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‎"CAYLEY, ARTHUR. - THE THEORY OF FORMS (QUANTICS) - A NEW ASPECT OF NON-EUCLIDEAN GEOMETRY.‎

‎A Sixth Memoir upon Quantics. Received November 18, 1858, - Read anuary 6, 1859.‎

‎(London, Richard Taylor and William Francis, 1859). 4to. No wrappers as extracted from ""Philosophical Transactions"" Vol. 149 - Part I. Pp. 61-90. Clean and fine.‎

‎First appearance of this pathbreaking paper in which Cayley unites 'Metrical Geometry' and 'Projectice Geometry' by introducing ""imaginary"" elements to metrical properties.""The fundamental notions in metrical geometry are the distance between two points and the angle between two lines. Replacing the concept of distance by another, also involving ""imaginary"" elements, Cayley provided the means for unifying Euclideangeometry and the common non-Euclidean gemoetries into one comprehensive theory.""(Bell in ""Men of Mathematics"").In non-Euclidean geometry prepared the way for Klein's splendid discovery that the geometry of Euclid and the non-Euclidean geometries of Lobatchewsky and Riemann are, all threee, merely different aspects of a more general kind of geometry which includes them as special cases..Dealing with the relations between metrical and projective geometry Klein remarks (In ""Entwicklung der Mathematik"", Teil I p. 148): ""Vor allem kommt für uns sein (Cayley's) berühmtes 'A Sixth Memoir upon Quantics"" im betrachtt. Quantioc heisst soviwel ""Form"", d.h. homogenes Polynom von zwei, drei oder mehr Variablen, wonach man binäre, tertiäre usw. Formen unterscheidet...""‎

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‎"ANDREWS, THOMAS. - THE ""CRITICAL TEMPERATURE"" OF GASES.‎

‎The Bakerian Lecture. - On the Continuity of the Gaseous and Liquid States of Matter. Received June 14, - Read June 17, 1869.‎

‎(London, Taylor and Francis, 1870). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1869 - Vol. 159 - Part II. Pp. 575-590 and 1 plate. Clean and fine.‎

‎First apperance of the paper in which Thomas Andrews announces his discovery of the ""CRITICAL POINT"", which states that for every gas there was a temperature above which pressure alone could not liquefy it.""This was a crucial discovery for it pointed the way toward the liquefaction of the permanent gases by demonstrating the necessity of dropping the temperature below the critical point before exerting pressure. This new view led within half a century to the work of Dewar and Kammerlingh-Onnes and the liquefaction of all known gases.""(Asimov).Magie: A Source Book in Physics, pp. 187-192. - Parkinson, Breakthroughs: 1869 C.‎

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‎HERSCHEL, WILLIAM. - INDICATION OF THE UNIVERSALITY OF NEWTON'S LAWS OF MOTION.‎

‎Account of the Changes that have happened, during the last Twenty-five Years, in the relative Situation of Double-stars" with an Investigation of the Cause to which they are owing. Read June 9, 1803.‎

‎(London, Bulwer and Co., 1803). 4to. Without wrappers as extracted from ""Philosophical Transactions of the Royal Society of London."" Year 1803-Part II. Pp. 339-382 and 2 engraved plates.‎

‎First appearance of a fundamental paper in cosmology and physics as it contains the first observational data to support that Newton's dynamical laws holds outside the solar system. Herschel shows here that the circulating motions of double-stars were under gravitational forces. Until then the validity of the law of gravity was only established within the solar system. Now, a century after the establishment of the law, it was traced out in the motion of incredibly distant stars and the theory first truly earned its title of Universal. The exact proof of the mutual gravitation of the double-stars was only obtained five years after Herschel's death, when the motions of the stars were more precisely dtermined.One of the most notable of Herschel's discoveries of double-stars, binary stars. A first cataloque of such pairs was published early in 1782 and contained 269, of which 227 were new discoveries. ""Twenty years after the publication of his first cataloque Herschel was of Michell's opinion - Michell had expressed the opinion that the odds in favour of a physical relation between the members of herschel's newly discovered double stars were ""beyond arithmetic"" - but was able to support it by evidence of an entirely novel and much more direct character. A series of observations of Castor, presented in two papers in the ""Philosophical Transaction"" in 1803 (the paper offered here) and 1804, which were fortunately supplemented by an observation of Bradley's in 1759, had shewn a progressive alteration in the direction of the line joining its two components, of such a character as to leave no doubt that the two stars were revolving round one another"" and there were five oher cases in which a similar motion was observed...it was shown that the double-star was really formed by a connected pair of stars near enough to influence one another's mortion.""(Berry in ""A Short History of Astronomy"" pp. 342-43).‎

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‎HAMILTON, WILLIAM ROWAN. - THE GENERAL PRINCIPLE OF LEAST ACTION - HAMILTON' S PRINCIPLE.‎

‎On a general Method in Dynamics" by which the Study of the Motions of all free Systems of attracting or repelling Points is reduced to the Search and Differentiation of one central Relation, or characteristic Function. Received April 1, - Read April 1...‎

‎London, Richard Taylor, 1834-35. 4to. No wrappers as extracted from ""Philosophical Transactions"" 1834 - Part II. and 1835 - Part I. Both titlepages to the volumes present.Pp. (2),247-308 a. (2),95-144. Both papers clean and fine.‎

‎First appearance of these two groundbreaking papers in which Hamilton carries further the dynamics of Lagrange by expressing the kinetic energy in terms of the momenta and the co-ordinates of a system, and discovers how to transform the Lagrangian equations into a set of differential equations of the first order for the determination of of the motion. The Hamilton principle is also called The Principle of ""Least Action"". The Hamilton Principle as stated in the papers offered here ""was the first of his two great ""discoveries"". he second was the quaternions, which he discovered...1843 nd towhich he devoted most of his efforts during the remaining 22 years of his life.""(DSB).Maupertouis, Euler, and Lagrange introduced the principle of ""Least Action"" covering the science of dynamics, and now Hamilton brought the principle into a form which was capable of expressing all the laws of Newtonian science in a representation as minimum-problems, that is, all gravitational, dynamical and electrical laws could be represented as minimum problems. In 1925 Heisenberg, Born and Jordan showed, that the Hamilton equations are still valid in quantum theoryAlthough formulated originally for classical mechanics, Hamilton's principle also applies to classical fields such as the electromagnetic and gravitational fields, and has even been extended to quantum mechanics, quantum field theory, relativity and criticality theories. Its influence is so profound and far reaching that many scientists regard it as the most powerful single principle in mathematocal physics and place it at the pinnacle of physical science.‎

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‎"MUDGE, WILLIAM. - FIRST MEASUREMENT OF AN ARC OF THE MERIDIAN IN ENGLAND.‎

‎An Account of the Measurement of an Arc of the Meridian, extending from Dunnose, in the Isle of Wright, Latitude ....,to Clifton in Yorkshire, Latitude.., in the coursee of the Opertions carried on foor the Trigonometrical Survey of England, in the ye...‎

‎(London, W. Bulmer and Co., 1803). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1803 - Part II. Pp. 383-508 and 8 engraved plates (3 folio size and folded, 1 map), depicting the apparatus for measuring.‎

‎First appearance of an importent paper, which contributed to the discussion of the dimension of the earth. William Mudge was appointed in 1791 to the ordnance trigonometrical survey, and became superintendent of the survey in 1798 and in that same year was also elected as a Fellow of the Royal Society. Shortly afterwards, he completed the first ever measurement of an arc of meridian stretching from Dunnose on the Isle of Wight to Clifton in Yorkshire. This was regarded as a very considerable advance in the scientific work of what had by then become the Ordnance Survey and contributed significantly to the international debate about the precise figure of the earth.‎

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‎DAVY, HUMPHRY. - ISOLATION OF BARIUM, MAGNESIUM, CALCIUM AND STRONTIUM FOR THE FIRST TIME.‎

‎Electro-Chemical Researches, on the Decomposition of the Earth" with Observations on the Metals obtained from the alkaline Earths, and on the Amalgam procured from Ammonia. Read June 30th, 1808.‎

‎(London, W. Bulmer and Co., 1808). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1808 - Part I. Pp. 333-370. Clean and fine.‎

