The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
No matter how early be the period which we consider, we find the same
causes to be in operation. There was a time when, owing to the internal
heat, the surface of the earth must have been as hot as boiling water.
The loss of heat by radiation must then have taken place much more
copiously than it does at present. The argument we are pursuing must
therefore have applied with even greater force in those early days.
There was a time when the materials at the surface of the earth must
have been intensely heated, when they must have even been red-hot. There
was a time when the earth’s surface must have had a temperature like
that of the lava as it issues from a volcano. There must have been a
time when the surface of the earth was not even solid, when indeed it
was a viscid liquid, and earlier still the liquid must have been more
and more incandescent. From that brilliant surface heat was vehemently
radiated. Each day the globe was hotter than on the succeeding day.
There is no break in the argument. We have to think of this glowing
globe passing through those phases through which we know that all matter
will pass if only we apply to it sufficient heat. The globe assumed the
liquid state from that state which is demanded by a temperature still
higher, the state in which the matter is actually in the form of vapour.
Even the most refractory substances will take the form of vapour at a
very high temperature.
Thus we are conducted to a remarkable conception of the condition in
which the materials now forming our solid earth must have been in the
exceedingly remote past. What is now our earth must once have been a
great quantity of heated vapour. It need hardly be said that in that
form the volume of the earth was much larger than the volume which the
earth has at present, while no doubt the mass of the earth then was even
less than the mass of the earth now, by reason of the meteoric matter
which has been drawn in by our globe.
But even when our earth was in this inflated state of vapour our
argument can be still maintained. Thus we see that the earth, or rather
the cloud of vapour which was ultimately to form the earth, is ever
growing larger and larger in our retrospect, ever becoming more and more
rarefied; and it may well have been that there was a time when the
materials of this earth occupied a volume thousands of times greater
than they do at present.
In a previous chapter we have seen how the sun was at one time in the
nebulous state, and now we have been led to a similar conclusion with
regard to the earth. At that time, of course, the sun was greatly in
excess of its present dimensions, and the earth was also greatly
swollen. The nebula which formed our sun, and the nebula which formed
our earth, were both so vast as to be confluent; they were indeed both
part of the same vast nebula.
Public-domain text, read in full here on John Shaqi.
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