Q76742598
star in the constellation Cygnus
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Q76742598
Summary
Q76742598 is a star[1].
Key Facts
- Q76742598's instance of is recorded as star[2].
- Q76742598's constellation is recorded as Cygnus[3].
- Q76742598's spectral class is recorded as G0V[4].
- Q76742598's catalog code is recorded as Gaia DR2 2134910633759357952[5].
- Q76742598's catalog code is recorded as KIC 11722058[6].
- Q76742598's catalog code is recorded as 2MASS J19444528+4951551[7].
- Q76742598's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8738'}[8].
- Q76742598's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.910'}[9].
- Q76742598's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.637'}[10].
- Q76742598's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.589'}[11].
- Q76742598's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5431'}[12].
- Q76742598's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.37'}[13].
- Q76742598's metallicity is recorded as {'unit': '1', 'amount': '+0.10'}[14].
- Q76742598's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+296.18864455678750'}[15].
- Q76742598's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.86529633285361'}[16].
- Q76742598's epoch is recorded as J2000.0[17].
- Q76742598's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6054'}[18].
- Q76742598's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+12000'}[19].
- Q76742598's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.535'}[20].
- Q76742598's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.855'}[21].
Body
Definition and Type
Q76742598's instance of is recorded as star[2].