Q78755582
red giant branch star in the constellation Perseus
Press Enter · cited answer in seconds
0 sources
Q78755582
Summary
Q78755582 is a red giant branch star[1].
Key Facts
- Q78755582's instance of is recorded as red giant branch star[2].
- Q78755582's constellation is recorded as Perseus[3].
- Q78755582's catalog code is recorded as 2MASS J03234831+3121526[4].
- Q78755582's catalog code is recorded as Gaia DR2 124080475606141952[5].
- Q78755582's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.067'}[6].
- Q78755582's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.383'}[7].
- Q78755582's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.204'}[8].
- Q78755582's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.2702'}[9].
- Q78755582's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5858'}[10].
- Q78755582's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+25.96'}[11].
- Q78755582's metallicity is recorded as {'unit': '1', 'amount': '-0.059'}[12].
- Q78755582's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.95133125141540'}[13].
- Q78755582's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+31.36459171814830'}[14].
- Q78755582's epoch is recorded as J2000.0[15].
- Q78755582's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4752'}[16].
- Q78755582's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+363'}[17].
- Q78755582's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.454'}[18].
- Q78755582's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.621'}[19].
Body
Definition and Type
Q78755582's instance of is recorded as red giant branch star[2].