A distant minor planet, or distant object, is any minor planet found beyond Jupiter in the outer Solar System that is not commonly thought of as an "asteroid". The umbrella term is used by IAU's Minor Planet Center (MPC),[1] which is responsible for the identification, designation and orbit computation of these objects.[2] As of July 2024[update], the MPC maintains 5710 distant objects in its data base.[3]
Most distant minor planets are trans-Neptunian objects and centaurs, while relatively few are damocloids, Neptune trojans or Uranus trojans. All distant objects have a semi-major axis (average distance from the Sun) greater than 6 AU.[3] This threshold, which is just beyond the orbit of Jupiter (5.2 AU), ensures that the vast majority of "true asteroids" – such as the near-Earth, Mars-crosser, main-belt and Jupiter trojan populations – are excluded from the distant minor planets.[3]
See also
editReferences
edit- ^ "Observable Distant Minor Planets". Minor Planet Center. Retrieved 19 July 2024.
- ^ "Main page". Minor Planet Center. Retrieved 19 July 2024.
- ^ a b c "Objects with orbit type; Distant object". Minor Planet Center. Retrieved 19 July 2024.
External links
edit- Data base query form, Minor Planet Center
- Orbital Plot – locations and orbits of distant objects, Minor Planet Center
