The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
that it now retains no more than a sixteenth of that amount. We know
also precisely how much was absorbed in the removal of the moon, and the
balance can be evaluated in heat. It can be shown, and the fact is a
very striking one, that the quantity of heat thus arising would be
sufficient to account many times over for the internal heat of the
earth. It might therefore be urged plausibly that the internal heat
which we actually find has had its origin in this way. And if this were
the case the argument which we are using in favour of the nebular origin
of the earth, would be, of course, invalidated.
We may state the issue in a slightly different manner, as follows. Heat
there is undoubtedly in the earth; that heat might have come from the
primæval nebula as we have supposed, and as in actual fact it did come.
But apparently it might have come from the tidal friction. Why then are
we entitled to reject the latter view, and say that the tidal friction
will not explain the internal heat, and why are we compelled to fall
back on the only other explanation?
Lord Kelvin suggested a test for deciding to which of these two sources
the earth’s internal heat was to be attributed. Professor G. H. Darwin
applied the test and decided the issue. We have dwelt upon the rate at
which the heat increases with the descent, this rate being about one
degree every sixty-six feet. Now the distribution of the heat, if it had
come from the tidal action, would be quite different from the
distribution which would result from the gradual efflux of heat from the
centre in the process of cooling. And, speaking quite generally, we may
surmise that the heat produced by tidal friction would be distributed
rather more towards the exterior of the earth than at its centre. We
might therefore reasonably expect that if the internal heat of the earth
arose from tidal friction it would be more uniformly distributed
throughout the globe, and there would not be so great a contrast between
the high temperature of the interior and the lesser temperatures near
the surface as there is when the heat distribution is merely the result
of cooling. It has been proved that if the internal heat had its origin
from the tidal friction, the rate of increase with the depth would be
totally different from what it is actually found to be. It would be
necessary to go down 2,000 feet to obtain an increase of one degree,
instead of only sixty-six feet, as is actually the case.
Public-domain text, read in full here on John Shaqi.
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