Q85522541
star in the constellation Boötes
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Q85522541
Summary
Q85522541 is a star[1].
Key Facts
- Q85522541's instance of is recorded as star[2].
- Q85522541's constellation is recorded as Boötes[3].
- Q85522541's spectral class is recorded as K2[4].
- Q85522541's catalog code is recorded as AG+08 1812[5].
- Q85522541's catalog code is recorded as BD+08 2979[6].
- Q85522541's catalog code is recorded as GSC 00920-00321[7].
- Q85522541's catalog code is recorded as PPM 161312[8].
- Q85522541's catalog code is recorded as SAO 120868[9].
- Q85522541's catalog code is recorded as TYC 920-321-1[10].
- Q85522541's catalog code is recorded as YZ 8 6915[11].
- Q85522541's catalog code is recorded as 2MASS J15091145+0821221[12].
- Q85522541's catalog code is recorded as Gaia DR2 1166768449105322368[13].
- Q85522541's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.877'}[14].
- Q85522541's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.153'}[15].
- Q85522541's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.963'}[16].
- Q85522541's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.28'}[17].
- Q85522541's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.62'}[18].
- Q85522541's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8264'}[19].
- Q85522541's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2561'}[20].
- Q85522541's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-55.57'}[21].
- Q85522541's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+796.1150'}[22].
- Q85522541's SIMBAD ID is recorded as BD+08 2979[23].
- Q85522541's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+227.29770003659900'}[24].
- Q85522541's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+8.35613069732400'}[25].
- Q85522541's epoch is recorded as J2000.0[26].