■/J^^'rV"*' -i ^:/^<:^ m^-^'^ 5i^ /A ■ > ■ .^y^ U.X. 1. THE LONDON, EDINBURGH, and DUBLIN PHILOSOPHICAL MAGAZINE AND JOURNAL OF SCIENCE. CONDUCTED BY SIR DAVID BREWSTER, K.H. LL.D. F.R.S.L.&E. &c. RICHARD TAYLOR, F.L.S. G.S. Astr.S. Nat.H.Mosc.&c RICHARD PHILLIPS, F.R.S.L.&E. F.G.S. &c. SIR ROBERT KANE, M.D. M.R.I.A. " Nee aranearum sane textus ideo melior quia ex se fila gignunt, nee noster vilior quia ex alienis libamus ut apes. ' Just. Lirs. Polit. lib. i. cap. 1. Not. VOL. XXXL NEW AND UNITED SERIES OF THE PHILOSOPHICAL MAGAZINE, ANNALS OF PHILOSOPHY, AND JOURNAL OF SCIENCE. .JULY— DECEMBER, 1847. LONDON: RICHARD AND JOHN E. TAYLOR, RED LION COURT, FLEET STREET, Printers and Publishers to the University of London; SOLD BY LONGMAN, SHOWN, GREEN, AND LONGMANS J SIMPKIN, MARSHALL AND CO.; S. HIGHLEY ; WHITTAKER AND CO.; AND SHERWOOD, GILBERT, AND PIPER, LONDON : BY ADAM AND CHARLES BLACK, AND THOMAS CLARK, EDINBURGH ; SMITH AND SON, GLASGOW ; HODGES AND SMITH, DUBLIN ; AND WILEY AND PUTNAM, NEW YORK. ^K " Meditationis est perscrutari occulta; contemplationis est admirari perspicua Admiratio general qusestionenij qusestio investigationem, investigatio inventionera." — Hugo de S. Victore. CONTENTS OF VOL. XXXI. (THIRD SERIES.) NUMBER CCV.— JULY 1847. Page Sir J. Lubbock on the Perturbations of Planets moving in Eccentric and Inclined Orbits 1 Prof. Schoenbein on the Discovery^of Gun- Cotton 7 The Rev. B. Bronwin on the Inverse Calculus of Definite In- tegrals 12 Mr. W. R. Grove on certain Phajnomena of Voltaic Ignition and the Decomposition of Water into its constituent Gases by Heat 20 Mr. C. R. Weld on the Invention of Fluxions 35 Sir R. Kane's Researches on the Composition and Characters of certain Soils and Waters belonging to the Flax districts of Belgium, and on the Chemical Constitution of the Ashes of the Flax Plant 36 Dr. Schunck on the Colouring Matters of Madder 46 Comparative Analysis of the Urine of the Calf and the Sheep. . 49 Mr. Hind on the expected Reappearance of the celebrated Comet of 1264 and 1556 50 Messrs. G. Merck and R. Galloway's Analysis of the Water of the Thermal Spring of Bath (King's Bath) 56 Notices respecting New Books 67 Proceedings of the Royal Society 69 Action of Chlorine on Alcohol. — Formation of Acetal 77 Bisilicate of Iron or Ferruginous Pyroxene 78 Chlorosulphuret of Silicium 78 Meteorological Observations for May 1847 79 Meteorological Observations made by Mr. Thompson at the Garden of the Horticultural Society at Chiswick, near London ; by Mr. VeaU at Boston ; by the Rev, W. Dunbar at Applegarth Manse, Dumfries-shire ; and by the Rev. C. Clouston at Sand wick Manse, Orkney 80 NUMBER CCVI.— AUGUST. The Rev. N. J. Callan on a new Voltaic Battery, cheap in its construction and use, and more powerful than any Battery yet made ; and on a cheap substitute for the nitric acid of Grove's Platina Battery 81 Sir J. Lubbock on the Perturbations of Planets moving in Ec- centric and Inclined Orbits (^concluded) 86 Sir J. Lubbock on the Heat of Vapours 90 a2 IV CONTENTS OF VOL. XXXI. — THIRD SERIES. Page Mr. W. R. Grove on certain Phsenomena of Voltaic Ignition and the Decomposition of Water into its constituent Gases by- Heat (concluded) 91 Mr. \V. R. Grove's Supplementary Paper on certain Phaeno- mena of Voltaic Ignition and the Decomposition of Water into its constituent Gases by Heat . . ' 96 Sir D. Brewster on the Modification of the Doubly Refracting and Physical Structure of Topaz, by Elastic Forces emanating from Minute Cavities. (With a Plate) 101 Sir R. Kane's Researches on the Composition and Characters of certain Soils and Waters belonging to the Flax districts of Belgium, and on the Chemical Constitution of the Ashes of the Flax Plant (concluded) . . . . 105 Mr. J. P. Joule on the Theoretical Velocity of Sound 114 Mr. E. C. Nicholson on the Composition of CafFein, and of some of its Compounds 115 Prof. J. R. Young's Note in reference to the extension of Euler's Theorem 123 Prof. A. Connell on the Precipitate produced in Spring and River Waters by Acetate of Lead 124 Mr. J. Mercer on the Action of a mixture of Red Prussiate of Potash and Caustic Alkali upon Colouring Matters 126 Dr. W. Gregory on the Preparation of Hippuric Acid 127 Proceedings of the Cambridge Philosophical Society 130 Royal Astronomical Society 143 On a new Test for Prussic Acid, and on a simple method of pre- paring the Sulphocyanide of Ammonium, by Prof. Liebig . . 146 On the Fusion of Iridium and Rhodium, by R. Hare 147 On Testing the Comparative Value of Astringent Substances for the purposes of Tanning, by Robert Warington, Esq 150 On the two varieties of Arsenious Acid, by M. Bussy 151 On the Preparation of Gun-Cotton 152 On Balsam of Tolu, and some products derived from it 153 On the Equivalent of Titanium, by M. Isidore Pierre 155 On a modification of the Apparatus of Varrentrapp and Will for the estimation of Nitrogen, by Warren De la Rue, Esq 156 On the Detection of Cotton in Linen, by G. C. Kindt 157 The Planet Hebe 158 Meteorological Observations for June 1847 159 Table 160 NUMBER CCVIL— SEPTEMBER. Dr. T. Anderson on certain Products of Decomposition of the Fixed Oils in contact with Sulphur 161 Mr. J. P. Joule on the Mechanical Equivalent of Heat, as de- termined by the Heat evolved by the Friction of Fluids. ... 173 CONTENTrxW VOL. XXXI. — THIRD SERIES. V Page Letter from Prof. Schoenbein to Prof. Faraday, F.R.S., on a new Test for Ozone 176 Dr. G. Wilson on the Decomposition of Water by Platinum and the Black Oxide of Iron at a white heat, with some observa- tions on the theory of Mr. Grove's Experiments 177 Mr. J. J. Sylvester's account of a Discovery in the Theory of Numbers relative to the Equation Ax^ +By^ + Cz'^=Dxyz . . 189 Experiment made at the Kew Observatory on a new Kite- Appa- ratus for Meteorological Observations, or other purposes . . 191 Dr. L. Playfair on Transformations produced by Catalytic Bo- dies 192 Sir W. R. Hamilton on Quaternions ; or on a New System of Imaginaries in Algebra (continued) 214 Notices respecting New Books 219 Proceedings of the Royal Society 222 Suggestions for the observation of the Annular Eclipse, Oct. 9, 1847, made by the British Association for the Advancement of Science, Oxford, June 26, 1847 228 On the Preparation and Composition of the Salts of Antimony, by M. E. Peligot 230 Action of Hydrochloric Acid in the Formation of Oxalic Acid 233 Projection of Aldebaran on the Moon 233 The PufF Parliamentary : — Disinfection 233 A Grant of 200/. to Mr. William Sturgeon 236 Observations on Creatine, by M. Heintz 236 The New Planet Iris 237 Suggestions for Promoting the Science of Meteorology 238 Meteorological Observations for July 1847 239 Table 240 NUMBER CCVIIL— OCTOBER. Prof. E. Wartmann's Fourth Memoir on Induction. (With a Plate.) 241 Mr. S. M. Orach on eliminating the Signs in Star- Reductions. . 251 Mr. J. Brown on the Molybdate of Lead. 253 Dr. R. D. Thomson's note on a new Test for Arseniates, &c.. . 258 Mr. E. W. Binney on Fossil Calamites found standing in an erect position in the Carboniferous Strata near Wigan, Lanca- shire 259 Mr. E. Frankland and Dr. H. Kolbe upon the Chemical Consti- tution of Metacetonic Acid, and some other Bodies related to it 266 Messrs. T. H. Rowney and H. How's Analysis of the Ashes of the Orange-Tree (Citrus aurantium) 271 Sir W. R. Hamilton on Quaternions ; or on a New System of Tmaginaries in Algebra (continued) 278 tl CONTENTS OF VOL. XXXI. — THIRD SERIES. Page Mr. J. J. Sylvester on the Equation in Numbers Ax^+By^ + Cz^ s^Dxyz, and its associate system of Equations (continued) . . 293 Mr. R. Taylor on the Invention and First Introduction of Mr. KcEnig's Printing Machine 297 Proceedings of the Cambridge Philosophical Society 301 On the Artificial Production of Minerals, and especially of Pre- cious Stones 311 Analysis of Kupfemickel 314 On the Dehydration of Monohydrated Sulphuric Acid 314 Observations on Silica, by M. Doveri 315 On Nitric Mannite, by M. Sobrero 316 On the Extraction of Silver, by MM. Malaguti and Durocher 317 Vanadiate of Lead and Copper 319 Meteorological Observations for August 1847 319 Table 320 NUMBER CCIX.— NOVEMBER. Prof. M. A. De la Rive's Researches on the Voltaic Arc, and on the influence which Magnetism exerts both on this Arc and on bodies transmitting interrupted Electric Currents . . 321 Mr. T. Richardson's Analyses of the Ashes of Rough Brown Sugar and Molasses 336 Letter from Prof. Loomis of the New York University to Lieut.- Colonel Sabine, Foreign Secretary of the Royal Society, on the determination of differences of Longitude made in the United States by means of the Electric Telegraph, and on projected observations for investigating the Laws of the gi-eat North American Storms 338 The Rev. B. Bronwin on the Algebraic Equation of the Fifth Degree 341 Letter from Capt. J. H. Lefroy, R.A., Director of the Mag- netic Observatory of Toronto in Canada, to Lieut. -Colonel Sabine, R.A., on a great Magnetic Disturbance on the 24th of September 1847 346 Dr. H. Kolbe on the Decomposition of Valerianic Acid by the Voltaic Current 348 Mr. R. Adie's Account of Experiments with Galvanic Couples immersed in pure water and in oxygenated water 360 Dr. R. Hare on certain Improvements in the Construction and Supply of the Hydro-Oxygen Blowpipe, by which Platinum may be fused in the large way , 356 Dr. J. W. Griffith on the Composition of the Bile of the Sheep 366 The Rev. J. Slatter's Notice respecting the Meteor of Septem- ber 25, 1846 368 Mr. J. Glaisher on the Aurora Borealis, as it was seen on Sun- day evening, October 24, 1847, at Blackheath 369 CONTENTS OF VOL, XXXI.— THIRD SERIES. Vll Page Proceedings of the Royal Society 372 ■ Cambridge Philosophical Society 376 Royal Astronomical Society 380 On the Gelatinous Substances of Vegetables 389 Preparation of Protoxide of Tin 392 On the Presence of Arsenic, Copper and Tin, in the Mineral Waters of Bavaria 392 Solubility of Common Salt in Alcohol 393 On some Improved Forms of Chemical Apparatus, by Thomas Taylor, Esq 393 Preparation and Composition of Lignin 397 Solubility of Chloride of Silver in Hydrochloric Acid 398 Daubeny on Active and Extinct Volcanos 399 Meteorological Observations for September 1847 399 Table 400 NUMBER CCX.— DECEMBER. Prof. M. Faraday on the Diamagnetic conditions of Flame and Gases 401 Prof. Zantedeschi on the Motions presented by Flame when' under the Electro- Magnetic Influence 421 Mr. T. Weddle on Asymptotic Straight Lines, Planes, Cones and Cylinders to Algebraical Surfaces 425 Mr. R. A. Couper on the Chemical Composition of the Sub- stances employed in Pottery 435 Sir D. Brewster on the Polarization of the Atmosphere 444 Mr. A. Smith on the Hydx*ates of Nitric Acid 454 Mr. F. Field on the Products of the Decomposition of Cuminate of Ammonia by Heat 459 Mr. J. J. Sylvester on the General Solution (in certain cases) pf the equation j:'^-\-i/^-\-Az^ = Mxyz, &c 467 Mr. W. De la Rue on Cochineal {Coccus Cacti). First Memoir 471 NUMBER CCXI.— SUPPLEMENT TO VOL. XXXI. Mr. W. De la Rue on Cochineal (Coccus Cacti). First Memoir (concluded) 481 Sir D. Brewster on the Existence of Crystals with different pri- mitive forms and physical properties in the Cavities of Mine- rals ; with additional Observations on the New Fluids in which they occur. (With a Plate.) 497 Mr. L. Thompson's Observations on Chloric Acid and the Chlorates 510 Vni CONTENTS OP VOL. XXXI. — THIRD SERIES. Page Prof. Sir W. R. Hamilton on Quaternions ; or on a New Sy- stem of Imaginaries in Algebra (continued) 511 Mr. J. H. Gladstone's Contributions to the Chemical History of Gun-Cotton and Xyloidine 519 Proceedings of the Royal Astronomical Society 528 On Osmiamic Acid, by MM. J. Fritzsche and H. Struve .... 534 On the Preparation and Properties of some Osmiamates, by MM. Fritzsche and Struve 535 On Sulphato- chloride of Copper, — a New Mineral, by Arthur Connell, Esq '. 537 On the Formation of Valerianic Acid, by M. Therault 538 Note on the Measurement of the double Sulphates of Zinc and Soda, and of Magnesia and Soda, by W. H. Miller 540 Native Carbonate of Nickel 541 An Examination and Analysis of the " Nadelerz," or needle ore of Bismuth, by E. .T. Chapman, Esq 541 Action of Anhydrous Phosphoric Acid on Ammoniacal Salts, by M. Dumas 544 Meteorological Observations for October 1847 545 Table 546 Index 547 PLATES, I. Illustrative of Sir D. Brewster's Paper on the Modification of the Doubly Refracting and Physical Structure of Topaz, by Elastic Forces emanating from Minute Cavities. II. Illustrative of Prof. Wartmann's Fourth Memoir on Induction. III. Illustrative of Sir D. Brewster's Paper on the Existence of Crystals with different primitive forms and physical properties in the Cavities of Minerals. Erratum in Mr. Sylvester's paper, p. 189 Line \^,for Ti'xyz read D'uviv. Errata in Sir Graves C. Haugaton's paper, vol. xxx. p. 437. P. 445, in the thirteenth line from the bottom,/or M024 read 1,1024. ninth line from the bottom,/o;- 256° read 256. — 456, in the third line from the bottom,/o;- Hare hair read Horse hair. — 518, in the thirteenth line from the bottom,/or oxide of hydrogen read protoxide of hydrogen. — 522, in the fifteenth line froni the top,/o>" in fault read at fault. THE LONDON, EDINBURGH and DUBLIN PHILOSOPHICAL MAGAZINE AND JOURNAL OF SCIENCE. [THIRD SERIES.] JULY 1847. I. On the Perturbations of Planets moving in Eccentric and Inclined Orbits. By Sir J. Lubbock, Bart.i F.R.S.* nPHE accuracy of the tables which give for an indefinite -*■ time the places of the older planets, is at present sufficient for the purposes of astronomy, and is commensurate with the accuracy of observation ; or if this statement appears to be exaggerated, it will at least be admitted that the sensible errors which remain are owing rather to inadvertence in the numerical computation than to the imperfection of the method itself. Such a result is owing to the uninterrupted labours of the greatest mathematicians from the time of Newton, and is justly regarded as one of the greatest triumphs of human in- telligence. But it must be recollected that these methods, by which the perturbations of the older planets have been obtained, are applicable only to the case of orbits nearly cir- cular, and little inclined to each other; so that the general solution of the problem of the three bodies, as it is called, remains to the present day imperfect. The methods in use for the older planets are founded, as is well known, upon the development of the disturbing function in terms of the mean anomalies. M. Binet has indeed carried this development to quantities of the seventh order inclusive ; but such a de,velop- ment is quite insufficient in the case of comets or planets moving in highly eccentric and inclined orbits, which problem presents far greater difficulty ; while the nature of the expres- sion is such, that it is evidently impracticable to carry further such a mode of development, even if the expressions were suf- ficiently convergent when the eccentricity passes a certain limit. The only memoir with which I am acquainted which pro- * Communicated by the Author. Phil. Mag. S. S. Vol. 31. No. 205. Juli/ 1847. B 2 Sir J. Lubbock on the Perturbations of Planets fesses to give a general solution of the problem otherwise than by mechanical quadratures, is clue to M. Hansen. This im- portant work is translated in the Co7in. des Temps for 1847. That great mathematician has considered the case when r< r', that is, when the disturbed body is inferior; and has illus- trated the question by the numerical calculation of the per- turbations of the comet of Encke by Saturn. M. Hansen develops the disturbing function according to multiple angles of the eccentric anomaly of the disturbed planet literally; and first, according to multiple angles of the true anomaly of the disturbing planet; M. Hansen next converts the cosines and sines of the multiple angles of the true anomaly of the disturb- ing planet into sines and cosines of multiple angles of the mean anomaly of that planet; so that finally the disturbing function is exhibited in terms of the eccentricanomaly of the disturbed planet and the mean anomaly of the disturbing planet ; but those series which serve to give the sines and cosines of the multiples of the true anomaly, in terms of sines and cosines of the mean anomaly, are not very convergent ; and the pro- cess becomes extremely laborious, even in the case which M. Hansen has considered, in which, in consequence of the great distance of Saturn, the approximation does not require to be carried nearly so far as in the case of the perturbations of the same comet by Jupiter, and in many others which may require consideration. Moreover, in this as in every other mode which can be devised of developing the disturbing function literally, all quantities must be retained of a given order ; although when they are of a different sign, in many instances they destroy each other ; but such reductions cannot be fore- seen. The numerical substitutions are also extremely labo- rious, in consequence of the multitude of terms which have to be considered. As the disturbing function, and others which require to be integrated, are finally exhibited by M. Hansen in terms of two variables, such that direct integration is impossible, M. Hansen has recourse to the integration ^ar joar/zW, in which each term by integration gives rise to a series of other terms, the nature of which is complicated. The method which I propose differs from that suggested by M. Hansen in every particular. Instead of attempting a literal development, I insert the numerical values of the ellip- tic constants in the earliest possible stage : by this means the radical, which expresses the mutual distance of the planets, is explicitly a function of sines and cosines of various angles with numerical coefficients. When r < r', I develop in terms of the eccentric anomaly of m, after having obtained expres- moving in Eccentric and Inclined Orbits, 3 sions for the co-ordinates of w' in terms of the eccentric ano- maly of m. Such expressions are very easy to obtain, and are very convergent. It will be recollected that before I endea- voured to develop the disturbing function in the lunar theory in terms of the mean motions of the sun and moon, the inva- riable practice had been (see MeQunique C6leste, vol. iii. p. 189) to express the co-ordinates of the sum in terms of the true longitude of the moon ; but the equation which connects the eccentric anomalies of two bodies is far simpler than that which connects the true anomalies, or xf and t;, and therefore the conversion which I employ is made with greater facility. The quantity under the radical sign in R may thus be considered as a function, of which the general term can be represented by sin /. , ., n' \ ^cosr + ^VV' a being a numerical quantity. The development of this 13 quantity to the power — ^ or — -, may be facilitated by the use of tables, which give the numerical coefficients in the development of {l—u4 cos a} ~^, {1— y4cos«}"% &c. Such tables have been calculated for me by Mr. Farley. By pro- ceeding in this way, no term is ever introduced which affects the final result beyond a given place of decimals. For the development of the radical admits of being exhibited in the form >4 + -B+C+Z) + &c.; such that 5=a^(a, C=(35(a, D=:yC(a, so that each term is deducible from the one which precedes it, by the multiplication of that term by a(B, /3®, &c., a, /3, y, &c. being proper fractions. If therefore the terms in the two quantities which form those products, such, for instance, as oiA and <^ which form B, are sorted and arranged in the order of their numerical magnitude, as soon as any one partial product sinks below any limit that may be assigned, all the succeeding terms are necessarily of inferior magnitude ; and the approximation stops, as it were, of itself, without any exercise of thought on the part of the computer. When r > r', that is, when the planet disturbed is superior to the disturbing planet, I am not able to suggest any other course than to develop in terms of the true anomaly of the dis- turbed planet, and the mean anomaly of the disturbing planet, B2 4 Sir J. Lubbock on the Perturbations of Vlanets and to integrate par parties. I have obtained the law of the coefficients in the series which resuhs in this process, and they are highly convergent. I am confident that, by the processes which I have attempted thus so briefly to describe, the per- turbations of planets moving in orbits, however eccentric and inclined, may be calculated jvith nearly as great facility as they are given by existing methods, in orbits nearly circular and in the same plane, and may be exhibited in tables, giving their values for an indefinite period, if required. If these me- thods, which I have described in detail elsewhere, possess the advantages which I ascribe to them, I hope the time is not distant when the perturbations of Pallas and of some of the comets may be reduced to a tabular form; but as the labour will be very considerable, it will be necessary to limit the in- quiry in the commencement to the cases of the greatest emer- gency. Although my methods are specially adapted to the deter- mination of the perturbations of bodies moving in eccentric orbits which cannot be developed in terms of the mean mo- tions, yet they embrace also the case of a planet moving in an orbit nearly circular ; and it is easy to show in what manner the labour is increased by the greater eccentricity. If the reciprocal of the radical which expresses the mutual distance of the planets be called the chief difficulty arises in developing {1+P}~5. If the numerical values of the elliptic constants are introduced, 1 +P=1— ^1 cos «!— ^2^08 «2 + &c.. Ay, A^ &c. are numerical coefficients, which I here suppose ranged in the order of their numerical magnitude. I make {1— -4iCosa,}{l— ^gcosag} • • • • {1— ^;COSa,.} = H-P+Q, including a limited number of terms in 1-|-P+Q. {l-^jcosai}"^, {1— .^gcosag}"^ &c., can be obtained at once by means of a table. But as the coefficients given by such a table do not readily furnish, by interpolation, the values required unless it be considerably extended, I take for A^, A^, &c. the nearest value given by the table, and I leave the residue to form part of Q. In this way it will generally be found sufficient to include not more than six terms in 1+P+Q, so as to leave Q consisting of 2-p- 72\» ^ ^^ ^^^^ angle included by lines drawn from moving in Eccentric and Inclined Orbits. 5 terms of which the coefficients are each below •! in numerical value, and the quantity {1 +P}"i^ can be developed accord- ing to powers of Q in a rapidly converging series. „ , 2)]^ a' r so 1+P=1 ^-r— COS^+ljV ' (T ?•' a '^ 2^_ 2aa' «'"2 r^ the sun to m and m\ p= -^ -^ — 1. 2y\^ a! r The terms contained in r- cos 8 obviously exceed fj r a •' greatly in magnitude those contained in )j^^, - cos 8=2 cosy 4- k siny ; f being the true anomaly of m', and u the eccentric anomaly ofw, i= — e^4-^cos 0— 'V^l —e^% sin y, ^=— eC + C cosy + ^1— e^Ssiny; S[, 93, C and 19 being constants, each necessarily less than unity, which depend only on the inclination of the orbits and the position of their line of intersection, and such that when they are in the same plane ^ = ja and 33 = C. The process is precisely the same in substance, whether the orbit of m is highly eccentric and inclined, or circular, and in the same plane with that of ;«' ; the only difference being that, while in the former case it may be necessary to detach as many as six terms to form the quantity 1+P+Q, in order that Q. may not contain any term of which the numerical coefficient exceeds •! in magnitude ; in the latter case, supposing e' the eccentricity of w' to be inconsiderable, 1+P+Qwill only contain one factor, and therefore {1+P+Q}~^, &c. can be calculated with greater facility. Thus, for example, in the perturbations of Pallas by Saturn, it is convenient that 1+P+Q should contain three terms. Pallas by Jupiter, it is convenient that 1+P+Q should contain four terms. Encke's comet by Saturn, it is convenient that 1+P+Q should contain five terms. Encke's comet by Jupiter, it is convenient that 1+P+Q should contain six terms. 6 Sir J. Lubbock on the Perturbations of Planets. And then in each of these examples Q will contain no term of which the coefficient exceeds -1 in numerical amount. If ^ - 1+P + Q {\+P]-^ = A + B-\-C+D, ^=(l + P+Q)-t, 5=|(a^, C=~(^B, o o The calculation of {1 +P+ Q}~^ is much facilitated by the use of a table which gives the values of the coefficients of {1— ^cosa}"^ -J and 1 +Pcontam terms multiplied by ~j-cosj', -jsmj', -j, and -j2, and none others require consideration. If the eccen- tricity of m' is small, they may be developed in terms of ^', the mean anomaly of m'; and it will be sufficient to consider the terms depending on cos ^'5 cos 2^', cos 3^', sin g', sin 2^', sin 3f'. If/ is the time reckoned from the time of the perihelion passage of w, r-, L w J sin ?^'=sin I < U' e sin 0 > ; and as — is a fraction, cos /^'and sin i^' can be developed in a series rapidly converging, and containing explicitly only the variable quantity u. [To be continued.] [ 7 ] II. On the Discovery of Gun' Cotton. By Professor Schcenbein*. THE substance to which I have given in German the name o'i schiesswolle^ and in English that of gun-cotton, having excited a lively curiosity, it may be interesting to the scientific world to become acquainted with some details of the way in which I was first led to its discovery. The results of my researches on ozone led me in the course of the last two years to turn my attention particularly to the oxides of nitrogen, and principally to nitric acid. The nu- merous experiments I have made on this subject have led me, as I have stated in detail in Poggendorff''s Ajinalen, to adopt a peculiar hypothesis on the so-called hydrates of nitric acid, sulphuric acid, &c., as well as on the normal nitrates, sulphates, &c. For a long time I had entertained doubts as to the exist- ence of compound bodies of this nature, which cannot be isolated, and which are stated to be capable of existing only in combination with certain other substances ; for a long time also I had come to the notion that the introduction of these imaginary combinations had only been an apparent progress in theoretical chemistry, and that it had even impeded its development. It is well known that what has most contributed to the admission of the existence of these compounds has been the opinion generally received among chemists respecting the nature of nitric acid. Starting from the existence of the com- pound of nitrogen NO5, as an undoubted and demonstrated fact, notwithstanding the impossibility ofisolating it, they always cite nitric acid to prove the existence of compounds which cannot exist in an isolated state. In my opinion, there is no degree of oxidation which is represented by NO5, and what these chemists designate by the formula NO5+HO must be considered as being really NO4+HO2; 1 am even inclined to regard the normal nitrates NO5+ RO, as compounds which must be expressed by NO4 + RO2. Amongst other motives which induce me to admit this opinion, I will mention the fact that we can obtain hydrated nitric acid or a normal nitrate by the direct mixture of NO4 with HO2 or ROg. Other consi- derations, which I have had occasion to detail elsewhere, in- duce me also to consider hydrated sulphuric acid to have the form SOa-f HO2, and not that of SOg+HO, and a normal sulphate that of SO2 + RO2. It is sufficient here to observe that SO2 placed in presence of HOg gives rise to what is * From the Archives des Sciences Physiques et Naturelles, 8 Prof. Schoenbein on the Discovery of Gun-Cotton. called hydrated sulphuric acid, and that SO^ placed in pre- sence of BaOg or PbO^ gives rise to what is called sulphate of the oxide of barium or of lead. Rose's compound, to which the formula 2SO3 + NO2 has been assigned, should have, in my opinion, 2863+ NO4. Admitting this, I considered it probable that the mixture of 2(S02+H02) ( = 2(803+00)) with NO4+HO2 ( = N05+H0) yields 28O2+NO4, and that at the same time SHOg is disengaged, or enters into a loose combination with what is called the bisulphate of deutoxide of nitrogen. In other words, I conjectured that a mixture formed with the hydrates of nitric acid and sulphuric acid would possess a very great power of oxidation, and would form a kind of aqua regia, in which the combination HOg would act the part of the chlorine. On this hypothesis, and abstracting HO2 from the acid mixture by means of a proper oxidable body, there ought to remain Rose's compound. Guided by these suppositions, which, I admit, may be as little founded as they are contrary to the ideas received among chemists, I commenced in December 184-5 a series of experi- ments with a view to put my hypothesis to the proof: it will be seen in the sequel whether the results at which I arrived tend to confirm it. I mixed some flowers of sulphur and a certain quantity of the acid mixture of which I have spoken : immediately, even at the temperature of 32° F., a lively disengagement of sulphurous acid gas took place without the production of deutoxide of nitrogen. After the reaction, which was accom- panied by a development of heat, there remained a colourless liquid, which, mixed with water, disengaged a considerable quantity of deutoxide of nitrogen, and acted generally as a solution of Rose's compound in hydrated sulphuric acid would have done. I should add here, that a mixture of four ounces of hydrated sulphuric acid with a single drop of nitric acid, on the addition of flowers of sulphur, disengages a sensible quantity of sulphu- rous acid. To assure himself of the presence of the latter, the operator has only to hold over the liquid a strip of paper which has been covered with iodide of potassium paste, and tinged slightly blue by exposure to chlorine. The liberated sulphu- rous acid will soon dissipate this blue colour. Selenium and phosphorus are oxidized in the same manner at low temperatures in the acid mixture in question ; and this latter is modified to such an extent, that, on the addition of water, an abundant disengagement of deutoxide of nitrogen gas takes place. Iodine even, in the state of powder and shaken up with the Prof. Sclioenbein on the Discoveiy ()f Gun-CoUon. 9 acid mixture, rapidly absorbs oxygen, when exposed to a low temperature; and there is formed, besides iodic acid, the compounds to which Millon has lately drawn attention. After the reaction a li(|uid remains, which, diluted with water, gives an abundant disengagement of deutoxide of nitrogen and liberates iodine. My experiments on ozone having shown that this body, whicfi I consider to be a distinct peroxide of hydrogen, forms, as well as chlorine, at the ordinary temperature, a peculiar compound with olefiant gas, without apparently oxidizing in the least either the hydrogen or the carbon of this gas, I had the idea that it would not be impossible that certain organic matters, exposed to a low temperature, would likewise form compounds, either with the peroxide of hydrogen alone, which, on my hypothesis, occurs in a state of combination or of mix- ture in the acid mixture, or with NO4. It was this conjecture, doubtless very singular in the eyes of chemists, which princi- pally led me to commence experiments with common sugar. I made a mixture of one part (volume) of nitric acid, of 1*5 spec, grav., and two parts of sulphuric acid of 1'85, at the temperature of 36° F. ; I then added some finely powdered sugar, so as to form a very fluid paste. I stirred the whole, and, at the end of a few minutes, the saccharine substance formed itself into a viscous mass entirely separated from the acid liquid, without any disengagement of gas. This pasty mass was washed with boiling water, until this last no longer exer- cised any acid reaction ; after which I deprived it, as much as possible, at a low temperature, of the water it still contained. The substance now possessed the following properties: — Ex- posed to a low temperature, it is compact and brittle ; at a moderate temperature, it may be moulded like jalap resin, which gives it a beautiful silky lustre. It is semi-fluid at the temperature of boiling water ; at a higher temperature, it gives off red vapours ; heated still more, it suddenly defla- grates with violence, without leaving any perceptible residue. It is almost insipid and colourless, transparent like the resins, almost insoluble in water, but easily soluble in the essential oils, in aether and concentrated nitric acid, and in most cases it acts in general like the resins in a chemical and physical point of view : thus friction renders it very electro-negative. I will add, that the acid mixture, by means of which this resi- nous body was obtained, has an extremely marked bitter taste. I wished to make experiments also with other organic sub- stances ; and I soon discovered, one after another, all those about which there has been so much said of late, especially in the Academy of Paris. All this passed in December 1845, 10 Prof, Schoenbein on the Discovery of Gun-^Cotton. and the first few months in 1846. In March, I sent speci- mens of my new compounds to some of my friends, in parti- cular to Messrs. Faraday, Herschel and Grove. It is neces- sary to note expressly that the gun-cotton formed part of these products; but I must add, that hardly was it discovered when 1 employed it in experiments of shooting, the success of which encouraged me to continue them. Accepting the obliging invitation which I received, I went in the middle of April to Wurtemburg, and made experiments with gun-cotton both in the arsenal of Ludwigsburg, in the presence of artillery offi- cers, and in Stuttgard, before the king himself. In the course of May, June and July, with the kind cooperation of the Commandant de Mechel, of M. Burkhardt, captain of artil- lery, and other officers, I subsequently made in this city (Bale) numerous experiments with arms of small calibre, such as pistols, carbines, &c., and afterwards with mortars and can- non,— experiments at which Baron de Kriidener, the Russian ambassador, was several times present. I may be allowed to mention, that I was the person who fired the first cannon loaded with gun-cotton and shot, on the 28th of July, if I remember aright, after we had previously ascertained, by ex- periments with mortars, that the substance in question was capable of being used with pieces of large calibre. About the same time, and indeed previously, I employed gun-cotton to blast some rocks at Istein in the Grand Duchy of Baden, and to blow up some old walls at Bale ; and in both cases I had opportunities of convincing myself in the most satisfactory manner, of the superiority of this new explo- sive substance over common gunpowder*. Experiments of this kind, which took place frequently and in the presence of a great number of persons, could not long remain unknown ; and the public journals soon gave, without participation on my part, descriptions, more or less accurate, of the results which I had obtained. This circumstance, joined to the short notice which I inserted in the May number of Pog- gendorff's Annalen, could not fail to attract the attention of German chemists : in the middle of August I received from M. Boettger, Professor at Frankfort, the news that he had succeeded in preparing gun-cotton and other substances. Our two names thus became associated in the discovery of the sub- stance in question. To M. Boettger the gun-cotton must have been particularly interesting, as he had previously discovered an organic acid which deflagrates readily. In the month of August I went to England, where, assisted * In tlie month of June I made also the first capsules, and employed them with success for muskets, in the presence of the above-named officers. Prof. Schoenbein o« the Discovery of Gun-CoUon, 11 by the able engineer, Mr. Richard Taylor of Falmouth, I made numerous experiments in the mines of Cornwall, which were entirely successful, in the opinion of all competent wit- nesses. Experiments on the action of gun-cotton were also made in several parts of England, under my direction, both with small fire-arms and with pieces of artillery, and the re- sults obtained were very satisfactory. Until that time there had been little or nothing said of gun-cotton in France ; and it will appear that the short notices which Mr. Grove gave at Southampton at the meeting of the British Association, and the experiments with which he ac- companied them, served first to attract the attention of French chemists to this substance. At Paris, the thing was at first considered hardly credible, and jokes even were passed upon it ; but when there could no longer remain any doubt as to the reality of the discovery, and when several chemists in Germany and other countries had published the processes which they employed to prepare the gun-cotton, then a lively interest was manitiested in a subject which had just before ex- cited derision, and it was soon pretended that the new explo- sive substance was an old French discovery. It was declared to be nothing more than the xyloidine first discovered by M. Braconnot, and afterwards investigated anew by M. Pelouze, and the only merit left me was to have conceived the happy idea of putting this substance into a gun-barrel. The know- ledge of the composition of xyloidine ought to have sufficed to convince those who put forward that opinion, that it is not suited for fire-arms, on account of its containing too much carbon and too little oxygen for the chief part to be converted into gaseous matters during the combustion. It was moreover very easy to discover the essential differences which exist be- tween the xyloidine of Braconnot and gun-cotton. Never- theless the error was kept up for some months. Matters stood thus, when, on the 4th of last November, a Scotch chemist, Mr. Walter Crum of Glasgow, published a memoir, in which he showed that gun-cotton is not the same product as xyloidine, but that it presents an essentially differ- ent composition ; and towards the end of the same month, the French Academy received a communication of the same na- ture. The gun-cotton was then no longer xyloidine, it was called pyroxyloidine, and the first was admitted to be unsuit- able for fire-arms. If, therefore, it is proved that from the commencement of 1846 I prepared gun-cotton, and applied it to the discharge of fire-arms, and that M. Bcetlger did the same in the month of August, — if it be admitted that xyloidine cannot serve the 12 The Rev. B. Bronwin on the Inverse Calculus same purposes as this cotton, and if it be notoriously known that what is now called pyroxyloidine was not brought before the French Academy and the scientific world until towards the middle of last November, the idea of attributing to France the discovery of gun-cotton cannot be seriously entertained, or of assigning to me merely a practical application of that which another would have discovered. I appeal to the justice of Frenchmen, to decide the point to whom belongs the honour of not only being the first to apply the new substance in question, but also of having first pre- pared it — to MM. Braconnot and Pelouze, or myself. I must, moreover, add expressly, that it was not xyloidine even which led to my discovery, however intimate may be its rela- tion with gun-cotton ; it was theoretical ideas, possibly very erroneous ones, but which are peculiarly my own, as well as some facts which I was also the first to discover. Suum cuique is a principle of morality on which society at large rests ; why should it not be strictly respected in the republic of sci- ence? M. Pelouze is a distinguished chemist, and already possesses a sufficiently high reputation not to require to ele- vate his pretensions on the merits of others ; and I am fully persuaded that this estimable chemist, of well-known truth of character, will, appreciating with impartiality the circum- stances which have occurred, freely render me the justice to which I consider myself entitled. Bale, Dec 28,1846. III. On the Inverse Calculus of Definite Integrals. ^ By the Rev. Biiice Bronwin*. "T^HIS paper contains several very simple and easy methods ■■ in the inverse calculus of definite integrals; and they show that the function under the sign of integration may have more than one form. The exponents n and p are always positive, and n+p = i an integer. First, let (p{x)='ZAmX"^i an ascending series. Then =2A;„a'"+'* /" x'^-^dx{\^x)'^ = r(w)2;A^«-+« r^^'^^^^j) =4'(«) suppose. * Communicated by the Author. of Definite Integrals. 13 Tlien also and or Operate with ( y j on both members, and we have by making a— ;r = «t;. Therefore A Next, let (p (a?) = 2-^, a descending series. Then ^ A;;, Tlm—n) ,, , and or (2.) 14 The Rev. B. Bronwin on the Lwerse Calculus Operate with (— j on both members; then {-iyT{n)T{p)^ ^ = {£)J^ ^v-d,^a + a^) ; or ^ 0 We may put ip [a) under a different form by making a+d?= -. The forms of f [a) obtained in (1.) and (2.) differ from those given by Mr. Boole in the Cambridge Mathema- tical Journal, No. 20 ; but by varying the process a little, we might obtain his results. We may observe that the least valueof 7win(l.) must be greater than (—1), and in (2.) greater than n+p or /. In (p(^) = e^^(p(0), which is Taylor's theorem (D standing for -r-), change (^[x) into

{a—x)', nn)np) Y{S^rU) "''^'■^^^°) ^fo""'" ^-^^(^-^^ Operating with ( y-) on both members, we find of Definite Integrals. [5 the same result as in (1.). In (a.) change

— f(a) Change the function e-''*'(p(^) into -'*(>-^)'-P=2»4'(^)='/^. {K0}V)=|(f). and , V 1 then 4/(a)='/a, as it should be. In (2.) let We find In the last example n and p are not conformed to the re- strictions, but the infinite quantity goes out by differentiation. The theorems (3.) and (4.) are likewise satisfied by these ex- amples. It must not be supposed that the values of

quantities undetermined. Urea Urinary animal matter Hippurate of potash Bicarbonate of potash Carbonate of lime Mucus Oxide of iron . . * From the Annates de Chimie et de Physique, Juin 1847. Phil. Mag. S, 3. Vol. 3 1 . No. 205. My 1 847. E 50 Mr. Hind on the expected Reappeaj-ance of IX. On the expected Reappearance of the celebrated Comet of 1264. and 1556. By Mr. Hind*. '^I'^HE time is now near at hand when the return of the comet -*- of 1264) and 1556, signalised by Mr. Dunthorne and M. Pingre, may be expected to take place. It is therefore de- sirable that observers should be in possession of everything that may tend to facilitate their search for the comet ; and 1 venture to communicate to the Society the results of some re- cent calculations of my own on the subject, preceded by a very brief view of the principal circumstances connected with former appearances of the comet, and a short notice of calculations already published. "The great and celebrated comet" of 1264, as Pingre terms it, is mentioned by nearly all the European historians of the time, and was observed by the astronomers of the dy- nasties then reigning in the north and south of China. It is described as presenting a most imposing appearance, with a tail 100° in length, stretching from the east part of the " mid- heaven." The comet was of "surprising magnitude," far exceeding any remembered by those who beheld it. Contem- porary writers generally considered it the precursor of the death of Pope Urban IV., and many of them relate that it disappeared on the same night that the pope died, or on Oc- tober 2 ; thus, in the words of Thierri de Vaucouleurs, " Quo (Urbano) moriente, velut mortem cognosceret ejus, Apparens minime Stella comata fuit." In 1556 the appearance of the comet was not on the same scale of splendour as in 1264, but still was sufficiently imposing to call forth from historians the epithets "ingens et lucidum sidus." It was observed by Paul Fabricius, a mathematician and physician at the court of the emperor Charles V. of Au- stria. M. Pingre, the celebrated cometographer, sought in vain for the original observations; the only information he could find on the subject was contained in a small rough chart found in Lycosthenes and other authors. I have before f suggested the probability that these observations were given by Fabricius in his work upon the comet, published at Niirnberg in 1556, and mentioned by Lalande in his Bibliographic ; but, as far as I am aware, tfiis work has not been discovered in any library. M. Pingre would have at his command the splendid collec- tions of St. Genevieve and the Royal Library at Paris ; and his ineffectual search for the observations in these libraries makes it at least doubtful whether they are now in existence. The chart just mentioned enables us to form a tolerably definite * From the Proceedings of the Royal Astronomical Society, No. 14. f Ast. Nach. 493. the celebrated Comet o/1264- and 1556. 51 idea of the path followed by the comet, and we have ample information for a rough determination of the elements. When Halley published his Synopsis of Cometary Astro- nomy, he gave a set of parabolic elements for the comet of J 556, founded upon the observations made by Paul Fabricius; but he remarks that these elements are not so certain as those of other comets he had computed, the observations being made "neither with sufficient instruments nor due care," and by no means to be reconciled with any regular calculation. The elements of the comet of 1264 were first computed by Mr. Dunthorne. His discussion of the observations and cir- cumstances relating to the comet's apparition are published in vol. xlvii. of the Philosophical Transactions. The elements are chiefly founded on the £Puthority of a manuscript preserved in the library of Pembroke Hall College, Cambridge, entitled Tractatusfratris JEgidii de Cometis. But it must be observed there are manifest contradictions in this account not easily set right. The other authorities consulted were the Chronicon Sampettinum Erphiirtense and the Chronicle of John Vitodu- ranus. The orbit deduced by Mr. Dunthorne much resem- bles that calculated by Halley for the comet of 1556. In the Memoirs of the Royal Academy of Sciences at Paris for 1760, appears a valuable memoir by M. Pingre on the comet of 1264. After collecting together a great number of accounts from different chronicles and histories of the day, he proceeds to the discussion of the elements. The contra- diction in the Cambridge manuscript which relates to the comet's motion in longitude is pointed out; and since this manuscript was Mr. Dunthorne's chief authority, it might be supposed that his orbit would differ entirely from M. Pingre's. This, however, was not the case ; for although there are dif^ ferences of some moment in one or two of the elements, there is still a striking similarity between the two orbits taken as a whole, and M. Pingre's approaches much nearer than Mr. Dunthorne's to the orbit of the comet of 1556. A closer agreement might have been produced if he had not wished to preserve the path laid down by Thierri de Vaucouleurs with as little alteration as possible. M. Pingre concludes from his researches that there is little doubt of the identity of the comets of 1264 and 1556, and, therefore, that the return to perihelion may be expected to take place in the year 1848. In No. 493 of the Astronomische Nachrichten will be found the results of my first calculations relating to this comet. I have there de- duced elements from the observations by Fabricius in 1556, and computed an ephemeris for comparison with the comet's observed path. The agreement, though not so close as could be wished, was the best that could be obtained from the data E2 52 Mr. Hind on the expected Reappearance of given by M. Pingre in his Cometography. I then reduced the elements to the year 1264, and with the assistance of a passage in Thierri's poem, I fixed the time of perihelion for July 9'9 (old style). The passage alluded to is as follows : — " Undecimumque gradum Phcebo superante Leonis, Ter deno Cancri restitit ilia loco." With M. Pingre, I have understood by " Ter deno Cancri,'' the 120th degree of longitude; but I am not quite sure that this is the true interpretation. With perihelion and node reduced as before stated, and the other elements as for 1556, an ephemeris of the comet's geo- centric path in 1264 was computed. During the month of July, calculation and observation agree pretty well ; but after the beginning of August the theoretical places entirely differ from the positions of the comet, as deduced from the accounts. Instead of traversing Orion towards the end of its appearance, as some historians relate, it would take a higher declination, passing through Auriga and Taurus. Since the publication of this paper in the AstronomiscJie Nachrichten, I have made some further investigations on the subject, and with more success than in my first calculations. A closer comparison of data showed pretty clearly that the observation of March 5, on which I had chiefly relied, must be erroneous as it is given by M. Pingre. In tome i. of his Cometography, p. 503, we learn that on March 5 the comet was almost in the right line joining the stars y and fl Virginis, and was equidistant from the stars. A trigonometrical cal- culation from these data gives the place of the comet in lon- gitude 188'^ l', and latitude +2° 19', and this position was employed in my earlier investigations. But I have recently satisfied myseltj that the observation as given above cannot be reconciled with those of March 3 and 4, and on subsequent days, by any set of elements. The cause of this anomaly is, I believe, an error in the name of the star. If instead of y and fl Virginis we read 8 and i9, then the place of the comet would be in longitude 188° 41', and latitude +5° 13', which agrees very well with the track which the comet ought to have followed, according to the other observations. A recalculation of the elements from an interpolated posi- tion for March 5, and from those of March 9 and 14, gives the following values: — Passage through perihelion, 1556, April 220233, G. M.T. [Old style.] o ' Longitude of perihelion 274 14"9 1 ,:, . ncK/j Ascending node 1^5 ^^.g j Equinox of 1556. Inclination 30 12-2 Log. least distance 970323 Motion direct. the celebrated Comet of 19,6^ and 1556. S3 The following ephemeris of the comet for the appearance in 1556, Greenwich mean midnight, old style, is deduced from these elements: — 1836. Old style. Geo. long. Geoc. lat. Log. r. A- March 3 188 13 0 / + 1 9 00732 0-193 4 188 0 3 40 00670 0-175 5 187 44 6 45 00606 0-157 6 187 22 10 36 0-0541 0-140 7 186 54 15 29 0-0476 0-124 8 186 14 21 43 00409 0-109 9 185 18 29 49 00341 0-096 10 183 49 40 12 0-0272 0085 11 181 11 52 50 00201 0-078 12 175 21 67 5 00130 0075 13 153 35 80 29 00057 0-078 14 55 19 82 30 9-9983 0085 15 27 16 73 26 99908 0095 16 20 37 65 30 9-9831 0-108 17 17 44 59 16 9 9753 0-122 27 12 19 34 58 9-8903 0302 April 6 12 7 27 1 9-7959 0-505 16 14 13 20 30 9-7178 0733 26 19 12 + 13 52 97130 0-974 If this ephemeris be compared with the descriptions of the comet's apparent path in the heavens, we shall find the agree- ment as close as could be expectetl, considering the uncer- tainty and irregularity of the data. With the above elements reduced to 1264, the time of pe- rihelion was found to be July 13*42, /. e. assuming with Pingre, that the comet was in longitude 120° when the sun had reached the 11th degree of Leo, according to the narration ofThierri de Vaucouleurs. The geocentric places of the comet, Green- wich mean midnight, old style, would then be as follows : — 1264. Old style. Geo. long. Geoc. lat. r. A. July 7 138° 10 + 18° 14 0-53 0-82 17 132 36 22 9 0-51 0-62 22 126 29 21 54 0-55 0-55 27 118 36 20 14 0-61 0-48 Aug. 6 101 14 + 10 17 075 0-41 16 85 23 — 3 47 0-92 0-39 26 70 47 17 10 109 0-42 Sept. 5 56 39 27 8 1-26 0-48 15 43 11 33 4 1-43 0-57 25 31 35 35 26 1-59 0-69 Oct. 5 22 47 -35 30 1-75 084 If we are to depend solely on the European accounts of this comet's path, the above is liable to two objections : first, too high a declination in August; and secondly, that the posi- 54 Mr. Hind on the expected Reappearance of tions are in Eridanus during the latter part of the comet's apparition; historians generally contenting themselves with stating that the comet " finally traversed Orion." M. Pingre's elements, which are not open to these objections, do not agree so well as mine with the more circumstantial details left us in the Chinese annals. The two orbits differ chiefly in the lon- gitude of the node and perihelion distance, but the discord- ances are by no means great. The results of my calculations have satisfied me that the comet of 1264< was, in all probability, the same as that of 1556, and consequently, that its return to perihelion must be very near at hand. The nodes of the comet's orbit lie very close to the earth's path. The ascending node is passed fifty days before perihelion, the radius vector being 1*193, and conse- quently the distance outside the earth's orbit about 0*197. The passage through descending node occurs 31| days after perihelion, and the distance of the point from the earth's orbit inside is 0*126. However, the nearest approach of the comet to the earth will not happen at the nodes, but soon after its passage through them; thus in 1556 the least distance between the two bodies was O'OT'i, nine days after the transit through ascending node. The effect of this close proximity to our globe on the period of revolution of the comet has been inves- tigated by Professor Madler, of the Dorpat Observatory, as detailed in No. 501 of the Astronomische Nachrichten\ it amounted to 14| days only, and the return of the comet to perihelion was fixed for the end of February 1 848. The following table contains the heliocentric co-ordinates referred to the equator and the log. radii vectores of the comet in my last orbit, reduced to 1848, for every tenth day, from ninety days before to 90 days after perihelion. Time from X. y. «. Log. r. perihelion pass. Days. -90 -1*7430 + 0-5750 -0-0603 0-2640 80 1-6231 0-4370 0-0445 0-2257 70 14931 0-2963 0-0284 0-1826 60 1-3504 0-1533 -0-0122 0-1333 50 1*1917 +0-0084 + 0-0041 0-0762 40 1-0120 -0-1363 0-0206 00092 30 0-8039 0-2770 0-0363 9*9300 20 0-5570 0-4031 0-0501 9-8385 -10 — 02611 0-4907 0-0592 9-7474 0 + 00738 0-4961 0*0583 9-7032 + 10 0-3929 0*3951 0-0450 9-7474 20 0-6507 0-2266 0-0239 9-8385 30 0-8503 —0-0352 + 0-0004 99300 40 1-0086 + 0-1590 -00233 0-0092 50 1-1385 0-3490 0-0463 0-0762 60 1-2484 0-5331 0-0685 0-1333 70 1-3433 0-7109 00900 0-1826 80 1-4268 0-8828 0*1107 0-2257 +90 + 1-5015 + 1-0492 -0-1307 0-2640 the celebrated Comet qfl264i and 1556. 55 With the above values for x, y and ;?, and those of X, Y, Z, taken from the Nautical Almanac, the position of the comet for different suppositions as to the time of passage through perihelion may be readily obtained. If vi^e suppose March 0, which is about the epoch fixed by Professor Madler, we shall have the following ephemeris for facilitating the discovery of the comet, mean noon at Greenwich : — 1847—8. R.A. Decl. A. Dec. 1 187 16 o / -11 22 2-16 11 193 .55 12 56 1-92 21 201 52 14 29 1-68 31 211 43 15 52 1-46 Jan. 10 224 16 16 50 1-26 20 240 18 16 47 Ml 30 259 53 15 3 1-02 Feb. 9 281 23 11 24 1-03 19 302 15 7 1 1-13 29 321 18 3 23 1-29 Mar. 10 338 5 — 0 54 1-48 20 352 11 + 0 50 1-66 30 3 50 2 9 1-84 April 9 13 32 3 11 201 19 21 46 3 59 2-17 29 28 52 4 35 2-32 May 9 35 5 4 58 2-46 19 40 36 5 11 2-59 29 45 31 + 5 12 2-69 It appears from this ephemeris, that according to the most probable supposition we can make respecting the time of pe- rihelion without actual calculation of the perturbations, the position of the comet in the heavens during the approaching reappearance will be extremely unfavourable for observation ; and it is therefore the more desirable that those who look out for comets should be on the alert. Nearly the whole of the vast trajectory of this comet lies below the plane of the ecliptic, and Jar Jt'om the paths of the larger planet s^ but it ex- tends into space more than twice the distance of Neptune ; and surely we are not yet able to say what causes may operate, at this immense distance from the sun, to affect the time of the next return to perihelion. If however the comet can be de- tected and observed, we shall then have the means of ascer- taining something more on these points [ 56 ] X. Analysis of the Water of the Thermal Spring of Bath {Kinfs Bath). By Messrs. George Merck and Robert Galloway*. THE water of this celebrated spring, the efficacy of which was known in the time of the Romans, has been analysed repeatedly by various chemists at different periods. Richard Phillipsf, Scudamorejj Walker§, and more recently Noad||, have occupied themselves in the investigation of this water. In their several analyses, the whole amount of the fixed ingre- dients of the water agrees very closely ; but in regard to the composition of these substances there are considerable dis- crepancies, as may be seen in a table which we have annexed at the end of this paper. Besides great differences in the quantitative analysis, we find discrepancies even in regard to the presence and absence of certain constituents. Among the chemists that have been mentioned, Walker is the only one who has recognised the presence of potash. The same chemist corroborated Scuda- more's statement as to the presence of magnesia, overlooked by their predecessors ; but he states also that he detected alumina, which none of the others found. In all these ana- lyses iodine has been omitted. Mr. Cuff ^ however has in- dicated the presence of this element in the spring. These discrepancies made another investigation of the mi- neral water of Bath very desirable ; the following analysis was performed at the suggestion of Dr. A. W. Hofmann. To obtain the water genuine, and especially for the pur- pose of ascertaining the amount of free carbonic acid it con- tained, we collected the water ourselves, an operation in which we were kindly assisted by Messrs. Green and Simms, lessees of the establishment. The water was taken from the principal w^ell, which sup- plies the King's and Queen's baths, which are the most esteemed and valued in the city. Of the two other w ells, one supplies the Hot Bath and the other the Cross Bath, ^vhich are in the neighbourhood of those first mentioned. * Communicated by the Chemical Society j having been read Nov. 16, 1846. t An Analysis of the Bath "Water, by Richard Phillips. London, 1806. X A Chemical and Medical Report of the properties of the Mineral Waters of Buxton, Matlock, &c., by Ch. Scudamore, M.D. 1820. § Quarterly Journal of Science, Literature and Arts, vol. xxvii. 78. 1829, II Pharmaceutical Journal, vol. iii. 526. ^ Memoir on the occurrence of Iodine and Bromine in certain Mineral Waters of South Britain, by Charles Daubeny; Transactions of the Royal Society of London, 1830, ii. p. 223. Analysis of the Water of the Thermal Spring of Bath. 57 The King's Bath is an oblong cistern, 65 feet long and 40 feet broad, in which the water stands at the height of 46 inches. It is supplied from the bottom by means of twelve large and about twenty smaller apertures. By far the largest amount of water rises however from an opening made in the centre of the bath, 18 inches in diameter. Although the water flows under the influence of a very small pressure, the quantity is such, that the two reservoirs, the King's and the Queen's bath, are entirely filled in about nine hours. The quantity of water entering each minute is 126 gallons, upon the authority of Dr. Daubeny*. I. Qualitative Analysis. The water as it issues from the well has a temperature of 46° C. (115° Fahr.), the temperature of the air being 20° C. (68° Fahr.) ; it is clear and without odour, and has no effect upon vegetable colours ; it has a saline and slight iron taste ; the iron is deposited as sesquioxide in rather large quantities in the pipes leading from the well. The following experiments gave the qualitative composition of the mineral water ; on boiling for some time a white cry- stalline precipitate formed. The qualitative analysis was therefore divided into two parts. a. The analysis of the precipitate formed on boiling. b. The analysis of the substances remaining dissolved. a. Analysis of the Precipitate formed on boiling. 1 . The precipitate was treated with hydrochloric acid ; a small portion of it dissolved with effervescence, indicating the pi-esence of carbonic acid. The portion insoluble in hydro- chloric acid dissolved on the addition of a large quantity of water : — Indicating sulphate of lime. Another portion of the water was boiled some time, with the precaution of replacing the evaporated water, in order that all the sulphate of lime should remain in solution ; in this case only a very small precipitate was formed, which was entirely soluble in hydrochloric acid. 2. On heating this solution and adding ammonia, a very slight flocculcnt precipitate of a yellowish-white colour was produced after some time: — Indicating oxide of iron. 3. In the filtrate from the sesquioxide of iron (2.), on the addition of oxalate of ammonia, a white precipitate was formed: — Indicating salts of lime. * On the Quantity and Quality of the Gases disengaged from the Thermal Spring which supplies the King's Bath in the City of Bath, by Charles Dau- beny ; Transactions of the Royal Society of London, 1834, 1. i. 58 Messrs. Merck and Galloway's Analysis of 4. In the liquid filtered off from the oxalate of lime (3.), phosphate of soda produced an exceedingly slight crystalline precipitate : — Shoiving the presence of magnesia. Note. — ^This precipitate could only be distinctly seen in testing a large quantity of the water. b. Analysis of the substances remainiiig dissolved. The liquid which was filtered from the precipitate (a.) formed on boiling had no alkaline reaction ; a portion of it was evaporated nearly to dryness and treated with hydro- chloric acid ; no carbonic acid was evolved, from which com- portment the absence of alkaline carbonates could with safety be concluded. 1. A portion of the liquid gave on addition of chloride of barium a copious white precipitate, insoluble in hydrochloric acid : — Indicating sulphuric acid. 2. In another portion of the liquid nitrate of silver pro- duced a copious white precipitate, easily soluble in ammonia : — Evidencing the presence of chlorine. 3. The entire solubility of the silver precipitate seemed to indicate the absence of iodides. To make ourselves perfectly certain of the absence of these salts, 30 or 40 pounds of the water were evaporated to 2 or 3 pounds, and the liquid filtered off from the precipitate which had been formed ; a part of this fluid was evaporated with precaution to dryness, the residue was mixed with some starch paste, and a few drops of nitric acid being added, feeble but distinct violet spots were ob- served : this experiment was repeated several times with the same success : — Indicating the presence of iodine. 4. Another portion of the liquid {b.) was treated with hy- drochloric acid, evaporated to dryness, and gently ignited : on treating the residue with a large quantity of water an insolu- ble portion remained: — Showing the presence of silicic acid. 5. Another portion of the liquid {b.) gave, on addition of chloride of ammonium and oxalate of ammonia, a white pre- cipitate : — Indicating lime. 6. On adding, to a portion of the filtrate, ammonia and phosphate of soda, a slight crystalline precipitate was formed : — Indicating magnesia. 7. For the discovery of the alkalies, the remaining portion of the filtrate from the lime precipitate Avas evaporated to dryness, and the residue ignited until the ammoniacal salts had been expelled. The ignited residue was then dissolved in water, the sulphuric acid and magnesia precipitated by baryta water, and after separation of the excess of baryta by means of carbonate of ammonia, the filtrate evaporated to dryness the Water of the Thermal Spring of Bath. 59 and ignited. The residue imparted a yellow colour to the blowpipe flame : — Evidencing the presence of soda. An alcoholic solution of the residue gave with a concen- trated solution of bichloride of platinum a yellow crystalline precipitate : — Indicating potassa. The precipitate which had formed on evaporating for the iodine determination, was treated with hydrochloric acid, the filtrate saturated with ammonia and precipitated by sulphide of ammonium ; this precipitate was re-dissolved in nitro-hy- drochloric acid mixed with chloride of ammonium, and the sesquioxide of iron separated by ammonia. The filtrate, eva- porated and fused with nitrate of potash and carbonate of soda, gave a green mass: — Showing traces of manganese. Lithia, alumina, bromine and phosphoric acid were found to be absent. In regard to the presence of gases in the water, it was scarcely necessary to test for the presence of free carbonic acid. On mixing a solution of lime with the mineral water a precipitate was formed, which dissolved in an excess of the mineral water. The quantity of free carbonic acid however is not very large ; the water has no reaction on blue vegeta- ble colours ; hydrosulphuric acid is not contained in the water. Acetate of lead gave only a white precipitate of sulphate of lead free from all trace of brown colour, which might indicate the presence of sulphur. A large quantity of gas is continually disengaged from the chief spring as well as from the secondary ones. Dr. Dau- beny* paid particular attention to the composition of this gas. He found that it consists principally of nitrogen, together with small quantities of carbonic acid and oxygen. He employed a peculiar apparatus, constructed on purpose for these experiments, by which he was enabled to collect the whole of the gases from the principal well, as well as from those adjoining it. The experiments of Daubeny are so nu- merous and accurate as to preclude any other researches on the subject. II, Quantitative Analysis, Determination of the Specific Gravity. A small bottle, which contained at the temperature of 16°'5 C. (60° Fahr.) 10 grms. of distilled water, contained at the same temperature 10*025 grms. of the mineral water; from this the specific gravity of the water is calculated as 1-0025. * Vide Memoir mentioned. 60 Messrs. Merck and Galloway's Analysis of 1. Estimation of Sulphuric Acid. The mineral water was heated with a little hydrochloric acid and chloride of barium added. I. 534*199 grms. of water gave l"340grm. of sulphate of baryta = 0'4605 grm., or 0*08620 percent, of sulphuric acid. II. 475*003 grms. of water gave 1*1791 grm. of sulphate of baryta = 0*4050 grm., or 0'08526 per cent, of sulphuric acid. Mean of the results, 0*08573 per cent. 2. Estimation of Chlorine. The water was treated with nitric acid and precipitated by nitrate of silver ; the precipitated chloride of silver was washed by decantatioUj fused and weighed. I. 101 grms. of water gave 0*1137 grm. of chloride of silver = 0*2811 grm., or 0*02778 per cent, of chlorine. II. 100*006 grms. of water gave 0*1093 grms. of chloride of silver =0*02702 grms., or 0*02701 per cent, of chlorine. Mean of the results, 0*02739 per cent. 3. Estimation of Silicic Acid. To the water was added nitric acid in excess ; it was then evaporated to dryness and the residue for some time heated on the sand-bath. On treating this residue with water and hydrochloric acid, the silicic acid remained behind; it was collected, washed and weighed. I. 765*325 grms. of the water gave 0*0342 grm., or 0*00446 per cent, of silicic acid. II. 732*015 grms. of water gave 0*0289 grm., or 0*00407 per cent, of silicic acid. Mean of the results, 0*00426 per cent. 4. Estimation of Iron. The iron was estimated, — A. In the precipitate formed on boiling the mineral water. B. In the water which had not been boiled. Both estimations gave the same results. A.^Estimation of the iron in the precipitate : — A certain quantity of the water was boiled for some time ; the precipitate which had formed was washed, dissolved in hydrochloric acid and precipitated by an excess of ammonia. I. 777*215 grms. of water gave 0*0079 grm., or 0*00101 per cent, of sesquioxide of iron. B. Estimation of the iron in the water which had not been boiled : — the Water of the Thermal Spring of Baih. 61 The liquid filtered off from the silicic acid (3.) was concen- trated and precipitated by an excess of ammonia. II. 765-325 grms. of Mater gave 0-0078 grm., or O'OOlOl per cent, of sesquioxide of iron. III. 732-015 grms. of water gave 0*0086 grm., or 0-00116 per cent, of sesquioxide of iron. Mean of the results, 0-00106 per cent., corresponding to 0*00153 per cent, of carbonate of oxide of iron. 5. Estimation of Lime. The estimation of the lime was divided into — A. Estimation of the lime contained in the water in the state of carbonate. B. Estimation of the lime contained in the water in the state of sulphate. C. Estimation of the total amount of lime for control. A. Estimation of the lime combined with carbonic acid : — The ammoniacal liquor filtered off from the precipitate of sesquioxide of iron was precipitated by oxalate of ammonia ; the oxalate of lime was converted in the known way into carbonate. I. 712-747 grms. of water gave, on boiling, a precipitate containing 0*0904 grm. of carbonate of lime = 0-05062 grm., or 0'00712 per cent, of lime. II. 623-881 grms. of water gave, on boiling, a precipitate containing 0*0782 grm. of carbonate of lime = 0*0437 grm.j or 0*00700 per cent, of lime. Mean of the results, O-OO7O6 per cent. B. Estimation of the lime combined with sulphuric acid: The mineral water was kept boiling for one or two hours, replacing the water w^hich evaporated ; the precipitate formed was filtered off, washed, and to the filtrate was added chlo- ride of ammonium, ammonia, and oxalate of ammonia; the oxalate of lime was converted into carbonate. I. 710747 grms. of water gave in this way 0*6072 grm. of carbonate of lime = 0-3400 grm., or 0-04783 per cent, of lime. II. 623-881 grms. of water gave 0-5165 grm. of carbonate of lime = 0-2892 grm., or 0*04635 per cent, of lime. Mean of the results, 0*04709 per cent. C. Estimation of the total amount of lime for control : — The ammoniacal liquid which was filtered off from the pre- cipitate of sesquioxide of iron was precipitated after the addi- tion of chloride of ammonium by oxalate of ammonia, and the oxalate of lime converted into carbonate. 62 Messrs. Merck and Galloway's Analysis of I. 765*325 grms. of water gave 0*7211 grra. of carbonate of lime = 0*4038I6 grm., or 0*05276 per cent, of lime. II. 732*015 grms. of water gave 0*6981 grm. of carbonate of lime = 0*3909 grm., or 0*05340 per cent, of lime. Mean of the results, 0*05308 per cent. Mean of the lime combined with carbonic acid 0*00706 Mean of the lime combined with sulphuric acid 0'04709 Total amount found by addition 0*05415 Mean of the total amount found by direct ^sti-l ^ „^^^q mation j 6. Estimation of Magnesia. The estimation of the magnesia was divided in the same manner as the estimation of lime into — A. Estimation of the magnesia combined with carbonic acid. B. Estimation of the magnesium combined with chlorine. C. Estimation of the total amount of magnesia for control. A. Estimation of magnesia contained in the water as car- bonate : — To the liquid filtered off from the oxalate of lime was added phosphate of soda ; on stirring, after some time a pre- cipitate of phosphate of magnesia and ammonia was formed, which was converted by ignition into pyrophosphate of mag- nesia. I. 777*215 grms. of water gave, on boiling, a precipitate which contained 0*0046 grm. of pyrophosphate of magnesia = 0*001685 grm., or 0*00021 per cent, of magnesia. II. 623*881 grms. of water gave, on boiling, a precipitate which contained 0*0044 grm. of pyrophosphate of magnesia = 0*00016 grm., or 0*00025 per cent, of magnesia. Mean of the results, 0*00023 per cent. B. Estimation of the magnesia contained in the water as chloride of magnesium. The liquid filtered off from the oxalate of lime was con- centrated by evaporation, ammonia added filtered off from a small portion of silicic acid which separated, and the mag- nesia precipitated by phosphate of soda. I. 414*279 grms. of water gave in this way 0*1007 grm. of p3'rophosphate of magnesia = 0*03689 grm., or 0*008906 per cent, of magnesia. II. 427*1 grms. of water gave 0*1050 grm. of pyrophos- phate of magnesia = 0*03846 grm., or 0*009004 per cent, of magnesia. Mean of the results, 0*008955 per cent. the Water of the Thermal Spring of Bath. 63 C. Estimation of the total amount of magnesia for con- trol :— The liquid filtered off from the precipitate of oxalate cf lime was concentrated, ammonia and phosphate of soda added. I. 7G5*325 grms. of water gave 0-1936 grm. of pyrophos- phate of magnesia = 0-070929 grm., or 0*00926 per cent, of magnesia. II. 732-015 grms. of water gave 0*1837 grm. of pyrophos- phate of magnesia = 0*0673 grm., or 0*00919 per cent, of magnesia. Mean of the results, 0*00922 per cent. Mean of the magnesia combined with carbonic acid 0*00023 Mean of the magnesia contained in the water asl o*00895 chloride of magnesium j _^_ Total amount found by addition 0*00918 Mean of the total amount found by direct estimation 0*00922 7. Estimation of the Alkalies. For the estimation of the alkalies the mineral water was evaporated to one-third of its volume and baryta water added in excess, the precipitates of sulphates of baryta, lime, mag- nesia and sesquioxide of iron were filtered off, and the excess of baryta precipitated by means of carbonate of ammonia. To get rid of the silicic acid the filtrate was evaporated to dryness with hydrochloric acid, gently ignited, dissolved in water, again filtered and evaporated to dryness ; the mixed chlorides obtained in this manner were weighed. I. 632*481 grms. of the mineral water gave 0*2937 grm. of chloride of sodium and chloride of potassium = 0*04643 per cent, of the mixed chlorides. II. 546*032 grms. of water gave 0*2538 grm. of chlorides of sodium and potassium = 0*04648 per cent, of the mixed chlorides. Mean of the results, 0*04645 per cent. 8. Estimation of the Potassa. The chlorides of potassium and sodium were dissolved in a small quantity of water and an excess of bichloride of platinum added ; the liquid was then evaporated to dryness in the water-bath, the residue digested with alcohol, the in- soluble chloride of platinum and potassium filtered off from the soluble sodium salt and washed with alcohol ; the preci- pitate was dried in the water-bath and weighed. I. 632*481 grms. of the mineral water, or 0*2987 grm. of the mixed chlorides, gave 0*124 grm. of chloride of platinum 64 Messrs. Merck and Galloway's Analysis of and potassium = 0*0378 grm. of chloride of potassium = 0*00597 per cent, of chloride of potassium, which equals 0*00377 per cent, of potassa. II. 546*032 grms. of water, or 0*2538 grm. of the mixed chlorides, gave 0*0975 grm. of chloride of platinum and po- tassium = 0*02977 grm. of chloride of potassium = 0*00545 per cent, of chloride of potassium, which equals 0*00342 per cent, of potassa. Mean of the results, 0*00571 per cent, of chloride of potas- sium and 0*0359 per cent, of potassa. 9. Estimation of the Soda. The quantity of soda was found simply by the difference of the mixed chlorides and the quantity of chloride of potas- sium found by direct estimation. Mean of the mixed chlorides . . . 0*04645 Mean of the chloride of potassium . 0*00571 Chloride of sodium . . 0*04074 corresponding to 0*02168 per cent, of soda. 10. Estimation of Carbonic Acid. To find the quantity of free carbonic acid contained in the water at the moment it was taken from the well, a siphon of exactly known capacity was immersed in the well, and the water obtained in this way put in bottles, containing a mix- ture of ammonia and chloride of calcium. In this way the free carbonic acid as well as the carbonic acid in combination was precipitated in the form of carbonates. Four bottles were filled with mineral water by this method. The capacity of the siphon was exactly 533 cubic centimetres, therefore 533 X 4 X 1*0025 = 2137 grms. of water were taken. The precipitate from the water contained in these four bot- tles was collected, washed, dried and weighed; it yielded 1*4748 grm. of carbonate mixed with some alumina from im- purity in the solution of chloride of calcium. To estimate the quantity of carbonic acid in this precipitate, tw^o portions of it were taken and estimated separately after the method proposed by Drs. Fresenius and Will. I. 0*66 grm. of the carbonate, &c. gave in this way 0*22 grm. of carbonic acid, therefore 1*4748 grm. of the carbonate, or 2137'0 grms. of water, gave 0*4916 grm. of carbonic acid. II. 0*718 grm. of the carbonate, &c. gave 0*23 grm. of car- bonic acid, therefore 1*4-748 grm. of the carbonate, &c., or 2137*0 grms. of water, gave 0*4718 grm. of carbonic acid. tJie Water of the Thermal Spring of Bath. 65 Mean of the results. 0*48l7grm. of carbonic acid,which equals 0*02254 per cent. Total amount of carbonic acid . . 0-02254 Carbonic acid existing in combination — With oxide of iron . . . 0-00057 With lime . . . . . 0-00554 With magnesia .... 0-00024 Sum total ...... 0-00635 Free carbonic acid remaining 0*01619 From the details contained in the preceding pages, it fol- lows that the thermal spring in the King's Bath contains the following constituents in 100 parts : — Carbonate of lime . . . . 0-01260 Carbonate of magnesia Carbonate of oxide of iron . 0-00047 . 0-00153 Sulphate of lime . . . Sulphate of potassa . . Sulphate of soda . . . Chloride of sodium . . . 0-11436 . 0-00663 . 0-02747 . 0-01806 Chloride of magnesium . Silicic acid . 0-02083 . 0-00426 0-20620 Traces of manganese and iodine. Estimation of the total amount of the fixed ingredients in the water for control. The water was concentrated in a porcelain dish, and after- wards evaporated to dryness in a platinum basin. The resi- due was heated in an air-bath until the weight was constant. Two estimates were made. I. 217*058 grms. of water gave 0*4540 grm., or 0*20916 per cent, of residue. II. 319*57 grms. of water gave 0*6726 grm., or 0*21040 per cent, of residue. Mean of the results, 0*20978 per cent. But in this experiment the iron was obtained in the state of sesquioxide, whilst in the preceding calculation it is taken as the carbonate of the oxide, in which form it exists in the water. On calculating the absolute weights from the above, we obtain the following numbers : — Phil. Mag. S. 3. Vol. 3 1 . No. 205. Jidij 1 847. F 66 Analysis of the Water of the Thermal Spring of Bath. Carbonate of lime . . Carbonate of magnesia . Carbonate of oxide of iron Sulphate of lime . . . Sulphate of potassa . . Sulphate of soda . . . Chloride of sodium . . Chloride of magnesium . Silicic acid In a litre 0-1260 grm. 0-0047 0-0153 1-1436 0-0663 0-2747 0'1806 0-2083 0-0426 0-20621.. In an imperial gallon (70,000 grs.). 8-82000 grs. 0-32900 ... 1-07100 ... 80-05200 ... 4-64100 ... 19-22900 ... 12-64200 ... 14-58100 ... 2-98200 ... 144-01800 According to our experiments, 1 litre of the water contains 95-64 cubic centimetres of free carbonic acid at the tempera- ture of 46° C. (115° F.) and normal atmospheric pressure. One imperial gallon contains therefore 26-45 cubic inches of free carbonic acid of 46° C, being more than double the quantity which has been determined by former experiments. This however is not surprising, as the estimations previ- ously made had been effected by the expulsion of the carbonic acid from the water. Besides the difficulty of avoiding a loss of carbonic acid before the operation, it is scarcely possible, as Mr. Philli])s justly notices in his paper, to expel all carbonic acid by simple ebullition. Besides, we see from the experi- ments of Daubeny, that the gas which escapes from the well contains at different periods highly varying amounts of car- bonic acid. He found by several experiments that the King's Bath evolves on an average 267 cubic inches of gas per minute, or 223 cubic feet in twenty-four hours. He further ascer- tained that this gas consists nearly entirely of nitrogen, mixed with a small amount of oxygen and carbonic acid, and that these gases were generally in the following proportion : — Nitrogen . . =91 '9 Oxygen . . . = 3-8 Carbonic acid = 4*3 In many instances, however, he observed as much as 7 '4 to 8-2, and even once 11*5 parts of carbonic acid. From these observations there is no doubt that the quan- tity of carbonic acid dissolved in the water is very variable. In the following Table we give the analyses of former ex- perimenters, calculated in an imperial gallon (70,000 grs.). Notices respecting New Booh. 67 Phillips. Scudamore*. Walker. Noad. 7-680 0-274 86-460 14-460 31-680 1-960 5-280 0-200 98-320 i-520 12-240 15-360 i-920 10-667 0-243 81-624 2-927 19-371 15-122 13-339 0-150 3-233 0-521 5-760 96-240 27-456 7-142 3-360 Carbonate of oxide of iron Carbonate of soda Sulphate of lime Sulphate of potassa Sulphate of soda Chloride of sodium Chloride of magnesium ... Alumina Silicic acid ..,.• Quantity directly observed Carbonic acid 142-394 144125 134-840 146-676 147-622 140-479 149-72 11-52 cub. in. 7-60 cub. in. Our analysis agrees, as may be seen, best with that of Walker. According to Professor Liebig'sf arrangement of mineral M'aters, the thermal spring of Bath would belong to the saline waters containing carbonic acid. XI. Notices respecting New Books. On the Correlation of Physical Forces : being the substance of a Course of Lectures delivered in the London Institution, in the year 1843. ByW. R. Grove, Esq., M.A., F.R.S., Barrister-at-Law. Printed at the request of the Proprietors of the London Institution. London ; Samuel Highley, 32 Fleet Street. ''r^HIS publication treats of subjects which might have been advan- -*• tageously considered at much greater length ; but it must be acknowledged that in the brief space to which the author has con- fined the announcement of his views and speculations, he has done them no small degree of justice ; it may indeed be questioned whether the opinions broached are not of such a nature as to defy the test of experiment to realise or to refute them. This is certainly the case as far as experiment has yet been carried ; but although we discover great reason for doubting whether the difficulties which beset the subjects may ever be overcome, we discover no cause for despair, seeing that new modes of research and new instruments for carrying them out are of almost daily occurrence. As a proof of this we may cite the author's excellent invention of his well-known and justly- appreciated voltaic battery ; and his still more recent discovery, that water may be decomposed by heat so as to exhibit both its elements in the gaseous form. Mr. Grove states tliat "the position which he seeks to establish in this Essay is, that the various imponderable agencies, or the affec- tions of matter which constitute the main objects of experimental * Recalculated according to a more correct principle by Walker, t Handworterhuch der Cliemie, Art. ' Analyse der Mineral wasser,' F2 68 Notices respecting New Books, physics, viz. heat, light, electricity, magnetism, chemical affinity and motion, are all correlative, or have a reciprocal dependence ; that neither, taken abstractedly, can be said to be the essential or proxi- mate cause of the others, but that either may, as a force, produce or be convertible into the other ; thus heat may mediately or imme- diately produce electricity, electricity may produce heat ; and so of the rest." In further illustration of the author's views, we may quote what he states to be the sense that he has attached to the word correlation, which is, that " of a reciprocal production or convertibility ; in other words, that any force capable of producing or being convertible into another, may, in its turn, be produced by it, — nay, more, can be itself resisted by the force it produces, in proportion to the energy of such production, as action is ever accompanied and resisted by reaction ; thus, the action of an electro- magnetic machine is reacted upon by the magneto-electricity developed by its action." In order to support his speculations by facts, the author appeals in the first place to the agency of electricity. " To commence, then, with electricity as an initiating force, we get motion directly pro- duced by it in various forms ; for instance in the attraction and re- pulsion of bodies, evidenced by mobile electrometers, such as that of Cuthbertson, where large masses are acted on ; the rotation of the fly wheel, another form of electrical repulsion, and the deflection of the galvanometer needle, are also modes of j)alpable, visible motion. Electricity directly produces heat, as shown in the ignited wire, the electric spark, and the voltaic arc, in the latter the most intense heat with which we are acquainted, so intense, indeed, that it cannot be measured, every sort of matter being dissipated by it. Electricity directly produces light in the same pha?nomena. It directly produces magnetism in all ferruginous bodies placed at right angles to its line of direction, and, indeed, in the substances, of whatever nature, traversed by the electrical current, in a direction at right angles to that of the current ; in this case giving us a new character of force, viz., a force acting, not in direct straight lines, but in a tangential or rather rectangular direction. " Lastly, electricity directly produces chemical affinity, and by its agency we are enabled to obtain efi^ects of analysis or synthesis, with which ordinary chemistry does not furnish us. Of these effects we have examples in the brilliant discoveries by Davy of the alkaline metals, and in the peculiar crystalline compounds made known by Crosse and Becquerel." Having stated thus much respecting electricity in support of his peculiar views, Mr. Grove adduces additional confirmation of them from considering the action of light, in a passage which we shall quote at length. He observes that "light is, perhaps, that mode of force the reciprocal relations of which with the others has been the least traced out. Until the discoveries of Daguerre and Talbot, very little could be definitely predicated of the action of light in produ- cing other modes of f^rce ; and, even, since these discoveries, it is doubted by many competent investigators, whether the phsenomena Royal Society^ 69 of photography are not mainly dependent upon a separate agent accompanying light, rather than upon light itself. It is, indeed, dif- ficult not to believe that a picture, taken in the focus of the camera obscura, and which represents to the eye all the gradations of light and shade shown by the original luminous image, is not an effect of light ; certain it is, however, that the different coloured rays exer- cise different actions upon various chemical compounds, and that the effects on many, perhaps on most of them, are not proportionate in intensity to the effects upon the visual organs ; those effects, however, appear to be more of degree than of specific difference, and without pronouncing myself positively upon the question, hitherto so little examined, I think it will be safer to regard the action on photographic compounds as resulting from a function of light : so viewing it, we get light as an initiating force, capable of producing, mediately or immediately, the other modes of force. Thus, it imme- diately produces chemical action ; and having this, we at once ac- quire a means of producing the others." Mr. Grove then relates the following beautiful experiment, by which he conceives th.it he showed the production of all the other modes of force by light : — " A prepared Daguerreotype plate is in- closed in a box filled with water, having a glass front, with a shutter over it ; between this glass and the plate, is a gridiron of silver wire ; the plate is connected with one extremity of a galvanometer coil, and the gridiron of wire with one extremity of a Breguet's helix ; the other extremities of the galvanometer and helix are connected by a wire, and the needles brought to zero. As soon as a beam of either daylight or the oxyhydrogen-light is, by raising the shutter, permitted to impinge upon the plate, the needles are deflected : thus light being the initiating force, we get chemical action on the plate, electricity circulating through the wires, magnetism in the coil, heat in the helix, and motion in the needles." We have had some difficulty in selecting passages for quotation from this publication, on account of the profusion of interesting matter which it contains, though in so small a space ; we believe, however, that the selections which we have given are such as will well and sufficiently illustrate the interesting views of their author. XII. Proceedings of Learned Societies. ROYAL SOCIETY. [Continued from vol. xxx. p. 207.] Feb. 11, "/^N the Amount of the Radiation of Heat, at night, 184'7. ^^ from the Earth, and from various Bodies placed on, or near the surface of the Earth." By James Glaisher, Esq. Com- municated by G. B. Airy, Esq., F.R.S., Astronomer Royal, &c. The author enters into a very detailed description of the construc- tion of the thermometers he employed in these observations, and the precautions he took to ensure their accuracy ; and gives tabular records of an extensive series of observations, amounting to a num-» 70 Royal Society, ber considerably above ten thousand, with thermometers placed on nearly a hundred different substances, exposed to the open air, under different circumstances, and in various states of the sky, at the Royal Observatory at Greenwich. Feb. 18. — " On the Diurnal Variation of the Magnetic Declina- tion of St. Helena." By Lieut.-Colonel Edward Sabine, R.A., For. Sec. R.S. It has long been known that the diurnal variation of the magnetic needle is in an opposite direction in the southern, to what it is in the northern hemisphere ; and it was therefore proposed as a pro- blem by Arago, Humboldt and others, to determine whether there exists any intermediate line oi' stations on the earth where those diurnal variations disappear. The results recorded in the present paper are founded on observations made at St. Helena during the five consecutive years, from 1841 to 1845 inclusive; and also on similar observations made at Singapore, in the years 1841 and 1842; and show that at these stations, which are intermediate between the northern and southern magnetic hemispheres, the diurnal variations still take place ; but those peculiar to each hemisphere prevail at opposite seasons of the year, apparently in accordance with the position of the sun with relation to the earth's equator. Feb. 25. — " On certain Properties of Prime Numbers." By the Right Hon. Sir Frederick Pollock, M.A., F.R.S., Lord Chief Baron of the Exchequer, &c. The author of this paper, after noticing Wilson's Theorem, (pub- lished by Waring about the year 1770, without any proof), which theorem is that, if A be a prime number, 1. 2. 3. . . . (A — l)-f-l is divisible by A ; refers to Lagrange's and Euler's demonstrations, and mentions Gauss's extension of the theorem, to any number, not prime ; provided that instead of 1, 2, 3, &c. (A — 1), those numbers only be taken which are prime to A, and 1 be either added or sub- tracted. This theorem was published by Gauss without a proof in 1801, with a rule as to the cases in which 1 is to be added or sub- tracted, the correctness of which is questioned by the author, who proceeds to propound the following theorem, which he had previ- ously, for distinctness, divided into three. If any number, prime or not, be taken, and the numbers prime to it, and less than one half of it be ascertained, and those be rejected whose squares +1 are equal to the prime number, or some multiple of it (which may be more than one), then the product of the re- maining primes (if any), + 1 shall be divisible by the prime number. He gives as examples, 14, the primes to which, and less than one half, are 1, 3, 5, and 1.3. 5=15; therefore 1.3.5 — 1 = 14; also 15, the primes to Avhich and less, are 1, 2, 4, 7; but 4x4 = 16 = 15 + 1 ; therefore 4 is to be rejected, and 1. 2. 7 + 1 = 15. The author adds another theorem, that if A be a prime number, all the odd numbers less than it (rejecting as before) ; also, all the even numbers (making the same rejection except A — 1) will, multiplied together, be equal to A+1. The author then proceeds to prove Gauss's extension of Wilson's Rmjal Society, 71 theorem, and to give the cases in which 1 is to be added or sub- tracted ; and in the course of the proof, he mentions that the num- bers prime to any number not only are found in pairs, one greater and one less than one-half of the number, but that they associate themselves in sets of four, with an odd pair in certain cases. Thus, the primes to 7 are 1, 2, 3, 4, 5, 6, — 2x4=8=7 + 1. Put the complemental numbers underneath crosswise, thus, — 2x4 \/ / \ y \ 3X5 80 that 2 + 5 and 4+3 may equal 7 ; and then 3x5=15=2x7 + 1 2x3= 6=7-1 4x5=20=3x7-1 Multiplied together one way the product exceeds 7, or a multiple of it, by 1 ; multiplied the other way, the product is less than 7, or some multiple of it, by 1. By assuming the prime number to be A, and the two primes to it to be jo, q, and that p-\-q he not equal to A, but j05'=wA+l, it is shown that the complemental primes {A—q) and (A—/?) will have a product=w'A+l, and that, in- stead of 1, the number may be any other prime to A. Upon this foundation the author proceeds to show that Wilson's theorem, and also Gauss's, may be made much more general ; that if A be a prime number, as 7, the numbers less than it may be arranged in pairs, not only with reference to 1, but to any number less than 7. Take 4 as an example : — 1 X 3=7-4 4 X 6=4x7—4 2 X 5=2x7—4 therefore 1.2.3.4.5 . 6=7w— 4' ; therefore ] .2.3.4.5.6+43=7^; that is, is divisible by 7. The same is then shown as to numbers not prime, provided those numbers alone are taken which are prime to it, and the number of pairs will be half the number of primes. The general theorem therefore is this : — If A be any number, prime or not, and m be the number of primes to it, which are l,p, q, r, &c. ; then 1 .p.q.r, &c., m + Z2 will be divisible by A, provided Z be prime to A, whether it be greater or less. It follows from this that z^+ 1 must be divisible by A, and there- fore that z"*- 1 must be divisible by A. If A be a prime number 74 Royal Society. and z a number prime to it (which every number not divisible by it is), this is Fermat's theorem, and the author has given a new proof of it. But the theorem is true though A be not a prime number, provided z be prime to A and m be the number of primes to A, and less than it ; and instead of 1 , any other number prime to A raised to the mi\\ power may be substituted : and z'^—if"^ will be di- visible by A, provided z and y be primes to A, and m be the number of primes to A and less than it. The author has therefore in this paper offered a proof of Gauss's theorem, and proved that it applies in certain cases to one half of the primes, and in all cases, with certain modifications, has shown that a similar property belongs to the product of the odd numbers, and also of the even numbers which precede any prime number ; and lastly, has shown the intimate connexion between Wilson's theorem and Fermat's, and shown that each is but a part of a much more general proposition, which, he observes, may itself turn out to be part only of a still more universal one. In a postscript, the author has shown that the well-known law of reciprocity of prime numbers is an immediate corollary from his theorem ; and that it may be extended thus : if A and B be any two numbers (not prime numbers but) prime to each other, and the primes to A, and less than it, are (in) in number, and the similar primes to B are (?^), then (A"—!) is divisible by B, and (B""— 1) is divisible by A. " On the reabsorption of the Mixed Gases in a Voltameter." By Professor M. H. Jacobi, in a letter to Michael Faraday, Esq., F.R.S. Communicated by Dr. Faraday. The author found that if the mixed gases developed from the decomposition of water by a voltaic current, be allowed to remain in the voltameter in which they were collected, in contact with the fluid which produced them, they by degrees diminish in volume, and ultimately disappear by being absorbed by the fluid. He has not yet fully determined the precise conditions on which this phe- nomenon depends ; but he is inclined to think that it is owing to a portion of the mixed gases, diffused throughout the whole liquid, comipg into contact with the platinum plates, and being recombined on the surface of those plates ; and this process being renewed with every fresh portion of the gases which takes the place of the former, the whole of the gases are thus reconverted into water. March 4. — " Researches into the effects of certain Physical and Chemical Agents on the Nervous System." By Marshall Hall, M.D., F.R.S., &c. The professed object of the author, in the present paper, is " to detail the results of an investigation of the phenomena and the laws of production and action of certain secondary or induced conditions of the nervous system, which are effected by a voltaic, and proba- bly by any other electric current, but persistent after the influence of that current is withdrawn." This condition he designates by the new term electrogenic, as describing at once the origin and the inde- pendence of that condition. On the present occasion he confines Royal Society. 73 himself to the subject of the electrogenic condition of the muscular nerves, postponing to future inquiries that of the incident nerves and of the spinal marrow ; and also the modes of action of other physical and chemical agents, such as mechanical injury, heat and cold, strychnine, and the hydrocyanic acid. The bones and muscles of the brachial lumbar and pelvic regions of a frog, being isolated from all the other parts of the body, except- ing only by means of their respective brachial and lumbar nerves, which were perfectly denuded on all sides, and raised from the glass on which the limbs were laid, a voltaic current from a pair of the " couronne de tasses" was passed downwards through the nerves, in a direction from their origin in the spinal marrow towards their ter- minations in the muscles. Energetic muscular movements were at first excited ; and the current was thus continued during the space of five, ten, or fifteen minutes, and at the end of this period was withdrawn. No sooner was the current discontinued than the mus- cles were affected with spasmodic contractions, and with a tetanoid rigidity, constituting the secondary, or what the author denominates the electrogenic condition ; an effect, which as instantly subsides on the restoration of the voltaic current. ' The author proceeds to state the precautions which must be taken to ensure the success of experiments on this subject; and traces the effects of desiccation of the nerves from spontaneous evaporation, and 6f the application of external moisture, on the phenomena ; and also the modifications introduced by varying the extent of voltaic contact. Various experiments are then described, which the author instituted with a view to ascertain the nature of the electrogenic condition of the nerves, and the circumstances under which it is in- duced ; and he is led to the conclusion that the phenomena involve some voltaic principle which has not hitherto been fully investigated. March II. — "On the cause of the discrepancies observed by Mr. Baily with the Cavendish Apparatus for determining the Mean Density of the Earth." By George Whitehurst Hearn, Esq., of the Royal Military College, Sandhurst. Communicated by Sir John F. W. Herschel, Bart., F.R.S. After taking a summary review of the methods employed by Mr. Baily for determining, on the plan devised by Mr. Cavendish, the mean density of the earth, and of the anomalies, hitherto unac- counted for, which had introduced jierplexity in the results obtained, the author, suspecting that these anomalies had their source in the variable magnetic states of the masses which were the subject of experiment, traces the effects which such an influence might be supposed to have on those results. He finds that, the attraction arising from gravitation between a mass and one of the balls being exceedingly minute, an almost inconceivably feeble magnetic state may be the cause of great perturbations. He then proceeds to in- vestigate the subject by the application of mathematical analysis ; from which he is led to the conclusion that the masses and balls do actually exert on one another influences which are independent of the action of gravitation. He finds that such influences are of a 74 Royal Society. very fluctuating nature ; the action arising from them being either positive or negative, and its sign also changing in each revolution as the masses are turned round a vertical axis ; and he observes that such action may either fall short of that arising from gravitation or exceed it many times. Such disturbing force he conceives can be no other than a magnetic influence ; not however one of the ordinary kind, but that which Faraday has recently discovered as affecting all diamagnetic bodies. The author concludes by proposing methods by which the inquiry should in future be conducted, so as to obviate or eliminate this source of error. Such an inquiry, he remarks, would, by exhibit- ing the magnetic and diamagnetic powers under new aspects, lead, in all probability, to important consequences. March 18.—" Researches to determine the Number of Species and the Mode of Development of the British Triton." By J. Hig- ginbottom, Esq., F.R.C.S. Communicated by Thomas Bell, Esq., F.R.S. The observations of the author, of which he gives a detailed ac- count in the present memoir, have led him to the following con- clusions : — Two species only of the genus Triton are met with in England ; namely, the Triton verrucosus and the Lisso-triton punctatus. It is three years before the animal is capable of propagating its species, and four years before it attains its full growth. In its tadpole state, it remains in the water till its legs acquire suflficient strength to qualify it for progressive motion on land. While a land animal, it is in an active state during the summer, and passes the winter in a state of hybernation ; but does not then, as has been erroneously supposed, remain at the bottom of pools. Very dry, or very wet situations are incompatible with the preservation of life during the period of hybernation. At the expiration of the third year, the triton revisits the water, in the spring season, for the purposes of reproduction, and again leaves it at the commencement of autumn. Impregnation is accomplished through the medium of water, and not by actual contact. The growth and development of the triton are materially influenced by temperature, and but little by the action of light. The triton possesses the power of reproducing its lost limbs, provided the temperature be within the limits of 58° and 75° Fahrenheit ; but at lower temperatures, and during the winter, it has no such power. April 15. — " On the Proper Motion of the Solar System." By Thomas Galloway, Esq., A.M., F.R.S. The object of this paper is to communicate the results of a calcu- lation for determining the direction of the proper motion of the solar system from the apparent proper motions of stars in the southern hemisphere, deduced mostly from a comparison of the observations made by Lacaille at the Cape, about the middle of the last century, with the recent observations of Mr. Johnson and the late Professor Henderson at St. Helena and the Cape respectively. After adverting to the papers of Sir William Herschel in the Philo- Royal Society. 75 sophical Transactions for 1783 and 1805, and some other investi- gations of the same subject, the author remarks that up to a recent period astronomers seem generally to have entertained the opinion that our knowledge of the proper motions of the stars is not sufficiently advanced to enable us to pronounce positively either on the fact or the direction of the motion of our own system. This opinion was grounded on the discrepancies which present them- selves when it is attempted to explain the observed displacements of individual stars by referring them to the motion of the sun in an opposite direction ; it being always found that whatever direction is assigned to the sun's motion, there are many stars whose proper motions cannot thereby be accounted for. But if the sun be in motion it is very improbable that any star is absolutely at rest; hence the proper motions deduced from a comparison of catalogues must be regarded as the effect partly of the true proper motions of the stars, and partly of the apparent systematic or parallactic mo- tion caused by the displacement of the point of view ; and as we have no reason for supposing the true proper motion of a star to be more probable in one direction than in another, it may be expected, a priori, that the observed directions will form angles of all different values with the direction of the sun's motion, or any other fixed line. The observed discrepancies are therefore not incompatible with a general drifting of the stars towards a particular region of the heavens ; but in order to deduce the direction of the systematic motion, it becomes necessary to take account of a very considerable number of proper motions, and to represent them by equations, involving the unknown quantities required for determining the direction of the sun's motion, and to solve the equations so as to obtain the most probable values of those quantities. The first person who investigated the subject under this point of view was Professor Argelander of Bonn, in a paper published in the Petersburg Me- moirs for 1837. From the proper motions of 390 stars deduced from a comparison of Bessel's catalogue of Bradley's observations with his own catalogue of stars observed at Abo, Argelander found the direction of the sun's motion, for 1792*5, to be towards the point of the sphere whose right ascension is 259° 47'*6 and declination -1-32° 29'*5. Lundahl, subsequently, from a comparison of the places of 147 stars in the catalogues of Besseland Pond, and not included among those considered by Argelander, found the co-ordinates of the point to be ^=252° 24'-4, Dec. + 14° 26'-l ; and Otto Struve, still more recently, from the comparison of about 400 of Bradley's stars with the positions determined at the Dorpat Observatory, ob- tained the result ^=261° 23'-l, Dec. + S7° 35'-7. The mean of those results taken with respect to their probable errors, was found by O. Struve to be ^=259° 9'-4, Dec. + 34° 36'-5. All the stars included in the calculations of Argelander, Lundahl, and O. Struve being situated to the north of the tropic of Capri- corn, it appeared to be a point of some interest to determine whe- ther the southern stars agree with the northern in their indication of the direction of the solar motion, or afford any confirmation of 76 Royal Society, the hypothesis of the sun's translation. Unfortunately, we have no observations made in the southern hemisphere in the last century equal in precision to those of Bradley, but the catalogue given by Lacaille in his * Astronomise Fundamenta,' furnishes a means of comparison of considerable value in reference to the present in- quiry. In Mr. Johnson's 'Catalogue of 606 Stars in the Southern Hemisphere' (London, 1835), there are sixty-one which, on com- paring their places in 1830 with those of Lacaille reduced to the same epoch, appear to have sliifted their positions not less than 8" in space in the interval of eighty years between the epochs of the catalogues, or to have an annual proper motion of not less than one-tenth of a second in space. Prof. Henderson's catalogue (Mem. 11. Astron. Society, vols. x. and xv.) furnishes thirty-six stars, which, on a like comparison, appear to have an annual proper motion ex- ceeding the same limit. Of these, however, thirty-two are contained in Mr. Johnson's catalogue, but Henderson gives the proper motions of sixteen other stars (in the southern hemisphere), from the com- parison of his own places with those of Bradlej'-. On the whole, therefore, the two catalogues furnish eighty-one different stars whose proper motions are given both in right ascension and declination. The method of investigation is the same as that of Argelander. From the differences of M. and Dec. given by comparison of the cata- logues, the direction of the apparent motion of each star is com- puted. It is then assumed that the sun is moving towards a point whose right ascension A=259° 46'*2 and declination D=-f-32° 29'*6 ; and the direction in which each star would appear to move, if it were itself at rest, is computed on this hypothesis. The differ- ence of these two directions is treated as an error of observation, and its numerical value substituted for the differential of the angle which determines the direction of the parallactic motion ; this diffe- rential being expressed by a formula containing the differentials of A and D multiplied by known coefficients. An equation is thus obtained of the form 0 = ac? A -fMD+w, in which a, b, and n are known quantities. Each star furnishes a similar equation ; and the equations, being first multiplied respec- tively by the sine of the star's distance from the point assumed as the apex of the sun's motion, in order to give them all the same weight, are solved by the method of least squares, and the result- ing values of c? A and dT) applied as corrections to the assumed values of A and D. The results are as follows: — the whole of the eighty-one equations give (for 1790) as co-ordinates of the point towards which the sun's motion is directed, ^=263° 38'-0 + 5° 14'-5 ; Dec.=:-f 37° 15'-0+6° 17'-6. But two of the stars compared with Lacaille move in a direction so nearly opposite to that of their motion on the assumed hypothesis, that (in one case especially) a slight error of observation would change the sign of n in the equations of condition. It therefore appears necessary to reject those two stars ; and a further reason Intelligence and Miscellaneous Articles. 77 for rejecting them is, that they are both situated within 8° of the pole, in which position Lacaille's determination of the right ascen- sion is probably not to be depended upon. Setting aside, there- fore, the two stars in question, the remaining seventy-nine equa- tions give M^'ISQ" 51'-5 + 4° 45'-l ; Dec.= + 34° 14.'-3+5° 36'-2. The author further observes, that one of the stars compared with Bradley's catalogue is also remarkable as appearing to move in a direction nearly opposite to the mean direction of the whole, and that if this star be rejected also on account of the great probability there is that the parallactic motion is in this case concealed by the larger proper motion of the star itself in an opposite direction, the co-ordinates of the solar apex become ^=259° 47H+4° 31'-9 ; Dec.= +34° 19''5 + 5° 17'-7, a result differing less than a degree either in right ascension or de-^ clination from the mean, as above stated, of the three previous de- terminations. XIII. Intelligence and Miscellaneous Articles. ACTION OF CHLORINE ON ALCOHOL. — FORMATION OF ACETAL. MSTAS states that he has observed that the causes which give • rise to acetal are not always oxidating causes. When chlorine is made to act upon alcohol, acetal is the principal product, as long as it does not act by substitution, and it is at once a dehy- drogenating and an oxidizing body. This discovery, the author is of opinion, throws great light on the hitherto obscure action of chlorine upon alcohol. In order to obtain acetal by the action of chlorine upon alcohol, it is sufficient to pass a current of chlorine into alcohol of 80 per cent., cooled to 50° or 60° F. The action is to be discontinued when chlorinated bodies commence formation by substitution : this is readily ascertained, for the alcohol then becomes turbid on the addi- tion of water ; the liquid, which has become very acid, is to be di- stilled, and one-fourth of the quantity is to be preserved. This is to be neutralized by means of chalk, and by a fresh distili3,tion one- fourth of the product is again to be obtained ; in this fused chloride of calcium is to be dissolved, which immediately separates a large quantity of a very volatile fluid, containing, like common rough acetal, aldehyd, acetic aether and alcohol ; by the addition of more chloride of calcium, the utmost quantity of alcohol and acetic aether are separated ; the purification of the acetal is to be completed. The analysis of the acetal thus obtained was similar to that pro- cured in the usual way ; and thus the chlorine acts, as already stated, both as a dehydrogenating and oxidizing body: C''^H'*0^-f- 2Ch-2HO=C'2H'<0* + 2CH + 2HO.— Jw». de Chim. et de Fhys., Feb. 1847. 78 Intelligence and Miscellaneous Articles. BISILICATE OF IRON OR FERRUGINOUS PYROXENE. This new mineral is described in a memoir presented by M. Du- fr^noy to the Academy in the name of M. Gruner, mining engineer, and Professor in the School of Mines at St. Etienne. It corresponds in composition to a pyroxene with a base of iron. M. Gruner states that this mineral resembles certain varieties of asbestos, or more nearly fibrous amphibole. Its specific gravity is 3* 7 13, which exceeds that of the densest epidotes, amphiboles or pyroxenes. By analysis M. Gruner obtained — Silica 43-9 Protoxide of iron 52*2 Lime '5 Magnesia , . . . 1 ' 1 Alumina 1*9 99-6 Admitting that the greater portion of the foreign bases is derived from a small quantity of the gangue, it will be seen that this mineral is bisilicate of iron, or ferruginous pyroxene with one base only. — Comptes Rendus, Mai 5, 1847. CHLOROSULPHURET OF SILICIUM. M. Isidore Pierre states that M'hen hydrosulplmric acid and chlo- ride of silicium in vapour are passed through a porcelain tube heated to redness, they react upon each other : much hydrochloric acid is produced, which is disengaged with excess of hydrosulphuric acid gas and a little chloride of silicium, which escapes the reaction. If the products of this reaction be passed into a U-shaped tube immersed in cold water, a fuming liquor condenses, which has a sharp foetid odour, resembling that of hydrosulphuric acid and chloride of sulphur. The liquor thus obtained was slightly opake by sul- phur suspended in it: this was deposited by being left forty-eight hours in a well- stoppered bottle. There were also deposited on the sides of the bottle, clear lemon-yellow crystals, which were sulphur in the form of oblique rhombic prisms, without any modification. The condensed liquor has consequently the power of dissolving sulphur, and of depositing it in crystals belonging to the same system as those which are obtained in the dry way. The smallness of these crystals prevented the author from determining their angles ; but he reckons upon being able soon to do so. No sensible traces of sul- phuret of silicium were found in the minute deposit produced in the porcelain tube. The liquid condensed in this operation was distilled in an oil-bath from a retort furnished with a thermometer : the more volatile por- tions, which usually distil from 140° to 176° F,, were rejected. They consist principally of chloride of silicium mixed with a small quantity of chlorosulphuret. Afterwards there is obtained a limpid colourless liquid which fumes in the air, and has an odour resembling that of chloride of silicium and hydrosulphuric acid. Meteorological Observations. 79 Its specific gravity at 60° F. is about 1 "45 ; that is, a little less than that of chloride of silicium. When it is thrown into water, it occasions an abundant disengagement of sulphuretted hydrogen gas and a slight deposit of sulphur. It boils at above 212" F. ; but the small quantity obtained did not allow of ascertaining its exact boil- ing-point. By analysis, it yielded such proportions of its constituents as to indicate for its formula CP S Si, which would give — Chlorine 65-47 Sulphur 14-83 Silicium '. 19-70 10000 M. Pierre proposes the name of chlorosulphuret of silicium for this compound. — Ibid, Mai 5, 1847. METEOROLOGICAL OBSERVATIONS FOR MAY 1847. Chiswick. — May 1, Very fine. 2. Cloudy. 3. Rain, 4. Cloudy. 5. Cloudy and fine. 6. Slight fog : fine. 7. Overcast: showery. 8. Rain. 9. Fine: cloudy: densely overcast : rain. 10. Very fine : slight showers, 11. Cloudy. 12. Very fine. 13. Cloudy and fine t showers. 14. Showery. 15. Fine: rain at night. 16. Rain: cloudy: rain at night. 17. Cloudy. 18. Fine: rain. 19,20. Cloudy and fine. 21,22. Very fine. 23. Very hot and sultry. 24. Cloudy and fine. 25 — 27. Very fine. 28. Slight haze : sultry. 29. Cloudy : thunder and heavy rain. 30. Clear and fine. 31. Cloudless: exceedingly fine. JNlean temperature of the naonth 56°*83 Mean temperature of May 1846 56-16 Mean temperature of May for the last twenty years ... 55 '01 Average amount of rain in May 1 "84 inch. Boston. — May]. Fine. 2. Cloudy: rain early a.m. : rain p.m. 3. Cloudy: rain A.M. and P.M. 4. Cloudy. 5. Fine: rain p.m. 6. Cloudy. 7. Fine: rain P.M. 8, Cloudy : rain P.M. 9. Cloudy. 10. Cloudy : rain early a.m. II. Rain. 12. Fine: rain, with thunder i'.m. 13. Fine: rain p.m. 14, 15. Fine: rain early a.m. 16. Rain: rain, with thunder p.m. 17. Cloudy. 18. Cloudy; rain p.m. 19, 20, Cloudy, 21—24. Fine. 25. Windy. 26, 27. Fine. 28. Fine : 1 o'clock p.m. thermometer 82°. 29. Rain : 4 o'clock a.m. thunder, hail and rain : rain all night. 30. Fine : rain early a.m. 31. Fine. Sandmck Manse, Orkney. — May 1. Bright: clear. 2. Bright: drops. 3. Bright : clear. 4. I3right : damp. 5. Fine. 6, 7. Cloudy : damp. 8, 9. Drizzle: fog. 10. Clear : fine. 11. Cloudy : rain. 12. Rain ; cloudy. 13. Cloudy. 14. Rain: fog. 15. Damp: rain : fog. 16. Bright : cloudy. 17, 18. Cloudy : clear. 19. Showers: drizzle. 20. Fog : cloudy. 21. Bright: rain. 22. Showers. 23. Clear. 24. Fine. 25. Bright : cloudy. 26. Bright : showers. 27. Fine : clear. 28. Fine : cloudy : fine. 29. Rain: thunder: cloudy: fine. 30. Clear: fine. 31. Cloudy: fine. Applegarlh Manse, Dumfries-shire. — May 1. Fine summer day. 2. Mild: showers. 3. Cloudy : keen. 4. Spring, but keen. 5. Cold : wet p.m. 6. Grow- ing: wet P.M. 7. Dull : showers. 8. Dull : wet p.m. 9. Mild: dull: wet p.m. 10. Fine growing day. 11 — 14. Dull: showers. 15. Fine summer day. 16. Stormy : wet all day. 17. Wet and cold. 18. Wet and stormy. 19. Dull: wet. 20. Sunshine : fine. 21. Dry : cloudy. 22. Cloudy : showers. 23. Warm : thunder: rain. 24. Fine : clear : wet p.m. 25. High wind : clear. 26. Fine: clear : light : cloudy. 27. Fine : clear: thunder. 28. Fine : wet p.m. 29. Fine : heavy rain P.M. 30. Fine : warm. 31. Remarkably fine. Mean temperature of the month 51°*1 Mean temperature of May 1846 52 '6 Mean temperature of May for twenty-five years 5i "1 Mean rain in May for twenty years 1*69 inch. '9JIIJS -saujiund •jjoiAvsiqo « : «s o o TfiC'^'* •'-<<^^ooo^o^ • CJ — — oo :ooo — o :o : in 'Xau^JO I i S S' « i i « « « « c; cs « « « S s 1 1 ^* s:' s' ^ " «• i « ^ S 2 •ajiqs -sauj'iuna ^i^^^'^il^i^^'i'^iii^iilii^^i ^ ^ ^ i i s s i^^^ii .' ^i-^ii^iiill i i i ^ i ^ ^ii^ ^'-g-g •5lO!aiS!q3 Sf A aJ to a3 u5 is fe' ^* ^ ^ SJ 5f fe ^ w ^ S a 6t B: fe > ^ a; m w ^ g" O »! ?6 Sic Q •XBJ\[ •W8 ¥8 •uo^soa •U!H -eig 00 ONfooo o oo mr^oo o^o "o ^^o^^^o^-- OMn-^-^ i>-t~o -«>g •UOJSOa JO sXbq 2S O^O^O^O^C> O^O^O^C^^O^O^C?^O^O^O^O^o^C C^O^O^O^O^a^O^O^O o^o^O O O^St^C•^OOIO^o«^C^Olomt:^coO<^lTtl>.o^^OO^OOO^C^^O•^-HlO ■^d

