Q79768049
red giant branch star in the constellation Monoceros
Press Enter · cited answer in seconds
0 sources
Q79768049
Summary
Q79768049 is a red giant branch star[1].
Key Facts
- Q79768049's instance of is recorded as red giant branch star[2].
- Q79768049's constellation is recorded as Monoceros[3].
- Q79768049's catalog code is recorded as 2MASS J07021952+0127008[4].
- Q79768049's catalog code is recorded as Gaia DR2 3115378373814870144[5].
- Q79768049's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.554'}[6].
- Q79768049's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.792'}[7].
- Q79768049's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.594'}[8].
- Q79768049's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8955'}[9].
- Q79768049's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2981'}[10].
- Q79768049's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.92'}[11].
- Q79768049's metallicity is recorded as {'unit': '1', 'amount': '-0.247'}[12].
- Q79768049's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+105.58136774792830'}[13].
- Q79768049's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+1.45023818246910'}[14].
- Q79768049's epoch is recorded as J2000.0[15].
- Q79768049's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4283'}[16].
- Q79768049's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+54'}[17].
- Q79768049's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.212'}[18].
- Q79768049's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.899'}[19].
Body
Definition and Type
Q79768049's instance of is recorded as red giant branch star[2].