Q80537761
star in the constellation Cygnus
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Q80537761
Summary
Q80537761 is a star[1].
Key Facts
- Q80537761's instance of is recorded as star[2].
- Q80537761's constellation is recorded as Cygnus[3].
- Q80537761's spectral class is recorded as K2.5III[4].
- Q80537761's catalog code is recorded as Gaia DR2 2053204653393345920[5].
- Q80537761's catalog code is recorded as KIC 4748817[6].
- Q80537761's catalog code is recorded as 2MASS J19294254+3949283[7].
- Q80537761's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9829'}[8].
- Q80537761's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.991'}[9].
- Q80537761's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.386'}[10].
- Q80537761's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.239'}[11].
- Q80537761's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2347'}[12].
- Q80537761's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.3'}[13].
- Q80537761's metallicity is recorded as {'unit': '1', 'amount': '-0.05'}[14].
- Q80537761's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4260.76'}[15].
- Q80537761's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.42728698038127'}[16].
- Q80537761's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.82453638223944'}[17].
- Q80537761's epoch is recorded as J2000.0[18].
- Q80537761's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4491'}[19].
- Q80537761's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.089'}[20].
- Q80537761's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.114'}[21].
Body
Definition and Type
Q80537761's instance of is recorded as star[2].