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The images at right attempt to explain the relation between the precession of the Earth's axis and the shift in the equinoxes. These images show the position of the Earth's axis on the celestial sphere, a fictitious sphere which places the stars according to their position as seen from Earth, regardless of their actual distance. The first image ...
Axial precession is the trend in the direction of the Earth's axis of rotation relative to the fixed stars, with a period of about 25,700 years. Also known as the precession of the equinoxes, this motion means that eventually Polaris will no longer be the north pole star .
Earth axial precession: Image title: The precession of Earth's axis as viewed from the north, drawn by CMG Lee. The seasons indicated pertain to the Northern Hemisphere and are reversed for the Southern Hemisphere. The tilt of Earth's axis and the eccentricity of its orbit are exaggerated. Width: 100%: Height: 100%
Precession of Earth's rotational axis due to the tidal force raised on Earth by the gravity of the Moon and Sun. Date: 5 May 2008: Source: Vectorized by Mysid in Inkscape after a NASA Earth Observatory image in Milutin Milankovitch Precession. Author: NASA, Mysid
A slow motion of Earth's axis, precession, causes a slow, continuous turning of the coordinate system westward about the poles of the ecliptic, completing one circuit in about 26,000 years. Superimposed on this is a smaller motion of the ecliptic, and a small oscillation of the Earth's axis, nutation. [4]
The precession of Earth's axis was later explained by Newtonian physics. Being an oblate spheroid, Earth has a non-spherical shape, bulging outward at the equator. The gravitational tidal forces of the Moon and Sun apply torque to the equator, attempting to pull the equatorial bulge into the plane of the ecliptic, but instead causing it to precess.