Q90896610
star in the constellation Cygnus
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Q90896610
Summary
Q90896610 is a star[1].
Key Facts
- Q90896610's instance of is recorded as star[2].
- Q90896610's constellation is recorded as Cygnus[3].
- Q90896610's spectral class is recorded as K1.5III[4].
- Q90896610's catalog code is recorded as Gaia DR2 2125957825971622784[5].
- Q90896610's catalog code is recorded as KIC 8030745[6].
- Q90896610's catalog code is recorded as 2MASS J19301099+4348286[7].
- Q90896610's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9988'}[8].
- Q90896610's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.275'}[9].
- Q90896610's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.707'}[10].
- Q90896610's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.610'}[11].
- Q90896610's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1591'}[12].
- Q90896610's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-22.4'}[13].
- Q90896610's metallicity is recorded as {'unit': '1', 'amount': '+0.00'}[14].
- Q90896610's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.54577800631415'}[15].
- Q90896610's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.80795860624944'}[16].
- Q90896610's epoch is recorded as J2000.0[17].
- Q90896610's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4631'}[18].
- Q90896610's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+355'}[19].
- Q90896610's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.557'}[20].
- Q90896610's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.956'}[21].
Body
Definition and Type
Q90896610's instance of is recorded as star[2].