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
20. IN the first case the waters, like the body which they equalled
in velocity, by the action of the moon would be brought nearer the
center under and opposite to the moon, than in the parts in the middle
between these eastward or westward. That such a body would so alter
its distance by the moon’s action upon it, is clear from what has
been mentioned of the like changes in the moon’s motion caused by
the sun[270]. And computation shews, that the difference between the
greatest and least distance of such a body would not be much above 4½
feet. But in the second case, where all the parts of the water preserve
the same situation continually in respect of the moon, the weight of
those parts under and opposite to the moon will be diminished by the
moon’s action, and the parts in the middle between these will have
their weight increased: this being effected just in the same manner,
as the sun diminishes the attraction of the moon towards the earth in
the conjunction and opposition, but increases that attraction in the
quarters. For as the first of these consequences from the sun’s action
on the moon is occasioned by the moon’s being attracted by the sun in
the conjunction more than the earth, and in the opposition less than
it, and therefore in the common motion of the earth and moon, the moon
is made to advance toward the sun in one case too fast, and in the
other is left as it were behind; so the earth will not have its middle
parts drawn towards the moon so strongly as the nearer parts, and yet
more forcibly than the remotest: and therefore since the earth and
moon move each month round their common center of gravity[271], while
the earth moves round this center, the same effect will be produced,
on the parts of the water nearest to that center or to the moon, as
the moon feels from the sun when in conjunction, and the water on the
contrary side of the earth will be affected by the moon, as the moon is
by the sun, when in opposition[272]; that is, in both cases the weight
of the water, or its propensity towards the center of the earth, will
be diminished. The parts in the middle between these will have their
weight increased, by being pressed towards the center of the earth
through the obliquity of the moon’s action upon them to its action
upon the earth’s center, just as the sun increases the gravitation
of the moon in the quarters from the same cause[273]. But now it is
manifest, that where the weight of the same quantity of water is least,
there it will be accumulated; while the parts, which have the greatest
weight, will subside. Therefore in this case there would be no tide or
alternate rising and falling of the water, but the water would form it
self into an oblong figure, whose axis prolonged would pass through the
moon. By Sir ~ISAAC NEWTON~’s computation the excess of this axis above
the diameters perpendicular to it, that is, the height of the waters
under and opposite to the moon above their height in the middle between
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