Classics of modern science : $b (Copernicus to Pasteur)
History
Classics of modern science : $b (Copernicus to Pasteur)
Science; Science -- History
Each of these bodies excites, by its attraction upon the waters of the
sea, two gigantic waves, which flow in the same direction round the
world, as the attracting bodies themselves apparently do. The two waves
of the moon, on account of her greater nearness, are about three and a
half times as large as those excited by the sun. One of these waves has
its crest on the quarter of the earth’s surface which is turned towards
the moon, the other is at the opposite side. Both these quarters
possess the flow of the tide, while the regions which lie between have
the ebb. Although in the open sea the height of the tide amounts to
only about three feet, and only in certain narrow channels, where the
moving water is squeezed together, rises to thirty feet, the might of
the phenomena is nevertheless manifest from the calculation of Bessel,
according to which a quarter of the earth covered by the sea possesses,
during the flow of the tide, about 25,000 cubic miles of water more
than during the ebb, and that therefore such a mass of water must, in
six and a quarter hours, flow from one quarter of the earth to the
other.
The phenomena of the ebb and flow, as already recognized by Mayer,
combined with the law of the conservation of force, stand in remarkable
connection with the question of the stability of our planetary system.
The mechanical theory of the planetary motions discovered by Newton
teaches, that if a solid body in absolute vacuo, attracted by the sun,
move around him in the same manner as the planets, this motion will
endure unchanged through all eternity.
Now we have actually not only one, but several such planets, which
move around the sun, and by their mutual attraction create little
changes and disturbances in each other’s paths. Nevertheless Laplace,
in his great work, the _Mecanique Celeste_, has proved that in
our planetary system all these disturbances increase and diminish
periodically, and can never exceed certain limits, so that by this
cause the external existence of the planetary system is unendangered.
Public-domain text, read in full here on John Shaqi.
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