Q80547224
star in the constellation Cygnus
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Q80547224
Summary
Q80547224 is a star[1].
Key Facts
- Q80547224's instance of is recorded as star[2].
- Q80547224's constellation is recorded as Cygnus[3].
- Q80547224's spectral class is recorded as K3III[4].
- Q80547224's catalog code is recorded as Gaia DR2 2052446059090944896[5].
- Q80547224's catalog code is recorded as KIC 4065015[6].
- Q80547224's catalog code is recorded as 2MASS J19341756+3909393[7].
- Q80547224's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7766'}[8].
- Q80547224's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.064'}[9].
- Q80547224's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.525'}[10].
- Q80547224's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.402'}[11].
- Q80547224's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4088'}[12].
- Q80547224's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.92'}[13].
- Q80547224's metallicity is recorded as {'unit': '1', 'amount': '-0.01'}[14].
- Q80547224's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2446.18'}[15].
- Q80547224's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.57319442867960'}[16].
- Q80547224's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.16091202867028'}[17].
- Q80547224's epoch is recorded as J2000.0[18].
- Q80547224's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4699'}[19].
- Q80547224's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.483'}[20].
- Q80547224's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.748'}[21].
Body
Definition and Type
Q80547224's instance of is recorded as star[2].