Q90895162
star in the constellation Cygnus
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Q90895162
Summary
Q90895162 is a star[1].
Key Facts
- Q90895162's instance of is recorded as star[2].
- Q90895162's constellation is recorded as Cygnus[3].
- Q90895162's spectral class is recorded as K1V[4].
- Q90895162's catalog code is recorded as Gaia DR2 2126307127071189120[5].
- Q90895162's catalog code is recorded as KIC 8170212[6].
- Q90895162's catalog code is recorded as 2MASS J19334285+4404316[7].
- Q90895162's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.1352'}[8].
- Q90895162's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.599'}[9].
- Q90895162's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.102'}[10].
- Q90895162's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.001'}[11].
- Q90895162's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9014'}[12].
- Q90895162's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-29.92'}[13].
- Q90895162's metallicity is recorded as {'unit': '1', 'amount': '+0.02'}[14].
- Q90895162's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1109.39'}[15].
- Q90895162's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.42854755718050'}[16].
- Q90895162's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.07545520748555'}[17].
- Q90895162's epoch is recorded as J2000.0[18].
- Q90895162's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5043'}[19].
- Q90895162's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.696'}[20].
- Q90895162's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+10.540'}[21].
Body
Definition and Type
Q90895162's instance of is recorded as star[2].