Q88105180
star in the constellation Aquila
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Q88105180
Summary
Q88105180 is a star[1].
Key Facts
- Q88105180's instance of is recorded as star[2].
- Q88105180's constellation is recorded as Aquila[3].
- Q88105180's spectral class is recorded as G3IV[4].
- Q88105180's catalog code is recorded as BD-10 5105[5].
- Q88105180's catalog code is recorded as GSC 05726-00663[6].
- Q88105180's catalog code is recorded as HD 183854[7].
- Q88105180's catalog code is recorded as PPM 202999[8].
- Q88105180's catalog code is recorded as SAO 143504[9].
- Q88105180's catalog code is recorded as TYC 5726-663-1[10].
- Q88105180's catalog code is recorded as YZ 99 6841[11].
- Q88105180's catalog code is recorded as 2MASS J19315058-0950493[12].
- Q88105180's catalog code is recorded as Gaia DR2 4194282512286505088[13].
- Q88105180's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.31'}[14].
- Q88105180's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.429'}[15].
- Q88105180's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.945'}[16].
- Q88105180's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.801'}[17].
- Q88105180's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.19'}[18].
- Q88105180's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9825'}[19].
- Q88105180's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.5779'}[20].
- Q88105180's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.68'}[21].
- Q88105180's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+279.4936'}[22].
- Q88105180's SIMBAD ID is recorded as HD 183854[23].
- Q88105180's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.96079576599180'}[24].
- Q88105180's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-9.84703636559040'}[25].
- Q88105180's epoch is recorded as J2000.0[26].