Q85476818
star in the constellation Corvus
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Q85476818
Summary
Q85476818 is a star[1].
Key Facts
- Q85476818's instance of is recorded as star[2].
- Q85476818's constellation is recorded as Corvus[3].
- Q85476818's spectral class is recorded as G0[4].
- Q85476818's catalog code is recorded as BD-18 3448[5].
- Q85476818's catalog code is recorded as GSC 06107-00548[6].
- Q85476818's catalog code is recorded as PPM 226230[7].
- Q85476818's catalog code is recorded as SAO 157459[8].
- Q85476818's catalog code is recorded as TYC 6107-548-1[9].
- Q85476818's catalog code is recorded as YZ 0 6295[10].
- Q85476818's catalog code is recorded as YZ 108 4866[11].
- Q85476818's catalog code is recorded as 2MASS J12424451-1852092[12].
- Q85476818's catalog code is recorded as Gaia DR2 3521907821632136832[13].
- Q85476818's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.561'}[14].
- Q85476818's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.077'}[15].
- Q85476818's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.910'}[16].
- Q85476818's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.34'}[17].
- Q85476818's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.28'}[18].
- Q85476818's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0698'}[19].
- Q85476818's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.1940'}[20].
- Q85476818's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-6.70'}[21].
- Q85476818's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+455.7885'}[22].
- Q85476818's SIMBAD ID is recorded as BD-18 3448[23].
- Q85476818's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+190.68549114108920'}[24].
- Q85476818's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-18.86926475387500'}[25].
- Q85476818's epoch is recorded as J2000.0[26].