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See also:COLD (in O. Eng. cald and ceald, a word coming ultimately from a See also:root cognate with the See also:Lat. gelu, gelidus, and See also:common in the See also:Teutonic See also:languages, which usually have two distinct forms for the substantive and the See also:adjective, cf. Ger. Kolte, kalt, Dutch koude , koud) ,subjectively the sensation which is excited by contact with a substance whose temperature is See also:lower than the normal; objectively a quality or See also:condition of material bodies which gives rise to that sensation . Whether See also:cold, in the See also:objective sense, was to be regarded as a See also:positive quality or merely as See also:absence of See also:heat was See also:long a debated question . Thus See also:Robert See also:Boyle, who does not commit himself definitely to either view, says, in his New Experiments and Observations touching Cold, that " the dispute which is the primum frigidum is very well known among naturalists, some contending for the See also:earth, others for See also:water, others for the See also:air, and some of the moderns for See also:nitre, but all seeming to agree that there is some See also:body or other that is of its own nature supremely cold and by participation of which all other bodies obtain that quality." But with the See also:general See also:acceptance of the dynamical theory of heat, cold naturally came to be regarded as a negative condition, depending on decrease in the amount of the molecular vibration that constitutes heat . The question whether there is a limit to the degree of cold possible, and, if so, where the zero must be placed, was first attacked by the See also:French physicist, G . See also:Amontons, in 1702–1703, in connexion with his improvements in the air-thermometer . In his See also:instrument temperatures were indicated by the height at which a See also:column of See also:mercury was sustained by a certain See also:mass of air, the See also:volume or " See also:spring " of which of course varied with the heat to which it was exposed . Amontons therefore argued that the zero of his thermometer would be that temperature at which the spring of the air in it was reduced to nothing . On the See also:scale he used the boiling-point of water was marked at 73 and the melting-point of See also:ice at 512, so that the zero of his scale was See also:equivalent to about -240° on the centigrade scale . This remark-ably See also:close approximation to the See also:modern value of -273° for the zero of the air-thermometer was further improved on by J . H . See also:Lambert (Pyrometrie, 1779), who gave the value -270° and observed that this temperature might be regarded as See also:absolute cold . Values of this See also:order for the absolute zero were not, however, universally accepted about this See also:period .
See also:Laplace and See also:Lavoisier, for instance, in their See also:treatise on heat (178o), arrived at values ranging from 1500° to 3000° below the freezing-point of water, and thought that in any See also:case it must be at least 600° below, while See also: Poynting (" Radiation in the See also:Solar See also:System," Phil . Trans., A, 1903, 202, p . 525) showed that as regards bodies in the solar system the effects of radiation from the stars are negligible, and calculated that by solar radiation alone a small absorbing See also:sphere at the distance of Mercury from the sun would have its temperature raised to 483° Abs . (21o° C.), at the distance of See also:Venus to 358° Abs . (85° C.), of the earth to 300° Abs . (27° C.), of See also:Mars to 243° Abs . (– 3o° C.), and of See also:Neptune to only 54° Abs . (– 219°C.) . The French physicists of the See also:early See also:part of the 19th See also:century held a different view, and rejected the See also:hypothesis of the absolute cold of space . See also:Fourier, for instance, postulated a fundamental temperature of space as necessary for the explanation of the heat-effects observed on the See also:surface of the earth, and estimated that in the interplanetary regions it was little less than that of the terrestrial poles and below the freezing-point of mercury, though it was different in other parts of space (See also:Ann. chim. phys., 1824, 27, pp . 141, 150) . C . S . M . Pouillet, again, calculated the temperature of interplanetary space as – 142° C . (Comptes rendus, 1838, 7, p . 61), and See also:Sir John See also:Herschel as -150° (Ency . Brit., 8th ed., See also:art . " See also:Meteorology," p . 643) . To attain the absolute zero in the laboratory, that is, to deprive a substance entirely of its heat, is a thermodynamical impossibility, and the most that the physicist can See also:hope for is an indefinitely close approach to that point . The lowest steady temperature obtainable by the exhaustion of liquid See also:hydrogen is about – 262° C . (I I° Abs.), and the liquefaction of See also:helium by Professor Kamerlingh Onnes in 1908 yielded a liquid having a boiling-point of about 4.3° Abs., which on exhaustion must bring us to within about 22 degrees of the absolute zero . (See LIQUID GASES.) For a "cold," in the medical sense, see See also:CATARRH and See also:RESPIRATORY SYSTEM: See also:Pathology .
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