Q80537526
star in the constellation Cygnus
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Q80537526
Summary
Q80537526 is a star[1].
Key Facts
- Q80537526's instance of is recorded as star[2].
- Q80537526's constellation is recorded as Cygnus[3].
- Q80537526's spectral class is recorded as F6IV-Vs[4].
- Q80537526's catalog code is recorded as Gaia DR2 2074318953158630144[5].
- Q80537526's catalog code is recorded as KIC 5483545[6].
- Q80537526's catalog code is recorded as 2MASS J20001382+4039428[7].
- Q80537526's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6408'}[8].
- Q80537526's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.378'}[9].
- Q80537526's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.095'}[10].
- Q80537526's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.004'}[11].
- Q80537526's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7361'}[12].
- Q80537526's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+1.4'}[13].
- Q80537526's metallicity is recorded as {'unit': '1', 'amount': '+0.03'}[14].
- Q80537526's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1358.51'}[15].
- Q80537526's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+300.05762536789507'}[16].
- Q80537526's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.66189043383444'}[17].
- Q80537526's epoch is recorded as J2000.0[18].
- Q80537526's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6222'}[19].
- Q80537526's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.631'}[20].
- Q80537526's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.191'}[21].
Body
Definition and Type
Q80537526's instance of is recorded as star[2].