Li Sie if; eases sy Bas Pe F wiys we PY i ay are Vipera 4 \ Ny: Bay reveal EDINBURGH NEW PHILOSOPHICAL JOURNAL. THE EDINBURGH NEW PHILOSOPHICAL JOURNAL, EXHIBITING A VIEW OF THE PROGRESSIVE DISCOVERIES AND IMPROVEMENTS . SCIENCES AND THE ARTSE. IN CONDUCTED BY se ‘ ROBERT. JAMESON, uiSTE REGIUS PROFESSOR OF NATURAL HISTORY, LECTURER ON MINERALOGY, AND KEEPER OF THE MUSEUM IN THE UNIVERSITY OF EDINBURGH; Fellow of the Royal Societies of london and Edinburgh ; Honorary Member of the Royal Ivish Academy ; of the Royal Society of Sciences of Denmark ; of the Royal Academy of Sciences of Berlin; of the Royal Academy of Naples ; of the Geological Society of France; Honorary Member of the Asiatic Society of Calcutta; Fellow of the Royal Linnean, and of the Geological Societies of London ; of the Royal Geological Society of Cornwall, and of the Cambridge Philosophical Society ; of the Antiquarian, Wernerian Natural History, Royal Medical, Royal Physieal, and Horticultural Societies of Edinburgh ; of the Highland and Agricultural Society of Scotland ; of the Antiquarian and Literary Society of Perth; of the Statistical Society of Glasgow ; of the Royal Dublin Society; of the York, Bristol, Cambrian, Whitby, Northern, and Cork Institutions ; of the Natural History So- ciety of Northumberland, Durham, and Newcastle ; of the Imperial Pharmaceutical Society of Petersburgh ; of the Natural History Society of Wetterau ; of the Mineralogical Society of Jena ; of the Royal Mineralogical So- ciety of Dresden; of the Natural History Society of Paris ; of the Philomathie Society of Paris ; of the Natural History Society of Calvados ; of the Senkenberg Society of Natural History ; of the Society of Natural Sciences and Medicine of Heidelberg ; Honorary Member of the Literary and Philosophical Society of New York; of the New York Historical Society ; of the American Antiquarian Society ; of the Academy of Natural Sciences of Philadelphia ; of the Lyceum of Natural History of New York ; of the Natural History Society of Montreal ; of the Franklin Institute of the State of Pennsylvania for the Promotion of the Mechanical Arts ; of the Geological Suciety of Pennsylvania ; of the Boston Society of Natural History of the United States; of the South African Institution of the Cape of Good Hope ; Honorary Member of the Statistical Society of France ; Member of the Entomological Society of Stettin, &c. &c. &c. OCTOBER 1852. .... APRIL 1853. VOL. LIV. TO BE CONTINUED QUARTERLY. EDINBURGH : ADAM AND CHARLES BLACK. LONGMAN, BROWN, GREEN, & LONGMANS, LONDON. 1853. EDINBURGH: PRINTED BY NEILL AND COMPANY,OLD FISHMABKET. CONTENTS. PAGE Arr. I. Biography of Berzelius. By Professor H. Ross of Berlin. (Concluded from vol. liii., p. 221), 1 II. Notes on the Geology of Ceylon.—Laterite For- mation.—F luviatile Deposit of Nuera Elia. By E. F. Keraart, M.D., F.L.S., F.G.S8., As- sistant Surgeon to the Forces. Communicated by the Author, rts Rit 4s: III. On the Condition and Prospects of the Aborigines of Australia. By W. Westeartu, Esq. (Con- cluded from vol. liii., p. 241), 9. Past and Present’ Methods, and Proposed Plans for the Welfare of the Aborigines, . 36 10. Prospects of AWoriginal Civilisation, , 4] 1l. General Review, eye ie ; ; ; 42 IV. Synopsis of Meteorological Observations made at the Observatory, Whitehaven, Cumberland, in the year 1851. By Jouw FLEtcHER MILLER, Esq., F.R.S., F.R.A.S., Assoc. Inst. C.H., &. Communicated by the Author, . 4 a V. On the Basin-like Form of Africa. By Sir R. I. Muvrcuison, late President of the Geographical Society, , ¥ : : ‘ i, oe VI. Solidification of the Rocks of the Florida Reefs, and the Sources of Lime in the Growth of Corals. By Professor Horsrorp, of Harvard, 56 VII. Observations on a remarkable Deposit of Tin-Ore at the Providence Mines, near St Ives, Corn- wall. By Witi1am Jory Henwoop, Ksq., F.R.S., F.G.8S., Member of the Geological So- il CONTENTS. _ PAGE ciety of France, &c. Communicated by the _ Author, . ; ; : : : + ee VIII. Arctic Natural History, 1, Cause of Intense Thirst in Arctic Regions, 72 2. Thickness of the Ice, : ; , : i 8. Warmth of Snow-Burrows, : ; : 74 4. Snow a bad conductor of Sound, : : 74 5. The Breaking up of an Iceberg, : ; 75 6. Refrigerating power of Icebergs, A a 75 7. The Droppings of Hider Ducks, : : 76 8. Arctic Minute Animal and Vegetable Forms and Colour of the Sea, 76 9. On the Flesh of little Auks or Rotel and ze Fowl generally, . : : : 78 10. Red Snow, ; 79 11. On the Colouring Matter of Marine Ais ee Dr DIckIE, . : : 79 12. Nostoc Arcticum (Berk). By Dr Brow 81 i3. Onthe Magnitude of Arctic Glaciers—and their advance towards and termination in the Sea, 82 14. Ice and Sea-Water Coloured by the Diatomacer, 89 IX. On an Improvement in Sikes’ Self-Registering Thermometer. By Ricnarp Aoptz, Esq., Li- verpool. Communicated by the Author, (With a Plate), ; : ‘ : : > Be X. Memoir of the late Dr Thomas Thomson, F.R.S., M.W.S., &c., Professor of Chemistry in the College of Glasgow. Communicated by his re- lative, Dr R. Dunpas Tuomson, ; e.. - OO XI. On the Reconcentration of the Mechanical Energy of the Universe. By Wittiam Jonn Mac- quorn Rankine, C.E., F.R.S.E., pay eae XII. The Classification of Insects from Embryological Data, By Professor Acassiz, . Rye | XIII. Humboldt, one of the first Philosophers who de- livered Popular Courses of Lectures on Science to the People, , d , Re 8 XIV. Professor Oken, the originator of the now Popu- lar Assemblies for the Advancement of Science, 112 CONTENTS. ~ XV. The Earl of Rosse’s Telescopes, and their Reve- lations in the Sidereal Heavens. By the Rev. Dr Scoressy, F.R.S.L. & E., Member of the Wernerian Society, and Corresponding Mem- ber of the Institute of France, &c. Communi- cated by the Author, XVI. Of the Proper Application of Reservoirs to the Improvement of Rivers. By Cuarues ELLet, Jun., Civil Engineer, United States of Ame- rica, XVII. Notices of various Animal Remains, as Bos lon- gifrons, &c., found with Roman Pottery, near Newstead, Roxburghshire: with Notes in re- ference to the Origin of our Domestic Cattle, and the Wild White Cattle of this Country. By Jounw ALEXANDER SmitH, M.D. Commu- nicated by the Author. (With a Plate), XVIII. General Results of the Microscopical Examina- tion of Soundings, made by the U. S. Coast Survey off the Atlantic Coast of the United States. By Professor J. W. Baitzy, of the Military Academy, West Point, XIX. The Reply of the President and Council of the Royal Society, to a Letter addressed to them by the Secretary of State for Foreign Affairs, on the subject of the co-operation of different Nations in Meteorological Observations, XX. On the Diurnal Variations of the Magnetic Needle, and on Aurore Boreales. By AUGUSTE DE LA Rive; being an extract from a Letter to M. ARAGO, . XXI. Meteorological Phenomena in connection with the Climate of Berlin. Translated by Mrs ANNE RamspEN BENNETT from the German of Pro- fessor Dove, iil PAGE 113 118 122 142 144 148 155 iv CONTENTS. XXII. Gieseckite and Bergmannite (Spreustein), two Pseudomorphoses of Transformation from Ne- pheline. By Professor J. R. Brum, of Hei- delberg. Communicated by the Author (from Poggendorff), . XXIII. On the Colours of a Jet of Steam and of the At- mosphere, By R. Cxraustus, XXIV. Description of the Tongue and Habits of the Aard- vark or Ant-eater of the Cape (Orycteropus Capensis). By Wiit1am T. Brack, Assistant- Surgeon to the Forces, South Africa. Com- municated by the Author, XXV. On the Negroes of the Indian Archipelago and Pacific Islands. By W. Joun Crawrurp, KEsq., ERs : ; t : . F XXVI. ScrentiFic INTELLIGENCE :— METEOROLOGY. 1. Analyses of Snow and Rain Water, by M. Eu- gene Marchand. 2. Notes on the Climate of Rangoon, by Dr A. Christison. 3. On the Re- PAGE 162 166 168 175 cent Earthquake felt at Adderley, . 179-180 MINERALOGY. 4. Pseudomorphous Minerals. 5, Large Deposit of Graphite. 6. Sulphur Mine in Upper Egypt. 7. Strontiano-calcite. 8. Platinum and Iridos- mine in California. 9, Identity of Donarium with Thorium. 10. Native Iron. 11. Crystal- lisation and Amorphism, . j d T81-183 GEOLOGY. 12, Flora of the Tertiary Formation. 13. On the Tides, Bed, and Coasts of the North Sea or Ger- man Ocean, ‘ : ; ’ : 183-186 ZOOLOGY. 14. On the Bones and Eggs of a Gigantic Bird in Madagascar. 15. Domestication of Fishes, 186-188 MISCELLANEOUS. 16. Freedom of the Arabs from Leprosy. 17. Obi- tuary, : . . ; : 188 CONTENTS. PAGE Art. I, Biographical Account of the late Wint1am Macait1i- vray, A.M., LL.D., Regius Professor of Natural History in the Marischal College and University of Aberdeen. Communicated by ALEXANDER THomson, Esq. of Banchory, Aberdeen, | » 189 II. Influence of Terrestrial Magnetism on Iron, and the effect that results from it upon the direction of the Compasses in Vessels, . o> 206: . III. Meteorological Phenomena in connection with the Climate of Berlin. Translated by Mrs ANNE RAMSDEN Bennett, from the German of Professor Dove. ss ened from page 162,) Rfrg il fee IV. On the Glacial Phenomena in Scotland and Parts of England. By Ropert CHAMBERS, Esq. F.R.S.E. Communicated by the Author, : .177*229 VI. i Oe VIll. Lx XI. XII. XIII. CONTENTS. . Meteorological Observations taken at the Ordnance Survey Office, 18 Royal Circus, Edinburgh, dur- ing the Year 1852, 130 feet above the mean level of the Sea. Communicated by Captain James, Royal Engineers, On the Valuation of Indigo. By Dr Freperick Penny, F.C.8., Professor of Chemistry in the Andersonian University, Glasgow, On the Origin of Stratification. By D. A. WELLs, Esq., of Cambridge, United States, North Ame- ~ rica, Relation of the Chemical Constitution of Bodies to Light. By Professor E. N. Horsrorp of Har- vard, North America, Notes on the Distribution of Animals available as Food in the Arctic Regions. By Aucustus Pr- TERMANN, Esq., F.R.G-S., &., . The Effect of Heat on the Perpendicularity of Bunker Hill Monument. By Professor KE. N. Horsrorp, of Harvard, North America, . On the Geological Distribution of Marine Animals. By Professor Epwarp ForBeEs, On the Change of Temperature in Europe, and the Variation of the Magnetic Needle. By MrG. A. Rowett. Witha Map. Communicated by the Author, The Paragenetic Relations of Minerals, PAGE 282 285 291 294 295 308 311 312 323 CONTENTS. XIV. Some Remarks on the probable Present Condition of the Planets Jupiter and Saturn, in reference to Temperature, &c. By James Nasmytu, Esq., XV. Captain H. Dennam, F.R.S., on Deep Sea Soundings obtained in lat. 36° 49’ S., long. 37° 6’ W., XVI. Critical Remarks on Astronomical Observations made XVII. XVIII, TX. XX. XXI. with Airy’s Zenith Sector, from 1842 to 1850, in the determination of the Latitudes of various Trigonometrical Stations used in the Ordnance _ Survey of the British Isles. Published by order of the Master-General and Board of Ordnance, under the direction of Lieutenant-Colonel Lewis A. Hatt, Royal Engineers, Superintendent of the Ordnance Survey, Notes on the Scales of the Government Survey of Scotland, On a Quartziferous variety of Trachyte, found in Iceland. By TuHreopor Kyerute, of Christiania. Communicated for the Edinburgh New Philoso- phical Journal, Biography of the celebrated Naturalist, Baron Lxo- POLD von Bucu. Communicated for the Philo- sophical Journal, Register of the Weather and Climate of Rangoon for September 1852, On the Reduction in the Height of Waves after pass- ing into Harbours. In a Letter to Professor Jameson by THomas Stevenson, Esq., Civil En- gineer, ; f ii PAGE 341 346 350 362 367 373 377 378 iv CONTENTS. XXII. Screntiric INTELLIGENCE :— GEOLOGY AND GEOGRAPHY. 1. Extent of Glaciers in the Polar Regions, 2. Sir Walter C. Trevelyan on the Faroe Islands. Ina Letter to Professor Jameson, - $79, ZOOLOGY. 3. Numerical List of Species of the Animal King- 8. dom. 4. Dr Hamilton on the Guano Birds of the Lobos Islands. 5. The Cod Fish of the Whale Fish Islands. 6. Electricity applied to the Capture of Whales. 7. Preservation of Eggs, . 5 : : 380, BOTANY. The Genus Nostoc. 9. Preservation of Vege- tables, PAGE 380 382 383 THE EDINBURGH NEW PHILOSOPHICAL JOURNAL. . Biography of Berzelius. By Professor H. Ross of Berlin. (Concluded from vol. liii., page 221.) BERZELIUS criticised this argument with justice. He de- clared that it seemed to him the same as if a man who is stumbling in the dark, should hesitate to make use of a light, because he would then see more than he required, and be- cause he hoped to find his way without it. In order to appreciate fully the great merit of Berzelius, in putting forward his mineral system, it is only necessary to call to mind how great was the chaos in mineralogy before his time, and especially with regard to the classification of the numerous compounds of silica. Although both Débereiner and Smithson commenced to regard silica as an acid, at about the same time as Berzelius, still it was he who first made an extended application of this view, in the new mineral system ‘which he proposed, by means of which siliceous minerals were included under the head of saline compounds, and the correct conception of their composition first rendered possible. The greater number of natural compounds of silica are double salts ; and observing the great diversity among them, Berzelius raised the question, as to whether it was probable that the individual members of such double salts were different stages of saturation. As he had previously assumed only the most simple relations in chemical compounds, he was at first led to infer upon theoretical grounds, that the VOL. LIV. NO. CVIL.—JANUARY 1853. A 2 Biography of Berzelius. existence of dissimilar stages of saturation in the double salts of silica, was less probable, especially as he had never met with any similar phenomena in his investigations of the double salts of other acids. Nevertheless, he subsequently altered this view, after he had himself first prepared the re- markable double salt of neutral carbonate of magnesia and bicarbonate of potash. The salts of silicic acid, and indeed all true compounds oc- curring in natural as well as artificially prepared salts, re- ceived formule which expressed their composition. But as Berzelius was long doubtful how many atoms of oxygen he should assume in silica, and even whien he afterwards decided for three atoms, did not regard this assumption as perfectly certain, he introduced more simple formulz for siliceous com- pounds, which he termed mineralogical, and distinguished from the chemical formule by the printers’ type employed. The establishment of correct formule, especially for sili- ceous compounds, involved great difficulties since the composi- | tion of very few minerals was known with any degree of cer- tainty. The first quantitative analyses of minerals were made by Torbern Bergman, but according to such imperfect methods that they scarcely indicated anything more than the qualita- tive composition. After these came the analyses of Klaproth, which compared with those of Bergman were a considerable and encouraging advance, for he had not only employed better methods of investigation, but also worked with much greater accuracy. But even the analyses of Klaproth as well as those of Vauquelin and others, who worked simultaneously with him, when put to the test of definite chemical propor- tions were not found to be unquestionable. It is true that at first Berzelius could very often only propose a conjectural formula for the composition of many minerals, and generally only when he made some slight alterations in the results of the then known analyses, in doing which, however, he always proceeded with great caution. Afterwards these incorrect analyses were replaced by correct ones, and indeed especially by Berzelius himself and his pupils, who employed in their analyses the most accurate methods proposed by him. Berzelius first arranged minerals according to their electro- Biography of Berzelius. 3 positive constituents. But after Mitscherlich’s discovery of isomorphism, which has exerted so important an influence upon the arrangement of the system, he considered it more ad- vantageous to classify minerals according to their electro-ne- gative constituents, because the substitution of isomorphous substances is far more frequent among the bases than among the acids; and therefore the classification according to the electro-negative constituents corresponded more with the requirements of mineralogists. Both methods have their advantages; they are equally philosophical, and may be em- ployed with equal justice ; it is therefore a great injustice that Berzelius should have been charged with inconsistency in making this alteration. The mineral system of Berzelius is not even yi completed. He was far from wishing to affirm that it was incapable of improvement, on the other hand, during his whole after-life he continually improved it, and from time to time published it in a more perfect form. The last edition was superin- tended by Rammelsberg in 1847 at the request of Berzelius. The most important modifications still to be made on this system, are perhaps those which would result from a more simple application of the doctrine of isomorphism. It is cer- tainly difficult to harmonize the opinions as to how this ought to be done. Berzelius was not quite right in affirming that it is the constituents of a substance alone which must determine its place in a system. Even in the last “ Jahresberichte” published by him, he declares that, in a mineral system, the sole question for consideration is the elements and their inorganic combinations, and that it is these which must be _ systematically arranged. But he himself directs attention to the difficulties which this view necessarily involves. Is it, he asks, admissible to make one species of diamond and graphite, or of rutile, Brookite, and anatase, or of calcareous spar and arragonite? It is scarcely to be expected that mi- neralogists will give their consent to such a course. However, Berzelius decides in the affirmative. Still I am of opinion that there are even many chemists who will not unconditionally agree with him in this. For itis not alone A 2 + Biography of Berzelius. from the constituents that all the characteristic properties of the compound result, but also from the mode and action of their combination, which is frequently indicated by the form. Taking all this into consideration, it appears probable that dolomite is more closely related to calcareous spar than arragonite, and even that tinstone is nearer to rutile than anatase and Brookite. Since the external characters of minerals are determined, as well by their constituents as by the mode in which these are combined with each other, it follows that that chemical system of mineralogy which approaches most closely to the natural systems, or which even corresponds with them, must be the most perfect. Some time after the appearance of the mineral system, Berzelius published his work “ Ueber die Auwendung des Léthrohrs in der Chemie und Mineralogie.’ He had, in Fahlun, under the guidance of his older friend Gahn, a pupil of Torbern Bergman, acquired an uncommon dexterity in the use of the blow-pipe, enriched this special part of chemistry with a number of original investigations, and brought it to a high degree of perfection. In the above-mentioned work he makes known everything connected with the subject, as well what he learned from Gahn as what he had himself dis- covered. It is rarely that a work has been welcomed by chemists as this was ; but it is also seldom possible at once to recognise the practical value of a work, as in the case of this. It was immediately translated into most European languages ; and in some, especially the German, passed through several edi- tions. Everywhere it met with merited appreciation ; and Mr Children alone, the editor of the English edition, allowed himself to add remarks as superfluous as ill-natured. Besides the behaviour of the most important chemical compounds, all metallic oxides, acids, and their salts, sul- phurets, &e., before the blow-pipe, Berzelius described the behaviour of all minerals which he could obtain, and which were so much the more readily placed at his disposal, as he required only very small quantities for these experiments. He entered upon this investigation with untiring industry, Biography of Berzelius. a) and was thus able to furnish even those mineralogists who but unwillingly admitted the influence of chemistry upon mineralogy, with an extremely welcome gift, since, by simple blow-pipe experiments, it was possible to distinguish minerals with ease and certainty, especially among siliceous com- pounds, which were with difficulty, or only ambiguously, recognisable by means of their external characters. This work bore so manifestly the stamp of perfection, even on its first appearance, that, with the exception of Plattner, in Freiberg, no one has contributed any essential additions or improvements to blow-pipe investigations ; and it is quite as indispensable to the chemist and mineralogist at the pre- sent day as it was thirty years ago. About this time, Berzelius discovered selenium, and was engaged upon the admirable investigation of this ele- ment. Never was there an examination so accurate and tho- roughly exhaustive, of an interesting and hitherto unknown element, comprising all its characters and remarkable com- binations, so that, if we except the discovery of selenic acid by Mitscherlich, which escaped Berzelius, nothing essentially new was added to our knowledge of this element during the next thirty years. Our astonishment at this must be raised, when it is-recollected that all these investigations were car- ried on with a very small quantity of material, only about an ounce of selenium, of which quantity a part was lost, owing to the carelessness of a servant. This paper upon selenium can only be compared with that by Gay-Lussac upon iodine, which appeared several years before, and has yielded, in so many respects, such valuable results. It must, nevertheless, be remarked, that Gay- Lussac was not the discoverer of iodine, and did not under- take the investigation until after the first chemist of that _time, Davy, had almost established the true nature of io- dine; and that he had large quantities of material at his disposal. Almost at the same time that Berzelius was engaged in the examination of the compounds of selenium, Arfvedson occupied himself in his laboratory with the analysis of some Swedish minerals ; and under the guidance of Berzelius, suc- 6 Biography of Berzelius. ceeded in discovering lithium, which, as it came so unex- pectedly, justly created great interest. The following larger papers of Berzelius form, as it were, a Series of monographs upon separate and important branches of chemistry, which were at that time still obscure. It was natural, that when he commenced the demonstration of the law of definite proportions by means of a succession of labo- rious investigations, that he must throw aside much, in order to sketch the groundwork of his system. The investiga- tions which he now undertook, were all instituted in accord- ance with a matured plan, and he had long meditated upon them before actually entering upon them. The first of these investigations was upon the ferruginous cyanogen compounds. Gay-Lussac had, in his very import- ant paper upon cyanogen, neglected to study these com- pounds. After him several chemists had occupied themselves with their examination, but all obtained very different results, the greater number, however, assuming that the iron in the so-called ferro-prussic acid salts was an essential constituent of the acid which was combined in the salts with an oxidized body. Berzelius, however, shewed that these salts contained neither prussic acid nor oxidized bases, but that they con- sist of cyanide of iron combined with the cyanide of an alka- line metal, and consequently were double cyanides. He also extended his investigations to the so-called sulpho-cyanic acid salts, and shewed that they consist of metal, sulphur, and cyanogen, the latter two united to form a radical (which he subsequently called Rhodan); and that in them likewise there was neither prussic acid nor oxidized bases. These investigations, which fully confirmed the views of Gay-Lussac regarding cyanogen, were, however, of still greater importance to Berzelius in another respect. After Davy had been induced, by his researches in 1810, to con- sider that it was simpler and more correct to look upon chlorine as elementary, and not, as he had formerly done, as a compound of oxygen with a radical that had not been iso- lated ; most chemists concurred with him in this view. Gay- Lussac and Thénard, who, even before Davy, considered a Biography of Berzelius. 7 similar view possibly correct, although not exactly more pro- bable than the old one, after the discovery of iodine, openly declared themselves, with Vauquelin and all the other French chemists, in favour of the new doctrine; and the famous paper of Gay-Lussac upon iodine, which appeared in 1818, is written in this spirit. Berzelius alone, who from the first had disputed the hypo- thesis of Davy, continued to defend the old doctrine, even after the discovery of iodine. He did this especially in a paper which first appeared in Gilbert’s Annalen for 1815. He there endeavoured, with a profound sagacity which cannot but be highly admired by every one, even on reading the paper after the lapse of so long a time, to prove the truth of the doctrine of the compound nature of chlorine. He directed attention to the remarkable phenomenon that the constitu- ents of chloride of nitrogen, which are united only by a very feeble affinity, separate with such an energetic evolution of heat as is never observed except in chemical combinations. But above all, he pointed out the analogy which existed be- tween muriates, which, according to the new theory, in the -anhydrous state contain no oxygen, and the sulphates, phos- phates, and other salts, which are indisputably compounds of oxygen acids with oxygen bases, and in which the presence of oxygen may be readily detected. The great authority of Berzelius, and the soundness with which he carried out his refutation of all the evidence brought forward in favour of the new theory, were the reasons why many chemists, especially in Germany, did not adopt Davy’s view of the nature of chlorine. The immediate cause of Berzelius undertaking the inves- tigation of the cyanides of iron was evident, viz., he expected to find in them a more compound radical (united with oxy- gen forming an acid) associated with an oxygen base, and similar to that which he assumed to exist in muriates. It cannot be disputed that to some extent he doubted the ac- curacy of Gay-Lussac’s experiments on cyanogen. Then, as the salts of the ferrocyanic radicals resemble so closely in their characters the ordinary oxygenous salts, and especially as several metallic cyanides, such as cyanide of mercury 8 Biography of Berzelius. or silver, correspond so completely with the analogous chlo- rine compounds, he was of opinion that if he could by this investigation detect oxygen in theferrocyanic compounds, it would be a strong proof of its presence in muriates likewise, and, consequently, evidence in favour of the old theory of the nature of chlorine. However, the result of these investigations was the oppo- site of that which he expected, and thus the main argument against the new doctrine of the nature of chlorine fell to the ground. When gradually other reasons for the greater pro- bability of the new theory were discovered, Berzelius adopted it with the most amiable candour, and relinquished the old theory which he had so long and so ably defended. One, among other, of these reasons was, as I know, the fol- lowing :—Immediately after Berzelius’ investigations on the cyanides of iron, Leopold Gmelin obtained the interesting red double salt of cyanide of potassium and cyanide of iron, which is anhydrous and contains no oxygen. The red colour of the peroxide of iron, which is more or less communicated to all its salts except the neutral ones, was to Berzelius an addi- tional reason for regarding the red perchloride of iron as an actual salt with an oxygenous base; and, as in the salt obtained by Gmelin, notwithstanding its red colour, the iron was not in the state of oxide, but directly combined with cyanogen, one double atom of iron with three double atoms of cyanogen, Berzelius saw that it was probable that the red colour of iron compounds was not owing alone to the pre- sence in them of peroxide, but was also common to those in which one double atom of iron is combined with three double atoms of chlorine or cyanogen. Another main inducement to adopt the new theory of the nature of chlorine, consisted in the results which he derived in favour of it from his subsequent comprehensive researches upon alkaline sulphurets. According to Berthollet’s inves- tigations, these bodies were regarded as combinations of sul- phur with alkalies until Vauquelin put forward the opinion, that when a fixed alkali was melted with sulphur, a part of the alkali was reduced to the metallic state, sulphuric acid was formed, and a mixture of alkaline sulphate and sulphu- Biography of Berzelius. 9 retted metal was obtained. This which Vauquelin was only able to put forward conjecturally, and could not demonstrate by convincing proofs, was immediately proved most satisfac- torily by Berzelius through his successful reduction of sul- phate of potash by means of hydrogen or the vapour of the sulphuret of carbon. He thus obtained sulphuret of potas- sium in which there could not be any oxygen. By treating anhydrous lime with sulphuretted hydrogen at a high tem- perature, Berzelius likewise obtained water and sulphuret of calcium. This experiment rendered it obvious that when liver of sulphur is obtained by melting together sulphur and carbonate of potash, the solution in water contains sulphuric acid, which is not, as Berthollet conjectured, first formed by the decomposition of water, but is a joint product with the liver of sulphur of the reduction of the alkali. Berzelius found, moreover, that the alkaline metals combine in several definite proportions with sulphur forming substances which are all soluble in water. Thus arose the question: What is contained in such a solution ‘—a question, the answer to “which is especially important when regarded in connection with the solutions of metallic chlorides. Is this liquid a solu- tion of the unaltered sulphuret in water, or is the alkaline metal oxidized, and, consequently, a compound of sulphuret- ted hydrogen with alkali formed, or a compound of sulphu- retted hydrogen, sulphur, and alkali? Since, in the last case, it would be necessary to assume as many compounds of sulphur with hydrogen as there are compounds of sulphur with the alkaline metals, Berzelius decided in favour of the second view. Subsequent investigations of the solution of sulphur compounds of the metals of alkaline earths in water, Have, in fact, shewn that a decomposition of water really does take place in this case, and that a compound of metallic sulphuret with sulphuretted hydrogen and alkaline oxide is formed. Berzelius regarded these investigations as proving that sul- phur compounds exist which are very analogous to the mu- riates, and that there might likewise be bodies which, with- out containing an acid and an oxygenous base, possess, like the chlorides, all the peculiar characters of salts; and, con- sequently, if this were so, all that evidence against the new 10 Biography of Berzelius. theory of chlorine fell to the ground which he had derived from the perfect analogy of muriates with salts, which con- sist of an oxygen acid and an oxygenous base. With this investigation of alkaline sulphurets was con- nected the equally important one upon the sulphur salts, which, however, did not appear until several years afterwards. In the former paper Berzelius had directed attention to the fact, that the sulphur compounds of alkaline me- tals and of earthy metals combine with other metallic sul- phurets in the same way as the oxides of these metals com- bine with other oxides. Double sulphurets are thus formed which admit of being compared with ordinary salts, inasmuch as one metallic sulphuret constitutes the electro-positive, that is, the basic part of the compound; the other, on the contrary, the electro-negative part, representing the acid. But here only the lowest sulphurets of the alkaline metals, that is, those corresponding as regards their composition with the basic oxides of these radicals, will fill the place of basic sulphurets ; the higher sulphurets behave, as it were, like peroxides; they may sulphurise other metals, but do not combine with their sulphur compounds. The different stages of sulphuration of the electro-negative metals which Berzelius called sulphides, and whose composi- tion is analogous to that of the metallic acids, combine with the electro-positive or basic sulphurets in such proportions, that if the sulphur were replaced by an equal number of atoms of oxygen, some one of the salts would be formed which the same radicals would yield in their oxidized state. Of the sulphur compounds of the non-metallic elements, those of carbon and hydrogen alone combine with the basic sulphurets of the metals ; the latter class of compounds,— those of sulphuretted hydrogen with alkaline sulphurets,— were already known under the name of hydrothio-alkalies, but their true composition was not recognised until now. Berzelius regarded this extensive series of sulphur com- pounds quite appropriately as salts, and gave them the suit- able name of sulphur salts, in order to distinguish them from the oxygen salts, or those which had been long known, and the so-called haloid salts, under which name Berzelius com- Biography of Berzelius. 11 prised the compounds of chlorine, bromine, iodine, fluorine, and cyanogen, as well as other compound radicals with metals. This discovery of sulphur salts is indisputably one of the most important extensions of chemistry. Berzelius entered upon their study with great industry, and the number of sul- phur salts examined by him amounted to about 120, to many of which he certainly could only give a passing attention, although he analyzed many quantitatively. Next to this followed his investigation of hydrofluoric acid, one of the most important which Berzelius executed, Since it has thrown such an unexpected light upon several of the most interesting departments of chemistry. Thénard and Gay-Lussac had indeed already prepared hydrofluoric acid in a pure state, and several of its com- pounds. But as they were at the same time occupied with a number of other important researches, they did not pur- sue this subject further, and especially did not study with Sufficient accuracy the phenomena which presented them- selves when potassium was heated in fluoride of silicium. Berzelius, in the first instance, prepared the most impor- tant metallic fluorides; then he went on to the remarkable compounds which hydrofluoric acid forms with electro-ne- gative fluorides, especially fluoride of silicium, and fluoride of boron, but also with fluoride of titanium and others. It was through him that we first acquired a correct conception of the composition of hydrofluosilicic acid and the fluosilicates, as well as of the action of water upon fluoride of silicium. But the most productive part of this investigation was when Berzelius repeated the experiments of Gay-Lussac and _ Thénard, for the purpose of decomposing fluoride of silicium by means of potassium. He had just at this time learned from Wohler how to prepare potassium by means of car- bonate of potash and carbon according to Brunner’s method, and thus provided himself with large quantities of this metal. On decomposing fluoride of silicium by potassium he obtained the same results as the French chemists, namely, the brown non-metallic substance which they regarded as a com- plex compound of fluosilicide of potassium and of fluoride of 12 Biography of Berzelius. potassium with silica. Berzelius found that it was impure sili- cium, which, when washed with water, could be obtained free from all fluorine compounds. It then contained only an ad- mixture of silica, which could be extracted by concentrated hydrofluosilicic acid, after having previously been slowly heated to redness. He moreover shewed that the silicium could be obtained in different states of density, and with dif- ferent characters. This unexpected result induced him to undertake similar investigations with fluoride of boron. Weare indebted to him for a correct knowledge of the decomposition of fluoride of boron by water, and of the composition of the fluoborides, as well as an easy method of preparing boron, by treating fluo- boride of potassium with potassium. He likewise disco- vered at this time the gaseous chloride of boron, and correct- ed the views of the composition of boracic acid by his own experiments and those of Arfvedson. He moreover prepared the compounds of fluoride of titanium with metallic fluorides, especially fluoride of potassium, from which body he shewed how metallic titanium was to be obtained by means of potas- sium. This is the only method by which titanium can be obtained in a pure state ; for the experiments of Wohler have proved that the substance found in the slags of iron furnaces, and formerly called metallic titanium, contains nitrogen and cyanogen. The compounds of fluoride of tantalum with me- tallic fluorides were also prepared, and he obtained metallic tantalum in the same way as titanium. He then reduced zir- conium from the zirco-fluoride of potassium by means of potassium, studied the characters of zirconia, and finally turned his attention to the double compounds of fluoride of molybdenum and fluoride of wolfram with metallic fluorides, of which, however, he only prepared the compounds of fluoride of potassium with molybdate and tungstate of potash. Berzelius had intended to pursue these very interesting investigations of fluorine compounds further. But when he found that a distinguished French chemist had also com- menced the study of fluorine compounds, and had already named some newly discovered ones, he gave up his intention. It must be remarked, that in these investigations Berzelius Biography of Berzelius. 13 assumed that fluoric acid was an oxygen acid, and that it con- tained a radical, combined with two atoms of oxygen, as he had previously done in the case of hydrochloric acid. Butin the same year that he gave up his study of fluorine compounds, viz., in 1825, he observed in the first part of the third German edition of his ‘* Lehrbuch,” that it was more probable that fluoric acid, like hydrochloric acid, was a hydrogen acid ; and he described all the fluorine compounds according to this view. Together with these comprehensive researches, Berzelius published a number of less extensive ones. They all origi- nated in his meeting with a number of doubtful statements while editing his ‘“ Lehrbuch,” in reference to which he im- mediately instituted experiments in his laboratory, for the purpose of quickly deciding uponthem. From among these I will here mention only the research upon chloride of lime, which was formerly regarded, according to Gay-Lussac, as a compound of chlorine with lime, and the chlorides of potash and soda were likewise regarded as similar in composition. Berzelius, on the contrary, directly after adopting the view of the elementary nature of chlorine, declared these bleaching compounds to be mixtures of metallic chlorides with salts, containing an oxide of chlorine as an acid. He was of opin- ion, aS he did not closely examine the subject, that the acid was chlorous acid, until the researches of Balard proved that it was hypochlorous acid. Berzelius proved, that all the other explanations of the composition of the bleaching compounds were incorrect, by shewing that these contained an oxide of chlorine. He dis- solved, in a solution of carbonate of potash, as much chloride of potassium as it would take up, and passed chlorine through the liquid without saturating it. After a few minutes chlo- ride of potassium was precipitated, which contained no chlo- rate of potash, or scarcely any; the liquid had acquired the power of bleaching. When the liquid was separated from the precipitated chloride of potassium, and perfectly saturat- ed with chlorine, chlorate of potash was precipitated, con- taining scarcely any chloride of potassium. Consequently, during the first action of the chlorine, chloride of potassium must have been formed from potash, the oxygen of which 14 Biography of Berzelius. could only have combined with chlorine, giving rise to the production of the bleaching compound. It had long been the wish of Berzelius to investigate the rare metals accompanying platinum, the knowledge of which had been left imperfect by the chemists who discovered them. He was enabled to carry this into execution, when, after the discovery of the large quantities of platinum in the Ural, he received, through Herrn von Caucrin, a considerable quan- tity of native platinum, as well as native Osmium-Iridium. This circumstance led him into a very important investiga- tion of the process for decomposing native platinum ores, by means of which the rare metals accompanying platinum were first properly made known. He studied the characters, de- termined the atomic weights of Rhodium, Palladium, Iridium, and Osmium, and prepared a ‘number of their compounds. Owing to the great number of the oxides and chlorides of these metals, and their great similarity to each other, this investigation was very difficult; and, as regarded osmium and osmic acid, a very unpleasant one. But although Ber- zelius himself declared that he had as it were given only the first sketch of the history of these metals, still this re- search, like all that came from his hands, was an extreme- ly accurate, and to a certain extent, perfect one. The next investigation of Berzelius was in reference to a new and peculiar earth, Thoria, which he had discovered in a mineral from Brevig, in Norway. He had previously, on examining the mineral near Fahlun, found an earthy sub- stance in very small quantity, which he regarded, although not with certainty, as a new earth, which he called Thoria ; subsequently, however, he convinced himself that it was phosphate of Yttria. Since the newly discovered earth re- sembled, in some of its peculiar characters, alumina, he called it likewise Thoria; the mineral in which he had detected it, Thorite, and the metal which he obtained from its volatile chlorine compound, Thorium. Thoria belongs to a group of earths which are very similar in their characters to zir- conia, and of which Svanberg, Bergemann, and Sjogren have recently discovered several. At first Berzelius assumed that thoria contained only one atom of oxygen; the experiments, Biography of Berzelius. 15 however, which he made for the purpose of determining the atomic weights of the metal and earth, are probably not quite decisive, and it is perhaps more likely that the earth is com- posed of two atoms of metal and three atoms of oxygen. The next subject to which Berzelius turned his attention belongs to organic chemistry. It was a comparative investi- gation of tartaric and racemic acids. He first corrected his former analysis of tartaric acid, in which he had given an atom more hydrogen than Prout and Hermann, and adopted the results of these chemists. But he then found that the crys- tallised tartaric acid had precisely the same composition as the effloresced racemic acid, and that both acids had the same capacity of saturation,—facts which, especially at that time, were in the highest degree remarkable. This was one of the first clearly demonstrated examples that bodies of different characters may have the same composition. Berzelius had, sometime before, observed a somewhat similar fact in re- ference to the oxides of tin, and Faraday, a short time after- wards, in reference to the compounds of carbon and hydro- gen. Clarke had also discovered the remarkable modifica- tion of phosphoric acid, which he called pyrophosphorie acid. On this occasion Berzelius combined together, in an interest- ing manner, what was known of these bodies, to which he gave the name Isomeric. This term has been universally adopted, now that the number of such bodies has been so greatly increased. From this time Berzelius frequently occupied himself with subjects which are certainly of the greatest interest for every thinking chemist, and indeed for every scientific man, since they are calculated to unfold to us somewhat more fully the nature of matter. He made known his views on this subject repeatedly, both in his “ Jahresberichte,” and in the several editions of his “ Lehrbuch.” Finally, he assumed two essen- tially distinct kinds of isomerism, and, in the strictest sense of the word, called those bodies only isomeric in which the elementary atoms may be regarded as grouped in different ways, forming compound bodies. These isomeric bodies may again be of two different kinds. They consist either of com- pounds which, with equal atomic weights, present different 16 Biography of Berzelius. characters, or of compounds in which, though they possess different characters, the relative proportion of the constitu- ents is the same, but in which the atomic weights are not equal, but twice, thrice, etc., times as great as that of each other. Such bodies Berzelius termed, for the sake of anti- thesis, Polymeric compounds. The other kind of isomerism Berzelius called Allotropism. It refers solely to elementary bodies, which, owing to causes not yet sufficiently understood, assume a different character from that which is usual to them, and, as it appears, retain this difference in many combinations, when it may be the cause of differences in the character of these compounds. When isomeric conditions are observed in compound bodies, which consist of only two elements, combined in very simple proportions, this isomerism is, according to Berzelius, to be regarded less as owing to the different arrangement of the elementary atoms than to the allotropic condition of one or both of these elements ; nevertheless, instances may occur in which both causes are simultaneously at work. It is possible that Berzelius may sometimes have gone too far in his assumption of allotropic conditions, for there are some grounds for believing that an apparent allotropism may result merely from a different state of division. Thus, a few years before the discovery of the first example of isomerism, Magnus observed the interesting fact, that when the oxides of iron, nickel, and cobalt, are reduced by means of hydrogen to the lowest possible temperature, the metals obtained ignite spontaneously, and oxidize when exposed to the atmosphere. This pyrophoric character evidently results from the finer : subdivision of these metals, and it is destroyed when a higher temperature is employed in their reduction, which causes the particles to cohere together. The differences in platinum, according as it is reduced from its salts by the humid process, or obtained by igniting the ammonio-chloride: likewise the unequal combustibility of silicium, and its variable solubility in hydrofluoric acid, may probably be explained in the same way. Nevertheless, Berzelius was inclined to ascribe all these differences to allotropic conditions. Shortly after the appearance of the paper in which Berze- Biography of Berzelius. UT lius treated of bodies which, with the same composition, have dissimilar characters, Dumas went so far as to put forward the bold question, Whether many elementary bodies were not allotropic conditions of one substance, especially such as have the same, or very nearly the same, atomic weight, as nickel and cobalt, platinum and iridium, &c.? Berzelius fa- voured this hypothesis, and regarded it as befitting, that new ideas should be followed up in all directions, even when it is not possible at the same time to adhere strictly to that which is, for the moment, to be regarded as probable ; for truth sometimes appears inconsistent at the first glance, and in any case this was a way to arrive more rapidly at the results which might follow from a new idea. Certainly, upon the other hand, it cannot be denied that the question respecting a relation similar to isomerism between elements which have analogous but still distinctly different chemical characters, belongs to a domain, where perhaps our conjectures will never admit of being put to the proof. The next paper by Berzelius was upon Vanadium. Sefstrém had found a new metal in the bar-iron of Taberg, which he called by this name. He had, however, restricted his in- vestigation to the preparation of the oxide, or rather the acid of this metal, from the finer slags of the Taberg iron, and the determination of its distinguishing characters. He then transferred his stock of Vanadic acid to Berzelius, in order that he might investigate the characters and history of the new metal. This investigation is a very extended one, and through it we have become acquainted with the new body in all its relations; whilst, as these are manifold and interesting, and as the acid has but little resemblance to other acids, it was difficult to assign to it its true position among them. In this respect the paper of Berzelius on va- nadium may almost be compared with that upon selenium ; for both have this peculiarity in common, that by them we have become so thoroughly acquainted with new and hitherto en- tirely unknown bodies, although in both instances but very mi- nute quantities of rare material could be employed, that sub- sequent investigations have added but little more at all, and nothing essential. Vanadium was afterwards found at several VOL. LIV. NO, CVII.—JANUARY 1853. B 18 Biography of Berzelius. places, although always in very small quantities. Wohler directed especial attention to the fact, that the acid of the new metal was contained in the lead ores of Zimapan, in Mexico, in which, as early as 1801, Del Rio discovered a new metal, and called it Erythronium; but, misled by the authority of Collet-Descotils, who declared it to be chromium (with which Vanadium has certainly some similarity), he afterwards admitted that his discovery was an error. His next researches, which were upon Tellurium, were of a similar nature. Berzelius had already instituted experiments with very minute quantities of this metal, in so many respects interesting, but he was compelled to discontinue them for want of material. When Wohler sent him a considerable quantity of this rare metal, which he had prepared from the telluric bismuth of Schemnitz, he again commenced the investigation. He first shewed how this metal can be prepared in its purest state. He then prepared all the compounds of tellurous acid (peroxide), as well of telluric acid, discovered by him, with bases, and indeed the different isomeric modifications which these acids form. These researches are likewise so complete, that they have fully developed the history of this remarkable metal in all its relations. The last great investigation by Berzelius, is that upon meteoric stones. He undertook this with the intention of studying these bodies, as my brother and Nordenskjold had already done, as species of rocks, and, by this means, to de- termine what individual minerals they contained. The im- mediate inducement was a meteoric stone sent to him by Reichenbach, which had fallen a year previously in Moravia. But besides this, he examined three other earthy meteoric stones, and two masses of metallic iron. Berzelius inferred from his analyses that meteoric stones consist entirely of such minerals as are found upon the earth, and that they certainly do not contain any elementary constituent which is not met with in terrestrial bodies. It was only in the meteoric stone of Alais that he found carbon in an unknown state of combi- nation: this stone, when placed in water, disintegrated and fell to powder, which had a mixed smell of clay andhay. This shewed that if, as Berzelius considered, meteoric stones origi- Biography of Berzelius. 19 nated from other cosmical bodies, in their native state they could be converted into clayey mixtures, like the rocks on our own globe. He then raised the question as to whether this carbonaceous earth from the surface of another cosmical body contained organic remains, and consequently, whether there were upon its surface organised bodies, more or less resem- bling those on our earth ? It is easy to conceive the interest with which he attempted to solve this question. This solu- tion was not affirmative, but the results of his experiments did not justify a negative inference. Water and alkalies did not extract anything organic from the meteoric mass; on dry distillation, however, carbonic acid, water, and a blackish- grey sublimate were obtained, but no empyreumatic oil and no hydrocarbon ; the carbonaceous matter was, therefore, not of the same nature as the humus upon the earth’s surface. The sublimate heated in oxygen, gave no carbonic acid or water, and changed into a white insoluble substance, whose nature could not be determined on account of the minute quantity. But to have pronounced it to be an elementary body, not origi- nally belonging to our earth, would have been an exaggera- tion. This was the last extensive research made by Berzelius. His health, which, never strong, had already often necessi- tated the interruption of his labours, became, with increasing age, more delicate, and no longer admitted of his remaining continuously in the laboratory. He suffered, as is not unfre- quent with intellectual men, especially from nervous head- _ aches, which could not be mitigated by the most moderate living. He now began to complain of a failing of the senses, especially his sight, and also of the weakness of his memory. But his scientific activity did not on this account. cease. ‘He interested himself to the last for every branch of chemis- try, and took the most active share in all the achievements of this science. Indeed, now that he was no longer occupied by important practical labours, he concentrated his activity more especially upon undertakings of a literary character, and with a zeal and industry which deserve the greater ac- knowledgment, since his bodily sufferings increased every year. Ba 20 Biography of Berzelius. Among the products of the literary activity of Berzelius, I will here only make especial mention of the different editions of his “ Lehrbuch der Chemie,” and his ‘“ Jahresberichte ueber die Fortschritte der Physikalischen Wissenschaften.” His other works, the lectures upon Animal Chemistry, and his work on the Blowpipe have already been spoken of. The “ Lehrbuch der Chemie’”’ first appeared in Swedish. It was translated into German first by Blumhof, then by Bléde and Palmstedt, and the later editions were translated by Wohler and Wiggers. It was also translated into other languages, but did not pass through so many editions in any, as in the German, for besides the translations of Blumhof and Blode, five editicns have appeared. The last but one, the fourth, consisted, on completion, of ten parts. The fifth and last was commenced by Berzelius in 1842, but was not completed, only five volumes having appeared, certainly very Jarge, each one containing nearly sixty sheets. The inor- ganic chemistry alone is completed. Of the organic part con- tained in the last two volumes, the most pe isi ani- mal chemistry—is wanting. In this work Berzelius has treated very fully of all the facts appertaining to the science, with a remarkable clearness, perspicuity, and apt illustration. At the same time, every Subject is criticised in such an impartia] and just manner as can be displayed only by one who stands as high in science aS he did. The arrangement which he selected is indeed not a strictly systematic one, which, in a science so imperfect as chemistry, can certainly only be called conve- nient. But especially in the inorganic part, there is still a certain well-founded succession, such that it is very easy to ° become familiar with the work. In the organic part the facts are not arranged according to a strict scientific principle, and a classification adapted for inorganic compounds could not possibly be carried out with organic bodies. For although Berzelius had always declared himself strongly in favour of the application to organic chemistry of what we know of the mode of combination of the elements in inorganic nature, as the clue by which alone we could arrive at a knowledge of organic bodies, still he was compelled to admit, that we were Biography of Berzelius. 21 far from having advanced so far as to be able to treat of all organic bodies as radicals, oxides, chlorides, &c., as in inor- ganic chemistry. Most of the assumed organic radicals, often of a complicated nature, are of a hypothetical nature; they gain a somewhat certain character only when some com- pounds of the radical with other simple radicals can be pro- duced, and the oxygen in them replaced by chlorine, sulphur, &e. In addition to this, chemists are of very different opi- nions as to how the composition of organic bodies is to be represented, even when they agree in a fundamental prin- ciple. Moreover, as is natural, the different arrangements vary, according as more new facts are discovered. For the present, therefore, it is at least more advantageous to treat of organic bodies in an elementary work in such a way as Berzelius has done, namely, in groups containing those bodies which have the greatest general similarity in chemical cha- racters. It has frequently been seen, that works in which atheoretical principle has been strictly followed throughout, do not so well fulfil their principal object. In the organic part of his work, Berzelius has declared himself against the so-called substitution theory, and the law of types. He assumes, on the contrary, that conjugate compounds exist in organic bodies, in which, for instance, acids are united with compound radicals, or with their oxides, chlorides, &c¢., in such a way that the acid is not saturated, but is still capable of combining with bases without separa- tion of the associated substance,—the conjunct,—which enters with the acid as a constituent of the salt. When an acid has entered into such a conjugate combination, it has generally acquired such altered characters, that neither the acid nor its _ salts are similar to the free acid and its salts. When hydro- gen is replaced in an organic substance by chlorine, or an- other halogen, this generally takes place in the conjunct and not in the acid, and the former does not on this account cease to play its former part, of modifying the character of the salts into which it enters, with its acids, more or less, and accordingly as its composition is altered by substitution. {t has been asserted that the replacement of hydrogen by chlorine, in organic compounds, was not to be explained 22 Biography of Berzelius. at all in accordance with the electro-chemical views of Ber- zelius, and that consequently these views were incorrect. But when such a substitution takes place, it is, as already mentioned, generally only in the compound radical,—that is, the conjunct, and a newradical is thus formed, in which chlo- rine may perhaps occupy the place of hydrogen, but cannot play the same part as it did. Substitution of elements may therefore be very satisfactorily explained, according to the principles of Berzelius ; and if his theory be impartially com- pared with the others which have been put forward in such number in organic chemistry, the inference will be, that in the present state of the science it is in a position to explain the facts more satisfactorily than any other. On looking carefully through the various editions of this work, it is impossible not to regard it with admiration. It is not only the clear and comprehensive description which attracts,—the sound, impartial criticism, which compels men of opposite opinions to appreciate justly,—or the great mi- nuteness which has not left unnoticed a single fact, however trifling, if it was of any influence—but it is also the enor- mous industry which must create astonishment. A scientific man who had done nothing more than publish this excellent work, in so many editions, each of which was so completely revised that but little of the previous edition was retained, could not be refused by us our grateful acknowledgments of his great industry: and yet this constitutes but a fraction of the achievements of Berzelius. It is touching to call to mind the words with which he concluded the preface to the last German edition, which he could not quite complete; it is dated November 1842. He says, ‘‘ I cannot overlook that, even if the Almighty should grant me life and power to complete the edition of which the first part is now published, this will be the last. For this reason, I considered it necessary to revise it so thoroughly, that I could express the final views which have appeared to me as the most probable during the long space of time in which I was so fortunate as to be able to follow with unin- terrupted attention the development of the science, from the first growth of the antiphlogistic chemistry up to the present Biography of Berzelius. 