometimes represented by a tree. We know too that the Tree of Knowledge was represented on the same astrono- eal principle by the Oriental nations, and by the Platonists themselves; and this is proved by Evyptian and Mithraie monuments. For instance, they painted it by a Tree with one trunk, with three branches, and seven different kinds of fruit, typifying the Planets, and represented the Fruit of Life by the Sun, and of Death by the Moon. The Rab- bins, indeed, express themselves in the same manner in mysticizing on the branches of the Sephyroth. If then we.re- fer this m0) slicizing theory to the branches of the Pyramidal cavers, we shall find an exact and striking coincidence. «<< As to the magnificent passave which leads to the Solar chamber, I shouldi imagine, from the benches which accoms pany the course of the walls, aud their distinct division into something like the stalls ‘of monastic temples, that it was occupied by the assen:bled College of Priests, who pos- sibly witnessed the efforts and triumphed in the success of the blindfold initiate. The descent of Ulysses and of Or- pheus seem both to allude to ihe jaiter circumstance ; but the curiosity of Orpheus removed the veil. «© Bat however this may have been, there can be lite doubt, that most of the poetical dresaelicg into Heil ongi- nated in the third passage. The deseription of it,singularly coincides with that of Virzi!. ‘There are atethe end of the second gallery, three wavs, the one Icading to Elysium, {the abode of the Sun, according to Bry ant,) the other to the abode of Prose Tpine’ (the Queen’ ’s chamber), and the Jast to Taitarus, that is to the Catacombs, the only Infera of K 3 the 150 Wernerian Natural History Society. the Egyptians. It was here then that three priests were stationed to prevent the intrusion of improper persons, who in the Coptic language were called Caen, a word which the Greeks translated Dogs, and thence the triple-headed Dog Cerberus of the poets. And here, if I may be allowed to speculate on the description of Virgil, that beneath an over- shadowing rock, to the left, the city of Tartarus was placed at the entrance of these ways, |] should place the dungeon of the Temple in the grotto beneath ; for there is little doubt that the Tartarus of the poets originated in the penances of the Priests, exemplified either in the persons of their re- fractory satellites, or on those of initiates who had violated their oaths. Hence arose the stories of Sisyphus, Ixion, of the Danaides, victims, as it would appear, cond+mned to draw water, to raise stones, or to move the wheels of ma- chinery.” Mr. Clarkson then proceeds with an interesting descrip- tion of Elysium, which he contends was the garden of the Monastic College ; detailing rather at large the mystic dra- mas that were there represented, and ending with a learned and curious argument on the Origin and Effects of Drama~ tic Representation. _ Upon the whole, we take our leave of Mr. C. with con- siderable feelings of respect. We have derived at once pleasure and information from his lectures, and we sympa- thize cordially with his future objects. WERNERIAN NATURAL HISTORY SOCIETY. At the first winter meeting of this Society, an interesting communication from Dr. Artbur Edmondstone was read, concerning the Larus parasiticus, or Arctic Gull. Owing to the remote situation of the haunts of this gull, its history and manners have hitherto been little known. Dr. Ed- mondstone has now illustrated them. He has observed two kinds of arctic gulls in.the Shetland islands; the common sort, with the breast and belly of a mouse colour; and an- other sort with the breast and belly pure white. Each kind keeps together; aud the white is a larger and heavier bird, but less bold than the other. The Doctor is therefore in- clined to consider these not merely as varieties, but as di- stinct species. ; At the same meeting, Professor Jameson read to the So- ciety a short description of several varietics of the precious stone named Zircon, which he had lately discovered im- bedded in sienite, in Galloway. [He also informed the So- en : ‘ciety, Wernerian Natural History Society. 151 ciety, that he had observed in the same rock in Galloway, both the brown and the yellow subspecies of that very rare ore, known to mineralogists by the name of Rutilite or Sphene. At the meeting on the 30th of November last, Professor Jameson read a paper on Granite. He cescribed three principal formations of granite, and two of sienite. Two of the granite formations belong to the primitive class; the third to the transition: and of the sienites, one is primi- tive, and the other transition. He mentioned particularly the appearances that present themselves at the junctions and alternations of the granite and sienite with gneiss and A7/das (which last is probably a newer gneiss), and the relations of these rocks to mica-slate, clay-slate, gray wacke, and gray-wacke slate. The descriptions were illustrated by numerous sections and specimens from Galloway, island of Arran, and other parts of Scotland. The Professor af- terwards gave the natural history of a mew genus of con- camerated fossil shell. In describing this shell, he em- ployed the usual zoological language; but in detailing the other particulars, the method followed was that used in giving the natural history of minerals. At the same meeting the Secretary read a communication from the Rev. Mr. Fleming of Flisk, containing an account of a bed of fossil shells which occurs on the banks of the Frith of Forth near Berrowstounness. The bed is three feet thick, nearly three miles in extent, and is situated about thirty-three feet above the present level of Spring tides. The kinds of shells which compose this extensive bed are still fourd in a recent state in the Frith. At the same meeting, also, Mr. Leach gave a description of a new British species of Bchinus, which he had observed in plenty at Bantry Bay in Ircland, aud which he proposed to call E. lithophagus, from the circumstance of its forming a smail hollow for itsdf in che substance of the submarine rocks. At the meeting on the 14th of December, Professor Jame- son read a short general account of the geognosy of the stewartry of Kirkcudbright. 1t would appear from the Pro- fessor’s description, that the greater portion of this part of Scotland is composed of gray-wacke, gray-wacke slate, and transition slate, with suberdinate beds of transftion por- phyry, twousition greenstone, and fiinty-slate. But three tracts, the first of which contains the mountain of Criffle 5 the second, Cairnsmuir of Dee, &c.; and the third, Loch Doune, are composed of BBA Se signite, sienilic porphyry, . 4 and 152 Vaccination. — and kiilas. The sienite and granite in some places are coe vered by the killas; in other places the granite and sienite rest upon the killas 5 ; and Professor Jameson also observed the killas alternating with beds of granite and sienite, and veins shooting from the granite into the adjacent killas. The granitous rocks, besides felspar, quartz, mica, and hornblende, also contain imbedded rotilite, titanitic iron- ore, and molybdena; and, in rolled masses of a reddish- coloured sienite, crystals and grains of zircon were observed. Professor Jameson also stated several of the characters of the killas, described the magnetic pyrites it contains, noticed its affinity with certain rocks of the transition class, and exhibited specimens to illustrate this affinity. At the same meeting there was read a series of ther- mometrical observations on the temperature of the Gulf stream, by Dr. Manson, of New Galloway: and a descrip- tion of a new craniometer, proposed by Mr. W. E. Leach, iustrated by a sketch. ate oO _ XXII. Intelligence and MRRtaools Articles. VACCINATION. Ox this subject we have lately seen an address by Edward Rigby, £sq. senior surgeon of the Norfolk and Norwich hospital, to the Corp: yration of Guardiaus of the Poor of the city, which presents some facts that cannot be too generally known. This gentleman, while variolous ino- culation was the only method known for lessening the ravages of the stall-pox, was ever ready, not only to inoculate the poor gratuitously, but omitted no opportu- nity, either by writing or by conversation, to promote lis cencral adoption ; but Providence having placed in our hands means of security against that Joathsume disease equally efficacious and much fess exceptionable, namely vaceination, Mr. Rigby has been one of its most strenu- ous advocates, and has exerted himself to root out the small-pox entirely, fron: Norwich and its neighbourhood, After stating some of the measures that he ‘had recom- mended, bat which it would appear had not been suffi- iently Mtended to,—he states, that * the small-pox did disappear in the antumn of 1806: it had seized on all the ns within its reach, and, like a fire, ceased to burn only for want of additional fucl ; hor did it again visit the city till August 1807, when it was introduced in the fol- Jowing w ay t— $6 On the Monday of the Assize- week in that year, Mr. Robinson, Vaccination, 153 Robinson, one of your surgeons, called upon me in the morning, to say he had been to visit a poor woman at the Waggon and Horses, in St. Giles’s-street, who had just been brought thither from the London waggon, and that she was in the eruptive stage of the small-pox, and he was very anxious that I should advise him how she could be dis- posed of. I told him, i feared I had now no power either as a magistrate or as a guardian to direct in such a case, as a late resolution of the court had rescinded the orders, under which, heretofore, patients under such circumstances had been sent to the Infirmary ; but I wished him to apply to Mr. Simpson, the clerk of the court of guardians, to Mr. Lubbock, the mayor’s justice clerk, and to the chief magistrate himself; al! which Mr. Robinson took the trouble of doing, but to no purpose—there was no place to which she could be sent, and she was under the necessity of going through this infectious disease at a public-house, in a pub- lic street, and at a public time when there was a more than usual number of strangers in the city. The consequences were obvious—a person in the public:house caught the disease, from whom it was communicated to another in the neighbourhood, and thence it gradually spread to the several parts of the city, and continued its ravages among the poor to the end of the year 1809; during which time, no Jess a number of deaths from this dreadful disease than TWO HUNDRED AND THREE were recorded in the weekly bills of mortality. The greatest fatality was in 1S08, in soine weeks ten, thirteen, and even fifteen died; and from June 1808 to June 1809 the number of deaths was 171. I ain satisfied that these accounts are correct; and I feel no small gratification in reflecting, that a record so impor- tant to humanity would not have existed, had I not, when mayor, directed the keeper of the bills of mortality to no- tice every death from the small-pox. In a statistical as well as moral view, these facts are highly interesting. I think it likely, as there are few adults in populous places who have not had the small-pox, that this long list of deaths consisted almost entirely of children; and if the common average of deaths trom small-pox, as derived from tables kept for a series of years in London, Paris, Vienna, and other large cities in Europe, be correct, and which is One in six, itis evident, that within this period more than twelve hundred individuals must have had the disease; and the probability of these being children is increased, by this number so strikingly corresponding with the number of births in three years in that class of society liable to the disease, 154 Vaccination. disease, reckoning from the time when the smali-pox dis- appeared at the end of 1806, to the end of 1809, when it again ceased, The annual births im Norwich for the last four years are about nine hundred ; somewhat less than half of this number, or four hundred, probably belong to the lowest or unvaccinating class; which in three years will produce by births about the number of individuals who had the disease at this period, and which, as I before observed, must havé been somewhat more than twelve hundred *. ‘* The moral reflections which necessarily arise from this melancholy detail need not now be insisted upon. _ I will however just observe, that had this patient been fortunately sent to the Infirmary at the time Mr. Robinson called upon me, and which was, { believe, before the disease had reached that stage which renders it infectious, she would not have been i a situation to have communicated it; and the city, in that instance at least, would have been spared the dread- ful visitation to which so many human lives were sacrt- ficed; and had the former wise regulations of this court remained in force, itis sufficiently clear that she would haye been sent thither,” eee ©To Mr. Tilloch. S1r,—In plate xvii. of the 3d vol. of Mr. Parkinson’s valuable ** Organic Remains,’’ is figured at fig, 2. the im- pression of an insect, whose species the author professes himself unable to determine. He will probably therefore not be sorry to be informed through your medium, that it is clearly the impression of the larva of a species of Li- bellula or Dragon Fly ; I conjecture, of 1. quadrimaculata, a figure of which may be seen in the 6th vol. of Remains, tab. xxxvi. fig. 1. and 2.. What Mr. Parkinson terms ‘the sting,” is the intermediate one of the three pointed pro- cesses found at the anus of many of the tribe, but not at allanalogous toasting. The Jegs have not been, as Mr. P. supposes, eight, but six, the usual number in insects. Jan. 27, 1812. I am, sir,/ &c.. &c. C. E. * Admitting this conjecture to be well founded, as more than two years have elapsed since the small-pox was in Norwich, it follows, that at this time there are more than eight hundred children liable to catch the disease, should it again find its way into the city. If also it be true, that this disease is fatal toa sixth of the individuals infected, it is equally clear, that unless some efficient means are adopted to secure the lower classes from the infec- tion, an average annual loss to ou? population of more than sixty persons will be sustained, 7 0 New Process for refining Sugar. 155 To Mr. Tilloch. Siz,—I beg to ask for information of some of your cor- respondents, respecting the cause of an optical phenome- non, for an explanation of which I have in vain looked in books. Surveying lately through a compound microscope at a friend’s, one of the sliders, IT was struck by the figures which I knew to be impressed upon it appearing to my sight to be in relief; and was sti!] more surprised to find, that to my friend, who at my request looked through the microscope, they retained their actual impressed appearance. I then put one of the old penny pieces under the glass, and the letters indented round the margin appeared in relief, while the head seemed as obviously excavated ; yet to my friend’s eye, as well as to that of a lady present, the na- tural appearances only presented themselves, I am not aware of any peculiarity in my visual organs, except that of being in a slight degree short-sighted, which does not seem sufficient to account for the difference. Iam, sir, your most obedient servant, SP. eee > NEW PROCESS FOR REFINING SUGAR. A valuable and simple process has lately been discovered by Edward Howard, Esq. F. R.S. for refining sugar, which promises to be of great advantage. The following is an . outline of the process, but a more detailed account of it may be expected to be published by that gentleman him- self :—** Take brown sugar, sift it through a coarse sieve, then put it lightly into any conical vessel having holes at the bottom (like a coffee machine). Then mix some brown sugar with white syrup, that is, syrup of refined sugar, to the consistency of batter or thick cream, and pour it ently on the top of the sugar in the vessel till the surface 1s CO- vered. The syrup will soon begin to percolate, and leave the surface in a state which will allow more syrup to be poured upon it, which is to be done carefully. The treacle will be found to come out at the bottom, having left the whole mass perfectly white. The first droppings are to be kept apart, as the last will serve to begin another operation. The sugar is now ina pure state, except as to its contain - ing insoluble matter, which may of course be separated by solution in water.—The clarification is to be performed by the best pipe-clay and fuller’s-earth, and the addition of neutral . 156 List of Patents for new Inventions. neutral alum, if lime be previously contained therein ; the whole to be agitated together; and, if expedition be re- quired, it should be heated to the boilmg pot: the fecu- Jencies will then subside. The brown syrup may also be much improved by means of tannin and the above earths. To make the sugar, into snow-white powder, it is only ne- cessary to evaporate the clarified. solution to dryness on a water-bath. To make loaves, the common methods may be resorted to, or the syrup drawn off by exhaustion, or small grains may be made. according to M. Du Trone’s process, with much water, and these grains may be cemented by hot eoncentrated syrup.” Mr. Saumarez will shortly publish a work on the Philo- sophy of Physiology and of Physics; comprehending an examination of the modern systems of philosophy. LIST OF PATENTS FOR NEW INVENTIONS. To Jasper Augustus Kelly, of Kentish Town in the county of Middlesex, engineer and architect, for certain improvements in the construction or formation of arches, and other erections and buildings, which, in respect to the patron of the said invention, they denominate ‘* Moore’s modern Architecture.”’—15th Jan. 1812. To John Taylor the younger, of Chesterfield in the county of Derby, gentleman, for a machine and rods for. cutting, spreading, and preparing wicks for dip candles. — 20th Jan. To John Rafheld, of Edward-street, Cavendish Square, in the county of Middlesex, architect, for an apparatus to be attached to fire stoves, of all descriptions, for rooms, for the removal of cinders and ashes, and the better preventing of dust arising therefrom.—20th Jan. To Jacob Zink, of Glove Road, Mile End, in the county of Middlesex, chemist, for a new method of manufac- turing verdigris, which he denominates British verdigris.— 20th Jan. To George White, of Worthing in the county of Sus- sex, snuith and ironmonger, for a new or improved method of preventing accidents from carriages.— 20th Jan. To Andrew Patten, of Hulme, in the parish of Manches- ter, in the county of Lancaster, iron lignar manufacturer ; ~ and Charles Hankinson, of Hale, in the parish of Bowden, in the county of Chester, tanner, for their improyement in the Meteorological Observations made at Clapton. 157 the tanning of leather by the use of pyrolignus or wood acid. —20th Jan. To George Dodd, of Vauxhall Place, in the county of Surry, engineer, for certain machinery and the application of steam to communicate heat and motion to wines, porter, and other liquids.or fluids, in cellars, storehouses, warehouses, or other places. —23d Jan. To John Beale, of Chad’s Row, in the parish of St. Pan- cras and county of Middlesex, mathematica! instrument and umbrella maker, a for machine or engine for cutting of trunnels and spiles, and various other articles —23¢ Jan. To William Onions, of Paulton, in the county of Somer- set, engineer, for a mew engine or machine which may be wrought by steam or other power.—23d Jan. To Richard Rowland, of the city of Bristol, mathema- tical instrument maker, for certain improvements, in ships’ steering wheels, compasses, and binnacles, and in\ the mode of hghting the same with lamp or candle, by which same light the cabin or other part of the vessel may be lighted ; likewise a method of preserving the candles in hot cli- mates,—23d Jan. To George Babb, of Bordesley, near Birmingham, in the county of Warwick. enginecr, for a new method or prin- ciple of producing files, plane-irons, fire-irons, and other articles. —923d Jan. To Jobn Brown, of Mile End New Town, in the county of Middlesex, stationer, for a pocket on an improved con- struction to be used about the person or otherwise.—25th January. Meteorological Olservations made at Clapton in Hackney, from Jan. 21, to Feb. 20, 1812. Jan. 21.—Fair day, cirri and others. N. Jun. 22.—Clouded and hazy day. N.N.W. Jan, 23.—Lofty and ill-defined cumulative masses of cloud. N.E. Jan. 24.—Lofty cumulative clouds like yesterday: a co- loured phenomenon was described as having been seen at Walthamstow, this evening, about the moon, which from description appears to have been what have called the halo discoides. Jan, 25,—Calm fogey day, with westerly wind. Jan. 26.-Hazy morning; evening fair, though a strong mist prevailed. Jan, 27.