Q84255982
red giant branch star in the constellation Monoceros
Press Enter · cited answer in seconds
0 sources
Q84255982
Summary
Q84255982 is a red giant branch star[1].
Key Facts
- Q84255982's instance of is recorded as red giant branch star[2].
- Q84255982's constellation is recorded as Monoceros[3].
- Q84255982's catalog code is recorded as 2MASS J07012240-0306049[4].
- Q84255982's catalog code is recorded as Gaia DR2 3108642426286693376[5].
- Q84255982's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.252'}[6].
- Q84255982's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.404'}[7].
- Q84255982's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.143'}[8].
- Q84255982's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9086'}[9].
- Q84255982's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3017'}[10].
- Q84255982's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+83.92'}[11].
- Q84255982's metallicity is recorded as {'unit': '1', 'amount': '-0.146'}[12].
- Q84255982's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+105.34338044897170'}[13].
- Q84255982's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-3.10136031737170'}[14].
- Q84255982's epoch is recorded as J2000.0[15].
- Q84255982's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4317'}[16].
- Q84255982's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+51'}[17].
- Q84255982's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.145'}[18].
- Q84255982's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.423'}[19].
Body
Definition and Type
Q84255982's instance of is recorded as red giant branch star[2].