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
385. The assertion that, in the planetary motions, we discover no
mark, either of the commencement or termination of the present order,
refers to the late discoveries of LA GRANGE and LA PLACE, which have
contributed so much to the perfection of physical astronomy. From
the principle of universal gravitation, these mathematicians have
demonstrated, that all the variations in our system are periodical;
that they are confined within certain limits; and consist of alternate
diminution and increase. The orbits of the planets change not only
their position, but even their magnitude and their form: the longer
axis of each has a slow angular motion; and, though its length remains
fixed, the shorter axis increases and diminishes, so that the form of
the orbit approaches to that of a circle, and recedes from it by turns.
In the same manner, the obliquity of the ecliptic, and the inclination
of the planetary orbits, are subject to change; but the changes are
small, and, being first in one direction, and then in the opposite,
they can never accumulate so as to produce a permanent or a progressive
alteration. Thus, in the celestial motions, no room is left for the
introduction of disorder; no irregularity or disturbance, arising from
the mutual action of the planets, is permitted to increase beyond
certain limits, but each of them, in time, affords a correction for
itself. The general order is constant, in the midst of the variation of
the parts; and, in the language of La Place, there is a certain mean
condition, about which our system perpetually _oscillates_ performing
small vibrations on each side of it, and never receding from it
far.[199] The system is thus endowed with a stability, which can refill
the lapse of unlimited duration; it can only perish by an external
cause, and by the introduction of laws, of which at present no vestige
is to be traced.
[Footnote 199: Exposition du Systéme du Monde, par La Place, Livre iv.
chap. 6. p. 199. 2d edit.]
386. The same _calculus_ to which we are indebted for these sublime
conclusions, informs us of two circumstances, which mark the law
here treated of as an effect of wise design, to the entire exclusion
both of necessity and chance. One of these circumstances consists in
the planetary motions being all in the same direction, or all _in
consequentia_ as it is called by the astronomers. This is essential
to the compensation and stability above mentioned:[200] had one planet
circulated round the sun in a direction from east to west, and another
in a direction from west to east, the disturbances they would have
produced on one another's motion would not necessarily have been
periodical; their irregularities might have continually increased, and
they might have deviated in the course of ages from their original
condition, beyond any limits that can be assigned.
[Footnote 200: La Place, _ibid._]
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