Lord Kelvin: An account of his scientific life and workGray, Andrew
Science
Lord Kelvin: An account of his scientific life and work
Gray, Andrew
Kelvin, William Thomson, Baron, 1824-1907
If then the earth be rotating more and more slowly, as time goes on, at
present, it must have been rotating more rapidly in past time. A
thousand million years ago, at the present rate of retardation, the
earth must have been rotating one seventh part of its speed faster than
it is rotating at present, and this would give for centrifugal force at
the surface one thousand million years ago, greater than the centrifugal
force at present, in the ratio of 64 to 49. Apparently therefore the
earth must have solidified at a much later date than that epoch, a date
when it was rotating much more nearly with the angular speed which it
has now; otherwise the figure of the earth would have deviated much more
from the spherical form than it actually does. On the other hand, one
hundred million years ago centrifugal force would be only three per
cent. greater than it is at present, and consolidation of the earth at
that less remote period would give a shape to the earth not very
different from that which it now possesses. The argument therefore from
tidal retardation would cut down the time available for geological and
biological changes to something not much more than one hundred million
years, perhaps to less.
A second argument for limitation of the time available for such
processes is derived from the sun's heat. The sun cannot be regarded as
a miraculous body producing its light and heat from nothing. Changes of
the constitution of the sun must be continually proceeding, to account
for its enormous radiation of energy into space, a radiation of which
only an infinitesimal part is received by the bodies of the solar
system, and a still more minute portion by the earth. The effects of the
sun's light and heat on the earth show how enormous must be the quantity
of energy lost from the sun in a year. How is this loss of energy to be
accounted for? What is the physical change which gives rise to it? In
1854 Thomson put forward the theory that the sun's heat is kept up by
the falling in of meteors on the sun's surface, but he afterwards saw
reason to abandon that view. Helmholtz had advocated the theory that the
sun was a body heated by the coming together of the matter composing it
by its mutual attraction, a process which, although the sun is now a
continuous mass, is to be regarded as still going on. It is easy to
calculate the exhaustion of potential energy caused by the coming
together of the matter of the sun from universal dispersion through
infinite space to a sphere of uniform density of the present size of the
sun. The result is about as much energy as would be generated by burning
seven million million million million million tons of coal. The amount
radiated in each hour is about as much as would be generated by burning
something like nine tons of coal every hour on every square yard of the
sun's surface. It is certain that the sun must be still contracting, and
if it contracts sufficiently to just make good this expenditure by the
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