23 time—fortunate if, among the many views which a future extended experience will alter or correct, at least some few may prove to have been rightly conceived. With the pro- foundest conviction of the uncertainty of our theoretical views as well as of their indispensability, I have endeavoured, in presenting them to the reader, not to inspire him with any more firm conviction of their accuracy than they appear to me to merit, and I have therefore always directed his attention to the uncertainty in the selection of modes of explanation. It is a great obstacle to the progress of science to attempt to cause conviction of the truth of that which is uncertain. What is believed is not submitted to any further examina- tion; and the history of science shews that a deeply-rooted belief in theoretical conceptions has often withstood the most palpable proofs of their inaccuracy. Many of the defenders of Phlogiston required a regular development of the doctrine of oxidation in order to be convinced of its truth, and many distinguished men died believing in Phlogiston.” An undertaking by no means less gigantic than his ‘“ Lehr- buch’’ was the publication of the “ Jahresberichte,”’ which ap- peared regularly from the year 1820 until the death of Ber- zelius. The last completed volume comprises the discoveries of the year 1846. SBerzelius therefore published twenty- seven volumes. After Berzelius had been elected, as successor of the botanist Olaf Swartz, to the office of perpetual secretary of the Aca- demy of Sciences, he succeeded, among other important _ changes which he considered necessary in the statutes of the Academy, in carrying into effect the arrangement that annual reports on the progress made in the various physical sciences should be written by members of the Academy, especially the different curators of the Natural History collections of the Academy, and that these reports should be presented at the annual public meeting held upon the 31st of March, the anniversary, and extracts read from them, after which they should appear in print. Members of the Academy undertook to write such annual reports in the departments of Botany, Zoology, Astronomy, Mathematics, and Technology. Berze- lius himself undertook the reports on Physics, Inorganic 24 Biography of Berzelius. Chemistry, Mineralogy, Vegetable and Animal Chemistry, and Geology. It was only a man like him, who as it were surveyed at one glance the whole range of chemistry, and himself-worked so much in all its branches, that could have adequately exe- cuted such an undertaking. These reports will long remain an example of the way in which such productions ought to be carried out. They were very comprehensive in those depart- ments with which Berzelius was most intimately acquainted, —inorganie chemistry, chemical mineralogy, and vegetable and animal chemistry ; less so in the other parts, which con- tained only the most important discoveries in those sciences with which Berzelius had not especially occupied himself, or which he had not pursued during the latter half of his scien- tific career, such as physics and geology. The reports were generally objectively written. If the views of the author of the original paper corresponded more or less with those of Berzelius, he gave an abstract, proportionate in extent to the importance of the subject, but always most admirable. If, on the contrary, their views differed from his, he allowed himself to express his opinion upon them, and observed a noble and impartial criticism, which rarely became at all violent. In this respect, it is certainly to be regretted that precisely his last “‘ Jahrbericht” closes with an energetic attack upon another celebrated chemist. But Berzelius never mixed up personalities with his judgments; and if some- times one could not agree with them, still they were always of such a nature, that although they occasionally gave pain to those upon whom they were passed, they could never ex- , cite any bitterness. For the science itself these reports were of the greatest value. Berzelius, on several occasions, drew from the investi- gations of others important conclusions, which had entirely escaped the notice of their authors; and as frequently did he direct attention to new experiments which should be made in order to strengthen the results already obtained, or upon which to found new arguments. In this manner he exercised a very beneficial influence. He was also led to make experiments himself by these reports; and he then gave their results, Biography of Berzelius. 25 when they contradicted, improved, or. extended those of others, in the reports. | These reports were especially long when it was necessary to refute opinions and views which Berzelius considered as detrimental to the progress of science. Thus, the reports of the discoveries of the years 1838 and 1839 contain very de- tailed arguments against the hypothesis that all organic acids are hydrogen acids, and against the substitution theory. These arguments have always a rare clearness and simplicity. The objection has often been made to this report, that it was sometimes very complete, and in some instances too extended ; sometimes, on the contrary, especially in the phy- sical part, scanty and imperfect. ‘This 1s certainly true; but it was very natural that Berzelius should have a partiality for the treatment of those subjects in which he especially interested himself and of which he was most master; but as he was almost equally at home in all parts of chemistry, this objection cannot be made to the strictly chemical parts of the reports. With regard to the physical part of the reports, Berzelius had only undertaken it because no other member of the Academy would or could do so. It was only in the years 1838 and 1839 that the report was written by Von Wrede. As Berzelius had only occupied himself with those parts of physics which were intimately connected with che- mistry, it is almost only these parts which are touched upon in his reports. In the same way, there was no other reporter to be found. for the geological part; but as Berzelius had never occupied himself specially with geology, and only in so far as it was connected with chemistry, he treated only of the _ chemical part of that science in his reports, and otherwise noticed only the geological researches referring to Sweden. In the latter volumes reports upon geology are altogether omitted. I have thus attempted to furnish a sketch of the compre- hensive scientific activity of Berzelius. It is probably seldom that science is so greatly advanced through the labours of one man, and there is scarcely any chemist who has furnished such admirable and sound contributions as he. 26 Biography of Berzelius. This representation of his scientific merits would, how- ever, give only a feeble idea of the whole greatness of the man, were we to judge from it alone. It is rare that so perfect a correspondence of mind and character is found in a man as in him. That which so irresistibly attached those who had the happiness to have any long intercourse with Berzelius, was not merely the lofty genius visible in all his researches ; it was not merely the clearness, the aston- ishing copiousness of ideas, the untiring care, and the great industry—the general impression which he made was that of the highest perfection. It was—and every one who knew him intimately will agree with me—it was at the same time those characters which placed him so high as a man; it was the consideration for others, the noble friendship which he evinced towards all whom he considered worthy of it, the lofty disinterestedness, the extreme conscientiousness, the perfect and just recognition of the merits of others ; in short, it was all those traits together which spring from a worthy and honourable character. These were the sentiments which inspired all those who for a longer or shorter time came into contact with him, especially his pupils—of whom our Aca- demy contains more than all the rest of Germany—with the most pious respect for his memory. Berzelius travelled the path of Science together with other distinguished men, who likewise advanced chemistry with giant steps. This was a time such as no other science has yet known, for no other has grown up from its childhood to a certain maturity in so incredibly short a space of time. Berzelius was born almost in the same year as H. Davy and Gay-Lussac. However similar were the labours of these ~ three men in science, they were in other respects very dif- ferent. Davy’s brilliant discoveries, especially that of the metallic nature of the alkalies, gave chemistry an extraordinary impulse, and caused great enthusiasm in its pursuit. He achieved great things by his discoveries, the further following out of which, however, he left to others. He died in the prime of life, but in a certain degree his intellectual blossom was already past. Born poor, he had attained to great Biography of Berzelius. 27 honours and great riches, which were perhaps obstacles to his being subsequently as active for science as formerly. It is, moreover, in the highest degree to be regretted that, in the latter years of his life, his very extraordinary talents were entirely estranged from that science for which he might have achieved so much. Gay-Lussac commenced his scientific career with the dis- covery of an important law in physics, but he afterwards applied himself wholly to chemistry, and advanced it as much by accurate investigations as brilliant discoveries. To him is owing, among other important facts, the law, so important for the doctrine of definite proportions, that gases unite in simple relations of volume,—a discovery of which, however, he did not at first make many applications of which it was capable. But the most brilliant researches of Gay-Lussac are indisputably,—besides those published in common with Thénard on physico-chemical subjects,—the two sets of re- Searches upon cyanogen and iodine. Even independently of the extremely important influence which these researches exercised upon the whole range of chemistry, they may be regarded as models of investigation, both as regards the total results, the strict consistency of the reasoning, and the admirable description. As often as they are read, even at the present day, they will be regarded with astonish- ment. But when, soon after the appearance of his paper upon cyanogen, Gay-Lussac undertook, in conjunction with Arago, the editorship of the “‘ Annales de Chim. et de Physique,” his Scientific activity became gradually less. The first volumes of this Journal certainly contain several small papers and remarks which call to mind the author of those on Iodine and Cyanogen ; but after a few years he ceased to write almost altogether; and it is almost more to be sincerely regretted than in the case of Davy, that Gay-Lussac, who died but a short time since, and after Berzelius, should already in the vigour of life have renounced his active scientific career, which seemed to promise so much. It was not so with Berzelius. He also, after years of po- verty, gradually attained, if not to great wealth at least to 23 Dr Kelaart’s Notes on the Geology of Ceylon. external honours, without having sought them in the least. But these could not estrange him from science; on the con- trary, he took advantage of every higher position for its benefit. Science was always solely the object of his en- deavours, and he never employed them for a purpose foreign to it. So completely was his whole life dedicated to science, that, even under the sufferings resulting from a painful disease during his latter years, his whole thoughts remained bent upon it alone. Such men present in their inspired labours, as it were, the type of the true man of science; and who does not feel him- self happy to meet them in life ? Notes on the Geology of Ceylon.—Laterite Formation.— Fluviatile Deposit of Nuera Elia. By HE. F. Keiaart, M.D., F.L.S., F.G.S., Assistant Surgeon to the Forces. Communicated by the Author. ) Though the geological formations of Ceylon are of a simple nature, and described as such by writers, that attention has not been paid to the laterite formation of the island which it deserves ; some have called it decayed clay ironstone, others have described it to be granitic rocks weathered in situ. It has not, however, been so slightly regarded by Indian geolo- gists ; their more recent researches have discovered new fea- tures in this peculiar formation, which have thrown great doubts as to its being the mere result of disintegrated or de- composed trappean rocks in situ. Captain Newbold of the, Madras Engineers has even gone so far as to suspect it to be of tertiary origin. It is with a view of drawing the attention of observers in this island, for a more complete elucidation of this subject, that this communication is submitted to the Ceylon Asiatic Society. The term laterite (derived from later, a brick) is applied to those masses of reddish clay, more or less indurated, and containing pebbles or crystals of quartz. It is called by the Singalese cabook, and it is used extensively for building purposes. There are several varieties of laterite, and which Dr Kelaart’s Notes on the Geology of Ceylon. 29 admit of classification. 1. Laterite, properly so called, of a hard, compact, almost jaspedeous rock, formed of indurated clay, tubular or sinuous, in which are impacted quartz cry- stals of various sizes and colours; generally of a reddish or brick colour. To this kind, the term Quartzose may be applied, as it contains a larger proportion of undecomposed quartz. The cavities and sinuosities are lined or sometimes filled with a whitish, yellowish or reddish clay. 2. A second variety of laterite, and that most frequently met with in Ceylon, is of a softer consistence, and can be cut easily with a knife, but hardens on exposure to the atmosphere. The term Lithomargic laterite has been applied to this kind. 3. There is another form, which my friend Staff-Surgeon Dr Clark calls Detrital. This is found in nullahs or ravines. It is evidently formed of pebbles of quartz, loosely imbedded in clay, both being washed down to these nullahs by the heavy rains. The detritus of laterite is seen about Colombo form- ing a breccia with marine shells. Women and children and old men are particularly objects for the distribution of blankets. In some instances the men are apt to barter them away for spirits or tobacco. Some of the witnesses considered that none who were able to work should get a blanket, without giving an equi- valent in labour. Captain Fyans, on the other hand, thinks they are sometimes the * 40 On the Condition and Prospects occasion of riot and assassination, and had better not be distributed, or at least not without an equivalent in labour. Mr Wickham says, that blankets seldom remain long in their possession, and considers that a long robe or shirt of blue cotton cloth would be more suitable. This garment would be more decent, and cost but a trifle. Count Strzelecki suggests the justice and humanity of supplying the wants of the Aborigines by a weekly simultaneous issue of rations of bread and meat. Legislation.—The present state of the criminal law with regard to the Aborigines is somewhat anomalous and oppressive. In the first place they are declared subjects of the British Crown,—an honour conferred without either their knowledge or concurrence, and which ‘it is verily believed they have never yet been able to comprehend.” Again, they are accountable to British laws for offences not only against the colonists, but also for those committed among themselves. Ti hey are at the same time legally disqualified from giving evidence in acourt of justice ; a circumstance which, in Mr Robinson’s opinion, has tended to accelerate the destruction of the Aborigines among the whites. Mr Thomas urges the necessity for some special law adapted to their case. Mr Powlett considers that native evidence, when strongly corroborated, might be permitted to go to a jury, to be re- ceived for what it might be thought worth. Count Strzelecki reflects upon the anomalous nature of the whole policy pursued by the government towards the Aborigines, He con- siders they should have been placed more directly under the public authorities, have been supplied with food, and have been declared a conquered race, to render their actual position intelligible to them- selves. Mr Parker recommends some stringent enactments to prevent the prostitution of the native women by the labouring population. He is convinced, from minute inquiry on the subject, that this is the most frequent cause of Aboriginal outrages. At Swan River, an island is appointed exclusively for Rhecpinat criminals ; and according to the reports of the Rotnest establishment, the best results have been realised.* Suitable Agents.—Mr Dredge strongly contends that the Christian missionary is the only qualified party to civilise the Aborigines. Suitable agents should be supplied by the church, a term he would by no means use in a sectarian or exclusive sense. * In consequence of incessant mutual hostility between the Aborigines and the colonists of Van Diemen’s Land, the entire body of the former were hunted out and removed, in the year 1835, to Flinder’s Island, in Bass’s Straits, where the miserable remnant still resides. They numbered 210 on their first arrival, but in 1842, when Count Strzelecki visited the island, they were reduced to 54. There had been only 14 children born during eight years.— (Strzelecki, pp. 352-5,) ee ee of the Aborigines of Australia. 4] 10. Prospects for Aboriginal Civilisation. _ If the prospects of the Aborigines with reference to civilisation are to be estimated by what has hitherto been accomplished, they are miserable indeed. The difference of opinion that prevails on this subject can scarcely relate to the actual results of the past, which have been so uniformly unfortunate; it is due rather to theoretical deductions connected with views and principles of religion. _ Mr Dredge contends that Christianisation must be the pioneer and parent of civilisation, and that all attempts to reverse this process must fail, and always have failed. “ The degradation and moral verétchedness of the heathen are the sad and direful results of moral and spiritual causes; and for their removal the only adequate and appointed instrument is the Gospel, the spirit of Christianity.” He then exhibits the various steps that will be successively taken by these heathens, after the Gospel has begun to operate on their minds, concluding that “it can thus be clearly demonstrated that vital heart- felt Christianity, truly embraced and spiritually enjoyed, develops _the only plan for emancipating the heathen from their moral thral- ‘dom,’’* But judging from past and present experience, these applications of the abstract truths of religion are probably little adapted to forward practically the cause of Aboriginal civilisation. In opposition, also, to the usual views that, the teaching of religion should precede all other modes of Ron, Count Strzelecki remarks that the Aborigines’ institutions being as it were sapped by the preaching of Christianity among them, some civil organisation should have pre- ceded the new faith. But he conceives very slender hopes as to any ultimate good that may result to the Aborigines, from these attempts to initiate them into feelings and habits so widely different from their own. ‘ From what has been observed of the two races, one may _ affirm, without fear of contradiction, that 2 will be easier to bring the whites down to thé level of the blacks, than to raise the latter to - the ideas and habits of our race.” The Australian savage has been suited to the circumstances which surround him, In these he is seen healthful and contented, “ securing all the worldly happiness and enjoyment of which his condition is capable.” But this economy has been disturbed by the arrival of Europeans. He can neither stem the inpouring torrent, nor imbibe the civilisation that is offered him ; he retreats, and finally disappears. Amidst the wrecks of schemes, says the traveller with pathetic elo- quence, there remains yet one to be adopted for the benefit of the Aborigines—to listen and attend to the last wishes of the departed, * Mr Parker speaks to the same effect, adding, that he is well assured there is nothing either in the nature of true religion, or the capacity of the Abori- ginal intellect to exclude this race from a full participation of its benefits.— (Hutracts in Robinson’s Replies, 18.) 42 On the Condition and Prospects and to the voice of the remaining few :—‘ Leave us to our habits and customs; do not embitter the days which are in store for us, by constraining us to obey yours; nor reproach us with apathy to that civilisation which is not destined for us,” 11. General Review. Regard the Aboriginal Australian, as he now appears, surrounded by civilised man. Behold him a wandering outcast ; existing, ap- parently, without motives and without objects ; a burden to himself, a useless cumberer of the ground! Does he not seem pre-eminently a special mystery in the designs of Providence, an excrescence, as it were, upon the smooth face of nature, which is excused and abated only by the resistless haste with which he disappears from the land of his forefathers? Barbarous, unreflecting, and superstitious, how strangely contrasted is an object so obnoxious and so useless, with the brightness of a southern sky, and the pastoral beauty of an Aus- tralian landscape. Such are the reflections that will naturally occupy the mind of the passing observer, after a cursory glance at the wandering tribes of Australia, But the arrangements of Providence for the benefit of the great and varied family of mankind, should not be studied in accordance with one uniform standard of customs and _ institu- tions. The instinctive and mental faculties peculiar to each race, though widely different one from another, may yet exist in perfect accordance with the circumstances by which each is surrounded. To the philosophic traveller who beholds the Aboriginal native in his yet uninvaded haunts, and remarks his health, his cheerfulness, his content, his freedom from anxieties and cares, few spectacles can be more gratifying ;* and he readily admits that the broad and beaten tract of civilisation is by no means the only road which the Creator has left open to man for the attainment of happiness. These mutual relations have been destroyed by the approach of civilised man. In his irresistible progress he has either driven off the Aboriginal tribes, or subdued their native spirit, and subverted their social polity. Their peculiar habits and ideas, the result of physical and psycological laws operating throughout many successive generations, are permanently engrafted in their constitution, and are not to be eradicated without the long continued use of counteracting moral and physical appliances, involving a far greater lapse of time than is usually considered necessary in the estimate of the philan- thropist or the missionary. Deeply feeling the alien occupation of their country, yet their savage arts are utterly powerless against the arms and authority of * Strzelecki, pp. 338, 342, 343, where he describes the real enjoyment of existence among the Aborigines after their own fashon—now moving about, hunting, fishing, with occasional war, alternated by feasting, and lounging on the spots best adapted to repose, —_—_ of the Aborigines of Australia. 43 their opponents. The prostration of spirit, the listless indifference of the Aboriginal mind, are the natural result of this relative position to the whites. The Aboriginal native, widely different in his habits and pursuits, is unable to rise to a comprehension of the actions, motives, and principles that compose the structure of civilisation. Simple in his ideas, his griefs are evanescent, and he is in general cheerful, and even docile and gentle. The vicinity of civilised man acts, after a time, like a powerful spell upon his conduct; but the mind remains radically unchanged ; and when he again returns to the security and undisturbed solitude of his native wilds, this in- fluence is quickly counteracted and thrown off. All efforts to civilise and Christianise the Aborigines have hitherto _ proved singularly abortive. True, indeed, as might be anticipated, the management of the young children presents fewer difficulties than that of the adult natives. There is also with Aboriginal tribes, as with civilised nations, a conspicuous diversity of individual character. They are not all equally fierce or barbarous, or untractable ; and the dark phalanx is occasionally relieved by the advance of some solitary member, whose comparative aptitude and docility have too readily stimulated the anticipations of sanguine and zealous minds. But the care and diligence of the missionary, though they cannot convert the mind of the Australian savage, may yet tame and subdue his spirit ; and by removing, as far as practicable, every known in- ducement to his barbarous customs and wandering habits, maintain him at least in quietness, without injury to himself or the colonists. Isolation and solitude, the total absence of hostile tribes, the pe- riodical and regular supply of food at the missions or stations ; all these circumstances, so different from those in which his habits have been moulded, must gradually weaken that stimulus which gives a zest and pleasure to his erratic and turbulent existence. The savage is deprived of much of the enjoyment congenial to his disposition. But his primitive manner of life is no longer attainable in the present circumstances of the colony. His country has been occupied by a race, whose habits and customs, and daily avocations of life, are to him alike unenticing, irksome, and monotonous, destitute of visible motive or of adequate results. He has neither the desire nor the capacity to associate with the whites; and when he would retreat from their blighting presence, into territories still uninvaded in the progress of colonisation, he is repulsed by other tribes of his own race, who already occupy the locality to which he might retire. His lot is truly hard and unfortunate. The tranquillity of an Australian Savage is not that of enjoyment, but rather of quiescence and torpor. The restraints and deprivations to which, in the attempt to reclaim his mind and habits, it is sought to subject him, are to be excused and justified only in the view, that they are the means of avoiding still greater impending evils. All projects for the civilisation of the Aborigines should be framed 44 On the Condition and Prospects in consonance with the view that in other circumstances than the present, (that is, in the previously undisturbed condition of these tribes,) these appliances for their behoof would be a positive injury and injustice. To remove the Australian savage from all intercourse, whether amicable or otherwise, with other tribes, to anticipate, by a gratuitous supply of food, the necessity for his accustomed corporeal and mental exertion, are simply to undermine the chief sources of the variety, excitement, and happiness of which his existence is sus- ceptible. In the moral and physical conditioy in which the Aboriginal Australian has been placed, even the mutual wars of the tribes must not be overlooked, as incorporated with those various adaptations by which the energy and activity of the mind and body are duly maintained. It is indeed only considerations of a different and a higher character than the mere miseries, great as these may often be, that immediately result from war, that will eventually banish such scenes from the catalogue of human. affairs. In all localities where the Aborigines are peaceably conducted, and contrive to pick up a subsistence sufficient for their wants, it appears advisable to leave them to themselves. In places where the sources of their support are diminished, the women and old men, or, if necessary, all the individuals of the tribe, should be regularly and simultaneously supplied with weekly rations of bread and meat.* All the women and old men, otherwise unprovided for, should be supplied at stated intervals with blankets: to the children may be given the long robe or shirt of blue cotton cloth recommended by Mr Wickham. It cannot, indeed, be considered too great a stretch of generosity on the part of the Colonial Government to supply blankets, at stated intervals, to all Aborigines applying for and properly using them, whose territories have been occupied by the Colonists. Some degree of success may undoubtedly be anticipated in the train- ing of the Aboriginal children, particularly where they can be separated from their parents and tribes. On this principle, the present Ab- original School is conducted at the Merri Creek, near Melbourne, under charge of Mr Peacock. It now contains 14 boys and 7 girls. As its existence dates only from the end of last year, the result of the experiment cannot as yet be decided on ; but the prospects appear favourable. ‘The children are noways deficient in ability in learn- ing to read. 3 The experiment of Mr Tuckfield, at Buntingdale, may also be regarded as successful; namely, that of isolating a single tribe of Aborigines upon a reserve of ground, and separating its members * Tribes which are inclined to be turbulent, are probably best kept in check by a force of Aboriginal police. In the Port Philip Herald, of the 30th of June 1846, an estimate is made of the expense of the Native Police (Aborigines), as compared with that of the Border Police (Colonists), each of the former cost- ing annually £36, 14s. 4d.; each of the latter £53, 7s. If the native Police, therefore, continue to give the same satisfaction as heretofore, there is every inducement to employ the Aborigines in this capacity. ° EEE = -—_ i of the Aborigines of Australia. 45 alike from those of other tribes, and from the colonists, and engaging the various individuals in useful, active, and self-supporting occu- pations, | The means of support should be extended by the Government to each of such descriptions of schools or missions, both by conditional grants of land, and by the assistance of money or rations. Where a locality has been thickly settled with squatting stations, it is indeed highly desirable that the scattered remnants of surviving tribes should if possible be transferred to the care of the missionary. _ In such localities, the Aborigines usually wander about, either begging from or plundering the settlers, and with but little scope or stimulus for the exercise of their primitive manner of life. At the missionary reserve, on the other hand, they would be secured from the disease and dissipation to which their restless habits continually expose them. The plan of the Protectorate is unsuited to the case of the Ab- origines, from the circumstance of the mutual distrust and animosity of the tribes. Another mistake, and of a more evident character, has also been made in committing to the accidents of a civil appoint- ment the responsible and laborious duties attending the work of Christianising and civilising the Aborigines. The, exalted motives, strength, and perseverance of religious zeal, form, generally speak- ing, the only efficient agent in such a work.* It appears desirable, however, except in particular instances, and in the case of the native children, to leave the Aborigines, as far as circumstances will permit, to the free enjoyment of their own mode of life. Interference should be the exception, not the rule, and the apparatus of the Protectorate appears to be no longer necessary. In other respects this establish- ment might perhaps have been continued with advantage under a modified form. The heavy expenses attending it were unavoidable, under any practical arrangements for the civilisation and maintenance of large bodies of the Aborigines. Such of the natives as were not under the special care of mis- _sionaries, or employed by the colonists, might be nominally under charge of the Crown Land Commissioners, who should furnish periodical reports on the numbers and condition of the Aborigines in their respective districts. The services of a few of the magistrates residing in different parts of the colony might be made available for the occasional distribution of such provisions and clothing as the neighbour- ing tribes might be considered to require.;—(Vide Westgarth on the Condition and Prospects of the Aborigines of Australia, in Journal of the Indian Archipelago and Eastern Asia, vol. v. p. 704.) * From the evidence given by the two present assistant Protectors, Messrs _ Parker and Thomas, it is very apparent that they have been actuated in their labours by a missionary spirit, and stimulated by religious zeal. They have in fact been missionaries, operating on an extensive scale. {1 These remarks are intended to apply to the Port Philip District only, which is best known to the writer. J. F. 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Air. of Air, Grs. Grs. January 42:02} 44-28 || 40°62 | 42°34 || 38°92] 39-99 2°58 0°98 February 40°78 | 44:55 || 39°27 | 42°10 || 37:50 | 39-37 2°45 1°32 March 43:16| 46:95 || 41°09 | 44°11 || 38°58] 40-91 2°51 1°37 April 45°66 | 50-26 || 42°65 | 46°35 39°29 | 42°40 2°49 2°45 May 52:24! 54°66 || 47°85 | 49°65 || 438°40| 45°76| +2°76 2°46 June 58°10! 61°04 || 53°78 | 55°54 || 50°79! 51°70! . 3-54 2°52 July 59°89 | 62:08 || 55°45 | 56°48 || 52°35! 62:58 3°64 2°63 August 60°34} 64°51 || 57°19 | 59°41 || 55:00| 56°13} 4°25 2°51 September|| 56°55 | 59°63 || 53-48 | 55°12 || 51:37} 51:93] 3:74 2°03 October 51:94| 54°53 || 50°37 | 51°43 || 48°80] 49:02] 3°50 1:44 November || 38°94 | 42°13 || 37°40 | 39°87 || 35-00 | 37:26] 2°30 1:03 December || 41-71} 43-75 || 40-94 | 42°88 || 40°05] 41:88] 3:05 0°44 1851, 49-27 | 52°36 || 46:67 | 48°77 || 44°25] 45:74| 3:07 1:76 1850, 49°27 | 52-35 || 46-62 | 48°46 || 44°19| 45°17 1849, 52-00 48°21 44:91} 361 1:10 1848, 51:93 48°23 44-98 1847, 51°94 44°12 Remarks. January.—tThe wettest on record at this place. Those months which approach the nearest to January 1851 in point of wetness during the last nineteen years, are December 1853, January 1834, and July 1846, in each of which the fall of rain slightly exceeded 9 inches. At Scathwaite in Borrowdale, the fall was 28°63 inches, and on the “Stye’’ it amounted to no less than 38-86 inches, by far the greatest quantity ever measured in the same period in Great Britain. The mean temperature is 4°66 above the average of the preced- ing eighteen years. February.—Wet till the 19th; fine and clear during the re- mainder of the month, Mean temperature, 2°09 above the average. During January and February, the thermometer reached the freez- ing point on two nights only. March.—Mild, with an unusual absence of easterly winds. Temperature 1°:87 above the average. The temperature of the quarter ending March 31, is 2°-87 above the average. The deaths in the town and suburb of Preston Quarter, are 155, | being three above the calculated average of the preceding twelve — years, allowing for increase in population. April.—A very fine, but somewhat cold month. Sun shone out more or less on 29 days. Mean temperature, 0°57 below the average. Meteorology of Whitehaven. 49 Swallows were seen at St Bees on the 9th, and in the immediate neighbourhood of ‘this town on the 20th. On the 28d, the Cuckoo was heard in various parts of the Lake District. On the 18th, at 6.30 p.m., a magnificent triple rainbow with gorgeous colours. On the 27th, about 10.5 p.m., being in the Ob- servatory, my attention was attracted by a sudden blaze of light illuminating the sky, and on reaching the open air, I perceived a very large comet-shaped meteor proceeding from the head of Draco through Cassiopeia, but I did not see it more than a couple of seconds. The meteor greatly resembled a rocket ; its body might be 14 degrees in length, and it was followed by a long and brilliant train of bluish coloured sparks. JI am told that when first seen, it resembled an ordixary shooting-star. The light of the meteor ex- ceeded that of the full moon, and I feel assured, moderate sized print might have been read by it. It was seen at 10 p.m. in the neighbourhood of Manchester, Rochdale, and other places. ‘It pro- ceeded in (query? from) a south-easterly direction, and, to the eye, the luminous appendage appeared to be twenty yards in length; it was followed by repeated flashes of lightning.” Frequent showers of hail and snow during the latter part of the month; and on the 28th, the Ennerdale mountains were as thickly covered with snow as at any time during the winter. May.—A fine and dry, but ungenial month, Temperature, 2°:13 below the average of the previous eighteen years. On the 3d and 4th, the ground was covered with hail. | June.—Cold and wet till the 26th, which, with one exception, was the first really warm and summer like day in 1851. On the 27th, the maximum of the thermometer rose from 65° to 77°; and on the 28th, 29th, and 30th, it reached 82°, 83°5, and 79°, respectively; and these were the three hottest days during the season. ‘Temperature, 1°52 under the average. On the morning of the 5th, there was frost in Gosforth, and snow on the Enner- dale mountains. All the mountains visible from Keswick were likewise covered with snow. On the 5th, at 4 p.m., there was a smart hail-shower at Whitehaven, which measured ‘04 in the Plu- _viometer. During the month, five parhelia and four solar halos were seen. On the 11th, between 7 and 7.30 p.m., a solar halo and two par- helia were seen at Whitehaven. The sun was surrounded by a ring or halo of a reddish tinge, which intersected two bright spots or discs, one to the right, the other to the left. The parhelion to the left or west side of the sun was somewhat fainter than its com- panion, the cloud being more dense in that direction. Altogether, the phenomenon was visible twenty minutes or upwards. On the evening of the 13th, about half-past 6 o’clock, two very beautiful parhelia were seen by Isaac Fletcher, Esq., from the village of Eaglesfield. The parhelia appeared on each side of the true sun VOL. LIV. NO. CVII.— JANUARY 1853. D 50 J. F. Miller, Esq., on the at a distance of about 23°, and the diffused light in their vicinity was slightly prismatic. A line drawn through the three luminous dises was not parallel to the horizon, but slightly inclined upwards towards the north. The northern parhelion had attached to it a bush of light, 3° or 4° in length, which tended upwards, and evidently formed a segment of a circle, which, if complete, would have had- the sun for its centre, whilst the southern parhelion had a similar luminous appendage of about the same size, stretching downwards, and which, doubtless, was another segment of the same circle. Nearly a quarter of an hour elapsed before the phenomenon en- tirely disappeared. On the evening of the 26th, between 6 and 6.30 p.m., a similar, but much less perfect exhibition of parhelia was noticed by the writer at Whitehaven. On the night of the 22d, about 10 p.m., when in the Obser- vatory, my attention was directed to a singular white serpentine cloud in the NNW., at an altitude of about 15°. The cloud was luminous, and white as frosted silver. Between it and the horizon, separated by blue sky, were two inky black cirrostrati in strong contrast. The luminous cloud was visible about fifteen minutes. The sky was generally clear, and, at midnight, it was perfectly cloudless, but there was no trace of aurora or other visible cause for the appearance, though it was probably of electric origin. June 16, A field of hay in cock near Workington; 28th, first east of bees; 30th, met with glow-worms in Borrowdale. The temperature of the quarter ending June 30th, is 1°-40 below the average. The deaths are 39 below the corrected average num- ber, which is 124. July.—Temperature 1°-06 under the average. On the morning of the 4th, ice of the thickness of half-a-crown was found on the glass of the hotbeds in Holm Rook gardens. The potatoes in the neighbourhood were completely blackened by the severity of the frost. Similar accounts have reached us from Ulver- stone, and various places in this vicinity. Three solar halos were seen during the month. August.—Temperature 0°72 above the average of 18 years. Several bright meteors or falling stars were noticed; one on the evening of the 8th conveyed the impression of such extreme proximity as to resemble a spark from a distant chimney. The grain har- vest commenced in this neighbourhood on the 26th. Several fields near Egremont, and one at Distington, are already cut. September.—A beautifully fine month ; very heavy dews at night. Temperature 0°63 wnder the average. On the dth, the tempera- ture fell 20°°5 in 10 hours, and between the 24th and 25th at 3 — p.M., 18° in 24 hours. During the nights of the 28th and 29th, a — naked thermometer on wool, exposed on a grass-plot, fell 21°5 below the temperature of the air at 4 feet above the ground. The terrestrial radiation is now at a maximum. Meteorology of Whitehaven. | 51 ~ On the 25th, the Borrowdale mountains were capped with snow. The temperature of the quarter ending September 30, is 0°:32 below the average. The deaths in the town and suburb are 92, being 30 below ‘the average number. October.—Mild and wet. Temperature 2”'77 above the ave- rage. Aurore on the nights of the lst and 2d; the latter covered three-fourths of the sky, and it was partisalorly noticed that the streamers did not generally emanate from the horizon, but at vari- ous altitudes above it. One very bright streamer appeared to pro- ceed from Arided, and shot beyond the zenith. A. still more splendid aurora occurred on the night of the 1st October 1850, which is described in my report for that year, published in this Journal. On the 24th, a very singular iridescent phenomenon was witnessed on Windermere Lake, but as the.description of it would occupy too much space in this report, it will probably form the subject of a separate paper. November.—The coldest November on record at this place. The temperature is 4°32 below the average, and a naked thermometer exposed on a grass-plot, fell below the freezing point on 21 nights. December.—A mild but exceedingly dull and damp month. The air Was nearly saturated with moisture, yet the rain-fall did not exceed 1:67 inches. The solar rays pierced through the thick stratum of cloud on 11 days only. The mean temperature of the last quarter. of 1851 is nearly coincident with the average of the preceding 18 years. The deaths are 120, or 15 under the average number. ~ Winds.—In 1851 the winds have been distributed as under :— N., 25 days: NE., 52 days; E., 193 days; Sk., 233 days ; S., 69 days; SW., 89 days; W., 27 days, and NW., 60 days. Weather.—In the past year, there have been 19 perfectly clear days; 195 wet days; 151 cloudy without rain; 276 days on which the sun shone out more or less; 22 days of frost; 5 snow showers, and 13 days on which hail fell. There have also been 9 solar and 4 lunar halos; 5 parhelia ; 1 day of thunder and lightning ; 5 days of thunder without lightning ; 1 day of lightning without thunder ; and 13 exhibitions of the aurora borealis. The mean temperature of the year 1851 is about a quarter of a degree above the average of 18 years, and the fall of rain is 3°83 inches under the mean annual quantity. The deaths in 1851 are 452, being 82, or 18 per cent. under the average number ; the births exceed the deaths by 285, and are 72 above the average of the preceding 12 years, from 1839 to 1850 inclusive. The mortality i in the town and suburb in 1851, with a population of 19,281, is equivalent to 23-4 deaths per thousand, or 1 death in every 49:6 inhabitants. D 2 52 Sir R. I. Murchison on the The average number of deaths in the 12 years ending with 1850, is 503, which, with an assumed population of 18,148, gives 27:7 deaths per thousand, or 1 death in every 86 persons. In 1846, 1847, and 1848 (assumed average population, 18,329), the mean annual number is 694, being 37°8 deaths per thousand, or one in every 26-4 inhabitants, in those exceedingly fatal years. In 1849, the mortality is equivalent to 32:2 deaths per thousand, or 1 in every 31 persons; and in 1850, to 24:9 deaths per thou- sand, or 1 in every 40 inhabitants. The improvement in the sani- tary conditionof Whitehaven during the last two years is very striking, and is probably to be attributed, in a great measure, to the abun- dance and cheapness of food, and to the copious supply of pure water conveyed to the town from Ennerdale Lake. a OBSERVATORY, WHITEHAVEN, November 6, 1852. On the Basin-like Form of Africa. By Sir R. I. MurcHison, late President of the Geographical Society. Geographers will be gratified to learn that a map of South Africa, compiled by our learned associate Mr Cooley, and extending from the equator to 19° S. latitude, is about to appear under the execution of Mr Arrowsmith. With such a valuable document, and with the map of the whole of the Cape Colony, we shall soon have before us a general sketch of the physical features of a large portion of this quarter of the globe. So much, however, has our knowledge increased by the valuable original map of the Cape Colony made upon the spot by Mr Hall (of which Mr Arrowsmith is preparing a reduction), that we are, as I will now endeavour to shew, almost entitled to speculate on the prevailing structure of Africa being similar to that of its southernmost extremity. In support of the general view to which I now call your attention, I must state that it has been suggested to my mind by the explanation of the geological phenomena of the Cape Colony by Mr A. Bain. This modest but resolute — man, having been for many years a road-surveyor in the — colony, had, in all his excursions, collected specimens of the rocks and their organic remains; and, gradually making himself acquainted with the true principles of geology, he — Basin-like Form of Africa. 53 has at length traced the different formations, and delineated them on the above-mentioned map. In this way he has shewn us that the oldest rocks (whether crystalline gneiss or clay-slate, here and there penetrated by granite) form a broken coast fringe around the colony, from the southern to its western and eastern shores, and are surmounted by sand- stones which, from the fossils they contain, are the equiva- lents of the Silurian or oldest fossil-bearing rocks.* These primeval strata, occupying the higher grounds, of which the Table Mountain is an example, and dipping inland from all sides, are overlaid by carboniferous strata, in which, if no good coal has yet been found, it is clear that its true place is ascertained ; and as Mr Bain has detected many species of fossil plants of that age, we may still find the mineral pabulum for the steamers which frequent these coasts. Above all these ancient strata, and occupying, therefore, a great central trough or basin, strata occur which are remarkable from being charged with terrestrial and fresh- water remains only; and it is in a portion of this great ac- cumulation that Mr Bain disinterred fossil bones of most peculiar quadrupeds. One of the types of these, which Pro- fessor Owen named Dicynodon from its bidental upper jaw, is a representative, during a remote secondary period, of the lacertine associates of the hippopotami of the present lakes and waters. The contemplation of this map has, therefore, led me to point out to you how wide is the field of thought which the labours of one hard-working geologist have given rise to, and to express, on my part, how truly we ought to recognise the merits of the pioneer among the rocks, who enables us, however inadequately, to speculate upon the entirely new and grand geographical phenomenon, that such as South Africa is now, such have been her main features during countless past ages, anterior to the creation of the human race. For the old rocks which form her outer fringe, unquestionably circled round an interior marshy or lacustrine country, in which the Dicynodon flourished at a time, when _ Mr Bain himself so styles these rocks in the Map deposited in the Library of the Geological Society. 54 Sir R. I. Murchison on the not a single animal was similar to any living thing which now inhabits the surface of our globe. The present central and meridian zone of waters, whether lakes, rivers, or marshes, extending from Lake Tchad to Lake Ngami, with hippopotami on their banks, are, therefore, but the great modern, residual, geographical phenomena of those of a mesozoic age. The differences, however, between the geo- logical past of Africa and her present state are enormous. Since that primeval time the lands have been much elevated above the sea-level—eruptive rocks piercing in parts through them ; deep rents and defiles have been suddenly formed in the subtending ridges, through which some rivers escape outwards, whilst others flowing inwards are lost in the in- terior sands and lakes; and with those great ancient changes entirely new races have been created. Travellers will eventually ascertain whether the basin- shaped structure, which is here announced as having been the great feature of the most ancient, as it is of the actual geography of Southern Africa (t. e. from primeval times to — the present day), does or does not extend into Northern Africa. Looking at that much broader portion of the con- tinent, we have some reason to surmise, that the higher mountains also form, in a general sense, its flanks only. Thus, wherever the sources of the Nile may ultimately be fixed and defined, we are now pretty well assured that they lie in lofty mountains at no great distance from the east coast. In the absence of adequate data, we are not yet en- titled to speculate too confidently on the true sources of the White Nile; but, judging from the observations of the mis- sionaries Krapf and Rebmann, and the position of the snow- capped mountains called Kilmanjaro and Kenin (only distant from the eastern sea about 3800 miles), it may be said that there is no exploration in Africa, to which greater value would be attached than an ascent of them from the east coast, possibly from near Mombas. The adventurous tra- vellers who shall first lay down the true position of these equatorial snowy mountains, to which Dr Beke has often directed public attention, and who shall satisfy us that they not only throw off the waters of the White Nile to the north, Basin-like Form of Africa. 5d but some to the east, and will further answer the query, whether they may not also shed off other streams to a great lacustrine and sandy interior of this continent, will be justly considered among the greatest benefactors of this age to geographical science ! The great east and west range of the Atlas, which in a similar general sense forms the northern frontier of Africa, is, indeed, already known to be composed of primeval strata and eruptive rocks, like those which encircle the Cape Colony on the south, and is equally fissured by transverse rents. As to the hills which fringe the west coast, and through aper- tures of which the Niger and the Gambia escape, we have yet to learn if they are representatives of similar ancient rocks, and thus complete the analogy of Northern with Southern Africa. But I venture to throw out the general suggestion of an original basin-like arrangement of all Africa, through the existence of a grand encircling girdle of the older rocks, which, though exhibited at certain distances from her present shores, is still external, as regards her vast imterior. | Let me, therefore, impress on all travellers who may visit any part of Africa, that their researches will always be much increased in value, if they bring away with them (as I have just learned that Mr Oswell has done) the smallest speci- mens of rocks containing fossil organic remains, and will note the general direction and inclination of the strata. With no region of the old world have we been till very lately so ill acquainted as Africa. But now the light is dawning quickly upon us from all sides ; and in the genera- tion which follows, I have no doubt that many of the links in the chain of inductive reasoning, as to the history of the successively lost races of that part of the globe, will be made known, from the earliest recognisable zones of animal life, through the secondary and tertiary periods of geologists. Passing thence to the creation of mankind and to the subse- quent accumulations of the great delta of the Nile, we have recently been put in the way of learning what has been the amount of wear and tear of the upland or granitic rocks, and what the additions to the great alluvial plain of Lower 56 Professor Horsford on the Egypt, since man inhabited that almost holy region, and erected in it some of his earliest monuments.* But how |} long will it be before we shall be able to calculate backwards | by our finite measure of time, to those remote periods, in which some of the greatest physical features of this con- tinent were impressed upon it, when the lofty mountains from which the Nile flows were elevated, and when the centre of Africa (certainly all its southern portion) was a great lacustrine jungle, inhabited by the Dicynodon and other lost races of animals *—( Vide Address at the Anni- versary Meeting of the Royal Geographical Society, 1852.) Solidification of the Rocks of the Florida Reefs, and the Sources of Lime in the Growth of Corals. By Professor HORSFORD, of Harvard. I. It is required to ascertain by what processes, chemical or mechanical, or both chemical and mechanical, the surface and the submerged coral rocks have become hardened. By the surface rock is intended that thin brown crust, com- — posed of numerous layers, which is distinguished by great compactness, and a peculiar ring, when, in detached condi- tion, it is struck by a hammer, and which occurs on the ab- rupt ocean side, and more abundantly on the long slopes on the land side of the Keys. By the submerged rock, is intended the rock of oolitie ap- pearance which has solidified under water, and which is of inferior hardness to the surface rock. The surface rock, so called, has, in many places, no longer , the outermost position, though it had at the time of its for- mation. It is, indeed, interstratified with friable light colour- ed limestone. The epithet indicates the circumstances of its ipriation, not its presen pain _—— %* See the account t of the instructive iieaetione of my friend Mr Phong Horner, to ascertain the amount of the successive deposits in the Lower Valley — of the Nile, as given in Jameson’s Edinburgh Philosophical Journal of July 1850. Mr Horner informs me that the researches are now going on vigorously on the site of Memphis, having been already applied to the site of Heliopolis, our Consul-General in Egypt, the Hon. C. Murray, taking a lively interest in — their progress. Rocks of the Florida Reefs. 57 1. We are familiar with the fact that a mixture of quick- lime, water and sand, spread out upon walls and ceilings ex- posed to an atmosphere containing more or less of carbonic — acid, in a few days becomes hard. Analyses have shewn that two chemical phenomena are concerned in the solidification, to wit—the absorption of carbonic acid from the air, forming carbonate of lime (which salt, uniting in equivalent propor- tions with the hydrate, forms, according to Fuchs, a com- pound of great stability) ; and the union of the outer portions of the sand-grains with the lime, forming a silicate. Investi- gation has shewn that sand fulfils mechanically a more im- portant office, by increasing the extent of surface to which the compound of the hydrate and carbonate may attach itself. The latter office may also be performed, and equally well, by pulverized limestone. 2. It is well known that calcareous springs deposit carbo- nate of lime in crystalline forms. The salt had been held in solution by carbonic acid contained in the water. Upon reach- ing the surface, under less pressure and the influence of a high temperature, its carbonic acid is given up, and with it a precipitate of carbonate of lime takes place. The process is exclusively chemical. 3. The value of hydraulic cements is now conceived to de- pend chiefly upon the presence of silica and lime, the oxide of iron having little or nothing to do with the process of solidi- fication. The alumina, in the form of a silicate, yields its silica to the lime, which, for its transportation, requires water. This explains the necessity of its being retained under water periods of variable length, according to the pro- portions of the ingredients. The processes are both chemical and mechanical. 4. Gypsum, from which the two atoms of water of crystal- lisation have been expelled by heat, rapidly hardens upon being mixed with water. This is ascribed to the reunion of the sulphate of lime with the water. Do either of the above processes suggest the method by _which the rocks of the Florida reefs have been hardened ? The facts presented in the furnished specimens are as follow :— 58 Professor Horsford on the The rock formed under water exclusively is composed of grains of size less than that of a mustard seed, which to the naked eye appear quite globular, and of uniform diameter. More carefully examined with a microscope, they are found to be far from regular in form or uniform in size, but pre- sent numerous depressions and prominences. Distributed throughout the intervening spaces is a fine deposit of carbon- ate of lime, which adheres with considerable tenacity to the surface upon which it rests. The surface or crust-rock, though not strictly homogeneous, is composed of particles so minute as not to be distinguished from each other. It dissolves in hydrochloric acid, leaving a flocculent residue. The solution, when evaporated to dry- ness, and ignited, readily redissolves in hydrochloric acid, with only an occasional residue. The solution gives no pre- cipitate with chloride of barium. Nitrate of silver gives, in a nitric acid solution, a white precipitate, soluble in ammonia. The aqueous extract gives to alcohol flame the characteristic soda tint. The powdered rock, dried at 100° C., when heated in a dry tube, gives off water. Thus the qualitative analysis of the incrusting rock shewed it to consist of lime, soda, carbonic acid, hydrochloric acid, water, and organic matter. There were also variable traces of peroxide of iron, magnesia, and silica. The former two were wanting in most of the specimens examined, and the silica in some. Numerous specimens were examined for alumina, without in any instance finding a trace of this sub- stance.* * T examined, also, all the species of coral at my command, without finding a trace of alumina in any of them. The hydrochloric acid solution of the coral was precipitated with ammonia. The washed precipitate was digested for several hours with potassa (previously tested for, and found to be free from, alumina), and filtered. The filtrate was then neutralised with hydrochloric acid, and ammonia added, After standing for several hours, there appeared filaments which were soluble neither in potassa nor nitric acid, and which, ex- amined with the microscope, proved to be paper; they had been derived from the filter. Beside these, there was no precipitate. The quantities employed were, in several instances, from a quarter to half a pound of material. There were examined, Millepora alcicornis; Meandrina labyrinthica, two specimens ; Manicina palmata; Mycedia areolata; Astrea microcosmos, two specimens ; rock subaerial and rock submarine, numerous specimens, an i Rocks of the Florida Reefs. 59 In a quantitative analysis by Homer, and another by Mari- ner, the following results were obtained :— The total loss by prolonged ignition, included organic mat- ter, water as hydrate of lime, and carbonic acid, was as fol- lows :— I, 2°7875 er. lost 1:2687 gr. II. 0:5910 er. lost 0°2600 gr. The water was determined in a chloride of calcium tube, with the aid of a low red-heat and an aspirator. (A heat of 175° C. in an oil-bath, expelled but a very small proportion of the water.) I. 0°7519 or. lost 0°0259 gr. II. 1:2890 or. lost 0:0280 or. The organic matter was determined by washing on a dried filter the hydrochloric acid residue. I, 1:7181 er. gave 0-0028 pr. II. 0°4461 gr. gave 0:0021 gr. The carbonic acid was determined in an evolution flask glass. The results with different specimens varied greatly, and ate far from being satisfactory. I. 0°8605 gr. lost 0°3347 gr. III. 0:1720 gr. lost 00585 or. TI. 0:1745 er. lost 0:0600 gr. IV. 1:6116 or. lost 06277 gr. The lime was precipitated as oxalate and weighed as car- bonate. I. 1:3248 gr. gave 1:2581 gr. II. 0-2550 gr. gave 0°2330 or. The silica was determined in the usual way. I. 1°3245 gr. gave 0:0002 gr. II. 0°3760 gr. gave 0-0005 or. The chlorine of the chloride of sodium was determined as chloride of silver. I. 0:8933 gr. gave 0:0303 gr. IT. 0°6850 gr. gave 0:0101 gr. Expressed in per-cents. we have :— Volatile Matter from . 43:99 w cent. to 45°51 w cent. Water Set ng vated . d'44 Organic Matter ... . 0:16 APE UG | : 34:01 .. § 38°89 Carbome Acid ... . { 34-38 ee { 38-94 Lime xt 51:17 ... 