—Cloudy and hazy morning; windy eS a unar pT ad 158- Meteorological ‘Observations Junar corona,‘ somewhat coloured, appeared about severi o’clock ; about ten a Aalo of the usual size*. -S.W. Jan. 28.—Clouds and wind from the S.S.W, Jan. 29.—Before sunrise lofty cirri appeared highly co- Joured, which kind of lofty and confused cirrus prevailed all the morning, with latge spreading sheets of cirrostratus, followed in the evening by wind and rain. S.W. Jan. 30.—Hazy morning, followed by clear day and evening showers. S.W. Jan. 31.—Cloudy, calm, hazy day. S.S.W. Feb. 1.—Much cloud all day with haziness. S. Feb. 2.—Fair morning 3 various cirrocumuli and cumuli, followed by high wind, with some rain by night. S.W. Feb. 3.—Fair morning, with lofty cumulative clouds : dark rainy evening. S.W. Feb, 4.—Hazy, with some small rain. S.W. Feb. 5.—Misty, followed by a warm rainy day. S. Feb. 6.—Dall, clouded, unpleasant day. ‘eb. 7.—Fine clear morning and W. wind, with flimsy cirri and cirrocumuli followed by much cloud, increased temperature, and rain at night, with a gale from S.W. Feh, 8.—Fair morning with various clouds followed by @rainy evening. N.E. feb. 9.—Much cloud, in the evening a general obscurity prevailed. W.and N.W. : Feb. 10.—Fine day; much cirrus spread about aloft, in a lower region massy and spreading cumulus; clear night. S. and S.E. Feb. 11,—Clear morning and frosty, afterwards the clouds assumed the cirrocumulative aggregation, and were fol- lowed by increased temperature, and a clouded night. % The ancient writers seem to have been well acquainted with these phe- nomena, but they did not well distinguish the kalo from the corona. “ Existunt exdem corone circa Lunam, et circa nobilia astra ceelo quoque inhzrentia. Circa Sulem arcus apparuit L. Opimio Q. Fabio Coss.. Orbis L. Portio M. Acilio.”—Plin, Hist. Nat. lib. ii. cap. 29. “ Circulus rubri coloris L, Julio P. Rutilio Coss."— Cap. 30. The parhelion and paraselene were also noticed by Pliny. “Et rursus plures soles simul cernuntur, nec supra ipsum nec infra, sed ex obliqué, numquam juxta semel et meridie conspecti in Bosphoro produ- cuntur, qui a matutino tempore duraverunt in occasum.”—Cap. 31. “Lung quoque trinz Cn. Domitio C. Fannio Consulibus apparuére, quas plerique appellaverunt soles nocturnos.” —Cap, 32. Aristotle's descriptions appear more accurate than Pliny’s. “© Thegs Os haw rots igidas, Th F txarsgov xo die sw carina yyverat Reyaouty, x2? wig rugnrsoy nous polowy, &c.—Arist, Meteor. lib, iti. cap. 2. By #2630 I understand radii; and I suppose the author to have meant some such phxnomenon as is described by Virgil as a prognostit of bad’ weather : ** Aut ubi sub lucem densa inter nubila’sese Diversi erumpunt radii,” &c.—Georg. lib, i, 445, Fi che omatle at Clapton. 159 Feb. 12.—Overcast and hazy day; towards night the wind rose and became high with some small rain. Fel. 13.—Qine clear morning, with cirrocumulus and cirrus, while cumuli sailed along lower down: afterwards cumulostratus coatinued to form through the day; bnt the night became clear, and the stars shone bright I observed a very small meteor about eleven o'clock. W. Feb. 14.—Rain set in early, and its streams continued to increase in size and strength all the morning, with rising wind; in the afternoon it cleared, but the wind continued high, and got from S.W. to N.W. The phenomenon of the old moon in the new moon’s horns, as it is called, was very clearly conspicuous this evening. Some common kind of small meteors by night. Fel. 15.—Fine morning; very high up much spreading cirrus passed on gently from N.N.W. breaking out into various forms, in some places giving the idea of fine gra- nulations; in others arranged im beautiful rows of spots, approaching to cirrocumulus, or stretched along in tufts, its fibres verging in different. directions: lower down loose flimsy ctrrocumulus ; and still lower, masses of cumulus and what sailors call scud floated rapidly along in the west wind: by and by cumulostratus formed by inosculation, as it « seemed, and obscured the sky. Feb. 16.—Features of confused cirrus appeared aloft ; cumulus lower; afterwards cumulostratus, and general ob- scurity: rain at night. W. Feb. 17.—Cirrus, &c. followed by wind and rain in the morning; afterwards showers and clear intervals 5 at night very cloudy with rain and very boisterous wind. W. Fel, 18.—Misty overcast morning, and fair day. N.W. Fel. 19,—Misty, overcast and windy; clear night with a few light clouds. S.W. and S. Feb. 20.—Clear morning with much linear cirrus ex- tending north and south; afterwards various cirrus and cirrocumulus in different altitudes. At night a corona* round the moon was sometimes double and coloured, at others single and of various sizes, according to varieties in the intervening cloud. | Five Houses, Clapton, Feb. 21, 1812, Tuomas FORSTER. * At times the corona appeared almost triple. I have said in my paper on Halanes, that a triple corona was seldom seen. I have, however, since writing that, seen several, METEORO- 160 Meteorology. METEOROLOGICAL TABLE, By Mr. Cary, oF THE STRAND, For February 1812. Thermometer. Sars a eel. 1S eight of |S 38 ote a § as the Barom. eae Weathier. 33 Z, bie Inches. sg o ~ Nae ——eee = | | Jan. 27} 43 | 47°} 46°} 29°92 12 {Cloudy 28} 45 | 48 | 40 ‘60 17 |Cloudy 29} 36 | 47 | 41 °192 oO Stormy 30} 42 | 48 | 37 °22 1Q {Fair 31] 36 | 46 | 47 ‘78 13. |Fair ‘ Feb. 1} 46 | 47 | 46] ‘59 oO (Small rain Q| 45 | 47 | 492 "52 o |Rain 31 42}48 | 46) °492 4 |Cloudy 41 47 | 47 | 47 hy i 7 |Cloudy 5| 47 | 47 | 46 *45 o {Rain 6| 46 | 46 | 49 °62 0 {Cloudy 7\ 34 | 47 | 40 °52 6 {Fair 8} 38 | 48 | 40 ay fe) , 0 Rain g| 42 | 43 | 40 “92 0 |Foggy 10} 40 | 46 | 33 82 10. |Fair 11] 32 | 46 | 40 °72 95 |Fair 12} 40 | 50 | 42 *36 oO. |Showery 13| 40 | 46 |} 33 “56 a1 {Fair 14) 40 | 48 | 4) *30 O |Stormy 15| 40 | 47 | 43 *60 10 ‘Showery 16] 42 | 50 | 48 “63 30. '!Cloudy. 17| 50 | 52 | 43 *33 O |Stormy 18} 43 | 53 | 40 90 98 {Fair 19] 45 | 54 | 43 | 30°03 27. |Cloudy 20| 38 |} 56 | 47 | 29°90 30. =|Fair 21} 47 | 56 | 46 ‘67 28 {Cloudy 22} 46 | 55 | 43 “46 0 (Storms with 23} 44 | 52 | 40 °45 40 {Fair [thunder 24| 33 | 43 | 33 "62 18 |Fair 25| 40 | 44 | 35 *38 oO |Rain 26| 32 | 42 | 33 °56 25 {Fair N.B. The Barometer’s height is taken at one o'clock, a ERRATA in our last Number. Page 8, line 15, for 23°read 12°. Page 16, line 48, for O’ read 12, Page 18, line 26, for ‘0011 read ‘011, [ 161 j &, and in two instances for 9. Though the five flats would seem to indicate D, as the t i * For the convenience of printing, ! have taken the liberty of substituting the old English capital () for the $ with curved points for the Semi- tone medius = 47% + f + 4min our Sth plage in vol. xxviii and was so written jn the copy; and the old English small (# ) for the scrip capital S a the Semitone minor = 362 + f + 3m in the Table, and inthe copy.—~ DITOR. Key On Douzxeaves, or Musical Scales with twelve Notes. 415 Key major, in this case, yet it will appear, on counting up from D, that many of the intervals are false above that note, in this arrangement of the Douzeave. Mr. Liston denominates that the original Scale (p. 28), which the twelve finger-keys give on his Organ, without the use of any pedal, viz. I ee Wa ae pee amy I View? all Vee CC: D f° FF “Fs “G.Ge ABB c Be SR ar So eg Sa eS | coe! oS i $ + + = + 4 3 l Bee 1 Rel: ee) kes ales ah dpy hg gl Wherein, when compared with the last Scale, we have, instead of the minor Second jn the first line, the redundant Unjson ; instead of the 5th we have the IV, and instead of the minor sixth the Redundant Fifth, or Diesis-defective minor Sixth. The second line shows, that three sharps and two flats occur in this original scale. The third shows the intervals between the several half notes, as they are yulgarly called, in. Chromatic Elements, where 7S + 39 + 2\=VIII, as betore; the fourth shows the ratios; and the fifth, the order of the two tempered douzeave Elements Land! mentioned jn the note p. 375, and where 7L + 5] = VIII, as before. The following Tables, will show the consonances that can be taken érue, in the Douzeaves last mentioned,. either Perfect or Tempered, and the Wolves or false notes which eat for the want of additional notes, beyond the num- er 12. me: ges Be main nk a Sp Ags rp aed A TABLE OF TRUE CONSONANCES. . » & © Hi a Ee Re Reeularl Bas Regular) Bs : Perfect. Terinerre | 2 5 Perfect. Pecuecdi AS | As oO | 5 aI] S 1] V4S+eSe4 31 4L+43] 2| 8 LE lfaV 48405425) 4L441 Il) S+ g — 6 5S+25+ 2|5L+3! Il} S+ 5 L+ 1] VI [5S --2% +23] 5L+4! 3 \2S+ eL+ | 7 6S+ &+3°|—— IIT |\2S4+ S4+45)eL+4 al 7 \6S+25+2 | 6L+41 (4138+ S+\/sL + 2 V1li6S+35+2 |6L+4+5l IV /3S425-+9|3L+ 31 8 179425 +25|7L+41 5 \4S+ S+s4L+ el | Vill 7$+-35+23| 7L+5) Dd4 A TABLE 416 Scales of the Temple and Foundling- Hospital Organs. A TABLE OF WOLVES, OR RESULTING TEMPERED CONSONANCES. Douzeave Conso- Bass and Treble Notes. i nances, 2 |CCx, EbE, FFs, GGx, and BbB . 1 II |Cx Eb. afta Se FD ads a «nizhs bain cide ere ate $8 |Eb Fx, FGs, and Bb cx ......a0-ce: L+2l IILiCx F, Fx bb, Gsc, and Beb ........| 3L 4+ 1 ee A eo Pee 2L +31 5 ICFx, DGx, EbA, FB, Gex, and Beb} 3L +31 Iv ICxG, EBb, Fxc, GH, Aeb, and BF | 4L+ 21 V Geb WE Meet fee renege io eS Lae ee 6 ICGx, EbB, Fex, and Bots oo emee ce 4b an VIIC=Be, Faeb) Geb 2 Ok 28)... eee ot 7 IRbcK, and Buel 2, ee a ee VII |Cxc, Eeb, Fxf, Gre, and : Bbb . | 7L + 4) In the above Tables, where two consonances are linked together, only one of these can be tuned or taken on a douzeave Instrument, and they are only inserted here, for explaining the effects of different modes of tuning these notes, which so frequently require to be changed, in the taking of chords and in modulating. The 2nds in the first line in the last Table, are not in reality Wolves, because | is the proper value of a sharp or a flat, in Tempered Sy- stems, but are inserted to show, that they differ from L the minor Second, The Quatorzeave Scale of 14 Notes, on the Inner Tem- ple Organ, effected by two divided finger- -keys, is as fol- Jows; viz. C Cx D DeEb E F Fe G GeAb A Bb Bc S S§ st ¢« 8 'S*S°S 6 % gs S e558 ape as aR RE a ee a ie: ee Here the Octave in perfect Intervals, consists of 55 + 35 + 45 + 2, as in the second line, and since g +2 =S, this is equivalent to 7S + 32° 4+ 23, as in the doligeave scale above. In the third line the elements of a regularly Tempered Scale on this Instrument are shown, the octave consisting of 5L + 71+ 2d; and since the minor Limma + Tam sorry to be obliged to substitute the small Greek epsilon (¢ (<) for the scrip capital E, used for the Enharmonic Diesis 212 + 2m in the Table, Plate V in vol. xxviii. and in the copy.—Ep1r,. F an y ~ On the Scales of Christchurch and Russel’s Organs. 417 and Diesis make the major Limma in all such scales, or 1+d=L; wehave 7L+5I=VIII, as in the douzeave above. - The Siexave Scale of 16 Notes, on the Foundling Hos- pital Organ, effected by moving a stop sideways by the hand, is as follows; viz. C CxDb D Dx Eb E FFxG Gx Ab A AxBb Be SeSs3 -s8S$eS8et8D@e95S85 Pepi 1) ote NB ds a, Goad 0 SB, ed Here the Octave in perfect Intervals, consists of 4S + A> +4354 92+ 9G; andsincee 5 +@=Sands+:2=S, this equation reduces to 78 +3 + 28, as before. The regularly Tempered Octave in this case, consists of 3L +- gl + 4d; and since |] + d=L, this becomes 7L + 5] = VIII, as above. The Diaseptave Scale of 17 Notest, on the Christchurch Organ, in Surry Road, erected by Mr. Thomas Elliot, in May, 1812, under Mr. Hawke’s Patent, effected by two Pedals; or, on the Piano Fortes now exhibiting by Mr. Bill, at No. 75, in Newman-street, is as follows, viz. C Cx Db D Dx Eb E F FxGb G GxAb A AxBb Be SeS8-« $SSeQD82-53 SESS ed Ad Aedge Td OOTP ad oe TB Here the Octave in perfect Intervals, consists of 2S + 65+ 45 + 2¢+ 3@; and which, since 35 = 35 + 3g, and 2S = 23 + 2%, becomes 78 + 35 + 28, as before. The regularly Tempered Intervals here are, 2L + 10] + 5d in the Octave ; which, since 5L= 5] + 5d, becomes 7L. + 5] as before. : The. Dixneufave Scale of 19 Notes, on an Organ which Mr. Russell senior, made about the year 1780 (see Dr. Kemp’s Musical Magazine, vol. i. p. 170 and !88,and Mr, J. Marsh’s Theory vf Harmonics, p. 18), is as follows, viz. C CxDb D DxEb E ExF FxGb G GxAb A AxBb Bob c Se@e5>3 -§ -@S5eHU3 « $5@5E9 Oe ee de eee ed) Td Ak ad Here 8 + 45 + 2% + 5G = VIII; and since 5S = 53 + 5@, and 29S = 2° + 2, we have 7S + 35) + 23, as before. Also 12) + 74 = VIII, and since 7L = 7] + 7d, we have 7L + 51, as before. + Mr. Kirkman is said to have made Instruments with 17 notes, before the year 1790, see Dr. Kemp's Musical Magazine, vol, i. p.134; and the late Mr. Charles Clagget also did the same. The 418 On the Scales of Clagget’s and Loeschman’s Organ, &e. The Vingtunave Scale of 21 Notes, on Dr. Robert Smith’s Harpsichords, made by Mr. Kirkman about the year 1758, effected by moving 6 stops sideways by the hands, (see Dr. Smith’s “ Harmonics,’ 2nd Eait. p. 186,) is as fol- lows, viz. ~~ ee rr C CxDb D DvEb EFb ExF FxGb G GxAb A Sess - Ge 1 GSE HS ¢ SH Tedge ho 2 iedeua 8 tod. ded ie AxBb )Beb. Bee Se es GT Gotaeg Here 65 + 49 + 234 4¢ +5e@ =VIII, and since 35 = 35 + 3g, 2S = 23 + 2%, and 2S = 20 + % + 2g, the above equation reduces to 7S + 34) + 23 = VIII, as before. Also, 101 + 9d + 21 = VIII, and since d+ 0 =1 we have 121 = 7d, as for the 19 Notes above; or, since 1+4-d = L, we have 7L + 5] = VIII far-12 Notes, as before. ‘The Vingtduxave Scale of #2 Notes, on the Teliochordan Harpsichord in the Royal Library at Buckingham- House, made by Mr. Charles Clagget in 1790, effected by two Pedals, acting on movable Bridges, is as follows, viz. C.GxDb D DxEb EFb EsF FaGb FexG a tre Be Boe 8 ED, a Ce ee Cue to Ned edie ae. de hot a GxAb A AxBb Bceb Be «& $$ @e Se ste rs ae I (a ME eT Here 53 + 49 + 304+ 5¢+5@= VIII, and since 26= 25 + 26, 2S = 23 + %, and 3S = 33 + 3e | 3@, we have 7S + 35 + 23, as before. Also, 9] + 10d +. 33 = VIII, and since 4L = 41 +. 4d; and 3L= Gd + 3), we have 7L + 5! =VIII, as in the Douzeave. The Vingtquatreave Scale of 24 Notes, on the Patent Harmonic Piano Forte and Organ invented by Mr. David Loeschman in 1809, now exhibiting at his house, No. 82, Newman-street, effected by six Pedals, is as follows, viz. C GsDb GxxD De Eb EFb Ex F Fax Gh Fax G 5 @ © #)8 & Sedo Se? i.e 8 Lod Bd eee de te oa Gx Ab Oa Loeschman’s and Liston’s Organs. 419 Gx Ab ABbb AxBb Beeb Bie me verted “@ iS este: eet sa CR ca aie abe od Here 35 + 4% + 504 7e + 5@ =VIII, and since 25= 63 +2, and 5S=50 +5 +5@, we have 7S+4+35 + 23 = VIII, as before. Also, 71 + ied + 53 = VIII, and since 2L = al + ed, and 5L= i0d + 53, we have 7L+ 51 = VIII, as before. The Cinguanteneufave Scale of 59 Notes, on the Patent Euharmonic Organ invented by the Rev. Henry Liston, im 1810, and made by Messrs. Flight and Robson, in 1812, now exhibiting at their house, No. 101, in St. Martin’s Lane, effected by 11 Pedals, is as follows, viz. C C’ C’* Cw Db C’e D’b Cae D* C’xe D D’ { ew 20's ue er CARR Ae ee O 11 36 47 #57 58 68 83 93 94 104115 Dx Eb D's Eb E’b E Fb E’ Fb Fb E'x RE REI AT Ie HEE al BE 140 i150 151 161 172 197 207 208 218 229 233 Ex F Ee FP Fx Fe Gb Fx Gb Fee 1 Gstto got) 8 ue oe) ef 1744 254 255 265 290 301 311 312 322 337 G Fixx G G’ Gs Ab Ge Ab Ab A { ee aR Rte A iia eee he 347 348 358 369 304 404 405 415 4296 451 A’ Bob Bébb A's» Aw Bo A’ Bie B B { ge Cpe!) Ge ae 48h eo 462 472 483 487 498 508 509 5139 544 555 Oy Bb Ch Ber 2 By Re SO 565 566 576 591 601 602 612 Here 71 +374 13c+2°@+2 +! 1E=VITI, and because 5{ + 6g + 11E = 39 + 13c + 27, the above equation be- gomes 12° + 20@ + 223, as in the Table of Intervals at page 276 of vol. xxxvii; and also, since 7S = 7! + 21g + 142.3 = 39 + Oc — 35, and 25 = 4c + 9G + SB, we have 78 + 3 + 2 = VIII, as above. In the thir line the number of schismas or Es, answering (in my Notation) to each of Mr. Liston’s Notes, are given; these, by some + Iam obliged to substitute the old English small c (¢) for the f¢ with a dash across pap ew for the semi-comma major 4% + f in vel. xxviii. Plate V, and in the copy.—Epiroa. h ave 420 On the Scale and luning of the Rev. Mr.Liston’s Organ. have been called my Artificial Commas, in imitation of Mercator’s artificial commas 53 in the Octave, (Holder’s Treatise, Ist Edit. p. 79), the reason or derivation of whose. curious approximate common-measure to Intervals, was unknown, I believe, until | had expressed and arranged Intervals in the notation by ¥,; f and m, when the number of ms to any note in such new Notation, was found to agrce exactly with Mercator’s numbers. With respect to these and all other artificial commas, it is to be observed, that they form a sort of musical (whole number) logarithms, having the least Interval as their wnit, and will, by addition and subtraction, eorrectly show the values and relations of intervals larger than their unit, and between which no dif- ferences occur smaller than their unit ; all smaller intervals, and some of those very near to the value of the unit, are however erroneously expressed by them: but in perfect Harmony, as I have before observed (vol. xxxvii. p. 274), no less Interyal than = occurs, and therefore they may be safely used, in all its calculations. In the Table which [ gave in vol. xxxvii. p. 276, of the Notes on Mr. Liston’s former Instrument, nine of the above notes aré omitted, viz. f = £ p B’bb 9 S, 18 Fob 4 & 8 Bob 9 23 17 Pe, 4 AIO 17 Exe 7 16. 13 Cx? 4.4 Pgs 7) 15 19 Cex 2... 2° 2 Fb. 4° (12 And the 10 following were: inserted unnecessarily in that Table, on account of there being no shades to produce these notes, as being foand unnecessary in the widest range of modulation; viz. Bx, C’b, B‘b, A‘, G'x, Go; F’, E’, D*‘» and D'b, by which the scale for the new Organ is re- duced to 59 Notes, as above. The shades by which the alteration of a comma is pro- duced in the sounds of the Pipes, as explained in vol. xxxvil. p- 328, and in Mr, Liston’s Essay, p. 45, not being able to raise their sounds, only to depress their pitch, one, or two commas, the Pipes in Mr. L.’s Organ, are necessarily tuned to the acute notes ; a standard Pipe, a major comma higher than Concert Pitch, heing used for. pitching C’f, from whence the Tuning is conducted upwards, thus, viz. t Or, having the pitch of C, we may tune upwarts CyGyDy A’ y FB’, and then downwards F’ ),, C’ whichisthe proper pitch for com mencing Tuning, as Mr. L, shows, p. 44. , Cc’ On the Scale and tuning of the Rev. Mr. Liston’s Organ: 421. Cyeo Vv D’: then C’ Ill Er Vv B/ y Fx Vv C’x, and Bath A’; then E’ il G's y Ds y Aey E’x; then G’« J), Be y Pee y Cre. Then downwards C’ y, ¥” vy Be ; then ey II A’b heh E’b: then A’b y, D’b 1, Gib y Cbs and’ then A’b yy F’b Vv B’bb; which completes the Tuning of the Pipes. Three Fifths are then tuned downwards by help of the one-comma shades to obtain C, viz. A’ yDyG y © Then C 57; Ey By Fas &c. just as above, except being a comma lower, or without acute accents. In like manner three other Fifths are tuned downwards, by means of the two-comma shades, to obtain C’, viz. Ay D’ ve V C’, Then upwards G’ wp Ps thera ee Wy. * yy Ae: and then A yy) C* yy, E's. Then downwards C* iy 4e3 then G iy E'es and then Cb Vv Fb. Which completes the tuning of the 59 Notes of this Grand harmonic Scale; at the multiplicity of whose Notes, the intelligent student need not be at all alarmed, since the excellent contrivance of Mr. Liston’s Organ, en- ables the whole to come mto play when wanted, through the means of the 12 ordinary finger-keys, and a pedal to be pressed now and then, when the key changes, so as to re- quire the use of notes beyond those twelve that are in the scale at the time and at'others, when certain notes require, altering a comma to perfect the harmony, all of which are marked in numerous examples and pieces of music, in Mr. Liston’s Book, and in other printed Music that he has ready rovided, for those Professors or Amateurs who may honour him by a trial of his Instruments, at Messrs. Flight and Robson’s. / The commendable disposition shown by the ‘people of this: metropolis, for encouraging an extension and improve- -ment of the Musical Scale of Keyed Instruments (tor with Voices and Violins, &c. Mr. Liston’s scale always has and always will be im tise), in the instanees that | have mens tioned above, seems in a particular manner to have alarmed the German Organist Mr. Kollmann, for the fate of his modern. | 422 Kollmann’s Opposition to all the preceding Improvements. modern “ scale of nature,” or 12 sounds only in the Octaves placed at equal distances, on which his ** new Theory” appears entirely built, that he so pompously and incessantly compares with the best writings of British Musicians, to their disadvantage, in his Quarterly Review; which * won- derful compound of twelve Diatonic Chromatic Enhar- monic Scales in one!’’, it is admitted by Mr. K. must be abolished, as the first cotisequerice of the establishment of the © artificial Temperamenis” of Hawkes, Loeschman, and Liston !, and