The story of the universe. Volume 2 (of 4) : $b The earth : land and sea
History
The story of the universe. Volume 2 (of 4) : $b The earth : land and sea
Astronomy; Earth (Planet); Natural history
In the course of such vast ages the reaction of the earth on
the moon’s orbit has not only become perceptible, it has become
conspicuous; it has not only become conspicuous, but it has become
the chief determining agent in making the moon’s orbit as we find it
at the present day. We have seen that as we look into the past the
length of the day seems ever shorter and shorter; and concurrent with
this decline in the day is the diminution in the moon’s distance from
the earth. There was a time when the moon, instead of revolving at
a distance of two hundred and forty thousand miles, as it does at
present, revolved at a distance of only two hundred thousand miles.
As we think of epochs still earlier we discern the moon ever closer
and closer to the earth, until at last, at that critical time in
the history of the earth-moon system, when the earth was quickly
revolving in a period of a few hours, our satellite seems to have
been quite close to the earth; in fact, the two bodies were almost in
contact
The study of the tides has therefore conducted us to the knowledge
of a remarkable configuration exhibited in the primitive earth-moon
system. The earth was then spinning round rapidly in a day which
was only a few hours long, while close to the earth, or almost in
contact with it, the moon coursed around our globe, the period of
its revolution being shorter to such an extent that the satellite
completed its circuit in the same time as the earth required for one
turn round its axis.
We must remember that the materials destined to form the pair of
allied planets did not then form two solid bodies as they do at
present; they were both, in all probability, incandescent masses
glowing with fervor, and soft, if not actually molten, or incoherent,
or even gaseous. These aggregations were close together, and one of
them was whirling around the other in a period of a few hours, the
duration of that period being equal to the time in which the larger
mass revolved on its axis. In fact, the two objects, even though
distinct, seem to have revolved the one around the other as if they
had been bound together by rigid bonds. The rapid rotation with which
they were animated suggests a cause for this state of things. It is
well known that a fly-wheel, when driven at an unduly high speed,
is liable to break asunder in consequence of its rapid motion. If a
grindstone be urged around with excessive velocity the force tending
to rend the stone into fragments may overcome its cohesion, and it
will fly into pieces, often projected with such violence that fearful
accidents have been the consequence.
Public-domain text, read in full here on John Shaqi.
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