2012 VK6

Summary

2012 VK6 is an asteroid^[1].

Key Facts

• 2012 VK6's instance of is recorded as asteroid^[2].
• 2012 VK6's instance of is recorded as potentially hazardous asteroid^[3].
• 2012 VK6's instance of is recorded as near-Earth object^[4].
• 2012 VK6's instance of is recorded as near-Earth asteroid^[5].
• 2012 VK6's minor planet group is recorded as Apollo asteroid^[6].
• 2012 VK6's parent astronomical body is recorded as Sun^[7].
• 2012 VK6's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.7054449427436342'}^[8].
• 2012 VK6's absolute magnitude is recorded as {'unit': '1', 'amount': '+20.1'}^[9].
• 2012 VK6's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+1.839895545493723'}^[10].
• 2012 VK6's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1276.637602847703'}^[11].
• 2012 VK6's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.0192503908353'}^[12].
• 2012 VK6's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+2.303100043810547'}^[13].
• 2012 VK6's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+3.927810322349341'}^[14].
• 2012 VK6's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.6783897652717543'}^[15].
• 2012 VK6's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+339.3128028025249'}^[16].
• 2012 VK6's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+20.21226595157134'}^[17].
• 2012 VK6's epoch is recorded as November 11, 2012^[18].
• 2012 VK6's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2456170.8229479096'}^[19].

Body

Definition and Type

Recorded instance of include asteroid^[2], potentially hazardous asteroid^[3], near-Earth object^[4], and near-Earth asteroid^[5].