Q82222467
star in the constellation Cygnus
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Q82222467
Summary
Q82222467 is a star[1].
Key Facts
- Q82222467's instance of is recorded as star[2].
- Q82222467's constellation is recorded as Cygnus[3].
- Q82222467's spectral class is recorded as G9III[4].
- Q82222467's catalog code is recorded as Gaia DR2 2126403128178998016[5].
- Q82222467's catalog code is recorded as KIC 8304476[6].
- Q82222467's catalog code is recorded as 2MASS J19341909+4415536[7].
- Q82222467's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.2594'}[8].
- Q82222467's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.484'}[9].
- Q82222467's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.883'}[10].
- Q82222467's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.763'}[11].
- Q82222467's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2743'}[12].
- Q82222467's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-45.5'}[13].
- Q82222467's metallicity is recorded as {'unit': '1', 'amount': '-0.05'}[14].
- Q82222467's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3645.64'}[15].
- Q82222467's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.57955126550330'}[16].
- Q82222467's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.26488683948722'}[17].
- Q82222467's epoch is recorded as J2000.0[18].
- Q82222467's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4419'}[19].
- Q82222467's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-9.046'}[20].
- Q82222467's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.251'}[21].
Body
Definition and Type
Q82222467's instance of is recorded as star[2].