Q94177281
star in the constellation Cygnus
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Q94177281
Summary
Q94177281 is a star[1].
Key Facts
- Q94177281's instance of is recorded as star[2].
- Q94177281's constellation is recorded as Cygnus[3].
- Q94177281's spectral class is recorded as G5III-IVp[4].
- Q94177281's catalog code is recorded as Gaia DR2 2132673196314038272[5].
- Q94177281's catalog code is recorded as KIC 11605285[6].
- Q94177281's catalog code is recorded as 2MASS J19151970+4939037[7].
- Q94177281's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8347'}[8].
- Q94177281's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.377'}[9].
- Q94177281's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.900'}[10].
- Q94177281's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.832'}[11].
- Q94177281's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2193'}[12].
- Q94177281's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+2.18'}[13].
- Q94177281's metallicity is recorded as {'unit': '1', 'amount': '-0.59'}[14].
- Q94177281's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+288.83214813294876'}[15].
- Q94177281's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.65104164335472'}[16].
- Q94177281's epoch is recorded as J2000.0[17].
- Q94177281's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4974'}[18].
- Q94177281's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+320'}[19].
- Q94177281's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.246'}[20].
- Q94177281's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.274'}[21].
Body
Definition and Type
Q94177281's instance of is recorded as star[2].