Precession
PRECESSION
Due to the interaction between the Earth and the Moon, the rotation axis
of the Earth is not stationary. The interaction arises because the Moon
is not in the equatorial plane of the Earth; there is a misalignment
between the spin axis of the Earth and the orbital axis of the Moon
In the interaction the Moon tries to force the two axes to
coincide. This force causes the direction in
which the rotation axis points to change slowly.
The motion is
regular and is known as
precession; the
path on the Celestial Sphere is roughly
circular. The radius of the circle is large, ~ 23.5 degrees (because
for the most part, the angle which the Earth's rotation axis makes with
the vertical doesn't change.).
The period of the motion is long,
25,800 years, due
to the weakness of the effect.
- Because the
point where the direction in which the rotation axis points changes, this
affects the period on which the seasons vary. This is why the Tropical
Year is shorter than the Sidereal Year.
- Because
the point where the projection
of the rotation axis of the Earth strikes
the Celestial Sphere moves around (the stars are still not in
motion), the
North Celestial Pole also moves through the stars.
This produces changes in the coordinates of
stars (even though they are not moving).
Today, it is fortuitous that
the North star is Polaris.
At other times, other stars will be
the North star:
In 12,000 years or so, Vega in the constellation Lyra will be near
the North Celestical Pole.