Q80535800
star in the constellation Cygnus
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Q80535800
Summary
Q80535800 is a star[1].
Key Facts
- Q80535800's instance of is recorded as star[2].
- Q80535800's constellation is recorded as Cygnus[3].
- Q80535800's spectral class is recorded as K1II[4].
- Q80535800's catalog code is recorded as Gaia DR2 2052253438395948416[5].
- Q80535800's catalog code is recorded as KIC 3123577[6].
- Q80535800's catalog code is recorded as 2MASS J19321412+3814309[7].
- Q80535800's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9334'}[8].
- Q80535800's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.114'}[9].
- Q80535800's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.481'}[10].
- Q80535800's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.370'}[11].
- Q80535800's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4076'}[12].
- Q80535800's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.27'}[13].
- Q80535800's metallicity is recorded as {'unit': '1', 'amount': '-0.11'}[14].
- Q80535800's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2453.39'}[15].
- Q80535800's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.05884293859590'}[16].
- Q80535800's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+38.24191365256139'}[17].
- Q80535800's epoch is recorded as J2000.0[18].
- Q80535800's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4850'}[19].
- Q80535800's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.580'}[20].
- Q80535800's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.931'}[21].
Body
Definition and Type
Q80535800's instance of is recorded as star[2].