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COMBUSTION (from the Lat. comburere, ...

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Originally appearing in Volume V06, Page 759 of the 1911 Encyclopedia Britannica.
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COMBUSTION (from the
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Lat. comburere, to burn up)
  , in chemistry, the
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process of burning or, more scientifically, the oxidation of a substance, generally with the production of flame and the
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evolution of heat . The
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term is more customarily given to productions of flame such as we have in the burning of oils,
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gas, fuel, &c., but it is conveniently extended to ether cases of oxidation, such as are met with when metals are heated for a long time in air or oxygen . The term " spontaneous combustion " is used when a substance smoulders or inflames apparently without the intervention of any
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external heat or
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light; in such cases, as, for example, in heaps of cotton-waste soaked in oil, the oxidation has proceeded slowly, but steadily, for some time, until the heat evolved has raised the mass to the temperature of ignition . The explanation of the phenomena of combustion was at-tempted at very early times, and the early theories were generally bound up in the explanation of the nature of fire or flame . The idea that some extraneous substance is essential to the process is of ancient date; Clement of Alexandria (c . 3rd century A.D.) held that some " air " was necessary, and the same view was accepted during the
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middle ages, when it had been also found that the products of combustion weighed more than the
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original combustible, a fact which pointed to the conclusion that some substance had combined with the combustible during the process . This theory was supported by the French physician
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Jean Ray, who showed also that in the cases of tin and lead there was a limit to the increase in
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weight . Robert Boyle, who made many researches on the origin and nature of fire, regarded the increase as due to the fixation of the particles of fire . Ideas identical with the
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modern ones were expressed by John Mayow in his Tractatus quinque medico-physici (1674), but his
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death in 1679 undoubtedly accounts for the neglect of his suggestions by his contemporaries . Mayow perceived the similarity of the processes of respiration and combustion, and showed that one constituent of the atmosphere, which he termed spiritus nitro-aereus, was essential to combustion and
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life, and that the second constituent, which he termed spiritus nitri acidi, inhibited combustion and life . At the beginning of the 18th century a new theory of combustion was promulgated by Georg Ernst Stahl . This theory regarded combustibility as due to a principle named phlogiston (from the Gr .

4Ao'yuar6s, burnt), which was

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present in all combustible bodies in an amount proportional to their degree of combustibility; for instance,
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coal was regarded as practically 1 ay 1 or say pure phlogiston . On this theory, all substances which could be burnt were composed of phlogiston and some other substance, and the operation of burning was simply
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equivalent to the liberation of the phlogiston . The Stahlian theory, originally a theory of combustion, came to be a general theory of chemical reactions, since it provided
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simple explanations of the ordinary chemical processes(when regarded qualitatively) and permitted generalizations which largely stimulated its acceptance . Its inherent defect— that the products of combustion were invariably heavier than the original substance instead of less as the theory demanded—was ignored, and until
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late in the 18th century it dominated chemical thought . Its overthrow was effected by Lavoisier, who showed that combustion was simply an oxidation, the oxygen of the atmosphere (which was isolated at about this time by K . W . Scheele and J . Priestley) combining with the substance burnt .

End of Article: COMBUSTION (from the Lat. comburere, to burn up)
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