Precession refers to a change in the direction of the axis of a rotating object.
In certain contexts, "precession" may refer to the precession that the Earth experiences, the effects of this type of precession on astronomical observation, or to the precession of orbital objects.
The revolution of a planet in its orbit around the Sun is also a form of rotary motion.
(In this case, the combined system of Earth and Sun is rotating.) So the axis of a planet's orbital plane will also precess over time.
The major axis of each planet's elliptical orbit also precesses within its orbital plane, in response to perturbations in the form of the changing gravitational forces exerted by other planets.
Shift of equinox The precession of the equinoxes refers to the precession of Earth's axis of rotation with respect to inertial space. The precession of the equinoxes ... >
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Gravitation Gravity is a force of attraction that acts between bodies that have mass. Gravity is the reason for the very existence of the earth, the sun and ... >
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Mercury (planet) Mercury is the innermost and smallest planet in the solar system, orbiting the Sun once every 88 days. It ranges in brightness from about −2.0 ... >
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Solstice The summer solstice is an astronomical term regarding the position of the sun in relation to the celestial equator. The summer solstice is the day of ... >
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General relativity General relativity (GR) is the geometrical theory of gravitation published by Albert Einstein in 1915. It unifies special relativity and Sir Isaac ... >
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Planetary habitability Planetary habitability is the measure of an astronomical body's potential to develop and sustain life. It is generally assumed that any ... >
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Geosynchronous orbit A geosynchronous orbit is a geocentric orbit that has the same orbital period as the sidereal rotation period of the Earth. It has a semi-major axis ... >
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Equatorial bulge An equatorial bulge is a planetological term which describes a bulge which a planet may have around its equator, distorting it into an oblate ... >
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Ellipse In mathematics, an ellipse is a plane algebraic curve where the sum of the distances from any point on the curve to two fixed points is constant. An ... >
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