A View of Sir Isaac Newton's PhilosophyPemberton, Henry
Science
A View of Sir Isaac Newton's Philosophy
Pemberton, Henry
Newton, Isaac, 1642-1727. Principia
7. THIS finishes the discoveries made in the action of the primary
planets upon their secondary. The next thing to be shewn is, that the
sun acts upon them likewise: for this purpose it is to be observed,
that if to the motion of the satellite, whereby it would be carried
round its primary at rest, be superadded the same motion both in
regard to velocity and direction, as the primary it self has, it will
describe about the primary the same orbit, with as great regularity,
as if the primary was indeed at rest. The cause of this is that law
of motion, which makes a body near the surface of the earth, when let
fall, to descend perpendicularly, though the earth be in so swift a
motion, that if the falling body did not partake of it, its descent
would be remarkably oblique; and that a body projected describes in
the most regular manner the same parabola, whether projected in the
direction, in which the earth moves, or in the opposite direction, if
the projecting force be the same[185]. From this we learn, that if the
satellite moved about its primary with perfect regularity, besides its
motion about the primary, it would participate of all the motion of its
primary; have the same progressive velocity, with which the primary
is carried about the sun; and be impelled with the same velocity as
the primary towards the sun, in a direction parallel to that impulse
of its primary. And on the contrary, the want of either of these,
in particular of the impulse towards the sun, will occasion great
inequalities in the motion of the secondary planet. The inequalities,
which would arise from the absence of this impulse towards the sun are
so great, that by the regularity, which appears in the motion of the
secondary planets, it is proved, that the sun communicates, the same
velocity to them by its action, as it gives to their primary at the
same distance. For Sir ~ISAAC NEWTON~ informs us, that upon
examination he found, that if any of the satellites of Jupiter were
attracted by the sun more or less, than Jupiter himself at the same
distance, the orbit of that satellite, instead of being concentrical to
Jupiter, must have its center at a greater or less distance, than the
center of Jupiter from the sun, nearly in the subduplicate proportion
of the difference between the sun’s action upon the satellite, and upon
Jupiter; and therefore if any satellite were attracted by the sun but
1/1000 part more or less, than Jupiter is at the same distance, the
center of the orbit of that satellite would be distant from the center
of Jupiter no less than a fifth part of the distance of the outermost
satellite from Jupiter[186]; which is almost the whole distance of the
innermost satellite. By the like argument the satellites of Saturn
gravitate towards the sun, as much as Saturn it self at the same
distance; and the moon as much as the earth.
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