Q90896506
star in the constellation Cygnus
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Q90896506
Summary
Q90896506 is a star[1].
Key Facts
- Q90896506's instance of is recorded as star[2].
- Q90896506's constellation is recorded as Cygnus[3].
- Q90896506's spectral class is recorded as K1III[4].
- Q90896506's catalog code is recorded as Gaia DR2 2078098936675109504[5].
- Q90896506's catalog code is recorded as KIC 7901860[6].
- Q90896506's catalog code is recorded as 2MASS J19413335+4341209[7].
- Q90896506's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.8689'}[8].
- Q90896506's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.994'}[9].
- Q90896506's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.390'}[10].
- Q90896506's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.279'}[11].
- Q90896506's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2534'}[12].
- Q90896506's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-20.9'}[13].
- Q90896506's metallicity is recorded as {'unit': '1', 'amount': '-0.09'}[14].
- Q90896506's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3946.33'}[15].
- Q90896506's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.38894089972000'}[16].
- Q90896506's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.68913758360139'}[17].
- Q90896506's epoch is recorded as J2000.0[18].
- Q90896506's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4734'}[19].
- Q90896506's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.943'}[20].
- Q90896506's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.911'}[21].
Body
Definition and Type
Q90896506's instance of is recorded as star[2].