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. TO begin therefore, the reader will remember what has been said
above, that if the moon without the sun would have described an orbit
concentrical to the earth, the action of the sun would make the orbit
oval, and bring the moon nearer to the earth at the new and full,
than at the quarters[268]. Now our excellent author observes, that
if instead of one moon, we suppose a ring of moons, contiguous and
occupying the whole orbit of the moon, his demonstration would still
take place, and prove that the parts of this ring in passing from the
quarter to the conjunction or opposition would be accelerated, and be
retarded again in passing from the conjunction or opposition to the
next quarter. And as this effect does not depend on the magnitude of
the bodies, whereof the ring is composed, the same would hold, though
the magnitude of these moons were so far to be diminished, and their
number increased, till they should form a fluid[269]. Now the earth
turns round continually upon its own center, causing thereby the
alternate change of day and night, while by this revolution each part
of the earth is successively brought toward the sun, and carried off
again in the space of 24 hours. And as the sea revolves round along
with the earth itself in this diurnal motion, it will represent in some
sort such a fluid ring.
19. BUT as the water of the sea does not move round with so much
swiftness, as would carry it about the center of the earth in the
circle it now describes, without being supported by the body of the
earth; it will be necessary to consider the water under three distinct
cases. The first case shall suppose the water to move with the degree
of swiftness, required to carry a body round the center of the
earth disingaged from it in a circle at the distance of the earth’s
semidiameter, like another moon. The second case is, that the waters
make but one turn about the axis of the earth in the space of a month,
keeping pace with the moon; so that all parts of the water should
preserve continually the same situation in respect of the moon. The
third case shall be the real one of the waters moving with a velocity
between these two, neither so swift as the first case requires, nor so
slow as the second.
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