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  2. Precession - Wikipedia

    en.wikipedia.org/wiki/Precession

    Torque-induced precession (gyroscopic precession) is the phenomenon in which the axis of a spinning object (e.g., a gyroscope) describes a cone in space when an external torque is applied to it. The phenomenon is commonly seen in a spinning toy top , but all rotating objects can undergo precession.

  3. Apsidal precession - Wikipedia

    en.wikipedia.org/wiki/Apsidal_precession

    The apsidal precession is the rate of change of ω through time, ⁠ dω / dt ⁠. Animation of Moon 's orbit around Earth - Polar view Moon · Earth. In celestial mechanics, apsidal precession (or apsidal advance) [1] is the precession (gradual rotation) of the line connecting the apsides (line of apsides) of an astronomical body's orbit.

  4. Phase precession - Wikipedia

    en.wikipedia.org/wiki/Phase_precession

    The finding that theta wave phase precession is also a property of grid cells in the entorhinal cortex demonstrated that the phenomenon exists in other parts of the brain that also mediate information about movement. [11] Theta wave phase precession in the hippocampus also plays a role in some brain functions that are unrelated to spatial location.

  5. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    The precession of Earth's axis is a very slow effect, but at the level of accuracy at which astronomers work, it does need to be taken into account on a daily basis. Although the precession and the tilt of Earth's axis (the obliquity of the ecliptic) are calculated from the same theory and are thus related one to the other, the two movements ...

  6. Astronomical nutation - Wikipedia

    en.wikipedia.org/wiki/Astronomical_nutation

    An example of precession and nutation is the variation over time of the orientation of the axis of rotation of the Earth. This is important because the most commonly used frame of reference for measurement of the positions of astronomical objects is the Earth's equator — the so-called equatorial coordinate system .

  7. Retrograde and prograde motion - Wikipedia

    en.wikipedia.org/wiki/Retrograde_and_prograde_motion

    Retrograde orbit: the satellite (red) orbits in the direction opposite to the rotation of its primary (blue/black) Retrograde motion in astronomy is, in general, orbital or rotational motion of an object in the direction opposite the rotation of its primary, that is, the central object (right figure).

  8. Category:Precession - Wikipedia

    en.wikipedia.org/wiki/Category:Precession

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  9. Orbital precession - Wikipedia

    en.wikipedia.org/wiki/Orbital_precession

    Apsidal precession, where the major axis of an elliptical orbit cycles its orientation within its orbital plane. Nodal precession, where non-spherical objects cause orbiting objects to change their orbits. Not to be confused with: Axial precession, where the rotation axis of a spinning object traces a conical path like a top.