Q93718941
star in the constellation Cygnus
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Q93718941
Summary
Q93718941 is a star[1].
Key Facts
- Q93718941's instance of is recorded as star[2].
- Q93718941's constellation is recorded as Cygnus[3].
- Q93718941's spectral class is recorded as K2V[4].
- Q93718941's catalog code is recorded as Gaia DR2 2129914482983292416[5].
- Q93718941's catalog code is recorded as KIC 11915075[6].
- Q93718941's catalog code is recorded as 2MASS J19284396+5015251[7].
- Q93718941's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4479'}[8].
- Q93718941's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.953'}[9].
- Q93718941's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.489'}[10].
- Q93718941's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.353'}[11].
- Q93718941's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.1862'}[12].
- Q93718941's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.72'}[13].
- Q93718941's metallicity is recorded as {'unit': '1', 'amount': '+0.07'}[14].
- Q93718941's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+238.88'}[15].
- Q93718941's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.18313913203207'}[16].
- Q93718941's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.25697034397084'}[17].
- Q93718941's epoch is recorded as J2000.0[18].
- Q93718941's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5128'}[19].
- Q93718941's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+20.424'}[20].
- Q93718941's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.463'}[21].
Body
Definition and Type
Q93718941's instance of is recorded as star[2].