A History of Science — Volume 3Williams, Henry Smith
History
A History of Science — Volume 3
Williams, Henry Smith
Science -- History
Nor is this a mere theoretical assumption; it is a determination of
experimental science, quite independent of theory. The physicist in the
laboratory has produced artificial conditions of temperature enabling
him to change the state of the most persistent gases. Some fifty years
since, when the kinetic theory was in its infancy, Faraday liquefied
carbonic-acid gas, among others, and the experiments thus inaugurated
have been extended by numerous more recent investigators, notably
by Cailletet in Switzerland, by Pictet in France, and by Dr. Thomas.
Andrews and Professor James Dewar in England. In the course of these
experiments not only has air been liquefied, but hydrogen also, the most
subtle of gases; and it has been made more and more apparent that gas
and liquid are, as Andrews long ago asserted, "only distant stages of
a long series of continuous physical changes." Of course, if the
temperature be lowered still further, the liquid becomes a solid; and
this change also has been effected in the case of some of the most
"permanent" gases, including air.
The degree of cold--that is, of absence of heat--thus produced is
enormous, relatively to anything of which we have experience in nature
here at the earth now, yet the molecules of solidified air, for
example, are not absolutely quiescent. In other words, they still have
a temperature, though so very low. But it is clearly conceivable that
a stage might be reached at which the molecules became absolutely
quiescent, as regards either translational or vibratory motion. Such a
heatless condition has been approached, but as yet not quite
attained, in laboratory experiments. It is called the absolute zero
of temperature, and is estimated to be equivalent to two hundred and
seventy-three degrees Centigrade below the freezing-point of water, or
ordinary zero.
A temperature (or absence of temperature) closely approximating this
is believed to obtain in the ethereal ocean of interplanetary and
interstellar space, which transmits, but is thought not to absorb,
radiant energy. We here on the earth's surface are protected from
exposure to this cold, which would deprive every organic thing of life
almost instantaneously, solely by the thin blanket of atmosphere with
which the globe is coated. It would seem as if this atmosphere,
exposed to such a temperature at its surface, must there be incessantly
liquefied, and thus fall back like rain to be dissolved into gas again
while it still is many miles above the earth's surface. This may be the
reason why its scurrying molecules have not long ago wandered off into
space and left the world without protection.
Public-domain text, read in full here on John Shaqi.
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