Q90352792
star in the constellation Cygnus
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Q90352792
Summary
Q90352792 is a star[1].
Key Facts
- Q90352792's instance of is recorded as star[2].
- Q90352792's constellation is recorded as Cygnus[3].
- Q90352792's spectral class is recorded as G8.5IIIb[4].
- Q90352792's catalog code is recorded as Gaia DR2 2129247839637928832[5].
- Q90352792's catalog code is recorded as KIC 10665770[6].
- Q90352792's catalog code is recorded as 2MASS J19273916+4759060[7].
- Q90352792's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9916'}[8].
- Q90352792's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.170'}[9].
- Q90352792's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.605'}[10].
- Q90352792's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.434'}[11].
- Q90352792's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1877'}[12].
- Q90352792's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-25.29'}[13].
- Q90352792's metallicity is recorded as {'unit': '1', 'amount': '-0.28'}[14].
- Q90352792's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.91323180285040'}[15].
- Q90352792's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+47.98500755803361'}[16].
- Q90352792's epoch is recorded as J2000.0[17].
- Q90352792's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4817'}[18].
- Q90352792's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+320'}[19].
- Q90352792's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.650'}[20].
- Q90352792's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.024'}[21].
Body
Definition and Type
Q90352792's instance of is recorded as star[2].