Q78471718
red giant branch star in the constellation Hercules
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Q78471718
Summary
Q78471718 is a red giant branch star[1].
Key Facts
- Q78471718's instance of is recorded as red giant branch star[2].
- Q78471718's constellation is recorded as Hercules[3].
- Q78471718's catalog code is recorded as 2MASS J16445292+4807189[4].
- Q78471718's catalog code is recorded as Gaia DR2 1408866272293897344[5].
- Q78471718's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.603'}[6].
- Q78471718's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.108'}[7].
- Q78471718's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.031'}[8].
- Q78471718's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.0355'}[9].
- Q78471718's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3017'}[10].
- Q78471718's metallicity is recorded as {'unit': '1', 'amount': '-0.331'}[11].
- Q78471718's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3314.5509'}[12].
- Q78471718's SIMBAD ID is recorded as 2MASS J16445292+4807189[13].
- Q78471718's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+251.22048624479980'}[14].
- Q78471718's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.12194254076360'}[15].
- Q78471718's epoch is recorded as J2000.0[16].
- Q78471718's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4933'}[17].
- Q78471718's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1585'}[18].
- Q78471718's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.564'}[19].
- Q78471718's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.644'}[20].
- Q78471718's Gaia ID is recorded as 1408866272293897344[21].