Q90078614
star in the constellation Cygnus
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Q90078614
Summary
Q90078614 is a star[1].
Key Facts
- Q90078614's instance of is recorded as star[2].
- Q90078614's constellation is recorded as Cygnus[3].
- Q90078614's spectral class is recorded as G0.5V[4].
- Q90078614's catalog code is recorded as Gaia DR2 2139346819577325312[5].
- Q90078614's catalog code is recorded as KIC 13032621[6].
- Q90078614's catalog code is recorded as 2MASS J19193337+5235450[7].
- Q90078614's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9812'}[8].
- Q90078614's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.970'}[9].
- Q90078614's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.668'}[10].
- Q90078614's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.619'}[11].
- Q90078614's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4692'}[12].
- Q90078614's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-25.6'}[13].
- Q90078614's metallicity is recorded as {'unit': '1', 'amount': '-0.10'}[14].
- Q90078614's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+680.643'}[15].
- Q90078614's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.88905071592126'}[16].
- Q90078614's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.59585893159250'}[17].
- Q90078614's epoch is recorded as J2000.0[18].
- Q90078614's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5777'}[19].
- Q90078614's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.484'}[20].
- Q90078614's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.171'}[21].
Body
Definition and Type
Q90078614's instance of is recorded as star[2].