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
Now, therefore, in the system of the bodies T, P, S, when the apsides
of the orbit PAB are in the quadratures, the ratio of that increase
and decrease is least of all, and becomes greatest when the apsides
are in the syzygies. If the apsides are placed in the quadratures, the
ratio near the apsides is less, and near the syzygies greater, than the
duplicate ratio of the distances; and from that greater ratio arises a
direct motion of the line of the apsides, as was just now said. But if
we consider the ratio of the whole increase or decrease in the progress
between the apsides, this is less than the duplicate ratio of the
distances. The force in the lower is to the force in the upper apsis in
less than a duplicate ratio of the distance of the upper apsis from the
focus of the ellipsis to the distance of the lower apsis from the same
focus; and, contrariwise, when the apsides are placed in the syzygies,
the force in the lower apsis is to the force in the upper apsis in a
greater than a duplicate ratio of the distances. For the forces LM in
the quadratures added to the forces of the body T compose forces in a
less ratio; and the forces KL in the syzygies subducted from the forces
of the body T, leave the forces in a greater ratio. Therefore the ratio
of the whole increase and decrease in the passage between the apsides
is least at the quadratures and greatest at the syzygies; and therefore
in the passage of the apsides from the quadratures to the syzygies
it is continually augmented, and increases the eccentricity of the
ellipsis; and in the passage from the syzygies to the quadratures it is
perpetually decreasing, and diminishes the eccentricity.
COR. 10. That we may give an account of the errors as to latitude,
let us suppose the plane of the orbit EST to remain immovable; and
from the cause of the errors above explained, it is manifest, that,
of the two forces NM, ML, which are the only and entire cause of
them, the force ML acting always in the plane of the orbit PAB never
disturbs the motions as to latitude; and that the force NM, when
the nodes are in the syzygies, acting also in the same plane of the
orbit, does not at that time affect those motions. But when the nodes
are in the quadratures, it disturbs them very much, and, attracting
the body P perpetually out of the plane of its orbit, it diminishes
the inclination of the plane in the passage of the body from the
quadratures to the syzygies, and again increases the same in the
passage from the syzygies to the quadratures. Hence it comes to pass
that when the body is in the syzygies, the inclination is then least of
all, and returns to the first magnitude nearly, when the body[Pg 209] arrives
at the next node.
Public-domain text, read in full here on John Shaqi.
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