Q80535577
star in the constellation Cygnus
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Q80535577
Summary
Q80535577 is a star[1].
Key Facts
- Q80535577's instance of is recorded as star[2].
- Q80535577's constellation is recorded as Cygnus[3].
- Q80535577's spectral class is recorded as G0V[4].
- Q80535577's catalog code is recorded as Gaia DR2 2053628171526555648[5].
- Q80535577's catalog code is recorded as KIC 6125433[6].
- Q80535577's catalog code is recorded as 2MASS J19293708+4129313[7].
- Q80535577's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7996'}[8].
- Q80535577's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.729'}[9].
- Q80535577's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.412'}[10].
- Q80535577's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.367'}[11].
- Q80535577's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6417'}[12].
- Q80535577's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+9.3'}[13].
- Q80535577's metallicity is recorded as {'unit': '1', 'amount': '-0.10'}[14].
- Q80535577's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1558.36'}[15].
- Q80535577's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.40447380229546'}[16].
- Q80535577's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+41.49206357071694'}[17].
- Q80535577's epoch is recorded as J2000.0[18].
- Q80535577's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6103'}[19].
- Q80535577's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.594'}[20].
- Q80535577's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.179'}[21].
Body
Definition and Type
Q80535577's instance of is recorded as star[2].