Newton's Principia : $b The mathematical principles of natural philosophyNewton, Isaac
General
Newton's Principia : $b The mathematical principles of natural philosophy
Newton, Isaac
Celestial mechanics -- Early works to 1800; Mechanics -- Early works to 1800
COR. 20. If, now, the annulus becomes hard, and the globe is
diminished, the motion of flux and reflux will cease; but the
oscillating motion of the inclination and the præcession of the nodes
will remain. Let the globe have the same axis with the annulus, and
perform its revolutions in the same times, and at its surface touch
the annulus within, and adhere to it; then the globe partaking of the
motion of the annulus, this whole compages[Pg 213] will oscillate, and the
nodes will go backward, for the globe, as we shall shew presently, is
perfectly indifferent to the receiving of all impressions. The greatest
angle of the inclination of the annulus single is when the nodes are in
the syzygies. Thence in the progress of the nodes to the quadratures,
it endeavours to diminish its inclination, and by that endeavour
impresses a motion upon the whole globe. The globe retains this motion
impressed, till the annulus by a contrary endeavour destroys that
motion, and impresses a new motion in a contrary direction.
And by this means the greatest motion of the decreasing inclination
happens when the nodes are in the quadratures, and the least angle
of inclination in the octants after the quadratures; and, again,
the greatest motion of reclination happens when the nodes are in
the syzygies; and the greatest angle of reclination in the octants
following. And the case is the same of a globe without this annulus,
if it be a little higher or a little denser in the equatorial than in
the polar regions; for the excess of that matter in the regions near
the equator supplies the place of the annulus. And though we should
suppose the centripetal force of this globe to be any how increased, so
that all its parts were to tend downwards, as the parts of our earth
gravitate to the centre, yet the phænomena of this and the preceding
Corollary would scarce be altered; except that the places of the
greatest and least height of the water will be different; for the water
is now no longer sustained and kept in its orbit by its centrifugal
force, but by the channel in which it flows. And, besides, the force
LM attracts the water downwards most in the quadratures, and the force
KL or NM - LM attracts it upwards most in the syzygies. And these
forces conjoined cease to attract the water downwards, and begin to
attract it upwards in the octants before the syzygies; and cease to
attract the water upwards, and begin to attract the water downwards in
the octants after the syzygies. And thence the greatest height of the
water may happen about the octants after the syzygies; and the least
height about the octants after the quadratures; excepting only so far
as the motion of ascent or descent impressed by these forces may by the
vis insita of the water continue a little longer, or be stopped
a little sooner by impediments in its channel.
Public-domain text, read in full here on John Shaqi.
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