Q85430278
star in the constellation Cygnus
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Q85430278
Summary
Q85430278 is a star[1].
Key Facts
- Q85430278's instance of is recorded as star[2].
- Q85430278's constellation is recorded as Cygnus[3].
- Q85430278's spectral class is recorded as A7[4].
- Q85430278's catalog code is recorded as AG+35 1907[5].
- Q85430278's catalog code is recorded as BD+35 3885[6].
- Q85430278's catalog code is recorded as GSC 02682-03459[7].
- Q85430278's catalog code is recorded as HD 226780[8].
- Q85430278's catalog code is recorded as PPM 83893[9].
- Q85430278's catalog code is recorded as SAO 69152[10].
- Q85430278's catalog code is recorded as TYC 2682-3459-1[11].
- Q85430278's catalog code is recorded as 2MASS J19572811+3603467[12].
- Q85430278's catalog code is recorded as Gaia DR2 2059714380740011520[13].
- Q85430278's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.998'}[14].
- Q85430278's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.918'}[15].
- Q85430278's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.821'}[16].
- Q85430278's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.783'}[17].
- Q85430278's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.62'}[18].
- Q85430278's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.5578'}[19].
- Q85430278's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.8606'}[20].
- Q85430278's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+23.72'}[21].
- Q85430278's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+145.7598'}[22].
- Q85430278's SIMBAD ID is recorded as HD 226780[23].
- Q85430278's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+299.36714801214460'}[24].
- Q85430278's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+36.06300468243230'}[25].
- Q85430278's epoch is recorded as J2000.0[26].