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
passed the place opposite to the moon, but subside before it comes
to the middle between the places opposite to and under the moon; and
lastly it shall come to its lowest, before it comes a second time
under the moon. If A (in fig. 112, 113, 114.) represent the moon, B
the center of the earth, the oval C D E F in fig. 112. will represent
the situation of the water in the first case; but if the water kept
pace with the moon, the line C D E F in fig. 113. would represent
the situation of the water; but the line C D E F in fig. 114. will
represent the same in the real motion of the water, as it accompanies
the earth in its diurnal rotation: in all these figures C and E being
the places where the water is lowest, and D and F the places where it
is highest. Pursuant to this determination it is found, that on the
shores, which lie exposed to the open sea, the high water usually falls
out about three hours after the moon has passed the meridian of each
place.
22. LET this suffice in general for explaining the manner, in which the
moon acts upon the seas. It is farther to be noted, that these effects
are greatest, when the moon is over the earth’s equator[274], that
is, when it shines perpendicularly upon the parts of the earth in the
middle between the poles. For if the moon were placed over either of
the poles, it could have no effect upon the water to make it ascend and
descend. So that when the moon declines from the equator toward either
pole, it’s action must be something diminished, and that the more, the
farther it declines. The tides likewise will be greatest, when the moon
is nearest to the earth, it’s action being then the strongest.
23. THUS much of the action of the moon. That the sun should produce
the very same effects, though in a less degree, is too obvious to
require a particular explanation: but as was remarked before, this
action of the sun being weaker than that of the moon, will cause the
tides to follow more nearly the moon’s course, and principally shew it
self by heightening or diminishing the effects of the other luminary.
Which is the occasion, that the highest tides are found about the
conjunction and opposition of the luminaries, being then produced by
their united action, and the weakest tides about the quarters of the
moon; because the moon in this case raising the water where the sun
depresses it, and depressing it where the sun raises it, the stronger
action of the moon is in part retunded and weakened by that of the sun.
Our author computes that the sun will add near two feet to the height
of the water in the first case, and in the other take from it as much.
However the tides in both comply with the same hour of the moon. But at
other times, between the conjunction or opposition and quarters, the
time deviates from that forementioned, towards the hour in which the
sun would make high water, though still it keeps much nearer to the
moon’s hour than to the sun’s.
Public-domain text, read in full here on John Shaqi.
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