The Book of History (Vol. 1 of 18): A History of All Nations from the Earliest Times to the PresentVarious
History
The Book of History (Vol. 1 of 18): A History of All Nations from the Earliest Times to the Present
Various
World history
It became obviously a question of the first importance to discover
what proportion of the earth’s crust consists of radium, and an
investigation was undertaken for this purpose by the Hon. R. J.
Strutt, who finds that the rocks composing the earth’s crust contain
a superabundance of radium--sufficient, if this element is uniformly
distributed through the whole earth in the same proportion as it occurs
at the surface, not only to make good the heat which is radiated away
into space, but actually to raise the temperature of our planet, which,
on this evidence, should, therefore, be growing not colder, but hotter.
This is a result as disconcerting at first sight as it is astonishing,
and its effects are very wide-reaching. Of course, it completely
destroys the validity of Lord Kelvin’s argument, but it also deprives
the nebular hypothesis of one of its cherished lines of evidence--a
loss which the force of the general argument enables us to bear with
equanimity.
[Sidenote: On the Eve of great Events]
In any case, the vast body of facts bearing on the history of the earth
suffices to show that its temperature cannot be rising. Mr. Strutt
has, therefore, imagined that the radium is not uniformly distributed
throughout the mass of the planet, and supposes that it is restricted
to an external zone forty-five miles in thickness; this would suffice
to maintain the earth at its existing temperature. If, however, we
admit a restriction of this kind, we are in no way bound to fix the
limit at forty-five miles. All we can say is that we do not know how
far downwards the radium reaches--for aught we know five miles, or even
less, is as likely a limit as forty-five miles. Professor Joly, indeed,
maintains that the radium we meet with is not proper to the earth at
all, but comes from the sun.
Radium is a short-lived element, its existence being limited to a
few thousand years; but as fast as it decays it is reproduced at the
expense of another element--uranium--the lifetime of which is measured
by hundreds of millions of years.
The last quarter of a century has proved fertile in great
discoveries--more so than any corresponding period in the past. As a
result, the whole world of scientific thought has been thrown into
commotion; old-established theories, and even the most fundamental
notions, seem to be in a state of flux. Under the stimulus of new ideas
great questions, such as the constitution of matter, the origin of
species, and the birth of worlds are being re-investigated with renewed
energy, and we seem to be on the eve of great events.
WILLIAM JOHNSON SOLLAS
FOUR PERIODS OF THE EARTH’S DEVELOPMENT
A Postscript to Professor Sollas’s Chapter on the Wonderful Story
of the World’s Birth, beginning on page 79
The earth was once “a fluid haze of light.” The whole solar system
once formed a vast nebula, consisting of glowing gas, or a swarm of
meteoroids. Our planet was slowly shaped into a globe out of this
primitive nebula.
Public-domain text, read in full here on John Shaqi.
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