therefore, he takes especial pains to cry them all down as useless and absurd. . What alamentable case! that the progress of Science and Improvement in one of the most delightful of arts, should render the sale less certain, of the voluminous works of this profound Theorist!, who, to the honour, or disgrace rather of the age, broadly asserts, that violins, violoncellos, and voices, ought not to make any difference between Ab and Gx, Db and Cx, &c.!!, but should use, “as nearly equal a temperament} as possible,” or in other words, < follow the (his) true standard scale, on which all modern music depends.” Wot doubting but the scientific and de- monstrable principles advanced in the “‘ Essay on perfect Intonation,” will make their way, confirmed a3 they are in every case, by an appeal to experiment, unimpeded by such antiquated and unphilosophical, not to say interested, op- position, as that I have been alluding to; I remain, sir, Your obliged and very humble servant, 12, Upper Crown-Street, Westminster, Jorn Farey Sen: June 4, 1812. P.S. In conversation a few days ago with Mr. Loesch- + A Temperament as nearly equal as it is possible for the ear to judge of it, results from taking each Fifth a s¢hisma flat, or making the same to cou- sist of 2t + SH, as first mentioned in your 28th volume, p. 65 (see also xxxvi. p. 48). Now, in Mr. Liston’s Scale above described, there are 15 pairs of notes exactly at this distance apart, viz. Cx & A’b, C’® & Ab, C%q & A, D! & Bob, D’x & Bb, EF’ & Ch, Ex &c', Bx & FR & db, Fixx & d', Gk & eb, A’ & f'b, A’e & f, B’ & gb, and B* g*, And 15 pairs of equal temperament Fourths, the complements of the above, as A'b & Cx, Ab & C’x, &c. whose value is 3ST —H or 2552 + 5f + 22m. Twenty-six major Thirds and as many minor Sixths are found in his scale that differ only $¥ from the equal Temperament, and 24 minor Thirds and as many major Sixths that differ only 2¥ from these favourite chords of Mr. Kollmann, but no concords except I, VIII, V and 4, that exactly agree with that Scale. Iam not aware, how far the construction of Mr. L’.s new Organ, admits of trying the notes together, of the above equal temperament Scale, many lo a 4 et O'S ome 2 On Vegetable Wax, &e. 493 man, he informed me, that he could introduce this extended. scale of 59 Notes ona Grand Piano Forte; using movable bridges, for producing the sharpening of one or of two commas, of an improved consiruction, that for such small alterations, would be free of the evils formerly produced by Mr. Clagget’s movable bridges, for changing sharps to flats, &c.; but he has no inclination to embark in such a speculation, unless some Nobleman or Gentleman would order such an Instrument. Mr. Liston informs me, that this was one of the first applications of his principles, that occurred to him; but that on application to Mr. Stoddard, he dissuaded him from thinking of applying them, on any Instrument but the Organ. LXII. On Vegetable Wax, &%c. By R. Mac-Cuitocn, M.D. Woolwich. Communicated by the Author. Ir is now well known that wax is a vegetable product, as well as the result of an animal process in bees and other insects, and the wax of various plants has been successively examined by different chemists. Some slight differences have been observed in the several varietiegs but they are not sufficient to lead us to consider them aMaifferent species ; rather, like the generality of the resins, to be varieties of one common substance. To those already described there is still to be added one, which as far as I know has not yet been noticed. This is a substance held in solution in the essential oil of the rose (the attar of roses) and in that of lavender. I have not searched among the other oils, but it will probably be found in.some of them. All the varieties of these two oils do not however contain it; it is frequently absent in the oil of lavender, alth$ugh but rarely in that of the rose. I am not acquainted with the circumstances under which this variation occurs. When these oils are cooled below a certain point, a portion of this matter is deposited in the form of minute crystals, giving them an appearance some- what similar to that which the fixed oils assume on freezing. On the addition also of alcohol it is separated in the form of minute brilliant scales, and by this method J obtained the portion which I examined. It is equally separated by water, which, if enough be used, dissolves the whole of the oil, and leaves it in a pure state. It is thus that itis col- lected in the pipes of the stills in which rose-water is made, as it is yolatilized in combination with the oil, and precipi- tated 424 On Vegetable Wax, Sc. tated by the action of the water which is condensed in the worm. That with which I made the following experi- ments was procured from lavender; but it seemed to differ in no respect from that which I have procured from the oriental attar of roses, or from the distillation of rose-water. Although I have called it wax in consideration of its vegetable origin, it bears in fact a much nearer resemblance to spermaceti in its general properties. Like that, its feel is greasy, and it is deposited in a crystallized mass at the bottom of the vessel, just as that substance is deposited from the oil of the Cachalot whale. The few comparative experiments which follow, will show its nature more completely. Having but a very small quantity, [ could not conveniently determine its specific gravity ; but it is much lighter than either wax or sperma- ceti, since it swims in sulphuric ether. It crystallizes from its solutions in resplendent scales, and in this property it approaches rather to spermaceti than wax. Its colour 1s white, and its texture flaky. It is fusible at 96°, while wax is only fusible at 120°, and spermaceti at 102°. This account of the fusibilities of wax and spermaceti differing from that commonly received, which states them at 142° and 133° respecigely, it is necessary to say that the mode which I took to Wetermine this temperature, and to which I was compelled by the scantiness of my materials, was by causing them to melt on hot water in which a thermometer was immersed, and noting the heat at the momentof con- gelation. In boiling alcohol it dissolves readily and in as large proportion as spermaceti, more readily and in larger proportion than wax; and it is deposited again on cooling. The three substances seemed, equally soluble in boiling ether, which however dissolves less of them than alcohol does. Its habits with the other compound inflammables, and with the alkalies, resemble those of wax and-spermaceti, and afford no distinction. It is volatilized without apparent change in a tempera- ture considerably lower than spermaceti, and I need not add, that its vapour is equally inflammable. I had no adi- pocire with which to compare it. Considering these circumstances, we may perhaps regard it as a vegetable concrete oil, resembling spermaceti rather than wax, yet differing from it in the characteristic circum- stances of superior volatility and inferior specific gravity, and bearing a relation to essential oils similar to that which spermaceti does to the fat ones. LXIIT. On fants ..} LXIII. Correction of an erroneous Statement in the Account of Mr. Bakewr_y’s Lectures, as to his Originality in exhibiting a Geological Map of England: with Remarks on the Geological Questions, Whether the lower Derbyshire Strata anywhere else appear in England ? ; Were Caverns ormed by subterranean Currents of Water ?; and, How were Mineral Veins opened and filled ?. By Mr. Joun Farey Senior. To Mr. Tilloch. Sir, Waen I first read in your account of Mr. Robert Bakewell’s Lectures, at the Russell Institution, p. 234, of your March Magazine, that Mr. B. exhibited to his auditors, ‘ = Pemmigge i 2 PF 1808. May and June. 480 On the outside brick-walls of other dwell- ing-houses there, for W. Hellyer, Esq. of East Coke, nearyYeovil - 9 -, 7 1810. May and June. 480 910 On the outside brick and rough stone-walls 1809. of his dwelling-house, at that place June. 1040 For the Rev. Joseph Fawcett, of Yeovil. On the outside rough stone-walls of his dwelling- house there = Liens N.B. Mr. Faweett’s house being built the year before, with a view to being stuc- coed, the walls were left rough. Yards.|. 2983 1 hereby 1810. June. _ Cases of Hernia. ° 435 I hereby certify, that the whole of the foregoing two thousand nine hundred and eighty-three square yards of stucco were done with the before-mentioned composition, by me and my men under my directions, and I verily be- lieve it is the cheapest stueco known, and that it will prove very durable, both without doors and within, and that it has given entire satisfaction to the gentlemen who have tried it; and I am now engaged, if I can the ensuing sum- mer, to stucco the outside of one house at Bridport, and another at Yeovil, also the inside of a cottage for labourers that I have just built for Mr. H. B. Way, at Bridport Har- bour. | Tuomas EVERETT, Shipton George, near Bridport, Stone Mason, Bricklayer, and Plasterer. Dorset, April 22,1811. Witness, JAamMEs BuDDEN. LXVI. Cases of Hernia. By Joun Taunton, Esq. To Mr. Tilloch. Sir, Tue following statement of the situation and occur- rence of hernia at different periods of life, has been ob- tained principally from patients relieved by the City of London Truss Society*, and entirely under my own ob- servation within the short period of four years and a half, It appeared to me to form an interesting article of reference, * 'The following are the outlines of the plan of this most excellent Insti- tution. Epiror.—* The objects of this Charity are to provide trusses for every kind of rupture—to furnish bandages and other necessary instru- ments for all cases of prolapsus—to perform every necessary operation— to administer surgical aid promptly—and to supply medicines and atterd- ance during the cure of the patient. «Annual subscribers of one guinea or more to this Charity shall be go- vernors as long as they continue such subscription; and be at liberty to re- commend three patients within the year for single trusses, or one patient for a double, and one for a single truss, for each guinea subscribed. “ Subscribers of ten guineas or upwards shall be governors for life, with the same privileges ; besides being members of all committees. The moneys arising from all life subscriptions are regularly invested in the public funds. “ Mr. Taunton attends at the City Dispensary on Wednesdays and Satur- days, at one o'clock precisely, to ‘examine the cases recommended; or the patients may apply at his house, No, 21, Greville-street, Hatton Garden, any morning Lefore nine u’clock. “ Governors recommending patients who cannot come to London, on ac- count of the distance, are required to send to the surgeon the name, age, and residence of the patient, the exact measure round the body at the part where the hernia is seated, and the particular situation of the hernia, and also to say if it can be returned when the patient lies down in bed,—AIl letters or orders for trusses must be sent post paid.” to 456 Cases of Hernia. to the medical, philosophical, and general reader. As such, J have taken the liberty of transmiting it for publication in your valuable Journal, if it meets your approbation. In 3,176 patients, 2,702 were males, and 474 were fe- males. The situation of the hernia in each case will be seen in the following table : 704 Left inguinal 1,206 Right inguinal 154 Left femoral 130 Right femoral 728 Double inguinal 64)\Double femoral [°° "°°" 8888 ee 172 Umbilical 1,910 inguinal : 2,194 Single. \ 284 femoral 792 Double. 18 Veniral SDP eee compere reasen ee 1900 202 Patients were relieved with trusses, under 10 years of age. _ 160 Ditto between 10 and 20. ditto. 310 Ditto ...... 20 and 30 ditto. 596 Ditto ...... 30 and 40 ditto. 632 Ditto ...... 40 and 50 ditto. 664 Ditto ...... 50 and 60 ditto. 432 Ditto ...... 60 and 70 ditto. 168 Ditto ...... 70 and 80 ditto. 10 Ditto ...... 80 and 90 ditto. 2 Ditto ...... 90 and 100 ditto. 3,176 From the most accurate estimation which I have been enabled to make, I have no doubt of this malady existing in one person in eight through the whole male population of this kingdom, and even ina much greater proportion among the labouring classes of the community, in manu- facturing districts, particularly in those persons who are employed in weaving. 21, Greville Street, Hatton Garden, Joun Ta UNTON, June, 1812. Surgeon to the City of London Truss Society, the City and Finsbury Dis- pensaries, and Lecturer on Anatomy and Surgery, LXVII. On. [ 437 ] LXVII. On the Culture and Preparation of Hemp in Dor- setshire, and on the Growth of Sea Cale*. Dear Sir, As you informed me when you was lately in Dorsetshire, that the Society of Arts, &c, were anxious to obtain information ‘concerning the culture and preparation of hemp in this neighbourhocd, I am induced to send you some accounts thereof. I fear my memorandums on the subject will not be wortliy the notice of the Society, and I should scarcely have ventured to have put pen to paper upon it, if I had not uniformly found, that the persons who are concerned in the growth and management of that article are shy of giving information. If what I have sent should induce persons equal ta the task, to make the needful inquiries in this county, Somerset, Suffolk and Norfolk, (which T believe to be the parts of England where hemp is most cultivated,) and make the culture more generally known than it now seems to be, I shall be much gratified. I hope, if you again visit this neighbourhood, to show you a very fine crop of wheat on the field where you last year saw the persons employed in collecting the male hemp; also another large field of exceeding good wheat, that produced hemp last year, neither of which have had any fresh manure upon them since the hemp was taken from the fields. I have added some observations on the growth of Sea Cale: this useful vegetable, growing naturally on some of the Cliffs near Bridport Harbour, and being one of the most valuable esculent plants that I know, I have found the culture of it in the kitchen garden more easy to manage than has been generally supposed. I have sent different specimens of the seed, and some of the natural soil, for inspection ; and remain, dear sir, ; Your friend and obedient servant, Bridport Harbour, March 1, 1811, H. B. Way. To C. Taylor, M.D. Sec. Account of the Culture and Preparation of Hemp in y Dorsetshire. Hemp is usually sown about the 15th of May, on the best arable Jand, on which about twenty cart loads of good * From Transactions of the Soviety for the Encouragement of Arts, Manu- factures, and Commerce, for 1811. The thanks of the Society were voted to Mr. Way for this communication. rotten 438 On the Culture and Preparation of Hemp rotten dung has been spread, say about a ton to the load = this is well ploughed in, and the ground well ploughed two or three times, and well dragged and harrowed, to get the soil as fine as possible, and about two or two and a half bushels of seed sown to the acre; what produces no seed, called by some male or summer hemp, and by others cinner hemp, is drawn about five or six weeks after the plant comes up, it is at that time in blossom; when drawn, it is tied up in bundles, and carried to some meadow land, and there spread to ripen: when ripe and dry, it is bundled and stacked. What stands for seed has no flower that can be discovered; it is the female hemp, and is generally ripe early in September, when it is drawn, bundled up, and stowed up in the field for the seed to dry and harden, when it is thrashed out in the fields. Most commonly in Dorset the seed is sold on the spot, at from 2s. 6d. to 7s. per bushel ; an acre of hemp produces eighteen or twenty bu- shels. In Somerset they have sometimes thirty bushels of seed to the acre. In the sowing season I bave known 21s. ‘per bushel-paid for seed ; when thrashed the hemp is carried to the meadows, and spread to ripen as the other, and stacked in the same way, to prepare it for sale; it is sent to the houses of the poor in the parishes round which it is raised, to be what is called scaled, that is, each separate stalk of hemp is broken in the hand, and the hemp, which is the outside rind or bark, is stripped off, in which state it is sent to market. The scaling is the employment of old men, women and children, and of the whole of the labouring family in the evening, as in winter they make but poor wages of jt, and one principal inducement for them to do itis, that the woody parts of the hemp make them a fire, but it soon burns out. Complaints are made of a great deal of the hemp being often wasted fram improper management, and want of care in the scaling of it; at the Comptons and Bradford, a good deal more hemp would be raised if they could get it scaled, which they find much difficulty in do- ing; and if it were possible to construct a mill that would swingle it at a moderate expense, on some such plan as the flax swingling mills, and to afford some encouragement to the erecting them, as well as flax swingling mills, it would encourage the growth of both articles materially; an acre of hemp im a good season will produce'l4, 16 or 18 weights, of 32Ibs. to the weight in Dorsetshire ; in Somersetshire they reckon their weight two pounds less, and they some- times get as much as 35 weights to the acre; the price of the in Dorsetshire, and the Growth of Sea-Cale. 439 the weight of hemp is from 16s. to 20s. per weight. The rotation of crops as follow: On ground well manured ..... Hemp. Wheat. Barley or Oats. Clover with the abve. W heat. - Barley or Oats. Ground well manured........ Hemp. But sometimes they dress the ground well for hempever third year. The quantity of bemp sown in Dorset 1 very trifling in comparison to what is sown in Somerset. in the former it is chiefly confined to eight or nine parshes ; whereas very large quantities are raised in Somerset,in the parishes of Misterton, Crewkerne, Hinton, St. Gorge, Lopen, Seavingtons, Ilminster, Stocklinch, Donyatt King- stone, Shipton, Beauchamp, Barington, South Petierton, Martlock, Norton, Chiselborough, Stoke-under-ham,Mont- a-cute, Odcombe, the Chinniocks, the Cokers, the Somp- tons, Bradford, and a great many other parishes Mr. Emanuel Pester, of Preston, near Yeovil, is in the middle of the hemp and flax county, and he can doubtless obtain and give every information that may be wished on the subject, being so extensively engaged in agricultural pursuits himself, and so competent to give that sort of information wanted ; a bounty of 3d. per stone on hemp, and 4d. per stone on flax, was for many years given by Government, but is now discontinued ; it was paid by the Clerk of the Peace for the counties; and as the late Mr. Wallace managed that for the county of Dorset uncommonly well, it is most probable that a very correct return for the county of Dorset could be ob- tained from the office of the Clerk of the Peace for this county, of the quantity raised each vear of both articles, during the continuance of the bounty; also from Devon and Somerset similar returns could be got. There are large quantities of hemp raised in Suffolk, the writer thinks, near St. Edmunds Bury and Stow market, in that county. He has been told they make linen so fine of hemp, as to be worth 5s. and 6s. per yard, and used for shirts in preference to lvish, being considered much more durable and better, so much so, as to induce the !rish to imitate the fabric, and stainp the cloth, Suffolk Hemp. It is also raised in Nor- foik, in the neighbourhood of Lynn and Wisbeach, but it must be watered and prepared im some other way; indeed he is convinced that all the hemp imported from the Baltic #8 prepared differently from the mode used in Dorset and Somerset, 440 On the Culture and Preparation of Hemp Somrset, and must have been swingled before it was sent to te different ports it was shipped at for this country. Thesiving the former bounty on the growth, and increas- ing ion hemp and flax, would encourage the growth ; but if gien on the number of acres sown, the grower, as his grou|d would be in high erder for a crop of turnips and whea after, might be careless ahout his crop of hemp, as the bunty, to be worth notice, must be worth more than the vlue of the seed in common years and the labour of sowie. Hemp in this county and the next is never sown in new ground fresh broke up, but flax always by choice, when fresh ground can be got. Mr. John Pitfield is going to breakup great part of the West Clift at Bridport Harbour, and sw it with flax this season. The writer, while on the subjec of hemp, is led to mention, that when travelling in the yar 1792, in the province of Massachusets near Bos- ton, in North America, was assured that considerable quan- tities of hemp were raised in the township of Sunberry, about ten miles from Boston, and that it was always raised on thesame