03°12 — Chloride of Sodium 0-04 Sad VO O4 Stlica ee 0-01 Aili sig Ug. It is conceivable that the variability in the carbonic acid 60 Professor Horsford on the and water is due to the more or less advanced stages of change which the rock has undergone. In the ultimate form of limestone all the water existing as hydrate in the earlier stages will have become carbonate. These ingredients permit no action like that occurring in hydraulic cements, in which silica plays an important part ; or like that presented in the hardening of gypsum, in which | sulphuric acid is necessary. To one of the two remaining processes, if to either, must it be ascribed ; and as hydrate of lime is present, it cannot be exclusively assigned to a place with calcareous spring deposits. Now, how could hydrate of — lime be provided from carbonate of lime ? The completeness of the suite of collections provided for me by Prof. Agassiz, has enabled me to answer this question in such a manner as leaves, I think, little room for doubt. On the main land against the Keys, there are depressions © which are filled with water only at long and irregular inter- vals. This water, like that within and about the Keys, abounds with animal life. As the water evaporates, these — animals die, and fall upon and mingle with the coral mud at the bottom. As the beds become more and more completely dry, the layer of mud and animal matter hardens till it forms a mass resembling the surface or crust rock. Of this soft, growing rock, specimens were collected. Agitated with water, it yielded a turbid, foetid solution. Tested with acetate of lead, it betrayed the presence of hy- drosulphuric acid. After standing some hours, a delicate white film was deposited upon the containing vessel, at the — surface of the water, which proved to be carbonate of lime. Test-paper shewed the liquid to be alkaline. The addition — of soda solution set ammonia free, and the addition of chloride of barium and hydrochloric acid shewed the presence of sul- phuric acid. Conceiving this soft rock to be in the condition in which — the solidified crust was at first, the process of hardening seemed of easy explanation. ; The animal matter mixed with the carbonate of lime, con- taining sulphur and nitrogen, besides carbon, hydrogen, and — oxygen, in the progress of decay, which warmth and a small Rocks of the Florida Reefs. 61 quantity of water facilitated, gave, as an early product of decomposition, hydrosulphuric acid; this, by oxidation at the expense of the oxygen of the atmosphere, became water and sulphuric acid. The sulphuric acid coming in contact with carbonate of lime, a salt soluble in 10,600 parts of water, resolved it into sulphate of lime, a salt soluble in 388 parts of water. The carbonic acid set free, uniting with an unde- composed atom of carbonate of lime, rendered it soluble. The nitrogen going over into the form of ammonia, at a later period, decomposed the sulphate of lime, forming sulphate of ammonia and soluble hydrate of lime. This hydrate of lime, with an atom of carbonate of lime, united to form the com- pound in ordinary mortar investigated by Fuchs. The car- bonate of lime in solution from the added carbonic acid, as the water is withdrawn by evaporation, takes on the crystal- line form, giving increased strength and solidity to the rock. That this explanation may serve, in however small measure, for the crust rock on the land slopes of Key West and all localities of a similar character, it is necessary that there be animal exuvie in coral mud, or finely divided carbonate of lime. Both these occur. The water about the Keys abounds in animal life. With the influx of the tide, the slopes became overspread with the water and what it contains in suspension. The retreating water, at ebb tide, leaves a thin layer of the animal matter, mixed always when the water is agitated with the fine caleareous powder. Before the return of flood tide, exposure to the atmosphere and warmth have secured the succession of chemical changes enumerated above, and a thin layer of rock is formed. A repetition of this process makes up the numerous excessively thin layers of which this rock is composed. On the ocean side the deposit is formed from spray, during winds which drive the froth of the sea, containing, with coral mud, the exuviz from the barrier of living corals upon the low bluffs of the Keys.* _ * Professor Dana in a note to his last paper on Coral Reefs and Islands in the July number of this Journal, p. 83, after enumerating briefly the details of the above process of consolidation, remarks :— 62 Professor Horsford on the To these chemical changes must be added the simple ad- mixture of the animal and vegetable matter, which, like “ Tn the first place, his (Prof. H.’s) paper only alludes to the rock formed above low-tide level, which I have called the coral sand-rock. Again, the amount of organic matter in corals, as found by analysis, does not exceed five per cent. ; and the sulphur present in this organic matter, is not over one-tenth of one per cent. It hence appears that the amount of sulphur is altogether in. adequate for such changes. “ But as the sands of the beach (which have a peculiarly white and clear ap- pearance) are washed by the breakers, and the animal matter they contain is either undecomposed within the several grains, or is borne off by the waters, even the animal matter present cannot contribute to the consolidation. The waters of the tides along a sand beach on the open ocean have certainly not been proved to carry in dissolved animal matter for dissemination among the sands.” Two or three points in this note demand attention from me, The first sentence of the first paragraph should be read in connection with the conclusions I. and II., expressed at the end of my paper. In reply to the remainder of the paragraph, the criticism would be just, if I had any where ascribed the solidification, or any part of it, to any action of the organic matter in corals. Since the publication of my article in the Proceedings of the pecdeprer: there have been made quantitative analyses of the more important ingredients of the soft rock, corresponding, as I conceive, with the rock of sub-aerial soli- dification in the first stages of its formation. When first supplied to me, it was of the consistency of well-tempered pottery clay. It is now so hard as to yield only to a severe blow with a hammer, and is, beside, brittle and coated with fibrous crystals of common salt. The following analyses made by Everett and Warren, upon samples differing but little from each other in appearance, have been conducted with great care. They vary, it will be seen, considerably from each other :— Dried at a temperature of 100° C. By prolonged ignition. I. 1:1450 gr. lost 0°0890 gr. 0°8270 gr. lost 0°4870 gr. II. 15325 gr. lost 01175 gr. 1:9020 gr. lost 0°8000 gr. The hydrochloric acid solution left a residue of organic matter. I. 1:1450 gr. gave 0°2930 gr. IJ. 16424 gr. gave 0°2805 gr. The mass, digested in diluted hydrochloric acid, yielded from existing sul- phate upon the addition of chloride of barium to the filtrate, sulphate of baryta. I. 2°3380 gr. gave 0°1040 gr. II. 1°5325 gr. gave 0:1304 gr. The organic matter by itself, oxydated in nitro-hydrochloric acid, with addi- tion of pulverized chlorate of potassa, yielded to chloride of barium a aig tate of sulphate of baryta. I. 1:5325 gr. gave 0°1505 gr. The whole mass oxidated in a mixture of fused nitrate of potassa and car- bonate of soda, yielded to chloride of barium and hydrochloric acid, a precipss tate of sulphate of baryta. . Rocks of the Florida Reefs. 63 mucilage or glue, fills up the interstices, increases the extent of surface, and’ with it the cohesive attraction ; and still I. 2°3090 gr. gave 0:2850 gr. II. 1:4322 gr. gave 0°1550 gr. The hydrochloric acid solution filtered from the organic matter gave a preci- pitate of oxalate of lime, which was determined as carbonate. I. 0:8770 gr. gave 0°4100 gr. Expressed in per cents. the above determinations give of Water, expelled at 100° C. I. 7:77 per cent. II. 7:66 per cent. Average, 7°72 per cent. Total volatile matter, I. 41°17 per cent. II. 42-06 per cent. Average, 41-58 per cent. The following per cents. are estimated upon the substance as dried at 100° C, Sulphur existing as sulphate and soluble in diluted hydrochloric acid. I. 0°65 percent. II. 0°90 per cent. 1:26 per cent. Average, 0:94 per cent. Sulphur in organic matter. Poet, ; ; . ° . . : F 1°45 per cent. Total sulphur of the above determinations, 2°39 per cent. ° Total sulphur by oxidation of the mass, including the organic and inorganic parts. J. 161 percent. II. 1°84 percent. Average, 172 per cent. Average by the two A ei : . . : 2:05 per cent. Lime, I. : . ; 30:09 per cent. Placing side by side the results of the they determinations with the quan- tities which Prof. Dana justly conceives to be inadequate to the changes ascribed, we have, : Per cent. Per cent. Organic matter, . . . . ; 5° 20:16 Sulphur, F ‘ : i _ 0-1 2°05 The conditions of this soft rock, and of the surface or crust rock at the time of its formation, I conceive to have been quite identical. The soft rock is the residue left by spontaneous evaporation of a considerable body of sea-water thrown, with its mingled coral mud and animal matter, into an inland basin, at the rare juncture of favourable high wind and tide. A single layer of the surface rock is the residue left by evaporation of the water mingled with coral mud and animal matter, thrown up in spray from the dashing of the waves, or carried up by flood-tide, and left by evaporation in the interval between the two tides. This will account for its stratification, for its- occurrence on emi- nences as well as in depressions and along abrupt slopes, for its interstratified arrangement with the coarse coral sand; indeed, for all the phases and pecu- liarities of it which are presented in the extensive suite of collections sub- mitted to me. In addition to the changes enumerated in the above paper as resulting from the decay of the animal matter, another may be mentioned. The ammonia - evolved in the process of decomposition, would provide hydrate of lime from _ the sulphate present in the sea-water. This ingredient, taking the average of Bibra’s analysis, is to the chloride of sodium as 1 to 16, and may be conceived 64 Professor Horsford on the further to the decomposition of the organic matter furnishing carbonic acid, which gives solubility to the pulverulent car- bonate of lime. The exceeding fineness of the coral mud is due in part to the stone plants which flourish in the waters within the reef, and which admit of ready reduction to a powder of extreme fineness. Of these, two species of Millepora, I., II., and one of Opuntia, III., were analysed by Mr Scoville in my labo- ratory. I. ire III. ENGR Ag LSS Organic matter, 4°45 4°45 1:26 2°58 4:18 5:72 Carbonic acid, 40°09 39°64 41-08 270 37°68 35°81 Sulphuric acid, 0:0056 0:0056 ae a4 fe. A Lime, 47°71 47°98 46°35 4680 51:81 51:36 Magnesia, 5a ae 6°23 5°90 ae a Water, 3°67 = 330 4°52 mY 5°59 5°92 95°92 95°37 99°44 8 99°26 98°81 The discrepancies in the analyses of the different speci- mens of the same species are due to the circumstance that different parts of the stone plant contain organic matter in unlike proportions; and it is very difficult to procure two to have furnished no inconsiderable amount of hydrate of lime for the process of consolidation. Prof. Dana attributes the formation of this crust-rock which has been the more prominent object of my investigation, to the action of simple rain-water, dissolving the carbonate of lime and again depositing it upon evaporation.* This would account for its occurrence in depressions of the rock, but would not account for its occurrence on eminences or on abrupt slopes; nor would it ac- count for the presence of water as hydrate of lime. The first sentence of the second paragraph of the above criticism has been re- plied to. I have ascribed no solidifying action to the animal matter in corals. In regard to the second:—It will not be questioned that there is a great amount of organic matter in various stages of decomposition about coral reefs. Bibra found organic matter in all the ten specimens of sea-water analysed by him. I have, in the paper above, repeated the statement made to me by the parties who collected the specimens, that the waters within the Keys abound in animal life. That procured for analysis from within the Keys was found ex- ceedingly offensive from the decomposition of animal matter. It yielded the odour and reactions of hydrosulphuric acid, and gave a total amount of organic matter of 2°98 per cent. Now, it is difficult to see how sea-water should fail to carry the animal matter it holds in solution, and more or less of that it holds in suspension into the coral sands, which are saturated at every high water and again drained at low tide. * Am, Jour. Sci. [2], xiv. 67 and 81. Rocks of the Florida Reefs. 65 specimens which, when pulverized, will present homogeneous powders of the same constitution. II. Source of Lime in the Growth of Corals. Marcet,* as early as 1823, observed carbonate of lime in the sea-water near Portsmouth. Jackson} found it in two Specimens of sea-water furnished by the United States Kx- ploring Expedition; one from 600 feet, and the other from 2700 feet below the surface. J. Davyt found the sea-water of Carlisle Bay, Barbadoes, to contain about yz}, 5th part of carbonate of lime. There was found scarcely a trace near the voleanic island of Fayal. Whitel| is of the opinion that it fails only near the surface ; but the elaborate analysis by Bibra,§ of no less than ten specimens taken generally from a depth of twelve feet, but in one instance from a depth of four hundred and twenty feet, in various latitudes.on both sides of the equator, shews quite conclusively that it is not a constant ingredient of sea-water. His analyses do not mention a trace of carbonate of lime. The quantity found by Davy is very nearly that which is soluble in water and is obviously due to the calcareous marl which abounds near the Barbadoes. The water from within the Keys was carefully analysed in my laboratory ; it contained lime and sulphuric acid among its ingredients, but not a trace of carbonic acid. The total want of carbonic acid in a water in which coral life is so luxuriant, suggests naturally that the stone plant, as well as the coral animal, possesses the power of abstract- ing lime from the sulphate; the change being due to double decomposition with carbonate of ammonia excreted from the plant and animal, yielding carbonate of lime, quite insoluble, and sulphate of ammonia of the highest solubility. The building up of the calcareous skeleton becomes, upon this hypothesis, of exceeding simplicity. The surrounding ele- * Annals of Philosophy, April 1823, p. 261. tT Am. Jour. Science, [2] vol. v., p. 47. { Phil. Magazine, [3] xxxv., p. 232. | Ib., p. 308. § Ann. de Chemie et de Pharmacie, Ixxvii., 90. VOL. LIV. NO. CVII.— JANUARY 1853. E 66 Professor Horsford on the ment yields at once to the exhaling carbonate of ammonia the framework of stone. With this view, there is no difficulty in finding a supply of carbonate of lime for the vast masses of coral. The sulphate of lime, decomposed to furnish the carbonate, is perpetually renewed through rivers from the continents and islands. The following inferences are legitimately deducible from this view :— 1st, Corals would soon die in bodies of salt water wholly eut off from the ocean. 2d, They might flourish to some extent in waters accessible to the sea only at high tide. In Dana’s Report on Coral Reefs and Islands,* he states that ‘‘where there is an open channel, or the tides gain access over a barrier reef, corals continue to grow, &c. At Henuake the sea is shut out except at high water, and there were consequently but few species of corals, &e. At Ahit there was a small entrance to the lagoon ; and though com- paratively shallow, corals were growing over a large portion.’ f These facts seem to me to give some support to the view expressed above. It was of interest to ascertain, in the case of corals, whether the formation of new coral without was attended with absorption or partial solution in the interior, and a cor- responding reduction of its specific gravity. Specimens of coral, from the centre, periphery, and midway between, of a * Am. Jour. Science, [2] xii., 34 to 41, and Geol. Report Expl. Exp., p. 63. + In my article, as published in the Proceedings of the Association, I have further quoted from Professor Dana’s papers in support of other inferences de- duced from the foregoing view. I have since learned from the author that I had misconceived the sense in which the quotations were to be understood, and have become satisfied, especially after examination of the map of the Feejee Islands accompanying Professor Dana’s last article, that the inference, that fresh-water streams, by their supply of sulphate of lime, exerted any consider- able influence upon coral formations, is not sustained. The sulphate of lime of sea-water, however, being one-sixteenth of the chloride of sodium, is abundant for the supply of the carbonate of lime, without the aid to be derived from such ~ a source, Rocks of the Florida Ree/s. 67 mass of Meandrina, a foot in diameter, were reduced to pow- der, washed with hot water until the chloride of sodium was all removed, and their specific gravity ascertained by Storer. The average of three specimens from the centre, three from the middle, and two from the periphery, gave the following specific gravities :— Centre. Middle. Periphery. 2.695 2,749 2,785 These results so far support the affirmative of the sugges- tion above, as to make a repetition of the determinations desirable. The chief conclusions to which the above research has conducted are :— I. That the submerged or oolitic rock has been solidified by the infiltration of finely powdered (not dissolved) carbonate of lime, increasing the points of contact; and the introduc- tion of a small quantity of animal mucilaginous matter, Serving the same purpose as the carbonate of lime, that of increasing the cohesive attraction. IJ. That the surface rock has been solidified by having, in addition to the above agencies, the aid of a series of chemi- cal decompositions and recompositions resulting in the for- mation of a cement. And I may add that it lends support to the suggestion, III. That the carbonate of Jime of corals is derived from the sulphate in sea-water, by double decomposition with the carbonate of ammonia exhaled from the living animal.—(Si/- liman’s American Journal, vol. xiv. 2d Series, No. 41, p- 224.) 68 Observations on a remarkable Deposit of Tin-Ore at the Providence Mines, near St Ives, Cornwall. By WILLIAM JorY Henwoop, Esq., F.R.S., F.G.S., Member of the Geological Society of France, &e. Communicated by the Author.* The Providence Mines, in the parish of Lelant, comprise the mines formerly known as Wheal Speed, Wheal Laity, Wheal Comfort, and Wheal Providence, long worked on the eastern side of the hill which slopes from Knill’s monument to the sea. (a) Observations on the eastern workings in the slate, and on the western within the granite formation, have already appeared in the Royal Cornwall Geological Society’s Transactions.| The interme- diate tract, now to be described, is wholly in granite, of which the upper beds are composed of a basis of greyish felspar and quartz, imbedding medium-sized crystals of white felspar, as well as numer- ous small groups of schorl in radiating crystals: but near the produc- tive parts of the lodes the rock is mostly rather coarse-grained, its basis is greenish-grey felspar, black mica, and quartz; and the included porphyritic crystals of felspar are either of a pale buff, a pink, or a reddish-brown hue. (b) These veins are— The Cross-course or Trawn, which bears about 22° W. of N., and dips H.f W. Wheal Comfort lode - 15° W. of N., e and Wheal Laity lode or lodes bs 178; of Ww. 3 8. Connected with the Wheal Comfort lode there is a ‘‘ Carbona,’’§ to which further reference will be made presently. It may be here stated generally, that the Cross-course is from one foot aud a half to two feet in breadth, and is composed of disin- tegrated fine-grained granite, divided by numerous joints parallel to the ‘‘ walls;’’ as well as by many other curved and irregular ones which intersect each other in every imaginable manner, and are filled with oxide of iron, and closely but unconformably striated. The Wheal Comfort lode varies in width, from a few inches to more than six feet. Ata distance from the Wheal Laity lodes it is of granite, very thinly impregnated with tin-ore;—the remainder consists of quartz, schorl-rock (capel), brown iron-ore, and greenish and brownish felspar, in some places,—near the Wheal Laity lodes, —abounding in tin-ore. * For the Paper in full vide vol. vii. of Transactions of the Royal Geological Society of Cornwall. t Vol. v., pp. 16-20; Plate ii., fig. 7; Tables 21 and 22. {t The “ directions” have reference to true north, the “ dips” are from the horizon. § I have already described a similar though a much smaller formation in one of these mines. Corn, Geol. Trans., v., Table 22. : Observations on a remarkable Deposit of Tin-Ore. 69 At about 105 fathoms deep this lode is connected with one of those curious deposits of tin-ore locally called “‘ Carbonas,” * as yet unknown in any other part of Cornwall. The union takes place about 14 fathoms south of the contact between the Wheal Comfort and the Wheal Laity lodes ; and for 10 fathoms above and 20 fathoms below, as well as for the whole distance between the Wheal Laity lodes and the Carbona, the Wheal Comfort lode, when alone, is very productive: but immediately as the Wheal Comfort lode and the “ Carbona’’ separate in descending,—each taking its own downward course,—the lode becomes unproductive, and so also re- mains as far southward as it has yet been traced. At the northern contact of the Wheal Comfort lode and the Car- bona” there is a rich mass of quartz, felspar, schorl, and tin-ore, at least 15 feet in width for about 5 fathoms in length: both south- ward of and below this spot the lode preserves its usual direction and dip; but the “ Carbona’’ southward bears about 5° east of the course of the lode, and holds nearly perpendicularly downward. Descending about 5 fathoms, it abuts on the granite rock, and is seen no deeper; except that as it is pursued southward the irregular granitic bed on which it rests declines at an angle of about 8°. With the exception of a single short string or pipe no trace whatever of the “* Carbona” has rewarded the numerous researches which have been made at greater depths. Nothing can, however, be more irregular than its size and various ramifications, Though the upper edge of the ‘“* Carbona”’ generally continues to touch the lower side (foot-wall) of the lode, in some places the contact is only a few inches, but in others as much as two fathoms and a half wide. Again, in some cases the continuity of the “ Carbona,” where it joins the lode, is almost entirely cut off by intervening masses of ‘ granite ; the union with the main body being still preserved, though merely by “ pipes” or “ pillars’’ of lode-like matter. Many portions of the “ Carbona” are as much as five or six fathoms high; others not more than four or five feet ; some parts are two fathoms and a half wide; whilst others do not exceed six inches. The largest portions are, however, seldom or never entirely separated from each other by the containing rock ; for there is always a sufficient connec- tion to conduct the miner from one large and rich mass to another. The composition of the Wheal Comfort lode has been already noticed : but, notwithstanding their intimate connection, that of the “ Carbona” is widely different, as its tin-ore occurs chiefly in quartz and schorl, which minerals, either separate or mixed, consti- tute the far greater portion of this remarkable deposit. * Some persons pretend to derive this term from the ancient Cornish lan- guage, whilst others suppose it to have been recently coined by the miners. Both the word itself and the metalliferous deposit it is meant to designate are, I believe, confined to the St Ives mining district. Corn. Geo. Trans., v., p. 21, note. 70 W. J. Henwood, Esq., on a Everywhere eastward the Wheal Laity lode is but a single vein of about a foot and a half wide, and composed of quartz, earthy brown iron-ore, greenish, and in some places brick-red, felspar, a little tin-ore, together with some vitreous copper-ore, and iron pyrites. Westward, however, it consists of at least two separate veins, called, for distinction sake, the Wheal Laity north and south lodes ; and sometimes there is also a third vein. At one spot the third vein is simply crystallized felspar, and the axes of the crystals are parallel to each other, but lie across the vein; in other parts it is slightly productive of tin-ore. The Wheal Laity north, and Wheal Laity south, lodes, in general from a foot to a foot and a half in width, are occasionally much wider. Greenish felspar, quartz, schorl, and occasionally brown iron-ore, are their chief ingredients : in some parts both veins are rich in tin-ore ; vitreous copper-ore, copper and iron pyrites also occur, but are not common constituents. In the deepest part of the mine (i. e., at 150 fathoms deep), the Wheal Laity north lode is for some fathoms in length about two feet in width, and is then composed of chlorite, vitreous copper-ore, and iron pyrites, and has a vein of rather fine-grained granite on one side. Ata depth of 120 fathoms, and about 60 fathoms west of the portions already described, where the same lode consists of gra- nite, quartz, red iron-ore, and a little tin-ore, there is connected with its northern side ( foot-wall) an off-shoot or excrescence, about four fathoms in all directions, but most irregular in figure, and having many small vein-like branches. This mass, consisting chiefly of chlorite, quartz, and iron pyrites, is not only far richer in tin ore than the adjoining portion of ‘the lode, but is remarkably different in mineral composition. We have thus the same ore richly im- pregnating, not only the Wheal Comfort lode and the “ Carbona,’’ two parallel but entirely dissimilar deposits, but also the Wheal Latty - lode, which has a direction nearly at right angles to them. (c) The intersections of the lodes just mentioned exhibit almost an epitome of that class of phenomena. (1) The Wheal Laity and the Wheal Comfort lodes cross each other : still at some levels there is no evidence to show that either is cut through; whilst at others the Wheal Comfort lode not only intersects, but also heaves the Wheal Laity lode. . It is not the least remarkable circumstance attending this intersection, that the Wheal Laity lode is a single vein everywhere eastward of the Wheal Comfort lode, whereas westward of their contact it is divided into two, and in some places even into three distinct and separate veins. (2) All these veins are intersected by the Cross-course, and all are heaved by it: the two larger (the Wheal Laity north and the Wheal Laity south lodes) in general from 10 to 15 fathoms: the displacement of the smaller vein is, however, much less considerable, and does not exceed six fathoms and a half, Again, notwithstanding the Wheal Comfort lode and the Cross- Remarkable Deposit of Tin-Ore. 71 course have opposite inclinations, they respectively heave the Wheal Laity lodes in the same direction. Ata depth of 110 fathoms, where the Wheal Laity north lode is for some distance unproductive, whilst the Wheal Laity south lode is rich in tin ore on both sides of the Cross-course, and for some fathoms both above and below the gallery (/evel), the Cross-course consists of a rich vein of tin-ore for the whole interval (five fathoms) between the eastern portions of the two lodes, as well as of a fine mass of the same ore at its contact’ with the western part of the _ Wheal Laity south lode. (3) At 130 fathoms deep the Wheal Laity south lode is also heaved, but in an opposite direction, by a vein of granitic clay (the Flucan), This flucan is not prolonged to either of the other Wheal Laity veins; nor, indeed, does it reach any other gallery (devel) even on the same lode. (4) The Wheal Comfort lode and the Cross- course have the same direction, but, as already observed, opposite inclinations; and are so situated that they come into contact on the line of their dips at about 130 fathoms deep. From the point where they first touch each other they descend perpendicularly side by side for about three fathoms, each keeping the same relative position it had previously when separate (viz., the Cross-course on the west, and the Wheal Comfort lode on the east). At length, however, the lode cuts through the Cross-course. After this intersection, though they have changed sides, and their relative position is reversed, they still proceed together, but now take the line of the lode’s previous under- le for several fathoms. When they separate the lode preserves its dip; but the Cross-course, though it resumes the previous direction of its inclination, dips eastward far more rapidly than before. It may, indeed, be generally observed, that a vein which has been dis- placed by another, whether the intersection be horizontal or vertical, makes (if I may be permitted the expression) an effort to resume its original course. (5) The Wheal Laity lodes are intersected as well by the Wheal Comfort lode and the Cross-course, during their union, as by each of them when separate; the union, however, has little or no influence on the extent of the heave. Many details of local, and some, indeed, of general interest, scarcely need be mentioned here, as this paper may be deemed sup- plementary to my remarks on the Saint Ives District ;* and espe- cially to a deseription of a similar interesting formation at the St Ives Consolidated Mines, which has already appeared in the Trans- actions of the Royal Geological Society of Cornwall.t A small stream issues from the Wheal Laity north lode at 150 fathoms deep, having a temperature of 71°; whilst that of the water VOL Woy Gabe: + Idem, p. 21. 72 Arctic Natural History. discharged by the pump at the adit (45 fathoms from the surface) is only 63° 6’,* The Orchard, Penzance, Oct. 15, 1851. Arctic Natural History. The following interesting statements illustrative of Arctic Natural History we select for the information of our readers. 1. Cause of Intense Thirst in Arctic Regions. 2. Thickness of the Arctic Ice. 3. Warmth of Snow Burrows, 4. Snow a bad Conductor of Sound. 5. The breaking up of an Aretic Iceberg. 6. Refrigerating Power of Icebergs. 7. The droppings of Eider Ducks. 8, Arctic Minute Animal and Vegetable Forms, and Colour of the Sea. 9. On the Flesh of Little Auks and Rotges, and Sea-Fowl generally. 10. Red Snow. 11. On the Colour- ing Matter of Marine Alge, by Dr Dickie. 12. Nostoe Arcti- cum, by Dr Dickie. 138. On the Magnitude of Arctic Glaciers and their advance towards and their termination in the Sea. 14. Ice and Sea-Water Coloured by the Diatomacee. 1. Cause of Intense Thirst in Arctic Regions. After saying farewell to Mr Mecham and his party Mr Stewart returned to the ships in Assistance Bay, where he arrived in the evening a little fatigued, having suffered as usual from excruciating thirst. I believe the true cause of such intense thirst is the extreme dryness of the air when © the temperature is low. In this state it abstracts a large amount of moisture from the human body. The soft and extensive surface which the lungs expose, twenty-five times or oftener every minute, to nearly two hundred cubic inches’ of dry air, must yield a quantity of vapour which one can hardly spare with impunity. The human skin, throughout its whole extent, even where it is brought to the hardness of horn, as well as the softest and most delicate parts, is con- tinually exhaling vapour, and this exhalation creates in due proportion a demand for water. Let a person but examine * Observations on the temperature of other parts of the Providence Mines are recorded in the Society’s Transactions, vol. v., p. 390. 5 . rs , : - a ae ee ee ee ee ee ee eee Arctic Natural History. 73 the inside of his boots after a walk in the open air at a low temperature, and the accumulation of condensed vapour which he finds there will convince him of the active state of the skin. I often found my stockings adhering to the soles of my Kilby’s boots after a walk of afew hours. The hoar frost and snow which they contained could not have been there by any other means except exhalation-from the skin.—(Suther- land’s Journal of Captain Penny’s Voyage to Wellington Channel, in 1850-51, vol. i., p. 404.) 2. Thickness of the Ice. The ships were by this time almost completely banked up with snow, and a gangway of the same material with two parapet walls sloped gradually from the door in the awning to the surface of the ice. The dogs were now located on the ice in a little snow house at the ship’s bow, with a quantity of straw between them and the cold and soft ice beneath. The ice in the harbour was upwards of 2 feet thick. Since the 26th of September, when it was 10 or L1 inches, it in- creased at the rate of half-an-inch per day. The ice on Kate Austin Lake presented the same thickness with that in the harbour, although it was 7 or 8 inches thick when the harbour was one continuous sheet of water. This may appear rather strange, seeing that fresh water freezes at a higher tempera- ture than sea water; but it may be proper to observe that sea water ice, from the saline matter which it contains, will probably conduct the heat faster from the water underneath _ than fresh water ice, and also, that the saline matter, reduced to a low temperature at the surface, sinks while the water is congealing, and cools the stratum into which it descends. The lakes a little beyond the beach, to which allusion has been made already, were frozen to the bottom, although the depth of some of them was more than 2 feet. This is pro- bably owing to the proximity of the ice on the surface with the bottom, which must conduct the heat away from the water laterally, in addition to the action of the air at the surface. It is not improbable that in the centre of Kate Austin Lake the bottom does not present ice even after the winter has de- voted itself to the extension of the ice from the sides towards » 74 Arctic Natural History. the centre. Here, then, we would find a perforation in the frozen crust which envelops the earth’s surface in this high latitude. Were it not so, it is highly improbable that the sal- mon could exist between two ices.—(Sutherland’s Journal.) 3. Warmth of Snow-Burrows. Captain Penny suggested the idea of ascertaining what amount of warmth and comfort could be attained in a close burrow in the snow. In November, a single individual raised the temperature of one from 4°, that of the air at the time, to + 20° in about twenty minutes; but the heat of the snow and the ice must have been much greater than it was at this time. ‘T'wo burrows, each six and a-half feet long, and two and a-half feet wide, were excavated about six inches above the level of the blue ice, in a wreath which had accumulated during an easterly gale. There was a thickness of at least four feet above each from the surface of the snow down- wards ; and the entrances into both were made so as to shut very closely. A thermometer inclosed in one of them for four hours rose to — 2°, the temperature of the external air at the time being — 29°. Two persons, the capacities of whose lungs were represented by 240 and 210, were inclosed in them for an hour and a quarter, at the end of which time the temperature had risen from — 28°, that of the air, to + 3° and — 3° respectively ; the person with the most ca- pacious lungs raising it seven degrees higher than the other. To say the most of the burrows, they were not warm; and closed up in them, as the two persons were, an idea of being buried alive was continually uppermost in their minds. How- ever, there is no doubt, had our circumstances demanded it, we should have overcome this idea, and have appreciated the comforts of burrowing in preference to sleeping in the open air. 4, Snow a bad conductor of Sound. While inclosed in the burrows, the two persons kept up a conversation through the partition of dense snow that inter- vened between them. They had to bawl loudly to one an- other, although the thickness of the partition did not exceed a foot; and when they were spoken to through the doorway, Arctic Natural History. 75 which was securely closed also with firm snow, one had to call out in quite a stentorian voice before a reply could be obtained. The thickness of the slab of snow which closed the doorway was not above nine inches. This is at once a proof of the bad conductor of sound we have in snow. It is very probable that the property of conducting sound dimi- nishes with the density from ice down to the softest snow.— (Sutherland's Journal.) 5. The Breaking up of an Iceberg. When an immense iceberg begins to tumble to pieces and change its position in the water, the sight is really grand,—perhaps one that can vie with an _ earthquake. Masses inconceivably great, four times the size of St Paul’s Cathedral, or Westminster Abbey, are submerged in the still blue water to appear again at the surface, rolling and heaving gigantically in the swelling waves. Volumes of spray rise like clouds of white vapour into the air all round, and shut out the beholder from a scene too sacred for eyes not immortal. The sound that is emitted is not second to terrific peals of thunder, cr the dis- charge of whole parks of artillery. The sea, smooth and tranquil, is- aroused, and oscillations travel ten or twelve _ miles in every direction ; and if ice should cover its surface in one entire sheet, it becomes broken up into detached pieces, in the same manner as if the swell of an extensive sea or ocean had reached it ; and before a quiescent state is assumed, probably two or three large icebergs occupy its place, the tops of some of which may be at an elevation of upwards of two hundred feet, having, in the course of the revolution, turned up the blue mud from the bottom ata depth of two to three hundred fathoms. 6. Refrigerating power of Icebergs. When we lost sight of this iceberg, or, I should rather say, of its ruins, a state of perfect rest had not been ac- quired. One half of it had but turned over upon its side, so that the pinnacled top had become the one side, while the bottom bad become the other; and the other half ap- 76 Arctic Natural History. peared to have been reduced to three or four smaller mas- ses, on the smooth parts of which muddy spots were dis- tinetly visible. When such immense quantities of ice are floating about in and on the sea in Baffin’s Bay, one need not wonder at the low temperature of the water. We very rarely had it above 32°, and at that degree it would hardly effect a per- ceptible change upon the icebergs, although certainly it might dissolve the floating ice of the sea water. The tower- ing ice-bergs, over which the water exercises so little control in this latitude, are the store-houses of cold, carrying it into the depths of the ocean, and there concealing it from the searching rays of the sun.—(Sutherland’s Journal.) 7. The Droppings of Hider Ducks, The droppings of so many large birds accumulating for thousands of years would soon raise an island to a consider- able height above its original level. This happened on several islands on the coasts of Africa and South America; but I do not believe it has ever been found extending to any great distance into the temperate zones, especially the zones of con- stant precipitation of rain, although sea-fowl are sufficiently abundant in those parts to produce it in very large quantities. There is little doubt this is owing to its being washed away by rains or melting snow, or it may be owing to vegetation, by which it becomes dissipated into the atmosphere, or con- verted into a thin coating of brown mould on the rock, in which grasses and other plants take root and flourish luxuri- antly, affording shelter to myriads of flies and their enemies, the spiders, even on and beyond the 74° of north latitude. At the distance we were from the island with the ships the luxu- riant vegetation could be clearly discerned, and in that re- spect it was in the most striking contrast with the rugged and bleak-looking land on both sides of the bay.—(Sutherland’s Journal.) 8. Arctic Minute Animal and Vegetable Forms and Colour of the Sea. Wherever the ice had been very much decayed a dirty “Saaer Soe Arctic Natural History. 77 brownish slimy substance was observed floating in loose jloc- culi amongst it, in the surface of the water. The naked eye could detect in it no structure whatever ; but on viewing a drop of it through a microscope which magnified about two hundred and fifty diameters, it was found teeming with ani- mal life, and minute vegetable forms of very great beauty. Now would have been the time to perpetuate them with the pencil and chalk, but unfortunately I could only consign them to the bottle, with the expectation that their delicate silicious shells would retain their forms until our arrival in England. No one can conceive the vast numbers of these infusorial ani- malcules in the polar seas. Varying in size from 535 to zo'o5 of an inch, a single cubic inch will contain perhaps four or five hundred millions of individuals, each furnished with per- fect instruments of progression. In some of them I could see the cilia in rapid motion, while, to use the words of Professor Jones, “they were swimming about with great activity, avoid- ing éach other as they passed in their rapid dance, and evi- dently directing their motions with wonderful precision and accuracy.’* In others no cilia could be detected; but as they too were seen in motion, although not so often as the others, there is no doubt that they also possess similar delicately constituted organs. ‘UINO *fO1g —SM0d 8.19430 puv ‘T[nq eq 0} pasoddns ‘amis JoS1eyT (*¢) ‘soyemaSpiag “Soq ‘spoom JW (*F) ‘(toyemyserz) spoq uojov[Q ‘uMorg ay (-¢) ‘Y}eaMTISAAA ‘S0q “Teg IW CZ) ‘Soq ysty ‘uerzeyunzy (7) 4 Sh | TL a G+ BG | &g pg fo Ce) | (8) rary “uy | “uty “Uy t'sueuoedg Sunox ‘punry Jo ‘MOss[IN' ‘Jorg “pvoleiog JO a.1N}NS [e1}U99 0} 9409 ULOY euUO Jo di} ay} Woy YSUET eq} Suljqnop sq poureyqo oie syUaMeaNsveul esoyT, x neem sere tala AIC Pad ons ooe eee cee ere °.h P ° > ‘s,10110480d seyApuov [@}1d1990 Jo Wi peaig . ° ° . ° . . e ry ‘6 nys a be 6-9 TLS 8} JO oseq oy} 0} OSpra [eqId1900-eadns woss [[N Ys JO pasted aie te Fe Sa B. 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C.S 3-5 ° . cen ; . . “$}1q.10 JO U}preig #- she ea gar i oes ee a 9.3 9.2 te : : : ‘ : ; . ‘sytqao Jo. re a oe eee a is er 9. 9-¢ or $}1q10 Jo espe raddn 0} sai09 UsOY JO sjoo1 WouZ Sl aa ies gh 8 8 oe 8 8 9.8 ; ‘souoq [eseu 0} oSpr4 Teyidio00-eadns wmoay yySuery ars 9 Tae ae Be cb : ‘ : * u0q Atel IxeulIeyUt JO espe yuoaz 9T 9T LT | 9-81 { 0} ‘esprit yeyidiooo-eadns 04} Wosy [[NYS oy} Jo yySuery (CD | Ce) | CH) Ce) | Ca) | CD) Aren|tirontit ‘on| ‘1 ‘on “UNE UL | surp uy | ary ay | UTE Uy | UE Uy | UTE ey |) erp ey | ory euy | wry uy | cary oy ‘WIR ‘SOY YlIg SUeMO JOIg WOLg || :peesmoN vou puNo; s][nyxG 142 General Results of the Microscopical Examination of Sound- ings, made by the U.S. Coast Survey off the Atlantic Coast of the United States. By Professor J. W. BAILEY, of the Military Academy, West Point. 1st, The most remarkable fact determined by the exami- nation of the above-mentioned soundings is, that in all the deep soundings, from that of 51 fathoms south-east of Mon- tauk Point, to that of 90 fathoms south-east of Cape Hen- lopen, there is a truly wonderful development of minute or- ganic forms, consisting chiefly of Polythalamia, which occur in an abundance rivalling those vast accumulations of ana-. logous forms constituting the marls under the city of Charles- ton, S. C. 2d, While there is a general resemblance between the species found in all the deep soundings above mentioned, the same species of Polythalamia occurring with few exceptions at each locality, yet each place has its predominant species ; thus in the most southerly sounding (H. No. 1, 90 fathoms), there occurs a much greater number of Globigerina than in any of the others; while Textilaria atlantica, although pre- sent, is by no means so abundant as in G. No. 8, 89 fa- thoms. 3d, Infusoria, as well as Polythalamia, occur in the deep soundings ; but the Infusoria are few in number, and consist of Coscinodisci, Galionella sulcata, and other species, which probably swim freely in the ocean; while none of the littoral parasitic species, such as Achnanthes, Isthmia, Biddulphia, Striatella, and Synedra are found. 4th, It is worthy of notice, that in the deep soundings not a single specimen was found of Polythalamia belonging to | the Plicatilia of Ehrenberg (Agathistiques of D’Orbigny’, _ while a number of these forms were found in the shallow — soundings, and they are well known to occur in vast quanti- ties around the shores of Florida and the West India Islands. | This group of Polythalamia appears to have been created — after the deposition of the chalk formation, in which no trace — of such forms occur, while they are very abundant in the © Results of Microscopical Examination of Soundings. 145 tertiary deposits. Their entire absence in the deep sound- ings, where vast numbers of other Polythalamia occur, and their presence in littoral deposits, would seem to indicate that for their abundant development comparatively shallow seas are necessary; thus affording additional evidence of difference in the depths of the seas from which the cretaceous and tertiary bed were deposited. 5th, The deep soundings were all from localities which are more or less under the influence of the Gulf Stream, and it is not improbable that the high temperature of the waters along the oceanic current may be the cause of immense deve- lopment of organic life, making its path, as is shewn by the soundings, a perfect milky way of Polythalamia forms. The deposits under Charleston may have been produced under the similar influence of an ancient Gulf Stream. 6th, From the presence of such great numbers of Polytha- lamia in the deep soundings, there results a very large pro- portion of calcareous matter, thus presenting a striking dif- ference between them and the quartzose and felspathic sands nearer shore. 7th, The littoral sands obtained in shallow soundings at first view appear to give little promise of affording any In- fusoria. But notwithstanding their coarse, and, in some cases, even gravelly nature, they all yield by levigation a considerable-number of siliceous Infusoria, which, in variety and abundance, exceed those found in the deep soundings. 8th, None of the soundings present anything resembling the vast accumulations of Infusoria which occur in the Miocene infusorial marls of Virginia and Maryland; and indeed, I have never found, even in estuaries, any recent deposit at all resembling the fossil ones, in abundance and variety of Species, with the exception of the mud of a small ereek opening into the Atlantic near Rockaway, Long Island. 9th, The occurrence of the pebble of limestone with encri- nal plates in the gravel of F. No. 10, south-east of Little Ege Harbour, is of some interest, as the nearest beds from which it could have come are the Silurian formations of Pennsylvania or northern New Jersey. It indicates a trans- portation of drift to a considerable distance seaward. 144 Co-operation of diferent Nations 10th, In addition to the quartzose grains in the soundings, fragments of felspar and hornblende (recognisable under the microscope by their cleavage planes and colour) are found. The quartz, however, predominates, its grains being sharp and angular in the deep soundings, and often rounded or even polished in the shallower ones. The Reply of the President and Council of the Royal Society, to a Letter addressed to them by the Secretary of State for Foreign Affairs, on the subject of the co-operation of diferent Nations in Meteorological Observations. SOMERSET House, l0th May 1852. Srir,—I have the honour to acknowledge the receipt of your letter of March the 4th, transmitting, by direction of the Earl of Malmes- bury, several documents received from foreign Governments in reply to a proposal made to them by Her Majesty’s Government, for their co-operation in establishing a uniform system of recording meteoro- logical observations, and requesting the opinion of the President and Council of the Royal Society in reference to a proposition which has been made by the Government of the United States, respecting the manner in which the proposed co-operation should be carried out. Having submitted your letter, with its enclosures, to the President and Council of the Royal Society, I am directed to convey to you the following reply. With reference to the subject of well-directed and systematically conducted meteorelogical observations generally, and to the encou- ragement and support to be given to them by the Governments of different countries, the President and Council are of opinion that they are highly deserving of much consideration, not only for their scientific value, but also on account of the important bearing which correct climatological knowledge has on the welfare and material interests of the peop!e of every country. With reference to the proposal for the establishment of a uniform plan in respect to instruments and modes of observation, the Presi-~ 4 dent and Council are not of opinion that any practical advantage is likely to be obtained by pressing such a proposition in the present — state of meteorological science. Most of the principal Governments — of the European Continent, as Russia, Prussia, Austria, Bavaria, and Belgium, have already organised eutdblistivionts for climatological re-— searches in their respective states, and have placed them under the — in Meteorological Observations. 145 _ superintendence of men eminently qualified by theoretical and prac- tical knowledge, and whose previous publications had obtained for them a general European reputation. Such men are Kupffer, Dove, Kreil, Lamont and Quételet ; under whose direction the meteorolo- gical observations in the above-named countries are proceeding ; the instruments have been constructed under their care, and the instruc- _ tions drawn up and published by them under the sanction of their respective governments. The observations as they are made are sent to them, are reduced and co-ordinated under their superintendence, and are published at the expense of the governments. Every year is now producing publications of this nature in the countries referred to, and by the rapid intercommunication of these, the results of. the experience of one country, and the modifications and improvements which experience may suggest, become quickly known to all. To call on countries already so advanced in systematically-conducted meteorological observations, to remodel their instructions and instru- ments, with a view of establishing uniformity in these respects, would probably, if pressed, elicit from other governments also the reply which Her Majesty’s Government have received from Prince Schwarzenberg, conveyed in the Earl of Westmoreland’s letter to Viscount Palmerston, viz., the transmission of a copy of the instruc- tions which have been given to the Meteorological Observatories, forty-five in number, in the Austrian dominions, and a reference to the results obtained at those observatories, which are stated to be in regular course of publication. In an earlier stage, when these establishments were either form- ing or were only in contemplation, it was considered that advantage | might arise from a discussion of the objects to be principally kept in | view, and of the instruments and methods by which these might be most successfully prosecuted. or this purpose, a conference was | held at Cambridge, in England, in 1845, which was attended by |}many of the most distinguished meteorologists in Europe, and amongst them by all the gentlemen whose names are above stated, }and who were expressly sent by their respective governments, The impulse communicated by this assemblage was without doubt highly | beneficial, and the influence of the discussions which took place may | perhaps be traced in some of the arrangements under which the re- | searches in different countries are now proceeding; but in the stage - 'to which they have advanced, it may be doubted whether any mea- )sures are likely to be more beneficial than those which would increase the facilities of a cheap and rapid intercommunication of the results of the researches which are in progress. | With reference “ to the suggestions made by the scientific men of ithe United States,” the proposition of Lieutenant Maury, to give a igreater extension and a more systematic direction to the meteorolo- gical observations to be made at sea, appears to be deserving of the most serious attention of the Board of Admiralty. In order to un- = VOL. LIV. NO. CVII.M JANUARY 1858. K 146 Co-operation of diferent Nations derstand the importance of this proposition, it will be proper to refer to the system of observations which has been adopted of late years in the navy and merchant service of the United States, and to some few of the results to which it has already led. Instructions are given to naval captains and masters of ships, to note in their logs the. points of the compass from which the wind blows, at least once in every eight hours; to record the temperature of the air, and of the water at the surface, and when practicable, at considerable depths of the sea; to notice all remarkable phenomena which may serve to charac- terise particular regions of the ocean, more especially the direction, the velocity, the depths, and limits of the currents: special instruc- tions also are given to whalers, to note down the regions where whales are found, and the limits of the range of their different species. A scheme for taking these observations regularly and systematically, was submitted by Lieutenant Maury to the Chief of the Bureau of Ordnance and Hydrography, in 1842, and instantly adopted: de- tailed instructions were given to every American shipmaster, upon his clearing from the Custom-House, accompanied by a request that he would transmit to the proper office, after his return from his voyage, copies of his logs, as far at least as they related to these ob- servations, with a view to their being examined, discussed, and em- bodied in charts of the winds and currents, and in the compilation of sailing directions to every part of the globe. For some years the instructions thus furnished received very little attention, and very few observations were made or communicated; the publication, how- ever, in 1848, of some charts, founded upon the discussion of the scanty materials which had come to hand, or which could be collected from other sources, and which indicated much shorter routes than had hitherto been followed to Rio and other ports of South America, was sufficient to satisfy some of the more intelligent shipmasters of the object and real importance of the scheme, and in less than two years from that time it had received the cordial co-operation of the masters of nearly every ship that sailed. At the present time, there are nearly 1000 masters of ships who are engaged in making these observations ; they receive freely in return the charts of the winds and currents, and the sailing directions which are formed upon them, corrected up to the latest period. Short as is the time that this system has been in operation, the results to which it has led have proved of very great importance to the interests of navigation and commerce. The routes to many of the most frequented ports in different parts of the globe have been materially shortened, that to San Francisco in California by nearly one third: a system of southwardly monsoons in the equatorial regions of the Atlantic and on the west coast of America has been discovered ; a vibratory motion of the trade-wind zones, and with their belts of calms and their limits for every month of the year, has been determined; the course, bifurcations, limits and other pheno- in Meteorological Observations. 147 mena of the Great Gulf-stream have been more accurately defined, and the existence of almost equally remarkable systems of currents in the Indian Ocean, on the coast of China, and on the North-western coast of America and elsewhere has been ascertained: there are, in fact, very few departments of the science of meteorology and hydro- graphy which have not received very valuable additions; whilst the more accurate determination of the parts of the Pacific Ocean, where the sperm-whale is found (which are very limited in extent), as well as the limits of the range of those of other species, has contributed very materially to the success of the American whale fishery, one of the most extensive and productive of all their fields of enterprise and industry. The success of this system of co-operative observations has already led to the establishment of societies at Bombay and Calcutta, for ob- taining, by similar means, a better knowledge of the winds, currents, _ and the course of the streams of the Indian seas. But it is to the government of this country that the demand for co-operation, and for the interchange of observations, is most earnestly addressed by the government of the United States; and the Presi- dent and Council of the Royal Society express their hope that it will not be addressed in vain. We possess in our ships of war, in our packet service, and in our vast commercial navy, better means of mak- ing such observations, and a greater interest in the results to which they lead, than any other nation. For this purpose, every ship which is under the control of the Admiralty should be furnished with instruments properly constructed and compared, and with proper in- structions for using them: similar instructions for making and record- ing observations, as far as their means will allow, should be sent to every ship that sails, with a request that the results of them be trans- mitted to the Hydrographer’s Office of the Admiralty, where an adequate staff of officers or others should be provided for their prompt examination, and the publication of the improved charts and sailing directions to which they would lead; above all, it seems desirable to establish a prompt communication with the Hydrographer's Office of _the United States, so that the united labours of the two greatest naval and commercial nations of the world may be combined, with the least practicable delay, in promoting the interests of navigation. The President and Council refer to the documents which have been submitted to them, and more especially to the ‘ Explanations and Sailing Directions to accompany wind and current charts” prepared by Lieutenant Maury, for a more detailed account of this system of co-operative observations, and of the grounds upon which they have ventured to make the preceding recommendations. S. Hunter Curistiz, Sec. R.S. H. U. Addington, Esq, K2 148 On the Diurnal Variations of the Magnetic Needle, and on Aurore Boreales. By AUGUSTE DE LA RIVE; being an extract from a Letter to M. ARaGo.