Q80538024
star in the constellation Cygnus
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Q80538024
Summary
Q80538024 is a star[1].
Key Facts
- Q80538024's instance of is recorded as star[2].
- Q80538024's constellation is recorded as Cygnus[3].
- Q80538024's spectral class is recorded as K3III[4].
- Q80538024's catalog code is recorded as Gaia DR2 2076227567889008768[5].
- Q80538024's catalog code is recorded as KIC 4669559[6].
- Q80538024's catalog code is recorded as 2MASS J19421598+3943494[7].
- Q80538024's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7613'}[8].
- Q80538024's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.749'}[9].
- Q80538024's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.094'}[10].
- Q80538024's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.930'}[11].
- Q80538024's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2492'}[12].
- Q80538024's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-68.6'}[13].
- Q80538024's metallicity is recorded as {'unit': '1', 'amount': '+0.08'}[14].
- Q80538024's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4012.84'}[15].
- Q80538024's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.56661804623080'}[16].
- Q80538024's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.73038572053639'}[17].
- Q80538024's epoch is recorded as J2000.0[18].
- Q80538024's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4406'}[19].
- Q80538024's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.167'}[20].
- Q80538024's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.999'}[21].
Body
Definition and Type
Q80538024's instance of is recorded as star[2].