‎First printing of a historical paper in chemistry, his third Bakerian Lecture, in which he obtained for the first time, by means of electrolysis, the metals barium, magnesium, calcium and strontium. He further utilized the strong reducing power of potassium to prepare boron.""Humphry Davy was one of the most brilliant chemists of the early nineteenth century. His early study of nitrous oxide brought him his first reputation, but his later and most importent investigations were devoted to electrochemistry. Following Galvani's experiments and the discovery of the voltaic pile, interest in galvanic electricity had become widespread. The first electrolysis by means of the pile was carried out in 1800 by Nicholson and Carisle, who obtained oxygen and hydrogen from water. Davy began to examine the chemical effects of electricity in 1800, and his numerous discoveries were presented in his Bakerian lectures."" - Not in Wheeler Gift. - The Ronalds Library p. 128.‎

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‎"DANIELL, J. FREDERIC. - THE DANIELL-CELL.‎

‎Further Obervations on Voltaic Combinations. In a Letter addressed to Michael Faraday. Received March 30, - Read April 6, 1837.‎

‎(London, Richard and John E. Taylor, 1837). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1837 - Part I. Pp. 141-160 and 1 engraved plate.‎

‎First appearance of Daniell's second paper on the construction of the famous ""Daniell-Cell"". In 1836 (in a paper in the Transactions, also addressed to Faraday with the title ""On Voltaic Combinations""), he announced his invention of the battery. In his second paper, the paper offered here, he further develops his invention. In the new invention by Charles Wheatstone of the electric telegraph in 1837, the Daniell cell was used as the electric source.In 1831 Daniell was appointed proffesor of Chemistry at King's College London. He invented several scientific instruments, including a hygrometer for measuring humidity he is best known for his work in electrochemistry, his interests having been aroused by the work of his good friend faraday. Volta's battery had the defect of rapid diminution in current. What was needed, however, was a battery yielding a constant current over a considerable lenght of time. In 1836 Daniell succeeded, producing the Daniell cell, of copper and zinc. his was the first reliable source of electric current.‎

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‎"RUTHERFORD, ERNST. - THE MAGNETIC DETECTOR INVENTED - WIRELESS TELEGRAPHY MADE POSSIBLE.‎

‎The Magnetic Detector of Electrical Waves and some of its Applications. Communicated by J.J. Thomson. Received June 11, - Read June 18, 1896.‎

‎(London, Harrison and Sons, 1897). 4to. No wrappers as extracted from ""Philosophical Transactions"" Year 1897, Vol. 189 - A. Pp. 1-24., texfigs.‎

‎First appearance of this importent paper, the first paper by Rutherford published in England, in which he describes his invention of the ""Magnetic detector"" before Marconi made use of it in his wireless telegraphy across the Atlantic in 1901.On his arrival at Cambridge (in 1895) his talents were quickly recognized by Professor Thomson. During his first spell at the Cavendish Laboratory, he invented the detector for electromagnetic waves, an essential feature being an ingenious magnetizing coil containing tiny bundles of magnetized iron wire. The detector made it possible to send wireless signals.‎

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‎HERSCHEL, WILLIAM. - THE SUN AN INHABITED GLOBE.‎

‎Observations tending to investigate the Nature of the Sun, in order to find the Causes or Symptoms of its variable Emission of Light and Heat" with Remarks on the Use that may possibly be drawn from Solar Observations. Read April 16, 1801.‎

‎(London, W. Bulmer and Co., 1801). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1801 - Part I. Pp. 265-318 and 2 folded engraved plates. Wide-margined. A few small marginal brownspots.‎

‎First appearance of an remarkable paper containing an extensive set of observations on the sunspots intermingled with what Herschel called ""ideas that obtruded themselves"" at the time of observation.""Herschel's interest in the sun was naturally stimulated by the realization that, of all the stars, it alone is close enough for detailled examination. he was aware of the various existing theories of the physical constitution of the sun. In a long paper published in 1795 he mentions some of them before his own observations...In 1801, in a second long paper (the paper offered here) in which he arranged his observations according to relevant physical questions, he modified his earlier account of the sun to include in its constitution an interior layer of dark clouds not unlike our own, this layer serving to shield the solar inhabitants from the exterior, luminous layer.‎

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‎"HERSCHEL, WILLIAM. - THE BASIS OF INTERFEROMETRIC IMAGING IN ASTRONOMY.‎

‎Experiments for ascertaining how far Telescopes will enable us to determine very small Angles, and to distinguish the real from the spurious Diameters of celestial and terrestrial Objects: with an Application of the Result ofthese Experiments to a ser...‎

‎(London, W. Bulmer and Co., 1805). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1805 - Part I. Pp. 31-64 and 1 engraved plate. Clean and fine.‎

‎First appearance of an importent paper, founding the metric of interstellar space.It was the contemporous discoveries of the first minor planets, ceres in 1801, Pallas in 1802 and Juno in 1803, that prompted Herschel to investigate the origin of the spurious diameters of stars. ""Were their apparent diameters as real as those of planets or spurious as for stars? To address this question Herschel conducted an extensive series of experiments in his garden in Slough, examining through his telescope small globules of differing sizes and materials placed in a tree some 800 ft (ca. 244 m) away (Herschel 1805). His observations showed that for the smallest globules the diameters were all spurious and all of the same size. Furthermore, he found that, if just the inner part of the aperture of the telescope were used, the spurious diameters, whether of globules or of stars, were larger. If the whole aperture was employed, the diameters were smaller, and if only an outer annular aperture was used the diameters were smaller still. This experimental discovery that unfilled apertures can be used to obtain high angular resolution remains today the essential basis for interferometric imaging in astronomy (in particular Aperture Masking Interferometry). The theoretical justification of this result came with Airy's analysis of the diffraction pattern of a circular aperture 30 years later (Airy 1835), and it took a further 30 years before the idea of using multiple apertures was developed. In an early study the Reverend W. R. Dawes noted that he had frequently found great advantage from the use of a perforated whole aperture' and that when observing Venus this produced a central image of the planet perfectly colourless, and very sharply dened' (Dawes 1866). But it was left to Fizeau, in his submission to the Commission for the Prix Bordin the following year, to remark on une relation remarquable et n´ecessaire entre la dimension des franges et celle de la source lumineuse' and suggest that by using an interferometric combination of light from two separated slits il deviendra possible d'obtenir quelques donn´ees nouvelles sur les diametres angulaires de ces astres' (Fizeau 1868).""‎

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‎"DARWIN, G.H. - A PIONEERING WORK IN COSMOLOGY BY THE ""FATHER OF GEOPHYSICS""‎

‎On the Secular Changes in the Elements of the Orbit of a Satellite revolving about a Tidally distorted Planet. Received December 8, - Read December 18, 1879.‎

‎(London, Harrison and Sons, 1880). 4to. No wrappers as extracted from ""Philosophical Transactions"", Vol. 171 - Part II. Pp. 713-891. A few textilustr. Clean and fine.‎

‎First printing of a main work by the ""Father of Geophysics"", in which he set up the hypothesis, that the results from his earlier investigations on the relations between the tidal frictions on the earth and the motion of the moon away from the earth, could be used to explain the formation of satellites of the other planets and their movements in relation to the sun.. (In DSB it is called ""a monumental paper"").""Darwin's most significant contribution to the history of science lies in his pioneering work in the application of detailled dynamical analysis to cosmological and geological problems. That many of his conclusions are now out of date should in no way diminish the historical interest in his experiments, nor the importent service thet he rendered cosmogony by the example he gave of putting various hypotheses to the test of actual calculations. Darwin's method remains a milestone in the development of cosmogony, and subsequent investigators have favored it over the merely qualitative arguments prevalent until that time.""(DSB).‎

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‎"DARWIN, G.H. - THE MOON THEORY.‎

‎Problems connected with the Tides of a Viscous Spheroid. Received November 14, - Read December 19, 1878.‎

‎(London, Harrison and Sons, 1880). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1879, Vol. 171 - Part II. Pp. 539-593.‎

