A Preliminary Dissertation on the Mechanisms of the Heavens — John Shaqi
A Preliminary Dissertation on the Mechanisms of the HeavensSomerville, Mary
Science
A Preliminary Dissertation on the Mechanisms of the Heavens
Somerville, Mary
Celestial mechanics
The high temperature of mines, hot springs, and above all, the internal
fires that have produced, and do still occasion such devastation on our
planet, indicate an augmentation of heat towards its centre the increase
of density in the strata corresponding to the depth and the form of the
spheroid, being what theory assigns to a fluid mass in rotation, concur
to induce the idea that the temperature of the earth was originally so
high as to reduce all the substances of which it is composed to a state
of fusion, and that in the course of ages it has cooled down to its
present state; that it is still becoming colder, and that it will
continue to do so, till the whole mass arrives at the temperature of the
medium in which it is placed, or rather at a state of equilibrium
between this temperature, the cooling power of its own radiation, and
the heating effect of the sun's rays. But even if this cause be
sufficient to produce the observed effects, it must be extremely slow in
its operation; for in consequence of the rotation of the earth being a
measure of the periods of the celestial motions, it has been proved,
that if the length of the day had decreased by the three hundredth part
of a second since the observations of Hipparchus two thousand years ago,
it would have diminished the secular equation of the moon by 4"·4. It
is therefore beyond a doubt, that the mean temperature of the earth
cannot have sensibly varied during that time; if then the appearances
exhibited by the strata really owing to a decrease of internal
temperature, it either shows the immense periods requisite to produce
geological changes to which two thousand years are as nothing, or that
the mean temperature of the earth had arrived at a state of equilibrium
before these observations. However strong the indication of the
primitive fluidity of the earth, as there is no direct proof, it can
only be regarded as a very probable hypothesis; but one of the most
profound philosophers and elegant writers of modern times has found, in
the secular variation of the eccentricity of the terrestrial orbit, an
evident cause of decreasing temperature. That accomplished author, in
pointing out the mutual dependences of phenomena, says--'It is evident
that the mean temperature of the whole surface of the globe, in so far
as it is maintained by the action of the sun at 8 higher degree than it
would have were the sun extinguished, must depend on the mean quantity
of the sun's rays which it receives, or, which comes to the same thing,
on the total quantity received in a given invariable time: and the
length of the year being unchangeable in all the fluctuations of the
planetary system, it follows, that the total amount of solar radiation
will determine, _cœteris paribus_, the general climate of the earth. Now
it is not difficult to show, that this amount is inversely proportional
to the minor axis of the ellipse described by the earth about the sun,
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