+Precession describes the slow, continuous change in the orientation of an astronomical body's rotational axis, much like a wobbling top. This subtle shift, often caused by [Gravitational Force](/wiki/gravitational-force), gradually alters the apparent position of stars over vast periods, affecting phenomena like the timing of the [Equinox](/wiki/equinox).
+## See also
+- [Nutate](/wiki/nutate)
+- [Axial Tilt](/wiki/axial-tilt)
+- [Orbital Mechanics](/wiki/orbital-mechanics)
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