Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
The solid earth is represented surrounded by a shell of water. The
water on the side toward the moon is more attracted than the centre
of the earth, C; the water on the opposite side is less attracted.
The lines of force from the moon to the parts of the water lying
toward A and B are inclined to the direct line between the centres
of the earth and the moon, and the forces acting along these lines
tend to draw the water in the directions shown by the arrow points.
These are resultants of the horizontal and vertical components of
the moon's attraction at the corresponding points on the earth, and
the force acting along them tends to increase the weight of the
water wherever the lines are inclined more toward the centre of the
earth than toward the moon. On the side opposite the moon the same
effects are produced in reverse, because on that side the general
tendency is to draw the earth away from the water. Consequently if
the earth did not rotate, and if it were surrounded with a complete
shell of water, the latter would be drawn into an ellipsoidal shape,
with the highest points under and opposite to the moon, and the
lowest at the extremities of the diameter lying at right angles to
the direction of
the moon.
]
Some persons, when this statement is made, inquire: “Why, then, does not
the moon take the water entirely away from the earth?” The answer is,
that the effect of the tidal force is simply to diminish very slightly
the weight of the water, or its tendency towards the earth's centre, but
not to destroy, or overmaster, the gravitational control of the earth.
The water retains nearly all its weight, for the tidal force of the moon
diminishes it less than one part in 8,000,000. Still, this slight
diminution is sufficient to cause the water to swell a little above its
general level, at the points where it feels the effect of the tidal
force. On the other hand, around that part of the earth which is
situated half-way between the two tides, or along a diameter at right
angles to the direction of the moon, the latter's attraction _increases_
the weight of the water, _i. e._, its tendency toward the earth's centre
(see Fig. 6). Perhaps this can better be understood, if we imagine the
earth to be entirely liquid. In that case the difference in the force of
the moon's attraction with difference of distance would be manifested in
varying degrees throughout the earth's whole frame, and the result would
be to draw the watery globe out into an ellipsoidal figure, having its
greatest diameter in the line of the moon's attraction, and its smallest
diameter at right angles to that line. The proportions of the ellipsoid
would be such that the forces would be in equilibrium.
Public-domain text, read in full here on John Shaqi.
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