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
We have seen that at the present moment the day is becoming gradually
longer and the moon is steadily receding further and further from the
earth. At present these changes take place with extreme slowness,
but in the primitive periods of which we have already spoken, the
changes in the length of the day, and the changes in the distance
of the moon, proceeded at a rate far more rapid than at present.
As the moon has receded further from the earth its efficiency as a
tide-producer has declined, and consequently the rate at which the
consequences of tidal action have proceeded is continually lessening.
It must therefore be expected that the progress of tidal evolution
in the future will be ever getting slower and slower, so that the
periods of time required for the further development of the phenomena
far exceed those which have elapsed in the course of the history
already given. We can, however, foreshadow what is to happen in the
following manner. The length of the day will slowly increase; and
we can indicate a state of things in the excessively remote future
toward which it may be said the system is tending. The day will grow
until it becomes not merely twenty-five or twenty-six hours, but
until it becomes as long as two or three of our present days. In
fact, as we stretch our imagination through ages so inconceivable
that I forbear to specify any figures which might characterize them,
we seem to discern that the length of the day may go on ever getting
longer and longer until at last a stage is reached when the day is
about fifty or sixty times as long as our present day.
All this time, in accordance with the general law of action and
reaction, the moon must be gradually retreating. As the orbit of
the moon is gradually enlarging, the time that the moon takes to
revolve around the earth must be continually on the increase; from
the present month of twenty-seven days the length of the month will
gradually augment as the ages roll by until at last when the moon
has reached a certain distance the period of its rotation will have
become double what it is at present, or indeed rather more than
double, and we shall have the day and the month equal, each being
about fourteen hundred hours long. When this state of things is
reached, the earth will always turn the same face toward the moon,
just as the moon at present always turns the same face toward the
earth.
Public-domain text, read in full here on John Shaqi.
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