‎First printing of a main paper by the ""Father of Geophysics"" in which he shows that the effect of the tides was to force a retreat of the moon from the earth - thus going backward in time in the history of the earth, he concludes that the earth had been in contact with the moon, and this represents the time at which the whirling earth threw off a portion of its outer crust by centrifugal action, loosing angular motion in that way.""Darwin's most significant contribution to the history of science lies in his pioneering work in the application of detailled dynamical analysis to cosmological and geological problems. That many of his conclusions are now out of date should in no way diminish the historical interest in his experiments, nor the importent service thet he rendered cosmogony by the example he gave of putting various hypotheses to the test of actual calculations. Darwin's method remains a milestone in the development of cosmogony, and subsequent investigators have favored it over the merely qualitative arguments prevalent until that time.""(DSB).‎

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‎"CROOKES, WILLIAM. - THE FOURTH STATE OF MATTER.‎

‎The Bakerian Lecture. - On Radiant Matter Spectroscopy: The Detection and wide Distributium of Yttrium. Received May 24, - Read May 11, 1883. (+) On Radiant Matter Spectroscopy.- Part II. Samarium. Received May 21, - Read June 18, 1885. (2 Papers).‎

‎(London, Harrison and Sons, 1884 a. 1886). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1883. Vol. 179 - Part II. Pp. 891-918 and 1885. Vol. 176 - Part II. Pp. 691-723 and 1 plate (chromolithographed spectra), many textillustr. of spectra. The plate with small spots in margins.‎

‎First appearance of these papers in which Crooles continues his cathode rays experiments with his Crookes tube, obtaining spectra of elements which he regarded as new. His experiments lead him here to his speculative theory of the elements having a common ancestor, a primordial matter.Sir William Crookes (1832-1919) studied at the Royal College of Chemistry , London, and served there as an assistant to Hoffmann. In 1859 he founded the Chemical News and remained its proprietor and editor until his death. he early attracted attentuion by his discovery of the element thallium by spectroscopic methods. he was an active investigator in many fields of physics and contributed greatly to the advance of knowledge by his study of the radiometer and of the electric discharge in rarefied gases.‎

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‎"LOCKYER, JOSEPH NORMAN - THE DISCOVERY OF HELIUM.‎

‎Spectroscopic Observations of the Sun.- No. II. Received November 19,- Read November 19 and 26, 1868. (With additional notes Nov. 26, April 9, 1869, Oct. 10, 1869).‎

‎(London, Taylor and Sons, 1870). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1869, Vol. 159 - Part I. Pp. 425-444 and 2 lithographed plates (1 with the spectrum of helium, 1 with his spectroscope (not requiring eclipses to function)). Clean and fine.‎

‎First appearance of this milestone paper in chemistry, physics and astronomy, announcing the discovery of helium in the sun and naming it 'helium' for Helios, the Greek God of the Sun. In the same paper he demonstrates his invention of the spectroscope by which the prominences of the sun could be observed and studied without an eclipse by leading the light from the very edge of the sun through a prism. - Helium was not discovered on the earth before 1895 by William Ramsay, and it was Crookes who established its identity with the helium Lockyer observed in the spectrum of the sun.""This (the last discovery) was announced on the same day by the French astronomer Janssen, who was in India observing a total eclipse. As a result, the French government some ten years later struck a medallion showing the heads of both scientists.By that time, the two men had made a much more dramatic discovery at the same time, this time in cooperation. Janssen, studying the spectrum ofthe sun during the eclipse, had noted a fine line he did not recognize. he send a report on this to Lockyer, an acknowledges expert on solar spectra. Lockyer compared the reported position of the line with lines of known elements, concluding that it must belong to a yeat unknown element, possibly not even existing on the earth. He named the element, from the Greek word for the sun.""(Asimov).‎

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‎"DARWIN, G.H. - ANNOUNCING THE ""RESONANCE THEORY"" OF THE ORIGIN OF THE MOON.‎

‎On the Procession of a Viscous Spheroid, and on the remote History of the Earth. Received July 22, - Read December 19, 1878.‎

‎(London, Harrison and Sons, 1880). 4to. No wrappers as extracted from ""Philosophical Transactions"", 1879, Vol. 170 - Part II. Pp. 447-538 and. 1 plate. Clean and fine.‎

‎First appearance of an importent paper, announcing Darwin's so-called ""Resonance Theory"" of the origin of the moon, according to which the moon might have originated from the fission of a parent earth as the result of an instability produced by resonant solar tides.""Darwin's most significant contribution to the history of science lies in his pioneering work in the application of detailled dynamical analysis to cosmological and geological problems. That many of his conclusions are now out of date should in no way diminish the historical interest in his experiments, nor the importent service thet he rendered cosmogony by the example he gave of putting various hypotheses to the test of actual calculations. Darwin's method remains a milestone in the development of cosmogony, and subsequent investigators have favored it over the merely qualitative arguments prevalent until that time.""(DSB).‎

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‎"WHEATSTONE, CHARLES. - THE WHEATSTONE BRIDGE.‎

‎The Bakerian Lecture, - An Account of several new Instruments and Processes for determining the Constants of a Voltaic Circuit. Received June 15, - Read June 15, 1843.‎

‎(London, Richard and John E. Taylor, 1843). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1843 - Part II. Pp. 303-327 and 2 lithographed plates.‎

‎Frst appearance of an importent paper in the history of electricity. ""In 1843 Wheatstone published an experimental verification of Ohm's law, helping to make the law (already well known in Germany) more familiar in England. In connection with the verification he developed new ways of measuring resistances and currents. In particular, he invented the rheostat and popularized the Wheatstone bridge (in the paper offered), originally invented by Samuel Christie.""(DSB).‎

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‎(BERNOULLI, JEAN (JOHANN) & BERNOULLI, DANIEL. - THE MECHANICS OF THE HEAVENS.‎

‎Essai d'une nouvelle Physique celeste. Servant à expliquer les principaux Phenomenes du Ciel, & en particulier la cause physique de l'inclinaison des Orbites des Planetes par rapport au plan de l'Equateur du Soleil. Qui a partagé le Prix doub...‎

‎Paris, Imprimerie Royale, 1735. 4to. Fine recent marbled boards. Printed titlelabel on frontcover. (6),144 pp. and 1 double-page folded engraved plate. Johann B's paper: pp. (1-) 91. - Daniel B's papers: pp. (93-) 122 and pp. 123-144. A few marginal brownspots.‎

‎First edition of these prize winning papers by father (Jean) and son (Daniel). - Both papers deals with the cause of the inclination of the planetary orbits relative to the solar equator. - In Daniel's paper he put foreward the hypothesis of the existence of an atmosphere, resempling air, and rotating around the solar axis, resulting in an increasing inclination of the planetary orbits toward the equator of the sun. Daniel was the first importent Newtonian outside Great Britain. The problems faced here (by Daniel) are treated in Newtonian manner.The publication of these papers by father and son resulted in a controversy between the two, forcing Daniel to leave his fathers house. - Poggendorff I:161.‎

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‎"WOLLASTON, WILLIAM HYDE. - THE DISCOVERY OF THE ELEMENT RHODIUM.‎

‎On a new Metal, found in crude Platina. Read June 24, 1804.‎

‎(London, Bulwer and Co., 1804). 4to. Without wrappers as extracted from ""Philosophical Transactions of the Royal Society of London."" Year 1804-Part II. Pp. 419-430. Clean and fine.‎

‎First appearance of the paper in which Wollaston announced his discovery of the metallic element Rhodium.""Dr. Wollaston dissolved a portion of crude platinum in qgua regia, and neutralized the excess acid with caustic soda. He then added salammoniac to precipitate the platinum as ammonium chloroplatinate, and mercurous cyanide to precipitate the palladium as palladium cyanide. After filteringoff the precipitate, he decomposed the excess mercurous cyanide inthe filtarate by adding hydrochloric acid and evaporating to dryness. When he washed the residue with alcohol, everything dissolved except a beautiful dark red powder, which proved to be a double chloride of sodium and a new metal, which because of the rose color of its salts, Dr. Wollaston named 'Rhodium'. He found that the sodium rhodium chloride could be easely reduced by heating it in a current of hydrogen, and that after the sodium chloride had been washed out, the rhodium remained as a metallic powder. he also succeeded in obtaining a rhodium button.""(Weeks: Discovery of the Elements. p. 104-05.)‎

