Buffon's Natural History. Volume 10 (of 10): Containing a Theory of the Earth, a General History of Man, of the Brute Creation, and of Vegetables, Minerals, &c. &cBuffon, Georges Louis Leclerc, comte de
History
Buffon's Natural History. Volume 10 (of 10): Containing a Theory of the Earth, a General History of Man, of the Brute Creation, and of Vegetables, Minerals, &c. &c
Buffon, Georges Louis Leclerc, comte de
Natural history
It is well known, that heat grows less, or cold becomes greater, the
higher we ascend on the mountains. It is true that the heat which
proceeds from the terrestrial globe, is of course sensibly less on
those advanced points, than it is on the plains; but this cause is not
proportionable to the effect; the action of heat, which emanates from
the terrestrial globe, not being able to diminish but by the square of
the distance, it does not appear that at the height of half a mile,
which is only the three thousandth part of the semi-diameter of the
globe, whose centre must be taken for the focus of heat, that this
difference, which in this supposition is only a unit and nine millions,
can produce a diminution of heat nearly so considerable; for the
thermometer lowers at that height, at all times of the year, to the
freezing point. It is not probable, that this great difference of heat
simply proceeds from the difference of the earth; and of that we must
be fully convinced, if we consider, that at the mouth of the volcanos,
where the earth is hotter than in any other part on the surface of the
globe, the air is nearly as cold as on other mountains of the same
height.
It may then be supposed that the atoms of light, though very hot at the
moment of quitting the sun, are greatly cooled during the seven minutes
and a half in which they pass from that body to the earth; and this
in fact would be the case if they were detached; but, as they almost
immediately succeed each other, and are the more confined as they are
nearer the place of their origin, the heat lost by each atom falls on
the neighbouring ones; and this reciprocal communication supports the
general heat of light a longer time; and as their constant direction is
in divergent rays, their distance from each other increases according
to the space they run over; and as the heat which flies from each
atom, as a centre, diminishes also in the same ratio, it follows, that
the light of the solar rays, decreasing in an inverted ratio from the
square of the distance, that of their heat decreases in an inverted
ratio of the square of the same distance.
Public-domain text, read in full here on John Shaqi.
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