* Allow me to communicate to you, with the request that you will make it known to the Académie des Sciences, an extract of a memoir recently read before our Société de Physique et d'Histoire Natu- relle, on the cause of the diurnal variations of the magnet needle, and of Aurore Boreales. In assigning successfully these two classes of phenomena to the same origin, I have but followed the path you have pointed out; for more than thirty years ago you established, with indefatigable perseverance, by your numerous observations, the remarkable agreement which prevails between the appearances of the aurora borealis and the disturbance of the magnet needle. The following is my theory,—you will observe that it rests solely upon well ascertained facts, and on principles of physics positively established. IT had already, in 1836, in a notice upon hail,} attempted to shew that the atmospheric electricity owes its origin to the unequal distri- bution of temperature in the strata of the atmosphere. It is well known that, in a body of any nature whatsoever, heated at one of its. extremities and cooled at the other, the positive electricity proceeds from the hot part to the cold, and the negative electricity in the con- trary direction; it thence results that the lower extremity of an — atmospheric column is constantly negative, and the upper one con- stantly positive. This difference of opposite electric conditions must be so much the greater, the more considerable is the difference of — temperature ; consequently more marked in our latitudes in summer — than in winter, more striking in general in the equatorial than in the polar regions. It must be observed that the negative state of the lower portions of the atmospheric columns must be communi- — cated to the surface of the earth on which they repose, whilst the positive state of the upper portions is diffused, more or less, from above downwards, through nearly the whole of each of the columns, according to the facilities offered by the greater or less degree of humidity of the air to the propagation of the electricity. An at- mospheric column, therefore, resembles a high-pressure battery, on account of the imperfect conductibility of the elements of which it — is composed, A battery, the negative pole of which is in constant — and direct communication with the terrestrial globe, discharges itself — upon the globe, whilst it becomes itself charged with the electricity — of its positive pole, which is distributed over it with an intensity de-_ ¥ * From the Annales de Chimie et de Physique, for March 1849, +t Bibliotheque Universelle, vol. iii. p. 217. Nouvelle serie. Diurnal Variations of the Magnetic Needle. i49 creasing with the distance from this pole; this explains why the positive electricity increases with the height of the atmosphere. The causes which determine the accumulation of negative electri- city at the surface of the earth, and of positive electricity in the upper regions of the atmosphere, act in a continuous manner: there should thence result an unlimited tension of the two opposite electric states, if, having attained a certain degree of energy, they did not neutralize each other by the aid of different circumstances. In other words, having reached a certain limit of tension which varies with the state of the atmosphere and the surface of the earth, the two electricities cannot go beyond it, and unite or neutralize each other as regards the excess over that limit. This neutraliza- tion is effected in two ways, in a normal or constant manner, and in an irregular and accidental manner. This second mode is exhibited under a variety of forms; some- times it is simply the humidity of the air, and better still, the rain or snow, which re-establish the electrical equilibrium between the earth and the atmosphere; in some cases waterspouts manifest in an energetic form the mutual action of the two electricities, which tend to unite. Sometimes the winds, by mixing the air in contact with the surface of the earth, and like it negative, with the positive air of the more elevated regions, give rise to sheet-lightning, or to storms, when there is at the same time a formation of clouds and condensa- tion of aqueous vapours, owing to the humidity and different tempera- ture of the strata of air which become mixed. The attraction of clouds by mountains, the luminous phenomena exhibited at the ex- tremity of elevated points, are likewise due to the same cause. But I will not stop to discuss further all these natural and intelligible consequences of the theory which I expound. I shall confine my- self to one single remark, which*is, that we must bear in mind, that in observations of atmospheric electricity, the intensity of the electric signs perceived is not always a proof of the intensity of the electri- city itself; for the humidity of the atmosphere, by favouring the propagation of the electricity of the upper strata, may give rise, as is frequently seen in winter, to very powerful electrical manifestations even when the cause producing them is not very powerful. The contrary is frequently seen in summer. I now pass to the regular and normal mode of neutralization of the two electricities. I had already suspected the existence of this mode in my notice of 1836; but I did not announce it positively, because there was then wanting a fact, which science now possesses, viz., the perfect conductibility of the terrestrial globe, with which the employment of the electric telegraph has made us acquainted. To make it understood how I conceive this mode of neutralization, I divide the atmosphere into annular strata parallel with the equa- tor; the positive electricity accumulated at the external portion of this layer cannot exceed a certain degree of tension without traver- ~~ 150 Diurnal Variations of the Magnetic Needle. sing rarefied and more or less humid air until it reaches the polar regions, where finding an atmosphere saturated with humidity, it will combine readily with the negative electricity accumulated on the earth, We have thus the circuit formed; each annular stratum of the atmosphere gives rise to a current, which proceeds, in the elevated regions, from the upper portion of the stratum towards the pole, re- descends to the earth through the atmosphere surrounding the poles, and returns by the surface of the globe from the pole to the lower part of the stratum from which it started. These currents will constantly be the more numerous, and the more concentrated, the nearer we approach the pole; and as they all proceed in the same direction, that is to say, from south to north, in the upper portion of the atmosphere, and from north to south on the surface of the earth, their effect will become the more perceptible in proportion as we leave the equator and approach the pole. But as the currents pro- duced by the equatorial strata are individually stronger than those proceeding from more northerly strata, the difference, although real, will notwithstanding be less than would be believed. What passes in our northern hemisphere must occur in exactly the same manner in the southern hemisphere ; the currents proceed equally from the equator to the pole in the upper regions of the air, and from the pole to the equator on the surface of the earth; consequently, for an observer travelling from the north pole to the south, the current would proceed in the same direction from the northern pole to the equator and in a contrary direction from the equator to the southern pole: I speak here of the current circulating on the sur- face of the earth. 1 ought, moreover, to observe that the limit which separates the regions occupied by each of these two great currents, is not the equator properly so-called, for it must be vari- able; it is, according to my theory, the parallel between the tropics which has the sun at its zenith; it changes consequently each day. Now, it is‘easy to conceive the cause of the diurnal variations of — the magnetic needle. In conformity with the laws established by Limpére, the current which proceeds from the northern pole to the equator ought to cause the north pole of the needle to deviate to the west, which is what takes place in our hemisphere; and the current which proceeds from the southern pole to the equator should cause the north pole of the needle to deviate to the east, which is precisely what occurs in the southern hemisphere. The deviation should be in one and the same place; the more considerable the greater the difference of temperature, and consequently of the elec- tric conditions between the lower and the upper stratum of the atmo- sphere; thus the deviation increases from the morning to 1° 80" — p.M. It is more considerable in those months during which the sun is longer above the horizon; it is at its minimum in the winter — months. Lastly, these diurnal variations increase in magnitude in — proportion as we recede from the equator and approach the pole ; Diurnal Variations of the Magnetic Needle. 151 a result which again perfectly agrees with what I have stated re- specting the increase in number of the currents towards the polar regions. In these regions themselves, the variations may be very irregular, and: may be entirely absent if the magnetic needle happens to be placed in those very localities where the electric cur- rents traverse the atmosphere to reach the earth ; in fact, a needle surrounded thus on all sides by currents, is no longer affected by them, or at least is no longer affected in a regular manner. This remark may explain certain observations, especially those made at Port Bowen, which appeared rather exceptional. On examining carefully all the magnetic observations I was able to consult, and in particular those of Colonel Sabine, I was espe- cially struck by the remarkable manner in which they agreed with my theory. I will cite but one example—the observations recently made at St Helena, and just published by Colonel Sabine. At St Helena, the diurnal variation occurs to the west, as long as the sun is to the south of the island, and to the east, as soon as the sun is to the north. In fact, in the first case, as I have previously observed, St Helena must form part of the region in which the electric currents proceed on the surface of the earth from the north pole to the equatorial regions; and, in the second case, it forms part of the region in which these currents pass from the south pole to the equator. The hour of the maximum of the diurnal variation is not the same at the island of St Helena as in the continental countries, which is owing to the temperature of the surface of the ocean not following the same laws in its diurnal variations as the temperature of the surface of the earth. Now, the temperature of the lower stratum of the atmospheric column is always that of the surface of the ocean, or of the soil on which it rests. This cireum- stance explains certain apparent anomalies exhibited by the diurnal variations in some parts of the globe; as for instance, at the Cape _ of Good Hope, which is surrounded almost on every side by a vast extent of ocean. I wish it to be understood that in the preceding I have only taken notice of the causes disturbing the direction of the magnetic needle, ‘and not of the cause of this direction itself; that is to say, of terres- trial magnetism—a cause which I do not at all believe to be of the same nature, but upon which I at present express no opinion. I am content to consider the terrestrial globe as a large spherical magnet, and to study the external causes capable of modifying the direction which it tends to impart, in its quality of magnet, to mag- netic needles. Now, what is the aurora borealis, according to the theory which I have just expounded ? It is the luminous effect of electric currents avelling in the high regions of the atmosphere towards the north le, an effect due to the combination of certain conditions which 152 Diurnal Variations of the Magnetic Needle. are not always exhibited in the same manner, nor at all seasons of the year. It is now well proved that the aurora borealis is an atmospheric phenomenon, as we long ago suspected. The name of magnetic storm, by which Von Humboldt designates it in his Cosmos, implies the same idea, which is moreover confirmed by the interesting de- tails which he gives of this meteor. The observations of Parry, Franklin, and especially those of MM. Bravais and Lottin, so nu- merous and carefully made, are likewise quite favourable to this opinion, which followed equally from the observations of M. Biot at the Shetland Isles. Admitting this point, I explain the production of the aurora borealis in the following manner :—When the sun having passed into the northern hemisphere, no longer heats so much our hemi- sphere, the aqueous vapours which have accumulated during the sum- mer in this part of the atmosphere begin to condense; the kind of humid cap enveloping the polar regions extends more and more, and facilitates the passage of the electricity accumulated in the upper por- tions of the air. But in these elevated regions and especially at this period of the year, the aqueous vapours must most frequently pass into the state of minute particles of ice or snow floating in the air, similar to those which give rise to the halos; they form, as it were, a kind of semi-transparent mist. Now these half-frozen fogs con- duct the electricity to the surface of the earth near the pole, and are at the same time illumined by these currents or electric discharges. In fact, all observers agree in asserting that the aurora borealis is constantly preceded by a mist which rises from the pole, and the margins of which, less dense than the remainder, are coloured the first ; and indeed it is very frequent near the pole in the winter months, and especially in those where there is abundance of vapour in the air. For it to be visible at great distances from the pole, it is necessary that these clouds, composed of frozen particles, extend in an almost uninterrupted manner from the polar regions to some- what southern latitudes, which must be of rare occurrence. These same clouds, when they are partial, which is frequently the case, produce the halos. Now the analogy pointed out by nearly all observers between the mists which accompany the aurora borealis and those which produce the halos, is a somewhat remarkable circumstance. It is easy to verify by direct experiment the identity which exists between the — light of the aurora borealis, and that obtained by passing a series of electric discharges into rarified air containing a large quantity of aqueous vapour, and especially through a very thin layer of snow, or a slight layer of hoar-frost deposited on the glass. I have ascer- — tained that highly rarefied, but perfectly dry air, gives but a very faint light, and that in the experiment of the vacuum tube it is e Diurnal Variations of the Magnetic Needle. 153 sentially the moisture adhering to the inner sides of the tube, which, by conducting the electric discharges, gives rise to the luminous effects. It will be conceived that the electric discharges transmitted by this kind of network of ice must, on becoming concentrated near the pole, produce there a far more brilliant light than they develop when they are distributed over a much greater extent. But why does the magnetic pole, and not the terrestrial pole, appear to be the cause of the phenomenon? Here is my answer. Place the pole of a powerful electro-magnet beneath a large surface of mercury; let this surface communicate with the negative pole of a powerful battery ; bring near to it the point of a piece of charcoal communicating with the positive pole of the battery ; immediately the voltaic arc is formed, and the mercury is seen to become agitated above the electro-magnet; and wherever this is placed, luminous currents are observed to rotate around this pole, and throw out from time to time some very brilliant rays. There is always, as in the case of the aurora borealis, a dark portion in the form of a circular point over the pole of the magnet: this peculiar effect disappears without the voltaic light being interrupted when the electro-magnet ceases to be magnetised. With a continuous current of ordinary electricity arriving at the pole of a powerful electro-magnet in rare- fied and moist air, luminous effects, still more similar in appearance to those of the aurora borealis, are obtained. These phenomena result from the action of magnets on currents : now the same should apply to the action of the magnetic pole of the earth ; the neutralisation of the two electricities probably takes place - over a somewhat large extent of the polar regions; but the action of the magnetic pole causes the conducting mists to rotate around it, sending forth those brilliant rays which, by an effect of perspec- tive, appear to us to form the corona of the aurora. The sulphu- reous odour, and the noise which is said sometimes to accompany the appearance of the aurora, would not be inexplicable; for the odour would be due, like that which accompanies lightning, to that modifi- eation which the passage of electric discharges produces upon the oxygen of the air, which M. Schonbein has called ozone; while, as regards the noise, it would be analogous to that which, as I have shewn, the voltaic arc produces when it is under the influence of a very near magnet. If it seldom occurs in the case of the au- rora, it is owing to its being very rare that the luminous arch is sufficiently near the earth, and consequently to the pole. However, the description which has been given of this noise by those who have heard it, is perfectly identical with that which I have given, without suspecting the analogy, of the noise which the voltaic arc produces in the action of the magnetism. The magnetic disturbances which always accompany the appear- ance of an aurora borealis are now easily explained. This accidental union of a greater proportion of the accumulated electricities must 154 Diurnal Variations of the Magnetic Needle. derange the normal action of the regular current; with respect to - the directions of the disturbance, it will depend on the portion of the current acting upon the needle, and consequently upon circumstances impossible to foresee, since they depend on the extent of the pheno- menon, and the position of the needle in relation to it. In fact, according as the horizontal plane in which the declination needle moves, comprises above or below some of the region in which the greatest activity of the phenomenon takes place, it will be either the current circulating on the earth, or that travelling in the air (cur- rents which proceed in a contrary direction), which will act upon the needle: even during the same aurora, it may be sometimes one, some- times the other of these two currents which will act. The variable directions in which the needle is deflected during an aurora borealis agree very well with this explanation, at least as far as I have been able to judge from the different observations published in the An- nales de Chimie et de Physique, and in several scientific voyages. The remarkable effect observed by M. Matteucci in the apparatus of the electric telegraph between Ravenna and Pisa during the magni- ficent aurora of the 17th of last November, fully proves the exist- ence of a current circulating on the surface of the earth, and which, ascending the wire of the telegraph, passed in part through this better conductor, The sounds which long iron wires, strung in the direction of north to south, give out under certain meteorological cir- cumstances, are undoubtedly a proof that they are traversed by a current which is probably derived from the currents circulating on the surface of the earth from north to south in our hemisphere. It would be highly interesting and important to profit by those telegraphic wires, which are found to have a direction more or less approaching to that of the declination needle, in order to make with them, when they are not in use for ordinary purposes, some obser- vations which would enable us to demonstrate and to measure the electric currents which probably traverse them ; it would be: easily accomplished by means of a multiplying galvanometer, by com- pleting the communication of these wires with the earth at one of their extremities. The comparison of the results obtained in this manner with these furnished by the simultaneous observation of the diurnal variations of the needle, would certainly present considerable interest, and might lead to meteorological results of a remarkable nature. I cannot conclude this abstract without drawing attention to the circumstance, that M. Arago had already pointed out in 1820, shortly after Girsted’s discovery, the possibility of acting upon the voltaic are by this magnet, and the analogy which might result between this phenomenon and that of the aurora borealis. 155 Meteorological Phenomena in connection with the Climate of Berlin. Translated by Mrs ANNE RAMSDEN BENNETT from the German of Professor Dove. Attention has generally been awakened to atmospherical appear- ances, where the usual course of nature has been intercepted by striking meteorological phenomena. The cloudless serenity of a tro- pical sky, and the regular recurrence of periodical changes, attract little observation. The interest which meteorology excites is much more directly associated with uncertainty of weather. It would scarcely occur to any one here to begin a conversation with the re- mark, that the sun had really set at its appointed time ; and as little would it occur to any one in tropical climates to make the weather a subject of conversation. It is for this reason we possess so few meteorological observations on more favoured climates. How, in- deed, could it be expected any one should note down changes which regularly take place at certain periodical times. . He alone feels prompted to such a course who finds himself transported out of the variable conditions of one atmospherical life into the untroubled re- gularity which distinguishes tropical regions ; and which appears to him in such striking contrast with the weather to which he has been accustomed, that he requires the confirmation afforded by meteoro- logical instruments before he can trust the immediate evidence of his senses. For this reason we so often acquire a more accurate knowledge of the peculiarities of a climate from travellers resident in it for only a short time, than we do from the partial accounts given us by its inhabitants. The only disadvantage which results _ from this is, that the lively imagination of strangers makes the con- trasts appear too striking; thus dwellers in the north see every- thing in the south through a rose-coloured medium; and in like manner, we rarely forget, when reading Tacitus’s description of Germany, that it is an Italian who is speaking of our native land. The uniformity which distinguishes tropical climates is denied to our latitudes. Europe has been called the April climate of the world; but this description applies in general only to those parts of it which, without being washed by the sea, are still not sufficiently distant from it to be entirely-free from its influence. Where this is not the case, the temperature degenerates into sharp contrasts, and a glowing summer succeeds to an icy winter; but when the influence of the sea preponderates, both seasons of the year lose their more marked characteristics. In Italy and the Canary Islands finer grapes are not to be found than grow in Astrachan, and yet in order to pro- tect these vines from the frosts during winter, they are sunk deep into the earth; for even south of Astrachan, at Kitzlar, near the mouth of the Terek, the temperature in winter sinks as low as 36° Fahr. The difference between both extremes is so great, that on the steppes of Orenburg, the camel, the ship of the desert, and the 156 Meteorological Phenomena in reindeer, the agile inhabitant of the mossy plains of Siberia, mect together. It is quite otherwise in England, In Ireland, which is situated in the same latitude as Koningsberg, the myrtle flourishes equally well as in Portugal; it scarcely freezes in winter, and yet its climate will not ripen grapes. On the coast of the Lake of Kil- larney the arbutus grows wild ; in the island of Guernsey hortensias bloom in the open air; and laurels grow in Cornwall, in the same latitude as Prague and Dresden. England is indebted to this equal distribution of a warm, moist temperature, for the soft ver- dure of her meadows, and the clear complexions of her population. ** Oh ye blooming youthful cheeks,” exclaims Moritz; ‘‘ ye green meadows and ye clear streams of this happy land, how have ye en- chanted my heart! Oh Richmond! Richmond! never shall I forget the evening, when, full of ecstasy, I rambled up and down on the flowery banks of the Thames. But all these delights shall not hinder me from returning again to those barren, sand-bestrewed fields, where my destiny has decreed that the little sphere of my ac- tive life should be situated.’’ My readers will readily perceive, by the patriotic feeling which will have found its way into their breasts whilst listening to the closing words of Moritz, that he spoke of Berlin. If, however, I confess that the study of meteorology offers peculiar difficulties here, because, in addition to the constituent parts of the atmosphere, sand enters so largely as to form an essential in- gredient, and to stand a chance of becoming a meteor, I still assert, that it does not appear to me difficult to take delight in the ever- varying aspect of our skies, when we recal to mind the rigid coun- tenance of their eastern, and the melancholy severity of their western neighbours. Our atmosphere is certainly often obscured, but never to such a degree as in the dense fogs of London, in whose streets boys went about with flaming torches on the 24th May 18388, in order, as they said, to honour the Queen’s birth-day with a brilliant illumination. Certainly it often rains with us, but never in such a way as is described in the burden of the song in “‘ What you will.” * With heigh ho! for the wind and the rain, For the rain it raineth every day.” Although Shakespere lays the scene of his play in Illyria, we see at once by these words, that the fool who sings them is a true Eng- lish fool, who had received his youthful impressions in a country where, in reply to the impatient inquiry of the traveller, ** Does it always rain in Bristol?” the satisfactory answer was given. * No! it snows between-whiles.”” What a continual succession of sunshine and rain, on the contrary, with us! What frequent returns of cold after the warmth seems to have set in! As our poet, says :— * The sunshine beguiles With its mild, false smiles, And even the swallow lies, For alone he hither flies,” Connection with the Climate of Berlin. 157 But with this circumstance there is a question connected, which affects us closely. It is this, Can we hope to discover a stationary point amidst this eternal change ? Is there, in the closely-associated chain of causes and effects, any prospect of our being able to dis- tinguish between the settled and the variable ? Our older meteoro- logists thought so; for they described the temperature of a place by giving the highest degree of its observed warmth and cold. They were of the opinion that nature does not lawlessly deviate from cer- tain rules, and that she remains conscientiously between the two ex- tremes which limit her regularity. And they were right; for at a moderate depth below the surface of the earth we find that invari- able degree of warmth which we fix upon as the mean tempera- ture of the place of observation. Thus, at the depth of 30 inches, there is no difference between day and night; at 30 to 35 feet the difference between summer and winter disappears. So slowly, in- deed, does the warmth of the atmosphere penetrate into the soil, that at the depth of 3 feet the warmest day is the 22d of August ; at 6 feet, the 30th of August; at 12 feet, the 9th of October; and at 24 feet, the 15th of December, whilst at that depth the greatest cold falls here on the 13th of June. Springs which rise from this depth preserve the same temperature all the year through; thus the one on the road from Potsdam to Templin stands’ at 50° F. the same as that of the Lomsenbrunnen at Berlin. How surprised the skater must be, when he finds the places where the springs rise in the ponds are not frozen over in winter, though they are the very spots which he had avoided in summer, whilst bathing, on account of their cold. So little power has the stratum in which the life of the earth pulsates in higher latitudes, that the ground which still bears on its surface woods of pine and fir trees, is, even during the summer, frozen so hard at a very moderate depth, that in the year 1821 on Menzikoff’s grave being opened at Beresoff, the lines of sorrow might still be traced on the features of the banished exile, whose heart had ceased to beat for more than a century. If we can imagine this variable stratum removed from the earth, _we should obtain on the new surface the simple representation of a climate of mean temperature; of that temperature which every place would shew if its thermometer stood always at the same height. In this way we should find that in Berlin it would stand every day at 48°-875 Fahr. that in Hindostan there are places where the mean temperature would be 81°-5 Fahr.; that Parry, on the contrary, would fix his winter quarters in a place where the mean temperature would sink to — 2° Fahr., or 34° below the freezing point. This varia- tion, however, does not entirely depend on distances from the pole, for places situated in the same degree of latitude are much warmer on the western than on eastern coasts. Scotland, Denmark, and Poland, have climates of equal warmth. Ireland, England, Belgium, and Hungary, enjoy the mean temperature which would characterise a Naples lying on the east coast of Asia. In America we find the 158 Meteorological Phenomena in climate of Naples in the latitude of Morocco. Canada, which lies south of Paris, has the temperature of Drontheim in Norway. Height above the level of the sea occasions a diminution in the temperature, and therefore Germany has in general a very equal temperature ; the greater height of the land in southern Germany compensating for the difference of latitude. Munich and Berlin shew a remark- able harmony in the barren uniformity of the country which surrounds them, as well as in the mean temperature which, without any detri- ment to either, might be somewhat higher. But results such as these are not the final ones which we have to seek. They may indeed suffice for Troglodytes who live in cellars and caves, but not for us who breathe the pure fresh air. We must find some means of getting back from this abstract uniformity to the animated reality of atmospherical phenomena. We only arrive at it, however, when we have attained to the consciousness, that in what is apparently arbitrary, a law is concealed ; that the language in which nature herself speaks to us though the thunder and the lightning is a reasonable one; and that even the flaming flash of the lightning with which she writes in the night-season is capable of interpreta- tion. We live on the bed of a sea whose waves roll over our heads with- out our being able to rise above their surface. This aérial ocean was named by the Greeks the atmosphere; that is to say, a globe of moisture. Whilst our perceptions take in all its constitutent ele- ments, the Greeks thought of that one alone, the deficency of which destroys all animal and vegetable life, and whose enlivening in- fluence the Bedouin Arab recognises when he reaches the edge of the desert, and though still far from the stream, perceives the air becoming moist, and stretching out his hans towards it exclaims with joy, ‘‘ I taste the Nile.” Steam has become of such essential importance to our life, that I ought to presuppose every one to be acquainted with this miracu- lous child of dissimilar parents,—this son of water and of fire. But of those who so often use the word steam-engine how few there are who really think of the oldest of them all, the atmosphere. All the water which either falls in soft spring showers, or rushes down in storms, has been raised by the atmosphere in the form of steam generated by heat. The mill which is driven by the mountain stream is also a steam-mill, only that the sun kindly undertakes to produce the heat which continually guides anew the circulation of the water. The steam of water is a perfectly transparent elastic fluid ; clouds, mists, and vapours, are not steam, but condensed moisture, which has returned from the aérial into the liquid form, If we observe a locomotive, when conscious of its power it raises the valve, and contemptuously casts off the superfluity, with which electro-mag- netism might win its promised prize; at the place where the steam issues forth it is perfectly transparent, the white cloud only appears when it has risen to some little height. Air mixed with this transparent connection with the Climate of Berlin. 159 steam is called a moist air, air mixed with condensed steam is termed a cloudy atmosphere. Both may be distinguished from each other, just as our breath in a warm room is distinguished from the clouds which form before our mouths in winter, but which we do not ex- hale as clouds. Water mixed with spirits of wine produces a trans- parent mixture, because both are fluids. Air, however, mixed with opaque solid or fluid bodies, produces an opaque mixture which becomes more opaque in proportion as the mixture is more entire. Thus snow may be formed out of comminuted ice; white sand out of pounded rock- crystal; foam, mist, vapour, or whatever we like to call it, out of water. We look upon clouds habitually as on something really existing, as a kind of magazine in which rain, snow, and hail, are stored up ; bodies which, when they come into contact with one another, produce thun- der; which are attracted by mountains and torn asunder by their rocky teeth, when out of the breach thus formed water streams forth ; and what is most remarkable of all, we think of these clouds as floating with all their heavy contents in the air. If, however, we only get amongst the clouds on the top of a mountain we find that they consist of nothing but common mist, and that of all the magni- ficence we had attributed to them not a trace remains. We might have spared ourselves the trouble of ascending so high to discover this, for a cloud is nothing more than a mist above, and a@ mist is nothing more than a cloud below. Any one that has been accus- tomed to think of a cloud as of something tangible and lasting, of which he can take a photography ; or, if he has the talent for it, make out in it resemblances to the forms of men and animals, must be aware how often he is obliged to change his comparison. It may be said, however, that we often see a cloud lying all day long on the top of a mountain. Does not Mount Pilate take his name from the very circumstance that he alway wears a cap? Is not the Table Moun- tain at the Cape celebrated for it ? Who, however, that sees the white foam lying on a clear mountain stream, looked down upon from a hill, believes it to be anything lying on the ground ? And is the cloud lying on the top of a mountain, anything more than this? The stream is the air, the stone on which the foam rests is the mountain, the foam is the cloud. Does it not move continually if we ascend the moun- tain in order to see if it really lies quietly upon it, as it seems to do when we look up at it from below? The appearance of stability is there- fore nothing but a delusion, the cloud endures only whilst arising, and in the act of vanishing. Do we find the plains of Lombardy covered with the clouds which are attracted down from the St Gothard in quick succession into the valley of Trevola? No! they have entirely disappeared from the hot plains, and the cloudless heaven above them forms a strange contrast to the thick covering which, whenever we look back, conceals the Alps from our view. Do _ we not often see a storm, which, with the intention of raining in good earnest, comes down from the Charlotten Berg, entirely dissi- 160° Meteorological Phenomena in - pated when it arrives over the glowing city. If, on the contrary, the atmosphere is very moist, already the absorption does not take place —a long strip of cloud leans down from the top of the mountain, where its first germ had formed itself, and the rain pours down. If the air has lost its absorbing power, it will soon become saturated with water. This is what takes place before a shower, and it is for this reason they say in the Bernese Oberland, _“ Does the Riesen his rapier wear ? Then it shews that rain is near ; Is his cap upon his head ? Then that shews the rain has fled.” But these rules are only applicable to mountains whose points rise boldly into the higher regions of the air, not to lesser heights on our own German plains. IPf the moisture be already great enough for it to take the form of clouds, then it will soon shew itself in the shape of rain, and therefore they say in Thuringia of the Kyffhauser, “ Has Frederick cast his crown away, The weather will be fine to-day ; If on his head his crown is set, The weather soon will change to wet.” “The mountains are heaving, the Bohemian mists are coming; it will rain,” they say in the Hazy Mountains. ‘ The Zoblen is clear ; it will continue fine weather,” they say in Silesia: and in England the proverb is, | “When the clouds are on the hills, They will come down by the rills.” In winter, clouds often conceal the dome of the Gensd’armes Tower ; in-summer storms pass over the dark Aachorn, the Jungfrau, and Mont Blanc. But what a difference there is between the fine drops of winter rain, and the large splashes of a summer shower. If, however, we ascend a mountain during this splashing rain, we shall find that the higher we ascend the smaller the drops become ; higher still we shall find only a mist; at that height it is no more the cloud which rains, but the whole stratum of air between the cloud and the ground. ‘This is so true, that upon the roof of the King’s castle in this place, only 18 inches of rain fall annually, whilst 20 inches fall on the pavement of the castle-yard ; for a continually renewed condensation of the mist of water takes place, and meeting with the — rain drops in their descent, makes them continually increase in size. This applies equally to snow and hail, which do not therefore pro- duce the destruction which we should expect from the size of the grains if they fell down from a considerable height. If a crow, for example, were to slip down the steep roof of a church at the begin- ning of a thaw, the descending snowball would become at last a little — avalanche. But did the crow cast it down; those must believe so who ascribe the rain to clouds alone. connection with the Climate of Berlin. 161 But how do clouds of snow and rain originate over our plains, which are situated far from the cooling summits of the mountains ? A celebrated amateur gathered together a large assembly in the council-hall of a northern residence. It was one of those icy star- bright nights which are so aptly called iron nights in Sweden. In the saloon, however, there was a fearful crowd, and the heat was so great that several ladies fainted in consequence. An officer tried to end this distressing state of things by attempting to open a window. But it was impossible, so fast it was frozen to the window cill. Like a second Alexander he cut the Gordian knot by breaking a pane of glass, and now, what happened? It snowed in the room. Circum- stances so favourable as these seldom present themselves for obser- vation here. But I have, even in Berlin, seen a thick mist, form itself at a private ball, when, on one occasion, the doors opening upon the balcony were thrown open for a moment. Thus, wherever warm air becomes mixed with cold-and moist air, a precipitation takes place. This is the reason why an eternal mist overclouds the sea of Okotsk, where the warmth so sensibly declines towards the north, that, on the same neck of land, shapeless sea-horses, the in- habitants of the polar seas, and elegant certhiadee, the feathered mes- sengers of the south, meet together. It is the same phenomena on a smaller scale which one sees at St Petersburg, at the magnificent festivals given in the winter palace, when a continual condensation is always taking place in the outer apartments. In order, therefore, to understand our weather, we must seek out the principles on which such mixture of unequally warmed air takes place; but to do this I must somewhat enlarge, whilst choosing for my guides two of the learned men of the present day, about whom geology, geography, and meteorology dispute as their heroes, each of the three sciences wishing to claim the two philosophers for itself. If we open a door leading from an outer passage into a warm room, a double draught of air takes place, the cold air streaming in cay. and the warm air flowing out above. This may easily be proved by the flame of a candle. Placed on the ground it is wafted towards the room, held half-way up it stands upright, above it is wafted towards the outer air. On the earth the polar regions repre- sent the outer passage, and the torrid zone represents the warm chamber. ‘There are two cold zones and one torrid, that is to say, a warm room between two cold passages, the doors between the two are always open, the room is always heated to a very high tempera- ture, and there is a constant draught of air, which is called the “‘trade-winds.” Where both currents of air meet, is a region of calms, and it is so named. As, however, the apparent course of the sun varies between the tropics, the region of calms does not always remain in the same place, but follows the sun, and the whole pheno- mena of trade-winds follow in its train. Where the trade-winds pre- vail, the sky is perfectly cloudless, because flowing towards warmer VOL, LIV. NO. CVII—JANUARY 1858. L 162 Professor Blum on Pseudomorphic Minerals. regions, the air naturally becomes drier; in the region of calms, on the contrary, it rains constantly, because the lower warm currents in the act of rising lose some of their heats and therefore allow the moisture they contain to be precipitated. Every place between the tropics has therefore a dry season whilst under the influence of the trade-winds, and arainy season while the calms prevail,—*‘ a time of sun and a time of cloud,’’ as the Indians near the Orinoco say. In the higher regions of the atmosphere, the ascending air flows back towards the poles. We see it often in the light clouds which are attracted towards the lower trade-winds; yes, we even reach this upper opposing current when we ascend high mountains, such as the Peak of Teneriffe, on Mawnaroa, on the island of Hawaia. More strongly still is the influence of this returning upper current seen in yoleanic eruptions. (To be continued in our next Number.) Gieseckite and Bergmannite (Spreustein), two Pseudomor- phoses of Transformation from Nepheline. By Professor J. R. Buu, of Heidelberg. Communicated by the Author, from Poggendorff. At Jyalikko-Fiord, not far from Julianenhaab in Greenland, there occurs, implanted in drift porphyry, a mineral in the form of hexagonal prisms, generally known by the name of Gieseckite. From the similarity of its form, and for the most part amorphous condition of its mass, it was formerly regarded as a variety of Pinite, with which its chemical composition to a considerable extent coincides. It was afterwards grouped by Tamnau with Eleolite (Nepheline), with which it has the same crystalline form, and is said to be, in its fresh condition, as regards hardness, specific gravity, and lustre, identical. But most of the crystals are found in an altered condition, and coincide neither with the qua- lities just mentioned, nor with the chemical composition of the Eleolite. The cause of this is to be sought in the alteration which the Eleolite has undergone. A short time since there came into my possession a crystal of this sort, which, upon my breaking off a small portion at one end, in order to observe the nature of its interior, was seen to con- Professor Blum on Pseudomorphic Minerals. 163 sist entirely of a fine scaly aggregate of very minute mica- ceous lamelle. Thus Giesecke is neither more nor less than Elzolite in process of transformation into mica, at one stage of which a condition resembling Pinite, I believe, occurs very frequently. The final result of the transformation is here likewise mica; and with this view both the chemical compo- sition of the mineral, and the mode in which it is affected by the blowpipe and by acids, closely coincide. Whilst the Eleolite fuses before the blowpipe, and under the action of acids dissolves and forms gelatine, Gieseckite is but slightly affected by the latter, and is likewise more difficult of fusion. If we compare the results of analysis,—that of the green Eleolite of Fredericksviirn by Scheerer (a), with that of Gieseckite by Stromeyer (b),—the process of alteration be- comes very apparent. Their constituents are :— (a) (b) Silicic acid, 45°31 46:0798 Alumine, 32°63 90°8280 Natron, 15:95 0:0000 Potash, 5°45 6°2007 Oxide of iron, 0:45 Protoxide of iron, 3°3587 Chalk, 0°33 Magnesia, 1:2081 Water, 0-60 4:°8860 100°76 Oxide of manganese, 1:1556 96°7119 According to these analyses, there must have been a loss of natron and an absorption of protoxide of iron and water, to- gether with a small quantity of magnesia and oxide of man- ganese. Under the name of Bergmannite or Spreustein, there has long been known a mineral which has been regarded by some mineralogists as a distinct species, and by others as a variety of Wernerite. It is not unfrequently found as a secondary constituent of zircon syenite in Norway, especially in the environs of Brevig, Laurvig, and Fredericksvarn. Scheerer, to whom the external appearance of the Spreustein seemed to indicate that it was not a variety of Wernerite, subjected _ it to an analysis of which the results are given (Annalen, L2 164 ~ Professor Blum on Pseudomorphic Minerals. vol. Ixv., p. 277-8,) and according to which it is a normal natronite (natron-mesotyp.) I lately received several pseudomorphoses from Dr Krantz of Bonn, amongst which was a specimen labelled “ Spreus- tein nach Beryll und Scapolith von Breveg.” I could recog- nise no scapolitie form in the prismatic crystals of the spreustein, whilst, as hexagonal prisms, they appeared iden- tical with the forms of beryl. But as the occurrence of beryl in the zircon syenites of Norway is very far from ascertained; and as Scheerer (op. cit. p. 280) expressly ob- serves that all which he had met with belonged to the apa- tite; and as, moreover, the origination of spreustein from this mineral appeared to me exceedingly doubtful, I carefully examined the specimens of this substance in my own collec- tion, in hopes that I might perhaps obtain some solution of my doubts. It was not long before I observed ina piece of — ore a small hexagonal prism, which superficially had the ap- pearance of spreustein ; but at the end, where a portion was — broken off, was perceived to be Eleolite; and eleolite ac- cordingly it was, from which the other mineral had borrowed its form. But in order to attain greater certainty upon this point, I imparted my views to Dr Krantz, with a request that he would be good enough again to look through his own specimens, and acquaint me with the result of his observa- — tions. The following is an extraet from Dr Krantz’s answer: —*T have again examined my small collection of pseudo- morphous Spreusteins, and have come to the precise conclu- sion you anticipated, namely, that the hexagonal prisms were formerly not beryl but nepheline (Eleolite). The small prism which you will herewith receive, and which is adherent to unaltered felspar (Orthoklas), with which it has nothing in common, consists, at the unaltered-looking greenish end, upon trial with the blowpipe, entirely of mesotype; there is, therefore, nothing more of the original mineral remaining. — } The other and larger prism still contains at one end pure white nepheline, but farther in the interior Eleolite. It is remarkable that the nepheline appears here of such a pure white colour as it has never been found with anywhere in — Norway. The specimen establishes, I think, in a very satis- Professor Blum on Pseudomorphic Minerals. 165 factory manner, that the pseudomorphoses were formerly Nepheline. Spreustein from Wernerite I have never met with.” : The alteration in these two cases commenced at the sur- face of the crystals, spreading from thence to. the interior ; and this process may be observed in various individuals, which are found in its most various stages. Whilst the above-mentioned small crystal is changed into spreustein merely at its surface, the large one mentioned by Dr Krantz (which is about 14 in. long by 1 in. in thickness, and is broken off at both ends) consists at one end entirely of an aggregate of red and white spreustein, but at the other still contains a nucleus of nepheline, surrounded by a crust of whitish-red spreustein of from one to two lines in thickness; and other erystals, again, are entirely changed into the latter substance. Even crystalline particles of Eleolite have undergone this change. The surrounding felspar (orthoklas) is for most part perfectly fresh, merely exhibiting here and there, at its points of contact with the Spreustein, a slight red colour, arising from oxide of iron, which has interpenetrated its cleavage surfaces. The process of transmutation itself con- sists in a loss of potash, in the emission of a small quantity of natron and alumine, and the absorption of water, whereby this process occurred in a rock, which—although water was the agent—presents a perfectly fresh character. Nor will it ever occur to any one that the natrolite was here an ori- ginal formation, or that the water was originally present; _ for the pseudomorphous nature of the spreustein crystals is too plain to be called in question. They are not genuine erystals ; for they consist of a mass of which the composition is confusedly radiated, (whence the name Spreustein given them by Werner)—of an aggregate, which sometimes even includes a nucleus of the original mineral. But if it must be admitted to be a transformation, then it is a transforma- tion that can have been effected only by means of water which has penetrated into the mineral, extracted and re- moved constituents of the Nepheline, partly deposited itself in their room, and formed mesotype ; for the phenomenon can- 166 Mr R. Clausius on the not be explained by assuming either intense pressure or the original presence of water in the mineral. We have here also a beautiful example of the manner in which water, ope- rating upon inorganic bodies, calls into existence new crys- talline forms ; and we may perceive what a misapprehension it would be of this process, which plays such an important part in the formation of pseudomorphoses, were we to limit it to the originating of kaolins, clays, and other “ mineral mires.”” Moreover, it would seem as if the Elolite itself were nepheline in process of transformation; at least this would appear to be indicated by the fluctuating amount of water which the mineral contains. Scheerer has observed of the green and brown Eleolites of Fredericksvirn, that when these are finely pulverised and decomposed with concentrated muriatic acid, the resulting siliceous earth possesses the same colour, though in a fainter degree, which the mineral pos- sessed before, and that it disappears only on its being dis- solved in nitric acid, or by being brought to a glow; where- upon he remarks: ‘“ This is quite sufficient to prove that the colour is of organic origin.” —(Pogg. Ann., v. 49, p. 380.) But how can this organic colouring matter have found its way into the mineral unless by means of water? Sure enough it was not there originally.—(Poggendorf’’s Annalen., bd. 87, st. 2, 1852, No. 10.) On the Colours of a Jet of Steam and of the Atmosphere. By R. CLAUSIUS. To the Editors of the Philosophical Magazine and Journal. GENTLEMEN,—In the August Number of the Philosophical Magazine (p. 128) Mr Reuben Phillips describes a series of interesting experiments on the colours of a jet of steam, which connect themselves with the known experiments of | Professor Forbes upon the same subject. At the end of his paper Mr Phillips writes— ‘Professor Forbes, after discovering the red colour of ajet of steam, by transmitted light, connected the red colour of the clouds with this fact; and the truth of this connection is be- Colours of a Jet of Steam. — 167 yond dispute. So far, however, as I have been able to go, the colours of the steam-jet are manifestly only influences of _ ordinary interference, greatly resembling that produced by thin transparent plates. Thus in (192) the transmitted light is red, as in Professor Forbes’s experiments, but the re- flected light is blue. It is therefore to be inferred, that all the colours of the clouds originate in interference, caused by minute drops of water, the size of which determines their colour; while the blue jet (192) is, I think, strictly analogous to the blue sky.” With reference to this passage I permit myself to make the following remarks:—The blue colour of the firmament and the morning and evening red were explained by me in 1849* upon the principles of “ ordinary interference ;” and some time afterwards} I applied the same explanation to the colours of a jet of steam observed by Professor Forbes. In one point, however, my view diverges from that of Mr Reuben Phillips. He names the water-particles which cause the interference “ drops of water,” while I believe that they are water-bladders, for which view I have adduced my rea- sons in a separate paper.{ Besides this, I should like to mention two points, with re- gard to which I have been unable to obtain from the paper of Mr Phillips a clear notion of the author’s opinion. (1.) Among the various colours of the atmosphere there appears to me to exist only two simple originating ones; namely, the blue colour in all its shades, from dark blue to white, due to interference by reflection; and orange-red _ colour in the corresponding shades, due to interference by transmission. ‘The other colours exhibited at times in va- rious portions of the heavens, as, for example, purple or green, I hold to be due to the mixing of the above ok: colours in their different shades. * Poggendorff’s Annalen, vol. lxxvi., p. 188. { Die Licht Erscheinungen der Atmosphire, described and explained by R. Clausius. Leipzig, BH. B. Schwickert, 1850. Also under the title Beitrdge zur Meteorologische Optik, published by John Aug. Grunert. Part 1, No. 4, p. 395, _ and in Pogg. Ann., vol. Ixxxiv., p. 449. t Pogg. Ann., vol. Ixxvi., p. 161, 168 Description of the Tongue and 423 When clouds appéar coloured, I believe that the colour exhibited 4 is for the most part not formed in the cloud itself, inasmuch as’ the little bladders generally differ too much in thickness to cause the production of a single determinate colour ; but that the light, partly on its way to the cloud, and partly between the cloud and our eye; assumes its colour ; even in the apparently clear air there always exist bladders, which,’how ever, are for the most part so attenuated, that they favour in a particular manner the formation of the /irst colours of interference, namely blue and orange-red.—I re- main, Gentlemen, very respectfully yours, HO. 4 10 GILO9 Did : R. CLAUsIUS. BERLIN, Oct. 13, 1852, \ Description of. the Tongue and Habits of the Aardvark or Ant-eater of the Cape (Orycteropus Capensis). By WILLIAM T. BLACK, Assistant-Surgeon to the Forces, South Africa. Communicated by the Author. In Professor Jones’ General Outline of the Animal King- dom, is to be found a description of the elongated tongue of the Ant-eaters of South America, and the Echidna of New Holland. The Aardvark (the Earth-hog, Dutch) and these two animals, belong to the order of Edentata, but the last is further distinguished by being monotrematous. Whether Professor Jones’ description is intended to refer to the tongues of all the animals in that order that possess them as instruments of prehension does not appear, and it may be correct ; but from two or three specimens of the organ dis- sected by me in the Aardvark, I am led to doubt its applica- bility to this Animal. Professor Jones speaks of two proper — muscles not found in the tongues of other mammalia, an ex- ternal annular one, and an internal elongated spiral one, invested by the former. These I have been unable to detect in the tongue of the Cape Ant-eater, and I subjoin the fol- lowing description of my acquaintance with its lingual ana- tomy :— — Pee. I a i, i i i i le) Be id Habits of the Ant-eater of the Cape. 169 - The tongue is from 10 to 12 inches long, when stretched out. The mucous membrane of its upper surface is rough and of a file-like feeling, when the finger is passed backwards along it. There are three papille near the base, situated in the form of atriangle. On the outside, at about the posterior half, are the conjoined palato and stylo-glossus muscles, and internally to them, the lingualis, running from the base to the tip of the tongue; and at the posterior fourth in the mesial line is the lingual attachment of the mylo-hyoglossus muscle. The lingual sensory nerve is very large, and lies in a groove between the mylo-hyoglossus and the lingualis, and after passing the former, the two nerves lie side by side in the mesial line between the two linguals. The muscular nerves branch off; the fifth enters the mylo-hyoglossus, gives branches to it, and then passes forwards alongside the lingual nerve. The muscle to which I would attribute the protruding action | of the tongue, or the Hatensor lingua, consists of perpendicular fibres passing from the thick mucous membrane of the upper surface and sides, to the cellular tissue investing the linguales muscles ; this occurs throughout the whole length of the tongue, 1. The mucous coat. 2. The perpendicular fibres. and engrosses more and more of BaNanyes and vessels. the comparative thickness of the 4, Linguales and genio-hyoid. Bee alato-clossus, tongue towards the point from the base. ‘The best way of de- monstrating the course of its fibres, which are otherwise visible enough, is to incise the tongue either transversely or longitudinally, just through the thickness of the mucous membrane, and then tear open the incision. The laceration ‘is easy, and goes in the direction of the fibres to their attach- ment at the upper surface of the lingualis. The contraction of this muscle, in all its body, will produce a contraction of the diameter or thickness of the tongue, and at the same time, from the consequent increase of the diameters of the sepa- _ rate muscular fasciculi, must the tongue elongate. It may be otherwise stated, if the mass of the tongue is decreased in ) = 170 Description of the Tongue and one direction, it must correspondingly increase in another— like a bladder nearly full of water, which elongates in the direction lateral to the points of pressure. Should the mesial fibres of this perpendicular or transverse muscle be thrown into action, then the upper surface of the tongue would become flattened or hollowed out. The retrac- tion of the tongue is of course accomplished by the lingualis, and the other motions of the organ by the other muscles as ordinarily shewn. This action of the perpendicular fibres also renders the tongue, when projected at the same time, somewhat elastic and firmer, so as to allow of the stronger action of the others in bending it in different directions ; one or the other lingualis laterally, or both downwards, when the lower fibres of this muscle are thrown into action; and when the upper fibres are in a similar state, the point of the tongue would be directed upwards. What share the muscles of the base of the organ particularly have in its motions, I do not enter upon, merely having considered the actions of the free part of the tongue. On section of the upper surface of the mucous membrane between the muscular fasciculi, appear yellow oblong ovoid bodies, about a line in length each, probably mucous glands, or, as I had not means of deciding this point, may be particles of fat, though not likely, as they only occur among the mus- cular fasciculi at the upper surface, and not at the lower ex- tremities of the fasciculi. When the perpendicular or radiating fibres are in action, the secretions from these glands would evidently be expressed out upon the surface of the tongue, thereby supplying the adhesive fluid which is the means employed by the ant-eater for the capture and reten- tion of its insect food. The specimen of the animal which I procured for the above dissection, was a female, had four teats, and was 6 feet 2 inches in length from the nose to the | end of the tail. The next one which I dissected afforded the following description :—The mylo-hyoid muscle, or flat muscle next the skin ;—Genio-hyoid of two bands, on each side of the mesial line between the chin and hyoid-bone ;—Genio-hyoglossus between the chin hyoid-bone and tongue, the lingual fibres | | | 4 Habits of the Ant-eater of the Cape. 171 radiating upwards to the tongue; the latter part is broader behind where it is attached to the root of the tongue, and terminates, conically forwards, to about the middle of its length ;—Palato-glossus, a large flat band on each side of the former, and, together with the lingualis, forms the lateral and inferior muscular of the tongue, from the root to the tip ;— Stylo-glossus, a small band of fibres, descending from the styloid process, perpendicularly to the root of the tongue, where it comes again forward on the outside, and parallel to the former muscle, and is finally lost at about one-third from the root, in the fibres of the palato-glossus and lingualis. Lying above this mass of muscle, composed of the palato, and stylo-glossus, and lingualis, which—after passing the anterior edge of the genio-hyoglossus, lie side by side, and form also the inferior half of the muscular mass of the tongue where it _is free—is the perpendicular muscle already described, part of which, at the base of the tongue, is attached below to the lingual termination of the genio-hyoglossus. In the mesial line between the perpendicular fibres and the longitudinal ones, lie the nerves and vessels of the tongue. There is also @ vein, running in the mesial line on the upper surface of the tongue, just underneath the mucous membrane, having trans- verse branches falling into it from the muscular substance and mucous coat. This specimen was also a female, had four teats, and was 5 feet 4 inches in length from the nose to the tail. In support of the views which I have been led to take of the powers of the perpendicular fibres, I may mention that a similar muscle exists in all mammiferous tongues which I have examined, and I believe is the co-efficient of all those peculiar movements connected with the protrusion of the tongue ; and that the other longitudinal muscles are connected with this -aet chiefly to guide the organ in different directions, as the sole and separate action of these latter muscles would be that of retracting the organ in one or other directions. Pro- trusion is, then, the province of the perpendicular muscles ; retraction that of the longitudinal ones ;—different combina- _ tions of the two produce the several movements out of the axis of the tongue, whether the organ is in a state of protru- 172 Description of the Tongue and sion or retraction. In the Lwmbricus tines, or round intes- tinal worm, may be noticed fasciculi passing from the walls of the abdomen to the integument, and apparently firmly connected to each attachment. ‘These transverse fasciculi seem to exist nearly the whole length of the animal, and to encircle the interior digestive tubes: each fibre is of toler- ably visible size, and pale in colour. As these fasciculi pass between the peritoneal lining of the abdominal cavity, and not from the walls of the proper intestinal canal, to the in- teguments, so each attachment is a fixed point, especially the interior one. That they are not glands may be inferred from their disconnection with the intestinal mucous mem- brane, though this point can only be strictly determined by the microscope. I have, however, by inspection and ana- logy, been led to hold that these fasciculi are muscular and perpendicular to the axis of the body of the animal, and to have a similar action to the perpendicular fibres in the tongue of the Cape Ant-eater. On the above supposition, that their action would be to elongate the animal, without, at the same time, compressing the contents of the digestive cavity, as the action of circular fibres would do in producing the same elongating effect. The digestive process would thus be in- terrupted by such a mode of progression, and defecation would otherwise only result, when the alleged circular fibres were thrown into action. If any effect of the cavity of the abdomen were produced by the perpendicular fibres, it would be to cause a tendency to a vacuum, both by the elon- gation of the animal, and also by the inner peritoneal walls being made the fixed point of action of these alleged muscu- lar fibres. Ingestion of food and fluids would be thus aided most considerably, and independently of any provision for such a purpose at the mouth. It would, however, require further research to see whether analogous muscles, having — actions similar to those attributed to the perpendicular fibres in the tongue of the Aardvark, or the body of the round in- testinal worm can be found to bear out the above general interpretation of their actions ; but I presume that instances might be obtained to shew such a peculiar modification of muscular power, and make it a more general physiological Habits of the Ant-eater of the Cape. 173 property—as in the arms of some of the Cephalopoda, the tongue of the chameleon, the trunk of the elephant, &c. &c. Habits of the Aardvark.