Q79774211
red giant branch star in the constellation Perseus
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Q79774211
Summary
Q79774211 is a red giant branch star[1].
Key Facts
- Q79774211's instance of is recorded as red giant branch star[2].
- Q79774211's constellation is recorded as Perseus[3].
- Q79774211's catalog code is recorded as 2MASS J03264782+5256030[4].
- Q79774211's catalog code is recorded as Gaia DR2 443389200756458752[5].
- Q79774211's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.612'}[6].
- Q79774211's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.849'}[7].
- Q79774211's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.676'}[8].
- Q79774211's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.1729'}[9].
- Q79774211's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5011'}[10].
- Q79774211's metallicity is recorded as {'unit': '1', 'amount': '-0.314'}[11].
- Q79774211's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1995.6097'}[12].
- Q79774211's SIMBAD ID is recorded as 2MASS J03264782+5256030[13].
- Q79774211's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+51.69924178558620'}[14].
- Q79774211's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.93418685526340'}[15].
- Q79774211's epoch is recorded as J2000.0[16].
- Q79774211's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4860'}[17].
- Q79774211's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1047'}[18].
- Q79774211's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.607'}[19].
- Q79774211's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.530'}[20].
- Q79774211's Gaia ID is recorded as 443389200756458752[21].