Q90966407
star in the constellation Pegasus
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Q90966407
Summary
Q90966407 is a star[1].
Key Facts
- Q90966407's instance of is recorded as star[2].
- Q90966407's constellation is recorded as Pegasus[3].
- Q90966407's spectral class is recorded as K5[4].
- Q90966407's catalog code is recorded as AG+21 2504[5].
- Q90966407's catalog code is recorded as BD+20 5182[6].
- Q90966407's catalog code is recorded as GSC 01708-00005[7].
- Q90966407's catalog code is recorded as PPM 114566[8].
- Q90966407's catalog code is recorded as SAO 90593[9].
- Q90966407's catalog code is recorded as TYC 1708-5-1[10].
- Q90966407's catalog code is recorded as YZ 21 8672[11].
- Q90966407's catalog code is recorded as 2MASS J22330944+2115533[12].
- Q90966407's catalog code is recorded as Gaia DR2 1873774388773280640[13].
- Q90966407's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.40'}[14].
- Q90966407's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.154'}[15].
- Q90966407's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.506'}[16].
- Q90966407's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.361'}[17].
- Q90966407's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.69'}[18].
- Q90966407's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0264'}[19].
- Q90966407's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0495'}[20].
- Q90966407's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-25.87'}[21].
- Q90966407's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+952.8347'}[22].
- Q90966407's SIMBAD ID is recorded as BD+20 5182[23].
- Q90966407's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+338.28937259173800'}[24].
- Q90966407's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+21.26482845163450'}[25].
- Q90966407's epoch is recorded as J2000.0[26].