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Nodal precession information


Nodal precession is the precession of the orbital plane of a satellite around the rotational axis of an astronomical body such as Earth. This precession is due to the non-spherical nature of a rotating body, which creates a non-uniform gravitational field. The following discussion relates to low Earth orbit of artificial satellites, which have no measurable effect on the motion of Earth. The nodal precession of more massive, natural satellites like the Moon is more complex.

Around a spherical body, an orbital plane would remain fixed in space around the gravitational primary body. However, most bodies rotate, which causes an equatorial bulge. This bulge creates a gravitational effect that causes orbits to precess around the rotational axis of the primary body.

The direction of precession is opposite the direction of revolution. For a typical prograde orbit around Earth (that is, in the direction of primary body's rotation), the longitude of the ascending node decreases, that is the node precesses westward. If the orbit is retrograde, this increases the longitude of the ascending node, that is the node precesses eastward. This nodal precession enables heliosynchronous orbits to maintain a nearly constant angle relative to the Sun.

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Nodal precession

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Nodal precession is the precession of the orbital plane of a satellite around the rotational axis of an astronomical body such as Earth. This precession...

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Lunar precession

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precession followed by spinning objects. In addition, the orbit of the Moon undergoes two important types of precessional motion: apsidal and nodal....

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Precession

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Precession is a change in the orientation of the rotational axis of a rotating body. In an appropriate reference frame it can be defined as a change in...

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Lunar node

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ecliptic, occur during a comparatively brief period once every nodal period. The precession of the lunar nodes has a small effect on Earth's tides – atmospheric...

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Orbital precession

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orbital precession may refer to: Apsidal precession, where the major axis of an elliptical orbit cycles its orientation within its orbital plane. Nodal precession...

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Exoplanet orbital and physical parameters

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to detect the precession. The effect of general relativity can be detectable in timescales of about 10 years or less. Nodal precession is rotation of...

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Apsidal precession

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In celestial mechanics, apsidal precession (or apsidal advance) is the precession (gradual rotation) of the line connecting the apsides (line of apsides)...

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Orbit of the Moon

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eastward by 360°. The Moon's apsidal precession is distinct from the nodal precession of its orbital plane and axial precession of the moon itself. The mean inclination...

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Lunar standstill

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to Earth's axial precession, altering Earth's axial tilt over a very long period relative to the direction of lunar nodal precession. Put simply, the...

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Synodic day

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orbital periods that are a fraction of a synodic day. Combined with a nodal precession, this allows them to always pass over a location on Earth's surface...

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Ground track

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stable (minimally time-varying) orbit elements. These orbits use the nodal precession effect to shift the orbit so the ground track coincides with that of...

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Wet moon

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the equinoxes. Black moon Blue moon Libration Lunar precession Lunar standstill Nodal precession Orbit of the Moon Orbital node Lunar node StarChild Question...

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Saturn

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intersect (both the length of Saturn's year and the 18.6-Earth-year nodal precession period of the Moon's orbit influence the periodicity). Statistics of...

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Climate of Triton

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tilt of roughly 28°. Triton's orbit also experiences rapid precession, with a nodal precession period of 637 ± 40 years. The combination of these factors...

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Space rendezvous

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bodies Flyby (spaceflight) Lunar orbit rendezvous Mars orbit rendezvous Nodal precession of orbits around the Earth's axis Path-constrained rendezvous – the...

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Rings of Neptune

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{\displaystyle {\dot {\Omega }}_{s}} and n s {\displaystyle n_{s}} are the nodal precession rate and mean motion of the moon, respectively. CIR supports 2m stable...

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Transit of Mercury

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transit increases over centuries as a result of Mercury's nodal precession and Earth's axial precession. Transits of Mercury occur on a regular basis. As explained...

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J2

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{\displaystyle J_{2}\,} , a celestial body's second dynamic form factor in the nodal precession J 2 {\displaystyle J_{2}\,} , the second invariant of the deviatoric...

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Eclipse season

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a lunar or solar eclipse with a full or new moon, showing how the nodal precession of the moon's 5° orbital inclination means eclipses happen only about...

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Siarnaq

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resonance with Saturn, in which Siarnaq and Saturn have matching apsidal precession periods. Siarnaq's high orbital eccentricity and inclination places it...

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Year

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This term is sometimes erroneously used for the draconic or nodal period of lunar precession, that is the period of a complete revolution of the Moon's...

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Orbital resonance

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moons). A secular resonance occurs when the precession of two orbits is synchronised (usually a precession of the perihelion or ascending node). A small...

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Orbital period

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the Sun before the orbit completes. This cycle of axial precession for Earth, known as precession of the equinoxes, recurs roughly every 25,772 years. Periods...

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Hipparchus

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trigonometry, but is most famous for his incidental discovery of the precession of the equinoxes. Hipparchus was born in Nicaea, Bithynia, and probably...

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Nutation

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diagram indicates the combined effects of precession and nutation, while nutation in the absence of precession would only change the tilt from vertical...

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