Q87111220
star in the constellation Cygnus
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Q87111220
Summary
Q87111220 is a star[1].
Key Facts
- Q87111220's instance of is recorded as star[2].
- Q87111220's constellation is recorded as Cygnus[3].
- Q87111220's spectral class is recorded as K2III[4].
- Q87111220's catalog code is recorded as Gaia DR2 2136277086191288576[5].
- Q87111220's catalog code is recorded as KIC 12604697[6].
- Q87111220's catalog code is recorded as 2MASS J19280486+5138509[7].
- Q87111220's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.0580'}[8].
- Q87111220's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.282'}[9].
- Q87111220's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.694'}[10].
- Q87111220's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.592'}[11].
- Q87111220's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4172'}[12].
- Q87111220's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-8.02'}[13].
- Q87111220's metallicity is recorded as {'unit': '1', 'amount': '+0.01'}[14].
- Q87111220's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2396.93'}[15].
- Q87111220's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.02024295305330'}[16].
- Q87111220's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+51.64748283811610'}[17].
- Q87111220's epoch is recorded as J2000.0[18].
- Q87111220's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4629'}[19].
- Q87111220's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.900'}[20].
- Q87111220's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.199'}[21].
Body
Definition and Type
Q87111220's instance of is recorded as star[2].