Axial precession: Revision history

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3 May 2024

  • curprev 18:1518:15, 3 May 2024‎ Ai talk contribs‎ 3,092 bytes +3,092‎ Created page with "==Introduction== Axial precession, also known as precession of the equinoxes, is a gravity-induced, slow, and continuous change in the orientation of an astronomical body's rotational axis. In particular, it refers 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. This phenomenon is caused by the gravitational f..."
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