Q78754199
red giant branch star in the constellation Monoceros
Press Enter · cited answer in seconds
0 sources
Q78754199
Summary
Q78754199 is a red giant branch star[1].
Key Facts
- Q78754199's instance of is recorded as red giant branch star[2].
- Q78754199's constellation is recorded as Monoceros[3].
- Q78754199's catalog code is recorded as 2MASS J06474410+0957563[4].
- Q78754199's catalog code is recorded as Gaia DR2 3158563896315392896[5].
- Q78754199's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.276'}[6].
- Q78754199's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.439'}[7].
- Q78754199's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.236'}[8].
- Q78754199's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7775'}[9].
- Q78754199's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0927'}[10].
- Q78754199's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+94.14'}[11].
- Q78754199's metallicity is recorded as {'unit': '1', 'amount': '-0.087'}[12].
- Q78754199's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+101.93374499149920'}[13].
- Q78754199's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+9.96563082462510'}[14].
- Q78754199's epoch is recorded as J2000.0[15].
- Q78754199's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4154'}[16].
- Q78754199's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+31'}[17].
- Q78754199's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.217'}[18].
- Q78754199's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.183'}[19].
Body
Definition and Type
Q78754199's instance of is recorded as red giant branch star[2].