p'piprO'P'7<'0 "^r^oo 0^ r^\ rT\ (T\ fTN 0^ ON (?T\ f^T\ fT\ 0\ f?s f^s CTS CTS ON 0\ '5N 0\ ON ON 0\ ON 0\ ON ON ON (TN rTN CTN C^N /TN C^O^O^O^O^O^o^o^O^O^CNO^O^O^O^^^O^O^O^O^C^C^O^O^O^c^^o^(^O^ONC^ C< lO t^OO lO < ■<* CO 00 00 -^ •^ cj us QO t^OO 00 On -^ CO in Ti>oo CO lO (N ON > CO r^r^ip \ ON Cn On On CO 00 — o vs T* T 9^ 6 6 ON COCOOI CO -^00 (N QO o^ o — ^!pH^>- i ^''s constants which depend only on the elliptic constants of the planet tw, and such that ^ = cos TT + 2 sin^ — sin (tt — v) sin v, 3"= — sin 7r+2 sin^— cos (tt — v) cos V, ^ = sin TT — 2 sin^ — - sin (w — v) cos V, (J = cos TT— 2 sin^ — cos (tt — v) cos v, 3"= sin(7r— v) sin i, ^= cos (tt— v)sin I. * I have had occasion to use so many alphabets in the course of the work from which this is extracted, that I have had recourse to this artifice of reversing the letters in order not to use the same symbol in two different significations. 88 Sir J. Lubbock on the Perturbations of Planets Mr. Farley has calculated for me a table of the values of these quantities for all the planets, and also for the comet of Encke, the comet of Bieia, and the comet of Halley. ciR m' a' f gtt' 7- J, ,, , ui-^l — = r^ 0-2--, -cosff — »){! +>•} * >•. [X, }L r \^ r a ^ 'J l+P=l-^^{{^^Cos/-l3^sin/}f;cos/' + {C^cos/+^rsin/}isin/'} + cH ci' V 7' I r I call the quantities -^ cos/', -jSin/', - cos^ — sm/, -5, a'2 --J25 &c. the elementary quantities, because they are the elements which, by means of various Combinations, form the disturbing function IL —z—, &c., and if the numerical values of the con- ar slants are introduced before the development is begun are alone required. Mr. Farley has calculated the coeflicients of these quantities when they are developed in terms of the mean motions for the planets, and also other tables for eccentricity, •1, -2, ... . •?, which show the convergence to be so slight, that such mode of development can only be employed when the eccentricity is small. These tables have all been con- structed by means of mechanical quadratures. These tables are not wanted for the comets, because their co-ordinates cannot be developed in terms of their mean anomalies in suf- ficiently converging series. When the method of mechanical quadratures is applied to the determination of the perturbations of comets, a correction is required ; but when that method is used for the determina- tion of coeflicients of this nature, the limits of the integral are 0 and 360°, and the correction vanishes ; so that by means of several particular values, rigorous values of the coeflicients are easily obtained. Nor does the width of the interval matter, provided it is not made too large. It is difficult to give pre- • cise rules to regulate the width that should be employed ; but in the formation of these tables it was easy to employ various modes of verification. As this inquiry is in its infancy, I considered it sufficient to retain only those terms which are moving in Eccentric and Inclined Orbits. 89 due to the elliptic motion ; but hereafter it may be desirable to reconstruct the tables of the elementary quantities for each of the planets, retaining some of the principal inequalities due to the disturbing force. Pingre, in his work On comets rtiariy years since, gave a list of comets, with their elements. At that time, however, the method of finding the orbit, or even the distance of a comet, was understood by so few persons, that, from that and other causes, the numbers contained in that table may not be accu- rate: many other comets have been discovered since, and such a table brought Up to the present tittle appears tO be an impor- tant desideratum in astronomy. Mr. Hind has kindly favoured me with the following list of comets which have been made out to be periodic: — Elements of Halley's comet, by Westphalen, for 1835. Ast. Nach.^ No. 588. ^=•96739 7r = 304° 31' 32"-19 v = 55° 9' 59"'S^ i=\T ^b' 5"'\S a=17'9879i Retrograde. Elements of Encke's comet by Encke, for 1829. Ast. Nac/i., No. 489. f =-84462 ff=157° 17' 53"-35 v = BW 29' 3i"*62 i = 1 3° 20' 34"'49 a = 2-22394 Direct. Elements ofBiela's comet, 1846j by Prof. Plantamour. Ast. Nach., No. 584. ^ = •75700 7r=109° 2' 20"-10 v = 245° 54' 38"-8 »=12° 34' 53"-47 a = 3-52452 Direct. Elements of the comet of Faye, by M. Le Verrier, for 1844, omitting the terms multiplied by jw,". Ast. Nach., No. 541. €='55596 7r = 49° 34' 19"-39 v = 209° 29' 19"'26 1 = 11° 22° 31"-40 a = 3-81179 Direct. Elements of DeVico's first comet,byDr.Brunnow, for 1844. Ast. Nack., No. 563. ^=•61765 7r = 342° SO' 49"-64 v = 63° 49' 0"-l 1 « = 2° 54' 50"-33 « = 3- 10295 Direct. Elements of Brorsen's first comet, byDr.Brunnow,forl846. Ast. Nach., No. 557. ^ = •79362 7r=116° 28' 34" i/= 102° 39' 36"'3 » = 30° 55' 6"-6 a = 3-1502l Direct. The following are the elements of the comet of Encke for 1829 used by M. Hansen : Additions a la Conn, des Temps, 1847, p. 54. ^ = •844676 ' *f=157° 18' 24"'6 v^334° 29' 28"-8 »=i3° 20' 40"-2 a = 2-21997. Ast. Nac/i.y No. 5^1. [ 90 ] XVI. On the Heat of Vapours. By Sir J. Lubbock, Bart.^ F.R.S.* T ET V be the quantity of absolute heat, considered as a -■-' function of the sensible heat or temperature 9, p being the density, p the pressure, k and u constants, dp _ «p dp _ up dQ~~ l+uQ dS "" l+«fl* If c is the specific heat of a gas, the pressure being con- stant, and Cf its specific heat when the volume is constant, so that _dFdp _dfd^ _£ """dpdfl ""''dpdQ '^^ c, dV dV ^ ^d7+y^d^=^- Laplace evidently considered 7 constant, and he integrated this equation upon that hypothesis, " En supposant cette quan- tite rigoreusement constante, &c.," Mec. Cel. vol. v. p. 127. Again, Poisson, in repeating the same theory, Traite de M^c, vol. ii. p. 6^Q, "En regardant y comme une quantite constante, &c." If y is constant, 2. V=A + B^^=A + B-(-+^p^-\ p a \u / (see vol. xviii. p. 507) which is identical with the equation given in the Comptes Rendus, Seance de 31 Mai 184'7, p. 920, q=m-\-n{a-\-t)p-'^, m — A, n= — , a= —, t=9. 2;=! , A: = y; a. a. y but if, as Professor Holtzmann maintains (see Taylor's Sci- entific Memoirs, vol. iv. part 14), z is variable, the integral of Laplace does not necessarily obtain, nor does the equation {Comptes Rendus, p. 920) obtain ; because if s is a function of t, -^^^7ip-^-n{a-\-t)p-<'\ogp-^, * Cuiumunicated by the Author. Mr. Grove on the Decomposition of Water by Heat. 91 and q—q^=zn{a-\-t)p-'' —n{a-^t^)p^-\. It has not, I believe, been remarked, that the integral ? will however still satisfy the differential equation If or pAV , AV ^ f> dp 50*658 matter and loss . . J 100-000 No. 3. This water is from a large pond similar to that from which No, 1 is taken, but from a different part of the country, and a much larger body of water. It was clear, containing but very little suspended matter. 100,000 grains left on evaporation 50*68 grains of solid residue, which consisted of, per cent., — Protoxide of iron .... 2*584 Lime 17*829 Magnesia 1-530 Soda 30*232 Potash ....... 15-762 Sulphuric acid 11-627 Muriatic acid 2-580 Phosphoric acid .... no trace Carbonic acid, with organic^! , >, ^ -^ 11 ° ^ 17*856 matter and loss • • J 100-000 No. 4. This water is from the river Lys, so celebrated for its steeping qualities. It was taken from the river in France before it had reached the highest retting place. The specimen was clean, but there was some suspended matter, principally organic. 100,000 grains, evaporated to dryness, left a residue of 45-1 1 grains, consisting of, in 100 parts, — Protoxide of iron .... 6-200 Lime 5-484 Magnesia 1-192 Soda 28-298 Potash 5-405 Sulphuric acid 9*300 Muriatic acid 7*754 Phosphoric acid .... -079 Carbonic acid, with organic"! matter and loss . . J___^ 100-000 Phil. Mag. S. 3. Vol. 31 . No. 206. Aug. 1 847. I 114 Mr. J. P. Joule on the Theoretical Velocity of Sound. No. 5. This watei'' was from a retting pit in Holland. 100,000 grains, evaporated to dryness, gave a residue of 42*4< grains, which consisted, per cent., of — Protoxide of iron . . . . 1*183 Lime ... . . . . . 3-613 Magnesia 7-601 Soda 19-277 Potash 8-205 Sulphuric acid 5*607 Muriatic acid ..... 9*439 Carbonic acid, with organic! a ^ r^^r- a\ f 45-075 matter and loss. . . J 100-000 With regard to the constitution of these several specimens of water, it can only now be remarked, that in all there was present a large quantity of mineral impurities ; and that in Nos. 2 and 4, the very samples which are of the most remark- able and celebrated steeping waters in Belgium, a large quan- tity of iron is present, so that they might be in a degree termed chalybeate waters. How this regards their excellence for preparing flax 1 do not pretend to say, and indeed it will require much more extended investigation before a satisfactory solution of it can be given. All these waters are further remarkable for containing a larger quantity of potash than ordinary waters are found usu- ally to have. I shall not, however, enter minutely into the discussion of their constitution, as I shall have to resume the subject at another time; and I wish only to place on record for the present the analytical results which the samples of waters forwarded to me from Belgium by Mr. Marshall, had afforded. XXI. On the Theoretical Velocity of Sound. By J. P. Joule *. THE celebrated French mathematician De Laplace has, it is well known, pointed out that the heat evolved by the compression of air is the cause of the velocity of sound, according to the theory of Newton, being so much less than that actually observed. He has also given a formula by which the velocity may be determined when the ratio of the specific heat of air at constant pressure to that at constant volume is known. The determination of the elevation of temperature in air by compression has however been hitherto attended with difficulty, and hence the theorem of De Laplace has never yet been fairly compared with experiment. I was therefore anxious * Communicated by the Author. Mr. Nicholson on the Composition of Caffein. 115 to ascertain how far the mechanical equivalent of heat, as de- termined by my recent experiments on the friction of fluids, might be able to contribute to clear up this question. The capacity of air at constant pressure, according to the experiments of De la Roche and Berard, is 0*2669. Conse- quently a quantity of heat capable of increasing the tempera- ture of a lb. of water by 1°, will give 1° also to 3'747 lbs. of air, while the air will be expanded i^^j', an expansion in which a force equal to 200*7 lbs. through a foot is expended in raising the atmosphere of the earth. The equivalent of a degree of heat per lb. of water, determined by the careful experiments brought before the British Association at Oxford, is 775 lbs. through a foot. Hence 200*7 lbs. through a foot is equal to 0°-259. We see, therefore, that for every degree of heat employed by Qe la Roche and Berard in expanding and heating air, 0°'259 was occupied in producing the mechanical effect, leaving 0°*741 as that actually employed in raising the temperature of the air. Hence the actual specific heat (commonly called capacity at constant volume) is 0*2669 x 0*741 = 0*1977. Ta- king this as the specific heat of air and the equivalent 775, it follows that if avolume of air of 17r6 cubic inches be com- pressed to 170*6 cubic inches, it will be heated 1°, a quantity of heat which will occasion an increased pressure of ^|y. So that the celerity of sound will be increased by this means in the subduplicate ratio of 491 to 661*6, or in the simple ratio of 2216 to 2572, which will bring it up from Newton's estimate of 943 to 1095 feet per ", which is as near 1130, the actual velocity at 32°, as could be expected from the nature of the experiments on the specific heat of air, and fully confirms the theory of Laplace. Oak Field, near Manchester, July 17, 1847. XXII. On the Composition of Caffein, and of some of its Compounds. By Edward Chambers Nicholson, Esq."^ /^AFFEIN was first analysed by Professors Liebig and ^^ Pfafft in 1832. The result of this investigation was confirmed by a subsequent analysis of Prof. Wohler %. In 1838 Professor Liebig induced M. Jobst § to analyse thein, who proved this body to be identical with caffein. His analyses gave the same results as his predecessors. The same remark apphes to the experiments of Mulder I| on thein, * Communicated by the Chemical Society; having been read Feb. 15, t Liebig's Jnnalen, i. 17. % Ibid. § Ibid. xxv. 63. II Bulletin des Sciences Phys, et Nat. de Neerlande. 1838, p. 32. 12 116 Mr. Nicholson on the Composition of Caff em, and also to an analysis which M. Martins * made of guaranin, a substance, the identity of which with cafFein and thein had previously been pointed out by Berthemot and Dechastelusf. Lately Dr. Stenhouse :j:, when examining Paraguay tea, has also made some analyses of thein. The following table, in which I have recalculated these ana- lyses according to the atomic weights, carbon 6 and hy- drogen 1, allows a comparison to be made of the results ob- tained by these chemists. Mean of the Analyses. CafFein. Thein. Guaranin. -> Liebig & Pfaff. Wohler. Mulder. Jobst. Stenhouse. Martius, Carbon » 49-30 49-25 49-18 49-47 48-95 49-23 Hydrogen 5*22 5-43 5-49 5-20 5*15 5-08 Nitrogen. 28-86 28-53 28-90 28-83 The most simple expression which can be deduced from these numbers is Cs Hg Ns O^. Stenhouse's analysis however of the platinum compound proves that this formula must be doubled, and that the atom of cafFein or thein is CjsH.oN^O^. The theoretical numbers of this formula are the following: — 16 eqs. Carbon ... 96 49-48 10 ... Hydrogen . . 10 5-15 4 ... Nitrogen . . 56 28-86 4 ... Oxygen . . . _32 16-51 ] 94 100-00 From these numerous experiments the composition of caf- fein might have been considered as perfectly established. In a recent investigation of coffee, however, M. Payen§ states that he has obtained results which differ very sensibly from those obtained by his predecessors, and which he has trans- lated into the formula which contains 1 equiv. of oxygen less than the formula up to the present time admitted. The theoretical numbers of Payen's formula are — 16 eqs. Carbon . . . 96 51*43 10 ... Hydrogen . . 10 5*35 4 ... Nitrogen . . 56 30-34 3 ... Oxygen . . . ^ 12-88 186 100-00 * Liebig's Annalen, xxxvi. 93. t Ibid, xxxvi. 90. % Mem. Chem. Soc, vol. i. pp. 215, 237. [Phil. Mag., xxiii. p. 426.] § Compies Rendus de I'Academie, tome xxiii. 8. and of some of its Compounds, 117 We observe here a difference of 2 per cent, of carbon, which M. Pay en has obtained over the results of the above-men- tioned chemists. In order to elucidate this discfTepancyy Dr. Hofmann in- duced me to make some experiments under his direction, partly m ith a quantity of beautiful caffein \vhich he gave me* and partly with a specimen which I have prepared myself. Caffein, To ensure perfect purity of the substance it was crystal- lized three times from dilute alcohol, washed and dried. Thus purified, it formed very beautiful long white prisms, perfectly transparent when dried in the air, but which became opake if exposed to a higher temperature. The crystals dried in the water-bath lost no weight when kept in an air-bath for four hours at a temperature of 130° C. The specimen which I had prepared myself was obtained from Costa Rico coffee, by boiling the bruised fruit in water, precipitating the decoctions by basic acetate of lead and treat- ing the filtrate with hydrosulphuric acid ; after the whole of the lead had been removed, I evaporated the liquid to dry- ness in a water-bath, in order to get rid of acetic acid, and dissolved the residue in a small quantity of boiling water : upon cooling, the caffein crystallized out of a dark colour, and very impure. To purify it, it was washed and recrystal- lized three times from water, and finally from alcohol. It was then perfectly white, and had exactly the same appearance as the specimen which I obtained from Dr. Hofmann. Analysis. I. 0*3827 grm. of substance, dried at 100° C. and burnt with chromate of lead, gave 0*6948 grm. of carbonic acid, and 0'1800 grm. of water. II. 0*417 grm. of substance, burnt with chromate of lead and chlorate of potash, gave 0*7552 grm. of carbonic acid, and 0*1965 grm. of water. III. 0*3934 grm. of substance of my own preparation gave 0*7123 grm. of carbonic acid and 0*1878 grm. of water, which calculated in 100 parts gives — I. II. III. Carbon . . . 49*51 49*39 49*37 Hydrogen . . 5*22 5*23 5*30 * I owe this specimen, of great beauty, to the well-known kindness of Mr. E. Merck of Darmstadt.— A. W. H. 118 Mr. Nicholson on the Composition of Caffein, which agrees with Professor Liebig's formula, as is seen by the following : — Mean of experiments. 49-42 5-28 Theory. 16 eqs. Carbon . . . 96 49-48 10 ... Hydrogen . 10 5-15 4 ... Nitrogen . . 56 28-86 4 ... Oxygen . . . 32 16-51 194 100-00 Caffein and Bichloride of Platinum, On precipitating a solution of cafFein in hydrochloric acid with bichloride of platinum, as Dr. Stenhouse has shown, a precipitate of an orange-yellow colour is obtained. If the two solutions are mixed hot, the fluid on cooling deposits the com- pound in beautiful granular crystalline tufts, which, when thrown on a filter and washed with alcohol, are perfectly pure. This double salt is only sparingly soluble in alcohol, aether, and water. It does not alter when exposed to light, nor does it lose in weight when kept at 100° C. for a considerable time. The analyses of salts, all prepared at different periods and dried at 100° C, gave the following results: — I. 0'5382 grm. of substance, burnt with chromate of lead, gave 0-4765 grm. of carbonic acid, and 0-1387 grm. of water. II. 0*4881 grm. of substance gave 0*1196 grm. of platinum. III. 0-4779 grm. of substance gave 0-1172 grm. of pla- tinum. IV. 0*6022 grm. of substance gave 0-1482 grm. of pla- tinum. V. 0*5781 grm. of substance gave 0-1425 grm. of pla- tinum. VI. 0-5246 grm. of substance gave 0*1293 grm. of pla- tinum. VII. 0-3847 grm. of substance made of caffein of my own preparation, gave 0-0945 grm. of platinum. Which give the following per-centages : — I. II. III. IV. V. VI. VII. Carbon . 23-80 Hydrogen 2-86 Platinum ... 24-51 24-52 24-60 24*64 24-64 24-56 leading exactly to the formula given by Dr. Stenhouse, viz. Ci6H,oN4 04HCl,PtCl2, as is seen when placed in comparison with the calculated numbers. and qf some of its Compounds. 119 Theory. Mean of my experiments. Dr. Stenhouse's mean. 16 eqs. Carbon . 96-0 23-97 23-80 24-22 11 ... Hydrogen . 11-0 2-74 2-86 2-89 4 ... Nitrogen 56-0 13-98 4 ... Oxygen . . 32-0 8-02 3 ... Chlorine . . 106-5 26-59 * 1 ... Platinum 98-9 24-70 24-58 24-49 1 ... CafFein and' bichloride -400-4 100-00 of platinum The analysis of cafFein, as well as that of the platinum compounds, agree so perfectly with the numbers of Professor Liebig's formula, that there can be no doubt about its accu- racy. Assuming 1 equiv. of oxygen less in the equivalent of caf- fein, as is proposed by M. Pay en, the platinum compound should contain not less than 24-46 per cent, of carbon and 25-12 of platinum. Now three determinations by Dr. Sten- house, and six which I have made, never gave more than 24-64 per cent., that is, 0-6 per cent, less of platinum. Not satisfied, however, with these proofs, I have tried to find some other compounds by which the atomic weight of cafFein could be determined with equal accuracy. In what follows a description of several new double salts of cafFein will be given, the analyses of which correspond equally well with the original formula of this substance. Caffein and Nitrate of Silver. This compound is obtained when a solution of nitrate of silver is added in excess to an aqueous or alcoholic solution of cafFein. If the solutions are concentrated it falls down in white hemispherical nodules, which adhere firmly to the side of the vessel. When washed with water and crystallized from alcohol it is absolutely pure. This compound is indistinctly crystalline, of a perfectly white colour, and if dry undergoes no change when exposed to light, but if moist acquires a purplish hue. It is very soluble in hot M'ater and alcohol, sparingly soluble in cold, and may be boiled in either solvent without vmder- going decomposition. It loses no weight in the water-bath, but at a higher temperature it is decomposed, cafFein sublimes, and metallic silver is left. Analysis. — When burnt with chromate of lead — I. 0-4514 grm. of substance gave 0-4345 grm. of carbonic acid, and 0'1162 grm. of water. 120 Mr. Nicholson on the Composition of Caffein, II. 0*2500 grm. of substance gave '0744 grm. of silver. III. 0*2716 grm. of substance gave '0810 grm. of silver, which give the following per-centages : — I. II. II. Carbon . . . 26*45 Hydrogen . . 2*86 Silver 29*76 29*82, and the formula — Cjs Hjo N4 O4 + AgO, NO5, as may be seen by the following calculation : — Theory. Found. 16 eqs. Carbon . . . 96 26*37 26*45 10 ... Hydrogen . . 10 2*74 2*86 5 ... Nitrogen . . 70 19*23 10 ... Oxygen . 80 22*00 1 ... Silver . . . 108 29*66 29*79 364 100*00 The only analogues to this singular compound which I know are those of urea and nitrate of silver, analysed by Wer- ther* : the formulae of which are— Co H4 Ng Og + Ag O, NO5, andC,H4N,0, + 2(AgO,N05). These compounds, however, in consequence of the peculiar nature of xarea, are not very stable, being decomposed when boiled with water into nitrate of ammonia and cyanate of silver. There likewise exists a compound of nitrate of silver and glycocoll, lately described by Horsfordfj having the for- mula C4H4N03+AgO,N05; and, according to H. Rose, a compound of nitrate of silver with ammonia, 3 equivs. of this gas being absorbed by 1 equiv. of the former salt. Chloride of Mercury and Caffein. This beautiful compound is obtained w^hen an aqueous or alcoholic solution of caffein is added to a solution of chloride of mercury ; the latter being kept in excess, the fluid remains perfectly clear, but after the lapse of a few seconds solidifies into a mass of very small crystals, W'hich when recrystallized from water or alcohol and washed on a filter, are quite pure. "When pure and crystallized from water it is very similar in appearance to caffein, the crystals not being however quite so large. It is very soluble in alcohol and water, hydrochloric, nitric, and oxalic acids, and seems to form with the latter a crystalline compound. It is nearly insoluble in aether. In reference to its constitution, it is distinguished from the dou- * Liebig's Annalen, Ivi. 262, t Ibid. Ix. 36. and of some of its Compounds. 121 ble salt of platinurrij for in this instance the cafFein is in direct combination with the chloride of mercury, and is exactly analogous to the corresponding compounds of leucoline and aniline investigated by Dr. Hofmann*. The mercurial com- pounds of this kind are generally easily decomposed, but the compound of chloride of mercury and cafFein is so stable, that it may be boiled in water for a considerable time without un- dergoing the slightest change in its properties. It may be dried at 100° C. and loses no M'eight at that temperature. I endeavoured to combine the determination of the carbon, hydrogen and mercury of this substance in one combustion, and have perfectly succeeded. The operation was conducted as follows : — The substance was mixed with chromate of lead and introduced into a combustion-tube of at least 26 inches in length. About 6 inches of copper turnings are placed above the mixture, leaving a space of 8 inches from the copper to the anterior end of the tube. A receptacle for the mercury is formed out of the tube itself by contracting it about an inch from the copper turnings, and again so as to leave an elongated bulb of an inch in length. At the close of the ope- ration the tube is cut with a file at the posterior contraction. In order to separate the water from the mercury, the chloride of calcium tube (which has not been detached) is connected with an aspirator and air admitted through chloride of cal- cium, the bulb being kept at a temperature of 100'^ C. I obtained in my analysis the following numbers : — 0'7833 grm. of substance gave 0*5832 grm. of carbonic acid, 0*1639 grm. of water, and 0*3365 grm. of mercury, corresponding to the following per-centage, which I place in comparison with the theoretical numbers : — Theoiy. Expt. 16 eqs. Carbon 96 20*68 20*30 10 ... Hydrogen 10 2*15 2*32 4 ... Nitrogen 56 12*11 4 ... Oxygen 32 6*89 2 ... Chlorine 70 15*08 2 ... Mercury 200 43*09 42*91 464 100*00 Caffein and Terchloride of Gold. This compound is formed when a solution of terchloride of gold is added in excess to cafFein dissolved in dilute hydro- chloric acid. If concentrated solutions are employed, the whole immediately solidifies into a mass of a most splendid lemon-yellow colour; this is to be washed with cold water ♦ Liebig's Annalen, xlvii. 37. 132 Mr. Nicholson on the Composition of Caffein. and crystallized from alcohol, and finally dried in the water- bath. The crystals from on alcoholic solution are in the form of long needles, of an orange-yellow colour and a very bitter metallic taste; they are soluble in alcohol and water. When boiled in water for a short time, the 'salt is decomposed, a yellow flocculent matter precipitating, which is insoluble in alcohol, ether and water, but soluble in hydrochloric acid. If an aqueous solution is kept on the sand-bath for some hours at a temperature of about 68° C. it is also decomposed, and metallic gold separates in shining scales. It is not altered when exposed to light, and when dry may be heated to 100° C. without undergoing decomposition. Analysis. — When burnt with chromate of lead — I. 0*8530 grm. of substance gave 0*5525 grm. of carbonic acid and 0*1622 grm. of water. II. 0*3224 grm. of substance gave 0*1197 grm. of metallic gold. III. 0*301 9 grm. of substance gave 0*1115 grm. of metallic gold, which give the following per-centages : — I. II. III. Carbon . . 17*72 Hydrogen .2*11 Gold . . . 37*12 36*93 corresponding to the formula Cjg Hjo N4O4 HCl Au CI3, as may be seen by the following table, where the calculated and quantities found are placed in comparison : — Theory. Found. 16 eqs. Carbon . 96*00 17*98 17-72 11 ... Hydrogen 11*00 2*06 2*11 4 ... Nitrogen . 56*00 10*50 4 ... Oxygen . 32*00 6*01 4 ... Chlorine . 142*00 26*60 1 ... Gold . . 196*66 36*85 37*02 533*66 100*00 The caffein compounds which I have analysed are there- fore— Caffein Cjg Hjo N4 O4. Platinum compound Cjg Hiq N4 O4, HCl Pt Clg. Silver compound . Cjg Hjq N4 O4, AgO, NO5. Mercury compound Cjg Hjo N4 O4, 2(Hg CI). Gold compound . . Cjg Hjo N4 O4 HCl, Au CI3. There exist several other double compounds of caffein, which I have however not subjected to analysis. Prof. Young oti the Extension o/'Euler's Theorem. 123 On mixing a hot alcoholic solution of caffein with an alco- holic solution of cyanide of mercury, beautiful needles of a double salt are deposited upon cooling, which correspond most likely to the mercury salt I have just described. A so- lution of caffein in hydrochloric acid gives a beautiful brown precipitate with chloride of palladium ; and the filtered solu- tion deposits another compound in the form of yellow scales, very similar in appearance to iodide of lead. CaiFein gives no precipitate with solutions of sulphate of copper, chloride of tin, acetate of lead, and nitrate of suboxide of mercury. When boiled with sesquichloride of iron, a red- dish-brown precipitate subsides upon cooling, which is per- fectly soluble in water, and is most likely a double compound of caffein and sesquichloride of iron. XXIII. Note in reference to the exteiision o/Euler's Theorem, By J. R. Young, Professor of Mathematics in Belfast College. To Richard Taylor^ Esq. Dear Sir, IN the Philosophical Magazine for June last a communica- tion of mine was published respecting an extension of a certain theorem of Euler concerning the products of the sums of squares. At the time that notice was written, I was under the impression that the theorem admitted of an extent of ge- neralization which a further investigation of the matter proves to me has not place. I am now prepared to show that the proposition does not hold beyond the case for eight squares, the formulae for which I have already printed in the Proceed- ings of the Royal Irish Academy ; in the Transactions of which body it is probable that the entire investigation of the theorem for eight squares, and the proof that it does not apply beyond that number, will hereafter appear. It may perhaps be interesting to algebraists to find the real limits to this theorem demonstrably established ; and thus to know — in any attempts that may hereafter be made to extend Sir W. R. Hamilton's remarkable and very fertile theory of quaternions — beyond what boundaries such attempts must prove fruitless. I remain, dear Sir, Very faithfully yours, Belfast, July 16, 1847. J. R. YouNG. [ 124 ] XXIV. On the Precipitate produced in Spring and River Waters by Acetate of Lead, By A. Connell, Esq., Professor of Chemistry in the University of St. Andrews*. ^V^YLYj white precipitate which it is well known is usually JL produced in spring and river waters by acetate of lead, has been commonly attributed to the presence of sulphates, chlorides and carbonates. The comparatively trifling action of silver salts, however, shows that it is very rarely, unless in the case of what are called mineral waters, due to chlorides ; and the ready solubility of the precipitate in acetic acid in whole or in great part, proves that it is not due to sulphates or phosphates, except in so far as it may be insoluble in acetic acid. Carbonates therefore remain as the probable cause ; and this is established by the circumstance, that although effervescence cannot be noticed on the immediate addition of acetic acid, effervescence will be observed if the precipitate is allowed to subside, and the greater part of the solution de- canted, and an acid then added. 1 have found on investiga- tion that carbonate of lime is the usual source of the reaction. The remarkable fact however on this view is, that the reaction is scarcely diminished by boiling and filtering the water; and indeed in some instances does not take place unless these steps are had recourse to, and acetic acid still dissolves the whole or great part. If the waters referred to are boiled and filtered and then largely concentrated by evaporation, they usually deposit carbonate of lime, and do not indicate any such alka- line reaction as shows an alkaline carbonate. The carbonate of lime causing the reaction is therefore evidently held dis- solved in the water independently of the presence of free carbonic acid ; and I do not think that chemists, generally speaking, are aware that common water may still retain enough of carbonate of lime to give, with acetate of lead, a consider- able precipitate of carbonate of lead, although they may have been boiled and filtered. If in any such case the precipitate should be found to dissolve in acetic acid truly mthout effer- vescence, the probable cause would be the presence of a suffi- cient quantity of some organic matter, such as crenic or apo- crenic acid, which precipitates lead salts ; for it is not the least likely that fluorine, which has been found in some spring waters, should ever be present in sufficient quantity to affect lead salts, and fluoride of lead would very likely not be so- luble in acetic acid. The question then arises, whence proceeds this carbonate * Communicated by the Author. On the Precipitate produced in Water by Acetate of Lead. 125 of lime. To know whether it arises from the water redis- solving carbonate of lime, which had been held dissolved by carbonic acid and then precipitated by boiling, I transmitted a current of carbonic acid through lime water tilLit completely redissolved the precipitate which had at first formed. I then boiled the solution for a short time, as in experimenting with the spring waters, and filtered the liquid; but although it was slightly precipitated by acetate of lead, the effect was very much less than that on common water ; showing that we cannot account for the effect on common water by supposing that all the carbonic acid had not been driven off by the ebul- lition. Again, when distilled water was left in contact with marble in impalpable powder for several days, both acetate of lead and oxalate of ammonia showed less lime than in the common waters, although rather more than in the lime-water experiment. I incline therefore to think that the carbonate of lime owes its origin to double decomposition between an alkaline carbonate and a lime salt, such as a chloride. If to a few ounces of distilled water a drop or two of muriate of lime and a drop or two of carbonate of soda be added, the liquid remains quite transparent ; and the reaction of common water with acetate of lead and acetic acid may be exactly imi- tated with this liquid. And in all the common waters yielding the reaction, I could detect alkalies in union with acids. The common water of the town of St. Andrews, I found, after being boiled and filtered, to yield by evaporation -^j^-^-^ of carbonate of lime; and other well and river waters may contain still more. Fresenius has stated that water is capable of holding in solution yy^oT ^^ carbonate of lime, after being saturated with that salt by long-continued boiling, and left in contact for four weeks with the deposit formed on cooling. Nature of course does not take such pains to charge spring waters with lime ; and I think the method I have suggested affords a much more simple and probable means of effecting this end. The St. Andrews' water also contains a trace of carbonate of magnesia after being boiled and filtered ; and it is probable that this substance may sometimes be in part the cause of the reaction referred to, but to a much less extent*. * I have given fuller details on this subject in a paper inserted in the Transactions of the Royal Society of Edinburgh for the present year. [ 126 ] XXV. On the Action of a mixt^ire of Red Prussiate of Potash and Caustic Alkali upon Colouring Matters. By John Mercer, Esq.^ A BOUT ten years since I discovered and used extensively -^^ in calico-printing the oxidizing properties of a mixture of red prussiate of potash and caustic alkali. For many years I have been in the habit of communicating to my friends several applications of this interesting reaction, among whom I may mention Mr. Crura of Glasgow and Dr. Lyon Playfair. Since then Boudault t has directed attention to the oxidizing power of the same mixture, as far as relates to metallic oxides, but has not shown any important practical application of the knowledge thus acquired. There are but few processes known in the arts for bleach- ing indigo, the principal of these being that in which chromic acid liberated from the bichromate of potash by means of an acid is used. In certain cases this process is attended with various disadvantages, and the cloth requires to be subjected to a clearing process to remove the oxide of chromium. The topical application of a mixture of red prussiate of potash and an alkali at once effects the same pm*pose, and in a most com- plete manner, leaving a brilliant white on the spot where the colour is discharged without rendering any injury to the fabric. The manner of applying this discharge may be ar- ranged to suit the conditions of the calico-printer. As a class experiment for a lecture-table it is convenient to impregnate the indigo-blue calico with a solution of prussiate of potash, and then dip it into a weak solution of alkali. This action is a beautiful illustration of those double affi- nities which we frequently find at play in combinations or decompositions. Thus, though neither chlorine nor charcoal can decompose alumina per se, the same gas passed over a mixture of alumina and charcoal combines with the metallic radical ; the charcoal in this case having aided the combina- tion by withdrawing the oxygen. It is the same kind of action in the case under consideration. Red prussiate of potash, Feg Cyg 3K, differs from the yellow prussiate, Fcg Cyg 4K, by containing one atom less potassium. When pot- ash is presented to the former, this deficient atom of potas- sium is supplied, but the affinity is not strong enough to liberate the oxygen. When however a second body having an attraction for oxygen, such as litharge or indigo, is pre- sented to the potash and red prussiate, this second affinity * Communicated by the Chemical Society; having been read Feb. J, 1847. t Journal de Pharmacie. [Phil. Mag., vol. xxvii. p.307.] Dr. W. Gregory on the Preparation ofHippuric Acid. 127 acting in a different direction withdraws the oxygen and allows the potassium to unite with the compound radical fer- rocyanogen ; thus Fe^ Cyg 3K + KO + PbO = Fcg Cyg 4K + Pb02, the decomposition being of the same kind when an organic matter is substituted for the oxide capable of further oxidation. Soda and ammonia may be substituted for potash in the above decomposition, producing the oxidation or dis- charging the indigo. This is curious in the case of ammonia, for it cannot be explained by any other than by the ammo- nium theory, and shows the complete analogy between the oxide of ammonium and the oxide of the simple metallic ra- dicals, potassium and sodium. It is interesting also to ob- serve that the last member in the formula Fe^ Cyg 4R, may be substituted by any alkaline base. Thus, that it may either be Fe^ Cyg 3K K, or Fe^. Cyg 3K Na,or Fe^ Cyg 3K NH4. This circumstance points to important theoretic^ considerations in the atomic constitution of the prussiates, which would be foreign to the present paper, the principal object of which is to furnish a means of discharging indigo, and thus supply a process much wanted in the art of calico-printing, and which I have followed for many years with success. XXVI. On the Preparation of Hippuric Acid. By William Gregory, M.D."^ SINCE the discovery of hippuric acid by Liebig, that body has at all times attracted much attention. Its composition and the products of its decomposition, among which were ben- zoic acid and benzamide, rendered it interesting, and various ingenious views were entertained of its constitution. Its detection in human urine by Liebig gave it additional im- portance. The beautiful discovery of Dessaignes, that hippuric acid, when heated with strong acids, is resolved into benzoic acid and glycocoU, has greatly increased the interest already at- tached to hippuric acid, which now affords the best means of obtaining glycocoll, and has enabled Horsford, in his elabo- rate researches on that substance, to fix its formula in a very satisfactory manner. If to hydrated hippuric acid . Cjg N Hg Og, we add 1 equiv. water ... HO, and from the sum Cjg N H,q O7, subtract 1 equiv. glycocoll . . C4 N H4 O3, there remain C14 Hg O4, which is hydrated benzoic acid. * Communicated by the Chemical Society; having been read March 15, 1847. 128 Dr. W. Gregory on the Preparation of Hippuric Acid. There cannot, I think, be any longer a doubt that C4 N H4 O3 is the true formula of glycocoll, and Hor^ford has, in esta- bUshing this point, at the same time confirmed and explained in the most satisfactory manner the observation of Dessaignes. The researches of Horsford, however, have also demon- strated that glycocoll is in itself one of the most interesting compounds known to chemists, and it is evident that the fur- ther study of this most singular body will lead to very va- luable results. I have already stated that glycocoll is best obtained from hippuric acid, but as soon as I began to prepare for this pur- pose a considerable quantity of hippuric acid, I found, as all who have done so must have found, that the operation as pre- scribed in books is not only tedious and troublesome, but un- certain. The usual process consists in evaporating the urine of the horse or cow at a moderate temperature to about one-eighth of its bulk, and adding hydrochloric acid, when on standing a few hours, crystals of impure hippuric acid are deposited. But it is well-known that if the temperature should rise too high, although still to a point short of boiling, the hippuric acid will partially or totally disappear, and benzoic acid will be found in its place. Now when we bear in mind that the urine contains but little hippuric acid, it is evident that to obtain this acid in quantity we must operate with a very large bulk of urine, and those who have done so well know how tedious the evaporation is, since if we attempt to hasten it by raising the temperature, we run the risk of losing the whole ; and this indeed frequently happens. The impure, highly-coloured acid first obtained has been purified by different chemists in a great variety of ways. Some have used chloride of lime ; but this method is not easily managed, and often converts the whole into benzoic acid. The last and by far the best method of purification is that of Schwarz, who boils the impure acid with an excess of milk of lime, and strains the alkaline liquid from the undissolved lime. It passes rapidly and clear through calico, and the lime retains the colouring matter, so that the addition of acid to the filtered liquid causes the deposition of crystals of hippuric acid nearly white. Schwarz recommends the addition of chloride of calcium to the filtered or unfiltered liquid, and the precipitation of the lime as carbonate by carbonate of potash or soda, when the precipitated carbonate of lime carries with it the last traces of colouring matter. I have not found this necessary, as a repetition of the process with the milk of lime never fails to yield colourless crystals. Dr. W. Gregory on the Preparation of Hippuric Acid. 129 As it was clear that the hippuric acid was not in the slight- est degree decomposed by boiling with excess of lime, al- though so easily metamorphosed by acids, I thought that by applying the same principle to the urine directly, I might be enabled to boil it down, and thus shorten the process, and at the same time prevent the decomposition of the hippuric acid, since it would appear that hippurate of lime is not affected by boiling, nor by excess of lime. Accordingly, I took some urine of the horse, mixed it with excess of milk of lime and boiled for a few minutes. I then strained the solution, which was very materially decolorized, and boiled the clear liquid as rapidly as possible down to the requisite bulk. On adding hydrochloric acid I obtained a copious deposit of crystals, which when pressed had a slight red colour. I then treated them by Schwarz's method and obtained an abundant crop of almost colourless crystals, which consisted entirely of the needles of hippuric acid, with- out a visible trace of benzoic acid, the crystallization of which is easily recognized. A second treatment with milk of lime, which was hardly needed, and probably would have been quite unnecessary had a greater excess of lime been used in the previous one, yielded snow-white crystals of the utmost beauty and purity. The improvement which I have thus introduced in the preparation of hippuric acid may seem trifling, and is indeed only the application of Schwarz's method to the urine, in- stead of to the crude acid ; but any one who tries to prepare some ounces, not to say pounds, of hippuric acid, will soon find that the difference is practically important. By my me- thod it is possible to extract in one day the hippuric acid from as much urine as would require a week to operate upon on the usual plan, so that the quantity of hippuric acid which we can thus obtain is only limited, as it were, by the quan- tity of urine to be procured. The tedious evaporation at low temperatures is got rid of, and we are sure of obtaining the whole hippuric acid originally present ; whereas, on the for- mer plan, however carefully the evaporation is conducted, and it requires constant superintendence, it almost ahvays happens that some of the hippuric acid is decomposed ; while a very slight accidental rise of temperature may destroy the whole of it, as I have often seen. On the whole, I am satisfied that all who wish to study hippuric acid and glycocoll will find on trial that what was formerly a disagreeable and troublesome operation is now a very easy and short one ; and that they may now easily ob- tain these remarkable compounds in any desired quantity. Phil. Mas. S, 3. Vol. 3 1 . No. 206. Aus. 1847. K [ 130 ] XXVII. Proceedings of Learned Societies. CAMBRIDGE PHILOSOPHICAL SOCIETY. [Continued from vol. xxx. p. 367.] Nov. 9.#^N the Structure of the Syllogism, and on the application 1846. ^-^ of the Theory of Probabilities to Questions of Argument and Authority*. By Professor De Morgan. The object of this paj^er is twofold : first, to establish two distinct theories of the syllogism, both differing materially from that of Ari- stotle, and each furnishing a general canon for the detection of all its legitimate forms of inference ; secondly, to investigate the mode in which the distinctive character of the two great sources of convic- tion, argument and authority, affects the application of the notion of probability to questions not admitting of absolute demonstration. The two theories of the syllogism arise out of simple notions con- nected with the /onns of propositions and their quantities. The dif- ference between a positive and negative assertion is not essential, but depends on the manner in which objects of thought are described by language. If Y and y be names so connected that each contains everything which is not in the other, and the two have nothing in common (a relation which is described by calling them contrary * Upon this paper a controversy has arisen, which, up to the present time, may be summed up as follows : — ^piilSO. Mr. De Morgan published a statement in answer to an assertion ot SirW. Hamilton of Edinburgh, to the effect that the second, or quantitative, system of syllogism, was a wilful plagiarism from certain letters which Sir W. Hamilton had written to Mr. De Morgan. Maj/ 22. Sir W. Hamilton replied at length in another pamphlet, retracting the assertion o^ wilful plagiarism, but maintaining that the system was taken, unconsciously, from those letters. This was followed by a letter from Mr. De Morgan in the Athenaeum of May 29, and another from Sir W. Hamilton in the same publication for June 5. The point at issue now seems to be as follows : — Mr. De Morgan challenges Sir W. Ha- milton to show anything in his second system which was not substantially contained in a digressive section of the description of his first system, ad- mitted to have been sent to Cambridge before any communication had taken place. SirW. Hamilton, in reply, contends that the digression above- mentioned contains nothing to the purpose. Mr. De Morgan defers further reply until he publishes a work which he states himself to be preparing on logic. In the Athenaeum of June 19, appeared a letter from Mr. James Broun, asserting certain mistakes on the part both of Sir W. Hamilton and Mr. De Morgan, and giving certain extensions to the quantitative forms of the latter. Again, June 26, appeared in the same publication a letter from Mr. De Morgan, dated June 19, stating that he also had arrived at Mr. Broun's forms, giving reasons for their rejection in favour of certain simpler forms, giving the heads of an extended system of quantitative syllogism, and asserting that he had materially extended both his systems. So the matter stands. The subject of the structure of the syllogism seems to be likely to excite some attention ; and, without pronouncing any opinion on the personal claims or conflicts of the several parties, we recommend the attention of our readers to this rather neglected branch of pure science. — Ed. Phil. Mag. Cambridge Philosophical Society. 131 names), the propositions ' Every X is Y ' and ' no X is y ' are sim- ply identical. In the same manner, the particular and universal proposition are only accidentally distinct. If in ' some Xs are Ys ' the Xs there specified had had a name belonging to them only, say Z, then the preceding proposition would have been identical in mean- ing with * every Z is Y,' From the above it is made to follow, that every legitimate syllo- gism can be reduced to one of universal affirmative premises, either by introduction of contrary terms, or invention of subgeneric names. In considering the nature of the simple proposition, Mr. De Mor- gan uses a notation proposed by himself. Thus — Every X is Y is denoted by X)Y A NoXisY . . . . X.Y E Some Xs are Ys . . . XY I Some Xs are not Ys . . X:Y O and names which are contraries are denoted by large and small let- ters. Aristotle having excluded the contrary of a name from formal logic, and having thereby reduced the forms of proposition to four, these forms (universal affirmative, universal negative, particular affir- mative, particular negative) the writers on logic in the middle ages represented by the letters A, E, I, O. Thus X)Y and Y)X are equally represented by A. When contraries are expressly intro- duced, all the forms of assertion or denial which can obtain between two-terras and their contraries, are eight in number ; and the most convenient mode of representing them is as follows : — Let the letters A, E, I, O have the above meaning, but only when .the order of sub- ject and predicate is XY. Then let a, e, i, o stand for the same propositions, after x and y, the contraries, are written for X and Y. The complete system then is — A=X)Y a=x)y~Y)X 0=X:Y o=a^:y=Y:X E:=X.Y e-=-x.y I=XY i-=-xy and every form in which subject and predicate are in any manner chosen out of the four X, Y, x, y, so that one shall be either X or x, and the other either Y or y, is reducible to one or other of the pre- ceding. The propositions e and i, which are thus newly introduced, are only expressible as follows, with reference to X and Y. (t.) There are things which are neither X nor Y. (e.) There is nothing but is either X. or Y or both. The connexion of these eight forms is fully considered, and the various syllogisms to which they lead. Rejecting every form of syl- logism in which as strong a conclusion can be deduced from a weaker premise ; rejecting, for instance, Y)X+Y)Z=XZ because XZ equally follows from Y)X4-YZ, in which YZ is weaker than Y)Z — all the forms of inference are reduced to three sets. 1 . A set of two, called single because the interchange of the terms K2 132 Cambridge Philosophical Society. of the conclusion does not alter the syllogism. Neither of these forms are in the Aristotelian list. One of them is X)Y+Z)Y-xz; or if every X be aY, and also every Z, then there are things which are neither X nor Z ; namely, all which are not Ys. 2. A set of six, in which the interchange produces really different syllogisms of the same form, and in which both premises and con- clusion can be expressed in terms of three names, without the con- trary of either. This set includes the whole Aristotelian list, except those in which a weaker premise will give as strong a conclusion, or the one in which the same premises will give a stronger conclusion. 3. A set of six resembling the last in everything but this, that no one of them is expressible without the new forms e and i ; that is, requiring three names and the contraries of one or more of them. Those of the third set are not reducible to Aristotelian syllogisms, as long as the eight standard forms of assertion are adhered to. The second theory of the syllogism has its principles laid down in the memoir before us ; but those principles are only applied to the evolution of the cases which are not admitted into the Aristotelian system. The formal statement of the manner in which the ordinary cases of syllogism are connected with those peculiar to this second system is contained in an Addition. In providing that premises shall certainly furnish a conclusion, the common system requires that one at least of the premises shall speak universally of the middle term ; that is, shall make its asser- tion or denial of every object of thought which is named by the middle term. Mr. De Morgan points out that this is not necessary : m being the fraction of all the cases of the middle term mentioned in one premise, and n in the other, all that is necessary is that m + n should be greater than unity. In such case, the real middle term, being the collection of all the cases by comparison of which with other things inference arises, is the fraction m + w — 1 of all the possible cases of the middle term. Thus, from the premises ' most Ys are Xs ' and ' most Ys are Zs,' it can be inferred that some Xs are Zs, since m and n are both greater than one-half. The assignment of definite quantity to the middle term in both premises, gives a canon of inference, of which the Aristotelian rule is only a particular case. In the addition above alluded to, this same canon, namely ' that more Ys in number than there exist separate Ys shall be spoken of in both premises together,' is made to take the following form : — If in an affii'raation or negation, in ' As are Bs ' and ' As are not Bs,' definite numerical quantity be given to both subject and predicate, if it be stated how many As are spoken of and how many Bs — the number of effective cases of the middle term is seen to be the nnici- her oi subjects in an affirmative proposition, whether the middle term be subject or predicate. Hence, defining the effective number of a premise to be the number of subjects if the proposition be affirmative, and the number of cases of the middle term if it be negative, all that is necessary for inference (over and above the usual condition Cambridge Philosophical Society. 133 that both premises must not be negative) is that the sum of the effective numbers of the tvro premises shall exceed tlie number of existing cases of the middle term ; and the excess (being the fraction denoted by m + « — 1 in the Memoir) gives the number of cases in which inference can be made. To attempt to combine these two systep^ oiform and of quantity is rendered useless by language not possessing the forms of mixed assertion and denial, which the syllogisms deduced from the combi- nation would require. As far as the combination can, in Mr. De Morgan's opinion, be made, nothing is required but a distinct con- ception of, and nomenclature for, the usual modes of expressing a logical form, and implying one or the other of the alternations which the mere expression leaves unsettled. Mr. De Morgan proposes the following language. Two names are identical when each contains all that the other contains : but when all the first (and more) is contained in the second, then the first is called a subidentical of the second, and the second a superidentical of the first. Two names are contrary when every- thing (or everything intended to be spoken of) is in one or the other and nothing in both. But when the two names have nothing in common, and do not between them contain everything, they are called subcontraries of one another. And again, if everything be in one or the other, and some things in both, they are called supercon- trari.es of one another. Lastly, if the two names have each some- thing in common and something not in common, and moreover do not between them contain everything, each is called a complete par- ticular of the other. A table is then given, which contains every form of complex syllogism. If X and Z be the terms of the conclusion, and both be described in terms of Y, the middle term : it can be seen from this table what can be affirmed and what denied, of X with respect to Z. For in- stance, if X be supercontrary of Y, and Z subcontrary, then X must be a superidentical of Z : but if X and Z be both subidenticals of Y, nothing can be affirmed ; only it may be denied that X is either contrary or suj^ercoiitrary of Z. The remaining part of this paper relates to the application of the theory of probabilities above-mentioned. Mr. De Morgan asserts that no conclusion of a definite amount of probability can be formed from argument alone ; but that all the results of argument must be modified by the testimony to the conclusion which exists in the mind, whether derived from the authority of others, or from the previous state of the mind itself. The foundation of this assertion is the circumstance that the insufficiency of the argument is no index of the falsehood of the conclusion. Various cases are examined; but it must here be sufficient to cite one or two results. If n be the probability which the mind attaches to a certain con- clusion, a the probability that a certain argument is valid, and b the probability that a certain argument for the contradiction is valid : then the probability of the truth of the conclusion is (1-% (l-%-f-(l-a)(l-j«)- 134 Cambridge Philosophical Society. If J=0, or if there be no argument against, and if the mind be unbiassed, or if u= — , this becomes t* 2' or « + ^^ —. 2— fl 2— a For this writers on lo^c generally substitute a, confounding the absolute truth of the conclusion with the validity of the argument, and neglecting the possible case of the argument being invalid, and yet the conclusion true. Nov. 23. — On a New Notation for expressing various Conditions and Equations in Geometry, Mechanics and Astronomy. By the Rev. M. O'Brien. If A, P, P' be any three points in space, whether in the same straight line or not, and if the lines AP and AP' be represented in magnitude and direction by the symbols u and u' , then,, according to principles now well-known and universally admitted, the line PP' is represented in magnitude and direction by the symbol u' —u. Now if AP and AP' be equal in magnitude, and make an indefinitely small angle with each other, PP' is an indefinitely small line at right angles to AP, and u' —u becomes du. Hence it follows, that, if u be the symbol of a line of invariable magnitude, du is the symbol of an in- definitely small line at right angles to it ; and therefore, if X be any arbitrary coefficient, \du is the general expression for a right line perpendicular to u. The sign \d therefore indicates perpendicularity, when put before the symbol of a line of invariable length. The object of the author is to develope this idea, and to show that it not only leads to a simple method of expressing perpendicularity, but also furnishes a notation of considerable use in expressing various conditions and equations in geometry, mechanics, astronomy, and other sciences involving the consideration of direction and magnitude. The author first reduces the sign \d to a more convenient form, which not only secures the condition that u is invariable in length, but also defines the magnitude and direction of the perpendicular which Kdu denotes. This he does in the following manner. He assumes u=^xa,-\-y^ + zy, (where a- ^ y reipresent three lines, each a unit in length, drawn at right angles to each other, and if y z are any arbitrary numerical coefficients,) and supposes that the differentiation denoted by d affects a j3 y, but not x y z. This secures the condition that u is invariable in length, and leads to the following expression for Kdu, viz, Xdu={zy' —z'y)(x, + (oaz' —x'z)^ + (yx' —y'a;)y, x' y' z' being arbitrary coefficients. Assuming u'=x'a,+y'fi + z'y, it appears from this expression for Xdu, that du=0 when u=u', and therefore that c? denotes a differen- tial taken on the supposition that u' is constant. On this account the author substitutes the symbol Du' in place of Ac? ; he then shows that the operation D^/ is distributive with respect to u' (i. e. that Dm'+m"s=D„/4-Dm")> and to indicate this he elevates Cambridge Philosophical Society, 186 the subacript index m', and writes Dm'.m instead of Dm/m, Thus he obtains the expression Du' .u=i{zy'~z'y)a,-\-ixz' —x'z)^-\-iyx' —y'x)y. From this it follows that Dm'.m is a line perpendicular both to u' and u, and that the numerical magnitude of Dm'.m is rr' sin ^, where r and r' are the numerical magnitudes of u and m', and fl the angle made by u and u' . Having investigated the principal properties of the operation Dm'., the author, by a similar method, obtains another notation, Au'.u, which represents the expression xx' -{-yi/'+zz', or rr' cos Q. He then gives some instances of the application of these two notations to mechanics, which may be briefly stated as follows : — 1st. If U, U', U", &c. be the symbols* of any forces acting upon a rigid body, and m, m', m", &c. the symbolsf of their respective points of application, then the six equations of equilibrium are included in the two equations 2U=0 and I:Dm.U=0. 2nd. That these two equations are the necessary and sufficient conditions of equilibrium, may be proved very simply from first prin- ciples by the use of the notation Dm. 3rd. The theory of couples is included in the equation 2Dm.U=0. In fact the symbol Dm.U expresses, in magnitude and direction, the axis of the couple by which the force U is transferred from its point of application U to the origin. 4th. Supposing that the forces U, U', TJ", &c. do not balance each other, and putting 2U=V, 2;Dm.U=W, we may show immediately, by the use of the notation Am, that the condition of there being a single resultant is AV.W = 0; and when there is not a single resultant, the axis of the couple of minimum moment is AV.W y AV.V. ■ * 5th. The three equations of motion of a rigid body about its centre of gravity are included in the equation -('2Du. — Sm\='LDu.VSm; (1.) dt\ dt J u being the symbol of the position of any particle hm of the body, and U the symbol of the accelerating force acting on Jm. 6th. If u) be assumed to represent the expression cWia + cwojS + Wjy, where Wy, w.^, Wj are the angular velocities of the planes of yz, zx, xy about the axes of x, y, z respectively, then the symbol of the * By the symbol of a force is meant the expression X«+Y/3+Zy, where X Y Z are the three components of the force. t By the symbol of a point is meant the expression jf«-t-^/3+2y> where X y z are the coordinates of the point. 1 36 Cambridge Philosophical Society. velocity of ^m is Dcu.w ; from which follow immediately the three well-known equations, dx dy dz _ The symbol w represents in direction the axis of instantaneous rotation, and in magnitude the angular velocity about that axis. 7th. The equation (1.) maybe reduced to the form -^ { A w la + BwzjS + C Way } = SDm .U Jot, which includes Euler's three equations of motion about a fixed point. 8th. If the forces U, U', U", &c. arise from the attraction of a distant body, the symbol of whose position is u' , this equation may be further reduced to the form ^ / Aw.a+BwajS-i- Cwgy") = ^' DM'.(Aa?'a+By/3 + CzV)- 9th. In the case of the earth attracted by the sun or moon, this equation becomes y being the polar axis, and A= . 10th. The mean daily motion of y is given by the equation 5 = ^X(A«'.7)(D«'.y); dt nr^ which equation gives immediately all the well-known expressions for solar and lunar precession and nutation, for -5- is the symbol of the velocity of the north pole, representing that velocity both in magnitude and direction. Supplement to a Memoir on some cases of Fluid Motion. By G. G. Stokes, M.A., Fellow of Pembroke College, Cambridge. In a former paper the author had given the mathematical calcula- tion of an instance of fluid motion, which seemed to offer an accurate means of comparing theory and observation in a class of motions, in which, so far as the author is aware, they had not been hitherto com- pared. The instance referred to is that in which a vessel or box of the form of a rectangular parallelepiped is filled with fluid, closed, and made to perform small oscillations. It appears from theory that the effect of the inertia of the fluid is the same as that of a solid having the same mass, centre of gravity and principal axes, as the solidified fluid, but different principal moments of inertia. In this supplement the author gave a series for the calculation of the prin- cipal moments, which is more rapidly convergent than one which he had previously given. It is remarkable that these series, though numerically equal, appear under very diflferent forms, the wthterm of Cambridge Philosophical Society. 137 the latter containing exponentials of the forms e"** and e " , while the «th term of the former contains exponentials of the second form only. In conclusion, the author referred to some experiments which he had performed with a box, such as that described, filled with water, employing the method of bifilar oscillations. The moment of inertia of the fluid about an axis passing through its centre of gra- vity (?'. e. the moment of inertia of the imaginary solid which may be substituted for the fluid), was a little greater as determined by experiment than as determined by theory, as might have been ex- pected, since the friction of the fluid was not considered in the cal- culation. The diff"erence between theory and experiment varied in difi^erent cases from the Jgth to the -J^st part of the whole quantity. Dec. 7. — On the Principle of Continuity in reference to certain results of Analysis. By Professor Young of Belfast College. The object of this paper is to inquire into the influence of the law of continuity, as it affects the extreme or ultimate values of variable functions, more especially those involving infinite series and definite integrals. The author considers that this influence has hitherto been impro- perly overlooked ; and that to this circumstance is to be attributed the errors and perplexities with which the different theories of those functions are found to be embarrassed. He shows that every parti- cular case of a general analytical form — even the ultimate or limiting case — must come under the control of the law implied in that form ; this law being equally efficient throughout the entire range of indi- vidual values. Except in the limiting cases, the law in question is palpably impressed on the several particular forms ; but at the limits it has been suffered to escape recognition, because indications of its presence have not been actually preserved in the notation. It is in this way that the series 1 — 1 + 1 — 1-|- &c. has been con- founded with the limits of the series \—x-\-x°—x^+ &c. ; these limits being arrived at by the continuous variation of x from some inferior value up to x=\, and from some superior value down to x=si\. It is shown however that the series 1 — 1 + &c. has no equi- valent among the individual cases of 1— a? + a?^— &c., with which latter, indeed, it has no connexion whatever. By properly distinguishing between the real limits, and what is generally confounded with them, the author arrives at several con- clusions respecting the limiting values of infinite series directly op- posed to those of Cauchy, Poisson, and others. And to prevent a recurrence of errors arising from a neglect of the distinction here noticed, he proposes to call such an isolated series as 1 — I + 1 — &c. independent or neutral; and the extreme cases of l—x+x''^ — &c., dependent series : the difference between a dependent and a neutral series becomes sufficiently marked, as respects notation, by introdu- cing into the former what the author calls the symbol of continuity, which indeed is no other than the factor, whose ascending powers Poisson introduces — and, as here shown, unwarrantably — into the successive terms of strictly neutral series ; thus bringing such series 138 Cambridge Philosophical Society, under the control of a law to which in reality they owe no obedi- ence. An error somewhat analogous to this is shown to be committed in the treatment of certain definite integrals, which are here submit- ted to examination and correction, and some disputed and hitherto unsettled points in their theory fully considered. The author is thus led to what he considers an interesting fact in analysis ; viz. that the differentials of certain forms require indeterminate corrections, in a manner similar to that by which determinate corrections are intro- duced into integrals ; and he attributes to the neglect of these the many erroneous summations assigned to certain trigonometrical series. This is illustrated by a reference to the processes of Poisson. The paper concludes with some observations on what has been called discontinuity ; a term which the author thinks is sometimes injudiciously employed in analysis, and prefers to treat discontinuous functions as implying distinct continuities ; and by considering these in accordance with the principles established in the former part of the paper, he arrives at results for definite integrals of the form /+» x~P dx totally diflferent from those obtained by Poiseon. Two ■m notes are appended to the paper ; one explaining what the author denominates insensible convergency and insensible divergency, and the other discussing some conclusions of Abel in reference to certain trigonometrical developments. March 1, 1847. — On the' Theory of Oscillatory Waves. By G. G. Stokes, M.A., Fellow of Pembroke College. The waves which form the subject of this paper are characterized by the property of being propagated with a constant velocity, and without degradation, or change of form of any kind. The principal object of the jiaper is to investigate the form of these waves, and their velocity of propagation, to a second approximation ; the height of the waves being supposed small, but finite. It is shown that the elevated and depressed portions of the fluid are not similar, as is the case to a first approximation ; but the hollows are broad and shallow, the elevations comparatively narrow and high. The velocity of pro- pagation is the same as to a first ajiproximation, and is therefore independent of the height of the waves. It is remarkable that the for- ward motion of the particles near the surface is not exactly compen- sated by their backward motion, as is the case to a first approxima- tion ; so that the fluid near the surface, in addition to its motion of oscillation, is flowing with a small velocity in the direction in which the waves are propagated ; and this velocity admits of expression in terms of the length and height of the waves. The knowledge of this circumstance may be of some use in leading to a more correct estimate of the allowance to be made for leeway in the case of a ship at sea. The author has proceeded to a third approximation in the case in which the depth of the fluid is very great, and finds that the velocity of propagation is increased by a small quantity, which bears to the whole a ratio depending on the square of the ratio of the height of the waves to their length. Cambridge Philosophical Society, 139 In the concluding part of the paper is given the velocity of pro- pagation of a series of waves propagated along the common surface of two fluids, of which the xipper is bounded by a horizontal rigid plane. There is also given the velocity of propagation of the above series, as well as that of the series propagated along the ujjper sur- face of the upper fluid, in the case in which the upper surface is free. In these investigations the squares of small quantities are omitted. March 15. — Contributions towards a System of Symbolical Geo- metry and Mechanics. By the Rev. M. O'Brien. The distinction which has been made by an eminent authority in mathematics between arithmetical and symbolical algebra, may be extended to most of the sciences which call in the aid of algebra. Thus we may distinguish between symbolical geometry and arithmC' tical geometry, symbolical mechanics and arithmetical mechanics. This distinction does not imply that in one division numbers only are used, and in the other symbols, for symbols are equally used in both ; but it relates to the degree of generality of the symbolization. In the arithmetical science, the symbols have a purely numerical signi- fication ; but in the symbolical they represent, not only abstract quantity, but also all the circumstances which, as it is expressed, aj^ect quantity. The arithmetical science is in fact the first step of generalization, the symbolical is the complete generalization. In this view of the case, the author has entitled his paper Contri- butions towards a System of Symbolical Geometry and Mechanics. The proposed geometrical system consists, first, in representing curves and surfaces, not by equations, as in the Cartesian method, but by single symbols ; and secondly, in using the differential notation proposed in a former paper* to denote perpendicularity, and to ex- press various equations and conditions. The proposed mechanical system is analogous in many respects. Examples of it have already been given in the paper just quoted. The author uses the term direction unit to denote a line of a unity of length drawn in any particular direction ; and he employs the symbols a j3 y to denote any three direction units at right angles to each other. He defines the position of any point P in space by the symbol re- presenting the line OP (O being the origin) in magnitude and direc- tion. U X y zhe the numerical values of the coordinates of P, and a ^ 7 the direction units of the coordinate axes, the expression xoc+y^ + zy represents the line OP in magnitude and direction, and therefore defines the position of P. This expression he calls the symbol of the point P. If r be the numerical magnitude, and e the direction unit of OP, we have rs—xa.+yfi+zy: re is therefore another form for the symbol of the point P. * Read Nov. 23, 1846. 140 Cambridge Philosophical Society, The following is the method by which the author represents curves and surfaces. If the symbol of a point involves an arbitrary quantity, or, as it is called, a variable parameter, the position of the point becomes inde- terminate, but so far restricted that it will be always found on some line or curve. Hence the symbol of a point becomes the symbol of a line or curve when it involves a variable parameter. In like manner, when the symbol of a point involves two variable parameters, it becomes the symbol of a surface. The parameters here spoken of are supposed to be numerical quantities. An arbitrary direction unit is clearly equivalent to two such parameters ; and therefore, when the symbol of a point involves an arbitrary direction unit, it becomes the symbol of a surface. The following are examples of this method : — 1 . If M be the symbol of any particular point of a right line whose direction unit is e, then the symbol of that right line is M + rg, r being arbitrary. 2. If M be the symbol of the centre of a sphere, and r its radius, the symbol of the surface of a sphere is e being an arbitrary direction unit. 3. If M be the symbol of any particular point of a plane, e and s' the direction units of any two lines in the plane, the symbol of the plane is M + rg+r'g', r and r' heing arbitrary. 4. If £ be the direction unit and r the numerical magnitude of the perpendicular from the origin on a plane, the symbol of the plane is re + Dv-e. V being an arbitrary line symbol, i. e. denoting in magnitude and direction any arbitrary line. 5. If M and u' be the symbols of two points, the symbol of the right line drawn through them is u + m(u' — m), m being arbitrary. 6. If M be the symbol of any curve in space, the symbol of the tangent at the point u is u -\- mdu, m being arbitrary. 7. The symbol of the osculating plane at the point u is u+mdu + m'd"u, m and m' being arbitrary. 8. If s denotes the length of the arc of the curve, and e the direc- tion unit of the tangent, then du Cambridge Philosophical Society, 141 9. _ or — d{ — \ represents a line equal to the reciprocal of the ds ds \ dsj radius of curvature drawn from the point u towards the centre of curvature, i. e. it represents what may be called the index of curva- ture in magnitude and direction. " Hence, since « = xa + y/3 + zy, the numerical magnitude o^ y ^ ( ;r- ) which is the general expression for the reciprocal of the radius of curvature. 10. The symbol of the normal which lies in the osculating plane is u+md /du\ [Ts)' m being arbitrary. 1 1 . The symbol of any normal at the point u, i. e. the symbol of the normal plane, is M + Dy.rfw, V being an arbitrary line symbol. 12. The symbol of the normal perpendicular to the osculating plane is u-\-rnDd"~u.du, m being arbitrary. 13. If M be the symbol of a surface, involving therefore two vari- able parameters, A and /* suppose, then the symbol of the normal at the point u is TV du du u + mD -— . — -, d\ dji m being arbitrary. 14. The symbol of the tangent plane at the point u is J , du , du u+mdu, or u-\-m 1- n — , d\ d^h m and n being arbitrary. 15. The symbol of the plane which contains the three points u tt' u" is u + m{u'—u) + n{u"—u). 16. If M be the symbol of a right line, the symbol of the plane containing it and the point u' is u+m(u'—u). The following are examples of the proposed mechanical system in addition to those given in the paper already quoted. 1 . If r be the radius vector of a planet, and a /3 y be chosen so that a is the direction unit of the radius vector, and y perpendicular to the plane of the orbit, it may be shown immediately by the sym- 142 Cambridge Philosophical Society. bolical method, that the symbol of the force acting on the planet is \dt° / r dt where la is the angular "velocity of the planet, and to' that of the plane of the orbit about the radius vector. The expressions for the three component forces along r, perpendicular to r, and perpendicular to the plane of the orbit, are the coefficients of a /3 7 in this expres- sion. 2. The equation of motion of the planet, when the force is the attraction of a fixed centre varying as the inverse square of the di- stance, is d'^u _ jua It is curious that this equation is immediately integrable, the in- tegral being the two equations r h The latter equation is the symbolical equation of a conic section, the origin being focus, h c and s being the arbitrary constants intro- duced by integration. 3. The application of this method to the case of a planet acted on by a disturbing force is worthy of particular notice, as it expresses the variations of the elements of the orbit with great facility, in the following manner : — If U be the symbol of the disturbing force, we have ^M:=VU,\J (1.) dt ^)=if!:/3Aj8.U + U. ..... (2.) dt h^^ ^ These two equations determine with great facility all the elements of the orbit. For y is a direction unit perpendicular to the plane of the orbit {i. e. it is the symbol of the pole of the orbit), and there- fore it defines completely the position 01 the plane of the orbit. Also 8 is a direction unit in the plane of the orbit at right angles to the axis major, and therefore it determines the position of the axis major ; in fact the direction unit of the axis major is Dy.g. The letters h and e have their usual signification. To find h and y separately from (1.), suppose that we obtain by integration of (1.) then A2=:AW.W ; and h being thus found, we have y= — . The same observation applies to (2.). Royal Astronomical Society. H3 4. The expression for the parallax of the planet is These instances suffice to show the nature of the proposed sym- bolical method. ROYAL ASTRONOMICAL SOCIETY. [Continued from vol. xxx. p. 211.] April 9, 1847. — On an important error in Bouvard's Tables of Saturn. By Mr. Adams. Having lately entered upon a comparison of the theory of Saturn witli the Greenvirjch observations, I was immediately struck with the magnitude of the tabular errors in heliocentric latitude, and the more so, since the whole perturbation in latitude is so small, that it could not be imagined that these errors arose from any imperfection in the theory. In order to examine the nature of the errors, I treated them by the method of curves, taking the times of observation as abscissae, and the corresponding tabular errors as ordinates. After elimina- ting, by a graphical process, the effects of a change in the node and inclination, a well-defined inequality became apparent, the period of which M^as nearly twice that of Saturn. One of the principal terms of the perturbation in latitude (viz. that depending on the mean lon- gitude of Jupiter minus twice that of Saturn) having nearly the same period, I was next led to examine whether this term had been cor- rectly tabulated by Bouvard. The formula in the introduction ap- peared to be accurate; but on inspecting the Table XLIL, which professes to be constructed by means of this formula, I was surprised to find that there was not the smallest correspondence between the numbers given by the formula and those contained in the table, the latter following the simple progression of sines, while the formula contained two terms. The origin of this mistake is rather curious. Bouvard's formula for the terms in question is 9"-67sin{(p-2^'-60°-29}-f.28"-19sin{2^-4^'-h66°-12}; but in tabulating the last term he appears to have taken the simple argument ^ — 2^' instead of 2f — 4ip', so that the two parts may be united into a single term, 25"-85 8in{^-2^' + 43°-88}. which I find very closely to represent Bouvard's Table XLII. After correcting the above error, and making a proper alteration in the inclinations and place of the node, the remaining errors of latitude are in general very small. I subjoin a correct table to be used instead of Bouvard's. The constant added being 36"'0 instead of 26"'0, it will be necessary to subtract 10''"0 from the final result. 144 Royal Astronomical Society. Table XLII. — Argument III. de la Longitude. Argiunent. Equation. Aliment. Equation. Argument. Equation. Argument. Equation. 0 5^-4 2500 17-4 5000 68-1 7500 u 100 54-4 2600 16-2 5100 69-4 7600 40 200 56-0 2700 15-5 5200 70-2 7700 2-3 300 57-2 2800 15-2 5300 70-5 7800 11 400 580 2900 15-2 5400 70-4 7900 0-4 500 58-3 3000 15-7 5500 69-8 8000 01 600 58-3 3100 16-6 5600 68-7 8100 0-4 700 57-8 3200 17-9 5700 67-2 8200 1-0 800 56-9 3300 19-6 5800 65-3 8300 2-2 900 55-7 3400 21-7 5900 62-9 8400 3-7 1000 541 3500 241 6000 601 8500 5-7 1100 52-2 3600 26-7 6100 57-1 8600 8-0 1200 500 3700 29-7 6200 53-7 8790 10-7 1300 47-5 3800 32-8 6300 50-0 8800 13-7 1400 44-9 3900 36-2 6400 46-2 8900 16-8 1500 421 4000 39-6 6500 421 9000 202 1600 39-2 4100 431 6600 38-0 9100 23-7 1700 36-2 4200 46-5 6700 33-9 9200 27-3 1800 33-3 4300 500 6800 29-8 9309 310 1900 30-4 4400 53-3 6900 25-7 9400 34-5 2000 •21-7 4500 56-5 7000 21-8 9500 380 2100 25-1 4600 59-4 7100 181 9600 41-4 2200 22-8 1 4700 621 7200 14-6 9700 44-6 2300 20-6 4800 64-5 7300 11-4 9800 47-5 2400 18-8 1 4900 66-5 7400 8-5 9900 50-1 2500 17-4 5000 681 7500 61 1000 52-4 Constante ajoutee 36"'0. On the Development of the Disturbing Function R. By Sir John Lubbock. The greatest practical difficulty which is encountered in the pla- netary theory consists in the development of the expression for the reciprocal of the linear distance between the disturbed and disturbing planets. The algebraical expression of this development may be obtained either by means of the binomial theorem or by Taylor's theorem applied to several variables ; by the latter method M. Binet has carried the development as far as terms of the 7th order. But when high powers of the eccentricities and inclinations are retained, the expressions become excessively complicated, so that further pro- gress in this direction appears utterly hopeless. The numerical coefficients of the series may also be obtained by quadratures ; but to determine all the coefficients in this way would involve very great labour. In considering the problem of the perturbations of bodies whose eccentricities and inclinations are considerable, the author has been led to another mode of development, which he conceives to possess great advantages over those just mentioned, and the use of which may be greatly facilitated in all cases by special tables, which may be prepared beforehand. Royal Astronomical Society. 145 The principle of this method consists in expressing the square of the ratio of the distance between the two planets to the radius vector of the more distant planet, under the form of P— Q, in which P is the product of any convenient number of factors of the form 1 + A cos a, and all the terms in Q have small coefficients. Then (P— Q)""'' may be developed by the binomial theorem in a series of ascending powers of Q, which consequently converges rapidly, and the values of the quantities P"*^, P""*, &c., which enter into the successive terms of this series, may be found by multiplying together the developments 1 3 of the several factors (1 + A cos a) ^, (1 + A cos a) ^, &c. If then tables were prepared, giving for different values of A the coefficients of the development of these quantities in cosines of multiples of a, all the operations requisite for the development of the disturbing function might be performed with great facility. The author remarks, in conclusion, that instead of developing, as is usually done, in powers of the ratio of the mean distances ( — )' it would be preferable to develope according to powers oi ,-^ which is much less than the former when a and a' do not widely from each other. Observations of Hind's Second Comet in full Sunshine*. By Mr. Hind. I take the liberty to send you two positions of the comet discovered here Feb. 6, obtained yesterday in full daylight, and about five hours before the perihelion passage. The visibility of a comet in the day- time, and within 2° distance from the sun, is a phBenomenon of so rare occurrence, that it may in some measure interest you if I give very briefly the particulars of our observations. I had determined, by theory, that the intensity of light on March 30 ought to be 100 times stronger than that of a star of fourth mag- nitude, and was induced to make preparations for a daylight obser- vation. I first saw the comet about 11 a.m. When the sky was perfectly cloudless about the sun, it had a whitish appearance, which rendered it a matter of no little difficulty to see the comet ; but during the passage of some cumuli clouds over the sun, and between the breaks, I obtained some excellent views of the comet, and several observations, which will no doubt be of great assistance in the accu- rate determination of the elements. The nucleus was nearly, if not perfectly, round, beautifully defined and planetary, the diameter 8" or 1 0". Two faint branches of light formed a divided tail, extend- ing about 40" from the head, like two longish erect ears or horns rising from each side of the disc. At times I felt certain that the nucleus twinkled. The tail resembled a thin smoke. With respect to the observations for position, I can only add that they were as good as could possibly be made, under the circum- * The comet was seen at noon near the sun by two other observers, at Truro and in the Isle of Anglesey. Phil. Mag, S. 3. Vol. 31. No. 206. Aug. 1847. L 146 Intelligence and Miscellaneous Articles. stances, by instrumental comparisons. The index errors are very- constant, and were accurately determined last evening. Greenwich M.T. Comet's R.A. Comet's Dec. Weight, h m s o I II o I II March 30 1 23 40 7 32 27 -1-1 48 43 1 1 55 8 7 33 56 +1 45 21 2 In the observations for the first position the centre of the field was estimated, and nine single results are tolerably accordant. The second place depends on one good observation with cross wires, clouds preventing any further comparisons. Had the sky been free from the whiteness which is so fatal to vision by daylight, I should have obtained much better places. I communicated an ephemeris to Mr. Dawes, who has observed the comet with extreme care, but I do not know at present whether he saw it yesterday in daylight. XXVIII. Intelligence and Miscellaneous Articles. ON A NEVr TEST FOU PRUSSIC ACID, AND ON A SIMPLE METHOD OF PREPARING THE SULPHOCYANIDE OF AMMONIUM. BY PROF. LIEBIG. WHEN some sulphuret of ammonium and caustic ammonia are added to a concentrated aqueous solution of prussic acid, and the mixture heated with the addition of pure flowers of sulphur, the prussic acid is converted in a iew minutes into sulphocyanide of am- monium. This metamorphosis depends on the circumstance, that the higher sulphurets of ammonium are instantly deprived by the cyanide of ammonium of the excess of sulphur they contain above the monosulphuret ; for instance, if a mixture of prussic acid and ammonia be added to the pentasulphuret of ammonium, the solution of which is of a deep yellow colour, and the whole gently heated, the sulphuret of ammonium is soon decolorized ; and when the clear colourless liquid is evaporated, and the admixture of sulphuret of ammonium expelled, a white saline mass is obtained, which dissolves entirely in alcohol. The solution yields, on cooling or evaporation, colourless crystals of pure sulphocyanide of ammonium. Only a small quantity of sulphuret of ammonium is requisite to convert, in the presence of an excess of sulphur, unlimited quantities of cyanide of ammonium into sulphocyanide ; because the sulphuret of ammo- nium, when reduced to the state of monosulphuret, constantly reac- quires its power of dissolving sulphur and transferring it to the cyanide of ammonium. The following proportions will be found to be advantageous: — 2 oz. of solution of caustic ammonia of 0'9^ spec. grav. are saturated with sulphuretted hydrogen gas ; the hydrosulphate of ammonia thus obtained is mixed with 6 oz. of the same solution of ammonia, and to this mixture 2 oz. of flowers of sulphur are added ; and then the product resulting from the distillation of 6 oz. prussiate of potash, 3 oz. of the hydrate of sulphuric acid, and 18 oz. water. This mixture is digested in the Intelligence and Miscellaneous Articles. 147 water-bath until the sulphur is seen to be no longer altered and the liquid has assumed a yellow colour; it is then heated to boiling, and kept at this temperature until the sulphuret of ammonium has been expelled and the liquid has again become colourless. The deposited, or excess of, sulphur is now removed by filtration, and the liquid evaporated to crystallization. In this way from 3^ to 3^ oz. of daz- zling white dry sulphocyanide of ammonium are obtained, which may be employed as a reagent, and for the same purposes as the sulpho- cyanide of potassium. Of the 2 oz. of sulphur added, ^ an oz. is left undissolved. The behaviour of the higher sulphurets of ammonium towards prussic acid furnishes an admirable test for this acid. A couple of drops of a prussic acid, which has been diluted with so much water that it no longer gives any certain reaction with salts of iron by the formation of prussian blue, when mixed with a drop of sulphuret of ammonium and heated upon a watch-glass until the mixture is be- come colourless, yields a liquid containing sulphocyanide of ammo- nium, which produces with persalts of iron a very deep blood-red colour, and with persalts of copper, in the presence of sulphurous acid, a perceptible white precipitate of the sulphocyanide of copper. — Liebig's Annalen, Jan. 1847. ON THE FUSION OF IRIDIUM AND RHODIUM. BY R. HARE. This communication respects mainly my success in fusing both iridium and rhodium, neither of which, in a state of purity, had been previously fused. It may be supposed that the globule of iridium, obtained by Children's colossal battery, forms an exception ; but the low specific gravity and porosity of that globule may justify a belief that it was not pure, and at any rate the means employed were of a nature not to be at command for the repetition of the process, so that iridium might as well be infusible, as to be fusible only by such a battery. The first specimen of the last-mentioned metal on which I ope- rated was one given me by Mr. Booth, a former pupil of Wohler, whom he had assisted in obtaining it by the excellent process de- vised by that distinguished chemist. This specimen was fused in the presence of Mr. Booth. Subsequently I procured specimens, warranted pure, severally from the house of Pelletier at Paris, and from Messrs. Johnson and Cock, London. Another specimen was given to me by a friend, who had received it as pure, from a source on which reliance may be placed ; and lastly, I obtained myself, by Wohler's process, a specimen of about sixty grains, from the inso- luble residue of platinum ore. All the specimens thus procured were found to be fusible under my hydro-oxygen blowpipe. The specimen obtained from Messrs, Johnson and Cock, after repeated fusions, by which it was much consolidated, weighed sixty-seven grains. During fusion there appeared to be an escape of volatile matter, supposed to be osmic acid, arising from the presence of a minute portion of osmium, between which and iridium an affinity of L2 148 Intelligence and Miscellaneous Articles, a peculiar degree of energy exists. At a certain point of the process a reaction took place sufficiently explosive to throw a portion of the metal, in globules, off from the support. One of these, about twice as large as the head of a common brass pin, proved to be hollow. By prolonged and repeated fusion the metal became more compact and more fusible. Fused iridium has nearly the grain of soft cast steel, with the pale whiteness of antimony, and appears to be susceptible of a fine polish. Although as hard as untempered steel, it is somewhat sectile, since, when split by means of a cold chisel, the edge penetrated about the eighth of an inch before a division was effected. By light ham- mering a corner was flattened without fracture, although under heavier blows the mass cracked. I infer that although nearly un- malleable and very hard, iridium may be wrought in the lathe. I have already mentioned that I fused into a globule a specimen of iridium obtained by me from the insoluble residuum of platinum ore by Wohler's process. From this globule, while congealing, a portion ran out from the inside, leaving a cavity and covering one of its sides externally with an incrustation, among which crystalline spangles, or facets, were discernible. The specific gravity of the globule of iridium, from the specimen furnished by Messrs. John- son and Cock, was taken by Mr. T. R. Eckfelt of the United States mint at Philadelphia, and by Dr. Boye, both having balances of the greatest accuracy, and being very skilful in the employment of them. In the first instance there was a perfect coincidence in the results obtained, 21*83 being the numbers found by both of these gentlemen. Agreeably to another trial made by Dr. Boye, using river-water instead of distilled, the number was 21*78, water being in either case about sixty-eight, with allowance for the diflference of the water, and the temperature being above the standard of 60°. The specific gravity of the specimen may then be estimated at 21*80. The specific gravity of fused platinum, purified according to the instructions of Berzelius, before subjection to the hammer, proved in one specimen to be not more than 19*70, although by hammering it became equal to 21*23. It is with fused platinum that fused iridium should be compared. Of course the specific gravity of the last-mentioned metal, when both are obtained by fusion, may be assumed to be one-tenth greater than that of the former. Moreover, as this metal is the only impurity existing in the standard platinum of London, of Paris, or of St. Petersburg, it follows that a high specific gravity is not to be viewed as a proof of purity. Accord- ingly a specimen of platinum, purified from iridium by the Ber- zelian process, and which had proved eminently susceptible of being beaten into leaf, was found only to be of the gravity of 21*16, while that of a specimen of standard Russian platinum, very briUiantly white but inferior in malleability, presented to me by his Excellency Count Cancrine, as a specimen of the purest platinum of the Russian mint, was 21*31. Of rhodium I have fused two specimens, one of five pennyweights, purchased of Messrs. Johnson and Cock, the other received through IntelUsence and Miscellatieous Articles. 149 "b the same channel as the specimen of iridium above-mentioned*. Rhodium is at least as fusible as iridium, both of the specimens alluded to having been converted into fluid globules. That pro- cured from Messrs. Johnson and Cock gave a globule weighing ninety grains. On a second fusion it formed a perfect globule as fluid as mercury ; and yet in congealing lost its brilliancy by be- coming studded with crystalline facets all over its surface, excepting the portion in contact with the support. The facets had the ap- pearance of incipient spangles. The rapidity with which they were formed seemed anomalous. The mass being split by a cold chisel and viewed by a microscope, it appeared porous immediately beneath the facets. When the mass was first fused, I found by the gravimeter the specific gravity to be 11 '0, which coincides with the observations of WoUaston. Yet by a careful trial made at the United States mint by Mr. Eckfelt, after the second fusion and the forma- tion of the facet, the specific gravity proved to be only 10'8. This is sufficiently explained by the porosity above mentioned. In fact the porosity to which rhodium and iridium are liable may render it difficult to find specimens of precisely the same specific gravity. In sectility, malleability and hardness, rhodium did not appear to differ much from iridium, but it is not of so pale a white as iridium. The one has the pale white of antimony, the other the ruddy hue of bismuth. Osmiuret of iridium, as existing in the native spangles associated with platina ore, or as otherwise obtained, is far more difficult of fusion than pure iridium. The propensity to assume the crystalline form, and to adhere to it, is even greater in this alloy than in the last-mentioned metal. On first exposure to the most intense heat of the hydro-oxygen blowpipe some slight appearances of fusion may be seen, and the spangles or grains may be made to cohere. Nevertheless it yields very slowly, aijd requires an expenditure of gas too great to be incurred unless it were for the purpose of once well determining the question of its ultimate fusibility. This ob- ject was obtained completely as respects a globule of 45 grains in- weight. The specific gravity of this globule appeared to be 20*4, but this result was evidently less than tliat whicii would have been obtained had there not been some minute cavities, which, after splitting the globule, were detected by a magnifier. The specific gravity of some large spangles of osmiuret of iridium from South American ore was, by Dr. Boye, found to be 19*835. That of some grains heavier but not so flat, presented to me by Count Cancrine, was found to be 20'938. That the alloy of iridium with osmium should be more difficult to fuse than pure iridium, leads to the inference that osmium must be the most infusible of the metals, although, like carbon, very sus- ceptible of combustion, and capable, like tliat infusible non-metallic radical, of forming a volatile peroxide. Of course its liability to oxidizement would render it impossible to fuse it by the hydro- * One other larger specimen from the same source has been fused since the above was written. 