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
But if the nodes are situate at the octants after the quadratures,
that is, between C and A, D and B, it will appear, from what was
just now shewn, that in the passage of the body P from either node
to the ninetieth degree from thence, the inclination of the plane
is perpetually diminished; then, in the passage through the next
45 degrees to the next quadrature, the inclination is increased;
and afterwards, again, in its passage through another 45 degrees
to the next node, it is diminished. Therefore the inclination is
more diminished than increased, and is therefore always less in the
subsequent node than in the preceding one. And, by a like reasoning,
the inclination is more increased than diminished when the nodes
are in the other octants between A and D, B and C. The inclination,
therefore, is the greatest of all when the nodes are in the syzygies
In their passage from the syzygies to the quadratures the inclination
is diminished at each appulse of the body to the nodes; and becomes
least of all when the nodes are in the quadratures, and the body in the
syzygies; then it increases by the same degrees by which it decreased
before; and, when the nodes come to the next syzygies, returns to its
former magnitude.
COR. 11. Because when the nodes are in the quadratures the body P is
perpetually attracted from the plane of its orbit; and because this
attraction is made towards S in its passage from the node C through the
conjunction A to the node D; and to the contrary part in its passage
from the node D through the opposition B to the node C; it is manifest
that, in its motion from the node C, the body recedes continually from
the former plane CD of its orbit till it comes to the next node; and
therefore at that node, being now at its greatest distance from the
first plane CD, it will pass through the plane of the orbit EST not
in D, the other node of that plane, but in a point that lies nearer
to the body S, which therefore becomes a new place of the node in
antecedentia to its former place. And, by a like reasoning, the
nodes will continue to recede in their passage from this node to the
next. The nodes, therefore, when situate in the quadratures, recede
perpetually; and at the syzygies, where no perturbation can be produced
in the motion as to latitude, are quiescent: in the intermediate
places they partake of both conditions, and recede more slowly; and,
therefore, being always either retrograde or stationary, they will be
carried backwards, or in antecedentia, each revolution.
COR. 12. All the errors described in these corollaries are a little
greater[Pg 210] at the conjunction of the bodies P, S, than at their
opposition; because the generating forces NM and ML are greater.
Public-domain text, read in full here on John Shaqi.
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