THE TIDES.

London _Nature_, in a recent issue, says: From a scientific point of

view, the work done by the tides is of unspeakable importance. Whence is

this energy derived with which the tides do their work? If the tides are

caused by the moon, the energy they possess must also be derived from

the moon. This looks plain enough, but unfortunately it is not true.

Would it be true to assert that the finger of the rifleman which pulls

the trigger supplies the energy with which the rifle bullet is animated?

Of course it would not. The energy is derived from the explosion of

gunpowder, and the pulling of the trigger is merely the means by which

that energy is liberated.

In somewhat similar manner the tidal wave produced by the moon is the

means whereby a part of the energy stored in the earth is compelled to

expend itself in work. Let me illustrate this by a comparison between

the earth rotating on its axis and the fly-wheel of an engine: The fly

wheel is a sort of reservoir, into which the engine pours its power at

each stroke of the piston. The various machines in the mill merely draw

off the power from the store accumulated in the fly-wheel. The earth

is like a gigantic fly-wheel detached from the engine, though still

connected with the machines in the mill. In that mighty fly-wheel a

stupendous quantity of energy is stored up, and a stupendous quantity of

energy would be given out before that fly-wheel would come to rest. The

earth's rotation is a reservoir from whence the tides draw the energy

they require for doing work. Hence it is that though the tides are

caused by the moon, yet whenever they require energy they draw on the

supply ready to hand in the rotation of the earth. The earth differs

from the fly-wheel of an engine in a very important point. As the energy

is withdrawn from the fly-wheel by the machines in the mill, so it is

restored thereto by the power of the steam engine, and the fly runs

uniformly. But the earth is merely the fly-wheel without the engine.

When the work by the tides withdraws energy from the earth, that energy

is never restored. It, therefore, follows that the earth's rotation

must be decreasing. This leads to a consequence of the most wonderful

importance. It tells us that the speed with which the earth rotates on

its axis is diminishing. We can state the result in a manner which has

the merits of simplicity and brevity. The tides are increasing the

length of the day. At present, no doubt, the effect of the tides

in changing the length of the day is very small. A day now is not

appreciably longer than a day a hundred years ago. Even in a thousand

years the change in the length of the day is only a fraction of a

second. But the importance arises from the fact that the change, slow

though it is, lies always in one direction. The day is continually

increasing. In millions of years the accumulated effect becomes not only

appreciable, but even of startling magnitude.

The change in the length of the day must involve a corresponding change

in the motion of the moon. If the moon acts on the earth and retards the

rotation of the earth, so, conversely, does the earth react upon the

moon. The earth is tormented by the moon, so it strives to drive away

its persecutor. At present the moon revolves around the earth at a

distance of about 240,000 miles. The reaction of the earth tends to

increase this distance, and to force the moon to revolve in an orbit

which is continually growing larger and larger. As thousands of years

roll on, the length of the day increases second by second, and the

distance of the moon increases mile by mile. A million years ago the

day, probably, contained some minutes less than our present day of

twenty-four hours. Our retrospect does not halt here; we at once project

our view back to an incredibly remote epoch which was a crisis in the

history of our system. It must have been at least 50,000,000 years ago.

It may have been very much earlier. This crisis was the interesting

occasion when the moon was born. The length of the day was only a very

few hours. If we call it three hours we shall not be far from the truth.

Purhaps you may think that if we looked back to a still earlier epoch,

the day would become still less, and finally disappear altogether. This

is, however, not the case. The day can never have been much less than

three hours in the present order of things. Everybody knows that the

earth is not a sphere, but there is a protuberance at the equator, so

that, as our school books tell us, the earth is shaped like an orange.

It is well known that this protuberance is due to the rotation of

the earth on its axis, by which the equatorial parts bulge out by

centrifugal force. The quicker the earth rotates the greater is the

protuberance. If, however, the rate of rotation exceeds a certain limit,

the equatorial portion of the earth could no longer cling together. The

attraction which unites them would be overcome by centrifugal force, and

a general break up would occur. It can be shown that the rotation of the

earth, when on the point of rupture, corresponds to a length of the day

somewhere about the critical value of three hours, which we have already

adopted. It is, therefore, impossible for us to suppose a day much

shorter than three hours.

Let us leave the earth for a few minutes and examine the past history

of the moon. We have seen the moon revolve around the earth in an

ever-widening orbit, and consequently the moon must, in ancient times,

have been nearer the earth than it is now. No doubt the change is slow.

There is not much difference between the orbit of the moon a thousand

years ago and the orbit in which the moon is now moving. But when we

rise to millions of years, the difference becomes very appreciable.

Thirty or forty millions of years ago the moon was much closer to the

earth than it is at present; very possibly the moon was then only half

its present distance. We must, however, look still earlier, to a certain

epoch not less than fifty million of years ago. At that epoch the moon

must have been so close to the earth that the two bodies were almost

touching. Everybody knows that the moon revolves now around the earth

in a period of twenty-seven days. The period depends upon the distance

between the earth and the moon. In earlier times the month must have

been shorter than our present month. Some millions of years ago the moon

completed its journey in a week instead of taking twenty-eight days as

at present. Looking back earlier still, we find the month has dwindled

down to a day, then down to a few hours, until at that wondrous epoch

when the moon was almost touching the earth, the moon spun around the

earth once every three hours.

In those ancient times I see our earth to be a noble globe, as it is as

present. Yet it is not partly covered with oceans and partly clothed

with verdure. The primeval earth seems rather a fiery and half-molten

mass, where no organic life can dwell. Instead of the atmosphere which

we now have, I see a dense mass of vapors in which perhaps, all the

oceans of the earth are suspended as clouds. I see that the sun still

rises and sets to give the succession of day and of night, but the

day and the night together only amounted to three hours, instead of

twenty-four. Almost touching the chaotic mass of the earth is another

much smaller and equally chaotic body. Around the earth I see this small

body rapidly rotating, the two revolving together, as if they were bound

by invisible bands. The smaller body is the moon.

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Scientific American Supplement, No. 324, March 18, 1882 · 第 42 / 50 题