Q94178047
star in the constellation Cygnus
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Q94178047
Summary
Q94178047 is a star[1].
Key Facts
- Q94178047's instance of is recorded as star[2].
- Q94178047's constellation is recorded as Cygnus[3].
- Q94178047's spectral class is recorded as K3V[4].
- Q94178047's catalog code is recorded as Gaia DR2 2132781292050783872[5].
- Q94178047's catalog code is recorded as KIC 11604061[6].
- Q94178047's catalog code is recorded as 2MASS J19122993+4936019[7].
- Q94178047's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.4088'}[8].
- Q94178047's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.862'}[9].
- Q94178047's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.280'}[10].
- Q94178047's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.214'}[11].
- Q94178047's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.8918'}[12].
- Q94178047's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-65.3'}[13].
- Q94178047's metallicity is recorded as {'unit': '1', 'amount': '-0.02'}[14].
- Q94178047's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+256.951'}[15].
- Q94178047's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+288.12479596265290'}[16].
- Q94178047's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.60051992119111'}[17].
- Q94178047's epoch is recorded as J2000.0[18].
- Q94178047's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4558'}[19].
- Q94178047's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-12.084'}[20].
- Q94178047's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-16.188'}[21].
Body
Definition and Type
Q94178047's instance of is recorded as star[2].