2010 WH1
asteroid
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2010 WH1
Summary
2010 WH1 is an asteroid[1].
Key Facts
- 2010 WH1's instance of is recorded as asteroid[2].
- 2010 WH1's instance of is recorded as near-Earth object[3].
- 2010 WH1's minor planet group is recorded as Apollo asteroid[4].
- 2010 WH1's parent astronomical body is recorded as Sun[5].
- 2010 WH1's JPL Small-Body Database SPK-ID is recorded as 3552534[6].
- 2010 WH1's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.1574289912446674'}[7].
- 2010 WH1's absolute magnitude is recorded as {'unit': '1', 'amount': '+26.2'}[8].
- 2010 WH1's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+12.21788839685078'}[9].
- 2010 WH1's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+407.9842380715009'}[10].
- 2010 WH1's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+243.7279630986184'}[11].
- 2010 WH1's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+1.076539506626928'}[12].
- 2010 WH1's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+1.246018035190237'}[13].
- 2010 WH1's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.9070609780636187'}[14].
- 2010 WH1's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+97.68460308162209'}[15].
- 2010 WH1's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+36.97967445982112'}[16].
- 2010 WH1's Google Knowledge Graph ID is recorded as /g/12z653c8k[17].
- 2010 WH1's Minor Planet Center body ID is recorded as 2010 WH1[18].
- 2010 WH1's epoch is recorded as May 5, 2025[19].
- 2010 WH1's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2460758.591321365'}[20].
Body
Designation and Status
Recorded instance of include asteroid[2] and near-Earth object[3].