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
18. ANOTHER effect of the sun’s action, consequent upon this we have
now explained, is, that though the moon undisturbed by the sun might
move in a circle having the earth for its center; by the sun’s action,
if the earth were to be in the very middle or center of the moon’s
orbit, yet the moon would be nearer the earth at the new and full, than
in the quarters. In this probably will at first appear some difficulty,
that the moon should come nearest to the earth, where it is least
attracted to it, and be farthest off when most attracted. Which yet
will appear evidently to follow from that very cause, by considering
what was last shewn, that the orbit of the moon in the conjunction
and opposition is rendred less curve; for the less curve the orbit of
the moon is, the less will the moon have descended from the place it
would move into, without the action of the earth. Now if the moon were
to move from any place without farther disturbance from that action,
since it would proceed in the line, which would touch its orbit in that
place, it would recede continually from the earth; and therefore if
the power of the earth upon the moon, be sufficient to retain it at the
same distance, this diminution of that power will cause the distance
to increase, though in a less degree. But on the other hand in the
quarters, the moon, being pressed more towards the earth than by the
earth’s single action, will be made to approach it; so that in passing
from the conjunction or opposition to the quarters the moon ascends
from the earth, and in passing from the quarters to the conjunction and
opposition it descends again, becoming nearer in these last mentioned
places than in the other.
19. ALL these forementioned inequalities are of different degrees,
according as the sun is more or less distant from the earth; greater
when the earth is nearest the sun, and less when it is farthest off.
For in the quarters, the nearer the moon is to the sun, the greater is
the addition to the earth’s action upon it by the power of the sun; and
in the conjunction and opposition, the difference between the sun’s
action upon the earth and upon the moon is likewise so much the greater.
Public-domain text, read in full here on John Shaqi.
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