Illustrations of the Huttonian Theory of the EarthPlayfair, John
Science
Illustrations of the Huttonian Theory of the Earth
Playfair, John
Geology; Hutton, James, 1726-1797. Theory of the earth
168. Some recent experiments, seem to make the suggestions in this
query applicable to an opaque body like the earth, as well as to
luminous bodies, such as the sun and fixed stars. The radiation of
heat, where there is no light, was first rendered probable by the
experiments of M. PICTET of Geneva;[77] and the only objections to
which the conclusions from those experiments seemed liable, are removed
by the late very important discoveries of Dr HERSCHEL.[78] From these
it appears, that heat is capable of refraction and reflection, as well
as light, so that it is not absurd to suppose, that _the heat of great,
dense, and faced bodies, may be conserved by the greatness of the
bodies, and the mutual action and reaction between them and the heat
which they emit_.
[Footnote 77: Essai sur le Feu.]
[Footnote 78: Phil. Trans. 1800, p. 84.]
The existence of subterraneous heat is still further rendered probable
from the researches of MAIRAN, which tend to show, that there is
another source of terrestrial heat besides the influence of the solar
rays.[79]
[Footnote 79: Mém. de l'Acad. des Sciences, 1765, p. 143.]
Whatever be the truth with regard to these conjectures, it is certain,
that the first and original source of heat is independent of burning.
Burning is an _effect_ of the concentration of heat; and though, by a
certain reaction, it has the power of continuing and augmenting that
heat, it never can be regarded as its primary and material cause. When,
therefore, we suppose a source of heat, independent of fire and of
burning, we suppose what certainly exists in nature, though we are not
informed of the manner of its existence, nor of its place, otherwise
than from considering the phenomena of the mineral kingdom.
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