Q81050001
star in the constellation Cygnus
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Q81050001
Summary
Q81050001 is a star[1].
Key Facts
- Q81050001's instance of is recorded as star[2].
- Q81050001's constellation is recorded as Cygnus[3].
- Q81050001's spectral class is recorded as K1V[4].
- Q81050001's catalog code is recorded as KIC 4168344[5].
- Q81050001's catalog code is recorded as 2MASS J19362836+3912407[6].
- Q81050001's catalog code is recorded as Gaia DR2 2052392011221367552[7].
- Q81050001's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.187'}[8].
- Q81050001's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.718'}[9].
- Q81050001's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.659'}[10].
- Q81050001's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.5823'}[11].
- Q81050001's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.1135'}[12].
- Q81050001's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-54.2'}[13].
- Q81050001's metallicity is recorded as {'unit': '1', 'amount': '-0.02'}[14].
- Q81050001's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+321.1819'}[15].
- Q81050001's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+294.11822025163990'}[16].
- Q81050001's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.21130253575380'}[17].
- Q81050001's epoch is recorded as J2000.0[18].
- Q81050001's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5093'}[19].
- Q81050001's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-25.580'}[20].
- Q81050001's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+11.677'}[21].
Body
Definition and Type
Q81050001's instance of is recorded as star[2].