ground every year, no other crop being sown in their hemp lands, and that it was manured every year, at the rate of about ten tons of manure to the acre of hemp. Respecting seed, he cannot learn that there is any for sale - at Bridport, with the buyers who purchase it up for the growers at the hemp harvest, and he expects that very little can be got from the growers round here. Somersetshire is a more likely place to get it, as he has known some of the hemp farmers to have upwards of an hundred acres of hemp in one season; round this they generally are only in a small way. A change of hemp seed is much wanted in Somer- set and Dorset. Trials have been made two or three times to get it from Russia; but if is not possible to get new seed from the interior early enough in the fall at the shipping ports, and some old seed which has been shipped has not answered the purpose ; if new could have been got, it would as generally have been used for a change, as the new Riga barrel flax seed is by the flax-growers. As the seed sown in Russia was considered a good sample, and its appearance much liked, possibly it might, at a future period, be ob- tained in the fall from Odesea, or some other port on the Black Sea, as it 1s understood that a good deal of hemp shipped at Riga and St. Petersburgh grows much nearer to the Black Sea than the Baltic; or possibly the seed of the Italian hemp raised in the neighbourhood of Bologna, or that of America, might be obtained in time to answer. Perhaps Dorsetshire, and on the Growth of Sea-Cale. 441 Perhaps tares, called by some vetches, might be cleared from the ground early enough for manuring and sowing the ensuing crop of hemp, and vetches might make it worth the farmer’s attention: tu this an objection was stated, which I do not just now remember. On talking with the gentle- man before mentioned, and stating the American practice, with what had passed on it with my neighbours, he said, he had long been persuaded that it was a good practice, and that he had the last season 2 very good crop of hemp on a piece of ground that had hemp the year before, and that he did not Jet the hemp stand for seed, but had it all down at the usual time for drawing the summer or male hemp, and the ground immediately sown with turnips, which were fed- off with sheep, and the ground then slightly manured, and hemp sown again at the proper season; and that he had then, October 27, 1808, a piece of turnips after his hemp, ’ which were worth 6/. per acre. It is to be observed, that the acre here meant is the British acre of one hundred square poles, three hundred and four square yards each. The manure mostly used for hemp is good rotten stable dung, which is much preferred to any other, though lime is frequently used; but manufacturers pretend to assert, (with what foundation I cannot say,) that they can di- stinguish a material difference in the quality of the hemp, where lime has heen used instead of dung, as from lime. they say hemp is more harsh and brittle, and not of such a soft silky quality as where dung has been used. The writer has endeavoured to throw together every thing that occurs to hint on the subject of the culture of hemp, which, from being born and residing great part of his life in a part of the county where it has been extensively cultivated for ages, he has been able to collect; but where it is not very easy to obtain direct information, as both the growers and manufacturers are very shy of giving any, under an idea that it might injure their own interest by assisting to ex- tend the culture to other countries. He believes that his statement may be depended upon; but he is no farmer, and therefore the loose hints thrown together here on the sub- ject may not be so clearly and satisfactorily explained as he could wish; but if they in the smallest degree assist In en- couraging the growth of an article so essential to the wel- ware and prosperity of the kingdom, it will afford him the most heartfelt pleasure. H. B, Way. Vol. 39. No. 170, June 1812. Ff Account 442 On the Culture of Sea-Cale. Account of the Culture of Sea-Cale, or Sea- Kale. Tue mode which I consider the best for the culture of sea-cale, is to draw lines in a very dry soil and dry situation, on ground with a southern aspect, about two feet one way by about eighteen inches the other, and where the lines cross to put in three or four good perfect seeds in a square or triangle, about three inches apart; this may be done any time in November or December in open weather, and it will require no other care afterwards but keeping the ground clear from weeds till the autumn of the following year, when all the plants but one of the finest in each square may be taken up, which if wanted will serve to form other beds set the same distance apart. The ground in the intervals of the plants should be dug in the spring and fall of the year, taking care not to injure the plants. The leaves should be left on the plants till they fall off naturally, which will not in general be sooner than the latter end of November. In the autumn of the second year the same attention should be paid to the plants, and to remove the dead leaves. In the third year, about the middle or latter end of No- vember, when the leaves have been cleared away, and the ground dug, each plant should be covered over close with a tub, pan, a heap of small stones, coarse cinders, or coarse bark, raised about ten or twelve inches over the crown of each plant, and from about the latter end of February to the Jatter end of March the plants will be very fine and fit for use. I prefer that which has been bleached with our round sea-cravel, about the size of large peas or beans, to any other mode whatever. The plants should be cut but once in a year, as cutting it oftener weakens and lessens the size of the plants. If itis not desired to have the plants large, they may Be bleached and cut a year sooner. I have sent a specimen of the sandy soil in which it grows naturally here, as I think the generality of gardeners are too careful, and manure the ground too highly for it. In the month of April last, after cutting my plants, I co- vered the ground all over, at least six inches above the crown of the plants, with this earth: they soon shot up through it, and never looked finer or produced: a larger quantity of good seed than that year. I am thus particular in order to show that this vegetable will succeed as well, if not better in poor ground than in rich, provided the soil be dry, and care taken in the ma- nagement; I speak from long experience, having been well acquainted with the management of this valuable plant from my. Compound of carbonic Oxide and Chlorine. 443 my youth. WhenI cut the sea-cale for use, I immediately draw up the earth with a trowel, so as completely to cover the whole of the plant; this I fancy makes them grow more luxuriantly. This plant, if properly managed, is sue perior to asparagus, and if more is cut than wanted for immediate use, it will keep for some days in a pan of cold water, but of course it cannot be better than when recently cut. It precedes the use of asparagus, being ready for the table in February and March. H.B. Way. LXVIII. On a gaseous Compound of carbonic Oxide and Chlorine. By Joun Davy, Esq. Communicated by Sir Houmenry Davy, Knit. LL.D. Sec. R.S.* Since the influence of electricity and solar light, as che- mical agents, are analogous i many respects, and as the former produces no change in,a mixture of carbonic oxide and chlorine, it was natural to infer the same respecting the latter. MM. Gay Lussac and Thenard assert that this is the case ; they say that they have exposed a mixture of car- bonic oxide and chlorine, under all circumstances, to light, without observing any alteration to take place f. Mr. Mur- ray has made a similar statement f. Having been led to repeat this experiment, from some objections made by the last-mentioned gentleman to the theory of my brother, Sir Humphry Davy, concerning chlorine, I was surprised at witnessing a different result. The mixture exposed, consisted of about equal volumes of chlorine and carbonic oxide; the gasses had been pre- viously dried over mercury by the action of fused muriate of lime, and the exhausted glass globe into which they were introduced from a receiver with suitable stopcocks, was carefully dried. After exposure for about a quarter of ‘ an hour to bright sunshine, the colour of the chlorine had entirely disappeared ; the stopcock belonging to the globe being turned in mercury recently boiled, a considerable ab- sorption took place, just equal to one ha'f the volume of the mixture, and the residual gas possessed properties per- fectly distinct from those belonging either to carbonic oxide or chlorine. Thrown into the atmosphere, it did not fume. Its odour * From the Philosophical Transactions for 1812, part i. + Recherches Physico-Chimiques, tom. ii. p. 150. ¢ Nicholson’s Journal, vol. xxx. p. 227. f2 was 444 On a gaseous Compound was different from that of chlorine, something like that which one might imagine would result from the smell of ehlorine combined with that of ammonia, yet more into- Jerable and suffocating than chlorine itself, and affecting the eyes in a peculiar manner, producing a rapid flow of tears and occasioning painful sensations. [ts chemical properties were not less deeidedly marked than its physical ones, Thrown into a tube full of mercury containing a slip of dry litmus paper, it immediately rendered the paper red. Mixed with ammoniacal gas, a rapid condensation took place, a white salt was formed, and much heat was pro- duced. The compound of this gas and ammonia was a perfect neutral salt, neither changing the colour of turmeric or lit- mus; it had no perceptible odour, but a pungent saline taste ; it was deliquescent, and of course very soluble in water; it was decomposed by the sulphuric, nitric, and phosphoric acids, and also by liquid muriatic acid ; but it sublimed unaltered in the muriatic, carbonic, and sulphu- reous acid gasses, and dissolved without effervescing in acetic acid. The products of its decomposition collected over mercury were found to be the carbonic and muriatic acid gasses; and in the experiment with concentrated sul- pburic acid when accurate results could be obtained, these two gasses were in such proportions, that the volume of the Jatter was double that of the former. I have ascertained by repeated trials, both synthetical and analytical, that the gas condenses four times its volume of the volatile alkali, and I have not been able to combine it with asmaller proportion. © . Tin fused in the gas ina bent glass tube over mercury, by means of a spirit lamp, rapidly decomposed it; the li- quor of Libavius was formed; and when the vessel had cooled, there was not the least change of the volume of the gas perceptible ; but the gas had entirely lost its offen- sive odour, and was merely carbonic oxide; for like car- bonic oxide it burnt with a blue flame, afforded carbonic acid by its combustion, and was not absorbable by water. | The effects of zinc, antimony, and arsenic heated in the gas, were similar to those of tin ; compounds of these me- tals and chlorine were formed, and carbonic oxide in each experiment was liberated equal in volume to the gas deecom- posed. In each instance the action of the metal was quick ; the decomposition being completed in less than ten mi- nutes ; but though the action was rapit, it was likewise tranquil, of carbonic Oxide and Chlorine. 445 tranqail, no explosion ever took place, and none of the me- tals became ignited or inflamed. The action even of potassium heated in the gas was not violent. But from the great absorption of gas, and from the precipitation of carben indicated by the blackness pro- duced, not only the new gas, but likewise the carbonic oxide, appeared to be decomposed. The white oxide of zine heated in the gas quickly decom- posed it, just as readily indeed as the metal itself there was the same formation of the butter of zine; but instead of carbonic oxide being produced, carbonic acid was formed ; and, as usual, there was no change of volume. The protoxide of antimony fused in the gas rapidly de- composed it ; the butter of antimony and the infusible per- oxide were formed; there was no change of the volume of the gas, and the residual gas was carbonic oxide. Sulphur and phosphorus sublimed in the gas, produced no apparent change ; the volume of the gas was unaltered, and its characteristic smell was undiminished. Mixed with hydrogen or oxygen singly, the gas was not inflamed by the electric spark, but mixed with both, in proper proportions, viz. two parts in volume of the former and one of the latter to two parts of the gas, a violent ex- plosion was produced, and the muriatic and carbonic acid gasses were formed. The gas transferred to water was quickly decomposed, the carbonic and muriatic acids were formed, as in the last experiment, and the effect was the same even when light was excluded. From the mode of the formation of the gas and the con- densation that takes place at the time, from the results of the decomposition of its ammoniacal salt, and from the analysis of the gas by metals and metallic oxides, it appears to be a compound of carbonic Oxide aid chlorine condensed into half the space which they occupied separately. And from its combining with ammonia, and forming with this alkali a neutral salt, and from its reddening lit- mus, it seems to be an acid It is similar to acids in other respects ; in decomposing the dry sub-carbonate of ammo- nia, one part in yolume of it expelling two parts of car- bonic acid gas ; and in being itself not expelled from am- monia by any of the acid gasses, or by acetic acid. In- dependent of these circumstances, were power of saturation to be taken as the measure of affinity, the attraction of this gas for ammonia must be allowed to be greater than that of any other substance, for its saturating power !s greater; no Fi3 acid 446 On a gaseous Compound acid condenses so large a proportion of ammonia; carbonic acid only condenses half as much, and yet does not forma neutral salt. The great saturating and neutralizing powers of this gas are singular circumstances, and particularly singular when compared with those of muriatic acid gas. Tn consequence of its being decomposed by water, I have not been able to ascertain whether it is capable of com- bining with the fixed alkalies. Added to solutions of these substances it was absorbed, and carbonic acid gas was dis- engaged by an acid. I have made the experiment on the native carbonates of lime and barytes, but the gas did not decompose these bo- dies. This indeed might be expected, since quick-lime, I find, does not absorb the gas: acubic inch of it, exposed to the action of lime in a tube over mercury, was only di- minished in two days to nine-tenths of a cubic inch, and no further absorption was afterwards observed to take place. But even this circumstance does not demonstrate that the gas has no affinity for lime, and is not capable of combin- ing with it; for on making a similar experiment with car- bonic acid, substituting this gas for the new compound, the result was the same; in two days only about one-tenth of a cubic inch was absorbed. Though the gas is decomposed by water, yet it appears to be absorbed unaltered by common spirits of wine, which contains so considerable a quantity of water; it imparted its peculiar odour to the spirit, and its property of affecting the eyes ; five measures of the spirit condensed sixty mea- sures of the gas. It is also absorbed by the fuming liquor of arsenie, and by the oxymuriate of sulphur. The former appeared to require for saturation ten times its own volume; six measures of the liquor condensed about sixty of the gas. The liquor thus impregnated was thrown into water, and a pretty appearance was produced by the sudden escape of bubbles of the gas: had not its in- tolerable smel] convinced me that the gas was unaltered, I should not have conceived that it could pass through water undecomiposed, I cannot account for the assertion of MM. Gay Lussac and Thenard and of Mr. Murray, that oxymuriatic gas does not, when under the influence of light, exert any ac- tion on carbonic oxide: I was inclined at first to suppose that the difference between -their results and mine, might be owing to their not having exposed the gasses together to bright sunshine; but T have been obliged to ee idea, of carbonic Oxide and Chlorine. 447 idea, since I have found that bright sunshine is not essen- tial, and that the combination 1s produced in less than twelve hours by the indirect solar rays, light alone being necessary. The formation of the new gas may be very readily wit- nessed, by making a mixture of dry carbonic oxide and chlo- rine in a glass tube over mercury: if light be excluded, the chlorine will be absorbed by the mercury, the carbonic oxide alone remaining ; but if bright sunshine be immediately ad- mitted when the mixture first is made, a rapid ascension of the mercury will take place, aud in less than a minute the ‘colour of the chlorine will be destroyed, and in about ten minutes the condensation will have ceased, and the com- bination of the two gasses will be complete. It is requisite that the gasses should be dried for forming this compound; if this precaution is neglected, the new gas will be far from pure; it will contain a considerable admixture of the carbonic and muriatic acid gasses, which are produced in consequence of the decomposition of hy- grometrical water. Indeed there is considerable difficulty in procuring the new gas tolerably pure ; a good air pump is ‘required, and perfectly tight stopcocks, and dry gasses, and dry vessels. I have endeavoured to procure the gas, by passing a mix- ture of carbonic oxide and chlorine through an earthenware tube heated to redness ; but without success. The specific gravity of the gas may be inferred from the specific gravities of its constituent parts jointly with the condensation that takes place at their union. According to Cruickshank, 100 cubic inches of carbonic oxide weigh 29°6 grains, and according to Sir Humphry Davy, 100 of chlorine are equal to 76°37 grains: dence, as equal volumes of these gasses combine, and become so condensed as to occupy only half the space they before filled, it follows that 100 cubic inches of the new compound gas are equal to 105°97 grains. Thus this gas exceeds most others as much in its density as it does in its saturating power. To ascertain whether chlorine bas a stronger affinity for hydrogen than for carbonic oxide, I exposed a mixture of the three gasses in equal volumes to light. Both the new compound and muriatic acid gas were formed, and the affi- nities were so nicely balanced, that the chlorine was nearly equally divided between them. And tbat the attraction of chlorine tor both these gasses is nearly the same, appears to be confirmed by muriatic acid not being decomposed by car- banic oxide, or the new gas by hydrogen. : . Fi“: The 448 New Tables for finding the Deviation of a Siar The chlorine and carbonic oxide are, it is evident from# these last facts, united by strong attractions ; and as the pro- perties of the substance as a peculiar compound are well characterized, it will be necessary to designate it by some simple name. I venture to propose that of phosgene, or phosgene gas; from ws, light, and yivouat, to produce, which signifies formed by light; and as yet no other mode of producing it has been discovered. I have exposed mixtures consisting of different propor- tions of chlorine and carbonie acid to light; but have ob- tained no new compound. The proportions in which bodies con:bine appear to be determined by fixed laws, which are exemplified in a variety of instances, and particularly in the present compound. Oxygen combines with twice its volume of hydrogen and twice its volunie of carbonic oxide to form water and car- bonic acid, and with half its volume of chlorine to forma euchlorine ; and chlorine reciprocally requires its own vo- lume of hydrogen and its own volume of carbonic oxide to form muriatic acid and the new gas. | This relation of proportions is one of the most beautiful parts of chemical philosophy, and that which promises fair- est, when prosecuted, to raise chemistry to the state and eertainty of a mathematical science. LXIX. New Tables for finding the Deviation of a Star in North Polar Distance and Right Ascension. By Mr. T. FirMIncER, late Assistant Astronomer at the Royat Observatory, Greenwich *. Ts the present improved state of astronomy, every means which tends to simplify calculation is readily embraced by the practical astronomer. With this view a variety of tables at different times have been published, and some of them so coneise and simple that they seem to afford but little if any room for further tmprovement ; whilst others, however, have not yet been so far improved, but that they still admit of a considerable degree, of simplification ; and of these the means of determining the nutation of a star in north polar distance from tables as heitherto published, is an instance. - Finding a considerable inconvenience in the computa- tion of this equation of constant use in the reduction of meridional zenith distances from Dr. Maskelyne’s Tables, « * Master of an Academy for the Instruction of a limited Number of Young Gentlemen in the Theory and Practice of the Mathematics and Ma- thematical Sciences, tH published in North Polar Distance and Right Ascension. 