Q84238176
red giant branch star in the constellation Cassiopeia
Press Enter · cited answer in seconds
0 sources
Q84238176
Summary
Q84238176 is a red giant branch star[1].
Key Facts
- Q84238176's instance of is recorded as red giant branch star[2].
- Q84238176's constellation is recorded as Cassiopeia[3].
- Q84238176's catalog code is recorded as 2MASS J00291258+5538530[4].
- Q84238176's catalog code is recorded as Gaia DR2 421244727337370112[5].
- Q84238176's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.006'}[6].
- Q84238176's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.250'}[7].
- Q84238176's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.008'}[8].
- Q84238176's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3231'}[9].
- Q84238176's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2492'}[10].
- Q84238176's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-60.58'}[11].
- Q84238176's metallicity is recorded as {'unit': '1', 'amount': '-0.095'}[12].
- Q84238176's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.30244825568490'}[13].
- Q84238176's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.64806186784800'}[14].
- Q84238176's epoch is recorded as J2000.0[15].
- Q84238176's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4297'}[16].
- Q84238176's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+45'}[17].
- Q84238176's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.606'}[18].
- Q84238176's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.653'}[19].
Body
Definition and Type
Q84238176's instance of is recorded as red giant branch star[2].