150 Intelligence and Miscellaneous Articles. oxygen blowpipe, of which the efficacy requires the simultaneous presence of oxygen and the most intense heat. It might be fused by exposure in vacuo to the discharge of a powerful voltaic series, by means of the apparatus of which a description with engravings has been given in a recent volume of the Transactions of the Ame- rican Philosophical Society, and republished in ' Silliman's Journal' for 1841, vol. xl. p. 303. I have obtained osmium by heating the osmiate of ammonia in a glass tube with sal-ammoniac, agreeably to the instructions given by Berzelius. In this way a result was obtained which the information given by that distinguished chemist had not led me to anticipate. The tube became coated with a ring of osmium, which it would be impossible by inspection merely to distinguish from the arsenical ring on the peculiar features of which reliance has been placed for the detection of arsenic. It follows from my experiments and observations, that of all metallic bodies, osmiuret of iridium is the most difficult to fuse ; that rhodium and iridium are both fusible by the hydro-oxygen blow- pipe, properly employed ; that the former has the rosy whiteness of bismuth, the latter the pale white of antimony ; and that both of them are slightly sectile, though extremely hard and nearly un- malleable ; that iridium merely fused is heavier than platinum con- densed by the hammer. Thus it follows from my experiments, and from the recent observations of Breithaupt, on some specimens of native iridium, that the metal, whether in this state or pure as ob- tained by chemical skill and consolidated by fusion, must be allowed that pre-eminence in density, which, until of late, was given to platinum. It may be proper to add, that subsequently to the writing of the preceding narrative, receiving some large quantities of iridium and rhodium from Messrs. Johnson and Cock, my experiments were successfully repeated on a larger scale, but without any result be- sides that of confirming the facts above stated. — Silliman's Journal for Nov. 1846, p. 365. NOTE ON THE MEANS OF TESTING THE COMPARATIVE VALUE OF ASTRINGENT SUBSTANCES FOR THE PURPOSES OF TAN- NING. BY ROBERT WARINGTON, ESQ. Having been frequently called upon to examine the value of astringent substances imported into this country for the purposes of tanning, such as valonia, divi-divi, sumac, cutch, &c.,-I am induced to believe that the detail of the manipulation adopted may not be without interest to some of the members of the Society. As the manufacture of leather was the object of the purchaser of these materials, gelatin was selected as the basis for the estimation of their comparative value ; and after several trials with various kinds of natural and manufactured gelatin, such as varieties of isinglass, glue, patent gelatin, &c., the finest long staple isinglass was found to be the most constant in its quality and least liable to undergo change. Intelligence and Miscellaneous Articles. X&\ With this therefore the test solution was prepared, of such a strength, that each division, by measure in the ordinary alkalimeter tube, should be equivalent to the one-tenth or one-fourth of a grain of pure tannin, and thus the number of divisions used would indicate the proportion of available tannin or substance precipitable by ge- latin contained in any specimen. A given weight of the sample under trial was then infused in water, or if necessary the astringent matter extracted by boiling, and the clear liquid precipitated by the test solution until no further deposit occurred. It was necessary in the course of this operation to test at intervals a portion of the solution under examination, to ascertain the pro- gress of the trial ; and this, from the nature of the precipitate, was attended at first with some little difficulty : paper filters were inad- missible from the quantity of the solution they would absorb, and thus introduce a source of extensive error ; subsidence rendered the operation very tedious. The plan I have adopted is as follows : — a piece of glass tubing, about twelve inches in length and about half an inch internal diameter, is selected, and this has a small piece of wet sponge loosely introduced into its lower extremity, and when it is wished to abstract a part of the fluid under investigation for a separate testing, this is immersed a few seconds in the partially pre- cipitated solution ; the clear liquid then filters by ascent through the sponge into the tube, and is to be decanted from its other extremity into a test glass ; if on adding a drop of the gelatin solution to this a fresh precipitate is caused, the whole is returned to the ori- ginal bulk, and the process proceeded in, and so on until the opera- tion is perfected ; this method of operating is facilitated by conduct- ing the examination in a deep glass. After a few trials the mani- pulation will be found extremely easy, and in this way considerable accuracy may be arrived at. — From the Proceedings of the Chemical Society. ________ ON THE TWO VARIETIES OF ARSENIOUS ACID. By M. BUSSY. The author first gives a new process for determining the quantity of arsenious acid. This process is based on the employment of stand- ard reagents. The reagent which he uses is permanganate of pot- ash, which M. Marguerite has already successfully employed for the quantitative determination of iron. When a solution of permanganate of potash is poured into a solu- tion of arsenious acid, it becomes arsenic acid, and the red colour of the reagent disappears. The liquor begins to become coloured only when the transformation of arsenious acid is complete. When, then, a standard solution of permanganate of potash is prepared, the quan- tity of arsenious acid contained in any solution may be determined by that of the permanganate required to convert it into arsenic acid. M. Bussy states that the two varieties of arsenious acid, the vi- treous and opake, absorb the same quantit}'' of permanganate, and consequently that the diiFerences observed in their solubility is not derived from any difference of oxidizement. With respect to the solubility of the two varieties of arsenious 152 Intelligence and Miscellaneous Articles. acid, M. Bussy has arrived at the following conclusions : — 1st. The vitreous, so far from being less soluble in water than the opake acid, as stated by chemists, is, on the contrary, much more soluble. This difference is nearly in the proportion of 3 to 1, at about 53° to 55° of F. ; the same quantity of water which dissolves 36 to 38 parts of the vitreous acid, will take up only 12 to 14 of the opake. 2nd. The vitreous acid dissolves much more rapidly than the opake acid. 3rd. Neither of the varieties possesses a degree of solubility which is to be regarded as strictly peculiar to it. 4th. The opake acid is converted into vitreous acid by long boiling in water ; that is to say, it then acquires the same degree of solubility as the vitreous arsenious acid, which is such that 11 parts are dissolved by 100 of water. 5th. Under the influence of water and a low temperature, the vitreous acid is converted into opake acid ; that is to say, a solu- tion of vitreous acid becomes reduced after a certain time to the point of saturation which belongs to the opake acid. 6th. The mix- ture of the two varieties of acid in the same solution explains the anomalies observed in the solubility of arsenious acid, which in fact offers nothing opposed to the principles admitted by chemists. 7th. Division, which facilitates the solution of the opake acid, without however increasing its solubility, considerably diminishes that of the vitreous acid ; and to such an extent, that this acid, reduced to fine powder and levigated, is not sensibly more soluble in water than the opake acid ; this resulting unquestionably from a transformation which it undergoes, either at the moment of pulverization, or of its contact with water. 8th. Acid which has been rendered opake by the action of ammonia, and acid crystallized in water, act similarly with water, and appear to belong to the samevariety. 9th. The opake acid dissolves more slowly than the vitreous in dilute hydrochloric acid. This circumstance, which thus modifies the nature of the products formed during solution, explains why the luminous phseno- mena observed by M. Rose in the crystallization of the vitreous acid, are not in general observable with so great intensity in the solution of the opake variety. ] 0th. The difference which has been observed in the action of the two arsenious acids on tincture of litmus is merely apparent. If the opake acid does not redden the tincture, it is on account of its slight solubility, and especially because it dis- solves slowly ; whilst the vitreous acid, which dissolves quickly, immediately reddens the tincture. But if comparative experiments be made, and the tincture be exposed to the action of the powder, it becomes gradually red, and no difference is perceptible at the ex- piration of three or four days. — Comptes Rendus, Mai 1847. ON THE PREPARATION OF GUN-COTTON. Mr. Coathupe recently forwarded to the Chemical Society two specimens of gun-cotton, with a view to illustrate the greatly in- creased explosive effects that are to be derived from a subsequent immersion of the gun-cotton, when properly prepared in the ordi- nary way, in a saturated solution of chlorate of potash. Intelligence and Miscellaneous Articles. ] 53 " Having experimented with solutions of nitrate of ammonia, ni- trate of potash, nitrate of soda, bichromate of potash, &c. &c., for the purpose of increasing the explosive properties of this interesting substance, I can affirm that none of the results will bear the slight- est comparison with those obtained from the solution of chlorate of potash, either in rapidity of ignition or in intensity of flame. The process adopted for preparing the inclosed specimens was as follows : viz. into a mixture of equal measures of strong nitrous acid and of oil of vitriol, spec. grav. 1*845, the cotton was immersed and stirred with a glass rod during about three minutes : it was then well- washed in many waters and dried ; a portion of it was then soaked for a few minutes in a saturated solution of chlorate of potash, well- squeezed and dried." ON BALSAM OF TOLU, AND SOME PRODUCTS DERIVED FROM IT. M. E. Kopp states that the experiments which he has made on this substance confirm the greater number of the results previously obtained. He remarks that the balsam is composed of a very small quantity of tolene C'oH"', C=75H=6"25; of free cinnamic acid, CIS H'6 O* ; of a resin very soluble in alcohol, C^e H?8 O^ ; of a resin slightly soluble in alcohol, C'« H^o O*, or C^e H^o Qio. Tolen. — This carburetted hydrogen was prepared by exactly fol- lowing the plan proposed by M. Deville. It is colourless, very fluid, of a penetrating taste somewhat like pepper, and its smell resembles that of elemi. Its density at 60° F. is 0'858 ; its boiling-point is between 310° and 320° F. Exposed in an imperfectly closed tube, it gradually becomes resinous and very slightly coloured. M. De- ville gives as its formula C'^H'^. M. Kopp states that his analysis, which diff'ers but little from that of M. Deville, indicates 0'° H'^, Cinnamic Acid. — The free acid of balsam of Tolu, as observed by M. Fremy, is merely cinnamic acid. This fact was proved by ana- lysis, and by its conversion into nitrocinnamic acid, very slightly soluble in cold alcohol ; whereas benzoic and nitrobenzoic acids are very soluble in it. The results obtained by M. Deville are probably derived from his having examined the acids procured by the distilla- tion of the balsam, or extracted by concentrated alkaline solutions. M. Kopp has shown that, under these two circumstances, the resins of balsam of Tolu are so changed as to give rise to a large proportion of benzoic acid. The resins, cautiously distilled with caustic soda, yield pure benzoen, and a coaly residue which contains much benzoate of soda. Cinnamic acid, mixed with cold concentrated caustic soda, and submitted to a current of chlorine, is converted into chlorocin- namic acid C'** (H^* Cl^) O*. If however the temperature be raised and the action is very strong, the chlorinated oil described by Mr. Stenhouse is disengaged, and chlorobenzoic acid, C* (H'o Cl^) O*, is formed. These two acids strongly resemble each other ; but the latter is more soluble in water and in alcohol, and its salts crystallize more readily. Cinnamic acid, treated with concentrated nitric acid, is at 1 54 Intelligence and Miscellaneous Articles. first converted into nitrocinnamic acid, then into benzoic acid, and finally into nitrobenzoic acid. Cinnamic and benzoic sethers are both, though with great diffi- culty, converted into nitrocinnamic acid and nitrobenzoic aether. There is almost always a great part of the sether decomposed, and the acids are set free. Nitrobenzoic sether is solid, colourless, and of an aromatic odour and taste. It crystallizes in fine rhombic lamina;. Its melting-point is 11 6°, and its boiling-point 664°. It is easily obtained by exposing an alcoholic solution of nitrobenzoic acid to a current of hydrochloric acid gas. Its formula is C* (H« N^ O*) 03 + C* H'oOrrC's H'^ N^ O^. Nitrocinnamic acid dissolved in an alcoholic solution of sulphuret of ammonia is reduced with the assistance of a gentle heat. Sulphur is deposited, and two distinct substances are formed, one of which is of a yellowish colour and belongs to the class of resins, and the other to that of alkaloids. The latter is solid, colourless, crystallizes in small indistinct masses, insoluble in water, soluble in alcohol and in aether, and forms difficultly crystallizable salts. Resin a, C^^ H^s O^. This substance is brown, translucent, brittle when cold ; its powder agglomerates at 59° F. and fuses perfectly at 140° F. Concentrated sulphuric acid imparts a purple colour to it. When dissolved in potash and exposed to the air, it is readily oxi- dized, and is converted into resin /3. By dry distillation it yields benzoen and benzoic acid. It dissolves readily in alcohol and in aether. Resin jd, C's H^° O^ Colour dull brownish-yellow, without taste or smell, slightly fusible (above 212° F.), but little soluble in alcohol or ajther. It is less alterable than the preceding resin. Sulphuric acid renders it of a violet colour ; potash dissolves it with a brown colour. The mixture of the two resins treated with nitric acid yields, as gaseous products, carbonic acid, nitrous vapours and nitric oxide ; as volatile products, hydruret of benzule, hydrocyanic acid, and a little benzoic acid ; as residue, a flocculent yellowish substance, which is benzoic acid intimately combined with a yellow colouring matter of a resinous nature, which destroys its crystallizing power, and accompanies it in all its combinations, even in that of aether. By the action of heat, especially by distillation, the resinous matter is destroyed, and perfectly pure benzoic acidis obtained. The resin yields nearly one-third of its weight of benzoic acid. As to the constitution of balsam of Tolu, it seems very simple. Primarily it is formed of the soft resinous matter C^'^ H^s O'', or of that which gives rise to it. This resin, under the influence of the air, is converted into cinnamic acid and resin /3 : C^^ H38 + 0^=C'8 H'" O^ + C'sH^oO^-fH'^O. In fact it is observed that in time balsam of Tolu becomes hard, and contains a larger quantity of cin- namic acid. The resin C'^ W^ O* may itself easily furnish benzoic acid for C'sH^o 0^=0'^ Hi^O^ + H^ O + C* H^ The carburetted hydrogen perhaps gives rise to tolene ; but it is more probable that it is converted by the action of oxidizing bodies into resinous colour- Intelligence and Miscellaneous Articles. 156 ing matter, or perhaps into water and carbonic acid. — Ann. de Ch. et de Phys., Juillet 1847. ON THE EQUIVALENT OF TITANIUM. BY M. ISIDORE PIERRE. The author remarks that chemists generally agree that it would be difficult to add to the precision of the numbers which represent the equivalents of hydrogen, carbon, chlorine, bromine, iodine, phos- phorus, arsenic and silicon, as determined by the researches of Du- mas, Marignac and Pelouze. M, Pierre thinks however that this is not the case with titanium ; and that if the labours of different periods respecting this substance be examined, it will be evident that its equivalent requires renewed examination. M. H. Rose originally obtained, by various methods, numbers which varied between 380 and 450 ; but he afterwards found that the sulphuret of titanium which he employed in his experiments, was procured free from titanic acid with great difficulty. In his last experiments, M. Rose made use of chloride of titanium, which he decomposed by water. He precipitated with ammonia the titanic acid derived from this decomposition, and afterwards treated the filtered liquor with nitrate of silver, in order to separate the chlorine in the state of chloride of silver : this method gave him 303*686 as the equivalent of titanium. The chloride of titanium used by M. Pierre was not prepared from rutil, but from calcined artificial oxide of titanium : it was free from oxide of iron and from chloride of silicium, and its boiling-point was perfectly stationary. The chloride employed had been kept in a small tube from the time of its preparation hermetically sealed : it was broken by agitation in a stopped bottle, one quarter filled with distilled water. By frequent agitation, Avithout unstopping the bottle, the whitish cloud at first produced above the liquid disappears. Without this precaution there would be a probable loss of hydrochloric acid in opening the bottle too soon, or by introducing the solution of silver, which would expel a small quantity of this vapour. The following results were obtained : — gr. I. Chloride of titanium employed. . 0"8215 Silver 1'84523 indicating Chlorine 0'60623 Titanium by difference 0*21727 These results gave 314*76 as the equivalent of titanium. II. Chloride of titanium employed. . 0*774 Silver 1*73909 indicating Chlorine 0*57 136 Titanium by difference 0*20264 These numbers give for the equivalent of titanium 314*37. III. Chloride of titanium employed. . 0*7775 Silver 1*74613 indicating Chlorine 0*57367 Titanium by difference 0*20383 The equivalent of titanium deduced from this experiment is 31 4*94 . 156 Intelligence and Miscellaneous Articles, IV. Chloride of titanium employed. . 0*716 Silver 1-61219 indicating Chlorine 0'52966 Titanium by difference 0*1 8634 Equivalent of titanium 31 1*84 . V. Chloride of titanium employed. . 0"8085 Silver 1-82344 indicating Chlorine 0*59907 Titanium by difference 0-20943 Equivalent of titanium 309*38. The three first numbers agree perfectly, but the two latter are notably less, especially the last, since it differs from the three first by five whole numbers, or more than 1^ per cent. It was difficult to attribute this difference entirely to deficient precision in the me- thod used. It occurred to the author that it might be owing to the partial decomposition of the chloride of titanium, by the moisture of the air during manipulation, and this was soon found to be the case by direct experiment. M. Pierre proposes to adopt, as the nearest approximation to truth, 314-69, the mean of the three first experiments, as the equivalent number for titanium. This number is very different from 355 deduced from 6-536, the density of the vapour of the chloride of titanium observed by M, Dumas. Its density, calculated from 314-69, would be 6-614. — Ann. de Ch. et de Phys., Juillet 1847. ON A MODIFICATION OF THE APPARATUS OF VARRENTKAPP AND WILL FOR THE ESTIMATION OF NITROGEN. BY WARREN DE LA RUE. My attention having been called to a communication by Mr. Alex. Kemp in the number of the ' Chemical Gazette' for the 1st of April 1847, in which he describes a modification of Messrs. Varrentrapp and Will's tube for nitrogen determinations, of a very similar con- struction to one I employed as far back as November 1845 in the laboratory of the Royal College of Chemistry, and which I have re- peatedly shown to my friends, I am induced to lay before the So- ciety a description of my form of apparatus, which differs somewhat from that described by Mr. Kemp. By the drawing, it will be seen that the tube B E, instead of opening immediately into the bottom of the flattened bulb C, is pro- longed and rises for some distance into the bulb curving over to- wards its side ; in this respect Mr. Kemp's apparatus does not differ materially from mine. I found it necessary however to have a third bulb (D) blown (which is best of a spheroidal form), in order to ef- fectually prevent the acid from being drawn into the tube G when- ever a sudden absorption took place ; this third bulb communicates with C by a narrow neck. If the apparatus be constructed without Intelligence and Miscellaneous Articles. 1 57 the third bulb D, a portion of fluid generally passes into the tube G from the rotary motion induced in the fluid in C. The dotted lines indicate the height of fluid in the bulbs, and this quantity is quite sufficient for the condensation of all the ammonia likely to be formed. I would remark, that if during the progress of the combustion a cessation of the production of gas should occur, the construction of the apparatus is such as to prevent the whole of the acid ever being carried over into the bulb C, so that on the evo- lution again commencing no fear need be entertained for the com- plete condensation of the ammonia. It only remains for me to add, that though this new form of ap- paratus is not so readily rinsed out as the original one of Messrs. Varrentrapp and Will, no great inconvenience is experienced from that cause, as the acid can, at the close of the operation, be easily caused to flow into the bulb C and out at the tube G, by properly inclining the bulbs, &c., and when this is done water or alcohol may be introduced by a pipette through the limb H. From the Proceedings of the Chemical Society. ON THE DETECTION OF COTTON IN LINEN. BY G. C. KINDT. This subject has frequently engaged the attention of commercial and scientific men ; many experiments have been made in order to detect cotton thread in linen ; many processes have been recommended, but none have hitherto proved satisfactory. I was therefore much sur- prised when a stranger, a few weeks ago, showed me a sample of linen from the one-half of which all the cotton filaments had been eaten away. He had obtained it in Hamburg, and asked me whether I could give him a process for eflfecting this purpose. Now since, as far as I am aware, nothing has been published on this subject, and it is of very general interest, I consider it a duty to communi- cate the results of my experiments. I had already observed, in ex- perimenting with explosive cotton, flax, &c., that these two sub- stances behave somewhat diflferently towards concentrated acids ; and although it has long been known that strong sulphuric acid con- 158 Intelligence and Miscellaneous Articles^ verts all vegetable fibre into gum, and when the action is continued for a longer period, into sugar, I found that cotton was metamor- phosed much more rapidly by the sulphuric acid than flax. It is therefore by means of concentrated sulphuric acid that cotton may be removed from linen when mixed with it ; and this object may be obtained by the following process : — The sample to be examined must be freed as perfectly as possible from all dressing by repeated washing with hot rain- or river-water, boiling for some length of time, and subsequent rinsing in the same water; and I may expressly observe, that its entire removal is requisite for the experiment to succeed. When it has been well- dried, the sample is dipped for about half its length into common oil of vitriol, and kept there for about half a minute to two minutes, according to the strength of the tissue. The immersed portion is seen to become transparent. It is now placed in water, which dis- solves out the gummy mass produced from the cotton ; this solution may be expedited by a gentle rubbing with the fingers ; but since it is not easy to remove the whole of the acid by repeated washing in fresh water, it is advisable to immerse the sample for a few in- stants in spirits of hartshorn (purified potash or soda have just the same eifect), and then to wash it again with water. After it has been freed from the greater portion of the moisture by gentle press- ure between blotting-paper, it is dried. If it contained cotton, the cotton threads are found to be wanting in that portion which had been immersed in the acid; and by counting the threads of the two portions of the sample, its quantity may be very readily estimated. If the sample has been allowed to remain too long in sulphuric acid, the linen threads likewise become brittle, or even eaten away ; if it were not left a sufficient time in it, only a portion of the cotton threads have been removed ; to make this sample useful, it must be washed, dried, and the immersion in the acid repeated. When the tissue under examination consists of pure linen, the portion im- mersed in the acid likewise becomes transparent, but more slowly and in a uniform manner, whereas in the mixed textures the cotton threads are already perfectly transparent, while the linen threads still continue white and opake. The sulphuric acid acts upon the flax threads of pure linen, and the sample is even somewhat trans- parent after drying as far as the acid acted upon it, but all the threads in the sample can be seen in their whole course. Cotton stuffs containing no linen dissolve quickly and entirely in the acid; or if left but one instant in it, become so brittle and gummy that no one will fail to recognise it as cotton when treated in the above manner. — Liebig's Annalen, Feb. 1847. THE PLANET HEBE*. On July 1, M, Henke of Driessen in Prussia, discovered another planet, which appears to belong to the singular group lying between the orbits of Mars and Jupiter. It was first observed accurately at • Communicated by J. R. Hin(|, E8q.,F.R.A.S. Meteorological Observations. 159 Berlin by Prof. Encke on July 5, and since that date observations have been made very generally at the different European observato- ries. The following are the elements according to different calcu- lators :— - Galle and d' Arrest. Neumann. H*nd. Epoch. July 10-0 Berlin. July 8-41864 Berlin. July 00 Greenwich. Mean anomaly Long perihelion ^L^scending node Inclination 268 5.5 50-6 19 4 14-9 139 5 31 14 88 58-5 10 41 16-7 0-3772450 283 9 4^-6 9 3 9-6 138 12 16-2 14 49 536 13 5 48-2 0-3955266 283 56 54-0 8 17 24-1 137 25 351 15 2 561 13 49 200 0-4016899 Sin-i e Log. semi-axis major The longitudes in first and second set are counted from M. Equi- nox of 1847-0 ; in the third set from M. Equinox of July 0. METEOROLOGICAL OBSERVATIONS FOR JUNE 1847- Chiswick. — June I — 3. Clear and very fine. 4. Light clouds and fine. 5. Cloudy. 6. Light clouds : clear, 7. Clear : cloudy. 8. Rain : thunder-showers. 9. Clear and fine. 10. Rain: cloudy: clear. 11, 12. Clear and very fine. 18. Rain : cloudy. 14. Densely clouded : showery. \5. Rain: thunder and heavy shovt^ers. 16. Cloudy : rain. 17,18. Rain. 19. Cloudy and fine. 20. Cloudy: slight showers. 21. Cloudy: fine. 22. Very fine. 23. Very fine : heavy showers, with thunder. 24. Cloudy and fine. 25. Rain : cloudy and fine. 26. Very fine. 27. Drizzly : cloudy and fine, 28. Fine. 29. Very fine, 30. Light clouds : very fine : overcast. Mean temperature of the month 58°*46 Mean temperature of June 1846 66 '63 Mean temperature of June for the last twenty years 66*90 Average amount of rain in June l-88inch, ^os7fi :>;-07<0— i-Jt^OOOO-^iT'Oi^ OOOOOC«OOI'7<-7iOOOO : to CI lo >-< — ' ; coo o o o ^ 01 B S S C 0) & fe « g ^ " a '^ S2 S S ^ ^ : aJ ^ ^' s' ^ i i ^ i ^ ^ " ^ ^ I ^ ^ ^ C cn c/3 {/I fe fc ^' V C « « ^' S S c c -3 ^- . . . s s . . a fe a 2 ^^' • a • q S o 2 oJ aJ 2 aj J aJ ^' (i ^ > ^* g:* g: 6- B: ^' j-' ^ ^ B= fe" ^ ^ fe 6t ^* aJ .00 00^Oa\-<--^O'OtC'^ «llM HS «I(M «!« mIo Hd h|s ^IS «]« 0^■^C^cooo^»0^a^OO^(M^OOO<^^coco^o'o — -"t^O-^-^-^io-HOOovo "I« «I« rtldi-tel i o lo «N vo — < o^ r^ >-4 o^ — CO r^ CO •^ CO IC O lO IC lO LfS »0 to <0 lO ^ <0 lO lO m lO lO VO lO lO !> !>. «>. ip ip ip ip »p OM3NONC0— a>t--'^inTtibd o — o co'o6>qo ctn— ' co-^'-icsincs lO'-" (m lOiO»0^'0»OiOlOlOir>»0'£>*OVOlO>0>OlO>OlO>O^OVO^OlO>OlOO*OlO •u'W •XBH Hwg -Wg O0000OM3^OO'--(TiQ0r-CClt>.O00MOpco'^co« oi^ (n cooi O O O O O O O^O^C^O^O^O^O^O^O^O^C^O^C^O^O^C^O^O^O^O^O O O O COrorocOCOCO(MO00'^OOOt0OmiCQ0i0O-i«MOI:^«M(N0MCCNO ■^^cococ-i o o^ioop ipopcp >pco(N kp-^ip ir-i>--pco'^?pc<>^o07o lO-'S' — o 00 •^vo t^ O lO o^oo COOM3>IO CPiO O « ip ip ip ip CTi o^ cr\ ON CI d d CI lOO^ t--in ON-<* CO CI 6 6 coco O CO d o 00 lO IC -^ O co*0 lO ^ 00 00 00 o 0\ 6 d> cOd 00 00 -< 00 t^io d in C--0 t^t^ •«* o 00 d -rf -H Tf -^lO d O d d d d d O IC t^d ON*© *0 lO I>. -< d d d d 6 6 6 6 6 CO CO CO CO CO JO SiiBQ F^C(C0TfiO(Ot^00ONO'- I. 11. Carbon 75-27 75*40 75-55 ^34 2500-0 Hydrogen 12*51 12-66 12*59 H34 425-0 Oxygen . 12-22 11*94- 11*86 O4 400-0 100-00 100-00 100-00 3325-0 These results agree completely with the formula for margaric acid, and were further confirmed by the analysis of its silver salt and aether. 4*643 grains of the silver salt gave 1*325 of silver =28*53 per cent. 7*926 grains of the silver salt gave 2*284 of silver =28*70 per cent. The calculated result for margarate of silver gives 28*65 per cent. The aether was prej:>ared in the usual manner, by dissolving the acid in absolute alcohol, and passing dry hydrochloric acid gas through the solution. The product, which possessed all the properties of margaric (ether, gave the following re- isults of analysis: — of the Fixed Oils in contact with Sulphur. 167 {5-596 grains of the asther gave 15*662 ... carbonic acid, 6-399 ... water. Experiment. Calculation. Carbon Hydrogen Oxygen . . 76-33 . 12-70 . 10-97 76-51 12-74 10-79 C38 O4 2850-0 475-0 400-0 100-00 100-00 3725-0 Tiiese analyses establish, in a satisfactory manner, that the acid produced was margaric acid. It is scarcely possible how- ever, in the present state of the investigation, to give anything like a rational explanation of the mode in which it is here formed. Its production from oleic acid has been already observed by Laurent as the first product of oxidation by nitric acid; but the action of sulphur is certainly of a, very different character, and cannot be considered as bearing any analogy to that of an oxidizing agent. The quantity of margaric acid produced does not appear to be constant, but varies with the rapidity of the distillation, and is always most abundant when it is slowly performed. The oil which distils previous to and along with the mar- garic acid, and constitutes by far the most abundant product of the action of sulphur upon oleic acid and oil of almonds, is a very complex substance, and contains some of its constituents in very small proportion. On this account I found it neces- sary to prepare it in very large quantity; and in doing so I abandoned the use of almond oil and employed linseed oil instead, which is a much cheaper substance, and yields the same fluid products. When the product of the action of sul- phur is carefully rectified, the first portions which pass over are perfectly transparent and colourless, highly limpid and mobile, and boil at the temperature of 160 Fahr. Only a small quantity however passes at this temperature, and the immersed thermometer gradually rises without indicating any fixed boiling-point for the fluid. My first attempts to purify this oil and separate it into its various constituents, did not afford any satisfactory conclusions. Numerous analyses of the more volatile portions were made without obtaining com- parable results, although all indicated the presence of carbon and hydrogen nearly in the proportion of equal atoms. The following are the details of three of these analyses : — f 4-657 grains of the most volatile oil gave I. ■< 12-688 ... carbonic acid, and I 5-127 ... water. 168 Dr. T. Anderson on certain Products of Decomposition {5*50 J grs. of an oil less volatile than the preceding gave 15*762 ... carbonic acid, and 6*292 ... water. r 4*191 grains of another portion of oil gave III. < 12*185 ... carbonic acid, and L 4*720 ... water. Which correspond to the following results per cent. : — I. II. III. Carbon . . 75*03 78*79 79*95 Hydrogen . 12*20 12*72 12*75 All these oils, when treated with fuming nitric acid, yielded an abundant precipitate of the sulphate of barytes; but as the results of the combustion were not constant, no quantitative determination was made. The action of precipitants however upon this oil afforded a more satisfactory method of obtaining some of its consti- tuents. It gives with corrosive sublimate a bulky white pre- cipitate, and with bichloride of platinum a yellow compound, the characters of which vary slightly, according as it is pre- pared from the more or less volatile portion of the oil. Ni- trate of silver and acetate of lead, mixed with the alcoholic solution of the oil, produce only a slight cloudiness, but on boiling the solutions, the sulphurets of silver and lead are de- posited. The Mercuri) Compound, — In order to obtain this substance in the pure state, the oil was dissolved in alcohol, and an alcoholic solution of corrosive sublimate added. The preci- pitate which fell was collected on a filter, and washed with lEther until the oil was thoroughly extracted, for which pur- pose a considerable quantity of aether is required. It is then boiled with a large quantity of alcohol, which dissolves a part of it ; and the solution being filtered hot, allows the compound to deposit, on cooling, in the pure state. It is then in the form of a white crystalline powder, having a very fine pearly lustre, and exhibiting under the microscope crystals of a very peculiar form. They are six-sided tables, two opposite angles of which are rounded off, so as to give them a very close re- semblance to the section of a barrel. It possesses, even after long-continued washing with aether, a peculiar slight sickening smell, which becomes more powerful on heating, and its pow- der irritates the nose. It is insoluble in water, which moistens it with difficulty. It requires several hundred times its weight of boiling alcohol for solution, and is almost entirely deposited, on cooling, in microscopic crystals. In aether it is almost in- soluble. When heated, it is decomposed with the evolution of the Fixed Oils in contact with Sulphur, 169 of a peculiar nauseous smelling oil. The sparing solubility of this compound in alcohol renders its preparation in sufficient quantity for analysis an extremely tedious process, and I have sought in vain for a more abundant solvent. The only sub- stance which I have found capable of taking it up in larger quantity is coal-tar naphtha; but its employment is inadmissible, as the best which can be procured is an extremely impure substance, and the crystals of the compound deposited from it always acquire a rose or violet tint from some of its impu- rities. Oil of turpentine likewise dissolves it, but not more abundantly than alcohol. By many successive solutions in alcohol, I obtained enough of this substance for an analysis, of which the following are the results : — r 12*302 grains, dried in vacuo, gave < 6'592 ... of carbonic acid, and L 3-018 ... ofwater. 8*061 grains deflagrated with a mixture of nitre and car- bonate of soda, gave 7*297 grains of sulphate of baryta = 1-0067 = 12*48 per cent, of sulphur. The mercury and chlorine were determined together by mixing the substance with quicklime, and introducing the mixture into a combustion-tube. The end was then drawn out into an elongated bulb, into which the mercury sublimed, and which was afterwards cut off, dried in the water-bath, and weighed, both with and without the mercury; the chlo- rine was determined in the usual way from the residue in the tube. 9*958 grains gave 5'976 mercury =60*01 per cent., and 4'*310 grains chloride of silver =10-67 per cent, of chlorine. 5*797 grains gave 2*409 of chloride of silver = 10*25 per cent, of chlorine. These results correspond closely with the formula C^q Hjg S,^ Hg4 CI2, as is shown by the following comparisons : — Experiment. Calculation. -T-^ 11.^ A ( 1 Carbon . 14*61 ... 14*46 C16 1200*0 Hydrogen 2*72 ... 2*42 His 200-0 Mercury . 60*01 ... 60*32 Hg4 5003*6 Chlorine . 10*67 10*25 10*67 CI2 885*3 Sulphur . 12*48 ... 12*13 S5 1005*8 100*49 100*00 8294*7 It is sufficiently obvious that the formula O^q Hig S5 Hg4 Clg 170 Dr. T. Anderson on certain Products of Decomposition cannot be supposed to represent the rational formula of this substance. On the contrary, the remarkable analogy between its properties and those of the mercury compound of sulphuret of allyle appear clearly to indicate a similarity in their chemical constitution, — a similarity which, as we shall after- wards see, is borne out by the properties of the platinum com- pound. I consider this substance to contain an organic sul- phuret analogous to sulphuret of allyle, the constitution of which must be represented by the formula Cg Hg Sg, to which I give the provisional name of sulphuret of odmyl (from oS/aij, odow)^ and that the rational formula of the mercury com- pound is — (Cg Hg S,+ Hg, CI,) + (Cg Hg S, + Hg, S). On contrasting this with the formula of the allyle compound, which is — (Cfi H5 CI + Hg, CI,) + (Ce H5 S + Hg, S,), . two important points of difference are apparent, namely, that in the new compound we have the sulphuret, and not the chloride, of the base in union with corrosive sublimate, and the presence of subsulphuret in place of sulphui-et of mercury in the second member of the compound. It is even possible to approximate more closely the formulae of the allyle and odmyle compounds, by assuming the sulphuret of odmyle to be represented by C4 H4 S; in which case the oiercury compound becomes — {3(C4 H4 S) + Hg, S,} + (C4 H4 CH- Hg, CI). This formula is however incompatible with its reactions, as it involves the presence of calomel in the compound. Treat- ment with caustic potash however shows that this is not the case, as it immediately becomes yellow, from the separation of oxide of mercury, while the black suboxide would have been formed had calomel been present. When a current of sulphuretted hydrogen is passed through the mercury compound suspended in water, it becomes rapidly black, a peculiar smell is observed, along with that of sulphu-' retted hydrogen ; and by distillation an oil passes over, which is obtained floating on the surface of the water. It is per- fectly transparent and colourless. Its smell is peculiar, and resembles the nauseous odour developed by crushing some umbelliferous plants. When dissolved in alcohol, it gives with corrosive sublimate a white precipitate, soluble in hot alcohol, from which it is deposited in crystals precisely similar to those from which it had been originally separated, and with bichloride of platinum a yellow precipitate, slightly soluble in of the 'Fixed Oils in contact mth Sulphur, 1*71 hot alcohol and aether. This oil is in all probability the sulphuret of odmyle Cg Hg Sg j but the small quantity in which I have been able to obtain it, has prevented my performing any analysis of it. The Flaiinum Compound. — When a solution of bichloride of platinum is added to the alcoholic solution of the crude oil, a yellow precipitate makes its appearance, which does not fall immediately, but goes on gradually increasing for some time, precisely as is the case with the allyle compound. The pro- perties of this precipitate are not however perfectly constant, but vary according to the portion of the oil employed to yield it. That obtained from the more volatile portion has a fine sulphur-yellow colour, but the less volatile oil gives an orange precipitate. It is insoluble in water, sparingly soluble in alcohol and aether. When heated it becomes black, an oil is evolved smelling exactly like that obtained from the mercury compound, and sulphuret of platinum is left behind, which requires a high temperature to drive off all its sulphur, and leaves metallic platinum as a silver-white mass. When treated with hydrosulphuret of ammonia, it is converted into a brown powder, exactly like that obtained under similar circumstances from allyle. The analysis of the yellow compound has not hitherto given results of a satisfactory character. I have found the amount of platinum to oscillate between 43'06 and 49*66 per cent. The former of thes'e was obtained from the most volatile oil, the latter from that which boiled between 300° and 400° F., and intermediate results were obtained at intermediate tem- peratures. T!ie results obtained from the oil which boiled at a high temperature were remarkably constant; thus I have found, in different experiments, 49*00, 49*51, and 49*66 per cent, of platinum, which appear to indicate the presence of some compound of rather sparing volatility. The precipitate obtained from the most volatile oil appears to be that corre- sponding to the mercury compound which has just been de- scribed. Of it I have been able only to perform a very incom- plete analysis, which is insufficient to establish its constitution, especially as it is impossible to ascertain whether it is a homo- geneous substnnce. As the results, however, approximate to a formula analogous to that of the mercury compound, I give the details, such as they are. ["9*155 grains of the platinum compound gave ■< 7*474 ... carbonic acid, and 1^3*294 ... water. 5*701 grains gave 2*455 grains of platinum = 43*06 per cent. t72 On certain Products of Decomposition of the Fixed Oils. These results approximate to a formula similar to that of the mercury compound ; viz. — (C8H8S2+PtCg + (C8H8S, + PtS). Experiment. . 22-26 Ci 20-83 alculation. Carbon Cjg 1200-0 Hydrogen 3-99 3-47 Hie 200-0 Platinum . . 43-06 42-84 Pt2 2466-6 Chlorine . . ••• 15-38 CIg 885-3 Sulphur . . 17-48 Ss 1005-8 100-00 5757*7 The analogy which those substances bear to allyle is exceed- ingly interesting, as showing the possibility of forming, by artificial processes, substances similar in constitution to so remarkable a compound, which is not a product of decompo- sition, but exists ready-formed in a variety of different vege- tables, where it must obviously be produced under circum- stances very different from the artificial substance ; for allyle cannot exist at all at a high temperature, and is entirely de- composed at, or even below, its point of ebullition. Unfor- tunately, however, the examination of this substance is much complicated by the necessity of examining its compounds in place of itself. Had it been possible to separate it directly from the crude oil, the determination of its constitution and that of its compounds would have presented comparatively little difficulty, and been arrived at with much less labour than that expended upon the imperfect details I have been able to accumulate. Another point worthy of observation, is the total alteration of the products of decomposition of oleic acid pro- duced by the presence of sulphur ; no sebacic acid, and, in fact, none of its ordinary products being evolved, although all the substances produced contain carbon and hydrogen in the proportion of equal atoms, just as they exist among the ordi- nary products, — a circumstance which, taking into considera- tion the abundant evolution of sulphuretted hydrogen, we certainly should not have anticipated. The oil which remains after the separation of the mercury compound, likewise contains sulphur as one of its constituents ; but I have not yet had time to commence the investigation of this part of the subject. The discussion of it, as well as va- rious other points connected with the compounds already de- scribed, I hope to make the subject of a future communica- tion. [ 173 ] XXX. On the Mechanical Equivalent of Heat^ as determined by the Heat evolved by the Friction of Fluids. By J. P. Joule, Secretary to the Literary and Philosophical Society of Manchester *, IN the Philosophical Magazine for September 1845 I gave a concise account of some experiments brought before the Cambridge Meeting of the British Association, by which I had proved that heat was generated by the friction of water produced by the motion of a horizontal paddle-wheel. These experiments, though abundantly sufficient to establish the equivalency of heat to mechanical power, were not adapted to determine the equivalent with very great numerical accuracy, owing to the apparatus having been situated in the open air, and having been in consequence liable to great cooling or heating effects from the atmosphere. I have now repeated the experiments under more favourable circumstances, and with a more exact apparatus, and have moreover employed sperm oil as well as water with equal success. The brass paddle-wheel employed had, as described in my former paper, a brass framework attached, which presented sufficient resistance to the liquid to prevent the latter being whirled round. In this way the resistance presented by the liquid to the paddle was rendered very considerable, although no splashing was occasioned. The can employed was of cop- per, surrounded by a very thin casing of tin. It was covered with a tin lid, having a capacious hole in its centre for the axle of the paddle, and another for the insertion of a delicate ther- mometer. Motion was communicated to the paddle by means of a drum fitting to the axle, upon which a quantity of twine had been wound, so as by the intervention of delicate pulleys to raise two weights, each of 29 lbs., to the height of about 5^ feet. When the weights in moving the paddle had descended through that space, the drum was removed, the weights wound up again, and the operation repeated. After this had been done twenty times, the increase of the temperature of liquid was ascertained. In the second column of the following table the whole distance through which the weights descended during the several experiments is given in inches. I may observe also that both the experiments on the friction of water, and the interpolations made in order to ascertain the effect of the surrounding atmosphere, were conducted under similar circumstances, each occupying forty minutes. * Read before the Mathematical and Physical Section of the British Association at Oxford, and communicated by the Author. 174- Mr. J. P. Joule on the Mecha?iical Equivalent of Heat. Table I.— Friction of Distilled Water. Nature of experiment. Total descent of each weight of 29 lbs. in inches. Mean tem- perature of the room. Difference. Tempcrature of the water. Gain or loss of heat. Before ex- periment. After ex- periment. Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation 1268-5 0 1266-1 0 1265-8 0 1265-4 0 1265-1 0 1265-3 0 1265-2 e 1262-4 0 1262-3 0 60°839 61-282 61-007 61-170 57-921 58-119 58-152 58-210 57-860 58-162 57-163 57-602 57-703 58-091 56-256 56-888 57041 67-612 0-040- 0120- 0-408+ 0-570+ 0-809- 0-628- 0-293- 0-003+ 0-215+ 0'25G+ 0-220+ 0-121 + 0-359+ 0-304+ 0-015- 0-285 - 0-078- 0-285- 60'-452 61-145 61-083 61-752 56-752 57-472 57-51 1 58-207 57-735 58-416 57-050 57-716 57-731 58-393 55-901 56-590 56-617 57-310 6f-145 61180 61-748 61-729 57-472 57-511 58-207 58-219 58-416 58-420 57-716 57-731 58-393 58-397 56-582 56-617 57-310 57-344 0-693 gain, 0-035 gain. 0-665 gain. 0-023 loss. 0-720 gain. 0-039 gain. 0-696 gain, 0012 gain. 0 681 gain. 0-004 gain. 0-666 gain, 001 5 gain, 0-662 gain. 0-004 gain, 0-681 gain. 0027 gain. 0-693 gain. 0-034 gain. Mean friction experiments j 1265-13 0-0037- 0-6841 gain. Mean of the interpolations } » 0-0071- 00163 gain. Corrected re- 1 1265-13 0-6680 gain. We see then that the weights of 29 lbs., in descending through the altitude of 1265'13 inches, generated 0°-668 in the apparatus. But in order to reduce these quantities, it became necessary in the first place to ascertain the friction of the pul- leys and that of the twine in unwinding from the drum. This was effected by causing the twine to go once round a roller of the same diameter as the drum, working upon very fine pivots, the two extremities of the twine being thrown over the pul- leys. Tlien it was found that, by adding a weight of 3150 grain.s to either of the two weights, the friction was just over- come. The actual force employed in the experiments would therefore be 40G000 grs. —3150 grs. = 402850 grs. through 1265*13 inches, or 6067*3 lbs. through a foot. The weight of water being 77617 grs., that of the brass paddle-wheel 24800 grs., the copper of the can 11237 grs., Mr. J. P. Joule on the Mechanical Equivalent of Heat. 175 and the tin casing and cover 19396 grs., the whole capacity of the vessel and its contents was estimated at 77617 + 2319 + 1056-4-363 = 81355 grs. of water. Therefore the quantity of heat evolved in the experiments, referred to a pound of water, was 7°-7636. The equivalent of a degree of heat in a pound of water was therefore found to be 781-5 lbs. raised to the height of one foot. I now made a series of experiments in which sperm oil was substituted for the water in the can. This liquid, being that employed by engineers as the best for diminishing the friction of their machinery, appeared to me well-calculated to afford another and even more decisive proof of the principles con- tended for. Table II. — Friction of Sperm Oil. Nature of experiment. Total descent of each weight of 29 lbs. in inches. Mean tem- perature of the room. Difference. Temperature of the oil. Gain or loss of heat. Before ex- periment. After ex- periment. Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation Friction Interpolation 1263-8 0 1269-0 0 1268-7 0 1268-5 0 1268-1 0 1268-3 0 1268-7 0 1267-6 0 12680 0 56-677 57-316 56198 56-661 57-958 57-051 58-543 57-153 59097 57-768 56-987 57-156 57-574 57-336 58-537 59-641 59-131 60-164 0-453 + 0-595 + 1-024+ 1-221 + 0-588+ 0-773+ 1-685- 1-504- 0-534- 1-927- 0-186- 0-413+ 0-734+ 0-237+ 0-829- 0-364+ 0-148+ 0-138- 56-354 57-906 56-516 57-929 57-813 57-836 55-951 55-568 57-766 55-731 56-029 57-573 57-581 57-565 56-884 60-026 58-532 59-984 57-906 57-917 57-929 57-836 59-280 57-813 57-766 55-731 59-361 55.951 57-573 57-565 59036 57-581 58-532 59-984 60026 60-069 1-552 gain. 0-011 gain. 1-413 gain. 0-093 loss. 1-467 gain. 0023 loss. 1-815 gain. 0-163 gain. 1-595 gain. 0-220 gain. 1-544 gain. 0 008 loss. 1-455 gain. 0-016 gain. 1-648 gain. 0-042 loss. 1-494 gain. 0-085 gain. Mean friction experiments 1 1267-85 0-034+ 1-5537 gain. Mean of the interpolations } " 0-004+ 0-0366 gain. Corrected re- sult j 1267-85 1-5138 gain. 176 Prof. Schoenbein on a tiew Test for Ozone. In this instance, the force employed, corrected as before for the friction of the pulleys, was equal to raise eOSO*^ lbs. to the height of one foot. In estimating the capacity for heat of the apparatus, it was necessary in this instance to obtain the specific heat of the sperm oil employed. For this purpose I employed the method of mixtures. 43750 grs. of water were heated in a copper vessel weighing 10403 grs. to 82°-697. I added to this 28597 grs. of oil at 55°" 593, and after stirring the two liquids together, found the temperature of the mixture to be 76°'583. Having applied to these data the requisite corrections for the cooling of the liquids during the experiment, and for the capa- city of the copper vessel, the specific heat of the sperm oil came out 0*45561. Another experiment of the same kind, but in which the water was poured into the heated oil, gave the spe- cific heat 0'46116. The mean specific heat was therefore 0-45838. The weight of oil employed was 70273 grains, and the paddle, can, &c. were the same as employed in the first series of experiments ; consequently the entire capacity in this in- stance will be equivalent to that of 35951 grs. of water. The heat evolved was therefore 7°'7747 when reduced to the ca- pacity of a pound of water. Hence the equivalent deduced from the friction of sperm oil was 782" 1, a result almost identical with that obtained from the friction of water. The mean of the two results is 781*8*, which is the equivalent I shall adopt until further and still more accurate experiments shall have been made. XXXI. Letter from Prof. Schcenbein to Prof. Faraday, F.E.S., on a neiso Test for Ozo7ief. My dear Faraday, HAVING a good opportunity for sending you a few lines, I will make use of it to tell you something about my little doings. You are no doubt struck with the peculiarity of the ink in which this letter is written, and I am afraid you will think it a very bad production ; but in spite of its queer colour, you will like it when I tell you what it is, and when I * This number is slightly different from 775, the equivalent stated at Oxford, and used by me as one of the data for calculations on the velocity of sound. The reason of the difference was that by an oversight 1 had taken the friction oiboth pulleys as the correction of each weight instead of both weights. The whole of the experiments are exactly the same as those presented to the Oxford meeting. The slight alteration in the equi- valent will make only a very trifling alteration in the theoretical velocity of sound given in the last Number of this Magazine. t Communicated by Professor Faraday. Dr. Wilson on the Decomposition of Water by Platinum. 177 assure you that as long as the art of writing has been practised no letter has ever been written with such an ink. Dealing now again in my ozone business, I found out the other day that all manganese salts, be they dissolved or solid, are decomposed by ozone, hydrate of peroxide of manganese being produced and the acid set at liberty. Now to come round again to my ink, 1 must tell you that these lines are written with a solution of sulphate of manganese. The writing being dry, the paper Is sus})encled within a large bottle, the air of which is strongly ozonized by means of phosphorus. After a few minutes the writing becomes visible, and the longer you leave it exposed to the action of ozone the darker it will become. Sulphurous acid gas uniting readily with the peroxide of manganese to form a colourless sulphate, the writing will instantly disappear when placed within air containing some of that acid ; and it is a matter of course that the writing will come out again when again exposed to ozonized air. Now all this is certainly mere playing; but the matter is interesting in a scientific point of view, inasmuch as dry strips of white filtering paper drenched with a weak solution of sulphate of manganese fur- nish us with rather a delicate and specific test for ozone, by means of which we may easily prove the identity of chemical, voltaic and electrical ozone, and establish with facility and certainty the continual presence of ozone in the open air. I have turned brown my test-paper within the electrical brush, the ozonized oxygen obtained from electrolysed water and the atmospheric air ozonized by phosphorus. The quantity of ozone produced by the electrical brush being so very small, it requires of course some time to turn the test-paper brown. As it is rather inconvenient to write with an invisible ink, I will stop here; not however before having asked your kind indulgence for the many blunders and faults which my ozone bottle will no doubt bring to light before long. Yours most truly, Bale, July 1, 1847. C. F. SCH(ENBEIN. XXXII. On the Decomposition of Water by Platinum and the Black Oxide of Iron at a white heat, with some observations on the theory of Mr. Grovels Experiments. By George Wilson, ilf.D.* THE remarkable discovery recently made public by Mr. Grove, that water in certain circumstances, when raised to a white heat, is resolved into its constituent gases, has na- ♦ Communicated by the Chemical Society; having been read March 15, 1847. Phil. Mag. S. 3. Vol. 31. No. 207. Sept. 1847. N 178 Dr. Wilson on the Decomposition of Water by Platinum turally excited much attention. It furnished the unexpected confirmation of the truth of an opinion expressed by James Watt so far back as 1783, that if steam could be made red hot [white hot] so that all its latent heat should be converted into sensible heat, either the steam would be converted into permanent air, or some other change would take place in its constitution *. In the greater number of Mr. Grove's experiments, water was raised in temperature through the medium of platinum ; and it became a question accordingly, as Sir John Herschel and my friend Dr. Lyon Playfair suggested, how far the de- composition of water observed was owing to the mere heat of the metal, how far to the peculiar surface-influence, or so- called catalytic force, which has been so long recognized as possessed by platinum and the other noble metals. jDr. Play- fair also referred to the fact, " that many bodies at high tem- peratures exhibited a great affinity for oxygen, which they did not possess at lower temperatures ; as, for instance, silver, gold, and even platinum itself, which metals absorb oxygen when intensely heated, and give it out again on cooling. If the experiments had been tried in tubes of quartz or silica, they would not have been open to the objection which the use of so peculiar a metal as platinum appeared to involve -f." There was indeed one form of Mr. Grove's experiment not liable to the exception urged against those where platinum was used. He found it quite possible to decompose steam by sending Leyden-jar discharges through it, and refers the de- composition solely to the heat evolved by the electric spark. The same view has been suggested as not improbable by Faraday, in relation to the decomposition of water in the liquid form by electric discharges J. With great diffidence, however, I would remark, that the spark decomposition of water cannot be regarded as an experimentum crucis. Al- though the electric spark cannot decompose steam electroly- tically, we may not at once infer that it cannot decompose it in another way. I have no wish to assert that it can, but it is possible that it may, and a crucial experiment should be unexceptionable. Again : the spark discharge of a Leyden jar exerts a great disruptive force, and acts topically with much violence. There is reason moreover to believe that mechanical agitation or disturbance of a chemical compound can in many cases cause the separation of its elements. It may seem an extravagant idea to suppose that oxygen may be torn or detached from hydrogen by the action of a dis- » Phil. Trans. 1783, p. 41G. t Athenagum for September 19th, 1840, p. 966. J Researches in Electricity, 3rd series, paragraph 337. and the Black Oaeide of Iron at a white heat. 179 ruptive force on the molecules of water, as if chemical affinity were but a kind of mechanical cohesion, which may be over- come by division. On the other hand, however, it must not be forgotten, that v/e are how acquainted with a large num- ber of fulminating compounds, which can be decomposed by friction, by a touch, or a stroke. These compounds are all fragile, and water is a very stable combination ; but fragility and stability are but terms of degree, in relation to stability of union : and if it shall appear that a feeble mechanical force can overcome a small intensity of affinity, it will be acknow- ledged as quite possible that a powerful mechanical agency may overcome a great one. We have no means perhaps of making an unexceptionable experiment as to the decomposing power of mechanical force ; for we cannot bring it into play without calling into action other agencies. If we touch, or rub, or strike a fulminate, for example, we cause the evolution of heat, and add its decomposing power to that of the mecha- nical impulse. It would be a mere petitio principii, however, to assume that the heat produced alone effects the decompo- sition observed. It seems to me, therefore, that the decom- position of steam by the electric spark furnishes a more complex problem for solution than the action of M'hite-hot platinum on the same compound does ; and that the experi- ments made with the metal are more likely to throw light on those tried with the spark, than to be explained by them. Whilst thinking over these difficulties, and the objections to Mr. Grove's conclusions suggested by Herschel and Play- fair, I had occasion to perform the familiar class-experiment of burning iron wire in oxygen. I observed with an interest I had not felt previously, although I had carelessly noticed the phenomenon before, that bubbles of apparently perma- nent gas rose from the globules of white-hot oxide of iron as they fell into the water. It seemed to me possible that this gas might be a mixture of oxygen and hydrogen separated by the influence of the metallic oxide, acting as platinum did in Mr. Grove's experiments. It was certain, moreover, that if this should prove to be the case, it would supply a powerful argument in favour of that gentleman's conclusion, which seems, in spite of all the objections noticed, in the highest degree probable, namely, that heat, apart altogether from the medium through which it is applied, can resolve water into its elements. As the following experiments were made solely in the hope of substantiating Mr. Grove's view, which unfortunately, how- ever, they leave exactly as they found it, I trust that gentle- man will not consider their publication an interference with his researches. I was led to try them incidentally, and N2 * 180 Dr. Wilson on the Decomposition of Water by Platinum abandoned them as soon as I found I could render Mr. Grove no assistance by means of them. It would be difficult to conceive a more rapid and effectual way of raising a body to a white heat than that afforded by the combustion of iron in oxygen. I took for granted also (as it afterwards appeared, too hastily) that the metal could not but be saturated with oxygen and converted into a de- finite oxide, which would be chemically ijidifferent to each of the elements of water, and if it decomposed it at all, would reject both its constituents. The convenient way, moreover, in which the globules of oxide detach themselves and fall into the water, and the rapidity with which the whole process goes on, make it a very easy matter to collect in considerable quantity whatever gases are evolved. A stoppered bottomless jar of the ordinary construction for the iron-wire experiment, and of 291 cubic inches' capacity, was made use of in the fol- lowing trials. Eighteen experiments were made with it, and from 100 to 110 grains of fused globules were obtained from each combustion. A test-tube, with a funnel fixed into it by a perforated cork, and filled with water, was arranged so as to receive the gas. In some experiments it was placed within the oxygen jar, so that the coil of wire when introduced hung close to it, a piece of tin plate being arranged so as to guide the globules within the edge of the inverted funnel. In the greater number of trials however the tube and funnel were placed outside of the vessel containing the oxygen, and an inclined plane of tin plate was so placed as to carry the globules past tlie edge of the jar, and within the mouth of the funnel. No difference of result was observed in experi- ments made in both ways, but the latter arrangement was preferred as more convenient, and as enabling more oxygen to be employed at each trial. In all the experiments, permanent gas was evolved when the fused globules fell into the water. This statement is to be considered as applying to each combustion considered as a whole ; for individual globules were frequently observed to give off no gas at all, or to evolve so very little, that it might be air separating from the water, in which it had previously existed in solution. The quantity of gas obtained at each combustion varied greatly. Sometimes as much as a cubic inch was procured, more frequently only half that quantity, and occasionally less. The globules from thick coils of wire gave off a larger volume of gas than those from thin ones. Portions of the gas were transferred to a Grove's eudio- meter over water, and exposed to a white-hot platinum wire. They did not kindle or detonate, nor were they sensibly diminished in volume. Other portions were subjected to and the Black Oxide of Iron at a white heat. 181 electric sparks and discharges in a syphon eudiometer over water, with the same negative results ; but when air or oxy- gen was mingled with the gas, it exploded sharply with heated platinum or the electric spark. When a match was ap- plied to the open end of a tube containing the unmingled gas, it burned rapidly with a pale blue flame, but did not explode. The gas given off during the action of the fused globules on water was not then a mixture of oxygen and hydrogen. Its freedom from all but a trace of oxygen Avas ascertained in other ways. To. one portion of the gas standing over water nitric oxide was added, but no ruddy fume or yellow colora- tion showed itself. When phosphorus was introduced into the gas, in one instance it did not smoke, but in the greater number of cases it fumed for a brief period, and occasioned an amount of contraction barely perceptible. The gas ap- peared to be nearly pure hydrogen. To ascertain if it cer- tainly were so, a portion of it was carefully dried, by chloride of calcium, and transferred to a eudiometer over warm mer- cury. Dry oxygen was then added, and the mixtiu'e exploded. When the whole had cooled, the walls of the eudiometer ap- peared dimmed by a very thin layer of moisture, but the quantity of gas operated on was too small to admit of visible drops being produced. Another portion of the gas was mixed with half its volume of oxygen and fired by the electric spark. The contraction which followed explosion varied in different ex- periments, but was frequently such as to leave not more than one-twentieth part of the mixed gases unconsumed. Phos- phorus smoked in this residue for a short time, showing that excess of oxygen had been made use of, and left a minute volume of gas which was not diminished by caustic potash, and must have been nitrogen. It seemed possible that the trace of carbon present even in malleable iron might affect the quality of the gas resulting from the action of the globules of oxide on water, and that carburetted hydrogen, carbonic oxide or carbonic acid might be produced. It seemed desirable to know whether the latter were present or not, as the oxygen might have gone to form them. It was impossible to be certain that carbonic acid was absent, for the gas from the globules being necessarily collected over water, the temperature of which was low, car- bonic acid would be retained in solution by that liquid. All that I can say on this point is, that lime-Avater was not ren- dered muddy or in the slightest degree opalescent by the gas. It was several times detonated with oxygen over lime- water, but the latter remained quite transparent, so that nei- ther carbonic oxide nor carburetted hydrogen can have been present. In short, the gas evolved from water by the white- 182 Dr. Wilson on the Decomposition of Water by Platinum hot globules of oxide of iron, was hydrogen mingled with a small quantity of air, previously no doubt in solution in water. As only the hydrogen, then, of the water decomposed was obtained, it became necessary to account for the absence of the oxygen. I was tempted for a moment to think it pos- sible that the black oxide of iron might have changed into the red oxide of the same metal, by combining with the oxygen not obtained in the elastic form : ex. gr. thus 2 Fcg 04 + 0 = 3Fe2 O3. But the proto-peroxide of iron is known to be a very stable compound, little if at all prone to become the peroxide ; and it seemed more likely that unoxidized iron might be present in the fused globules, which occasioned the evolution of hy- drogen when it came in contact with water. To ascertain this point, portions of the globules were dissolved in dilute muriatic and sulphuric acids, and were found in most cases to evolve hy- drogen. Some specimens of the globules gave off not a trace of gas when they dissolved, and must have consisted of the definite oxide ; a point of interest in connection with the fact already mentioned, that globules were frequently ob- served to drop into water without any bubbles of gas rising from them. The volume of hydrogen however given off in some of the trials, when the product of combustion was placed in acid, was very considerable. A graduated gas jar was filled with dilute sulphuric acid, and inverted over a small capsule con- taining 100 grains of the crushed globules, which was placed in a basin also containing dilute acid. By this arrangement the gas was collected and measured at the same time, Mithout risk of mixing with air, or necessity for watching the process, which is a slow one. 100 grains treated in this way gave off 16 cubic inches of hydrogen, corresponding to 9 grains of iron. The experiment was accidentally stopped at this point whilst the gas Mas still rising in undiminished quantity. Metallic iron, then, was certainly present in many of the globules, and of this I had direct ocular demonstration. On crushing some of them in a mortar, they were found to sepa- rate into a shell of pulverizable oxide, and a core of iron which formed a nearly spherical pellet. In one case 50 grains of the globules were crushed, the pellets separated, and the residue placed in diluted sulphuric acid. It did not evolve a trace of hydrogen in the course of twenty-four hours. The pellets were then added to the same acid, and gave off 12 cubic inches of gas = 13*6 per cent, of iron in the globules*. The shell of oxide is frequently imperfect or perforated, so • In none of the experiments was the thermometer or barometer spe- cially observed, as minute accuracy was not aimed at. and the Black Oxide of Iron at a white heat, 183 that water or any other liquid penetrates to the iron core, and is subject to its influence. When this becomes known, it need not surprise us that most of the globules should rapidly decompose water. After observing this fact, I tried the effect of thin and thick coils of wire, and found that the latter invariably gave off the greater volume of gas. When the coil is so thin that the metal all oxidizes, no gas is evolved at all. A thick coil indeed furnishes a striking mode of illustrating to a class the principle of Lavoisier's mode of decomposing water, and forms a beautiful addition to the iron-wire expe- riment. From these observations then, it would seem that white- hot oxide of iron cannot decompose water in the way white- hot platinum does. But before any conclusion can be drawn from this fact inimical to Mr. Grove's views, or favourable to the opinion that a specific property of the platinum has more to do with the decomposition of water than its mere tempera- ture has, we should require to know how far the two white- hot bodies are to be considered as at the same temperature. In Mr. Grove's experiments, platinum is raised to as high a heat as it can bear without fusing. It must then be elevated to a temperature much above that necessary to make iron white-hot, or to fuse its oxide, for our forges can melt iron and its oxides, but do not fuse platinum. It may also be re- marked, that bright as the light emitted by burning iron is, it falls short in intensity of that given off by platinum on the verge of fusion. It seems accordingly probable, that during the combustion of iron in oxygen the temperature never rises high enough to confer upon the resulting oxide the power of decomposing water. The question admits of direct decision, by ascertaining whether oxide of iron, heated by the oxy- hydrogen blowpipe to as high a temperature as fusing pla- tinum, acquires the power of decomposing water without ap- propriating to itself either of its elements. But it would have been an interference with Mr. Grove's own researches to have made experiments of this kind, and I have accordingly left the question undecided. Meanwhile the experiments I have recorded are of some little interest, as at least showing that not only a white heat, but a high white heat, is essential to the successful perform- ance of Mr. Grove's experiments. Unfortunately, we have not at present any method of measuring high temperatures which admits of ready application or secures great accuracy. " W^hite heat " is in fact a vague expression for a range of temperature, of the extremes in either direction or extent of which we have no very precise knowledge. The power of the eye to measure the relative intensities of the light evolved 184) Dr. Wilson ow the Decomposition of Water by Platinum. by white-hot bodies is very limited, and varies greatly in different individuals. But the experiments 1 have recorded seem to supply the means of so far at least defining the white heat requisite for the separation of the elements of water, inasmuch as they show that it must at least exceed the tem- perature necessary for the fusion of malleable iron or its black oxide. If, moreover, the decomposing powers of the electric spark be solely referable to its temperature, we seem entitled to conclude, from the experiments I have detailed, that the heat of the smallest spark that can decompose water is at least equivalent to that of fusing platinum. They appear also to Avarrant another conclusion. It was suggested by Dr. Leeson and by Mr. Hunt, that the bursting of steam-boilers might occasionally be owing to the metal they consist of be- coming white-hot and decomposing water like platinum, with the rejection of both its elements*. This ingenious sugges- tion seemed to myself, before making experiments with iron, likely to prove just; but as fusing white-hot iron appears •unable to decompose water, otherwise than by combining with its oxygen, it is impossible that the walls of a boiler can ever be raised to a temperature sufficiently high to enable them to separate the elements of water in the way platinum does. I may now be permitted to make some comments on the rationale of the results obtained by Mr. Grove. That gentle- man, if I understand him aright, considers the decomposition of water by white-hot platinum not only, as assuredly it is, a remarkable and unexpected result, but as evidencing on the part of heat a power to produce opposite or dissimilar chemi- cal effects in the same circumstances. He is reported in the Atheneeum (Sept. 19th, 1846, p. 966) to have "announced his discovery that all the processes by which water may be formed are capable of decomposing water" (p. 966). If by this statement be simply meant, that heat combines oxygen and hydrogen into water, and decomposes water into these gases, it will be admitted to be a just conclusion ; but it may be questioned, I think, whether Mr. Grove's experiments add anything to our knowledge of the power of heat to effect chemical changes, except in so far as they supply an addi- tional very remarkable example of its twofold analytical and synthetical agency, which has been so long recognised. Hy- drogen, which as a gas is probably the vapour of a very vola- tile metal, may be compared with mercury, also a volatile substance. If mercury and oxygen be heated together to the temperature of 662° F., they combine and form the red oxide of the metal. If this resulting oxide be raised to a low red heat, * Athenaeum, Sept. 19th, p. 9Q6. and the Black Oxide of Iron at a white heat. 185 it is decomposed into mercury and oxygen. In like manner, if hydrogen and oxygen be raised together to the tempera- ture of 660° F.*, they unite and form water. If the resulting Mater be raised to a white heat, it is resolved into hydrogen and oxygen. Both metals (?) present the same phaenomena. At one temperature (nearly the same in both cases) combina- tion with oxygen occurs ; at a higher temperature, decompo- sition of the oxide happens. Many other examples might be given in illustration of the same fact. Such cases, however, do not seem to warrant a conclusion as to heat exhibiting anything like a polarity of force, by which I understand the manifestation in opposite directions of opposite powers of equal intensity. At all events, if the opposite effects of dif- ferent intensities of the same agent be considered equivalent to a polarity of action, it is difficult to see what force may not be called a polar one. The decomposing and combining power of heat of different intensities, seems exactly compara- ble to the opposite effects of different intensities of mechanical impulse. If two pieces of smooth glass are laid together and struck gently or compressed slightly, they unite or cohere. If the united pieces are thereafter exposed to a sharp blow or to great compression, the union is dissolved, or they are shat- tered to fragments. Here the same force effects mechanical synthesis and mechanical analysis. But in these contrasted actions, as seems to be the case also in Mr. Grove's experi- ments, the results are occasioned by a difference in degree of intensity of the same power, not as in the opposite effects of a polarizing force like electricity, by a difference in the kind of power which appears, whatever be its intensity. There is one form, indeed, of Mr. Grove's experiment which at first sight does not appear to admit of the explanation proposed in reference to the other trials — I allude to the decomposition of steam by the electric spark, which is well known to have the poM^er of combining hydrogen and oxygen into water. A similar experiment w^as made in perhaps a still more in- structive form in the latter part of last century by Beccariaf, Pearson and Van Troostwyk, and more recently by WoUas- ton J, in his well-known decompositions of water with guarded poles. In certain of these trials it was found that Leyden jar discharges sent through water, decomposed it till the ac- cumulation of permanent gas left the wires bare ; after which the first spark that passed recombined the gases into water, which again covered the wire, when decomposition could * Graham's Elements, 1st edit. p. 259. t Lettere dell' Electrecismo, quoted in Lardner's Electricity, vol. i.p. 78. j Faraday's Electrical Researches, series 3, paragraph 328. 186 Dr. Wilson on the Decomposition of Water by Platinum anew be obtained. Here, to appearance, the same agent act- ing with the same intensity, alternately decomposed and re- composed water. For argument's sake, let it be acknow- ledged that the heat alone of the spark was the cause of che- mical change. Nevertheless it may be questioned, whether it acted with equal intensity in both cases. The electric spark must be conceived, according to the results already given, to be at first at a high white heat, and whilst retaining this tem- perature we may believe it to possess a power of disuniting the elements of water, and of preventing their union. But as soon as the spark falls to the temperature of 660° F., it loses its power of decomposing water, and, on the other hand, ac- quires a power of uniting hydrogen and oxygen. Although therefore the spark is always furnished of the same intensity, its action may change, and even be reversed, as its intensity diminishes. Moreover, even when the spark is white-hot, it is only the amount of matter directly in its track that will be raised to a white heat. Contiguous portions will have their temperature much lower, so that in the case of hydrogen and oxygen, at some little distance from the route of the spark, the temperature will be 660° F., and there combination will begin, and ultimately extend through the whole mass of gas. In like manner, when a platinum wire is made white-hot in a mixture of hydrogen and oxygen, it causes their combination. Here we may suppose that union occurs as soon as the tem- perature of the metal I'ises to 660" F., and before it acquires a white heat. Or if we were to arrange matters so that the wire should be made white-hot in a vacuum and hydrogen and oxygen afterwards admitted to it, still union of the gases should happen ; for although the wire might prevent com- bination immediately around itself, at no great distance where the temperature was below 700° F. it would compel union. In all such experiments the combining effect of heat will be much more manifest than its decomposing power ; not that perhaps the former is in reality greater than the latter, but because flame is propagated through a mixture of hydrogen and oxygen by a series of combustions. The hot wire or the electric spark kindles only the portions of gas immediately adjacent to it, but the combustion of those sets fire to the molecules contiguous to them, and these in their turn to their neighbours, till all are made to burn. Thus the flame travels after the original cause of combustion has ceased to operate directly, and the momentary action of a small spark, or the transient heat of a red-hot capillary wire may suffice to fire an infinitely large mass of hydrogen and oxygen. There is no provision for a similar propagation of decomposition through water or steam when either is made white-hot j the and the Black Oxide of Iron at a white heat. 187 absolute amount accordingly of disunion of the elements of M'ater occasioned is very small. If allowance, however, be made for the apparent difference in extent of effect which heat shows in uniting and in dis- uniting the elements of water, the phaenomena otherwise seem referable solely to the intensity of the temperature to which hydrogen and oxygen are exposed. The opposite pro- cesses might go on simultaneously, union or disunion being determined simply by the different temperatures to which different portions of the gases were raised. At least it seems not improbable that if a mixture of steam and of hydrogen and oxygen were exposed to electric discharge, decomposition of the steam and combination of the hydrogen and oxygen might be effected by the same spark, provided the volume of steam were not large. In the track of the spark decompo- sition would occur, so long as a white heat prevailed. When the temperature fell, combination would happen where the spark had passed, if it had not already commenced in the neighbourhood of its direct route. Similar remarks apply mutatis mutandis to the action of a hot platinum wire on a mix- ture of steam with oxygen and hydrogen. It may be objected to this view, that Mr. Grove decora- poses steam in his eudiometer, and obtains a permanent bub- ble of gas, consisting of hydrogen and oxygen. The bubble however obtained in this way is very small, and could not probably be greatly increased. Mr. Grove has not mentioned how large a volume of hydrogen and oxygen he could obtain in the same eudiometer, by alternately boiling the water till the steam produced caused the liquid to fall below the wire, and allowing the steam to condense till the water rose above the metal. But I venture to say that no large volume of per- manent gas could be procured by this process if the same eudiometer were employed many times successively. The combining action of the wire might not take effect on the hydrogen and oxygen when their quantity was small, and they were diluted through a large volume of steam, for in virtue of the law of diffusion, the molecules of hydrogen and oxygen would be separated from each other by molecules of water-vapour; but when the latter diminished in bulk, it seems impossible to doubt that kindUng of the gases would occur. Mr. Grovels experiments then do not appear to prove that heat of the same intensity is able in the same circumstances to form water and to decompose it. When therefore it is stated that water can be produced by the processes that dis- unite its elements, the word ^process ^ can only be understood to signify that the general arrangement in both cases is the 188 Dr. Wilson on the Decomposition of Water by Platinum. same, not that the intensity of the agent called into play, or its mode of action is identical. If this could be affirmed, we should be able to announce as a general proposition, that manifestations of the same force absolutely identical as to quality, quantity and intensity, could produce totally oppo- site results, which would be tantamount to affirming that un- like effects may flow from the same cause, without any altera- tion in the qualities or conditions of the latter. The last observation I would make refers to the curious fact noticed by Mr. Grove, namely, that when a platinum wire is heated white-hot in steam, " in a few seconds a small bub- ble of gas is formed; but if the action be continued for a week, it does not increase in quantity *.^^ Are we to suppose that the wire is at the same time decom- posing water around itself, and producing water at a little distance, undoing in one place what it effects in another, so that no permanent accumulation of gas is allowed to take place ? This is possible, but I think not likely. The ob- servation made by Mr. Grove seems sufficiently explicable, on the supposition that as soon as the wire is completely en- veloped in steam, the thermo-circulatory currents which the high temperature occasions in the vapour prevent it from remaining long enough in contact with the wire to become heated white-hot. The steam probably circulates endlessly around the wire without a trace of decomposition occurring in it. It seems not unlikely indeed that in Mr. Grove's ex- periments with his eudiometer it was not steam that yielded the hydrogen and oxygen obtained, but the last film of water below the wire, which could not escape from the metal, but tended rather, in consequence of its expansion, to rise towards it, and was thus compelled to acquire a white heat, and to break up into its elements. If this view be correct, an ar- rangement where a white-hot wire or sheet of platinum foil was kept grazing the surface of water, might be found to effect a continuous decomposition of the liquid in question. It is no objection to this view that an electric spark decom- poses steam readily, for the duration of the spark is so short, that there is no time for the production of thermo-currents, nor any possibility of the steam escaping from the powerful topical action of the discharge. The spark may be compared to fulminating silver, whose action is instantaneous and vio- lent, but quite local, — the heated platinum to gunpowder, the effect of which is cumulative and more general. * Athenaeum, Sept. 19tli, 1846, p. 966. [ 189 ] XXXIII. An account of a Discovery in the Theory of Numbers relative to the Equation A.x^ + Bj/^ + Cs^ = Tixyz. By J. J. Sylvester, Esq-^ M.A., F.R.S.^ First General Theorem of Transformation. TF in the equation Kx^-\-^y^->tC^ = 'Dxyz . . (1.) A and B are equal, or in the ratio of two cube numbers to one another, and if 27 ABC — D^ (which I shall call the De- terminant) is free from all single or square prime positive factors of the form 6n+ 1, but without exclusion of C7ibic factors of such form, and if A and B are each odd, and C the double or quadruple of an odd number, or if A and B are each even and C odd, then, I say, the given equation may be made to depend upon another of the form A'm3 + Wv" + C'«)3 = B'xyz ; where A'B'C' = ABC D'=D u.v .iv =some factor of z. The following are some of the consequences which I deduce from the above theorem. In stating them it will be convenient to use the term Pure Factorial to designate any number into the composition of which no single or square prime positive factor of the form 6 n+1 enters. The equations x^ + 2^ + 22^=Dxys: a^ + y^ + 4!Z^ = T)xyz 2a^ + ly^ + z^ = Yixyz are insoluble in integer numbers, provided that the Determi- nant in each case is a Pure Factorial. The equation a^-\-y^-\- K^'rs.^Vtxyz is insoluble in integer numbers, provided that the Determinant, for which in this case we may substitute A — 27B^, is a pure factorial whenever A is of the form 9w+l, and equal to 2p3!±i Qp 4.p3i±i^ jp being any prime number whatever. I wish however to limit my assertion as to the insolubility of the equations above given. The theorem from which this conclusion is deduced does not preclude the possibility of two of the three quantities a?, ?/, z being taken positive or negative units^ either in the given equation itself or in one or the other of those into which it may admit of being transformed. Should such values of two of the variables afford a particular solution, then instead of affirming that the equations are insoluble, I should affirm that the general solution can be obtained by equations in finite differences f. * Communicated by the Author. t Take for instance the equation ifi-\-y^-\-^z^'=9xyz. The Determinant 1 90 Ofi a discovery in the Tlieory of Numbers. Second General Theorem of Transformation, The equation f^oi^-\-^y^-{-h^z^=^^xyz . . . (2.) may always be made to depend upon an equation of the form Aw^ -f Btfi + Cwr^ = Tiuim, where ABC=:R3-S3 D = 3R; and u.v.vo =. some factor o^fx-^gy + hz. R representing K + 6fgh S ... K-3/^A. I have not leisure to show the consequences of this theorem ef transformation in connexion with the one first given, but shall content myself with a single numerical example of its applications: x^-{-'y^-{-z^=—Qxyz may be made to depend on the equation and is therefore insoluble. It is moreover apparent that the Determinant of equation (2.) transformed is in general — 27R% and is therefore always a Pure Factorial, and consequently the equation f^a^ +g^y^ + h^i^ = ^xyz will be itself insoluble, being convertible into an insoluble form, provided that K + Gfgh is divisible by 9, and provided further that {K + Qfghf — {K — Sfghf belongs to the form m^.Q, where Q is of the form 9«+ 1, and also of one or the other of the two forms ^Ip^'^^^ 4;>^'*>, p being any prime number what- ever. Pressing avocations prevent me from entering into further developments or simplifications at this present time. It remains for me to state my reasons for putting forward these discoveries in so imperfect a shape. They occurred to me in the course of a rapid tour on the continent, and the results were communicated by me to my illustrious friend M. Sturm in Paris, who kindly undertook to make them known on my part to the Institute. Unfortunately, in the heat of invention I got confused about 27"25 is a Pure Factorial : consequently if the solution be possible, since in this case the transformed must be identical with the given equation, this latter must be capable of being satisfied by making x and y positive or ne- gative units. Upon trial we find that x=.\ i/=.\ z=2 will satisfy the equa- tion. I believe, but have not fully gone through the work of verification, that these are the only possible values (prime to one another) which will satisfy the equation. Should they not be so, my method will infallibly enable me to discover and to give the law for the formation of all the others. Here, then, under any circumstances, is an example, the first on record, of the complete resolution of a numerical equation of the third degree be- tween three variables. On a new Kite- Apparatus for Meteorological Observations. 191 the law of oddness and evenness, to which the coefficients of the given equation are in the first theorem generally (in order for the successful application of my method as far as it is yet developed) required to be subject. I stated this law erro- neously, and consequently drew erroneous conclusions from my Theorems of Transformation, which I am very anxious to seize the earliest opportunity of correcting. I venture to flatter myself that as opening out a new field in connexion with Fermat's renowned Last ' Theorem, and as breaking ground in the solution of equations of the thii'd degree, these results will be generally allowed to constitute an important and substantial accession to our knowledge of the Theory of Numbers. 26 Lincoln's Inn Fields, August 24, 1847. XXXIV. Experiment made at the Kew Observatory on a new Kite- Apparatus for Meteorological Observations^ or other purposes^, MR. W. R. BIRT (on the Uth of this month) took some kites, &c. to the Kew Observatory, for the purpose of endeavouring to ascertain how far it might be practicable to measure the force of wind at various elevations by their means, and (in the mere manipulation of his experiments) was assisted by Mr. Ronalds. After several trials, &c. they agreed that the sudden variations, horizontal and vertical, in the position of the kite, the great difficulty of making a kite which should present and preserve a tolerable approximation to a plane, that of measuring, with sufficient accuracy, at any required moment, its inclination, and lastly, the influence of the tail, would always tend to render the observation somewhat unsa- tisfactory. Mr. Ronalds then proposed to try the following method of retaining a kite in a quasi invariable given position. Three cords were attached to an excellent hexagonal kite of Mr. Dirt's construction : one in the usual manner, and one on each side (or wing). The kite was then raised as usual ; the two lateral cords were hauled downward by persons stand- ing at the apices of a large equilateral triangle (described upon the ground) until the ascending tendency became considerable (even when the force of the wind was at its minimum), and the three cords were made fast to stakes or held in the hand. He had entertained no expectation of the favourable result of this simple and obvious contrivance. 1 he place of the kite did not seem to vary so much as one foot in any direction, and it really appears to him probable that a very large kite or kites might be employed in this kind of manner often and very * Comraunicated by Mr. Ronalds. 1 92 Dr. Playfair on Transformations cheaply as a substitute for a captive balloon in meteorological inquiries, or even (on a very extensive scale) for other require- ments in military science, &c. An anemometer, a thermo- meter, an hygrometer, &c. of some registering kinds, &c., might be hauled up and lowered at pleasure (like a flag) by a person standing in the centre of the triangle (above referred to), and by means of a line passing through a little block attached to the kite. The cords and kite should of course be of pure silk, for»the sake of lightness, combined with extreme strength, and the size and thickness in some measure adapted to the breeze or lighter air. The silk might be advantageously covered with a very light coat of elastic varnish. XXXV. On Transformations produced by Catalytic Bodies. By Lyon Playfair, Esq,^ T> ERZELIUS rendered a most useful work to science, when ■^-^ he collected into one class those varied phaenoraena of chemical action resulting from causes certainly very different from the ordinary manifestations of those affinities, which produce combinations or promote decompositions. This phi- losopher believes the power f? which causes decomposition without the acting body participating in its result, to be a distinct electro-chemical agency different from other recog- nised powers, and he named it the " Catalytic force." Ac- cording to this view, catalytic bodies do not act by chemical affinity, but they excite inherent affinities in other substances, in consequence of which new combinations or decomposi- tions ensue. Mitscherlich J, adopting this view, considered a number of catalytic decompositions in detail, and showed the important influence exerted by the state of surface of bodies in favouring this peculiar action, which he denominates decomposition by contact. The examples, adduced in this interesting memoir, of the favourable action of an extended surface upon combi- nation, fully prove that the physical condition of bodies ex- ercises an important influence upon the action of this force ; but they do not remove the necessity for studying the force itself, as it may either be a vis occulta, entirely distinct from powers already recognised, as Berzelius supposes, or may be modified forms of those in continual operation. Liebig§ views the catalytic power as a dynamical action * Communicated by the Chemical Society ; having been read April 5, 1847. "t" Jahresbericht, xv. 237. X Taylor's Scientific Memoirs, Part xiii. ; or Fogg. Ann, xxxi. 281. § Liebi^'s Chem. of Agriculture, 4th edit., p. 284. produced by Catalytic Bodies. 193 on the atoms of a complex molecule, conceiving that the ac- tivity of the atoms of a body in a state of motion may be communicated to those of another body in a state of rest. The atoms of a compound, according to this view, if in a state of exact statical equilibrium, arrange themselves according to new affinities, when the vis inertice is overcome by motion. In proof of this view, Liebig carefully examines a large num- ber of decompositions, and accounts for some of the most difficult transformations in organic chemistry. But there are many instances, to which I shall have to draw attention in the present memoir, where catalytic de- compositions ensue when there is no intestine motion in the atoms of the exciting body ; and hence we cannot do more than consider motion as favourable to the development of dormant affinities, in a manner similar to the surface action described by Mitscherlich. The power of peroxide of hy- drogen and of pyruvic acid to reduce oxide of silver is cer- tainly a singular phaenomenon, and appears favourable to Liebig's views ; but the cause of the original decomposition of the peroxide of hydrogen cannot be ascribed to motion, as the atoms of the oxide of silver are not in that state, and those of the peroxide of hydrogen either not at all or only slightly so. Neither will it suffice to suppose that the escape of gas during such decompositions is due to the presentation of angular points from which the gas may escape *, because solutions of alkalies equally effect the decomposition, accord- ing to Thenard -f. The cause, therefore, which enables cer- tain substances to hasten the decomposition of such bodies as peroxide of hydrogen or persulphuret of hydrogen, al- though favoured by the state of surface and by motion, is in- dependent of mere physical condition. In further proof of the importance of motion in causing com- bination or decomposition, Liebig cites the favourable effects of agitation on the precipitation of potash by tartaric acid. It may be questioned, however, whether this is not either a me- chanical breaking up of a combination or the simple effect of cohesion. Thus when water is saturated with a gas, a brisk agitation with a rod causes the separation of bubbles of gas previously dissolved. The mechanical force may here be sup- posed to have broken up the compound molecule of water and gas by detaching the former, and thus enabling the gas to escape by its elasticity. In the precipitation of potash by tartaric acid, cohesion may effect the same result that elasti- city does in the case of gas, the agitation knocking off the • Ann. der Pharm., ii. 22. f Ann. de Chim. et de Phys., xlviii. 79. Phil. Mag. S. 3 . Vol. 3 1 . No. 207. Sept. 1 847. O 194 Dr. Play fair on Transformations atoms of water which are feebly attached. In fact we know that the addition of alcohol equally aids the precipitation, the action here being a chemical separation of the water, as in the other it is mechanical. The diminished solubility of the salt, after it has been influenced by cohesion and sepa- rated from water, has its counterpart in many similar in- stances ; for example, in the small solubility of anhydrous sulphate of iron. The effect of agitation on a solution of sulphate of soda, saturated while hot and allowed to cool, I ascribe to the same cause. The supposed effect of cohesion or elasticity in these cases is nothing more than that con- stantly observed in ordinary phagnomena, when the gravity of a substance is different from that of the medium in which it exists. The vesicles of water in the atmosphere may be so small that they float in it and produce fogs ; but when ag- gregated together by the motion of the air, they form drops, which precipitate to the ground with a rapidity proportionate to their size : the converse of this is also true. Thus, the particles or aggregated atoms of carbonic acid in water may be so very small, that, with the slight affinity of the latter added, they may be enabled, when in a state of rest, to re- main without resuming their elastic form; but agitation causes a larger system of aggregated atoms, and the gas now escapes in small bubbles. The first instance of cohesion applies in the precipitation of tartar. At the moment of formation the particles may be so widely apart, that, aided by their slight affinity for water, they remain without aggregating to any considerable extent. Brisk agitation, and the presentation of an extended surface, effect their aggregation and cause a speedy precipitation. It may be that these are really instances of combination favoured by motion ; but presuming that they are, the general argu- ment is not aflfected, that other decompositions perfectly ana- logous are produced where the exciting body is in a state of rest. The third theory of these decompositions is, that catalytic bodies act by exerting a feeble chemical affinity on one of the constituents of the body decomposed. This view was intro- duced by Mercer *, and supported by several very ingenious experiments communicated to the British Association at its meeting in Manchester. One of these was, that protoxide of manganese had the singular power of hastening the oxidation of starch in nitric acid f. The metallic protoxide, from its * Reports of British Association, vol. xi. 2d Part, p. 32. f The experiment is easily made by dissolving 1 ounce oxalic acid in J- a pint of water at 180° F., and adding to this 1 oz. colourless nitric acid of produced by Catalytic Bodies. 195 disposition to pass into the state of peroxide, aids the oxalic acid to decompose the nitric acid, the united affinities of both being able to accomplish what neither by itself could do. The protoxide remains unaffected at the end of the experi- ment, because, under the circumstances (the presence of acid), it cannot gratify its desire to become peroxide, and, therefore, it passes over its oxygen to the carbon, which escapes as carbonic acid. Mercer cited, as further examples, the action of protoxide of copper in eliminating oxygen from a solution of hypochlorite of lime, and of peroxide or binoxide of nitro- gen in commencing the oxidation of a mixture of protochlo- ride of tin and nitric acid. Mercer implied by these instances, that catalysis is an affinity of the catalytic agent for an ele- ment in the body acted upon, that affinity being feeble and incapable of gratification under the circumstances. It would be advantageous to science if we could arrange under a known power the cases of decomposition which ap- peared so mysterious as to induce the great Berzelius to ascribe them to the action of a new force. It may not be possible in the present state of our knowledge to comprehend the whole of the instances observed, but, if most are included in one category, we have a right to suppose that the others may be embraced as our knowledge progresses. I shall there- fore endeavour to show that many catalytic decompositions are merely cases of chemical affinity exerted under peculiar con- ditions. In no instance of chemical union does there seem to be such a complete gratification of affinity as to suppress the at- tractions of the elements. The inherent affinities still remain more or less powerful, for, if it were not so, the compound would be permanent under all circumstances and not liable to further change by the action of external agents. When manganese unites with 1 atom of oxygen, the affinity of the metal for oxygen is not wholly merged, but is still strong enough to attach to itself 1, 2 or 3 atoms more oxygen. When the oxide is one of the lowest of the series, this affinity exhibits itself in a basic power by attaching itself to any com- plex highly oxygenized molecule, such as the oxygen acids, or of radicals playing the part of oxygen. When, on the other hand, the manganese or other radical becomes highly oxygenized, we find it possessing acid properties, that is, the 1-30 sp. gr. No action ensues on this mixture, but it immediately com- mences on the addition of a protosalt of manganese, which for simplicity may be the oxalate or nitrate. The action is also strikingly shown by heat- ing a mixture of oxalic acid until tlie action commences, then diluting it till all action ceases. A little protosalt of manganese now added to the solution causes an immediate renewal of the oxidation. 02 196 Dr. Play fair on Transformations additional atoms of oxygen, being less firmly attached, are capable of gratifying the disposition of a less oxygenized atom (the base) to attach itself to a higher oxide, or, to use the convenient phraseology of Graham, the base becomes zincous to the acid, which is now chlorous. On heating the nitrates, nitric acid is not given off, but NO4 + O. The decomposition readily results from the dis- position of the base to appropriate more oxygen and pass into the higher oxides. If the base be oxide of nickel, the oxygen becomes attached to the oxide and remains ; if, how- ever, an oxide which has but a feeble affinity for oxygen at an elevated temperature, the elasticity of that element is able to overcome the affinity, which succeeded in break- ing up the nitric acid. The final action is so obviously de- pendent upon the oxygenous part of the acid, as to make Schonbein believe that salts contain peroxides ready-formed ; thus that NO5, IIO=N04 + H02, or PbO, N05 = N04-f PbOg. This however is an unnecessary supposition, the pre- vious view accounting sufficiently for the decomposition of a nitrate, so as to produce NO4 and O. Admitting this view to be correct in the expression that the preponderating quan- tity of a chlorous element in an acid renders the latter chlo- rous to a base, the mechanical attachment being to the chlo- rous element, we can understand why the number of atoms of oxygen in a base should regulate the number of atoms of acid attached to it. Thus RO presents only one chlorous element of attachment to the acid, and therefore the latter adheres to it in one proportion ; whereas Rg O3, which pos- • sesses three atoms of a chlorous element equally distributed round a zincous nucleus, presents three points of attach- ment, and therefore produces a salt Rg O3, 3A. This view in result gives all the simplicity of the acid radical theory, both views entertaining the idea that the oxygenous atoms of the base and acid are attached to each other. We have cer- tain instances, as for example KO, CIO5 ; PbO, NO5, where the elastic atoms of oxygen combine as closely together as non-elastic atoms, such as lead or silver. Although to aid conception we may suppose the atoms of oxygen of the base and of the acid to be in mechanical con- nexion, the true arrangement is probably not so, seeing that in a base there is always a part more zincous than the oxy- genous atom, although the base as unity is zincous to the acid. We see many instances in chemistry of union of atoms in pairs, or what may be called dual affinity. This Graham* * Trans. Royal Soc. Edin. vol. xiii. ; Phil. Trans. 1837, p. 47 etseq,-, Phil. Mag. Third Series, vol. xxiv. p. 401 et seq. produced by Cdtalytic Bodies. 197 has proved to be the case with regard to atoms of water, and we know of numberless instances in the case of oxides. Thus RO uniting with oxygen forms ROg. In this case RO + O corresponds to RO + A, the acid here representing the chlo- rous element from its oxygenous character. It is not neces- sary to suppose that A and O are associated in one continu- ous line, the probability being that the molecule may really be represented by ARO. Thus also in Rg O3, where the O3 are probably grouped equally round Rg, there is room for three more of a chlorous element to gratify the dual affinity, and the general formula Rg Og, 3A is the result, the 3A here representing three of a simple chlorous element. The result, as regards affinity;, will still however be the same, the whole '. depending upon the attraction of the central nucleus R. It ig therefore only for simplicity of expression in studying the phaenomena of catalysis, that I view the atoms of oxygen of an acid as associated in mechanical continuation with the atoms of oxygen of the base, the ejf'ect being represented by this expression : the whole views of molecular or atomic con- stitution of bodies are in my opinion only convenient fictions to enable us to study the forces themselves, and the concep- tion of a mechanical arrangement I only adopt as expressive of the manifestations of powers residing in matter. To show that the tendency of bases to N O5, even without being combined, is to attach themselves to the oxygenous part of the acid, a curious phaenomenon observed by Mercer may be cited. A portion of alumina may be taken and placed at the bot- tom of a vessel containing warm NO5 ; no action ensues, ex- cept partial solution ; a slip of calico coloured in indigo-blue may now be introduced into the mixture, and remains unaf- fected in the clear acid, but is immediately discharged when pressed with a glass rod into the alumina. Here the alumina acts by placing the oxygen of the nitric acid in a state of ten- sion without however succeeding in decomposing it, but the moment an assistant affinity comes into play, that state is shown by the decomposition of the nitric acid and oxidation of the indigo. The alumina in the presence of the acid could not oxidize (in fact, we know of no higher oxide), and there- fore the indigo appropriates the oxygen. I find that various other oxides, such as calcined Crg O3 and SnOg, have the same power, the latter showing this disposition more strongly than any of the other oxides. The best mode of trying these ex- periments is to heat a certain quantity of nitric acid, and then dilute it till indigo cloth ceases to be bleached. The oxide of tin is now added and allowed to fall to the bottom. On in- 198 Dr. Playfair on Transformations troducing a slip of indigo-blue calico, the portion in the clear acid will be found to remain unaffected, while that in contact with the insoluble oxide will be bleached in a few seconds. That this decoloration of the indigo is due to the assistant affinity of another body acting in the same direction, i. e. also having a disposition to unite with oxygen, may perhaps best be shown by the following experiment : — Warm nitric acid is diluted to such extent that it just ceases to discharge indigo- blue calico ; it is then divided into two portions, with slips of coloured calico in each, and through one of these binoxide of nitrogen is passed. In the latter the indigo becomes quickly bleached, while it remains unaffected in the former, the action obviously being due to the accessory affinity of the nitric oxide for more oxygen. In the same w'ay indigo-blue is discharged during the decomposition of a nitrate by heat, other kinds of organic matter being oxidized under like cir- cumstances ; in these instances the decomposition of the ni- tric acid is much facilitated, — 1. by the affinity of the base for oxygen ; 2. the affinity of the organic matter for oxygen, which unites with it at the elevated temperature. There are many similar instances of this kind, where the behaviour of NO2 or NO4 as an assistant is too clearly contrasted with the action of other bodies to permit mistake. Thus urine when kept is unfit for the preparation of urea, that substance ha- ving been converted into carbonate of ammonia during the action of the air upon the mucus or colouring matter con- tained in the fluid. Colourless nitric acid unites wdth urea and may be heated with it without decomposition ; but nitric acid containing any of the lower oxides of nitrogen, such as NOg or NO4, immediately decomposes urea into carbonic acid and ammonia*. We cannot conceive that a lower oxide can more readily oxidize urea than a higher oxide, and hence we can only view the NO4 as aiding the urea to oxidize itself, as the mucus does in urine. In the same way, the action of pure nitric acid on colourless uric acid is to form alloxan, if the operation has been conducted so as to prevent the forma- tion of nitrous acid (NO4) during the oxidation. But if NO4 has been evolved, or if the colouring matter of the urine be still contained in the uric acid, the products are only carbo- nate and oxalate of ammonia. The colouring matter of the urine and NO4 are thus seen to possess a similar action, which is exactly the same as that of protonitrate of manga- nese on a mixture of starch and nitric acid, no oxalic acid being formed in the presence of this salt, the only product of * A solution of urea in nitric acid is immediately decomposed with lively effervescence when a little NOj is passed through it. produced by Catalytic Bodies. 