Q79812251
red giant branch star in the constellation Cassiopeia
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Q79812251
Summary
Q79812251 is a red giant branch star[1].
Key Facts
- Q79812251's instance of is recorded as red giant branch star[2].
- Q79812251's constellation is recorded as Cassiopeia[3].
- Q79812251's catalog code is recorded as 2MASS J02051050+6549277[4].
- Q79812251's catalog code is recorded as Gaia DR2 518584216866547200[5].
- Q79812251's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.767'}[6].
- Q79812251's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.055'}[7].
- Q79812251's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.831'}[8].
- Q79812251's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.3933'}[9].
- Q79812251's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4542'}[10].
- Q79812251's metallicity is recorded as {'unit': '1', 'amount': '-0.207'}[11].
- Q79812251's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2201.6733'}[12].
- Q79812251's SIMBAD ID is recorded as 2MASS J02051050+6549277[13].
- Q79812251's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+31.29376377315760'}[14].
- Q79812251's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+65.82437185746890'}[15].
- Q79812251's epoch is recorded as J2000.0[16].
- Q79812251's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5053'}[17].
- Q79812251's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+708'}[18].
- Q79812251's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.840'}[19].
- Q79812251's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.972'}[20].
- Q79812251's Gaia ID is recorded as 518584216866547200[21].