449 published at the end of the Greeenwich Observations of the year 1798, wherein the argument is applied to take out the equation by double entry, induced me to compute new tables for more readily finding it. The formula which I deduced for this purpose, is expressed by — 17,22 X Sy. (x R-+Long. p*Q)+8”,33° (¥ Ai—Long. D® Q ) taking the semi-axis major and minor at 9”,55 and 7,11 re- spectively. The table will therefore be easily computed at any subsequent period, should the major and minor axis of the ellipse of nutation be hereafter determined of different values from that which has been used in the above for- mule. ; In taking out the equation of nutation, the algebraic sum of the two parts of the table, give the whole equation, entering the first part of the table with sum of the star’s right ascension, and longitude of the moon’s ascend- ing node; and the second part of the table with the right ascension of the star minus the longitude of the moon’s ascending node. Examples. Example 1. To find the nutation in north polar di- stance for Arcturus, on July 1, 1812. Right ascension Arcturus 7° 1° 47’ 39” Longitude )* Q ..+e-- 5 1 31 09 x M+ Long. py’ B «0 3 18 39 PartI —17,13 *:MR—Long. °° B . 20 16 39 Part II —8”,11 Nutation required... —9”,24 To find the deviation of Sirius in north polar distance on July 1, 1812. Right ascension Sirius .. 3° 9? 13’ 28” Long. 26 8 i..sssaae Dd, 1 31 00 x' M+ Long. )' Bs. 8 10 44 28 +1%,13 ** AR— Long. D' QB. 10 7 42 28 +6",60 ——— Deviation required... +7573 When the longitude of the moon’s ascending node ex- ceeds the star’s right ascension, asin the last example; twelve signs must be added to the star’s right ascension before the subtraction can be made. These tables may be also applied to finding the deviation of a star in right ascension, but in this they require a little more 450 New Tables for finding the Deviation of a Star, &c. more labour than in the above application. The method ‘is by adding three signs to the star’s right ascension, if its declination 1s north; and on the contrary, subtract three signs if the declination be south ; then proceed as directed above, and multiply the equation so found by the natural tangent of the star’s declination, and the product converted into time will give the deviation required. | *°A.R. + Long. )* 8 * A.R. —Long. }* 8 fstype Ob pipe. Sitio = fey) egee. S. |VE + |VIL4 JVIN4 S- | VI 4 | VII + |VIT+ “ 7] ‘ ° “ “a “ o 0 | 0,00 | 0,60 | 1,04 | 30 © | 0,00 | 4,17 | 7,22 | so | 1 | 0,02 } 0,62 | 1,05 | 29 1] 0,15 | 4,80 | 7,29 | 29 | 2] 0,04 | 0,64 | 1,06 | 28 2] 0,29 | 4,42 | 7,36 | 28 { 3 |°0,06 | 0,65 | 1,07 | 97 3 | 0,43 | 4,54] 7,43 | 27 4 | 0,08 | 0,67 | 1,08 | 26 4] 0,58 | 4,66] 7,50 | 26 5 | 0,10 | 0,69 | 1,09 | 25 5 | 0,73 | 4,78 | 7.56 | 25 6 | 0,13 | 0,71 1,10 | 24 6 | 0,87 | 4,90 | 7,62 | 24 7 | 6,15 | 0,72 | 1,10 | 23 7 | 1,02 | 5,02 | 7,68 | 23 8 | 0,17 | 0,74 | 1,11 | 22 8 | 1,16 | 5,14] 7,73 | 22 9 | 0,19 | 0,76 | 1,12 | 21 9} 1,30 | 5,25 | 7,79 | 21 10 | 0,21 | 0,77 | 1,13 | 20 10 | 1,45 | 5,36 | 7,84 | 20 11] 0,23 | 0,79 | 1,18 | 19 Li | 1,59 | 5,47 | 7,89 | 19 12 | 0,25 | 0.80 | 1,14 | 18 12 | 1,73 | 5,58 | 7,93 | 18 13 | 0,27 | 0,82 | 1,15 | 17 13 | 1,88 | 5,69} 7,98 | 17 14} 0,99 | 0,83 | 1,15 | 16 14 | 2.02 | 5,79 } 8,02 | 16 15 | 0,31 | 0,83 | 1,16 | 15 15 | 216 | 5,89 | 806 | 15 16 | 0,33 | 0,86 | 1,16 | 14 16 | 2,29 | 6,00 | 8,09 | 14 17 | 0,35 | 0,88 | 1,17 | 13 17 | 2,44 | 6,10 | 813 | 13 18 | 0,37 | 0,89 | 1,17 | 12 18 |°2,58 | 6,20 | 816 | 12 19 | 0,39 | 0,91 | 1,18 | 12 19 | 2,72 | 6,29 | 8,19 | 11 20 | 0,41 | 0,92 | 1,18 | 10 20 | 2,86 } 6,40 | 8,21 | 10 21 | 0,43 | 0,93 | 1,19 | 9 21 | 2,99 | 6,48 | 824] 9 22 | 0,45 | 0,95 | 1,19 | 8 22 | 3,12 | 6.57 | 826 | 8 23 | 0,47 | 0,95 | 1,19 | 7 23 | 3,26 |. 6,66 | 8.28 |] 7 24| 0,49 | 0,97 | 1,19} 6 24 | 3,39 | 6,75 | 829 | 6 25 | 0,51 | 0,98 | 1,20] 5 25 | 3,53 | 682] 831 | 5 26 | 053] 0,99 | 1,20] 4 26 | 3,66 | 691 | 832} 4 27! 0,54] 1,01 | 1,20] 3 27 | 3,79 | 699 | 833 | 8 28 | 0,56 | 1,02] 1,20] 2 28 | 3,92 | 7,07 | 854] 2 29 | 0,58 | 1,03] 1,21 | 1 29 | 404 | 7,15 | 8,94]. 1 | 30 | 0,60 | 1,04 | 1,21 | 0 go | 4,171 7,22 | 8,34 | 0 X1+/X + |IK + XI + |X + |X + | Viv —} i= ey ant by | 1 LXX. 4 Nar- [ 451 ] LXX. A Narrative of the Eruption of a Volcano in the Sea off the Island of St. Michael. By S. Titvarp, Esq. Captain in the Royal Navy. Communicated by the Right Hon. Sir JoseeH Banks, Bart. K.B.P.R.S.* A pproacutne the island of St. Michael’s, on Sunday the 12th of June 1811, in His Majesty’s sloop Sabrina under my command, we occasionally observed, rising in the ho-- rizon, two or three columns of smoke, such as would have been occasioned by an action between two ships, to which cause we universally attributed its origin. This opinion was, however, in a very short time changed, from the smoke increasing and ascending in much larger bodies than could possibly have been produced by such an event ; and having heard an account, prior to our sailing from Lisbon, that in the preceding January or February a volcano had burst out within the sea near St. Michael’s, we immediately concluded that the smoke we saw proceeded from that cause, and on our anchoring the next morning in the road of Ponta del Gada, we found this conjecture correct as to the cause, but not to the time; the eruption of January having totally subsided, and the present one having only burst forth two days prior to our approach, and about three miles distant from the one before alluded to. Desirous of examining as minutely as possible a conten- tion so extraordinary between two such powerful elements, I set off from the city of Ponta del Gada on the morning of the 14th, in company with Mr. Read, the Consul General of the Azores, and two other gentlemen. After riding about twenty miles across the NW. end of the island of St. Michael’s, we came to the edge of a cliff from whence the volcano burst suddenly upon our view in the most ter- rific and awful grandeur. It was only a short mile from the base of the cliff, which was nearly perpendicular, and formed the margin of the sea; this cliff being as nearly as Tcould judge from three to four hundred feet high. To give you an adequate idea of the scene by description is far beyond my powers; but for your satisfaction I shall attempt it. . Imagine an immense body of smoke rising from the sea, the surface which was marked by the silvery ripling of the waves, occasioned by the light and steady breezes incidental to th e climates in summer. In a quiescent state, it had the appearance of a circular cloud revolving on the water * From the Philosophical Transactions for 1812, part i. like 452 A Narrative of the Eruption of a Volcano like an horizontal wheel, in various and irregular involu- ‘tions, expanding itself gradually on the lee side, when sud= denly a column of the blackest cinders, ashes, and stones would shoot up in form of a spire at an angle of from ten to twenty degrees from a perpendicular line, the angle of inclination being universally to windward: this was rapidly succeeded by a s¢cond, third, and fourth, each acquiring greater velocity, and overtopping the other till they had attained an altitude as much above the level of. our eye, as the sea was below it. As the impetus with which the columns were severally propelled diminished, and their ascending motion had nearly ceased, they broke into various branches resembling a groupe of pines, these again forming themselves into festoons of white feathery smoke in the most fanciful manner imaginable, intermixed with the finest particles of falling ashes, which at one time assumed the appearance of innumerable plumes of black and white ostrich feathers surmounting each other ; at another, that of the light wavy branches of a weeping willow. During these bursts, the most vivid flashes of lightning continually issued trom the densest part of the volcano; and the cloud of smoke now ascending to an altitude much above the highest point to which the ashes were projected, rolled off in large masses of fleecy clouds, gradually ex- panding themselves before the wind in a direction nearly horizontal, and drawing up to them a quantity of water spouts, which formed a most beautiful and striking addi- tion to the general appearance of the scene. 1 That part of the sea where the volcano was situated, was upwards of thirty fathoms deep, and at the time of our viewing it the volcano was only four days old. Soon after our arrival on the cliff, a peasant. observed he could discern a peak above the water: we looked, but could not see it: however, in less than half an hour it was plainly visible, and before we quitted the place, which was about three hours from the time of our arrival, a complete crater was formed above the water, not less than twenty feet high on the side where the greatest quantity of ashes fell; the dia« meter of the crater being apparently about four or five hun- dred feet. The great eruptions were generally attended with a noise like the continued firing of cannon and musquetry inter- mixed, as also with slight shocks of earthquakes, several of which having been felt by my companions, but none by myself, IT had become half sceptical, and thought their opinion in the Sea off the Island of St. Michael. 455 opinion arose merely from the force of imagination: but while we were sitting within five or six yards of the edge of the cliff, partaking of a slight repast which had been brought with us, and were all busily engaged, one of the most magnificent bursts took place which we had yet wit- nessed, accompanied by a very severe shock of an earth- quake. The instantaneous and involuntary movement of each was to spring upon his feet, and I said ‘* This admits of no doubt.”” The words had scarce passed mv lips, be- fore we observed a large portion of the face of the cliff, about fifty yards on our left, falling,-which it did with a violent crash. So soon as our first consternation had a little subsided, we removed about ten or a dozen yards further from the edge of the cliff, and finished our dinner. On the succeeding day, June 15th, having the Consul and some other friends on board, 1 weighed, and proceeded with the ship towards the volcano, with the intention of witnessing a might view; but in this expectation we were greatly disappoimted, from the wind freshening and the weather becoming thick and hazy, and also from the vol- eano itself being clearly more quiescent than it was the preceding day. It seldom emitted any lightning, but oc- casionally as much flame as may be seen to issue from the top of a glass-house or foundery chininey. On passing directly under the great cloud of smoke, about three or four miles distant from the volcano, the decks of the ship were covered with fine black ashes, which fell in- termixt with small rain. We returned the next morning, and late on the evening of the same day I took my leave of St. Michael’s to complete my cruize. On opening the volcano clear of the NW. part of the island, after dark on the 16th, we witnessed one or two eruptions that, had the ship been near enough, would have been awfully grand. It appeared one continued blaze of lightning ; but the distance which it was at from the ship, upwards of twenty miles, prevented our seeing it with effect. Returning again towards St. Michael’s on the 4th of July, I was obliged, by the state of the wind, to pass with the ship very close to the island, which was now completely formed by the volcano, being nearly the height of Mat- Jock High Tor, about eighty yards above the sea. At this time it was perfectly tranquil; which circumstance deter- mined me to land, and explore it more narrowly. [left the ship in one of the boats, accompanied by some of the officers. As we approached, we perceived that it was 454 A Narrative of the Eruption of a Volcano. was still smoking in many parts, and upon our reaching the island found the surf om the beach very high. Rowing round to the lee side, with some little difficulty, by the aid of an oar, as a pole, I jumped on shore, and was followed by the other officers. We found a narrow beach of black ashes, from which the side of the island rose in general too steep to admit of our ascending; and where we could have clambered up, the mass of matter was much too hot to allow our proceeding more than a few yards in the as- cent. ‘The declivity below the surface of the sea was equally steep, having seven fathoms water scarce the boat’s Jength from the shore, and at the distance of twenty or thirty yards we sounded twenty-five fathoms. From walking round it in about twelve minutes, I should judge that it was something less than a mile in cir- cumference ; but the most extraordinary part was the cra- ter, the mouth of which, on the side facing St. Michael’s, was nearly level with the sea. Jt was filled with water, at that time boiling, and was emptying itself into the sea by a small stream about six yards over, and by which I should suppose it was continually filled again at high water. This stream, close to the edge of the sea, was so hot, as only to admit the finger to be dipped suddenly in, and taken out again immediately. It appeared evident, by the formation of this part of the island, that the sea had, during the eruptions, broke into the crater in two places, as the east side of the small stream was hounded by a precipice, a cliff between twenty and thirty feet high forming a peninsula of about the same di- mensions in width, and from fifty to sixty feet long, con- nected with the other part of the island by a narrow ridge of cinders and lava, as an isthmus of from forty to fifty feet in length, from which the crater rose in the form of an amphitheatre. This cliff, at two or three miles distance from the island, had the appearance of a work of art resembling a small fort or block house. The top of this we were determined, if possible, to attain ; but the difficulty we had to encounter in doing so was considerable; the only way to attempt it was up the side of the isthmus, which was so steep, that the only mode by which we could effect it, was by fixing the end of an var at the base, with the assistance of which we forced ourselves up in nearly a backward direction. Having reached the summit of the isthmus, we found another difficulty, for it was impossible to walk upon it, we the On the primitive Crystals of Carbonate of Lime. 455 the descent on the other side was immediate, and as steep as the one we had ascended; but by throwing our legs across it, as would be done on the ridge of a house, and moving ourselves forward by our hands, we at length reached that part of it where it gradually widened itself and formed the summit of the cliff, which we found to have a perfectly flat surface, of the dimensions before stated. Judging this to be the most conspicuous situation, we here planted the Union, and left a bottle sealed up contain- ing a small account of the origin of the island, and of our having landed upon it, and naming it Sabrina Island. Within the crater I found the complete skeleton of a guard-fish, the bones of which being perfectly burnt, fell to pieces upon attempting to take them up; and by the account of the inhabitants on the coast of St. Michael’s, great numbers of fish had been destroyed during the early part of the erupt on, as large quantities, probably suffocated or poisoned, were occasionally found drifted into the small inlets or bays. The island, like other volcanic productions, is com- posed principally of porous substances, and generally burnt to complete cinders, with occasional masses of a stone, which I should suppose to be a mixture of iron and lime-stone; but have sent you specimens to enable you to form a better judgement than you possibly can by any de- scription of mine. ’ LXX. On the primitive Crystals of Carbonate of Lime, Bitter-Spar, and Iron-Spar. By Witttam HypE Wot- Laston, M.D. Sec. R.S.* Warr I formerly described to the society a goniometer + upon a new construction for measuring the angles of cry- stals, I expressed an expectation that we should thereby be enabled to correct former observations made by means of less accurate instruments. I took occasion to mention one instance of inaccurate measurement in the primitive angle of the common carbonate of lime; and J have had the sa- tisfaction to find the necessity of a correction, in that in- stance, confirmed by Mons. Malus, and admitted by the Abbé Haiiy, ina work f published nearly at the same time. * From the Philosophical Transactions for 1812, part I. + Bhilosophical Transactions for 1809. ‘See Phil. Mag. vol. xxxv. p.94. $ Tableau Comparatif des Résultats de la Crystallographie et de l’Analyse Chimique. / I t 456 On the primitive Crystals of Carbonate of Lime, It is by no means my design to detract in any degree from the merit of that justly celebrated crystallographer, to the surprising accuracy‘of whose measurements [ could, in va- rious instances, bear testimony. I hope, on the contrary, that in bringing forward two more observations similar to the preceding, and intimately connected with it, I shall offer what will not only appear interesting: to crystallogra- phers in general, but will be peculiarly. gratifying to the Abbé Haiiy. In his Traité de Minéralogie, and again more recently in his Tableau Comparatif, the same primitive form is as- signed to three substances very different in their compo- sition, to carbonate of lime, to magnesian carbonate of lime (or bitter-spar), and to carbonate of iron. It has been objected to Mons. Haiiy, that according to his method identity of form should be accompanied by identity of composition, unless the form were one of the common regular solids. For though in that case any geo- metrician would readily admit it to be very probable, that many different substances might concur in assuming the same form of cube, of octohedron, or of dodecahedron, &c. there does not appear a corresponding probability that any two dissimilar substances would assume the same form of a peasatar rhomboid of 105°.and a few minutes, to which no such geometric regularity or peculiar simplicity can be ascribed. But though so accurate a correspondence, as has been hi- therto supposed to exist in the measures of the three car- bonates above mentioned, might be justly considered as highly improbable, no degree of improbability whatever attaches to the supposition, that their angles approach each other by some difference, so small as bitherto to have es- caped detection. And this in fact I find to be the case. Since the angles observable in fractures of crystalline substances are subject to vary a little at different surfaces, and even in different parts of the same surface (as 1s evident from the confused image seen by reflection from them), I shal] not at present undertake to determine the angles of these bodies to less than five minutes of a degree. This, indeed, is the smallest division of the goniometer that I usually employ, as I purposely decline giving so much time to these inquiries as would be requisite for attempting to arrive at greater precisiou. The most accurate determination of the angle of car- bonate of lime is probably that of Mons. Malus, who mea~_ sured it by means of arepeating circle, and found it to be 105°"'9’, Bitter-Spar, and Iron- Spar. 457 05° 5°. And this, indeed, is the result to which T for- merly came by a different method *. If it differ in any re- spect from this quantity, [am inclined to think that it will more likely be found to be deficient by a few minutes, than to exceed the measure here assigned; and accordingly to differ still more widely from those angles which I am about to mention, In the magnesian carbonate of lime, or bitter-spar, the primitive form is well known to be a regular rhomboid, as well as that of carbonate of lime, and so nearly resembling it, as to have been hitherto supposed the same. I find, however, a difference of 12 10’ in the measures of these! crystals; for that of the magnesian carbonate is full 1064°, as [ have observed with uniformity in at least five ditterent specimens of this substance obtained from situations very distant from each other, The primitive angle of iron-spar is still more remote from that of the carbonate of lime, which it execeds by nearly two degrees. I have examined various specimens of this substance, some pure white, others brown, some transparent, others opake. That which gives the most _ distinct image by reflection is of a brownish hne, with the semi- transparency of horn. It wasobtained from a tin mine, called Maudlin Mine, near Lostwithiel in Cornwall. By repeated measurement of small fragments of this specimen, the angle appears to be so nearly 107°, that I cannot form any judgement whether in perfect ery stals it will prove to be greater or less than that angle. ' Jn this instance the carbonate of iron is nearly pure, and so perfectly free from carbonate of lime, as to render it highly probable that in other specimens having,the same angle, but containing also carbonate of lime er other i ingre- dients intermixed, the form is really depeudent on the car- borate of iron alone. It appears however not unlikely, that when substances which agree so nearly in their primitive angle are inter- mixed m certain proportions, they may each exert their powers; and may occasion that confused appearance of cry- stallization with curved surfaces, known by the name of peari-spar. [ cannot say that I have made any accurate comparative analyses which may be adduced in support of the hypothesis, that mixtures are more subject to curvature than pure chemical compounds ; bat it is very evident from , the numerous analyses that have been made of iron-spar by * Phil. Trans. 