Q85088710
star in the constellation Boötes
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Q85088710
Summary
Q85088710 is a star[1].
Key Facts
- Q85088710's instance of is recorded as star[2].
- Q85088710's constellation is recorded as Boötes[3].
- Q85088710's spectral class is recorded as K0[4].
- Q85088710's catalog code is recorded as AG+16 1444[5].
- Q85088710's catalog code is recorded as BD+17 2778[6].
- Q85088710's catalog code is recorded as GSC 01477-00271[7].
- Q85088710's catalog code is recorded as PPM 130824[8].
- Q85088710's catalog code is recorded as SAO 101178[9].
- Q85088710's catalog code is recorded as TYC 1477-271-1[10].
- Q85088710's catalog code is recorded as YZ 16 5318[11].
- Q85088710's catalog code is recorded as 2MASS J14442781+1645593[12].
- Q85088710's catalog code is recorded as Gaia DR2 1234762316886144768[13].
- Q85088710's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.49'}[14].
- Q85088710's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.44'}[15].
- Q85088710's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.855'}[16].
- Q85088710's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.361'}[17].
- Q85088710's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.254'}[18].
- Q85088710's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3165'}[19].
- Q85088710's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6362'}[20].
- Q85088710's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.08'}[21].
- Q85088710's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+611.1722'}[22].
- Q85088710's SIMBAD ID is recorded as BD+17 2778[23].
- Q85088710's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+221.11588489304450'}[24].
- Q85088710's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+16.76646083522720'}[25].
- Q85088710's epoch is recorded as J2000.0[26].