A Preliminary Dissertation on the Mechanisms of the HeavensSomerville, Mary
Science
A Preliminary Dissertation on the Mechanisms of the Heavens
Somerville, Mary
Celestial mechanics
If the moon attracted the centre of gravity of the earth and all its
particles with equal and parallel forces, the whole system of the earth
and the waters that cover it, would yield to these forces with a common
motion, and the equilibrium of the seas would remain undisturbed. The
difference of the forces, and the inequality of their directions, alone
trouble the equilibrium.
It is proved by daily experience, as well as by strict mechanical
reasoning, that if a number of waves or oscillations be excited in a
fluid by different forces, each pursues its course, and has its effect
independently of the rest. Now in the tides there are three distinct
kinds of oscillations, depending on different causes, producing their
effects independently of each other, which may therefore be estimated
separately.
The oscillations of the first kind which are very small, are independent
of the rotation of the earth; and as they depend on the motion of the
disturbing body in its orbit, they are of long periods. The second kind
of oscillations depends on the rotation of the earth, therefore their
period is nearly a day: and the oscillations of the third kind depend on
an angle equal to twice the angular rotation of the earth; and
consequently happen twice in twenty-four hours. The first afford no
particular interest, and are extremely small; but the difference of two
consecutive tides depends on the second. At the time of the solstices,
this difference which, according to Newton's theory, ought to be very
great, is hardly sensible on our shores. La Place has shown that this
discrepancy arises from the depth of the sea, and that if the depth were
uniform, there would be no difference in the consecutive tides, were it
not for local circumstances: it follows therefore, that as this
difference is extremely small, the sea, considered in a large extent,
must be nearly of uniform depth, that is to say, there is a certain mean
depth from which the deviation is not great. The mean depth of the
Pacific Ocean is supposed to be about four miles, that of the Atlantic
only three. From the formulæ which determine the difference of the
consecutive tides it is also proved that the precession of the
equinoxes, and the nutation in the earth's axis, are the same as if the
sea formed one solid mass with the earth.
The third kind of oscillations are the semidiurnal tides, so remarkable
on our coasts; they are occasioned by the combined action of the sun and
moon, but as the effect of each is independent of the other, they may be
considered separately.
Public-domain text, read in full here on John Shaqi.
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