199 oxidation being carbonic acid. The NO4 or NOg acts in these cases clearly by aiding the compound ready to oxygenate, but which, under the conditions, has not sufficient power to de- compose the nitric acid without additional aid. The same ex- planation probably applies to the singular discovery of Pro- fessor Graham*, that the addition of NO4 to non-accendible phosphuretted hydrogen renders it inflammable. In this case the two combined affinities produce the union of oxygen with one of the bodies. The presence of the small quantity of another compound of phosphuretted hydrogen in the spon- taneously accendible gas, as described by Leverrierf and by ThenardJ, may probably act in the same manner. The action of this compound (PHc2) corresponding to ami- dogen (NH2) may be conceived so to disturb the attraction of the phosphorus to the hydrogen in the gas PH3 as to produce the inflammability. Both the elements of this gas are highly combustible, uniting with oxygen at a low temperature. Their mutual attractions are sufficiently strong to prevent the oxygen breaking up this union ; but when the second body is present, the desire of PHg for another atom of hydrogen may be supposed so far to draw the third atom of hydrogen from the PHg, that oxygen has now the power to unite with the two inflammable elements. In disturbing the existing equilibrium, it is presumed to act just as a spark would do by elevating the already strong affinities of the two elements for oxygen. When a solution of hypochlorite of lime is poured into a solution of muriate of ammonia in excess, a very pun- gent volatile compound results, which has no bleaching pro- perties, and therefore does not contain hypochlorous acid. The decomposition is expressed by the equation NH4 CI + CaO, CIO = NH2 CI + 2HO + Ca CI. The volatile com- pound NHg CI has an affinity for hydrogen in order to pass into NH4 CI. This body was well-fitted to test the view of the cause of the inflammability of phosphuretted hydrogen (even supposing PH2 is not spontaneously inflammable, as it is stated to be by Thenard), On placing gas (which had en- tirely lost its inflammability by standing several days over water), in contact with the above mixture, in about an hour it acquired the property of smoking strongly in the air, although it did not inflame spontaneously. This showed that the affinity of PH3 for oxygen was much elevated, although the attraction was not sufficient for inflammation. * Trans, Royal Soc. Edin. vol. xiii. p. 5. t Ann. de Ch. et de Phys. Ix, 174. X Comptes Rendus des Seances de VAcademie des Sciences, t. xviii. pp. 252, Ol-l ; t. xix. p. 313. 200 Dr. Playfair on Transformations There cannot be any doubt that the atoms of a body may be placed in a greater or less degree of tension by varying conditions. The experiments of Mr. Joule* and myself on AUotropism have fully proved that the space occupied by the same body alters under different circumstances. It is there- fore not an unreasonable assumption that the affinity of one body for a particular element may be sufficiently great to produce a tense state of the atoms without effecting decom- position! : hence the added affinity of a second body acting in the same direction may cause that change which each alone could not effect. Anything that disturbs the state of statical equilibrium in such a body will often effect its decomposition. This accessory affinity is recognised when both bodies enter into union. Charcoal and chlorine decompose alumina at a red heat, though neither can do so separately. In the same way BoudaultJ has shown that a mixture of potash or soda and red prussiate of potash oxidizes various me- tallic oxides, while Mercer has for many years made use of this mixture to discharge indigo-blue on calico §. Red prussiate of potash (FcgCygSK) has a great disposition to attach to itself another atom of potassium to become yellow prussiate of potash (Fe2Cyg4K). It cannot gratify this de- sire without aid ; but when assisted by a substance having an affinity for the oxygen of the potash, and capable of appropriating it, decomposition follows. There are often cases in which the body exercising the accessory affinity may be unable to effect the union, either by the influence of un- favourable chemical conditions or of cohesion or elasticity. Thus, in the case with which we first started, the affinity of protoxide of manganese for oxygen aids in the decomposition of nitrate of protoxide of manganese, and sesquioxide of man- ganese remains. If the temperature during the decomposition * Memoirs of Chemical Society, vol. iii. p. 93. t The alteration in volume is best seen in those oxides which contract and increase in specific gravity by tlie application of heat, for example, when the brown oxide becomes the green oxide of chromium. The two oxides must have a different molecular constitution, and this may be sup- posed to result from the elastic powers of one of its elements and the cohe- sive force of the other. The first eflTect of heat on oxide of chromium must be to expand the atoms of oxygen, and removing them further from the two atoms of chromium, permit the cohesive attraction of the latter to be gratified. Hence the compound acquires properties dependent upon cohesion, such as indiflference to union and diminished solubility. X Journal de Pharmacie, tome vii., 437. [Phil. Mag. Third Series, vol. xxvii. p. 307.] § Phil. Mag. Third Series, vol. xxxi, p. 126. In justice to Mercer, al- though this does not remove Boudault's claim of prioi'ity of publication, I cannot refrain from stating that the former chemist pointed out to me tlie oxidizing powers of the prussiates four or five years since. produced by Catalytic Bodies. 201 be elevated, the oxygen resumes its elastic state and refuses to form this higher oxide, as in fact we know is the case in Mer- cer's experiment Avith oxalic acid and nitric acid, where the presence of hot NO5 is an unfavourable chemical condition to the existence of Mug Og, and therefore it is not formed, but in its stead the oxygen is passed over to the organic mat- ter, which is able to unite with it under the circumstances. A similar instance of the effect of such conditions is seen when the peroxides of copper, manganese or lead, are thrown into a solution of bleaching powder. The affinity of these oxides for an additional quantity of oxygen enables them to decompose the hypochlorite of lime, converting it into chlo- ride of calcium. When the protoxides are used, this liberated oxygen unites and converts them to peroxides. The latter themselves have sufficiently strong affinity for oxygen to cause the decomposition to proceed ; but not uniting with it, pure oxygen is given off in the gaseous state. Here elasticity has come into play, and being more powerful than the feeble che- mical affinity, causes the oxygen to escape as a gas. When the solution is cool the gas goes off in a succession of small bubbles ; but when hot, the escape is tumultuous, the heat aiding the oxygen to enter into the elastic state*. A solution of chloride of lime evolves oxygen slowly at the boiling-point ; but the decomposition is much accelerated by the accessory agents referred to. The action of certain oxides upon peroxide of hydrogen is exactly similar to that on a solution of hypochlorite of lime. Thus peroxide of manganese, the protoxides of cobalt and lead, minium, peroxide of iron, and the protoxides of nickel, copper and bismuth, all exert this action on peroxide of hy- drogen with a force indicated by their orderf. In none of these cases does the oxide unite with a further proportion of oxygen. The violence of the action is however in proportion to their power of uniting with more oxygen. The first five oxides in the list have higher oxides of definite composition and of a certain degree of stability, with the exception of ferric acid; while the protoxides of copper and bismuth, although possessing the power of uniting with more oxygen, do not present superior oxides of a marked character. We should have * The best mode of instituting the experiment is to make a mixture of chloride of soda and caustic soda, lieat this to a temperature near ebuUition, and add sulphate of copper. The oxide of copper precipitated in the fine state of division causes such a copious evolution of oxygen gas that the con- tents are apt to be thrown out of the vessel : a mixture of chloride of lime and lime, or the ordinary unfiltered bleaching-powder of commerce, are also well-fitted to show the action. f Thenard's Traite de Chetnie, 6th edit. vol. i. p. 216. 202 Dr. Playfair on Transformations expected the oxides of nickel and cobalt to have exerted the same power, but from Thenard's description of the former being in the state of a black powder, it may have been the oxide of increased specific gravity, to which attention has already been drawn*. In all these cases the affinity is sup- posed to be sufficiently strong to break up the atoms of a body yielding to the slightest disturbance of its state of stati- cal equilibrium. Two affinities are at play in these decompo- sitions, viz. the attraction of the metaUic oxide for oxygen and that of the water for the same body ; both these affini- ties resist the union, and therefore, elasticity coming into operation, robs both oxides of the gas. The affinity causing the decomposition is so slightly preponderating in its in- fluence, that a second cause coming into operation is quite sufficient to alter the conditions under which it was originally exerted, and to draw one of the elements of the body acted upon beyond the sphere of its affinity. The balance of affinities in all such cases is so near that we not unfrequently find apparently contradictory effects result- ing from their gratification. Thus the addition of oxide of silver to peroxide of hydrogen expels oxygen from the latter, but at the same time it is robbed of its own oxygen and re- duced to the metallic state. In this case we have two feeble compounds instead of one, with affinities very nearly balanced, and with atoms so tense as to yield readily to the first dis- turbing cause. We can scai'cely adopt as sufficient the ex- planation of Thenard and Mitscherlichtj that the reduction is due to the elevation of temperature accompanying the de- composition, because even when that is lowered by the ad- dition of much water to the peroxide of hydrogen, the silver still becomes metallic. It is a point yet undetermined, whether a lower oxide is to be considered as unity to a higher oxide, or whether all the atoms of oxygen are held by equal attractions. We know that tartaric acid is able to separate potash from nitric acid in forming a bitartrate, and yet acetic acid is sufficient to re- move the second atom of potash from the neutral tartrate. But in a bibasic acid, like tartaric acid, it may be either atom of potash that is abstracted, and the superior affinity for the remaining one may be owing to attractions resulting after the expulsion of the first. Thus MnOg may have its atoms of oxygen distributed round the central nucleus Mn, and held by equal attractions, and the stability of the red oxide pro- duced by its calcination does not show that it pre-existed * Memoirs of the Chemical Society, vol. ii. p. 381, and vol. iii. p. 81. f Poggendoi-fF's ^nwa/e«, Iv. 321. produced by Catalytic Bodies. 203 in the black oxide, but merely that the attraction became stronger when one of the elements which divided it was removed. If it be admitted that the attraction of a radical for oxygen is equally divided between all the atoms of that element associated with it, the action to ^^ hich we have al- luded becomes comprehensible. In an oxide mc have the attraction of affinity opposed by the elasticity of its oxygen and by the cohesive force of the metal. If a be the attraction of the central nucleus or radical, c the cohesive force of the metal, and e the elasticity of the oxygen, then the molecular formula of a protoxide will be , of a sesquioxide — j and of a binoxide r— . Now if, as in oxide of silver, the a c + 2e and e are nearly equal, or the a only slightly preponderating, and the c or cohesive force very powerful, we can readily con- ceive that the added force of a second e may overcome the small amount of preponderating force in favour of a. Thus, when oxide of silver is placed in contact with peroxide of hydrogen, its affinity for more oxygen is sufficient to draw the second atom of oxygen beyond the sphere of attraction of H, and deliver it over to its own elasticity. But in doing this the attraction of silver for oxygen has been divided be- tween its own oxygen and that of the peroxide of hydrogen. Scarcely at any time capable of retaining its own oxygen, this division of its attractive force has been fatal to the exist- ence of its oxide, and the water in statu nascens at the same time exerting an affinity for the oxygen just ready to escape ; all these causes combined result in the reduction of the silver*. When pyruvic acid is in contact with oxide of silver, it unites and forms a salt; but when acting on carbonate of silver, a certain quantity of oxygen also leaves the oxide during the escape of carbonic acid, and metallic silver re- mains-}-. As Liebig J suggests, motion may aid this result; but were this the only explanation, we should expect that * During the passage of this paper tlirough tlie press, Mr. Brodie, in a lecture at the Royal Institution, showed that peroxide of potassium reduces chloride of silver, the two atoms of oxygen passing off in the gaseous state, while chloride of i-utassium and metallic silver remain behind, a singular decomposition, when the behaviour of potash is remembered. But the action is strictly the same as that here described ; the atoms of oxygen, - being liberated at the same time, are presented to the silver, which, dividing its attractive force between them, is not able to overcome the influence of elasticity of the oxygen and its own cohesion, and therefore remains in a metallic state. f Berzelius, Lehrhuch der Chemie, fifth edit. vol. iv. p. 231. I Chemistry of Agriculture, 4th edit., page 283. 204 Dr. Playfair on Transformations silver would constantly be reduced during the action of other feeble acids on carbonate of silver. If, however, we suppose that the pyruvic acid, Cg Hg O5, from its affinity for more oxygen, exerts an attraction for that element at the moment of the liberation of the carbonic acid, the decomposition would be similar to those we have already considered, espe- cially if the previous view of the molecular constitution of salts be admitted. In that case the oxygen of the oxide being attached to that of the carbonic acid, will be made highly tense during the escape of the latter, and may therefore be detached by a very feeble force, its elasticity finally over- coming the weak affinity. An extension of the explanation however strikes me as more probable, but it would be prema- ture to insist upon it without being supported by experiments which I have not yet been able to conclude. The action of metals and of charcoal on peroxide of hydro- gen may be explained by the same feeble affinity. Alkalies also, from their attraction for oxygen, as indicated both by their capability of uniting with more oxygen and by their basic power or disposition to attach themselves to a com- pound behaving as an oxygenous or chlorous element, favour the decomposition of HOg, while acids, on the other hand, render it more stable, perhaps, as Thenard himself suspected*, from there being an inferior oxide (Hg O3?). In this instance the elasticity of the oxygen tends to conceal the play of affi- nities by preventing combination. When the acting body is present in large quantity, or ex- hibits an increased surface, the action goes on with propor- tionate rapidity. Thus, when nitric acid is in contact with starch, the action is moderate until a certain quantity of per- oxide of nitrogen has been evolved by decomposition, after which it proceeds with a violence difficult to control. The per- oxide of nitrogen surrounding every particle of starch aids it in the decomposition of the nitric acid. That this is the real cause of the phaenomenon may be proved by the following simple experiment. Nitric acid is heated with starch to a tem- perature at which the action has a tendency to commence but has not yet begun. A stream of N04or NOg is then passed through the liquid, when action immediately begins with an activity proportionate to the quantity of gas added. The ele- vation of temperature due to the progressive action influences the decomposition, by causing the atoms of nitric acid to be- come more tense. Exactly the same accessory affinity is used by the manufacturer of oxymuriate of tin, when he adds a fragment of tin to the mixture of chloride of tin and * Traite de Chemie, p. 211. produced by Catalytic Bodies. 205 nitric acid. The tin eliminating some nitric oxide quickens the action, which commences with difficulty with pure nitric acid ; nitric oxide gas passed through the solution answers the same purpose. This accessory affinity also enables oxide of copper or per- oxide of manganese to evolve copious streams of oxygen from chlorate of potash in a state of fusion. The heat of fusion decomposes the compound slowly, but on adding a body ha- ving an affinity for the element acted upon by the heat (oxy- gen), the decomposition proceeds with greatly increased ra- pidity. We cannot ascribe this action to the presentation of points from which the gas may escape, as in the lowering of the temperature of ebullition by particles of sand, because silica has no influence in accelerating this decomposition*. In the examples previously given we have the decomposi- tions aided by the tendency of one of the bodies to assume the elastic form. But when the body acted upon has two elements, one of which is influenced by elasticity, the other by cohesion, we find it peculiarly liable to be acted upon by external agents. Persulphuret of hydrogen is a compound of this class, and has been closely studied in its decompositions by Thenardf. The same bodies which decompose peroxide of hydrogen act catalytically upon this sulphuret. The de- composition cannot be due to points for the escape of gas, as suggested by LiebigJ, to explain the decomposition of per- oxide of hydrogen, because solutions of the alkalies act with equal power. The sulphurets, especially those of the alkaline metals, decompose it very readily. As in the case of per- oxide of hydrogen, the acids afford stability to its sulphur analogue. In the view of acids given, they are supposed to have become chlorous or electro-negative, representing and behaving as oxygen, and therefore exerting no affinity, we should anticipate that they would not show any disposition to break up an oxygenous compound or its analogue of sul- phur. Another instance of accessory affinity is seen in the nitrosulphates § ; the formula (RO, SO^ + NOg) given by Pe- louze to these compounds does not allow us to understand their decompositions, which however becomes intelligible if we view nitrosulphuric acid as nitric acid, in which the fifth atom of oxygen has been replaced by one of sulphur (RO, NO4 S). In this acid we have two elements — the nitrogen and the sulphur — sharing the oxygen, their mutual affinities being nearly balanced when the acid is united with an al- * Taylor's Scientific Memoirs, vol. iv. p. 9. t Ann. de Ch. et de Ph. xlviii. 79. + Ann. der Pharm, ii. 22. 4 Ann, de Ch. et de Ph. Ix. 151. 206 Dr. Playfair on Transformations kali, although in a free state, the sulphur exhibits a superior affinity, as shown by the decomposition which then results, NO4S = NO + SO3. Now any substance which acts as an accessory to the sulphur by aiding the withdrawal of oxygen from the nitrogen decomposes it. This instability is especially exhibited in NH4O, NO4S ; the 3 atoms of hydrogen of the ammonia in their attraction for oxygen introducing another affinity, which accelerates decomposition. And, in fact, we do find that the same agents which so readily decompose the oxygenous compounds, chloride of lime and peroxide of hy- drogen, do equally cause the disruption of nitrosulphate of ammonia into protoxide of nitrogen and sulphate of ammonia. Alkalies are an exception to this rule, as they render the ni- trosulphates more stable, while they make the peroxide of hy- drogen prone to decomposition ; but the cases are different, the latter substance having none of the properties of an acid. The basic character of alkalies, defined as their power of uniting with more oxygen, or with an acid playing the part of an oxygenous element, is illustrated by several curious decompositions. Thus, though grape-sugar reduces sulphate of copper with ease, cane-sugar alone does not readily do so, but M'hen mixed with potash and boiled with the salt, sub- oxide of copper is produced, as in the mode of preparation of that oxide suggested by Boettger*, or the reduction of chloride of silver as proposed by Levolf. Here the disposi- tion of the organic matter to unite with oxygen is able to gratify itself when aided by the accessory affinity of the pot- ash for oxygen. That the potash in this state acts by aiding the oxidation, is seen by heating CugO with a solution of caustic potash, exposed to the air, when it oxidizes much more rapidly than when boiled with water alone J. When suboxide of copper is dissolved in ammonia it oxidizes with surprising rapidity. In this instance the hydrogen of the ammonia adds to its disposition as an alkali to absorb oxy- gen. The quick oxidation is not merely due to the fact of ♦ Ann. der Pharm. und Chemie, xxxix. 176. f Berzelius, Jahreshericht, vol. xxv. X This experiment may be simply made as follows : — Three shallow eva- porating basins of the same size and form, each containing the same quan- tity of suboxide of copper, are taken, and to one is added a solution of potash or soda; to the second, a solution of chloride of manganese; to the third, common water, taking care that the same volume of each fluid is added. The whole are now placed on a sand-bath, so as to be exposed to equal temperatures, and stirred occasionally. The suboxide of copper in the basin containing chloride of manganese oxidizes very rapidly ; that in contact with the potash more slowly; and that with simple water is scarcely effected when both the others have lost their red colour. These actions are strictly in accordance with theory. produced by Catalytic Bodies. 207 the suboxide being in a state of solution, because the soluble salts of the suboxide do not oxidize with such extraordinary ease, nor is it to be expected that they should, if we admit that the acid itself plays the part of oxygen. The accessory affi- nity of alkalies for oxygen is exhibited in many other cases of chemical action. Thus, colouring matters, such as deoxidized logwood, Brazil-wood, peach-wood, japan, fustic and catechu are oxidized more rapidly in contact with alkalies than in water alone ; and various dyeing principles, such as orcine and erythrine, absorb oxygen with great avidity in the presence of ammonia. Sugar may be boiled with potash without de- composition, but when air is admitted, formic, melassic, and glucic acids are produced. Hydruret of benzyle when ex- posed to air gradually absorbs oxygen and passes into benzoic acid, but in contact with potash this absorption is very much accelerated. The rapid decomposition of the gallates and of hematine in the presence of free alkali and air is aphaenome- non of the same kind. In fact, numberless instances of this catalytic action of the alkalies are known to chemists. We find the influence of an accessory oxidation in many cases of chemical union. Thus Campbell has shown * that the transformation of cyanide of potassium into cyanate of potash is much accelerated by the presence of the iron in yellow prussiate of potash, the iron being converted into oxide during the transformation. Here the iron plays the part of the protoxide of manganese in the cases of oxidation already re- ferred to, or it perhaps bears a more direct relation to the action of lead in communicating a tendency to the base metals to seize oxygen during the process of cupellation. The in- fluence exerted by peroxide of manganese in first converting cyanide of potassium into cyanate of potash and afterwards into the carbonate of that base, is another instance of accessory affinity ; for only a portion of the oxygen is derived from the oxide employed. The solution of an alloy of silver and pla- tinum in nitric acid may be supposed to be a similar affinity. It is not necessary to believe that this is a case proving the communication of intestine motion to the atoms of platinum, by which it acquires the power of decomposing nitric acid f ; for an equally simple explanation is given by assuming that the united affinities of platinum and silver are able to decom- pose nitric acid, both these affinities acting in one direction at the same time, and enabling the platinum to dissolve. We have only to suppose that the atoms of nitric acid are placed by the silver in a state of such tension that the platinum can * Phil. Mag. Third Series, vol. xix. p. 513. t Liebig's Elements of Agriculture, 4th edit., p. 280. 208 Dr. Playfair on Transformations now seize oxygen, which it could not do from the nitric acid when in a less tense state. The quartation of gold is ob- viously a phaenomenon of the same kind. In these instances the interposing silver much reduces the cohesive or aggregative force of the platinum or gold, which opposes so strongly the action of nitric acid upon them. But when we have every atom of platinum or of gold separated by one of silver, great facility is given to the nitric acid to act upon these metals, especially when the silver at the same time aids them by its assistant affinity. We have seen, in the consideration of the previous in- stances of catalysis, that the play of affinities was occasionally so nearly balanced, that a second disturbing cause determined the direction of the action. In the case of non-accendi- ble phosphuretted hydrogen, the addition of another oxi- dizable body, NO4, decided the union of oxygen with the gas. In accendible phosphuretted hydrogen the compound PHg played the same part. When the accessory agent is present in small quantity, the preponderating affinity of the body acted upon shows itself in the result. But, as the ac- tion is due to two affinities nearly equal in amount, it is easy to conceive that the increased quantity of the accessory agent may exactly balance affinities, and that the catalytic phaeno- menon will be prevented. Thus one-twentieth of the volume of binoxide of nitrogen, according to Graham*, added to ac- cendible phosphuretted hydrogen, does not deprive it of in- flammability, the bubbles of gas escaping into the air with a kind of explosion, although one-tenth volume of the same gas altogether prevents the accendibility. This nitric oxide, when pure, does not, like protoxide of nitrogen, render phos- phuretted hydrogen spontaneously inflammable, the reason obviously being that its own affinity for oxygen is more powerful than that of the phosphuretted hydrogen. When added however in such small proportion to the accendible gas that the foreign constituent in it preponderates, then it becomes an accessory to the oxidation, though an increase of the quantity renders it more powerful, and prevents accendi- bility by itself seizing oxygen. Thus also larger volumes of gas, having an affinity for oxygen, but incapable like NO4 of gratifying that desire under ordinary circumstances, may exactly balance the feeble affinity of the foreign accessory body and prevent oxidation. Five volumes of hydrogen, 2 volumes of carbonic acid, 1 volume of olefiant gas, and 1 volume sulphuretted hydrogen, deprive 1 volume of phos- * Phil. Mag., Tliird Series, vol. v. p. 405. produced by Catalytic Bodies. 209 phuretted hydrogen of its spontaneous inflammability*. The very conception of a catalytic agent, on the view adopted, implies the exertion of an affinity, which is passed over or added to that of the body acted upon. If, therefore, a third body claim this added affinity, the increase of power being divided, may be insufficient to exert the force which it did when wholly applied to aid the affinity of one body. It may be this balancing of affinities which prevents the action of platinum on a mixture of oxygen and hydrogen. The plati- num by its surface affinity condenses oxygen, and presenting it to hydrogen in a condensed form produces union. But in the presence of small quantities of certain oxidizable gases, such as sulphuretted hydrogen, carbonic oxide, and defiant gases f , it ceases to exert this action, the assumption in this case being that the affinity of the added gases for oxygen balances that of hydrogen for the same gas. This balancing of affinities may account for several phaeno- mena otherwise inexplicable. On the decay of vegetable mould we find the hydrogen constantly diminishing in quan- tity until a certain period of decomposition, when the affinity of the carbon of the humus for its hydrogen balances the affinity of the surrounding oxygen. It seems to be the same balancing of affinities which renders corrosive sublimate so antiseptic in its properties ; but, in this case, the balance re- sults from the affinity of the second atom of chlorine in the bichloride of mercury for the hydrogen of the organic sub- stance, thus preventing its union with oxygen. It is probable that the same affinity of chlorine for hydrogen causes turpen- tine and the volatile oils to act cataly tically in exploding chlo- ride of nitrogen. The chlorine attracted by the hydrogen of these substances is drawn without the sphere of its attraction for nitrogen, and a disruption of the elements consequently ensues, compounds such as this resting on the very verge of separation between physical and chemical attraction. The antiseptic action of corrosive sublimate is very different from that exerted by sulphurous acid and sulphate of iron, these bodies acting by their superior affinity for oxygen, and neu- tralizing the power of the ferments or accessory oxidizers present in the organic body. There is no difficulty in applying these notions of catalysis to organic compounds, which from the complexity of their • The influence which the vapours of turpentine exert in jjreventing the oxidation of phosphorus in the air is probably another instance of this balancing of affinities. t Faraday, Phil. Mag., Third Series, vol. v. p. 405 ; Turner, Jameson's Journal, xi. 99 and 311. Phil. Mag. S. 3. Vol. 31. No. 207. Sept, 184.7. P 210 Dr. Play fair on Transformations molecules are peculiarly liable to change. If it once be ad- mitted that an assisting affinity may exist in the sense defined in the present paper, then we see the same cause operating upon organic as well as inorganic molecules. When nitric acid acts on oxalic acid or starch, an inorganic body (a pro- tosalt of manganese) lowers the temperature necessary for the oxidation, and exerts its influence until all the starch is converted into carbonic acid, being equally efficacious on the addition of more nitric acid and starch. Here the body acting as an assistant remains unchanged, and there- fore continues its action ad infinitum, rendering it impossible to prepare oxalic acid from nitric acid and starch or sugar, carbonic acid being the only product*. Had the assistant oxidizer passed from solution during the progress of the oxida- tion, it could not of course continue its favourable effect, and a new portion of it must have been added. Here the inor- ganic salt enables the sugar to oxidize itself from the sur- rounding medium just as yeast does, the only difference being that the yeast itself suffers change, and therefore can only continue its action for a limited period. It is exactly in the same condition as a mixture of nitric acid and binoxide of nitrogen made to act on protochloride of tin. A. small portion of the latter added to such a mixture is oxidized, but when the solution is heated until all the NOg is expelled, oxidation does not ensue on the addition of a new portion at the same low temperature as before. Now Saussure and Colin have shown that j^east only induces fermentation when it is in a position to absorb oxygen. It acts therefore strictly as bin- oxide of nitrogen, or a protosalt of manganese, in the previous instances, by adding its affinity for oxygen to that of the sugar, the added affinities of both completing the union. The only difference between these two decompositions is, that in one case the oxidizing agent is nitric acid, in the other it is water. The composition of sugar shows it to contain the elements of alcohol and carbonic acid minus an atom of water. In such a compound we have the affinity of carbon for hy- drogen and of carbon for oxygen. The yeast by its nitrogen also exerts an affinity for hydrogen, and by its carbon for oxygen. The united affinities of the sugar and of the yeast acting upon water decompose it, its elements on their libera- tion being shared by the carbon of the sugar, for which it may be supposed to have the strongest affinities, Cjg IIn On • In this it resembles the action of oxalic acid in converting an unlimited quantity of oxamide into oxalate of .ammonia, with this difference, that the oxalic acid, which causes the change, may not be the same, but a regene- rated portion, while the salt of manganese always remains unchanged. produced by Catalytic Bodies. 211 + HO=4C02 + 2 (C4 Hg O2). To show the exact similarity of the two processes of oxidation when the assisting body is either organic or inorganic, I may cite the curious manufac- turing process for oxidizing oils in the method of dyeing Turkey-red used in this country, and included in Mercer's patent for that colour. It consists in oxidizing oils by blow- ing hot air through them, the oils being in contact with a solution of a salt of copper or of bran ; the contact of either of these solutions is found very materially to accelerate the oxidation. The catalytic action of oxide of copper in evolving oxygen from hypochlorite of lime was adduced as showing its affinity for more oxygen, and this feeble affinity is well known and used empirically by all calico-printers, who are in the con- stant habit of mixing a salt of copper with their colours for the purpose of ageing them more speedily ; in other words, of causing them to unite with oxygen. This also is the assisting cause in Mercer's process for oxidizing oils ; bran in solution answers the same purpose from its affinity for oxygen. The addition of common salt or muriate of ammonia favours the oxidation in all the cases referred to, the oxidation proceeding much more quickly in their presence. No sub-chloride is ever formed, the action being purely catalytic, and probably depending on the conversion of the salt of copper into a chloride, the chlorine of which may be supposed to exert a slight affinity for the hydrogen of the compound, thus withdrawing it somewhat from the sphere of its own special attractions in the body; the copper now aiding the chlorine, delivers the hydrogen more easily into the power of the oxy- gen of the atmosphere. It is therefore immaterial whether the body exercising the assistant affinity be organic or inor- ganic, if the conditions be favourable to the exercise of this influence. The action of a body in acetous fermentation on the transformation of bi'andy into vinegar must be recognised as a phenomenon of a like kind. We know that brandy may trickle m ithout change over a large surface of wood shavings, through which air circulates at the heat of the human body, but that it is quickly converted into vinegar if brandy in the act of oxidation be mixed with it. Here the added ferment exerts its assisting affinity in precisely the same way as the salt of copper, when it aids the oxidation of oils or colours, or as protonitrate of manganese or peroxide of nitrogen during the oxidation of starch. The conversion of hydrogen and oxygen into Mater by the action of fermenting silk, cot- ton, or woody fibre, as observed by Saussure, is obviously a phaenomenon of the same kind, and can only be exerted slowly and in the immediate vicinity of the assisting oxidi- P2 212 Dr. Playfair oh Transformations zers, just as a ball of spongy platinum silently effects the union of these two gases. In these cases we must admit that the action is indepen- dent of a state of intestine motion of the atoms of one com- pound molecule imparted to those of another, or, if we do not allow this, we must create two new powers and separate de- compositions caused by inorganic bodies from those produced by organic compounds, although all the phaenomena of the decomposition show them to belong to one category. In a body in a state of such incessant change as the blood of living animals, it would naturally be expected that an added agency, such as that described, would render it prone to abnormal actions and oxidations, and in fact we do recognise by all the recent progress in the study of public hygeine that the addition of any oxidizing miasm or putrid matter to the blood does produce those changes which are known by their results in the different forms of disease. These and other catalytic agents no doubt exercise most important in- fluence on the processes of animal life and on the action of medicaments on the system, but it would be foreign to the object of this paper to examine them in detail. The limits of a paper such as this compel me to avoid including many other instances of catalytic decompositions which come under this explanation, or of drawing special attention to those which cannot be included in the present state of our knowledge. Thus diastase, acting on starch, converts it into sugar, but we have so little knowledge of the composition or properties of the first body, that it would be unwarrantable to embrace a case such as this. But in analogous changes produced by bodies which are under- stood, the same power is recognised. Sulphuric acid in converting starch into grape-sugar offers an example of combination Avhich may fairly be examined by the same method employed in investigating other decompositions. Graham has shown* that heat is evolved even on the addi- tion of the 48th atomic proportion of water to sulphuric acid, or, in other words, that the affinity of that acid for water is not gratified as long as our instruments of research can follow the change. This is merely another proof of the doctrine with which I started, that there is no evidence of such a complete gratification of affinity as ever to merge entirely the attractions of the elements of any body. In the case referred to, the development of heat on each successive addition proves that the water is condensed on entering into union with the acid. When the heat of the sulphuric acid is arti- * Phil. Mag. Third Series, vol. xxii. j). 334. produced by Catalytic Bodies. 213 ficially increased, this compound is broken up, for distil- lation drives off the water and concentrates the acid. Now when starch is in the presence of this weak combination of sulphuric acid and water, at a temperature at which the latter is just able to exert its affinity and again have it de- stroyed by heat, it is not at all extravagant to suppose that the starch may seize the water in its nascent state at the mo- ment of expulsion, or even that it may be able to unite with the last atoms of the series of acid and water when presented in that condensed state, although it cannot do so when the water is free and not nascent. Any such union would explain the transformation of starch into grape-sugar, the change merely being in the acquisition of water, Cjg Hiq Oio + 4HO = C,2 Hi4 O14. The action here is not the same, but the very reverse of that which ensues in the preparation of aether. In the one case the sulphuric acid abstracts water, in the other it is the means of adding it, and the difference of the action depends on the relative strength of the acids employed. Without at all giving an opinion in favour of the necessity for the formation of sulphovinic acid, as supposed by Liebig*, or as to its not being an essential condition, as argued by Mitscherlichf, the final result is simply of the order now under consideration. In this decomposition the sulphuric or phosphoric acid is so strong that it combines with the water instead of yielding it, and the elevation of temperature essen- tial to the change may either be due to the formation and after decomposition of sulphovinic acid, or it may be simply owing to the necessity of rendering the molecule of alcohol tense by heat, the elasticity of the aether and water both tending to break up the hydrate, the decomposition of which is determined by the presence of the strong acid now also aiding and abstracting the water. The final result is certainly purely catalytic in whatever light it is considered, although there may be more than one step in the process. In conclusion, facts have been brought forward to show that there is at least as m\ich probability in the view that the catalytic force is merely a modified form of chemical affinity exerted under peculiar conditions, as there is in ascribing it to an unknown power, or to the communication of an intes- tine motion to the atoms of a complex molecule. Numerous cases have been cited in which the action results when the assisting or catalytic body is not in a state of change, and attempts have been made to prove by new experiments that the catalytic body exercises its peculiar power by acting in * Geiger's Pharmacie, vol. ii. p. 711 ei seq. t Lehrbuch der Chemie, vol. i. p. 247 et seq. ^14 Sir W. Rowan Hamilton on Qiiaternions, the same direction as the body decomposing or entering into union, but under conditions in which its own affinity cannot always be gratified. The catalytic body is therefore a sub- stance which acts by adding its own affinity to that of an- other body, or by exerting an attraction sufficient to effect decomposition under certain circumstances, without being powerful enough to overcome new conditions, such as elasti- city and cohesion, which occasionally intervene and alter the expected result. At the same time the theory is far from being fully proved ; but if I have succeeded in rendering probable that the ca- talytic force is only chemical affinity recognised under an aspect which chemists have not been accustomed to view it, and exerted under conditions which can only be developed by close attention to details, it will not have been useless to direct increased study to this interesting class of phenomena. XXXVI. 0« QiiaterJiions / or on a Nexv Si/stem of Imaginaries in Algebra. By Professor Sir William Rowan Hamilton, LL.D., V. P.R.I. A.^ F. R.A.S., Correspofidhig Member of the Institute of France^ and of other Scientifc Societies in British and Foreign Countries^ Andrews^ Professor of Astronomy in the University of Dublin ^ and Royal Astronomer of Ireland. [Continued from vol. xxx. p. 461.] 33. T^OR the sake of those mathematical readers who are •*- familiar with the method of co-ordinates, and not with the method of quaternions, the writer will here offer an inves- tigation, by the former method, of that general property of the ellipsoid to which he was conducted by the latter method, and of which an account was given in a recent Number of this Magazine (for June 1847). Let X y z denote, as usual, the three rectangular co-ordi- nates of a point, and let us introduce two real functions of these three co-ordinates, and of six arbitrary but real con- stants, I mnV m' n', which functions shall be denoted by ic and V, and shall be determined by the two following relations: u{ll' -f mm' + nn') = Vx + fri'y + n'% ; i^{ll' 4- mm' + nn^Y = [ly — mxf + [mz — nyf + [nx — hf ; then the equation u^^v'^=i\ (1.) will denote (as received principles suffice to show) that the curved surface which is the locus of the point x y zhtm ellip- soid, having its centre at the origin of co-ordinates ; and con- versely this equation u'^ + i^=l may represent any such ellip- Sir W. Rowan Hamilton on Qjiaternions, 215 soid, by a suitable choice of the six real constants ImnV rri 11!, At the same time the equation will represent a system of two parallel planes, which touch the ellipsoid at the extremities of the diameter denoted by the equation v = 0', and this diameter will be the axis of revolution of a certain circumscribed cylinder, namely of the cylinder denoted by the equation the equation of the plane of the ellipse of contact, along which this circular cylinder envelopes the ellipsoid, being, in the same notation, M=0: all which may be inferred from ordinary principles, and agrees with what was remarked in the 29th article of this paper. 34. This being premised, let us next introduce three new- constants, p, g, r, depending on the six former constants by the three relations 2p = l + l'j 2q = m + m'f 2r=zti-\-n'. We shall then have I'x + m'j/ + n'z = 2 {px -\-qi^-\-rz)— [Ix -\-my-^ nz) ; and the equation (1.) of the ellipsoid will become {W -\-mm' -^nn'f - {p + m^ + n^)(^x^ ^f + 2'^) —^{lx-\- my + nz)[px -\-qy-{-rz) + ^{px-^qy-\-rzY if we introduce three new variables, of, y\ s', depending on the three old variables .r, y^ z, or rather on their ratios, and on the three new constants p, q, r, by the conditions, *' _ V _ ^' _ 2{px-{-qy + rz) x~ y z x^-\-y^-\-z^ These three last equations give, by elimination of the two ratios of ,r, y, z, the relation ^'2 ^ya ^ ^n = 2(/?y + qy' + rz') ; the new variables a/, y\ z' are therefore co-ordinates of a new point, which has for its locus a certain spheric surface, passing through the centre of the ellipsoid ; and the same new point 216 Sir W. Rowan Hamilton on Quaternions. is evidently contained on the radius vector drawn from that centre of the ellipsoid to the point .r 3/ g', or on that radius vector prolonged. We see, also, that the length of this radius vector of the ellipsoid, or the distance of the point x y z from the origin of the co-ordinates, is inversely proportional to the distance of the new point a^ y' z' of the spheric surface from the point / m n, which latter is a certain fixed point upon the surface of the ellipsoid. This result gives already an easy and elementary mode of generating the latter surface, which may however be reduced to a still greater degree of simplicity by continuing the analysis as follows. 35. Let the straight line which connects the two points a' y z' and / m n be prolonged, if necessary, so as to cut the same spheric surface again in another point a?" y ^": we shall then have the equation from which the new co-ordinates a/', y", 2" may be eliminated by substituting the expressions ;r" = Z+^(^'-/), i/' = m + t{y'-m), z"=n + l{z'-n); and th^ root that is equal to unity is then to be rejected, in the resulting quadratic for t. Taking therefore for t the pro- duct of the roots of that quadratic, we find Z^ + m^ + n^ — 2(lp + mq-\- nr) therefore also, by the last article, X^ -\- 7f -{■ Z^ consequently ,2_ x^ + y^-\-z^ and finally, {x"-l)^-\-{y"-m)^ + {is"-n)^=x'' + y^ + z\ . (2.) Denoting by a, b, c, the three fixed points of which the co-ordinates are respectively (0, 0, 0), (/, m, w), (p, q, r) ; and by D, d', e, the three variable points of which the co-ordinates are (y, y, s'), (:i", y, z"), (xy y^z)', abed' may be regarded as a plane quadrilateral, of which the diagonals ae and bd' intersect each other in a point d on a fixed spheric sur- face, which has its centre at c, and passes through a and d'; so that one side d'a of the quadrilateral, adjacent to the fixed side AB, is a chord of this fixed sphere. And the equation (2.) expresses that the other side be of the same plane quadrilateral^ adjacent to the same Jixed side ab, is a chord of ajixed ellipsoid. Sir W. Rowan Hamilton on Quaternions. 217 if the two diagonals ae, bd' of the quadrilateral be equally long ; so that a general and characteristic property of the ellipsoid, sufficient tor the construction of that surface, and t'or the in- vestigation of all its properties, is included in the remarkably simple and eminently geometrical formula AE=BD'; ,(3.) the locus of the point E being an ellipsoid, which passes through B, and has its centre at A, when this condition is satisfied. This formula (3.)} which has already been printed in this Magazine as the equation (10.) of article 30 of this paper, may therefore be deduced, as above, from generally admitted prin- ciples, by the Cartesian method of co-ordinates ; although it had not been known to geometers, so far as the present writer has hitherto been able to ascertain, until he was led to it, in the summer of 1 846 *, by an entirely diiFerent method ; namely by applying his calculus of quaternions to the discussion of one of those new formsf for the equations of central surfaces of the second order, which he had communicated to the Royal Irish Academy in December 1845. 36. As an example (already alluded to in the 32nd article of this paper) of the geometrical employment of the formula (3.), or of the equality which it expresses as existing between the lengths of the two diagonals of a certain plane quadrilateral connected with that new construction of the ellipsoid to which the writer was thus led by quaternions, let us now propose to investigate geometrically, by the help of that equality of dia- gonals, the difference of the squares of the reciprocals of the greatest and least semi-diameters of any plane and diametral section of an ellipsoid (with three unequal axes). Conceive then that the ellipsoid, and the auxiliary sphere employed in the above-mentioned construction, are both cut by a plane abV, on which b' and c' are the orthogonal projections of the fixed points B and c ; the auxiliary point d may thus be conceived to move on the circumference of a circle, which passes through A, and has its centre at c' ; and since AE, being equal in length * See the Proceedings of the Royal Irish Academy, t In reprinting one of those new forms, namely the following quater- nion form of the equation of the ellipsoid: a slight mistake of the press occurred at p. 459, vol. xxx. of this Magazine, which however, with the assistance there given by the context, can scarcely have embarrassed the reader. In the preceding page, for a hyperboloid of one sheet, touching the same cylinder in the same sheet, should have been printed, .... in the same ellipse. 218 Sir W. Rowan Hamilton on Quaternions. to BD' (because these are the two equal diagonals of the qua- drilateral in the construction), must vary inversely as BD (by an elementary property of the sphere), we are to seek the difference of the squares of the extreme values of BD, or of B'D, because the square of the perpendicular BB' is constant for the section. But the longest and shortest straight lines, B'D], B'Dg, which can thus be drawn to the auxiliary circle round C, from the fixed point B' in its plane, are those drawn to the extremities of that diameter DiC'D2of this circle which passes through or tends towards B' ; so that the four points Di C Dg B' are on one straight line, and the difference of the squares of B'Dj, B'Dg is equal to four times the rectangle under B'C and C'D^, or under B'C and C'A. We see therefore that the shortest and longest semi-diameters AEj, AEg of the diametral section of the ellipsoid, are perpendicular lo each other,because (by the construction above-mentioned)they coin- cide in their directions respectively with the two supplementary chords ADi, ADg of the section of the auxiliary sphere, and an angle in a semicircle is a right angle; and at the same time we see also that the difference of the squares of the reciprocals of these two rectangular semlaxes of a diametral section of the ellipsoid varies, in passing from one such section to another, proportionally to the rectangle under the projections, B'C and C'A, of the two fixed lines BC, CA, on the plane of the vari- able section. The difference of the squares of these recipro- cals of the semi-axes of a section therefore varies (as indeed it is well-known to do) proportionally to the product of the sines of the inclinations of the plane of the section to two fixed dia- metral planes, which cut the ellipsoid in circles; and we see that the normals to these two latter or cyclic planes have precisely the directions of the sides BC, CA of the generating triangle ABC, which has for its corners the three fixed points employed in the foregoing construction : so that the auxiliary and (liacentric sphere, employed in the same construction, touches one of those two cyclic planes at the centre A of the ellipsoid. If we take, as we are allowed tO do, the point B external to this sphere, then the distance BC of this external point B from the centre C of the sphere is (by the construc- tion) the semisum of the greatest and least semiaxes of the ellipsoid, while the radius CA of the sphere is the semidiffer- ence of the same two semiaxes: and (by the same construc- tion) these greatest and least semiaxes of the ellipsoid, or their prolongations, intersect the surface of the same diacen- tric sphere in points which are respectively situated on the finite straight line BC itself, and on the prolongation of that line. The remaining side AB of the same fixed or generating Notices respecting New Books. 219 triangle ABC is a semidiameter of the ellipsoid, drawn in the direction of the axis of one of the two circumscribed cylinders of revolution ; a property which was mentioned in the 32nd article, and which may be seen to hold good, not only froni the recent analysis conducted by the Cartesian method, but also and more simply from the geometrical consideration that the constant rectangle under the two straight lines BD and AE, in the construction, exceeds the double area of the triangle ABE) and therefore exceeds the rectangle under the fixed line ABand the perpendicular let fall thereon from the varia- ble point E of the ellipsoid, except at the limit where the angle ADB is right; which last condition determines a cir- cular locus for D, and an elliptic locus for E, namely that ellipse of contact along which a cylinder of revolution round AB envelopes the ellipsoid, and which here presents itself as a section of the cylinder by a plane. The radius of this cylinder is equal to the line BG, if G be the point of intersection, di- stinct from A, of the side AB of the generating triangle with the surface of the diacentric sphere; which line BG is also easily shown, on similar geometrical principles, as a conse- quence of the same construction, to be equal to the common radius of the two circular sections, or to the mean semiaxis of the ellipsoid, which is perpendicular to the greatest and the least. Hence also the side AB of the generating triangle is, in length, a fourth proportional to the three semiaxes, that is to the mean, the least, and the greatest, or to the mean, the greatest, and the least, of the three principal and rectangular semidiameters of the ellipsoid. [To be continued.] XXXVII. Notices respecting New Books. Notice of a Memoir on Meteors of various sorts. By T.I. M. Forster, F.R.A.S., &;c. Bruges, 1846. EXPERIENCED in observing and in treating of these phseno- mena, Dr. Forster refers his readers to his former communica- tions of them, and to the numerous articles in the Royal Society's Transactions, as well as in the Gentleman's and Philosophical Ma- gazines. He carefully examines the theory of phosphorescent jets of gas rising unperceived while traversing the low and damp strata of the atmosphere, but becoming ignited as soon as they reach a sufficiently dry stratum. The ignition is then supposed to run down the column of gas, and reveal the several bends it had been subjected to by Various currents of wind. The occasional explosions may be ex- plained by supposing the running fire to reach a spot overabounding itl hydrogen, instances not unfrequent after heavy rains. 220 Notices respecting New Booh. It was not till the 10th of August 1811 that the idea of their periodicity occurred to Dr. Forster, when he and his father counted some hundreds, and by their journal perceived their recurrence on that same day. Indeed, in copying a curious old manuscript calen- dar, he found the 10th and 18th of August called stellibvndce and meterodes ; but he acknowledges their frequency at all times and in all places. Inclined to assign them a gaseous origin, our author has yet, in deference'to the learned men who differed from him, endeavoured to relate fairly the various arguments in favour of their several theories. Aristotle regarded meteors as arising from exhalations denoting an approaching change of weather. Theophrastus thought they pro- gnosticated wind from the quarter towards which they rushed. And Aratus agreed with him, especially if they left long lingering tails, in which he was imitated by Virgil. Lucan in his Pharsalia rather confounds meteors with the fixed stars. Homer compares the descent of Minerva to the rush of a meteor. Passing over the middle ages, when meteors were feared as indica- tions of Divine anger, we find that in the seventeenth century electri- city began to be suspected, and was supported by the highest names of that sera. Then the magnificent meteor of the 18th of August 1783 brought out the elaborate paper by Dr. Blagden in the Philosophical Transactions for the following year. As to their velocity, it varies so much that this element cannot suffice to decide from what height they fall. The meteor above alluded to moved at only six miles per second when at about ninety miles above our heads. Cavallo esti- mated its diameter at 3200 feet, and its elevation at 560 miles. Cer- tainly the explosion not being heard for ten minutes after it was seen is a sufficient proof of its distance. The general electric state of the atmosphere that year over half the globe is well known, by the remarks made in consequence of the violent earthquakes that occurred. In support of the theory that meteors are occasioned by the igni- tion of columns of inflammable gas. Dr. Forster mentions the ignis fatuus, and the flitting lights that are seen in May on cabbages. Many naturalists regard meteors as one of the various phaenomena attributable to electricity, and some expected to find that they chiefly pointed to the magnetic pole. Many roofs of thatch have been ignited by the fall of meteors upon them, and this must be the explanation of towns recorded to have been burnt by fire from heaven. The explosion of the meteor of the 25th of September 1846, was heard a few seconds after it was seen : but if, instead of the ambiguous term a few, spectators would count slowly, they would aff^ord a much nearer approach to the true time elapsed, especially if they would afterwards count at the same rate when they can compare with a seconds watch, or with a clock. (A.S.) The tail of that meteor was larger than usual, and lasted longer, some persons stating fifty seconds, others some minutes. More precise details are requisite. It was at first whitish, then purplish, and lastly red, when it became curved, and faded in a serpentine Notices respecting New Books. 221 form. This last phaenoraenon was observed in another instance about twenty years since. Even the luminous arc of the 28th of September 1828 might, our author thinks, be a still more dilatory tail of a meteor that had shot across our hemisphere just before sunset, and for that reason was not perceived. In July 1799 Dr. Forster's father saw a meteor cross the sky from south to north, then return southward, and finally bend to the north-west. Another peculiarity is that of rising in the sky instead of descending, which has been reported as occurring sometimes near the equator, where they are very numerous. And Dr. Forster himself saw a whitish globe stationary for two seconds, and then turn a fine red. A shower of small meteors is recorded to have occurred on the 25th of April 1095 ; and Dr. Forster saw an approximation to this on a bright winter night in 1832, inasmuch as the whole firmament was in a glow from an immense number of very fine luminous tails nearly parallel from E.N.E. to W.S.W. They might deserve the name rather of streaks, no heads being visible. The duration of each might not exceed a second, but the phaenomenon altogether lasted a quarter of an hour and then ceased suddenly. And in November 1830 he saw a similar multiplicity of little streaks, but crossed by others at right angles. Another peculiarity was described by a clergyman near Epping, that of seeing a meteor, after descending to the earth, undergo a sort of reverberation by rising in an oblique direction, and then break into sparks. Among the numerous authors who have treated of this subject, perhaps M. Quetelet's catalogue is the most complete, with the ex- ception of his omitting the interesting meteor of 1783. M. Arago and M. Biot have also treated the subject ably. A copious journal of meteors has been kept in Dr. Forster's family from 1767, but no periodicity was suspected till the 10th of August 1811 ; though then, on looking back through the journal, it was per- ceived that there had been a great preponderance in the Novembers ever since 1799, and in the Augusts from 1779. When employed a few years after to construct perennial calendars. Dr. Forster indicated a number of meteors as a phsenomenon to be expected on the 10th of August. This became confirmed in 1831 by other observers, and they added the second period of the 13th of November. M. Queteletnow adds April and December, while others suggest January, May, June and July. He thinks their usual height in the atmosphere is from six- teen to twenty leagues or more, though they are occasionally seen slanting very near the ground. The most numerous sort, distin- guished by the name of etoiles filantes, may revolve in trajectories by swarms, forming a belt round the sun, which we have occasionally to traverse. Then, owing to the earth's motion, these luminous corpuscles would naturally, as they have been observed to do, appear to " have their point of divergence towards /3 Camelop. in August, and towards v Leonis in November, agreeing with our annual mo- tion in the ecliptic." According to the known laws of optics, the swarm would seem to separate in radii as we neared them, and. 222 Boyal Society, owing to the compound velocities, seem to tend from N.E. to S.W. Although meteors differ very much from each other in some in- stances, it is very difficult to classify them ; but an abundance of them seems connected with a change of weather, and especially with cirrostratus and cirrocumulus clouds. As to their direction, though they sometimes converge towards one point, they rush at others towards every point of the compass. He therefoi'e wavers only be- tween an electric and a gaseous origin, — quoting electric experiments referred to in England by the Abbe Bertholon, and gaseous ones by Constable, as having produced excellent imitations. In the terrible night of the 7th of July 1834, a crowd of nimbi collected around Vesuvius about 9 o'clock, shooting their lightnings down towards the mountain accompanied by rain and hail. The lightning was sometimes bluish and sometimes reddish. As to the periodicity of meteors. Dr. Forster finds that there are decided changes in the electrometers also on the 10th of August and 13th of November ; and the greatest number he ever saw fell on the 10th of August 1811, just after a violent storm ; but when a storm has happened some time before, the meteors are fewer at the two periods observed. Also if one or more large meteors occur, there are no small ones afterwards for a proportionate time, as if the atmo- sphere had been cleared of the requisite material. Also it may be remarked in general, that the winter and the higher latitudes are least prolific of them. Fiery balls do not often occur, but are very powerful. Thus the one seen in France and in England the 17th of July 1771, must have been at an elevation of fifty-four miles, and the report of its explosion was not heard till two minutes after its occurrence, like the rolling of thunder ; but the observatory windows at Paris were " ebranlees." It appeared larger and brighter than the]), and its swiftness was estimated at twenty-four miles per second. From the quickly-increasing rarity of our atmosphere, Arbuthnot thinks that at the height of sixty miles (the estimated height of tlie meteor in 1718) the air is 30,000 times purer than on the level of the sea. Yet Pringle estimated the height of the meteor of 1738 to have been ninety miles. The diameter of some globes has been estimated at 1^ mile. XXXVIII. Proceedings of Learned Societies. nOYAL SOCIETY. [Continued from p. 770 June 17, " 13 ESEARCHES on the Function of the Intercostal 184<7. "-^ Muscles and on tlie Respiratory Movements, with some remarks on Muscular Power, in Man." By John Hutchinson, M.li.C.S. Communicated by Sir I3enjamin Brodie, Bart., F.R.S., &c. The object of this paper is to demonstrate by models and dis- sections the action of the intercostal muscles. Royal Society, 223 After premising an account of the views of several eminent phy- siologists, and in particular those promulgated by Haller, the author shows that they resolve themselves into the general opinion that the scalene or other muscles of the neck fix the first rib, in order to enable the two sets of inlei'costal muscles to act either separately or conjointly, as inspiratory or expiratory muscles. He then proceeds to state the proofs that the intercostal muscles possess an action which is independent of any other muscle, and also independent of each other, so that any of the twelve ribs may be elevated or de- pressed by them either separately or conjointly. He demonstrates the nature of this action by means of models, producing oblique tensions betweeti levers representing the ribs, and allowing of rota- tion on their centres of motion ; and he shows that such tension in the direction of the external intercostal muscles, elevates both the levers until the' tension ceases, or the position of the bars by proxi- mity obstruct each other. If the tension be exerted in a contrary direction, as in the internal intercostal muscles, the bars are both depressed. This movement was demonstrated by a model. It was farther shown that two tensions decussating can, according to the position of the fulcra, be made to act as associates or antagonists to each other. Such motions are to be considered with reference to the fulcra, bars with one fulcrum common to each having no such action ; and the author accordingly draws the following conclu- sions : — 1st. All the external intercostal muscles are true inspiratory mus- cles, elevators of the ribs, and with this act they dilate the inter- costal spaces, thus increasing the cavity of the chest. 2nd. The internal intercostal muscles have a double action; the portions situated between the cartilages are associates in action with the external layer, and act as elevators of the cartilages, while the portion between the ribs are depressors, or antagonists of the external layer, and are here true expiratory muscles ; with this they decrease the intercostal spaces. 3rd. These muscles can elevate or depress the ribs independently of any other muscle, fixing the first or last rib. Any one lamella, or series of muscles, can, as required, independently perform in- spiration or expiration at any one of the twenty-two intercofctal spaces. 4th. In inspiration, the intercostal spaces increase, with a short- ening of the muscle ; and in expiration, they decrease their perpen- dicular distance, with a shortening of the muscle. 5th. All parallel intercostal muscles, acting with uniform force, concur in the same effect, whether near the fulcrum or more distant from it, and these muscles gain power with their increasing obliquity as well as speed. In the third part of the paper an account is given of the differ- ence between the external thoracic space and the internal pulmonic space. The respiratory movements are described in health and disease, and it is shown that tiie chest is rarely enlarged at two places at one and the 9ame time. 224 Royal Society. In conclusion the author conceives that he has established the following propositions : — 1st. Costal breathing may be distinguished from abdominal by determining which part is first put in motion, and the kind of re- spiration may be designated according to the name of such part. 2nd. Healthy costal breathing begins with the motion of a supe- rior rib, which is followed by that of the lower ones in succession. 3rd. Ordinary respiration in men is abdominal, in women, costal ; extraordinary breathing is the same in both sexes. 4th. Any of the ribs, from the twelfth to the first, may carry on respiration. 5th. Diseased respiration is of various kinds ; the movements may be symmetric or not symmetric, costal or abdominal; all or none of the ribs may move ; the abdomen may or may not move ; the chest may dilate in all its dimensions at one and the same time; costal and abdominal breathing may alternate with one another ; costal motion may be undulating or not ; and all these may be combined in one, which the author terms " hesitating breathing ;" and lastly, the quan- tity of air breathed is diminished when there exists pulmonary dis- ease. " On the Structure and Development of the Liver." By C. Handfield Jones, M.B., Cantab. Communicated by Sir Benjamin C. Brodie, Bart., F.R.S., &c. The author gives a detailed description of the structure of the liver in animals belonging to various classes of the animal kingdom. He states that in the Bryozoon, a highly organized polype, it is clearly of the follicular type ; and that in the Asterias, the function of the liver is probably shared between the closed appendage of the stomach and the terminal cteca of the large ramifying prolongations of the digestive sac contained in the several rays. Among the Annulosa, the earthworm presents an arrangement of the elements of the he- patic organ, corresponding in simplicity with the general configura- tion of the body, a single layer of large biliary cells being applied as a kind of coating over the greater part of the intestinal canal. In another member of the same class, the Leech, in which the digest- ive cavity is much less simple, and presents a number of sacculi on each side, these elements have a very diflferent disposition ; and the secreting cells, although some remain isolated, for the most part coalesce to form tubes, having a succession of dilatations and constrictions, and finally uniting and opening into the intes- tine. In Insects, the usual arrangement is that of long curved fila- mentary tubes, which wind about the intestine ; these, in the meat fly, are sacculated throughout the greater part of their course, till they arrive quite close to the pylorus, where they open ; near their origin they appear to consist of separate vesicles, which become gradually fused together, but occasionally they are seen quite sepa- rate. The basement membrane of the tubes is strongly marked, and encloses a large quantity of granular matter of a yellowish tinge, \rith secreting cells ; another portion of the liver consists of sepa- rate cells lying in a granular blastema, which cells, in a later stage Royal Society. 225 of development, are seen to be included in vesicles or short tubes of homogeneous membrane, often coalescing and exhibiting a more or less manifestly plexiform arrangement ; this portion of the liver is regarded by Mr. Newport as really adipose tissue. The author has termed it the Parenchymatous portion of the liver, on account of its general appearance and mode of development, though he has not been able to determine whether the tubes always origi- nate from it. Among the Arachnida, the follicular type of arrange- ment prevails; and the same is the case with the Crustacea, the folli- cles in these last being distinctly visible to the naked eye. In Mol- lusca also, we find the follicular arrangement universally to obtain ; yet in certain cases the limiting membrane of the follicles cannot be shown to exist, and the author therefore thinks that its importance is probably not great, but that it serves chiefly to fulfil the me- chanical function which its synonym " basement" indicates. The quantity of retained secretion in the liver of molluscs seems clearly to imply that the bile in them is not an excrementitious fluid ; it is used slowly on account of the imperfect character of the respira- tion. In passing from the Invertebrata to the Vertebrate division of the animal kingdom, and beginning with the class of Fishes, a great change is inimediately manifest in the form and character of the biliary organ ; it is now a gland of solid texture, to which the term parenchymal is justly applied. Two portions may be distinguished in it, namely, the secreting parenchyma, consisting of delicate cells, or very often of nuclei, granular and elaborated matters in great part, and the excreting ducts, which, though completely obscured bj'- the surrounding bulky parenchyma, may yet be satisfactorily de- monstrated, and traced often to their terminal extremities in the following manner. If a branch of the hepatic duct be taken up in the forceps, it may be dissected out without much difficulty from the surrounding substance, which is very soft and yields readily to gentle manipulation ; when a trunk is in this way removed and placed under the microscope, a multitude of minute ramifications are seen adhering to it ; among these not a few may be discovered, which do not appear to have suffered injury ; some are occasionally seen terminating by distinctly closed extremities ; more usually the duct becomes very minute and gradually loses all definite structure, appearing at last like a mere tract of granular matter ; in either case there is no communication by continuity with the surrounding parenchyma. Large yellow corpuscles, peculiar cells, and a consi- derable quantity of free oily matter usually existing in the liver of various fishes, seem generally to indicate a great superiority in the amount of secretory over that of excretory action, and to betoken clearly the feeble intensity of the aerating function. In Reptiles, there is the same arrangement in the liver, namely, a secreting parenchyma of cells and an apparatus of excretory ducts, which have the same essential characters as those of fishes ; but there exists very frequently in the parenchyma remarkable dark corpuscles, which appear to be masses of retained biliary matter, Phil. Mag. S. 3. Vol. 31. No. 207. Sept. 1847. Q 226 Royal Society. the import of which, in the situation they occupy, is doubtless the same as that of the similar masses existing in fishes. In Birds, the parenchyma of the liver is remarkably free from oily or retained biliary matters; it often consists almost wholly of free nuclei and granular matter, with scarcely a single perfect cell ; the excretory ducts often greatly resemble those of reptiles, sometimes rather those of mammalia; the essential character is, however, always the same, namely, that they terminate without forming any important connexion with the jiarenchyma. In Mammalia, the parenchyma of the liver consists usually of per- fect cells, which are arranged often in linear series of considerable length, radiating from the axis of each lobule ; these unite at variouf points with each other, so as to present a more or less decidedly plexiform appearance. Each lobule, as described by Mr. Kiernan, is separated from the adjacent ones by the terminal twigs of the portal vein, and to a greater or less extent by a " fissure," though in most animals the lobules are continuous with each other both above and below the fissure. The elaboi'ation of the secreted product seems to be most completely effected in the cells adjoining the margins of the lobules, which are often seen to contain a larger quantity of biliary matter than those in the interior, and to be appa- rently in the act of discharging it into the fissure; the margin of the lobule then presents an irregular surface with large globules of the secretion clustering together all over it. The capsule of Glisson surrounding the vessels in the portal canals gives a fibrous invest- ment to those surfaces of the lobules which are towards the canal ; but when it has arrived in the fissures, it forms a continuous mem- brane lining the surfaces of opposite lobules ; this membrane is often truly homogeneous, and closely resembles the basement tissue : there appears occasionally to be a delicate epithelium on its free surface ; but this, as well as the membrane itself, is often absent, when the margin of the lobules is in that condition which has just been de- scribed and which may be termed active. The minute branches of the hepatic duct as they approach their termination undergo a re- markable alteration in their structure ; they lose their fibrous coat, which blends itself with the membranous expansions of the capsule of Glisson ; their basement inembrane becomes gi-adually indistinct, and at last ceases to exist, and the epithelial particles no longer retain their individuality, but appear to be reduced to mere nuclei, set very close together in a faintly granular basis substance. The mode of their termination is not uniformly the same; frequently they present distinctly closed rounded extremities, between one and two thousandths of an inch in diameter; at other times they seem to cease gradually in the midst of fibrous tissue, the nuclei alone being disposed for some little way in such a manner as to convey the idea of a continuation of the duct. These ducts can seldom be dis- cerned in the fissures, but have several times been seen in the " spaces," where several fissures unite ; they do not form anything like a plexus between the lobules. From the anatomical relation of the ducts to the parenchyma, and from the circumstance that a Royal Society. 227 distinct vessel conveying a different kind of blood is distributed to the hepatic duct, as soon as the liver assumes the parenchymal form, it seems probable that the mode in which the secreted bile is con- veyed out of the organ, is by its permeating the coats of the minute ducts in obedience to an endosmotic attraction, which takes place between the bile in which the ducts may be said to be bathed, and a denser (perhaps mucous) fluid formed in their interior. The large quantity of oily matter frequently existing in a free state in the secreting parenchyma of the liver, which must be regarded as a product of secretory action, seems to suggest the idea, that a cer- tain quantity of the biliary secretion may be directly absorbed into the blood, and in this manner conveyed away from the organs, just as occurs in the thyroid body, suprarenal capsules, and other glands unprovided with efferent ducts. With respect to the development of the liver, the author considers the opinion of Reichart to be decidedly the correct one, namely, that its formation commences by a cellular growth from the germi- nal membrane, independently of any protrusion of the intestinal canal. On the morning of the fifth day, the oesophagus and stomach are clearly discernible, the liver lying between the heart, which is in front, and the stomach which is behind ; it is manifestly a parenchy- mal mass, and its border is quite distinct and separate from the digest- ive canal ; at this period, the vitelline duct is wide, it does not open into the abdominal cavity, but its canal is continued into an anterior and posterior division, which are tubes of homogeneous membrane, filled, like the duct, with opaque oily contents ; the anterior one runs forwards, and forms behind the liver a terminal expanded cavity, from which then passes one offset, which, gradually dilating, opens into the stomach; a second, which runs in a direction up- wards and backwards, and forms apparently a caecal prolongation ; and a third and fourth, which are of smaller size, arise from the anterior part of the cavity and run to the liver, though they cannot be seen to ramify in its substance ; at a somewhat later period, these offsets waste away, excepting the one which is continued into the stomach, and then the mass of the liver is completely free and un- connected with any part of the intestine. As the vitelline duct contracts, the anterior and posterior prolongations of it become fairly continuous and form a loop of intestine, the posterior division being evidently destined to form the cloaca and lower part of the canal. The final development of the hepatic duct takes place about the ninth day by a growth proceeding from the liver itself, and Consisting of exactly similar material ; this growth extends towards the lower part of the loop of duodenum, which is now distinct, and appears to blend with the coats of the intestine ; around it, at its lower part, the structure of the pancreas is seen to be in process of formation. The further progress of development of the hepatic duct will, the author thinks, require to be carefully examined, but the details he has given in this paper have satisfied him of the cor- rectness of the statement that the structure of the liver is essentially parenchymal. Q2 [ 228 ] XXXIX. Intelligence mid Miscellaneous Articles. SUGGESTIONS FOR THE OBSERVATION OF THE ANNULAR ECLIPSE, OCT. 9, 1847, MADE BY THE BRITISH ASSOCIATION FOR THE ADVANCEMENT OF SCIENCE, OXFORD, JUNE 2(), 1847. n[ "^HE following directions and suggestions, relative to the ensuing -■- annular eclipse of the sun, which will take place Oct. 9, 1 847, are proposed for the assistance of less-practised observers, or those who may not have better information at hand, but who may nevertheless render great service by noticing and recording, as well as circum- stances permit, any of the various points herein alluded to. I. As a general direction as to the limits within which the eclipse can be seen annular in England and Ireland, if on any map a line be drawn through Greenwich and Gloucester and produced, it will give the northern limit at which the eclipse ceases to be annular. A line parallel to the last, through Padstow in Cornwall on the west, and Torbay on the east (which will extend across the channel to Havre, &c., and passes just below Cape Clear on the west), will be the line along which the eclipse is both annular and central. The southern limit lies wholly below England. II. As a rough guide to the time, the commencement of the an- nulus will be nearly at 7** 23™ a.m. (civil reckoning) for the extreme south-west of Ireland, at 7** 24"^ for a line through Land's End and Milford Haven, at 7^* 2.5"" through the Isle of Wight and Reading, at 7^* 25"" 50^ forWalmer (Greenwich mean time). III. For the observations requisite, a telescope of very moderate power is best. As the annulus will not last more than three or four minutes, those unaccustomed to such observations should be cau^ tioned against attempting to observe all the phsenomena, or they may thus run the risk of observing «OMe. If possible several observers should combine for the purpose, and each agree to attend to one, or some few of the phsenomena. IV. To obviate some of the difficulties arising from the rapid passage of the phsenomenon, the observer may be referred to Capt. Smyth's Cycle (i. 141, 146), where some valuable practical hints are thrown out for tranquillizing the observer's nerves in so transitory a phsenomenon ; especially by previously making a careful drawing of the spots (if any) existing on the sun's disc, which may be made useful in marking and ascertaining the progress of the ecHpse. V. With the view of correcting the moon's tabular north polar distance and semidiameter, it is peculiarly desirable that observations should be made along or near the line (passing through Greenwich and Gloucester) on which the eclipse is barely annular. At some of these the echpse will be completely annular, and here the follow- ing observations should be made : — The time of beginning of annularity and end of annularity should be observed. As the duration only is required, a common watch showing seconds will suffice for this purpose. Intelligence and Miscellaneous Articles. 229 If possible, by means of a graduated pearl scale or other equivalent means, the breadth of the narrowest part of the annulus should be measured several times about the middle of the time of the annular appearance, as well as it can be estimated. At other places the eclipse will not be completely annular, and here the principal object must be to make several measures of the distance between the cusps about the time when that distance is smallest. This measure may probably be made by means of a gra- duated pearl scale, or by means of a divided object-glass applied in front of the object-glass of the telescope, or by the use of a common sextant. VI. As to the particular points of physical interest to which at- tention should be directed, they may be stated as follows : — 1 . It will be desirable in general to notice the fact of the appearance of what are denominated " beads " and " threads " by the late Mr. Baily and others, just before and after the completion of the annulus. For details of older observations the observer should consult Ast. Soc. Memoirs, i. 142-146, x. 10-17, 33-38. The beads were observed by Mr. Baily, ib. x. 210, in 1842, when they were not seen by Mr. Airy, ib. x. 218. They were observed by Prof. Henderson at Edinburgh. Ast. Soc. Notices, v. 186. 2. Whether in the neighbourhood of the cusp the limb either of the sun or moon appears distorted ? Whether the beads appear steady or waving, disappearing and reappearing, &c. ? See the observations of Mr. Caldecott at Trevandrum, Ast. Soc. Notices, vi. 81. Whether they present any peculiar changes when viewed through differently coloured glasses, the observer alternating the colours, which should be as dissimilar as possible, such as red and green ? See Silliman's Journal, Jan. 1842. 3. Whether they are seen when the eclipse is projected on a screen? In this way Prof. Chevallier saw none when others with coloured glasses saw them. Ast. Soc. Notices, v. 186. 4. The drawing out of the beads into threads when very near junction; and whether they waver and change, and the number of them? See Ast. Soc. Mem., x. 15-17, 39 ; waving and changing, ib. x. 12, 13 ; not seen in 1842 by Mr. Baily, Notices, v. 210. 5. Whether before and after the formation of the threads the moon's dark disc is elongated towards the point of contact ? This was observed, ib. x. 29 ; and wavy motion in the limb, ib. X. 12, 14, 30. 6. The beads are ascribed by some to lunar mountains : What mountains exist at that part of the limb ? See Ast. Soc. Mem., X. 9, 16, 30-36. 7. The exact intervals of time elapsed between the first and last complete contact, and that of the first and last formation of beads or other irregularities in or about the cusps, should be determined. The difiference of the times being all that is wanted, a good ordinary watch will be sufficient. 230 Intelligence and Miscellaneous Articles. The remarkable fact of a recurrence of cusps observed by Mr. Airy in 1842, and his explanation of it, should be attentively coneidered. See Ast. Soc. Notices, v. 296. 8. If possible, accurate measures should be taken of the apparent diameter of the dark disc of the moon upon the sun, which may be expected to be greatly less than the truth, owing to the irradiation of the sun's light. 9. It should be noticed whether any external luminous arch is formed over the part between the cusps, a little before the first junc- tion and after the final separation, and the colour of the light. It was observed, and appeared brown to De Lisle (Phil. Trans., 1748, 490), reddish in other cases (Ast. Soc. Mem., i. 144, X. 37), Siadi purple in others (ib. x. 16). ON THE PREPARATION AND COMPOSITION OF THE SALTS OF ANTIMONY. BY M. E. PELIGOT. Sulphates of Antimony. — When oxychloride of antimony (CI Sb^O-) is treated with hot concentrated sulphuric acid, a salt is formed which is deposited in acicular crystals, hydrochloric acid being at the same time evolved. This salt, as well as another sulphate to be described, can only be obtained in a dry state by long remaining in vacuo, or in perfectly dry air upon porous plates of pipe clay. These plates were heated to redness before the crystalline magma was placed upon them, and they were left to cool in air deprived of moisture. This method of drying yields products which usually contain a slight excess of sulphuric acid. If however the points of contact between the salt to be dried and the absorbent earth be re- newed from time to time, and the absorption goes on for several months, compounds of sufficient purity to remove all doubts of their true composition may be obtained. One hundred parts of the sulphate of antimony, obtained by com- mon sulphuric acid and oxychloride of antimony, gave — Sulphuric acid 51*9 Oxide of antimony (by carbonate of ammonia) .... 50*2 The composition of this salt is therefore — 4S03 2000 51-2 Sb^O* 1912 48-8 3912 100-0 Another specimen gave 53* 1 of sulphuric acid, and 44'3 of oxide of antimony. Another sulphate of antimony was obtained in the form of small brilliant crystals, by treating sesquioxide of antimony with Nord- hausen sulphuric acid. After remaining ten months on the dried clay, it gave — Sesquioxide of antimony .... 63"0 643 Sulphuric acid 37"1 35*0 The formula 2S03, Sb® O^ gives 65 "6 oxide of antimony and 34*4 sulphuric acid. Mixtures of these salts in different proportions were also obtained ; Intelligence and Miscellaneous Articles. 231 but no analysis indicated the existence of the compound 380^, 5Sb'-03, which, according to Berzelius, would be the neutral sul- phate of antimony. On treating the above-described salts with hot water, a subsalt is obtained, the composition of which is represented by the formula — Calculation. Experiments. 2Sb2 0' 3824 88-4 88-6 S03 '.. 500 11-6 11-4 4324 100-0 100-0 The analysis of two other specimens is correctly represented by the formula 2Sb2 O^, SO^, 2H0. Nitrate of Antimony. — This salt was obtained in the form of pearly crystals by dissolving the oxide in cold fuming nitric acid, and adding water to the solution. Its composition is 2Sb- O^, NO*. Oxychlorides of Antimony. — Powder of Algaroth was prepared by treating chloride of antimony with cold water. After some days the mass became crystalline ; when well- washed its composition agreed with the analyses which have served to fix the formula of this com- pound. This formula is more simply replaced by CI Sb- 0'^ When the sesquichloride of antimony, or rather the sesquioxide dissolved in a great excess of hydrochloric acid, is treated with hot water, another oxychloride is obtained, which, on the cooling of the liquor, precipitates in dense brilliant crystals. Its composition is represented by the following formula : — Calculation. Experiments. CI 443 10-6 11-1 11-4 4Sb 3224 77-3 76-5 76-8 O' 500 12-1 4167 100-0 This compound consequently must here presented by the formula, ClSb^O'^ + Sb^Os. Tartrates of Antimony. — By allowing a syrupy solution of tartrate of antimony, obtained by dissolving the oxide of the metal in tartaric acid, to remain for a long time, large transparent crystals of tartrate of antimony were obtained. The mother- water, after the separation of the crystals, furnished more afterwards by spontaneous evapora- tion. This salt is very soluble in water. It is deliquescent in a moist atmosphere. Its composition is represented by the following for- mula : — Calculation. Experiments. , ^ . C'6 1200 19-6 18-9 19-0 H'G 200 3-2 3-5 3*5 028 2800 46-0 Sb«03.... 1912 31-2 31-5 6112 100-0 At 320° F. this salt lost 23-1 per cent, of water. 232 Intelligence and Miscellaneous Articles. On decomposing the formula as follows, the loss of twelve equi- valents of water represents 22 per cent, of the weight of the salt — 2CsH2 08,Sb2 03, 12H0. On pouring alcohol into a concentrated solution of the acidulous tartrate of antimony, a precipitate is obtained which, when dried at 320° F., yielded 16*4 of carbon and TS of hydrogen. The compo- sition of this salt is represented by the formula C^ H'^ O^, Sb^ O^, HO, which requires 17*2 of carbon and 1 of hydrogen. The salt which M. Peligot analysed contained a little more water than the quantity required by this formula, but not enough to allow of the addition of another equivalent. Acidulous Tartrate of Antimony and Potash. — This salt was de- scribed by M. Knapp, who obtained it by mixing solutions of tar- taric acid and tartarized antimony. The salt which was analysed by M. Peligot was in very regular crystals. It yielded — Carbon 19-5 18-7 Hydrogen 2-7 2*7 Sesquioxide of antimony 3 TO The formula C'^ H* O'^, Sb^ O^, KO, 8H0 represents its composi- tion. It gives — Carbon 19-1 Hydrogen 2*3 Sesquioxide of antimony . . 30"5 According to M. Knai)p it contains one equivalent less of water. Oxalate of Antimony. — M. Peligot prepared this salt by four pro- cesses : — 1st, by boiling in a solution of oxalic acid oxide of antimony prepared from the chloride by carbonate of ammonia ; 2nd, by treat- ing the powder of Algaroth with oxalic acid ; 3rd, by pouring hydro- chloric acid into a hot solution of the double oxalate of potash and antimony ; the oxalate of antimony precipitates in the state of a crystalline powder ; 4th, by adding oxalic acid to a solution of the same double salt. The oxalates of antimony obtained by these processes are similar in composition. The author attempted, but in vain, by varying the proportions, to obtain other compounds of oxalic acid and oxide of antimony. This salt is crystalline and insoluble in water. It is decomposed by boiling water into oxalic acid, which dissolves, and sesquioxide of antimony- Its composition is represented by the following formula, : — Calculated. Experiments. , ^ . C-* 300-0 10-2 10-1 10-6 10-6 06 600-0 20-6 Sb203 .... 1912-9 65-4 66-7 65-6 HO 112-5 3-8 3-8 4-5 40 2925-4 100-0 Double Oxalate of Potash and Antimony. — The preparation and analysis of this salt are very difficult. The salt obtained by M. Pe- Intelligence and Miscellaneous Articles. 233 ligot was crystallized in transparent prisms ; it is readily soluble, and is decomposed by a large quantity of water. The quantity of water in this salt appeared to vary from unknown causes, but apparently dependent on the temperature at which the salt crystallizes. The formula appeared to be 70^ O', Sb^ 03, 3K0, 6H0. This gives as the composition of 100 parts of the salt — Carbon 13-9 Water 90 Oxide of antimony 25*7 Potash 23-5 M. Peligot obtained — Carbon 13-7 14-3 14-4 14-0 Water 9-7 9-2 lO'l 8-9 Oxide of antimony 25-7 26-2 24-8 A7in. de Ch. et de Phys., Juillet 1847. ACTION OF HYDROCHLORIC ACID IN THE FORMATION OF OXALIC ACID. M. Kopp states that the presence of hydrochloric acid in nitric acid is peculiarly favourable to the formation of oxalic acid. The resins of benzoin andTolu, treated with pure nitric acid, yield no oxalic acid ; but with an impure acid it is obtained. Pure nitric acid occasions the formation of terebic acid only, in acting upon oil of turpentine, and to oxypicric acid, in oxidizing the gum-resins. By using nitric acid containing much hydrochloric acid, oxalic acid only is obtained under the same circumstances. — Ibid, Juillet 1847. PROJECTION OF ALDEBAKAN ON THE MOON. At the British Association in Oxford a question arose respecting the apparent projection of Aldebaran on the disc of the moon in occultations. Pi-of. Airy and Dr. Forster stated having seen this phaenomenon, which Prof. Struve seemed disposed to attribute to to some mal-adjustment of the telescopes. On looking back, how- ever, to the Philosopliical Magazine, it will be found that this ap- pearance has been three or four times recorded ; as well as some other circumstances calculated to show that the light of different stars is very differently refracted. See Phil. Mag. for April and May 1824. THE PUFF PARLIAMENTARY:— DISINFECTION. The art of puffing has not yet exhausted its resources ; and a Parliamentary Report well got up, printed at the expense of the public, and from which extracts may go the round of the news- papers, seems to be the last and boldest device for the purpose, which however has been fearfully exposed in the Dublin Quarterly Journal of Medical Science. The Times newspaper in a leading article of the 20th of August, felicitates itself on having " the pleasant task of giving what publi- city it may to a discovery made by a French gentleman, M. Ledoyen, SS4 hitelligence and Miscellaneous Articles. a Parisian chemist, in concert, it would appear, with a Mr. F. C. Calvert, who seems to have received his education as a chemist at Paris, and who is now lecturer at the Royal Institution of Man- chester. This discovery, which, under the auspices of Lord Mor- peth, has been submitted to the most searching tests by Dr. South- wood Smith, Mr. Toynbee and Mr. Grainger, promises fair to be one of the greatest boons ever conferred on suffering humanity. The discovery is nothing less than the means of disinfecting all foetid animal substances and gases by a liquid which is very cheap, simple, and can be applied by any person with the greatest facility. " The three medical gentlemen appointed by Lord Morpeth to inquire into the real value of M. Ledoyen's discovery, present us in their report with a dismal catalogue of the offensive and dangerous vapours from animal and vegetable substances which at all hours infect the air we breathe, in a greater or less degree, accordingly as we moreor less neglect their impure origins." "The Commissioners state that they have tried the effect of this fluid, — 1, on substances already in a state of decomposition ; 2, on substances undergoing that process ; 3, on night soil ; 4, on impure air. In every instance excepting the second these experiments have been attended with the most miracidous result." *' It would almost seem that some mysterious power had sent us M. Ledoyen and his discovery to compensate for the shortcomings of the Premier and Lord Morpeth*." So far The Times. — We now give a few extracts from the Dublin Journal, and refer our readers to the article which it contains for the details of the means by which these puffs have been procured, and for a full account of the matter. This boasted discovery professes to furnish "the means of disin- fecting all foetid animal substances and gases by a liquid which is very cheap, simple, and can be applied by any person with the greatest facility. It disinfects night-soil, not destroying but in- creasing vegetation, more particularly as regards agriculture, com- pletely preventing the disease in potatoes when the land is manured with disinfected night-soil. It disinfects hospital-wards of miasma ; also cellars, water-closets, and buildings infected by impure gases. It disinfects sailors suffering from fever on board of vessels ; it will also disinfect ships at sea, and under quarantine. It disinfects patients suffering with infectious disorders and wounds, also dead bodies, so that they may be kept nearly a month ; also different parts of the body can be kept for the purposes of dissection, for coroners' inquests, &c." * No wonder that competitors should have started up asserting their claims to 80 wonderful a discovery. Mr. W. Maddick thus begins his letter to the Editor of the Times; of whose judgement in matters of science he seems to have a most exalted opinion: " Siu,— All the world knows that a laudatory notice in your columns is a very high honour; and as in your excellent leader of yesterday you have highly eulogized Messrs. Ledoyen and Calvert for their alleged discovery, I appeal with confidence to the proverbial justice ofThe Times, • fe s J s s •wd I •JiatMsiqj oj oJ aJ lu „; g: g:* • S: ^' ^ ^ fe > ,; J 2 ,; g oj ^ jj ^ 2 u CI wtei phIct »^!« F-!« Mte* --lei Mid ^Ici iHjci tH!« t^vo t:^t^r^t--io*ovo r^iovo^o r~i>.>0'0 c^t>.« i>>vo*o*o r^c^toio^oo^o •lU'B ^8 •uoisoa n 0=2 •«!W XBIM c<5^cofOcoa\oooooocri'NooooiO'troioioci>-T)'cx)oo -wg cotN--O^C^ooc^<»QpO^O•7'l7-7OOC>OOO^O^c^C^0000^0^0^0^0^2> QDQOOlO•^pp90^g^9opg^c»op 0000^6^0^0^0^0^6^0^C>OOOCOOO^O^O^O^OOO^O^OO^O^O^O^ •tu*8 ?8 •uoisoa JO sXbq t>-ao o o\o O 0^c^ Qp r~Qp C^ 0^ 0^ (M ' . 00 -^ ' Tf 00 o c^ t^CO o op 6 CTi COCN oo""od^ CO CO O 0^ 6 a\ cod lO !>• O «3 «3 CSI 00 00 O 1 O CN -^ to (N I ^O -^ lO ; O O O I o ao r~ qc CO -^ ^^ ON o (N CI CO 00 (yi CI 7< 6 6 coco r-oo 0^0 irjQO ys o o o 6 6 6 CO CO CO lOOO COLO o o ^ ci co'*in« rioo a.6 -^ 2 co^invd r^* O'S S gi c5d d d d d d oo ^ A (^ O THE LONDON, EDINBURGH and DUBLIN PHILOSOPHICAL MAGAZINE AND JOURNAL OF SCIENCE. [THIRD SERIES.] OCrOBRR 1847. XL. Fourth Memoir on Induction. By M. Elie Wart- MANN, Professor of Natural Philosophy in the Academy of Geneva *. [With a Plate.] [Continued from vol. xxx. p. 272.] § XIV. On the Commutators employed to render noltaic cur' rents discontinuous.^ and to separate currents of induction, 116. TT is exactly a century since a remedy for various ail- Jl ments was first sought in the electric fluid. The first experiments were made at Geneva by Prof. Jallabert in IT^Tt* At a later period, when the voltaic battery was invented, its physiological effects were studied, and they are now employed for the cure of various affections, such as obstinate ulcers J, dumbness§, deafness II, blindness^, tic-doIoureux**,paralysisff, &c. Lastly, since the discovery of magnetic and electric in- duction in 1831 by Mr. Faraday, it has been found that the induced currents, as well as the electrical discharges of the Leyden jar, have an extremely short duration, and produce greater shocks than batteries of a large number of elements. The idea therefore has occurred of rendering the current of the electromotor apparatus discontinuous, to approximate it * Communicated by the Author. \ Experiences sur I' Electricite, p. 127. 8vo. Geneva, 1748. J Becquerel, Traiie de P/ii/sique,vo].'n. p. 638. Paris, 1844. § Namias, De alctini effetti delV elettnco sopra I Animate Economia, &c., p. 27. Venice, 1841. 11 Giornale per servire ai progressi delta Patologia et delta Terapeutica. Gennajo, 1843, p. 108. Giornale delle Scienze Mediche di Torino, vol. iv. p. 430. ^ Giornale per servire, &c.,'DecQmh&t 1841, p. 658. Biblioteca Italiana, fascicolo 25, p. 12, &c. ** Zantedeschi, Trattaio delta Elettricitd, vol. ii. p. 525. tt Giornale di Fisica, S^c. di Pavia, decade II. vol. vii. p. 284 ; and vol. viii. p. 219. Annali delle Scienze del Regno Lombardo-Veneto, January and February 1833, &c. PhiL Mag. S. 8. Vol. 3L No. 208. Oct. 1 847. R 242 Prof. E. WaYtm&nn' sjburth Memoir on Induction. to the cases of induced currents. Dr. NeefFof Frankfort on the Maine, in 1835*, and M. Masson in the following yearf, have made very conclusive experiments on this subject. An instrument described by M. Poggendorff under the name of inversorX, is intended to render the current of an ordinary battery at the same time discontinuous and in an alternate direction through a given conductor. 117. At the present day the employment of induced cur- rents seems to become more and more general. In place of the original magnets employed in the apparatus of Ritchie§, Pohl||, Pixii^, Saxton**, Clarkeftj StorerJ:}:, and others, a simple voltaic pair has been substituted, and an instrument has been constructed, of small size, easy of transport, and producing almost unlimited effects, called an electro-electric machine, or a shock-machine. M. Bonijol constructs this machine with such perfection that it has been generally adopted, and there is at the present day scarcely an hospital where it is not found. It is employed in the treatment of a multitude of nervous affections; in that of amaurosis§§, in assisting parturition ||||, and as a dia- gnostic to ascertain the state of vitality of the foetus. 118. I have had more than one opportunity of convincing myself that many persons make use of the shock-machine without understanding either its construction or its theory. This maciiine, arranged on a different plan, might be rendered both more intelligible in its mode of action and more useful to the physicist and the physiologist. I will point out some of the cases in which it may be employed, and afterwards the arrangement applicable to each of them. 119. A voltaic current being given, it may be proposed — 1. To render it discontinuous, without changing its direc- tion, in a conductor a ; * Das BUtzrad, ein Apparat zu rasch abwechselnden gnhanischcn ScklieS' sungen und Trennungen. Pogg. Ann., vol. xxxvi. p. 352, and vol. xlvi. p. 104. f Comptes Rendus de PAcad. des Sciences de Paris, vol. iv. p. 456. X Pogg. Ann., vol. xlv. p. 372 and 385. § Phil. Trans., Oct. 1833, II Pogg. A/m., vol. xxxiv. p. 185 and 500. H Ann. de Ch. et de Phi/s., vol. 1. p. 322. ** Phil. Mag. N. S. vol. ix. p. 360. ft Ibid. p. 262. XX Pogg. Ann , vol. Ixi. p. 417, 1844. §§ Cunier, Dr., Annates d' Oculistique, vol. xii. and vol. xvi., where will be found a memoir by Dr. Hcering On the Employment of the Electro-mag- netic rotatory apparatus in Diseases of the Eyes. nil See on this subject, P. Kerz, De ctcctro-viagvetisvii vi et iisu in arte obstetricia. Bonn, 1846. — J. A. Schmidtmuller, Ilandbuch der medizinischen GcburtsJiulfe. — T. Radford, Galvanism applied to the treatment of uterine Haemorrhage. Manchester. — Von Kilian, Die Geburtslchre von Seiten der Wissenschaft und Kunst, — Neue zeitschrift fiir Gcbtirtsfcunde, von H. Bursh, d'Oiitrepont, &c., vol. xvi. No. 26, &c. Prof. E. Wartmann* s^^ntrth Memoir on Induction, 243 2. To render it discontinuous, and in alternately contrary directions. This current being employed to react on a wire B, near the conductor A, it may be required — 3. To isolate the direct currents, induced from the closing of the circuit A ; 4. To isolate the inverted currents, induced on breaking this circuit; 5. To emit these currents successively, giving them the same direction ; 6. To emit them alternately in contrary directions, just as they are produced directly. It is known that there is a reaction of the induced currents on the principal current. We may therefore desire — 7. To collect the totality of their reaction; 8. To avail ourselves only of the reaction of the direct in- duced currents; 9. To avail ourselves only of that of the inverted induced currents ; 10. To collect only the induction of the inductor on itself. 120. Physicists have studied the majority of these cases; but the mechanical instruments which they have imagined and described under the names of disj'unctor^, tachytrope\, rheo- tropeX, gyrotrope^^ or co7nmutator\\, are scarcely applicable except to one or other of the first two categories. The most complete of these instruments, reinvented in Paris seven years after having been described and employed in Germany, is composed of four isolated wheels on the same axis, the outline of which presents successively metallic and ivory arcs, against which press conducting springs. The axis is set in motion by means of a handle or tooth-wheel. Sometimes the interval of the teeth is left void, and the spring in escaping determines the opening of the circuit. Other commutators are formed with needles arranged on isolated axes, in such a manner that one is immersed in mercury at the instant when the other * Dove, Magneto-elektrischcr Apparat zum Hervorbringen inducirter Strome gleicher hitensitdt in von einander vollkommen getrennten Dr'dhten Pogg. Ann., vol. xliii. p. 51 1 . ] 838. "^ Dove, Ueber den Gegenstrom zu Avfang tend Ende eines prim'dren, Pogg. Ann.y vol. Ivi. p. 251. X Masson et Breguet, Memoirc sur ^induction. Ann. de C/i. et de Phys.t vol. iv. p. 134. 1842. § Pogg. Ann., vol. xxxii. p. 539 ; and vol. xxxiv. p. 18S and 500. 1834-35. II Jacobi, Sur P application de V Eleclro-magnetisme au monvement des via- chines, § VII. Potsdam, 1835. Taylor's Scientific Memoirs, vol. i. p. 503, 4rcMvc'8 de PElectr., vol iii. p. 244. R2 244- Prof. E. Wavtmann' sjburth Memoir on Induction. comes out of it*. These different systems are complicated, and subject to several inconveniences. The rheotrope, which I shall proceed to describe, and which is especially applicable to electro-electric machines, combines with the advantage of * On the 18th of June, 1840, I communicated to the Society of Physics and Natural History of Geneva an apparatus of this kind, the construction of which presents no difficulty, and which is deposited in the Cabinet of Physics in the Academy of Lausanne. The following is a description of it : — " My commutator is composed of a pure copper stem a b (Plate II. fig. 1), intersected in the middle by a piece of ivory c : the latter is hollowed into the nut of a screw, in such a manner that the two halves of the stem screw into it. Between these metallic extremities some sealing-wax is run, in order to isolate them entirely. The cylinder thus formed is arranged ho- rizontally, and each of its branches is furnished with symmetrical pieces at equal distances. These pieces are two copper teeth ef, placed perpendi- cularly and at a right angle on the axis ; then a copper circleg. Lastly, to one of the extremities of the stem is fixed a pulley h, m the groove of which there runs a ccrd i, which again passes over a lower pulley k, which is much larger, vertical, and moveable by means of the handle m in one of the supports of the apparatus. "The six projecting pieces of copper dip into a glass vessel w (fig. 2), placed on two small horizontal barso; it presents six isolated compart- ments full of mercury. The extreme circles remain immersed in tliis liquid during the entire rotation of the stem, the arrangement of the teeth causing one to be immersed whilst the neighbouring one is not. It is easy to regulate the quantity of mercury in the troughs so that the immer- sion of the one may correspond exactly to the exit of the other. " Supposing it be desired to emit into a rheometer the two induced cur- rents, giving to them the same direction, it is sufficient to bring the extre- mities of the wire in which the induction is produced in the extreme com- partments reserved for copper circles. The ends of the wire of the mul- tiplicator are tied to bars of copper connecting the troughs ef, ef, cor- responding on the right and left of the isolator c to the needles fixed at a right angle. So likewise on connecting the extremities of the rheometric wire only with the troughs//, or with the troughs e e, it is evident that the direct or inverted induced currents only may be collected. " I have combined with this arrangement one which M. Bonijol has employed in some of his apparatus. It consists (fig. 3) of planting one of the ends of the stem in a flattened wooden cylinder ?•, on which a spring s presses, passing into a circular cylinder t of hard wood, and the free extre- mity of which u is placed by the rotation of r in contact with an amalga- mated metallic capsule x, or is removed from it. Then, by connecting the spring on one side, and the capsule on the other, with the wire which the direct current of the pile traverses, we obtain by the simple rotation of the stem any number of inductions. "This apparatus enabled me to discover that the thermo- electric cur- rents are capable of induction like the hydro-electric currents. I employ a single bismuth-antimony pair, the solder of which is kept at 100° by steam. The bismuth extremity is connected with the spring s, the antimony ex- tremity with a wire covered with silk, which makes seventy turns on a frame, and terminates at the capsule x. On the same frame is rolled an isolated and finer copper wire which makes 1200 coils (110.), and both ends of which terminate in the troughs p q. The induced circuit is closed by a very delicate rheometer (5 a), which deviates five degrees and more, Prof. E. Wartmann's/owr^i^ Memoir on Induction. 