1802, p. 285. Vol. 39. No. 170. June 1819. other o i] 458 Notices respecting New Books. other chemists, how extremely variable they are in their composition, and consequently how probable it is, that the greater part of them are to be regarded as mixtures; al- though it be aiso possible, that there may exist a triple car- bonate of lime and iron as a strict chemical, compound. It seems not unlikely, that there may hereafter be found some carbonate allied to the preceding, which may owe its form to the presence of manganese: but notwithstanding the liberality which happily prevails in general amorfg those who have it in their power to assist in such inquiries, I have not had the good fortune to meet with any such com- pound; and I am unwilling, merely in the hope of mak- ing such an addition, any longer to defer communicating an observation, which I bope will be of real utility in the discrimination of bodies that difler so essentially in their composition. LXXII. Notices respecting New Books. Paar I. of the Philosophical Transactions of the Royal Society for 1812 has just made its appearance. The follow- ing are its contents : 1. On the Grounds of the Method which Laplace has given in the second Chapter of the third Book of his Mé- canique Céleste for computing the Attractions of Spheroids of every Description. By James Ivory, A.M. Commu. nicated by Henry Brougham, Esq., F.R.S. M.P.—2. On the Attractions of an extensive Class of Spheroids. By J. Ivory, A.M. Communicated by Henry Brougham, Esq. F.R.S. M.P.—-3. An Account of some Peculiarities in the Structure of the Organ of Hearing in the Balena My- sticetus of Linnzeus. By Everard Home, Esq., F.R.S.— 4, Chemical Researches on the Blood, and some other Ani- mal Fluids. By William Thomas Brande, Esq., F.R.S. Communicated to the Society tor the Improvement of Ani- mal Chemistry, and by them to the Royal Society.—-5. Ob- servations of a Comet, with Remarks on the Construction of its different Parts By William Herschel, LL.D. F.R.S. —6. On a gaseous Compound of carbonic Oxide and Chlo- rine. By John Davy, Esq. Communicated by Sir Hum- phry Davy, Knt., LL.D., Sec. R.S.—7. A Narrative of the Eruption of a Volcano in the Sea off the Island of St. Mi- chael. By S, Tillard, Esq., Captain in the Royal Navy. Communicated by the Right Hon. Sir Joseph Banks, Bart. K.B. P.R.S.—8. On the primitive Crystals of rigs | te) Royal Society. 459 of Lime, Bitter-Spar, and iron-Spar. By William Hyde Wollaston, M.D. Sec. R.S.—9. Observations intended to show that the progressive Motion of Snakes ts partly per- formed by means of the Ribs. By Everard Home, Esq. F.R.S.—10. An Account ef some Experiments on the Combinations o: different Metals and Chlorine, &c. By Join Davy, Esq. Communicated by Sir Humphry Davy, Kut. LL.D. Sec. R.S.—11. Further Experiments and Ob- servations on the Action of Poisons on the Animal System, By B. C, Brodie, Esq. F-R.S. Commiunicaied to the So- ciety for the Improvement of Animal Chemistry, and by them to the Royal Society. The Twelfth Number of Levbourn’s Mathematical Repository contains, 1. Solutions to the Mathematical Questions proposed in Number X —2. Ou the irreducivle Case of Cubic Equations.——4. New Prope rues of the Conie Sections. —4. Indeterminate Problems.—5. On the Ellipse and Hyperbola.x—6. On the Roots of Equations of all Di- mensions.—7. Properties of the Right-angled Trianyle.— 8. Continuation of Le Gendre’s Memoir ou Elliptic Tran- scendentals.—g. A Series of new Quesiions to be answered in a subsequent Number. LO LOE DEEL aE See een ees LXXIII. Proceedings of Learned Societies. ROYAL SOCIETY. Sixce our last Report, a paper by Mr. John Davy was read on some of the combinaiions ot the fluoric prine:ple. fn this paper Mr. John Davy gave the results of some experi- ments on silicated fluoric gas and fluoboric gas, and de» scribed a new and more simple method of procuring this last gas; namely, by distilling together a mixture of diy boracic acid, fluor spar, and oil of vitriol. He stated the specific gravity of these gasses, and gave an account of their combinations with ammonia. Fluoboric gas combines in three proportions wiih ammonia, and with the largest pro- portions of the alkalin€ gas forms saline combinations, fiuid at the common temperatures of the atmosphere. A paper by Sir H. Davy was read, on some combina- cions of phosphorus and sulphur, and on other objects of themical inquiry. In this paper Sir H. Davy desembed pure phosphorous acid as a solid crystalline body, vuiatile at a moderaie de~ Gp22 ; gree 460 Royal Society. gree of heat. “He described a combination of this acid with-water, likewise a crystalline solid, very combustible, and when decomposed by heat affording a peculiar elastic fluid absorbable by water, not spontaneously inflammable, and consisting of phosphorus united to two volumes of hy- drogen condensed into the space of one volume, and which he proposes to call hydrophosphoric gas. . He entered into the detail of some experiments on sul- phuric acid, which, he stated, cannot exist independently of the presence of water; and he described a solid compound of nitrous acid gas, sulphurous acid gas, and water. He considered all the facts advanced in this paper as affording confirmations of the theory of definite proportions. And he drew some general conclusions respecting the impor- tance of water as a chemical agent. Most of the bodies called oxides, when precipitated from aqueous solutions, are in truth (said Sir H. Davy) hydrats; and their colours and their properties depend upon the combined water. June 11.—Dr. Wollaston “read to the Society a short paper on improvements in the camera obscura and simple microscope, founded on the same periscopic principles by which he improved the construction of spectacles a few years since *, In his camera obscura the light is admitted through a : en oie : circular opening to the concave surface of a large meniscus placed behind it, at such a distance that all pencils of rays pass nearly at right angles through its posterior surface. Hence those that come from objects obliquely situated, form more distinct images, and afford a larger field of view than is obtained by the common construction. His microscope consists of two plano-convex lenses with their flat surfaces towards each other, but prevented from touching by a thin plate of metal. A small perforation in the centre of the metal suffers no rays to pass but what are at right angles to both the exterior surfaces, and hence give -a distinct field of view of great extent. He observes also that the camera lucida in its most sim- ple form, with the upper surface of its prism concave, has the same advantage as the periscopic construction. GEOLOGICAL SOCIETY. a May 1, 1812. The president in the chair.—A_ paper by Dr. M‘Culloch (member of the Society), ‘* On Bistre and * Philosophical Magazine, vol. xviii. p. 165. alt other Geological Society. 461 other substancés produced in the distillation of wood; and on their analogy with the native Bitumens,”’ was read. When wood is submitted to destructive distillation, there is obtained, among other products, a black substance re- sembling common tar. This tar is very inflammable, and so liquid that it may be burnt ina lamp. By washing it with water either hot or cold, or submitting it to the action of lime or of the mild alkalies, a large portion of acetic acid is separated, and the residue becomes pitchy and tena- cious. It is entirely soluble in caustic alkali, in alcohol, in ether, in acetic acid, and in the mineral acids. The fat oils and the recent essential oi!s dissolve but little of it; but if the former are made drying, and if the latter have become brown by keeping, they then act more readily and copi- ously. Colvured oil of turpentine takes up a considerable quantity, but naphtha only acquires a scarcely sensible brown colour by digestion upon it. When carefully di- stilled at a gentle heat it is decomposed into an oily mat- ter, at first limpid and aftérwards brown, a quantity of acetic acid combined with a little ammonia; and a spongy coal remainsin the retort. In this process no inflammable gas is given out; but at a high temperature the oi! is niore or less decomposed, and an inflammable gas is produced, which, however, does not burn with a flame by any means so bright as the gas from pit-coal. If this destructive di- stillation is not carried very far, the matter in the retort will be found, when cold, to be solid, brilliant, shining, and possessed of a conchoidal fracture: its taste is burn- ing and pungent, and its odour is that of wood smoke ; it is fusible and readily inflammable. When kept melted in _ an open vessel till it ceases to be fusible, it becomes more and more brilliant, its fracture passes to splimtery, and it assumes the perfect appearance of asphaltum. In propor- tidn as it approaches this stare it becomes Jess aud Jess so- luble in alcohol, and at length scarcely gives a stain to this menstruum. | Naphtha has no action on it, and in this cir- cumstance alone it differs from asphaltum. Dr. M. then proceeds to an examination of the Bitumens, and shows that the difference between the products of recent vezetable matter, and of the bitumens when subjected to distillation, consists in the former yielding empyreumatic acetic acid and a black pitchy matter insoluble in naphtha: while the latter afford ammonia and naphtha, but little er no acid. He then enters into a detailed investigation of the proper- ties of the very important class of Lignites, or those sub- Gg3 stances, 462 Geological Society. stances, such as peat, surturbrand, Bovey coal, &e. in which the traces of vegetable origin are not obliterated. Submerged wood from. peat mosses gave a brown oil smelling of wood- -tar, and refusing to dissolve in naphtha. A compact pitchy-looking peat gave a fetid oil resem- bling in odour neither wood-tar nor bitumen, and very slightly soluble in naphtha. Bovey brown coal gave an oil resembling in odour that of wood-tar, but much more soluble in naplitha: that por- tion of the oil which was insoluble in this menstruum had a strong odour of wood smoke. The oil of jet was almost perfectly soluble in naphtha, and smelled strongly ot petroleum ; but it afforded also em- pyreumatic acetic “acid. Thus it appears that there exists a class of fossils of un-, donbted vegetable origin, which exhibit the gradual pro- gress from wood to bitumen, and in which this change has been brought about by the action not of heat but of water. The experiments, however, of Sir James Hall seem to show that heat with compression 1s also capable of con- verting wood into coal._—A oe examination of this tact was the next object of Dr. M.; and he found on heating wood in close gun-barrels that a black coaly-lvoking sub- stauce was indeed produced, but that it consisted wholly of charcoal, empyreumatic acid, and wood-tar, and did not contain the smallest portion of real bitumen. Hence the experiments alluded to do by no. means prove the possibj- lity of converting vegetable matter into real coal by mere heat. It appears however to Dr. M, that the consolidas tion of bituminized vegetables into coal is not unhkely ta be the effect of subterranean heat. The paper concludes by showing the identity of the pitch procured from the distillation of wood and the pigment called Batre; and points out methods of obtaining 1 in a state beiter fitted than common bisire for the purposes of the artist: and also enumerates several other uses fo which this substance may be ceconomicdlly applied. : Some notes on the mineralogy of the neighbourhood of Si. David’s, in Pembrokeshire, by Dr Kidd, (Prot. chem, Oxford, and member of the Geolozical Sacietyv,) were read. The country about St. David’s when view el from an eminence presents the appearance of an extensive uneverr plain, interspersed with numerous deiached hills or rocky summits of an irregular conical shape. The two highes' of ‘ these, Geological Society. 463 these hills are Penbury and Carn-Llidy, the western por- tion of the latter of which forms the promontory of St. David’s-head. These hills present no appearance of stratification, and are composed of feldspar and hornblend in various propor- tions and states of aggregation. They are each surrounded by mantle-shaped strata of slate, elevated at a bigh angle, and presenting the characters of grauwakke-slate. This latter is traversed by veins of quartz, from which very fine specimens of rock-crystal are procured. No carbonate of lime appears to be contained either in the unstratified trap or in the élaty grauwakke; nor did there occur in them, with the exception of one equivocal instance, the smallest trace of any organic remain. May 15. The president in the chair.—An account of the island of Teneriffe, by the hon. Henry Grey Bennet, (member of the Geological Society) was read. The greatest length of this island from north to south is about seventy miles, its greatest breadth does not exceed thirty miles. In the south-western part of the island is si- tuated the mountain called by the Spaniards El Pico di Tiede, but better known by the name of The Peak of Te- neriffe, the height of which, from the mean of several ob- servations, appears to be about 12,500 English feet. The rocks and strata of this island appear to be, wholly voleanic. A Jong chain of mountains passes through the , interior, sloping on the eastern, western, and northern sides to the sea, but on the S. and SW. elevated into nearly perpendicular mountains which are intersected by deep and narrow ravines... i The lowest bed of the island is porphyritic lava composed of hornblend and feldspar, in its upper part porous, sco- riform, and sometimes passing into the state of pumice. Upon this rests a hed of the same substances as already mentioned, but in structure nearly approaching to green- stone. This is covered by a thick bed of pumice, which itself is overspread with basaltic lava, on which in many places rest beds of tufa and volcanic ash. This basaltic lava decomposes sooner than any of the other rocks, and contains the greatest variety of imbedded substances: it is sometimes divided by a layer of olivine in crystals some inches long, and is often intersected by thick veins of porphyritic. slate. Zeolite and chalcedony also occur in it. _The number of small craters and extinct volcanos is pro- digious ;—they are to be found in all parts of the island, Gg4 but 464 Geological Society. but none of them have heen in activity of late years. The great streams of lava have flowed from the peak: those of the years 1704 and 1797 (which was the last) are basaltic. This latter flowed so slowly, notwithstanding the sharp de- scent of the mountain, that it was several days i in advancing three miles. On the south-western side of the peak is an ancient lava not at all decomposed several miles in length, and in a perfect state of vitrification resembling obsidian. ‘dune 5. The president in the cbair.—Lord viscountValentia and W,. Franklin, M. D. were elected ordinary members. «An account,” by Thomas Webster, esq. (member of the Geological Society,) ‘ of some new varieties of Aley- onia, found in the Isle of Wight,” was read. In viewing the rocks about Ventnor Cove and in various parts of the undercliff, Mr. Webster remarked, in at sandstone stratum immediately under the chaik-marl, great number of small prominences resembling in ee the branches of trees. They were of various. sizes, from half an inch to three or four inches in diameter : their sub-~ stance was sandstone of the same kind as the rocks they were in; but the part resembling the bark was somewhat harder, which enabled it to endure longer than the rest. of the stone, and thus project above its surface. Some of them were straight, others a little crooked, and in a few instances he observed them forked. He faund fragments of these bodies in every part of the island where the sandstone stratum can be seen, and particularly among the masses of rock lying under the cliffs of Western Lines. To this last place he found that the stems above described had frequently heads or bulbaus terminations attached ta them, in form somewhat resembling a closed tulip, and in some of these he found distinet traces of organic structure, from which it appeared that these heads consisted of a group of tududi now converted into and enveloped with stony matter. Besides these extraordinary shapes which pro- jected in relief, Mr. W. observed a variety of very regular white figures ag if painted upon the rock, being even with its surface. ‘Phev consisted of circles from two inciies tu half an inch im diameter, ellipses of various eccentricities, and pareitel lines both straight and. crooked. By a caretul examination Mr. W. found that these white fi- gures belonged to the other class of bodies already described; that ‘the cylinders weré only the internal parts of the same body, .whose various sections formed the white circular and elliptical fieures. The vast masses ef rock which have fallen down, having separated from the cliff at the divisions between * 7 Geological Society. 465 between the beds, showed their upper and under surfaces covered with layers of these bodies heaped upon each other and lying prostrate in every possible direction; and in the joints between the beds where they were not separated, they were distinctly seen. The green sandstone and the Jimestone he found to be the chief repositories of these bodies. In the ferruginous sand below the green sandstone he found none, and only a tew fragments of cylinders in the blue marl on which the sandstone rests. He traced them upwards into the chert; but they there became rare, and they totally disappeared in the chalk-marl. He tound them, however, frequently in the fragments of flint lying on tie shore. Mr. Webster having brought away an extensive series of specimens (which he has since deposited in the cojlection of the Society), submitted them to the examination of Mr. Parkinson, who is of opinion that they belong to the genus Aleyonium, but that they are of three or four different species, neither of which have been hitherto described. From the resemblance which these bodies bear to a closed tulip attached to its stalk, Mr. W. suggests that the name of Tulip Alcyonium may be not improperly applied. : «© Some observations,’ by James Parkinson, esq. (mem- ber of the Geological Society,) ‘ on the specimens of Hip- purites from Sicily,” presented to the Society by the hon. Henry Grev Bennet, (a member) were read. These specimens Mr. Parkinson considers to be such as demand particular atiention, as they possess those charac- ters which will probably serve to correct some erroneous opinions respecting the nature and habits’ of the animals of which these shells were the dwellings. One of the specimens contains a nearly perfect shell, Jongitudinally divided so as .o display the two ridges with the numerous septa and chambers. From an examination of these specimens, and by com- paring them with the observations lie has before had an op- portunity of making, Mr. Parkinson is of opinion that the structure of the shell of the Hippurites is such as would enable the animal to raise itself to the surface of the water. This opinion is in opposition to that of M. Denys de Montfort and most of the French oryctologists, who con- sider the Hippurites as belonging to what they term pela- gian shells, or such as constantly inhabit the bottom of the sea, never rising to the surface or appearing on the shores, and therefore that there is uo reason to believe them as be- longing 466 Geological Saciety. - Jonging to animals which are now extinct, but only that their recent analogues have not yet been brought to view. June 1g. The president in the chair.