Q80539442
star in the constellation Cygnus
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Q80539442
Summary
Q80539442 is a star[1].
Key Facts
- Q80539442's instance of is recorded as star[2].
- Q80539442's constellation is recorded as Cygnus[3].
- Q80539442's spectral class is recorded as K1IV[4].
- Q80539442's catalog code is recorded as Gaia DR2 2077036258687496704[5].
- Q80539442's catalog code is recorded as KIC 6299274[6].
- Q80539442's catalog code is recorded as 2MASS J19433267+4138208[7].
- Q80539442's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.4097'}[8].
- Q80539442's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.313'}[9].
- Q80539442's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.574'}[10].
- Q80539442's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.415'}[11].
- Q80539442's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1880'}[12].
- Q80539442's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.82'}[13].
- Q80539442's metallicity is recorded as {'unit': '1', 'amount': '-0.15'}[14].
- Q80539442's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+5319.15'}[15].
- Q80539442's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.88615885307580'}[16].
- Q80539442's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+41.63917427296139'}[17].
- Q80539442's epoch is recorded as J2000.0[18].
- Q80539442's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4464'}[19].
- Q80539442's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.675'}[20].
- Q80539442's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.411'}[21].
Body
Definition and Type
Q80539442's instance of is recorded as star[2].