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‎"OWEN, RICHARD. - ESTABLISHING THE GENUS NESODON.‎

‎Description of some Species of the extinct Genus Nesodon, with remarks on the primary Group (Toxodontia) of Hoofed Quadrupeds, to which that Genus is referable.‎

‎(London, Richard Taylor and William Francis, 1853) 4to. No wrappers as extracted from ""Philosophical Transactions"" 1853, Vol. 143 - Part I. Pp. 291-310 and 4 lithographed plates.‎

‎First appearance of this importent paper, in which Owen established a new genus, Nesodons on the basis of the fossils found by B.J. Sulivan in the Tertiary beds of Patagonia in 1845.‎

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201,45 € Acheter

‎"CROOKES, WILLIAM. - ARGON - THE FIRST OF THE INERT GASES.‎

‎On the Spectra of Argon. Received January 26, - Read January 31, 1895.‎

‎(London, Harrison and Sons, 1895). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1895 - Vol. 186 - Series A, Part I. Pp. 243-251 and 1 plate (The Spectra of Argon). Clean and fine.‎

‎First appearance of a classic paper in which Crookes by his spectrographic methods confirms the discovery of argon by Ramsey and Rayleigh in 1895. The plate is the first to show the spectra of argon, the first of the inert gases to be discovered.The paper first describes the spectra obtained by passing an electric discharge through argon at very low pressures,. Several specimens of argon (some containing traces of nitrogen) were invested. Crookes distinguished between the spectral lines attributable to argon and those of nitrogen and verified that the argon isolated by Lord rayleigh and William Ramsay was truly a new chemically inert element. (Neville I:p. 313).Sir William Crookes (1832-1919) studied at the Royal College of Chemistry , London, and served there as an assistant to Hoffmann. In 1859 he founded the Chemical News and remained its proprietor and editor until his death. he early attracted attentuion by his discovery of the element thallium by spectroscopic methods. he was an active investigator in many fields of physics and contributed greatly to the advance of knowledge by his study of the radiometer and of the electric discharge in rarefied gases. -(PMM: 386 describing J.J. Thomson's Cathode Rays). - Magee, Source Book in Physics p. 564 ff.‎

Référence libraire : 42531

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‎"HENRY, WILLIAM. - A CRUCIAL STEP TOWARDS THE ATOMIC THEORY - HENRY'S LAW.‎

‎Experiments on the Quantity of Gases absorbed by Water, at different Temperatures, and under different Pressures. Read December 23, 1802. (and) Appendix to Mr. William henry's Paper, on the Quality of Gases absorbed by Water, at different Temperature...‎

‎(London, W. Bulmer and Co., 1803). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1803 - Part I. Pp.29-42 and 1 engraved plate and Appendix: pp. 274-276. With titlepage to the volume Part I. A paperflaw in margin of the first leaf, neathly repaired, no loss. The plate with a few small brownspots. Verso of titlepage with a small stamp, otherwise clean and fine, wide-margined.‎

‎First appearance of this highly importent paper in which Henry announced his discovery of the law, which later was termed ""Henry's Law"". The law states that when a gas is absorbed in a liquid the weight of the gas dissolved is directly proportional to the pressure of the gas over the liquid. This discovery contributed directly to the atomic theory of Dalton.(Parkinson: Breakthroughs: 1803 C) ""Dalton's own experiments on the solution of gases and the stimulus afforded by Henry's work have been seen as crucial in the development of the atomic theory.""(DSB VI p. 285).A paper by Humphrey Davy: ""An Accont of some Experiemnts and Observations on the constituent Parts of certain astringent Vegetables"" and on their Operating in Tanning. Read February 24, 1803"", comes with. In the same volume Pp. 233-273.‎

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738,65 € Acheter

‎"STOKES, G.G. - COINING THE WORD 'FLUORESCENCE'‎

‎On the Change of Refrangibility of Light. (No. I). Received May 11, - Read May 27, 1852. (+) On the Change of Refrangibility of Light.- No. II. Received June 16, - Read June 26, 1853. (2 Papers).‎

‎(London, Richard Taylor and William Francis, 1852 and 1853). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1852 - Part II. Pp. 463-562 a. 1853 - Vol. 143. Part III. Pp. 385-396. Clean and fine.‎

‎First appearance of two importent papers in the physical theories of light and the atomic structure.""Sir John Herschel first noticed that sulpahte of quinine shows a blue colour when light is incident on it under certain circumstances"" later it was found that many other substances, if placed in a dark room and exposed to invisible radiations beyond the viloet end of the visible spectrum, emit a bluish or greenish light. To this phenomenon the name 'flourencence' was given by Stoken in 1852 (the paper offered), in a famous paper disclosing its true nature.""(Whittaker in ""A History of the Theores of Aether and Electricity"" Vol. I.p. 262).""However, long before the discovery of the electron made the compositeness of atoms explicit, the clearest signals that structure was called for came from spectra. Already in 1852, Stokes, in the importent memoir ""On the Change of Refrangibility of Ligh"" (to which Kelvin referred) had written. ""In all probability...the molecular vibrations by which...light is produced are not vibrations i which the molecules move among one another, but vibrations aming the constituent parts of the molecules themselves, performed by virtue of the internal forces which hold the parts of molecules together"". Please notice...at that time, the term 'molecule' often meant what we call 'atom'.""(Pais in""Inward Bound"", p. 175).‎

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‎DALTON, JOHN. - ON THE CONSTITUTION OF THE ATMOSPHERE.‎

‎Sequel to an Essay on the Constitution of the Atmosphere in the Philosophical Transactions for 1826" with some Account of the Sulphurets of Lime. Received June 9, - Read June 15, 1837.‎

‎(London, Richard and John E. Taylor, 1837). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1837 - Part II. Pp. 347-363. Clean and fine.‎

‎First printing of Dalton's last paper submitted to the ""Transactions"". This paper, one of his last, deals with the constitution of the atmosphere, just as his first love was meteorology.""In an essay of mine on the constitution of the atmosphere, which was printed in the Transactions for 1826, I signified my intention of following it with a sequel of experiments to ascertain if possible which of the two views therein developed was most counntenanced by facts. I now proceed to give an account of such investigations relating to this subject as havee engaged my attention during a long period of years.""(John Dalton). - (Smith: John Dalton. A Bibliography. No. 78).‎

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201,45 € Acheter

‎"LABAT, R.P. - FROM THE LIBRARY OF A.G. MOLTKE.‎

‎Nouveau Voyage aux Isles de l'Amerique, contenant l'Histoire naturelle de ces Pays, l'Origine, les Moeurs, la Religion & la Gouvernement des Habitans anciens & moderne. Nouvelle Edition...enrichie des Figures en Taille-douce. Tome Sixieme (seul).‎

‎Paris, Theodore Le Gras, 1742. Small 8vo. Contemporary full calf. Spine and covers worn. From the library of Count A.G. Moltke with his large gilt coat of arms on both covers. (4),502 pp. Large fold. engraved plate (plan du Connvent artinique), 1 fold. Plan du Port, du Fort et du Bourg Grenade. plan du Fort, Grenade, 2 maps (L'isle de saint Christophle, L'isle de la Barbade, 1 folded plate showing natives preparing tobacco leaves, 5 botanical plates (2 with cacao), 3 zoological plates. Internally fine, some light yellowing to margins.‎

‎This volume describes the isles Martinique, Guadeloupe, Barbade (Barbados) and Grenade (Grenada).""A very pleasant and instructive work in many respects""(Chalmers) - ""The most copious that we possess on the Antilles"" very full on the Natural history and productions of the islands."" (Sabin: 38412).‎

Référence libraire : 42613

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241,74 € Acheter

‎"LABAT, R.P. - FROM THE LIBRARY OF A.G. MOLTKE.‎

‎Nouveau Voyage aux Isles de l'Amerique, contenant l'Histoire naturelle de ces Pays, l'Origine, les Moeurs, la Religion & la Gouvernement des Habitans anciens & moderne. Nouvelle Edition...enrichie des Figures en Taille-douce. Tome Troisieme (seul).‎