—Charles Bell, esq. F. R.S.E., Daniel Moore, esq. F. R.S. &c., and the Rev. Edward Slater, were elected ordinary members. A paper by Joseph Skey, M.D. entitled ‘* Some remarks upon the structure of Barbadoes, as connected with speci- “mens of its rocks,” communicated by Arthur Aikin, esq. secretary, was read ; together with a Note by Mr. Parkin- son on some of the specimens presented by Dr. Skey. The island of Barbadoes is totally unlike those immedi- ately near it, both in appearance and in structure. The land rises in a gentle swell from the coast towards the imd- dle of the island, except in one small district. Its highest hills do not exceed 800 or 906 feet, and their general direc- tion is nearly NW. and SE. Upon the north-eastern coast the shores are bolder than in the other parts of ‘the island, as is the case in many of the islands of these seas. Barbadoes is composed of limestone, in great part of fossil madrepores, and traces of organic structure are to be — met with in almost every part of the island, more particu- larly along the whole of the S. and SW, coast. The land which when seen from the sea appears to rise uniformly from the coast, is observed on a nearer view to consist of successive terraces rising in two or three grada- tions, one above the other, each forming a plain of a quar- ter or half a mile in breadth, and terminated by a cliff of coral rock varying in elevation from twelve to twenty feet, and sometimes considerably bigher. Deep fissures have in many places of the island rent asunder the cliffs, and these gullies (as they are called) are continued across the terraces in irregular lines. Numerous caves are every where to be met with, and they are some- times of very large dimensions. On the S. and SW. side of the island there may be seen at very low water a bed of calcareous sandstone dipping SW. thirty degrees. To the eastward of the garrison of St. Ann, there is found adull compact chalky-looking limestone with ramose alcyonia, while considerably to the westward the rock is more distinctly coralloidal. Upon the northern and north-eastern side of the island js a small mountainous district cojled Scotland. It consists almost entirely of limestone, but of a kind less marked by organic remains than in the other districts. In Mr, Parkinsan’*s Note it is observed that some of Dr. Skey’s specimens illustrate the nature of some fossil corals; showing Geological Society. 467 showing that the forms in which they at present exist, are not those which belong to those substances in their original state, and consequently ought not to affect their specific or generic distinctions. A letter from E. L. Irton, esq. describing some remark- able tubes found in the drifted sand at Drigg in Lancashire, was read; together with an account, by W. H. Pepys, esq. (Treasurer G. S.), of a chemical examination made by him of the substance of these tubes. These tubes are nearly in a perpendicular position, 1m- bedded in the midst of the hills of drifted sand, on the sea shore, without any communication with the surface; and there are ramifications’ extending from them which gene- raliy point downwards and terminate in fine points. The tube sent to the Society is above an inch in diameter, and of an irregular form: the outside consists of black and white sand agglutinated together ; the inside is smooth, and has a vitrified appearance. When dug out of the sand it was soft, and in some degree flexible ; and the inside coat- ing at its first exposure to the air was soft to the touch and rather unctuous; but in less than a quarter of an hour it hardened into the staie in which it now exists. The tnbe when found was filled with the sand of the hill, and that sand is quite different from the sand of which the outside of the tube consists. Both the sand and the vitreous part of the tube scratch glass; and on the latter, when viewed by a lens, there are seen small air-blebs, such as are common to imperfect vi- trification. Both are insoluble in sulphuric and nitric acids ; infusibie before the blowpipe without addition, and partially fusible on the addition of boracie acid; but with soda a complete fusion took place, and the residue was nearly soluble in water. ¢ A paper by Dr. M‘Culloch (member of the Society), 6 On the vitrified Fort of Dun MacSmochain, neai Oban in Argyleshire,” was read. fn the discussion which some time ago took place re- specting the vitrified forts of Scotland, the question om which the two contending parties were most at Issue, Was, whether the vitrification was the effect of design or of acct dent —It occurred to Dr. M. that hight might be thrown on — the subject by examining with mineralogical accuracy the substance of which these structures were composed, and noting the changes which each had undergone in conses quence of the fire, and also by observing “hence the stones had been derived which were used in them; and that the question 468 Geological Society. question of accident or design might be illustrated, by exa~ mining in the laboratory the degree of heat required to pro- duce the appearances in the stones which actually existed in these structures, The fort of Dun MacSniochain stands on a long narrow hill, which is nearly precipitous along three parts of its cir- cumference, and at the other end it rises from the plain with a very accessible acchivity. The walls, which are all at present buried under the soil, are about eight er ten feet in thickness. They bear marks of vitrification through their whole extent; but in no case does it appear to have extended more than a foot or two upwards, and the most perfect slags are found at the bottom of the foundation. » In the higher parts of these are stones roasted by the action of the heat, bat unvitrified, and at length the marks of fire almost entirely disappear. The hill consists of alternate beds of schistus and limestone, but the latter is the predo- minant rock. It is perfectly imsulated in a great alluvial plain. The mountains of Benediraloch, which bound the plain to the west, consist of granite gneiss, mica-slate, quartz and por- phyry. On the edge of these rocks are found large de- tached masses of puddingstone, consisting of rounded pebbles of greenstone of different varieties, of ainygdaloid and quartz cemented by a paste which appears to consist chiefly of trap sand, united by the hard variety of calea- reous spar. The paste contains also in small quantity zeo- lite, prehnite, garnet, and diallage. This puddingstone where nearest the fort 1s at Jeast half a mile distant from it. The walls of the fort consist principally of granite gneiss, mica-slate, clay-slate quartz, puddingstone and py- ritical slate entangled together with a very small proportion of the particular rock on which the fort itself is founded; puddingstone forming the greater part of them. This pud- dingstone Dr. M. shows to be the only vitrifiable ingre- dient of the walls; and from the distance from which it must bave been brought, and the great quantity of it em- ployed in the work, he considers it probable that the build- ers of the fort must have been acquainted with its vitrifiable nature, and that 4 was on account of this quality that they had employed so great labour in transporting it. For if their object had not been. to produce vitrification, but mere- ly to erect a-dry wa'l of stone, the limestone of the bill would have answered their intentions, or perhaps the loose stones of the adjoining plain. That they did not obtain the puddingstone from the latter Russell Institution. A690 Jatter source, is evident; for although the plain and shore are covered with fragments, these consist almost entirely of the primary rocks: and besides the pieces of the wall which have not felt the fire, there are angular fragments, showing pretty clearly that they were not collected on an alluvial plain, but broken from the rocks where they are found. Dr. M. next proceeds to describe the various states in which the different stones are found. The puddingstone exhibits the greatest variety of changes. It is found in every state, from a black glass to a spongy scoria capable of floating in water, sometimes ex- hibiting the gradual succession of changes from incipient calcination to complete fusion. To ascertain the degree of heat necessary to produce the corresponding changes in this rock, Dr. M. submitted various parts of it to the furnace, and found that some of the fused substances must have been brought to that state in a heat not less than 100° of Wedgwood’s ‘scale; a heat at which many varieties of earthen-ware are baked. Dr. M. next gives a short account of the vitrified fort of Craig Phadric in Invernessshire, and of another in Gallo- way; in both of which, but more particularly in the former, he observed circumstances quite analogous to what he had already found at Dun MacSniochain ; and the con- elusion he has been led to form is, that the vitrification of these forts is the effect of design. ; The Society adjourned till November. RUSSELL INSTITUTION. ees the fourth Lecture Mr. Bakewell proceeded to describe the stratified rocks containing rock-salt and coal. The coal districts in England and in other parts of the world, he said, were generally separated from the compact fimestone which contains metallic veins, by thick beds of coarse grit-stone and sand-stone, in which some vegetable remains first make their appearance. In the midland counties of England, there are two kinds of rock interposed between the coal and the lime, forming together a mass of three hundred yards in thickness. The lower bed consists of a dark reddish-brown shale, in which strata of micaceous sand-stone and beds of dark limestone occasionally occur, The upper rock was called by Mr. Whitehurst mill-stone grit, from its containing beds of hard siliceous grit-stone, used for mill-stones, This rock varies both in cclour and quality 470 Russell Institution. quality in different parts. It was first observed hy Mr. Whitehurst that under this rock no coal is ever found. Thig observation Mr. Bakewell said was correct, as applied to workable coal, or such beds that were of sufficient thickness to be got with profit, but very thin seanis of coal, as wel} as vegetable impressions, are not unfrequent in these rocks, They extend over a considerable part of the northern coun- ties, and form the range of central hills from the north of Derbyshire to Craven in Yorkshire. Mr. Bakewell said he was inclined to believe that the lower bed, a dark-brown shale, changed its quality as it passed into Cheshire, and was there the red sand rock of that and the adjacent counties. He observed that he did not consider some dife ference in external character alone sufficient to disprove the identity of strata which may spread over a large tract of country. In this red sand rock the rack-salt of Cheshire is found. He described the various repositories of salt in Spain and different parts of the world, and observed, that it had been tound at the height of 9000 teet above the level of the sea; and from its position, as well as from the dif- ference of its constituent parts from those of sea-salt, he was inclined to believe that it had not been formed by the evaporatoin of sea-water, as some geologists have asserted. The rock-salt of Cheshire is remarkably free from im- purities, containing, according to the correct analyses of Dr. Henry,. not the least sulphat of magnesia, and not one grain in 1000 of muriate of magnesia. In the same quan- tity of sea-salt not less than 46 grains of these two saline impurities occur. In the strata over these rocks we meet with beds of coal occupying distinct districts called coal-fields. Mr. B. then described the various kinds of stone-shale, and iron:stone, that alternate with coal, and the appearances which offer indications of its presence. The position into which coal Strata are thrown by faults and dykes in different parts of England were explained by drawings and sections. A most singular elevation of a bed of coal in the vicinity of the red rock in Lancashire was particularly noticed. Where this rock comes nearly in contact with the coal, the stratum is raised up vertically, whilst seven other beds of coal in the same field are all inclined at an angle of 25 degrees. Mr. Bakewell stated, that he had communicated an account of this coal-field to the Geological Society, as he conceived that it might lead to some discoveries respecting the geo logical relations of the red sand rock with the coal strata. The obstacles which impede the working of abit rom London Philosophical Society. 47h from the fire- and choak-damps were described. The nature aud properties of these noxious vapours were illustrated by experiments, and some account given of the different modea of clearing the mines in different districts. Mr. Bakewell observed, that Dr. Miller and other writers on the coal districts of England had entirely overlooked the coal of the West Riding of Yorkshire, although the quantity procured there supplied a population nearly equal to that of London, besides the extensive manufactories of that county. He described the manner in which the quan- tity of coal in the coal-fields of Northumberland and Dur- ham had been estimated ; from whence it appeared that at _ the present rate of consumption they would be entirely ex- hausted in the space of three centuries. Were there no other repositories but these, he observed that it would be- come the duty of a wise statesman to prevent exportation to foreign countries, and to plant all our waste Jands, and provide against impending though remote calamity. Let any person, said he, reflect on the condition of the metro- polis were it deprived for three months of the supply of coal. All the wood in the country would be destroyed, our manufactories would be annihilated, and a scene of national calamity would ensue, of which we can scarcely form an idea. But besides extensive coal-fields in Yorkshire and other parts of England, at present scarcely touched, there exists a great repository in South Wales of one thousand square miles of coal, which, from the thickness of the different strata, he calculated would supply the consumption of Bri- tain for several thousand years to come, estimating that consumption at twelve million tons annually. He con- cluded by giving a short outline of the coal districts in different parts of the world, and the periods at which coals appear to have been introduced for fuel. It may excite a smile, said he, at the ignorance of our ancestors, to find an act of parliament in the reign of Elizabeth, prohibiting the burning of coal in London during the sitting of parlia- ment; but probably posterity at mo distant period may look with equal surprise at the general indifference evinced by landed proprietors of tie present day, respecting the mineral substances on their own estates. LONDON PHILOSOPHICAL SOCIETY. {Continued from p- 395.] Mr. Clarkson next proceeded to investigate the charac- ters of moral existence, observing, that pathognomy had already 47% London Philosophical Society. already proved its action, and anatomy the effects of its action, in the second division of the face. All that was necessary, therefore, was an ideal standard, by which. to judge of the moral or immoral propensities of ‘the individual, and this the Greeks had already erected. Their statuaries had two objects im view ; one of which was to eradicate all violent passions from the faces of their deities, (and this they eflected by reducing and softening down the museles of the cheeks and nose,) and the second was to leave upon their faces the character of some quality for which, they were distinguished, (and this they effected by strict phy- siognomical rules.) He then detailed the different phy- siognomical expressions of the ancient gods ;—the senti- mental laxity of Venus, the purity of Diana, the fortitude and taste of Minerva, the pride of Juno, the benevolence of Apollo, and the conscious calm security of Hercules,—all of which he proved by drawings and busts of the antique physiognomically exprest; nor could his conclusions, he said, be denied without .a eulicalous dilemma, that the head of one deity would have answered as well for another. We need look no further, then, fora standard for the nobler pro- pensities of our nature. Nor were the characteristics of the ignobler less apparent to investigation, Drunkenness and every species of intemperance “distort and caricature the face in proportion as they destroy the intellect and the sentimental emotions—and here the Lecturer alluded to the head of Nero at the Museum, asserting that it was im- possible to contemplate that head without recognising in it the i intemperance, the gluttony, the pride, and impiety of that sanguinary monster. Originally handsome, every thing proclaimed the lapse of the man into the brute: the elevated chin, the swollen throat, and depending cheeks, the breathing nostrils, and staring eyes, spoke a language not to be mistaken. Mr. C. next adverted to the contrast observable in the faces of Cupid, or Venus and Minerva. It was as evident as the contrast between ambition and love, the master- passions of human nature. In the former, the cheeks are rotund; in the latter, concaves—in the former, the nostrils are dilated, i in the latter, rectilinear and compact 5—the in- terval, therefore, affords a standard to judge of the mixture of these passions in the individual. But the Greek head of Pan, the lecturer observed, was a kind of silent phy- siognomical lecture. No one will pretend to say that it dovs not express passions in quiescence, and no one can doubt the nature of the passions it conveys. —The diagonal bearing London Philosophical Society. 473 bearing of the eye, the brutal projection of the mouth, the lapse of the eyebrows and nose, and the complete distor- tion of the latter characteristic, express a total debasement and abandonment of the mind. If, then, we assume the face of Pan as the lowest state of sensual degadation to which man can fall, as the boundary which separates him from brutes, and assume the unpolluted face of the Greek ideal as the shade which mingles him with gods, we obtain another standard to judge of moral brutalization or refine- ment, We are sorry that our limits will not allow us to follow the lecturer through a masterly analysis of the passions, their physiognomical effects, and their modification by the different temperaments of the body, whether phlegmatic, sanguine, or melancholic. We have stated enough in de- tailing his remarks on Greek statuary to render his object jucid and practicable,—the erection of a standard for moral propensities as well as intellectual energies. Animal life and its territory was the Jast division of his | subject. Its mdications, he said, were extremely simple, aud easily explained. All relaxation is accompanied by a separation of the jaws—total debility is accompanied by a total laxity of the under-jaw, the extreme of which is death. Firm strength is designated by a firm closure of the teeth, the last extreme of which is the elastic unnatural animal power, which imparts its convulsive violence to madness, and which, as well as anger, classically called a short mad- ness, is expressed by a vehement compression of the jaws or gnashing of the teeth. A rectilinear chin, said Mr. C, like a rectilinear forehead, is the ideal standard. All great philosophers have possessed an angularity of chin. Glut- tons, and men who sacrifice intellect to sense, the contrary. The chins of the fair sex are always smaller and chaster in their form than those of men. A chin that projects, un- less beyond a certain point, displays animal strength; that which recedes, animal! deficiency. The same rules, there- fore, which apply to the forehead apply to the chin. Nor is the mouth a less strong hiercglyphic than the eyebrow. Every one is aware of the distortion to which contempt and sensuality subject the mouth; but there is a more ge- neral and universally applicable axiom depending on this subject, for the forehead of brutes is not more dissimilar from that of man than their mouths. The intermediate degrees between them are pregnant with the same deduc- tions. A scale, therefore, may be applied to all the gra- dations of character in the human face; and if a scale, the Vol. 39. No. 170. June 1812. Hh ground 414 Earthquakes and Volcanic Phenomena ground plot for the elevation of physiognomy as a portion of the great scientific fabric is marked out and arranged. Mr. C. then descanted on the benefits which would re- sult from thus reducing physiognomy to something like a regular science; for man, as he is at present constructed, will and must form-some physiognomical opinions ; and it is surely much better that he should form them upon scien- tific principles, than on the vague suggestions of fancy or association. But Mr.C. protested against an individual assuming the right of judging his neighbour’s character in the present imperfect state of the study, or without long initiation, When, however, certain pathognomical indi- cations coincide, a very accurate judgement may certainly be formed by a student who has refined his perception of character by experience as well as rule. These indications may be discovered in the regular or irregular walk, in the erection or depression of the head, in the shortness or length of the neck, in the steadfast or wavering look of the eye, when the individual is engaged in conversation ; in the attitude or gestures, whether violent or relaxed, of the speaker; in the sound of the voice, whether base or treble, in the address, whether open, imposing, or retiring; and lastly, in the first words uttered on acquaintance. Mr. C. concluded by an interesting argument on the physiogno- mical effects of education, and the drama, which afforded us a degree of pleasure invariably our attendant when list- ening to his ingenidus inquiries. LXXIV. Intelligence and Miscetlaneous Arositert EARTHQUAKES AND VOLCANIC PH NOMENA IN THE WEST INDIES. Is the short space of time between the 26th of March and the 2d of May last, a succession of dreadful physical events has demolished some of the finest cities in South America, and shaken several of the islands to their foundations, wasting them with fire, and covering them with ashes and dust. The General commanding the troops of Coro de Domingo Campo Verde writes to the Governor of the pro- vince of Coro, that the city ef Barquisimeto was on the 26th of March buried in ruins by a most dreadful earth- quake. And he communicates the followimg moral event, which immediately succeeded. The inhabitants of the district, conceiving the phenomenon to have been an im- mediate manifestation of divine displeasure for having re- belled 4 in the West Indies. 