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  2. (612533) 2002 XV93 - Wikipedia

    en.wikipedia.org/wiki/(612533)_2002_XV93

    2002 XV 93 is locked in 2:3 resonance with Neptune, meaning that for every two revolutions it makes around the Sun, Neptune makes exactly three. [ 2 ] The rotation period of this object is currently unknown.

  3. Neptune - Wikipedia

    en.wikipedia.org/wiki/Neptune

    There do exist orbits within these empty regions where objects can survive for the age of the Solar System. These resonances occur when Neptune's orbital period is a precise fraction of that of the object, such as 1:2, or 3:4. If, say, an object orbits the Sun once for every two Neptune orbits, it will only complete half an orbit by the time ...

  4. Orbital period - Wikipedia

    en.wikipedia.org/wiki/Orbital_period

    The orbital period (also revolution period) is the amount of time a given astronomical object takes to complete one orbit around another object. In astronomy , it usually applies to planets or asteroids orbiting the Sun , moons orbiting planets, exoplanets orbiting other stars , or binary stars .

  5. (119951) 2002 KX14 - Wikipedia

    en.wikipedia.org/wiki/(119951)_2002_KX14

    It has a semi-major axis, orbital period and orbital eccentricity close to that of a plutino. [10] The orbital periods of plutinos cluster around 247.2 years (1.5 times Neptune's orbital period), close to 2002 KX 14 's orbital period. However, 2002 KX 14 is not a plutino, as it is not actually in a resonance with Neptune, and it may have formed ...

  6. 385695 Clete - Wikipedia

    en.wikipedia.org/wiki/385695_Clete

    Clete orbits near Neptune's L 4 Lagrangian point about 60° ahead of Neptune and thus has the about same orbital period as Neptune. It orbits the Sun at a distance of 28.5–31.6 AU once every 164 years and 9 months (60,182 days; semi-major axis of 30.06 AU).

  7. Kepler-413b - Wikipedia

    en.wikipedia.org/wiki/Kepler-413b

    Kepler-413b is a Neptune sized planet with an orbital period of about 66.262 days. The orbital misalignment of Kepler-413b causes extreme seasonal variations for the planet due to its constantly changing axial tilt.

  8. Laomedeia - Wikipedia

    en.wikipedia.org/wiki/Laomedeia

    Laomedeia / ˌ l eɪ ə m ə ˈ d iː ə /, also known as Neptune XII, is a prograde irregular satellite of Neptune. It was discovered by Matthew J. Holman , et al. on August 13, 2002. [ 6 ] Before the announcement of its name on February 3, 2007 (IAUC 8802), it was known as S/2002 N 3 .

  9. 2001 KY76 - Wikipedia

    en.wikipedia.org/wiki/2001_KY76

    2001 KY 76, also written 2001 KY76, is a trans-Neptunian object from the Kuiper belt.It is classified as a plutino, a minor planet locked in a 2:3 mean-motion orbital resonance with the planet Neptune.