In
astronomy,
axial precession is a gravity-induced, slow, and continuous change in the orientation of an astronomical body's
rotational axis. In particular, it can refer to the gradual shift in the orientation of
Earth's axis of rotation, which, similar to a wobbling top, traces out a pair of
cones joined at their
apices in a cycle of approximately 26,000 years. The term "precession" typically refers only to this largest part of the motion; other changes in the alignment of Earth's axis—
nutation and
polar motion—are much smaller in magnitude.