Q85577077
star in the constellation Cygnus
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Q85577077
Summary
Q85577077 is a star[1].
Key Facts
- Q85577077's instance of is recorded as star[2].
- Q85577077's constellation is recorded as Cygnus[3].
- Q85577077's spectral class is recorded as K3II-III[4].
- Q85577077's catalog code is recorded as Gaia DR2 2080124232792841088[5].
- Q85577077's catalog code is recorded as KIC 9103185[6].
- Q85577077's catalog code is recorded as 2MASS J19460789+4528199[7].
- Q85577077's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.2834'}[8].
- Q85577077's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.247'}[9].
- Q85577077's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.576'}[10].
- Q85577077's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.419'}[11].
- Q85577077's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2467'}[12].
- Q85577077's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-43.50'}[13].
- Q85577077's metallicity is recorded as {'unit': '1', 'amount': '-0.02'}[14].
- Q85577077's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+296.53290861020460'}[15].
- Q85577077's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.47220191645945'}[16].
- Q85577077's epoch is recorded as J2000.0[17].
- Q85577077's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4359'}[18].
- Q85577077's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+150'}[19].
- Q85577077's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.341'}[20].
- Q85577077's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.959'}[21].
Body
Definition and Type
Q85577077's instance of is recorded as star[2].