Q80536518
star in the constellation Cygnus
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Q80536518
Summary
Q80536518 is a star[1].
Key Facts
- Q80536518's instance of is recorded as star[2].
- Q80536518's constellation is recorded as Cygnus[3].
- Q80536518's spectral class is recorded as K3III[4].
- Q80536518's catalog code is recorded as Gaia DR2 2053295947217613440[5].
- Q80536518's catalog code is recorded as KIC 4927163[6].
- Q80536518's catalog code is recorded as 2MASS J19310029+4004512[7].
- Q80536518's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1043'}[8].
- Q80536518's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.367'}[9].
- Q80536518's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.806'}[10].
- Q80536518's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.678'}[11].
- Q80536518's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2103'}[12].
- Q80536518's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-43.7'}[13].
- Q80536518's metallicity is recorded as {'unit': '1', 'amount': '+0.00'}[14].
- Q80536518's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4755.11'}[15].
- Q80536518's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.75122226558085'}[16].
- Q80536518's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.08089392701000'}[17].
- Q80536518's epoch is recorded as J2000.0[18].
- Q80536518's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4713'}[19].
- Q80536518's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-7.902'}[20].
- Q80536518's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.875'}[21].
Body
Definition and Type
Q80536518's instance of is recorded as star[2].