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COMBUSTION (from the See also: process of burning or, more scientifically, the oxidation of a substance, generally with the production of flame and the See also: evolution of heat
.
The See also: term is more customarily given to productions of flame such as we have in the burning of oils, See also: gas, fuel, &c., but it is conveniently extended to See also: ether cases of oxidation, such as are met with when metals are heated for a long See also: time in air or See also: oxygen
.
The term " spontaneous combustion " is used when a substance smoulders or inflames apparently without the intervention of any See also: external heat or See also: light; in such cases, as, for example, in heaps of See also: 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 See also: ancient date; See also: Clement of Alexandria (c
.
3rd century A.D.) held that some " air " was necessary, and the same view was accepted during the See also: middle ages, when it had been also found that the products of combustion weighed more than the See also: 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 See also: Jean Ray, who showed also that in the cases of tin and See also: lead there was a limit to the increase in See also: 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 See also: modern ones were expressed by See also: John
See also: Mayow in his Tractatus quinque medico-physici (1674), but his See also: 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 See also: 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 See also: Ernst Stahl
.
This theory regarded combustibility as due to a principle named phlogiston (from the Gr
.
4Ao'yuar6s, burnt), which was See also: present in all combustible bodies in an amount proportional to their degree of combustibility; for instance, See also: 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 See also: 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 See also: 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 See also: 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
.
See also: Scheele and J
.
See also: Priestley) combining with the substance burnt
.
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