Q80536118
star in the constellation Cygnus
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Q80536118
Summary
Q80536118 is a star[1].
Key Facts
- Q80536118's instance of is recorded as star[2].
- Q80536118's constellation is recorded as Cygnus[3].
- Q80536118's spectral class is recorded as K2V[4].
- Q80536118's catalog code is recorded as Gaia DR2 2051665921231275520[5].
- Q80536118's catalog code is recorded as KIC 2451465[6].
- Q80536118's catalog code is recorded as 2MASS J19325640+3743360[7].
- Q80536118's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.4775'}[8].
- Q80536118's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.039'}[9].
- Q80536118's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.551'}[10].
- Q80536118's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.276'}[11].
- Q80536118's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8325'}[12].
- Q80536118's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-2.5'}[13].
- Q80536118's metallicity is recorded as {'unit': '1', 'amount': '-0.04'}[14].
- Q80536118's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1201.2'}[15].
- Q80536118's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.23499001598750'}[16].
- Q80536118's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.72668688591388'}[17].
- Q80536118's epoch is recorded as J2000.0[18].
- Q80536118's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5125'}[19].
- Q80536118's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-10.505'}[20].
- Q80536118's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.580'}[21].
Body
Definition and Type
Q80536118's instance of is recorded as star[2].