Q84240917
red giant branch star in the constellation Perseus
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Q84240917
Summary
Q84240917 is a red giant branch star[1].
Key Facts
- Q84240917's instance of is recorded as red giant branch star[2].
- Q84240917's constellation is recorded as Perseus[3].
- Q84240917's catalog code is recorded as 2MASS J02050194+4926464[4].
- Q84240917's catalog code is recorded as Gaia DR2 358357369508542080[5].
- Q84240917's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.529'}[6].
- Q84240917's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.052'}[7].
- Q84240917's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.861'}[8].
- Q84240917's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1554'}[9].
- Q84240917's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3724'}[10].
- Q84240917's metallicity is recorded as {'unit': '1', 'amount': '-0.109'}[11].
- Q84240917's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2685.2846'}[12].
- Q84240917's SIMBAD ID is recorded as 2MASS J02050194+4926464[13].
- Q84240917's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+31.25810315993080'}[14].
- Q84240917's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.44622705211020'}[15].
- Q84240917's epoch is recorded as J2000.0[16].
- Q84240917's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4977'}[17].
- Q84240917's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1480'}[18].
- Q84240917's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.341'}[19].
- Q84240917's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.290'}[20].
- Q84240917's Gaia ID is recorded as 358357369508542080[21].