2010 WB3
asteroid
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2010 WB3
Summary
2010 WB3 is an asteroid[1].
Key Facts
- 2010 WB3's instance of is recorded as asteroid[2].
- 2010 WB3's instance of is recorded as near-Earth object[3].
- 2010 WB3's minor planet group is recorded as Apollo asteroid[4].
- 2010 WB3's parent astronomical body is recorded as Sun[5].
- 2010 WB3's JPL Small-Body Database SPK-ID is recorded as 3552537[6].
- 2010 WB3's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.7736220047085148'}[7].
- 2010 WB3's absolute magnitude is recorded as {'unit': '1', 'amount': '+19.95'}[8].
- 2010 WB3's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+8.912125382474368'}[9].
- 2010 WB3's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+699.8018418253877'}[10].
- 2010 WB3's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+334.6775114848338'}[11].
- 2010 WB3's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+1.542592099894081'}[12].
- 2010 WB3's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+2.735975292661657'}[13].
- 2010 WB3's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.3492089071265044'}[14].
- 2010 WB3's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+195.2102170527088'}[15].
- 2010 WB3's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+159.2913244593954'}[16].
- 2010 WB3's Google Knowledge Graph ID is recorded as /g/12z65wzg2[17].
- 2010 WB3's Minor Planet Center body ID is recorded as 2010 WB3[18].
- 2010 WB3's epoch is recorded as May 5, 2025[19].
- 2010 WB3's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2460490.8545493237'}[20].
Body
Designation and Status
Recorded instance of include asteroid[2] and near-Earth object[3].