Q80539824
star in the constellation Cygnus
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Q80539824
Summary
Q80539824 is a star[1].
Key Facts
- Q80539824's instance of is recorded as star[2].
- Q80539824's constellation is recorded as Cygnus[3].
- Q80539824's spectral class is recorded as K3V[4].
- Q80539824's catalog code is recorded as Gaia DR2 2051741306494116864[5].
- Q80539824's catalog code is recorded as KIC 2163351[6].
- Q80539824's catalog code is recorded as 2MASS J19282985+3730538[7].
- Q80539824's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2023'}[8].
- Q80539824's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.592'}[9].
- Q80539824's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.056'}[10].
- Q80539824's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.961'}[11].
- Q80539824's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.5970'}[12].
- Q80539824's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-39.82'}[13].
- Q80539824's metallicity is recorded as {'unit': '1', 'amount': '-0.05'}[14].
- Q80539824's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+217.533'}[15].
- Q80539824's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.12437718998785'}[16].
- Q80539824's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.51495993630056'}[17].
- Q80539824's epoch is recorded as J2000.0[18].
- Q80539824's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4571'}[19].
- Q80539824's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+24.879'}[20].
- Q80539824's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+27.206'}[21].
Body
Definition and Type
Q80539824's instance of is recorded as star[2].