Q89176442
star in the constellation Cygnus
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Q89176442
Summary
Q89176442 is a star[1].
Key Facts
- Q89176442's instance of is recorded as star[2].
- Q89176442's constellation is recorded as Cygnus[3].
- Q89176442's spectral class is recorded as F8V[4].
- Q89176442's catalog code is recorded as Gaia DR2 2132505314632635008[5].
- Q89176442's catalog code is recorded as KIC 11239399[6].
- Q89176442's catalog code is recorded as 2MASS J19173075+4858161[7].
- Q89176442's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9330'}[8].
- Q89176442's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.929'}[9].
- Q89176442's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.681'}[10].
- Q89176442's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.568'}[11].
- Q89176442's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3722'}[12].
- Q89176442's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-13.5'}[13].
- Q89176442's metallicity is recorded as {'unit': '1', 'amount': '-0.10'}[14].
- Q89176442's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.37820133231880'}[15].
- Q89176442's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.97114864682500'}[16].
- Q89176442's epoch is recorded as J2000.0[17].
- Q89176442's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5967'}[18].
- Q89176442's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+13000'}[19].
- Q89176442's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-14.014'}[20].
- Q89176442's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.211'}[21].
Body
Definition and Type
Q89176442's instance of is recorded as star[2].