Q76747566
star in the constellation Cygnus
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Q76747566
Summary
Q76747566 is a star[1].
Key Facts
- Q76747566's instance of is recorded as star[2].
- Q76747566's constellation is recorded as Cygnus[3].
- Q76747566's spectral class is recorded as K1IV[4].
- Q76747566's catalog code is recorded as Gaia DR2 2079112411520409344[5].
- Q76747566's catalog code is recorded as KIC 8709951[6].
- Q76747566's catalog code is recorded as 2MASS J19535236+4451413[7].
- Q76747566's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.5387'}[8].
- Q76747566's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.443'}[9].
- Q76747566's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.712'}[10].
- Q76747566's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.573'}[11].
- Q76747566's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2765'}[12].
- Q76747566's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.96'}[13].
- Q76747566's metallicity is recorded as {'unit': '1', 'amount': '-0.32'}[14].
- Q76747566's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3616.64'}[15].
- Q76747566's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+298.46818177119290'}[16].
- Q76747566's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.86147961513722'}[17].
- Q76747566's epoch is recorded as J2000.0[18].
- Q76747566's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4814'}[19].
- Q76747566's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.216'}[20].
- Q76747566's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.198'}[21].
Body
Definition and Type
Q76747566's instance of is recorded as star[2].