Q85341786
horizontal branch star in the constellation Capricornus
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Q85341786
Summary
Q85341786 is a horizontal branch star[1].
Key Facts
- Q85341786's instance of is recorded as horizontal branch star[2].
- Q85341786's constellation is recorded as Capricornus[3].
- Q85341786's catalog code is recorded as [LML2013] 10301793[4].
- Q85341786's catalog code is recorded as Gaia DR2 6816581112749746816[5].
- Q85341786's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.62'}[6].
- Q85341786's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.57'}[7].
- Q85341786's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.5409'}[8].
- Q85341786's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1326'}[9].
- Q85341786's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-177.9'}[10].
- Q85341786's metallicity is recorded as {'unit': '1', 'amount': '-2.22'}[11].
- Q85341786's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19'}[12].
- Q85341786's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+325.12025769284730'}[13].
- Q85341786's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-23.17370128815620'}[14].
- Q85341786's epoch is recorded as J2000.0[15].
- Q85341786's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+9376'}[16].
- Q85341786's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+2500'}[17].
- Q85341786's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.993'}[18].
- Q85341786's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.790'}[19].
Body
Definition and Type
Q85341786's instance of is recorded as horizontal branch star[2].