2002 VE131
trans-Neptunian object
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2002 VE131
Summary
2002 VE131 is a trans-Neptunian object[1].
Key Facts
- 2002 VE131 is credited with the discovery of Marc Buie[2].
- 2002 VE131's instance of is recorded as trans-Neptunian object[3].
- 2002 VE131's instance of is recorded as asteroid[4].
- 2002 VE131's minor planet group is recorded as trans-Neptunian object[5].
- 2002 VE131's parent astronomical body is recorded as Sun[6].
- 2002 VE131's JPL Small-Body Database SPK-ID is recorded as 3144135[7].
- 2002 VE131's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.18'}[8].
- 2002 VE131's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.182865619252272'}[9].
- 2002 VE131's absolute magnitude is recorded as {'unit': '1', 'amount': '+6.5'}[10].
- 2002 VE131's absolute magnitude is recorded as {'unit': '1', 'amount': '+6.4968'}[11].
- 2002 VE131's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+18.7272287623254'}[12].
- 2002 VE131's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+112972.3472105103'}[13].
- 2002 VE131's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+239.758436204293'}[14].
- 2002 VE131's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+45.73504915272775'}[15].
- 2002 VE131's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+54.09841723757441'}[16].
- 2002 VE131's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+37.3716810678811'}[17].
- 2002 VE131's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+9.95587188505654'}[18].
- 2002 VE131's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+180.0692397244587'}[19].
- 2002 VE131's Google Knowledge Graph ID is recorded as /g/12z655f04[20].
- 2002 VE131's epoch is recorded as November 28, 2002[21].
- 2002 VE131's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2509070.94534361'}[22].
Body
Works and Contributions
2002 VE131 is credited with the discovery of Marc Buie[2].