245 being more simple, and consequently less subject to derange- ment, that of not requiring the employment of mercury, and of serving to solve all the cases above stated. 121. H (Plate II. fig. 4) is a reel on which two insulated wires are wound ; one the inductor A, by which the current of the battery j9 n is made to pass; the other the induced B, intended to become the seat of the currents of induction. Three brass wheels r, 5, t, of the same diameter, are isolated from one another on a common axis; their circumference pre- sents an equal number of parts alternately of metal and wood. Two metallic springs a, b are fixed against the wheel r, in such a manner that the first leans against a conducting arc, and the other against an insulating arc. The wheels s and t are each pressed by two springs c d, ef^ similarly arranged. The central metallic parts of the three wheels are in constant communication with the springs ^, ^, i. 122. If it be desired to collect the voltaic current always in the same direction after having rendered it discontinuous, it is sufficient to connect the spring / with the pole p by a wire «, and the other pole n with the spring^ by means of any con- ducting wire different from the wires A and B wound upon the reel. If it is wanted to obtain, as with the inversor, the discontinuous current in directions alternately contrary, we must join the springs c and e as well as the springs d and/j and then connect the extremity of the conjunctive wire of the battery with the spring h. 123. When it is desired to employ currents of induction, the contact of the extremity / of the inducting wire with the pole w is established permanently, and that of the extremity m with the spring/*. Now, to isolate the direct currents induced at the closing of the circuit A, we have only to connect the ends x and y of the wire B respectively with the springs h and g. — To isolate the inverted currents, we unite .r with h and y with d. — To cause the direct and the inverted currents to pass one after another in the same direction through the rheometer G, for example, we connect the springs a and c with the end s of the wire of the instrument, the springs b and d with the end t, the extremity x with the spring h, and the extremity y with the spring g. — To collect the induced currents alter- nately in contrary directions, just as they are produced directly, when it is traversed by direct and inverted currents in the same direction." (See the Transactions of the Helvetic Society of Natural Sciences for 1840, pp. 173, 195.) Prof. Dove has demonstrated thermo-electric induction by a different process. His researches were made at the same time as mine, and in an independent manner. (See Pogg. Ann., vol. xlix, p. 97* 1840.) 246 Prof. E. "WaYlmann'sJourth Memoir on Induction. we disconnect the extremities .2? and y of the wire B from the springs of the rheotrope. 124>. Lastly, if we propose to employ the reaction of the induced wire B on the inductor A, and that of the inductor wound in a helix on itself, we substitute for the wire a the body which is to be subjected to the effects of these reactions. We then employ one of the four arrangements above described (123.), according as we wish to obtain the totality of influence of the two currents induced in the same direction, or in di- rections alternately opposed, or again, the separate influence of the direct or the inverted currents. The simple induction of the inductor on itself is obtained with a reel with a single wire in place of the conductor a, and the arrangement de- scribed (122.). 125. It remains for me to give some details on the con- struction of the rheotrope. The three metallic wheels r, 5, t (fig. 5) present on their periphery twelve hollows filled in with hard wood. These heterogeneous wheels have been worked together by the lathe ; they are each C^'SO in diameter, and 0'^"Q6 in thickness. A metallic tooth of the middle wheel s exactly corresponds to one isolating part of the extremes r and t. They are placed on the same brass axis /cl, v/hich is turned by a winch ti or a tooth-wheel. The spring / and the wheel t are in metallic contact with the axis. The wheels r and 5 are, on the contrary, each isolated from it by an ivory ring covered externally with a brass cylinder. These two cylinders bear the wheels, and are constantly pressed by springs g^ /i, which embrace them on a semi-circumference. The three springs^, ^, i terminate on the three heads ^>', h', i', by means of which they can communicate together. Lastly, the six springs a,b,c,cl,e,J'iire made of plates of hammered copper; they are fixed to the base of the instrument by screws, ?',s',^', the heads of which, similar tog', and pierced like them with two holes, can receive the metallic wires intended to establish a connexion between the different wheels. These springs are cleft in order that the groove may facilitate the adjustment of their length. Above they bear a screw (fig. 6) in the part which has to rest on the circumference of the wheels ; the opposite notch allows of regulating the elasticity of the spring and the degree of friction. The play of these pieces may thus be regulated with minute precision. 126. If it is not wanted to impart the same direction to the two induced currents, the apparatus may be simplified by giving it only two wheels. One is reserved to render the cur- rent of the battery intermittent; the other is joined to the in- duced wire; and according as there is coincidence or alter- Prof. E. Wai'tmann'sj^?^rM Memoir on Induction. 247 nation in the closing of the two circuits, only either the direct or the inverted currents are received. This double effect may be obtained by changing the point of contact with one of the springs, or by varying the position of one of the wheels on the axis relatively to the other. Two wheels do not permit of giving the same direction to the direct and the inverted cur- rents ; because as it is evident that the induced circuit must communicate with the two wheels when the principal current is closed, a part of this current may proceed from the wire of induction and modify the effect of the direct induced current. 127. Lastly, if it be desired to isolate only the inverted in- duced currents, the rheotrope may be reduced to a single wheel. It is sufficient for the proposed object to open the induced circuit when the inducting circuit is closed, and vice versa. But this arranijement would not be suited to isolate the dn-ect induced currents, because it would be necessarj' to close simultaneously the two circuits, and the voltaic current would be propagated in the double channel presented to it. 128. It will be found convenient to mark letters on the dif- ferent pieces ^, h\ i', r', s', t\ and to repeat them at the extre- mities of the metallic conductors employed to connect these pieces. These conductors will be fixed to the interior of the lid of the case which contains the whole electro-electric ma- chine; and a brief direction will indicate which ought to be employed to produce the effects corresponding to the differ- ent possible cases. 129. It is understood that the commutator with three or with two wheels is applicable to all magneto-electric machines, telegraphs, clocks, &,c., whose motive principle is the electri- city of the magnet or of the battery. § XV. Employment of induced currents to restore sensation. ISO. The cases of nervous weakness which have yielded to a judicious application of electro-physiological shocks and discharges are too well ascertained to admit of any question. Since the marvellous effects of aether have been known, I have proposed to several physicians the employment of the electro- electric machine, or at least of intermittent currents of very short duration, to obviate the dangers which the injection of too strong a dose of this liquid, or a too prolonged inhalement of it, might produce. I have made some experiments* with a view to verify the accuracy of my expectations; and although they are so few as to require to be repeated and varied, I shall * In company with Dr. A. P. Prevost, and Mr. Schnetzler. I take this opportunity of thanking these gentlemen for their zealous cooperation. 248 Prof. E. Wartmann^s fourth Memoir on Induction. give them here, because similar results have recently been announced by M. Ducros*. 131. The animals subjected to experiment were a rabbit three months old, a chicken nine months old, and some frogs of both sexes. They are all very sensitive to electric shocks. The action of aether upon them is also very powerful, espe- cially on the frogs, which should not be moistened with this liquid. 132. The rabbitand the chicken appeared to have recovered their sensation sooner under the influence of the shocks of induction than by simple exposure to the air. In the frogs no difference in this respect was remarked. 133. The aetherization was effected by plunging the animal into a glass cylindrical vessel, in which boxes were arranged furnished with sponges moistened with aether ; it was covered with a piece of linen dipt in water. The internal atmo- sphere was removed from time to time by removing the co- vering. 134. The most remarkable case was presented by the chicken. A quantity of aether, more than sufficient to produce insensibility, was injected into its rectum. When it arrived at this state, two or three shocks of the electro-electric appa- ratus (110.) were passed from one wing to the opposite leg, which shocks were effected by a Grove's pair; immediately the eyes opened. On continuing the discharges in a very inter- mittent manner, the animal was seen to struggle, to rise on its feet, and then to fly to the end of the laboratory, relapsing gradually into an insensible sleep under the influence of the portion of injected aether which had not as yet produced its effect. 135. The rabbit and the chicken were subjected to several successive setherizations. The former, young and weak, died six or seven hours after the fourth trial (injection). At the end of fifteen hours its body was stiff, as if death had re- sulted from natural causes. Its nerves exhibited the soften- ing mentioned by some anatomists. The chicken, on the contrary, survived, and even on the following day laid an egg with a soft shell. It subsequently produced several others perfectly healthy. It did not appear to feel the effects of the shocks or injections to which it had been subjected. It ate corn greedily, and the rabbit lettuce leaves, as soon as the stupefaction produced by the aether had terminated. 136. Experiments were made on the frogs and the chicken ; one while with the effect of the induced currents successively * Comptes Rendus de l* Academic des Sciences de Paris, sitting of the 22nd of February 1 847, p. 286. Prof. E. Wartm&nn* sjburth Memoir on Induction. 24-9 direct and inverted, at anotlier with inverted currents only, employing the arrangement above described (127.)« There w^as no perceptible difference between the two methods of electrifying, even on circulating the inverted currents from the feet to the wings, or vice versa. § XVI. Action of Induced Currents on Albumen. 137. Brande was the first who pointed out the coagulation of albumen on the positive pole of the battery. M. Matteucci, in treating of the physiological action of electric currents *, says, that if the pole which was first positive be rendered negative, the albumen is not seen to redissolve, and that consequently an electric current may very well produce a cataract, but not destroy it. On the other hand. Prof. Zantedeschi affirms that he has seen the liquefaction of the albumen at the negative polef. Repeated experiments have never shown me this re- turn to the fluid state, and lead me to adopt entirely the con- clusion of the celebrated physiologist of Pisa. 138. The coagulation of albumen does not present any re- markable phase, when, under the immediate influence of a battery, we substitute either direct or inverted induced cur- rents, or the voltaic current rendered intermittent and strength- ened by the reaction of the induction which it has engendered in its own conductor and in the neighbouring conductor (124-.). But the phaenomenon changes when the liquid is traversed by induced currents in alternate directions. 139. Through the inducting wire A of an electro-electric machine furnished with a bundle of iron wires, I passed the current of five Grove's pairs of 0™'l square surface. The extremities x and y of the induced wire B (fig. 7) terminated in cups gg full of mercury. The circuit was closed by two platina wires a, b of l"^"^ in diameter, one part immersed in the cups, the other in the glass o full of the white of egg. The latter immediately coagulated around each wire, especially round that which communicated with the extremity of the circuit B, from whence proceeded the inverted induced current, and which corresponded to the positive termination of the rheophorus A. At the end of a few minutes some bubbles of gas appeared on the circumference of the coagulum. Some, having increased in volume, rose lightly to the surface of the viscous medium in which they were formed. The albumen, riddled with holes, by which the gas escaped and continued * Lezioni sopra ifenomenifisico-chimici del corpi viventi, p. 173. Pisa, 1844. t Trattato del Magnetismo et delta ElettricUd, vol. ii. p. 511. Venice, 1845. % 250 Prof. E. Wartmann's^wr/// Memoir on Induction. to be disengaged, turned black in several places: then a series oi luminous spar/cles, and lastly real sparks of a bright yellow glittered on the whole immersed part of the platina wire. At the same time the induced wire B was heated around the reel, the metallic pieces of the rheotrope rose in temperature, and the upper sides of the glass, not filled whh the albumen, were coated with aqueous vapour. 140. This remarkable phaenomenon is doubtless compli- cated. The coruscations do not dart from one wire to the other in the liquid ; they are seen along the wire. I thought at first that the combustion (for it was such) only took place on one of the electrodes (139.) ; but on repeating the experiment many times, I saw it alternate on both of them according as I reversed the poles of the battery, or present itself first upon one wire, then upon the other, without the direction of the current being changed ; or lastly appear upon only one of them, whatever changes were made in the positions of the rheophori and the extremities of the induced circuit. I attri- bute this latter case, which only occurred when the surface of the albumen was covered with a layer of aether, to the differ- ence of the conditions of contact of the two platina electrodes with the liquid : one, in fact, was then only covered with a slight coagulum, whilst the other gave rise to a considerable quantity of gas. These gases were collected on the aether in a tube traversed by a [)latina wire cemented at its top. They presented neither free carbonic acid, nor oxygen, nor hy- drogen. I think that they were a mixture of oxide of carbon and carburetted hydrogens. HI. The albumen solidified around platina conductors acquires the consistence of very soft glue; it is ductile, brown- ish, even blackish, and diffuses a marked odour of burnt horn or phosphoretted hydrogen. The platina does not take the pulverulent appearance nor black colour which are communi- cated to it by discontinuous alternate currents in other media; it preserves its metallic appearance. With the assistance of Prof. Marignac I analysed the coagulum; it contained no trace of platina. There is therefore here no catalytic action. 142. These various remarks lead me to think that, in cir- cumstances of imperfect conductibility of the albumen, and of great power in the induced currents employed, the immersed wires become heated when the coating of coagulum and of gaseous bubbles has put a new obstacle to the passage of the alternate currents (an obstacle rendered evident by the eleva- tion of temperature of the external circuits), whence results a true igneous decomposition and a burning, under the influence of oxygen in a nascent state, of combustible elements exposed. On eliminating the Signs in Star-Reductions, 251 l^S. Whatever value this opinion may have, it seems to me that the decomposition of albumen by the passage of very intense induced currents is a fact which deserves the serious attention of physicians and physiologists. The presence of this body in the blood, in urine, in the eye, in amniotic liquors, &c., requires caution in the employment of violent alternate currents. 14'1<. The appearances which I have described equally take place in the albumen extracted from new-laid eggs, immersed for some hours in the vapour of aether. They appear even to be developed there more easily. 145. It is perhaps well to add, that the production of these bright coruscations indifferendyon the two electrodes negatives any explanation founded on a different polarity of the platina wires, and all analogy with the pheenomena investigated by MM. Gassiot*, Haref, and NeeH'|. Geneva, June 18, 1840. XLI. On eliminating the Sigtis in Star-Reductions. By S. M. Drach, F.R.A.S. To the Editors of the Philosophical Magazine and Journal, Gentlemen, THE subject of this paper was broached by the Astro- nomer Royal in the Monthly Notices of the Royal Astro- nomical Society for January 1847. 1 beg to propose the fol- lowing extension, eliminating even the indices of the logs, em- ployed. Let A = E-P, B = F-Q, C = G-R, D = H-S; a = e—pi &c. a' = ^—p' for decl., or =p' — ^ for N. P. Dist, P, p, p'i &c. are numerical constants afterwards determined. Corr. R.A. = SAa=2E^-2^P-SEp + 2Pp: Corr. ^.P.D. = XAa' = ^Ee'-Xe'P-XEp' i-^Pp'. Let P=28'75, Q = 30-5, R = 1'35, S = 20 (R. A. given in time). L Right ascension, ^? = 2% q = 2, r = 30*5, 5 = 2. * Archives de V Electricite, vol. iii. p. 240. \ Siliiman's American Journal, January 1841. I succeeded several years ago in melting in an intermittent manner an iron wire of S"" diameter, employed as a negative electrode on the surface of impure mercury in which a copper wire bound to the positive pole is immersed. Twenty Daniell's couples, or forty smaller Bunseu's, suffice for this experiment. X Archives des Sciences Physiques et Naturelles, vol. i. p, 30. 252 On eliminating the Signs in Star-Redtictions. < 1+ — sec 8 sin a +14'^ 53"" 14.s >- + 32^-937 \ 1 + — tan 8 sin a +T4M8m^s \ - SEp= - 308^-392 + 55^-422 { 1 + sin© +42° 32' 4"} + 1 -324(1+ sin 2© +55° 29'} (J.) + 30'5(1— ^) + 21'254{l+ sin 53 +60° 30' 44"} + 0-2l7{l+ sin 2 £3 +235° 52'}. Sum =2Art—2E^=— 387^*386 + periodical terms. II. North Polar Distance, // = 2, (7' = 2, >'' = 30-5 5 — 2. 2Pp'— 2^P= — 74"'849 + 1 2"-476 cos 8 + 41"'912 (K.) {1+ sin 8 sin a + 8^1 53°^ 14^} + 32"-937{l+ sin a +8^18'"49s} >. -XW = _?^=_S 15 308"-392 + &c. (J'.) (K'.) Sum =SAa — 2Ee=— 383"-241+ periodical terms. Now if we add to (J.) and (J'.) the constant 180, and to (K.) the constant 420 seconds, there will be only positive quantities, and we shall have merely to subtract 10°^ or 10' from the mean place ; the corrections being E=28'75- 18-732 cos © -i I— I (N ^ r-H eo-i >-< o o in o »o «o «o eo ;oo CO (M »o GO :ifs (N «p OS «p i,co CO "^ OS ©^ " IN n 0010 (N §^ (N '-< NiN (N 05 CO OJ ^ i-i t^ eooq M QO C3S IN 10 0 (N -* (NiN ■— 1 ei5«o toeo OOS 10 » 1— 1 OS t>» 03 (N 00 50 coco l-H ao F-< S? o OS to >f5 CO to GO OS OS OS 5p -^ T)< Ai lis 1^ IN COIN °-^ So P< SL -f= -13 . s-a S -^ u S o -rj o w "C =^ "d 2 •3. © »n • g(N rN '* 91 ^ -* ©>>.©© M B ©CO l-H © Hf 0 1 o6 -*© & © ©©© © • © >0 CO >-< 1— 1 © -N -<#»>.©© © 2--* l>>03 CO CO t^ CO » QO ^ „g - 2 CO «>• (N CO CO " fe?$ r-, CO ^ 00 CO © © '"' © l>« CO CO '^ © >-i 10 ^ CO 1 ©C. ■* CO © CO CO 10 If? © © © »n '^ (>( © c -^ CO "fe?^ CO © qp CO © CO CO 10 -^ CO "* © <>J CO r-H CO »^ 1 5 >{5 J^ N r-. 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Potash .... 12-54 12*40 12*47 Soda 3-72 3-57 3*64 Lime 40' 16 40-31 40-23 Magnesia . . . 5*55 5-60 5-57 Sesquioxide of iron 0*83 0-82 0-83 Chloride of sodium 1*01 0-91 0*95 Phosphoric acid . 10*80 10-93 10-86 Sulphuric acid . . 4*61 4-76 4*68 Silicic acid ... 1*38 1*45 1*42 Carbonic acid . . 19-04 19-04 19-04 Sand and charcoal 0-42 0-63 0*53 100-06 100-37 100-22 Per-centage of the ash after deduction of the unessential constituents, carbonic acid, sand and charcoal : — Potash . . . . 15-43 Soda 4-52 Lime 49-89 Magnesia. . . . 6-91 Sesquioxide of iron 1-02 Chloride of sodium 1*18 Phosphoric acid . 13*47 Sulphuric acid . . 5*78 Silicic acid . . . 1*75 100*00 Analysis of the Ashes of the Stem. Amount of ashes left by 100 parts of the stem . . 2*74 I. II. Mean. Potash .... 9-66 9-73 9-69 Soda 2*61 2*47 2-54 Lime 45-46 45*96 45-71 Magnesia . . . 5*28 5-24 5-26 Sesquioxide of iron 0*48 0*48 0-48 Chloride of sodium 0-19 0-24 0-21 Phosphoric acid . 14*18 14-17 14-17 Sulphuric acid . . 3*90 3-79 3-84 Silicic acid . . . 0*92 1-14 103 Carbonic acid . . 16-51 16-50 16-50 Sand and charcoal 0-33 0-21 " ■ 0-27 99-52 99-93 99-70 T2 276 Messrs. Rowney and How*s Analysis of Potash . . . . 11-69 Soda . . . . 3-07 Lime 55*13 Magnesia. . . . 6-34 Sesquioxide of iron 0-57 Chloride of sodium 0-25 Phosphoric acid . 17*09 Sulphuric acid . . 4-64 Silicic acid . . . ]-22 10000 Analysis of the Ashes of the Leaves. Amount of ashes left by 100 parts of the leaves . . 13-73 I. II. Mean. Potash .... 12-87 12-48 12-67 Soda 1-22 1-38 1-30 Lime 43-32 43-44 43-38 Magnesia . . . 4-49 4-30 4-39 Sesquioxide of iron 0-3G 0-44 0-40 Chloride of sodium 5-08 5-17 5-12 Phosphoric acid . 2-46 2-58 2-52 Sulphuric acid . . 3-35 3-47 3-41 Silicic acid . . . 3-67 3-78 3-72 Carbonic acid . . 23-22 22-97 23-09 Sand and charcoal 0-24 0-21 0-23 100-28 100-22 100-23 Potash .... 16-51 Soda 1-68 Lime 56-38 Magnesia. . . . 5-72 Sesquioxide of iron 0-52 Chloride of sodium 6-66 Phosphoric acid 3-27 Sulphuric acid . . 4-43 Silicic acid . . . 4-83 100-00 the AsJiea of the Orange-Tree. 277 Analysis of the Ashes of the Fruit. Amount of ashes left by 100 parts of the fruit . . 3-94 I. II, Mean. Potash .... 28-21 28-32 28-26 Soda 8-73 8-99 8-86 Lime 19-20 18-83 19-02 Magnesia . . . 6-39 6-14 6-26 Sesquioxide of iron 0-35 0-36 0-35 Chloride of sodium 2-93 309 302 Phosphoric acid . 8-55 8-64 8-59 Sulphuric acid . . 2-88 2-93 2-90 Silicic acid . . . 0-31 0-38 0-34 Carbonic acid . . 20-38 20-22 20-30 Sand and charcoal 1-69 1-62 1-65 99-62 99-52 99-55 Potash 36-42 Soda . 11-42 24-52 Lime . . Magnesia • • . . 8-06 Sesquioxide of iron 0-46 Chloride of sodium 3-87 Phosphoric acid 11-07 Sulphuric : acid . . 3-74 Silicic acid . . . 0-44 10000 Analysis of the Ashes of the Seed. Amount of ashes left by 100 parts of the seed . . 3*30 Potash . , . Soda *. . . . Lime 16-59 Magnesia . . . Sesquioxide of iron Chloride of sodium Phosphoric acid . Sulphuric acid . . Silicic acid . , . Carbonic acid . . Sand and charcoal 100-30 10002 100^ I. II. Mean. 35-22 35-29 35-26 0-77 0-84 0-81 16-59 16-65 16-62 7-87 7-51 7-69 0-68 0-72 0-70 0-77 0-67 0-72 20-33 20-39 20-36 4-46 4-48 4-47 1-02 0-96 0-99 6-83 6-83 , 6-83 5-76 5-78 5-77 278 Sir W. Rowan Hamilton on Qjiaternions, Potash .... 40-28 Soda 0-92 Lime 18-97 Magnesia . . . 8*74 Sesquioxide of iron 0'80 Chloride of sodium 0-82 Phosphoric acid . 23-24 Sulphuric acid . . 5-10 Silicic acid . . . 1-13—100-00 The preceding analyses furnish a new confirmation of the fact first observed by De Saussure, namely, that the largest amount of mineral constituents is deposited in those parts of the plant in which the process of assimilation appears to be most active. While the ash left by the root, stem, fruit and seed did not exceed from 3 to 4 per cent., the leaves left not less than 13 per cent, of fixed residue on incineration. Regarding the composition of the different ashes, the great amount of carbonic acid found in the ashes of the root, the stem, and the fruit is at once obvious ; proving that not only the fruit, but also the roots and stem, contain a large quan- tity of organic acids. From the composition of the ashes of the root, the stem, and the leaves, the orange-tree belongs decidedly to the lime plants. In these three ashes the joint amount of lime and magnesia exceeds the quantity of the rest of the mineral con- stituents. In the ashes of the fruit and seed, however, the alkalies are as prevalent as they have been found in analogous cases. The amount of phosphoric acid (23-24) in the ash of the seed is considerable, as might be expected, still it is in- ferior to the quantities (34'81 and 42-02) which Mr. Souchay found on analysing the seeds of the citron [Citrus Medico) and quince-trees [Pyrus Cydonia). Nevertheless the ash of the orange-seed is very analogous in composition to the ashes of the last-mentioned seeds, as may be easily seen on com- paring their analysis *. XLVI. On Qjiaternions ; or on a New System of Imaginaries in Algebra. By Sir William Rowan Hamilton, LL.D., V. P.R.I, A. i F.R.A.S., Corresponding Member of the Insti- tide of France,) Sfc., Andrews^ Professor of Astronomy in the University of Dublin j aiid Royal Astronomer of Ireland, [Continued from p. 219.] 37. 1)ESUMING now the quaternion form of the equa- -*■*' tion of the ellipsoid, («p + H'-(/3f-p/3)^ = l> (1.) • Liebig's Annals, liv. p. 343. Sir W. Rowan Hamilton on Quaternions, 279 and making '^+^=jz:;^9? «-/3=;2Z^> • • • (2-) and !t±£^,=Q, f^=Q', .... (8.) the two linear factors of" the first member of the equation (1.) become the two conjugate quaternions Q and Q', so that the equation itself becomes QQ'=1 (4.) But by articles 19 and 20 (Phil. Mag. for July 1846), the product of any two conjugate quaternions is equal to the square of their common tensor; this common tensor of the two qua- ternions Q and Q' is therefore equal to unity. Using, there- fore, as in those articles, the letter T as the characteristic of the operation o^ taking the teiisor of a quaternion, the fequaiion of the ellipsoid reduces itself to the form TQ = 1; (5.) or, substituting for Q its expression (3.), (6.) which latter form might also have been obtained, by the sub- stitutions (2.), from the equation (3.) of the 30th article (Phil. Mag., June 1847), namely from the following*: T(«p + pa + /3p-p/3)=l (7.) 38. In the geometrical construction or generation of the ellipsoid, which was assigned in the preceding articles of this paper (see the Numbers of the Philosophical Magazine for June and September 1847), the significations of some of the recent symbols are the following. The two constant vectors « and X may be regarded as denoting, respectively, (in lengths and in directions,) the two sides of the generating triangle ABC, which are drawn from the centre c of the auxiliary and diacentric sphere, to the fixed superficial point b of the ellip- soid, and to the centre a of the same ellipsoid ; the third side of the triangle, or the vector from a to b, being therefore de- noted (in length and in direction) by » — x: while p is the radius vector of the ellipsoid, drawn from the centre a to a • See equation (35.) of the Abstract in the Proceedings of the Royal Irish Academy for July 1846. The equation of the ellipsoid marked (1.) in article 37 of the present paper, was communicated to the Academy in December 1845, and is numbered (31.) in the Proceedings of that date. 280 Sir W. Rowan Hamilton on Quaternions. variable point e of the surface ; so that the constant vector I — X is, by the construction, a particular value of this variable vector p. The vector from a to c, beiufr the opposite of that from c to A, is denoted by — x; and if d be still the same auxiliary point on the surface of the auxiliary sphere, which was denoted by the same letter in the account already printed of the construction, then the vector from c to d, which may be regarded as being (in a sense to be hereafter more fully considered) the reflexion of — x with i-espect to ^, is = —pxp-'^; and consequently the vector from d to b is =j-j-pxp~^ The lengths of the two straight lines bd, and ae, are therefore re- spectively denoted by the two tensors, T(i + ^x^-') and Tp; and the rectangle under those two lines is represented by the product of these two tensors, that is by the tensor of the product, or by T(»p4-px). But by the fundamental equality of the lengths of the diagonals, ae, bd', of the plane quadri- lateral ajbed' in the construction, this rectangle under bd and ae is equal to the constant rectangle under bd and bd', that is under the whole secant and its external part, or to the square on the tangent from b, if the point b be supposed ex- ternal to the auxiliary sphere, which has its centre at c, and passes through d, d', and a. Thus T{ip + pK) is equal to (Ti)^— (Tx)% or to x.^ — 1% which difference is here a positive scalar, because it is supposed that cb is longer than ca, or that Ti>Tx; (8.) and the quaternion equation (6.) of the ellipsoid reproduces itself, as a result of the geometrical construction, under the slightly simplified form* T(i^ + px) = x2-.2 (9.) And to verify that this equation relative to p is satisfied (as we have seen that it ought to be) by the particular value P = '-x, (10.) which corresponds to the particular position b of the variable point E on the surface of the ellipsoid, we have only to observe that, identically, <(» — 1) + (< — x)x = »^ — »X + JX— x^ and that (by article 19) the tensor of a negative scalar is equal to the positive opposite thereof. 39. The foregoing article contains a sufficiently simple * See the Proceedings of the Royal Irish Academy for July 1846, equa- tion (44.). Sir W. Rowan Hamilton 07i Qiiaternions. 281 process for the retraiidation of the geometrical construction * of the ellipsoid described in article 31, into the language of the calculus of quaternions, from which the construction itself had been originally derived, in the manner stated in the 30th article of this paper. Yet it may not seem obvious to readers unfamiliar with this calculus, why the expression — p>tp~* was taken, in that foregoing article 38, as one denoting, in length and in direction, that radius o/the auxiliary sphere which was drawn from c to d; nor in what sense, and for what reason, this expression —p)cp~^ has been said to represent the reflexion of the vector — X with respect to p. As a perfectly clear answer to each of these questions, or a distinct justification of each of the assumptions or assertions thus referred to, may not only be useful in connection with the present mode of considering the ellipsoid, but also may throw light on other applications of quaternions to the treatment of geometrical and physical problems, we shall not think it an irrelevant digression to enter here into some details respecting this expression— pxp~^, and respecting the ways in which it may present itself in calcula- tions such as the foregoing. Let us therefore now denote by 0- the vector, whatever it may be, from c to d in the construc- tion (c being still the centre of the sphere) ; and let us pro- pose to find an expression for this sought vector a; as a func- tion of p and of X, by the principles of the calculus of quater- nions. 40. For this purpose we have first the equation between tensors, Tcr=Tx; (11.) which expresses that the two vectors o- and x are equally long, as being both radii of one common auxiliary sphere, namely those drawn from the centre c to the points d and a. And secondly, we have the equation V.(o- — x)/5 = 0, (12.) where V is the characteristic of the operation of taking the vector of a quaternion ; which equation expresses immediately that the product of the two vectors cr — x and p is scalar, and * The brevity and novelty of this rule for constructing that important surface may perhaps justify the reprinting it here. It was as follows : From a fixed point a on the surface of a sphere, draw a variable chord au; let d' be the second point of intersection of the spheric surface with the secant bd, drawn to the variable extremity d of this chord ad from a fixed external point b; take the radius vector ae equal in length to bd', and in direction either coincident with, or opposite to, the chord ad; the locus of the point e, thus constructed, will be an ellipsoid, which will pass through the point b (and will have its centre at a). See Proceedings of the Royal Irish Academy for July 1846. 382 Sir W. Rowan Hamilton 07i Quaternions. therefore that these two vector-factors are either exactly similar or exactly opposite in direction ; since otherwise their product would be a quaternion, having always a vector part, although the scalar part of this quaternion-product (o-— x)p might vanish, namely by the factors becoming perpendicular to each other. Such being the immediate and general signi- fication of the equation (12.), the justification of our establish- ing it in the present question is derived from the consideration that the radius vector p, drawn from the centre a to the sur- face E of the ellipsoid, has, by the construction, a direction either exactly similar or exactly opposite to the direction of that guide-chord of the auxiliary sphere which is drawn from A to D, that is, from the end of the radius denoted by x to the end of the radius denoted by cr. For, that the chord so drawn is properly denoted, in length and in direction, by the symbol (T — X, follows from principles respecting addition and subtrac' tion of directed lines, which are indeed essential, but are not peculiar, to the geometrical applications of quaternions; had occurred, in various ways, to several independent inquirers, before quaternions {as 2)roducts or qnotieiits of' directed lilies in space) were thought of; and are now extensively received. 41. The two equations (11.) and (12.) are evidently both satisfied when we suppose (r = x; but because the point d is in general different from a, we must endeavour to find another value of the vector o-, distinct from x, which shall satisfy the same two equations. Such a value, or expression, for this sought vector J-^K". . . (20.) The part — x' of this last expression, which is parallel to p, is the same as the corresponding part of — x; but the part +t", perpendicular to p, is the same with the corresponding part of + X, or is opposite to the corresponding part of — x ; we may therefore be led by this process also to regard the expres- sion (17.) as denoting the reflexion of the vector — x, with respect to the vector p, legarded as a reflecting line ; and we see that the direction of p, or that of —p, is exactly interme- diate between the two directions of — x and —pxp~^f or be- tween those of X and of pxp~'. 4-4-. The equation (9.) of the ellipsoid, in article 38, or the equation (4.) in article 37, may be more fully written thus: (,p+px)(p. + xp) = (x2-.T. . . . . (21.) And to express that we propose to cut this surface by any diametral plane, we may write the equation OTp+pOT=0, (22.) where ■bt denotes a vector to which that cutting plane is perpendicular: thus, if in particular, we change ot to x, we find, for the corresponding plane through the centre, the equa- tion Sir W. Rowan Hamilton on Qiiaterniotis. 285 xp + pK = Oy (23.) which, when combined with (21.), gives (x2 - «2)2 ={i-K)p.p{i-x)- (» - x)p2(, _ x) = (. - x) V, that is, /«2 _,2\2 (24.) ■=(^7 but this is the equation of a sphere concentric with the ellip- soid ; therefore the diametral plane (23.) cuts the ellipsoid in a circle^ or the plane itself is a ajcHc plane. We see also that the vector x, as being perpendicular to this plane (23.), is one of the cj/clic normals, or normals to planes of circular section; which agrees with the construction, since we saw, in article 36, that the auxiliary or diacentric sphere, with centre c, touches one cyclic plane at the centre a of the ellipsoid. The same construction shows that the other cyclic plane ought to be perpendicular to the vector i ; and accordingly the equation ip + pi = Q (25.) represents this second cyclic plane; for, when combined with the equation (21.) of the ellipsoid, it gives and therefore conducts to the same equation (24.) of a con- centric sphere as before; which sphere (24.) is thus seen to contain the intersection of the ellipsoid (21.) with the plane (25.), as well as that with the plane (23.). If we use the form (9.), we have only to observe that whether we change px to —xp, or ip to — f)», we are conducted in each case to the following expression for the length of the radius vector of the ellipsoid, which agrees with the equation (24.) : Tf='i^) (^«-) And because x^ — »^ denotes the square upon the tangent drawn to the auxiliary sphere from the external point b, while T(i — x) denotes the length of the side ba of the generating triangle, we see by this easy calculation with quaternions, as well as by the more purely geometrical reasoning which was alluded to, and partly stated, in the 36th article, that the com- mon radius of the two diametral and circular sections of the ellipsoid is equal to the straight line which was there called BG, and which had the direction of ba, while terminating, like it, on the surface of the auxiliary sphere ; so that the two last lines ba, and bg, were connected with that sphere and with each other, in this or in the opposite order, as the whole se- 286 Sir W. Rowan Hamilton on Quaternions. cant and the external part. In fact, as the point d, in the construction approaches, in any direction, on tlie surface of the auxiliary sphere, to a, the point d' approaches to g; and bd', and therefore also ae, tends to become equal in length to Bci ; while the direction of ae, being the same with that of ad, or opposite thereto, tends to become tangential to the sphere, or perpendicular to ac: the line bg is therefore equal to the radius of that diametral and circular section of the ellipsoid which is made by the plane that touches the auxiliary sphere at A. And again, if we conceive the point d' to revolve on the surface of the sphere from g to g again, in a plane per- pendicular to Bc, then the lines ad and ae will revolve to- gether in another plane parallel to that last mentioned, and perpendicular likewise to bc ; while the length of ak will be still equal to the same constant line bg as before : which line is therefore found to be equal to the common radius of both the diametral and circular sections of the ellipsoid, whether as determined by the geometrical construction which the calculus of quaternions suggested, or immediately by that calculus itself. ^5. We may write the equation (21.) of the ellipsoid as follows: /(p) = l, ...... (27.) if we introduce a scalar function^/of the variable vector p, defined as follows : [a^—i'^ffip) = {ip + px)(pi + xp) = ip^j -}- ipxp + pxpi + pK^p ; or thus, in virtue of article 20, (x2_,2^V(p) = (.2 4.x2)p2 + 2S..pxp. . . (28.) Let p+T denote another vector from the centre to the sur- face of the same ellipsoid ; we shall have, in like manner, /(F + r) = l, (29.) where /(f-fr)=/(/») + 2S.VT+/(r), . . . (30.) if we introduce a new vector symbol v, defined by the equation {K^^i^fv={i^ + x^)p + ipK + xpi; . . . (31,) because generally, for any two vectors p and t, (p-f-T)' = p' + 2S.pr + T2, .... (32.) and, for any four vectors, i, x, p, t, S.iTXp = S.TXp»=S .xp»T=S .p and (31.), that we have also this simple relation : S.vp = l (34.) Subtracting (27.) from (29.), attending to (30.), changing t to Tt. Ut, where U is, as in article 19, the characteristic of the operation of talcing the verso?- of a quaternion (or of a vector), and dividing by Tt, we find : • 0 = -^:^^^:^^=2S.vUr + TT./(Ur). {35.) This is a rigorous equation, connecting the length or the tensor Tr, of any chord r of the ellipsoid, drawn from the extremity of the semidiameter p, with the direction of that chord T, or with the versor Ur ; it is therefore only a new form of the equation of the ellipsoid itself, with the origin of vectors removed from the centre to a point upon the surface. If we now conceive the chord t to diminish in length, the term TT./(Ur) of the right-hand member of this equation (35.) tends to become =0, on account of the factor Tt; and therefore the other term 2S . vUt of the same member must tend to the same limit zero. In this way we arrive easily at an equation expressing the ultimate law of the directions of the evanescent chords of the ellipsoid, at the extremity of any given or assumed semidiameter p ; which equation isO = 2S.vUT, or simply, 0=S.VT, (36.) if T be a tangential vector. The vector v is therefore perpen- dicular to all such tangents, or infinitesimal chords of the ellipsoid, at the extremity of the semidiameter p ; and conse- quently it has the directiim of the normal to that surface, at the extremity of that semidiameter. The tangent plane to the same surface at the same point is represented by the equation (34.), if we treat, therein, the normal vector v as constant, and if we regard the symbol p as denoting, in the same equation (34.), a variable vector, drawn from the centre of the ellipsoid to any point upon that tangent plane. This equation (34.) of the tangent plane may be written as follows: S.v(p-v-')=0; (37.) and under this form it shows easily that the symbol v"' repre- sents, in length and in direction, the perpendicular let fall from the origin of the vectors p, that is from the centre of the ellipsoid, upon the plane which is thus represented by the equation (34.) or (37.); so that the vector v itself, as deter- mined by the equation (31.), may be called ihe vector ofproxi- 288 Sir W. Rowan Hamilton on Quaternions. mity^ of the tangent plane of the ellipsoid, or of an element of that surface, to the centre, at the end of that semidiameter p from which v is deduced by that equation. 46. Conceive now that at the extremity of an infinitesimal chord dp or t, we draw another normal to the ellipsoid ; the expression for any arbitrary point on the former normal, that is the symbol for the vector of this point, drawn from the centre of the ellipsoid, or from the origin of the vectors p, is of the form p + nv, where n is an arbitrary scalar ; and in like manner the corresponding expression for an arbitrary point on the latter and infinitely near normal, or for its vector from .the same centre of the ellipsoid, is p + dp + (w + dw)(v + dv), where d« is an arbitrary but infinitesimal scalar, and dv is the differential of the vector of proximity v, which may be found as a function of the differential dp by differentiating the equa- tion (31.), which connects the two vectors v and p themselves. In this manner we find, from (31.), (x2-,2)2dv = (,2 + x2)dp + .dpx + xdp.; . . (38.) and the condition required for the intersection of the two near normals, or for the existence of a point common to both, is expressed by the formula p + dp + (w + d«)(v + dy) = p + wv; . . . (89.) which may be more concisely written as follows : dp + d.nv=0; (40.) or thus : dp + ndy + dnv = 0 (41.) We can eliminate the two scalar coefficients, n and An, from this last equation, according to the rules of the calculus of quaternions, by the method exemplified in the 24th article of this paper (Phil. Mag., August 1846), or by operating with the characteristic S . vdv, because generally S.yft2=o, S.vjttv = 0, whatever vectors ft, and v may be ; so that here, S . vdvwdv = 0, S . vdvdwv = 0. • This name, "vector of proximity," was suggested to the writer by a phraseology of Sir John Herschel's; and the equation (31.), of article 4.5, which determines this vector for the ellipsoid, was one of a few equations which were designed to have been exhibited to the British Association at its meeting in 1846: but were accidentally forwarded at the last moment to CoUingwood, instead of Southampton, and did not come to the hands of the eminent philosopher just mentioned, until it was too late for him to do more than return the paper, with some of those encouraging expressions by which he delights to cheer, as opportunities present themselves, all per- sons whom he conceives to be labouring usefully for science. Sir W. Rowan Hamilton on Quaternions, 289 In this manner we find from (4 d?v d^u dv db^+d^ + d^ + ^'dF"^' under the new and more symbolic form, (<=-r')-'" (^0 while < V denotes, in quantity and in direction, the flux of heat, at the time t and at the point xy%. 50. In the Proceedings of the Royal Irish Academy for July 1846, it will be found to have been noticed that the same new characteristic < gives also this other general transforma- tion, perhaps not less remarkable, nor having less extensive * In that paper itself, the characteristic was written V ; bi't this more common sign has been so often used with other meanings, that it seems desi- rable to abstain from appropriating it to the new signification here proposed, U2 292 Sir W. Rowan Hamilton on Quaternions. consequences, and which presents itself under the form of a quaternion : , ^ /dt du i\v\ /dv du\ . (dt dv\ , (du \d~v ~ Tz) +"^ Vd^^ ~ dI7 ■^'^ Vd^ + 1 di\ d3// (e.) In fact the equations (a.) give generally (see art. 21 of the present series), ( ix -{-jy + kz) {it +ju + kv)=:— {xt + yu-{- s:v) + i[yv—zu) +j{zt — xv) + 1i{xu —yt), }• (f.) \{ xyztuv denote any six real numbers ; and the calculations by which this is proved, show, still more generally, that the same transformation must hold good, if each of the three symbols iyj^ k, subject still to the equations (a.), be commutative in arrangement, as a symbolic factor, with each of the three other symbols .v, _?/, z ; even though the latter symbols, like the former, should not be commutative in that way among themselves ; and even if they should denote symbolical instead of numerical multipliers, possessing still the distributive cha- racter. We may therefore change the three symbols x,y, z, respectively, to the three characteristics of partial differentia- tion, -r-i -r-) -,- ; and thus the formula (e.) is seen to be in- dx dy dz eluded in the formula (f.). And if we then, in like manner, change the three symbols /, ?/, v, regarded as factors, to -T-i» -T-n -r-.i that is, to the characteristics of three partial dif- dx' dy' d.s' ferentiations performed with respect to three new and inde- pendent variables x', y\ z\ we shall thereby change -p to -T--r-;, and so obtain the formula: dd^da? ^ d .d-d ^dx^^dy-^^'dz )0- d_ ._d_ _d^\ d^'"^'^d7/''^ d^7 \dxdotI ^ + dy dj/' dzdy .(±± _i.A^ '^ \dxdy' dydx'J' .{d d '^'KdydF' z)+J' dy' dzdz'J ./d_ d_ Vd^d^' dx d^' ) (g.) On the Equation in Numbers A.r^+ B7/^+ C2^=D.27/2;. 293 which includes the formula (c), and is now for the first time published. This formula (g.) is, however, seen to be a very easy and immediate consequence from the author's fundamental equa- tions of IS-l-a, or from the relations (a.) of the foregoing article, which admit of being concisely summed up in the following continued equation: t^=:f = k^ = ijk=-l (h.) The geometrical interpretation of the equation S. vt«xt = 0 of the lines of curvature on the ellipsoid, with some other appli- cations of quaternions to that important surface, must be re- served for future articles of the present series, of which some will probably appear in an early number of this Magazine. [To be continued.] XLVII. On the Equation in Numbers Aa^ + By^ + Cz^^Dayz, atid its associate si/stem of Equatio7is. By J. J. Sylvester, Esq., M.A., F.R.S* [Continued from p. 191.] IN the last Number of this Magazine I gave an account of a remarkable transformation to which the equation is subject when certain conditions between the coefficients A, B, C, D are satisfied ; which conditions I shall begin by ex- pressing with more generality and precision than I was enabled to do in my former communication. 1. Two of the quantities A, B, C are to be to one another in the ratio of two cubes. 2. 27 ABC — D^ must contain no positive prime factor what- ever of the form 6n + }. I erred in my former communication in not excluding cubic factors of this form. 3. If 2"^ is the highest power of 2 which enters into ABC, and 2" the highest power of 2 which enters into D, then either m must be of the form 3«+ 1, or if not, then m must be greater than 3w. These three conditions being satisfied, the given equation can always be transformed into another, where A'u^ + WtP + Cxn^ = D'uvwy A'B'C = ABC D' = D uvw = a. factor of z. The consequence of this is, as stated in my former paper, that wherever A, B, C, D, besides satisfying the conditions above stated, are taken so as likewise to satisfy the condition, — P, of ABC being equal to 23'»±', or 2°, of ABC being equal to 23m±ip3u±i^ provided in the first case that ABC is also of the * Communicated by the Author. 294 Mr. J. J. Sylvester on the 'Equation in form 9«+l, and in the second case ABC again of the same form 9m ±1, but likewise D divisible by 9, j:? being in both cases a prime, then the given equation will be generally inso- luble. And I am now enabled to add that the only solution of which it will in any case admit, is the solitary one found by making two of the terms A.^■^, B?/^, Cz^ equal to one another ; so that, for instance, if the given equation should be of the form ^ +y + AB C . a^ = D^ys, then the above conditions being satisfied, the one solitary so- lution of which the equation can possibly admit, is J7= 1 ^=1, Az^- 02 + 2 = 0, which may or may not have possible roots. I call this a soli" tary or singular solution, because it exists alone and no other solution can be deduced from it ; whereas in general I shall show that any one solution of the equation A*^ + B?/3 + C^^=Da3/0 can be made to furnish an infinity of other solutions indepen- dent of the one supposed given, /. e. not reducible thereto by expelling a common factor from the new system of values of x^y^ z deduced from the given system. The following is the Theorem of Derivation in question : Let A«3 + B^3^C/=D«/3y. Then if we write F=A«3 G=B/33 H=Cy3, and make .r=F2G + G2H + H2F-3FGH j/=FG2 + GH2 + HF2-3FGH z=l{F3 + G3 + H3-3FGH}, or = «/3y{F2 + G2+H2-FG-FH-GH}, we shall have x^ -f- 2/3 -f. ABCs:^ = Yyxyz. I am hence enabled to show that whenever x^ -^-y^ -\- kz^ = Djcyz is insoluble, there will be a whole family of allied equations equally insoluble. For instance, because x^ + y^ + z^ = 0 is insoluble in integer numbers. I know likewise that x^ +y^ + z^=x^y^ + x^z^ + y^^ a^ + y*^ + a« = .ry + a^^ — 2^/3^3 are each equally insoluble. Numbers kx^ -\-'Qif -{■ Cz^ —T>xyz, 295 In fact = t^ + x^ + li:^, where u, v, w are rational integral functions ofx,i/, z. Hence each of the factors must be incapable of becoming zero*. As a particular instance of my general theory of transfor- mation and elevation, take the equation x^ + y^ + 22^ = Mxi/z. Then, with the exception of the singular or solitary solution x=l .^=lj of which 1 take no account, I am able to affirm that for all values of M between 7 and —6, both inclusive, with the exception of M=— 2, the equation is insoluble in integer numbers. Take now the equation where M= — 2, viz. x^+j/^ + 2z^+2xi/z = 0. One particular solution of this is x=l y— — \ z = l. Another, which I shall call the second f, is xszl j/=3 2=— 2. From the first solution I can deduce in succession the follow- ing: j;=ll j/=5 z=— 7 a?=— 793269121 3/=11794900O 2;= — 1189735855 &c. &c. &c. From the second, ^=—10085 j/ = 8921 2;=— 844-2 a? = &c. y=&c. z = hc. As another example, take the equation x^-\-Tl/^ + 6z^=6xyz. One solution of the transformed equation ^3 ^ 2v^ + Str* = Qumso is evidently * It is however sufficiently evident from their intrinsic form, which may be reduced to — (M^+SN^), that this impossibility exists for all the factors except the first, t See Postscript. 296 On the Equation in Numbers Aa;^ + By^+C2;*D=a^a. Hence I can deduce an infinite series of solutions of the given equation, of which the first in order of ascent will be a;=5 y=1 z-=S. Again, the lowest possible solution in integers of the equation will be A-=17 .?/=37 z—'-^i. The equation admits of the solutions 37=1 j/=2 z=- — 1 ^'=—271 J/ = 919 2= -438. I trust that my readers will do me the justice to believe that I am in possession of a strict demonstration of all that has been here advanced without proof. Certain of the writer's friends on the continent have, in their comments upon one of his former papers which appeared in this Magazine, complimented his powers of divination at the expense of his judgement, in rather gratuitously assuming that the author of the Theory of Elimination was unprovided with the demonstrations, which he was too inert or too beset with worldly cares and distractions to present to the public in a sufficiently digested form. The proof of whatever has been here advanced exists not merely as a conception of the author's mind, but fairly drawn out in writing, and in a form fit for publication. P.S. It must not be supposed that the two primary or basic solutions above given of the equation a^ -]-if -\- 2r^ + 2x1/ z = 0, viz. x = \ j/=— 1 z=l x=l t/=3 2;= — 2 are independent of one another. The second may be derived from the first, as 1 shall show in a future communication. In fact there exist t/iree independent processes, by combining which together, one particular solution may be made to give rise to an infinite series of infinite series of infinite series of correlated solutions, which it ma}' possibly be discovered contain between them the general complete solution of the equation x^-\-if^-ir kz^=\)xyz, J. J. S. 26 Lincoln's Inn Fields, Sept. 20, 1847. [To be continued.] [ 297 ] XLVIII. Oil the Invention and First Introduction of Mr. KcEnig's Printing Machine. By Richard Taylor, F.S.^.^c. " As a step in the progress of civilization the Steam Press can only be compared to the original discovery of Printing itself." — Times Newspaper, j2cli/29, 1847, on the death of Mr. J. Walter. MORE than a century after its introduction the first inven- tion of the Art of Printing became a subject of long-con- tinued controversy, remarkable for the insufficiency and fallacy of the most confident assertions resting upon pretended tradi- tions and unsupported conjectures. And, as Hadrian Junius in 1575 first disputed the claims of Gutemberg after so long a period had elapsed, so did Atkyns as late as 1664 first deny the title of Caxton to the honour of having introduced the art into our own country. Hence one of the writers in this controversy remarks that " the Art of Printing, which has given light to most other things, hides its own head in dark- ness." It will be our own fault if we allow any unfounded asser- tions and pretensions to obtain currency with regard to an improvement in the art, of which The Times newspaper has said that "from the days of Faust and Gutemberg to the present hour there has been only one great revolution in the art of printing, and it occurred in the year 1814. Of that revolution Mr. Walter was t lie prominent and leading agent.'' Now though I would on no account detract from the ge- neral merits of the late Mr. Walter, as set forth in the Obi- tuary and extended Memoir which appeared in The Times of the 29th of July and 16th of September, yet I cannot allow the representations which are made in these articles, as to any share which he is alleged to have had in this important invention, to pass without the most unqualified contradiction. In the Obituary we read as follows : — "But one achievement alone is sufficient to place Mr. Walter high in that list which the world, as it grows older and wiser, will more and more appreciate — ' Inventas aut qui vitam excohiere per artes, Quique sui memores alios fecere merendc' He first brought the steam-engine to the assistance of the public press. Familiar as the discovery is now, there was a time when it seemed fraught with difficulties as great as those which Fulton has overcome on one element and Stephenson on another. To take off 5000 impressions in an hour was once as ridiculous a conception as to paddle a ship fifteen miles against wind and tide, or to drag in that time a train of carriages weighing 100 tons fifty miles. Mr. Walter, who, without being a visionary, may be said to have thought nothing impossible that was useful and good, was early resolved that there should be no impossibility in printing by steam. It took a long time in those days to strike oiF the 3000 or 4000 copies of The 298 Mr. R. Taylor on the Inveniion and First Introduction Times. Mr. Walter could not brook the taedium of the manual process. As early as the year 1804 an ingenious compositor, named Thomas Martyn, had invented a self-acting machine for working the press, and had produced a model which satisfied Mr. Walter of the feasibility of the scheme. Being assisted by Mr. Walter with the necessary funds, he made considerable progress towards the comple- tion of his work." " On the very eve of success he was doomed to bitter disappoint- ment. He had exhausted his own funds in the attempt, and his father, who had hitherto assisted him, became disheartened, and re- fused him any further aid. The project was therefore for the time abandoned." [Why abandoned, we may ask, if so feasible, and on the very eve of success ?] " Mr. Walter, however, was not the man to be deterred from what he had once resolved to do. He gave his mind incessantly to the subject, and courted aid from all quarters, with his usual munificence. In the year 1814 he was induced by a clerical friend, in whose judge- ment he confided, to make a fresh experiment ; and accordingly the machinery of the amiable and ingenious Koenig, assisted by his young friend Bauer, was introduced — not, indeed, at first, into The Times office, but into the adjoining premises, such caution being thought necessary from the threatened violence of the pressmen. Here the work advanced, under the frequent inspection and advice of the friend alluded to. At one period these two able mechanics sus- pended their anxious toil, and left the premises in disgust. After the lapse, however, of about three days, the same gentleman dis- covered their retreat*, induced them to return, showed them to their surprise their difficulty conquered, and the work still in progress." Who would not infer from the above, that Mr. Walter, having determined " to make a fresh experiment," in pur- suance of those which he had long before abandoned (not- withstanding his early resolution that there should be no im- possibility in it), and " courting aid from all quarters with his usual munificence," had been actually the person that enabled Mr. Koenig to pursue his labours on Mr. Walter^s premises, " under the inspection and advice of Mr. Walter's clerical friend," and thus to produce his invention? Whereas, in truth, Mr. Walter knew nothing of Mr. Koenig till after his invention had been completed. He was merely the first newspaper proprietor who purchased from the Patentees the Printing Machines long before invented by Mr. Koenig. Of these patentees I was one, and as I am now the sole survivor, it devolves upon me to contradict any erroneous statements and unfounded pretensions. I feel this to be the more ne- cessary, as already the misstatements of The Times are cir- culated, with additions and exaggerations, in other journals, * To me this story appears not a little extraordinary : — the " discovery of the retreat" of Messrs. K. and B. ! who were every day to be found su- perintending our factory in Whitecross Street. — R. T. of Mr. Koeuig's Printing Machine. 299 Thus, in an article in the Mechanics' Magazine for Sept. 18, copied into the newspapers, I find the following passage : — " No sooner were presses made of iron, than the idea occurred of working them by steam ; and the first to welcome the new and happy thought was the proprietor of a journal which stood in instant need of some such powerful auxiliary to enable him to keep pace with a circulation unexampled in the history of the press, and who, with- out it, would most assuredly never have been able to attain to that prodigious influence which for many years past has at once asto- nished and awed the world. Koenig, the ingenious inventor of the steam-press*, found in the proprietor of The Times his natural and best possible patron. With the liberal aid of the late Mr. Walter, he produced a machine of somewhat gigantic size, but nevertheless possessing a completeness of design and purpose which cast all other surface printing-presses into the shade." And again — " The steam-press has given occupation to many thousands, who, but for its introduction, would have been standing idle, and who ought, one and all, to bless the memory of Mr. Walter for enabling the inventor to work out his ideas, and perfect his great and glorious undertaking." Now the whole of this is a fable. Mr. Walter was no " natural and best possible patron " of Mr. Koenig's, — gave him no " liberal aid in producing his machine," nor did any- thing whatever to "enable him to work out his ideas." These had all been worked out long before ; patents had been taken out, a machine had been made, and was in operation on the premises of the Patentees, before ever Mr. Walter, or any- other newspaper proprietor, was applied to and invited to adopt it. Mr. Perry of the Morning Chronicle declined, alleging that he did not consider a newspaper worth so many years' purchase as would equal the cost of machines. Mr. Walter, "being a cautious man of the world," but enterprizing, " it being," as his biographer says, " his habit in tiie game of life never to throw away a chance," when he had fully sa- tisfied himself by seeing that the invention was accomplished, and in effective operation, consented to give an order for two machines, for the cost of which he paid us a certain sum, and a rental according to the number of copies printed ; and this rent we received, until it was commuted for a sum agreed upon. I do not mean to charge the writer in the Mechanics' Ma- gazine with any intentional misrepresentation. He has evi- dently been misled by the articles in The Times, which though they do not directly assert all that he has inferred from them, yet they imply as much. Thus a story gains in the telling, * Mr. Kcenig's invention is very inappropiiately designated by the terms " steam-press," and " the working of iron presses by steam." Its construc- tion is wholly independent of the motive power employed. SOO On the Invention of Mr. Koenig's Printing Machine. till the most vague and unfounded suggestions, if uncontra- dicted, are assumed as indisputable facts ; and it would be recorded that if Koenig was the Gutemberg of the new dis- covery, Walter was at least the Faust or Schoeffer of the affair, or rather, both in one. I am convinced that Mr. Walter, were he living, would disclaim the pretensions that have been made in his name : and indeed he has done so in the announcement which ap- peared in The Times, Nov. 20, 1814, the day on which that journal was first printed by the machines, and \yhich contains the following passage : — " That the completion of an invention of this kind, not the effect of chance, but the result of mechanical combinations methodically arranged in the mind of the artist, should he attended with many obstructions and much delay may be readily admitted. Our share in the event has indeed only been the application of the discovery, under an agreement with the patentees, to our own particular business." " The time for effecting the great revolution in the art of printing," says Mr. Walter's biographer, " did not arrive till the year 1814." Now it was in 1809 that, together with the late Mr. George Woodfall, I joined Mr. Kcenig and Mr. Bensley in taking out patents*, the machine being even then so far advanced as to satisfy us as to the prospect of success, and to enable us to have the specifications drawn up. Kcenig had gone on with Bensley, to whom 1 had recommended him some few years before, up to the year 1809, when the taking of premises and the purchase of lathes, tools, &c., and the employing of workmen, with the salaries of Mr. Koenig and his able and excellent assistant Mr. Bauer, led Bensley to in- vite us to a partnership in the undertaking. For several years it occupied much of our time and attention, and cost us much money (from which we had no return f ) and much anxiety. Each experiment suggested some improvement, and one im- provement led to others, so that additional patents had to be taken out. But with Mr. Walter we had none of us any com- munication, until, as I have before stated, the machine had been completed and was at work on our own premises. I have thought it right, under the circumstances, to put on * One of the four patents bears date March 29, 1810 (See Phil, Mag. vol. XXXV. 1st Series, p. 319). It was taken out in the name of Frederick Koenig, and was assigned by articles of partnership to the firm of Bensley, Koenig, Woodfall and Taylor. •f Mr. Koenig left England, suddenly, in disgust at the treacherous con- duct of Bensley, always shabby and overreaching, and whom he found to be laying a scheme for defrauding bis partners in the patents of all the ad- vantages to arise from them. Bensley, however, while he destroyed the prospects of his partners, outwitted himself, and grasping at all, lost all, becoming bankrupt in fortune as well as in character. Cambridge Philosophical Society. SOI record my own recollections as to the progress and introduc- tion of this invention : and though they relate to transactions which took place from thirty to forty years ago, I believe they are in the main correct, and can be confirmed by documentary evidence. XLIX. Proceedings of Learned Societies, CAMBRIDGE PHILOSOPHICAL SOCIETY. [Continued from p. 143.] ON the Partitions of Numbers, on Combinations, and on Permu- tations. By Henry Warburton, M.P., F.R.S., F.G.S., Mem- ber of the Senate of the University of London ; formerly of Trinity College, A.M. The use made by Waring of the Partitions of numbers in develo- ping the power of a polynome, induced the author to seek for some general and ready method of determining in how many different ways a given number can be resolved into a given number of parts. On his communicating the method described in article 5 of Section L of this abstract, to Professor De Morgan, in the autumn of 1846, that gentleman intimated a wish that the author would turn his attention also to Combinations ; and such was the origin of the re- searches which form the subject of the 2nd and 3rd sections. I. Gn the Partitions of Numbers. 1. Let [N, p»j] denote how many different ways there are of re- solving the integer N into ^J integral parts, none less than ij. Then [N.p„] = [N±;,9,p„+^] (I.) 2. Such of the p-partitions of N as contain ij as a part, and no part less than t], are obtained by resolving N— ij into p — 1 parts not less than tj, and by adding ij, as a pXh part, to every such (p— 1)- partition. That is, [N,2.«]-[N,p]=[N-o,,i.-l]. . . . (IL) 3. In (IL), substitute ij + l, ij + 2, &c. successively for ij. The sum of the results is [N,^,]-[N,2?,+^+i]=Sj[N-,j-ri?,p-l]. . (III.) Z tl Inthisexpression, when 9=1* (—)—ij, the term [N,^„^^^.l] vanishes, and the formula then becomes analogous to one published anonymously by Professor De Morgan in a paper printed in the fourth volume, p. 87, of the Cambridge Mathematical Journal. 4. In(IL), for [N,p„^i] substitute [N— pij.p,], and transpose « I f — jis employed to avoid the long phrase, "the integer nearest to N and not exceeding — ." P 302 Cambridge Philosophical Society. the terms. Then [N,^„]-[N-,.j;-l] = CN-2)>j.p,]; . . (IV.) *) and this leads to [N-i3,p-l]-[N-2ij,2?-2] = [N-pij,2j-l]; n ri vt and that leads to the summation [N.^„] = S^[N-;5,j.^.] (V.) 2 The lower limit of z in (V.) is made 0, in order that the formula may comprehend the extreme case [0, Uj = 1, analogous to the ex- treme case in Combinations. 5, After substituting 1 for ij, the author applies formula (IV.) to determining in how many different ways N can be resolved into p parts not less than 1. Let [N.^jJ be the term in a table of double entry corresponding to column N, line p, in the table. From the head, in line 0, of each of the columns 0, 1, 2, 3, &c., draw a diagonal, advancing one column and one line at a time. Take these diagonals one after another, and in each of them compute by formula (IV.) the terms situate on lines 0, 1, 2, 3, &c., one by one in succession. If N be the number at the head of the column from which any diagonal takes its departure, there will be only N terms to compute on that diagonal, the further terms being only repetitions of the term on the line N. For the diagonal in question intersects line N in column 2N ; and, by formula V, [2N,NJ = S^[N,r,] z = the sum of all the terms in column N. But, moreover, [2N+y,Ni+y] = S?[N,r,] z as the same constant. The leading property of the table, indicated by the formula [N,p,]=S^[N-p,^.], z is, that the term [N, Pi] = the sum of all the terms in column N— j?, from line 0 to line p inclusive. After the publication of the anony- mous paper before referred to, Professor De Morgan discovered this theorem also, but he did not announce it*. II. On Combinations. 1. In ordinary Combinations, the combining elements are of differ- ent kinds, and there is but one element of a kind : in the case here considered, there are different kinds of elements, and there may be many elements of a kind ; and more than one element of a kind may enter into the same combination. 2. If II elements enter at a time into each combination, and the * The author has recently discovered an equivalent formula in p. 264 of Euler's Int. in An. Infinitoruni ; but investigated by a totally different method, and not applied as the author has applied it. Cambridge Philosophical Society. 303 kinds are determinate in number, and their number is 5, let < > denote how many diflferent combinations can then be formed: if the elements are determinate in number, and their number is tr, let the number of the combinations which can then be constructed, be denoted by {m, (tJ. If (p (a:) be any function oi x, let D" (p(a;) denote the co- efficient of a?" in that function developed according to the powers oix. 3. The same things as before being assumed, let a given set of elements consist of a elements of the kind A, +/3 elements of the kind B, + &c. Take the product, K, of the 5 geometrical progres- sions, •[H-Aa + A2a;2+ + A"a?"], [l+B^ + B2a;'+....+B'^a^],&c. Then K will be of the form, l+S[A]a? + S[A2 + AB]a;2+S[A3 + A«B + ABC]a:3+&c., and D«[K] will be of the form S[A/'B^/C'-&c.], the last expression being an aggregate of terms of the form A^'B'i'C'' ... , each containing a different combination of u of the given elements, and their sum comprehending all the possible combinations of those elements taken m at a time. Now, if A, B, C, &c. be each made equal to 1, K will become each of the terms A^.B*?. C''. &c. will become 1, and the number of all the terms of the form A^B'i'C'" .. . which Dw[K] or S [A^B^C''...] contains, that is to say, |m, (t} will be represented by D" [A] ; which latter coefficient the author next proceeds to determine. Now « ^ . — 1— — -. &c. =[1— .-r ^ iri— ar^ ]..[1 — a;] \—X \—X ^ -"- J L J =[i---+']ci-»^+']...sTr^*-»i u Ll"|i J =[i-^"+'][i— ^+']...p^,s^[[«+ir-''V](vii.) For brevity, write u^, a,^, /3i, &c. respectively, forM-l-l,a+l,/3 + l, &o.; andalsowrite [l]for[l-^x]-^ [2]for[l-a;«i][l-a.]-*; that is, for [1-.t"i] . [1]; [3] for [l-a;«i] [l-.r^i] [l-ar]"*; that is, for [1— a;^i].C2], and so on. Then D«[2]=D«[l]-D«-«i[l]; and D«[3] =D«[2] -D«-^i[ 2] ; * According to the factorial notation, here used by the author, «wl±i represents s [s-4 1][5+2J. ..[*+_(«— 1)]. ^VI.) 304 Cambridge Philosophical Society. and D"[4]=D«[3]-D"-5'i[3]; and soon; (VIII.) and the developed product of the binomes, [l-a;«i],Cl-aA],[i_a;yi],&c.; that is to say, 1— a?*i+^«i+^i-a'"i+'^i+yi+ &c. — &c. +&C. when multiplied into the development of [1 —a;] ~*, manifestly leads to the following formula : D«M=D«[l]-S[D«-«i[l]]+S[D«-«>-^.[l]]l - S [D^-^i-'^i-yiCl]] + &c. J where, since the powers of a?, in (VI.) or (VII.) developed, are to be all positive, no expression of the form («—«,), (m — ai— /3i), (m— ai— /5i— 7,), &c, is to be negative. Then by giving to D«[l],D"-«i[l],D«-«i-^i[l],&c. . . (IX.) their respective values, we obtain the series of expressions : where in all the kinds the elements are plural without limit ; a for- mula given by Hirsch : where the elements A are limited in number to a, but those of the other (s— 1) kinds are plural without limit : J p-iuL _|-„^_^j.-iii J-Lo where, moreove«r, the elements B are limited in number to /3, but those of the other (s— 2) kinds are plural without limit : and so for the rest. The law of the terms being evident, they need not be continued further. Example of (IX,). Given one element of 1 kind, two elements of a 2nd kind, three of a 3rd, and four of a 4th ; and let m=5. Then 1 {"•''} =1:2:3 -4.5.6 -3.4.5 + 1.2.3 ^•^•S -2.3.4 -1.2.3 = 22. Cambridge Philosophical Society. 305 4. If «=/5=y=&c., formula (IX.) becomes {"■•■} =-i;4ip s'"l.2.3^4.5.6[^-^-^-^-^-^Q~^-^-^-^-^-^-^]= 203. 5. If it is required to determine many, or all, of the terms of the series {0, s, the upper limit of 2 is .9; and the number of tj^pes to be formed is [w +5, sj . (See articles 4 and 5, Section I.) But, if the repetition is finite, some of these partitions may fail to yield combinations. 11. If the elements A, B, C, &c. represent different prime num- bers, all the methods and theorems contained in this section will apply, mutatis mutandis, to the composite numbers of whicli those primes, or the powers of those primes, are divisors. III. On Permutations. 1 . Let the given elements be of 5 different kinds. We can de- termine in two known cases, by an explicit function of u, when the elements are taken m at a time, in how many different ways they can be permuted. The number of the permutations is denoted, when there is but one element of a kind, by s'«l-i ; and when in all the kinds the elements are plural without limit, by s". When the plu- rality is finite, it is only in the particular case of all the elements being permuted at a time, that there is a known formula to express the number of their permutations. 2. Every combination constructed on a given type, u=.mv-\-m'v' + m"v"+ &c., will generate the same number of permutations, ]^ ^p Mciinwi rii)'ii-im'n""in»»" . &c. Therefore, if the number of the different combinations which can be constructed out of the given elements in conformity with that type, is represented by Q, Q X P will be the number of the permutations corresponding to the type and to those elements. If the plurality be without limit, xP JWlll^ 1»»'|1. l»i"|l^ gjg will be the number of the permutations. If the given elements be finite in number, as in formulas (XIV.) and (XV.), the number of Cambridge Philosophical Society. 309 the permutations corresponding to those elements and to the type, will be JtoU * \m'\\ ' jm"!! &c. X P. Every different partition of u that may be formed within the limits pointed out in art. 10, Section II., will give rise to a similar product, QxP ; and the sum of all these particular products, S[Q x P], will show how many different permutations can be formed from the given elements, taken m at a time. The author illustrates this method of computing the number of permutations, by examples. 3. Let P < " I denote how many different permutations can be formed when u elements are taken at a time out of 5 kinds ; and P {m, (TJ denote how many different permutations can be formed when u elements are taken at a time out of c, a finite number of elements. If all the elements may be repeated without limit, =i>[i«i.[i+..+£i + ....^+. ...]*]• Hence the author infers that, if the elements A are limited in num- ber to a, while those of the other (s— 1) kinds are plural without limit, that if, moreover, the elements B are limited in number to /3, while the other (s— 2) kinds are plural without limit, p{^}=D»[l«l..<->[l+.+ ^+..^] and so on, until finally, if all the elements are finite in number, and the elements A, B, C, &c. are respectively limited, in point of num- ber, to a, /3, 7, &c,. fi -^'\ (XVII.) 4. Hence, if in all the s kinds the elements are dual, (XVII.) becomes • . . (XVIII.) SIO Cambridge Philosophical Society. This is the only addition which the author has been able to make to the cases wherein PJ " , or P|m, o-} is expressed by an explicit function of u, symmetrical in form. Example. Let there be five kinds of elements, and two of each kind. Let m=3. 5. The author gives the following theorem, which is precisely analogous to that of art. 6, Sect. II., formula (XL), in Combina- tions ; viz. P{«,^}=S ;[^^'p(.,r}. ?{«-„, cr-r}]. (XIX.) 6. By a mode of proof precisely analogous to that employed in art. 7, Sect. II., he shows that P{(r-1, o'}=P{(r, tr} ; that is to say, that l«l'.l/3|l.iy|l. &c. denotes the number of permutations that can be formed with a ele- ments A, (i elements B, &c. (where [a+/3 + y+ 3cc.] = (r), as well when (T— I elements, as when c elements, are taken at a time. Since correcting his paper for publication, the author has had his attention called to the work of Bezout on Elimination (4to. Paris, 1779, p. 469), as containing a formula similar in structure to that numbered VIII*. in the present abstract. Bezout investigates the composition of a polynome function of 5 quantities. A, B, C, &c., consisting of terms which are of the form ApE'iO', and of every dimension from 0 to m inclusive. Let [*]" denote such a polynome, complete in all its terms, and N[]s]" the number of its terms. Then, 1st, and 2nd, the number of the terms in [«]« which are not divisible by either A*, or B^, or C, &c., he expresses by N W-N[«]«-« -f-N[s]«-*-/^- &c. -NM«-^+ &c. — &c. Intelligence and Miscellaneous Articles. 311 He also observes (p. 89) that when A* B^, C^, &c. are the high- est powers of A, B, C, &c. which a jjolynome, agreeing in other respects with [s]", contains, the terms of such incomplete polynome will agree in point of number with those terms in [s]" which are not divisible by either A*+l, or B'^+^j or C>'+^ &c. The polynomes from which Bezout proposes to eliminate certain terms, contain terms of all dimensions from 0 to m inclusive. The terras which are to remain after the others have been eliminated, and which are enu- merated by means of the condition, that they are not divisible by certain powers of A, or B, or C, &c., may be of all dimensions indis- criminately from 0 to M inclusive. Bezout's object is exclusively Elimination, and he makes no allusion to any other application of his formulae. The polynomes considered by the author, taken in their entirety, agree in their general structure with those considered by Bezout ; but the nature of the author's inquiries led him to confine his atten- tion to the composition of those particular terms in a polynome which were of the same dimension ; and to seek to express the number of the terms, not of all dimensions indiscriminately, but of each particular dimension separately. To show how it has hap- pened that researches, very different at their point of departure, have, as regards one point of investigation, ended in nearly similar formulae, the author proceeds to deduce his formula (VIII*.) from the investigations of Bezout. Such a deduction, he conceives, might readily have been made by any one to whom it had occurred to make it ; and the application of such a deduction, when once made, to pro- blems in Combinations, would have been much too obvious to have remained long unnoticed. Expressions of the form above considered are regarded by Bezout as of the nature of Differences ; and the truth of this view of the subject may be shown in the following brief manner. If (p(a;) generates \J/(m),[1 — a;«]f (a;) will generate \|/(m)— \|/(m— a), which we may denote by A^vKm). Consequently \\—x^'\ [1 —x»'\ e silver exists occupied their attention. As the subject appeared a difficult one, it was simplified by inquiring in what state the silver existed in galena, blende and pyrites, and they supposed it could exist only in the native state, as chloride or sulplmret. Experiments appeared to show that in these sulphurets the silver is not in the metallic state ; and experiments still more numerous and decisive seemed also to prove that the silver could not be in the state of chloride ; and on this occasion they remarked a circumstance which has hitherto escaped the observation of chemists : — Tliey found that all metallic sulphurets, properly so called, and even some arseniurets, possess the property of decomposing a certain quantity of chloride or bro- mide of silver. This decomposition is effected more or less slowly when contact is effected merely by water ; but it is produced much more rapidly, and in some cases even instantaneously, when the chloride or bromide of silver is in solution. By comparative trials the authors succeeded in determining the decomposing power of a great number of sulphurets and several arseniurets. Thus — 318 Intelligence and Miscellaneous Articles. 100 of sulphuret of zinc decompose 3 of chloride of silver 100 .... cadmium ..14- .... 100 .... bismuth .. 2 .... 100 lead . . 5 .... 1 00 protosidphuret of tin "a • • • • 100 of bisulphuret of tin ..SO .... 100 protosulphuret of copper 360 .... 100 arseniuret of antimony 120 .... 100 .... cobalt 166 .... In operating with natural sulphurets, the authors remarked very considerable differences in their decomposing power. They attri- bute these differences to the presence of small quantities of sulphu- rets or arseniurets of very high decomposing power ; and they sup- pose they may sometimes attach to the molecular condition of the bodies. They found, for example, that a very pure and well-cry- stallized blende from Kiinigsberg possessed decomposing power equal to that of artificial sulphuret of zinc; while a blende equally pure and as well crystallized, but coming from Radna, had a decom- posing power which was twice as weak, and yet these two blendes were of equal density. The authors draw the following conclusions from the results of their experiments : — AH pure metallic sulphurets possess the power of decomposing, under certain circumstances, a given quantity of chloride of silver, and even of other insoluble chlorides. This power appears to be modified in some cases by the molecular condition. The decomposition of chloride of silver by sulphurets may be effected, — 1st, by double decomposition ; 2nd, by reduction; 3rd, by simultaneous reduction and double decomposition. Natural sulphurets sometimes exhibit very high absorbent powers, on account of the presence of minute quantities of foreign sulphurets or arseniurets, acting by the reduction of the chloride of silver. The decomposing action of sulphurets is exerted proportionally on the bromide of silver, and it is but slightly appreciable on the iodide. In these phaenomena the solvent exerts no influence ; for the same results are obtained, except as to time, by simple contact aided by water. The general fact of the decomposition of insoluble chlorides by sulphurets appears then to render it probable that, in natural sul- phurets, the silver is in the state neither of chloride nor bromide. Having then shown the improbability of the presence of metallic silver or chloride in the natural argentiferous sulphurets, the authors are of opinion that it must exist in the state of sulphuret ; but if this conclusion were correct, how does it happen that blende, pyrites and galena, do not yield silver to mercury? Is not the sulphuret of silver almost as readily acted upon by mercury as metallic silver itself? The authors propose shortly to communicate the second part of this inquiry to the Academy. — Comptes Rendus, Juillet 26, 1 847. Meteorological Observations. 319 VANADIATE OF LEAD AND COPPER. M. Dufr^noy presented to the Academy, in the name of M. Do- meyko, Professor of Chemistry and Mineralogy in the college of San Yago, Chili, an account of this new mineral, which is composed of — Oxide of lead 54-9 Oxide of copper 14'6 Vanadic acid 1 3*5 Arsenic acid 4*6 Phosphoric acid 0*6 Chloride of lead 0-3 88-5 Comptes Rendus, Mai 5, 1847. METEOROLOGICAL OBSERVATIONS FOR AUG. 1847. ChinvicL- — August 1, 2. Very fine : sultry. 3. Very fine : clear. 4. Very fine : densely overcast. 5. Rain. 6. Overcast. 7. Very tine. 8. Very fine : cloudy. 9. Cloudy: shower: clear. 10. Rain: showery. 11. Very fine. 12. Light clouds, with bright sun at intervals: clear at night. 13. Overcast: very fine. 14, Very fine : cloudy. 15. Cloudy : clear : lightning at night. 16, Rain. 17. Overcast. 18. Heavy rain. 19. Overcast: lightning at night. 20. Uniformly overcast : slight fog. 21. Slight fog : fine. 22. Overcast : rain : cloudy. 23. Cloudy : rain. 24. Cloudy : clear at night. 25. Very fine. 26. Overcast : very fine. 27, 28. Very fine. 29. Rain : very fine. 30. Very fine : cloudy. 31. Very fine : clear at night. Mean temperature of the month 62^*68 Mean temperature of Aug. 1846 64 •]6 Mean temperature of Aug. for the last twenty years 62 -32 Average amount of rain in Aug 2*41 inches, Boston. — Aug. 1. Fine : 2 o'clock p.m. thermonn.eter 83°. 2. Fine : rain p.m. 3, 4. Fine. 5. Cloudy : rain p.m. 6. Fine. 7. Fine : rain p.m. 8. Fine. 9,10. Cloudy. 11. Cloudy : rain early A.M. 12. Cloudy. 13, 14. Pine. 15. Cloudy. 16. Cloudy : rain a.m. and p.m. 17. Cloudy: rain p.m. 18, 19. Cloudy. 20— 25. Fine. 26. Cloudy. 27. Fine. 28. Rain. 29. Cloudy : rain early a.m. : rain p.m. 30, 31. Cloudy. Sandivick Manse, Orkiiey. — Aug. 1, 2. Brijiht : clear. 3. Bright: cloudy. 4. Cloudy : drops. 5. Bright : cloudy. 6. Cloudy : fine. 7. Rain : fine. 8. Cloudy: rain. 9. Cloudy: fine. 10. Cloudy: rain. 11. Clear : showers. 12. Cloudy. 13. Clear : cloudy. 14. Cloudy : fine. 15. Bright : fine. 16, 17. Clear: fine. 18. Cloudy: fine. 19, 20. Cloudy. 21. Showers : rain. £2. Cloudy : showers. 23. Clear : showers : cloudy. 24. Cloudy : rain. 25. Cloudy. 26. Cloudy : rain. 27. Cloudy : clear. 28, Bright : showers : clear. 29. Showers. 30. Rain : showers. 31. Bright: rain. Apjtlegarlh Manse, Dumfries-shire, — Aug. 1. Fair, but cloudy. 2. Fair and fine: shower early A.M. 3. One slight shower. 4. Rain early a.m. 5. Rain nearly all day. 6. Frequent showers. 7. Heavy showers and sUn. 8. Rain. 9. Cloudy : cool : dry, 10. Heavy rain. 11. Fine a.m. : rain p.m. 12. Rain nearly all day. 13, Fair and fine. 14. Very fine. 15, 16. Very fine : heavy dew. 17. Fine, though cloudy. 18. Very fine. 19. Still fine, but dull. 20. Heavy showers. 21. Slight showers. 22, 23. Fine : clear. 24. Rain p.m. 25, 26. Fine, though cloudy. 27. Fine, though cloudy : a few drops. 28. Fine, though cloudy : one slight shower, 29. Fair and fine, 30. Fine : one slight shower. 31. Fine harvest day. Mean temperature of the month 57°'15 Mean temperature of Aug. 1846 61 '2 Mean temperature of Aug. for twenty-five years 57 '14 Average rain for twenty years .,, 3*16 iOCbes, -saiajiutiQ •ao)8og[ •3lO!.ttsm3 •JlOIiipUBS 'Xauiijo •ajiqs -saujiuna S^ CO o\ n O) r^ n •-> o •^"-< c — o -^ I'l i S S"ll c'l S:' » I* I "• « B? ^' fe' I i i c ^' S ^*l i fe S:* &' So QUO S? pa> y^ ^* ^' ^' «* i i £ i i i ii^foii] ^ ^ >• ^ ^ i i i ^ & i % i 1 ^* §"« » c 5: u u u u o § ■•"■« " f6 H« ^i« "-tte? •HJN co*o icr>-oo o^io c>-oi u:)0^o^r>.oo t^ON^ooooio loto-^^o^o o ot^-ioiO'^ 3 <" 'am •Ul'Bfg •uojsoa •uiH •XBK -wg ■^s •iioisoa •q^uOH JO sXbq *^ to «0^t-0<^lO^^O^O^OlOO^^Ol r^oooo^o■^o•^u^«^ot^ooc^•^^^'7ooo^ooo — criir^'P 0^6^6^C^0^6^CT^^^C^^3^a^CT^O O O O O O 6^6^0^6^0 ^^0 O O O O^CTM3^ I:^oooo^^•^"o■^^Ol^^lOoo*o--lcoc^(^Io^^^■^c>•l^~oo^op•7OOO^o^o^OOOOOOOO^O^ 0*000 r^t^o t^o coo ir^-^oo •^co i>-oo cot^-^rot^oo ooo OMnt^'tcyioo ■^ (N O CTNCX3 O — "^-lO ro -^O O 0 lO rtoo — a\ o o o 00 ■^^O 00 I t^(0 00 • CI T- 6 6 I CO CO t^lO — c O OMJ^ 00 •^o> ^ -^o ooo 6 6 6 CO CO CO lO O CO CO ■^ 'S' CO t^ ^ VO -" ' CO c^oo t^OO 00 coio es 00 UO — i • O T* 7H 9^ 6 6 6 6^ CO CO CO (N — coo — vo 10 OM>-0 ■^ CO r^ «M I— oi — — "5}<«5 o — 00 6 6 6 CO CO CO i-JeJco-^m•Qoo^o — — >.. vj-4^ — — rHi-ipH — ^rH — — 3a9=C4— 2«3 + fl2~2ai, 3^10=^4+ ^3~2a2—2ai, which may be verified by putting for a„ «2, &c. their values in a-'i, .^2, &c. Therefore six of the roots «i, ag, &c. are linear functions of the remaining four, and the equation in a of the tenth degree is reducible to one of the fourth. We also find ^l=-3 (^l + '^2 + «3 + «4)» •^•2=-3-(2«l — «2-^3 — «4)> I ^3=3- (-«l + 2Cf2-«3-«4)» •^4=3-(-«l-% + 2^3-«4)> K^O ^^5= -(~a,-fl2-«3+2«4)- Now let the reduced equation in a be a'^ + mc^-\-tia'^+pa + r=0, .... (4'.) the roots of which are «i, «2» ^3> ^4? ^"^ therefore — »2 = 2(«x), « = S(a?i«2)> — J^=^(^i«2^3)j r—a^acfi^a^. Consequently, — m = 3a?i by (3.), w = 6a?2 + 2.ri (372 + ^3 + ^4 + ^5) + '^[Xy':^ — ^x\ + '^{XyX^ because S(^i) = 0; —7; = ^x\ + 2.r2 (a;2 + .^3 + X4 + 075) + ^i2 (a^i^-g) + 2 (a^i^a-^s) 2 1 = 2^3 + ^iSCj^-ja^g) -\-X{x^x^^ — — — n^— — mk—V>\ r = x\-\- x''^{x^x^ + 2(^13^2^3.^4) = — »i4 + _ ^^2^ ^ c^ Hence w, 7?, and /- are given in terms of 'm, and m=^ —Zx^ can only be found by solving (1.); or the resolution of the pro- posed into factors, one of which is of the second degree, de- pends upon the solution of the proposed itself. We may introduce fifth roots if we please; thus, let A'*+^^3-f^X^ + ^X + /=0, .... (5.) Equation of the Fifth Degree, 343 the roots being Xj = rt6, A2=a«, A3=a5, X^-a\. Here we shall find, as before, putting for a^^ Cg* &c. then* values in w^, Xc^ &c., that ■\-5x^{xl^x\ + x\ + x*^+xl + x\ + xl + xlz=z~27x\ We may find h, k, and / in terms ofg, as we found n, p, and r in terms of ?w ; and as S(^j), 2(a:^), &c. are known functions of A, B, &c., we shall have g, h, &c. functions of x^. The determination of these therefore may be said to depend upon the solution of the given equation. If otherwise found, as they may be by finding the equation on which g depends, it must be by an equation of the fifth degree not reducible ; for the five values of Xy, .r^, &c. being distinct, there will be as many distinct values of ^. It may be observed that if we make A any other integer function of a, not passing the fifth degree, we shall still have an ultimate equation to solve of the same degree. To give two very simple examples of the equation in g, let x^ + Kx+B — O. Then 2:K) = 0, 2:(a;?)=0, 2(^t)=-4A, 2(^J) = -5B; and g=27:rf + 20A.ri4-5B. Eliminating x^ between this and a:J + Aa*j + B=0, we hav {g + 22B)5 + 74A^(^ + 22 B) - l^M'B = 0. Again, leta?^ + Aa;^ + B = 0. In this case and g=z'21x\ + iiOAx\+5^. Eliminate -Tj from this and x\-{- Ax\->r^ = 0, and there results {g + 22B)* + 3W(g + 22B) - 3*A^^B = 0. By making g + 22B = i; in the first of these examples, and ^-l-22B = t;^ in the second, the equations in v are similar to those in .r, and are no way in a more solvable form. Let us now take the equation of the sixth degree, a^ + ha^ +^x^ + Cx^ + Dx + ¥.=: {af^ ^ aa^ -{■bx'^ + ex + d) {x^—ax+f)=0. 844 The Rev. B. Bronwin on the Algebraic There are fifteen ways in which this may be done, and con- sequently the equation in a will be of the fifteenth degree. As before, &c., and 0 = a?! + ^2 + a73 + 0^4 + a?5 + OTg. If we eliminate x^, Xc^ &c. from these sixteen equations, we shall have ten resulting equations between a^, «2» &C'j which will give fl!g, ^7, &c. in terms of the first five of these quantities. The equation of the fifteenth degree is therefore reducible to one of the fifth, or a^ 4- ma!^ + nc^ -i-pa^ + qa + r=0, where — m=ai4-«2 + «3 + «4 + «5=4)A'i. The determination of m then will be the same thing as solving the given equation of the sixth degree. And it is easy to see that we shall arrive at results precisely the same in equations of a still higher degree. If we resolve the given equation into the factors x^-^ax^ + bx + c and x^—ax'^+Jlr+g, we shall have ^j — — •*'| ~T" <^2 "1 ill^g, fltg =S i^j -j- ^2 -j- iJ?^, OCC, and the equation in a will be of the twentieth degree. But since 0^= — «i, «i2= ~^'2.i &c., the equation in a^ will be only of the tenth degree. The reduced equation however, whether we find by it a or a^, will be of a higher degree than the fifth. Let us now return to (1.), or the equation of the fifth de- gree, in order to find Lagrange's final equation of the sixth degree. Make ^, = Q\ + Q\ + fl*3 + a*4, x^ = aS^i + u^\ + et^a + uH\, Whence we find 5Q\=x^ + u'^x^ + ^% + y'*^4 + 8% 59^2 = -^1 + «% + ^% + y^^4 + ^-^5 59^3 = a?i + a^^g + fi% + /^4 + 1% 5d*4 = 0?! + (SMJj + /ScVg + yx^ + dx^f where 1, a, /3, 7, 8 are the five roots of unity. If we make ^ = 01.% y^ct^, 8=«% we have Equation of the Fifth Degree, 34f5 5S*2 = J^i + a^^2 + '^^'^a + *'*'^4 + "^^ Sd\ = a?i + «*^2 + «*^3 + <''^4 + ^^^, 56*4 = iTi + a^3 + ^^^3 + *^^4 + "''^S' Let 5i, figj 635 ^4 be the roots of fl4 + Mg3^Nfl2 + Pfl + Q=0. Then -M=0, +624-63+64; to find which I employ (m + u + to + 3 + ^)5 = 2(«^) + 5X Ku) + 1 02(w3u^) + 202 (M^tw) + 302(w^u^w) + 602(m^«W2) + l^Owmzt, collecting the terms separately, and reducing by means of l+ot + a%+a3 + a^ = 0, 0:1 + 5-2 + ^3 + ^4 + ^-5=0, and also X\ - X^X^ = - x\{Xc^ + 0^3 + ^4 + ^bli a^lx^x^ + x^x^) = - x\xlx^ - x\xlx^ - x\x\x^ - x\xlx^ —x\[XciX^X^ + Xc^XgXr^ + Xc^X^X^ + x^x^x^, &c. We thus find 5^(3i + fl2 + S3 + M = 192«)-102(o;^)X«)-202(^^^2^3) — 1 302(^^4^3) ~ 4-OS (^?a;2a:'3^4) + 4i^0x^Xc^QX^x^ + 250 + 5;^o-«or, + aX^i + ^K^4 + ^^X) • The first six terms of the second member are all given, being symmetrical functions of a7j, a?2j &c. Let their sum be R; then, putting — M for 5)(6i), the above will be -5^M-R=s260(a?2ar2a74 + x2a?2a?j + ). Or if we make 5^M + R_ 250 ~'^* it will become -<^=x\xlx^^x\xlx^-\- ' (6.) Now if we make a?i, x^ change places in the second member of the last, then a'^, ajg, and o-g* ^3> &c., we shall find that it has six different values, as stated by Lagrange. Thus 846 Capt. J. H. Lefroy o« a great Magnetic -<^^-x\x\x^^x\xlx^^ -(p„=a;2^X + ^I-^I^i + — <^^=-X^X^X^-\-X^Xi^^ + -(^^-x\x\x^ + x\x\x^ + (pg — c*^./.5X_^-t-(D2+c2)-'»(a;-('»-i) .g/Q*'.P)} ; of which various particular cases and transformations are given and discussed ; including the well-known forms D^M + — Dm + c": M = P, X — ^ ,^ / m(m—\)\ ^ and extensions of these forms. The application of the process to equations of the third and higher orders gives rise to solutions of analogous forms ; and in particular the equation is solved in the form bnZ^ + bn-iZ"-^ + ..._b„ A , B where — s—. „_. ,- — t 1 « + ... a»2;»-f-a„_iz" '-)-... a„ x—a x—p ; and by the application of the theorems first referred to, a still more general form is solved. The solutions above-mentioned are subject to the important re- striction that m, A, B, &c. (denoting the number of times that the operations are to be repeated) must be integer ; but in the subse- quent part of the paper, a mode is suggested of instantaneously con- verting these solutions into definite integrals not affected by the re- striction. 3. The interchange of symbols above suggested frequently renders available forms of solution which otherwise would not be interpret- able in finite terms. The ojjeration (fD)^ is not intelligible if m be a fraction ; but if by any legitimate process this be changed into the factor ( and where the number of operations to be performed is denoted by a fraction, solutions are found in the form of definite integrals. The solution of the first when Q^=0 is tly 0 +y/3(a»^;'»+. •a.t' + ao)" V''(^-'^)M^-^)^2 • • -^^-^^^ + &c. ; and that of the second is somewhat similar. From some investigations effected by interchanging the symbols X and D in the solution of the general linear equation in finite dif- ferences of the first order, it would seem that definite summations may be used to represent the solutions of certain forms of equations. Thus a partial solution of is c2(r;2!)»f*« from «= — a to z==0. 7. In attempting the solution of some equations by means of suc- cessive operations, not consisting exclusively of D combined witli 376 Cambridge Philosophical Society. constants, but involving also functions of x, the only result which appeared to the author worthy of notice is the solution of D%+6Dm+c2m-w(w+ 1)3;^= X ; from a particular case of which, the general solution of Laplace's equation, may be found in the simple form with a similar function using — V^ — l for v — 1. CAMBRIDGE PHILOSOPHICAL SOCIETY. [Continued from p. 311.] On the Symbolical Equation of Vibratory Motion of an Elastic Medium, whether Crystallized or Uncrystallized. By the Rev. M. O'Brien, late Fellow of Caius College, Professor of Natural Philo- sophy and Astronomy in King's College, London. The object of the author in this paper is twofold : first, to show that the equations of vibratory motion of a crystallized or uncrj^stal- lized medium may be obtained in their most general form, and very simply, without maldng any assumption as to the nature of the mo- lecular forces ; and secondly, to exemplify the use of the symbolical method and notation explained in two papers read before the Society during the present academical year. First, with regard to the method of obtaining the equations of vibratory motion. This method consists in representing the disarrangement (or state of relative displacement) of the medium in the vicinity of the jioint X1/Z by the equation i. dv X' , dv r. , dv ^ I d-v ^ ,, , d"v j i> , n -o ov= --dx+ — 01/ + — dz-\ ?x^+ dxdy + &c. — &c. dx dy dz 2 dx'^ dxdy (where i' = ^a + ij/3 + ^y, ^15^ denoting, as usual, the displacements at the point xyz, and ajSy being the direction units of the three coordinate axes), and in finding the ivhole force brought into play at the point xyz (in consequence of this disarrangement) by the symbo- lical addition of the different forces brought into play by the several terms of Bv, each considered separately. It is easy to see that these different forces may be found with great facility, without assuming anything respecting the constitution of the medium more than this, that it possesses direct and lateral elasticity. By direct elasticity we mean that elasticity in virtue of which direct or normal vibrations Camh'idge Philosophical Society. 377 take place ; and by lateral, that in virtue of which lateral or transverse vibrations take place. The forces due to the several terms of h are obtained by means of the following simple considerations. Let AB be any line in a perfectly uniform medium, and conceive the medium to be divided into elementary slices by planes perpen- dicular to AB ; let OM{=x) be the distance of any slice PP' from any particular point O of AB, and suppose this slice to suffer a dis- placement equal to — cx'^ (c being a constant) in the direction OAB, and the other slices to be similarly displaced. Then it is evident that the medium suffers by these displacements a uniformly increasing expansion in the direction OB, and a uniformly increasing condensa- tion in the direction OA ; the rate of increase both of the expansion and condensation being c. Now in all known substances, whether solid, fluid, or gaseous, a disarrangement of this kind would bring into play on the slice O a force along the line AB proportional to the rate of increase c, i. e. a force Ac, A being a constant depending upon what we may call the direct elasticity of the substance. Again, suppose that the slice PP' receives a displacement — cx'^ in the direction OC perpendicular to AB, and the other slices similar displacements. Then the line AB will become curved into a para- bola A'OB', and all the lines of the medium parallel to AB will be similarly curved, the radius of curvature being equal to — and per- pendicular to AB. Now in all known substances* a disarrangement of this kind would bring into play upon the slice O a force in the direction OC proportional to the curvature c, i. e. a force Be depend- ing upon what we may call the lateral elasticity of the substance. Lastly, suppose that M.V^=y, and that the point P of the medium receives a displacement cxy parallel to AB, and the other points similar displacements. Then the slice PP' will, in consequence of this kind of displacement, turn through an angle tan~'(ca;) into the dotted position, and the other slices will suffer similar rotations, those on the other side of O, such as QQ', turning the opposite way. Now it is easy to see that a disarrangement of this kind produces a uniformly increasing expansion in the direction OC, and a uniformly increasing condensation in the direction OC, the rate of increase both of the expansion and condensation being c. But the expansion and condensation here described are quite different from that pre- viously noticed ; since it is produced, not by displacements parallel to C'C, but by lateral displacements, i. e. perpendicular to C'C. On this account all that we can assert without further investigation is, that the force brought into play upon an element at O by this dis- arrangement acts along the line C'C, and is proportional to c, i. e. equal to Cc, where C is some constant evidently depending in some way both upon the direct and lateral elasticity of the medium. * Fluids and gases possess lateral elasticity as well as solids, only in a comparatively feeble degree. 378 Cambridge Philosophical Society, There is however a very simple way of finding the precise value of the force brought into jilay by a disarrangement of this kind ; for if we turn the axes of x and y in the plane of the paper through an angle of 45°, it appears that this disarrangement is nothing but a combination of the two kinds of disarrangement previously noticed ; and from this it immediately follows, in the. case of an uncrystallized medium, that the force brought into play at O is (A— B)c ; in other words, the coefficient C, which must be multiplied into c, in order to give the force brought into play by the disarrangement cxy, is equal to the coefficient of direct elasticity (A) minus the coefficient of lateral elasticity (B). In the case of a crystallized medium, it may be shown that six relations, corresponding to the relation C=A— B, are most probably true, and are essential to Fresnel's theory of transverse vibrations ; that is to say, the medium is capable of propagating waves of trans- verse vibrations if these six conditions hold, but otherwise it is not. In employing the above considerations to determine the equations of vibratory motion, the directions AB and C'C are always taken so as to coincide with some two of the three coordinate axes ; and it is this circumstance that makes the method peculiarly applicable to crystallized media. Indeed, if it were necessary to take the lines AB and C'C in any directions but those of the axes of symmetry, the above considerations would not apply without considerable mo- dification. The equations of vibratory motion obtained by this method for an uncrystallized medium, are the well-known equations involving the two constants A and B. The equations obtained for a crystallized medium are perfectly free from any restriction of any kind, are appli- cable to all kinds of substance, whether we suppose its structure to be analogous to that of a solid fluid or gas, and hold for all kinds of disarrangement, whether consisting of normal or transverse displace- ments, or both. When we introduce the six relations between the constants above alluded to, and moreover assume that the vibrations constituting a polarized ray are in the plane of polarization, we arrive at Professor MacCuUagh's equations*. If, on the contrary, we suppose the vi- brations to be perpendicular to the plane of polarization, we arrive at equations which agree exactly with Fresnel's theory in every par- ticular-j-. If we introduce these six relations into the equations for crystal- lized media deduced from M. Cauchy's hypothesis, that the mole- cular forces act along the lines joining the different particles of the medium, it will be found that these equations are immediately re- duced to the equations for an uncrystallized medium. From this it follows that M. Cauchy's hypothesis cannot be applied to any but uncrystallized media. In fact, it may be easily proved that if the * Given in a paper read to the Royal Irish Academy, Dec. 9, 1839, page 14. t On this subject see a paper by the late Mr. Greene in the seventh volume of the Cambridge Transactions, p. 121. Cambridge Philosophical Society. 379 equations derived from this hypothesis be true, a crystallized medium is incapable of propagating transverse vibrations. Secondly, respecting the use of the symbolical method and notation above alluded to. The application of the symbolical method and notation to the subject of vibratory motion is very remarkable, and leads to equations of great simplicity. In the case of an uncrystallized medium, the three ordinary equations of motion are included in the single symbolica- tion equation dt^ \d9!'' dy'' dz^i ^ \ dx '^ dy ' dz ) \dx ^ dy ^ dz ) If we employ the notation Am'.m, £md 9,ssurae the symbol 50 to re- present the operation d I /oj^ , d dx dy dz ' the equation of nogtion becomes ^ =B(AlD.3D)v+(A-B)-i-AlD.v ; or, by using the notation Dm'.w also, it may be put in the form ^ = { AIDAlD.-B(DlD.)°-}y. The symbol 3D written before any quantity U which is a function of xyz, has a very remarkable signification ; the direction unit of the symbol 3DU is that direction perpendicular to which there is no va- riation of U at the point xyz, and the numerical magnitude of 3DU is the rate of variation of U, when we pass from point to point in that direction. The symbols AiP.u and DiD.v have also remarkable significations. AlD.u is a numerical quantity representing the degree of expansion, or what is called the rarefaction of the medium at the point xyz. DtD.u represents, in magnitude, the degree oi lateral disarrangement of the medium at the point xyz, and, in direction, the axis ^bout which that displacement takes place. These two symbols may be found separately by the integration of an equation of the form d''\J _^ (d^V rfnj rf2U\ dt^- \c?j?2 dy'^ dz^J' When the six conditions above alluded to are introduced, the equation of motion for a crystallized medium becomes 380 Royal Astronomical Society. where Aj A^ A3 are the three coefficients of direct elasticity with reference to the three axes of symmetry, and B, B/ B^ B2' B3 MJ the six coefficients of lateral elasticity with reference to the same axes. If the vibrations be transverse, this equation is reducible to the form ^ = -(DID.) V?a+&^oj/3 + c^?7) = — (DlD.)^(a -aAa + i^jS A/3 + c^^y)v, assuming the vibrations of a polarized ray to be perpendicular to the plane of polarization. The well-known condition that a plane polarized ray may be transmissible without subdivision, and the velocity of propagation may be immediately deduced from this equation. If we assume the vibrations of a polarized ray to be in the plane of polarization, the equation becomes 1!H = _DlD.(a^aAa+62/3A/3 + c2yA7)D5D.u. This includes Professor MacCullagh's three equations. ROYAL ASTRONOMICAL SOCIETY. [Continued from p. 146.] May 14, 1847. — Extract of a letter from Mr. Adams, with new Elements of Neptune. " The following elements of Neptune have been obtained by taking into account Prof. Challis's observations made since the reappear- ance. * * * The elements are now sufficiently correct to enable me to approximate to the perturbations of Neptune by the action of Uranus, in order to compare more accurately the ancient observa- tions of 1795 with those .... made recently. I have used the old observations, supposing the elements not to have changed. I hope immediately to set about a new solution of the perturbations of Uranus, starting with a very approximate value of the mean distance. * * * I do not think, with Professor Pierce, that the near commen- surability of the mean motions will interfere seriously with the re- sults obtained by the treatment of perturbations ; but it will be in- teresting to see how nearly the real elements can be obtained by means of the perturbations." Elements of the Orbit of Neptune. Mean longitude, Jan. 1, 1847, G. M. T... 328 13 54-5 T Longitude of perihelion (on the orbit)... 11 13 41-5 LM. Eq. 1847-0 Longitude of ascending node 130 5 39-0 J Inclination to ecliptic 1 47 I'S Mean daily motion 213774 Semi-axis major 302026 Eccentricity of orbit 0-0083835 On the communication of Mr. Adams's paper, the Astronomer Royal Astronomical Society. 