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Unformatted text preview: D.) Hence, from Equation (491), the precession rate of the angular velocity vector about the symmetry axis, as viewed in a
geostationary reference frame, is (512) giving a precession period of (513) [Of course, (sidereal) day.] The observed period of precession is about 434 days (Yoder 1995). The disagreement between theory and observation is attributed to the fact that the Earth is not perfectly rigid
(Bertotti et al. 2003). An improved treatment of the free precession of the Earth that takes into account its
lack of complete rigidity is given in Appendix C.
The Earth's symmetry axis subtends an angle [see Equation (495)] with its angular momentum vector, but it lies on the opposite side of this vector to the angular velocity vector. This implies that, as
viewed from space, the Earth's angular velocity vector is almost parallel to its fixed angular momentum
vector, whereas its symmetry axis subtends an angle of
with both vectors and precesses about them.
The (theoretical) precession rate of the Earth's symmetry axis, as seen from space, is given by
http://farside.ph.utexas.edu/teaching/celestial/Celestialhtml/node72.html Page 1 of 2 Free precession of Earth 11/6/13 1:25 AM (514) The associated precession period is (515) The free precession of the Earth's symmetry axis in space, which is known as the Chandler wobble--because
it was discovered by the American astronomer S.C. Chandler (1846-1913) in 1891--is superimposed on a
much slower forced precession, with a period of about 26,000 years, caused by the small gravitational torque
exerted on the Earth by the Sun and Moon, as a consequence of the Earth's slight oblateness. (See
Section 7.10.) Next: MacCullagh's formula Up: Rigid body rotation Previous: Euler angles
Richard Fitzpatrick 2013-06-15 http://farside.ph.utexas.edu/teaching/celestial/Celestialhtml/node72.html Page 2 of 2...
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