Q80545492
star in the constellation Lyra
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Q80545492
Summary
Q80545492 is a star[1].
Key Facts
- Q80545492's instance of is recorded as star[2].
- Q80545492's constellation is recorded as Lyra[3].
- Q80545492's spectral class is recorded as G8V[4].
- Q80545492's catalog code is recorded as Gaia DR2 2099174272473317504[5].
- Q80545492's catalog code is recorded as KIC 2424240[6].
- Q80545492's catalog code is recorded as 2MASS J19062627+3747177[7].
- Q80545492's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.3645'}[8].
- Q80545492's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.797'}[9].
- Q80545492's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.294'}[10].
- Q80545492's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.181'}[11].
- Q80545492's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1898'}[12].
- Q80545492's metallicity is recorded as {'unit': '1', 'amount': '-0.36'}[13].
- Q80545492's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+149'}[14].
- Q80545492's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+286.60946779789460'}[15].
- Q80545492's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.78823516789333'}[16].
- Q80545492's epoch is recorded as J2000.0[17].
- Q80545492's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4920'}[18].
- Q80545492's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+600'}[19].
- Q80545492's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.630'}[20].
- Q80545492's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.900'}[21].
Body
Definition and Type
Q80545492's instance of is recorded as star[2].