881 Royal gave orally a continuation of the history of Neptune, embra- cing the ])rincipal points that have been ascertained since his com- munication of Nov. 14, 1846. The planet having been actually dis- covered in the heavens by means of certain predicted elements, the fair presumption was that those elements were very approximately correct. Adopting these elements, therefore, Mr. Hind examined Lalande's and other observations, with the hope of finding some former observation of the planet as a star now missing, but satisfied himself that there was none. In the meantime, the continuation of the observations of the planet in the last months of 1846, and the comparison of them with Professor Challis's early observations of August, led to some unexpected conclusions. It was found that, though one^/«ee of the planet might be very well represented by M. Le Verrier's or Mr. Adams's elements, yet the apparent movement of the planet could not be represented within several minutes. Elements were then investigated from the observations themselves (without any reference to the preceding deductions from the perturbations of Uranus) by Mr. Adams in England (see Monthly Notices for March, p. 244), and by Professor Pierce and Mr. Sears C. Walker in Ame- rica. Attention is particularly due to the former of these investiga- tions, in which are exhibited, not only the results for the different elements, but also for the probable error of each. The most import- ant conclusion was, that the planet certainly moved in a much smaller orbit, and probably in an orbit of much smaller eccentricity, than that indicated by the calculations of perturbation. With elements thus roughly corrected, the orbit was again traced back through the ancient observations ; and it was found by Dr. Petersen of Altona, and Mr. Sears C. Walker, that a star observed by Lalande on May 10, 1795, and now missing from the heavens, was very probably the planet. The observation however vi'as marked doubtful in Lalande's printed volume : and to this circumstance is probably due a most remarkable discovery. The manuscripts of Lalande's observations were some years ago transferred by his representatives to the obser- vatory of Paris. To examine into the presumption of doubt in the observation, the astronomers of the Observatory of Paris referred to the originals, and there they found that the observation of May 10, 1795, was entered without any expression of doubt at the time; that an observation of May 8, 1795, was omitted in the printed vo- lume ; that it was omitted solely because it could not be reconciled with the observation of May 10 ; and that, upon reducing both pro- perly, they exhibit most distinctly the retrograde motion of a planet nearly parallel to the plane of the ecliptic, the right ascension and the polar distance having both changed in the proper proportion. It seems now inconceivable to us that an astronomer, having his atten- tion strongly called to the difference between the two days' results, should rather assume that there were in the observations two inde- pendent errors (one of right ascension and one of polar distance), than that the body observed was really a planet. With the place of the planet at an epoch so distant, its elements are ascertained with great accuracy. S82 Royal Astronomical Society. It is remarkable that the missing star, to which allusion has been made, is actually entered as an observed star in the Berlin Star-Map ; and this circumstance prevented Mr. Adams from tracing the new orbit of the planet so soon as he would otherwise have done. This insertion of an unobserved star can be accounted for only on the supposition that the star had been taken by the observer in his work- ing-catalogue as a zero-star, and had then been inserted as a matter of course. The mean distance of Neptune from the sun now appears, instead of 38, to be something near 30 ; and its periodic time, instead of 220 years, to be nearly 166. It is certainly a most curious thing (in which much is owing to chance) that elements, now known to be extremely erroneous, should have accounted for the perturbations of Uranus through 150 years with such accuracy, and should also have given the planet's place, for the particular year in which the attention of astronomers was first strongly directed to it, with such precision. It remains to be seen whether the new elements of Nep- tune will, with any possible mass, explain the perturbations of Uranus. In any case, Bode's law, on the assumption of which the original investigations of M. Le Verrier and Mr. Adams entirely de- pended, fails completely. Calcul detaille d'une In^galit6 Nouvelle a Longue Periode, qui existe dans la Longitude moyenne de la Lune. By M. Hansen. The author states that he has lately made known to some astro- nomers a discovery of two inequalities in the motion of the moon, whose periods are respectively nearly 273 and 239 years. Denoting by g, g' , g" the geocentric mean anomaly of the moon, and the helio- centric mean anomalies of the earth and Venus, these inequalities are^— 27"-4x sm(-g-l6g'+l8g" + 35° 20'-2) -f-23"-2 X sin (8i^"-13^'-f-315° 30') ; of which the first depends on a new argument, while the second depends on the argument of an equation of long period in the motion of the earth, discovered by Mr. Airy. As the calculation of those parts of the coefficients which depend on the product of the square and cube of the sun's disturbing force by the disturbing force of Venus is extremely laborious, and is more- over connected with other unpublished calculations of other inequa- lities of the moon, it does not appear possible to publish it at pre- sent. Indeed M. Hansen does not consider himself able yet to answer for their perfect correctness, though he has the strongest reason to believe that they are very nearly correct. The present paper therefore includes only the calculation of that part of the co- efficient of the first inequality which depends on the first power of the disturbing force. It appears difficult to abstract very completely the remaindef of this paper, but the following indications will enable a person ac- quainted with the developments of physical astronomy to follow the whole process. The perturbing function CI for the moon as disturbed by Venus being formed, it will be found that it may be expanded in a rapidly lloyal Astronomical Society. 383 converging series of fractions, whose numerators contain successive powers of r, the moon's radius vector, and whose denominators contain different powers of the same multinomial (which, when ec- centricities and inclinations are omitted, is a trinomial) that occurs in computing the perturbations of the earth by Venus. Upon ex- panding any of these fractions with trinomial denominator, there occur terras depending on \Q(j" — \Gg\\lg" —ilg' ,axidi \Sg" —\%g' : then, upon introducing the inclinations and eccentricities, the first (among other combinations) will be multiplied by sin^ \ inclin. x cos 2g"—'2 V (where v is the difference of longitude of node and pe- rihelion of Venus), and also (in other terms) by e"'^ cos 2 g' ; the second by e". e' cosg" + g' ; and the third by e'^ cos 2 g'. Each of these combinations produces terms whose argument is IS g''—16 g'. Then upon multiplying these terms by a power of r, since the ex- pression for any power of r contains e. cos g, the product will contain terms depending on IS g''— 16 g'~g. The coefficient necessarily contains one of the following products of three small quantities : p. sin^ ^ inclin., e . e"^, e.e'.e', c.e''^ (of which the first is the most im- portant), and it is therefore extremely small; but the resulting perturbation is made important by the excessive smallness of the divisor introduced in integration. It is well known that the divisor in this case will be proportional to ( 18 -^ — 16 -^ ^ | ; and, *^ ^ \ dt dt dt) tin" taking for -—-, & dt to a Julian year. dn" taking for -^, &c., the value in sexagesimal seconds corresponding dt ^ =2106G41"-3 dt ^=1295977-4 dt *^ = 17179167'4 , dt whence 18^ -16^' -^ =4747"-7, dt dt dt a quantity very small in comparison with -^. dt In this manner the greatest part of the term in question is pro- duced. Other parts arise from the circumstance that, the dimen- sions of the moon's orbit being slightly altered, the perturbing force of the sun upon the moon is not the same as it would otherwise be. M. Hansen remarks that this term is remarkable as depending upon higher multiples of the anomalies than have ever before been considered, and as having the longest period in proportion to the periodic time of the disturbed body that is yet known. The term depending on S g" —\^ g' arises mainly from the cir- cumstance, that, the earth's motion in its orbit being different from what it would have been without the perturbation by Venus, the disturbing force of the sun upon the moon is not the same as if that perturbation had not existed. SS* lioyal Astronomical Society. M. Hansen states that he has examined several inequalities of long period in the moon's motion which hitherto have escajjed notice, but that in no other instance does the coefficient amount to 1". In concluding the account of this remarkable discovery, it is gra- tifying to add that it explains almost precisely the observed inequa- lity in the moon's mean motion, which for the last fifty years has troubled physical astronomers. After the reading by the Secretary of a portion of this paper, the Astronomer Royal gave an oral explanation of its general subject in the following manner : — The disturbing effect of Venus upon the moon is not the whole attraction of Venus upon the moon, but the difference of the two attractions, of Venus upon the moon and of Venus upon the earth. Thus, when the moon is between the earth and Venus, the attrac- tion of Venus upon the moon is stronger than that of Venus upon the earth, and therefore it tends to pull Venus away from the earth. When the moon is more distant from Venus than the earth is, the attraction of Venus on the earth is the stronger, and tends to ])ull it away from the moon, which, in regar'd to the disturbance of the relative jilaces of the earth and moon, is the same thing as pulling the moon away from the earth. In both these positions, therefore, the disturbing force of Venus tends to pull the moon away from the earth. When the earth and the moon are equally distant from Venus, the attractions of Venus upon the two are equal, but not in parallel lines ; the attractions tend to draw them along the sides of a wedge whose point is at Venus, and, therefore, to diminish the distance between them, or to push the moon towards the earth. Inasmuch as, in one pair of positions of the earth and moon, the disturbing force of Venus tends to increase the distance between them, and in another pair of positions it tends to diminish that di- stance, it is important to ascertain which of these disturbances is the greater. Suppose the distance of the moon from the earth to be Y^ part of the distance of the earth from Venus. Then, when the moon is between the earth and Venus, its distance from Venus is yW of ^^^ whole ; the force upon it is '^^y* ^^ ^^^^ upon the earth ; the excess of this (or the disturbing force tending to pull the moon away from the earth) is -gV^' °^' nearly -^^ of that on the earth. In like manner, when the moon is further from Venus than the earth is, its distance from Venus is -Lg-^ of the earth's distance ; the force upon it is ^g^g° of that upon the earth ; the defect of this (or the disturbing force tending to pull the earth away from the moon) is , gg' . or nearly -A- of that on the earth. But when the earth and 10201' J 5 1 , -,. the moon are at equal distances from Venus, the proportion of then- relative approach (as produced by the action of Venus) to the whole effect of Venus upon them, is evidently represented by the inclina- tion of the two lines drawn from them to Venus, or is the same as the proportion of the distance of the moon from the earth, to the distance of the earth from Venus, and is therefore yi^^ of the whole. Thus the force tending to pull the moon from the earth at one time is about double the force tending to push the moon towards the earth at another time ; and therefore, upon the whole, the tendency of the Royal Astronomical Society. 585 disturbing force of Venus is to pull the moon from the earth. To arrive at this conclusion, we have considered only four points of the moon's orbit : in other points the effects of the perturbation are more complicated ; but they do not alter this general conclusion. The same remark applies to the disturbing effect of Venus upon the moon when at a given point of its orbit, provided the nature of that point be such that at different times it is in all possible posi- tions relative to Venus. For instance, the moon's apogee is (in consequence of the motion of the line of apses, and of the relative motions of the earth and Venus) sometimes between the earth and Venus, sometimes more distant from Venus than the earth is, some- times 90° to the right, sometimes 90° to the left. We may assert therefore that, upon the whole, the disturbing force of Venus upon the moon, when she is in apogee, tends to draw her away from the earth. The same may be predicated when the moon is in perigee. Next, it is important to ascertain how the disturbing force de- pends upon the moon's distance from the earth. For this purpose, instead of supposing, as before, that the moon's distance is y^-g- part of the distance of the earth from Venus, let us suppose it y^ part of that distance. Then when the moon is between the earth and Venus, the force upon the moon is VWx" °^ ^^^^ upon the earth, and there- fore the excess, or the disturbing force, is ^qj, or nearly -^ of the whole force upon the earth. In the former assumed instance it was ■gL. Thus, upon doubling the moon's distance from the earth, the disturbing force is doubled. And similarly for other distances of the moon from the earth, the disturbing force (in similar positions with regard to Venus) is proportional to the moon's distance. Thus, when the moon is at apogee, in a given position with regard to Venus, the disturbing force is greater than when the moon is in perigee in the same position. And, upon the whole, in all possible relative positions of the moon and Venus, the action of Venus pulls away the moon from the earth, more when she is in apogee than when she is in perigee. Now we may consider the general effect of these forces upon the dimensions of the moon's orbit. So long as the force which draws the moon towards the earth is always the same at the same distance, the moon will continue to describe an orbit of the same dimensions over and over again. But if at any time the force directed towards the earth suddenly grows smaller, the moon will immediately rush off in an orbit which, on the opposite side, is larger. If the force towards the earth gradually grows smaller, the dimensions of the orbit will gradually increase. And the periodic time in the orbit described at every successive revolution will undergo the change corresponding to the change of dimensions (that is, to the change of major axis) of the orbit, and will therefore become continually greater and greater. These are the changes which produce the most serious disturbance in the apparent place of the moon. If a force, after acting for a long time, produce a small change in the eccentricity of the moon's orbit, the effect on the moon's place is simply the amount of the corre- Phil. Mag. S. 3. Vol. 31. No. 209. Nov. 1 847. 2 C 386 Royal Astronomical Society, spending change in the equation of the centre, and cannot possibly exceed that amount. But if the force have been for a long time gradually altering the major axis, and consequently the periodic time in the moon's orbit, then during the whole of that time the moon has been performing her revolutions quicker or slovi^er than we expected, and therefore at the end of that time she is in advance or in retard of her expected place by an amount equal to the accu- mulation of all the advances or retards in all the revolutions through which the change has been going on. The planetary inequalities of long period are all of this kind. The major axis here plays the same part as the pendulum of a clock. If a small force acting for a year pushed the seconds-hand forwards by an inch, the clock would be merely a few seconds wrong ; but if in the same time it shortened the pendulum by an inch, the clock would have gained fifty hours ; and if the time occupied by the change had been greater, the dis- turbance in the clock indication would have been proportionably greater. In order then to find inequalities of long period in the motion of the moon produced by Venus, we must seek for some alternate in- crease and decrease, occupying a very long period, in the force by which Venus draws the moon from the earth. No such slow increase and decrease have been found in the general force by which Venus disturbs the moon. The next point of inquiry is, whether a combination of the changes in the force of Venus with the changes in the position of the moon in its orbit can produce a force, which, for a very long time together, gradually increases the force drawing the moon from the earth, and then for an equal time gradually diminishes that force. A force which acts in opposite ways, nearly on opposite sides of the moon's orbit (pulling the moon from the earth on one side and pushing it towards the earth on the other side), may produce this effect, provided the period of the change in the nature of the force (from pulling to pushing) correspond nearly, but not exactly, with the time in which the moon moves from apogee to perigee. For (as we have seen) the effect of a certain force of Venus is to produce a greater disturbing force on the moon at apogee than at perigee ; and this force, or a change in this force, will, at apogee, produce a greater effect on the dimensions of the moon's orbit than at perigee, both because the disturbing force is actually greater, and because it acts on the moon when the moon's velocity is smaller. Therefore, if a pulling force, gradually increasing in magnitude, act on the moon at apogee, it will gradually increase the dimensions of the moon's orbit : if a corresponding pushing force act at perigee, it will gradually diminish the dimensions of the moon's orbit; but the former prevails, and the orbit will gradually increase in size. If after a time the pulling force at apogee gradually diminish, and at length become a pushing force, while the pushing force at perigee gradually diminishes, and at length becomes a pulling force, then the orbit will gradually diminish in size. And this change of forces would be produced by such a modification in Venus's force, as that Royal Astronomical Society. 387 of which we have spoken, namely, a force which acts in opposite ways on opposite sides of the moon's orbit, and in which the period in the change of the nature of the force coincides nearly, but not exactly, with the time in which the moon moves from apogee to pe- rigee ; for then the pulHng force at apogee will after a long time be changed to a pushing force, and the pushing force at perigee will in the same time be changed to a pulling force. If, for instance, the change in the disturbing forces of Venus (from pushing to pulling) occupied fourteen days exactly, and if the moon's motion from apo- gee to perigee occupied fourteen days and five minutes, then in 4032 anomalistic semi-revolutions of the moon (which would bring her from apogee to apogee), there would have been 4033 changes of the force (which would change it from pulling to pushing), and there- fore in this time, and no sooner, a complete pulling force at apogee would be changed to a complete pushing force at apogee. It is necessary now to point out how such a modification of the force of Venus can be found. The only disturbing forces which are yet completely brought under the management of mathematicians are of two kinds ; a constant force (always pushing or always pulling with the same amount of force), and a force alternately pushing and pulling, having equal periods and equal maximum magnitudes in each state. The latter of tliese, if projected graphically, with the time for abscissa, is re- presented by the ordinates of a line of sines : algebraically, it is ex- pressed by tt.cos (^bt + c). Now, while the relative positions of the earth and Venus change, the disturbing force on the moon (estimated by the force which, on the whole, it exerts to pull the moon from the earth) undergoes very great changes. When Venus is nearest to the earth, this force is about 250 times as great as when Venus is furthest from the earth. It declines very rapidly from its greatest magnitude. If therefore we represent the disturbing force from one conjunction to the next by a curve, this curve will be very high at the beginning and end, and very near the line of abscissa at the middle, and through the greater part of its extent. The separation of this foi-ce into a number of different forces, fol- lowing the two laws mentioned above, is effected by a process sug- gested and facilitated by algebra, but in which, nevertheless, every step has its physical meaning. It may be stated at once, that this remark applies universally to the algebraical operations of physical mathematics. As a simple instance, we may refer to the equation (a + bysz a3 -J- 3 a"^ b +3 ab'^ + b^, which probably was suggested by algebra ; but which may be illustrated by taking a cube, whose side is a + b, and (by three saw-cuts) cutting it into eight pieces, when the single piece representing a^, the three pieces each representing a- b, the three pieces each representing ab^, and the single piece representing b^, will be found. And there is perhaps no better dis- cipline for the mind than thus tracing the evidence of the truth of algebra, especially in its more profound processes. The separation, then, of the force of Venus goes on by the fol- lowing steps : — 2C2 888 Royal Astronomical Society. 1st. A constant pulling force, equal to the mean value of the force. 2nd. A force pulling when Venus is in conjunction, pushing at the time intermediate to the conjunctions, and pulling when Venus is in conjunction again ; thus going completely through its changes once between conjunction and conjunction. 3rd. A force pulling when Venus is in conjunction, then pushing, &c., going through its changes twice. 4th. A force pulling when Venus is in conjunction, then pushing, &c., going through its changes thrice. In this manner the forces go on, continually diminishing in magni- tude. When we arrive at the 18th, the force is extremely small. The algebraical expression for the collection of these terms, put- ting fl for the difference of mean longitude of the earth and Venus, is A-i-B . cos HC . cos 2 9 + D . cos 3 9 + &c, This is on the supposition that the orbits of the two planets are circular and in the same plane. But, in consequence of their eccen- tricities and inclinations, the forces of any one system alternately pushing and pulling (Nos. 2, or 3, or 4, &c.) will not have the same maximum magnitude throughout. But each can, in all cases, be expressed by the combination of three such forces, in each of which the maximum forces are equal throughout. Thus, if we combine a large force, going through its changes twenty times in a certain period, with a small force going through its changes nineteen times in the same period, and another small force going through its changes twenty-one times in the same period, then it will be found that both the small forces increase the large force (whether in its pulling or in its pushing state) near the beginning and the end of the time; that both diminish the large force near the middle of the time ; and that the two small ones destroy each other at a quarter and three-quarters of the time. The elFect of this combination is therefore precisely such as is spoken of above. Thus, then, for the complete expression of the force, we are driven to an infinite number offerees following the law of alternately pulling and pushing, but with very great variety of magnitudes of force and of periodic time. The greatest portion of these produce no sensible effect ; some because (though their magnitudes are large) they act for so short time in one way, or their periods are so little related to the periods of any movement of the moon, that their effects never accumulate ; others because their magnitudes are small, and there is no unusual circumstance favourable to their increase. But there is one of these forces which, in the algebraical expres- sion, depends on 18 x mean longitude of Venus — 16x mean lon- gitude of the earth, whose coefficient is exceedingly small, but which goes through all its changes, from pulling to pulling again, in the time, 27'^ 13»» T'^SS^'G; or from pulling to pushing, in the time 13d \^^ 33™ 47«-8. Intelligence and Miscellaneous Articles. 389 Now, the anomalistic revolution of the moon, from apogee to apogee again, is performed in the time 27d i3h i8«» 32«'3; or from apogee to perigee, in the time IS'i 18^^39"^ 16«-1. Here we have a real instance, exactly corresponding to the case which, for the sake of explanation, we assumed a short time back, and the results are truly such as were there described. During about 4000 half-revolutions of the moon, or 2000 revolutions, the pulling force at apogee is gradually diminishing till it becomes a pushing force, and during about 2000 more revolutions, the pushing force at apogee is gradually diminishing till it becomes again a pulling force ; the opposite changes going on in the force at perigee : and thus, for reasons fully explained before, the moon's orbit is gradually con- tracting during 2000 revolutions, and gradually expanding during 2000 revolutions more. And although the change in the size of the orbit is totally insensible in observation (for, according to a rough calculation, the utmost accumulation of change in the major axis of the moon's orbit is only ten feet, sometimes in increase and some- times in decrease), yet the consequent alteration in its periodic time, continued through so many revolutions, is sufficient to cause the irregularity in question. The inequality in longitude, as measured on the moon's orbit, exceeds thirty miles, sometimes in advance, and sometimes in retard. For a complete understanding of this matter, it must carefully be borne in mind that the force at the apogee, which has been described as a pushing force through 136 years, is not absolutely a pushing force through every month of that time, but that (in consequence of the motion of the moon's line of apses) if we take any period of nine or ten years, the moon's apogee will in that time have passed through every position with regard to Venus, and therefore, upon the whole, during that period of nine or ten years, the force at apogee will have been a pushing force. In like manner, in another period of 136 years, if we take any period of nine or ten years, upon the whole, during that period of nine or ten years, the force at apogee will have been a pulling force. The general cause of the inequality depending on the argument 8p"— 13^', has been sufficiently stated in one of the last paragraphs of the abstract of M. Hansen's paper. LXIII. Intelligence and Miscellaneous Articles. ON THE GELATINOUS SUBSTANCES OF VEGETABLES. MFREMY, in a memoir read before the Academy of Sciences, • has arrived at the following conclusions : — 1st. There exists in vegetables, along with cellulose, a substance which is insoluble in water, alcohol and aether, which the author 890 Intelligence and Miscellaneous Articles. n&mes peciose, and which, by the action of the weakest acids, is con- verted into pectin. Diluted acids produce this effect only at the temperature of ebullition ; and acetic acid, which, as is well known, does not act upon starch, is also without action on pectose. Pectose cannot be confounded with cellulose, for the latter, as was ascer- tained by M. Payen, gives no traces of pectin when treated with acids. M. Fremy's experiments confirm those of M. Payen. 2nd. The author has found in the greater number of fruits and roots, an amorphous substance, comparable to ferments, and espe- cially to diastase : the gelatinous substances contained in vegetables experience by its action a series of isomeric transformations. This substance M. Fremy calls pectase ; in acting upon the gelatinous sub- stances it gives rise to the different phsenomena which constitute pectic fermentation. 3rd. The acids which are employed to convert pectose into pectin, may, according to their nature and proportion, form different sub- stances, each of which possesses well-delined distinctive properties. Thus, when the acid is very weak, pectin, properly so called, is ob- tained, which does not render acetate of lead turbid. If the acid be more concentrated, or if the ebullition has been longer continued, the substance formed precipitates the neutral acetate of lead ; this substance the author calls parapectin; and lastly, by employing a powerful acid, a third substance may be formed, which is distin- guished by the name of metapectin ; this is feebly acid to coloured test-papers, and precipitates chloride of barium ; the other com- pounds are neutral. 4th. If a small quantity of pectase be added to a solution of pec- tin, and the temperature be kept at about 86° F., the pectin is soon observed to change into a gelatinous, consistent substance. This curious transformation, which explains the production of vegetable jellies, may be effected without the contact of the air ; there are formed in this case two acids ; one is new, and termed pectosic acid, and the other is pectic acid. Pectosic acid, which might be con- founded with pectic acid, is immediately distinguishable from it by its perfect solubility in boiling water. In the reaction of pectase on pectin, pectosic acid is first produced, and is afterwards changed into pectic acid by the prolonged action of the pectase. The free alkalies or their carbonates are capable of converting in the cold, pectin at first into pectosates and afterwards into pectates. The phsenomena now described are so easy of observation, accord- ing to M. Fremy, and characterize pectin so distinctly, that he finds it difficult to imagine how in later times pectin has been confounded with gums, mucilages, aad especially with pectic acid, which is insoluble in water. The author has particularly examined pectic acid, and is of opinion that he has overcome the difficulties attendant upon its analysis, and especially the determination of its equivalent. He has also found that pectic acid, heated to 392° F., loses water and carbonic acid, and a new pyrogenous acid, which he calls pyropectic acid, is pro- duced. InteUiaence and Miscellaneotts Articles. 391 "is Pectic acid possesses the singular property of dissolving in con- siderable quantity in neutral or acid salts ; it then forms com- pounds precipitable as jellies by alcohol ; these precipitates are often mixed with pectin, render it gelatinous, and prevent by their presence the recognition, by means of elementary analysis, of the simple relations which connect pectin with the other gelatinous bodies. 5th. The gelatinous bodies may undergo a last period of trans- formation, and be changed into two very soluble and energetic acids. It is sufficient to boil pectic acid in water for a certain time to con- vert it into an acid, called by the author parapectic acid, and into another acid termed metapectic acid. The parapectic and meta- pectic acids are also formed during the action of acids or alkalies on pectin or pectic acid : the pectates may by long boiling be con- verted into metapectates. These two acids are readily distinguished from each other ; for the first precipitates barytes water, and the second does not ; they decompose the double tartrate of copper and potash, as glucose does. To be certain that this property was not derived from the presence of sugar, the author had recourse to a polarizing apparatus and the action of yest. Guided by the advice of M. Biot, M. Fremy found that the parapectic and metapectic acids effected no rotary action on polarized light, and that the presence of yest produced no traces of fermentation. 6th. After having examined all the properties of the gelatinous bodies, and found that by employing very weak agents, comparable to those which exist in vegetables, their acidity might be suc- cessively developed, and from neutral bodies, which they originally were, they might be transformed into energetic acids, the author examined whether, during the act of vegetation, gelatinous substances did not undergo changes comparable to those which he had pro- duced artificially. On following for two years, with this intention, the modifications which are effected in fruits during their matura- tion, M. Fremy found that the gelatinous bodies which occur in them could pass through the different intermediate states which he has described ; thus green fruits contain abundance of pectose. As maturation advances the pectose is changed into pectin ; and when the fruits are perfectly ripe, the pectin is frequently completely con- verted into metapectic acid. The modifications examined in this memoir are then precisely those which occur during the maturation of fruits. The author found in the numerous analyses which he performed that the composition of the gelatinous bodies could not be repre- sented by carbon and water, and consequently that they were far removed from neutral bodies, properly so called. As experiment always indicates a larger quantity of hydrogen than really exists in organic bodies, the author states that he cannot attribute the differ- ence which he has obtained to an error of analysis. The table presented to the Academy shows that all gelatinous substances, similar to those which are derived from starch, are iso- meric, or at least they differ only by the elements of water. This Intellige7ice and Miscellaneous Articles. result might be foreseen ; for when a mixture of pectase and pectin is put into a bottle, and it is hermetically sealed, the pectin is suc- cessively converted into pectosic, pectic, parapectic, and metapectic acids, without forming any secondary product. The capacities of saturation given in the following table prove that the acidity of the gelatinous bodies increases in proportion as their equivalent diminishes. Thus parapectin, the equivalent of which is very heavy, forms a neutral salt with lead which contains 10 per cent, of oxide, and does not redden tincture of litmus ; and meta- pectic acid, the equivalent of which is very light, produces a salt of lead which contains 67 of oxide, and its acidity resembles that of malic or citric acid. Names of the gela- Composition of the Composition of the tinous substances. gelatinous substances. salts of lead. Pectose Pectin C6+ H« O^e, 8H0 Parapectin C^" H^o O^^ 8H0 C^ H^o 0^\ 7H0, PbO Metapectin ...... C^*W 0^\ 8H0 C«i H••>>.. . 43-85 Hydrogen 6*22 Oxygen 49-93 100-00 Blotting-paper treated with acids, alkalies, water, und alcohol, dried at 288° F. :— I. XL Carbon 43-87 43*84 Hydrogen 6-12 6*22 Oxygen 50-01 49*94 100-00 100-00 398 Intelligence and Miscellaneous Articles. Cotton treated only with boiling water, hydrochloric acid, and dilute solution of potash, cold : — I. II. Carbon 43-46 43*10 Hydrogen .... G'38 6-43 Oxygen 50-lG 50-45 100-00 99-98 Flax, treated like cotton : — I. II. Carbon 43-92 43'33 Hydrogen 6-01 6 41 Oxygen 50*07 50*26 100-00 100-00 Papyrin. — In employing sulphuric acid to determine the purity of lignin, the authors have discovered a new substance which consti- tutes a very curious modification of ligneous tissues. It results from the first action of sulphuric acid on lignin, and is the product which arises before its conversion into dextrin. Let blotting-paper be immersed for not more than half a minute in concentrated sulphuric acid, and then be immediately washed with a large quantity of water to prevent the action of the acid ; and if it be then immersed for a few moments into water containing a few drops of ammonia, a substance is obtained which possesses all the physical characters of an animal membrane. When moistened with water, it has the soft and greasy feel of animal membrane softened in water ; when dried it has the appearance and the toughness of parchment, and when glazed it has considerable transparency. This substance, which the authors call j^apijr'm, is identical in composition with lignin. It was found to yield— I. II. III. Carbon 43*30 43*89 44*44 Hydrogen 6*28 6-27 6-23 Oxygen 50-42 49*84 49*33 100*00 100-00 100-00 Journ. de Ph. et de Ch., Aout 1847. SOLUBILITY OF CHLORIDE OF SILVER IN HYDROCHLORIC ACID. M. Pierre states that concentrated hydrochloric acid is capable of dissolving j-i-^dth of its weight of chloride of silver ; when it has been diluted with twice its weight of water, it is capable of retain- ing more than -^i^dth of its weight. M. Gerhardt observes that this fact is important, and says he had previously stated it ; and it appears to him to be the cause of the difference of the numbers obtained by MM. Berzelius and Ma- rignac as to the theoretical number expressing the atomic weight of chlorine according to Dr. Prout's law of multiples. — Ibid. Sept. 1847. Meteorological Observations. 399 Daubeny on Active and Extinct Volcanos. Professor Daubeny of Oxford has in the press, and nearly ready for publication, a new and much-enlarged edition of his Description of Active and Extinct Volcanos. The present Edition will be found to contain nearly twice the amount of matter included in the preceding one, embracing not only such new facts and observations with respect to volcanos as have been brought to light since its first appearance in 1826, but likewise the allied phsenomena of Earthquakes and Thermal Springs, as well as a fuller discussion of the theories connected with those subjects. METEOROLOGICAL OBSERVATIONS FOR SEPT. 1847. Chiswick. — September 1. Clear: cloudy: clear. 2. Cloudy: boisterous. 3. Cold rain : overcast. 4. Fine. 5. Clear : shower : clear. 6. Very fine. 7. Clear and cold : cloudy : rain at night. 8. Rain. 9. Very fine. 10. Overcast : very fine. II, 12. Very fine. 13. Densely overcast: rain. 14. Very fine : slight shower: clear and cold at night. 15. Fine: boisterous, with rain at night. 16. Boisterous. 17. Rain. 18. Cloudy, with very clear intervals. 19. Cloudy: heavy rain at night. 20. Fine: slight showers. 21. Rain. 22. Cloudy: fine. 23. Cloudy and mild. 24. Foggy : very fine. 25, 26. Fine. 27. Frosty : clear : very fine : clear and frosty at night. 28. Slight fog ; overcast. 29. Slight fog : very fine. 30. Dry haze : overcast. Mean temperature of the month 53°'40 Mean temperature of Sept. 1846 60-79 Mean temperature of Sept. for the last twenty years 52 '77 Average amount of rain in Sept 2*73 inches. Boston. — Sept. 1. Fine. 2. Windy. 3. Cloudy : rain p.m. 4. Fine. 5. Fine: rain P.M. 6,7. Fine. 8. Cloudy. 9 — 11. Fine. 12. Windy. 13. Rain: rain A.M. and P.M. 14. Fine. 15. Fine: rain p.m. 16. Fine: stormy from 10 A.M. 17. Cloudy. 18 — 20. Fine. 21. Fine: rain p.m. 22. Cloudy : rain A.M. 23. Cloudy. 24—28. Fine. 29. Cloudy. SO. Fine. Sandwich Manse, Orkney. — Sept. 1,2. Showers. 3. Bright: showers: sleet. 4 — 6. Showers. 7, 8. Cloudy : showers. 9. Drizzle : showers. 10. Cloudy. 11. Cloudy: rain. 12. Showers. 13. Cloudy : clear. 14. Cloudy. 15,16. Bright : rain. 17. Cloudy : showers. 18. Showers. 19. Clear : showers : sleet. 20. Showers: rain: cloudy. 21. Bright: fine. 22. Damp: rain. 23. Showers. 24. Showers : cloudy. 25. Rain : clear. 26. Bright : clear. 27, 28. Clear. 29. Clear: aurora. 30. Clear. Applegarlh Manse, Dumfries-shire. — Sept. 1. Sharp showers and high wind. 2. Clear and fine harvest day. 3. Rain. 4. Fine clear sharp weather. 5. Fine harvest day. 6. Clear and bracing. 7. Rain, though not heavy. 8. Fair, but cloudy. 9. Close rain. 10. Fine : some drops p.m. 11. Fair a.m. : rain p.m. 12. Fair, but threatening. 13. Fine. 14. Bracing day : flying showers. 15. Fine a.m. : heavy rain p.m. 16. Rain and high wind. 17. Few drops of rain. 18. Fair, but dull. 19. Frequent showers. 20. A few drops. 21. Rain p.m. 22, 23. Showery. 24. Fair and fine. 25. Slight drizzle. 26. Very fine day. 27. Very fine day: frost a.m. 28, 29. Very fine days : no frost. 30. Fair, but cold. Mean temperature of the month 50°"9 Mean temperature of Sept. 1846 59*6 Mean temperature of Sept. for 25 years 53 '2 Mean rain in Sept. for 20 years , 3*13 inches. m •^loiAipaBg ■uoisog •5[3!.vis!qo •5{0!.»pu«g ■ajiqs -saiJjuinci ■uoisog •ui'd t 0:5? •lU'B 16 Sic •uojsoa •ii!H •XEJtt •*•£ ^§ ■uoisoa JO SiCBQ ^c« ^ & Bt & ^ g a a a a a § a G a c a ^ e P P ? « c8 a a M ^ ^ ^ C > ^ ? c' ^ ri 2 B:" >■ ^" ^' & & ^ 3 ^- ^' ^' i ■! i ^^i^tci^o cJ c a ^ m S p *■ fe • • J te J ^ ^ J ^ • -B • > f- -• t: -• t; J fe ^* 5= i.- u u u u o ^ ^ S S S cu S i 5^' i i i ?■ ^' ^* ^' ^ ^ i i ^ ^ ^i^i^i^^i^'^i-^'^ i o^O^O^<3^0^6^0^0^CT^O^'i) o^c^c^O^O^c^o^o^O^O^O^O^O^O O O O C O .i:— loooiyi— ^oOlOOO^t^ooa^-^lr5rt'*■<^l^o■^loaoc^^^oc^lOc»(^^l^co lr:l:-^t:^^-~l>.^:^t^^l>.l:^o^o^^p^o^ocpe^c^^py^ap^^^po«7•7'CO^0L0<~0l:^^0CM-^|-l ncoip-rPcocoipTfipip^p cocorO'^C^O O rj

    -^ ■^ CO 00 op O^ C?s 0^ (N !N o^ a\ c^io o lOOO — o o o 00 lO 00 r^ c^oo lO o 00 1-- o^oo tc CO CO ■<* LO « — CO lO (N CO o a^ — 1 -* — 1 C^ O O t-^ lO C^ COU5 cyvco — < — ^a;'5 to be taken away." And further down at(2435), " Whether the negative results obtained by the use of gases and vapours depend upon the smaller quantity of matter in a given volume, or whether they are the direct consequences of the altered physical condition of the substance, is a point of very great importance to the theory of magnetism. I have imagined in elucidation of the subject an experiment, &c., but expect to find great difficulty in carrying it into execution, &c." Happily P. Bancalari's discovery has now settled this matter On the hifluence of Eleclro-magnetism upon 'Flame. 421 for us in a most satisfactory manner. But where the trne zero is, or that every body is more or less removed from it on one side or the other, is not, as yet, experimentally shown or proved. I cannot conclude this letter without expressing a hope that since gases are shown to be magnetically affected, they will also shortly be found, when under magnetic influence, to have the power of aff'ecting light (Experimental Researches, 2186, 2212). Neither can I refrain from signalizing the very re- markable and direct relation between the forces of heat and magnetism which is presented in the experiments on flame, and heated air and gases. I did not find on a former occasion (Experimental Researches, 2397) that solid diamagnetic bodies were sensibly affected by heat, but shall repeat the ex- periments and make more extensive ones, if the Italian philo- sophers have not already done so. In reference to the effect upon the diamagnetic gases, it may be observed that, speaking generally, it is in the same direction as that of heat upon iron, nickel and cobalt ; /. e. heat tends in the two sets of cases, either to the diminution of magnetic force, or the increase of diamagnetic force; but the results are too few to allow of any general conclusion as yet. As air at different temperatures has different diamagnetic relations, and as the atmosphere is at different temperatures in the upper and lower strata, such conditions may have some general influence and effect upon its final motion and action, sub- ject as it is continually to the magnetic influence of the earth. I have for the sake of brevity frequently spoken in this letter of bodies as being magnetic or diamagnetic in relation one to another, but I trust that in all the cases no mistake of my meaning could arise from such use of the terms, or any vague notion arise respecting the clear distinction between the two classes, especially as my view of the true zero has been given only a page or two back. I am, my dear Sir, Yours, &c., Richard Taylor, Esq., M. Faraday. Ed. Phil. Mag., Src. Sfc. LXV. On the Motions -presented by Flame when wider the Electro-Magnetic Influence. By Prof. Zantedeschi. THE most eminent philosophers have at all times maintained the universality of the magnetism of bodies* ; and in our days Faraday is the only one who has placed the expansi- * Raccolta Fisico-Chimica Italiana, t. iii. Dei corpi magnetici e dia- magnetici. 422 Prof. Zantedeschi on the Motions presented hy Flame ble fluids at the zero of the scale of action among magnetic and diamagnetic bodies. On the 21st of September 1847, at the Physical Section of the Ninth Italian Scientific Congress in Venice, Padre Bancalari, Professor of Physics in the Royal University of Genoa, read a memoir on the universality of magnetism ; and the argument was considered by philosophers to be of such importance, that a desire arose to verify chiefly the action of magnetism on expansible fluids. It was an- nounced by the Reporter Belli at the sitting of the 27th of September, that it had been proved in the presence of various philosophers that, on the interposition of a flame between the two poles of an electro-magnet, it was repulsed at the instant the electric current was closed, to return to the first position the instant it was broken. This discovery received well- merited applause in the sitting of the 28th of September, from the General Secretary and the Secretary of the Section of Physics. A wish was expressed by some to witness the experi- ment of Bancalari; and a Daniell's apparatus having been got ready, often elements eighteen centimetres each in dimension, I endeavoured to repeat the experiment in the Cabinet of Physics of the Royal Imperial Lyceum of Venice; but I did not chance to see the asserted phaenomenon. My temporary magnet had the power of sustaining above 48 kilogrms. weight; but as my principle is, that a negative argument never destroys a positive one, I for my further information requested the machinist Cobres to give me the particulars of the apparatus; Belli not having treated of these in his report, and they having escaped Prof. Zambra, the Secretary of the Section. I knew that the two pieces of soft iron, which constituted the inter- rupted anchor, were perforated in the axial direction. I suspected that the repulsion of the flame was not the immediate effect of the magnetism, but of two currents of air issuing from the apertures of the perforated keeper generated by a vorticose movement produced by the magnetism, as the celebrated Faraday had observed in liquids* ; and I was confirmed in this suspicion by the negative experiment which I had instituted in Venice with solid pieces. On arriving in Turin, I communi- cated my doubts to the well-known mechanicians Jest, father and son, who to their professional abilities unite a rare courtesy. They soon furnished me in their laboratory with a Bunsen's ap- paratus, and constructed terminal pieces of soft iron forming the interrupted anchor, both solid and pierced, of a parallelepipe- don and cylindric form, as I pointed out to them ; and I have repeated the experiments in their company : the temporary * RaccoHa, cited above, t. ii. Relazione dell' influenza delle forze elet- triche e magnetiche sulla luce ed il calorico. ijohen und£r the Electro-Magnetic Influence. 423 magnet, made in the shape of a horseshoe, was formed of a cyhnder of soft iron of the length of 0"^*335 and the diameter of O'^'OIS; and its electro-magnetic spiral was formed of a copper wire 33"^ long, and of a diameter of a millimetre and a third ; the internal distance of the poles was 0'"'027; the two solid parallelepipedon contacts, forming the interrupted anchor, were 0'»-04 long; and of the sides 0«i'01 1 and 0°^-006 : and the hollow terminal pieces were 0™*035 long ; and of the side 0™*009. They were placed at a distance from one another of four to five millimetres, the magnet being kept in a vertical position with the poles turned upwards. In front of the in- terval of the separation of the contact pieces was placed the flame of a small candle, or of a little oil or alcohol lamp, so that it surmounted with its top by nearly a fourth the thickness of the contacts. The electric circuit was closed by copper wires, and the metallic unions were maintained both at the magnetic poles and at those of the pile by clamps : one of the wires therefore was divided into two equal parts, and the ends being dipped into a tumbler of mercury, allowed the closing and opening of the circuit at pleasure. / have constantly observed repulsion ifi the act of closing the circle, which lasted the xohole time that the magnetism was kept up ; and, when in the act of opening the circle, I saw thejlame . return to its primitive position. Well-satisfied with having in this manner confirmed this important fact which reflects honour on its discoverer, I applied myself to the study of the phaenomenon, and I found — I. That this happens with contacts of both solid and hollow soft iron; whereupon I abandoned my suspicion that the movement of the flame was attributable to currents of air; I convinced myself that it was an immediate action of the mag- netism upon the flame, — a fact of the greatest importance to science. II. That the repulsion, when it is quite distinct and the flame quite pure, and terminated in a well-shaped top, is ac- companied by depression : repulsion and depression are simul- taneously observed at the closing of the circle ; the return of the flame and rising of the same, at the opening of the circle. III. That, ceteris paribus, the greatest effect takes place when the flame is touching the convex of the magfietic curves indicated b\j iron filings. IV. That the action is tiull, or almost nullf when the flame is placed in the centre of the interval which separates the two contacts. V. That in the manifestation of the effects stated above, it is not necessary for the contacts to be entirdy separated: they may 424 On the Lifluence of Electro -magnetism upon Flame. be placed at an angle and touch at two corners; the flame placed within the base of this triangle, generally manifests the two phsenomena indicated. VI. That thei'e is a certain mass of the contacts {or keeper pieces) "vohich is the most efficacious : bej/ond a limits nsohich can he shown by experiment^ increase of the mass causes a diminution of the effect: from this I found the cause of my negative results, which I obtained in Venice in the first experiments that I made. VII. That the movements of the fame increase isoith the number of the pairs {of battery plates). With one pair the effect was not perceptible to me* : with two pairs the movements began to show themselves ; with three pairs they became distinct, and increased with the increase of the number of pairs up to ten, which was the greatest that I employed in this experiment. The pairs were of the known ordinary size. On the repetition of the phaenomena as above stated, the precaution was taken to cover the apparatus with a bell, which was open above and supported by two discs below, which left a free access to the air, by which to support the combustion : in this manner all agitation and danger of disturbance under the circumstances were avoided. I must not forget, in concluding this article, to state that the celebrated Prof. Gazzaniga, starting from his numerous experiments, which demonstrate the influence of magnetism upon the same aeriform fluids, in a manner therefore different from that of Bancalari, was induced to consider the sun and all the other celestial bodies as so many enormous magnets; by which he established that attraction is merely an effect of the magnetism of the great celestial masses placed at an enormous distance, — an idea which reappeared in IH^Q in Prussia, and in ISi? in France, as we see fi'om the Comptes Mendus of the Royal Academy of Sciences at Paris, The mystery that attraction operates at a distance without inter- media would be removed in this case, and the phaenomena of attraction would enter again into the class of those of common dynamics. Dalla Gazz. Piem,, Oct. 12, 1847, No. 242. • Messrs. Jest prepared for me last evening an electro-magnet of a circular form interrupted by a prismatic section having an interval of two millimetres ; and I had, without need of contact pieces, the phaenomena distinct with a single element. The most conspicuous movements here appeared in the greater proximity of the flame to the section. The complete apparatus, of a circular form, furnished with a glass bell with its accessories is sold in Turin by Messrs. Jest, at the price of thirty francs, not including the electro-motor. [ 425 ] LXVI. On Asymptotic Straight Lities, Plmiesy Cones and Q/- linders to Algebraical Surfaces. By Thomas Weddle*. IN the Cambridge Mathematical Journal, first series, vol. iv, pp. 42-4' 7, the late D. F. Gregory gave a very excellent method of determining the asymptotes to algebraical curves. I here purpose considering the corresponding subject relative to algebraical surfaces ; and as this seems to have as yet en- gaged but little attention (if any), I trust the discussion will not be unacceptable to the mathematical readers of this Journal. Definitions. 1. A straight line which passes through a point at a finite distance and touches a surface at an infinite distance, is called an asymptotic straight line, or simply an asymptote to the surface. 2. 1( eve7-y straight line drawn in a plane be an asymptote to a surface, the plane is styled a conical asymptotic plane to the surface. 3. If all straight lines drawn in a plane parallel to a straight line in that plane be asymptotes to a surface, the plane is de- nominated a CYLINDRICAL asymptotic plane to the surface. 4. An asymptotic cone or cylinder to a surface is a cone or cylinder having its generators asymptotes to the surface. If =0*, where D denotes the operation ^:^D— ^^_,+ !► (3.) d ^ d d dl dm dn This equation will determine the values of r at the points in which the straight line (2.) cuts the surface (1.); now for all lines parallel to an asymptote, one of these points is evi- dently at an infinite distance ; hence a root of (3.) being infi- nite, we must have f;> = 0; (4.) and this equation determines the directions of the asymptotes. The equation (3.) hence becomes + 2. ..(5-1) = 0; (5.) in which values of/, m, n satisfying (4.) must be substituted. Now an asymptote being a tangent at an infinite distance, it follows that the asymptote will be distinguished from all lines having the same direction by a root of (5.) being infinite ; we must therefore have that is, Dfj, + fp-i = 0; ^a+$^/3 + d'Pn dl- dm'-^-d^'^-^^^'-'^^- (6.) The equation (4.) shows that every asymptote is parallel to some generator or other of the cone ^/.(•^i/2r) = 0; (7.) * In this paper I restrict 6,^,^,x (either with or without a letter or figure subscribed) to denote homogeneous functions only ; and when these sym- bols stand alone, they are to be understood as functions of /, m, n ; in otiier cases the symbols of quantity must be written ; thu? X(i(^I/^) ^^ homogeneous function of x,i/,z of the qth degree) means the same function oix,y,z that x„ does of /, m, n. Cones and Cylinders to Algebraical Surfaces, 427 and since («|3y) may be any point in each asymptote, (6.) de- notes the locus (a, /3, y being the variable coordinates) of the asymptotes parallel to the same generator of (7.) ; this locus is therefore a cylindrical asymptotic plane, and it is parallel to that tangent plane of the cone (7.) which touches along the generator. Hence, to find the equation of a cylindrical asymp- totic plane, we have only to take such values of /, m, n as satisfy (4.) and substitute them in (6.). It thus appears that when the cone (7.) is not imaginary, there is an indefinite number of cylindrical asymptotic planes ; one indeed parallel to every tangent plane of the cone (7.)> with a few excep- tions, which I shall consider presently. Should (4.), or, which is the same thing, (7.) be resolvable into factors, then (7.) will in reality denote as many conical surfaces ; and if any of these factors be of the first degree, the corresponding conical surface will degenerate into a plane. Let ^q be any factor of ip^, and put hence (6.) becomes when dj = 0, this reduces to and this equation, together with fl,^=0, will supply the place of (4.) and (6.) for those cylindrical asymptotic planes that are parallel to the tangent planes of the cone $q{x}/z)=:0. Also similar equations may be found for every factor of th degree, we have dl dm d7i hence the equations (9.) amount only to four independent equations — the last four. 4-28 Mr. T. Weddle on Asi/mptotic StraigJit Lines, Planes, of the first power of r that does not vanish independently of any relation among a, /3, 7. If this coefficient be that of r^-^, we have (10.) This equation denotes a surface which is evidently the locus of the asymptotes which are parallel to that generator of (7.) whose equations are — = ^ = — . Hence (10.) must denote 1 ^^ 1 ^^ I a cylindrical surface; and as its generators are all asymptotes, it is an asymptotic cylinder of the second degree (which may in certain cases degenerate into one or two cylindrical asymp- totic planes). Should the values of /,?«,» satisfying (9.) also cause a, /3, y to vanish from (10.), there will be no correspond- ing asymptotic cylinder, unless J/-/3, ^-7) = 0 for the equation to the asymptotic cone, which is the locus of the innumerable asymptotes that pass through the point (a/3y). (The factor ;)^,^ may sometimes be resolvable into other factors, and then the preceding asymptotic cone of the qth degree will in fact consist of several cones of inferior degrees.) The division of (4.) and (6.) by X'l will give two equations, ^'p_qZ=0, andx"p-q-i = 0) which admit of no common measure. Now (4.) and (6.) will be satisfied by these two equations; but the equations ^'p_q = 0, x"p-q-i =^j will determine not more than iP~^){P~9~^) ^^^^ of values of the ratios l-^-m-^n, hence (excluding the generators of the cone corresponding to x — §')(/'— 2'—!) asymptotes can pass through the point (a, /3, y). In order to find those points (if any) which are the vertices of asymptotic cones, eliminate one of the quantities /, »?, n from (4.) and (6.), and find thosevaluesof a,/3,y thatwill renderallthe coefficients of the resulting equation equal to zero. If no such values be possible, the surface (1.) does not admit of an asymp- totic cone ; but if values a^, /3,, y^ of a,/3,y can be found, then the point (aj /Sj y,) will be the vertex of an asymptotic cone. To find the equation of this cone, we must substitute «i, /3j, y^ for 01, ^,y in (6.), and ascertain Qg the common measure of (4.) and (6.) thus modified ; then wilH,^(A'— «j, y— jSj, ^ — yj)=:0 be the equation to the asymptotic cone, having its vertex at the point (aj /Sj yj). If the equation resulting from the elimi- nation of/, m, or n from (4.) and (6.) can be rendered identically Cones and Cylinders to Algebraical Surfaces. 431 zero by other simultaneous valuesof a,/3,y, there will be as many asymptotic cones as there are sets of values. When the eli- mination referred to above is effected by the process for the common measure, the factor fl,^ will be the last of the remain- Qq corresponding to the factor {S^Y={Al+Bm + Cn}% we shall have A.r+By + C^ = Vi, Ax+Bi/+Cz=y^... Ax+By+Cz=Yt as the equations to the conical asymptotic planes relative to this factor. It appears from the preceding reasoning, that if the equation (4'.), or, which is the same thing, the highest homogeneous function in the equation to the surface (1.) can be resolved into a factors of the first degree, b factors of the second de- gree, c factors of the third degree, &c. (here a factor of the form {fl }* is to be accounted s factors), then the surface may admit of, but cannot have more than a asymptotic cones of the first degree, that is, a conical asymptotic planes, b asymptotic cones of the second degree, c asymptotic cones of the third degree, &c. Some of these cones may have the same vertex ; and since a + 2b + 3c . , . . =p, the degree of the aggregate of all the asymptotic cones to a surface can never exceed that of the surface itself. It will be seen that unless equal factors enter the highest homogeneous function, the asymptotic cones to a surface de- pend only on the two highest homogeneous functions in its equation ; and hence (the above case excepted) all surfaces having the two highest homogeneous functions in their equa- tions identical, will have the same asymptotic cones. Also conversely, it is plain that those surfaces that have the same asymptotic cones must have the two highest homogeneous functions in their equations identical, providing the degree of the equations to the surfaces be exactly equal to that of the aggregate of the cones. Now this aggregate may be consi- dered one of these surfaces ; hence if Wl = 0, Uq=:0, .... Ui = 0 be the equations to cones, the aggregate of which is of the j9th degree, the equation to all the surfaces of the j5th degree having these for asymptotic cones may be denoted by UiU^...Uf-i-Xp-2{^^z) +%p-3(a?2/2) +Xi('^^2;)+xo=0- (15.) Wimbledon, Surrey, Nov. 10, 1847. [ 435 ] LXVII. Oti the Chemical Composition of the Substances em- ployed in Pottery. By Mr. R. A. Couper*. A LL kinds of earthenware are composed of two parts, viz. -^^ the body and the glaze. The body is the principal part of the vessel, being the base or foundation, as indicated by the term itself. The glaze is a thin transparent layer of glass which covers the body and fills up its pores, giving it a smooth surface with a polished and a finished appearance. I. The substances principally employed to form the body of earthenware are, clays of different kinds, flint and Cornish stone. Clay which constitutes the base of the body of earthenware is distinguished from siliceous earth by becoming plastic when mixed with water, and being very soft and not gritty to the feel ; also when burned, it keeps its form, and becomes firm and solid; whereas siliceous earth crumbles into a powder when burned. Clay when intensely heated, as in porcelain manufactories, does not regain its plasticity, which it loses in the burning, although pounded very fine, in which state it is technically termed potsherd. Clay is obtained naturally from Cornwall, Dorset, and Devonshire, and is the finer particles of decomposed felspar deprived of its alkali. 1. The finest clay (termed China clay) used in Britain is obtained artificially from Cornwall, by running a stream of water over decomposed granite, which carries with it the finer particles of felspar, and is then received into catchpools or ponds where it is allowed to subside. The water is then run off, leaving a fine sediment, which is removed and exposed to the atmosphere for four or five months, when it is ready for export. By analysis of this clay previously dried at 212°, I found it to consist of — I. ir. Silica 46-32 46*29 Alumina 39*74 40*09 Protoxide of iron . . '27 '27 Lime '36 '50 Magnesia .... •44< Water and some alkali 12*67 12*67 99*80 99*82 For the second analysis I am indebted to Mr. John Brown. The more common clays, which are found naturally depo- * R ad before the Philosophical Society of Glasgow, April 28, 1847, and communicated by Dr. R. D. Thomson. 2 F2 436 Mr. R. A. Couper on the Chemical Composition of sited, are supposed to have been produced in a similar manner to the china clay ; the rains having washed from the hills the decomposed rock into a lake or estuary, where it has subsided and gradually displaced the water, and become in the course of time perfectly firm and solid, forming fields of clay. The clay is found in layers or strata lying over each other, each layer possessing some distinctive property from the othei*, which renders each clay fitted for a peculiar purpose. 2. Sandy clay (stiff or ball) is the upper layer of clay, and is used by itself for making salt glazed ware ; it is well adapted for this kind of ware, in consequence of the considerable quan- tity of silica or sand which it contains. By analysis of this clay, I found it to be composed of — Silica 66-68 Alumina 26*08 Protoxide of iron .... 1 "26 Lime 'S* Magnesia trace Water 5'1* 100-00 being previously dried at 212°, specific gravity = 2-558. 3. Pipe clay is the second layer, which is used in making tobacco pipes. This clay is not employed in manufacturing earthenware, owing to its possessing the property of contract- ing more than sandy clay. It was analysed by Mr. John Brown, who obtained — Silica 53*66 Alumina 32-00 Protoxide of iron .... 1*35 Lime '40 Magnesia trace Water 12-08 99-49 4. Blue clay is of a grayish colour, and is considered the best layer of clay in the whole series, owing to its burning perfectly white, and approaching in character nearest to the china clay. As analysed by Mr. John Higginbotham, it was found to consist of — Silica 46-38 Alumina 38*04 Protoxide of iron .... 1*04 Lime 1-20 Magnesia trace Water 13-57 100-23 the Substances emjjloyed in Pottery. 437 also previously dried at 212°. There is a variety of other clays obtained from these fields, which are of less value, and need not be enumerated here, as they are similar in appear- ance to those already noticed. 5. Red or brown clay, which is very abundant in the neigh- bourhood of Glasgow, is a surface clay, and contains a large quantity of peroxide of iron, which gives it a deep brown colour. It is of this clay that common black ware, flower- pots, and red bricks are made, which do not require a very high temperature, else they would fuse. The analysis gave — Silica 49-44. Alumina 34-26 Protoxide of iron .... 7*74 Lime 1-48 Magnesia ...... 1*94 Water 5-14 100-00 6. Yellow clay is obtained from various parts of the country, and is so called from possessing a yellow colour both before and after being burned, owing to the presence of iron. By mixing sandy clay and red clay together, we gain an artificial yellow clay, which is often employed. Yellow clay, as analysed by Mr. John Brown, was found to contain — Silica 58-07 Alumina 27-38 Protoxide of iron .... 3-30 Lime -50 Water 10-30 Magnesia ....... trace 99-55 7. Fire-clay is also very abundant in this country, and oc- curs both on the surface and several fathoms under ground. It is termed marl, and is used principally in potteries for ma- king saggars or vessels for placing the ware previous to burn- ing to protect them from the flame; and owing to its coarse particles, which cause the body to be very porous, is well adapted for strong heats: crucibles, or large pots for glass works, in which the glass is fused, are also made from fire- clay, as well as bricks known under the name of fire-brick. This clay was analysed by Mr. John Brown, who obtained — 438 Mr. R. A. Couper on the Chemical Composition of Silica 66-16 Alumina 22*54 Protoxide of iron . . . . 5*31 Lime 1*42 Magnesia trace Water 3'14 98-57 8. Flint as used in potteries is first calcined, then water- ground, in which state it is used for mixing with clays, and is called slop flint; but for glazes it is evaporated to dryness, and used in the dry state with other articles which constitute the glaze. 9. Cornish stone or granite is water-ground, then evapo- rated to dryness for mixing in glazes, and is used in the slop state for mixing with clays. 10. Plaster of Paris or gypsum, which is employed in form- ing the moulds in which certain kinds of pottery are cast, is a native sulphate of lime. It is a very important article to the manufacturer of earthenware, owing to its singular property of parting easily with the clay by the application of a slight heat. Plaster of Paris requires to be dried at a high tempe- rature before using it; but if it is over-dried, it will not again set for making moulds ; the drier the stucco the harder are the moulds that are made of it, and they will stand more readily a greater degree of wear. Plaster of Paris casts, as commonly prepared, cannot again be used for the same purpose. 11. The colours used for printing and painting on ware are similar to one another, excepting that the colours for painting may not be so expensive as for printing ; both however form an important and extensive part of the materials of a pottery. The manufacturers of earthenware are much occupied with the improvement of the variety and beauty of the colours, as well as of the patterns or styles that are produced, and hence a great emulation exists among those employed in the trade. 1. The blue colour in printing is produced from cobalt, which is used with flint, ground glass, pearlash, white lead, barytes, china clay, and oxide of tin in reducing its strength. 2. The brown colour by ochre, manganese, and cobalt. 3. The black colour by chromate of iron, nickel, ironstone, and cobalt. 4. The green colour by chrome, oxide of copper, lead, flint, and ground glass. 5. The pink colour by chrome, oxide of tin, whiting, flint ground glass, and china clay, which are mixed in various pro- portions, fused together at a high temperature, then pounded and mixed with oil, when it is ready for the printer's use. the Substances employed in Pottery. 489 For the following analysis of a blue cobalt calx, I am in- debted to Mr. John Adam : — Silica 17-84. Peroxide of cobalt 19'42 Peroxide of iron 25*50 Water 8'41 Carbonate of lime and magnesia . 28'45 99-62 The oil that is used for mixing with the colours, is made by boiling the following substances together; viz. linseed oil, rape oil, sweet oil, rosin, common tar, and balsam copaiba in various proportions. III. It is but recently since a new method has been applied to cause the colours to flow or spread over the surface of the ware. This object is effected by washing the saggars in which the ware is placed previous to its being fired in the glost kiln, mth a mixture of — 1. Lime, common salt, and clay slip. Dry flows are also used, which answer equally well, the mixture being sprinkled on the bottom of the saggar. The following are some of those flows: — 2. Lime, sal-ammoniac and red lead. S. Lime, common salt, and soda. 4. Whiting, lead, salt and nitre. 5. But there is a wash made of lime, clay slip, nitre, salt, lead, in general use for washing all the saggars employed in the glost kiln, which fuses on the inner surface of the saggar, making it perfectly close and not porous, otherwise the gloss required on the surface of the ware would not be obtained. IV. The colours used in producing the dipt or sponged ware are of a very cheap kind, as it is only for common pur- poses that they are employed. The colours when used for dipt ware are put on the ware before it is burned ; and when used for sponged ware, are put on the ware in the biscuit state. The following are some of those colours : — L A black dip is made from manganese, ironstone and clay slip. 2. A drab dip by nickel and slip. 3. A sage or a greenish-blue dip by green chrome and slip. 4. A blue dip by cobalt and clay slip. 5. A yellow dip by yellow clay alone, or a compound of white and red clay, which produces the same results. 6. A red dip is produced from the red or brown clay ; but it is not every quality of this clay that will answer, as it re- quires to burn red. The first four of these dips are prepared by mixing a little 440 Mr. II. A. Couper on the Chemical Composition of of the colouring agent with a quantity of clay slip ; whilst the two last-mentioned dips are mixed with water to produce the slip state, in which state they are employed. V. There are several kinds of bodies manufactured ; but they may be all classed under two heads, viz. porcelain and earthenware. 1. Porcelain or china is a rich, very smooth and transpa- rent ware, and is the finest quality that has yet been manu- factured. It is a fused body, and owes its transparency to this circumstance ; it also requires a very high temperature to burn it, and is manufactured in this country from flint, Cor- nish stone (granite), china clay, and bone-earth ; the lime employed acting as a flux, partly fusing it. By analysis of two pieces of china from different manufactories in Stafford- shire, I found them to be differently composed. The last of these pieces was also analysed by Mr. Crichton, the three analyses being as follows: — No. 1, by R. A. C. No. 2, byR. A. C. No. 2, by W.C. Silica 39-88 Alumina .... 21*48 Lime 10'06 Protoxide of iron ~\ nc.AA, Phosphate of lime J Magnesia Alkali or difference 2* 14 40-60 39-685 24-15 24-650 14-22 14-176 15-32 15-386 •43 •311 5-28 5-792 100-00 100-00 100000 2. Foreign manufacturers do not employ bone-earth ; but instead of it they use felspar, the alkali of which supplies the place of the phosphate of lime. The Germans make the best porcelain for chemical purposes, as that body is more vitrified and less liable to be acted upon by acids, as well as being capable of standing a very strong heat; and hence it is exten- sively used by chemists. By the analysis of some specimens of foreign porcelain, I obtained the following results: — Berlin. Silica 72-96 Alumina and protoxide of iron 24-78 Lime 1-04 Alkali 1-22 100-00 Specific gravity 2-419 VI. Earthenware is a very porous and less compact body than china or porcelain, owing to its containing little or no alkali, which is the great difference between these bodies. I had a piece of ware manufactured, resembling in appearance porce- lain, as regards the absence of porosity and its compactness, Chinese Porcelain, superior. inferior. 71-04 68-96 22-46 29-24 3-82 1-60 2-68 100-00 99-80 2-314 2-314 tJie Substances employed in Pottery, 44- 1 slightly transparent, and capable of standing a very strong and sudden heat; it was produced by mixing soda to the extent ol' 3^ per cent, in a 1 ittle clay prepared for the common white body, and was then fired in the biscuit kiln. The clay employed having been previously well dried, so as to weigh it without water, the proportional quantity of soda requisite was then calculated and weighed out ; the clay was again mixed with water along with the soda ; it was then formed into capsules, which after being fired and then broken, presented the appearance of a vitrified or fused body. 1. The common white ware or earthenware is made from flint, Cornish stone, china clay, and blue clay, and does not require such a high temperature in burning as the porcelain does. By analysis of a piece of white ware manufactured in this city, it was found to contain — Silica 68-55 Alumina and protoxide of iron . 29'13 Lime 1-24 98-92 Specific gravity 2*36 Coloured ware is also manufactured from the same sub- stances, but mixed with a colouring agent which stains the body. 2. The toqua or blue-coloured ware is coloured by cobalt. 3. The sage or greenish- blue coloured ware, by nickel and cobalt. 4. The drab or buff-coloured ware by chromate of iron. 5. The body for the cane or yellow-coloured ware is pro- duced by a mixture of sandy clay and common red clay, the same as used for red bricks, but is generally produced from the natural yellow clay found in particular localities. 6. The last-mentioned body is also employed for making Rockingham ware, which only varies from the cane ware by possessing a different glaze. 7. The common black ware body is made from the red clay alone. 8. The Egyptian ware body is made from ironstone, ball and red clay. These four last-mentioned bodies are not nearly so expen- sive as the white ware, and do not require nearly such a high temperature to burn them ; therefore they are, comparatively speaking, soft bodies. 9. Salt glazed wai'e is made from sandy clay and a little sand, to keep the body open, or make it less compact; but for large salt glazed ware, potsherd, which is ware that has 4«42 Mr. R. A. Couper on the Chemical Composition of been fired and then ground, is employed to render the body still more open or porous, and also to give it a greater capa- bility of standing sudden heats or colds. This ware is much used in public works for chemical purposes : it is exposed to the action of the flame during burning, whereas other kinds of ware are protected by saggars from the flames. VII. The glaze vitrifies the surface of the body, rendering it generally capable of withstanding acids. It is a very im- portant point with the manufacturer to obtain a glaze which will adhere to the body without crazing or peeling off, as he may discover a good body, but not find a glaze to answer it, since every glaze will not adhere to the same body, and hence every manufacturer has a glaze of his own composition. 1, The substances used in the preparation of the glaze for white ware, are borax, china clay, flint, Cornish stone, Paris white, and white lead. In preparing the glaze, a substance technically termed frett is first made, consisting of borax, china clay, flint, Cornish stone, and Paris white, which are fused together in a kiln, and when ready allowed to flow into water, which shortens it, owing to the water being mechanically lodged in it, and keeps it from adhering to the bottom of the vessel, rendering it much easier to pound. Frett is a beautiful glass, coloured by a little iron, and is pounded and water-ground along with Cornish stone, flint, and white lead : this constitutes the glaze for white ware. Analysis of Analysis of white glaze. frett. Silica 43-66 55-98 Lime ;........ -52 2-52 Alumina and protoxide of iron 9-56 10-38 Borax 20-08 3M2 Carbonate of lime .... 10*88 Carbonate of lead .... 15-19 99-89 100-00 Specific gravity 2*345 A piece of earthenware was brought from America, having been discovered several feet under ground, the glaze of which was tested, and found to be composed of silica, iron, alumina, lime, sulphate of lime and antimony, which was a beautiful rich white glaze concealing a common red clay body. 2. The glaze of Rockingham ware possesses a beautiful brownish metallic lustre, and is made from Cornish stone, flint, manganese, red lead and clay slip, the latter substance being a little clay mixed with water until it becomes of the consist- ency of milk, 3. The glaze for compapo blftck ware is made from the same the Substances employed in Pottery. 443 materials in different proportions, and has a brilliant black appearance. 4. The glaze used for cane or yellow-coloured ware is made from flint, red lead, and Cornish stone. 5. The Egyptian ware owes its value to the beautiful and rich tinted black glaze, made from flint, Cornish stone, red lead, and manganese, with which it is covered. These four last-mentioned glazes are made by stirring the substances together with a certain quantity of water, and pass- ing it through a very fine sieve or search. Glazes do not re- quire such a high temperature to fuse them on the surface of the ware, as the body does to be burned. 6. The glaze for salt glazed ware is common salt, which is thrown in at the top of the kiln through a number of small apertures in the crown of it, and diffuses itself through all parts of the kiln, giving the ware the required glaze. The action that is supposed to take place, when the salt is thrown into the kiln, is owing to its decomposition. The chlorine of the salt combines with the hydrogen of the water, which is mechanically lodged in the salt, forms muriatic acid gas, which passes off, while the sodium combining with the oxygen of the water then unites with the silica in the ware, forming a sili- cate of soda which fuses on its surface. The salt is not thrown in until the kiln has been raised to its greatest necessary tem- perature. Table of the Composition of Clays and Porcelain when free from Water. Cornish china clay Cornish china clay Sandy clay Pipe clay Blue clay Red clay Fireclay Yellow clay English china ware, No. 1 ... No. 2... No. 2.., Berlin ware Superior Chinese ware Inferior Chinese ware Common English white ware 53-16 5312 70-29 61-39 53-52 52-11 69-33 65-06 39-88 40-60 39-68 72-96 71-04 68-96 68-55 45-61 46-00 27-47 36-61 43-89 36-19 23-62 30-68 21-48 2415 24-65 24-78 22-46 29-24 29-13 -31 •31 1-33 1-54 1-20 8-17 5-56 3-70 -41 •57 -90 •46 1-39 1-56 1-49 -56 10-06 14-22 14-18 104 3-82 1-60 1-24 51 51 Trace Trace Trace 2-04 Trace Trace Trace 43 31 Trace Trace Trace Trace 26-44 15-32 15-39 2-14 5-28 5-79 1-22 2-68 2-558 2-419 2-314 2-314 2-360 ";^ [ 444 ] LXVIII. On the Polarization of the Atmosphere. By Sir David Brewster, K,H., D.C.L., F.Ii.S.y and V.F.R.S. Edin.^ WHEN the light of the sun or of any self-himinous body has been transmitted through certain crystallized sub- stances, or has been reflected from, or refracted by, bodies not metallic, it suffers a physical change, to which the name o^ plajie polarization has been given. This physical change consists in decomposing common light into two equal portions of polarized light, one of which is polarized in a plane at right angles to that in which the other is polarized. In doubly refracting crystals, the two pencils are polarized in opposite or rectangular planes ; and when common light is reflected from any body not metallic, whether it is solid, or fluid, or gaseous, a portion of the incident light enters the body ; and of the portions thus reflected and refracted, precisely the same quantity is polarized, — the light polarized by refraction being polarized in a plane at right angles to that which is polarized by reflexion. If the earth had no atmosphere the sky would appear ab- solutely black ; and when the sun sets we should be left in utter darkness. The existence of twilight, however, the blue colour of the sky, and the refraction of the rays which emanate from the stars and planets, place it beyond a doubt that the pure air in which we live and breathe is capable of acting upon light like all other bodies, and consequently of producing that physical change which constitutes polarization. The polarization of the blue sk}', or of the atmosphere, was there- fore observed and studied by different philosophers, both in France and England ; and it was speedily ascertained, in con- formity with the laws of polarization, that the polarization was a minimum in the vicinity of the sun, where his light is reflected at angles approaching to 90°, or where the incident and re- flected rays form an angle approaching to 1 80° ; that it was also a minimum in the region opposite the sun, where his light is reflected at an angle approaching to 0°, or at a perpendi- cular incidence; and that it was a maximum in those interme- diate parts of the sky, which are distant about 90° from the sun, and where his light is reflected at an angle of about 45°, the polarizing angle for air. Such was the first view which was naturally taken of the * This paper is reprinted, with the permission of Dr. Berghaus and Mr. A. K. Johnston, from the Seventh Part of their vakiablePh3sical Atlas now in the course of publication. A map representing the four neutral points, and the system of lines of equal polarization, will be found in that work. On the Polarization of the Atmosphere. 4''t5 polarization of the atmosphere, and a considerable time elapsed before its leading elements were determined, and its more important phaenomena observed and measured. It is to M. Arago, to whom this branch of science owes such deep obli- gations, that we are indebted for the discovery of the first and leading fact on which the law of atmospheric polarization depends. In examining the region of the sky opposite to the sun, he discovered a neutral point, or a point in which there is no polarization whatever. This neutral point he found to be 25° or 30° above the point diametrically opposite to the sun, or what we may call the antisolar point ; and we shall distinguish this pole of no-polarization by the name of M. Arago's neutral point, or the antisolar neutral point. It is best seen after sunset. In the year 1840, M. Babinet discovered a second neutral point, situated about the same distance above the sun as the neutral point of M. Arago is situated above the antisolar point. This point is most distinctly seen immediately after sunset, but is generally much fainter than the other, owing to the discoloration of the blue sky by the yellow light of the set- ting sun. Our readers are no doubt aware, that when light is reflected from the surfaces of transparent bodies, a certain portion of it, and at a particular angle the whole of it, is polarized in the plane of reflexion, or positively'^', while precisely the same quantity of the transmitted light is polarized in a plane at right angles to the plane of reflexion or refraction, or nega- tively. Now, in the part of the sky between the neutral point of M. Arago and that of M. Babinet, the light is polarized positively, while in the parts of the sky between the first of these neutral points and the antisolar point, or between the second and the sun, it is polarized negatively. Hence it became obvious that the two neutral points must be produced by a compensation, in which light polarized negatively neu- tralized light polarized positively, and that the negative light was either produced by reflexion in a plane at right angles to that passing through the sun, the neutral point, and the ob- server, or by refraction in a plane passing through these three points, or by both these causes combined. But in whatever way the negative polarization was produced, it was manifest that the same cause ought to produce a neutral point beneath the sun. After many fruitless attempts to discover this neutral point — owing chiefly to the predominance of the sun's light ♦ These terms are used for the purpose of abbreviation. An account of the laws of the polarization of light by reflexion and refraction, will be found in my papers in the Phil. Trans., 1815, p. 129, and 1830, pp. 69, 133. 446 Sir David Brewster on the Polarization at the part of the sky where it should be found — I at last ob- served, under a very favourable state of the atmosphere, that the polarization of the sky was negative in the space between the risen sun and the horizon. This observation placed it beyond a doubt that there must be a neutral point below the sun, where that «^orflr^/t;e polarization passed mio positive pola- rization; and by concealing the sun from view, and admitting no light to the eye but what came from the probable place of the neutral point, 1 succeeded in discovering it. After commu- nicating this discovery to M. Babinet*, early in 1845, he made several ineffectual attempts to confirm it; and it was not till the 23rd of July IS^G, when the state of (he sky was peculiarly favourable for the observation, that he succeeded in obtaining a distinct view of itf. Before proceeding to explain the map of the lines of equal polarization in the pure blue sky, I shall give a brief account of my observations on the three neutral points to which 1 have referred : — I. On M. Arago's Neutral Point. In the normal state of the lines of equal polarization, namely, when the sun is in the horizon, this neutral point is about 18^° above the horizon or above the antisolar point; but when the sun is about 11° or 12° above the horizon, and the antisolar point of course as much below it, the neutral point is in the horizon, and consequently only 11° or 12° above the antisolar point. As the sun descends to the horizon, and the antisolar point rises, the distance of the neutral point from the latter gradually increases ; and when the sun reaches the horizon, the neutral point is 16^° above it, and therefore 18|° distant from the antisolar point. After the sun has set, the distance of the neutral point from the antisolar point increases ; that is, it rises faster than the sun descends, and its maximum distance when the twilight is very faint, is about 25°. In the latitude of St. Andrews, M. Arago's neutral point is above the horizon all the day between the middle of November and the end of January. In the other months of the year it * Comptes Rendus des Seances de t'Acad. des Scieiices, torn. xxii. p. 801- 803,1845,17th Mars. •f- Comptes Rendus, &c,,i\n\\tt'^, 1846, torn, xxiii. p. 195; andAoiitS, 1846, torn, xxiii. p. 233. " M. Brewster," says M. Babinet, "a sans doute ^te guide dans sa recherche par des vues theoriques ; autrement il me parait pen probable qu'il eut fait, par observation seul de la polarization atmo- spherique, la decouverte remarquable de ce point neutre si difficile a recon- naitre, et que, depuis luij' avals plusieur fois tente inutilement de retrouver." Ibid. p. 235. of the Atmosphere, 447 never rises till the sun is within 11° or 12° of the horizon, and never sets till the sun is 11° or 12° above the horizon. II. On a secondary Neutral Point accompanying M. Arago's Neutral Point. I observed the first traces of this remarkable phsenomenon on the 8th of June 184-1, at 5^ 50', when the positive polari- zation was strongest close to the horizon, whether land or sea, and to about 1^ above it. Hence, when M. Arago's neutral point rose, it did not appear Jirst in the horizon^ but about l^-^ above it, the compensation being effected where the positive polarization was weaker than in the horizon. When this took place, we had the singular phaenomenon of a neutral point xmth positive polarization on each side of it. When this phae- nomenon was more fully developed, under a favourable state of the horizon, the positive polarization was overcome by the advancing negative polarization. The negative polarization was then immediately below the ascending neutral point; but at a certain distance, a few degrees below the neutral point, the negative polarization was compensated by the excess of positive polarization close to the horizon, and the beautiful phaenomenon was seen of two neutral points separated by bands of negative polarization ! This phaenomenon was best seen on the sea horizon, which was marked by an obscure band a ^Q.yi degrees high, that indicated the existence of a distant haze. On the 21st of April 1842, I observed the secondary neutral point under favourable circumstances. At 6^ 22' p.m., when the primary neutral point was 15° high, the secondary one was 2° 50' high. At 7^ positive bands were still seen above the sea line, and were strongest upon the obscure band above the visible sea line. III. On M. Babinet's Neutral Point. This neutral point is situated about 18° 30' above the sun, when he is rising or setting in a very clear sky. It is not so easily seen as that of M. Arago, and was therefore longer in being discovered. It is above the horizon during the greater part of the year in great latitudes, and being above the sun, it is of course always visible when the sun is above the horizon in a clear sky. When the sun is in the zenith, this neutral point coincides with the sun's centre. As the sun's altitude diminishes, it separates from the sun's centre, its distance gra- dually increasing till it becomes 18° 30', when the sun's alti- tude is nothing, or at sunrise and sunset. The neutral point of M. Babinet must^ like that of M. Arago, be accompanied, in certain states of the horizontal 448 Sir David Brewster on the Polarization sky, with a secondary neutral point; but I have never had an opportunity of observing M. Babinet's neutral point when it either rose above or set beneath the horizon, which, though not essential, is the most favourable for observing a secondary neutral point. IV. On the Neutral Point below the Sutz. This neutral point is, as we have previously noticed, much more difficult to be seen than that of M. Babinet. In No- vember, December and January, it cannot be seen in our lati- tudes, unless when, early in November and late in January, a higher degree of polarization in the sky brings it above the horizon at noon. As theory indicated the existence of this neutral point, I long sought for it in vain ; but when I was assured of its ex- istence by the discovery of negative polarization, which often extended from the sun to thehorizon even when the sun's altitude was 30°, I took such precautions for excluding all unnecessary light from the eye that I at last observed it near the horizon, with a small portion of positively polarized light beneath it. I afterwards observed it repeatedly when the sun had higher altitudes, and was able to measure its varying distance from that luminary. On the 18th of February 1842, at noon, when the sun's altitude was about 22°, I observed this neutral point in the most distinct manner, the polarized bands being nega- tive below the sun, and positive near the horizon. Its distance from the sun, therefore, was about 15° or 16°. I afterwards obtained the following measures of its distance from the sun : — Distance of neutral point h , 1842, February 21, 12 39 ... April 3, 11 45 6, 11 6 8, 2 7 from the sun. 15 13 12 16 0 0 0 0 estimated. On the 20th of April, in a very fine day, the wind being west and the barometer 30*02, I obtained the following mea- sures:— April 20, The maximum polarization of the sky at the time of these observations was equal to a rotation of 25^^°, about 4^° below the greatest maximum. 12 10 Di stance from sun, 11 20 12 37 10 40 2 21 12 0 3 45 12 35 of the Atmosphere. 449 On the 26th of April 184'2, when the barometer was at SO'OO, and not a cloud in the sky from morning till night*, I obtained the following measures : — April 26, 11 1 Distance from sun. 0 / 12 15 11 46 12 30 3 30 14 35 3 35 15 5 4 10 17 45 At 10^ 53', the maximum polarization of the sky, or the rotation, was 28f °, and at 1 1'^ 46', and 3*^ 42', it was 28|°. On the 27th of April I observed a remarkable series of phaenomena relative to this neutral point. The sky was sin- gularly fine — the barometer at 30-04, and at 10^ 41' the maxi- mum polarization of the sky 29|^°, the greatest that I have observed. At lO*" 45', the distance of the neutral point from the sun was 12° 3', and consequently about SS^° above the horizon. At 12^ 12', a fog came rapidly from the sea. The neutral point below the sun was driven beneath the horizon, and Babinet's neutral point rose almost to the zenith. At 1^ 20' the fog diminished. The neutral point below the sun reap- peared near the horizon, oscillating up and down, through a space of 5° or 6°, as the fog became alternately denser or rarer ! When the sky is clear, the neutral point below the sun approaches to the sun as his altitude increases, and finally coincides with the sun's centre when he is in the zenith. Hence it follows, that when the sun is in the zenith, the two neutral points in his vicinity meet in the sun, and the system of pola- rization lines becomes uniaxal. Were the sky sufficiently clear, we should doubtless find a secondary neutral point accompanying the primary one below the sun ; but in our climate there is little chance of this phae- nomenon being distinctly observed. In his observations on the antisolar neutral pointy M. Arago observed that it sometimes deviated from the plane passing through the antisolar point and the eye of the observer; and he justly ascribed this deviation to the influence of luminous clouds situated out of this plane. The same phaenomenon takes place in reference to the other neutral points, though the deviation is in these cases less distinctly seen, from the interference of the sun's light. But it is not merely the posi- tion of the neutral point that is influenced by the intrusion of * The lines in the spectrum were ilKdefined, from unequal refraction in the air. Phil. Mas. S. 3. Vol. 31. No. 210. Dec. 1847. 2 G 460 Sir David Brewster on the Polarization light different from that of the sky ; the degree of polarization is always affected whenever we measure it in parts of the sky which have luminous clouds or illuminated terrestrial objects in their vicinity, or any luminosity in the field of view of the polarimeter. If the neutral point happens to be above or below any such object, its distaiice from the antisolar point or from the sun is increased or diminished*. V. On the Maximum Polarization of the Sky. After having ascertained the position of the neutral points, or yoles of no-polarization as we may call them, the next most important element to be determined is the maximum •polariza- tion of the atmosphere. When a ray of common light is reflected from any trans- parent body, at an angle whose tangent is equal to the index of refraction, it is completely polarized ; or when a ray of light, completely polarized in a plane inclined 45° to the plane of reflexion, is reflected from any such body, its plane of polari- zation is brought into the plane of reflexion ; that is, its plane is turned routid 45°. Hence complete polarization is measured by a rotation of 45°. When the polarized ray is reflected at angles above or below the angle of maximum polarization, its plane is less turned round, and its rotation is more or less than 45°, according as the angle of reflexion is more or less distant from the angle of maximum or complete polarization f. Different degrees of rotation below 45° may also be pro- duced by the refraction of the polarized ray at one or more surfaces of glass if, the rotation increasing with the angle of incidence. Hence we may measure the degree of polarization wherever it exists, by observing at what angle of incidence it is compensated or neutralized, by reflexion from a transparent surface, or by refraction at one or more such surfaces. I have found the last method the most convenient, and have therefore constructed a polarimeter which measures the polarization of the sky, by observing with it either the varying angle at which * On the 16th of May 1842, barometer 30*3, the sun was faintly seen through a thick haze. At S*" 49' a.m. the polarization was positive all the way from the sun to the horizon, so that the neutral point below the sun was below the horizon. Immediately afterwards the sun was quite hid — a great glare supervened, and a quaquaversiis polarization was observed, in which the polariscope gave no coloured bands. On the 17th of May, at 6" 30', the sun's disc was quite white through a thick haze, and there was no neutral point either above or opposite the sun, the polarization being everywhere positive. When the haze is thicker on one side of the plane passing through the sun's spectrum, the neutral point deviates from that plane. f See Phil. Trans., 1830, p. 69. - + Ibid. p. 133. of the Atmosphere. 451 it is compensated or neutralized by a fixed number of thin glass plates, or the varying number of refracting surfaces, by which the same effect may be produced at a fixed angle, ca- pable also of being changed*. With apolarimeter thus constructed, I have determined that the maximum polarization of a clear blue sky is equivalent to a rotation in the plane of a polarized ray of 30^ ; and that this maximum takes place at a distance of from 88° to 92° from the sun, and in the plane passing through the sun and the zenith. This maximum is of course dependent on the state of the atmosphere, both with respect to its magnitude and posi- tion; but we shall assume 30° as its amount, and 90° from the sun as its position in a normal state of the atmosphere, and when the sun is in the horizon. VI. On the Form of the Lines of equal Polarization in the Atmosphere. It is obvious, from the phsenomena already described, that the polarization of the atmosphere, produced by the reflexion of the sun's light from the matter which composes the atmo- sphere, in planes passing through the sun, the point of re- flexion, and the eye of the observer, would have been equal in circles of which the sun and the antisolar point are the centre, had there been no disturbing causes, or had the atmosphere been a perfectly transparent medium. In this case the pola- rization would have been complete, or 45° ; and this maximum would have occurred at a distance from the sun, the half of which was the polarizing angle of the medium. There is ob- viously, however, a cause depending on the zenith distance of the polarizing point of the sky, which acts in opposition to the polarization produced by reflexion, and compensates it at the neutral point already described. When the sun, therefore, is in the horizon, these two actions are rectangular, as in biaxal crystals ; and we must therefore determine the form of the lines of equal polarization when the sun is in the horizon, and when the atmosphere is perfectly pure. When viewed, con- sequently, in their general aspect, the phasnomena of atmo- spherical polarization may be represented by the formula R=30°(sinDsinD'),; where R = rotation, or degree of polarization, and D and D' = the distances of the point whose polarization is required from the tvoo neutral points. This formula would make the lines of equal polarization * See the Transactions of the Royal Irish Academy, vol. xix. part S. 2 G2 452 Sir David Brewster on the Polarization Lemniscates, as in biaxal crystals, and consequently the po- larization in the horizon greater than in die zenith, which is contrary to observation. I have therefore added a correction, depending on the zenith distance and azimuth, which makes the formula coincide better with observation, namely, R = 33|-°(sin D sin D')— 6° 34' (sin Z sin A) ; Z being the zenith distance, and A the angle of azimuth. Assuming, therefore, that the distance of the neutral points from the sun and from the antisolar point is 18° 30', when the sun is in the horizon, and that the atmosphere is perfectly pure and uniformly transparent, the lines of equal polarization will have the forms and the degrees of polarization represented by the formula. The direction of the polarization follows the same law as in biaxal crystals, the lines without bands or colour corresponding with the black hyperbolic branches in the pola- rized rings produced by these crystals, being distinctly seen with the polariscope. VII. On the Construction of the Map of the Lines of equal Polarization. Had the map been on a greater or a less scale than it is, it might have been desirable to appropriate a single curve to every single degree, or to every two degrees of rotation or polarization. On the present scale, the curves would have been too numerous and close had there been one to each degree; and with only one to each two degrees, they would have been too distant, in so far as that the form of the curves round the neutral points would not have been sufficiently seen. I therefore adopted such a number of curves, viz. 18|, as enabled me to get the curves. No. 2, continuous round each neutral point. Hence the formula became N = 20-5 (sin D sin D')— 3-9 sin Z sin A, or in the plane passing through the sun and the zenith, in which Z and A become zero, N=25-5 (sin D sin D'). In the zenith itself we have N = 18*45, and at P, P' we have N = 0. The curves thus obtained do not represent values of N in degrees of rotation, but in numbers, each of which is equal to l°-626. Hence R = N 1°'626, and the distance between each curve is 1°*626. The following table contains the rotations or degrees of polarization, indicated by each of the curves num- bered from ^ to 18*45 in the map : — of the Atmosphere. 453 Corresponding degrees of rotation or polarization, or values of R. 6-813 1-626 2-439 3-252 4-065 4-878 6-504 8-130 9-756 11-382 13-008 14-634 16-260 17-886 19-Sil 21-137 22-764 24-396 26-016 27-642 29-268 30-000 Hence the maximum polarization of the atmosphere, as measured by a rotation of 30°, is equal to that produced by reflexion from a plate of glass at an angle of 65^°, and with a refractive index of r4826, or to that produced by a surface of diamond at an angle of 75^°. The number of refractions at a given angle, or the angle, with a given number of plates of glass, at which a rotation of 30° is produced, will be found from the formula in my paper on the Compensations of Po- larized Light*. As the sun rises above the horizon, the lines of equal pola- rization change their form, and the degree of polarization varies at points of the sky whose distance from the sun is in- variable. The neutral points above and below the sun approach •his disc till he reaches the meridian, when the distance of each from the sun is a minimum ; they then separate again, and attain their maximum distance, when he reaches the horizon. In countries where the sun passes across the zenith, these two neutral points coincide with the sun, when he reaches the zenith, and again separate. • Transactions of the Royal Irish Academy, vol. xix. part 2. p. 13. Values of N. 1 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 18-45 454 Mr. Smith on the Hydrates of Nitric Acid. As the sun descends beneath the horizon, the neutral point of M. Arago separates from the antisolar point, and when this point is first seen in the morning before sunrise, its distance from the antisolar point is a maximum ; it gradually ap- proaches that point till the sun rises, and also till the neutral point itself reaches the horizon, when its distance from the antisolar point is a minimum. When the altitude of the sun is 45°, the distance x of the neutral point above the sun is about 13° 5', and the distance a?' of the neutral point below the sun 6° 42'; at other altitudes we have X = A cos A, and j/=AcosA, tan Z, A being 18|°, A the sun's altitude, and Z the zenith distance of P', the neutral point below the sun. An interesting paper, entitled Delle Leggi della Polarizza- zione della Luce Solare ?iella Atmosphera Seretia, communicato con lettera al David Brewster, LL.D., F.R.S., Lond. et Edin., membro delle Principali Academie di Europa, del Prof. A. B. Francesco Zantedeschi, will be found in the Rac- colta Fisico-chimica Italiana, torn. i. fascic. 10. 1846. The details in this paper are chiefly historical. The results ob- tained by M. Zantedeschi himself, which are of a general nature, differ in several respects from mine ; but whether this difference arises from a difference in the methods of observa- tion, or from the different states of the atmosphere under which the observations were made, I am not able to determine. In a Memoir on the Polarization of the Atmosphere, which, I trust, will soon be published in the Transactions of the Royal Irish Academy, I shall give a full account of my obser- vations, and enter more deeply into the subject than would have been proper in the preceding popular explanation of a Map of the Lines of Equal Polarization. LXIX. On the Hydrates of Nitric Acid. By Mr. Arthur Smith, Assistant in the Laboratory of University College, London^. SOME doubt still hanging over the composition of the hy- drates of nitric acid, especially of the first hydrate, I was induced to try some experiments with a view of diminishing this uncertainty. For this purpose a quantity of the red fuming acid was procured, which I examined before com- * Communicated by the Chemical Society; having been readjune 7. 1847. Mr. Smith on the Hydrates of Nitric Acid, 455 mencing my experiments very carefully for chlorine, and found to be perfectly free from that impurity, and to have a specific gravity of 1"500. Fourteen ounces of acid of the above-named strength were mixed with 7 ounces of commercial oil of vitriol, and distilled in a sand-bath over a gas flame ; the first 2 ounces that came over were rejected, and the receiver changed directly the red fumes of nitrous acid were observed to fill the interior of the retort. The acid collected was almost as dark in colour as the acid before distillation. Its specific gravity was 1*522, and it turned out to be perfectly free from the smallest trace of sulphuric acid. I also examined the first two ounces of acid that came over very carefully for chlorine, and found it to contain scarcely a trace, nitrate of silver producing only a slight opalescence, and that which came over afterwards, being the portion that I selected for my experiments, contained none at all. This last acid, when diluted with water, gave off nitric oxide gas with a burst of effervescence, which was the principal reason why it could not be employed to ascertain the exact amount of real acid by saturation in its present dark-coloured condition. The apparatus employed in decolorizing the nitric acid consisted of a capacious retort, capable of holding about a pint, to the beak of which Avas attached a large tubulated receiver, which was kept surrounded with water, to condense any little acid that might come over during the process ; to the tubulure of this receiver was adapted a glass tube, bent at right angles, fitting tightly with a cork, the other extremity being in connexion with a large gas-holder, which was kept constantly filled with water, to be used as an aspirator. To the tubulure of the retort was also fitted a long glass tube bent at right angles, the one end of which terminated within an inch of its bottom, whilst the other was in connexion with a couple of tubes, each 2 feet 11 inches long, arranged side by side, and connected by means of a tube of a smaller diameter bent like the letter U. These long tubes, through which the air was to be aspired, were filled, the one with dried chloride of calcium, and the other with pumice-stone moistened with oil of vitriol, and by these means the absence of all moisture from the air was en- sured. In decolorizing the acid a quantity amounting to 6 or 7 ounces was introduced into the retort, and after having ascer- tained that the whole apparatus M'as perfectly tight, heat was applied to the bottom of a small sand-bath in which the retort was immersed, and the temperature kept up carefully to 1 70° F. Then, by removing the plug at the bottom of the 456 Mr. Smith on the Hydrates of Nitric Acid. gas-holder, and turning the stop-cock at the top, which was in connexion with the apparatus, a constant flow of perfectly dry air was caused to bubble through the nitric acid in the retort, the level of which was kept 2 or 3 inches above the orifice of the tube in the interior, the only passage for the air being through the long desiccating tubes. Aspiration kept up for two or three hours was found to be generally sufficient to decolorize completely 6 or 7 ounces of nitric acid. The acid before decolorization had a specific gravity of 1*522, and after the process fell to 1*503. Fifty grs. of the colourless nitric acid were accurately weighed out in a stoppered specific gravity bottle, to which was cautiously added, whilst in the bottle, with a view to prevent any loss from splashing, a known weight of perfectly pure carbonate of soda, recently ignited in a porcelain crucible, until the solution was perfectly neutral to test-paper. The absence of any sulphate or chlo- ride in the carbonate had been previously ascertained. I. Carbonate of soda required 40*23 grs. II. Carbonate of soda required 40*23 grs. The quantity of carbonate of soda that 50 grs. of acid re- quired for saturation, then, was 40*23 grs., which corresponds to 40*78 grs. of nitric acid, or 81*56 per cent. An acid containing 1^ equiv. of water would contain in 100 parts — Real nitric acid .... 80 Water 20 Too A portion of the prepared acid, amounting to about 5 ounces, was introduced into a small retort, through the tubu- lure of which was fitted tightly, by means of a stopping of moist clay, a delicate thermometer, which was kept immersed in the liquid. The acid began to boil at 190", and before the distillation had come to an end it had risen to 250°. The acid coming over between 190° and 200° was collected apart to be examined by saturation. 50 grs. of the acid which remained in the retort boiling at 250° were then examined, and found to require 31*20 grs. of carbonate of soda in the first experiment, and 31*07 in the second, for saturation ; the mean of the two experiments would correspond to 63*11 per cent, of nitric acid. 50 grs. of the most volatile portion, namely, that which came over between the temperatures of 190° and 200°, were then weighed out exactly ; this quantity was found to require no less than 41*92 grs. in the first experiment, and 41*91 in the second, corresponding to 84*96 per cent, nitric acid ; but then it must be remembered that this acid had a very dark red colour. Mr. Smith on the Hydrates of Nitric Acid, 457 A quantity of this red acid was introduced into the decolo- rizing apparatus, and a constant rapid stream of dry air made to bubble through it for two hours ; at the expiration of that time it was found to be perfectly limpid, and colourless as water, and to have a specific gravity of 1*516 at 60°. 50 grs. of the last acid were weighed out and neutralized with pure carbonate of soda as before. The numbers below will show the amount required for saturation : — Exp. Caib. of soda. Mean. 2* * * 41*69 l^^*^^^ corresponding to 42*27, or «' * * ^1 /.J I 84*54 per cent, nitric acid. 3. . . 41*64 J ^ This acid began to boil at about 184°, the greater part di- stilling over between the temperatures of 184° and 188°; it afterwards rose when near the end to 200°. The first portion that came over was collected apart, intro- duced into the decolorizing apparatus, and dry air again drawn through it until it was quite colourless. This was found to be necessary after each distillation, on account of the decom- position that it suffered upon boiling, which rendered it as dark in colour as the original acid. 50 grs. of the colourless acid, of the specific gravity of 1*517 at 60°, were weighed out, and carbonate of soda very carefully added until neutral to test-paper. The increase in the specific gravity this time only amounted to '001. Exp. Carb. of soda. Acid. Mean. 1. . . 41-79 = 42*361 . 2. . . 41-81 = 42*38/^"^ '^'* Hence in 100 parts — According to theory with 1 eq. water. Real acid . . 84*74 Real acid . . 85*71 Water . . . 15-26 Water . . . 