‎Paris, Theodore Le Gras, 1742. Small 8vo. Contemporary full calf. Spine and covers worn. From the library of Count A.G. Moltke with his large gilt coat of arms on both covers. (6),475 pp. With 30 engraved plates. (5 zoological plates, 19 botanical plates, 6 arts & crafts: Moulin a Sucre, folding, Moulin a Vent , folding, Camble de Moulin, folding, Moulin Rond, folding, Moulin a Eau droit, folding, Moulin a Eau couché, folding). Internally fine with only light yellowing to margins.‎

‎This volume describes the islands Guadeloupe, Martinique, Isles des Saintes.""A very pleasant and instructive work in many respects""(Chalmers) - ""The most copious that we possess on the Antilles"" very full on the Natural history and productions of the islands."" (Sabin: 38412).‎

Référence libraire : 42615

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‎"WILSON, C.T.R. - THE INVENTION OF THE WILSON ""CLOUD CHAMBER""‎

‎Condensation of Water Vapour in the Presence of Dust-free Air and other Gases. Communicated by J.J. Thomson. Received March 15, - Read April 8, 1897.‎

‎(London, Harrison and Sons, 1897). 4to. No wrappers as extracted from ""Philosophical Transactions"" Year 1897, Volume 189 - Series A. - Pp. 265-307. Clean fine. Textillustrations, depicting Wilson's famous apparatus‎

‎First printing of this groundbreaking paper in which Wilson describes the invention which made it possible to view the track of a single atomic projectile or electron. The invenvention of the ""Dust-Chamber"" made it possible for J.J. Thomson in 1897 to calculate the charge of the electron, and thereby finding its mass, since the ratio between the two was known. In most cases it was found that the track of the particle is a straight, or nearly straight line.""C.T.R. Wilson had been developing his cloud-chamber, which was to provide the most powerfull of all methods of investigation in atomic physics. In moist air, if a certain degree of supersaturation is exceeded this can be secured by a sudden expansion of the air) condensation takes place on dust-nuclei, when any are present: if by preliminary operations condensation is made to take place on the dust-nuclei, and the resulting droplets are allowed to settle, the air in the chamber is thereby freed from dust. If now X-rays or radiation from a radioactive substance are passed into the chamber, and if the degree of supersaturation is sufficient, condensation again takes place: this is due to the production of ions by the radiation. Thus the tracks of ionising radiations can be made visible by the sudden expansion of a moist gas, each ion becoming the centre of a visible globule of water. Wilson showed that the ions produced by uranium radiation were identical with those produced by X-rays."" (Whittaker in ""A History of the Theories of Aether & Electricity"" II:p.4).‎

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‎"IVORY, JAMES. - THE INTRODUCTION OF IVORY'S THEOREM.‎

‎On the Attraction of homogenous Ellipsoides. Read June 15, 1809.‎

‎(London, W. Bulmer and Co., 1809). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1809 - Part II. Pp. 345-372. Clean and fine.‎

‎First printing this importent paper in which Ivory introduces his well-known theorem which bears his name. It states that the attraction of an ellipsoid upon a point exterior to it is dependent upon the attraction of another ellipsoid upon a point interior to it.""In 1809 J. Ivory proved the three-dimensional version of this theorem by straightforward calculation and by using an appropriate parametrization. This theorem holds in the n-dimensional Euclidean space (n > 1). It has been shown that it is also true in the pseudo-Euclidean plane (Minkowski)"" (H. Stachel).""Ivory's scientific reputation, for which he was awarded many honours during his lifetime, including knighthood of the Order of the Guelphs, Civil Division (1831), was founded on the ability to understand and comment the work of the French analysts rather than any great originality of his own...Ivory's work, conducted with great industry over a long period, helped to foster in England a new interest in the application of analysis to physical problems."" (DSB VII. p. 37).‎

Référence libraire : 42620

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248,45 € Acheter

‎"HOME, EVERARD. - THE TUSKS OF THE NARWHALE.‎

‎On the Tusks of the Narwhale. Read february 18, 1813.‎

‎(London, W. Bulmer and Co., 1813). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1813 - Part I. Pp. 126-130 and 1 engraved plate.‎

‎First printing of this paper in which Home describes a female skull of the Narwhale given to him by Mr. Scoresby. The plate is a drawing of this skull.‎

Référence libraire : 42625

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‎"THOMSON, THOMAS & WILLIAM HYDE WOLLASTON. - THE LAW OF MULTIPLE PROPORTIONS CONFIRMED - THE FOUNDATIONS OF ATOMIC THEORY.‎

‎On Oxalic Acid. Read January 14th, 1808. (Thomson) (+) On Super-acid and Sub-acid Salts. Read January 28, 1808. (Wollaston). 2 Papers.‎

‎(London, W. Bulmer and Co., 1808). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1808 - Part I. Pp. 63-95 (Thomson) and pp. 96-102 (Wollaston:). Clean and fine.‎

‎First appearance of these two historical papers in chemistry in which Thomson and Wollaston, independently, presents experimental proofs of John Dalton's ""Law of Multiple Proportions"", and thereby laying the foundations of the Atomic Theory. - These demonstrations went far to influence chemists favorably toward Dalton's atomic theory. ""In January 1808 Thomson was the first to submit an experimental illustration of the law of multiple proportions, doing so at least four months before the publication of Dalton's ""New System of Chemistry Philosophy"" (1808). This paper, ""On Oxalic Acid"" also established a usefull method of determining empirical formulas.""(DSB XIII, p. 373).""This paper is also importent as he here introduces quantified chemical symbolism for compounds, a compound with, for instance, two parts oxygen (w) and one part carbon (c) being denoted by 2w + c."" (Parkinson in ""Breakthroughs"", 1808 C).""In 1808 he (Wollaston) described his experiments on carbonates, sulfates, and oxalates, which proved that the composition of these substances was regulated by the law of multiple proportions. These additional instances of the law were easely verifiable and were often mentioned as standard examples. Wollaston accepted that his findings were merely particular instances of Dalton's assertion that the atoms of elements united one to one, or by simple multiple relation.""(DSB XIV, p.488).‎

Référence libraire : 42626

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738,65 € Acheter

‎"NEWTON, E.T. - A NEW SPECIES OF THE FLYING REPTILE PTERODACTYL.‎

‎On the Skull, Brain, and Auditory Organ of a new Species of Pterosaurian (Scaphognathus Purdoni), from the Upper Lias near Whitby, Yorkshire. Received March 1, - Read March 22, 1888.‎

‎(London, Harrisn and Sons, 1889). 4to. No wrappers as extracted from ""Philosophical Transactions"", 1888, Vol. 179 - Series B. Pp. 503-537, textillustr. and 2 lithographed plates. Fine and clean.‎

‎First appearance of this importent paper describing for the first time a new species of the Jurassic flying reptile.The skull was collected in the 1880s by D.W. Purdon, who is honoured in the specific name ""Scaphognatus Purdoni, s Newton nmd it. It was recognizd as a distinct genus only decades later in 1919 by Gustav von Arthaber.‎

Référence libraire : 42627

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335,75 € Acheter

‎"BUNSEN, ROBERT & HENRY E. ROSCOE. - THE LAWS OF PHOTOCHEMICAL ACTION.‎

‎Photo-chemical Researches. - Part IV. Received May 26 - Read May 26, 1859.‎

‎(London, Taylor and Francis, 1860). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1859 - Vol. 149 - Part II. Pp. 879-926. Clean and fine.‎

‎First appearance in English of a classic paper in the investigations of chemical reactions produced by lightrays. Their joined work - from 1855-59 - founded scientific photochemistry, by determining the phenomena of induction, deduction and extinction. They found that the beginning of light reaction takes place at first very slowly and that the velocity increases gradually until it attains a constant value, observing also that steam accelerates the action and that air retards it. They also gave proofs of the ""Law of Reciprocity‎

Référence libraire : 42633

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‎"HERSCHEL, JOHN W.F. - THE DISCOVERY OF THE IRON-PRINTING PROCESS.‎