—This animal, inhabiting the Fish-River country, lives in immense holes, excavated by their powerful, hoof-like claws, in the ground, some six or ten feet below the surface. There are generally a collection of holes like a warren at these places, all intercommunica- © ting, and situated in or about a clump of trees or bushes. The calibre of these passages is so large in some as to allow a man to creep into. The animal mostly comes out at night, but may sometimes be seen during the day. It is planti- grade on the hind feet, but digitigrade on the fore ones. The fore-feet have four toes, and the hind-feet five each, armed with strong hoof-like claws, very similar except in size to the arrangement of those of the mole, so as to enable the animal to dig and scrape away the earth sideways from them, and also crosswise, the inner toes being longer than the outer ones. * The ponderous conical tail, 18 or 20 inches long, composed of bony joints, and a multitude of muscles, covered by an in- tegument as thick as an ox’s hide, hangs ordinarily down, like that of the Cape sheep, when the animal is walking. Its structure is similar to the tail of the Cape iguana or large water-lizard and its use may be, in one point of view, Similar, viz., as an instrument of defence from attack, as with it they strike dogs very forcibly that attack them. When surprised, they instantly make for their holes; but as they cannot run fast, they are therefore soon caught by dogs, and easily shot or assegaied. When seized by dogs by their very soft ears, or by their velvety nose, they double in their heads between their forelegs, and strike forwards, or kick with their hind-feet, so as to make their assailants loose hold _ and often repent their proceedings. They are best caught in moonlight nights, when out feed- ing, either by dogs, or waiting near a suspected warren till the animal returns before the break of day. They live chiefly on ants, and, as there are numbers of ant-hills all over the country, their food is ever at hand. They first dig away with their fore-feet, partly, as it were, sitting on their hind-_ od 174 Habits of the Ant-eater of the Cape. legs, supported by the tail, like the Cape Redistes or jerboa, a large hole at the base of the anthill, and, no doubt, when made sufficiently large, they lie down and thrust their nose in, which is protected from stinging by its velvety hair, when they ascertain the neighbourhood of their game. They then protrude their long, tapering tongue, well covered with secretions through their toothless gums, which, when well covered with ants, is retracted, and the burden disposed of in the mouth for mastication. The mouth is abundantly supplied with mucous glands under its covering membrane, and the sublingual glands are large and open, with many se- eretory ducts, to pour out an abundant lubricating secretion. From the want of both incisor and canine teeth, the bite of the animal is harmless, and besides, the orifice of the mouth is not much larger than suffices for a tongue-load of ants. By means of the flat grinders on each side, this minute kind of scaly food is ground into paste, and made fit for digestion. In exca- vating its habitation, no doubt, the very great muscular power of its hinder extremities come into action, and shovel- ling away, like a spade, the earth loosened by the fore- feet, the two extremities act the part of a pick and lever. From its beautiful buck-like ears, one would suppose its sense of hearing was exquisite, and perhaps of much more use to the animal than its small, laterally-directed eyes, especially for its nocturnal and subterranean habits of life. Its hide is as thick as that of an ox, impenetrable, no doubt, to all attacks from insects, and has much the appearance of a pig’s skin, but thicker, and has the same intimate con- nection with the underlying muscular structure as in the latter animal, so that the natives, when they slaughter the Aardvark for food, cut it up into pieces with the skin on, as we do pork. Dimensions of the Female killed near Fort Brown, whose — oval dissection is above given.—Length, 5 feet 4 inches from the nose to the tail end; nose to the root of the ear, 11 in.; ear to the wrist or carpus, 145 in.; ankle (tarsus) to the protuberance of the hip-joint, 15 in.; length of the tail, 184 in.; leg, from the ankle to the spine, over the protuberance of the trochanter, 21 in. ; arm, from the wrist over the shoul- On the Negroes of the Indian Archipelago. 175 der to the spine, 18 in.; round the belly, just in front of the thigh, 3 feet 3 in.; round the thorax, behind the shoulders, 2 feet 6 in.; round the neck, behind the ears, 153 in. P.S.—I have sent two entire skins to the museum at Fort Pitt, which were forwarded, with other specimens, after the breaking out of this war, and which have all since been ac- knowledged. W. T. B. The Negroes of the Indian Archipelago and Pacific Islands. By W. JOHN CRAWFURD, Esq., F.R.S. Oriental negroes are found thinly but widely scattered, from the Andaman islands, in about 80° of E. longitude, to the New Hebrides in the Pacific, in about 175° E. longitude, and from the Philippine islands, in 18° N. latitude, to New Caledonia, in about 21° S. latitude. These eastern negroes are known to Europeans under various names. The Malays term the inhabitants of New Guinea, Papua, or more cor- rectly Pua-pua. Europeans taking this as an authority, call New Guinea and its inhabitants both Papua. The word pua-pua is an adjective, and signifies crisp, frizzled, woolly. To complete the sense for the country or people, it is necessary to state the nouns-substantive, tanah =country, and oran=people. Thus oran pua-pua =a woolly headed man; and tanah oran pua-pua=the land of woolly- headed men, European writers have also sometimes termed them Alfores, which word has been converted by English and French writers into Arafura and Harafura, and referred to a Malay source. It is not, however, Malay, because the letter f is not to be found in any written language of the Indian Archi- pelago, and seldom does the sound occur in any of the un- written ones. The word is Portuguese, and means freedman, in which sense it is adopted by the natives of the country. It is nearly equivalent to the Indios bravos of the Spaniards, 176 =W.J. Crawfurd, Esq., on the Negroes of the as they term the free unsubjugated Indians of Spanish America. : Spanish writers term the negroes of the Philippine islands, from their diminutive size, Vegritos, or little negroes. Some English writers have lately termed them Austral negroes, which is manifestly improper, since they are found equally in the northern as in the southern hemisphere ; and this even in the islands of the Indian Archipelago. The oriental negro is even found in a state of civilisation below that of the brown-complexioned and lank-haired race in their neighbourhood, whether these be Malayan or Poly- nesian. There is great diversity in their civilisation; some, with the least possible knowledge of the commonest arts of life, live precariously on the spontaneous produce of their forests and waters, both animal and vegetable; while others practise a rude husbandry, construct boats, and undertake coasting voyages for the fishing of the tortoise and tripang, or holothurian. . . The negro of the Andaman islands is below five feet in stature, and is of the lowest civilisation. The negro of the northern portion of the Malay peninsula is also of short sta- ture. |F6E |¢.88 |6-1b |8-LF |0-6¢ |8-99 |2.8h | 22h |9-88 |8-4E 16-28 | 1-98 “WV 6 vereresseesSuoTqVInyes oja[du0s = 000-T *yurod Map jo dInjV1edMle} WoIZ poze[Noyeo ‘ate oy Jo Aytprumy uray Pee ee ete nse were eeee ‘qjyuow yore TOF ‘yurod MOp jo aang ~vraduio} UvaTA WOAy payepNoTeo ‘anodwva Jo aoaog oseyq | ‘uorjerodeao JO puv “ate ay} JO o1n}vAeduIe} 94} JO SUOTVAAASgGO WO1Z poze(noyes “yuiod Mep 93 Jo oangeasoduie} Uveyzy § THOR OHHH RHR HH eee eH eee EEE HEH EEE EEE HEHEHE EEE EEE EEE EE © x L-Lb |2-$h |-3F | F-9F [3-6 |6.8¢ |8-19 |6-6¢ |8-6F |¢-9% |9.0% |9.68 | 2-0F 4 aeg> aH f t ee ee eee eee ee ee ee eee ee ee 410} pue ‘U0 dBd AOJ SLoJOULOTAIS T-9h | F-1% |6-0% |9-FF | 2-09 |€-6G |0-6¢ [1-6 |FL2b |0-8% |0-68 |6-28 | €-88 “H’V 6 oe pe rea. os eee me SUOT}VAIOSGO WOIf ‘UOoTyeJodvae Jo oInjeAedui9} ULeTY S6-8F |9-3F |1-3h |8-9F | TS [0-19 | 1-49 | FEE |2-19 |6-96 | 1b 18-68 | 0-TF wee Teen eeeame nese eee eeeceescecceccess SJaz@MIOUIIIYY "UU pue GF | 4-38 |€-88 | 1-6 |8-8h |0-6G |FLE |¢-6h | 2.00 |1-0% | #98 |1-FE |3-9E “UTI ‘X¥UI SUIIO}s[Zo1-J[9s JO suOT}eatosqo A]rep Jo suvaut HFS | 1eLh | S-Lb |E-TS | F-6E (0-29 {802 |8-19 |2-L¢ |8-8¢ |1.9b |¢-26 | 6.FF “XBT 84} WoIZ Ae oY} JO oAnquseduis} uve oyeuITxorddy 9 |6-8h | 14h |6-6F | 2-29 | 9.49 [0-89 |8-8G | FEE |6-2G | GCF |1-8% | 1.24 ‘Wd § -— + =. oe Wie § PUVeNy 6 7e-su08 om T-6F | 1h |8-3F | 6-96 |6-€9 |9.09 |%89 |6-6¢ |6.1G | 29% |9-3F |6-0F |8-0F ‘WV 6 IOf pus *YIUOM YoVa AOJ Ale ayy JO aaNyeaodwie} ULoT_ E8L-66 IZF-6Z| 08F-62) 08-62) 616-66) 8% 21.62) ZL6-66| F19+6Z| €06-6Z| 6ST-0E| 98T-08| 198-62) 9¢8-62| "Wag ssrresees Savak oy} LOZ PuB *Y}RMOUT Yous AJ vas oy} JO 9ANT UvoUl 92 9AOQGR OpPNnjI}1B 10 9199.1.109 pur * ¥08-62) 80-62) 964-62, ZZ8-62| 686-62| 942-62| L26-62| 6Z9-62| L16-62| 891-08) ZIG-08| 028-6z| Z9F-6c| ‘wv 6 |) PAM Se ee ee et tt ppt | | JO o.anzesoduie} 9y} 3B 19JITIOAVq ay} JO WYSIey uveyy “Ivo *u0T} oy} JO| *oaq | ‘AON | “990 | "3dag | ‘3ny | -A[n¢g | oung | Lew | -prady |youep) ‘qoq | ‘uve | -easosqg *suot#eVarosqg Atreqg wor suvoyt jo sanoy Captain James on Meteorological Phenomena. ‘sdoouLsug [eho ‘SaNVE uIvydey Aq pozworunmUoy vas ayp fo Jana? Unau ay} en0gn joel OST 6 ZGRT “Vax ay? burwnp ‘ybunqupy ‘snourg yohoy gt ‘eG Kanung sounupag ay} 1D Uayn} sucrQDAWASqQ 72002.6070.L00}0 JT 282 Captain James on Meteorological Phenomena. 283 Remarks. 1. Barometric Pressure.— -The Maximum height observed was: on the 7th NS) A Mii on 5s ais din ase dove ARPES Av =30'612 The Minimum height observed was on the 27th . MCC MIG E At Oo AM Sv eeld once ovdtedo sre darting ss =27°895 Extreme range during the year,...= 2-717 So great a depression of the barometer has not occurred since January 1839. On the 13th of that month, Mr Adie informs me the height corrected for altitude was 27:53, when, as on the 27th December last, there was a violent storm, which, from observations made, was no doubt a rota- tory storm. The depression observed by Mr Adie was the greatest (as far as I can learn) which has ever been recorded in Edinburgh. It will be observed that the mean height of the barometer at 9 A.M., for each month, is higher than the mean height at 3 P.M., with the exception of the month of December. This isi result was caused by the sudden rise of the baro- meter on the 27th between those hours, amounting to -419, which, on the mean of the month, overpowered the difference due to the influence of temperature at the hours of observa- tion, though it very slightly affected the means for the year. It will also be observed that the mean height was greatest in March, closely following the lowest mean temperature of _ the air, and that the mean height was lowest in August, closely following the highest mean temperature. This fact, _ coupled with the fact that the barometer is always higher at 9 A.M. than at 3 P.M., whilst the temperature of the air is al- ways lower in the morning than in the afternoon, seems to _ prove that the effect of an increase of temperature, by caus- ing the air to expand and become specifically lighter, pro- _ duces a corresponding depression in the barometer ; but as _ the amount of vapour in the air, and the influence of clouds and currents in the upper strata of the atmosphere constantly | disturbs the effect of increased or decreased temperature at 284 Captain James on Meteorological Phenomena. the surface of the earth, we are not able to express numeri- cally the effect of any increase or decrease in the tempera- ture of the air upon the barometer ; but it has been shewn by Colonel Sabine, that when the pressure due to the amount of vapour in the air is deducted from the height of the baro- meter, that the influence of temperature upon the dry air is to produce a daily maximum and minimum, coinciding nearly with the coldest and the warmest hours. 2. Temperature of the air.— The maximum temperature registered on the 4th lly a ore ee BE ok ee BRS The minimum temperature registered on the 19th February, :! si ..vis. sis baudiew tt nerd) ae = 26°:0 Extreme range during the year,...... = 55°:5 The approximate mean temperature of the air for the year = 48°95, which is probably 2° or 3° higher than the mean temperature of the air in the neighbourhood, in places beyond the influence of the heat and shelter of the houses. 3. Humidity.—The degree of humidity of the air has so sensible an effect upon health, particularly on persons with delicate lungs, or those subject to irritability. of the skin, that it is much to be wondered at that medical men in gene- ral have paid so little attention to it, and more especially as _ the instrument for measuring the humidity of the air in any room is so simple and inexpensive. The gardener knows it is not sufficient that his greenhouse should be kept at a cer- tain temperature, but takes care that his plants shall have also the requisite degree of moisture in the air; without this the plants droop; and beyond doubt there is a certain degree of , moisture which is also necessary to the health of man. Every sick room therefore should have a dry and wet bulb hygro- meter ; and if the medical man considers that the tempera- ture should be preserved at 60°, then the wet bulb thermo- meter should indicate 55°, which would shew the air to be — ‘75, or three-fourths saturated with moisture. The amount of moisture might be regulated by exposing a larger or smaller surface of water to evaporate, for which the Dr F. Penny on the Valuation of Indigo. 285 numerous vases and other ornamental vessels usually found in drawing rooms would be found available. 4. Rain.—The greatest quantity of rain which fell in one day during the year was 1:37 inches, on the 24th August ; this is one-third-more than fell during the entire months of March and April. 5. Wind.—It will be seen from the table of the direction of the wind, that it blows at 9 A.M. 2} times more frequently from the W. to S. are than from the E. to N. arc; the num- bers being 199 days from the SW. arc, and 90 days from the NE. arc, and that the NE. winds are the least prevalent throughout the year, occurring principally in the spring and autumn. On the Valuation of Indigo. By Dr FrepEerick PENNY, F.C.S., Professor of Chemistry in the Andersonian Uni- versity, Glasgow. Several methods have been employed for estimating the comparative value of commercial indigo. The colorimetric processes with chlorine, proposed by Ber- thollet, and first practically applied by Descroizilles, have _ heen most extensively tried, and have been fully described by Berzelius,* Chevreul, + Schlumberger, Schubart,§ Persoz, || and others. In these processes chlorine-water or bleaching- powder was used as the source of the chlorine. Bolley { has proposed chlorate of potash and hydrochloric acid as the source of chlorine, and has reported very favour- _ ably of the results obtained by operating upon specimens of _ various qualities. _ Some chemists consider that the only method of accurately 4 _ determining the value of this article consists in removing the * Traité de Chimie. t Legons de Chimie appliquée a4 la Teinture. _ | Bullet. de la Soc. Industr. xv. 277. § Tech. Chimie. ll Traité de V’Impression des Tissus. s| Ann. Ch. Pharm. 1850, VOL. LIV. NO. CVIII.—APRIL 1853. U 286 _ Dr Frederick Penny on the various impurities by the successive action of diluted acid, caustic alkali, alcohol and water, and then ascertaining the quantity of indigo-blue that remains, the ash being deducted in the usual manner. Others, again, prefer the process of reducing the indigo-blue by deoxidizing agents, and after- wards precipitating and collecting it in the pure state. This method was, about the commencement of the present century, adopted by Pringle,* who employed the well-known mate- rials, sulphate of iron and lime, as the reducing and dissolvy- ing agents, and separated the indigo-blue from the clarified Solution with hydrochloric acid. The operations involved in this process are exceedingly tedious, and in consequence of the peculiar property which reduced indigo has of forming two distinct combinations with lime, the one soluble, and the other insoluble (a fact not known to Pringle); the results afforded by it are not always satisfactory. Danat has recommended another method, based, dl on the same principles. It consists in boiling the indigo in caustic soda, and cautiously adding protochloride of tin until the indigo-blue is completely reduced and dissolved ; the clear solution is then precipitated by bichromate of potash, and the precipitate being well washed with dilute hydrogmnee acid, is dried and weighed. A Fritzche {| has suggested cane-sugar, alcohol, and caustic soda for the reduction and solution of the indigo-blue. His process, which appears, however, to be better adapted for the preparation of pure indigo, than for testing its value, has been repeated and favourably spoken of by Marehand ; and Berzelius says, that it surpasses all other methods that have been employed for obtaining indigo-blue in a state of purity. Chevreul’s method of dyeing cotton until the indigo-solu- tion is exhausted is obviously very objectionable. Reinsch,§ after trying various modes, prefers that of dis-- solving a grain and a half of the indigo in concentrated sul- phuric acid, and then estimating its comparative value by the a —_————— ——————————————————————————————————————————————————————eNSoesese—esoeo—=—"*"] s * Annales des Arts et Manufac. vi., 214-239. t J. pr. Chem. xxvi., 398. t J. pr. Chem, xxviii. 16. § Jahrb. prak. Pharm, Valuation of Indigo. 287 quantity of water required to be added to reduce the colour of the solution to a certain shade. This process, which is simple and convenient, is in every respect similar to that long since applied by Ure,* though Persoz+} ascribes it to Houton-Labillardiére. The advantages and disadvantages of these processes have been So fully discussed by Bolley in his paper, before referred to, that it is unnecessary, I conceive, to make any further comment on their respective merits. The method I have now to propose, is based upon the cir- cumstance that indigo-blue in presence of hydrochloric acid, is decolorised by bichromate of potash. This salt has long been used for discharging indigo-blue and other colours in the printing of textile fabrics, as well as for bleaching oils, fats, and several other substances. In employing it for esti- mating the comparative value of commercial indigo, the necessary manipulations are extremely simple. Ten grains of the sample, in very fine powder, are carefully triturated with two drachms by measure of fuming sulphuric acid, and the mixture being excluded from the air is allowed to digest with occasional stirring for twelve or fourteen hours. A small flat-bottomed flask with a tightly fitting cork, is a very convenient vessel for this operation. Some pieces of broken glass should however be thrown in to facilitate the - contact of the indigo and acid during the agitation, and thus to prevent the aggregation of the former into small clots, which the acid by itself cannot penetrate. Ifa small capsule _ or test-glass be used, it should be covered, during the diges- _ tion, with an air-tight gas-jar. It will also be found advan- _ tageous to place the mixture in a warm situation, say be- _ tween 70° and 80° F., that the action of the acid may be fully developed; a higher temperature than this must be avoided, as sulphurous acid is liable to be produced, and the trial in " consequence completely vitiated. Great care must be taken to insure the perfect solution of the indigo-blue in the acid. This result being accomplished, the solution is poured slowly, with constant stirring, into a pint of water contained in a 7 * J. Roy. Inst., 1830, J Traité des Tissus, i, 434. ~ U2 288 Dr Frederick Penny on the basin, and 2 of a volume ounce of strong hydrochloric acid immediately added, the flask or capsule being rinsed clean with water. An alkalimeter of 100 equal measures, is now made up in the usual way with 74 grains of dry and pure bichromate of potash, and the solution added in small successive portions to the diluted sulphate of indigo in the basin, until a drop of the mixture, on being let fall on a white slab or slip of bi- bulous paper, presents a distinct light brown or ochre shade, unmixed with any blue or green. The process is then finished; the number of measures of bichromate used is read off, and this number shews the comparative value of the indigo sub- jected to the trial. In applying the test-drop to the bibulous paper, the best results are obtained by bringing the end of a glass rod into contact with the indigo-solution, and then gently pressing it against the surface of the paper. The stain thus produced will be circular, and conveniently localised to a small space. By using bibulous paper, it will also be found much easier to recognise the last traces of the blue colour than when a slab is employed, and the results, when dry, may be preserved unchanged, for reference or comparison. It is advisable to keep the indigo-solution gently heated while the chrome-liquor is being added; and it is essentially necessary that the mixture should be well stirred after each addition. Several measures of the chrome-solution may at first be poured in without risk of error, but towards the con- clusion, the liquor must be added very slowly and with great care, aS one or two drops will then be found to produce a very decided effect. The characteristic changes of colour which the mixture undergoes during the addition of the chrome-so- lution, will distinetly indicate the approach of the process to- — wards conclusion. The blue colour of the solution gradually — diminishes in intensity, becoming perceptibly lighter and lighter, and after a time it acquires a greenish shade, which soon changes to greenish-brown, and almost immediately to — light ochre-brown. | [ have tried this process very carefully upon pure indigo, prepared according to Fritzche’s method. The mean of three Valuation of Indigo. 289 experiments, which gave results almost identically the same, shewed that 10 grains of pure indigo require very nearly 73 grains of bichromate of potash ; and I have accordingly taken this quantity of the salt for solution in the alkalimeter. The following table contains the results of trials upon three Series of specimens of commercial indigo, and includes like- wise the price of each sample, and the amount of ash left after careful incineration, as well as the moisture expelled at 212°. The first series of samples was obtained from an in- digo broker in London ; the second from Messrs C. Tennant and Co., Glasgow ; and the third from Messrs R. and I. Hen- derson, Glasgow. FIRST SERIES. Alkalimeter SPECIMENS. pee measures og t boi ; i SENT per cent. per cent. Seyis thea East Indian 6 4 68 4-5 5.0 eee 6 0 66 58 6:0 e - 5 9 64 8-1 8:0 i; a 5 6 54. 11:0 70 »i * 4 9 514 2 Gd ie ie 4 8 54. 3°6 7:0 i 4 4 45 14:0 8-4. Spanish 4 3 55 12:3 6:0 sei 3 10 50 13:'0 7:0 id 3. (6 443 19-0 5:5 < 2 10 28 ook 4:5 ; SECOND SERIES. Biadeyscvos AUsetebes yi ivi Water | ee oa 1851. a a per cent. per cent. 1. Bengal 5 0 64 5-9 4-0 5 a ae, 47 24- 5:0 _ Benares 4 6 45 20:7 8-4 Guatemala 4 3 50 16:0 65 Madras ets: 41 10°6 6:7 _ Oude 3 8 46 6:3 8°5 _ Carraccas 3.6 52h 162 6-4 _ Madras Bir.g 35 83-3 6:0 5 a 290 Dr F. Penny on the Valuation of Indigo. THIRD SERIES. . Alkalimeter SPECIMENS. —— measures : hse bape’ i consumed. Pp = of BAP CARE £3 Java 5 6 635 54. 4.8 Bengal . 4 10 594 7.5 5-0 ’ 4 0 56 11.0 5:3 » : Lx 24 44:4 4:4 Manilla, 3 4 354 98-0 5:0 Hi yan) 261 50:0 5-4. The results in these tables clearly shew the uncertainty, and in several instances the positive inaccuracy, of the com- mon methods at present employed by commercial men for estimating the true value of this article. The indications of quality afforded by colour, fracture, texture, coppery hue when rubbed, cleanliness, weight, and other characters, should always, in my opinion, be confirmed by the application of a simple chemical process, such as I have here described. The objection, on the score of the time consumed, so strongly urged against many of the other methods, is certainly not chargeable against this ; for, by steeping the indigo in the acid over-night, twenty or thirty samples at least could be easily tested in a day, and at a trifling expense. I may mention that there was recently sent me for exami- nation, a specimen of indigo, offered in Glasgow as refined indigo, at 10s. per Ib. It gave 9 per cent. of ash, and 23 per cent. of moisture ; and 10 grains, when dissolved in sulphuric acid, consumed 82 measures of the bichromate of potash so- lution. It is in very fine powder, with a deep coppery-blue colour. Assuming its quality and purity to be uniform, it would unquestionably be more economical, even at the high price of 10s. per lb., than much of the indigo at present sold. Its tinctorial powers could be relied on; and, from the cir- cumstance of its being finely pulverized, it obviously admits of being rigorously tested by the bichromate process. The method here proposed is open, I am well aware, to — some of the many objections that have been advanced against — the well-known chlorine process. It is quite obvious, for in- Z stance, that unless particular care is taken in dissolving the — Mr D. A. Wells on the Origin of Stratification. 291 indigo in the sulphuric acid, not only is a part of it liable to escape solution, and proper estimation, but, in the case of inferior indigo, sulphurous acid may be produced, which would of course involve a larger consumption of the bichromate of potash than the indigo-blue itself would require. It may also be objected that bichromate of potash, in the presence of hy- drochloric acid, will act upon the other constituents of ordi- nary indigo; but, so far as I have been able to judge from a very extensive course of experiments upon a great variety of specimens, the amount of these influences is extremely slight, and altogether inappreciable when the process is executed with proper care. The same opinion has been expressed by Berzelius and Schlumberger regarding the chlorine process ; and it is further supported by the fact, that indigo contain- ing a large proportion of brown and other colouring matters, consumes avery small quantity only of the bichromate. While, therefore, this process has no pretensions to supply scientific men with the means of determining the actual amount of pure _ indigo-blue in samples of commercial indigo, it is, in my opi- nion, admirably adapted for ascertaining their relative values, being in many respects superior to those which have hitherto been proposed. The bichromate of potash possesses, in an eminent degree, all the qualities requisite for a trustworthy agent of valua- tion, being easy of purification, unchangeable by keeping, and of uniform composition. On the Origin of Stratification. By D. A. WELLS, Hsq., of Cambridge, United States, North America. The general idea respecting the origin or cause of stratifi- cation as expressed in geological text-books, or as inferred from the writings of geologists, seems to be this: that strata, or the so-called divisions of sedimentary matter, have been "produced either by an interruption of deposition, or a change ; “in the quality of the material deposited. This idea is well illus- trated by the deposition of matter by tides or inundations, its ubsequent consolidation, and a renewed deposition on the 292 Mr D. A. Wells on the plane of the former deposit. That such is really the cause of stratification in many cases, I do not dispute ; but that there are other causes which tend to produce, and have produced, stratification equally extensive and varied, is, I think, clearly shewn by the following observations :— My attention was first drawn to the subject during the past summer, while engaged in the analysis of soils. By the pro- cess adopted, the soil was washed upon a filter for a consi- derable number of days, in sume cases for a period as long as two weeks, and subsequently dried at a temperature of 250° F. The residue of the soil left upon the filter, consist- ing chiefly of silica and alumina, was found, after drying, in every instance, to be more or less stratified, and that too by divisional planes, in some cases not at all coincident with any division of the materials, lthough this is apt to take place. The strata so produced were in some instances exceedingly perfect and beautiful, not altogether horizontal, but slightly curved, and in some degree conforming to the shape of the funnel. The production of laminz was also noticed, espe- cially by the cleavage of the strata produced, into delicate, thin, parallel plates, when moistened with water. These arrangements, it is evident, were not caused by any interrup- tion and renewal of the matter deposited, or by any change in the quality of the particles deposited, but from two other causes entirely distinct, and which I conceive to be these :—- First, from a tendency in earthy matter, subjected to the filtering, soaking, and washing of water, for a considerable period, to arrange itself according to its degree of fineness, and thus form strata; and secondly, from a tendency in earthy matter, consolidated both by water and subsequent exsicca- tion, to divide, independently of the fineness or quality of its component particles, nto strata and lamine. The tendency of this earthy matter is generally to divide along the lines formed by the arrangement of the particles according to their nature or quality: this is not, however, always the case, as was proved by the observations noted, and which is also con- clusively shewn by the examination of almost any stratified rocks, In the valley of the Connecticut, where the sandstones re- Origin of Stratification. 293 main unaltered in any great degree by heat or dislocation, the stratification produced by the several causes may be clearly seen and studied. On the western edge of this deposit, we have rocks composed of strata, which would at once be referred to the action of tides or inundations by the most in- experienced observer. The strata here vary from one tenth of an inch to one inch in thickness; they are also covered with mud-cracks, and the various markings which are usually found upon a shore or beach. In other portions of the valley, we have strata divisions occasioned by the lines which separate materials differing either in quality or nature, as in the shales from the sandstone, the coarse conglomerates from the fine sandstone, or the highly bituminous shales from those less bituminous. And then upon the extreme eastern edge of this sandstone deposit, we find strata, the leaves of which mea- sure from one to two, and in some instances, three feet in thickness, each embracing in itself matter ranging from a coarse conglomerate to the finest sand; and yet none of these, within the limits of the particular strata in which they are included, exhibit the slightest tendency to break or divide in any one direction more than another. The observations here stated, I am happy to find, have been also noticed to some extent by others conversant with the subject of stratification. Sawdust, subjected to the filtering action of water, has been observed by Professor Agassiz to assume a regular stratified appearance. The same has also been noticed by Dr Hayes of Boston, in the vats into which _ clay, used for the manufacture of alum, is washed. I have also noticed regular stratification in the dried deposit of a puddle in the streets, where no apparent change in the cha- racter of the materials deposited could be noticed, and when there was certainly no interruption of deposition. If the divisions of stratification which I have thus pointed out be admitted, it is not improbable that many cases of what _ are now considered disturbed and tilted strata are none other than their normal condition. _ Dr Emmons remarked that he agreed entirely with the & views brought forward by Mr Wells, and referred to cases _ of clay beds, in which certain strata were contorted and in- 294 Professor Horsford on the Relation of the clined, apparently from forces acting laterally, or from below ; but which forces, from the undisturbed condition of the sur- rounding beds, could not have acted in such a manner as to have produced the disturbance referred to: they must there- fore be accounted for by peculiarities or changes in the method of deposition, and by subsequent changes. Professor Hall stated that he had also accumulated con- siderable evidence in regard to this subject, and regarded it as highly important in a geological point of view.—(Proceed- ings of the American Association for the Advancement of Science.) Relation of the Chemical Constitution of Bodies to Light. By Professor EK. N. Horsrorp, of Harvard. Professor Horsford called attention first to the well-known facts that the colour of the hair on animals varied, and was more intense on certain portions of the body. The metals also had colours which were affected by their composition. The change of their colour in summer and winter was also a well-known fact. He enumerated many metals which changed their tints by the simple process of heating. These were phenomena which ought to be investigated by means of chemistry. The change of tint is without change in chemical composition. The law appears to be that metals pass from a lighter to a darker tint. The loss of water causes a change from a lighter to a darker tint. In charring wood, we have a change from a lighter to a darker tint. He illustrated on the black board that blackness was the natural colour of all non-gaseous bodies; and he cited the series of compounds of gold, silver, nickel, platinum, tin, and other metals. He illus- trated how the compounds of the several metals, as they became more divided in their molecular structure, varied. He exemplified them by the series of compounds of lead with oxygen, in which, as the oxygen prevailed, the colours be- came lighter. This was in keeping with discoveries made by Liebig, and other eminent chemists whom he named. | Dr Draper had found the tints to vary in the order in which the metals had certain affinities, as in barium, strontium, and Chemical Constitution of Bodies to Light. 295 calcium: he thought it was due to the metals which were at the base. Blackness is appropriate to extreme dissolution ; Sony in this connection, it was worthy of remark that many nations had chosen that colour to express extreme grief. _ The conclusions of Prof. Horsford were, that the colour of bodies depends upon the extent of the surface of their smaller particles, or groups of atoms.. Transparency depends upon the arrangement of lesser atoms in certain order, constitut- ing large groups. Whiteness depends upon such extent of surface of the groups of atoms as shall reflect all light, or upon such number of these plates produced by pulverizing transparent bodies as will reflect all the light. Blackness depends upon the subdivision of groups to such minuteness that they no longer reflect light, or, by producing interference, destroy it. Heat, by subdivision, causes darker shades. He also observed, in a note, that there seem to be successive scales of colours produced by heat. Professor Smith, of Louisiana, did not agree with Professor Horsford in some of his conclusions, and shewed that there were numerous exceptions in the mineral kingdom. There has recently been discovered the amorphous or black diamond. The diamond is generally supposed to be a clear, transparent substance; yet here was a specimen of a black variety, which was proved by the investigations of Dufresnoy to contain 98 per cent. of carbon. ‘The colour of this variety of diamond proceeded entirely from molecular structure.—(Proceedings of the American Association for the Advancement of _ Science.) Notes on the Distribution of Animals available as Food in the Arctic Regions. By AUGUSTUS PETERMANY, Hsq., F.R.G.S., &c. % i >. The occurrence of animals in the Arctic regions, and its bearing on the missing expedition under Sir John Franklin, is a subject which has of late excited a good deal of interest, and has giving rise to the most conflicting and contradictory 296 Mr Petermnann’s Notes on the Distribution of opinions: some maintaining the existing of animals in the Arctic regions in great numbers, affording abundance of food to man; others as stoutly insisting upon the extreme scar- city, if not total absence, of them. On entering, however, into an analysis of all that has been said and written on.this point, it appears that a too confined view has been generally taken of the subject. Individual observations in certain localities have been separately con- sidered and reasoned upon for the entire region, and these localities only related to a comparatively small space on the American side, the whole Asiatic side of the Polar basin not zing taken into account at all, Again, it has been com- monly assumed that with ascending latitudes temperature descended, and animal and vegetable life decreased, attain- ing their minima at the Pole. Nothing could be more falla- cious than such an hypothesis in a region where the tempera- ture corresponds less with latitude than in any other part of the globe. When, therefore, the shores and waters of Wellington Channel were found to be “ teeming with animal life,”’ it was regarded as a wonderful fact that more animals should be found in that region than in those to the south of it; whereas this fact would seem to find an explanation when connected with other physical features. Indeed, the consideration of isolated facts alone can lead to no correct result; and it is only when the various natural features are compared and considered in their relative bearing, that the laws which govern nature can be traced and discovered. It is in this manner only that Physical Geography becomes a really useful and practical science. In the following outline it is attempted to take a compre- | hensive, though rapid, glance of the distribution of animals within the Arctic regions generally, and to inquire into the causes of certain apparent abnormities. I will, in the first place, proceed to indicate the regions to which these remarks refer; those, namely, which comprise — the Arctic fauna. On this point I have adopted narrower — limits than other authors, inasmuch as I have taken the northern limit of woods as the southern boundary of the — region under consideration. It is true that some Arctic ani- — : : . : Animals available as Food in the Arctic Regions. 297 mals, like the reindeer, are found to the south of this line— still these are not exclusively Arctic in their character, and they are also, more or less, of migratory habits. The ice-fox, a beautiful little animal, well known to Arctic voyagers, and decidediy of Arctic character, does not in general extend to the south of the line assumed ;* which also coincides with the extreme northern limit of the reptiles, and corresponds pretty closely with the line of 50°, mean summer temperature. The region thus comprises Iceland, Spitzbergen, Nova Zembla, the extreme northern shores of Europe and Asia, with the north-eastern extremity of the latter, including also the sea of Kamtschatka and the Aleutian Islands, but exclud- ing the peninsula of Kamtschatka, On the American side it comprises a considerable portion of British North America, the northern part of Labrador, and the whole of Greenland. Though several classes of the animal creation—as, for ex- ample, the reptiles—are entirely wanting in this region, those of the mammals, birds, and fishes, at least bear com- parison, both as to number and size, with those of the tropics,} * The only exception, I believe, where the Arctic fox ranges southward within the wooded district occurs in North America round Hudson Bay. This is owing to its habit of keeping as much as possible on the coast in migrating to the south ; thus, while they extend along the shore of Hudson Bay to about 50° N. lat., towards the centre of the continent they are very scarce, even in lat. 61°, and in lat. 65° they are only seen in winter, and then not in numbers.—(See Richardson, Fauna Boreali Americana, p. 87.) Throughout the whole of the Asiatic and Kuropean north the range of the ice-fox is nowhere found to be within the wooded region, as Baer has shewn in his masterly account of the distribution of this animal.—(See Bullet. Scientif. publiée par ? Acad. Imp.de St Pétersbourg, tom. ix. p. 89.) t Though the number of species is decidedly inferior, the immense multi- tudes of individuals compensate for this deficiency. Some years ago I wrote with regard to this point—“ If we were to conclude from a large number of species that there must be a large number of individuals, we should come to _ erroneous conclusions; for such is frequently not the case. The Arctic and ‘i tropical countries furnish an excellent example, at least in their Mammalian _ and Ornithological Faunas. We need only refer to the crowds of birds which a hover over the islands and shores of the north, or to the inconceivable myriads of penguins met with by Ross on the Antarctic lands, where there was not even _ the smallest appearance of vegetation; and, among the quadrupeds, to the _ thousands of fur animals that are annually killed in the Arctic regions. _ Wrangell gives a fine description of animal life in the Kolyma district of _ Siberia, one of the coldest regions of the globe: the poverty of vegetation is kg 298 Mr Petermann’s Notes on the Distribution of — the lion, the elephant, the hippopotamus, and others, being not more notable in the latter respect than the polar bear, the musk ox, the walrus, and, above all, the whale. Besides these, there are the moose, the reindeer, the wolf, the polar hare, the seal, and various smaller quadrupeds. The birds consist chiefly of an immense number of aquatic species. Of fishes, the salmon, salmon-trout, and herring are the principal, the latter especially occurring in such myriads as to surpass everything of the kind met with in tropical countries. Nearly all these animals furnish whole- some food for man. They are, with few exceptions, distri- buted over the entire region. The number in which they — occur is very different in different parts. Thus,onthe Ame- — rican side we find the animals increase in number from E. to W.—on the shores of Davis Strait, Baffin Bay, Lancaster Sound, Regent Inlet, fewer are met with than in Boothia Felix and the Parry Group. The abundance of animal life in Melville Island and Victoria Channel is probably not sur- passed in any part of the American side. Proceeding west- — ward to the Russian possessions, we find considerable num- bers of animals all round and within the sea of Kamtschatka, as also to the north of Behring Strait. The yearly produce of the Russian Fur Company m America is immense, and formerly it was much greater. Pribylow, when discovering the islands named after him, collected within two years 2000 skins of sea otters, 40,000 sea bears (Ursine seals), 6000 dark ice foxes, and 1000 pood of walrus teeth. Liitke, in his Voyage round the World, mentions that, in the year strongly contrasted with the rich abundance of animals; countless herds of reindeer, elks, black bears, foxes, sables, and grey squirrels, fill the upland forests ; stone foxes and wolves roam over the low grounds. Enormous flights of swans, geese, and ducks, arrive in spring, and seek deserts, where they may moult and build their nests in safety. Hagles, owls, and gulls pursue their prey along the sea-coast; ptarmigans in troops among the bushes, and little snipes are busy along the brooks and in the morasses. Baer also relates thata | walrus hunter on the rocks of Nova Zembla caught in a few hours 30,000 — lemmings. On the other hand, in Australia, and other regions of the tropical — and temperate zones, a traveller will frequently journey for weeks together, — and pass over hundreds of miles of country, without meeting with a single — quadruped.”—See Atlas of Physical Geography, by Petermann and Milner, | p. 130. Animals available as Food in the Arctic Regions. 299 1803, 800,000 skins of the Ursine seal alone were accumu- lated in Unalaska, one of the depots of the Russian Fur Com- pany; 700,000 of these skins were thrown into the sea, partly because they were badly prepared, partly in order to keep up the prices. In the Polar Sea to the north of Behring Strait, as is well known, the number of whales found is pro- digious ; during the last three years American whalers, at the rate of 150 every year, having been employed in that small portion of the ocean. But in no other part of the Arctic zoological region is animal life so abundant as in the north-eastern portion of Siberia, especially between the rivers Kolyma and Lena. A description of the Kolyma dis- trict has already been given in the preceding remarks, to which the following particulars may now be added. The first animals that make their appearance after the dreary winter are large flights of swans, geese, ducks, and snipes: these are killed by old and young; fish also begin to be taken in nets and baskets placed under the ive. In June, however, when the rivers open, the fish pour in in immense numbers. At the beginning of the present century several thousand geese were sometimes killed in one day at the mouth of the Kolyma; about twenty years later, when Ad- miral Wrangell visited that place, the numbers had some- what decreased, and it was then called a good season when 1009 geese, 5000 ducks, and 200 swans were killed. Rein- deer hunting forms the next occupation of the inhabitants. About the same time the shoals of herrings begin to ascend the rivers, and the multitudes of these fish are often such, that in three or four days 40,000 may be taken with a single net. On the banks of the river Indigirka the number of swans and geese resorting there in the moulting season is said to be much greater even than on the Kolyma. West of the Lena, and along the whole of the Siberian shores as ‘far as Nova Zembla, and including that island, animal life presents a great contrast to the preceding portion, as it is nowhere found in such abundance as in the districts already described, and in many parts it is extremely scarce. Spitz- bergen, although possessing considerable numbers of animals, 300 Mr Petermann’s Notes on the Distribution of especially reindeer of the best description, is greatly inferior to north-eastern Siberia in that respect. Having now completed this circumpolar view of the dis- tribution of animals, its causes remain to be considered. The development of vegetable and animal life in the Arctic regions chiefly depends on the warmth of two or three, or even one summer month ; and it may be in general assumed that where the summer warmth is the highest, there plants and animals will be found in greater number and bulk than in other regions where the temperature is lower. This as- sumption is found to be correct as far as actual observations have been extended. The distribution of temperature in the Arctic regions and its causes I have elsewhere* discussed ; in this place the summer temperature only requires to be considered. To afford, however, the elements of a complete view of the distribution of temperature within the frigid zone, I have collected the observations made at various points, in- cluding some interesting stations not strictly belonging to the Arctic regions: these results are given in the Table (pp. 306, 307) and enumerated with respect to latitude. According to Sir John Richardson, terrestrial animalsare abundant in the polar regions for two short summer months only. Birds fly to the north to perform the functions of incu- bation and rearing their young, which done, old and young, with the exception of some scattered flocks of dovekies, desert their breeding-places, and with the frost wing their way southwards. Reindeer, musk-oxen, and the beasts of prey which follow in their train, do not quit the continent to visit the Polar islands until the thaw has made some pro- ’ gress in thinning the snowy covering of the pastures, and — they return towards the woodlands again as soon as the sea is fast, or sooner, if the straits which separate their summer haunts from the main are narrow enough for them to swim — across. The temperature of the month of July, which cor- — responds with the summit of the summer, appears to be a — pretty sure index of the occurrence or abundance of animals — in those regions. The following table exhibits the places of * See Petermann’s “ Search for Franklin,” 1852. = Animals available as Food in the Arctic Regions. 301 the lowest mean July temperature of the American half of of the Arctic regions, being all below 40° :— Winter Islands . . . (latitude 6611) . . 804 Port Bowen. . . . (24 SOW TS Daye Ae 36°6 _ Assistance Harbour . ( ‘“ 74 40)... 37°8 RM laisse! D oreo, 6 2.69 DLP Sip4 1 89-1 Observations made on board of vessels navigating Bafiin Bay and Hudson Strait give the following additional re- results :*— Mean Mean Mean Latitude. Longitude. Temperature of July. Baffin Bay . . 70 «(0 59 0 33°5 Baffin Bay . . 70 0 58 0 34°8 Baffin Bay 3 75, 5 59 4 34:9 ‘Hudson Strait ’ 63 0 7 eens : 39°. } Anelliptical curve drawn round the foregoing points, having as its axis a line extending from the entrance to Hudson Strait to Assistance Bay, and including Davis Strait, Baffin Bay, Lancaster Sound, Barrow Strait, Prince Regent Inlet, Boothia Gulf, Fox Channel, with the land between, com- prises the coldest regions on the American side. This region is precisely that in which the fewest numbers of ani- mals have been met with. Beyond it, even to the N., where the July temperature—as in Melville Island—has been found to increase, there the animals also have been found in greater numbers. Dr Sutherland, in his valuable work already quoted, gives some interesting remarks on this head. He says,t “ That deer are more abundant on the N. ‘side of Cornwallis Island, adjacent to Barrow Strait, no person need doubt; for Captain Penny’s and MrjGoodsir’s ppevelling reports contain frequent allusions to the’ numbe s 4 *# As given by Dr Sutherland in his “ Journal of a Voyage to Bafiin Bay and Barrow Strait.” See Appendix, p. clxxvi. 4 _ t “Journal of a Voyage to Baffin “Bay and Barrow Strait,’ Introduction, p. xxxii. _ VOL. LIV. NO. CVHI.—APRIL 1853. x 302 Mr Petermann’s Notes on the Distribution of of these animals that were seen there; while not one, so far as I know, was ever seen during the whole year in any of the frequent excursions made from the ships in Assistance Bay.” Again: “ It will be rather peculiar if we find that these animals take towards the N. side of Cornwallis Island as the winter approaches, that they may share the modifying effect which the open water in Queen’s Channel must have upon the atmosphere in its vicinity ; and it will appear at variance with the generally received opinion that these animals mi- grate southward on the approach of winter.” It would have been interesting if a series of observations of the tempera- ture in the regions referred to by Dr Sutherland could; have been made, so as to draw a comparison in that respect with Assistance Bay. In Wolstenholme Sound, at the head of Baffin Bay, though having a July temperature of 40° 5’, a comparatively small number of animals were observed by the expedition of the “ North Star.” This is a point, however, from which animals can easily migrate to the 8. or N.; and if the temperature be higher farther N. during the summer, as is highly pro- bable, they unquestionably would extend their migration in that direction. Dr Sutherland has an interesting remark bearing on the point :— | “The Esquimaux lad whom Captain Ommanney took on board H.M.S. ‘ Assistance,’ at Cape York, says that the Esquimaux who inhabit the coast in the vicinity of Whale ~ Sound, at the top of Baffin Bay, clothe themselves with the skin of the musk-ox (umingmak). This statement, if — true, would lead one to the idea that the musk-ox inhabits still more northern regions than Melville Island—regions , whence they cannot return into a more southern latitude with the close of the season, owing to the open water in — the top of Baffin Bay throughout the whole winter. And | moreover, it may lead to the inference that such regions as can maintain the musk-ox throughout the year in so high a latitude as 77° and upwards, must present features with re- spect to temperature which are peculiar only to regions in ~ the vicinity of an extensive sea.” . On the Asiatic half of the Arctic regions the July tem- perature stands as follows :— Animals available as Food in the Arctic Regions. 303 Spitzbergen, NW. extremity . . (latitude 80 00) . . 386-0 Nova Zembla, Karische Pforte . ( “ 70387) . . 363 Ditto, Seichte Bay Mime F4QOy oxo S77 Ditto, Matothkin Shar . 4:07 OO) oh. ba. & 1600 Spitzbergen, Hecla Cove (hon FOGG) no. 402 TL OD, 9 1 48'8 « 670 58). w 586 68 82) 6 BLO Kovennoy Filipovskoy Ust Yansk Nishne Kolymsk NON ON SON nn n In this region the influence of the temperature is still more striking, as it has been shewn that north-eastern Siberia, comprising the warmest stations in the foregoing list, ex- hibits not only the greatest amount of animal life in northern Siberia, but throughout the whole of the Arctic regions, al~ though in winter it is the coldest on the face of the globe. It will be seen, by comparing the two tables of the July temperature, that Winter Island is the coldest of all stations ; and this is likewise the case with the mean of the three sum- mer months. This place is consequently the pole of cold of the northern hemisphere during the summer ; and Mr Ber- thold Seemann, the naturalist of H.M.S. Herald, informs me that it it is likewise the phytological North Pole, namely, that point which possesses the smallest number of genera and species.of plants, and whence the number increases in every direction. While thus in Winter Island the most scanty vegetation is found, in north-eastern Siberia, in a cor- responding latitude, noble forests are known to thrive in - considerable extent. It is curious to remember that already that distinguished navigator Frobisher, nearly three hundred _ years ago, in describing the country round the Strait named ; after him, says that under a latitude of 62° it was colder _ there than in Wardéhuus in Europe, in latitude 703°, the ; former being comprised in the district I have shewn to be the coldest in summer in the Arctic regions, as far as our _ present knowledge extends. It is much to be regretted that _ the efforts of the numerous Arctic expeditions in this cen- _ tury—in the hope to effect the so-called ‘‘ North-western’”’ _ passage—should have been almost exclusively directed and - accumulated upon that region,—the most desolate, and, per- 304 Mr Petermann’s Notes on the Distribution of haps, the most uninteresting, as well as the most difficult and dangerous portion of the Frigid Zone. Without going further into detail, I will merely add a few words as to the bearing of the foregoing observations on sans John Franklin’s Bepeditidn, The general opinion is that the missing vessels have been arrested somewhere between Wellington Channel and Behring Strait and the Siberian shores. Most probably their position is nearer to the latter than to the former points. As these three regions abound in animal life, we may fairly conclude that the intervening portion partakes of the same — character, and moreover, that the further Sir John Franklin may have got away from Wellington Channel, and the nearer he may have approached the north-eastern portion of Asia, the more he will have found the animals to increase in num- ber. The direction of the isothermal lines corroborates this assumption, as they are indicative of a higher summer tem- perature in that region than in any other within the Polar basin. Those countries being probably uninhabited by man, the animals there would have continued unthinned by the wholesale massacres by which myriads are destroyed for the sake only of their skins or teeth. An interesting fact was mentioned in this Society by Lieutenant Osborn, namely, that Captain Penny, in Septem- ber 1850, had seen enormous numbers of whales running southwards from under the ice in Wellington Channel. We know this to be also the case in the Spitzbergen Sea every spring, and that these animals are numerous along the Sibe- rian coasts. ‘This not only tends to prove the existence of — one, or perhaps two, Polar Seas, more or less open through-— out the year, but also that these seas abound in animal life, as to satisfy enormous numbers of whales a large amount of — foodis required. And it is well known among the Tchuktehi, on the north-eastern coasts of Siberia,—where land to the — N. is said to exist in contiguity and probably connected with the lands discovered by Captain Kellett,—that herds of rein-_ deer migrate between those lands and the continents. ‘Taking all these facts into consideration, the conclusion — seems to be a reasonable one, that Franklin, ever since enter- Animals available as Food in the Arctic Regions. 305 ing Wellington Channel, has found himself in that portion of the Arctic regions where animals probably exist in greater plenty than in any other. Under these circumstances alone his party could exist as well as other inhabitants of the Polar regions; but we must not forget that, in addition to the na- tural resources, they would in their vessels possess more comfortable and substantial houses than any of the native in- habitants. So far as food is concerned, reasonable hope therefore may be entertained that the missing Expedition would not alto- _ gether suffer by the want of it ;—their fate, however, depends - upon other circumstances as well, among which, that dire scourge of mariners, the scurvy, is probably more to be feared than any other. My authorities have been the works of the various expe- ditions undertaken in the Arctic regions by the English, Russian, Dutch, and other nations; the zoological accounts of Richardson, Baer, Wrangell, and others ;: also the valu- able papers on the distribution of mammals by Dr Wagner. The meteorological data are chiefly derived from Dove’s tables, and the works of Richardson, Sutherland, Middendorf, and others. 