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
443. That no very irregular figure is found among the planetary bodies,
may therefore be considered as a proof of the universality of that
system of waste and reconsolidation that we have been endeavouring to
trace in the natural history of the earth. A farther proof of the same
arises from considering, that for every given mass of matter, having a
given period of rotation, there are two different spheroids that answer
the conditions of establishing an equilibrium among its parts, the one
near to the sphere, and the other very distant from it, and so oblate
as to have a lenticular form. Thus the earth, supposing it homogeneous,
might either be in equilibrium, by means of the figure which it
actually has, or of one in which the polar was to the equatorial
diameter as 1 to 768. The same is true of the other planets; and yet we
no where find that this highly compressed spheroid is actually employed
by nature. The reason, no doubt, is, that in so oblate a spheroid, the
equilibrium between the gravitating and the centrifugal force is of
the kind that does not re-establish itself when disturbed; so that the
parts let loose, and not kept in their place by firm cohesion, would
fly off altogether. In such a body, the waste at the surface would
lead to an entire change of form, and therefore the constitution here
supposed could not be permanent.
444. In the system of Saturn, we have a great deviation from the
general order, which, nevertheless, has led to a very unexpected
verification of some of the conclusions deduced above. A principle
extremely like that which is the basis of all the foregoing reasonings,
led one of the greatest philosophers of the present age to discover
the revolution of Saturn's ring on its axis, and even to determine
the velocity of that revolution, such as it has been since found by
observation. LA PLACE, laying it down as a maxim, that nothing in
nature can exist, where there are causes of change, not balanced or
compensated by other causes,[234] concluded, that the-parts of the
ring must be held from falling down to the body of the planet by some
other force than their mere cohesion to one another. Were it otherwise,
every particle detached from the ring, by any means, must descend in a
straight line, almost perpendicular to the surface of Saturn; and the
final destruction of the ring must be inevitable. The only force that
could balance this effect of gravitation, seemed to be a centrifugal
force, arising from the rotation of the ring on an axis passing through
its centre, and perpendicular to its plane. La Place proceeded to
inquire what celerity of rotation was adequate to this effect, and
found that one of ten hours and a quarter would be required, which
is almost precisely the time afterwards determined by Dr HERSCHEL
from actual observation. If, with this rotation, the ring is a solid
annulus generated by the rotation of a very flat ellipsis about a given
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