475 bhelled against their sovereign, returned to their allegiance. ‘* All the villages,” says the General, ‘ belonging to this district and the city of Jouyo, with the greater part of the villages belonging thereto, have come and offered sub-. mission under the banners of Ferdinand VII.” and sub- sequently adds, “* By the panic and terror with which the inhabitants are struck- since the earthquake, | have no doubt that the army of Coro will eventually conquer the province of Venezuela.” During this terrible commotion of the earth, which appears to have -broken out at intervals between the g6th and 28th, the following cities were destroyed in the province of Coro: Barquisimeto, totally destroyed; Ari- Jaqua, sunk ; Santa Rosa, also sunk ; Caudare and Phelipe, destroyed ; and St. Charles and Caramavate greatly in- jered. In the province of Caraccas, the same calamity has. been equally tremendous. The cities of Caraccas, Victoria, Valencia, Porto Cavello, Laguira, New Barcelona, Mai- quetia and Cumana have been almost entirely ruined. The same or similar subterranean causes, which have so severely desolated the continent, about the end of April manifested their influence among the West Indian islands : and the following letters furmish several interesting and af- fecting circumstances. , Extract of a Letter from Barladoes, May 2. «© As faras I can relate, I will give you a true account of a most awful event, as witnessed and experienced bv myself. ‘¢] was lying in bed about six o’clock in the morning, when I observed my chamber more dark than usual. Some time after I arose and opened one of my windows, when I observed to the north a dark thick cloud, similar to the usual indication of a great deal of rain (which would have been very acceptable); but at the same time I perceived a most remarkable bright cloud to the southward; so much so, as to reflect light on the housés. We bad had what we conceived to be several rolling claps of thunder during the night, and the last was a quarter past seven, when an in- stantaneous total darkness ensued, and from that time till one o’clock I never saw so dreadful a phenomenon. I never beheld so dark a night in the gloomy month of No- vember ; in short, every thing appeared like chaos, and the lamps, handed about the streets in hundreds, were scarcely sufficient to give light to the persons who held them, much less to any one else. To paint the horror of the scene is utterly impossible. During the time of the dark- ness we were assailed by immense falls of calcareous matter (as I think) to such a degree that it was dangerous to go Hhe out 476 Earthquakes and Volcanic Phenomena out of the house: indeed it was impracticable to do so: without a hood or umbrella; and these were only tempo- rary screens, for by the time you had proceeded one yard you were completely covered by this stuff. «© At ten o’clock the rev. Mr. Garnett bad the church bells rung, and gave prayers: but such a scene of horror, dismay, terror, and consternation, cannot be imagined by one who did not see it. Thousands of people of all descrip- tions flocking to church, without rank or distinction, mis- tress and servant kneeling and praying by the side of each other, all fearing some dreadful catastrophe would hurry them out of the world before they could make their peace, and firmly believing they should never see the light again. I must confess to you I gave myself up, for the lava was gathering very fast on us, and no prospect but of starving or perishing under it. At first what fell was a large black substance, very coarse, but it gradually became as fine as Scotch snuff, and in a few hours the streets and the tops of the houses were many inches thick in this matter. _ About half past one o’clock a small.glimmering of light began to appear, and by half past two o’clock we could make out people mthestreets. It then gradually got lighter, so that we could see volumes of this matter floating in the air, but so thick as still to obscure the sun, nor have we yet seen the sun clearly. About half past six last night we saw like rays of fire in the southern quarter again. From all these circumstances | am led to think there must have been an explosion of some volcano very near us. To-day we have been busy in endeavouring to remove the lava, but I much fear, without we have a heavy fall of water to assist us, we shall be very long about it, and God only knows how it will end. The whole island is in one complete sheet of lava; the canes are all weighed down with it, and the | pour cattle and horses must die for want if we are not im- mediately relieved. We cannot see twenty yards before us for the immense volumes of this stuff continuaily falling from off the tops of the houses; for so soon as itis dry, it is exactly like flour. I am inclined to think now, the thun- der [thought Tf heard in the night was the explosion of some volcano. I herewith have sent you some of this dust, which [ hope you will receive safe.” Me To this we subjoin the account that has reached us from St. Vincent’s, where a volcano which had long been quies- cent has broken out with extraordinary violence. Extract of a Letter from St. Vincent, May 6.— Having been informed that you had not sailed from Grenada by the April fleet, I hasten to give you some account of a most alarming circumstance which took place here last night ‘in the West Indies. 477 and this morning. About sun-set, on Thursday evening, we observed an immense quantity of fire and smoke to proceed from the volcano, and continued till one o’clock this morn- ing, when a most tremendous explosion took place, and continued till four, throwing up immense quantities of stones and ashes all over the island. On the estates in the vicinity of the mountains the ashes are said to be from two to three feet deep ; that two of the principal rivers have been dried up, and new ones formed ; and that many of the estates in that quarter have been much injured. One white person and six negroes have been killed. Although Kings- ton is at the distance of about twelve miles from the volcano, the inhabitants were so much alarmed, that many of them went on board of the vessels in the bay for pro- tection, and it was not until past 8 o’clock that one person could distinguish another, in consequence of the atmo- sphere being darkened by the quantity of ashes. Iam much afraid that the extent of the damage sustained is not yet known.” — A second Communication from Mr. Wi1iu1amM Moors, on the Use of Oxymuriate of Magnesia in Bleaching. To Mr. Tilloch. S1r,—Since my former communication to you, I have received a letter from my brother (Mr. J. W. Moore, of Dublin), inclosing a copy of a letter he received from Mr. John Duppy jumor, relative to the use.of oxymuriate of magnesia by that enlightened gentleman in his manufactory near Dublin. ‘ ; I will thank you to add it (if possible) as an appendix to my former paper on this subject*: it is as follows: T have used the oxymuriate of magnesia on the large scale, ever since December 1810, and since then have been daily extending the application of it. To the communication T made Mr. Davy on this subject, 1 do not feel I could add any thing further, unless in generally stating my since ex- perience, as confirming its superiority over the oxymuriate of lime for whitening the grounds of delicate dyes, such as yellows, madder reds, &c.” The inaccuracy of Dr. Ogilby’s statements are still further confirmed by this second letter of Mr. Duppy’s; and although I did not entertain a doubt as to their fate in the scientific world yet they might deter the manufacturer, from adopting these improvements, Under these impres- sions I have been induced to trespass on your indulgence, I rgmain with respect, Your much obliged, | London, 25th June, 1812. Wm. Moore. * This communication reached us too Jate for insertion in the form wished by the author, 478 Meteorological Observations Copper and Manganese.—In the hill about a mile north of Stapleford, in Nottinghamshire, consisting of Gravel Rock, very similar to that of which Alderley-Edge NW _ of Mac- clesfield in Cheshire is composed, but not resting on and surrounded by Red Marl as that Hill does, but on and by Coal-measures, a vein of Ore of Manganese, Iron, and Copper, with much Mica, was lately discovered, on the Estate of Admiral Sir John Borlase Warren, Bart., who has caused some of the Ore to be smelted and the copper re- fined, which proves to be of the very best quality. Sir John had a Coal-seam seven feet thick Jatcly in work, about $00 yards S of this mine, and has proved the same Coal- Measures at about 4 or 500 yards N, while Lord Middle- ton’s large Collieries in Trowel are not more than 800 yards distant, in the same direction. ———_——— Meteorological Observations made at Clapton in Hackney, from May 21, to June 20, 1812. May 21.—W.S.W. Cloudy morning; afterwards rain, and long showers; fair, but damp evening: various clouds in the lucid intervals. — May 22.—N. Cloudy in the morning. Fine afternoon, but very cold with scud, and irregular masses of cumulus and cumulostratus. May 23.—N. Features of various modifications in dif- ferent heights. Fair day. May 24.—Clouded day ; in some places a wavy, in others ; mottled appearance of the sky: a little rain fell during the ay. May 25.—W.S.W. Small rain kept falling almost the whole of the day, but held up in the evening, which be- came fair. May 26.—Fine warm morning; eirrus, ciyrocumulus and cirrostratus in different altitudes, approaching to cumulo- stratus here and there; and a-sort of partial haze of a brownish colour floated gentle along in the south-west. Wind very calm. : May 27.—S. Fine warm day; cirrus, cirrocumulus, cirrostratus and cumuli irregularly disposed. May 28.—S. Clouds in two strata, followed by a fine warm rain in the evening. The sun appeared just ag it was setting, over a cirrostratus in the horizon; it appeared deep golden red, and threw a fine crimson blush op a cir- rostratus thinly diffused in a higher cat grate May 29.—S. All the modifications of cloud* appeared in made at Clapton. ATS in different stations, and fine petroid cwmuli in particular prevailed: slight showers in the course of the day: thunder showers at night. May 30.—Fine day; some lofty cirrus cloud and scud below sometimes appeared, but in general the clouds were of one character, particularly in the afternoon, being com- pact, but rather rocky cumuli. May 31.—Clouds in two strata, followed by nimbifica- tion; generally cloudiness by night with rising wind. June 1.—S.W. Rainy morning, but the rain was ge- nerally small. Evening irregular features of different clouds, and sun at intervals. Fine clear night. June 2.—W.S.W. Clear very early, then the sky be- came obscure; cumuli rose and general cloudiness pre- vailed; the day, however, became fair with various clouds. June 3.—S.W. Clouded morning, followed by some rain; fair afternoon ; the higher masses of cloud in dif- ferent strata put on the character of cirrocumulus ; indeed among others that kind of arge and clear feature of this cloud appeared which I have remarked to attend warm and healihy weather: cirrostratus, cumulostratus, &c. appeared, Night very clear. June 4.—S.W. Fine warm day, with diurnal cumuli, and some features of the other modifications; the clouds increased in the evening, but the night was fair. June 5.—W.S.W. Fine clear morning; in the day ap- peared cumuli ; evening cirri appeared aloft scattered irre- gularly. June 6.—Fine day, with cumuli; in the evening fine clear sky and beautifal yellow sunset, with lofty cirri scat- tered about, which became tinged with crimson. June 7.—S.E. Clouds early; fine clear dry day, with only a few little irregular cymudi here and there. June 8.—N. Cloudy in the morning; sun out by times in the day. Cloudy might again, and cooler than hitherto, June 9.—N.W. wind prevailed ; the morning was cloudy, the day became warm and fair, with masses of cumulus and some streaks of cirrus ; in the evening nimi, but no rain fel] hereabouts. : June 10.—N—E—SW. Sun and clouds in the morning ; cloudy evening, and rather warmer again towards night. June 1i.—Fair day ; some features of loose cirrocumulus early; cirvi scattered above, floating cumu/z below prevailed all day; the cirri in the evening became denser arid co- loured by the setting sun, and were accompanied by some cirrostrat}, June 480 Meteorological Observations made at Clapton. June 12.—Clouded morning ; cumuli, &c. per day; fine evening ; feature of cirrostratus. June 13.—W.S.W. Fine morning very early; about four o’clock I observed features of cirrocumulus, cirrus, &c. by about eight a mist, which had been coming on slowly, became thick, and the sky clouded; the afternoon was fair with much cloud. The evening clear, except some cirri and ctrrostrati. June 14. —SW—W. Very early the cirrus appeared breaking out into yarious and beautiful cirrocwmuli, and lower some cirrostratus seemed scattered along; the wind was quite calm, and the day became hot; cumudi sailed un- der the above clouds; cumulostratus formed, but subsided ; the evening was clear, except cirri fibrous and ramifying about in many directions and coloured by the setting sun *. June 15.—W.S.W. Fair day, with irregular features of several modifications in different altitudes ; the quantum of cloud increased in the afterncon, and wind rose. June 16.—S.W. Before light a hard shower, cumulo- stratus prevailed; fair afternoon with rows of plumose cirri, &c. June 17. —S.W—S. Very early cirrus confused and plumose with diverse kinds of loose cumuli ; then cumulo- stratus and hard showers, which prevailed all day; fair evening. June 18.—W—S.W. Fair morning, clouds in different altitudes; rainy evening and night, with pretty strong wind. June 19.—S.W. Wind and rain, which continued all night; also remained this morning: the day however be- came fair with cirrus and cirrocumulus aloft, and cumulé under nimbificaion commenced again in the evening with wind. June 20.—S.W. Showery, and rather windy all day. Fine evening; confused cirrus, cumulostratus, &c. as usual, between two nimlt. “Clapton, June 21, 1812. THOMAS FORSTER, * While the obliquely descending and angular fibres of the cirrus ap- peared to be equalizing the electricity of the surrounding air, they were also carried gently forward by the wind: (this shows that wind may pass. through a mass of atmosphere without destroying the inequality of its elec- tricity, which is slowly effected by the agency of ifs proper conductor, the cirrus. METEORO- Meteorology. METEOROLOGICAL TABLE, By Mr. Cary, OF THE STRAND, For June 1812. Thermometer. ‘aa at x Aaya ne oh cA Height of |‘% 8% 3 cothaed ae S 3 z the Bacon os A 2S cA ov. Inches. ag © | co ~ Qa May 27| 62 | 73°| 62°} 29°56 55 28| 60 | 66 | 63 °57 (6) 29 60 | 72 | 61 55 56 30) 61 | 70 | 60 82 60 31] 60 | 70 | 59 °75 48 June 1| 56 | 62 | 55 ‘78 e) 2| 55 | 67 | 59- 98 60 3| 56 | 60 | 53 | 30°00 Oo 4| 60 | 70 | 56 04 57 5| 61 | 69 | 54 05 50 6| 52 | 64 | 50 10 46 7| 53 | 65 | 52 16 49 8| 53 | 61 | 50 "22 53 9} 51 | 60 | 55 21 50 10| 50 | 57 | 48 28 46 11]| 55 | 70 | 62 -20 59 12) 62 | 72 | 6o 03 65 13| 59 | 70 | 62 | 29°94 60 14) 60 | 74 | 61 °84 65 15} 63 | 69 | 59 82 45 16] 56 | 65 | 52 *56 46 17; 52 | 55 | 50 "45 (0) 18] 51 | 62 | 49 *79 27 19} 52 | 57 | 50 34 36 20| 54 | 60 | 49 °37 40 21| 52 | 58 | 50 *52 10 23) 55 | 60 | 50 "89 35 24| 51) 63 | 54 “90 37 25) 53 | 66 | 54 *80 32 26) 53 | 52 | 48 "50 8) Ahn) Sy aa bal ee 481 Weather. Fair Rain Fair Fair Fair Rain Fair Rain Fair Fair Fair Fair Fair Fair Cloudy Fair Fair Fair Fair Cloudy Fair Rain Cloudy Stormy Stormy Stormy Showery Showery Showery Rain N.B. The Barometer’s height is taken at one o'clock, : f 482 j INDEX ro VOL, XXXIX. ACETATE of alumine, its use in dyeing, 180 Air. To free conduit-pipes from, 173 Alkaline matter in dropsical fluids, 122, 289 Allan's Dividing Instrument, 119; improved Reflecting Circle, 249 Alum, how used in dyeing, 175 Amber river. Description of, 196 Andree on Morbus Pedicularis, 49 Andrew s new solutionof two Fluxions proposed by Simpson, 363 Animal strengih as applied to ma- chines, 282 Antiquaries. Society of, 312 Antrim. Geological facts respecting, 266, 353 Aphelion of planets. What, 5 Architecture. Bridges, 409 Arsenic. Lambon, 311 Ascension, right. Tables for, 443 Astrop river described, 199 Astronomy. Syuopsis of elements of, 1; orbits of comets, 40, 85; tables for polar distance, &c. 448 Ainiosphere. Height of, 13 Attar of roses contains vegetable wax, i 423 Bailey’s synopsis of elements of as- tronomy, 1 Bakewell's lectures, 233, 313,469 Banks (Sir J.) Discovery by, re- specting snakes, 219 Barbadves. Remarks on, 465 Barton on Muscicapz, 107 Benexet’s way to found bridges, 410 Bennet’s account of Teneriff, 463 Bentham’s method of laying founda- tions under water, 409 Bistre. On, 461 Bitter-spar. On crystals of, 455 Bleaching with oxymuriates, 429, 477 Boilers. Way to convey steam from, 264 Books. New, 77, 217, 402, 458 Bootle rivulet described, 196 Boscovich on equations, 243, 400 Bradford river deseribed, 197 Bridges. On founding, 409 Brodie on poisons, 219 Brunton’s umproved pump, 862 Burne’s medical case, 117, 367 Camera obscura. Improved, 459 Campion on vision, 73 Campsie Hiils, Structure of the, 239 Carbonate of time. On crystals of, ; 455 Cary's Metereological Tatles, 80, 160 248 328, 408, 481 Cuvern, singular, described, 161 Ceres. Facts respecting, 5 Cheslire Rock-salt District, 210, 338 Clarkson on the Pyramids, 142 Ciaudius, (Emperor) his way to build in water, 409 Coal strata in Sutherland, 387 Coa!. Experiments on, 462 Cofferdam described, 409 Cold. On radiation of, 208 Comets. To determine orbits of, 40, 85 Conduit-pipes to free from air, 173 Consonances. 2 Of] styesvny s A \ ' Be “ [enppeey, Tle = - TPO MPOLL, vA ~S Nn Le on uojopsey a UOPSUP YINOL. pe =~ _ ot nee =e ‘ WUuPO Ss x CTALLEEHS os, eee 8 uyounnn(y a i 5 \ ace \ s \ ™~ : sHOY Ay = weyso Se IPL os es MOMIAINS PLEUY t . 6 . ’ e suas Kove Payor a 47 N Read \ “STH SALMA UVAN UNV NT Res Oe * Y VIMULS 9p JO SNOLIVIOTSIC JO SVTOVA ‘ AUOISTUA ‘es JOLM€ILT MYL JO YPRYS DY. Seale of Miles OL ZZ AGOTEGQWANRYBUG aly re iu ¥ , y ere + aE ij " . Wood, SEXIER PLT. uz Phil Mag Vol. XXXVX PLAN. rom lr. sis wpes 770m Qpparatus tor rreeing Water y By oN SO sn we b, \ S) \ N \ \\\ \ N ' ) \ ‘cP brhir soul 2 Bi): 4 ww 1. tle IY : Weve. “i Poet) wird Ms Tas PS eee aa = ee Sketeh of part af’ the Vountiinou, i(e DUBLIN, undry J, x anno Lay TK WE X F OR Dit Tiviz oe Qui Moors The Hills to the South of Dublin Bay.—tiom the Light House. Dathey. Lesser Sugar Loal, Quartz Greater Sugar Loar, Quart: Shonkhill. Quarts ’ Phal. Mag.Vol. XXX1X Fé MW" Brunton’ Improved Pump for Mines. : my aeewecueceeeetescesi tui TU \\ in cece maa IN % |W IU 3 = Nj s ? SSS) S. Porter ve. a= lL XXXIX LY c Mags Lhd. SS. ted Compa: sores Lypror “ eo M. Hodg i : : ‘ ‘ : ‘ m” olan pela Pk % : : ; phere . a f t w! DT 5 =f