Q90445088
star in the constellation Aquila
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Q90445088
Summary
Q90445088 is a star[1].
Key Facts
- Q90445088's instance of is recorded as star[2].
- Q90445088's constellation is recorded as Aquila[3].
- Q90445088's spectral class is recorded as F6V[4].
- Q90445088's catalog code is recorded as BD-05 4995[5].
- Q90445088's catalog code is recorded as GSC 05152-02036[6].
- Q90445088's catalog code is recorded as HD 183961[7].
- Q90445088's catalog code is recorded as PPM 203006[8].
- Q90445088's catalog code is recorded as SAO 143513[9].
- Q90445088's catalog code is recorded as TYC 5152-2036-1[10].
- Q90445088's catalog code is recorded as YZ 95 6677[11].
- Q90445088's catalog code is recorded as 2MASS J19321337-0511018[12].
- Q90445088's catalog code is recorded as Gaia DR2 4210039063668551296[13].
- Q90445088's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.250'}[14].
- Q90445088's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.014'}[15].
- Q90445088's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.917'}[16].
- Q90445088's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.55'}[17].
- Q90445088's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.21'}[18].
- Q90445088's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3630'}[19].
- Q90445088's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.6434'}[20].
- Q90445088's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+12.33'}[21].
- Q90445088's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+177.1981'}[22].
- Q90445088's SIMBAD ID is recorded as HD 183961[23].
- Q90445088's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.05574785053050'}[24].
- Q90445088's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-5.18385951447440'}[25].
- Q90445088's epoch is recorded as J2000.0[26].