Q90078830
star in the constellation Cygnus
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Q90078830
Summary
Q90078830 is a star[1].
Key Facts
- Q90078830's instance of is recorded as star[2].
- Q90078830's constellation is recorded as Cygnus[3].
- Q90078830's spectral class is recorded as G8III[4].
- Q90078830's catalog code is recorded as Gaia DR2 2139366473346908544[5].
- Q90078830's catalog code is recorded as KIC 12985952[6].
- Q90078830's catalog code is recorded as 2MASS J19242473+5229593[7].
- Q90078830's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1219'}[8].
- Q90078830's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.421'}[9].
- Q90078830's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.867'}[10].
- Q90078830's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.727'}[11].
- Q90078830's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2847'}[12].
- Q90078830's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-72.7'}[13].
- Q90078830's metallicity is recorded as {'unit': '1', 'amount': '-0.30'}[14].
- Q90078830's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3512.47'}[15].
- Q90078830's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.10310535150455'}[16].
- Q90078830's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.49980547078139'}[17].
- Q90078830's epoch is recorded as J2000.0[18].
- Q90078830's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4829'}[19].
- Q90078830's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.227'}[20].
- Q90078830's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.512'}[21].
Body
Definition and Type
Q90078830's instance of is recorded as star[2].