‎On certain Improvements on Photographic Processes described in a former Communication, and on the Parathermic Rays of the Solar Spectrum. Received November 17, - Read November 17, 1842.‎

‎(London, Richard and John E., Taylor, 1843. 4to. No wrappers as extracted from ""Philosophical Transactions"" 1843 - Part I. Pp. 1-6.‎

‎First appearance of a pioneer-paper in the history of early photography, as Herschel here for the first time describes his discovery of the iron printing process with ammonio-citrate of iron by both methods, namely with blue lines on a white background and white lines on a blue ground.‎

Référence libraire : 42662

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‎"HELE - SHAW, H.S. - THE ANALOGUE CALCULATING MACHINE.‎

‎The Theory of Continous Calculating Machines and of a Mechanism of this class on a New Principle. Received and Read June 19, 1884.‎

‎London, Harrison and Sons, 1886. 4to. No wrappers as extracted from ""Philosophical Transactions"", 1885. Vol. 176 - Part II, Pp. 367-402 a. 34 textillustr.‎

‎First appearance of an importent paper in the history of calculating machines.""In his first year at Liverpool he published a paper on 'The theory of continuous calculating machines and of a mechanism of this class on a new principle' in the prestigious Philosophical Transactions of the Royal Society. This work investigated how to advance the design of integrator mechanisms and fit them for tasks more complex than mere numerical calculating machines, and was extremely important in the development of analogue computing.""(Jane Carruthers)‎

Référence libraire : 42668

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‎MAJOR, C.I. FORSYTH. - THE EXTINCT LEMUR OF MADAGASCAR.‎

‎On Megaladapis madagascariensis, an Extinct Gigantic Lemuroid from Madagascar" with Remarks on the Associated Fauna, and of its Geological Age. Received June 14, - Read June 15, 1893.‎

‎(London, Harrison and Sons, 1894). 4to. No wrappers as extracted from ""Philosophical Transactions"", 1894, Vol. 185 - Part I. Pp 15-38 a. 3 lithographed plates. Clean and fine.‎

‎First printing of this importent paper, relating the discovery of a new family Megaladapidae with the genus and species of the extinct giant lemur of Madagascar. Major collected the bones on his expedition to Madagascar in the years 1894-96.""Its tree-grasping attributes probably made Megaladapis vulnerable to changes to the forests of Madagascar. Upon human arrival between 1,500 and 2,000 years ago, the forests of Madagascar were cleared to make farmland. Unable to adapt to these new environmental changes imposed by man and being a tempting target for hunters, Megaladapis became extinct approximately 500 years ago, around the time of European discovery of Madagascar.""‎

Référence libraire : 42670

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‎"ROBINSON, THOMAS RODNEY & THOMAS GRUBB. - THE GREAT MELBOURNE TELESCOPE.‎

‎Description of the Great Melbourne Telescope.‎

‎(London, Taylor and Francis, 1870). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1869 - Vol. 159 - Part I. Pp. 127-161 and 10 lithographed plates, showing the telescope and its parts. A few small weak brownspots to top of some plates.‎

‎First printing of the detailled description of the Great Melbourne Telescope, by Robinson, member of the commitee and Thomas Grubb, the constructor. With it a number of importent observations of Nebulae were carried out. For 20 years it was the largest in the world, and it was the first instrument to document gravitational lens light refraction. The telescope was destroyed during the bush fires of January 2003.""The construction of the grand instrument was entrusted to Mr. Grubb, F.R.S., of Dublin, Ireland. At the Commencement of the year 1868 the telescope was completed, and examined by the Commitee of the Royal Society, made up of Lord Rosse, Dr. Robinson and Warren de la Rue. Intheir report they expressed their opinion that the equatorial was a masterpiece of astronomical mechanism.""‎

Référence libraire : 42671

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‎"ROBINSON, THOMAS RODNEY - THE ROBINSON CUP-ANEMOMETER.‎

‎On the Determination of the Constants of the Cup Anemometer by Experiments with a Whirling Machine. Received March 14 - Read April 4, 1878.‎

‎(London, Harrison and Sons, 1879). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1879 - Vol. 169 - Part II. Pp. 777-822 a. 5 plates.‎

‎First printing of Robinson's new experiments and researches into the constants of the Cup-Anemometer which he invented in 1846 by modifying Whewell's instrument by the introduction of the now-familiar windmill with hemispherical cups.""A simple type of anemometer is the cup anemometer, invented (1846) by Dr. John Thomas Romney Robinson, of Armagh Observatory. It consisted of four hemispherical cups each mounted on one end of four horizontal arms, which in turn were mounted at equal angles to each other on a vertical shaft. The air flow past the cups in any horizontal direction turned the cups in a manner that was proportional to the wind speed. Therefore, counting the turns of the cups over a set time period produced the average wind speed for a wide range of speeds. On an anemometer with four cups it is easy to see that since the cups are arranged symmetrically on the end of the arms, the wind always has the hollow of one cup presented to it and is blowing on the back of the cup on the opposite end of the cross.""‎

Référence libraire : 42674

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‎"WHEWELL, WILLIAM - A PIONEER-WORK ON TIDES WITH THE FIRST COTIDAL WORLD-MAP.‎

‎Essay towards a First Approximation to a Map of Cotidal Lines. Read May 2, 1833.‎

‎(London, Richard Taylor, 1833). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1833 - Part I. Pp. 147-236, a few textillustr.,1 engraved plate and 2 large folded engraved maps (a general, representing the greater part of the world (42x93 cm) and Chart of the British Isles, drawn and engraved by J.& C. Walker.). A small tear to world map. Clean and fine.‎

‎First appearance of this classic, pioneering paper on the investigation of tidal phenomena. It is the first in a series of 16 papers Whewell made for the Royal Society. It contains the first printed cotidal world-map.""Whewell took over the subject of mapping cotidal lines from Lubbock with entusiasm....He exercised the pioneer's privilege of coining new words and phrases appropriate to his subject. Many failed to stick, some phrases of Whewell's origin still occasionally used are: 'age of the tides', 'luni-tidal interval', 'semi-menstrual inequality' etc, etc....Whewell's initial cotidal map for the world ocean was presented in his first paper of 1833 (the paper offered). By his own admission, it was entirely preliminary and tentative, what nowadays might be called a ""strawman"", to stimulate discussionm. He later (1836) suggested smll modifications, especially near the coast of North America"" these were incorporated in an 'improved' world map by G.B. Airy in his celebrated tratise on ""Tides and wave"", (Cartwright in ""Tides. A Scientific History"", pp.110-112.)‎

Référence libraire : 42692

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‎"OWEN, RICHARD. - THE EXTINCT HORNED TURTLE.‎

‎On Parts of the Skeleton of Meiolania platyceps (Ow.). Received March 29, - Read April 21, 1887.‎

‎(London, Harrison and Sons, 1889). 4to. No wrappers as extracted from ""Philosophical Transactions"", 1888, Vol. 179 - Series B. Pp. 181-191 a. 7 lithographed plates.‎

‎First appearance of a classical paper in which Owen describes a series of remains, in better condition, than the bones from Lord Howe's Island, which Owen described in 1886 and named Meiolania platyceps. The remains belongs to Horned Turtles, and not to a giant lizard, Meiolania (""Small roamer"") is an extinct genus of cryptodire turtle from the Oligocene to Holocene, with the last relic populations at New Caledonia which survived until 2,000 years ago.The animal was rather large, measuring 2.5 metres (8.2 ft) in length, making it the second-largest known nonmarine turtle or tortoise, surpassed only by Colossochelys atlas from Asia, which lived in the Pleistocene. It lived in Australia and New Caledonia. Remains have also been found on the island of Efate in Vanuatu, associated with settlements from the Lapita culture.‎

Référence libraire : 42702

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‎"ROLOFF, CHRISTIAN LUDVIG. - THE NORTH AMERICAN RACCOON DESCRIBED.‎

‎Description d'un Quadrupede D'Amerique, rapporté par M. Linnaeus au Genre des Ours. Traduit du Latin.‎

‎(Berlin, Haude et Spener, 1758). 4to. No wrappers, as issued in ""Memoires de Academie Royale des Sciences et Belles-Lettres"", Annee 1756, tome XI, pp. 149-162 a. 3 folded engraved plates.‎

