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See also:JULIUS See also:ROBERT See also:MAYER (1814-1878) , See also:German physicist, was See also:born at See also:Heilbronn on the 25th of See also:November 1814, studied See also:medicine at See also:Tubingen, See also:Munich and See also:Paris, and after a See also:journey to See also:Java in 1840 as surgeon of a Dutch See also:vessel obtained a medical See also:post in his native See also:town . He claims recognition as an See also:independent a priori propounder of the " First See also:Law of See also:Thermodynamics," but more especially as having See also:early and ably applied that law to the explanation of many remarkable phenomena, both cosmical and terrestrial . His first little See also:paper on the subject, " Bemerkungen giber See also:die Krdfte der unbelebten Natur," appeared in 1842 in See also:Liebig's Annalen, five years after the republication, in the same See also:journal, of an See also:extract from K . F . See also:Mohr's paper on the nature of See also:heat, and three years later he published Die organische Bewegung in ihren Zusammenhange mit dem Stoffwechsel . It has been repeatedly claimed for See also:Mayer that he calculated the value of the dynamical See also:equivalent of heat, indirectly, no doubt, but in a manner altogether See also:free from See also:error, and with a result according almost exactly with that obtained by J . P . See also:Joule after years of patient labour in See also:direct experimenting . This claim on Mayer's behalf was first shown to be baseless by W . See also:Thomson (See also:Lord See also:Kelvin) and P . G . See also:Tait in an See also:article on " See also:Energy," published in See also:Good Words in 1862, which gave rise to a See also:long but lively discussion .
A See also:calm and judicial annihilation of the claim is to be found in a brief article by See also:Sir G
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G
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See also:Stokes, Proc
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See also:Roy
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See also:Soc., 1871, p
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54
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See also See also:Maxwell's Theory of Heat, See also:chap. xiii
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Mayer entirely ignored the See also:grand fundamental principle laid down by Sadi See also:Carnot—that nothing can be concluded as to the relation between heat and See also:work from an experiment in which the working substance is See also:left at the end of an operation in a different See also:physical See also:state from that in which it was at the commencement
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Mayer has also been styled the discoverer of the fact that heat consists in (the energy of) See also:motion, a See also:matter settled at the very end of the 18th See also:century by See also:Count See also:Rumford and Sir H
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See also:Davy; but in the See also:teeth of this statement we have Mayer's own words, " We might much rather assume the contrary—that in See also:order to become heat motion must cease to be motion."
75", and consequently the See also:longitude at See also:sea to about See also:half a degree
.
An improved set was afterwards published in See also:London (1770), as also the theory (Theoria lunae juxta systema Newtonianum, 1767) upon which the tables are based
.
His widow, by whom they were sent to See also:England, received in See also:consideration from the See also:British See also:government a See also: Appended to the London edition of the See also:solar and lunar tables are two See also:short tracts—the one on determining longitude by lunar distances, together with a description of the repeating circle (invented by Mayer in 1V52), the other on a See also:formula for atmospheric See also:refraction, which applies a remarkably accurate correction for temperature . Mayer left behind him a considerable quantity of See also:manuscript, See also:part of which was collected by G . C . See also:Lichtenberg and published in one See also:volume (See also:Opera inedita, See also:Gottingen, 1775) . It contains an easy and accurate method for calculating eclipses; an See also:essay on See also:colour, in which three See also:primary See also:colours are recognized; a See also:catalogue of 998 zodiacal stars; and a memoir, the earliest of any real value, on the proper motion of eighty stars, originally communicated to the Gottingen Royal Society in 1760 . The manuscript See also:residue includes papers on atmospheric refraction (dated 1755), on the motion of See also:Mars as affected by the perturbations of See also:Jupiter and the See also:Earth (1756), and on terrestrial magnet-ism (176o and 1762) . In these last Mayer sought to explain the magnetic See also:action of the earth by a modification of See also:Euler's See also:hypothesis, and made the first really definite See also:attempt to establish a mathematical theory of magnetic action (C . See also:Hansteen, Magnetismus der Erde, i . 283) . E . Klinkerfuss published in 1881 photo-lithographic reproductions of Mayer's See also:local charts and See also:general See also:map of the See also:moon; and his See also:star-catalogue was re-edited by F . See also:Baily in 1830 (See also:Memoirs Roy .
Astr
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Soc. iv
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391) and by G
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F
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J
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A
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Auvers in 1894
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934
Mayer's real merit consists in the fact that, having for himself made out, on inadequate and even questionable grounds, the conservation of energy, and having obtained (though by inaccurate reasoning) a numerical result correct so far as his data permitted, he applied the principle with See also:great See also:power and insight to the explanation of numerous physical phenomena
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His papers, which were republished in a single volume with the See also:title Die Mechanik der Warme (3rd ed., 1893), are of unequal merit
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But some, especially those on See also:Celestial See also:Dynamics and Organic Motion, are admirable examples of what really valuable work may be effected by a See also:man of high intellectual See also:powers, in spite of imperfect See also:information and defective See also:logic
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Different, and it would appear exaggerated, estimates of Mayer are given in See also: Diihring's See also:Robert Mayer, der Galilei See also:des neunzehnten Jahrhunderts, See also:Chemnitz, 1880 . Some of the simpler facts of the See also:case are summarized by Tait in the Phil . Mag., 1864, ii, 289 . |
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