Q86956817
star in the constellation Cygnus
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Q86956817
Summary
Q86956817 is a star[1].
Key Facts
- Q86956817's instance of is recorded as star[2].
- Q86956817's constellation is recorded as Cygnus[3].
- Q86956817's spectral class is recorded as G5V:[4].
- Q86956817's catalog code is recorded as Gaia DR2 2136283580181949824[5].
- Q86956817's catalog code is recorded as KIC 12694492[6].
- Q86956817's catalog code is recorded as 2MASS J19292045+5149218[7].
- Q86956817's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3539'}[8].
- Q86956817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.878'}[9].
- Q86956817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.396'}[10].
- Q86956817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.306'}[11].
- Q86956817's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9798'}[12].
- Q86956817's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+0.49'}[13].
- Q86956817's metallicity is recorded as {'unit': '1', 'amount': '-0.21'}[14].
- Q86956817's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1020.62'}[15].
- Q86956817's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.33526705349834'}[16].
- Q86956817's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+51.82273737965723'}[17].
- Q86956817's epoch is recorded as J2000.0[18].
- Q86956817's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5438'}[19].
- Q86956817's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-13.199'}[20].
- Q86956817's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.129'}[21].
Body
Definition and Type
Q86956817's instance of is recorded as star[2].