Q80544842
star in the constellation Cygnus
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Q80544842
Summary
Q80544842 is a star[1].
Key Facts
- Q80544842's instance of is recorded as star[2].
- Q80544842's constellation is recorded as Cygnus[3].
- Q80544842's spectral class is recorded as K2III[4].
- Q80544842's catalog code is recorded as Gaia DR2 2076407441120636672[5].
- Q80544842's catalog code is recorded as KIC 5203208[6].
- Q80544842's catalog code is recorded as 2MASS J19435864+4021030[7].
- Q80544842's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.3141'}[8].
- Q80544842's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.338'}[9].
- Q80544842's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.738'}[10].
- Q80544842's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.589'}[11].
- Q80544842's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3192'}[12].
- Q80544842's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.70'}[13].
- Q80544842's metallicity is recorded as {'unit': '1', 'amount': '-0.06'}[14].
- Q80544842's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3132.83'}[15].
- Q80544842's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.99433640625455'}[16].
- Q80544842's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.35084434395500'}[17].
- Q80544842's epoch is recorded as J2000.0[18].
- Q80544842's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4664'}[19].
- Q80544842's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.955'}[20].
- Q80544842's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.522'}[21].
Body
Definition and Type
Q80544842's instance of is recorded as star[2].