14*28 100*00 99*99 This would give, when compared with the theoretical compo- sition of nitric acid with 1 equiv. of water, a deficiency of "97 in the acid, and an excess of '98 in the water. This hydrate, when pure, was a perfectly limpid and colour- less liquid, like so much water; it boiled at 184°, and had a specific gravity of 1*517 at 60°. It was found not to have the slightest action on tin or iron even when boiled. A por- tion of this acid placed in a freezing mixture composed of ice and salt suffered no change. These experiments leave little doubt concerning the com- position of the first hydrate of nitric acid, namely, that it is the true mono-hydrate, consisting of 1 equiv. of nitric acid and 1 of water, HO, NO5. Deuto-Hydrate. — In preparing this hydrate, I set out by obtaining a quantity of colourless strong nitric acid, the exact 458 Mr. Smith on the Hydrates of Nitric Acid, amount of real acid in which was ascertained by saturation to be 79*79 per cent. To reduce this acid to the proper strength, so as to contain exactly 2 equivs. of water, it was found by calculation that it would require 63*86 grs. of w'ater to every 1000 grs. of acid. The proper proportions of acid and water were weighed out carefully in a stoppered specific gravity bottle, and the two mixed. This mixture was cooled down to 60° and found to have the sp. gr. 1*486. 50 grs. of this hydrate were weighed out and saturated in the usual way with recently-ignited carbonate of soda. The quantities of carbonate of soda required were as follows : — Exp. Carb. of soda. Mean. 2* ' ' 37*53 y^^*^^' °^ ^^'^^ P^^ *^^°^* ^^^^• An acid containing 2 equivs. of water will contain 75 per cent, real acid. A portion of this acid was introduced into a small retort and distilled. It began to boil, as nearly as could be judged, at about 200°, it being difficult to come at the exact tempera- ture on account of the very rapid rise of the thermometer, which continued to take place until it had gained the tempe- rature of 218°; it afterwards rose when near the end to 250°. It appears, then, from these experiments, that no such thing as a deuto-hydrate exists, but that when a mixture is made in the proportions to form such a hydrate and subjected to di- stillation, it divides spontaneously into the first and another, at the same time suffering considerable decomposition ; and the acid which is found remaining in the retort has the exact boiling-point of the tetra-hydrate, namely, 250° ; and more- over, the first portion that came over had the exact density , of the first. A portion of this acid placed in a freezing mixture of ice and salt, suffered not the least solidification. Tetra-Hydrate. — This hydrate was prepared in the same way as the first, namely, by preparing a quantity of colourless acid, ascertaining its saturating power, and mixing it with the proper quantity of distilled water, ascertained by calculation. It was then tried afterwards by saturation to see if it was correct ; the numbers below will show the difference : — Exp. Cavb. ofsoda. Acid. Mean. \'. \ '. 29*87 = 30*27 }^^'^2' ^"^ ^^'^"^ P^"" ''^''^- ""^^^ ^'''^- According to theory with 4 eqs. water. Real acid . . 60*64 Real acid ... 60 Water , , . 39*36 Water .... 40 100*00 100 On the Decomposition ofCuminate of Ammonia hy Heat. 459 The acid had a density of 1*424 at 60°; it began to boil at 250°, and distilled over perfectly colourless and unchanged ; towards the end, when slight decomposition commenced, the temperature rose to 260°. Five or six ounces of very weak acid, of the density of 1*180, were introduced into a retort and kept heated just below its boiling-point for two or three hours ; the heat was increased from time to time so as to make it boil briskly, and a ther- mometer introduced through the tubulure ; when that which remained in the retort boiled uniformly at 250°, the heat was withdrawn and it was allowed to cool. When the specific gravity of this acid was taken, it was found to be close upon that of the tetra-hydrate, but not exactly ; probably if I had operated upon a large quantity, and carried it on for a longer time, it would have been more so; as found, its density was 1*412 instead of 1*424, which would make a difference of rather less than 1^ per cent, de- ficiency in the acid. This is, I have no doubt, the proper hydrate of nitric acid, HO, NO5 + 3HO, as it is generally considered; and as Dr. Dalton correctly observed, acids which are either stronger or weaker than this acid, are brought to this strength by conti- nued ebullition, the former losing acid and the latter water. LXX. On the Products of the Decomposition of Cuminate of Ammonia by Heat. By Mr. Frederick Field*. THE peculiar mode of decomposition which the ammonia salts of inorganic acids exhibit when exposed to the ac- tion of heat, occurs likewise in the ammonia compounds of organic acids, although the results in the latter instances are usually of a more complicated nature. In most of these cases a formation of water takes place, the hydrogen of which is derived from the volatile alkali, while the acid furnishes the oxygen, the residue of which combines in a more intimate manner with the nitrogen of the ammonia. In decompositions, however, of inorganic compounds this reduction seems to be carried at once as far as it can go, the Avhole of the hydrogen contained in the ammonia being converted into water ; while in organic salts this hydrogen is eliminated only by degrees, an intermediate body being produced between the original ammonia salt and the final product of the decomposition. Thus we find that nitrite and nitrate of ammonia, when ex- posed to heat, are at once converted into water, and respect- ively into nitrogen and nitrous oxide. Oxalate of ammonia, * Coramunicated by the Chemical Society; having been read June 7. 1847. 460 My. Field on the Products of the on the other hand, if submitted to a gentle heat, loses only two equivalents of water, the residue of both base and acid combining to form oxamide, and only by a strong and brisk application of heat Doebereiner converted it into cyanogen, the rest of the hydrogen being eliminated in the form of water. The dry distillation of oxalate of ammonia thus affords the prototypes of two series of compounds, which may arise from ammoniacal salts by the elimination of two or four equivalents of water respectively. There are few cases, however, in which the decomposition of ammoniacal salts have been carefully studied, and the instances in which we are acquainted with the representative of the two types are exceedingly scarce. We are indeed intimate with a very great number of amidogen compounds analogous to oxamide (fumaramide, salicylamide, succinamide, anisylamide, &c.), but only few of these have been obtained from ammoniacal salts by the action of heat. The greatest number of these bodies were produced by the change most compound aethers suffer under the influence of ammonia, a beautiful mode of decomposition pointed out first by Professor Liebig in the transformation of oxalate of ethyl into oxamide, or by the action of gaseous ammonia on other substances related in some manner with the acid : thus was chloride of benzoyle converted into benzamide by Wohler and Liebig, and lately lactide into lactimide by Pelouze. As yet, however, the members of the second class, those compounds standing to other acids in the same relation as cyanogen to oxalic acid, are very rare. From a beautiful ex- periment of Pelouze, we know that the vapour of formiate of ammonia, when passed through a red-hot tube, is converted into water and hydrocyanic acid. In their investigation on the radical of benzoic acid, Wohler and Liebig obtained a peculiar oil by the action of heat on benzamide, which at that time they did not study more closely. The same body was at a later period obtained in the dry distillation of benzoate of ammonia, and fully examined by Fehling, who found that this interesting substance, to which he gave the name henzo- nitrile, has the composition C14 H5 N, and is produced from benzoate of oxide of ammonium, exactly in the same manner as cyanogen and prussic acid are formed respectively from oxalate or formiate of ammonia. These facts did not long remain isolated. Schlieper, in an excellent examination he has lately published on the products of oxidation of gelatine by chromic acid, discovered that in these reactions, among other products, the body C,o Hg N is formed, valeronitryle or valerianate of ammonia — 4 equivs. of water. The members of this class acquire every day a greater degree of importance. A remarkable paper, read before the Decomposition of Cuminate of Ammonia by Heat. 461 Chemical Society a short time since by Dr. Kolbe and Mr. Frankland, has indeed opened a most interesting connexion between these bodies and another class of substances, which hitherto have been obtained by very different processes. The conversion of cyanide of ethyl into metacetonic acid by means of alkalies and acids, seems to indicate that cyanide of ethyl is nothing else than metacetonitryle. This experiment is likely to be of great importance, for it is exceedingly proba- ble that the whole class of substances alluded to must be con- sidered as a class of cyanogen compounds. It is evident that similar considerations may be applied to cyanide of methyl and cyanide of amyl, lately described by Balard ; and the con- version of these cyanides respectively into acetic and caproic acids, which w^e have a right to anticipate on treating them W'ith alkalies or acids, will prove that these compounds are the nitriles of acetic and caproic acids — acetonitryle and capronitryle — which as yet have not been obtained by the action of heat on the ammoniacal salts of these acids. The following experiments on the action of heat on cumi- nate of ammonia have been made with the hope of contri- buting to the history of the nitryles, or organic cyanides, as they perhaps should be more correctly designated. The cuminic acid employed in my experiments was prepared by the action of solid hydrate of potash on oil of cumin, and the product perfectly freed from the least traces of cymol which it might possibly contain by precipitating the potash salt by hydrochloric acid, dissolving the precipitated cuminic acid in ammonia, reprecipitating by hydrochloric acid, and crystallizing from water. The acid was then dissolved in strong ammonia, and the solution subjected to heat. The first portions which passed over, although consisting chiefly of water and ammonia, together with cuminate of ammonia, which is always carried over with the steam, presented more or less an opalescent appearance, indicative of traces of the oil. On evaporating the solution in the retort to dryness, a portion of the salt is decomposed, ammonia is evolved, and cuminic acid condenses in beautiful plates upon the sides and neck of the retort, separation going on even on raising the temperature ; but simultaneously another decomposition takes place, water is eliminated, in consequence of Avhich there are produced a peculiar white crystalline body, difficultly soluble in water, and subsequently a colourless oil of a most fragrant odour ; although the operation may seem very simple, expe- rience alone teaches the proper regulation of temperature ne- cessary to obtain these two bodies. Cuminamide. — Observing in ray first experiments evolution of ammonia and sublimation of cuminic acid on heating cu- 462 Mr. Field on the Products of the minate of ammonia, I thought that by heating it under pres- sure, the ammonia then not being able to escape, the desired change might be effected. Accordingly a portion of the salt was placed in a strong glass tube, and after sealing the other end, gradually heated in an oil-bath to nearly the boiling- point of the oil, and allowed to cool. On cooling the mass appeared to have been completely fused, but perfectly solid and of a highly-crystallized texture. On examination it was found to be insoluble in cold water and ammonia, but very soluble in hot water, from which it solidified into a crystalline mass as the temperature cooled ; this alone sufficiently indi- cated that a complete change had been effected, the cuminate of ammonia being readily soluble in cold water. In order to ascertain the nature of the change it was dissolved in hot water, and weak ammonia added to dissolve any cuminic acid that might be mixed with it, and crystallized; the crystals were separated by filtration, and once more dissolved in a hot weak solution of ammonia, from which they separated on cooling in brilliant white crystalline plates, similar in appear- ance to benzamide. These were dried at 212° in a water-bath, and analysed in the usual manner. I. 0-174 grm. of substance burnt with oxide of copper yielded 0*470 of carbonic acid and 0*128 of water. II. 0*248 grm. yielded 0*670 of carbonic acid and 0*181 of water. III. To estimate the nitrogen, 0*287 grm. ignited with soda- lime yielded 0*390 of ammonio-chloride of platinum*. From these analytic results the following per-centages are obtained : — I. 11. III. Carbon . . 73*66 73*67 Hydrogen'. 8*17 8*10 Nitrogen . 8*50 leading to the formula Cc^ Hjy NOg, as may be seen from the following comparison of the theoretical and experimental numbers : — 20 equivs. of Carbon , 13 ... Hydrogen 1 ... Nitrogen 2 ... Oxygen . This body therefore is cuminamide, NH2 Cgo Hn Og, having * In this operation a large quantity of an oily body is produced, which floats on the surface of the hydrochloric acid. It is evidently cumol. Theory. Mean of exp. 120 73*68 73*66 13 7*99 8*13 14 8*52 8*50 16 9*81 9*71 163 100*00 100*00 Decomposition of Cuminaie of Ammonia by Heat. 463 precisely the same relation to cuminate of ammonia as oxa- mide to oxalate of ammonia. In preparing large quantities of this substance the employ- ment of close tubes would be very inconvenient, and I soon found that it could be obtained in a retort by the continued application of a heat sufficient to keep the salt in a state of semi-fluidity. The analyses II. and III. vi^ere made with the product obtained in this manner. Cuminamide crystallizes like benzamide, in two forms, ac- cording to the state of the solution ; if crystalUzed imme- diately, or from a strong solution, it separates in the form of crystalline tables of great brilliancy, but if the solution be di- lute, it crystallizes after the lapse of some hours in long opake needles, both forms having exactly the same compo- sition. It is soluble in hot and cold alcohol in any propor- tion, as also in aether. This new amide differs from most others that have been described in remaining intact on the addition of strong solution of potash, or mineral acids ; from the former it crystallizes in large plates after some days. Long boiling with alkalies or acids is scarcely sufficient to produce the characteristic conversion of amides either into ammoniacal salts or combinations of the base with the acid and evolution of ammonia. Cumonitrile. — On heating cuminate of ammonia until it is perfectly fused, and keeping the fused mass in a state of brisk ebullition, large globules of a light yellowish oil pass over with water, evidently derived from the decomposition of the salt ; when the globules began to diminish the process was stopped, the oil was separated from the water in the receiver by means of a pipette, the remaining distillate added to the mass in the retort, and the process again repeated as before ; in this manner, after some half-dozen distillations, nearly an ounce of oil was obtained ; it was well- washed with ammonia to remove cuminic acid, which seemed to be soluble in the oil, then treated with hydrochloric acid to remove ammonia, thoroughly washed with water, and digested with chloride of calcium; after standing some days to separate chloride of calcitim, it was distilled and carefully rectified, the first por- tions being rejected, as possibly containing traces of water ; the middle portion was reserved and placed in a retort with a coil of platinum ; the liquid entered into ebullition at 239° C, at which point it remained stationary while at least a quarter of an ounce was passing over. This portion was employed in the following analyses : — I. 0*212 grm. burnt with oxide of copper yielded 0*644 of carbonic acid and 0*145 of water. 464 Mr. Field on the Products of the II. 0-225 grm. yielded 0*6835 of carbonic acid and 0-161 of water. III. 0-244 grm. ignited with soda-lime yielded 0-364 of ammonio-chloride of platinum*. From these analytical results the following per-centages are obtained : — I. ir. III. Carbon . . 82-82 82-84 Hydrogen . 7*59 7-96 Nitrogen . 9*34 leading to the formula Cgo Hji N, as may be seen from the following comparison of the theoretical and experimental numbers : — Tlieory. Mean of exp. 20 Carbon . . 120 82-76 82-83 11 Hydrogen . 11 7-58 7-77 * 1 Nitrogen . 14^ 9-66 9-34 145 This body is therefore cumonitrile, Cgo H^l N, standing in the same relation to cuminate of ammonia as cyanogen does to oxalate of ammonia. Cumonitrile is a perfectly clear and colourless liquid, pos- sessing a high refractive power; it has a most powerful and agreeable odour and a burning taste ; it is somewhat soluble in water, causing turbidity in that liquid ; it is soluble in all proportions of alcohol and aether ; it is lighter than water, having a specific gravity 0*765 at 14° C. (57°Fahr.). The boiling-point, when in contact with metal, is constant at 239° C. (462-2° Fahr.), at the barometric pressure 0-7585 m. = (29-85 inches). The equivalent ofcuminic acid containing 3C2 Hg more than the equivalent of benzoic acid, it was in- teresting to compare the boiling-points of benzonitrile and cumonitrile. According to Fehling's experiments, the boil- ing-point of benzonitrile is 191° C; on calculating from this observation the boiling-point of cumonitrile according to the rules first pointed out by Kopp, the boiling-point should be 191 -f- 3-1 9 = 248. Dr. Fehling does not hoNvever mention that he had this substance in contact with metal, and it is not improbable that the true boiling-point of benzonitrile is somewhat lower ; the vapour of cumonitrile is very inflammable and burns with a bright flame, which deposits much carbon. * Professor Fehling found it difficult to estimate the nitrogen in hetj- zonitrile in the form of ammonia, drops of oil passing over into the hydro- chloric acid. In the case of cumonitrile, this method gave very accurate results ; oil drops also passed over, but they were evidently cumol. Decomposition of Cuminaie of Ammonia by Heat. 465 The strongest nitric acid has but little action upon this substance ; after boiling, however, and setting aside for some days, crystals of cuminic acid are formed. On being heated with potassium it darkened, and apparently another oil was produced ; the mass on being washed and tested for cyano- gen in the usual manner gave a copious precipitate of prus- sian blue, which seems to be strongly in favour of the view which Kolbe and Frankland have recently promulgated. A strong alcoholic solution of potash has no immediate action on cumonitrile, but after a day or two, on pouring the li- quid into a watch-glass, it partially solidified into a yellow crystalline mass, a mixture of the original substance with white crystals. These crystals after purification had all the appearance of cuminamide, and in order to be satisfied of their composition — I, 0*174 grm. burnt with oxide of copper yielded 0*472 of carbonic acid and 0*124 of water; the calculated per-centage of carbon and hydrogen from these numbers being — Carbon . . 73*62 Hydrogen . 7*91 These numbers correspond to those of cuminamide, as may be seen by a comparison with the former analyses. It appears then that cumonitrile, on the addition of potash, is not, as might have been expected, converted into cuminate of ammonia, but into cuminamide, taking 2 instead of 4 atoms of water— -C20 H,i N + 2HO = Cgo HigNO^, the latter body being, as before remarked, in such a remarkable degree un- affected by alkalies or acids. Having obtained one amide with comparative ease, many other ammoniacal salts were heated for the purpose of obtain- ing analogous amidogen compounds. Benzoate of ammonia was tried unsuccessfully, and it appears from the account published by Fehling of his investigation of benzonitrile, that the residue in the retort consisted entirely of benzoate of am- monia, that salt appearing to have lost directly 4 equivs. of water without undergoing an intermediate conversion into an amide by the loss of 2 equivs. Nitrobenzoic acid was dis- solved in ammonia, evaporated, and cautiously fused for a considerable time ; when cold it was found to be insoluble in water and ammonia at the ordinary temperature, but dissolved by hot water, from which it crystallized in beautiful yellow needles. On analysis, the following results were obtained : — I. 0*222 grm. of substance burnt with oxide of copper yielded 0*410 of carbonic acid and 0*080 of water. II. 0*255 grm. yielded 0*472 of carbonic acid and 0*087 of water. P/iil. Mag. S. 3. Vol. 31 . No. 210. Dec. 1847. 2 H 466 On the Decomposition of Cuminate of Amnwnia by Heat. From these results the following per-centages were ob- tained : — I. II. Carbon . . . 50*36 50-43 Hydrogen . . 4*00 3-78 corresponding to the formula 0^4 Hg Ng Og, as may be seen from the comparison of the theoretical and experimental numbers : — 14 equivs. of Carbon . . 84 Theory. 50-60 Mean of exp, 50-39 6 ... Hydrogen . 2 ... Nitrogen . 6 28 . 3-62 16-87 3-98 6 ... Oxygen . . 48 28-91 166 100-00 This body is therefore nitrobenzamidej having the same rela- tion to nitrobenzoate of ammonia as cuminamide has to cumi- nate of ammonia. This beautiful substance can only be obtained with diffi- culty, as the nitrobenzoate of ammonia explodes violently unless very great caution is employed. A specimen of chlorobenzoic acid, made In the laboratory for some other investigation, was dissolved in ammonia and heated ; it fused readily, became perfectly insoluble in cold water and ammonia, but soluble in hot water, crystallizing as the solution cooled in long needles of great beauty. The specimen of acid afforded me, being all that could be spared, was insufficient for the manufacture of an amide ; I prepared a portion of chlorobenzoic acid by acting upon benzoic acid for some days with hydrochloric acid and chlorate of potash ; after purification it was burnt with chromate of lead and gave the following results : — I. 0-394 grm. = 0-769 of carbonic acid and 0-114 of water. From this result the following per-centage was obtained : — periment. Theory. 53-22 53-61 3-22 3-25 Carbon . Hydrogen leading to the formula HO, C,4 4 ^j* V Og, 1 equiv. of the hydrogen of benzoic acid replaced by an equivalent of chlo- rine. This acid, however, on being subjected to the usual treat- ment by solution in ammonia and subsequent heat, did not fuse but blackened, charcoal being separated. Unfortunately the specimen of ammoniacal salt from which I had made the former compound was not analysed, probably it would have On the equation x^ + j^ + As^zs'Man/z, Src, 467 proved to be C,4 {q T O3J HO, or C14 ^Qf^ O3, HO, a dichlorobenzoic or a trichlorobenzoic acid, such existing. These experiments were conducted in the laboratories of the Royal College of Chemistry under the direction of Dr. Hofmann, to whom I beg to offer my best thanks for his ad- vice and assistance during their progress. LXXI. On the General Solution {in certaiti cases) of the equation a:^ + i^-{-Az^=Mxyz, i^-c. By J, J. Sylvester, A.M., F.R.S., late Professor of Natural Philosophy in Uni- versity College, London*. T SHALL restrict the enunciation of the proposition I am -*- about to advance to much narrower limits than I believe are necessary to the truth, with a view to avoid making any statement which I may hereafter have occasion to modify. Let us then suppose in the equation a^ -\-y^ -f- Az^ = Msyz that A is a. prime number, and that 27 A — M^ is positive, but exempt from positive prime factors of the form 6/+ 1. Then I say, and have succeeded in demonstrating, that all the pos- sible solutions in integer numbers of" the given equation may be obtained by explicit processes from one particular solution or system of values of x, y, z, which may be called the Primi- tive system. This system of roots or of values of x, y, z is that system in which the value of the greatest of the three terms x, y, A^.z (which may be called the Dominant) is the least possible of all such dominants. I believe that in general the system of the least Dominant is identical with the system of the least Content, meaning by the latter term the product of the three terms out of which the Dominatit is elected. I proceed to show the law of derivation. To express this simply, I must premise that I shall have to employ such an expression as S'=f (S) to indicate, not that a certain quantify, S', is a function of S, but that a certain system of quantities disconnected from one another, denoted by S', are severally functions of a certain other system of quantities denoted by S; and, as usual, I shall denote "2 . ■], J=3ffm{gl—em) + S\m{U—en) — M{gd^ - eHm) ljJ=3Am{i7n —gl) -r Sel{ein —gl) — M{eim^—gHm) v' = 3el{en — d) + 3g7n(gn — nn) — M {egn^— iHm) ; we have then and in like manner '\I/ S being derived from '^ S by the mere interchange of e and g one with the other. I have stated that every possible solution of the proposed equation comes under one or the other of the orders, infinite 470 On the equation j:^+^' + A«^= M^n/^, S^c, in number and infinite to the power of infinity in variety of de- gree, above given: this is not strictly true, unless we understand that all systems of solution are considered to beequivalent which differ only in a multiplier common to all three terms of each; that is to say, which may be rendered identical by the expul- sion of a common factor. So that 7nu, m^, my as a system is treated as identical with a, /3, 7, which of course substantially it is ; and it should be remarked that there is nothing to pre- vent the operations denoted by

    1'50 phosphate of ammonia J 100-00 Pelletier* and Caventou, in a very long memoir read before the Institut de France in 181S, have gone very elaborately into the examination of cochineal and obtained many interest- ing results. In analysing this substance they employed the following process : — They removed the fatty bodies by boiling aether, in which they found the colouring matter but slightly soluble ; these fatty substances, recovered by distilling off the aether, were considered to consist of stearine, oleine, and an aromatic acid, from which latter substance it was difficult to remove the adhering colouring matter. The cochineal, exhausted M'ith aether, M'as treated with al- cohol of 40° Beaume, which dissolved the colouring matter, together with a small quantity of fatty and nitrogenous sub- stances. On cooling, and by spontaneous evaporation, they obtained a granular red residue of a semi-crystalline appearance, and which they considered to be the colouring matter contami- nated still with nitrogenous matter {maiiere animalisee) and some fatty bodies, the greater part of which remained undis- solved in strong cold alcohol; by repeating the operation once or twice they considered that the substance was ob- tained almost in a state of purity. To remove the last traces * /nnales de Chiniie ef. de Physique, ser. 2, tome viii. p. 250. Journal de Pharmacie, ser. 2, tome iv. p. 193. Mr. De la Rue on Cochineal. 473 of foreign matter it was dissolved in strong alcohol, and an equal volume of aether added, which precipitated the colouring matter and retained the fat, which was still ad- hering to it. The colouring matter thus purified they named carmine {carminium), and described as being very soluble in water, from which it did not crystallize, more or less soluble in alcohol, according to its strength, and quite insoluble in aether and the fixed and volatile oils. Acids did not precipi- tate it from its aqueous solution if free from animal matter. They found hydrochloric and sulphuric acid to decompose it; the latter with elimination of carbon. By the action of nitric acid they obtained an acid in prismatic crystals resem- bling oxalic acid, but differing in some of its properties. On heating the " carmine" it intumesced and gave off carbu- retted hydrogen, a considerable quantity of oily substances, a little acid water, but no trace of ammonia. Chlorine and iodine decomposed it; the alkalies in the commencement produced merely a change in colour, turning it violet, but by the assistance of time or heat they effected a complete altera- tion. They found an aqueous solution of " carmine " to exhibit the following comportment with reagents. Of the alkaline earths, lime only produced a precipitate ; hydrate of alumina showed a marked affinity, absorbing the whole of the colouring matter from an aqueous as well as an alcoholic solution ; the presence of alum prevented this reac- tion : iron, copper, and silver salts were without reactions ; terchloride of gold destroyed the colour ; neutral salts of lead merely changed it to violet, except the neutral acetate, which precipitated it, the free acetic acid retaining a little of the compound in solution; the colouring matter could be re- covered by decomposing the lead compound with hydrosul- phuric acid. The nitrate of mercury gave a purple, and the pernitrate a scarlet-red precipitate; the bichloride no pre- cipitate ; chloride of tin gave a violet precipitate ; the bichlo- ride changed the colour to scarlet without causing a precipi- tate. Albumen and gelatine had no marked action, but if precipitated by reagents the colouring matter was carried down. In a later communication (1832), Pelletier* gave the com- position of the colouring matter as prepared by himself and Caventou. In a previous qualitative examination they had failed to exhibit the presence of nitrogen which M. Pelletier now detected. The substance was dried in vacuo at a gentle heat to remove every trace of alcohol and aether, and burnt with oxide of copper it yielded — * Annales de Chimie et de Physique, sir. 2, tome li. p. 194. 474 Mr. De la Rue on Cochineal. Carbon 49'33 Hydrogen 6'66 Nitrogen 3*56 Oxygen 40*45 100-00 M. Pelletier stated, however, that he did not greatly rely on the correctness of this analysis. After alcohol had dissolved out all the colouring matter removable by it, they extracted the last traces, by repeatedly M'ashing the residue with boiling water, and along with it a little fatty and some nitrogenous matter ; the residue was a brownish transparent mass. The later decoctions, contain- ing no red colouring matter, left likewise on evaporation a brownish transparent mass, which they considered identical with the organic residue of the insect. This animal matter had, according to them, some analogy with gelatine, but dif- fered in many of its properties, as it did also from albumen and fibrine, they therefore considered it as peculiar to the cochineal insect; the alkalies and ammonia dissolved it readily ; chlorine precipitated it ; all acids and acid salts pre- cipitated it, as also acetate of lead, salts of tin and copper, and nitrate of silver ; and they considered the latter reagent as a good test of the purity of the colouring matter, as it did not precipitate the latter if free from nitrogenous substances. If the colouring matter were contaminated with nitrogenous sub- stances, all the salts which precipitated the latter carried down likcAvise some of the colouring matter. An examination of the ashes showed the presence of phos- phate of lime, carbonate of lime, chloride of potassium, and phosphate of potash, to the extent of 0'7 per cent. In the second part of the memoir they went into the theory of the technical applications of the colouring matter : this having no reference to the present subject, I do not think it necessary to reproduce it here. M. Lassaigne, in 1819*, examined Kermes {Coccus ilicis), an insect common in the South of Europe, and employed as a red dye before the discovery of America, and obtained by following the methods of Pelletier and Caventou, substances agreeing in their properties with the analogous ones found in cochineal. M. F. Preissert, in an elaborate paper on the origin and nature of colouring matters, has again drawn the attention of chemists to the subject. This gentleman, from a study of a variety of colouring substances, comes to the conclusion that all resemble indigo in its behaviour with reducing agents. * Journal de Pharmacie, ser, 2, tome v. p. 435. f Ibid, p. 191. Mr. De la Rue on Cochineal. 475 He affirms that he obtained by the action of hydrosulphuric acid on the lead compounds of a great number of organic colouring matters, substances bearing the same relation to the original colouring matters as white indigo does to blue indigo. In order to obtain the colourless modification of the colouring matter of cochineal, he adds what he terms "hydrate of oxide of lead " to an aqueous decoction of cochineal, the fats being previously removed by aether. The colouring mat- ter is entirely removed by the so-called oxide of lead, which is nothing but a basic nitrate of lead, 2(3PbO, NO5) +3HO. The lead compound suspended in water (hot?) was decom- posed by a stream of hydrosulphuric acid ; the nearly colour- less filtrate deposited on cooling needles of a pale yellow colour, which became perfectly white by washing with aether and pressing between bibulous paper ; these crystals, which, according to his statement, are soluble in water and alcohol, but less so in aether, assume in contact with the atmosphere the purple-red of the colouring matter of cochineal. He more- over asserts that his colourless modification gives a white lead salt on adding acetate of lead to its aqueous solution, and that this assumes a purple colour in contact with the air. He proposes to give the name carmine, hitherto applied to the red colouring matter, to the white crystals, and to desig- nate the red substance by the name " Carmeine." The statements of Preisser, generalizing most beautifully under one head the chemical character of all colouring mat- ters, making indigo as it were the prototype of them all, could but induce other chemists to M^ork out more in detail the relations cursorily pointed out in the memoir of this che- mist. Unfortunately a careful repetition of these experiments has not confirmed the basis on which his theory reposes. M. A. E. Arppe repeated Preisser's experiments on the colouring matter of cochineal*. He found that by proceed- ing in the manner described by Preisser that he could only obtain a red solution, which on evaporation was converted into white crystals of oxalic acid by the nitric acid derived from the basic lead salt, Arppe now prepared a pure oxide of lead by precipita- ting acetate of lead with potash. He found that this would not take down the colouring matter in the cold, but by boil- ing it is carried down as a blue lake, which he decomposed by hydrosulphuric acid ; the supernatant liquor was nearly colourless, the colouring matter he found adhered with great obstinacy to the sulphuret of lead, from which water, alcohol and ammonia failed to separate it ; but sulphuret of ammo- * Liebig's Annalen, vol. J.v. p. 101. 476 Mr. De la Rue on Cochineal. nium and acids rendered it perceptible. He likewise tried to obtain the colouring matter in a state of purity by pre- cipitating with hydrated oxide of lead an aqueous decoction of cochineal (previously purified from nitrogenous substances by nitrate of silver). On treating the precipitate by hydrosul- phuric acid, he obtained a red liquor of strongly acid reaction, the acid of which Avas not derived from the lead salt : on eva- poration it left a dark red mass, emitting the smell of burnt sugar. Wishing to separate the acid, which he thought contaminated the colouring matter, he prepared a strong aqueous decoction of cochineal, and after separating the ni- trogenous matter by means of nitrate of silver, filtering, and then saturating by ammonia, and afterwards adding the hydrated oxide of lead, he found that the supernatant am- moniacal liquor, which was nearly colourless, yielded by evaporation an acid liquid ; and on decomposing the lead lake with hydrosulphuric acid, he obtained a liquid slightly coloured (the colouring matter adhering to the sulphuret of lead), which was likewise acid. From this he concluded that the colouring matter had not up to that period been obtained in a state of purity. Microscopic Examination of Living Cochineal. By the kindness of Sir James Clark, who furnished me with specimens of the living insect, I have been enabled to examine the physical characters of the colouring matter as it exists in the organism of this little insect before it is subjected to the process of drying for commerce. On examination by the mi- croscope, the white dust which covers the insect and the ad- jacent parts of the cactus leaves, on which it feeds, has all the characters of an excrement ; it has a curled cylindrical form, is of very uniform diameter and of a white colour. On re- moving the powder with a little aether and piercing the side of the little creature, a quantity of a purplish red fluid exudes, which contains the colouring matter in minute granules as- sembled round a colourless and larger nucleus, and these groups float in a colourless fluid. It is evident from this, that, whatever may be the function of the colouring matter, it has a distinct and marked form, and does not pervade as a mere tint the fluid portion of the insect. Separation of the Colouring Matter. It became evident from a few preliminary experiments that the investigation would be greatly facilitated by the employ- ment of a large quantity of material ; and as in the course of the inquiry different methods were adopted for the prepara- Mr. De la Rue on Cochineal. 477 tion of the colouring matter, capital letters will be used to designate the various preparations. A. About 3 lbs. of ground cochineal (technically known as shelly black) was introduced into 15 gallons of boiling distilled water, and the mixture maintained at that temperature for twenty minutes ; the decoction, strained through a sieve, was allowed to subside for a quarter of an hour and then decanted off; whilst still hot the transparent liquid was mixed with basic nitrate of lead, added with caution to avoid excess ; a fine purple lake was thus obtained, the supernatant liquor retaining only a pale buff tinge. After decantation of the supernatant liquor, the lake was thrown on a cloth filter and washed with distilled water until the filtrate gave but a slight opalescence with chloride of mercury, which was found to be a test for the presence of nitrogenous matter. The lead lake was then suspended in distilled water and treated with a co- pious stream of hj'^drosulphuric acid, when a precipitate of sulphuret of lead and a deep red supernatant liquid was ob- tained ; on stirring the liquid this colour almost disappeared, the colouring matter being evidently absorbed by the sul- phuret, agreeing perfectly with Arppe's observation. A fresh stream of gas reproduced the colour, which was again absorbed on stirring; after continuous treatment with hydrosulphuric acid, the lead lake being completely decomposed, the filtered liquid was evaporated in a water-bath to a syrupy consistence, and the evaporation finished as far as possible at a tempera- ture of 38° C. The semi-solid substance thus obtained was of a deep purple colour, had a strongly acid reaction, and evolved the smell of burnt sugar, as noticed by Arppe. The weight of this substance, which I call crude carminic acid, was 3^ ozs., and 1 oz. more was obtained from the residue by similar treatment. B. On repeating the same process the whole product was lost. An excess of the basic nitrate having been employed, the nitric acid set free by the hydrosulphuric acid caused a violent decomposition, with evolution of nitrous fumes, as soon as the carminic acid arrived at a pasty consistence ; this agrees also with Arppe's experience. C. In this operation a decoction of cochineal, made in the described manner, was precipitated with a solution of acetate of lead acidulated with acetic acid (six parts by weight of crystallized acetate, and one part of strong acetic acid). The resulting lead lake, being very bulky, was washed by decan- tation with boiling distilled water, collected on a filter, dried in a current of warm air, and finely powdered; 17 ozs. of crude cai'minate of lead were thus obtained. 478 Mr. De la Rue on Cochineal. D. Half a pound of cochineal was boiled with five pints of alcohol, spec. grav. '830. The filtered tincture deposited on cooling a granular precipitate, consisting chiefly of fatty matter retaining a portion of colouring matter; on concen- trating the tincture by distillation a further quantity was deposited, which was filtered off; the filtrate was evaporated to dryness in vacuo, when after eight weeks a gummy resi- due was obtained. This mass dissolved with great difficulty in a large quantity of absolute alcohol, a red flocculent substance consisting chiefly of nitrogenous matter remaining undissolved. The alcoholic solution filtered off" from this deposit, concentrated by distillation and finally evaporated in vacuo over sulphuric acid, dried to a tenacious semi-solid mass, covered with a colourless oily fluid, and containing cry- stalline particles of a solid fat. After removal of the fats by means of sether, this mass was digested in water at 38° C, which partly dissolved it with a fine red colour, leaving a brown mass of resinous aspect behind, more of which de- posited on the cooling of the coloured liquid ; the decoction was now evaporated to the consistence of a syrup, and finally dried in vacuo over sulphuric acid. These are all the processes employed to extract the colour- ing matter from the cochineal; 1 may here remark, before entering on the details of its further purification, that I ob- tained other substances on evaporating the mother-liquors from which the colouring matter had been separated by lead salts, which will be hereafter described. Purification of the Carminic Acid. — In my first attempts to purify the colouring matter I proceeded in the following way : — An aqueous solution of the crude carminic acid (A) was precipitated with acetate of lead, the precipitate of car- minate of lead well-washed and decomposed by hydrosulphu- ric acid ; the red supernatant liquid was first concentrated on the water-bath and finally dried in vacuo; a highly hygro- scopic purple residue was thus obtained. I could not, by whatever means I adopted, effect the deco- lorization of the colouring principle. In several attempts I heated the solution for some hours to 100° C, keeping up a continuous current of hydrosulphuric acid, and in other ex- periments a stream was made to pass for several days through the disengaged colouring matter, but without the slightest change in its aspect. From these experiments, made with the greatest care and at several periods, I am led to the same conclusion as Arppe, that Preisser must have been mistaken in his results, and I regret that I cannot throw any light on the probable cause of his error. Mr. De la Rue on Cochineal. 479 Several combustions of the carminic acid thus purified were made, the resulting numbers however became useless by the subsequent observation that this acid was by no means pure. A sufficient quantity being incinerated left a residue of acid reaction, which was suspected to contain phosphoric acid. Carminic acid burning only with great difficulty, it was re- converted into carminate of lead, the oxide of lead dissolved out of the residue obtained after fuming by acetic acid, which left a white residue of metaphosphate of lead, together with a little lead. The white residue was soluble in dilute nitric acid, and exhibited, when treated before the blowpipe, the characters of metaphosphate of lead; other tests likewise confirmed the presence of phosphoric acid. It will hereafter be seen that the process of extracting the colouring matter by alcohol (D) does not exclude the phosphoric acid, which in all probability existed in the colouring matter analysed by Pelletier. It is further evident that the presence of phos- phoric acid explains most satisfactorily the facts observed by Arppe. a. In order to separate the phosphoric acid, another por- tion of crude carminic acid (A) was precipitated with acetate of lead. Three-fourths of the carminate of lead produced were decomposed by hydrosulphuric acid and evaporated to dry- ness in the way already mentioned. The dry mass being dis- solved in cold absolute alcohol, and filtered from a slight floc- culent brownish residue, was heated to ebullition in a water- bath and mixed with the remaining fourth of the carminate of lead, which had been previously reduced to a fine powder ; the ebullition was continued for a few hours. In this method the free phosphoric acid combined with the lead, liberating an equivalent proportion of carminic acid, which was taken up by the alcohol. The alcoholic solution was filtered whilst hot, concentrated by distillation, and then evaporated in vacuo in the presence of sulphuric acid; it dried into a granular mass of a deep purple-brown colour, detaching itself sponta- neously from the sides of the vessel, and on examination by the microscope was found to be a beautiful transparent crim- son substance, exhibiting only slight, if any, signs of crystal- line structure ; by pulverization it became of a fine scarlet colour ; it left a mere trace of ash, and was found to be per- fectly free from phosphoric acid. It was highly hygrome- tric*. * In consequence of this it was found convenient to dry the carminic acid intended for analysis in little stoppered tubes in tlie air-pump, as tlie stopper could be rapidly inserted after desiccation, and access of air effec- tually prevented. 480 Mr. De la Rue on Cochineal. Burnt with chromate of lead, — I. '4647 grm. gave '9096 grm. carbonic acid and '2175 grm. water. JI. •4630 grm. gave '9105 grm. carbonic acid and '2140 grm. water. For the latter analysis I am indebted to my friend Mr. Ni- cholson. b. A second preparation of carminic acid was made by operating on the crude carminate of lead (C) and treating the resulting crude carminic acid in the manner just described for the preparation a. It left on incineration 0*2 per cent, of ash (•1609 grm. giving '0003 grm. ash), which was neglected in the following analyses : — III. '3710 grm. gave '7316 grm. carbonic acid and '1710 grm. water. IV. '3685 grm. gave '7235 grm. carbonic acid and '1722 grm. water. c. To effect the purification of the carminic acid (D) ob- tained by digesting cochineal in alcohol, it was dissolved in water and precipitated by acetate of lead; the filtrate was found to contain nitrogenous matter,' and the carminate of lead to be contaminated wath phosphate of lead; it was therefore treated in the manner already detailed. V. "3925 grm. of this substance gave "7658 grm. carbonic acid and •1780 grm. water. d. A fourth preparation of carminic acid was obtained by substituting phosphoric acid for hydrosulphuric in the de- composition of the crude carminate of lead (C), and evapo- rating the carminic acid to dryness in contact with a fresh portion of carminate of lead ; this did not however separate entirely the phosphoric acid, it was therefore redissolved in boiling absolute alcohol, and maintained some time at that temperature with more carminate of lead. On analysis — VI. ^3805 grm. gave "7530 grm. carbonic acid and •1848 grm. water. Pelletier having obtained in his analysis of " carmine" (carminic acid) as much as 3*56 per cent, of nitrogen, all the before-cited preparations of carminic acid were carefully exa- mined qualitatively for nitrogen by heating with soda-lime, and without exception gave indications of its presence; in most cases but a mere trace was found, but I thought it ne- cessary notwithstanding to make a few quantitative determi- nations, especially as M. Berzelius* had pointed out the im- probability of it being an essential constituent. * Traite de Chim. t. iii. p. 808. Brussels, edit. 1839. Mr. De la Rue on Cochineal, 481 The last preparation {d) appearing to contain more than any of the others, it was chosen and burnt with soda-lime. It was indispensable in experiments of this nature to test the purity of the soda-lime as regarded the absence of am- monia. A tube having 9 inches of its length filled with soda- lime was heated to redness, just as in a nitrogen determi- nation ; the hydrochloric acid, being treated with bichloride of platinum in the usual manner, gave 7'5 milligrammes of ammonio-chloride of platinum ; and a repetition of the expe- riment gave a similar result. This allowance has been made on all the nitrogen determinations by soda-lime. •5938 grm. carminic acid {d) gave '0717 grna. ammonio- chloride of platinum = 0*76 per cent, of nitrogen. This quantity of nitrogen could not be supposed to belong to the composition of the colouring matter, but was evidently due to some foreign substance, and not improbably to am- monia. In order to purify the carminic acid still more, the same specimen {d) was dissolved in a small quantity of boil- ing absolute alcohol and the filtered solution mixed with three times its bulk of anhydrous aether ; a splendid scarlet precipi- tate was immediately produced, which absorbed water rapidly from the atmosphere, and agglutinated into a dark purple mass ; when dried it weighed 0*3 grm. (e). The filtrate, which was of a pale orange-red colour, left on evaporation 0*5 grm. of carminic acid (/"). •2635 grm. (e) burnt with soda-lime gave '0637 grm. am- monio-chloride of platinum = 1*52 per cent of nitrogen. •4732 grm. (/) gave "0150 grm. ammonio-chloride of pla- tinum = 0^2 per cent, of nitrogen. We have therefore (e) 0*3 grm. found to contain by ana- lysis 1^5 per cent, nitrogen, and (/) 0^5 grm. 0^2 per cent., (3 X 1-5) -I- (5 X 0^2) ^„ . u- 1, ^ = '69 average per cent., which agrees o closely with '76, found previous to treat]Tient with eether. (/. Another preparation of carminic acid was obtained by precipitating crude carminic acid with acidulated acetate of copper, which salt was found to carry down the carminic acid, and to leave in solution by far the greater portion of the phosphoric acid. The carminate of copper, which occupied a long time in washing, was collected and decomposed by hydrosulphuric acid. The filtrate was evaporated to dryness, dissolved in boiling absolute alcohol, filtered, concentrated by distillation, and again evaporated to dryness in vacuo. It still contained a trace of phosphoric acid. On evaporating the mother-liquor and filtering, from an impure carminate of copper which deposited as the acetic acid was driven ofi^, and Phil. Mag. S. 3. No. 2 11 . Suppl. Vol. 3 1 . 2 1 482 Mr. De la Rue on Cochineal, again concentrating to dryness, a brown mass was obtained, which on incineration left a greenish- white very hygrometric ash, in which phosphoric acid, soda and copper were found. Burnt with chromate of lead — VII. '4020 grm. carminic acid {g) gave '7842 grm. carbonic acid and '1662 grm. water. This acid however still retained some impurities : on inci- neration it left 0*4 per cent, of ash ('5489 grm. giving "0022 grm. ash), and examined for nitrogen it gave the following numbers : — •4731 grm. burnt with soda-lime gave 'OlSOgrm. ammonio- chloride of platinum = 0*2 per cent, of nitrogen. h. In order to separate these impurities the greater portion was dissolved in boiling absolute alcohol, and filtered from a slight residue ; the remainder, about an eighth, was converted into carminate of lead and digested with the boiling alcoholic solution for some hours ; the alcoholic tincture filtered off whilst hot and mixed with about six times its volume of an- hydrous aether ; this threw down a bulky precipitate of a fine red colour, which was separated by filtration and the filtrate concentrated in a retort, and finally evaporated to dryness in vacuo {h). i. The precipitate retained on the filter was dried in vacuo, then dissolved in as small a quantity of alcohol as possible, and again mixed with a large quantity of aether ; this deter- mined a precipitate which was no longer of a fine red but of a brown colour, and on re-solution and similar treatment it di- minished in quantity and became darker in colour, leaving the colouring matter in solution. From the filtrates a quan- tity of carminic acid {i) was obtained on evaporating to dry- ness in vacuo. It therefore appears that the aether precipi- tates a nitrogenous body which carries down with it variable quantities of carminic acid, according as a larger or smaller relative proportion is present. The carminic acid {h) was found to be free from phosphoric acid as well as nitrogen. •3003 grm. burnt with soda-lime gave "001 5 grm. ammonio- chloride of platinum = 0*03 per cent, of nitrogen. From this analysis I venture to assert that the colouring principle of cochineal contains no nitrogen, thus fully con- firming the anticipation of Berzelius. We can now under- stand from the preparation of the specimen of carminic acid (e), that the method employed by Pelletier for the prepara- tion of the substance he analysed was calculated to accumu- late all the nitrogenous matter contained originally in his alcoholic decoction ; a fact which fully explains the large amount of nitrogen he obtained in his analysis. Mr. De la Rue o« Cochineal. 48J An analysis of the carminic {h) acid by chromate of lead gave from — VIII. '3167 grm. '6203 grm. carbonic acid and •1402 water. The following table exhibits the per-centage results de- duced from the foregoing analyses : the specimens were all dried over sulphuric acid in vacuo, with the exception of ana- lysis VII., in which the carminic acid was dried at 100° C. I. II. III. IV. V. VI. VII. VIII. Mean. Carbon... 53-38 53-63 53-78 53-55 53-21 53-97 53-20 53-42 53-51 Hydrogen 5-20 5-14 5-12 5-19 5-04 5-39 4-59 4-92 5-07 By the analysis of a copper salt of carminic acid hereafter to be mentioned, it became probable that carminic acid might still retain, when only dried in vacuo, a portion of the solvents employed ; a presumption which was supported by the ana- lysis VII., in which the substance analysed had been dried at 100*^ C, and which gave a smaller per-centage of hydrogen. A portion of carminic acid {i), being first dried in vacuo, and then heated to a temperature of 121° C, was found to yield a small quantity of acetic acid, and was not altered in its properties, which were not in fact changed even at a tempe- rature of 136° C. In the following analyses the carminic acid, previously dried in vacuo * and then at a temperature of 120° C, gave, on burning with chromate of lead, the following results : — IX. '3347 grm. {h) gave '6648 grm. carbonic acid and •1381 grm. water. X. '3583 grm. (i) gave '7108 grm. carbonic acid and •1504 grm. water. These analyses give the following per-centage quantities : — IX. X. Carbon . . . 54*17 54-10 Hydrogen . . 4-58 4*66 The analysis IX. being of the same preparation as had served for analysis VI II., it is fair to presume that all the other specimens of carminic acid would have given the same per-centage quantities as the specimen (A) if dried at 120° C, as this particular specimen, dried in vacuo, yielded numbers in close accordance with the mean of the other analyses. These numbers converted into the most simple expression lead to the following formula, Cj4 H^ Og ; but an analysis of a copper salt renders it probable that this formula has to be * The carminic acid fuses if exposed to a temperature of 120° C, with- out having been previously dried. 2X2 4S4 Mr. De la Rue on Cochineal. doubled, and that the composition of carminic acid is ex- pressed by the formula, C28 Hi4 O16, as may be seen from the following table containing the com- })arison of the theoretical per-centages with the mean of ana- yses IX. and X. Theory. Experiment. C29 . 168 54-19 5413 Hi4 . 14 4-52 4-62 Oje- . 128 41-29 41-25 310 100-00 100-00 From the foregoing experiments, it seems that the best method of obtaining pure carminic acid is to precipitate the aqueous decoction by acetate of lead ; to decompose the washed carminate of lead by hydrosulphuric acid, and to throw down the carminic acid once more by acetate of lead, previously mixed with acetic acid ; to decompose the carmi- nate of lead by hydrosulphuric acid ; to evaporate to dryness and redissolve the carminic acid in absolute alcohol ; then to digest the alcoholic tincture with carminate of lead ; and lastly, to precipitate the trace of nitrogenous matter by aether, the pure carminic acid is obtained from the filtrate. As thus prepared, carminic acid has the following proper- ties. It is a purple brown friable mass, transparent when viewed by the microscope, and pulverizing to a fine red powder ; soluble in water and alcohol in all proportions, very slightly soluble in aither, which does not however precipitate it from its alcohoHc solution if free from nitrogenous matter. It is soluble without decomposition in concentrated hydro- chloric and sulphuric acids. It is decomposed by chlorine, iodine and bromine, which change its colour to yellow, and the latter on warming or by standing gives a yellow precipi- tate soluble in alcohol. Nitric acid decomposes it even if highly diluted : I shall have occasion to refer to this decom- position presently. It bears a temperature of 136° C. with- out decomposition ; on gradually increasing the temperature a quantity of an acid liquor is produced, and at a red heat it intumesces and gives oft" a small quantity of red fumes, which condense : it gives no trace of oily matter. The aqueous solution has a feeble acid reaction ; it does not absorb oxygen. A volume of this gas contained in a tube with carminic acid over mercury did not change by absorption after exposure for several months. The fixed alkalies and ammonia give no precipitate in the aqueous solution, merely changing its colour to purple j in the alcoholic tincture they Mr. De la Rue on Cochineal. 485 produce purple precipitates ; all the alkaline earths produce purple precipitates ; sulphate of alumina gives no precipitate, but on addition of a drop of ammonia the carminic acid is immediately taken down as a beautiful crimson lake ; acetates of lead, copper, zinc and silver give purple precipitates ; the latter is immediately decomposed, and silver deposited ; the nitrates of lead, mercury and silver reddish precipitates ; pro- tochloride and bichloride of tin no precipitates, but change the colour to a deep crimson. The acid character of carminic acid being so very little pro- nounced, I met with considerable difficulties in determining its atomic weight ; it is only with great reserve that I bring forward the formula before cited. Several attempts were made to produce soda, baryta, lead and copper compounds, but it was only with the copper salt that I obtained results agreeing in different preparations. It seems that carminic acid attaches itself to salts, for it was found that the precipitants could be removed from the precipitates only with the greatest difficulty. I omit several soda, baryta and lead determinations which have not led to any satisfactory result, and confine myself to the statement of the result of the analysis of the copper compound. It was obtained by acidulating an aqueous solution of pure carminic acid with acetic acid, and then precipitating by the cautious addition of acetate of copper, so as to leave an excess of car- minic acid in the liquid. The precipitate was well-washed by decantation (by which a great loss was sustained) and dried. It formed into masses of a bronze colour, very hard and dif- ficult to powder. Two specimens were prepared at different times (« and b). I. -2800 grm. (a) dried at 100° C. left, after ignition and treatment with nitric acid and re-ignition, '0330 grm. oxide of copper. II. -3782 grm. (b) dried at 100° C. gave -0426 grm. oxide of copper. III. '4702 grm. (b) dried at 100° C. gave on burning with chromate of lead '8210 grm. carbonic acid and '1743 grm. water. These numbers lead to the following per-centage results : — I. II. III. Carbon ... 47*62 Hydrogen ... 4*12 Oxide of copper 11-78 11-27 agreeing closely with the formula, C^ H^4 Ojg, CuO, as will be seen from a comparison of the theoretical and experimental numbers. 486 Mr. De la Rue on Cochineal. Calculated. Found. Carbon ... 28 168 48-05 47-62 Hydrogen . .14 14 4-01 4-12 Oxygen • . .16 128 36-61 36-74 Oxide of copper 1 39-6 11-33 11-52 349-6 100-00 100-00 Action of Nitric Acid on Carminic Acid. Nitrococcusic Acid. — ^When acting with nitric acid on " car- mine" (carminic acid), MM. Pelletier and Caventou obtained white acid crystals resembling oxalic acid, but differing from this acid in several of its properties. M. Arppe found that the acid produced was oxalic acid. In my experiments I ob- tained the following results : — One pound and a half of crude carminic acid was gradually introduced into ten pounds of nitric acid, spec. grav. 1-4, and digested at a moderate heat; a violent evolution of nitrous fumes succeeded each addition of the carminic acid ; after the whole quantity had been in- troduced and the action had somewhat subsided, the mixture was transferred into a smaller vessel and the action continued at the boiling-point for about two hours ; by this time the greater part of the nitric acid had evaporated, and on with- drawing the vessel from the fire and allowing the mixture to cool, a crystalline cake was obtained, which on examination M'as found to consist partly of a new acid and partly of oxalic acid. To separate the oxalic acid, it was dissolved in a large quan- tity of boiling water and treated with nitrate of lead as long as any precipitate formed ; this was collected and decomposed by boiling with dilute sulphuric acid ; the filtrate from the sulphate of lead yielded a large quantity of prismatic crystals of oxalic acid, which were obtained perfectly white and pure after two or three crystallizations with the aid of a little animal charcoal. The yellow liquid filtered from the oxalate of lead was con- centrated and separated from a fresh portion of oxalate which deposited on concentration, the evaporation was then continued until a large quantity of crystals formed; the solution on cooling deposited a very bulky mass of yellow rhombic prisms, which were drained and dried, and re-dissolved in a sufficient quantity of boiling water, which on cooling deposited the acid (for which I propose the name of nitrococcusic acid) in beautiful crystals free from any lead salt ; it was recrystal- lized twice more, by which means it was obtained perfectly pure. Several preparations were made, sometimes using pure car- Mr. De la Rue on Cochineal, 4A% minic acid, at other times carminate of lead, with similar re- sults. The analyses of four different preparations dried at 100° C. gave, on burning with chromate of lead (unless otherwise stated), the following numbers : — I. '3152 grm. {a) gave '3892 grm. carbonic acid and '0561 grm. water. II. "2500 grm. (a) gave '3080 grm, carbonic acid and '0445 grm. water. (For this analysis I am indebted to Mr. Nicholson.) III. '3068 grm. (a) gave '3820 grm. carbonic acid and •0502 grm. water. IV. '4498 grm. {b) gave '5626 grm. carbonic acid and •0757 grm. water. V. '4461 grm. (c) gave '5515 grm. carbonic acid and '0777 grm. water. VI. '4503 grm. (c?) gave, on being burnt with oxide of copper, '5585 grm. carbonic acid and '0757 grm. water. VII. '4796 grm. (c) gave, on being burnt with oxide of copper, and a layer of copper twelve inches long used so as to completely decompose the binoxide of nitrogen, '5882 grm. carbonic acid and '0815 grm. water. The foregoing analyses lead to the following per-centage quantities : — I. II. III. IV. V. VI. VII. Carbon . 33-67 33*60 33-95 34-11 33-72 33-82 33-44 Hydrogen 1-98 1-98 1-82 1-87 1-93 1-87 1*89 In the following experiments the nitrogen of the nitrococ- cusic acid was ascertained by burning with oxide of copper in an atmosphere of carbonic acid. VIII. -6808 grm. {h) dried at 100° C. gave 84 cub. cent, of moist nitrogen at 6°-5 C. and 0*7585 m., barometer corrected. IX. '7162 grm. (c) dried at 100° C. gave 91-5 cub. cent, of moist nitrogen at 17°*5 C. and 0*7641 m., barometer corrected. These numbers correspond to the following per-centage quantities : — VIII. IX. Mean. Nitrogen . . 15-03 14-92 14-97 X. In this experiment the nitrogen was determined accord- ing to Bunsen's* method, which consists inhuming the sub- stance mixed with oxide of copper in the presence of copper turnings in a hard glass tube. The tube being freed from air by a stream of hydrogen, is then exhausted, sealed hermetically, and placed in an iron mould filled with plaster of Paris ; it is then heated to redness and allowed to cool. After the com- * Liebig's ^nnalen, vol. xxxvii. p. 27. 488 Mr. De la Rue on Cochineal. bustion, the gas is transferred into a graduated jar over mer- cury and its volume noted ; the carbonic acid being absorbed by a potash ball, the volume is again read off. This analysis gave the following numbers : — Vol. Temp. Diff. of level. Barom. Carbonic acid -f nitrogen (moist) 123 20°'7 C. 0"'-0640 0'"-7543 Nitrogen 22-2 20°-0 O^-IGSO 0-"7529 The height of the column of mercury in the eudiometer above the level in the trough and the barometric column are corrected for temperature. Carbonic acid -\- nitrogen corrected to 0° C. and barom. 1™ := 76-84 Nitrogen 0° ... 1°' = 12-16 Carbonic acid 0° ... l'" = 64-68 ■ - ., - = 5-32, which is the ratio of carbon equivalents to one I2"lb nitrogen equivalent. The preceding analyses of nitrococcusic acid agree with the following formula, confirmed by the analyses of several of its compounds, C.,H,N3 0,„ as will be seen on referring to the table. Theory. Experiment. Carbon . 16 Hydrogen 5 Nitrogen . 3 Oxygen . 18 96 33-45 5 1-74 42 14-63 144 50-18 287 100-00 33-75 1-91 14-97 49-37 100-00 By analysis VII., in which the precaution was taken of using a very long layer of copper turnings, there was ob- tained, carbon 33-44, hydrogen 1-89 ; these numbers agree as closely as possible with the theoretical quantities, as does likewise the nitrogen determination (X.) by Bunsen's method ; in this experiment the ratio of carbon equivalents to nitrogen equivalents was found to be as 5*32 to 1, or as 16 equivs. of carbon to 3-007 equivs. of nitrogen ; taking analysis VII. as the basis of calculation, it gives 14'67 per cent, of nitrogen, the theoretical number being 14-63. The acid, as it separates from its aqueous solution, contains water of crystallization, which it loses at 100° C. ; four expe- riments gave the following results : — •4800 grm. lost -0289 grm. = 6-02 per cent. -6613 -0395 ... =5-97 •6586 -0385 ... =5-84 •4804 -0289 ... =6-01 Mean . . =5*96 Mr. De la Rue on Cochineal. 489 This mean corresponds perfectly with the formula C,6H5N3 0i8 + 2Aq, as may be seen by a comparison of the theoretical and expe- rimental numbers. Theory. Experiment. f ^ 1 Mean. 1 equiv. dry acid ... 287 94*10 94*04 2 ... water .... 18 5*90 5*96 1 ... crystallized niO 3^^ ^^^,^^ ^^^^.^^ trococcusic acid . .J Properties of Nitrococcusic Acid. — It is of a yellow colour, crystallizing in rhombic plates, and presenting very different aspects, according to the circumstances under which it is cry- stallized. Its solution stains the skin yellow, it is soluble in cold, but considerably more so in hot water; soluble in al- cohol, and very soluble in aether. All its salts dissolve readily in water, and most of them in alcohol ; it deflagrates violently on being heated ; it dissolves iron and zinc, becoming dark- coloured. It is decomposed by sulphuret of ammonium with separation of sulphur and the formation of the ammonia salt of a new acid, which I have not yet examined. Compounds of Nitrococcusic Acid. Nitrococcusate of Potash. — I have prepared this salt by two different methods. a. A solution of nitrococcusic acid in boiling water was accurately saturated with carbonate of potash ; by evaporation to a small bulk and cooling, the salt was obtained in small yellow crystals ; it was purified by draining and recrystallizing. b. An aetherial solution of the acid was precipitated by the cautious addition of an alcoholic solution of potash ; the pale yellow precipitate washed with aether and dried, then dissolved in as small a quantity of cold water as possible, and the solu- tion poured into about five times its bulk of absolute alcohol ; after standing some time the salt crystallized in well-formed crystals ; it was washed with aether and dried. The aetherial washings being added to the mother-liquor, a further portion was obtained and washed with aether. The latter process is less troublesome than the process a. I. *5469 grm. (a) dried at 100° C. were dissolved in a small quantity of boiling water and decomposed by sulphuric acid ; dried in a water-bath, the nitrococcusic acid, removed by aether and the residue ignited, gave '2606 grm. sulphate of potash. IT. *4383 grm. [b) dried at 132° C. gave -2103 grm. sul- phate of potash. III. '6251 grm, {b) dried at 100° C. and burnt with chro- 490 Mr. De la Rue on Cochineal. mate of lead, gave -6064 grrn. carbonic acid and -0662 grm. water. These numbers give the following per-centage quantities : — I. II. ■ III. Carbon ... 26-46 Hydrogen . ... ... 1*18 Potash . . 25-74 25-92 corresponding with the formula Ci6H3N3 0,6+2KO, as may be seen by comparing the theoretical and experimental numbers. Theory. Experiment. vj.6cin» Carbon . 16 96 26-45 26-46 Hydrogen Nitrogen . 3 3 3 42 -83 11-57 1-18 Oxygen . Potash 16 2 128 94 35-26 25-89 25-83 363 100-00 I was not successful in preparing a nitrococcusate of potash with one equivalent of fixed base ; the method I adopted was saturating a given weight of acid with carbonate of potash, and then adding the same amount of acid to the bibasic pot- ash salt ; on washing with tether the greater part of the ex- cess of acid was removed, leaving the bibasic salt behind. Nitrococcusate of Ammonia. — This salt was prepared by passing an excess of dry ammoniacal gas through an aetherial solution of the acid dried in the atmosphere ; the solution be- came turbid, and by standing for a short time deposited the salt in clusters of needles adhering firmly to the sides of the vessel ; these were removed, washed with jether, and dried on bibulous paper. It is volatile, and sublimes on being heated, most probably with decomposition, I. -6011 grm. of the salt dried in vacuo was dissolved in a small quantity of boiling water and decomposed by strong hydrochloric acid, which immediately separated the acid in f rystals ; the mixture was dried in a water-bath, and the ni- trococcusic acid removed by aether, a little bichloride of pla- tinum and alcohol being added to the aetherial washings to precipitate a trace of chloride of ammonium. The residue, precipitated as ammonio- chloride of platinum, gave -8208 grm. of the double chloride. II. -6126 grm. dried in vacuo and burnt with oxide of cop- per, the mixture being made in the combustion-tube, gave .'6525 grm. carbonic acid and -2191 grm. water. Mr. De la Rue on Cochineal, 491 These numbers correspond with the following per-centage quantities : — I. II. Carbon . » 29-05 Hydrogen 3*97 Oxide of ammonium . . 15"91 agreeing closely with the following formula, C,6H3N3 0,6,2NH4 0 + HO, as may be seen by a comparison of the theoretical and expe- rimental numbers. Theory. Carbon . 16 Hydrogen 12 Nitrogen . 5 Oxygen . 19 96 12 70 152 330 29-09 3-64 21-21 46'06 100-00 Experiment. 29-05 ' 3-97 Or Theory. Experiment. Acid 1 269 Water 1 9 Oxide of ammonium 2 52 15*76 15-91 330 Nitrococcusate of Baryta was prepared by adding an excess of a solution of baryta to an aqueous solution of nitrococcusic acid, a stream of carbonic acid gas being passed through the solution to separate the excess of baryta. The solution was warmed, filtered and evaporated in a water-bath, and again filtered from a small quantity of carbonate of baryta. The evaporation being continued until a pellicle formed on the surface, the solution on cooling deposited this salt in minute yellow crystals. It is insoluble in alcohol, which precipitates it in the form of a jelly from the aqueous solution. I. -6750 grm. of substance dried at 100° C. and decom- posed by sulphuric acid, gave '3602 grm. of sulphate of baryta. II. -6439 grm. of nitrococcusate of baryta dried at 100° C. and burnt with chromate of lead, gave -5185 grm. of car- bonic acid and -0800 grm. of water. These numbers correspond to the following per-centage quantities: — I. II. Carbon 21'96 Hydrogen 1*38 Baryta 35-06 492 Mr. De la Rue on Cochineal. agreeing with the formula CjgHgNgOig + 2BaO + 2HOj as may be seen from the following table : — Theory. Experiment. ( 1 Carbon . 16 96-00 21-80 21-96 Hydrogen 5 5-00 1-14 1-38 Nitrogen . 3 42-00 9-54 Oxygen . 18 144-00 32-71 Baryta . . 2 153-28 34-81 35-06 440-28 100-00 Nitrococcusate of Silver. — I attempted to make this salt by boiling oxide of silver with an aqueous solution of nitrococ- cusic acid, but there was an evident decomposition of the acid, a large quantity of carbonic acid being evolved ; after warming the filtered liquor a brown deposit was formed. On filtering off this brown deposit a silver salt was obtained by evaporation, which yielded on analysis — Carbon .... 23-64 Hydrogen . . . 1-26 Oxide of silver . . 38-10 per-centage numbers not reconcilable with those of nitro- coccusate of silver. On decomposing a hot solution of this salt with hydro- chloric acid a new acid was obtained, perfectly distinct from nitrococcusic acid ; it crystallized in long needles ; very in- soluble in water, but soluble in aether and alcohol. 1 refrain from giving any further account of this acid until the study is completed. In order to avoid decomposition the nitrococcusate of silver was prepared without the aid of heat, by dissolving carbonate of silver in a cold aqueous solution of nitrococcusic acid and evaporating the filtered solution in vacuo over sulphuric acid. The salt crystallized in long bulky needle-like crystals of a yellow colour; when dried at 100° C. the powdered salt be- comes deep orange. It is soluble in alcohol and water, and is highly explosive when heated ; in small quantities it may be decomposed by a progressive heat without any violent action ; but on attempt- ing to decompose a quantity amounting to -45 grm. in a porcelain crucible, heated in an air-bath, the salt exploded with great violence, shattering the copper air-bath and driving fragments of the crucible through the copper ; the tempera- ture was noted just before the explosion, the thermometer standing at 200° C. ; the silver was therefore determined as chloride. Mr. De la Rue on Cochineal. 493 I. -4698 grm. of substance (a) dried at 100° C. and decom- posed by nitric acid and the silver precipitated by the addi- tion of hydrochloric acid, gave -2675 grra. chloride of silver. II. -5085 grm. of substance {b) dried at 100° C. gave •2892 grm. chloride of silver. III. -8184 grm. of substance («) dried at 100° C. and Tjurnt with oxide of copper, gave -5700 grm. carbonic acid and -0554 grm. water. Corresponding to the following per-centage quantities : — I. II. III. Carbon ... 18-99 Hydrogen ... 0*75 Oxide of silver . . . 46-03 45-97 and agreeing closely with the following formula, C,6H3N3 0,s+2AgO, as may be seen by the following table : — Theory. Experiment. Carbon ... 16 96 19-162 Hydrogen . . 3 3 -599 Nitrogen . . 3 42 8-383 Oxygen ... 16 128 25-549 Oxide of silver . 2 232 46-307 501 100-000 18-99 •75 46-00 Nitrococcusate of Copper. — This was made by dissolving carbonate of copper in nitrococcusic acid and deposited on evaporation in pale apple-green needles. I made no analysis of this salt. The following is a synoptical table of the analyses of nitro- coccusic acid and its compounds : — Hydrate of nitrococcusic acid . C,gH3N30i(. + 2HO. Hydrate of nitrococcusic acidn 4_oTTn ■ oA as crystallized from water j "i 4- Nitrococcusate of potash +2KO. Nitrococcusate of ammonia +2NH40 + Aq. Nitrococcusate of baryta +2BaO + 2Aq. Nitrococcusate of silver +2AgO. The properties of nitrococcusic acid and its salts exhibit a great analogy with those of a number of acids obtained by the action of nitric acid on organic bodies, more especially nitropicric and styphnic acids, from which it differs by the greater solubility of its salts. If we assume with many chemists the nitrogen of these 494 ' Mr. De la Rue on Cochineal. acids to exist in the form of hyponitric acid, the formula of nitrococcusic acid will be represented by C,«/!lu To., 2HO. '16 This acid would consequently derive from a non-nitrogenous acid, having the composition expressed by the formula • Ci6H6 04,2HO. When I first began this investigation I imagined that a similar relation might exist between nitrococcusic acid and carminic acid ; the analysis of these acids, however, as well as the simultaneous production of a large quantity of oxalic acid in its oxidation, showed that this view was erroneous, and that nitrococcusic acid was derived from carminic acid in a more complex manner. Some attempts were made to pro- duce the non-nitrogenous acid, the coccusic acid, but unsuc- cessfully. The experiments of MM. Cahours and Laurent on the oxidation of the oils of anise and of tarragon [Oleum dracun- culi) have made us acquainted with anisic acid, the composi- tion of which is Cjg Hg Og. ■ The formula agrees with the composition of the hypothetical hydrated coccusic acid. Anisic acid, however, as well as nitranisic acid, being mono- basic, it was not probable that the further introduction of the elements of hyponitric acid Avould convert it into a bibasic one ; nevertheless it was my intention to have studied the further action of nitric acid on the acids mentioned, in order to obtain if possible trinitroanisic acid, and to compare this substance with the acid obtained from carminic acid, when an account of some new experiments of M. Cahours came under my notice, of the action of a mixture of concentrated sulphuric and nitric acids on anisic acid, by which he has succeeded in preparing trinitroanisic acid. The experiments of M. Ca- hours have not yet been published in detail, and from his short account it was not possible to decide on the identity or non-identity of nitrococcusic and trinitroanisic acids. A small specimen of anisic acid at my disposal was treated in the manner described by him ; after acting for some time water threw down an acid, from the insolubility of which I conclude that these acids are only isomeric. Investigation of the Mother-liquor from wJiick the Carminic Acid had been separated. On evaporating the mother-liquors of carminic acid and separating the lead held in solution by means of hydrosul- Mr. De la Rue on Cochineal. 495 phuric acid, they all gave the following results : on acquiring a syrupy consistence, a white chalky-hke matter subsided; this was separated by filtration, and proved to be a new cry- stalline body. The liquor filtered off from this substance deposited a small quantity more on further concentration, and could only be dried to a soft tenacious mass, partly soluble in alcohol, the rest being soluble in water. From three pounds of cochineal five ounces of this soft matter were obtained, showing that the precipitation by a lead salt had effected the separation of carminic acid from a large quantity of foreign matters. This gelatinous matter appears to be of a complex character, but I have not yet examined it fully. To purify the chalky-like matter, it was well-washed with cold water and crystallized twice by solution in boiling water and evaporation ; it w as then dissolved by boiling it in a just sufficient quantity of water ; animal charcoal was now added, and the ebullition continued for a few minutes ; the solution filtered whilst hot deposited on cooling a mass of silky cry- stalUne tufts, completely filUng the liquid, and when collected and dried they aggregated into paper- like masses of a silky aspect. I obtained in three experiments 4 parts of the new body from 1000 of cochineal. I. '4918 grm. of substance, preparation {a), dried in vacuo and burnt with oxide of copper, gave 1*0705 grm. carbonic acid and 0*2838 grm. water. II. '5680 grm. of substance {b) gave 1*2416 grm. carbonic acid and *3160 grm. water. III. '4700 grm. of substance {b) gave 1*0210 grm. car- bonic acid and *2660 grm. water. For the latter analysis I am indebted to the kindness of Mr. Nicholson. A qualitative examination having pointed out the presence of nitrogen, it Mas determined by Varrentrapp and Will's method. IV. '5046 grm. of substance (a) dried in vacuo and burnt with soda-lime, gave *6131 grm. ammonio-chloride of pla- tinum. V. '5076 grm. of substance [b) gave '6239 grm. ammonio- chloride of platinum. From these numbers the following per-centages are calcu- lated : — I. II. III. IV. V. Carbon . 59*36 59*62 59*25 Hydrogen 6*41 6*18 6*29 Nitrogen . ... ... ... 7*62 7'7l 496 Mr. De la Rue on Cochineal. These per-centages, translated into the most simple expres- sion, lead to the formula, Cgi Hu NOg as may be seen from the following table : — . 18 . 11 . 1 . 6 Theory. Experiment. Mean. 59-41 6-29 7-66 Carbon . . Hydrogen . Nitrogen . Oxygen . . 108 59-668 11 6-077 14 7-735 48 26-520 181 100-000 Careful and repeated examinations for sulphur proved the absence of this element as a component of the new white sub- stance. I have been unable to produce a compound to con- trol the proposed formula, though several methods were adopted ; amongst others, I attempted to form a lead com- pound by adding acetate of lead to an ammoniacal solution of the substance; I obtained merely a bulky precipitate, con- sisting of little else than oxide of lead. This substance is sparingly soluble in cold water, much more so in boiUng water ; insoluble in alcohol and aether ; soluble in hydrochloric acid, which appears to be driven off by evaporation, leaving the substance in large crystals. In a large quantity of nitric acid it dissolves with a slight evolu- tion of gas ; the solution evaporated spontaneously furnishes long crystals, which are in all probability a new acid ; if dis- solved in a small quantity of nitric acid, the mixture becomes spontaneously heated, violent action takes place, and the pro- duct is lost ; frequently the substance becomes blackened into charred masses. It is soluble in ammonia, from which it is again recovered by the evaporation of the ammonia. It is soluble in the fixed alkalies, and is precipitated from these solutions by saturating with an acid. In a short paper, entitled "Valerianic Acid and a new body from Casein," Baron Liebig* describes a new substance obtained by fusing casein with hydrate of potash until an evolution of hydrogen takes place along with ammonia. On saturating with acetic acid the aqueous solution of the fused mass an aggregate of fine needles was produced, which were purified by repeated solution in carbonate of potash and re- precipitation by acetic acid. A preliminary analysis led to the formula Cjg Hg NO^, differing from the result I obtained in the analysis of the white substance from cochineal by two carbon, two hydrogen, and one oxygen. The properties of the two bodies being however so analogous, it is extremely probable that they are identical, a presumption I am sup- • Liebig's Annalen, vol. Ivii. p. 127. On Crystals in the Cavities oj Minerals. 4-97 ported in by a comparison of a specimen kindly furnished me by Dr. Hofmann * ; further investigations will clear up this point : in the meantime I refrain from proposing a name, as Liebig f has lately proposed the name Tyrosine for the sub- stance prepared from casein. As the latter body arises evi- dently from a process of oxidation, and as I had obtained the first crop of crystals from a liquid from which the colouring matter had been precipitated by the basic nitrate of lead, I thought that this body might owe its formation to the action of the nitric acid liberated by the sulphuretted hydrogen ; but this supposition proved to be erroneous, for in later experi- ments in which acetate of lead had been used, the same body, and in exactly the same quantity, was obtained. From this we may assume that this substance is contained ready-formed in the cochineal insect. My engagements for the present preventing me from con- tinuing these researches, I must defer for a future period their completion, but hope to be enabled to communicate to the Society a second paper. In conclusion I may be allowed to express my thanks to my friend Dr. Hofmann for his valuable instruction in the methods of organic research, and his kind advice during the progress of this investigation. LXXIII. On the Existence of Crystals tvith different jn-imitive forms and j)hysical properties i7i the Cavities of Minerals ; with additional Observations on the Nexv Fluids in which they occur. By Sir David Brewster, K.H., LL.D., F.'R.S., and V.P.R.S. Edin.X [With a Plate.] IN 1823 and 1826 I communicated to the Society two papers on the nature and properties of two immiscible fluids, which I discovered, in contact with each other, in the cavities of topaz and other minerals §. Although the facts contained in these papers were of so extraordinary a nature as to be received with scepticism by some, and with ridicule by others, yet I am not aware that, during the twenty years which have elapsed since their publication, any person has either repeated my observations, or advanced a single step in the same path of inquiry. In showing to strangers some of the leading phaenomena of the two new fluids, my attention has been frequendy recalled to the subject ; but it was not till * This specimen had been prepared by Baron Liebig himself. — A.W.H. f Researches on the Chemistry of Food, p. 16. X Read before the Royal Society of Edinburgh on the 17th of February 1845, and published in their Transactions, vol. xvi. part 1. p. U. § Edinburgh Transactions, vol. x. p. 1 and 407. Phil. Mag. S. 3. No.211. Stippl. Vol. 31. 2 K 498 Sir David Brewster on the Existence of Crystals last spring, when I discovered cavities in topaz filled with the most beautiful crystals of various form, that 1 was induced to undertake a new investigation of their nature and properties. In this investigation I have examined, with various magnifying powers, and both in common and polarized light, more than 900 specimens of topaz from Scotland, New Holland, and the Brazils ; and I have had the good fortune to observe many new phaenomena connected with mineralogy, chemistry, and physics, which, in addition to the interest which they may possess as scientific facts, promise to throw a strong light upon the existing theories of crystallization, and to bring before us some of those recondite operations which had been going on in the primitive rocks of our globe, before the commencement of vegetable or animal life. 1. On the Form and Position of the Strata ifi which the Cavities lie. The cavities which contain the two new fluids, and their accompanying crystals, sometimes occur single, and in groups more or Jess numerous ; but, in general, they exist in millions, occupying extensive strata, which affect the transparency of the mineral, and render it unfit for the use of the jeweller, or even for the cabinet of the collector, who has not learned that it is in the deviations from her ordinary laws that Nature often discloses her deepest mysteries. Although the strata of cavities sometimes occur, as in arti- ficial salts, in planes parallel to the primary or secondary forms of the crystal, yet they occupy every possible position m reference to these planes ; and we therefore cannot account for them by supposing that certain spaces have been left in the crystal, without the primitive molecules which ought to have been there deposited. The strata of cavities, too, have every possible curvature. From a plane surface they pass into a curved one, sometimes of variable curvature, and some- times of contrary flexure, cutting and intersecting each other in the most capricious manner. In the shape of the strata the same irregularity presents itself; their outline is sometimes rectilineal, sometimes curved, and sometimes singularly irregular. In some specimens the whole crystal is intersected with the strata; and it is extremely probable, though it is impossible to determine the fact, that in every specimen some edge or angle of the stratum touches the surface. The succession of the cavities in composing the stratum, and their form in relation to the character of the stratum, present interesting phasnomena. I have found specimens in in the Cavities of Minerals. • 499 which the cavities lie in concentric arches, and have their sides concentric, and, as it were, a portion of the same arches, as if they had been formed under the influence of a rotatory force. In other cases they occupy parallel lines, and are sometimes so equidistant that they might be advantageously used as mi- crometers for microscopes. In one remarkable specimen they radiate from a centre, each radiation having a character of its own. One radiation will -sometimes throw off a diverging branch, while two or more radiations will converge and then diverge again, subsequently uniting themselves into a single radiation. When different strata of cavities lie parallel to each other in the specimen, which they sometimes do, to the number of four ovjivey each stratum has generally a distinct character ; flat and exceedingly thin cavities occupying one stratum, very deep cavities occupying another, minute cavities which the highest magnifying powers can scarcely resolve occupying a third, while a fourth consists of the most irregular and inde- scribable forms. When the forms of individual cavities are related to that of the stratum which contains them, they, of course, cut at all angles the primary and secondary planes of crystallization ; and the same is true of insulated cavities of great length, which are sometimes turned, and twisted, and bent in the most ca- pricious manner. It is impossible to read these details, and still more so to study the phaenomena themselves, without being driven to the conclusion, that the strata of cavities must have been formed under the influence of forces propagated through a soft and plastic mass, and carrying along with them gases and vapours which came to a position of rest previous to the regular crystallization of the topaz. This conclusion, which I have been led to draw, in another paper, from a series of entirely different facts, will be still further confirmed by the phaenomena of imbedded crystals, to which I shall have to refer in another section. 2. Additional Observations on the Nature and Properties oj the two New Fluids. In re-examining the phaenomena exhibited by the two nev^ fluids, I have found no occasion to modify or to correct any of the results contained in my former papers. In the cavities which appear to contain only one fluid, namely, the dense fluid, I have sometimes found a very small quantity of the volatile fluid, which, with a slight rise of temperature, passes into vapour, and prevents the apparent vacuity from disap- pearing by the application of a strong heat. When there is 2 K2 500 Sir David Brewster on the Existence of Crystals no volatile fluid present in such cavities, the vacuity is a real one, and disappears entirely by the application of such a heat. It* the heat is not instantly withdrawn on the disappearance of the vacuity, the crystal never fails to burst with great violence. In some specimens of Brazil topaz I have found cavities with two fluids, and without any vacuity in the volatile fluid at the ordinary temperature of an apartment. In such cases I have generally produced a vacuity by the application of ice. Had heat been applied, the crystals would have burst, as there were no empty .spaces into which the fluids could expand. When the cavities are flat, and have their faces perpendi- cular to the axis of the crystal, or parallel to the planes of easy cleavage, the application of heat does not burst the cry- stal, but produces a very remarkable phaenomenon. The cavity opens at its weakest point, and the fluid passes by starts, through a succession of resting places, to another part of the crystal where it finds the readiest exit. The fluid penetrates, as it were, the solid gem, and the laminae which it has forced asunder in its passage, again close into optical if not into me- chanical contact. If the heat is withdrawn when the first minute drop has passed, the laminae unite, and we can discharge the rest of the fluid whenever we please till the cavity is exhausted. This phaenomenon is represented in Plate III. fig. 1, where ABCD is a shallow cavity in a plate of topaz MN, and EF another cavity, which has been emptied of its fluid contents by reaching the surface at N, where it had been broken through. Upon looking at the cavity ABCD when slightly heated, I observed dark portions of fluid rushing from its sharp termination at D through the cavity at a, and then reappearing at b and c, and then passing into the empty cavity EF. The small lakes, as we may call them, at «, b and c, disappeared entirely when the discharged portions of fluid had passed, and reappeared with a change of form and size when the operation was repeated. In a specimen of topaz possessed by Major Playfair, and seen by many individuals, a white ball passed from one cavity to the edge of the specimen, as if projected from a mortar ; but by the application of too strong a heat it was shattered in pieces. In my first paper of 182:3*, I have described and figured a phaenomenon of an analogous kind ; but as it appeared un- expectedly, and was instantly followed by the explosion of the crystal, I could neither observe it accurately, nor confirm what I did observe, by a repetition of the experiment. I have, therefore, some satisfaction in describing a similar phaeno- * Edinburgh Transactions, vol. x. p. 11, plate 1. fig. 5, 6. in the Cavities of Minerals. 501 menon, seen frequently, and under more favourable circum- stances, not only from its intrinsic interest, but because a distinguished philosopher had treated with an air of incredu- lity an observation which I had made of a similar kind. There can be no higher testimony to the novelty and import- ance of a scientific fact, than when a competent judge raises it to the supernatural. I come now to describe a property of the dense fluid, so new and remarkable that it cannot fail to excite the attention of chemists. This fluid occupies the whole of a large cavity ABCDE, fig. 2, with the exception of a bubble at A, which must be either a vacuum, as it is in all cavities containing only this fluid, or a bubble of the expansible fluid, or the vapour of the dense fluid, or some gaseous body. It cannot be a vacuum, because it expands with heat, in place of being filled up by the expansion of the fluid. It cannot be the expansible fluid, because cold would contract it, and produce a vacuity. It cannot be the vapour of the expansible fluid, because there is no expansible fluid to throw it oif, and it has not the optical properties of its vapour. It cannot be the vapour of the fluid in the cavity, for it does not disappear by the application of cold, and does not become a vacuit}', which fills up by the expansion of the fluid. It is therefore an independent gas, which exhibits the following phaenomena. When heat is applied, the bubble A expands, not by the degradation of its circular margin passing into vapour, as in the vapour cavities described in a former paper, but by the rapid enlargement of its area. When it attains a certain size, it throws off a secondary bubble B, which passes over a sort of ridge or weir inno^ in the bottom of the cavity, and settles at B. If the heat is continued, these two bubbles increase in size ; but it was instantly withdrawn when B had begun to swell. As the topaz began to cool, both the bubbles A and B quickly contracted. The primary bubble A returned gra- dually to its original condition, and B, when reduced to a single speck, would have disappeared, had the cooling not been stopped. This speck swelled again by the application of heat, and so did the bubble A. When the speck at B was allowed to vanish, which it did on the spot which the bubble occupied, the fresh application of heat did not revive it at that spot, but merely expanded the primary bubble A, which again threw off" a secondary bubble B, which exhibited by heat and cold the same phaenomena as before. These ex- periments I repeated many times with the same result. It will naturally be asked, what was the condition of the fluid itself wliich has the properly of expanding by heat ; and what be- 502 Sir David Brewster on the Existence of Crystals came of it while a part of the space which it occupied was appropriated by the bubble B, and the addition to the bubble A? An accidental circumstance enables me to answer this question, which would have been otherwise a very perplexing one. Having applied too strong a heat to the specimen, the bubble A threw off beside B two or three smaller ones, which moved along the upper edge AE. My attention having been thus directed to this part of the specimen, I was surprised to observe a great number of capillary lines or pipes PQ, rising from the edge AE of the cavity, and into which the fluid was forcing itself, oscillating in these minute tubes like the mercury in a barometer, and sometimes splitting the laminae between them. The force of cohesion, thus overcome by the expan- sive efforts of the fluid, predominated over the capillary attrac- tion of the tubes and surfaces, and pressed back all the fluid into the cavity, when the body of fluid had contracted in cooling. If we now consider the body which occupies the vacuity A as a gas, and, consequently, the other bubble B as the same, it follows that the whole of the gas in B was absorbed by the fluid while cooling, and again given out by an increase of tem- perature. The gas, when in the act of being discharged, took its course to the locality of the speck at B, and to the bubble A ; but to the bubble A alone when the speck had disap- peared. Upon repeating these observations the cavity burst ; and I have now before me its two halves, forming its upper and its under surface. The portion of" the cavity at A has the same depth as the portion below mno, all the restof the cavity being much shallower. There was a fine doubly refracting crystal at MN, which polarized the blue of the second order; and its outline is still left on the cavity. There was a sort of crystal- line powder disseminated round MN to a considerable di- stance, and the roof of the bubble B, when the roof of the cavity was entire, was always mottled with this powder. In a former paper, I have distinguished vapour cavities from common cavities, by the manner in which the vacuity in the expansible fluid disappears. In the one case, the vacuity gradually enlarges by the degradation, as it were, of its mar- gin, as the fluid passes into vapour ; in the other, the vacuity gradually diminishes till it disappears. I have since found cavities of an intermediate character, in which the vacuity, on the first application of heat, diminishes, and then, when it has contracted to a certain size, it begins to expand ; and its margin becoming thinner and thinner, it finally passes into vapour. in the Cavities of Minerals. 503 3. On the Form and Position of Crystals in the Cavities of Topaz. In a former paper I have described a moveable group of crystals of carbonate of lime, which I discovered in a cavity in quartz from Quebec, containing a fluid with the properties of water. The crystals to which I am about to call attention are of a very different kind, and possess a very different kind of interest. The crystals which occupy the fluid cavities of topaz are either fixed or moveable. Some of the fixed crystals are often beautifully crystallized. They have their axes of double re- fraction coincident with those of the crystal, and, as I have ascertained by the examination of exploded cavities, they ac- tually form part of the solid topaz, though they exist in the fluid cavity. One or two of these are shown in fig. 4, plate 19, of my paper of 1826*, and they may be distinguished by their attachment to the sides of the cavity. In the same figure, as well as in figs, 10, 13, 20, and 21 of my paper of 1823tj I have drawn others which I then believed to be fixed, but which I have no doubt are moveable, and produced from one or other of the new fluids. In re-examining my specimens of topaz, I have been sur- prised at the great number of cavities which contain crystals. In some there are only one; in very many there are two, three, and four; and in a great number of specimens the cavity is so ci*ammed with them, like a purSe full of money, that the circular vacuity has not room to take its natural shape, and often can scarcely be recognised, in its broken-down con- dition, among the jostling crystals. The crystals of which I am treating are sometimes found in the volatile, and sometimes in the dense fluid, but chiefly in the latter. They are often found in an amorphous state in the narrow necks and narrow extremities of cavities, positions in which they remain fixed while they continue solid ; and some- times regularly formed crystals remain fixed between the pris- matic edges of cavities, in consequence of having either fallen into that position, or of having been formed there. The crystals in topaz cavities are, in genei'al, beautifully crystallized, and have a great variety of forms. I have ob- served the following : — 1. The tetrahedron. 2. The cube. 3. The cube, truncated on its edges and angles. 4. The rhombohedron. • Edinburgh Transactions, vol. x. f Ibid, plates 1 and 2. ' 504 Sir David Brewster on the Existence of Crystals 5. The prism, with plain and pyramidal summits. 6. The flat octohedron, truncated on its edges and angles, 7. Rhomboidal plates. 8. Hexagonal plates. 9. Long rectangular plates. Besides these, there are amorphous crystals and crystallized masses of various characters. 4. On the Physical Properties of the Crystals in Topaz Cavities. Although it vk^ould be desirable to submit these crystals, as well as the fluids which contain them, to chemical analysis, yet the task is loo difficult to be accomplished in the present state of chemical science. I must therefore limit my obser- vations to such of the physical properties of these crystals as can be rendered visible to the eye. When I first applied heat to the crystals under considera- tion, I employed a very fine specimen, with large and nume- rous crystallized cavities, ofaprismatical form, containing both the new fluids. In this specimen there wei'e seven cavities unlike all the rest, and each of them containing a single cry- stal, and apparently but one fluid, namely, the dense one. The cavities were exceedingly flat, and irregular in their shape, and very unlike one another. Upon applying the heat of only a lighted paper match beneath the plate of glass on which the specimen lay, I was surprised to see the crystals gradually lose their angles, and then slowly melt, till not a trace of them was visible. In this state one of the cavities had the appear- ance shown in fig. 3, where V was the vacuity, and v^ x/ other two bubbles, one of which v soon joined the principal one V. In all the other six cavities the crystals were speedily repro- duced, always at the point where they disappeai'ed, provided a small speck remained unmelted ; but otherwise in diflferent parts of the cavity. In the cavity AB, however, fig. 3, the crystal was very long in appearing. In the course of an hour, however, a fasciculus of minute crystals appeared in the centre of the vacuity, as in fig. 4, and to them the principal crystal attached itself, as in fig. 5, which exhibits a perfect rhomboidal plate, truncated on its obtuse angles. The elliptical vacuity was pressed into the shape of a heart : and, by the application of ice, I succeeded in precipitating the vapour of the expan- sible fluid, which existed in a very minute quantity in all the seven cavities. The expansible fluid is shown between the two heart-shaped outlines in the figure, and I repeatedly threw it into vapour, and reduced that vapour to a fluid state. The phaenomenon now described, of the melting of the crystals, and their subsequent recrystallization, I have shown to various in the Cavities of Minerals. 505 persons ; and it is very remarkable that they generally reap- pear in this specimen of the same form, though with consi- derable modifications. Upon applying heat to other cavities containing several crystals, I obtained very different results. Some of them melted easily, others with greater difficulty ; and some were not in the slightest degree affected by the most powerful heat I could apply. When the crystals melted easily, they were as quickly reproduced; sometimes reappearing more perfectly formed than before, but frequently running into amorphous and granular crystallizations. In some specimens of topaz all the crystals in the cavities refuse to melt with heat, and seem not to suffer the slightest change in their form. Hence we are entitled to conclude, that the crystals possessing such different properties must be different substances; and this conclusion is amply confirmed by an examination of their optical properties. In making this examination, I used a polarizing microscope, so constructed that the plane, passing through the optical axis of the topaz, could be readily placed either parallel or per- pendicular to the plane of primitive polarization. In this case the field of the microscope is wholly obscure, in so far as the depolarizing action of the plate of topaz is concerned ; but if there is any crystal in the topaz, either imbedded in its mass, or included in its cavities, that crystal will exhibit its doubly refracting structure, if it has any, by its depolarizing action. It may, indeed, happen, — and it does happen, — that the plane passing through their optical axes coincides, either accurately, or so nearly, with that of the topaz, that its depolarizing action is a minimum ; but an experienced observer will have no dif- ficulty in distinguishing this want of depolarization by position, from the v/ant of it by structure. When the specimen of topaz is rich in cavities full of cry- stals, the display of luminous and coloured crystalline forms in the dark field of the microscope, indicating, too, the impri- sonment of fluids, and the condensation of gases before vege- table or animal life had visited our primaeval globe, was as interesting to the imagination and the judgement as it was beautiful to the eye. Having had the privilege of being the first to see it, I felt the full influence of the sight ; and 1 have again and again contemplated it with renewed wonder and delight. When the cavities are so numerous as to mock cal- culation, and so infinitely small as to yield no visible outline to the highest powers, the bright twinkle of a crystalline atom within them reveals to us their nature as well as their contents. In the examination of the individual crystals, many interest- 506 Sir David Brewster on the Existence of Crystals ing facts present themselves to our notice. The crystals of the tessiilar class, which are modifications of the cube, are very numerous, and have no action upon polarized light. Many of them melt easily, while others refuse to yield to the action of heat ; and hence there must be two different sub- stances in the cavities which assume the same shape. In like manner, some of the doubly refracting crystals melt readily, others with very great difficulty, and others not at all ; so that there must be three different substances, which belong to the classes of forms that give double refraction ; a conclusion which is confirmed by the different secondary forms which I have already enumerated. I have seldom found any crystals in these cavities which depolarize white light, or the highest order of colours. I have found some that depolarize ybz/r orders of colours ; and when the crystal which does this is a flat hexagonal plate, it is highly interesting to see it pass through all the tints which these orders include, while slowly melting, and again reproducing them during its recrystallization. In a cavity which was so placed as to be entirely black from the total reflexion of the light which fell upon it, I observed three iiohite openings, a, b, c, of a crystalline form (see fig. 6). These appeared to be fixed crystals, or rather parts of the topaz, surrounded by a cavity. I found, however, that the hexagonal one C depolarized white light, while the rest had no action upon polarized light. Upon applying heat, the crystal c melted, and took up a position at e, fig. 1 5, in a nar- rower part of the cavity, where it remains of an irregular form, having been repeatedly melted and recrystallized. Upon turning the cavity into a position where it became transparent, I found that there was no fluid whatever in the cavity ; so that we have here an example of a crystal melting and recrystal- lizing without having been dissolved in one of the fluids. From the irregular state of the laminae close to this cavity, there is every appearance of the fluids having escaped from one of its extremities. In the course of these observations, I observed a phaeno- menon, produced by heat, of the most novel and surprising kind, and one which 1 feel myself utterly unable to explain. It piesented itself when I was studying the very interesting collection of crystals in the cavity AB, fig. 8. This cavity is filled with the dense fluid, in which there is a vacuity V : the fluid swells to sucli a degree with heat as to diminish very perceptibly the size of this vacuity ; and as I can find no trace of any portion of the volatile fluid, I have no doubt that this vacuity would disappear by an increased degree of heat. The in the Cavities of Minerals. 