Q93954519
star in the constellation Cygnus
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Q93954519
Summary
Q93954519 is a star[1].
Key Facts
- Q93954519's instance of is recorded as star[2].
- Q93954519's constellation is recorded as Cygnus[3].
- Q93954519's spectral class is recorded as K0III[4].
- Q93954519's catalog code is recorded as Gaia DR2 2079610765161367936[5].
- Q93954519's catalog code is recorded as KIC 8177203[6].
- Q93954519's catalog code is recorded as 2MASS J19423457+4402294[7].
- Q93954519's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7117'}[8].
- Q93954519's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.831'}[9].
- Q93954519's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.185'}[10].
- Q93954519's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.038'}[11].
- Q93954519's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2916'}[12].
- Q93954519's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-33.0'}[13].
- Q93954519's metallicity is recorded as {'unit': '1', 'amount': '-0.03'}[14].
- Q93954519's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3429.36'}[15].
- Q93954519's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.64406899260246'}[16].
- Q93954519's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.04149717877944'}[17].
- Q93954519's epoch is recorded as J2000.0[18].
- Q93954519's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4648'}[19].
- Q93954519's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-7.977'}[20].
- Q93954519's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.381'}[21].
Body
Definition and Type
Q93954519's instance of is recorded as star[2].