‎First printing of an early description of the North American Raccoon, Ursus Lotor, Washer Bear (Linné 10th ed.), with 3 fine engraved plates.‎

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‎"THOMSON, WILLIAM (LORD KELVIN) & JAMES PRESCOTT JOULE. - THE JOULE-THOMSON EFFECT DISCOVERED.‎

‎On the Thermal Effects of Fluids in Motion. Received June 15, - Read June 16, 1853.‎

‎(London, Richard Taylor and William Francis, 1853) 4to. No wrappers as extracted from ""Philosophical Transactions"" 1853, Vol. 143 - Part III. Pp. 357-365. Textillustrations. Clean and fine.‎

‎First appearance of this highly importent paper in the development of thermodynamics, describing the experiments leading to the discovery of the cooling effect when a gas is allowed to expand freely. This is the founding theory, later used in refrigeration.""The only substantial contribution to thermodynamics to which the joint names of Joule and Thomson are attached belongs to an idea conceived by Thomson, who saw the possibility of analyzing the deviations of gas properties from the ideal behavior. In particular a non-ideal gas, made to expand slowly through a porous plug so as to approximate a specified mathematical condition - constant enthalpy), would in general undergo cooling (essentially a transformation of atomic motion into work spent against the interatomic attractions)....But the appliocation of the Joule-Thomson effect to technology of refrigeration belongs to a later stage in the development of thermodynamics.""(DSB VII, p. 182).The Joule-Thomson effect or Joule-Kelvin effect describes the increase or decrease in the temperature of a real gas (as differentiated from an ideal gas) or a liquid when allowed to expand freely through a valve or other throttling device while kept insulated so that no heat is transferred to or from the fluid, and no external mechanical work is extracted from the fluid. The Joule-Thomson effect is an isenthalpic process, meaning that the enthalpy of the fluid is constant (i.e., does not change) during the process. It is named for James Prescott Joule and William Thomson, 1st Baron Kelvin who established the effect in 1852, following earlier work by Joule on Joule expansion in which a gas expands at constant internal energy. The Joule-Thomson effect is sometimes referred to as the Joule-Kelvin effect. Engineers often refer to it as simply the J-T effect.‎

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‎"GRAHAM, THOMAS. - A CLASSIC PAPER IN MEMBRANE SCIENCE BY THE FARTHER OF PHYSICAL CHEMISTRY.‎

‎On the Absorption and Dialytic Separation of Gases by Colloid Septa. Part I-(II). (I. Action of a Septum of Caoutchouc. - II. Action of Metallic Septa at a red Heat.).‎

‎(London, Taylor and Francis, 1866). 4to. No wrappers as extracted from ""Philosophical Transactions"", Vol. 156 - Part II, pp. 399-439. 2 Textillustrations.‎

‎Firat appearance of a groundbreaking paper in physical chemistry in which Graham describes the fundamental mechanism for gas transport across a polymer membrane. The mechanism is known as solution-diffusion model, and postulates a three-step process for gas transport through a polymer.‎

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‎"MAXWELL, JAMES CLERK. - THE KINETIC THEORY OF GASES.‎

‎The Bakerian Lecture. - On the Viscosity or Internal Friction of Air and other Gases. Received November 23, 1865 (+) Postscript.- Received December 7, 1865. - Read February 8, 1866.‎

‎(London, Taylor and Francis, 1866). Large 4to. Without wrappers. Extracted from ""Philosophical Transactions of the Royal Society of London."", Vol. 156 - Part I. Pp. 249-268 a. 1 lithographed plate. A few brownspots to the plate. Having the titlepage to vol. 156 - Part I. A few brownspots to lower margins.‎

‎First appearance of a major paper in the kinetic theory of gases, in which Maxwell proved that the viscosity was independent of pressure as predicted, and nearly a linear function of the absolute temperature T.One of Maxwell's major investigations was on the kinetic theory of gases. Originating with Daniel Bernoulli, this theory was advanced by the successive labours of John Herapath, John James Waterston, James Joule, and particularly Rudolf Clausius, to such an extent as to put its general accuracy beyond a doubt"" but it received enormous development from Maxwell, who in this field appeared as an experimenter (on the laws of gaseous friction) as well as a mathematician.""James Clerk Maxwell published a famous paper in 1866 (the paper offered) using the kinetic theory of gases to study gaseous viscosity. The internal friction (the viscosity) of the gas is determined by the probability a particle of layer A enters layer B with a corresponding transfer of momentum. Maxwell's calculations showed him that the viscosity coefficient is proportional to both the density, the mean free path and the mean velocity of the atoms. On the other hand, the mean free path is inversely proportional to the density. So an increase of pressure doesn't result in any change of the viscosity.‎

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‎"MAXWELL, JAMES CLERK. - ESTABLISHING THE SCIENCE OF RAREFIED GAS DYNAMICS.‎

‎On Stresses in Rarified Gases arising from Inequalities of Temperature. Recieved March 19, - Read April 11, 1878. (+) Appendix. (Added May, 1879).‎

‎(London, Harrison and Sons, 1880). 4to. No wrappers as extracted from ""Philosophical Transactions"", Year 1879, Vol. 171 - Part II. Pp. 231-256. Clean and fine.‎

‎First appearance of a major paper on Gas Dynamics, creating a whole new science. One of Maxwell's major investigations was on the kinetic theory of gases. Originating with Daniel Bernoulli, this theory was advanced by the successive labours of John Herapath, John James Waterston, James Joule, and particularly Rudolf Clausius, to such an extent as to put its general accuracy beyond a doubt"" but it received enormous development from Maxwell, who in this field appeared as an experimenter (on the laws of gaseous friction) as well as a mathematician.""Maxwell's last major paper on any subject was ""On Stresses in Rarified Gases arising from Inequalities of Temperature."" Between 1873 and 1876 the scientific world had been stirred by William Crooke's experiments with the radiometer, the well-known device composed of a partuially evacuated chamber containing a paddle wheel with vanes blackened on one side and silvered on the other, which spins rapidly when radiant heat impinges on it....Reynolds called this new effect ""thermal transpiration"". Maxwell gave a simple qualitative explanation in his report, and in an appendix added to his own paper in May 1879 he developed a semiempirical theory accounting for it and for the radiometer effect...Maxwell's paper created the science of rarified gas dynamics. His formulas for stress and heat flux in the body of the gas were contributions of permanent value, while his investigations of surface effects started a vast body of research extending to the present day...One other contribution of great beauty contained in notes added to the papwer in May and June 1879 was an application of the methods of spherical harmonic analysis to gas theory.""(DSB IX, p. 224-25).‎

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‎"KIES, (JOHANN). & CASSINI de THURY - LUNAR THEORY & THE BERLINER QUADRANT.‎

‎De la Situation la plus avantageuse des Planetes pour Découvrir les Irrégularités de leurs Mouvemens. (+ Kies:) Sur les Eclipses des Etoileas fixes par la Lune. (+ Cassini de Thury:) Memoire, dans lequel on examiné, si l'on peut esperer la meme Pre...‎

‎(Berlin, Haude et Spener, 1751). 4to. No wrappers, as issued in ""Mémoires de l'Academie Royale des Sciences et Belles-Lettres"", tome V, Année 1749, pp. 339-372, 1 folded geometrical plate (to the first paper) and 3 fine double-page folded engraved plates showing the quadrant.‎

‎Kies was one of the first to propagate Newton's discoveries in Germany, and dedicated two of his works to the Englishman. The crater Kies on the Moon is named after him.The paper on the instrument describes and depicts the large quadrant in the Berlin observatory invented by Hadley (described in Transactions of the Royal Society in 1732).""From 1742 to 1754, at the recommendation of the mathematician Leonhard Euler, he (Kies) was made professor of mathematics at Berlin's Academy of Sciences and astronomer at its observatory. His reports from this time include De la Situation la plus avantageuse des planètes pour découvrir les irrégularités de leurs mouvemens, Sur les Éclipses des étoiles fixes par la lune, and Description d'un instrument qui se trouve .""‎

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‎FISCHER, JOHANN LEONHARD. - ON THE GADFLY.‎

