On a Dynamical Top, for exhibiting the phenomena of the motion of a system of invariable form about a fixed point, with some suggestions as to the Earth's motionMaxwell, James Clerk
Science
On a Dynamical Top, for exhibiting the phenomena of the motion of a system of invariable form about a fixed point, with some suggestions as to the Earth's motion
Maxwell, James Clerk
Force and energy; Motion
We must remember that these motions of a body about its centre of
gravity, are _not_ illustrations of the theory of the precession of the
Equinoxes. Precession can be illustrated by the apparatus, but we must
arrange it so that the force of gravity acts the part of the attraction
of the sun and moon in producing a force tending to alter the axis of
rotation. This is easily done by bringing the centre of gravity of the
whole a little below the point on which it spins. The theory of such
motions is far more easily comprehended than that which we have been
investigating.
But the earth is a body whose principal axes are unequal, and from the
phenomena of precession we can determine the ratio of the polar and
equatorial axes of the “central ellipsoid;” and supposing the earth to
have been set in motion about any axis except the principal axis, or to
have had its original axis disturbed in any way, its subsequent motion
would be that of the top when the bob is a little below the critical
position.
The axis of angular momentum would have an invariable position in
space, and would travel with respect to the earth round the axis of
figure with a velocity $\displaystyle = \omega\frac{C - A}{A}$ where
$\omega$ is the sidereal angular velocity of the earth. The apparent
pole of the earth would travel (with respect to the earth) from west to
east round the true pole, completing its circuit in $\displaystyle
\frac{A}{C - A}$ sidereal days, which appears to be about 325.6 solar
days.
The instantaneous axis would revolve about this axis in space in about
a day, and would always be in a plane with the true axis of the earth
and the axis of angular momentum. The effect of such a motion on the
apparent position of a star would be, that its zenith distance should
be increased and diminished during a period of 325.6 days. This
alteration of zenith distance is the same above and below the pole, so
that the polar distance of the star is unaltered. In fact the method of
finding the pole of the heavens by observations of stars, gives the
pole of the _invariable axis_, which is altered only by external
forces, such as those of the sun and moon.
There is therefore no change in the apparent polar distance of stars
due to this cause. It is the latitude which varies. The magnitude of
this variation cannot be determined by theory. The periodic time of the
variation may be found approximately from the known dynamical
properties of the earth. The epoch of maximum latitude cannot be found
except by observation, but it must be later in proportion to the east
longitude of the observatory.
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