Q87501329
star in the constellation Cygnus
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Q87501329
Summary
Q87501329 is a star[1].
Key Facts
- Q87501329's instance of is recorded as star[2].
- Q87501329's constellation is recorded as Cygnus[3].
- Q87501329's spectral class is recorded as K3V[4].
- Q87501329's catalog code is recorded as Gaia DR2 2139357127497949312[5].
- Q87501329's catalog code is recorded as KIC 12886463[6].
- Q87501329's catalog code is recorded as 2MASS J19233716+5217520[7].
- Q87501329's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.1420'}[8].
- Q87501329's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.531'}[9].
- Q87501329's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.023'}[10].
- Q87501329's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.918'}[11].
- Q87501329's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.7163'}[12].
- Q87501329's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-65.04'}[13].
- Q87501329's metallicity is recorded as {'unit': '1', 'amount': '-0.08'}[14].
- Q87501329's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+212.031'}[15].
- Q87501329's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+290.90491043014583'}[16].
- Q87501329's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.29779210969917'}[17].
- Q87501329's epoch is recorded as J2000.0[18].
- Q87501329's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4871'}[19].
- Q87501329's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+47.594'}[20].
- Q87501329's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.857'}[21].
Body
Definition and Type
Q87501329's instance of is recorded as star[2].