Q94178131
star in the constellation Cygnus
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Q94178131
Summary
Q94178131 is a star[1].
Key Facts
- Q94178131's instance of is recorded as star[2].
- Q94178131's constellation is recorded as Cygnus[3].
- Q94178131's spectral class is recorded as G8IV-V[4].
- Q94178131's catalog code is recorded as Gaia DR2 2132672165521844096[5].
- Q94178131's catalog code is recorded as KIC 11553836[6].
- Q94178131's catalog code is recorded as 2MASS J19153088+4931479[7].
- Q94178131's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.8809'}[8].
- Q94178131's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.429'}[9].
- Q94178131's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.926'}[10].
- Q94178131's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.836'}[11].
- Q94178131's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5869'}[12].
- Q94178131's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.1'}[13].
- Q94178131's metallicity is recorded as {'unit': '1', 'amount': '-0.15'}[14].
- Q94178131's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1703.87'}[15].
- Q94178131's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+288.87872764478084'}[16].
- Q94178131's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.52998771571249'}[17].
- Q94178131's epoch is recorded as J2000.0[18].
- Q94178131's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5020'}[19].
- Q94178131's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.497'}[20].
- Q94178131's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.097'}[21].
Body
Definition and Type
Q94178131's instance of is recorded as star[2].