Q80539917
star in the constellation Cygnus
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Q80539917
Summary
Q80539917 is a star[1].
Key Facts
- Q80539917's instance of is recorded as star[2].
- Q80539917's constellation is recorded as Cygnus[3].
- Q80539917's spectral class is recorded as K1IV[4].
- Q80539917's catalog code is recorded as Gaia DR2 2078037737675467392[5].
- Q80539917's catalog code is recorded as KIC 7695179[6].
- Q80539917's catalog code is recorded as 2MASS J19432101+4322036[7].
- Q80539917's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.3943'}[8].
- Q80539917's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.382'}[9].
- Q80539917's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.722'}[10].
- Q80539917's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.571'}[11].
- Q80539917's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1982'}[12].
- Q80539917's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.52'}[13].
- Q80539917's metallicity is recorded as {'unit': '1', 'amount': '-0.40'}[14].
- Q80539917's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+5045.41'}[15].
- Q80539917's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.83753597725580'}[16].
- Q80539917's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.36767296128750'}[17].
- Q80539917's epoch is recorded as J2000.0[18].
- Q80539917's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4747'}[19].
- Q80539917's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.735'}[20].
- Q80539917's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.759'}[21].
Body
Definition and Type
Q80539917's instance of is recorded as star[2].