306 Mr Petermann’s Notes on the Distribution of THERMOMETRICAL OBSERVATIONS in the ArctT | = a Elev. Jan. | Feb. | March.) April.| May. | June. | July. 1} Spitzbergen . . . {| 80 2) Hecla Cove ay / 7) 3 Greenland Sea . .| 78 4+ Wolstenholme Sound! 76 Lat. 80° to 75°, ° | © ¢ | Feet. 5 | Mel -1si9 | - 821] 1682| 3621] 49.45 6 | Assistance Bay. «| 7440 | 9416] ... | -29 | -298 | -224 | -32 | IL | 843 | 37:8 7 | Novaia Zemlia 74 0] 58 Of ... | 9°32] 10°°9{ 10°38] 1069! 2430] 34:41] 87°67 (Seichte Bay). 8 | Port Bowen . . «| 73 14] 8856] ... | -28-91 | -27:32 | -28:38 | - 650 | 17:57 | 3612 | 36:55 9 | Novaia Zemlia (Ma-| 73 0 |- 57 20; ... 4:28 | - 7:74 4°46 826 | 1974 | 34:57] 39°97 tothkin Shar), 10 | North Cape, Island | 71 10 |- 26 11! ... 22°08 | 23°16 | 2475 | 80°02] 84:07] 4015] 4660 | of Mageroe. 11 /KovennoiFilipovskoi| 71 5 |-118 0 212) Ustyansk.. .. re 13 | Novaia Zemlia, Ka- | 79 37 |- 57 47]... 9.98 rische Pforte. | Lat. 70° to 65°. pee Se Ores i460 69,1 BB Tih, | caeieo 15 | Niabue Kotyvmsk . | 62 2 | 8b 53} .. | -1613 Pee es |” | G8 82 |-160 66.1"... Broker 17| Kotzebue Sound «| ¢g 9 | 163 9 | |. ; 1g | Fort Confidence | 6 54 | 118 49 | 500 | -21°57 dl Be ee ee eS oe wt) Rm } Lat. 75° to 70°, Melville Island .j| 74 47 | 11048] .,. | -31:28 | -82-45 20| Eyafiord . « - «| @§ 30! 2030! 2. | 2570! 18:50! 20°66! 2750] 3614! 4352] 4694 j2.) Winter Island . ./ g¢ 11 | 8311] ... | -2317 | -25:99 | -10-72| 6-48] 23-29 | 23:17] 35°86 22 | Sort Franklin 2. | 86 0 | 147 0 | 200% 26:85 | -26-44 | -1116 | 1266 | 41°24 | 53-49 | 65-75 723} Fort Franklin . . | 65 12 | 12313 | 500 | -23°33 | -16-75 | - 5:38} 1235] 85°18} 4802] 5210 Lat. 65° to 60°. 24) Archangel. - - | 6432 |- 4033] ... | 657) 923 21:00] S139) 4168] 5518) 602 25 hac mperpree - | 64 98 | 113 06 | 850 | -15°57 | -25°88 | -13-48 | 5°78] 81°20 t 26 Wat he cebu 2 Eee 10 pean ea 12:38 | 19°56 | 15°60] 22°01} 8216 | 89°09} 41:92 1A errmhut..,- | 64 10 | 52 40)| ... 9:05 | 22:10] 21°65 | 2480 | 32: 40°10 | 4033 20 Rone Reiss i ae Oe a oe Nea 1) | 29°82 | 28:31 | 29°86 | 36°46 | 44°80] 51:58} 5619 2) | yak, tek? * 1 | 62 46 | 109 0 | 650 | -25°00 | -18'84 | - 6-14 8:23 | 36°03 80 | eae Senpson’ . |-62 .1 |-d29 44| ... | 45-47 | 28°86 | - 643 | 16:36) 86-91 | 55:28 | ~ 68-79 BL elle Bapke . . 1 | 61 SL | 121 51 | 400 | -1254 | - 9°06 | 555 | 26-28 | 48:16 | 6364 | 60-07 p32 Ro - R aa Fibs >| 61 30 | 180 0 | 1400 J -21°95 | -14:73 | -— 0°99 | 20°44 2 B35 | Tl othtenau . . , | 64 10 | 118 51 | 500] 0-42 | -2560 | 995) 12°88) 40-14 ees 2 *| 60 35 | 46 ‘a 19°74 | 23: 27°63 | 3243 | 89°27] 43:09 | 45°37 Lat. 60° to 55°. | 95 | Friedrichsthal . . } 60 45 19°62 | 1872] 2210] 27°50 3 | 36| Petersburgh . . .| 59 56 |- 3018] ... 14°74 1868 | 25:50 | 87°18 | 48°52 v| 27 | Fort Churchill . . | 5902 | 9310] 20} ~21-21 | - 7.31 | - 463 | 1629 | 28-42 t f3s| Fort Chepewyan .| 58 43 | 118 20| 700] - 876 | - 4°01] 3808) 19°80 | 45-40 3 391) Hebron... « « + 58 0 64 0 Bag — §'24 | - 5°31 4°62 16°83 33-01 % Oy Okakistic. & > = ip }BT 80 086..05) ous 215 1°95 8°25 | 29:0 38:25 3 41| Nain. ; 57 10 | 6150] ... 095 | 3°51 752 | 2997 | 86°98 3 42| Sitka 2... .| 57 3/18518] 4. | 8418 | 3360] 38:01 | 40°64 | 48:18 {§ 43| York Factory . . | 57 0 | 9226) 20] - 512) - 660) 477 19:21 | 33°53 8 : | Lat, 55° to 47°. 44 Oxford House . .| 54 96 28 | 400 | -22-06 0| 857] 2862] 38-01 55 45 Cumberland House | 53 47 | yi 46) Hu'nk ... . .| 53 52 | 166 25 re 34°27 32° 47 | \\upert House . . | 51 21 | BO 1. St SOND fis. “a > : | London (for com- | 51 30 | 1 parison). The longitudes are East when - is prefixed, and West when tlere is no sign,——* Difference of the he Land’——S., Sutherland, ‘ Journal of a voyage to Baffin Bay and Barrow Straits.’-——M., Middendorf, ' . tious are from Dove (17th and 18th Reports British Association, 1847 & 48)———{ By interpolation, Animals available as food in the Arctic Regions. 307 i is m | Differ. z is . EH. &C.| Differ | > | Hour ‘zB * # Months.|S. & Wf 3 of sl Ly ok + é | Observation. | £ 4, | 4 *3 | 2-hourly. hourly. f 3 | da extr. } 1 {| 6 times. R.§ 1 | 2-hourly. 1 | 3 hourly. S.§ 1 | 2-hourly. d 1 | 2-hourly. 1 | 2-hourly. ‘ 1 f2 | 8,12, 4,12. 1 | 2hourly, ie hourly. 2-hourly. 8, 8. daily extr. 15 to 17 times. | R.f 8 times. RO RD bel BOBO ts} > 2 bo =3 ° (=| len] — te eo 2 6 times, He 09 9 CO wie CNiQi 7,2, 9. 10,10." d. extr. 15 times. 5 times. &. 5 times. 3 Oe —_ »| BODO a bv ts] mn by we = oOo faery LS) at SS =) SE Teen ea eee weE Rrwnm mow: 2333) 15°59 25°32 44 0 40-4 months,—-} Difference of Summer and Winter. R,, Richardson, ‘ Boat-Voyage through Rupert’s erston Norden und Osten Sibiriens.’ T., Transactions Royal Society ——The rest of the Observa- ons tO the 19th Aug, only,—|| 25--30 Apri] —T 1—26 October, 508 Professor Horsford on the Efect of Heat on the The Effect of Heat on the Perpendicularity of Bunker Hill Monument. By Prof. E. N. Horsrorp, of Harvard, North America. Soon after the pendulum was placed in Bunker Hill Monu- ment, it was observed that the ball when at rest was not always over the same point in the floor. The careful con- sideration of all the conditions of this fact resulted in ascrib- ing it to the unequal expansion of the sides of the monument, in consequence of unequal exposure to the sun. A brief description of the present condition of the monu- ment will aid in understanding the mode of observation pursued. The obelisk, thirty feet square at the base, rises, gradually lessening, to a pyramidal summit, two hundred and twenty- one feet. Within is a circular well, seven feet in diameter — at the bottom, and five at the top, where it opens into a chamber or observatory. The chamber is approached by a winding stairway. In the centre of the roof of the chamber is an iron staple which was securely fixed at the time of placing the capstone. It served at first to support machinery for carrying visitors up and down. From this staple, which is over the centre of the open space or well, the pendulum is suspended by means of a screw clamp. From a point in the floor directly below the index attached to the ball, circles were described and graduated, and radii drawn. On the day following the graduation, the index was found to be on the one side of the centre of the circle. As the screw clamp first employed did not admit of adjustment, a new apparatus, with the necessary modifications, were. sub- — stituted, and the ball brought precisely over the centre of the graduated circle. A few hours later, it was found out of the centre. Upon observing more carefully, it was found during clear — days that the motion of the ball in the morning was to the westward, at noon to the northwest, and at evening to the east. It was further observed that on days when the sun was obscured by clouds, that no motion of the ball or its in- dex point occurred. It was still further observed on one Perpendicularity of Bunker Hill Monument. 309 occasion, during a sudden shower, accompanied with strong wind from the southeast, at about three o’clock in the after. noon, to move in the space of a very few minutes a quarter of an inch to the eastward. Observations at seven o’clock in the morning, at twelve o’clock at noon, and at seven o'clock in the afternoon, were recorded through several weeks, and no doubt remains that a cause coincident with the sun in its progress produced the variation of the perden- dicular in the monument. A fact already hinted at, further confirmed this conclusion. The extreme departure of the ball from the centre was to the west of northwest; not to the north, as might at first glance be supposed. The explanation is found in the posi- tion of the monument. Its sides do not face the cardinal points, but are inclined about 20°. The expansion of a single side would produce inclination in a direction perpendicular to the side. ‘The expansion of two adjacent sides would pro- duce inclination in the direction of the diagonal. In the morning the shaft is inclined to the westward. At noon it _ is inclined but a little to the north of west. In the progress of the afternoon, it sweeps over twice the amount of move- ment in the morning; describing, in the twelve hours of ob- servation, an arc of an ellipse. During the night it sets back to the centre, and before seven o’clock in the morning, has already moved westward. The greatest diameter of the irregular ellipse, described by the index in twenty-four hours, is ordinarily less. than half an inch, while the least was less than a quarter of an inch. | It would not be difficult to find the expansion of the granite to which this movement of the ball corresponds. In the simpler case of a rectangular shaft, the departure of the ball from the centre would be the versed sine of an are (the side of the shaft), of which the pendulum was the sine. The difference between the are and sine would be the expansion of the granite. - The heat of the sun penetrates to but a moderate depth. This is evident from the prompt movement of the column when a shower falls only upon the more highly-heated sides, 310 3 =§ Perpendicularity of Bunker Fill Monument. and also from the ready change in inclination as the day ad- vances. The effects here observed, and which are now recorded from day to day, taken in connection with the meteorologi- eal record of Boston, Charlestown, and Cambridge, cannot fail to be of high interest. The expansion of granite by heat had before been observed. Mr Bond, the director of the Cambridge Observatory, noticed its effect on his transit instrument erected in the temporary establishment at the corner of Quincy and Harvard streets. The instrument rested on two granite pillars. In the morn- ing of a clear day, his meridian mark on a distant hill would be found east of the meridian line as indicated by his instru- ment; at noon, or a little past, coincident with it; and at evening west of it. Engineers have observed it in long walls of masonry. It can scarely be doubted that we have memorials of it in the ruins of Baalbec and Pestum, of Nimrod and Stonehenge; nor can we question that it has played a large part in the de- struction of cliffs, or the splitting of mountain masses. The mode of observation at the monument is this: On either side, about three-quarters of a inch from the centre, under the index of the ball, two slender needles have been driven into the floor, leaving not more than the sixteenth of an inch above. ‘These are made by pressure to pierce a card of thin drawing paper, which is kept from warping by slen- der bars of lead. When fixed the north and south and east and west lines are transversed in pencil mark from the floor to the paper. After bringing the ball to rest, in which the observer is aided by a contrivance enabling him to steady his hands, a dot is made with a pencil immediately under the index point, which is about the sixteenth of an inch above the paper. At the close of the day, the card, previously dated, is removed, and another takes its place for the observation of the next day. It is a grateful duty to state that the expense of the ne- cessary fixtures at the monument for the pendulum experi- ment, of which advantage has been taken in the observations here referred to, has been incurred by the Massachusetts On the Geological Distribution of Marine Animals. 311 Charitable Mechanics’ Association. The enlightened libe- rality of the directors of this association is only equalled by the generous and efficient co-operation of the officers of the Bunker Hill Monument Association.—(Proceedings of the American Association for the Advancement of Science.) rN NE enn On the Geological Distribution of Marine Animals. By Professor EDWARD FORBES. Professor Forbes, in his Map of the Geological Distribution © of Marine Life, and on the Homoiozoic Belts, shews the pro- vinces under which animals and vegetables are assembled, and these provinces are delineated so as to shew their pecu- liarities, relations, and contrasts. The character of each is marked by the entire assemblage of organised beings, consti- tuting its population, a considerable portion in most cases being peculiar, and a still larger number of species having their areas of maximum development within it. The several provinces vary greatly in extent, some being very small and some very large. The northern and southern limits of each province correspond with the boundaries of a latitudinal belt, to which, on account of similarity of organic features, pre- sented through its extension, the name of Homoiozoic is pro- posed to be applied. Nine of these belts are distinguished, of which one is unique, central, and equatorial, and four in the northern hemisphere represent as many in the southern. The boundaries of the belts on land appear to correspond with the isotherm ofsthe months in which there is the greatest vivacity of animal and vegetable life. The Homoiozoic belts are not of equal breadth inall parts; the polar belts include only a single province in each, the other severally include many provinces. There are twenty-five provinces. 1. Arctic; 2. Boreal; 3. Celtic; 4. Lusitanian; 5. Mediterranean ; 6. West African; 7. South African; 8. Indo Pacific; 9. Australian; 10. Japonian ; 11. Mantchourian; 12. Ochotyian; 13 Sitchian ; 14. Oregonian; 15. Californian ; 16. Panamian; 17. Peruvian; 18. Araucanian ; 19. Fuegian ; 20. Antarctic; 21. East Pata- gonian; 22, Urugavian; 23. Caribbean; 24. Carolinian; 25. 312 Mr G. A. Rowell on the Virginian.—(For an account of Professor Forbes’s regions of depths, vide vols. 50, 51, and 52, Edin. New Phil. Journal.) a On the Change of Temperature in Europe, and the Variation of the Magnetic Needle. By Mr G. A. Rowrnu.* With a Map. From the attention now given to the effects of glaciers in producing geological phenomena, much interest has been excited as to the cause which has brought about the change of temperature in Europe since the glacial period. This change of temperature is, I believe, intimately con- nected with the change of declination of the needle, and in the theory which I first submitted to this Society in 1839, on the cause of terrestrial magnetism, I attributed the change of declination in this hemisphere to a decrease of temperature in the higher latitudes of America, or to an in- crease of temperature in those of Europe and Asia. In a recent communication on Scandinavia, allusion has been made to several geological facts, which are, I believe, connected with the cause of these changes. I trust, therefore, I have chosen a proper time to bring the subject under the consi- deration of this Society, as I hope to shew the causes of this change of temperature, and also the probability that these causes have been in operation to a sufficiently recent time, to account for the variation of the needle. Before I proceed further, I will describe the accompany- ing Map, as I shall have to refer to it often. The lines of equal magnetic intensity are shewn by the broken lines; these are taken from Col. Sabine’s maps, in the Sixth Report of the British Association. The point of greatest intensity is shewn by the spot at 52° 19’ north lati- tude, 92° west longitude ; the intensity decreasing from this point as shewn by the lines 1.7 —16—-15—14 The American magnetic pole, according to Sir James Ross, is in north latitude 70° 51’, west longitude 96° 46’. The Asiatic magnetic pole, according to Hansteen’s observations, is in * Read before the Ashmolean Society, January 31, 1853. T LIV aaa ! Edin’ New Phil, Journal E Magnetic Intensity G C A ; Rk owe i Ksothermal Lines 2 Lint oem Spring —...-. > ON ae rae ’ : ' Line of Maximum Temp oc... Ch MIGES OF TEMPERATURE j / : | : American Magnetic Pole i | = ae é Asiatic Magnetic Tole aL UW IR O PP ae L . S k Greatest Magnetic Inlensiqu and the VARIATION of the : : i MAGNETIC NEEDLE. Ay 14 tnikerland ee \ | rps ons |: ~ — bay : if ~ SG; Ax iN aa i a 4, { 4. koWnb tec HW neertar va joe oy aaa a if Poe ia Azores y 2 all 2g by Wi AK Johnston Fain? — ieee : fel m eerie on EURTs bit # i wk, ae, aa . - ae | ae Ale 3 peli | $eai% Si aKe = ‘ * 4 S % e. j ory | é waagee , t 5 5 oe ‘ ’ mR . i x of r ». - = ie “a ! pt i sd ‘ hen Ser OF > y "7 ~ £ , Cd 4 % . ; c - , ‘ . - » x. J ‘ F, i « . ’ a ] * = : a 4 \ : : ‘ i n f ai VRSRS } a a LAT ' « f i ; ; wine eS p f / . a ¢ et ae a apes yay f betty 4 ; ’ ’ i 4 . a! J E , fi P - ae = F - . E i ‘ ‘ ; ie we by ~ yf «“ _ ~ ‘ .- a ’ 6 3 > . * ~~ ' ; ‘ . i ; m : 7 ~~ ft, 4: 1. , te 3 . us - ae, , - r f ‘ hae! 4 | fe — ‘ wv Pd i . ‘ " . s PO | 9 Variation of the Magnetic Needle. 313 85° north latitude, 116° east longitude. The plain lines shew the isothermal lines of 5°, 10°, 20°, 30°, and 40° of temperature ; the dotted line is the line of maximum tem- perature. This is not an isothermal line, as it varies from less than 80° to more than 85° of mean temperature. These lines are all from Johnston’s Physical Atlas. As few persons are acquainted with the theory I propose on the cause of terrestrial magnetism, it will be necessary to explain it; but I shall do so inas brief a manner as possible. As the trade-winds are caused by the cold and condensed air from high latitudes pressing onward and raising the warmer and lighter air in the tropical regions, the air thus raised must flow back again in an upper current towards the colder regions, to keep an equilibrium. Thus the air is in constant circulation from the colder to the warmer regions along the earth’s surface, and from the warmer to the cclder above. | . It is well known that during evaporation electricity is carried off, and the water from which the vapour has arisen is left in a negative state; it follows, therefore, that the - tropical regions must always be in a negative state, owing to the vapour and its electricity being carried from thence _ by the rising air; and the vapour and its electricity carried by the upper current to the polar regions must render those parts positively electrified, and it is to the rush of electricity from the positive to the negative parts of the earth that I attribute the direction of the needle. The cause of the magnetic poles in this hemisphere I be- lieve to be the vast quantities of ice blocked up both in winter and summer above the two continents, thus keeping _ those parts constantly colder than any other parts in the same latitudes ; consequently these centres or poles of cold are the magnetic poles. For as the density of the air in- creases with the degree of cold, it follows that there must be more air flow from these coldest parts towards the warmer _ regions than from any other district ; consequently there must be a greater flow of the upper currents of air with its _ vapour and electricity, from the warmer regions to these ¥ coldest parts, than to any other. ‘' ¥ 314 Mr G. A. Rowell on the Now, if the point of greatest cold were at the terrestrial pole, and the temperature and evaporation increased regu- larly from thence to the equator, the electricity would pass off from the pole towards the warmer parts of the earth, directly in the lines of longitude, and there would be no de- clination of the needle except that caused by the greater evaporation, where the sun may be above the horizon. But as the poles of cold are at a distance from the terrestrial pole, as there is more electricity received at these parts than in others in the same latitudes, the electricity cannot all pass off in the lines of longitude, but must diverge eastward and westward of them, to gain its equilibrium in passing off to- wards the more negative parts of the earth, and thus cause the declination of the needle as the currents of electricity from the frigid to the tropical regions in every meridian must, in some degree, be affected by the divergences of the currents from the magnetic poles. As I consider the poles of cold and magnetic poles identical, I shall use the terms as Synonymous. The lines of equal intensity of magnetism by no means correspond with the parallels of latitude. If we trace the line 1.5, it has its highest northern limit, 7, e. 73° north lati- tude, at about 10° east longitude. To the westward it de- scends through Iceland, passes west of the Azores, and reaches its lowest latitude, 23° north, in the Gulf of Mexico ; it then rises again, and about 20° west of Behring’s Strait has its second highest latitude 53°; it declines again to 41° in the meridian of the Asiatic pole, from whence it rises again to its highest northern limit. The course of this line shews the great intensity of the American pole as compared with the Asiatic. ‘The declination of the needle also shews the different effects of the two poles, as the declination ap- parently caused by the Asiatic pole does not extend over more than about 100° of longitude ; whilst the declination of the needle over the remaining 260° seems to be affected in some measure by the American pole. This difference in the intensity of the influence of the poles may arise from the American pole being the coldest, or from the air forming the upper current to that pole, being more loaded with va- Variation of the Magnetic Needle. 315 pour, and consequently electricity, than the current flowing to the Asiatic pole; or it may be caused by the ice in Ame- rica being blocked up at much lower latitudes than in Asia, thus producing in a greater degree those currents of air, vapour, and electricity, to which I attribute magnetic phe- nomena. It may be observed, that the point of greatest intensity is between Hudson’s Bay and the Gulf of Mexico, and that the lines shew the great intensity from the American pole in the direction of the warm equatorial seas between Africa and America. The intensity of effect from the Asiatic pole seems to be influenced by like causes, as it is directed towards the Indian Ocean, where the line of maximum temperature has its greatest northern latitude, i. ¢., 12° 30’, and where the tem- perature of that line is at the highest, viz. 853° of Fahrenheit, and consequently where the evaporation is greatest. Thus, in both cases the greatest intensity is from the poles towards the nearest parts where the evaporation is great. In the meridian, where the intensity is the least, we find no such pole of cold, and the tropical region is occupied by Africa, consequently the rate of evaporation is low; and in the meridian of Behring’s Straits the Arctic Sea is open, and the line of maximum temperature is about 7° south of the equator, so that this line is nearly 20° farther to the south in that meridian than it is in the Indian Ocean, and the temperature lower. The lines of equal temperature follow the same general direction as the lines of magnetic intensity, shewing that they are both influenced by the same cause, viz. the two great centres or poles of cold; and generally in the meridians _ where the temperature is highest, the intensity of magnetism is the least, and where the temperature is lowest the inten- sity is greatest. The lines of equal temperature do not differ so much from the parallels of latitude as the lines of magnetic intensity, but yet the difference is great, especially in high northern latitudes. Taking the line of mean temperature of 30° of Fahrenheit, it has its highest limit rather north-west of the North Cape, 316 Mr G. A. Rowell on the i. e. about 72° of north latitude. Passing westward: it de- scends to the 54th degree of latitude, and shews a mean tem- perature of 20° lower in the eastern parts of America, when compared with the same latitudes in Iceland, England, and the north-western parts of Europe. ’ This difference of temperature is generally attributed to the effects of the Gulf Stream; but although there is high authority for this opinion, I venture to suggest that other causes operate in a much greater degree in producing this phenomenon. That the temperature of the Atlantic Ocean has some effect I do not deny, but the proofs of a continua- tion of the Gulf Stream, or of there being any stream from the Atlantic into the Arctic Sea, are very meagre, chiefly, I believe, depending on the fact, that plants from the Guif of Mexico and the West Indian Islands are occasionally found on the shores of England, Iceland, Norway, &c.; but when we consider the vast quantity of such materials brought by the Gulf Stream into the midst of the Atlantic, it is reason- able to suppose that the whole of its shores must occasionally have some of these things thrown on them by storms, «ce. I am not aware that the Gulf Stream can be traced farther north than the 49th degree of latitude, and the fact that a bottle thrown into the sea by Sir W. KH. Parry, in latitude 53° 13’ north, longitude 46° 55’ west, was picked up on the shore ot Tenerifle, seems to support this idea, as it must have crossed the direction of this supposed stream. It is a very general opinion that the western sides of con-. tinents are always warmer than the eastern; but this is not supported by facts, as the temperature of Africa is lowest on the western side, and the same is the case with the whole of America, from ‘the 30th degree of north latitude to ae Horn. I beg to suggest, that the principal cause of the unequal distribution of temperature in high northern latitudes is the blocking up of the ice in the seas above the Asiatic and American continents, thus making those parts the poles of cold, whilst the Arctic Sea being open from Norway to Green!and no such accumulation of ice can take place there, consequently the temperature is higher there than in any Variation of the Magnetic Needle. 317 other parts in this hemisphere in the same parallels of lati- tude. The opening into the Arctic Sea through Behring’s Strait produces similar effects in those regions, but in a lesser de- gree. It is true that the isothermal lines in the North Pa- cific Ocean have not their highest northern limits in the meridian of the Strait, but to the east of it; this fact supports the theory, as the high temperature of the western parts of North America may fairly be attributed to the great height of the Rocky Mountains intercepting the cold breezes from Hudson’s Bay and the frozen seas above it. With respect to the changes of temperature which have taken place in Europe, it is evident, from glacial marks and deposits in Switzerland, Scotland, and in almost the whole of North-Western Europe, that the temperature of these regions has been much lower than at the present time. I will not attempt to give an opinion as to the depression of temperature which would produce such an extent of glaciers ; but M. Charles Martins, in an article* “on the Ancient Ex- tent of the Glaciers of Chamounix,” calculated that a mean temperature similar to that of the northern part of the State of New York, by lowering the line of perpetual snow, and enlarging the area for its accumulation, would be quite suffi- cient to account for the extent of ancient glaciers in the district around Mont Blanc. On this authority, therefore, I conclude that the extent of ancient glaciers in Europe may be accounted for by a temperature such as now prevails in similar latitudes in the eastern parts of America. - _ Ithas been suggested, that a change in the direction of _ the Gulf Stream may have been the cause of the change of _ temperature since the glacial period ; this cause alone seems insufficient to produce such effects, and the supposition of any change in the course of the Gulf Stream is purely hypo- thetical. I submit that this change of temperature may be fairly attributed to geological changes, of which we have evidence - at the present time. I believe the low temperature of the * Edinburgh New Philosophical Journal, No. 85. VOL. LIV. NO. CVIII.—APRIL 1853. ¥ 318 Mr G. A. Rowell on the eastern parts of America, from the 40th to the 65th degree of latitude, is caused by the vast quantities of ice blocked up in Hudson’s Bay, as it is a large sea open to receive the icebergs from more northern regions, and cut off from com- munication with the warmer waters of the Atlantic Ocean, the only opening into it being Hudson’s Strait, from whence the current sets into the Atlantic. I will endeavour to shew that there are fair nea for . assuming, that very similar circumstances prevailed in Europe in recent geological times, and consequently it had a like depressed temperature. I believe it is now considered proved, that since the creation of races of animals at present existing, England and the Continent were connected by dry land. If, then, we consider the British Channel to have no existence, the German Ocean would form a sea similar in latitude to Hudson’s Bay. We have farther the facts given by Sir R. Murchison, in his paper ‘‘ On the Superficial De- tritus of Sweden,” which shew, that since the southern part of Sweden was inhabited by man, the more northern parts and neighbouring districts were covered by water: that pre- vious to the elevation of this land, the last geological change was the distribution, by means of icebergs, of innumerable distinct angular blocks of stone over these districts. That these icebergs must have been immense is shewn by the size of some of the stones which have been so distributed, one measured by Sir R. Murchison was 40 feet long, 23 feet wide, and 25 feet high, and another was still larger. From the nature of these stones, it is evident that they have all been carried from north to south, shewing that the current was in that direction ; proving also that these regions were then open to the Frigid Ocean; and as this current was from north to south, it is fair to assume that it found its way into the German Ocean, and thence into the Atlantic. If I have taken a fair view of these subjects, the condition of North-Western Europe at that time was very similar to that which now prevails in the north-eastern parts of Ame- rica, Great Britain representing Labrador, Norway standing for Cumberland Island, the German Ocean, with its connec- — tion with the Baltic and Frigid Seas, forming another Hud- — Variation of the Magnetic Needle. 319 son’s Bay, the current from the Baltic and the German Ocean passing into the Atlantic, between Norway and the Shetland Islands, taking the place of the cold stream from Hudson’s Strait. It is to these circumstances I attribute the depression of temperature during the glacial period, and the subsequent | rise of temperature to the German Ocean becoming open to the Atlantic, and the descent of icebergs from the Arctic regions into the Baltic being a Ass by the elevation of land in the north of Europe. I will now endeavour to shew the probability that the variation in the declination of the needle has been caused by this change of temperature. All the earliest observations on the needle shew that Kurope was at that time within the influence of the European or Asiatic pole, as the declination was eastward. Columbus is said to have been the first European who observed a western declination. When on his voyage of discovery to America in 1592, he found the eastern declination become less and less,—near the Azores he crossed the line of no declination, and then found it become westward. Now, as there are two magnetic poles in this hemisphere, there must be a line of no declination where the influences of the two poles are equal; and it is obvious that it was this line of no declination which Columbus crossed, as the declination on each side diverged from it. In 1657 this line had passed eastward, and there was no declination in London,—at this time the declination was still eastward at Paris. In 1666, i.e. nine years later, it was at Paris, and the declination in London had become eastward,—since that time it has gone farther and farther eastward, and is now about 43° east longitude. Nearly all Europe has thus become under the influence of the American pole, and the declination in Lon- don has gradually changed from 11° 15’ east in 1580, to 24° 30’ west, in the early part of the present century, since which time no change of importance has taken place. During the time these changes of declination occurred in Hurope, no change of importance was observed in America; and there is positive proof, that in Jamaica, from 1660 to 2 320 Mr G. A. Rowell on the 1806 the declination did not vary in the slightest degree, although in London, during those years, it amounted to full 24°. This fact is important, as it shews that the American pole, during those years, has not shifted its position, and that the cause of the variation must be connected with the old continent. | In accordance with the theory of magnetism, I have ex- plained, the change of declination may be fairly accounted for, either by the cold of the Asiatic pole decreasing in in- tensity, or by an elevation of temperature in Europe driving the centre or pole of cold farther towards the east; and there can be no doubt that both these circumstances followed the geological changes I have alluded to. It may be difficult to prove that a change of declination, which has been going on up to the present century, can be owing to geological phenomena, which occurred so long pre- vious, but I hope to shew that there are fair grounds for such an opinion. Assuming that during the glacial period the condition of Europe was similar to that of America at the present time, we may conclude that ice extended from the shores of Nor- way, Scotland, Iceland, &e., in a similar way to what it now does from Greenland, Cumberland Island, and Labrador. (The extent of ice from these shores is given in Johnston’s Atlas, and is shewn in the Map). The Arctic Sea must, therefore, at that time, have been blocked up with ice much more than at present, consequently the Asiatic pole of cold could not then have been in its present position, but was proba- bly situate about Nova Zembla ; and if so, it must since that time have receded more than 40° of longitude towards the east. This change of position will account for the change of declination in Western Europe, as the Asiatic pole is now chiefly affected by the evaporation from the Indian Ocean, and quite removed from the influence of evaporation from the warmer parts of the Atlantic. It is impossible to prove how long was required to produce these results, after the geological changes to which I have alluded; to arrive at a fair conclusion on the subject, it may be well to suppose similar changes to take place in America at this time: the Variation of the Magnetic Needle. 321 question for consideration would then be ;—If by some geo- logical phenomenon the southern parts of Hudson’s Bay became exposed to the Atlantic Ocean by an opening similar to the British Channel, and from the 66th to the 70th degree of latitude the land was upheaved so as to cut off all com- - munication from the Arctic Seas, how long a time, under these circumstances, would it require for the whole of the north-eastern parts of America, together with the neighbour- ing Arctic regions, to arrive at the highest temperature they would ultimately acquire in consequence of these changes? For as long as any elevation of temperature was going on, so long would the pole of cold continue to recede towards the west; so long, also, would the variation of the needle go on, and the line of no declination would move from its present situation, near St Petersburg, towards the west. England might thus again be brought under the influence of the Asiatic pole, and the needle throughout Europe again have an eastern declination. In considering this subject, it is necessary to bear in mind how slowly heat is conducted by some earths, and also the fact, that 140 degrees of heat are absorbed by ice in melting without any increase of temperature. Many proofs might be given of the slow transmission of heat through earth, but I will only refer to one, as stated by Mr Nasmyth, in the Journal of the Geological Society, vol. iii, p. 233. “The instance in question” (says that gentleman), “ was that of a large plate-iron pot, containing 11 tons of white-hot melted cast-iron—a temperature so high as to be quite beyond all thermometric certainty, but well known to be the highest intensity of furnace heat, being quite equal to that of welding hot iron. ‘This vast mass of white-hot melted cast-iron, stood in the pot for upwards of 20 minutes, and but for a thin coating _ of elay and sand, of about half an inch thick, would have soon melted the bottom and sides of the pot. * This half-inch thickness of mineral substance, however, _ was quite sufficient to prevent the conduction of the heat to _ the exterior; so completely so, that after this mass of hot iron had remained for upwards of 20 minutes in the pot, you 322 Mr G. A. Rowell on the could place your hand on the side of the vessel without feel- ing any inconvenient degree of heat; and so slowly and imperfectly does this thin lining of half an inch of clay and sand permit the heat to pass outwards, that the entire mass might rest there till it became cool ere the outside of the pot would have reached a temperature high enough to car- bonize wood in contact with it.” With such facts as these, I think it fair to assume that, after the geological change I have supposed, thousands of years must pass ere the parts of America to which I have alluded could obtain their highest degree of temperature : for if half an inch of clay and sand thus intercepts the com- munication of so high a temperature as that of 11 tons of white-hot cast-iron, how can we estimate the time it would require for thousands of square miles of frozen land and sea to become elevated in temperature even a few degrees. _ Bringing these reasonings and facts to bear on the question of the change of temperature in Europe, I submit that there are fair grounds for attributing the change of declination to this change of temperature. For although the opening of the British Channel may date too far back to support this opinion, there are ample proofs that the connection of the Baltic with the Frigid Ocean, and the elevation of parts of Sweden, have been much more recent; and these were the principal causes of the change of temperature in the north of Europe. It has been shewn by Professor Nilsson that the northern parts of Sweden formed the bottom of a sea after the south- ern part was inhabited by man. The land since then has been elevated some hundreds of feet, but the fact that there are no dislocations of strata, shews that this elevation of land has been gradual, and even at the present time an elevation is going on in various parts of Sweden. Dr Daubeny, in his recent communication on Scandinavia, alluded to this fact, and, amongst other authors on the sub- ject, Professor Nilsson states that the elevation of the coast of Sweden has been going on gradually during the last 300° years at the rate of two feet in the century. In proof of the recent connection of the Baltic with the — Variation of the Magnetic Needle. 323 Arctic Sea, Professor Forchhammer may be cited. He says— «The Gulf of Bothnia has been connected with the White Sea, where, in the neighbourhood of Uleburg, 4 considerable depression towards its shores maybe observed, a complete water communication existing from the White Sea through the Gulf of Bothnia and the northern parts of the Ost Sea to the Cattegat ; and adds in a note, that between the Gulf of Bothnia and the White Sea, “a communication by water was kept up in the time of flood, even so lately as at the eommencement of the last century.” Some effects may be attributed to the elevation of land how Soing on, which, together with increased cultivation and drainagé, must tend to an elevation of temperature even ‘at the present time. In submitting these theories to the consideration of this _ Society, I am aware that I can only support them by proba- bilities; but as the change of temperature in Hurope, and - the variation of the needle are subjects on which no theories have been adopted, I have some hope that the opinions I have advanced may be thought worthy of farther considera- tion. The Paragenetic Relations of Minerals. * The natural association of mineral species has long attracted attention, and although since the time of Werner it has been made the basis upon which distinctions between rocks are established, still the subject has not been investi- gated so fully as it would appear to deserve. Minerals _ which occur together are enumerated in the description of one or other of them, but no adequate account is given of the mode of association, and their relations of date are even still less regarded. Professor Breithaupt has for several years especially ' * Die Paragenesis der Mineralien. Mineralogisch, geognostisch und chemisch beleuchtet mit besonderer Riicksicht auf Bergbau. Von A. Breithaupt. Freiberg, 1849, 324 The Paragenetic Relations of Minerals. directed his attention to these points, and has arrived at a number of very interesting results. Of these, and the infer-. ences he draws from them, his general views, and the argu- ments by which he supports them, it is the purpose of the following pages to give some account. By the paragenesis of minerals he understands the more or less definite mode of association, by means of which he endeavours to deter- mine their relative age; and he has conducted his observa- tions from the point of view expressed in a remark of Dolomieu’s, that every stone must have some connection with the general history of our globe, and although individu- ally it may possess but little interest, still in its relations to | others it may lead to important discoveries; further, that it is the study of the most common and most universal mine- rals, and from which valuable results may chiefly be an- ticipated. He in the first place brings forward some facts which are sufficient to shew that the paragenetic relations of minerals are deserving of being studied not only by the mineralogist but perhaps still more so by the geologist and the chemist. . In some instances the existence of a mineral species appears to depend upon the co or pre-existence of another mineral. Thus among epidotes, which are tolerably abundant; manganesian epidote occurs only in association with heter- ocline, consisting chiefly of oxide of manganese ;- and among the titanites, which are still more frequent, greenovite occurs at St Marcel in Piedmont, only together with the above two minerals. JBasaltine is the only amphibole, seme- line the only titanite, melanite the only garnet, and hyacinth the only zircon which occur in trachytic basalt or phonolite. Rhodizite has hitherto only been met with upon turmalin. There are again other minerals, whose existence may safely be said to depend upon the pre-existence of copper pyrites ; thus bismuthine, linneite and cobalt glance. Magnetic pyrites very generally accompanies copper pyrites, which is in this instance the most recent. It is perhaps still more remarkable, that all larger masses of variegated copper pyrites are accompanied by the more recently-formed cop- per pyrites, and the larger masses of copper pyrites by The Paragenetic Relations of Minerals. 325 the still.more recent iron pyrites. These facts shew that there are uniformities in the association of minerals worthy of being investigated. _The paragenetic phenomena met with in druses, further indicate that. the deposition of some more recent minerals has taken place more readily upon certain of the pre-exist- ing minerals than upon others, as if there had been an un- equal attraction. For instance, in the druses in greisen at the Zinnwald, the tungsten is more frequently implanted upon the smoke quartz than upon the mica. In the lode druses of the Friedrich August mine at Freiberg, the cale spar deposited upon surfaces consisting of iron pyrites and heavy spar, seems to have been attracted more by the latter than the former mineral. In the mine Beschert Gliick pyrargyrite, occurring in druses of galena and polytelite, is found almost only upon the latter. | The association of minerals likewise seems to determine the form in which. one of them appears. The galena occur- ring in druses near Freiberg is, when accompanied by diallogite, always in irregular rounded crystals, cale spar accompanying copper pyrites, probably always presents the most ordinary scalenohedron as the predominating form, and the calc spar upon iron pyrites is invariably in flat rhombo- hedric crystals. Another striking circumstance is, that the minerals occur- ring together in a particular district. or formation, possess a certain marked physiognomy, so easily recognisable that the localities of hand specimens may be determined by it. The amphiboles, pyroxenes, epidotes, &c. of Arendal, and the same minerals from New York and New Jersey, the older galena and zinc blende formations of Freiberg and _ those of Cumberland, as well as the minerals occurring in the lodes of Andreasberg (Harz) are sufficient illustrations of these peculiarities. _ Certain associations of minerals belonging to the same genus, sometimes admit of the establishment of specific dif- ferences between them. In a trachytic rock at Laach in Rhenish Prussia, there occur nosean, sodalite, and leucite, imbedded in a porphyritie manner. These three minerals 326 The Paragenetic Relations of Minerals. having been formed at the samé time and under the same | conditions, it may be inferred that they do not belong to one species. In the same manner antholite, anthophylite, and a dark green hornblende, with their characteristic peculiari- ties, occur in immediate contiguity at Kienrud in Norway. In relation to mining, Professor Breithaupt is of opinion that the study of the phenomena of paragenesis will be of great importance by leading to a knowledge of the condi- tions, under which the ores of the useful metals occur, so as eventually to do away with the element of chance, or the reliance upon mere empirical rules, and to substitute in their place a scientific system of mining operations. Al- though, as he admits, this result is undoubtedly very remote, he considers it time that the by no means inconsiderable number of known facts should be collected, systematised, and their universality tested, in order to obtain some positive basis for its future achievement. One of the most import- ant points in such an undertaking, is the progressive development of one imorganic mass from another—the accurate determination of relations of date, both as regards geological formations and individual minerals. He expresses his conviction, that as observation extends, it will become more obvious that the association of minerals has its defi- nite laws—that there exists, so to speak, a certain economy of inorganic nature, whose investigation will be no less attractive than practically useful. It will then be seen that the same uniformities of association present themselves under very different circumstances, in mixed rocks, as well as in isolated deposits, in vesicular cavities, as well as in lodes. It is here necessary to call attention to the fact, that mine- rals present two distinct kinds of structure—the crystalline and the non-crystalline. Although in many compact amor- phous minerals, the ultimate molecules may be crystalline both in structure and form, there are others whose structure | is unquestionably of a different character, for instance, opal and obsidian. Again, of the non-crystalline minerals there are at least two classes, of which the above substances may — be taken as the types, Obsidian bears all the characters of —_ wa EE —————— ss ee ae a a i] The Paragenetie Relations of Minerals. 327 a vitreous mass resulting from igneous fusion, and there is other evidence which strongly favours the opinion that it originated in this way. The opaline structure is equally peculiar, and more frequent, in minerals, than the vitreous. It would appear that those bodies which have an opaline structure, frequently present indications of having been originally in a plastic state; indeed, opal itself has actually been found so. Without taking into account those minerals which may have been formed from solutions, there is an abundance of facts which fairly admit of the inference that the substance of a very great number of minerals possessed at some period of their existence a certain degree of internal mobility, being either liquid, viscous, or plastic, although opinions differ as to the precise nature of this former state.* _ Fuchs is of opinion, that entire masses of rock have been in this state, and that the metamorphism of rocks is essen- tially connected with such a softening. The curvature in the axes of crystals, the partial fracture, contortion and separation of crystalline minerals as it were into slices, as in the garnets, in some schistose rocks, are favourable to this view. Some quartzose rocks consist of angular fragments cemented together by amorphous quartz, and it is not im- probable that the fragments have been formed by the con- traction of gelatinous or plastic silica, and that the cement has been subsequently introduced in a plastic state. Moreover, crystalline substances may, without losing their solidity, experience an alteration of structure, as in the con- version of arragonite into calcite, and there is in many in- stances a remarkable fact of paragenesis connected with the " ealcite, which has originated in this way. Crystals of celes- _ tine are found upon it, which would appear to indicate that _ sulphuric acid has had some share in the change. Stro- meyer’s investigations have shewn, that arragonite generally contains strontia; and as celestine 1s always accompanied by *Tn a physical point of view, it is probable that the molecular structure of bodies depends mainly upon the conditions under which solidification takes “place, and any inferences which may be drawn from the structure of minerals, would appear to refer rather to those conditions than to the former state of the masses from which they were formed. 328 The Paragenetic Relations of Minerals. calcite or limestone, and is always of more recent formation than these, it has possibly originated in all cases from stron- tiferous arragonite. The sulphuric acid may have been derived from the decomposition of iron pyrites. The association of minerals does not always indicate their simultaneous formation. The granular rocks appear to afford the best evidence of this; for while, in some cases, minerals implanted upon each other differ very little in date, in others a very long interval may have elapsed between their respective formations. The simultaneous formation of different mineral species is indicated by their regular twin growth, by juxtaposition, as in disthene and staurolite from St Gothard; dolomite, ripidolite; and a green amphibole, (Pfitschthal, Tyrol) perhaps also in graphic granite, although in the druses, of the three constituents pegmatolite appears to be oldest, mica most recent, and quartz intermediate. When minerals present mutual impressions, such as Fournet has observed in the garnet and mica near Lyons, this cireum- stance is evidence of their simultaneous formation. In most cases, the date of minerals which present a twin-growth by Superposition, is not precisely the same; thus the hexago- nites haplotypicus is rather older than the rutile with which it is compounded (Tavetschthal, Switzerland). The same is the case with the regular twin-crystals of iron pyrites, and spear pyrites (Litmitz, Bohemia); the twin crystals of chlorite upon and with magnetite (Fahlun, Sweden). It ought like- wise to be considered as a universal rule of superposition, at least with regard to varieties of the same species, that the non-crystalline, or least crystalline variety is followed by the crystalline ; instances of this are furnished by compact and fibrous brown iron ore; hornstone and quartz crystals; ‘ allochroite and garnets. Among the more uniform mixed rocks a certain geognosiie relation is presented by the minerals constituting those which possess a granular, schistose, or porphyritic structure. With regard to the phenomena of paragenesis, these rocks may be divided into two classes :— I. Those consisting of silicates, one of which is almoatll . always a felsite, rar ely replaced by nepheline. a The Paragenetic Relations of Minerals. 329 ‘II. Those consisting of silicates with quartz. This distinction is of great importance in the study of eruptive rocks, and in relation to the association of some minerals quite essential, indicating likewise the presence or absence of others. The most frequent of such silicates be- long to the genera felsite, pyroxene, amphibole, phengite, astrite, &c. The felsites are especially important both on account of their greater frequency, and because they include trisilicates as well as bisilicates almost entirely destitute of metallic oxides and magnesia, but rich in alumina and alkalies. ‘Together with these there occur in the first class of rocks pyroxenes and amphiboles containing much iron, though scarcely any alumina or alkalies. It must not be forgotten that some pyroxenes and. amphi- boles are similar in composition, and in such cases may be regarded as dimorphous bodies. Indeed, bronzite and antho- phyllite are identical in composition, corresponding with the formula Fe O Si O,+ 3 Mg O, 2 Si0,. It is therefore possible that certain eruptive masses may have yielded either diabase or diorite, according to the prevailing conditions. Mitscher- - lich has actually obtained crystals of pyroxene by fusing am- _ phibole; and G. Rose has shewn that crystals occur, consisting of a nucleus of pyroxene and an envelope of amphibole. In connection with this point, it is worthy of remark that some _ species of pyroxene occur only in rocks of volcanic, or un- doubtedly igneous origin, such as basalt, lava, &., while others do not occur; and in the former case, the pyroxenes are accompanied by astrites, but never by phengites. In such rocks, pyroxene and amphibole are indeed sometimes met with together, but the occurrence of amphibole is then limited ‘to one species—basaltic amphibole,—which is essentially distinct. e In the rocks consisting of silicates with quartz, for the _ most part the oldest known rocks, associations of such mine- _ rals are observed, as, in the present state of science, can _ Searcely be regarded as of simultaneous formation. When- _ ever quartz is present as an essential constituent, pyroxenes _ are not found, with the single exception of spodumene, which _ although mineralogically belonging to this genus, differs _ 330 The Paragenetic Relations of Minerals. widely in chemical composition from all the other members, inasmuch as alumina is an essential constituent. It is in the study of these more ancient rocks, as in that of the early history of Man, that the greatest mystery, the great- est difficulties are encountered, and the progress of observation would appear to prove not only that the conditions under which they were formed were widely different from those which now prevail, but also that these rocks have experienced many successive alterations. | With regard to porphyritic rocks, Werner entertained the opinion that the imbedded crystals were of earlier formation than the matrix ; however the contrary appears, with very trifling exceptions, more probable, and for the following rea- sons :— 1. The occurrence of crystals which contain nuclei of the mass in which they are imbedded.—This is the case with the large rhombohedrons of magnesite occurring in the talcose slate of the Tyrol. Crystals of leucite, from the old Vesu- vian lavas, not unfrequently contain the same lava in their — interior. The twin-crystals of pegmatolite from Llbogen, q Bohemia, contain not only scales of phengite and granules of — quartz, but nuclei of granite, presenting exactly the same F: appearance as the surrounding rock. Very finely developed | crystals of iron pyrites from Osterode, Harz, with smooth sur- 4 faces, contain nuclei of the gypsum in which they lie, and large | groups of iron pyrites crystals frequently contain intheircentre some of the clay by which they are surrounded. In the horn- stones of Schneeberg (Saxony) hexahedrons of tin white cobalt or smaltine occur with nuclei of the same hornstone. Some pseudomorphous minerals constitute an exception to this gene- ral rule; thus when an envelope of red hematite has been — formed over calcite, assuming its scalenohedron form, and the | latter mineral has been subsequently removed, and red hema-_ | tite deposited in its place. But in this instance the pseudo- _ morph was at a certain period hollow. Again, at Rothen- — berg (Saxony), the fluorspar formerly existing, and of which not a trace is now found, was first covered with fibrous red hematite, and then by some means removed, leaving a hol+ low east, which was afterwards filled with quartz. Some- - ‘ ; 3 . : é % é The Paragenetic Relations of Minerals. 331 times it is difficult, without collateral evidence, to tell which part of a pseudomorphous mineral was formed first, as in the case of rhombohedrons of compact brown iron ore, result- ing from the alteration of spathic iron, and covered with a thick crust of malachite. The latter, however, being a deriva- tive of copper pyrites must be more recent than the brown iron ore, because in the same lode copper pyrites is found im- planted upon spathic iron. 2. The occurrence in sedimentary strata of crystals, pre- senting such sharpness in their edges that they have ob- viously not been deposited as detritus, but formed upon the spot.—Near Meissen, sharply-defined crystals of iron pyrites occur in clay, together with water-worn fragments of quartz, and generally contain a nucleus of carbon. It is probable that they have been produced from ferrugineous solutions by | the reducing agency of carbonaceous matter. Where large groups or masses of iron pyrites occur im- bedded in stratified rocks, a curvature of the lines of strati- fication may frequently be observed immediately around them, to all appearance resulting from the formation of the pyrites on the spot. In the brown coal-formation, iron pyrites occurs chiefly where the coal-seams are in contact with large masses of clay. As might be expected, a carbonaceous nucleus can- not always be found in iron pyrites, but a nucleus of hepatic -pyrites is frequent, and this contains sulphuret of carbon. Again, other than carbonaceous nuclei occur in iron pyrites. In the alluvium at Meronitz (Bohemia), the iron pyrites con- _ tains nuclei of pyrope, and in perfectly developed dodecahe- rons of pyrites, nuclei of transparent quartz have been found. . _ This porphyritic formation of iron pyrites sufficiently proves _ the segregation of particular substances in rocks. It is not confined merely to deposits of clay, but may be observed even in the oldest schistose rocks. In some varieties of clay slate, _ the imbedded crystals of iron pyrites are covered, especially % on one side, by a layer of fibrous quartz, which must have been deposited after the formation of the pyrites; and this fact furnishes additional evidence that these two minerals ai have an attraction for each other. The Devonian slates of 332 The Paragenetic Relations of Minerals. the Eifel present abundant examples of this mode of occur- rence, and the curvature in the surrounding layers of rock may be easily recognised. Sometimes the pyrites has been completely removed, its former existence being indicated only by hexahedral cavities, and then the fibrous character of the quartz is more prominent. It is probable that iron pyrites is very extensively disseminated throughout some schistose rocks, for the stagnant water in slate quarries ne contains sulphate of iron. If, then, it is satisfactorily proved that the porphyritic formation of iron pyrites has taken place subsequently to the formation of the strata in which it occurs, there appears to be no reason why we should not consider other crystalline minerals present in the same rocks, and sometimes in imme- diate proximity to the pyrites, to have been formed in a simi- lar manner. In-some of the most ancient slates octohedrons of magnetic iron occur together with the pyrites, and even the granular rocks of eruptive and plutonic origin present analogous facts. In the granite of Saubersdorf (Voigtland) the iron pyrites is partially decomposed, and converted into crystallised specular iron, the granite itself being somewhat disintegrated. In the syenite of Zschitschewig, titanite is imbedded together with pyrites. It is, however, inconsistent with chemical principles to suppose that bisulphuret of iron existed in a melted eruptive mass;. in melting processes only mono- and sub-sulphurets are formed, and this renders it still more probable that the pyrites is of more recent formation than its matrix, likewise proving either that these rocks were not formed at any very high temperature, or had cooled considerably when the formation of pyrites took place. . Bunsen’s obsvrvations in Iceland would appear to prove — that the formation of iron pyrites in clay may sometimes be owing to other causes than those above mentioned. The prin- cipal gases associated with the exhalations of vapour in that island, are sulphuretted hydrogen and sulphurous acid, their mutual decomposition giving rise to the sublimation of im- mense masses of sulphur. When the sulphuretted hydrogen is in excess, the oxide of iron is converted, under the in- — The Paragenetic Relations of Minerals. 