The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
There is nothing more characteristic of the physical science of the
century just closed than the famous discovery of the numerical relation
which exists between heat and energy. We are indebted to the life-long
labours of Joule, followed by those of many other investigators, for the
accurate determination of the fundamental constant which is known as the
mechanical equivalent of heat. Joule showed that the quantity of heat
which would suffice to raise one pound of water through a single degree
Fahrenheit was the precise equivalent of the quantity of energy which
would suffice to raise 772 pounds through a height of one foot. It would
be hard to say whether this remarkable principle has had a more profound
effect on practical engineering or on the course of physical science. In
practical engineering, the knowledge of the mechanical equivalent of
heat will show the engineer the utmost amount of work that could by any
conceivable apparatus be extracted from the heat potentially contained
in a ton of coal. In the study of astronomy the application of the same
principle will suffice to explain how the sun’s heat has been sustained
for illimitable ages.
[Illustration: Fig. 16.—BROOKS’ COMET AND METEOR TRAIL.
(November 13th, 1893. Exposure 2 hours.)
(_Photographed by Professor E. E. Barnard._)]
It will be convenient to commence with a little calculation, which will
provide us with a result very instructive when considering celestial
phenomena in connection with energy. We have seen that the unit of
heat—for so we term the quantity of heat necessary to raise a pound of
water one degree—will suffice, when transformed into mechanical energy,
to raise 772 pounds through a single foot. This would, of course, be
precisely the same thing as to raise one pound through 772 feet. Suppose
a pound weight were carried up 772 feet high and were then allowed to
drop. The pound weight would gradually gather speed in its descent, and,
at the moment when it was just reaching the earth, would be moving with
a speed of about 224 feet a second. We may observe that the work which
was done in raising the body to this height has been entirely expended
in giving the body this particular velocity. A weight of one pound,
moving with a speed of 224 feet a second, will therefore contain, in
virtue of that motion, a quantity of energy precisely equivalent to the
unit of heat.
Public-domain text, read in full here on John Shaqi.
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