Q80536231
star in the constellation Cygnus
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Q80536231
Summary
Q80536231 is a star[1].
Key Facts
- Q80536231's instance of is recorded as star[2].
- Q80536231's constellation is recorded as Cygnus[3].
- Q80536231's spectral class is recorded as G9IIIb[4].
- Q80536231's catalog code is recorded as Gaia DR2 2076549175038635392[5].
- Q80536231's catalog code is recorded as KIC 5285328[6].
- Q80536231's catalog code is recorded as 2MASS J19384819+4024581[7].
- Q80536231's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.0468'}[8].
- Q80536231's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.155'}[9].
- Q80536231's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.614'}[10].
- Q80536231's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.436'}[11].
- Q80536231's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2229'}[12].
- Q80536231's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.3'}[13].
- Q80536231's metallicity is recorded as {'unit': '1', 'amount': '-0.33'}[14].
- Q80536231's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4486.32'}[15].
- Q80536231's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+294.70082942554580'}[16].
- Q80536231's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.41614605610889'}[17].
- Q80536231's epoch is recorded as J2000.0[18].
- Q80536231's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4782'}[19].
- Q80536231's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.643'}[20].
- Q80536231's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.611'}[21].
Body
Definition and Type
Q80536231's instance of is recorded as star[2].