333 fluence of alkaline’ sulphurets, into pyrites which remains imbedded in the clay. . As the principal object in the present instance is to prove that the formation of imbedded minerals is subsequent to that of their matrices, attention has been especially directed to one mineral alone. There are, however, two others of especial importance which occur in the same manner— gypsum and quartz—the former occurs in sharply-defined crystals in alluvial clays, shale, and even in the schistose and stratified clay iron ore of Yorkshire, &c. The absence of all traces of friction upon these very soft crystals does not, for a moment, admit of the supposition that they were deposited in a detrital manner, or with the matter of the sedimentary strata. It is indeed probable that, in some cases, their formation may have been owing to the presence of iron pyrites, and have taken place in the manner pointed out by Hausmann.” - Quartz being the mineral which principally gives the pecu- liarity of structure to the oldest and most frequent porphy- ritie rock, some mention of its mode of occurrence in more _. recent rocks may not be without interest. At Pdsneck (Thuringia), millions of very small and extremely sharp- edged diploheders of quartz occur in a marl belonging to a more recent period than the zechstein group. In a marly and compact limestone at Pforzheim, in Baden, larger crystals are found, which singularly enough contain some sulphur. Quartz crystals likewise occur in the gypsum of Grafintonna (Thuringia), and of St Jago di Compostella (Spain). Even some of the particles of sandstones are not invariably water- worn fragments, but sometimes actual crystals, as in the quader-sandstone of the Tharander Wald (Saxony). _ Another singular fact is the occurrence of small druses of felsite in the clay-stone of Floha (Saxony), together with the same mineral imbedded in a porphyritic manner. This would appear to admit of the inference, that imbedded felsite is, at least in some instances, more recent than its matrix. _ 3. It often happens that one mineral imbedded in another, * Bemerkungen iiber anhydrite und Karstenit, 1847, p. 25. VOL. LIV. NO. CVIII.—APRIL 1853, Z 334 The Paragenetic Relations of Minerals. which serves as a matrix, occurs implanted upon it in druses. In the Zillerthal (Tyrol), pistacite occurs imbedded in mica (astrite) slate, and in the same locality fine specimens of green epidote are found upon ripidolite. Chondrodite oc- curs in many places in saccharoid limestone and calcite ; but in the druses in the masses ejected from Vesuvius, it is im- planted upon calcite. Zeilanite likewise occurs imbedded in calcite, and in the above druses upon it. Yellow titanite oc- curs imbedded in chlorite at the Zillerthal (Tyrol), and at St Gothard, implanted upon it. Brown titanite occurs im- bedded in hornblende slate at the Stubeithal (Tyrol), and in the well-known druses of common hornblende from Arendal (Norway), it is implanted upon this mineral. The porphyritic occurrence of iron pyrites in copper pyrites is remarkably frequent, especially when the latter is in large masses. Sometimes the iron pyrites is quite porous, and only partially occupies the cavity in the copper pyrites. When these minerals are associated in druses, the copper pyrites always appears as the oldest of the two, Pseudomorphous iron pyrites, after copper pyrites, presents an apparent ex- ception to this rule, but it must be remembered that pseudo- morphs are in some sort abnormal products. There are, however, some real exceptions, though few in number. Copper glance is in many instances followed by erubescite and iron pyrites, a fact which perhaps admits of explanation upon chemical’ principles. If, for example, a solution con- aining oxide of copper and peroxide of iron, is acted upon by sulphuretted hydrogen, sulphuret of copper is first formed, while the peroxide of iron must be reduced to protoxide be- fore a bisulphuret can be formed ; and during this time it is readily conceivable that compounds of the sulphurets of iron and copper may be formed. The most direct illustrations of this third proposition are furnished by those instances in which minerals occur im- bedded in a rock, and at the same time implanted upon it in veins, sometimes even filling the fissures. Thin plates and lamine of tale occur imbedded separately in the chlorite slate of the Zillerthal (Tyrol); and this tale The Paragenetic Relations of Minerals. 335 is found filling veins in the same rock. Astrite occurs both: in and upon the finely granular calcite of the masses ejected from Vesuvius. The porphyry of Scharfefstein (Saxony) contains imbedded pistacite, and is likewise traversed by’ veins of the same mineral. It is also remarkable that the imbedded crystals are deposited around small nuclei of iron pyrites, and where epidote and iron pyrites are associated in druses, as at Arendal, the latter is always underneath. According to Haidinger, epidotes occurs in other places, as relatively very recent products. G. Rose states that the chlorospinel of Slatoust is both imbedded and in veins in the talcose slate. At Achmatowsk (Siberia), crystals of the same red garnet are imbedded in and implanted upon ripidolite. In-the serpentine of Dobschau (Hungary), a garnet of bright green colour is both imbedded and implanted upon the walls of the fissures. Tourmaline crystals occur imbedded in tal- cose and mica slate; and where there are veins in these’ rocks, the tourmaline forms druses upon them. Crystals of» cassiterite are imbedded in the felsite of the tin lodes at Marienberg (Saxony), and occur upon crystals of the same felsite. An arsenical pyrites, containing 0:8 to 0-9 per cent. of nickel,* occurs in chlorite slate near Sparnberg, in the same manner as the above-mentioned tale. Imbedded crystals of metallic copper occur in compact brown iron ore (Siberia) © and plates of copper in the fissures. Similar phenomena present themselves in essentially mixed rocks,—thus nepheline and apatite occur together imbedded in the granite of Miask (Siberia), in the syenite of Fredrik- _ swirn (Norway), and in the veins of graystone at Capo di _ Bovo, likewise in the small druses of the nepheline rock at _ Meigen (Darmstadt), in Saxony, and in the volcanic felsite rock of the lake of Laach. Cassiterite, beryl, columbite, and the several species of tantalites occur imbedded in granite, while in the druses and veins they are implanted upon the constituents of this rock. | 4 Beryl is found without columbite and tantalite, and these are * Breithaupt has found nickel in most arsenical pyrites, which are associated _ with chlorite minerals, Z 2 336 The Paragenetic Relations of Minerals. more recent than it; but, as Nordenskjold first pointed out, they never occur without beryl. It cannot therefore be doubted that their presence depends upon the pre- “existence of beryl. Tron pyrites, arsenical pyrites, galena, and zinc blende— the most frequent minerals in the Freiberg lodes, impregnate the adjoining gneiss to a distance of several fathoms. Al- though the walls of the lode fissures presented an abundant surface for their deposition, a considerable transfer of these substances from the lodes into the adjoining rock is some- times unquestionable, and in this case the rock is generally disintegrated. Frequently the mispikel occurs imbedded in the gneiss, at a distance of 15 to 20 feet from the lode, in such quantity as to be advantageously worked. The gneiss is then converted into tale, or a very analogous substance. The occurrence of calcite, both imbedded and in small veins, in the zechstein of Saalfeld, is a phenomenon vii should probably be included among the above. It may not be inappropriate here to make some mention of the artificial crystals obtained in smelting processes. The beautiful homogeneous and vitreous slags, from Hockeroda and Luisenthal, contain tabular, tetragonal-prismatic crys- tals, of a substance closely resembling idocrase, both imbed- ded and forming druses, in the larger vesicular cavities. Hexagonal-prismatic crystals, resembling nepheline, occur in the same manner in the slag from the Rothenthal at Osterode (Harz). 4. Some imbedded minerals are undoubtedly products of the decomposition of the mass in which they are inclosed, and are therefore more recent than it. In the brown coal of Artern (Thuringia), mellite and sul- phur occur in separate crystals and groups. At Luschetz (Bohemia), mellite and oxalite occur in a similar manner. Bischof considers that the carbonaceous matter of the coal has reduced sulphate of lime, and that subsequent contact of the sulphuret with sulphuric acid, resulting from the oxi- dation of pyrites has reproduced gypsum, with evolution of sulphuretted hydrogen, which, with oxygen, yielded water and sulphur. However, the sulphur in the brown coal of The Paragenette Relations of Minerals. 337 Langenbogen (Prussia) is very probably a product of sublima- tion. The spherical masses of hydrated pyrites, covered with an envelope of gypsum, the crystal points of which are turned inwards, have decomposed with considerable evolution of heat. The sulphate of iron has been washed away, and the masses are now hollow, with the surplus sulphur, result- ing from the decomposition, upon the points of the gypsum crystals. The heating of the pyrites has in this case been so great, that the coalimmediately surrounding the gypsum has been converted into a species of anthracite. It is not improbable that analogous changes may have taken place in other rocks possessing a porphyritic structure, but the difficulty here is, that we do not know what was the condition of the matrix previous to the formation of the im- bedded crystals. Graphite occurs imbedded in the sandstone of Charlottenbrunn (Siberia), and it is very probably a product of the alteration of organic remains at some period after the formation of the rock. When it is remembered that some of the mixed rocks must be regarded as really metamorphic, the fourth proposition will appear applicable to a much greater number of facts, although it may not always be possible to furnish positive explanations of them. 5. Certain minerals occur imbedded in the older rocks, only where they are in contact with more recent eruptive rocks. 3 | Several geologists state that the occurrence of the very frequently associated minerals, kyanite and staurolite, is limited, in the older schistose rocks, to those spots where they are in contact with granite, or some analogous rock. Here, then, the porphyritic separation of crystals is obviously owing to the influence of the more recent upon the older rock. It canhot be doubted that an essential part of the change consisted in a chemical readjustment of the atoms. Anda- lusite, which, according to Bunsen, is specifically identical with chiastolite, likewise occurs in mica and clay slates, under precisely similar circumstances. It has been found very fine in the clay slate of the Whealkind mine, at the surface of contact with granite, the clay slate at the same time being remarkably hard. The same phenomenon presents itself "338 The Paragenetic Relations of Minerals. near the mica slate and gneiss at Munzig (Saxony), and chias- tolite occurs in the clay-slate at Gefrees (Bavaria), close to granite. At Treuen (Saxony), the so-called “ Frachtochisier?4 occurs, surrounding a spheroidal mass of granite, and a perfectly similar-shaped black amphibole, with garnets, occurs. at Airolo (Switzerland), so that it may be inferred that the in- distinct and decomposed erystals in the “ Fruchtschiefer” were formerly amphibole. .The same kind of slate occurs at Schneeberg, near the granite ; and in the mines at that place it has been found that the clay-slate is harder and more sili- ceous near the granite, this contact phenomenon even extend- ing into the slate to a distance of 800 feet from the granite. ‘This fact is alone sufficient to shew to what a distance the atoms of relatively recent rock may be transferred. into an older one with which it comes in contact. The horn-slate, which forms a kind of mantle round the granite of the Brocken, affords almost precisely the same evidence. These altered, and in part essentially hardened slates, do not always ‘present evident porphyritic inclosures, but they probably exist as microscopic particles, or the slate has been otherwise che- mically altered. It is probable that the alterations which rocks have suf- fered under the influence of more recently-formed rocks rarely consisted in merely mechanical modifications of the molecu- lar aggregation ; they appear rather to have been far more deeply seated, to have been more or less chemical. In this point of view, the theory put forward by Von Buch, that, under certain circumstances, dolomite may have originated from limestone by the action of melaphyr, comes within the bounds of possibility, and, under one condition, perp much probability. | The mica-slate of Scharfenstein (Erzgebirge) is remark- ably altered in contact with the porphyry which traverses it, being converted into gneiss for short distances. In this in- stance felsite has been transferred from the porphyry into the mica-slate, which might, indeed, be termed porphyritic, were it not customary to call a schistose mixture of felsite, quartz, and mica, gneiss. se Th LS The Paragenetic Relations of Minerals. 339 The above mentioned transfer of mispikel, from a lode into gneiss, is an analogous fact, the more recent lode mass having acted upon a pre-existing rock, in the same way as a more recent rock mass. A. number of other instances might be brought forward, but as there are no facts at variance with this proposition, it is unnecessary. | 6. When the crystalline variety of a mineral is associated with the compact variety, the former is always the most re- cent. x Many porphyries consist of a mixture of compact felsite, with imbedded crystals of cleavable felsite. There is, there- fore, no reason to deny that the latter are of more recent formation than their matrix. In granular or slaty mixed rocks large crystals, of some one or more constituents, are sometimes imbedded, communicating to the rock a porphy- ritic character; and there can be little doubt that such -erystals are of more recent date, for not only do they contain nuclei of the rock in which they lie, but in the slaty rocks, the curvature of the layers surrounding the crystalsis likewise to be observed, as in the gneiss of Schwartzenberg (Saxony). Many minerals occur imbedded in the form, not of crystals but of nodules. In other respects they correspond precisely with the inclosures in porphyritic rocks, and there is no doubt that they have often originated in a similar manner. This is very evident in the case of iron pyrites, which frequently occurs, both in nodules and crystals, in the same bed of clay. Nodular iron pyrites occurs in all rocks up to the clay-slate. It is probable that many other nodular minerals must be re- garded as of later formation than the masses in which they lie, although water-worn fragments are also imbedded in this Shape. Again, agate occurs in the form of nodules, although it has been formed ina very different manner. Consequently very great caution must be exercised in forming any inferences with regard to the origin of imbedded nodules. Nodular mi- nerals are sometimes associated with imbedded crystals, and this is then additional evidence in favour of their analogous origin, thus spherulite occurs in pitchstone, pearlstone, and obsidian, together with crystals of astrite and felsite. The nodules of azurite, in the marl and sandstone of Miedezana 340 The Paragenetic Relations of Minerals. Gora (Poland), are remarkable, inasmuch as they are hollow, and lined with crystals, like amethyst balls. There can be no doubt that the formation of these. crystals was attended by a contraction of volume, and commenced from the periphery of the nodules. Nodular masses of.limestone are very common in transition rocks, especially slate ; at Obernitz (Thuringia), they are so numerous as apparently to form beds. Marl strata some- times contain nodules of very hard limestone or dolomite, traversed by veins of calcite, perhaps accompanied by celes- tine. Argillaceous spharosiderite would appear to have been formed by a segregation of carbonate of iron, after the for- mation of sedimentary rocks. Freiesleben states likewise, that the crystalline spathic iron of the Mansfeld district has in some places an oolitic structure. It must, however, be ex- pressly stated, that both limestone and spharosiderite, when exposed to the atmospheric influence, assume a nodular struc- ture, and this remark applies also to some sandstones, grau- wackes, &e, Heavy spar occurs in nodules in clay; yellow iron ore in the brown coal formation of Bohemia. At Miask (Siberia), the variety of chrysophan, called xanthophillite, occurs in nodules, generally surrounded by magnetic iron; the crystals point towards the interior, which is either hollow, or filled with a light green mineral resembling serpentine. Nodules of green epidote occur in a gray compact limestone, in the Banat. Quartz occurs in nodular masses, more rarely crystalline than uncrystalline. Crystalline nodules of quartz, which cannot be regarded as detrital, occur in the mica-slate of the Erzge- birge. The Jura limestone at Hichstadt (Bavaria) contains balls of hornstone, sometimes of considerable size, presenting in their interior concentric-coloured streaks, and even con- centric layers and fissures, the latter containing crystallised quartz. It is further interesting to observe, that the greater number of fossils in the chalk consist of flint, and that the larger nodules of this substance are particularly rich in ani- mal remains. It is probable that the formerly existing organic matter had some share in determining the segrega- tion of the silica, as it appears collected round the fossils. . Ua ; ; | Remarks on the Planets Jupiter and Saturn. 341 Olivine is much more frequently imbedded in basalt in nodules than in separate crystals. These masses consist of erystalline granular fragments, sometimes mixed with augite and bronzite. As in basaltic tuffs; similar nodules of olivine are found, which, on account of their less coherent granular structure, may be easily broken down, there is the greater reason to regard them as subsequent productions, because no small particles or angular fragments are found near the | large nodules. At Charkow, Swoszowice, and other parts of Poland, amor- phous sulphur occurs in nodules in marl; and where the marl has been converted into compact limestone, it presents vesi- cular cavities, containing crystallised sulphur and calcite. In the case of all these nodular formations, it may be assumed that there has been a segregation of the particles of the minerals, for it would be difficult to suppose that they were accidentally deposited in the manner they now occur ; and moreover, many such nodules contain small nuclei _ the substance in which they are imbedded. (To be continued.) Some remarks on the probable present condition of the Pla- nets Jupiter and Saturn; nm reference to Temperature, &e. By JAMES NAsmytH, Esq.* The remarkable appearances which characterise the aspect of the planets Jupiter and Saturn, as revealed by the aid of very powerful and excellent telescopes, have induced some reflections on the subject of their probable present condition _ astotemperature. With a view to excite more special and _ careful observation of the phenomenon in question, and pro- mote discussion on this interesting subject, I have been tempted to hazard the following remarks, which may per- haps prove acceptable to some of the members of the Royal Astronomical Society. In a former communication, in reference to the structure * Read at the Meeting of the Royal Astronomical Society. 342 Remarks on the Planets Jupiter and Saturn, and condition of the lunar surface, I made some remarks on the principle, which, as it appears to me, gives the law to the comparative rate of cooling of the planets, namely, that while the heat-retaining quality was due to the mass of the planet, the heat-dispensing property was governed by its surface ; and as the former increases as the cube of the dia- meter of the planet, while the latter increases only as the square of its diameter, we thus find that the length of time which would be required by such enormous planets as Jupiter and Saturn to cool down from the original molten and in- -eandescent condition to such a temperature as would be fitted to permit their oceanic matter to permanently descend and rest upon their surface, would be vastly longer than in the ease of such a comparatively small planet as the earth. Adopting the results which geological research has so clearly established as respects the original molten condition of the earth, as our guide to a knowledge of the condition of all the other planets, it appears to me that we may in this way be led to some very remarkable and interesting conclu- sions in reference to the probable present condition of such enormous planets as Jupiter and Saturn, tending to explain certain phenomena in respect to their aspect. Assuming as established the original molten condition of the earth, and going very far back into the remote and pri- mitive periods of the earth’s geological history, we may find glimpses of the cause of those tremendous deluges, of which geological phenomena afford such striking evidence,* and by — * The deluges here alluded to are quite distinct from those which have so fre- quently, during various periods of the earth’s geological history, swept over vast portions of its surface, and of whose tremendous violence we have such clear evidence, in the denudation of the hardest rocks, the debris of which has yielded the material of nearly every sedimentary formation, from the period of the old red sandstone formation upwards, : These vast and often repeated deluges I consider to have resulted from mighty incursions of the ocean, over vast continents, till then forming the dry portion of the earth’s surface, but which (by the retreat of the earth’s substance from be- | low, resulting from the progressive contraction, consequent on the gradual | cooling of the sub-surface matter) must have again and again permitted ex- tensive portions of the solid crust of the earth to suddenly crush down, like an r | “ae Remarks on the Planets. Jupiter and Saturn. 343 _ whose peculiar dissolving and disintegrating action on the _ igneous formations which at that early period of the earth’s history must have formed the only material of its crust, and ‘may in that respect obtain some insight into the source whence the material which formed the first sedimentary strata was derived. If we only carry our minds back to that early -period of the earth’s geological history, where the tempera- ture of its surface was so high as that no water in its fluid form could rest upon it, and follow its condition from such non-oceanic state to that period at which, by reason of the comparatively cooled-down condition of its surface, it began to be visited by partial and transient descents of the ocean, which had till then existed only in the form of a vast vapour envelope to the earth, we shall find in such considerations, not only the most sublime subject of reflection, in reference to the primitive condition of our globe, but also, as it ap- pears to me, a very legitimate basis on which to rest our speculations in regard to the probable present condition of Jupiter and Saturn,—both of which great planets, I strongly incline 40 consider for the reasons before stated, are yet in _ over-loaded ill-supported floor, and so permit the ocean to rush in with fearful F- violence, and occupy the place of the so submerged continent. Bid udging from the facts which geological phenomena yield us in abundance, _ these incursions of the ocean must have been sudden, violent, and of frequent -“oecurrence. | . The sudden sinking down of a continent to the extent of 1000 feet in depth, would be but an insignificant adjustment of the crust of the earth, to the re- _ treating or contracting interior, as compared to the actual diameter of the ' earth (being only about one four-thousandth part of its diameter), but yet such a subsidence occurring to any portion of a continent near the sea, would occa- sion a rush of waters over its surface, amply sufficient to perform all the feats 4 ‘of violence and denudation (of the occurrence and action of which we have : “most palpable evidence), which have taken place during many successive pe- _ riods of the earth’s geological history, not only in the vast accumulations of debris, caused by these violent incursions of the ocean, but also in the prodi- gious dislocations of strata, which have resulted from the crushing down of the crust of the earth, in its attempts to follow down and fill up the void or hollow ; spaces eaused by the contracting and retreating nucleus, which as before said, I consider to be the true cause of this class of deluges, the tremendous violence of which has yielded the old red sandstone, and all other sandstones, conglo- _ merates, boulders, gravel, sand, and clay. 344 Remarks on the Planets Jupiter and Saturn. so hot a condition, as not only not to permit of the permanent descent of their oceanic matter, but to cause such to exist suspended as a vast vapour envelope, subject to incessant disturbances by reason of the abortive attempts which such vapour envelope may make in temporary and partial descents upon the hissing-hot surface of the planet. Recurring again to this early period of the earth’s geolo- gical history, when it was surrounded with a vast envelope of vapour, consisting of all the water which now forms the ocean. The exterior portion of this vapour envelope must, by reason of the radiation of its heat into space, have been continually descending in the form of deluges of hot water upon the red-hot surface of the earth. Such an action as this must have produced atmospheric commotions of the most fearful character: and towards the latter days of this state of things, when considerable portions of what was after- wards to form our ocean came down in torrents of water upon the then thin solid crust of the earth, the sudden con- traction which such transient visits of the ocean must have produced on the crust of the earth would be followed by tre- mendous contortions of its surface, and belchings forth of the yet molten matter from beneath, such as yield legitimate material for the imagination, and the most sublime subject — for reflection. The extraordinary contortions and confusion which characterise the more primitive sedimentary strata, — such as the gneiss, schist, and mica slate, in so very remark- able a degree, shadow forth the state of things which must have existed during that period, when the ocean held a very disputed residence on the surface of the earth. Could the earth have been viewed at this era of its geolo- gical history from such a distance as the planet Mars, I doubt not it would have yielded an aspect in no respect very dissi- — milar to that which we now observe in the case of Jupiter: — namely, that while the actual body of the earth would have been hid by the vast vapour envelope then surrounding it, ie <> i oe >. the tremendous convulsions going on within this veil would — have been indicated by streaks and disruptions on the sur- face, which would be mottled over with markings such as we — observe in the case of the entire surface of Jupiter: and by Sa by i Remarks on the Planets Jupiter and Saturn. 345 © _ reason..of the belchings forth of the monstrous volcanoes which at that period must have been so tremendously active on the earth, the vapour envelope would be most probably _ marked here and there with just such dingy and black-and- _ white patches, as form such remarkable features about the equatorial region of Jupiter—probably the result of volcanic matter, such as ashes, &c.—which the volcanoes about his equator may from time to time vomit forth, and send so far up into the cloudy atmosphere as to appear on the exterior, and so cause those remarkable features which so often mani- fest themselves on the outward surface of his vapour enve- _ lope; for I doubt if we have ever yet seen the body of Jupi- _ ter, which will probably remain veiled from mortal eyes for countless ages to come, or until he be so cooled down as to ‘permit of a permanent residence on his surface, of his ocean, that is to be. 3 __ In applying these views to Saturn, it occurs to me that we _ may obtain some glimpses into the nature of those causes which have induced, and are now apparently inducing, those changes in respect to the aspect of his rings, which have, more especially of late, attracted so ok attention. If _ Saturn also be so hot, that his future ocean is suspended as a vast vapour envelope around him, it is possible, I conceive, that some portion of this vapour may migrate, by reason of _ the peculiar electrical conditions which it is probable his rings may be in, in respect to the body of the planet; and that such migration of vapour in an intensely frozen state, as it must be in such situation, may not only appear from time to time, as the present phantom ring does, but also encrust the inner portion of the interior old ring with such vast coatings _of hoar-frost as to cause the remarkable whiteness which so peculiarly distinguishes that portion of his rings. In fact, such are the extraordinary phenomena presented by this q o _ one is led to hazard a conjecture or two on the 346 lk Deep Sea Soundings. _ Captain H. Denna, F.R.S., on Deep Sea Soundings obtained in lat. 36° 49’ S., long. 37.°6 W. The following extracts from a letter received from Captain H. M. Denham, dated H.M.S. Herald, 29th of November 1852, Table Bay, Cape of Good Hope, give the results of some interesting experiments on the depth and temperature of the sea in the South Atlantic Ocean. The position, it will, be seen, is in about the parallel of the mouth of the river, Plata, and about half way between the American continent and Tristan d’Acunha. We have recorded similar experi- ments of Captain Sir James Ross, Sir Edward Belcher, and Captain E. Barnett. This, however, is far beyond any of theirs. The following are references to our volumes for accounts of deep soundings : 1840—pp. 347, 507, Sir James Ross, 2426, 27° 4’ S., 17° 5’ W.; 2677, 33° 3'S., 9° 1’ EB. 1848—>p. 796, Sir E. Belcher, 3065, 0° 4’ N., 10° 6° W.; 1620, 4° 2’ S., 9° 6’ W. 1849—p. 121, Captain Barnett, 41° 2’ N., 44° 3’ W. ; 3700 attempted, broke for want of more by effects of current. 1850—p. 699, American soundings, East of Bermuda. 1851—p. 275, Lieut. Gouldsborough, U.S.N., 3100, 28° 3’ S., 29° 3’ W.; p. 433, Commander J. Adams, from a New York paper, but unauthenticated by any other document we have seen, deepest being 5500 fathoms, in 32° I’ N., 44° 8 W. H.M.S. Herald, as follows (7706 fathoms), obtained in lat. 36° 49’ S., long. 37° 6’ W., on her exploring voyage to the South Seas, under the command of Captain H. M. Denham, ~ F.R.S. 30th October 1852. The following is the extract of the letter referred to :— ** We reached the lat. of 36° 49’ S,, and long. 37° 6’ W., on the 30th of October, when the fineness of the weather per- mitted me to employ the 15,000 fathoms of sounding line — which Commodore M‘Keever, of the United States Navy, had _ very generously presented to me, and we had the gratification _ of obtaining the (I believe) unprecedented sounding of 7706 fathoms, equal to 83 English miles, the particulars of which _ I have tabulated as enclosed. a ee a ee Deep Sea Soundings. 347 ** Such was the apparent increase of the magnetic variation as we proceeded eastward, on the parallel of 37° 8., that the effecting a landing on Tristan d’Acunha to test the actual amount, free from any local disturbances of the ship, appeared _ tome an essential step. Availing myself, therefore, of the tranquil state of the weather, on the day of sighting it (12th _ November), I effected a landing on the island, with the ne- _ cessary instruments for settling the longitude, as well as the variation of the compass, and the shore data at once confirmed what had been indicated afloat, viz., that the variation has doubled in amount since 1813, being now in that vicinity 20" 4’ W., instead of 9° 51’ W. “I took the opportunity of another calm day to ascertain the temperature of the sea at 900 and at 1000 fathoms. At both depths it proved the same, viz., 40° of Fahrenheit, whilst near the surface it was 58°. At the same time I employed means for tracing the depth to which the sun’s rays pene- trated, and found it to be 66 feet.” As we considered the foregoing statement would have been imperfect unless accompanied by particulars of this interest- ing proceeding, contained in Captain Denham’s letter to the _ Hydrographer, Sir Francis Beaufort, it is with much satis- faction that with his permission we are enabled to add to it the following extract :— _ «TJ must not omit, even in this, to allude to the generous offering to our expedition of 15,000 fathoms of sounding line _ by Commodore M‘Keever, of the United States Navy, whose broad pendant was flying on board the Oongress frigate at Rio. He was not content with presenting me with books, 7 &e., but having observed that he had something in our way, sent me, the day before he sailed, 10,000 fathoms on one reel, and 5000 on another, of most admirably adapted line for ex- _ perimenting in deep deep-sea casts. Without compunction as to ships’ stores, I determined to hazard the 10,000 fathoms (beautifully laid up, or grafted into one length) the very first opportunity ; and we as assuredly did get to the bottom at _ 7706 fathoms, as not actually bringing up a sample can per- _ mit me to say, for I and Lieut. Hutchison, in separate boats, with our own hands, drew the plummet up 50 fathoms several 348 Deep Sea Soundings. times, and after it had renewed its descent with the same velocity it had,done during the last hundred fathoms, it landed on each occasion abruptly to the original mark to a fathom, and would not take a turn more off the reel. By its parting at 140 fathoms from the surface, we lost a Six’s thermometer, which I had bent on at 3000 fathoms. With the remainder of the line I have obtained some 500’s, when our own lines could not have been employed to that extent; and on two occasions between Tristan d’Acunha and this (Cape of Good Hope), I obtained 900 and 1500 fathoms with thermometers attached, saving them each time, and shewing that 40° is the minimum temperature after 200, where it averages 50 and 52, no matter what the surface temperature may be. 1 have still 5000 fathoms to play upon, before reeling up spunyarn again, which from our junk I had done to the length of 8 miles before I had the present.” _ We have no doubt the worthy Commodore will be much gratified with this disposal of his line. We need scarcely. assure him that such generous marks of friendly feeling can- not fail to be appreciated, and particularly so when it is con-- sidered that he was giving away the means by which he him-. self might have gained the credit of finding the greatest depth of the ocean yet attained. But noble minds are above such personalities. The bottom was reached, and that was sufhi- cient. _ We shall leave our readers to form their own conclusions’ on the experiment, as to the up and down depth, as a seaman. would say. But we may add, that although the experiment. was made in a favourable part of the South Atlantic Ocean, we cannot suppose it possible that the ship would remain for - the nine hours during which it lasted in a vertical position — immediately over the lead, although nothing is said by Cap-. _ tain Denham as to the direction in which the line grows as- the ship drifts while the operation is going forward, nor whether the boats and the ship were separated by the effect — of any current. We by no means impugn the statement that — bottom was reached when 83 statute miles were out, but — should like to know whether or not some deduction should be made for drift, and what that should be, before an up and ~ down depth can be asserted.—Ep. VV. 1. ee et ee A Table shewing the Rate at which the 9 lb. Plummet (11:5 by 17 inches) descended witha Line of 1-10th of an inch dia- meter (and weighing, when dry, 1 1b. per, 100 fathoms), _through a depth of nearly 9 English miles of Ocean Water: at which depth it eenrrentis reached the bottom. a ps BAD ed. \. 3 | | ) i . i i ; nterval | Interval || i a ee re Successive Notation. api cael Succeésive Notation. =, ee Pothoms. h. |m.|s.|h.{m.}s.|b. mes. h. Immersion 8130/45 4000 Fms, 113s 100 I'ms. 32\15 1/30 4100 200 34/20) | 2] 5 4200 ... ce... 36/45} | 2195 ZaUuy ..,. LZ 400 ... 39/15 2|30 || 4400 500. <.. 42} 4) | 2/49 | 4500 COW. 45] 0 2'56 4600 760 ......| 48] 0], | ah 0 4700... 800 |. 61).5| | 3] 5 zt ea mm 900%...> *) * 154/20 3/15} * mC lala a BOO0",.:.../. 58| 0 3/40) 0.27/15} 5000... 1 moo ,.. 9| 1150 3/50 5100 7 1200.2. 5/45] | 3/55 5200 mroOO:. 2. 9/30 3/45 5300 12007 °..5° 12/45 3)15 5400 f 1500»... . 116/40 3/55 5500... {1600 ... 20/40} | 4! 0 5600. ... 2 a OU? * >; 24/50} | 4/10 WET es f 1800.°..., 29} 0| | 4\10 5600 #1900 ... 33/15} | 4/15 5900 =2000. .:. 37|40 4/25; 0/39/40)| 6000... 2100 - ...° 42} 0} | 4/20 Win eee a macov ... |. |46/30 4130 6200... 23005... | 51| 0 4/30) 6300 .:./ 25 {| 2400 .,,, 55/30 4/30 6400 ... 37/58 £2500 ... |10| 0] 5| | 4/35 a500 '.:, 48] 0 A 2600... 4|45 4'40 6600. ... 57/50}. } 2700 ... 9145| | 5] 0 6700... 4 2800 ...- 14/50} | 5}. 5] ° 6800 ... 19 20:19 5|20 6900... 30!: 25/50 5/40} 0/48/10)} 7000... 41 30}15) | 4/25 ROG oe J52|1 36/15) | 6).0 (eC eee 5 | {43/10; | 6/55 7300, ons 11)40 | -|50/40) | 7/30 San eas 2, 124/10 | 58/45 | 8) 5 7500 34 20) 11} 6/50) | 8/"5| | - 7600 44/22 14/45, | 7/45} | 7700 55/30! 22/30 7/45 ; 31/10; | 8/40 | : Total Interval, ; 9/24'45) ” - Total fathoms, 7706 = 15,412 yards = 8? English miles. TE. —This line could sustain 72 1b. in air, at a suspension of one fathom ; as the 7706 fathoms weighed 77 Ib. (in addition to the plummet) became hted one-half more by saturation (equal to 115 lb.), it could not bring up the met again to exhibit to us the nature of the bottom; it broke, whilst carefully eling it i aR at 140 fathoms below the water line. H. M, DENHAM, Captain, R.N. | 2 | VOL. LIy. NO, OVILI.—APRIL 1853. A 350 Ordnance Survey Astronomical Observations. Astronomical Observations made with Airy’s Zenith Sector, from 1842 to 1850, in the determination of the Latitudes of various Trigonometrical Stations used in the Ordnance Survey of the British Isles. Edited by Captain Y olland, R.E., under the direction of Lieutenant-Colonel Lewis A. Hall, Royal Engineers, Superintendent of the Ordnance Survey, and published by order of the Master-General and Board of Ordnance. This is a ponderous quarto volume containing 52 pages of letterpress, and 1009 pages of figures and numerical results, as a contribution towards an exact knowledge of the latitudes of twenty-six stationson the Ordnance Survey of Great Britain. It will doubtless be very favourably received by the scien- tific public, and is an excellent specimen of the searching manner in, and practical skill with, which this great opera- tion is now being carried on ; while persons in general will see, from the voluminous extent to which the observations ahd calculations in this one department have necessarily expanded,—how essential it is that the whole should be conducted by the Imperial Government. ; As the attention of persons in our neighbourhood has lately been attracted almost wholly to questions of the best scale for the maps of the survey, we may as well remind them, that to make a sensibly perfect map of the whole country on any of the scales proposed, two descriptions of operations are neces- sary; one consisting of terrestrial determinations of distances in feet and inches by means of measured base lines and trian- gles; the other, of astronomical observations, in terms of lati- tude and longitude, to fix the part of the globe wherein the en may be situated ;* and to furnish, by being compared SS EE ee ee ee eee See ee SE eee * Tt used to be objected against the old one-inch maps of the Ordnance Sur- vey, that however accurately the fields and villages might be laid down there- on, there was nothing to shew in what part of the world the places might be situated ; i. ¢., there were no markings of latitude and longitude on the sides of the sheet, as had from the first been introduced in the government maps of France. With their usual readiness to meet all the rational requirements of — Ordndiicé Survey Astroiomiedl Observations. 351 with the linear result, and with similar operations in other parts of the world, certain coefficients, relativeto the size and shape of the earth, and necessary to be employed in all the calculations of the base lines and triangles of the terres- trial measure. Of these coefficients, the most important is the quantity ue compression of the earth, which is derived with the greatest accuracy by comparing together measured lengths of the meri- dian indifferent latitudes; and the practical operation consists in éach country in determining astronomically the differences of latitude of two stations, and then from their measured distance astinder in feet, and their bearing the one from the other, ascertaining the angular space between them on the meridian, as viewed from near* the centre of the earth, and so deducing as it is popularly termed, the length of a degree of the meridian. Of the two proceedings, the terrestrial admits of being perfornied with far greater accuracy than the astronomical. ‘Thus the length of 60 miles, for example, a8 calculated from the carefully measured base lines and angles of the Ord- nance Survey, may be determined with certainty to consider- ably under one foot; and this will be equivalent to one-hun- the public, the omission has been supplied by the English officers in the recent maps on the six-inch scale; though to insert the points to such exactness that they may be depended on to the full extent of the terrestrial accuracy of the paper will be shewn presently to be a far more difficult matter than the ob- jectors were probably aware of. * From near to, not at, the centre of the earth, by reason of the spheroidal character of its figure ; which causes the direction of gravity in various parts of the surface to point, not to one and the same internal spot, but to the locus of a curve depending on the amount of compression; and thus it is that as we _ travel from the equator toward the Poles, the radius of curvature and the length _ of a degree on the surface increase, while the distance from the centre decreases, Hence may arise two different modes of reckoning Latitude, one by a practical astronomical operation on the surface; and the other by a theoretic reference to _ the centre of the world, and is deduced by calculation from the former, combined Mf with a ‘ktiowledge of the ellipticity. This theoretic, or as it is called Geocen- . 4 tric Latitude, is proper to be employed in certain astronomical calculations ; a but the former is that which i is more generally used, and knownas “Latitude,” and will be alone considered in the course of this notice. 352 Ordnance Survey Astronomical Observations. dredth only of a second of a degree of latitude. But the astro- nomical determination, on the other hand, even with the best existing instruments and methods yet invented by man, can hardly be brought within several tenths of a second; so great are the practical difficulties which beset the subject. All possible means and appliances should therefore be em- ployed, and even exhausted, in improving the accuracy of the astronomical determinations of the latitudes of the terminal points; and these when once well known, allow of the latitudes of any and all the other points in the country being computed from the terrestrial measurement with equal aceuracy, and of being duly inserted in the margin of the maps. Not only, therefore, our knowledge of the compression of the earth depends on these terminal points, but also the latitudes of every place in the country, and the indications of every single sheet of the thousands of which the survey consists. The lines of latitude and longitude extending over a coun- try are in fact an astronomical network, all the lines of which are obtained by computation from, and hinge on, the two or three stations, at which alone it has been possible to get the long and troublesome series of astronomical observations well performed. With any errors in the so determined posi- tions of those spots, every other in the whole length and breadth of the land are out also; and a greater uncertainty still is introduced into the results for the size and shape of the earth ; which again reacts prejudicially on the correctness of the formula employed in the calculations of all the triangles of the terrestrial portion of the survey. Hence the devotion of 1000 pages of closely-printed figures to the observations for determining the astronomical latitudes of a very limited number of places in the country. Were perfect observation possible, two stations would have been enough in Great Britian, one in the extreme south, and the other in the extreme north. But as such a comfortable state of things can exist nowhere under the sun, the whole. meridian length has been divided into several parts, and there. are meridian lengths also taken on either side of the king- dom, so as to have as many separate results as possible; _ te ee ot ee ns ee Ordnance Survey Astronomical Observations. 353 and moreover, at each intended station, observations have been made at several spots round about it, so as practically ‘to ascertain whether there be any local attraction in the neighbourhood that might prejudice the results. In this way the number of stations observed, has been increased to 26, extending from Saint Agnes in the Scilly Islands, in 49° 53’, to Saxavord in North Shetland, in 60° 49’ N. lat. The first step in this inquiry was, of course, to get a good ‘astronomical instrument, and the zenith sector made by Ramsden for the Ordnance having been destroyed in the fire at the Tower in 1840, application was made to the Astrono- mer Royal, G. B. Airy, Esq., to furnish a design for a new one, with any improvements he could suggest. The result of this was the instrument employed, wherein the following capital improvements were introduced over all other previous zenith sectors—Ist, the whole being made of metal, and in large pieces with few adjustments; 2d, A double - graduated arc, or readings, and with micrometer microscopes, ‘at either end of the telescope, which turned on an axis in the middle of its length; 8d, Levels were employed for the zero point in place of the old plumblines ; and 4th, The whole ar- rangement was such as to admit of the double observations, face E. and face W., being made at the same transit. The length ‘of the telescope was 46 inches, the diameter of the object-glass 3:75 inches ; the magnifying power usually employed 70; and the weight of the whole instrument, 10 ewt. This was screened from the weather by a portable wooden building, covered with canvass, and having an ea ving: slit in the roof, and weighing 23 cwt. From 1842 to 1844 the observations were made by com- missioned officers, Captains Hornby, and Driscoll Gosset, R.E., but subsequently, when the modus operandi was well settled, they were made and computed by non-commissioned officers, under charge of Captain Yolland, R.E. On the average, 800 observations of stars were taken at each station, and each observation is given in the body of the work, nearly as read off from the instrument itself, with all the necessary elements for its reduction, and the principal 3864 Ordnance Survey Astronomical Observations, steps of the reduction performed,-are also given, up to the complete result for latitude by each observation. In the subsequent part of the work, these quantities are collated together, and special corrections applied for certain instrumental peculiarities explained in the Introduction, and for errors of assumed declination of the stars observed, which being 491 in number, and confined between the parallels of 38° and 68° N. decl., necessarily included many small stars whose places had not previously been well fixed by any astronomer. In the concluding part of the Introduction, the final results are considered, and being compared with the geodetical caleu- lations, when the stations are but a few miles apart, some most startling conclusions are arrived at; shewing that the latitudes of places are affected by many more causes than most men’s philosophy has hitherto taken account of. For while the probable error of the astronomical determinations is hardly so much as "2, their differences from the geodeti- cal, are often ten to twenty times as great: nay, in one in- Stance, amount to the immense quantity of 9°48, The number of discordances is at the same time no less remarkable than their individual amount; and amongst the twenty-six stations observed are found all the following in- stances :— Lat. Lat. Discordance- St Agnes, . . 49 53 and be Sees Down, 50 2 —1-60 Southampton, . 50 54 Boniface Down, 50 86 41:28 Hees Sei : i ..» Week Down, . 50 86 +1:46 . Dunnose, ..-. 60. Bfx 4 8-7/1 . Port Valley, . 5089 40:42: bias ithay ths vee wee ppLaGk Down, -.... 60 40 0 1-10 Hungry Hill, . 5141 .. Feaghmaan, . 51 55 —3-73 Forth Mountain, 52 56 ... Precelly, . . 51 56 +0°60 Tawnymore, . 54 17 ... Lough Foyle,. 55 2 +3-20 Ben Heynish, . 56 27 ... Ben Lomond,. 5611 43°71 Cowhythe, . . 57 41 ... Great Stirling, 57 27 —9-48 North Rona, . 59 7%... Monach, . ., 68 21 ,—0:30 pap 5 Hip 69 °-"T" | © "Ben Hytich, . 08. bo cuaraae et Balta, . . . 60 44 .., Saxavord, . 60 49 —2:08 The — sign shewing that the ne is less than the astronomical amplitude. | i | Ordnance Survey Astronomical Observations.’ 355 .* What great events do flow from little things,” says an old comic writer, but the few numbers above are a veritable. Pandora’s box of trouble, likely to make every surveyor and geodesist throughout the earth to tremble, when considering the consequences which must certainly follow. That ‘nothing was given to man without great labour,’ was a proverb in the time of the Romans, and if true in ordinary matters, how much more pointed and impressive does it become when push- ing scientific affairs to the utmost attainable degree of accu- racy. To determine the latitude of a place to 30” is easy enough; to 15’, is not difficult; but to 1’, the difficulty is increased a thousand fold, nay, every property of Nature and of matter seem to combine to prevent our discovering this secret of the world. With a proposed accuracy of 1”, still more if 0’1 or 0’:01 be insisted on, an account must be taken, and an explanation rendered of the above discord- ances, preparatory to any hope of their being eliminated from the determinations for latitude. _Itis easy to attribute the discrepances to “ local erent tion, ”’ but that is merely giving the difficulty a name; and the question still remains as to how a numerical correction ean be obtained. It is by no means the first time that such a disturbing cause has been suspected, but previously obser- vations have been conducted at so few stations, or have heen liable to such great uncertainties from error of observer and instrument, that little attention has been paid to the allegation. Actual mountains have however been generally al- lowed to possess a sensible influence in this way; and then the observing places have usually been picked out at the greatest practicable distance from such questionable neighbours. Such, we conclude, were the precautions taken with the ordnance stations ; and certainly they are more numerous, and better and more uniformly observed, we believe, than any previous set that can be brought to bear on this ques- tion. The probable error of observation is here so small as _ for the time to disappear; and yet there are discordances of _ @ greater amount than ever before known, and therefore plainly and surely attributable to local attraction, whatever that may be. The accusation, in fact, against mother earth is fully proved, and must be proceeded with. 856 Ordnance Survey Astronomical Observations. Now this abnormal attraction can be only that of gravitation, which depends solely on weight ; as, for instance, a pound of gold, a pound of stone, and a pound of ice, placed at equal distances from each other, will act each on the other with precisely similar gravitating forces. If therefore the weight and distance of a mountain be known, its effect on the plumb- line can be computed ; and the first question is, whether the observed deviations can be completely explained by such visible and tangible excrescences on the surface of the earth, or whether they be owing to some heterogeneous construction beneath it? If the former be the case, the elimination is comparatively easy but laborious, for the mountain can in time be measured ; there it is; but in the latter case, where is it, i.e., the attracting body, or bodies ?: At one of their trigonometrical points in Peru, the savants of Louis XIV. found an attraction in the mass of the Andes to the amount of 7”: and more recently Mr Maclear found the attraction of Table Mountain equal to 3’, and that of Piket Berg equal to 2”, at the stations employed by a former measurer of an arc of the meridian in South Africa. In his own determinations therefore, Mr Maclear left the sheltered valleys around the foot of a mountain, and preferred all the inconveniences of placing his instrument on the exposed summit: for there, having the mountain beneath his feet, its attraction acted,—in so far as its mass was uniformly disposed about its culminating point,—in the direction of that of the earth, and therefore could produce no deviation from - the vertical. But in England and Scotland, there are no mountain ranges like the Andes; nay, in the neighbourhood of the survey ter- ° . minal stations, there are no masses comparable to TableMoun- tain or to Piket Berg; and yet the effects of local attraction at many of the stations are greater than were observed in ‘the actual neighbourhood of those giant ranges. The known configuration of the surface of the dry land therefore will not explain completely all the difficulties, nor will any probable shape that may be given to the land under the neighbouring seas. Magnetic and electric affinities, it need hardly be observed, Ordnance Survey Astronomical Observations. 357 are altogether powerless here ; and so we are driven to the only remaining hypothesis, viz., vast caverns underneath the surface of the earth in certain spots ; or, perhaps, immense masses of rock or metal of much less, and in other places, of much greater density and specific gravity, than the neigh- bouring material. But whether holes or masses, or veins or dikes, they must be something mighty in size, and by no means very distant, to produce such great, but at the same time, irregular, effects. : These discordances too appearing so very generally in the case before us, and acting of course on the longitude as well as the latitude, must render uncertain the astronomical elements of position of all places yet observed, by any instruments, in other countries as well as this; for in no place has any cor- rection for local attraction, under as well as above the sur- face, ever been applied, or indeed obtained, or attempted. ‘The multitudinous measures necessary for the purpose are still to be made. | - Hitherto men have fancied, or at least appear by their conduct, with the slight exception already noticed, to have ‘laid the flattering unction to their souls, that to determine the true astronomical position of a spot, they had merely to improve their instruments, and multiply their observations of the stars. But now it is shewn that there is another cause at work, which the above proceedings do not touch. In fact, even if we had a perfect astronomical instrument, and if angels were to observe with it, still the results would be in error by the full amount of the “local attraction ;”’ and that ‘may be far too large to be passed quietly by. ~ Our public observatories will not be affected by the anomaly, so far as their researches in cosmical astronomy are con- ‘cerned; it will only be of importance in geographical as- tronomy. But it will both greatly affect all existing ‘measures of arcs of the meridian, and greatly trouble the ‘mapmakers. How, for example, shall they draw the parallels of latitude through Great Stirling and Cowhythe, when there exists an anomaly there of 9”5, equal to one inch on the 6-inch-to-a-mile maps; and as yet there is nothing to shew on which side of either place, or whereabouts in the 358 Ordnance Survey Astronomical Observations. country the seat of disturbance, and its maximum effect, may be! . In fact, notwithstanding what the French have been in the habit of doing with their maps, and what the croakers com- plained of the Government not doing here, science is not far advanced enough to be able to insert the astronomical latitudes and longitudes with sensible accuracy on large sized maps. If, then, we see parallels of latitude represented by simple straight lines, we may be certain that they are wrong, 7. ¢., they do not represent what a perfect astrono- mical instrument would shew at one place, or a terrestrial measure give at another, and this, ‘too, by a quantity that would permit any amateur, with small observing means, to detect apparently gross errors in the National Survey. The volume, therefore, published by the Ordnance, opens a new and most important and difficult question, rather than it settles the latitudes of the trigonometrical stations. Further steps must, consequently, be taken in the research ; and means must be found of reducing, in all cases, what we may term the apparent, to the true astronomical latitude and longitude. The present book is an exceedingly good one as far as it goes, and it is not the fault of the authors that the case to be investigated has proved more difficult than had been antici- pated, by reason of the influence of occult natural causes ; nor is it at all to their discredit, if haply with the rapidly advancing improvements in astronomical instruments and me- thods, some more perfect instrument still to that which they employed, may now be contrived. Their work is a great ad- vance on all that has previously proceeded out of their office, and we must particularly admire the honesty with which all the original observations are given, together with the elements for their reduction, so that any person may verify the com- putations ; a method of publication, the example for which was mainly set by the present Astronomer Royal; and who ap- pears to have advised all the proceedings in the present case. The men who have satisfactorily carried on the work thus far are doubtless the best to continue its prosecution, and we hope will do so, and have full means afforded them for fol- lowing it out, through all its ramifications. Meanwhile the Ordnance Survey Astronomical Observations. 859 perusal of their record of the past, would seem to suggest,— if we rightly understand the numerous circumstances therein detailed,—the propriety of a few remarks for the future, something as follows :— first,—Of the instrument. The one in question, though a great advance on all previous ~ zenith sectors, still was a zenith sector, and was affected by some of their natural errors,—errors which have driven them out of all astronomical observatories, and have occasioned in this example, the necessity of applying a very ugly and rather arbitrary correction to all the results, depending on the ex- pansion of the arc by being squeezed out under the vertical pressure of the pivot screw at the top of the instrument; which screw at each station was turned different quantities to make more or less squeezing, according to the judgment or memory of the observer. The horizontal axis of the telescope, more- over, was very short, and being unbalanced, tended to wear unequally ; while the levels, being all on one side of the ver- tical axis, would all be similarly affected by centrifugal mo- tion in turning the instrument round, and might all, there- fore, shew too great or too small a reading, by the amount of the retardation of the bubble by friction. We should be inclined, indeed, in the present day, to re- form sectors and levels altogether, by having a transit circle, and obtaining the zero point with the collimating eyepiece. A single observation at each meridian transit, would then give a complete result, and with much greater ease and pro- bable accuracy, than when two observations have to be taken, and a large instrument reversed and reset all in afew seconds, with the stars, too, already beginning to describe downward paths, by reason of their distance from the meridian. 