Popular Scientific Recreations: in Natural Philosphy, Astronomy, Geology, Chemistry, etc., etc., etc.Tissandier, Gaston
Science
Popular Scientific Recreations: in Natural Philosphy, Astronomy, Geology, Chemistry, etc., etc., etc.
Tissandier, Gaston
Scientific recreations
The _pendulum_ is considered the nearest approach to perpetual motion.
This is so well known that no description is needed, but we may say
a few words concerning it. By the diagram, we see that if we lift
the ball to _b_, and let it fall, it will descend to _l_, and pass
it to _a_ opposite, nearly as far from _l_ as _b_ is from it. So the
oscillations will continue, each beat being less and less, till rest is
reached by the action of gravity (page 23). Were it not for friction
and the pressure of the air, the oscillations would continue for ever;
as it is, it declines by shorter swings till it remains in equilibrium.
[Illustration: Fig. 35.—The pendulum.]
The seconds’ pendulum oscillates sixty times an hour, and must be of a
certain length in certain places. In London it is 39·1393 inches, and
furnishes a certain standard of length, and by an Act of Parliament the
yard is divided into 36 parts, and 39·1393 such parts make the seconds’
pendulum in the latitude of London (_in vacuo_) in a temperature of 62°.
[Illustration: Fig. 36.—Centrifugal Force.]
But the same pendulum will not perform the same number of oscillations
in one minute in all parts of the globe. At the equator they will
be less, and at the pole more. Thus it was discovered that, as the
movements of the pendulum are dependent upon the force of gravity,
and as this force decreases the farther we get from the centre of the
earth, the equator must be farther from the earth’s centre than the
poles, and therefore the poles must be depressed. The decline of the
pendulum at the equator is also, in a measure, due to Centrifugal Force.
_Centrifugal Force_, which means “flying from the centre,” is the force
which causes an object to describe a circle with uniform velocity, and
fly away from the centre; the force that counteracts it is called the
_centripetal_ force. A very simple experiment will illustrate it.
[Illustration: Fig. 37.—Another illustration of centrifugal force.]
To represent its action, we shall have recourse to an ordinary glass
tumbler placed on a round piece of cardboard, held firmly in place by
cords. Some water is poured in the glass, and we then show that it can
be swung to and fro and round without the water being spilt, even when
the glass is upside down (fig. 36).
Another experiment on the same subject is as shown in the above
illustration, by which a napkin ring can be kept in revolution around
the forefinger, and by a continued force the ring may be even held
suspended at the tip of the finger, apparently in the air, without
support (fig. 37).
FOOTNOTES:
[8] The experiment we have just described is a very old one. M. V.
Sircoulon has told us that it was described at length in the works of
Rabelais. The following remarks are in “Pantagruel,” book II., chap.
xvii.
Public-domain text, read in full here on John Shaqi.
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