Q87726857
star in the constellation Cygnus
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Q87726857
Summary
Q87726857 is a star[1].
Key Facts
- Q87726857's instance of is recorded as star[2].
- Q87726857's constellation is recorded as Cygnus[3].
- Q87726857's spectral class is recorded as G1.5IV-V[4].
- Q87726857's catalog code is recorded as Gaia DR2 2135975231590828544[5].
- Q87726857's catalog code is recorded as KIC 12114957[6].
- Q87726857's catalog code is recorded as 2MASS J19352015+5037472[7].
- Q87726857's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7833'}[8].
- Q87726857's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.537'}[9].
- Q87726857's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.158'}[10].
- Q87726857's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.095'}[11].
- Q87726857's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7201'}[12].
- Q87726857's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-58.7'}[13].
- Q87726857's metallicity is recorded as {'unit': '1', 'amount': '-0.23'}[14].
- Q87726857's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.83395722576500'}[15].
- Q87726857's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.62978139124972'}[16].
- Q87726857's epoch is recorded as J2000.0[17].
- Q87726857's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5432'}[18].
- Q87726857's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+9100'}[19].
- Q87726857's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-10.857'}[20].
- Q87726857's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.076'}[21].
Body
Definition and Type
Q87726857's instance of is recorded as star[2].