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  2. Longitude of periapsis - Wikipedia

    en.wikipedia.org/wiki/Longitude_of_periapsis

    ϖ = Ω + ω in separate planes. In celestial mechanics, the longitude of the periapsis, also called longitude of the pericenter, of an orbiting body is the longitude (measured from the point of the vernal equinox) at which the periapsis (closest approach to the central body) would occur if the body's orbit inclination were zero.

  3. Apsis - Wikipedia

    en.wikipedia.org/wiki/Apsis

    The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1). An apsis (from Ancient Greek ἁψίς (hapsís) 'arch, vault'; pl. apsides / ˈ æ p s ɪ ˌ d iː z / AP-sih-deez) [1] [2] is the farthest or nearest point in the orbit of a planetary body about its primary body.

  4. Apsidal precession - Wikipedia

    en.wikipedia.org/wiki/Apsidal_precession

    The ancient Greek astronomer Hipparchus noted the apsidal precession of the Moon's orbit (as the revolution of the Moon's apogee with a period of approximately 8.85 years); [4] it is corrected for in the Antikythera Mechanism (circa 80 BCE) (with the supposed value of 8.88 years per full cycle, correct to within 0.34% of current measurements). [5]

  5. 2012 VP113 - Wikipedia

    en.wikipedia.org/wiki/2012_VP113

    2012 VP 113 is the minor planet with the farthest known perihelion (closest approach to the Sun) in the Solar System, greater than Sedna's. [13] Though its perihelion is farther, 2012 VP 113 has an aphelion only about half of Sedna's. It is the second discovered sednoid, with semi-major axis beyond 150 AU and perihelion greater than 50 AU.

  6. Argument of periapsis - Wikipedia

    en.wikipedia.org/wiki/Argument_of_periapsis

    An argument of periapsis of 0° means that the orbiting body will be at its closest approach to the central body at the same moment that it crosses the plane of reference from South to North. An argument of periapsis of 90° means that the orbiting body will reach periapsis at its northmost distance from the plane of reference.

  7. Biela's Comet - Wikipedia

    en.wikipedia.org/wiki/Biela's_Comet

    Perihelion distance at different epochs [5] [1] Epoch ... (1806) to calculate a definitive orbit. ... and come to perihelion in December 2023, ...

  8. Orbit of Venus - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Venus

    [1] [2] The low eccentricity and comparatively small size of its orbit give Venus the least range in distance between perihelion and aphelion of the planets: 1.46 million km. The planet orbits the Sun once every 225 days [ 3 ] and travels 4.54 au (679,000,000 km; 422,000,000 mi) in doing so, [ 4 ] giving an average orbital speed of 35 km/s ...

  9. Perihelion distance - Wikipedia

    en.wikipedia.org/?title=Perihelion_distance&...

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