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
these places eastward or westward caused by the moon, is about 8⅔ feet.
21. THUS the difference of height in this latter supposition is little
short of twice that difference in the preceding. But the case of the
sea is a middle between these two: for a body, which should revolve
round the center of the earth at the distance of a semidiameter without
pressing on the earth’s surface, must perform its period in less than
an hour and half, whereas the earth turns round but once in a day; and
in the case of the waters keeping pace with the moon it should turn
round but once in a month: so that the real motion of the water is
between the motions required in these two cases. Again, if the waters
moved round as swiftly as the first case required, their weight would
be wholly taken off by their motion; for this case supposes the body
to move so, as to be kept revolving in a circle round the earth by
the power of gravity without pressing on the earth at all, so that
its motion just supports its weight. But if the power of gravity had
been only 1/289 part of what it is, the body could have moved thus
without pressing on the earth, and have been as long in moving round,
as the earth it self is. Consequently the motion of the earth takes off
from the weight of the water in the middle between the poles, where
its motion is swiftest, 1/289 part of its weight and no more. Since
therefore in the first case the weight of the waters must be intirely
taken off by their motion, and by the real motion of the earth they
lose only 1/289 part thereof, the motion of the water will so little
diminish their weight, that their figure will much nearer resemble
the case of their keeping pace with the moon than the other. Upon
the whole, if the waters moved with the velocity necessary to carry
a body round the center of the earth at the distance of the earth’s
semidiameter without bearing on its surface, the water would be lowest
under the moon, and rise gradually as it moved on with the earth
eastward, till it came half way toward the place opposite to the moon;
from thence it would subside again, till it came to the opposition,
where it would become as low as at first; afterwards it would rise
again, till it came half way to the place under the moon; and from
hence it would subside, till it came a second time under the moon. But
in case the water kept pace with the moon, it would be highest where
in the other case it is lowest, and lowest where in the other it is
highest; therefore the diurnal motion of the earth being between the
motions of these two cases, it will cause the highest place of the
water to fall between the places of the greatest height in these two
cases. The water as it passes from under the moon shall for some time
rise, but descend again before it arrives half way to the opposite
place, and shall come to its least height before it becomes opposite
to the moon; then it shall rise again, continuing so to do till it has
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