Q82222915
star in the constellation Cygnus
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Q82222915
Summary
Q82222915 is a star[1].
Key Facts
- Q82222915's instance of is recorded as star[2].
- Q82222915's constellation is recorded as Cygnus[3].
- Q82222915's spectral class is recorded as K2[4].
- Q82222915's catalog code is recorded as Gaia DR2 2139509341138744192[5].
- Q82222915's catalog code is recorded as KIC 12883143[6].
- Q82222915's catalog code is recorded as 2MASS J19160555+5217438[7].
- Q82222915's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8133'}[8].
- Q82222915's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.418'}[9].
- Q82222915's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.003'}[10].
- Q82222915's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.880'}[11].
- Q82222915's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.8951'}[12].
- Q82222915's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-69.47'}[13].
- Q82222915's metallicity is recorded as {'unit': '1', 'amount': '+0.07'}[14].
- Q82222915's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+345.411'}[15].
- Q82222915's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.02317678261000'}[16].
- Q82222915's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.29549940452639'}[17].
- Q82222915's epoch is recorded as J2000.0[18].
- Q82222915's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5065'}[19].
- Q82222915's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+17.960'}[20].
- Q82222915's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+19.861'}[21].
Body
Definition and Type
Q82222915's instance of is recorded as star[2].