507 fear, however, of bursting so rare and interesting a cavity, has prevented me from making this experiment. The cavity contains a great number of crystals of different forms, not one of which melts with heat, and almost all of which possess double refraction. When I first submitted this cavity to the microscope, there were Jive small crystals lying between D and the vacuity V; one a flat prism, another a hexagonal plate, a third amorphous, and a fourth and fifth two irregular halves of a hexagon. Upon the first application of heat, one or two of these crystals leapt from their resting place, and darted to the opposite side of the cavity. In a iew seconds the others quitted their places one after another, performing the most rapid and extraordinary rotations. One crystal joined an- other, and, at last, four of them thus united revolved with such rapidity as completely to efface their respective shapes. They then separated on the withdrawal of the heat, and took the position which their gravity assigned them. On another oc- casion, a long flat prism performed the same rotation round its middle point; and I have repeated the experiment so often, in showing it to others, that the small crystals have been driven between the inclined edges of the cavity, from which I cannot extricate them. I have succeeded, however, in conducting a fine octohedral crystal, truncated on its edges and angles, into the arena at D, where I have just seen it perform its rotation, as indicated by the concentric circles on the right-hand of D. In seeking for the cause of so extraordinary a phaenomenon, we are reminded of the rotations of camphor and other vola- tile substances ; but in this case no gas or matter of any kind could be thrown off without becoming visible in the fluid. The pyro-electricity of topaz next suggests itself as a moving power; but though it might produce attractions and repulsions, we cannot see how it could turn a crystal upon its axis. The experiments of Libri and Fresnel, on the repulsions which heated bodies exert upon each other at sensible distances, afford us as little aid. They may enable us to account for the mere displacement of the crystals by the application of heal, or for their sudden start from their places of rest, but they do not supply us with a force fitted to give and to sustain a rapid rotatory movement. I have already had occasion to state, that the cavities often burst when too much heat is applied to the specimen. This generally takes place by a separation of the laminae, which fly off in splinters; but when the burst cavity is large and insulated, a piece of the solid crystal is scooped out on its weakest side. Sometimes a great number of cavities explode at the same time, and when they are small, or exist in a part 508 Sir David Brewster 07i the Existence of Crystals of the crystal where there are no large ones, the explosive force is not strong enough to separate the laminae. The fluid is merely driven between the laminae to a small distance around the cavity, and shows itself as a dark brown powdery matter, encircling the cavity as the burr of a comet does its nucleus. When the cohesion of the laminae is great, it resists the ex- plosive force over a large cavity, and the contents of the cavity are thrown to a considerable distance around it, and remains between the laminas, either as a sort of powder, or as a con- geries of minute crystals, which are sometimes large enough to show their depolarizing action. When the laminae sepa- rate, we find this crystalline matter either fluid or indurated ; exhibiting, when fluid, the extraordinary properties described in my former papers. If we breathe upon the indurated matter it becomes fluid, recrystallizes in new spicule and cry- stals; and, on several occasions, I have found fine examples of circular crystallization. After the explosion of cavities containing only the dense fluid, I have been surprised to find, and that in large cavities, that no trace of matter was left upon the sides of the cavity or around it. Whether this arose, as the fact seems to indicate, from the dense fluid being a condensed gas, or from some other cause, it will require new experiments to determine. In a very remarkable specimen, in which the cleavage plane passed through a great number of large flat cavities, the brown matter has been lodged near to the edges of each cavity, and marks them out even to the unassisted eye. These cavities were filled almost solely with the volatile fluid ; and since the faces of the cavities are corroded as if by the action of a sol- vent, developing crystalline forms, there is reason to think that the fluid has exercised this action, and that the phasnomenon is analogous to that external action, on the faces of hundreds of Brazil topazes in my possession, which I have described in the Cambridge Transactions*, and the singular optical figure formed by which, I have represented in a late volume of the Transactions of this Society f. The only chemical experiment on the contents of these cavities, which I have had occasion recently to make, is per- haps worth reporting. One angle of a cavity was blown off" by its explosion, and though the fluids escaped, a pretty large prismatic crystal remained within the cavity. I introduced water and alcohol successively into the cavity, and raised them to a considerable heat ; but they had no effect in dissolving the crystal. * Vol. ii. plate 1. fig. 16. t Edinburgh Transactions, vol. xiv. plate 10. figs, 1, 2. in the Cavities of Minerals. 509 5. On Solid Crystals and Crystalline Masses imbedded in Topaz. Among the new phaenomena which this section embraces, there is at least one intimately connected with the subject of the fluid cavities. How far the other phaenomena may have any such connexion, it remains to be seen. The imbedded crystals to which I refer, presented them- selves to me while the specimens which contain them were exposed to polarized light. Mineralogists have been long familiar with the beautiful crystals of titanium, imbedded in quartz, and I have found the same mineral imbedded under still more interesting circumstances in the Brazilian amethysts. In topaz, however, the imbedded crystals have never been noticed, and I have fortunately obtained specimens, in which they are displayed with singular beauty. Their axes of double refraction are not coincident with those of the topaz; and hence they are seen in the obscure field of the microscope splendent with all the colours of polarized light. These cry- stals are equally transparent with the topaz, with a ^evt slight exceptions. They sometimes polarize five or six orders of colours ; and, in general, they have very beautiful crystalline forms, which can be seen by the microscope in common light. In some cases they are mere crystalline masses, often of a reniform shape, but still with regular axes of double refraction. In some specimens of Brazil topaz, the crystals occur in branches or groups of singular beauty, consisting of prisms and hexagonal plates, connected apparently by filaments of some opake matter. I have occasionally met with another interesting variety of them, which have no visible outline by common light, and which could never have been detected but by the polarizing microscope. In one of these cases, the crystalline mass, which is nearly spherical, lies in a crowded group of small fluid ca- vities, none of which enters its mass ; a complete proof that the cavities were formed in the soft mass of topaz, when it en- circled the indurated crystal. Along with these interesting phaenomena, another occasion- ally occurs, which may still require a further examination. I have observed apparent doubly refracting crystals, which differ in some essential points from those which have been described. They depolarize a uniform, or nearly a uniform tint, notwith- standing the different thicknesses through which the polarized light passes ; and that tint is less brilliant than in the real im- bedded crystals. I conceive, therefore, that they are crystal- lized cavities, having their inner surfaces coated with a doubly 510 Observations on Chloric Acid and the Chlorates, refracting crust. This is^ in itself, a very natural supposition, seeing that the fluid may have discharged its gaseous portion, and left behind it the matters which it held in solution. The cavities however, of this kind, which I have described in a former paper, have no depolarizing action ; and I find that those now under consideration have regular axes of double refraction. Hence the matter which covers them must be a regular crystalline shell, with optical and crystallographic axes — a phaenomenon which has no parallel in mineralogy. St. Leonard's College, St. Andrew's, February 15, 1845. LXXIV. Observations on Chloric Acid and the Chlorates. By Lewis Thompson. To the Editors of the Philosophical Magazine and Journal. Gentlemen, A N easy and oeconomical mode of preparing chloric acid -^^*- and some of the chlorates has not been described in any chemical work that I am aware of: the following will be fonnd to answer extremely well. Dissolve in two separate portions of boiling water one atom (122-81) of chlorate of potash, and one atom (168-34) of bi- tartrate of ammonia; mix the two solutions together, and set the whole aside in order that the bitartrate of potash may crystallize; then mix the clear solution with an equal bulk of alcohol, and filter or pour off the alcoholic solution of chlorate of ammonia, which must now be boiled in a flask or other narrow-necked vessel, with an excess of recently-precipitated carbonate of baryta, until the ammonia is expelled, water being occasionally added ; then filter the fluid, evaporate, and cry- stallize. In dissolving the chlorate of potash and bitartrate of ammonia, as little water must be used as possible. The chlorates of strontla and lime may be prepared in a similar manner; and the metallic chlorates are easily prepared by decomposing the chlorate of baryta by means of asulphatef of the base required. Chloric acid is best obtained by dissolving a given weight of chlorate of baryta, and adding no more sulphuric acid than is sufficient to combine with the base ; several hours or eveif days, however, appear necessary to effect this decomposition in the cold ; after which the whole may be filtered and care- fully evaporated at a low heat. When sulphuric acid is added to a solution of the chlorate of baryta, as long as it gives ^ precipitate, I have always found an excess of it in the chloric acid. Sir W. Rowan Hamilton on Qtiaternions* 511 The bitartrate of ammonia may be readily made by dissol- ving tartaric acid in water, saturating one-lialf of the solution with ammonia or its carbonate, and adding to this the remain- ing half of the liquid tartaric acid; the bitartrate of ammonia immediately precipitates. For pyrotechnical purposes, the chlorates of baryta, stron- tia, lead, &c. may be made without alcohol. With combus- tibles containing hydrogen, the chlorate of baryta produces a green flame of surpassing brilliancy ; and the chlorate of strontia, although somewhat deliquescent, is much superior as a crimson to the nitrate of that earth. I am, Gentlemen, Your most obedient Servant, Byker Bar, Newcastle-on-Tyne, Lewis Thompson. October 14, 1847. LXXV. On Qiiaternions ; or on a New Si/stem of Imag manes in Algebra. By Sir William Rowan Hamilton, LL.D.^ V. P.R.I. A., F.R.A.S., Corresponding Member of the In sti' tute of France^ S^c., Ajidrews' Professor of Astronomy in the University of Dublin j a?id Royal Astronomer of Ireland. ■[Continued from p. 293.] 51. TT has been shown* that if the two symbols «, x denote J- certain constant vectors, perpendicular to the two cyclic planes of an ellipsoid, and if v, t denote two other and variable vectors, of which the former is normal to the ellipsoid at any proposed point upon its surface, while the latter is tan- gential to a line of curvature at that poin^, then the directions of these four vectors », x, v, t are so related to each other as to satisfy the condition f S . VT»Tx = 0 (49.), article 47 ; S being the characteristic of the operation of taking the scalar part of a quaternion. And because the two latter of these four directions, namely the directions of the normal and tan- gential vectors v and t, are always perpendicular to each other, this additional equation has been seen to hold good : S.vT=0 (36.), article 45. Retaining the same significations of the symbols, and carrying forward for convenience the recent numbering of the formulae, * See the Philosopliical Magazine for October 1847; or Proceedings of the Royal Irish Academy for July 1846. t Inadvertently transcribed as S . vtikt^O, towards the end of the last communication to this Magazine: but correctly printed in the formula (49.) here referred to. 512 Sir W. Rowan Hamilton on Quaierm'ons. it is now proposed to point out some of the modes of combining, transforming, and interpreting the system of these two equa- tions, consistently with the principles and rules of the Calculus of Quaternions, from which the equations themselves have been derived. 52. Whatever two vectors may be denoted by t and t, the ternary product tit is always a vector forrn^ because (by article 20) its scalar part is zero ; and on the other hand the square t^ is a pure scalar : therefore we may always write T*T = /AT% Ti = |XT, (52.) where jw. is a new vector, expressible in terms of » and t as follows : H* = Te of *', x', and t) are now parallel to one common plane, namely to the plane which touches the ellipsoid at the proposed point, and to which the fourth direction (that of v) is perpendicular. Decomposing the two quaternion products, t*' and tx', into their respective scalar and vector parts, by the general formulae, Tl'=S.Tl' + V.T*'; TX'=S.TX' + V.TX' and observing that the vectors V. n' and V. tx' both represent lines parallel to v, because v is perpendicular to the common plane of t, »', x'; so that the three following binary pi'oducts, V.Tj'.V. tx', vV. t«', vV. tx', are in the present question scalars ; we find that we may write S.vt«'tx' = vS.t/.V.tx' + vV.t.'.S.tx'. . . (71.) Hence the equation (69.) or (49.) reduces itself, after being multiplied by v~', to the form S.t/.V.tx' + V.t.'.S.tx'=0; .... (72.) which gives, in general, by the rules of the present calculus, V.t'T_V.Tx' sT?7-"sr;v' ^^^'> and by another transformation, V.i't-1 _ V.x't-' , ^ [s:?F^-~s:^?^' (^^•) which may perhaps be not inconveniently written also thus : V i' _ V x' S"'f"'"S*7' C^^') in using which abridged notation, we must be careful to re- V member, respecting the characteristic ^, of which the effect is to form or to denote the quotient of the vector 'part divided by the scalar part of any quaternion expression to which it is prefixed, that this Jiew characteristic of operation is not (like S and V themselves) distributive relatively to the operand. The vector denoted by the first member of (74.) or of (75.) is a line perpendicular to the plane of *' and t, that is to the tangent 618 Sir W. Rowan Hamilton on Quaternions, plane of the ellipsoid ; and its length is the trigonometric tangent of the angle of rotation in that plane from the direction of the line t to that of the line »'; while a similar interpretation applies to the second member of either of the same two equa- tions, the sign — in that second member signifying here that the two equally long angular motions, or rotations, from t to i', and from t to x', are performed in opposite directions. Thus the vector t, which touches a line of curvature, coincides in direction with the bisector of the angle in the tangent plane between the projections, i' and x', of the cyclic normals there- upon ; or with that other line, at right angles to this last bi- sector, which bisects in like manner the other and supplemen- tary angle in the same tangent plane, between the directions of »' and — x' : since x' may be changed to — x', without alter- ing essentially any one of the four last equations between t, *', x'. Those two rectangular and known directions of the tangents to the lines of curvature at any point of an ellipsoid, which were obtained by the process of article 53^ are therefore ob- tained also by the process of the present article ; which con- ducts, by the help of the geometrical reasoning above indicated, to the following expression for the system of those two tan- gents T, as the symbolical solution (in the language of the pre- sent calculus) of any one of the four last equations (72.),. .(75.): t=j!'(U.'±Ux'); (76.) where t' is a scalar coefficient. The agreement of this symbolical result with that marked (62.) may be made evident by observing that the equations (68.) give ,' = v-iV.v»; x' = v-iV.vx; . .-. . (77.) so that if we establish, as we may, the relation ^^'=(Tv)-S (78.) between the arbitrary scalar coefficients t and t', which enter into the formulae (62.) and (76.), those formulae will coincide with each other. And to show, without introducing geome- trical considerations^ that (for example) the form (73.) of the recent condition relatively to t is symbolically satisfied by the expression (76.), we may remark that this expression, when operated upon according to the general rules of this calculus, gives Tx'.V./t=±/'V..'x'; Tx'.S.i'T=^'(-T.i'x'±S..'x');'l ,^^ ^ Ti'.V.Tx'=/'V.i'x'; Ti'.S.Tx'=^'(S..'x' + T.i'x'); J '' and that therefore the two members of (73.) do in fact receive. On the Chemical History of Gun-Cotton and Xyloidine. 519 in virtue of (76.), one common symbolical ralue, namely one or other of the two which are included in the ambiguous form v.»y S.»'x' + T..'x'' ^^^'' respecting which form it may not be useless to remark that the product of its two values is unity. [To be continued.] LXXVI. Contributions to the Chemical History ofGun-Cotton and Xyloidine. By Mr. John Hall Gladstone, of Uni- versity College, London^. A T the commencement of the present year, having perceived -^^ that considerable doubt rested on the ultimate composi- tion of gun-cotton, I undertook a series of experiments with a view to ascertain it, if possible ; and during my investiga- tion my attention was drawn to various papers that appeared on the subject, where I found contradictory accounts, not only of the results of analysis, but also of the action of va- rious reputed solvents. The experiments detailed below, although they are far from exhausting the subject, may serve to explain some of these anomalies, and to point out a few facts, which, as far as I have been able to learn, have not been hitherto noticed. The cotton employed was that used by jewellers, well- carded, perfectly white, and free from imperfections. An analysis of the substance by combustion with oxide of copper in a stream of oxygen yielded the following results : — Cotton employed 3*16 grs. Carbonic acid produced . , . 5*14 ... Water produced 2*06 ... These proportions are, — Carbon . . . 44-37 Hydrogen . . 7*24 Oxygen . . . 48-39 100-00 Lignine calculated from the formula C24 H20 Ogo •' — Carbon . . . 44-44 Hydrogen . . 6-17 Oxygen . . . 49-39 100-00 The excess of hydrogen doubtless arises from moisture absorbed by the oxide of copper during the unavoidable delay in mixing it with the cotton. * Communicated by the Chemical Society; having been read June 7> 1847. 520 Mr. Gladstone on the This cotton, which may be considered as pure lignine, was steeped until thoroughly wetted in a mixture of nitric acid of spec. grav. 1*502, and nearly an equal bulk of strong sul- phuric acid, then well-washed with water, and dried at a temperature not exceeding 212°. In one instance 38*38 grs. of cotton became 66*84 grs,, being an increase'of 28*46 grs., or 74*15 per cent. In a second experiment 59*3 grs. of cot- ton gave an increase of 43*7 gi^s., or 73*7 per cent. The gun- cotton, or pyroxyline, thus produced resembled the original cotton in physical properties very closely, and exploded at about 370°, producing no smoke and leaving no residue. The action of various solvents and reagents upon this sub- stance was found to be as follows : — It is absolutely insoluble in pure water, and nearly so in strong alcohol, aether, m hether hydrated or anhydrous, and in a mixture of aether with y'^th part of alcohol ; but acetic aether instantly destroys its fibre, and dissolves it in large quantity. The solution yields on spontaneous evaporation a white powder of the same weight as the original pyroxyline, but I have found it very difficult to drive off the last traces of the solvent. The action of sul- phuric acid upon it differs from that exerted upon unaltered cotton ; for, while the latter is instantly dissolved by the strong acid, and charred upon a slight elevation of tempera- ture, pyroxyline dissolves with difficulty unless the acid be warmed, evolving at the same time nitric oxide and other gases, and not being charred even upon boiling. With the aid of heat it dissolves immediately in a solution of potash. By means of these three last-mentioned tests I was able to prove the absence of any unaltered cotton in the product under examination. The action of other reagents upon gun- cotton was not so decided ; it was dissolved, but not without long boiling, by ammonia, the alkaline carbonates, hydro- chloric acid, acetic acid, both glacial and dilute, and weak sulphuric acid. These solutions, as well as the two preceding, contained nitric acid; nothing could be precipitated from them by dilution or neutralization; and when evaporated they yielded only a dark brown amorphous matter. It is evident that none of these reagents restore the lignine in its original condition; and they do not afford any means of ascertaining whether the compound contains the elements of nitric or hyponitric acid. As there exists a great discrepancy in the accounts given of the increase of weight in making gun-cotton, I examined whether the length of time it was immersed in the acid liquor, or the proportions of the acids employed, were the cause. The length of immersion 1 found to produce no alteration ; but Chemical History of Gun-Cotton and Xyloidine. 521 upon employing two measures of sulphuric acid to one of nitric acid, 1 obtained a product resembling in all respects ordinary pyroxyline, yet 42*77 grs. gave an increase of only 24-31 grs., or 56*84 per cent. Upon a repetition of this ex- periment I found the increase to be 59*93 per cent., and again 70*6 per cent. Suspecting from the disparity of these results that something might be dissolved in the acid liquor, I im- mersed 6*7 grs. of cotton in a large quantity of the mixed acids, but it increased 4*9 grs., or 73*1 per cent. Perceiving that I had obtained an opposite effect to that anticipated, I treated 12*64 grs. of cotton with just sufficient of the mixture to wet it thoroughly : the fibre was evidently somewhat de- stroyed ; the increase in weight was only 6*54 grs., or 51 '74 per cent., and the acid liquor squeezed from the cotton, neu- tralized with ammonia, evaporated to dryness, and heated, gave abundant evidence of organic matter being present. Lest however it might be supposed that the whole had not been converted into pyroxyline, it was treated again with the mixed acids, but that produced an increase of only 0*12 gr. The action of various solvents confirmed its identity with ordinary pyroxyline, while its solubility in potash proved that the transformation had been very nearly complete. A repetition of the experiment gave similar results. It thus appears that the small increase in weight in the preparation of pyroxyline takes place when there is not sufficient nitric acid present to prevent the peculiar action of the sulphuric acid, namely, that of dissolving and altering it. When how- ever the increase amounted to about 74 per cent., I was never able to detect the presence of oxalic acid or other organic matter in the acid liquor ; and as no gas is evolved during the'preparation of pyroxyline, it may be concluded that there is no secondary product containing carbon. Subsequently, when Dr. Schcinbein had specified his me- thod of making gun-cotton, I treated 18*78 grs. of cotton with a mixture of three parts of sulphuric acid and one of nitric acid, sp, gr. 1*5, following his directions. The result was 32*92 grs. of a substance similar to that produced in former experiments, being an increase of 75*20 per cent. On another occasion SO* 95 grs. of cotton gave an increase of 61*10 grs., or 75*47 per cent. The action of solvents and re- agents confirmed the identity of this pyroxyline with that obtained in my previous experiments, and I was equally able to establish the absence of any secondary product containing carbon. In determining the ultimate composition of pyroxyline several precautions were found to be necessary. In the ana- 522 Mr. Gladstone on the lyses recorded below it was cut into small pieces, and, after the weight was taken, mixed carefully with oxide of copper. To prevent its caking together the admixture of a little as- bestos was found useful. This was introduced into a long combustion-tube, then some fresh oxide of copper, and upon it again some fused into lumps so as to fill the whole bore for about 7 inches. Lastly, was added a mixture of copper turn- ings and reduced copper for about 9 inches. The combus- tion conducted cautiously in the usual manner gave the fol- lowing results ; the pyroxyline burnt in the sixth experi- ment having been prepared by Schbnbein's method. I. II. III. IV. V. VI. Pyroxyline employed 4-09 4-61 3*57 4-85 4-55 2-905 Carb. acid produced 4*20 4-52 3*42 4*88 ... 2-84 Water produced . . 1-19 1*36 1*34 0-87 Hence in 100 parts, — I. II. III. IV. V. VI. Carbon . 27*90 26*74 26-10 27*44 ... 26-65 Hydrogen 3*22 3*27 3*27 3*32 In order to determine the amount of nitrogen the differ- ential mode was adopted, as the method of MM. Will and Varrentrapp is inapplicable to substances containing this element in so highly oxidized a state. The same precautions were taken as in the estimation of carbon ; and the collected gases gave the following results after due correction for baro- metrical pressure : — I. II. Another specimen. Carbonic acid . 25-0 38*5 23-9 Nitrogen ... 5*5 8-5 5*1 These proportions are, — Nitrogen. 1 Carbonic acid. 4-55 1 4-53 1 4-68 The volumes of the gases represent respectively equivalents of carbon and nitrogen, and since no secondary product is formed in the conversion of lignine into pyroxyline, the 24 equivalents of carbon in the former must be found in the latter. This will give the following ratio in equivalents of carbon and nitrogen according to the three experiments above cited : — I. II. III. Carbon .... 24-0 24*0 24-0 Nitrogen . . . 5*28 5-3 5'12 Chemical History of Gun-Cotton and Xyloidine. 523L or 24 : 5, which accords with the proportions assigned by M. Pelouze *. The formula which best agrees with these results is the following : — C24 -I ctuq f^^i which reckoned to 100 parts^ gives — Carbon 26*23 Hydrogen 2*73 Nitrogen 12-75 Oxygen 58*29 In order to compare pyroxyline with xyloidine, I treated starch with fuming nitric acid until the whole was converted into a gelatinous mass. The addition of water then threw down a white powder, which was subsequently well-washed and dried. The iodine test proved the absence of all unal- tered starch. The xyloidine thus obtained explodes at about 360°, leaving a carbonaceous residue. It is slightly soluble in aether, with which it is capable of forming a peculiar com- pound not yet investigated ; more so in alcohol, but most of all in aether mixed with a small proportion of alcohol, or in acetic aether. It is dissolved by strong sulphuric acid with- out the aid of heat, and by boiling solutions of potash, am- monia, hydrochloric acid and dilute sulphuric acid. These solutions contain nitric acid, and nothing is precipitated from them by dilution or neutralization. Xyloidine is also soluble in strong acetic acid, or in nitric acid, whether fuming or of sp. gr. 1*25, but is reprecipitated from either by dilu- tion. It was also found that nitric acid of ordinary strength (sp. gr. 1*45) answered equally well in the preparation of this substance ; but when acid of sp. gr. 1*41 was employed no such result was obtained. Starch treated with a mixture of equal measures of nitric and sulphuric acids produced a sub- stance of greater combustibility, and more closely resembling pyroxyline, but differing from it in being soluble in glacial acetic acid, and in a mixture of aether with one-tenth part of alcohol, as also in the action that acetic aether exerts upon it, Xyloidine also when subjected to the mixed acids gave a pro- duct identical with the above, as far at least as the action of solvents can prove. Xyloidine burnt by means of oxide of copper, with the usual precautions, gave the following results. The sub- stance employed in the third experiment was made from arrow-root. * Compttt Rendus, Jan. 4. II. III. 24-0 24-0 3-10 3-57 524 Mr. Gladstone on the I. II. III. Xyloidine employed . . 4' 7 7 5*23 6*75 Carbonic acid produced . 5*30 5*91 7*87 Water produced . . . 1-84 1*96 2-80 Hence in 100 parts, — I. II. III. Carbon . . 30-30 30*82 31-79 Hydrogen . 4-28 4-16 4*60 In the determination of nitrogen by the differential method the proportions of the gases obtained were, — I. II. III. Carbonic acid . 70-7 53-4 53-8 Nitrogen . . . 10*6 6*9 8-0 These are in the proportion of — I. Carbon . . 24-0 Nitrogen . . 3*59 These numbers suggest the simple substitution product {HI 3 NO I ^20' ^"^ which the per-centage of carbon would be 31-37, and of hydrogen 3*70 ; yet the amount of nitrogen is somewhat too great, and there is far from being sufficient evidence to prove the definiteness of the substance itself. The Avide difference also in the results obtained by various chemists can scarcely be accounted for, except upon the sup- position that they have operated upon very different sub- stances. The solubility of xyloidine in nitric acid led me to examine whether any alteration could be effected upon pyroxyline by similar means. The most dilute acid which I found to have any effect upon it in the cold was that of sp. gr. 1*414 ; but the alteration took place by means of this only after long standing, and but to a slight extent. Nitric acid of sp. gr. 1*45 how- ever is capable of dissolving pyroxyline, and alters both its composition and properties, as will be presently de- scribed ; whilst fuming nitric acid has not the slightest effect upon it. The new product just mentioned is acted upon somewhat differently by various solvents, according to whe- ther it exists in a fibrous condition, or in powder as precipi- tated from solution ; yet I have found by experiment that no alteration in weight is effected by this change of condition. When in fibre it is slightly soluble in strong alcohol, aether, a mixture of aether with one-tenth part of alcohol, and acetic aether ; but when in the pulverulent state it is very soluble in these menstrua, and in glacial acetic acid. In either con- Chemical History of Gun-Cotton and Xyloidine. 525 dition it leaves a carbonaceous residue on combustion, is dissolved by nitric acid, whether of sp. gr. 1'25 or 1*5, and reprecipitated upon dilution. Strong sulphuric acid also dissolves it in the cold, and chars it at a temperature below 180°. These two last properties show that the original pyr- oxyline was perfectly free from admixture with this new sub- stance. There occurs a considerable decrease of weight through this transformation. In the first experiment 32 grs. of sub- stance operated upon gave 25*82 grs. of the new product; in the second 43*64 grs. of the one yielded 34*68 of the other. Now assuming the increase in the preparation of pyroxyline to be 75 per cent., the weight of the new product above that of the original cotton would be, as calculated from these figures, 41*1 and 39*05 per cent. When this new product, whether in the fibrous or the pul- verulent condition, was treated with a mixture of equal parts of nitric and sulphuric acids, it increased considerably in weight, and the resulting substance had all the properties of pyroxyline as prepared in the usual manner, 11*16 grs. of the one yielded 13*56 grs. of the other ; the quantity that should theoretically have been obtained, calculating it from the decrease in making the new product, is 13*84 or 14*04 grs. Again, 12*35 grs. of the substance as precipitated from solution gave 15*75 grs., the theoretical amount would have been 15*31 or 15*54 grs. This result proves the distinct- ness of the new product from xyloidine, a fact that could not have been ascertained from the action of the before-mentioned solvents. Whilst engaged in obtaining these results, I also examined the action of nitric acid of various degrees of strength upon pure cotton. By treating it with nitric acid of sp. gr. 1*5 I obtained a product evidently different from gun-cotton, but as it did not appear to be homogeneous throughout, I passed on to investigate the action of a weaker acid. That of sp. gr. 1*45 gave a substance which proved to be identical with the product of the action of the same acid upon pyroxyline. Upon a repetition of the experiment 68*54 grs. increased in weight 14*61 grs., or 21*31 per cent. — a smaller increase than might have been anticipated, but which may easily be accounted for by the fact that the whole cotton had not been transformed, as was proved by a considerable portion being left undissolved by a boiling solution of potash. Nitric acid ofsp.gr. 1*414 produced the same alteration, but only to a small extent, and after long standing. 23*75 grs. of cotton soaked in nitric acid of sp. gr. 1*516 became a hard mass. 526 Mr. Gladstone on the and increased in weight 13-49 grs., or 56-8 per cent. ; the action of various solvents upon the resulting substance indi- cated that it was a mixture of pyroxyline and the new pro- duct. On another occasion, when the transformation by means of nitric acidsp. gr. 1-47 proved to be complete, 29-52 grs. of cotton increased 9-51 grs., or 32-89 per cent. But in order to obtain a substance sufficiently pure for analysis 16-29 grs. of cotton were treated with enough nitric acid to dissolve the whole ; the new product was precipitated by dilution, and the increase in \veight was found to be 5-34 grs., or 32*78 per cent. In these instances there occurred a secondary product containing carbon not precipitable by water. When this was subjected to combustion with oxide of copper, the following results were obtained : — I. II. Another specimen. Substance employed . 3-15 2*985 3*165 Carbonic acid produced 3-58 3-39 3'55 Water produced . . . 1-00 1-01 1*14 Hence in 100 parts, — Carbon . 30*99 30*97 30*59 Hydrogen 3*52 3*75 4*00 I was unable to obtain any very accurate estimation of ni- trogen by the differential method : the results most to be depended upon were — Carbonic acid . 120*7 76-7 Nitrogen . . . 13*6 8*3 In the proportion of Carbon . . . 24*0 24*0 Nitrogen . . . 2*7 2*6 These numbers lead me to think that there are 3 equiva- lents of nitrogen in the compound, especially as I observed during the combustion that the substance became charred even 1 or 2 inches beyond the glowing charcoal, which will account for the deficiency of nitrogen when compared with the carbonic acid. Hence the composition of the new pro- duct coincides very nearly with that calculated from the formula C24 \^'^q \^2q^ namely. Carbon . . . . 31-37 Hydrogen . . 3*70 Nitrogen . . . . 9-15 Oxygen . . . . 55-78 10000 Chemical History of Gun-Cotton and Xyloidine. 527 Under this supposition the increase in weight in the pre- paration would be 4r66 per cent. ; very similar to that cal- culated from the results obtained by the action of nitric acid, sp. gr. 1'45, on pyroxyline, namely, 3905 and 4ri per cent. In order to add an additional proof of the identity of the two substances obtained by the action of nitric acid of sp. gr. 1*45 on cotton and on pyroxyline, and also of the fact that pyroxyline is reproduced by the action of mixed sulphuric and nitric acids upon the new product, the experiment was re- peated with a portion of the substance made from pure cotton : the result was pyroxyline. In the transformation 26*56 grs. became 38'04 : now these 26*56 grs. were produced from 21*81 grs. of the original cotton ; hence the increase upon the cotton itself would be 16*23 grs., or 74*4 per cent., coinciding with the amount usually obtained in the preparation of pyr- oxyline. I. From these results it appears that in the treatment of woody fibre by nitric acid raised to its highest degree of strength by the addition of sulphuric acid, 5 equivalents of the acid combine with 1 of lignine to produce pyroxyline, displacing 5 equivalents of the elements of water, as indicated by the formula C24S c-vf/^ fOao* The amount per cent, of carbon and hydrogen hence deduced closely agrees also with that assigned by Mr. Ransome * and M. Pettenkofer f. Calculated. Ransome. Pettenkofer. Carbon . . 26*23 26*28 26*26 Hydrogen . 2*73 3*16 2*75 In this case the synthetical experiment would give an in- crease of 69*44 per cent. — nearly the amount obtained in the best experiments. My own analyses however have yielded a somewhat larger amount of carbon. II. If lignine be treated with nitric acid combined with more than 1 equivalent of water, another compound is pro- duced, containing a smaller proportion of the elements of nitric acid, most probably C34 < „ ^q > 0<^^ and very closely resembling, but not identical with, pyroxyline. C24H,oO^ + 3(NO„2HO) = C^|f^7^Jo,o + 9HO. Also if pyroxyline itself be treated with nitric acid con- taining 3 equivalents of water, the same compound results : * Phil. Mag., January ] 847. \ Pharmaceutisches Central BlattfTiec.ZOi^lS'lQ, 528 Royal Astronomical Society. ^2^{5N04}^=><'+2(N05, 3H0) = Cs^l J^jj'oj0jo+4(N05, HO). And this transformation may be reversed. Whilst completing my examination of this substance, my attention M^as drawn to the communication of M. Payen in the Comptes Rendus of Jan. 25th, where some properties of " coton hypoazotique " are described. It is possibly the same; yet, in order to express its distinctness from pyr- oxyline, I would propose as the appellation of my substance cotton-xyloidine. " Before concluding I would acknowledge my obligations to several chemists whose published investigations on the same subject have suggested many of my experiments, and more particularly to Professor Fownes for the valuable advice with which from time to time he has favoured me. LXXVII. Proceedings of Learned Societies. ROYAL ASTRONOMICAL SOCIETY. [Continued from p. 389.] June 11, /^N the Opinion of Copernicus with respect to the 1847. ^^ Light of the Planets. By Professor De Morgan. The common story is, that Copernicus, on being opposed by the argument that Mercury and Venus did not show phases, answered that the phases would be discovered some day. The first place in which I find this story is in Keill's Lectures, It is also given by Dr. Smith, in his well-known Treatise on Optics, by BaiUi, and by others. But I cannot find it mentioned either by Melchior Adam or Gassendil, in their biographies of Copernicus ; nor by Rheticus, in his celebrated Narratio, descriptive of the system of Copernicus ; nor by Kepler, nor by Riccioli, in their collections of arguments for and against the heliocentric theory ; nor by Galileo, when announcing ^and commenting on the discovery of the phases ; and, what is most to the purpose, Miiler, in his excellent edition of the great work of Copernicus, when referring to the discovery of the phases of Venus, as made since, and unknown to, Copernicus, does not say a word on any prediction or opinion of the latter. This story may then be rejected, as the gossip of a time posterior to Copernicus. If we try to examine what the opinion of Copernicus on this matter really was, a point of some little curiosity arises. It depends on one word, whether he did or did not assert his belief in one or other of these two opinions, — that the planets shine by their own light, or that they are saturated by the solar light, which, as it were, soaks through them. I support the affirmative : that is to say, I hold it sufficiently certain that Copernicus did express him- self to the effect that one or the other of these suppositions was the truth. If we take the first edition of the work Z)e Revolutionibus, which Royal Astronomical Society. 529 was printed from the manuscript furnished by Copernicus himself, there is little doubt about the matter. There are but two passages which bear or can bear upon the question. The first is in the ad lectorem, in which the writer (Osiander, though even Delambre make him Copernicus) asks whether any one acquainted with geometry or optics can receive the Ptolemaic epicycle then used to explain the motion in longitude of Venus ? But the meaning of the allusion to optics is explained in the next sentence, by a reference (and by no means a fortunate one) to the changes of apparent diameter of Venus derived from that epicycle ; changes which, as they made the peri- gean diameter more than four times as great as the apogean, were assured to be falsified by common experience. The second passage is the one on which this discussion must turn. In book i. chap, x., after noting that some had theretofore believed Mercury and Venus to come between the earth and sun, he mentions the difficulty arising from the absence of the remarkable phase, which we now call the transit over the sun's disc. He describes the opinion just mentioned favourably, referring, not to his own view, but to that of those others who had held it. This is not an uncommon idiom : persons advocating an unpopular opinion are very apt to describe the main- tainers of it in the third person, though themselves be of the number. But when he comes to describe what he takes to be the necessary consequence of the opinion, he lapses into the first person as fol- lows : — " Non ergo fatemur in stellis opacitatem esse aliquam lunari similem, sed vel proprio lumine, vel solari totis imbutas corporibus fulgere, et idcirco solem non impediri " These are the words of the first edition (Nuremberg, 1543)* That Copernicus could have answered any objection, either by word or writing, is impossible, since he drew his last breath within a few hours of the time when, not able to open it from weakness, he saw the first printed copy. The second edition (Basle, 1566) is usually said to have been edited by Rheticus. The reason of this is that the name of Rheticus appears in the title-page. But this appearance only arises from the Narratio, &c. of Rheticus being added to the edition ; and it is only the description of this edition which brings Rheticus into the title-page. There is no mark whatever of his having been the editor ; and as the work was printed at Basle, where I cannot find that Rheticus ever sojourned, and as the latter was deeply engaged at the time in his enormous trigonometrical calcu- lation, some proof of his editorship must be given before it is ad- mitted. As the point is of importance, I will notice, that unless Rheticus had made some stay at Basle, it is very unlikely he should have edited a work printed there. He did not edite the first edition, only because it was found convenient to print it at Nuremberg in- stead of at Wittemberg ; and it was accordingly entrusted to Osiander. Now, if ever there were a connexion between two men, and between one of them and the book of the other, which made it desirable and even necessary that the first should edite the second, it was the case of Rheticus and the first editio.n of the De Revolutionibus, &c. ; and yet no arrangement could be made by which the sheets printed at Phil. Mag, S. 3. No. 21 1 . Suppl. Vol. 3 1 . 2 M 630 Royal Astronomical Society. Nuremberg could be revised at Wittemberg. It is very unlikely, then, that Rheticus should have edited the second edition, when, as far as we know, a similar impediment existed. The third edition, by MUler (Amsterdam, 1617), has no authority as to the text above that of the second. Now both the second and third editions change the wox6^ fatemur into fatentur, thus causing Copernicus to throw the opinion in question upon his predecessors, instead of directly making it his own. Not that it would be conclusive, even if the emendation were adopted : for, as I have said, Copernicus is evidently speaking with approbation of the opinions which he describes ; and it would be difficult to say why comperiunt or putant in one sentence should imply approbation, and fatentur, in the next, should be at least dis- avowal, if not disapprobation. If Rheticus, who knew the mind of Copernicus better than any one, had been the editor, I can conceive that stress ought to be laid upon the change of the first into the third person as an emendation ; that is, I should be somewhat stag- gered by Rheticus having thought it necessary to make such an alteration. But, Rheticus not being in the question, as I think, for the rea- sons given above, the next best authority on an opinion of Coper- nicus is Galileo. Now the latter, in speaking of the phases of Venus, expressly attributes to Copernicus the maintenance of one of the two alternatives, — that the planet is either self-luminous or perfo- rated by the solar rays. Of these alternatives, he says, in his letter to Velser (Works, vol. ii. pp. 88, 89), " Al Copernico medesimo convien amettere come possibile, anzi pur come necessaria una delle dette posizioni." And that such was the opinion of Copernicus is also assumed by the writer of the note on the Sydereus Nuncius in the volume just mentioned, and by others, even down to our own time ; as by Mr. Drinkwater Bethune, in his life of Galileo. In fact, with the exception of the unsupported story mentioned at the be- ginning of this paper, there is nowhere, that I can find, anything against my conclusion. And it is to be remembered, that Copernicus nowhere shows any of that acumen in matters of phj^sics, apart from mathematics, which has often enabled the cultivators of the former to make steps more than proportionate to their knowledge of the latter. Ptolemy, the great promoter of the old theory, and Coper- nicus, its destroyer, were both mathematicians in a peculiar sense ; Ptolemy being far the more sagacious in questions of pure experi- ment. Their grounds of confidence are mathematical ; and Coper* nicus, in particular, dares to face his own physics (for there is no reason to suppose he was beyond his age in mechanical philosophy) with reasons drawn entirely from probabilities afforded by mathe- matics. There is much reason to regret the practice of associating with the names of those who have led the way in great discovery the glory which is due to their followers. The disadvantage is twofold. In the first place, it introduces into the history of science an index error of from one to two centuries ; secondly, those who come to in- Royal Astronomical Society. 531 quire are disappointed to find that they must lower their opinion of great men, and are perhaps led to do it to a greater extent than jus- tice requires. Our usual popular treatises speak of Copernicus as if, besides himself, he had in him no inconsiderable fraction of Kepler, Galileo, Newton and Halley. What is a person to think who comes from those histories to actual investigation, when he finds in Coper- nicus himself the immovable centrum mundi (only reading sun for earth) of the Ptolemaists, their epicycles, and a suspicion, at least, of the solid orbs ? On the Formation and Application of Fine Metallic "Wires to Optical Instruments. By Mr. Ulrich. Dr. WoUaston, in the Philosophical Transactions for 1813, pro- posed a method of forming wires of gold or platinum of any degree of tenuity. The discovery does not appear to have been much used, owing, as Mr. Ulrich supposes, to the difficulty of application. Mr. Ulrich forms the fine wire by inserting a gold or platinum wire in the centre of a silver cylinder of much larger dimensions, which is afterwards drawn out by the usual process. When the silver wire has been sufficiently extended, Mr. Ulrich cuts it into short lengths and attaches platinS. rings to each end. The rings are hooked upon a hooked fork, and the whole is plunged into heated nitric acid, when the silver coating is dissolved. The artist may now wire his cell according to his fancy. Mr. Ulrich's plan seems to be, to hold one end by an overplate ; then to allow the wire to be stretched by its platina ring, and to fix the other oveqjlate. He recommends using a cell of the same material as the wire, as, otherwise, a difference of expansion might break or slacken the w^ires. On the properties of Rock as a foundation of the Piers of Meridian Instruments, with an Account of the Detection of a hitherto un- suspected Cause of Error in the Edinburgh Transit. By Professor C. P. Smyth. Some years ago doubts were expressed of the fitness of a rock foundation for an observatory. It does not appear that any experi- ments were made, or that any reason was adduced beyond this, that as tremor was unfavourable to the performance of large telescopes, and as rock was more capable of transmitting tremors than less compact material, therefore rock was to be avoided when choosing a site for an observatory. The author or authors of this opinion were pro- bably but ill- acquainted with the mode of working an observatory, or the requisites for obtaining accuracy in meridian observations ; yet it is certain that an undue importance was attached in some cases to these very idle surmises. At the present time it is not likely that any intelligent person would be misled by such authorities, and it is therefore unnecessary to mention here the mischief they have caused *. It is to be wished that the founders of future observatories, * The effect of tremor on a telescope is probably familiar to every read- er of tfiis notice. It causes a sort of burr round the object, and destroys the sharpness of outline and definition. This is probably more injurious in reflecting than in refracting telescopes ; but we may fairly doubt whether it 2 M2 532 Royal Astronomical Society, •who can command a rock foundation, should make use of their good fortune ; and that those who cannot, would look carefully to the possible effects of moisture, which are probably more extensive, and vary more rapidly, than those of temperature. The observatory of Edinburgh is placed on the Calton Hill. This is chiefly of a porphyritic formation. The apex w^as blasted away to obtain a level area, on which the observatory was erected. The site of each pier was cut away until a sound part of the rock was arrived at (it was not necessary to go deeper for this purpose than six or nine inches), when the exact size of the foundation was at once marked out and the space carefully levelled. The foundation stone was also carefully smoothed, and then laid in its place with milk of lime. As the foundation and stone were both rather hollow, except for three inches at the outer edge, which was polished, the fitting was very perfect. There are no vertical joints, and each stone was laid in the same manner as the foundation stone. As one of the principal thoroughfares of Edinburgh runs about 100 feet below, and only 300 feet distant from, the observatory, tremors were con- fidently predicted by the alarmists. Professor Henderson, however, found none, nor any interruption to his observations in mercury. Professor Smyth adds that he finds no annoyance from the railroad about 300 feet below, and at a horizontal distance of 500 feet. So far the observatory founded on a rock came out victoriously from its ordeal, but Professor Henderson, in the course of his work, found a well-marked annual variation of the level of the transit, which he attributed to the expansion of the rock. This variation seemed so intimately connected with temperature that he latterly took his factor for level correction from the thermometer, having found a constant agreement between this and the indications of the spirit level. The maximum of this change amounted to between 0^-2 and 0**3 in the value of the level factor, and the variations were tolerably regular. On computing the azimuthal factors for 1841, Professor Smyth is more felt on solid than on loose foundations. In a standard observatory, where observations are made principally in the meridian, tremor scarcely affects the accuracy of observation at all, unless it is so excessive as to change the position of the microscopes, piers, &c. Now this is obviously the least likely to happen when the foundation is on rock ; the tremors are propagated through the substance, without in any respect altering its form. Sudden and discontinuous changes, which obey no law, are those only which are to be feared in a well-directed observatory. Tremor is chief!}' objec- tionable as disturbing the mercurial horizon, which, however, is now mostly used as a verification, not as the ordinary mode of observing; and when this inconvenience only occurs occasionally, it can generally be avoided or palliated by a little contrivance or foresight. Unless the adjustments are kept in a fluctuating and uncertain state by occasional small oscillations (and we believe no careful experiments have been directed to this point), they are minor evils. The experience of the Oxford and of the Edinburgh Observatory is, so far as it goes, conclusive against any danger from mo- derate exposiu'e to tremors in a well-founded and well-managed observa tory.— S. Royal Astronomical Society. 533 was very much disturbed on finding variations, which sometimes al- tered the factor as much as 0*"3 in a day, and more than P*0 in the course of the year. These changes in azimuth had been remarked by Professor Henderson, and were attributed to the irregular action of the counterpoises, which were consequently removed. On a com- parison of these errors with the indications of thermometers plunged in the rock there were apparent marks of correspondence. There are several thermometers inserted at different depths in the rock near the observatory, which had been carefully observed in the year 1841*. The indications of these thermometers were projected on paper, and the curves thus formed compared with a curve traced according to the course of the azimuthal deviation. It was thus made evident, that the curve of azimuthal deviation, though having, like the other curves, an annual maximum, did not otherwise resem- ble the curves belonging to the deep-seated thermometers at all ; and, in fact, it came nearest the curve traced out by the thermometer at- tached to the barometer and by the free thermometer exposed to the outer air. Hence the cause of the deviation was not to be looked for in the effect of temperature on the foundations or on the massive transit piers, but on smaller parts more readily affected, such as the metallic mounting. These were accordingly examined. In the azimuthal Y, the construction was found to be much as usual, but the artist has adopted an adjustment for the vertical Y, which seems liable to suspicion. There are two vertical screws applied from be- low ; one, pushing, on the north side of the middle, and the other, pulling, at the south side. The Y is prevented from turning in a vertical plane by jamming horizontal screws, which press a plate against the north face of the Y so as to bring the whole tightly against a stopping-piece, which blocks the south face. Professor Smyth's present opinion is, that the effect of expansion on the two screws, which are in contrary states of constraint, is to alter the ad- justment ; certainly the arrangement looks unmechanical. In the ordinary mode of construction, in this country at least, the elevating Y is either raised by one central screw, or by two screws, one on each side of the centre ; in which case a drawing-screw may be placed at the centre. There is thus no tendency to twist, and the side- plates which confine the Y laterally have to exert little restraining force. Professor Smyth has communicated with MM. Repsold, the makers of this magnificent instrument, and is awaiting their reply before adopting any remedy t- * Some years ago, Professor J. D. Forbes had four thermometers sunk in the rock with their bulbs at the depths of 24, 12, 6, 3 French feet and a fifth on the surface merely covered with sand. t Sudden and lawless changes in azimuth forbid independent determina- tions of the azimuthal deviation (which are also the best;, viz. from the consecutive semidiurnal transits of circumpolar stars. The possessor of an imperfectly mounted instrument must content himself with assuming the fundamental places of his close circumpolar stars, and determine his azi- muthal error from each of them. This will, with proper caution, be found quite sufficient for objects not too near the pole, especially when the clock- error stars are pretty numerous, and situated above and below the object to be determined. [ 534 ] LXXVIII. Intelligence and Miscellaneoics Articles. ON OSMIAMIC ACID. BY MM. J. FRITZSCHE AND H. STRUVE. WHEN caustic ammonia is added to a solution of osmic acid in excess of potash, the deep orange colour of the liquid becomes rapidly a bright yellow, and a new salt is produced and separated, either immediately or by evaporating the liquid at a gentle heat, which is a yellow crystalline powder. The formation of this new compound does not necessarily depend on the presence of potash or any other oxide, but uniformly upon that of ammonia ; the ammoniacal salt is, however, subject to altera- tion, and decomposes during evaporation. It is better therefore to cause a basic oxide to intervene. M. Gerhardt remarks that the formula of the osmiamates which the authors have given requires correction ; they agree, he states, with the formula OS, 03 N (M). The properties of the osmiamates are as follows : they decompose by heat with explosion ; and several of them undergo the same de- composition when struck. Among the products of this decomposi- tion are metallic osmium, an osmiate, or a less oxygenated osmic compound. Protosraiamate of mercury volatilizes without explosion, when heated quickly ; and it diffuses a strong smell of osmic acid. Osmiamic acid can be obtained only in solution in water. In order to prepare it, osmiamate of barytes is to be cautiously decom- posed by sulphuric acid, or recently prepared and moist osmiamate of silver is to be decomposed by dilute hydrochloric acid. After fil- tration a bright yellow-coloured solution is obtained, which may be preserved for several days, if it be sufficiently dilute ; on the other hand, if too concentrated, it becomes brownish and decomposes with the disengagement of gas, osmic acid is set free, and a black non- explosive substance is deposited which contains osmium. The same metamorphosis occurs when the weak acid is evaporated over sulphuric acid. Osmiamic acid not only expels carbonic acid from carbonates, but also decomposes chloride of potassium. In fact crystals of os- miamate of potash are obtained, if a crystal of chloride of potassium with a drop of solution of osmiamic acid be exposed to evaporation on a strip of glass. Zinc dissolves in solution of osmiamic acid, with the evolution of a little gas ; part of the acid is decomposed, and the zinc is covered with a very adherent black deposit, and flocculi appear in the liquid which possess the odour of osmic acid. When all the undecomposed acid is saturated with zinc, the metamorjihosis ceases. In the cold, acids do not decompose osmic acid or the osmiamates : sulphuric, nitric or hydrochloric acid may be added to their solutions without inconvenience ; but decomposition readily occurs when heat is applied, and it is rendered apparent by the disengagement of osmic acid and by the brown colour of the liquor ; the products vary ac- cording to the nature of the acid employed. Intelligence and Miscellaneom Articles. 635 Osmiamates are obtained, either directly by the action of osmic acid on a solution of bases in ammonia, as the salts of potash, zinc, and silver, or by precipitating the potash salt by metallic salts, or by decomposing the silver salt by chlorides. MM. Fritzsche and Struve have stated that these salts yield no hydrogen by analysis. In two experiments the potash salt gave by combustion vsrith oxide of copper only 0*072 and 0033 of hydrogen ; whereas 0'34 are required for one equivalent of hydrogen. The osmiamates undergo an interesting decomposition by the action of hydrochloric acid. The products vary according to the concentration of the acid. If the potash salt be sprinkled with con- centrated acid, energetic action immediately ensues, accompanied with the disengagement of chlorine and probably of its oxide ; the hydrochloric acid assumes a fine purple tint, and the crystals of osmiamate of potash are covered with a crust of small red crystals of two different kinds ; if the salt employed be powdered, and the action of the hydrochloric acid be long enough continued, all the osmiamate undergoes this change ; the nature of which the authors have not hitherto succeeded in explaining. If dilute hydrochloric acid be added to a solution of osmiamate of potash saturated cold, no decomposition occurs at common tempera- tures, the metamorphosis taking place only at a higher temperature. It is then more complicated, the liquor temporarily assumes a red and brown tint, and soon emits a smell of osmic acid, which is abundantly disengaged as soon as the liquor is heated to ebullition. If the solution be evaporated to the crystallizing point, as soon as it ceases to emit osmic acid, a mixture of salts is obtained, among which, as shown by the microscope, are hexagonal green tables, green needles, and another red salt, &c. These salts appear to be decom- posed by water, for they were not obtainable by solution and re- crystallization. — Journ. de Ph. et de Ch., Octobre 1847. ON THE PREPARATION AND PROPERTIES OF SOME OSMIA- MATES. BY MM. FRITZSCHE AND STRUVE. Osmiamate of Potash. — This salt is best prepared by dissolving golid osmic acid in a concentrated solution of caustic potash, with the addition of ammonia during the agitation of the mixture. The solution becomes of a bright yellow tint, and the osmiamate of potash is deposited in the state of a yellow granular powder. The product of the distillation of osmic liquors may also be directly passed into a solution of potash, containing ammonia and properly cooled; the simultaneous distillation of nitrous vapours must be carefully avoided, as they would decompose the osmiamate of potash. In both cases, the mother-water which has deposited osmiamate of potash is to be evaporated with a gentle heat ; carbonate of pot- ash may be used instead of caustic, but not so advantageously ; the osmiamate of potash is to be dissolved in a very small quantity of boiling water ; on cooling the solution yields small crystals of the salt of a lemon-yellow colour ; these crystals are of considerable size 536 Intelligence and Miscellaneous Articles. when prepared from a cold saturated solution by spontaneous evapo- ration, their form being an acute octahedron with a square base. Osmiamate of potash is much less soluble in alcohol than in water ; it dissolves without alteration, and decomposes but very little when the solution is evaporated ; it contains no water of crystallization ; it may be heated to 356" F, without decomposing, but it becomes brownish and is rapidly decomposed at a higher temperature, with violent projections. This salt yielded by analysis — Osmium 67*900 Nitrogen 4-126 4*820 Potash 16*126 M. Gerhardt gives as an amended formula 0S03N(K). Osmiamate of Soda is best obtained from the silver salt and chlo- ride of sodium ; the crystals are prismatic, contain water of ci*ystal- lization, and are very soluble in water. Osmiamate of Ammonia is prepared in the same manner. It forms large anhydrous crystals, which appear to be isomorphous with the salt of potash ; at 258° F. it decomposes with explosion. This salt is very soluble in water and in alcohol. Osmiamate ofBarytes readily crystallizes in yellow brilliant needles of several lines in length. 1'his salt is readily soluble in water, and explodes at about 300° F. It yielded by analysis — Barytes 23*88 Osmium „ 61*07 Nitrogen 4*269 the formula according to M. Gerhardt being 0S03N(Ba). Osmiamate of Ammonia and Zinc is obtained either by dissolving osmic acid in a solution of a salt of zinc in caustic ammonia, or by mixing a solution of osmic acid in ammonia with the solution of a salt of zinc. A yellow, bright crystalline powder is soon deposited, which is deprived of the mother-water by washings with ammonia. This compound is very permanent ; it may be dried in the air, and remains without losing ammonia. It is nearly insoluble in ammo- nia, water decomposes it even when cold ; when boiled in water it is completely decomposed with the deposition of oxide of zinc, the disengagement of half of its ammonia, and yielding osmiamate of ammonia. Formula according to M. Gerhardt 0S03N(Zn), 2NH3. Osmiamate of Lead. — A solution of nitrate of lead is not precipi- tated by a concentrated solution of osmiamate of potash ; after some time some crystals are however formed, which are not sufficiently stable for examination. A solution of acetate of lead gives with the solution of the osmiamates a non-crystalline precipitate, which is at first of a dirty yellow colour, but it soon becomes of a purple tint with the extrication of osmic acid. If a solution of chloride of lead, or a solution of nitrate of lead with the addition of hydrochloric acid, be added to a solution of osmia- mate of potash, a yellow crystalline precipitate is soon obtained, which the authors consider to be a compound of equal equivalents of chloride eind osmiamate of lead. Intelligence and Miscellaneous Articles. 537 Protosmiamate of Mercury forms a bright yellow precipitate ; it is not crystalline, and is insoluble in water ; the perosmiamate of mer- cury forms prismatic crystals. Osmiamate of Silver is obtained directly by dissolving osmic acid in an ammoniacal solution of a salt of silver, and afterwards super- saturating with nitric acid. It may also be obtained by adding to a solution of osmic acid in ammonia nitric acid in excess at first, and then a salt of silver. It may also be prepared by double decompo- sition with the salts of silver and soluble osmiamates, Osmiamate of silver is a crystalline powder of a lemon-yellow colour ; it is very slightly soluble in water and in cold nitric acid, more soluble in ammonia, and may be combined with it. It may be dried in the dark without blackening, in vacuo, over sulphuric acid ; eventually, however, it suffers decomposition, and then gives out osmic acid ; at 176° F. it decomposes suddenly and with violent de- tonation ; it is also decomposed by percussion, and likewise when sulphuretted hydrogen is passed over the dried salt ; nitric acid de- composes it readily when heated ; the liquor first acquires a brown tint, and gradually becomes colourless with the disengagement of osmic acid. This salt yields by analysis — Oxide of silver .. 32-08 32*060 32-13 Osmium 55-011 M. Gerhardt gives as its formula 0S03N(Ag). — Journ. de Ph. et de Ch., Octobre 1847. ON SULPHATO-CHLORIDE OF COPPER, — A NEW MINERAL. BY ARTHUR CONNELL, ESQ. This mineral occurs in small but very beautiful fibrous crystals, of a fine blue colour, which is pale when the fibres are delicate, but much deeper when they become somewhat thicker. Their form, according to Mr. Brooke, is a hexagonal prism with the edges re- placed, thus belonging to the rhombohedral system. They possess considerable translucency, and have a vitreous lustre. On account of the small quantity which he possessed, Mr. Connell was unable to state the specific gravity, hardness, or fracture. Their locality is Cornwall. Mr. Brooke is aware of the existence of only a very few specimens of the mineral : one is in the British Museum. Like atacamite, this mineral colours the blowpipe flame as well as the simple flame of a candle, of a fine greenish-blue, indicating the presence of chloride of copper. Reduced to powder, and mixed in sufficient quantity with charcoal powder, and then heated in a close tube, it gives decided, although not strongly marked, indications of the presence of sulphuric [sulphurous ?] acid by the smell, and partial bleaching of Brazil wood paper, the remainder of the paper being reddened, doubtless by muriatic acid vapours. Alone, in the close tube, it yields a little water, and other appearances resembling those afforded by atacamite. Heated alone on charcoal before the blowpipe, it decrepitates strongly ; but when previously deprived 5S8 Intelligence and Miscellaneous Articles. of the greater part of its water by gentle heat, and then powdered and moistened, and heated on charcoal, it gives no traces of arsenic, although arseniate of copper is associated with it in the specimens. The residue is a dark reddish slag or globule. The crystals are njjt soluble in boiUng water, but dissolve entirely and pretty readily in nitric or muriatic acid, especially by the aid of a gentle heat. The solutions have the colour belonging to copper solutions ; and in the act of dissolving a very few bubbles of gas may be observed to arise, indicating probably the presence of a mi^ nute quantity of carbonate. The solutions yield, with barytic salts, a white precipitate insoluble in acids ; and the nitric solution gives, with nitrate of silver, a white and curdy precipitate insoluble in acida or water, but soluble in ammonia. Ammonia in excess, added to the original solution, gives the fine deep blue of copper. These appearances, in conjunction with the blowpipe reactions, are sufficient to show that the constituents of the mineral are sul- phuric acid, chlorine, copper, and a little water ; but Mr. Connell had not sufficient of the mineral to determine the proportions of its constituents. The chloride is apparently more abundant than the sulphate. — Jameson's Journal, October 1847. ON THE FORMATION OF VALERIANIC ACID. BY M. THERAULT. The author remarks that it has been long known that the oil of potatoes yields valerianic acid under the influence of the caustic alka-* lies; and it has also been stated that the oil of valerian gave analogous results. M. Therault thought it would be an interesting subject of inquiry to determine in what manner this transformation occurs, and whether it is complete or only partial ; and in the latter case to ex- amine into the nature of the non-acidifiable product ; whether the alkalies directly produced a true chemical reaction on the elements of the oil ; and lastly, whether the intervention of other agents is not requisite to effect the transformation. In order to resolve these questions, the following experiments were performed, care being taken to operate with oil perfectly deprived of any trace of acid. 1 . A portion of oil was mixed with distilled water, and divided into two parts, one of which was exposed to the contact of the air, and the other put into a bottle to prevent its action. 2. Another portion of the oil was mixed with caustic potash, per- fectly dry and reduced to powder, and divided as in the preceding experiment. 3. A mixture was prepared of six parts of oil and three parts of potash, previously dissolved in one part of water, and the mixture was divided as in the foregoing experiments. The following observations were made on these mixtures. After the contact of a month, that portion of the mixture of the first ex- periment which had been submitted to the action of the air, had become sensibly acid ; in the second portion no change had occurred. In the second experiment no sensible trace of valerianic acid was Intelligence and Miscellaneous Articles, 589 produced ; the potash and the oil had nearly retained their original properties. Circumstances were quite different in the third experiment. The mixture had hardly been made when it became of the consistence of honey, and of a red colour of considerable intensity : perfect saponi- fication might be suspected. M. Bonastre had previously remarked this action of the caustic alkalies on some essential oils, and had proposed it as a means of distinguishing mixtures of them ; and he noticed the partial combination of the oil of valerian with soda. This fact might induce the belief that this oil was a substance of a com- plex nature ; M. Therault is, however, of opinion that this is not the case, but that the observation of M. Bonastre was derived from the circumstance of the oil which he employed containing valerianic acid, which would explain in this case the partial combination with soda. The author attentively examined the nature of this mixture : it was perfectly homogeneous, and comparable to crotonic soap. Treated with water and suffered to remain undisturbed, the oil soon collected on the surface ; it was separated, and the filtered liquor was saturated with acetic acid. No sensible trace of oil was reproduced, nor w«s the formation of valerianic acid detected ; it was therefore certain that no chemical action had occurred ; and the name of com- bination given to this mixture appears to the author to be improper under these circumstances. M. Therault relies upon this last fact as corroborating the result of the third experiment. The portion of the mixture kept from the contact of the air, underwent no change of properties after one month ; no combination had occurred between the oil and the pot- ash ; no valerianic acid was formed, or at any rate no appreciable quantity. On the contrary, that portion which had been exposed to the action of the air contained valerianic acid, in minute quantity certainly, but it was very appreciable : the matter was slightly decolorized. The action of the air was allowed to continue, and after six months' exposure nearly the whole of the oil had disappeared, and the mix- ture was almost entirely decolorized, a slight amber tint only re- maining. The decoloration occurred nearly in direct proportion to the quan- tity of acid formed : the action of the air was however continued, to ascertain whether the whole of the oil could be acidified ; the opera- tion required nearly six months, but it was then complete ; the mixture had assumed the aspect of white, slightly grumoua honey ; well-defined crystals of valerianate of potash had formed, and were dispersed throughout the mass. It was covered with a solution of this salt and of potash, without any trace of oil. It may be concluded from the experiments detailed, that valerianic acid does not pre-exist in valerian root ; that it is entirely the pro- duct of the oxidizement of its oil ; that this oxidizement is due to the oxygen of the air ; and that water and the caustic alkalies greatly facilitate this oxidizement. The author also concludes that the caustic alkalies exert no direct action on the elements of the oil ; that they act only by the property which they po§ses^ pf forming an 540 Intelligence and Miscellaneous Articles. intimate mixture with the oil, and exposing it in a state of perfect division to the oxygen of the air. Lastly, M. Theraultisof opinion that oil of valerian is not a substance of a complex nature, and that it may be entirely converted into valerianic acid. This conversion is readily explained. According to Ettling, the formula of valerianic acid isC*" H'^ O^ + H^ O ; if that of oil of va- lerian be C'^o H-o O^ and if tw^o atoms of oxygen be made to inter- vene, one of vvrhich combines with two atoms of hydrogen to form water, and the other be added, we shall have the following equation : C20HW 02 + 20=020 HIS 03 + H'^O. M. Tberault finishes his memoir with observing, that the process for extracting valerianic acid, proposed by Messrs. Smith of Edin- burgh in the Journal de Phannacie for January last, appears to be a good one ; excepting that he would propose to use a caustic instead of a carbonated alkali, and after having boiled the mixture, to expose it for a month to the air, stirring it several times a day ; not to subject the residue to pressure, and to distil with the roots, which greatly facilitate the operation. When afterwards the distilled liquor has been saturated by means of an alkali, and the valerianate of pot- ash or soda has been concentrated, it is essential not to employ an excess of sulphuric acid to separate the valerianic acid ; it would be better to leave a small portion of the valerianate undecomposed, for towards the end of the distillation, the organic matter mixed with the salt is carbonized and sulphurous acid is formed, which appears to react upon the valerianic acid. — Journ. de Pharm. et de Ch., Sep- tembre 1847. NOTE ON THE MEASUREMENT OF THE DOUBLE SULPHATES OF ZINC AND SODAj AND OF MAGNESIA AND SODA. BY PROF. W. H. MILLER. The crystals were not good enough for me to obtain a very satis- factory result from a few observations ; they are however sufficiently good to show that they are isomorphous. The crystals belong to the oblique prismatic system. The angles between normals to the faces are — for the oxide of zinc salt, nn' 113° 4 M u' 74° 12 the angle between a normal to c and the intersection of M, m'=10°22' u c 83° 46' r c 49° 54' The symbols of the simple forms, in the notation which I use, are — c 001, rlOl, « 110, u 120, e Oil, 5 121. The faces of the magnesian salt are more irregular than those of the former, so that I cannot pretend to determine the diflference be- tween the angles of these crystals. Intelligejice and Miscellaneous Articles. 541 The angles given above must be considered as rough approxima- tions only. In a little time perhaps I may be able to obtain more accurate values of them. — From the Proceedings of the Chemical Society, vol. iii. p. 391. NATIVE CARBONATE OF NICKEL. This new mineral was exhibited last year at the Philosophical Society's exhibition in Glasgow, and was examined at the time, at the request of Dr. R. D. Thomson, by his pupil Mr. John Brown, in the College Laboratory. It occurs in the form of thin green cry- stalline layers, on the surface of chrome iron ore from America. It dissolves with effervescence in dilute hydrochloric acid. The solu- tion is precipitated black by sulphohydret of ammonia ; is precipi- tated and dissolved in excess by caustic ammonia, yielding a cha- racteristic coloured solution. Caustic soda precipitates the solution green, without resolution. It is accompanied, apparently in union, by carbonates of lime and magnesia — isomorphous bodies. The fact of its occurring on the surface of chrome iron, and having been mis- taken for sesquioxide of chrome, renders it probable that oxide of nickel may exist in that mineral occasionally. — R. D. T. AN EXAMINATION AND ANALYSIS OF THE " NADELERZ," OR NEEDLE ORE OF BISMUTH. BY. E. J. CHAPMAN, ESQ. The "needle ore" occurs in thin prismatic crystals, generally forming more or less radiated groups imbedded in quartz, at Ekatherinen- burg in Siberia, the only known locality in which it has been hitherto found. The crystals are too imperfect to admit of measurement ; but they appear to belong to the Trimetric or Prismatic system, and to have for the primary form a right rectangular prism, or perhaps more correctly a right rhombic one, in which the angle MM closely approaches a right angle. The colour of this mineral is dark steel-gray on the fractured sur- face, but externally the true colour is usually masked by a yellow tarnish. The powder or "streak" is black; the degree of hardness 2*0 to 2*5, or between that of rock-salt and calc-spar ; and the spe- cific gravity about 6*1. Before the blowpipe it fuses instantly and may be almost entirely volatilized, forming a yellow incrustation of the mingled oxides of lead and bismulii on the support. The presence of bismuth and copper may be ascertained by fusion with " microcosmic salt" and a little tin on charcoal in the reducing flame, when the lead, which is clear whilst hot, becomes on cooling of a grayish-black colour with red patches. With carbonate of soda on charcoal in the same flame, it forms an alkaline sulphuret. The lead is best detected by boiling a fragment in nitric acid, filtering, dissolving the residue (sulphate of lead) in caustic potash, diluting the solution, and re- precipitating by sulphuric acid. This ore was first described by Karsten and analysed by John; and although a considerable period has elapsed since the date of this analysis, yet, probably from the rarity of the mineral, its composition J43 Intelligence and Miscellaneous Articles. has been examined by but one other chemist, Frick, in PoggendorfF's * Annalen,' xxxi. p. 529. These analyses have given — 1. By John :— Per cent. Atomic relations. Sulphur. 11-58 0-057 3 Bismuth 43-20 0-032 2 Lead 24-32 0-018 1 Copper 12-10 0-031 2 Nickel 1-58 Tellurium 1-32 Gold 0-79 94-89 2. By Frick :— Sulphur 16-61 0-0826 6 Bismuth 36-45 0-0410 3 Lead 36-05 0-0270 2 Copper 10-59 0-0267 2 99-70 The first analysis does not admit of any rational formula; but if we consider the loss, more than 5 per cent., to be sulphur, we may obtain by a little latitude, Cu2 S + PbS + Bi2 S», or 2 1 ^^^ \ + Bi^ S^, a formula analogous to that of the kobellite from Ilvena in Sweden, analysed and named by Setterberg, and in which the electro-negative atoms in the base are to the electro-negative atoms in the acid as 2 to 3. The following is its formula : — The second analysis yields also but an inexpressive and unsatis- factory result. The formula, if such it can be termed, obtained from it is — Cu« S + 2PbS + 3BiS, or otherwise Cu^ S, BiS + 2(PbS, BiS). I have now to enter into the details of a third analysis, executed lately by myself, on a specimen kindly given to me by Colonel Jackson, F.R.S., who brought it with him from Russia. The ore was accompanied in the quartz by minute tufts of malachite, which, together with the matrix, were carefully removed, by the aid of a microscope, from the substance analysed. 8-38 grs. of the mineral in powder were boiled in strong nitric acid. A residue of 4-92 grs. of sulphate of lead remained, and 0-26 grs. of sulphur. The 4-92 grs. of sulphate of lead (obtained, it should be stated, after solution of the residue in potash and subsequent re- conversion) = 3-36 grs. of lead and 0*52 of sulphur. Carbonate of ammonia in excess was then added to the clear so- lution ; and after remaining for three hours at a gentle heat, it was filtered from the precipitate, which (after being well-washed with Intelh'ge?ice and Miscellaneous Articles. 643 the same reagent, and the "washings" added to the original solu- tion) was dissolved in acetic acid ; and a slip of pure lead being im- mersed in the solution, the whole was covered up immediately and suffered to stand for four hours. The slip of lead weighed 22*63 grs. The four hours having elapsed, the lead was taken from the solu- tion, and, after separation of the precipitated bismuth, dried and weighed. It weighed 19*21 grs.; loss, 3*42 grs. On the addition of sulphuric acid, 5*03 grs. of sulphate of lead were obtained, which are equal to 3*435 of lead ; and this amount corresponding so nearly with the loss in the metallic precipitant, the whole of the lead pre- sent in the mineral may be considered to have been converted into PbO, SO^ by the first operation. The bismuth precipitate wad washed with cold distilled water (which had been boiled), dissolved in nitric acid, and again thrown down by carbonate of ammonia. The oxide of bismuth weighed 2"60 grs., equivalent to 2*33 grs. of bismuth. To tiie original solution (containing carbonate of ammonia) a few drops of ammonia were added, and it was then gently evaporated until the ammoniacal odour was entirely destroyed. Solution of potash was then added, and the whole boiled. The black oxide of copper, well-washed with hot water, ignited, and weighed in a covered crucible, came to 1*31 grs., an amount equal to 1*05 of copper. Finally, chloride of barium was added to the potash solution, which produced a precipitate of sulphate of baryta weighing 5*72 grs., an amount corresponding to 0*79 of sulphur. The whole of the sulphur present in the mineral was therefore 1*57 grs. (0*52 + 026 + 0*79). The following table exhibits the above analysis and its atomic de- ductions :— - Per cent. Atomic relations. Sulphur 1-57 18*78 0*0935 3 or 18 Bismuth 2*33 27*93 0*0315 1 or 6 Lead 3*36 40*10 0*0309 lor 6 Copper 1*05 12*53 0-0317 1 or 6 8*31 99*34 3Cu2 S, Bi^ S9 + 2(3PbS, Bi"- S^. This formula is identical with that of the bournonite (from the analyses of H. Rose, Smithson, &c.), substituting only Bi^ S' for Sb^ S^ as below : — Bournonite = 3Cu2 S, Sb^ S^ + 2(3PbS, Sb^ S^)- in each ore, the electro-negative atoms in the basic compounds are, to the electro-negative atoms in the acid compounds, as 1 to 1, as expressed in the accompanying general formula : — „ / Cu2 s \ , / Sb2 sn As the bournonite crystallizes also in the same system as the needle ore, and indeed affects probably the same primary form within close measurements, the isomorphous relationship of these minerals is sufficiently apparent. 544f Intelligence a7id Miscellaneous Ar fides. Most English mineralogists give a right rectangular prism for the primary form of the bournonite ; but Dufrenoy, in his recent Treatise, vol. iii. p. 18, after an examination of numerous crystals, considers a right rhombic prism in which the angle MM = 93" 40' to be the correct primary form. The modified rectangular prism in which the bournonite usually occurs is in this light a secondary form, de« rived from the primary by the replacement of its lateral edges by the planes g' h' in the notation of Hauy. The specimen of the needle ore which furnished the above ana- lysis, exhibited here and there in the quartz transverse rhombic sections, in which an accustomed eye might easily perceive that the obtuse angle was included between 90° and 100°. I could not detect in this specimen the presence of tellurium, found by John in the needle ore ; it is however perfectly conceivable that, under certain circumstances, a portion of the PbS may be re- placed by PbTe. — From the Chemical Gazette for September 1, 1847. ACTION OF ANHYDROUS PHOSPHORIC ACID ON AMMONIACAL SALTS. BY M. DUMAS. The author finds that when anhydrous phosphoric acid is made to react upon crystallized acetate of ammonia, there distils a liquid the fixed boiling-point of which is 170° F., and which is miscible with water in all proportions. When purified by digestion with a saturated solution of chloride of calcium, and then distilled from solid chloride of calcium and from magnesia, it still possesses the boiling-point above mentioned. Analysis gave the following numbers : — Experiment. Calculation. Carbon 57*4 58-5 Hydrogen 7"4 7'3 Nitrogen 34*4 34-2 99-2 100-0 The density of the vapour gave the number 1*45. The above results lead to the very simple formula C"* H^ N, which differs from acetate of ammonia by four equivalents less of water. Its composi- tion is similar to that of nitroguret of acetyle. But a point of view, which the reactions will warrant, would give to this substance the following rational formula. C^ NH, C- H^, which would make hydrocyanate of methylene of it, or an isomeric of it. The reactions w^hich have been examined gave rise to some curious phaenomena. Thus solution of potash at a boiling heat disengages ammonia and regenerates acetic acid ; chromic acid has no action ; nitric acid is not decomposed by this liquid even when heated to ebullition. Potassium acts vividly in the cold, and with the disen- gagement of heat ; cyanide of potassium is formed, and an inflam- mable mixture of free and carburetted hydrogen gases is evolved. It is well known that M. Fehling obtained a substance of analo- gous composition to that now described by distilling benzoate of ammonia with a naked fire : he did not however attach to the dis- covery the views which have been now developed, nor did he study Meteorological Observations. B^s its reactions. M. Dumas proposes to examine, under the new point of view described, the action of anhydrous phosphoric acid on the ammoniacal salts formed by the volatile organic acids. M. Dumas remarks that if the product which he has obtained should constitute a compound identical with hydrocyanate of methy- lene, all these ammoniacal salts, treated in the same manner, should yield aethers corresponding to certain alcohols, according to the ge- neral formula — C»H'»0^ NH3=C~H«-« N=C«-2H'»-2, C2NH. In decomposing the latter by potash, there might be produced alcohol C«-2H''-2, 2H0, and prepared by this method, all the alcohols from the fatty acids. — Comptes Rendus, Septembre 13, 1847. METEOROLOGICAL OBSERVATIONS FOR OCT. 1847. Chiaunck. — October 1. Hazy : cloudy. 2. Cloudy. 3. Light clouds and fine : overcast. 4. Foggy : fine. 5. Fine : light clouds : clear at night. 6. Dense fog : very fine : lightning and rain at night. 7. Fine : rain : lightning at night : clear. 8. Very fine. 9, 10. Rain. 11. Rain in forenoon: clear at night. 12. Slight fog: very fine. 13. Foggy : hazy : cloudy at night. 14. Hazy and drizzly: cloudy. 15. Hazy and cold : slight rain, 16. Foggy : very fine. 17. Foggy, with slight drizzle : very fine. 18. Slight fog : rain. 19. Exceedingly fine : rain. 20. Very fine : rain at night. 21. Rain : clear at night. 22. Fine. 23. Densely clouded and boisterous : rain. 24. Slight showers. 25. Very clear : fine: clear and frosty. 26. Frosty: uniformly overcast. 27. Fine: rain. 28. Hazy and mild. 29. Exceedingly fine. 30, Overcast and mild. 31. Cloudy and mild. Mean temperature of the month ., 52^*14 Mean temperature of Oct. 1846 50 '37 Mean temperature of Oct. for the last twenty years 50 '42 Average amount of rain in Oct 2*60 inches. Boston. — Oct. \.—5. Cloudy. 6. Rain. 7. Fine: rain p.m. 8. Fine. 9. Fog: eclipse of the sun invisible until three-quarters over : fog. 10. Rain : rain a.m. 11—13. Fine. 14,15. Cloudy. 16. Fine. 17, 18. Fog. 19,20. Fine. 21. Cloudy: rain a.m. 22. Fine. 23. Cloudy: rain p.m. 24 — 26. Fine. 27. Rain: rain a.m. and p.m. 28. Fog. 29. Rain: rain a.m. 30. Fine: rain A.M. 31. Cloudy. Sandwick Manse, Orkney. — Oct. 1. Clear: cloudy. 2. Cloudy: clear. 3. Cloudy. 4. Cloudy : drops. 5. Bright : showers. 6. Showers. 7. Drizzle. 8. Drizzle : clear : aurora. 9. Clear : cloudy. 10. Cloudy : drizzle. II. Clear : fog. 12. Fog. 13. Cloudy : clear : aurora. 14. Cloudy : clear. 15, 16. Clear: cloudy. "17. Showers : drizzle. 18. Rain. 19. Damp : rain. 20,21. Showers: clear. 22. Showers: rain. 23. Showers: sleet- showers. 24. Sleet -showers. 25. Clear. 26. Drops: showers. 27. Bright: drops. 28. Cloudy. 29. Cloudy: shower : lightning. 30. Showers : rain. 31. Bright : cloudy. Applegarth Manse, Dumfries-shire, — Oct. 1, 2. Chill and droughty. 3, 4. Dull, but fair. 5. Fair a. m. : showery p.m. 6. Heavy rain a.m. 7. Heavy rain a.m. : flood. 8. Frequent showers. 9. Fine a.m. : rain p.m. 10. Heavy rain. 11. Fair: rain in the night preceding. 12. Fair and fine. 13. Fair, but raw and cloudy. 14, 15. Fair, though chilly. 16. Very fine clear day. 17. Dull and cloudy. 18. Dull and cloudy : rain p.m. 19. Heavy rain. 20, 21. Occasional showers. 22. Rain a.m. : very heavy p.m. 23. Rain early a.m. : fine day. 24. Heavy showers. 25. Fair : fine : clear. 26. Rain nearly all day. 27. Heavy rain and flood. 28. Fog : cleared p.m. 29. Fair and fine. 30. Fair a.m. : heavy rain p.m. 31. Rain early a.m. : cleared. Mean temperature of the month 49°'5 Mean temperature of Oct. 1846 49*5 Mean temperature of Oct. for twenty-five years 49 "6 Average rain in Oct. for twenty years 3*56 inches. Rain in Oct. 1847 509 „ Fhil. Mag, S. 3. No. 2 11 . Suppl. 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CO t^iO COCM — '^i lo in O 00 — o 6 6 coco in ONOO in OvCM -« lO t^ covo 00 VO CM CO — in r>. ■t — c CO CO CM 6 6 6 CO CO CO CM Ol 00 CO CM CM 6 6 CO CO -^c.o6oi6--' -li-lF^^F-^r-i-lrHrtCMCMOICMeMOtC^CMCMCMCOCO « 0 P\ O ^ 547 INDEX TO VOL. XXXI. ACETAL, on the preparation and com- position of, 77. Acidii: — hippuric, 127; prussic, 146; ar- senious, 151; cinnamic, 153; nitrocin- namic, 154; margaric, 167; oxalic, 233; metacetonic, 266; valerianic, 348, 538; pectic and metapectic, 390; nitric, 454 ; cuminic, 459 ; carminic, 478 ; ni- trococcusic, 486; chloric, 510; osmi- amic, 534. Adams (Mr.) on an important error in Bouvard's tables of Saturn, 143; on the elements of Neptune, 380. Adie (R.) on some experiments with gal- vanic couples immersed in pure and in oxygenated water, 350. Airy (Mr.) on inequalities in the motion of the moon, 384. Albumen, action of induced electric cur- rents on, 249. Alcohol, action of chlorine on, 77. Aldebaran, projection of, on the moon,233. Algebraic equation of the fifth degree, on the, 341. Algebraical surfaces, on asymptotic straight lines, planes, cones and cylin- ders to, 425. Alizarine, 46. Anderson (Dr. T.) on certain products of decomposition of the fixed oils in con- tact with sulphur, 161. Annular eclipse of Oct. 9, 1847, obser- vation on the, 228. Antimony, on the salts of, 230. Apparatus, chemical, on some improved forms of, 156, 393. Arseniates, on a new test for, 258. Arsenious acid, on two varieties of, 151. Astringent substances, on the means of testing the comparative value of, 150. Astronomy, on a new notation for express- ing various conditions and equations in, 134. Atmosphere, on the polarization of the, 444. Aurora borealis of Oct. 24, 1847, obser- vations on the, 369. Balsam of Tolu, on some products de- rived from the, 153. Bancalari (M.) on the magnetism of flame, 421. Barrcswil (M.) on the dehydration of moaohydrated sulphuric acid, 314. 2 Bath, analysis of the water of the thermal spring of, 56. Bile of the sheep, on the composition of the, 366. Binney (E. W.) on fossil calamites found standing in an erect position in the carboniferous strata near Wigan, Lan- cashire, 259. Birt (W. R.) on a new kite-apparatus for meteorological observations or other purposes, 131. Bismuth, analysis of the needle ore of, 541. Blowpipe, improvements in the construc- tion of the hydro-oxygen, 356. Books, new, notices respecting, 67, 219. Braconnot (M.) on the urine of the calf and the sheep, 49. Brewster (Sir D.) on the modification of the doubly refracting and physical structure of topaz, by elastic forces emanating from minute cavities, 101 ; on the polarization of the atmosphere, 444 ; on the existence of crystals in the cavities of minerals, 497. Bronwin (Rev. B.) on the inverse calculus of definite integrals, 12; on the alge- braic equation of the fifth degree, 341. Brown (J.) on the molybdate of lead, 253. Buchner (M.) on the presence of arsenic, copper and tin, in the mineral waters of Bavaria, 392. Bussy (M.) on two varieties of arsenious acid, 151. Caffeine and its compounds, on the com- position of, 115. Calamites, fossil, observations on, 259. Callan (Rev. N. J.) on a new voltaic bat- tery, and on a cheap substitute for the nitric acid of Grove's platina battery, 81. Cambridge Philosophical Society, pro- ceedings of the, 130, 301, 376. Carminic acid, researches on, 478. Catalysis, observations on, 96, 192. Chapman (E. J.) on the constitution of the needle ore of bismuth, 541. Chloric acid and the chlorates, observa- tions on, 510. Clays, on the composition of, employed in pottery, 435. Coathupe (M.) on the preparation of gun- cotton, 152. Cochineal, researches on, 471, 481. Colouring matters, on the action of a N2 548 INDEX. mixture of red prnssiate of potash and caustic alkali upon, 126. Comet of 1264 and 1556, on the expected reappearance of the, 50. Commutators, remarks on, 241. Connell (A.) on the precipitate produced in spring and river waters by acetate of lead, 122 ; on the sulphato-chloride of copper, 537. Continuity, on the principle of, 137. Copernicus, on the opinion of, with re- spect to the light of the planets, 528. Copper, on the sulphato-chloride of, 536. Cotton, detection of, in linen, 157. Couper (R. A.) on the chemical compo- sition of the substances employed in pottery, 435. Creatine, observations on, 236. Cuminate of ammonia, on the products of the decomposition of, 459. Daubeny (Prof.) on active and extinct volcanoes, 399. De la Rive (A.) on the voltaic arc, 321. De la Rue (W.) on a modification of the apparatus of Varrentrapp and Will for the estimation of nitrogen, 156 ; on cochineal {Coccus cadi), 471. De Morgan (Prof.) on the structure of the syllogism, and on the application of the theory of probabilities to ques- tions of argument and authority, 130; on the opinion of Copernicus with re- spect to the hght of the planets, 528. Domeyko (M.) on vanadiate of lead and copper, 319. Doveri (M.) on some properties of silica, 315. Drach (S. M.) on eliminating the signs in star-reductions, 251. Dumas (M.) on the action of anhydrous phosphoric acid on ammoniacal salts, 544, Durocher (M.) on the extraction of silver, 317. Earth, on the amount of radiation of heat from the surface of the, at night, 69 ; on the determination of the mean den- sity of the, 73. Ebelmen (M.) on the artificial production of minerals, and especially of precious stones, 311; analysis of kupfernickel, 314; analysis of gray copper from Al- geria, 313. Elastic medium, on the symbolical equa- tion of vibratory motion of an, 376. Electric telegraph, on the determination of differences of longitude by means of the, 338. Electro-magnetic influence on flame and gases, 401, 421, Equations, on the solution of linear dif- ferential, 372; monogenous, observa- tions on, 467. Euler's theorem, notice in reference to the extension of, 123. Faraday (Prof.) on the diamagnetic con- ditions of flame and gases, 401. Field (F.) on the products of the decom- position of cuminate of ammonia by heat, 459. Figuier (M.) on the preparation and com- position of lignine, 397. Flame, on the diamagnetic conditions of, 401, 421. Flax, on the chemical composition of the ashes of, 36, 105. Fluid motion, on some cases of, 136. Fluxions, on the invention of, 35. Forster's (T. J, M.) memoir on meteors of various sorts, notice of, 219. Frankland (E.) on the chemical constitu- tion of metacetonic acid, and some other bodies related to it, 266. Fremy (M.) on the gelatinous substances of vegetables, 389. Fritzsche (J.) on the preparation and pro- perties of osmiamic acid and some os- miamates, 534. Galloway (R.) on the water of the ther- mal spring of Bath (King's bath), 56. Galloway (T.) on the proper motion of the solar system, 74. Galvanic couples, account of some experi- ments with, 350. Gases, on the re-absorption of mixed, in a voltameter, 72 ; on the diamagnetic conditions of, 401, 421. Geometry, on a new notation for express- ing various conditions and equations in, 134; contributions towards a system of symbolical, 139. Gladstone (J. H.) on the chemical history of gun-cotton and xyloidine, 519. Glaisher (J.) on the amount of the radia- tion of heat, at night, from the earth, and from various bodies placed on or near the surface of the earth, 69 ; on the Aurora Borealis, as it was seen on Sunday evening, Oct. 24, 1847, 369. Gregory (Dr. W.) on the preparation of hippuric acid, 127. Griffith (Dr. J. W.) on the composition of the bile of the sheep, 366. Grove (W. R.) on certain phsenomena of voltaic ignition and the decomposition of water into its constituent gases by heat, 20, 91, 96 ; correlation of physical forces, noticed, 67. Gruner (M.) on bisilicate of iron or fer- ruginous pyroxene, 78. Gun-cotton, history of the discovery of, INDEX. 7 ; on the preparation and composition of, 152, 519. Hall (Dr. M.) on the effects of certain physical and chemical agents on the nervous system, 72. Hamilton (Sir W. R.) on quaternions ; or on a new system of imaginaries in al- gebra, 214, 278, 511. Hansen (M.) on inequalities in the motion of the moon, 382. Hare (Dr. R.) on the fusion of iridium and rhodium, 147 ; on certain improve- ments in the construction and supply of the hydro-oxygen blowpipe, 356. Hargreave (C. J.) on the solution of linear differential equations, 372. Hearn (G. W.) on the cause of the discre- pancies observed by Mr. Baily with the Cavendish apparatus for determi- ning the mean density of the earth, 73. Heat, on the amount of radiation of, from the earth's surface, 69 ; on the mecha- nical equivalent of, 173. Hebe, notice respecting the planet, 158. Heintz (M.) on creatine, 236. Higginbottom (J.) on the number of spe- cies and the mode of development of the British Triton, 74. Hind (J. R.) on the expected reappear- ance of the celebrated comet of 1264 and 1556, 50 ; observations of Hind's second comet in full sunshine, 145 ; on the planet Hebe, 158; on the new planet Iris, 237. Hippuric acid, on the preparation of, 127. How (H.) on the analysis of the ashes of the orange-tree, 271. Hutchinson (J.) on the function of the intercostal muscles, and on the respi- ratory movements, with some remarks on muscular power, in man, 222. Induction, memoir on, 241. Ink, invisible, on a new, 176. Integrals, on the inverse calculus of de- finite, 12. Iridium, on the fusion of, 147, 365. Iris, notice respecting the new planet, 237. Jacobi (Prof. M. H.) on the reabsorption of the mixed gases in the voltameter, 72. Jones (C. H.) on the structxxre and de- velopment of the liver, 224. Joule (J. P.) on the theoretical velocity of sound, 114; on the mechanical equi- valent of heat, as determined by the heatevolvedby thefriction of fluids, 1 73. Kane (Sir R.) on the composition and cha- racters of certain soils and waters be- longing to the flax districts of Belgium, 36, 105. Kindt (G. C.) on the detection of cotton in linen, 157. Koenig (F.), inventor of the printing-ma- chine, 297. Kolbe (Dr. H.) on the chemical constitu- tion of metacetonicacid, and some other bodies related to it, 266 ; on the decom- position of valerianic acid, by means of the voltaic current 348. Kopp (M. E.) on balsam of Tolu, and some products derived from it, 153 ; on the action of hydrochloric acid in the for- mation of oxalic acid, 233. Ledoyen's disinfecting fluid, remarks on, 233. Lefroy (Capt. J. H.) on a great magnetic disturbance on the 24th of September 1847, 346. Liebig (Prof.) on a new test for prussic acid, and on a simple method of pre- paring the sulphocyanide of ammonium, 146. Lignine, on the preparation and composi- tion of, 397. Linen, on the detection of cotton in, 157. Liver, on the structure and development of the, 224. Longitude, on the determination of differ- ences of, by the electric telegraph, 338. Loomis (Prof.) on the determination of differences of longitude by means of the electric telegraph, 338. Lubbock (Sir J.) on the perturbations of planets moving in eccentric and inclined orbits, 1, 86 ; on the heat of vapours, 90 ; on the development of the disturbing function R, 144. Madder, on the colouring matters of, 46. Magnetic declination at St. Helena, on the diurnal variation of the, 70. Magnetic disturbance, on a great, 346. Magnetism, influence of, on the voltaic arc, 328. Malaguti (M.) on the extraction of silver, 317. Mannite, action of nitric acid on, 316. Margaric acid, observations on, 167. Mechanics, on a new notation for ex- pressing various conditions and equa- tions in, 134 ; contributions towards a system of symbolical, 139. Mercer (J.) on the action of a mixture of red prussiate of potash and caustic al- kali upon colouring matters, 1 26. Merck (G.) on the water of the thermal spring of Bath, 56. Meridian instruments, on the properties of rock as a foundation of the piers of, 531. Metacetonic acid, on the constitution of, 266. Metapectic acid, 389. 550 INDEX. Meteor of September 25, 1846, notice re- specting the, 368. Meteors, observations on, 219. Meteorological observations, 79, 159, 239, 319, 399, 545 ; on a new kite-apparatus for, 191. Meteorology, suggestions for promoting the science of, 238. Methylene, on the hydrocyanate of, 544. Miller (Prof. W. H.) on the measurement of the double sulphates of zinc and soda, and of magnesia and soda, 540, Mineral waters, analyses of, 56, 124 ; on the presence of arsenic, copper and tin in some, 392. Minerals : —ferruginous pyroxene, 78 ; mo- lybdate of lead, 253 ; gray copper from Algeria, 313 ; kupfernickel, 314 ; vana- diate of lead and copper, 319 ; sulphato . chloride of copper, 537; native car- bonate of nickel, 541 ; needle ore of bismuth, ib. Minerals, on the artificial production of, 311 ; on the existence of crystals in the cavities of, 497. Molybdate of lead, analysis of, 253. Moon, on inequalities in the motion of the, 382. Muscles, on the function of the intercostal, 222. Neptune, on the elements of, 380. Nervous system, on the effects of certain physical and chemical reagents on the, 72. Nicholson (E. C.) on the composition of caffeine and some of its compounds, 115. Nickel, on the native carbonate of, 541. Nitric acid, theoretical views on the na- ture of, 7 ; on the hydrates of, 454. Nitrococcusic acid, on the preparation and composition of, 486, Nitrogen, on some modifications of the apparatus for determining, 156, 393. Numbers, on certain properties of prime, 70; account of a discovery in the theory of, 189 ; on an equation in, 293 ; on the partitions of, 301. O'Brien (Rev. M.) on a new notation for expressing various conditions and equa- tions in geometry, mechanics and astro- nomy, 134 ; on a system of symbolical geometry and mechanics, 139 ; on the symbolical equation of vibratory motion of an elastic medium, whether crytal- lized or uncrystallized, 376. Odmyle, on the sulphuret of, 170. Oils, fixed, on certain products of the de- composition of, in contact with sulphur, 161, Optical instruments, on the formation and application of fine metallic wires to, 53 1 . Orange-tree, analysis of the ashes of the, 271. ^ Osraiamic acid and osmiamates, on the preparation and properties of, 534. Oxalic acid, formation of, 233. Ozone, on a new test for, 176. Papyrine, on the preparation and compo- sition of, 398. Pectic acid, 389. Peligot (M. E.) on the preparation and composition of the salts of antimony, 230. Phosphoric acid, anhydrous, action of, on ammoniacal salts, 544. Pierre (M. I.) on chlorosulphuret of sili- cum, 78 ; on the equivalent of titanium, 155; on the solubility of chloride of silver in hydrochloric acid, 398, Planets, on the perturbations of, 1,86; on the opinion of Copernicus with re- spect to the light of the, 528. Platinum, on the fusion of large masses of, 356. Playfair (L.) on transformations produced by catalytic bodies, 193. Pollock (Sir F.) on certain properties of prime numbers, 70. Pottery, on the chemical composition of the substances employed in, 435. Poumarede (M.) on the preparation and properties of lignine, 397. Printing-machine, invention and first in- troduction of, by Kceuig, 297, Prus«ic acid, on a new test for, 146. Pyroxene, ferruginous, analysis of, 78. Pyroxyline, contributions to the chemical history of, 7, 152, 519. Quaternions, on, 214, 278, 511. Reviews : — Grove's Correlation of Physi- cal Forces, 67 ; Forster on Meteors, 219. Rhodium, on the fusion of, 147, 365. Richardson (T.) on the ashes of rough brown sugar and molasses, 336. Ronalds (Mr.) on a new kite-apparatus for meteorological observations or other purposes, 191. Roth (M.) on the preparation of the prot- oxide of tin, 392. Rowney (T. H.) on the ashes of the orange- tree, 271. Royal Society, proceedings of the, 69, 222, 372, Royal Astronomical Society, proceedings of the, 143, 380, 528, Sabine (Lieut.-Col. E.) on the diurnal variation of the magnetic declination of St. Helena, 70. Salt, culinary, on the solubiUty of, in alcohol, 393. Salts, ammoniacal, action of anhydrous phosphoric acid on, 544. INDEX. 551 Saturn, on an important error in Bou- vard's tables of, 143. Schcenbein (Prof.) on the discovery of gun-cotton, 7 ; on a new test for ozone, 176. Schunck (Dr.) on the colouring matters of madder, 46. Silica, observations on, 315. Silicium, on the chlorosulphuret of, 78. Silver, on the extraction of, 31 7 ; solu- bility of the chloride of, in muriatic acid, 398. Slatter (Rev. J.) on the meteor of Sep- tember 25, 1846, 368. Smith (Mr. A.) on the hydrates of nitric acid, 454. Smyth (Prof. C. P.) on the properties of rock as a foundation of the piers of meridian instruments, and on the de- tection of a cause of error in the Edin- burgh transit, 531. Sobrero (M.) on nitric mannite, 316. Soils and waters of the flax districts of Belgium, on the composition and cha- racters of, 36, 105, Solar system, on the proper motion of the, 74. Sound, on the theoretical velocity of, 114. Spinelle, on the artificial production of, 312. Star-reductions, on ehminating the signs in, 251. Stas (M.) on the action of chlorine on alcohol — formation of acetal, 77. Stokes (G. G.) on some cases of fluid mo- tion, 136; on the theory of oscillatory waves, 138. Storms, observations relating to the laws of, 338. Struve (H.) on the preparation and pro- perties of osmiamic acid and some os- miamates, 534. Sugar, analyses of the ashes of rough brown, 336. Sulphocyanide of ammonium, simple me- thod of preparing, 146. Sulphuric acid, on the dehydration of, 314. Sulphates, on the measurement of some double, 540. Syllogism, on the structure of the, 130. Sylvester (J. J.) on a discovery in the theory of numbers relativatj^o the equa- tion kx^+By^ + Cz^^Bayz, 189, 293 ; on the general solution (in certain cases) of tbe equation or^+J/'+A^^ = M xyz, &c., 467. Taylor (R.) on the invention and first in- troduction of Mr. Koenig's printing- machine, 297. Taylor (T.) on some improved forms of chemical apparatus, 393. Therault (M.) on the formation of valeri- anic acid, 538. Thompson (L.) on chloric acid and the chlorates, 510. Thomson (Dr. R. D.) on a test for arse- niates, 258. Tin, on the preparation of the protoxide of, 392. Titanium, on the equivalent of, 155. Tolene, composition of, 153. Topaz, on the modification of the doubly refracting and physical stmcture of, 101 ; on the crystals in the cavities of the, 504. Triton, on the number of British species and mode of development of, 74. Tyrosine, on the properties and composi- tion of, 496. Ulrich, Mr,, on the formation and appli- cation of fine metallic wires to optical instruments, 531. Urine of the calf and the sheep, compa- rative analysis of the, 49. Valerianic acid, on the decomposition of, by the voltaic current, 348 ; on the for- mation of, 538. Vapours, on the heat of, 90. Veall (S.) on a means for promoting the science of meteorology, 238. Vegetables, on the gelatinous substances of, 389. Voltaic arc, researches on the, 321. battery, description of a new, 81. current, on the decomposition of valerianic acid by the, 348. ignition, on certain phaenomena of, 20, 91. Voltameter, on the reabsorption of mixed gases in a, 72. Wagner (M.) on the solubility of common salt in alcohol, 393. Walter (Mr. John), false statements in the Times newspaper and Mechanics* Magazine concerning him as regards Koenig's printing-machine, 297. Warburton (H.) on the partitions of num- bers, on combinations, and on permu- tations, 301. Warington (R.) on the means of testing the comparative value of astringent substances for the purposes of tanning, 150. Wartmann (Prof.. E.) on induction, 241. Water, decomposition of, by heat, 20, 91 ; on the decomposition of, by platinum, 177. Waves, oscillatory, on the theory of, 138. Weddle (T.) on asymptotic straight Unes, 68i INDEX. planes, cones and cylinders to algebraical surfaces, 425. Weld (C. R.) on the invention of fluxions, 35. "Wilson (Dr. G.) on the decomposition of water by platinum and the black oxide of iron at a white heat, 177. Young (Prof. J. R.) on the extension of Euler's theorem, 123 ; on the principle of continuity in reference to certain re- sults of analysis, 137. Xyloidine, contributions to the chemical history of, 519. Zantedeschi (Prof.) on the motions pre- sented by flame when under the electro- magnetic influence, 421. . END OF THE THIRTY-FIRST VOLUME. PRINTED BY RICHARD AND JOHN E. TAYLOR, RED LION COURT, FLEET STREET. FLAMMAM. ^K- J^.5. A Tig. 2. ^> S/^ /P A -^M /I Fvg.5. S y rtaiia.nn del. f % I%a. Miff. S.SYolSKZMFl.l Fi^.3. Fi^.4. Fi^.6. Fi^.6. Fig. 7. J'.Sasire, So. ^-:. ^. J^*- .J? 5;5*«ew*