Q80541205
star in the constellation Cygnus
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Q80541205
Summary
Q80541205 is a star[1].
Key Facts
- Q80541205's instance of is recorded as star[2].
- Q80541205's constellation is recorded as Cygnus[3].
- Q80541205's spectral class is recorded as G9III[4].
- Q80541205's catalog code is recorded as Gaia DR2 2053512924661293056[5].
- Q80541205's catalog code is recorded as KIC 5451477[6].
- Q80541205's catalog code is recorded as 2MASS J19305702+4036080[7].
- Q80541205's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3686'}[8].
- Q80541205's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.657'}[9].
- Q80541205's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.086'}[10].
- Q80541205's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.988'}[11].
- Q80541205's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4240'}[12].
- Q80541205's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-31.91'}[13].
- Q80541205's metallicity is recorded as {'unit': '1', 'amount': '-0.06'}[14].
- Q80541205's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2358.49'}[15].
- Q80541205's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.73761977984540'}[16].
- Q80541205's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.60223722838861'}[17].
- Q80541205's epoch is recorded as J2000.0[18].
- Q80541205's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4809'}[19].
- Q80541205's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.552'}[20].
- Q80541205's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.236'}[21].
Body
Definition and Type
Q80541205's instance of is recorded as star[2].