The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
Though lime in its different forms, in the rocks of the earth or the
waters of the ocean, is one of the most ordinary substances met with on
our globe, yet calcium, the essential element which goes to the
composition of lime, is, as we have already said, not by any means a
familiar body, and not many of us, I imagine, can ever have seen it.
Chemistry teaches that lime is the result of a union in definite
proportions between oxygen gas and the very shy metal, calcium. This
metal is never found in nature unless in such intimate chemical union
with some other element like oxygen or chlorine, that its characteristic
features are altogether obscured, and would indeed never be suspected
from the mere appearance of the results of the union. To see the metal
calcium you must visit a chemical laboratory where, by electrical
decomposition or other ingenious process, this elusive element can be
induced to part temporarily from its union with the oxygen or other body
for which it has so eager an affinity, and to which it returns with such
alacrity. Though calcium is certainly a metal, it is very unlike the
more familiar metals such as gold or silver, copper or iron. A coin
might conceivably be formed out of calcium, but it would have no
stability like the coins of the well-known metals. Calcium has such an
unconquerable desire to unite with oxygen that the unstable metal will
speedily grasp from the surrounding air the vital element. Unless
special precautions are taken to withhold from the calcium the air, or
other source from whence it could obtain oxygen, the union will most
certainly take place, and the calcium will resume the stable form of
lime. Thus it happens that though this earth contains incalculable
billions of tons of calcium in its various combinations, yet calcium
itself is almost unknown except to the chemist.
It is plain that calcium plays a part of tremendous significance on this
earth. I do not say that it is the most important of all the elements.
It would indeed seem impossible to assign that distinction to any
particular element. Many are, of course, of vital importance, though
there are, no doubt, certain of the rarer elements with which this earth
could perhaps dispense without being to any appreciable extent different
from what it is at present. I do not know that we should be specially
inconvenienced or feel any appreciable want unsatisfied, if, let us say,
the element lanthanum were to be struck out of existence; and there are
perhaps certain other rare bodies among the known eighty elements, about
which the same remark might be made.
[Illustration: Fig. 42.—THE H. AND K. LINES IN THE PHOTOGRAPHIC SOLAR
SPECTRUM (Higgs).]
Public-domain text, read in full here on John Shaqi.
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