Classics of modern science : $b (Copernicus to Pasteur)
History
Classics of modern science : $b (Copernicus to Pasteur)
Science; Science -- History
or an hyperbola, which, in consequence of the magnitude of its axis
will be as to sense confounded with a parabola in the part of its orbit
which is observed. It is not therefore surprising that hitherto no
hyperbolic motions have been recognized.
The attraction of the planets, and perhaps also the resistance of the
ethereal media, ought to change several cometary orbits into ellipses,
of which the greater axes are much less than the radius of the sphere
of the solar activity. It is probable that such a change was produced
in the orbit of the comet of 1759, the greater axis of which was not
more than thirty-five times the distance of the Sun from the Earth. A
still greater change was produced in the orbits of the comets of 1770
and of 1805.
If in the zones abandoned by the atmosphere of the Sun, there are any
molecules too volatile to be united to each other, or to the planets,
they ought in their circulation about this star to exhibit all the
appearances of the zodiacal light, without opposing any sensible
resistance to the different bodies of the planetary system, both on
account of their great rarity and also because their motion is very
nearly the same as that of the planets which they meet.
An attentive examination of all the circumstances of this system
renders our hypothesis still more probable. The primitive fluidity of
the planets is clearly indicated by the compression of their figure,
conformably to the laws of the mutual attraction of their molecules; it
is moreover demonstrated by the regular diminution of gravity, as we
proceed from the equator to the poles. This state of primitive fluidity
to which we are conducted by astronomical phenomena, is also apparent
from those which natural history points out. But in order fully to
estimate them, we should take into account the immense variety of
combinations formed by all the terrestial substances which were mixed
together in a state of vapour, when the depression of their temperature
enabled their elements to unite; it is necessary likewise to consider
the wonderful changes which this depression ought to cause in the
interior and at the surface of the earth, in all its productions, in
the constitution and pressure of the atmosphere, in the ocean, and in
all substances which it held in a state of solution. Finally, we should
take into account the sudden changes, such as great volcanic eruptions,
which must at different epochs have deranged the regularity of these
changes. Geology, thus studied under the point of view which connects
it with astronomy, may, with respect to several objects, acquire both
precision and certainty.
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