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- 2004_VN112 apoapsis "9.756773127054E10".
- 2004_VN112 orbitalPeriod "6542.0".
- 2004_VN112 periapsis "7.078971241524E9".
- 2004_VN112 absoluteMagnitude "6.4".
- 2004_VN112 abstract "2004 VN112, also written as 2004 VN112, is a detached object (because its perihelion is greater than 40 AU). It never gets closer than 47 AU from the Sun (about the outer edge of the main Kuiper belt) and averages more than 300 AU from the Sun. Its large eccentricity strongly suggests that it was gravitationally scattered onto its current orbit. Because it is, like all detached objects, outside of the current influence of Neptune, how it came to have this orbit cannot yet be explained. It has only been observed 25 times over 4 oppositions. To compare, the possible dwarf planet Sedna has been observed 88 times. Sedna and 2000 CR105 have similar orbits (perihelion greater than 40 AU and semi-major axis greater than 200 AU).2004 VN112 was observed by the Hubble Space Telescope in November 2008. It reached perihelion (closest approach to the Sun) in 2009, and is currently 47.5 AU from the Sun.Mike Brown's website lists it as a possible dwarf planet with a diameter of 314 km based on an assumed albedo of 0.04. The albedo is expected to be low because the object has a blue (neutral) color. But if the albedo is higher the object could easily be half that size.2004 VN112 is one of 12 object discovered in the Solar System to have a semi-major axis > 150 AU, a perihelion beyond Neptune, and an argument of perihelion of 340 ± 55°. Of these, only five, including 2004 VN112, have perihelia beyond Neptune's (current) influence.".
- 2004_VN112 albedo "0.04".
- 2004_VN112 apoapsis "9.756773127054E13".
- 2004_VN112 apparentMagnitude "23.3".
- 2004_VN112 epoch "2455800.5 (2011-Aug-27)".
- 2004_VN112 orbitalPeriod "5.652288E8".
- 2004_VN112 periapsis "7.078971241524E12".
- 2004_VN112 wikiPageExternalLink horizons.cgi?find_body=1&body_group=sb&sstr=2004VN112.
- 2004_VN112 wikiPageExternalLink sbdb.cgi?sstr=2004%20VN112.
- 2004_VN112 wikiPageExternalLink sbdb.cgi?sstr=2004VN112;orb=1;view=Far.
- 2004_VN112 wikiPageID "16010719".
- 2004_VN112 wikiPageRevisionID "603782375".
- 2004_VN112 absMagnitude "6.4".
- 2004_VN112 albedo "0.04".
- 2004_VN112 aphelion "652.2".
- 2004_VN112 argPeri "327".
- 2004_VN112 ascNode "66.06".
- 2004_VN112 bgcolour "#FFFFC0".
- 2004_VN112 designations "yes".
- 2004_VN112 dimensions "130".
- 2004_VN112 dimensions "314.0".
- 2004_VN112 discovered "2004".
- 2004_VN112 discovery "yes".
- 2004_VN112 eccentricity "0.8647".
- 2004_VN112 epoch "2455800.5".
- 2004_VN112 hasPhotoCollection 2004_VN112.
- 2004_VN112 inclination "25.52".
- 2004_VN112 magnitude "23.3".
- 2004_VN112 meanAnomaly "0.11".
- 2004_VN112 mpCategory "E-SDO".
- 2004_VN112 perihelion "47.32".
- 2004_VN112 period "6542".
- 2004_VN112 physicalCharacteristics "yes".
- 2004_VN112 semimajor "349.8".
- 2004_VN112 spectralType Trans-Neptunian_object.
- 2004_VN112 width "25".
- 2004_VN112 subject Category:Astronomical_objects_discovered_in_2004.
- 2004_VN112 subject Category:Scattered_disc_and_detached_objects.
- 2004_VN112 type CelestialBody.
- 2004_VN112 type Planet.
- 2004_VN112 type Planet.
- 2004_VN112 type PhysicalBody.
- 2004_VN112 comment "2004 VN112, also written as 2004 VN112, is a detached object (because its perihelion is greater than 40 AU). It never gets closer than 47 AU from the Sun (about the outer edge of the main Kuiper belt) and averages more than 300 AU from the Sun. Its large eccentricity strongly suggests that it was gravitationally scattered onto its current orbit. Because it is, like all detached objects, outside of the current influence of Neptune, how it came to have this orbit cannot yet be explained.".
- 2004_VN112 label "2004 VN112".
- 2004_VN112 label "2004 VN112".
- 2004_VN112 sameAs 2004_VN112.
- 2004_VN112 sameAs 2004_VN112.
- 2004_VN112 sameAs 2004_VN112.
- 2004_VN112 sameAs m.03qkpv9.
- 2004_VN112 sameAs Q2814017.
- 2004_VN112 sameAs Q2814017.
- 2004_VN112 wasDerivedFrom 2004_VN112?oldid=603782375.
- 2004_VN112 isPrimaryTopicOf 2004_VN112.