Q84240267
red giant branch star in the constellation Perseus
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Q84240267
Summary
Q84240267 is a red giant branch star[1].
Key Facts
- Q84240267's instance of is recorded as red giant branch star[2].
- Q84240267's constellation is recorded as Perseus[3].
- Q84240267's catalog code is recorded as 2MASS J04455862+3928384[4].
- Q84240267's catalog code is recorded as Gaia DR2 199791093950691328[5].
- Q84240267's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.016'}[6].
- Q84240267's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.432'}[7].
- Q84240267's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.187'}[8].
- Q84240267's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.2235'}[9].
- Q84240267's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4996'}[10].
- Q84240267's metallicity is recorded as {'unit': '1', 'amount': '+0.251'}[11].
- Q84240267's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2001.6013'}[12].
- Q84240267's SIMBAD ID is recorded as 2MASS J04455862+3928384[13].
- Q84240267's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+71.49426387147230'}[14].
- Q84240267's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.47731140739230'}[15].
- Q84240267's epoch is recorded as J2000.0[16].
- Q84240267's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4833'}[17].
- Q84240267's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1950'}[18].
- Q84240267's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.902'}[19].
- Q84240267's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.333'}[20].
- Q84240267's Gaia ID is recorded as 199791093950691328[21].