2011 GH3
asteroid
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2011 GH3
Summary
2011 GH3 is an asteroid[1].
Key Facts
- 2011 GH3's instance of is recorded as asteroid[2].
- 2011 GH3's instance of is recorded as near-Earth object[3].
- 2011 GH3's minor planet group is recorded as Apollo asteroid[4].
- 2011 GH3's parent astronomical body is recorded as Sun[5].
- 2011 GH3's JPL Small-Body Database SPK-ID is recorded as 3561033[6].
- 2011 GH3's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.7710642243449597'}[7].
- 2011 GH3's absolute magnitude is recorded as {'unit': '1', 'amount': '+18.38'}[8].
- 2011 GH3's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+11.25447135355622'}[9].
- 2011 GH3's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1353.035369555721'}[10].
- 2011 GH3's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+102.6435339262376'}[11].
- 2011 GH3's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+2.394090050664269'}[12].
- 2011 GH3's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+4.240087238591698'}[13].
- 2011 GH3's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.5480928627368391'}[14].
- 2011 GH3's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+218.0778804634274'}[15].
- 2011 GH3's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+248.9887652994925'}[16].
- 2011 GH3's Google Knowledge Graph ID is recorded as /g/12z65bltm[17].
- 2011 GH3's Minor Planet Center body ID is recorded as 2011 GH3[18].
- 2011 GH3's epoch is recorded as May 5, 2025[19].
- 2011 GH3's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2461217.7281304663'}[20].
Body
Designation and Status
Recorded instance of include asteroid[2] and near-Earth object[3].