Q82220920
star in the constellation Cygnus
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Q82220920
Summary
Q82220920 is a star[1].
Key Facts
- Q82220920's instance of is recorded as star[2].
- Q82220920's constellation is recorded as Cygnus[3].
- Q82220920's spectral class is recorded as G5[4].
- Q82220920's catalog code is recorded as Gaia DR2 2129976914626541312[5].
- Q82220920's catalog code is recorded as KIC 11660639[6].
- Q82220920's catalog code is recorded as 2MASS J19245264+4942543[7].
- Q82220920's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.6806'}[8].
- Q82220920's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.492'}[9].
- Q82220920's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.103'}[10].
- Q82220920's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.035'}[11].
- Q82220920's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.2108'}[12].
- Q82220920's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-69.72'}[13].
- Q82220920's metallicity is recorded as {'unit': '1', 'amount': '+0.12'}[14].
- Q82220920's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.21952571202120'}[15].
- Q82220920's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.71507075290251'}[16].
- Q82220920's epoch is recorded as J2000.0[17].
- Q82220920's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5594'}[18].
- Q82220920's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+22400'}[19].
- Q82220920's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+7.388'}[20].
- Q82220920's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-14.041'}[21].
Body
Definition and Type
Q82220920's instance of is recorded as star[2].