The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c.Stedman, John, teacher of astronomy
Science
The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c.
Stedman, John, teacher of astronomy
Astronomy -- Juvenile literature -- Early works to 1800
TUTOR. This difficulty will be removed when you consider that all bodies
moving in circles have a constant tendency to fly off from their
centers. Now, as the earth and moon move round their center of gravity,
that part of the earth which is at any time opposite to the moon will
have a greater centrifugal force than the side next her, and at the
earth’s center the centrifugal force exactly balances the attractive
force: therefore, as much water is thrown off by the centrifugal force
on the side opposite to the moon, as is raised on the side next her by
her attraction. Hence, it is plain, that at D, fig. 3, the centrifugal
force must be greater than at the center E, and at E than B, because the
part D is farther from the center of motion than the part B. On the
contrary, the part B being nearer the moon than the center E, the
attracting power must there be strongest, and weakest at D. And, as the
two opposing powers balance each other at the earth’s center, the tides
will rise as high on that side from the moon, by the excess of the
centrifugal force, as they rise on the side next her by the excess of
her attraction.
PUPIL. In this explanation you have mentioned nothing of the sun.
TUTOR. From what I have already said it must be plain to you that if
there were no moon the sun by his attraction would raise a small tide on
the side next him; and, it is as evident that the tides opposite would
be raised as high by the centrifugal force: for the sun and earth, as
well as the earth and moon, move round their center of gravity. This may
be exemplified by an easy experiment. Take a flexible hoop, suppose of
thin brass, tie a string to it and whirl it round your head, and it will
assume an elliptical shape; the tightness of the string drawing out the
side next to your hand, and the centrifugal force throwing off the
other.
PUPIL. This I clearly comprehend.
TUTOR. I shall now refer you to the next figure, (fig. 4.) where F
represents the moon at full: the sun and moon are in opposition, and yet
the tide is as high on each side as in the former case. I wish you to
shew me the cause.
PUPIL. I will use my endeavour to do it, Sir.
TUTOR. Then I doubt not you will accomplish it.
PUPIL. When the moon is at full, ten parts of water are raised from that
side of the earth next her, by her attraction; and, as the side which is
next her is opposite to the sun, three parts must be thrown off by his
centrifugal force, the sum of which will be thirteen parts next the
moon.—From the side opposite to the moon, and under the sun, ten parts
are thrown off by her centrifugal force, and three raised by his
attraction, making thirteen, the same as before.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account