‎Observationes de Oestro Ovino atqve Bovino factae. Disputatio...phil. ordinis defendet Iohannes Leonhard. Fischer...Respondente Bernhard Gottlob Schreger. Cum tabulis quatuor aeneis.‎

‎Leipzig, Officina Solbrigia, (1788) 4to. Orig. blank wrappers. Frontwrapper loose. (6),70,(2) pp. and 4 engraved plates with many figs. Titlepage and 2 lvs. brownspotted. Scattered marginal brownspots. Wide-margined copy, printed on good paper.‎

‎This dissertation is probably the first monograph on the Gadfly. - BMC (NH) II, p.576. - Horn &Schenkling, Fischer :76.‎

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‎"WILSON, C.T.R. - THE WILSON ""CLOUD-CHAMBER"".‎

‎On the Condension Nuclei produced in Gases by the Action of Röntgen Rays, Uranium Rays, Ultra-violet Light, and other Agents. Received October 29, - Read November 24, 1898.‎

‎(London, Harrison and Sons, 1899). 4to. No wrappers as extracted from ""Philosophical Transactions"", Vol. 192 - Series A. Pp. 403-453. Textillustrations. Clean and fine.‎

‎First printing of Wilson's second importent paper describing his further experiments with his ""Cloud Chamber"".""To the period 1895-1912 belongs the development of an instrument which to my mind is the most original and wonderful in scientific history.I refer to the cloud or expansion chamber of C.T.R. Wilson...It was a wonderful advance to be able to se, so to speak, the details of the adventures of these particles in their flight through the gas....""(Lord Rutherford).""C.T.R. Wilson had been developing his cloud-chamber, which was to provide the most powerfull of all methods of investigation in atomic physics. In moist air, if a certain degree of supersaturation is exceeded this can be secured by a sudden expansion of the air) condensation takes place on dust-nuclei, when any are present: if by preliminary operations condensation is made to take place on the dust-nuclei, and the resulting droplets are allowed to settle, the air in the chamber is thereby freed from dust. If now X-rays or radiation from a radioactive substance are passed into the chamber, and if the degree of supersaturation is sufficient, condensation again takes place: this is due to the production of ions by the radiation. Thus the tracks of ionising radiations can be made visible by the sudden expansion of a moist gas, each ion becoming the centre of a visible globule of water. Wilson showed that the ions produced by uranium radiation were identical with those produced by X-rays."" (Whittaker in ""A History of the Theories of Aether and Electricity."" II, p. 4).‎

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‎"HERSCHEL, WILLIAM. - THE DYNAMICAL THEORY OF STARS AND NEBULAE.‎

‎Astronomical Observations relating to the Construction of the Heavens, arranged for the Purpose of a critical Examination, the Result of which appears to throw some new Light upon the Organization of the celestial Bodies. Read June 20, 1811. (+)Astron...‎

‎(London, W. Bulmer and Co., 1811 a.1814). 4to. No wrappers as extracted from ""Philosophical Transactions"" Year 1811-Part II. 269-336 and 2 engraved plates showing the shapes of 42 nebulae and star-clusters. And 1814 - Part I. Pp. 248-84 a. 1 engraved plate. Both fine and clean.‎

‎First appearance of two milestone papers in cosmology in which Herschel demonstrates the irregular distribution of the stars in space, and ""for the first time recognized that the clusters in and near the Milky Way really belonged to it, and were not independent systems that happened to lie in the same direction as seen by us.""(Berry, Short History of Astronomy, p. 340).""In 1811 and 1814 (the papers offered) he published a complete theory of a possible process wherby the shining fluid consisting a diffused nebula might gradually condense - the denser portions of it being centres of attraction - first into a denser nebula or compressed star cluster, then into one or more nebulous stars, lastly into a single star or group of stars. Every supposed stage in this process was abundantly illustrated from records of actual nebulae and clusters which he had observed.""(Berry).""Illustrated with many examples at every stage, these papers (1811 a. 1814) showed brilliantly how dynamic changes can be inferred from virtually static evidence"" and Herschel concluded by characterizing the Milky Way in its present stage of dissolution as ""this mysterious chronometer"". (DSB VI, p. 333). A paper by Henry Kater attached: ""Further Experiments on the Light of the Cassegrainian telescope compared with that of the Georgian"". 1814. Pp. 231-247.‎

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‎"TYNDALL, JOHN. - A FUNDAMENTALPAPER IN BACTEOROLOGY - THE FINAL BLOW TO ""SPONTANEOUS GENERATION"".‎

‎Further Researches on the Deportment and Vital Persistence of Putrefactive and Infective Organisms from a Physical Point of View. Received May 14, - Read May 17, 1877.‎

‎(London, Taylor and Francis, 1878). 4to. No wrappers as extracted from ""Philosophical Transactions"" 1877, Vol. 167 - Part I. Pp. 149-206. Illustrations in the text. Clean and fine.‎

‎First appearnace of this important paper in which Tyndall announced his discovery of fractional sterilization ""Tyndallization"".""In my last paper I made some remarks upon this subject"" and in relation to our present experiments, the influence of drying and hardening was brought home to me by the fact that in all the foregoing cases the infusions which five minutes boiling proved sufficient to sterilize were, without exception, derived from fresh hay mowen in 1876, while the infusions which five minutes' boiling failed to sterilize were derived, without exception, from old hay mown either in 1875 or some previous year.""(p. 159 in the paper).""Tyndall interested himself in atmospheric germs and dust. His experiments on sterilization by heat lead him to the discovery in 1877 (the paper offered) of fractional sterilization (Tyndallization)....The reseraches of Tyndall, even more than those of Pasteur, dealt the final blow to the doctrine of spontaneous generation"" they were fundamental for the progress of bacteriology.""(Garrison & Morton 2495, listing his later book from 1881 ""Essays on the floating-matter of the air..."").During the 1870s Pasteur and Tyndall were in frequent communication.‎

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‎"HAHN, O. (OTTO). - THE DISCOVERY OF RADIOTHORIUM.‎

‎Über ein neues, die Emanation des Thoriums gebendes radioaktives Element.‎

‎Leipzig, S. Hirzel, 1905. No wrappers. Issued in ""Jahrbuch der Radioaktivität und Elekronik"", 2. Bd., Heft 3. Hahn's paper: pp. 233-264. Enntire issue: pp. 233-262 (= entire ""Heft 3""). Fine and clean.‎

‎First printing of this paper, which is Hahn's Habilitation paper, announcung his discovery of a new element in residues from a Ceylon mineral called Thorianite. He later showed that it is an intermediate disintegration product.""Because the sample (thorianite) was small, Ramsay proposed that Hahn confirm Marie Curie's determination of the atomic weight of radium by preparing it in some organic compounds (thereby greatly increasing the total amount being examined) and calculating the atomic weight from the measured molecular weights. Chance sometimes favors the unprepared mind, and Hahn, who familiarized himself with only the basic of radioactivity, followed the prescribed separationss technique and found himself the discovere of a new radioelement: radiothorium. The explanation was that the material given him came from an ore which contained a large percentage of thorium in addition to the radium. Thus, upon completion of the chemical procedure, not all the activity was confined in the radium-containg fraction"" indeed the nes subsyance in the remainder was several hundred thousand times more active than thorium and ultimately yielded the characteristic one.minute halflife of thorium emanation.""(DSB VI, p. 15). - Weeks, Discovery of the Elements,p. 308 ff.).‎

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‎"LUBBOCK, JOHN WILLIAM. - THE LUNAR THEORY.‎

‎On the Theory of the Moon. (I-II). Received November 30, Read December 12, 1833. (and Part II:) Received and Read March 13, 1834.‎

‎(London, Richard Taylor, 1834) 4to. No wrappers as extracted from ""Philosophical Transactions"" 1834 - Part I. Pp. 123-126 a. pp. 127-141.‎

‎First appearance of Lubbock's ""Lunar-Theory""""John Lubbock (1803-65), was an astronomer and mathematician. He made a special study of tides and of the lunar theory and developed a method for calculating the orbits of comets and planets. In mathematics he applied the theory of probability to life insurance problems.""‎

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