2017 TW4
asteroid
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2017 TW4
Summary
2017 TW4 is an asteroid[1].
Key Facts
- 2017 TW4's instance of is recorded as asteroid[2].
- 2017 TW4's instance of is recorded as near-Earth object[3].
- 2017 TW4's minor planet group is recorded as Amor asteroid[4].
- 2017 TW4's parent astronomical body is recorded as Sun[5].
- 2017 TW4's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.4583123258813022'}[6].
- 2017 TW4's absolute magnitude is recorded as {'unit': '1', 'amount': '+24.9'}[7].
- 2017 TW4's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+1.984034841178405'}[8].
- 2017 TW4's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+972.6282159109503'}[9].
- 2017 TW4's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+306.4977927018213'}[10].
- 2017 TW4's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+1.921169241962339'}[11].
- 2017 TW4's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+2.801664785657717'}[12].
- 2017 TW4's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+1.040673698266961'}[13].
- 2017 TW4's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+101.3637118938095'}[14].
- 2017 TW4's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+5.38371324686942'}[15].
- 2017 TW4's epoch is recorded as November 21, 2025[16].
- 2017 TW4's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2460985.9545794157'}[17].
Body
Definition and Type
Recorded instance of include asteroid[2] and near-Earth object[3].