Q92979883
star in the constellation Cygnus
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Q92979883
Summary
Q92979883 is a star[1].
Key Facts
- Q92979883's instance of is recorded as star[2].
- Q92979883's constellation is recorded as Cygnus[3].
- Q92979883's spectral class is recorded as K3III[4].
- Q92979883's catalog code is recorded as Gaia DR2 2129929055809249920[5].
- Q92979883's catalog code is recorded as KIC 11401437[6].
- Q92979883's catalog code is recorded as 2MASS J19241895+4912579[7].
- Q92979883's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6909'}[8].
- Q92979883's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.964'}[9].
- Q92979883's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.336'}[10].
- Q92979883's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.224'}[11].
- Q92979883's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2225'}[12].
- Q92979883's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-41.5'}[13].
- Q92979883's metallicity is recorded as {'unit': '1', 'amount': '-0.04'}[14].
- Q92979883's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4494.38'}[15].
- Q92979883's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.07897338417290'}[16].
- Q92979883's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.21607378811834'}[17].
- Q92979883's epoch is recorded as J2000.0[18].
- Q92979883's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4433'}[19].
- Q92979883's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.344'}[20].
- Q92979883's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.181'}[21].
Body
Definition and Type
Q92979883's instance of is recorded as star[2].