1, Thre prime-vertical transit instrument, has become a favourite for these purposes on the Continent; but although it may give very concordant and apparently accurate results, _ yet in the shape in which it is there manufactured, it must be liable to so much flexure, and in a vital direction to the _ integrity of the observations, that their absolute accuracy may be always doubted. ‘Tn the form of the ordinary transit, ¢. e., with a double axis, 360 Ordnance Survey Astronomical Observations. it may do better; though there is even then great doubt if the level ever can be ascertained as exactly as it should be; and after all, each observation occupies so very great a length of time, as to admit of but very few being taken during a night ; and those may be so seriously interfered with by the abundant clouds of this climate, that a practical man may well prefer a graduated circle in the Meridian. Second,—Of the mode of observing, and reducing the ob- Servations. Each observation before us is made to give an independent latitude, and this is therefore loaded, not only with the in- strumental errors in measuring the zenith distances, but also with the tabular errors of the star’s declination, and what is much more uncertain, its proper motion. The prejudicial consequence of this appears in the columns on the right hand pages giving the observed zenith distances and the computed latitudes, in which latter the discordances are often double the amount of the former. Uncertainties of refraction are certainly mixed up in the latitude results; but as the zenith distance is always small, there can never be any notable effect from that cause; yet we should like, in any future work, to see a discussion of the value of the constant of refraction ; for it would doubtless be found to vary at the different altitudes above the sea, and in the contrasting physical circumstances of the several stations. The greater part, then, of the increase of the discordances amongst the latitudes over the zenith distances, must rest with errors in the assumed values of the places and proper motions of the stars of comparison; and an easy way of remedying this difficulty is to have two instruments: keeping . — one always at a standard station, and having the same stars observed at the same times, with the stationary and with the travelling instrument: a method much practised by Mr Mac- lear in his excellent repetition of the South African are. Thirdly, we may observe, that while we should prefer, at the beginning of the volume, to see entered the very identical numbers read off from the instrument, without, as here, being — reduced from divisions of the micrometer to seconds of space; _ we should also like to see at the close, some investigation Ordnance Survey Astronomical Observations. 361 into the probable errors of the final results. These numbers are given to hundredths of a second, but when we examine the components, and find one star giving a result many whole seconds from another, and all the southern stars having a per- verse discordance to all the northern ones, we evidently cannot depend for certain on the last hundredth. To within how many hundredths of a second, then, can we depend +? What is the real breadth of the foundation on which we can securely build a superstructure of theory and inference, free from the effects of error of observation ? This quantity should be obtained with observations for lati- tude and for longitude also, wherever there may exist so per- fect a means as the electric telegraph for communicating time between two stations. The next step will then be to de- termine in each case the configuration of the neighbouring. ground, by careful contouring (a superb mode, by the way, of settling the levels of a country for engineering and other operations, though discountenanced by the late Committee of the House of Commons): and with the size of the hillocks so ascertained, and with the nearest approach that can be made to a knowledge of their specific gravity, their attrac- tion may be computed. Then according to the character of the residual quantity, obtained by applying the computed to the observed attrac- tion, deduced by comparison of one with many. stations,— further astronomical observations should be instituted at various places, until all the sources of local attraction, and the means of computing their effects for all distances, shall have been discovered. | So far for the elimination of the disturbing effects of the attraction of the mountainous masses. But that having been ascertained sufficiently well for practical purposes ; it is hoped that then the important scientific and physical result of the weight of the world will occupy the attention of the survey- ing department. So long a time has occurred since Dr Maskelyne tried the great experiment on Mount Schehallion, that much advantage might result from repeating his mea- _ sures again, both terrestrial and astronomical, with improved _ means: especially adding observations for longitude as well - as for latitude ; and so observing on four sides of the moun- 362 Notes on the Scales of the tain. But inasmuch as the geologic construction of Sche- hallion is very heterogeneous and uncertain, it might be better to search out some hill of more uniform constitution ; and such, according to the experienced testimony of Pro- fessor Jameson, may be met with amongst the mountains of Sutherland, some of which are of quartz from top to bottom. Ces s: Notes on the Scales of the Government Survey of Scotland. The seales upon which the Government Survey of Scotland should be engraved and published, having naturally excited great interest, and given rise to much diversity of opinion, we have endeavoured to collect some precise information as to the progress, up to the present time, which has been made in this great National work, and the special purposes for which it is designed. - The Government, or, as it is called, the Ordnance Survey of England and Wales, had, up to the year 1824, been pub- lished on the scale of one inch to the mile; and the whole country, with the exception of the six northern counties, was finished upon this scale, and has given great satisfaction to the country, as we learn, from the evidence of several eminent civil engineers, and geologists, to whom it has been found of great value in many important works upon which they have been engaged. But in the year 1824, the whole surveying force of the Ordnance was transferred to Ireland, and as the survey there was designed to form the basis of a general va- luation of the country, for which the scale of one inch to a mile was much too small, the Government directed, after a very mature consideration of the subject, that the scale of the county maps of Ireland should be on the scale of six inches to a mile, and that the large towns should be drawn on the scale of sixty inches to a mile, and that a general map on the scale of one inch to the mile, like that of England, should be prepared by reducing the six-inch maps to that scale. These orders were consequently carried into effect, and the whole kingdom has been engraved and published on the six- inch scale, and the one-inch general map is now in progress, Government Survey of Scotland. 363 On the completion of the survey of Ireland in 1845, that of England was resumed, and that of Scotland commence- ed, and in consequence of the very great advantages which the survey of Ireland had conferred on that country beyond the special object for which it was designed; the Go- vernment decided that, in the progress of the survey of Great Britain, the same series of maps should be published, as had been in Ireland—and in consequence the counties of Yorkshire and Lancashire, Wigtownshire, Kirkcudbright- shire, Edinburghshire, and Haddingtonshire, have been drawn, and the first four counties completely engraved on the six- inch scale; whilst the survey is proceeding in Durham and Fife. We also learn that the primary triangulation of the whole United Kingdom is now complete, and the measure- ment of the are of the meridian, from Dunnose in the Isle of Wight, to Balta in the Shetland Islands, is in course of publication. The progress of the survey of Scotland, which was neces- sarily slow in consequence of the small sums granted for the Service, having created much dissatisfaction, and many emi- nent persons having expressed an opinion that a survey on the seale of six inches to a mile was not required for Scot- land, a Committee of the House of Commons was appointed in 1851 to report upon this subject: The report of this Committee, and the evidence of the nu- merous witnesses examined, contains much valuable and de- tailed information, but much diversity of opinion between the several witnesses ; Sir R. Murchison, Lord Monteagle, Mr Stephenson, Mr Locke, and Mr Brunel, being of opinion that the one-inch scale, like that of the southern counties of England, was all that was required for Scotland ; whilst, on the other hand, Mr Griffiths, under whom the valuation of the whole of Ireland was conducted, and Sir John Macneill, the engineer to the Railway Commissioners of Ireland, and all the Ordnance officers, were of opinion that the scale should be six inches to a mile, like that of Ireland. The following are the recommendations of the Committee: 1. That the six-inch scale be abandoned. 2. That the system of contouring be abandoned. 364 Notes on the Scales of the 3. That.the survey and plotting on the two-inch scale be proceeded with as rapidly as is consistent with accuracy, with the view to the publication within ten years of a one- inch map, shaded and engraved in a manner similar to the Ordnance one-inch map of England. Orders in conformity with these recommendations were given to the Ordnance officers, and in the summer of last year, the survey for the one-inch scale was proceeded with, but as soon as this change became known to the public, great dis- satisfaction was very generally expressed, and numerous in- fluential meetings were held in several counties, in Edinburgh, Glasgow, and many of the principal towns, to memorialize the Government to proceed with the survey of Scotland as as they had begun it. On the receipt of these memorials, the Chancellor of the Exchequer (Mr Disraeli) ordered the survey for the one-inch scale to be discontinued, and the counties of Haddington and Fife to be surveyed on the six-inch scale, and that no other county should be taken up “ till this important subject shall have received further investigation.” _ It is greatly to be regretted that so much time and money should have been lost, but it was obviously better to stop the work for the small scale at once, than to allow it to proceed, and produce dissatisfaction in the country, with the prospect of eventually losing more time and money on a work not cal- culated to meet the wants of the Government, and the country at large. _Most of the memorials have appeared in the journals of the day, but we select that from the gentlemen of Dumfries- shire, as expressing what appears. to us to be the general feeling of the people of Scotland upon this subject. “To the Honourable the Lords Commissioners of Her Majesty's Treasury, the humble memorial of the Com- missioners of Supply of the County of Dumfries, ‘“ Sheweth,—That the memorialists had under considera- tion at their annual meeting held in April last, which was numerously attended, the subject of the Ordnance Survey of Scotland, when they had occasion to express their regret at the delay which has taken place in the prosecution of it; and on the motion of Sir William Jardine of Applegarth,. it ~ a ———— le SS hme CCC i tind 2 eh re ee Government Survey of Scotland. 365 was unanimously resolved to urge the Board of Ordnance to proceed with its completion, with as little further delay as possible, and that upon a scale of sz inches to a mile. “This resolution was accordingly communicated to the board; but the memorialists were informed that it rests with your Lordships alone to set aside or modify the present ar- rangement for completing what remains of the survey on a scale of one inch to a mile. ‘« The one-inch scale being considered by the memorialists so entirely useless for all nenedital purposes, the matter was again brought forward at their Michaelmas meeting, held on 5th October last, when (in consequence of the above infor- mation) it was resolved, on the motion of his Grace the Duke of Buccleuch and Queensberry, to present this memorial to your Lordships in support of the early completion of the survey of Scotland on the large scale; at the same time, calling attention to the peculiar advantages which a survey of Men county of Dumfries on this scale would confer, as in comparison with one on the reduced scale. | “ The: memorialists are humbly of opinion, that six-inch maps of the counties of Scotland would be much more useful for all public, local, and private purposes, than plans on the one-inch scale ; and indeed, that the latter would be even of less service than plans already existing ; while the difference of cost, having regard to the superior advantages of the large plans, would not be so great as to justify a departure from the system pursued in the survey of the United Kingdom up to a very recent period. | “The larger maps, with the levels inserted upon them, would be highly useful for all purposes connected with engi- neering; the formation of railways, canals, roads; the con- veyance of water to towns; sewerage ; the reclamation of marshes ; and the improvement of waste lands; the collec- tion of correct agricultural, mineral, and other statistics, in- cluding a correct census; the procuring of correct geological and hydrographical surveys; the valuation of property in re- ference to sales and to public and parish assessments ; the management of estates; the identification and registration of different properties, and in various other ways; for most VOL. LIV. NO. CVIII.—APRIL 1853. 2B 366 Notes on the Seales of the of which purposes the smaller maps would be of compara- tively little use, and for the more important would be of no service whatever. “The larger map would not merely be valuable for pbeiont purposes ; as an authentic record of the state of the country, and the boundaries of properties, parishes, and counties, it would in after ages be regarded with interest, and be found of great use in tracing the progress of improvement and the changes occurring in the course of time. “ The memorialists have respectfully to submit that there is no valid reason why Scotland should not have the benefit of a national survey on the enlarged scale. She contributed a proportion of the expense of the survey of the sister coun- tries. There are extensive tracts of as wild countryin Ireland as in Scotland, and upon the utility of surveying the former country on the large scale, the argument that large plans of such waste grounds were unnecessary was never raised. It appears to the memorialists, therefore, that it would be unjust to give Scotland inferior maps on the ground of expense. Besides, it is of manifest importance, in a national point of view, to have uniform connected maps, applicable to the entire United Kingdom.” These memorials would seem to have decided the Govern- ment to give to Scotland the benefit of a survey not inferior to that of Ireland; and we see, by a correspondence recently published between Sir Charles Trevelyan and Major Larcon, R.E., the present Under-secretary for Ireland, to whose energy and ability the perfection of the agricultural statistics of that country is mainly due, that the question of the best seales for the survey of Scotland is still under consideration. Major Larcon is asked if the six-inch survey of Ireland has fulfilled the objects for which it was designed, and whether, if the survey of that country had to be done over again, he would propose a larger scale; to this he replies, that the survey has fulfilled all the objects expected from it, and that he should recommend the same scale if the work had to be gone over again, and recommends that it should be extended — to the whole of Scotland. Mr Griffiths, to whom these replies were communicated, concurs fully in these views, which are Government Survey of Scotland. 367 in accordance with the evidence he gave before the Parlia- mentary Committee of 1851. We therefore confidently hope that the survey will now proceed without further interruption and delays. We have seen with great satisfaction that an additional grant of £10,000 appears in the Ordnance estimates for this year, making the grant for this year £35,000 for the survey of Scotland—a sum which will enable the Ordnance officers to proceed rapidly in their work, and give employment to a numerous body of assistants from our population. K. On & Quariziferous Variety of Trachyte, found in Iceland. By THEODOR KsHRULF, of Christiania. Communicated for the Edin. New Phil. Journal. Amongst the trachytic formations of Iceland, which appear from the investigations of Bunsen to exhibit, along with the greatest mineralogical differences, a remarkable chemical agreement, and which, in a paper inserted in the twenty-third volume of Poggendorff’s Annalen, he terms “ normal tra- chytic,” there are some which are characterised by the occur. - rence of interspersed quartz and rock crystal. These, as well as the other trachytes of Iceland, belong to Abich’s “ tra- chytic porphyries,” with which they harmonize, not only in their chemical compdsition, but also in the circumstance of their assuming, for most part, a porphyritic appearance by the interspersion of minute lustrous lamella of felspar. In the rocks referred to in the following paper, which belong to these formations, these felspar secretions are absent, although in them likewise the rock presents a porphyritic appearance, from being interspersed with quartz. We might give it the appellation of quartziferous trachytic porphyry. The mass appears decomposed, almost friable, and in colour varying from light green to yellowish red. In similar varieties of trachyte, the mass being the same, but quartz being absent, there could be distinguished small spicula of iron pyrites, _ which seemed to indicate a subterraneous formation by the _ disengagement of sulphureous vapours from fissures (Fumaro- q lenwirkung). In the present rocks, however, I could not, 2B 2 368 ~ M. Theodor Kjerulf on a even with the assistance of a lens, detect iron pyrites, with anything like certainty, although that variety 2 exhibited traces of sulphuric acid and spicula, resembling hydrous oxide of iron. The materials for the investigations of which the results ~ are here communicated, were collected by myself on the spot, during a journey to Iceland, in the summer of 1850, and the analyses themselves, were conducted according to the method followed by Professor Bunsen, and communicated by Dr Streng (Bietrag zur Theorie der vulkanischen Gesteinsbildung, Bresl., 1852.) In the environs of the Baula, a mountain from which so much instruction may be derived in regard to the trachyte of Iceland, I could not, after the most careful search, discover any of the quartziferous rocks. These I have observed only, not under the most favourable circumstances for observation, at Kalmanstunga in the western, and at Trollakirkja, in the northern, parts of the island. At Kalmanstunga, at the de- clivity of the mountain which stretches towards Koita, there is an alternation of numberless varieties of trachyte, com- pact, earthy, nodular, breccious; and it is amongst the frag- ments of the latter, that at the declivity in question, the quartziferous porphyritic trachyte is found. The contiguous rock and the junction of the two are, unfortunately, concealed from observation by heaps of rubbish. As far as could be recognised, the whole composed a veniform mass (eine stock =oder gangformige masse), which might probably extend over Tunga to the trachyte cliffs of the Nordlingafljot. It should also be mentioned that the trachyte mountain in the neighbourhood of the above-mentioned locality, has been broken through by a basaltic mass, which can be recognised at a considerable distance by its beautiful columns. The second variety subjected to analysis is from the northern dis- trict of the island, where the road from Fagranes to the Ska- gafjordr leads through the narrow valley of Vidadalr towards Grimstungur. Right across the valley, where it stretches in a southerly direction, there runs down from the mountain of Trollakirkja a vein of quartziferous trachytic porphyry, but here likewise the line of junction with the adjoining rock, which was a common dark augitic and palagonitic rock dis- ee ee ae Quariziferous Variety of Trachyte found in Iceland. 369 posed in beds, was nowhere to be observed; even the thickness of the vein itself, which seemed to run from 6 to 14 feet, could scarcely be determined. A dark green vitreous rock of june- tion (Contactgestein), which is found at the Baula as well as almost everywhere else in Iceland, where the trachyte sepa- rates from an augitic or tuff rock, was not observed here, but may very possibly have been concealed under the loose rubbish, which the unfavourable state of the weather unfortunately put it out of my power to subject to a very close examination. The rock No. 1, is composed of a greenish mass in which are imbedded small white globular particles, very distinctly separated from the matrix. These globules are either entirely filled with a hard white quartzose mass, or else they form a globular crust, of which the internal cavity is occupied with beautifully transparent points of rock crystals. The rock No. 2, appears to be more decomposed than the former; the mass, which is of a light yellow reddish colour, is almost friable, and the quartz crystals are found distributed in more irregular cavities. On comparing the two varieties, they seem to exhibit different phases of the same process of decom- position ; the globules disappearing and giving place to cavities, as the matrix itself becomes more friable. The reddish powder of No. 2, after being digested for a short time in con- centrated muriatic acid, totally loses its colour, and becomes snow-white. The composition of these two varieties, as appearing on analysis, calculated on the anhydrous substance, is as fol- lows :—No. 1 losing 1847 per cent., and No. 2 losing 1°656 per cent., by being brought to a red heat. No. 1. No. 2. Silica, . ; : : 78°149 81-364 Alumina, , j : 11°522 10-241 Oxide of iron, ‘ ; 1‘655 1°931 Lime, . . : 3 0°465 0-301 Macnesia, : : , 0:058 Protoxide of manganese, } wea bees 0-076 Potassa, : : ; 2°898 4:878 Soda, . ‘ : ‘ 4°195 2°030 98:951 100:879 570 M. Theodor Kjerulf on @ Or, to afford readier means of comparison with the compo- sition of normal trachyte, it may be calculated at 100, and with protoxide of iron, as follows :— Normal Trachyte, No.1. “No. 2. Silica, : : . ; 76:67 79°11 80°81 Alumina, . : ; ; 14-93 11-67 10:17 Protoxide of iron, 1°51 1:73 Lime, : : : : 1:44 0:47 0:30 Macenesia, , ; : 0:28 0:07 0:14 Potassa, . ; ; : 3°20 2:98 4:84 Dr ee etka te 4:18 4:24 2-01 100:00 100-00 100-00 Thus we have very nearly the composition of normal tra- chyte,—the proportion of silica being somewhat larger, espe- cially in the variety in which decomposition has proceeded farthest. In order to check the analysis, I endeavoured, with No. 2, which presented most facility for the purpose, to ascertain the per centage of quartz crystals. A certain quantity, after being weighed, was gently crushed, and water being after- wards poured over it, the light supernatant particles of the mass were removed, and the residuum dried and strongly heated: the quartz crystals, which could then be easily dis- tinguished, were separated mechanically from the small red- dish fragments of trachyte, and from a few particles of white quartz. The result was 29, or 3 per cent. In this experi- ment, which was very carefully performed, I cannot imagine that there was room for an error of more than one per cent. loss at the utmost, so that the proportion of ae cannot possibly exceed 4 per cent. The question now arises, whether this excess of silica has been conveyed into the rock by infiltration, or whether it has proceeded from a partial elimination of its basic constituents. The answer to this question is, geognostically, of some in- terest. If we take as our basis the composition of normal trachyte,—and from the local relations of the porphyritic varieties with other trachytic rocks at Kalmanstunga, it seems exceedingly probable that the former have been formed from the latter. We are able, either on the one hand, upon > Po Quariziferous Variety of Trachyte found in Iceland. 371 the supposition of an infiltration of silica into what was ori- ginally a mass of normal trachyte; or, on the other hand, upon the supposition of a partial elimination of the bases, to arrive by calculation, at compositions nearly identical with No. 2. For, if to 5 portions of normal trachyte we assume the infiltration of 1 portion of silica, the composition 3 will be the result; and we obtain the composition 4, if, of 8 por- tions of undecomposed trachyte, 2 portions undergo altera- tion in such a manner as that their contained bases are, by the action of volcanic vapours (Fumarolenthitigkeit), elimi- nated in the form of sulphuric salts,—their silica at same time remaining :— No. 3. No. 4. No. 5. Silica, .. : : : 80°56 80:76 80°22 Alumina and protoxide of iron, 11:86 11:98 12:27 Lime, ; - j ; 1:20 #21 0°31 Magnesia, , ; : 0:23 0:24 0:14 Alkalies, . : i g 6:15 5°78 7:06 100°00 100:00 100-00 _ Thus, it might seem as if the question were incapable of solution. But the alternative is really decided by the obser- vation, that in No. 2 there is contained not more than 3—4 per cent. of free silica. In the calculated composition 3, in which 1 portion of quartz becomes added to 5 portions of nor- mal trachyte, there would be required, not 3 or 4 per cent., but no less than 16-66 per cent. of free silicic acid. Where, again, (in 4) 0-2 of the whole mass is conceived to have been decomposed in the above manner, there remains just 3 per eent. of free silicic acid, which might very readily appear in the form of quartz and rock-crystal. Farther, if No. 2 had arisen under the influence of a process of infiltration, the re- sult of its composition must, after subtracting the 3 per cent. quartz, have been identical with that of normal trachyte. Such a calculation, however, gives as its result, not the com- position of normal trachyte, but one containing a larger amount of silica (5). If, then, an elimination of bases have actually taken place in 1 and 2, it may be anticipated that this process will not have extended in a precisely similar degree to the whole con- 372 Quartziferous Variety of Trachyte found in Iceland. stituents. Now this inequality will actually appear, if we calculate the composition of normal trachyte and that of the varieties 1 and 2, without reference to the silica, for like quantities of one of the bases, e. g., the alumina :— Yor Normal Trachyte. For l. For 2. Alumina and protoxide of iron, 100:00 100:00 100-00 Lime, : : ; ; 10°11 3°56 2°51 Magnesia, . ‘ : . 1°81 0°53 1:18 - Alkalies, . ; ; : 52°58 54:40 57°56 For these reasons, as well as from the external appear- ance of the rock, which of itself indicates the operation of volcanic gases (Fumarolenwirkung), I think we are entitled to conclude that the quartz, which we so unexpectedly find in this trachyte, is derived, not from the infiltration, but from the secretion of silica. Almost everywhere in Iceland, where trachytes occur, I have observed amongst them compact and earthy varieties, resembling the fumerolle clay, frequently along with spicula of iron pyrites,—as near the Baula, at the Indridastadir, near Skorradalsvatn, at the Illvidrishnukr, in the northern district of the island, not far from where variety 2 is found. The analysis of the trachyte of Langarfjall, at the Geisir, which continues to be decomposed by the influ- ence of fumerolles, exhibits a similar elimination of bases, especially a striking diminution of the alkalies. It is not im- probable that, whilst the silica secreted in 2, in the course of the partial decomposition, remained in the rock ; of the liber- ated bases, the alkalies, and about half the alumina, were eliminated in the form of alum, the other half of the alumina, together with the whole lime and magnesia, being eliminated in the form of sulphuric salts.* * Liebig’s Annalen der Chemie, &c., vol, lxxxv., part 3. 373 Biography of the celebrated Naturalist, Baron Leopold von Buch. Communicated for the Philosophical Journal. Berlin, March 6.—LEOPOLD VON BUCH is dead. He expired on the 4th instant, at two o’clock afternoon, after a short illness. The once so active pedestrian, who even in his old age used, when on geological excursions, by the extraordinary amount of fatigue which he underwent, to put many a junior to the blush, had of late been exhibiting, physically although not intellectually, distinct signs of advancing age. In him Germany loses not merely one of the most famous of her literati, but one of those rare and extraordinary men on whom the world, with its gifts and external distinctions, has nothing in its power to bestow. Leopold von Buch was totally ab-. sorbed in his science—in the most unselfish efforts after the attainment of truth. One must have seen and known himin | order to be able to comprehend the strength of his character —a character which, from that very quality—especially in _ such an atmosphere as Berlin—-could not fail to be distin- guished by some oddities. Buch was born, not, as has been commonly stated, in 1777, but on the 26th of April 1774, and was a contemporary stu- dent with Alexander von Humboldt in the Mining Academy of Freiberg. Of all Werner’s pupils it is he who has contri- buted the most to the progress of geology, and who can be most aptly compared with the Comte de Saussure, whom he not merely equalled in the comprehensiveness of his minera- logical and physical knowledge, in acuteness, in talent for observation, and in unwearied zeal, but also resembled in another respect : already in the possession of a fortune equal to his wants, he gave himself wholly to science, without the least reference to personal advantage, or its application to the practical purposes of life. In the year 1797 he published a little work under the title of “ An Attempt at a Mineralogical Description of Landeck in Silesia’? (Versuch einer mineralogischen Beschreibung von Landeck), which was a perfect model of clear and simple ex- position, and of concise and perspicuous description. In the 374 Biography of Baron Leopold von Buch. same year he quitted the north of Germany, different portions of which he had already examined, of course under the influ- ence of those neptunistic views which he had imbibed from Werner, and directed his footsteps to the Alps, of which he may,in a scientific point of view, be regarded as the Columbus. In examining the district of Salzburg, so rich in natural beauties and in striking geognostic phenomena, he enjoyed the congenial companionship of Humboldt. Of this profitable intercourse there remains an imperishable monument in the description of Salzburg, which may be regarded as a model of description of great mountain regions. In the spring of 1798 he instituted the first careful inquiry into the central alpine chain through the Tyrol; and from thence, after long impediments, arising from the continuous wars of the French Republic, he succeeded in February 1799 in reaching Naples. Here he directed his attention to the . study of Mount Vesuvius, and it was the phenomena of this volcano that first awakened doubts in his mind with regard to the soundness of Werner’s doctrines. An old Neapolitan still boasts with delight of having been the guide of Buch and Humboldt through the lava ruins. But it was not until the year 1805 that Buch had an oppor- tunity, in company of Humboldt and Gay-Lussac, of witness- ing agreat eruption. He then found himself enabled to cor- rect a number of erroneous views, hitherto generally enter- tained, with regard to the activity and products of voleanoes. His mind had been prepared for the subject by a previous journey through the south of France. In the year 1802 he had examined the extinct volcanoes in the district of Auvergne, and discovered that the volcanoes break out from the granite ; but, cautious inquirer as he was, he did not consider this as sufficient to overthrow the Wernerian theory. Recognizing the extraordinary scientific importance of a remarkable phe- nomenon, he was too cautious to make it the basis of a universal Jaw; and it was not until after more extended in- quiry, and the accumulation of new facts, that he allowed himself to assign a similar mode of origin to the German basalts. The fruit of his inquiries appeared in his ‘‘ Geognos- tical observations during travels through Germany and Biography of Baron Leopold von Buch. 375 Italy” (Geognostische Beobachtungen auf Reisen durch Deutschland und Italien), 1802-1809. _. Two full years—from 1806 to 1808—were passed by him in Scandinavia, where he found, to his extreme surprise, that granite, which had hitherto, in conformity with the views of Werner, been regarded as indubitably a primary rock, was to be met with betwixt younger formations. He was the first to ascertain the fact that the whole continental part of Sweden is undergoing a continuous but very slow upheaval. On his return home he passed through Lapland (“ Travels through Norway and Lapland,’’—Reise durch Norwegen, &c., 1810). In company with the Norwegian botanist Smith, who after- wards met his death in the unlucky English expedition to Congo, he made arrangements in England, which he had embraced this opportunity of visiting, for a voyage of disco- yery to the Canary Islands. In April 1815 the two naturalists landed in Madeira, and Buch was not long in recognising an axiom of the utmost weight for the theory of volcanoes, namely, that as the whole Canary Islands are collectively the _ work of a voleanic action on its grandest scale, so the other islands of the ocean had a similar origin, and the groups of islands of the South Sea are the remains of a pre-existing continent. . The voleanoes on the earth’s surface are for the most part collected in series that frequently stand in certain relations to each other, and result from immense fissures through which subterranean forces effected a passage for themselyes. These fissures follow the direction of promon- tories. The Lipari Islands, Etna, Iceland, the Azores, the Canaries, are to be regarded as central voleanoes. The con- tradistinction of craters of elevation and craters of eruption, which afforded a peculiar explanation of very interesting vol- canic phenomena, met with determined opposition, and one of the strongest opponents was Buch’s own principal scholar —whose early death was a severe loss to science—the justly regretted Hofmann, who, in the course of his travels through Sicily, had the good fortune, when at Sciacca, to be able to observe the origin of a small volcanic island. The “ Physical Description of the Canary Islands’’ (Physische Beschreibung der Canariochen Inseln), has now become exceedingly rare. 376 Biography of Baron Leopold von Buch. Buch, during his stay in the British Islands, made minute observations upon the Hebrides, and the Giant’s Causeway in the county of Antrim; and afterwards, in the Alps, he directed his attention to the study of porphyries. His ex- planation of dolomite has lately met with much and partly well-grounded opposition. How conscientiously he pursued his labours may be perceived from the circumstance that in. his old age he made a second journey to Norway, in order to observe some facts bearing upon the transition of primary rocks. The essential aim of Buch’s labours had always been to invest the science of geology with a universal and organic character, by comprehending all its elements in one vast whole—the geognostic and physical relations of the earth’s surface, temperature, soil, plants: at a later period of his life he enriched it by a profound study of petrifactions. He gave a direction to paleontology, by means of which it became possible to draw from the remains of an extinct animal crea- tion the most important conclusions with regard to the process of formation of the earth’s crust. This merit will remain, even though geology may resume the path of chemical analysis. But Germany may be especially proud of the very excellent geological map which she owes to the illustrious deceased ; and when his miscellaneous writings, and particularly those minor compositions which are now lying scattered through the Transactions of academies, become, by being collected— as no doubt they will be—accessible to the general reader, the noble language and scientific method by which every line that Buch wrote was distinguished, will become duly appre- ciated. In a work on Volcanoes which is now passing through the press, Alexander von Humboldt has unconsciously erected a worthy monument to his illustrious friend. 377 — (pausig 7s “saqpout TL:6), ‘uver 1e30 I ‘porod yey) Suzanp ate SUOLJEATOSGO XIS JO oSer0ae ay} JO ynser oYI—"G08z-,08 useq sey ‘(uosvas furer oy}) saquiazdeg ‘asnSny ‘king ‘oung ‘Key Sutanp San qiaq Aap oy} jo oanqesoduo, uvam of, “UvSOq SUIeI OY} OOUIS UGS U99q SuTAvY you ‘pournyor "uolyedodead 19}eaI19 Suryeorput sqinq Aap pue yom oyj—‘selmp yonut esoydsouye ‘yquout oy} jo yaed 1094R] ¢ Ajpenbs Aypeuorsevoo0 $sseduoo oy} Jo szojrenb ye ur ‘Xpeojsun fsoa puta, “yoy Aro pue ‘ouy uoeq ‘skep [Z uo ][9J—Soyour JQ-S]T YUOW sty} uret Jo AqUENe "‘ATUAVY “¢ souly oy} TZ 9} UO OY} SULINP SWA10}S-lapuny} Mo ® Sty J jo yred aoyjv] OY, “AoWA0F OY} ULY} Aolip U9dq Sv YOU SIU, | | | GZ0-0E | 96-64 | 40-08 || T46-63 | G6-6G | 10-0€ || 6686-62 | 16-62 | G0-0€ || 100-08 | $6-63 | 20-08 || FE0-0F | 86-6 OT-0€ | 4010-08 | 6-66 | 10-06 “UBOW “UIT “XBT *“UBOfL “UTTAL “XPT “UvOTT mtany “XPT “UvOTN “Ul, XPT “UVOTL “UTTNT | “XBL | UvOT “UT XVI "W'd 6 ‘OT ‘yosung ‘Od ‘Wd & ‘0d "U00ON ‘OM “WV 6 ‘OG | ‘asIIUNG 4B JoyouloIeg . t, | | ‘qing GG8-.84 | 3-94 | G8 || 886-84) LL el® 86-68 oll ol6 18h o68| GL 006 || 686-18 | 94 oV8 | V8¢-.l1] GDL ol8 iq we x SKE E OES e = LOT LL DL oL8 869 DL eGL G.8L GF-.84 of ol8 Fol: 8h oDh oV8 GS-84 oD ¢. ob L . GS: 9L ove ooh JOM “ “sy "S}EAL 5 I. "g é l-ssqeza.t0sq sAeATS0O| oy | xem [ee ato] samy | xen [ee yo ues) “uC | xen lez so woo] “WHE | “SPW log yo ucoyy| “UMN | XEN logyo weoy| “HC |W | | i U ee | | al Se ; ‘N'd 6 ‘OW “yasung ‘Od ‘W'd © ‘0d ‘WOON “OG | | ‘AV 6 ‘OG | ‘esluung 4% JeyemoUNTeyy, ‘NOSTESTNHO uLONVXUTY iq 4q payeorunuim0g ‘“zegT waquagdag sof uoobuny yp vajsiboy PA ribo ay? fo 200.498q 7 ‘ 378 On the Reduction in the Height of Waves On the Reduction in the Height of Waves after Passing into Harbours. In a Letter to Professor Jameson. By © THOMAS STEVENSON, Esq., Civil Engineer. Kdinburgh, 84 George Street, 16th March 1853. DEAR Sir,—In your number for October last I gave an approximate formula for the law of increase in the height of waves due to their distance from the windward shore; and I have now to trouble you with another formula relating to the subject of harbours. The great object of constructing harbours is, by lowering | the height of the waves to preserve the tranquillity of the area of water which is included by the piers, and this pro- perty is variously possessed by harbours of different forms, and depends much upon the shape of the entrance and the relation between the direction of its opening and that of the line of maximum exposure. It may here be observed, that when there is an inner harbour, or stilling basin, the ellipti- cal form seems to me the most promising. If one focus be supposed to be on the middle line of the entrance, and to coincide with the point from which the waves radiate, as from a centre, when they expand into the interior of the harbour; and if the other focus is situated inland of high- water mark, the waves will all tend to reassemble at the landward focus, and on their way will be destroyed by breaking on the beach. For it is a well-known property of the ellipse, that, if two radii vectores be drawn from the two foci to any point in the curve, they will make equal angles with the tangent at that point, and as the angles of incidence and reflection of a wave from any obstacle are practically equal, each wave will obviously be concentrated at the focus opposite to that from which it emanated. Irrespective of the considerations mentioned above, the reductive power of a harbour will be dependent on the rela-. tion between the breadth and depth of the entrance, and the form and capacity of the area within. Where the piers are high enough to screen the inner area from the wind, where after Passing into Harbours. 379 the depth is uniform and the quay walls are vertical, the following formula may be tried for cases in which D is not less than 50 feet :— H = height in feet of waves in the open sea. reduced height of waves in feet at place of observation in the interior of the harbour. = breadth of entrance to harbour in feet. breadth of harbour at place of observation in feet. = distance from mouth of harbour to place of observation 8 ll SS oo eo. lI in feet. Sire st etn Eat BS deg} B 50 This formula I have found to give good approximations at several harbours where the heights of the waves were regis- tered. When H is assumed as unity, w will represent the reductive power of the harbour.—I am, yours faithfully, THOMAS STEVENSON. Professor JAMESON. SCIENTIFIC INTELLIGENCE. GEOLOGY AND GHOGRAPHY. 1. Extent of Glaciers in the Polar Regions.—On every side of the southern pole, on every meridian of the great South Sea, the seaman meets icebergs. Notso in the north. In the 360° of longi- tude, which intersects the parallel of 70° north (about which paral- lel the coasts of America, Europe, and Asia, will be found to lie), icebergs are only found over an extent of some 50° of longitude, and this is immediately in and about Greenland and Baffin’s Bay. In fact, for 1375 miles of longitude we have icebergs, and then for 7635 geographical miles none are met with. ‘This interesting fact is, in ihy opinion, most cheering, and points strongly to the possibility that no extensive land exists about our northern pole,—a supposition which is borne out by the fact, that the vast ice-fields off Spitzbergen shew no symptoms of ever having been in contact with sand or gravel. Of course, the more firmly we can bring ourselves to believe in the ex- istence of an ocean-road leading to Behring’s Straits, the better heart ral 380 Scientific Intelligence—Zoology. we shall feel in searching the various tortuous channels, and different islands with which, doubtless, Franklin’s route has been beset. . It was not, therefore, without deep interest that I passed the boundary which nature had set in the west to the existence of icebergs, and endeavoured to form a correct idea of the cause of such a phenome- non.—(Osborne’s Arctic Journal, p. 94.) 2. Faroe Islands.—Sir Walter C. Trevelyan to Pr ofessor Jameson, —25th February 18538. My Dear Sir, As you have sometimes thought notices from the Faroe Islands oh sufficient interest to insert in your Journal, I now send you an extract from a letter I lately received, which you may, perhaps, like to publish in your next Number. “RAROE ISLANDS, 24th December 1852.. ‘** Turnips have been too little used here, but if the potato disease continues, and it has been worse this season, I am sure they will be more cultivated. As the porn failed, the inhabitants would have been badly off, but abundance ‘ of whales’ (Delphinus Tursio) hav- ing been caught last season, in some way made up for the loss. More than 2000 whales were killed in different places. In one har- bour (Westmanhavn) we take them in a large net, in which more than 300 have been caught at one time. The net is made of ropes, 200 fathoms long and ten fathoms deep, it is of sufficient strength, but the whales sometimes escape under it. * From the year 1819 to 1843, there were killed in Westmanhayn not more than 280 whales, although many shoals of them visited the harbour every year, in some years more than 1000. From June I, 18438, when the net was first used, up to this time, we have caught 2200 in Westmanhavn alone. Each whale being valued at an average to produce thirty gallons of oil, makes the value gained to be about £4000, besides the flesh, which furnishes abundance of wholesome food.” | ZOOLOGY. 3. Numerical List of Species of Animals.—Of the number of dis- tinct specific forms of animals at present existing upon the earth’s sur- face, it is scarcely possible to form even an approxiniate estimate : since, although we may be probably not far wrong in our calculation of the number of existing species, in certain classes which have been espe- cially studied (such as those of mammals and birds), and of which by far the greater part are certainly known to us; it is at least equally probable that our present acquaintance is limited (fom various causes) to a very small proportion of other classes, whose total amount, therefore, we can do little more than guess at. The num- ber of species of mammals known to naturalists is about 1700; and it is probable that scarcely 300 more remain to be discovered. Of Pe Scientific Intelligence—Zoology. 381 birds, about 8000 species are certainly known ; and to these we may perhaps add 4000 for those not yet discovered, or not yet clearly dis- tinguished. Of reptiles, about 1200 species are known; but it is probable that the proportion not yet discovered is larger, and that for this we should add at least 800 species. Of fishes about 8000 species are known; and to these, also, numerous additions may be expected, probably at least 4000 species. Thus of vertebrated ani- mals alone, nearly 19,000 species are known, and 9000 more are probably in existence. The number of mollusks has been hitherto reckoned chiefly by that of the shells contained in collections, no ac- count being taken of any but the testaceous species. Of these about 15,000 species have been collected ; and probably at least as many more yet,unknown to the conchologist. But the number of ‘“ naked” or shell-less mollusks is undoubtedly extremely large ; and of these it is probable that only a small proportion are yet known.* The class of insects far outnumbers all the preceding, both as to number of species already known, and still more as to the number of. whose existence we have presumptive evidence. | It is certain that at least 150,000 species are at present to be found in collections; and that these do not by any means include the total number existing even in the countries whose entomology has been best explored. So little, in fact, is this the case, that if anything like the same. proportion holds good elsewhere between flowering plants and insects, as obtains in our own country (namely at least ten species of insects to every species of flowering plant), we should have to estimate the total number of existing species of insects at little less than two millions. In regard to none of the inferior classes, have we at present adequate means of forming any estimate whatever.—(Carpenter’s Principles of General and Comparative Physiology, p. 239.) 4. Dr Hamilton on the Guano Birds of the Lobos I: Jaane Along the sea-coast of Peru and Bolivia, within the tropic of Capri- corn, countless numbers of aquatic fowls exist which live on fish, and lous excretions are exceedingly fertilizing. In some inealinien, the number of guanas is enormous, so that when alarmed by discharges of fire-arms, or otherwise, they rise from their resting-places in such masses as cannot be supposed by those who have never seen these birds darkening the air likea cloud. Guano producers change their habitation when continuously disturbed, but they do not permanently leave a locality which has long been tr equented by them in conse- quence of a temporary alarm ; for, in such a case, they soon return to their old haunts, and totally abandon them only when teased by - * Thus, of the tribe of Nudibranchiate Gasteropods, only about a dozen species were formerly known as inhabiting the coast of Britain; but in the beautiful monograph of Messrs Alder and Hancock (in course of publication by the Ray Society), more than a hundred species will be described. * VOL. LIV. NO. CVII.—APRIL 1853. 2 oO 382 Scientific Intelligence—Zoology. lasting annoyances. The ocean on the west coast of South America, within the tropics, teems with fish, the quantity seeming exhaustless, and guanas equally abound, so that their egesta is gradually accuniu- Jating somewhere either on or off that desert land, and now has become an object sought after, not only by the Peruvian mountaineer, but by the merchant, shipowner, and statesman. 0. The Cod Fish of the Whale Fish Islands.“ We are pre- paring,” says Mr Snow, in his Journal in the Arctie Seas, ‘‘ in calling at Whale Fish Islands, at which place it was hoped we should be on the following day, if the wind continued the same. : * Our dinner this day was greatly impoved by some ¢od fish that had been caught in the morning, before the wind sprung up. It was excellent eating, and I believe the fish is considered of sufficient worth and goodness to have a few vessels from Scotland eniployed in eatching and importing them. ‘There is one particular place on this coast where they are said to be very numerous, and some small ships have made it an excellent trade.”—(Mr W. Parker Snow's Journal in the Arctic Seas, p; 60.) 6. Electricity applied to the capture of Whales.—The most pro- minent features of this new method are thus described :—Every whale at the moment of being struck by the harpoon is rendered powerless, as by a stroke of lightning ; and, therefore, his subsequent escape or loss, except by sinking, is wholly impracticable, and the process of lancing and securing him is entirely unattended with dan- ger. The arduous labour involved in a long chase in the capture of a whale is superseded, and, consequently, the inconvenience and dan- ger of the boats losing sight of or becoming separated from the ship is avoided. One or two boats only would be required to be lowered at a time, and therefore a less number both of officers and seamen than heretofore employed would be ample for the purpose of the voyage. The electricity is conveyed to the body of the whale from an electio- galvanic battery contained in the boat, by means of a metallic wire attached to the harpoon, and so arranged as to reconduct the electric current from the whale through the sea to the machine. The ma- chine itself is simple and compact in construction, enclosed in a strong chest weighing about 860 lb., and occupying a space in the boat of about 84 feet long, by 2 feet in width, and the same in height. It is capable of throwing into the body of the whale eight tremendous strokes of electricity in a second, or 950 strokes in a minute, para- lysing, in an instant, the muscles of the whale, and depriving it of all power of motion, if not actually of life.—(Year Book of Facts, p- 141.) 7. Preservation of Eggs.—Eggs immersed while fresh in milk of lime will keep in it for years, doubtless because the carbonate of lime formed by the carbonic acid, evolved from the egg, completely stops up the pores of the shell. On pulling down a sacristy in the Scientific Intelligence—B otany. 383 neighbourhood of Lago Maggiore, eggs were found quite fresh, after having been surrounded with mortar and enclosed in a wall for 300 years.—(Hand-Book of Chemistry, vol. vil. of the Cavendish So- ciety, p. 116.) BOTANY. 8. The Genus Nostoc——Dr Joseph Hooker has read to the Linnean Society a paper on the genus Wostoc of botanists, more especially on a species brought by Dr Sutherland from the North Pole, during the late expedition in search of Sir John Franklin, under Captain Penny. The plant was found in great abundance in the ocean, and resembled the Nostoc commune of botanists. It was in sufficient quantities to be used as diet; and Dr Sutherland having eaten some of it, pronounced it more agreeable and nutritious than the Tripe de Roche. Specimens of this plant had been sent to Mr Berkeley; and, from certain points in structure, he con- sidered it a new plant, and referred it provisionally to the genus Hormosiphon, under the name of H. arcticus. Dr Hooker also gave an account of a species of Nostoc which he had discovered in Thibet, and of another in China, which seemed identical with the one brought from the North Pole. The T'ripe de Roche has lately been found in West Canada.—( Year Book of Facts, 1853, p. 223.) 9. Preservation of Vegetables—A cask provided with a door is three-fourths filled with sorrel, lettuce, endive, chicory (even if rancid), or asparagus; and a piece of rag steeped in sulphur, and attached to the end of a wire, is sét on fire and introduced through the door, the contamination of the vegetables, by the falling down of the burnt matter, being prevented by laying a board upon them ; the door is then closed, and the cask agitated to accelerate the absorption of the sulphurous acid. The sulphuring is twice more performed in the same manner, and the vegetables, together with the liquid which has oozed from them, are put into stoneware jars, which are then merely tied round with parchment and put into a cellar. Vegetables thus treated keep well till the April of the fol- lowing year. They do not, however, soften so quickly in water as fresh vegetables, and must therefore, before boiling, be soaked in cold water for some hours (asparagus in April for twenty-four hours). During the boiling, which generally does not last longer than with fresh vegetables, the sulphurous acid is given off. This method is applicable only to tender vegetables, which easily soften in boiling, —(Leopold Gmelin’s Hand-Book of Chemistry, vol. iii. of the Cavendish Society, p. 116.) 384 By the Patent Law Amendment Act of 1852 (15 and 16 Vict., cap. 83), it was provided, that Transcripts of all Patents should be transmitted to the Office of Director of Chancery in Scotland to be recorded, where they would be open to the inspection of the Public ; but that provision has never been complied with. And it is believed that there is a Bill now introduced into the House of Lords for the repeal of such a provision. | INDEX. Adie, Richard, Esq., Six’s self-registering thermometer improved by, 84. Africa, on the basin-like form of, by Sir R. I. Murchison, 52. Agassiz, Professor Louis, on the classification of insects from em- bryological data, 101. Anteater, Cape, account of, by W. T/ Black, i .» 168. Arabs, freedom from leprosy, 188. Arctic Natural History, 72. Australia, on the condition and prospects of the Aborigines of, by W. Westgarth, 36. Bailey, Professor J. W., on the microscopical soundings off the At- lantic Coast of the United States, 142. Bennett, Mrs Anne Ramsden, on meteorological phenomena in con- nection with the climate of Berlin, 155, 214. Bergmannite, pseudomorphous, an account of, by Professor J, R. Blum, 162, Berzelius, Biography of, by Professor H. Rose, 1. Black, W. T., assistant-surgeon, on the Anteater of the Cape, 168. Blum, Profossie J.R., on Gieseckite and Bergmannite, te. Buch, Leopold von, biographical notice of, 373. Christison, Dr Alexander, on the climate of Rangoon, 179. Dr Alexander, on a meteorological register kept at Ran- goon, 377. Chambers, Robert, Esq., on glacial phenomena in Scotland and parts of England, 229. Clausius, R., Esq., on the colours of a jet of steam, and of the at- _ mosphere, 166. Climate of Berlin, observations on, 214. Crawfurd, J. W., Esq., on the Negroes of the Indian Archipelago and Pacific Islands, 1°75. VOL. LIV, NO. CVIII.— APRIL 1853. 2D 386 Index. Corbett, Richard, Esq., on an earthquake felt at Adderley, 180. Crystallisation and Amorphism, 183. Denham, Captain H., on deep-sea soundings, 346. De la Rive, on the diurnal variations of the magnetic needle, 148. on the influence of terrestrial magnetism on iron, 206. Dinornis, bones and eggs of, 186. Donarium identical with Thorium, 188. Karthquake at Adderley, by Richard Corbett, Esq., 180. Eggs, preservation of, 382, Electricity applied to the capture of whales, 382. Filet, Charles, jun., on the application of reservoirs to the improve- ment of rivers, 118. Faroe Islands, noticed, 380. Fish, cod, of the Whale Fish Islands, 382. Fishes, domestication of, 187. Forbes, Professor Edward, on the geological distribution of marine animals, 311. Gieseckite, pseudomorphous, described by Professor J. R. Blum, 162, Glacial phenomena of Scotland, an account of, by R. Chambers, Esq., 229. Glaciers, extent of, in the Polar Regions, 879. Graphite, a large deposit of, in Glen Strath, Farer, Inverness-shire, and at St Johns, New Brunswick, 181. Guano birds of the Lobos Islands, 381. Henwood, John, Esq., on a remarkable deposit of tin ore at the Providence Mines, near St Ives, Cornwall, 68. Hisinger, M, Wilhelm, obituary of, 188. Horsford, Professor, on the solidification of the rocks of the Florida Reefs, and the sources of lime in the growth of éorals, 56. Horsford, Professor E. N., on the relation of the chemical constitu- tion of bodies to light, 294. on the effect of heat on the perpendicularity of Bunker Hill monument, 308. Humboldt, Alexander von, remarks on lectures on science to the people, by, 110. Indéx. 387 Insects, on the classification of, by Professor Louis Agassiz, Lai: Indigo, Dr Penny, on the valuation of, 285 Tron, native, 183. James, Captain, R.E., meteorological observations by, 282. Kjerulf, Theodor, on a variety of quartziferous trachyte, 367. Leprosy, Arabs exempt from, 188. ‘Macgillivray, the late Wijiam, Regius Professor of Natural History, Aberdeen, biographical account of, 189. Marchand, M. Eugene, on the analyses of snow and rain water, 179. Metereological observations, 144. Miller, John Fletcher, Esq., meteorological observations by, 46. Minerals, paragenetic relations of, 323. Murchison, Sir R. I., on the basin-like form of Africa, 52. Nasmyth, James, Esq., some remarks by, on the probable present condition of the planets Jupiter and Saturn, in reference to __ temperature, 341. Negroes of the Indian Archipelago, noticed by J. W. Crawfurd, 175. Nostoc, remarks on, 383. Obituary of Leopold von Buch, 369. Oken, Professor, on popular assemblies for the advancement of Science, 112. Ordnance Survey, astronomical observations on, 350. Patent law amendment act, 384. Penny; Dr Frederick, on the valuation of indigo, 285. Petermann, Augustus, Esq., on the distribution of animals available as food in the Arctic Regions, 295. Platinum and Iridosmine in California, 182. Rangoon, meteorological register of, 377. Reservoirs, application of, to the improvement of rivers, 118. Rocks, solidification of, in the Florida Reefs, and the sources of lime in the growth of corals, 56. Rose, Professor H., his biography of Berzelius, 1. Rowell, Mr G. A., on the change of temperature in Europe, and the variation of the magnetic needle, 312. a 388 Index. Scientific intelligence, 179, 379. Scoresby, the Rev. Dr, on the Earl of Rosse’s telescopes, 118, Silem, Professor, on pseudomorphous minerals, 181. Smith, Dr John Alexander, on animal remains found with Roman pottery, 122. Soundings, microscopical, off the Atlantic Coast of the United States, by J. W. Bailey, 142. Soundings, deep sea, in the Atlantic Ocean, by Captain Denham,346, Species, numerical list of, of animal kingdom, 380. Steam, colours of a jet of, by R. Clausius, 166. Stevenson, Thomas, Esq., on the gradual decrease of waters as they enter harbours, 378. Stratification, Wells on the origin of, 291. Strontiano-calcite, remarks on, 182. Sulphur Mine in Upper Egypt noticed, 182. Survey, Government geological, notes on the scales of, 362. Tertiary formation, flora of, described, 183. Tides, bed, and coasts of the North Sea or German Ocean, 185, Tin ore, deposit of, at the Providence Mines, Cornwall, 68. Thermometer, Six’s self-registering, improved by Richard Adie, Esq., 84. Thomson, Alexander, Esq., of Banchory, biographical account of the late Professor W. Macgillivray by, 189. the late Dr Thomas, biography of, 86. Trachyte, a quartziferous variety of, found in Iceland, deseribed, 367. Trevelyan, Sir Walter C. on the Faroe Islands, 380, Vegetables, preservation of, noticed, 383. Waves, Stevenson, T., Esq., on the reduction of the height of, 378. Wells, D. A., Esq., on the origin of stratification, Westgarth, w. , Esq., on the conditions and prospects of the wee rigines of Musiraisd 36. ERRATA 1 Vou. LN Wy er Page 84, throughout the article on Self-Registering Thermometter;-fo7 Sikes’ vead Six’s EDINBURGH: PRINTED BY NEILL AND COMPANY, OLD FISHMARKET. fe / tt He Oe ihe Z 4 " an} i iii ya fat Fa) P { Tiaoh ying: et yethabattes ian Hite 3 ayy i : ' (or A | vit, f ; a AS fue eal Hey iret haley tee ir {i { , sesh ity Lae we if ntact matitany he) an tee shyt Ha NL i Pabst ton j : deel) mt Eve to Spat! vee oe! gern aspl et fal Pos )2) ? Ue pdry lle tat if eae ray Ut ett ia fez, ‘lade ge