Q84238699
red giant branch star in the constellation Cassiopeia
Press Enter · cited answer in seconds
0 sources
Q84238699
Summary
Q84238699 is a red giant branch star[1].
Key Facts
- Q84238699's instance of is recorded as red giant branch star[2].
- Q84238699's constellation is recorded as Cassiopeia[3].
- Q84238699's catalog code is recorded as 2MASS J02521626+6500528[4].
- Q84238699's catalog code is recorded as Gaia DR2 468190266069647232[5].
- Q84238699's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.761'}[6].
- Q84238699's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.648'}[7].
- Q84238699's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.271'}[8].
- Q84238699's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.5783'}[9].
- Q84238699's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3561'}[10].
- Q84238699's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-19.94'}[11].
- Q84238699's metallicity is recorded as {'unit': '1', 'amount': '+0.003'}[12].
- Q84238699's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.06782459686790'}[13].
- Q84238699's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+65.01468316370040'}[14].
- Q84238699's epoch is recorded as J2000.0[15].
- Q84238699's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4424'}[16].
- Q84238699's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+91'}[17].
- Q84238699's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.653'}[18].
- Q84238699's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.344'}[19].
Body
Definition and Type
Q84238699's instance of is recorded as red giant branch star[2].