(584778) 2017 RG16
Trans-Neptunian object, centaur
Press Enter · cited answer in seconds
0 sources
(584778) 2017 RG16
Summary
(584778) 2017 RG16 is a trans-Neptunian object[1].
Key Facts
- (584778) 2017 RG16 is credited with the discovery of Pan-STARRS1[2].
- (584778) 2017 RG16's instance of is recorded as trans-Neptunian object[3].
- (584778) 2017 RG16's instance of is recorded as centaur[4].
- (584778) 2017 RG16's instance of is recorded as minor planet[5].
- (584778) 2017 RG16's instance of is recorded as asteroid[6].
- (584778) 2017 RG16's instance of is recorded as distant minor planet[7].
- (584778) 2017 RG16's site of astronomical discovery is recorded as Haleakalā Observatory[8].
- (584778) 2017 RG16's minor planet group is recorded as trans-Neptunian object[9].
- (584778) 2017 RG16's parent astronomical body is recorded as Sun[10].
- (584778) 2017 RG16's provisional designation is recorded as 2017 RG16[11].
- (584778) 2017 RG16's time of discovery or invention is recorded as +2017-08-06T00:00:00Z[12].
- (584778) 2017 RG16's JPL Small-Body Database SPK-ID is recorded as 20584778[13].
- (584778) 2017 RG16's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.9076129593805882'}[14].
- (584778) 2017 RG16's absolute magnitude is recorded as {'unit': '1', 'amount': '+11.32'}[15].
- (584778) 2017 RG16's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+74.86843938449755'}[16].
- (584778) 2017 RG16's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+248208.0032400093'}[17].
- (584778) 2017 RG16's longitude of ascending node is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+0.6235626804744085'}[18].
- (584778) 2017 RG16's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+77.29384334783465'}[19].
- (584778) 2017 RG16's apoapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+147.4467372506624'}[20].
- (584778) 2017 RG16's periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+7.140949445006854'}[21].
- (584778) 2017 RG16's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+323.2992285628759'}[22].
- (584778) 2017 RG16's mean anomaly is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.459088718926774'}[23].
- (584778) 2017 RG16's Minor Planet Center body ID is recorded as 584778[24].
- (584778) 2017 RG16's epoch is recorded as November 21, 2025[25].
- (584778) 2017 RG16's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2457926.106924459'}[26].
Body
Works and Contributions
(584778) 2017 RG16 is credited with the discovery of Pan-STARRS1[2].