Q88477922
star in the constellation Cygnus
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Q88477922
Summary
Q88477922 is a star[1].
Key Facts
- Q88477922's instance of is recorded as star[2].
- Q88477922's constellation is recorded as Cygnus[3].
- Q88477922's spectral class is recorded as G6IV[4].
- Q88477922's catalog code is recorded as Gaia DR2 2126756380648993152[5].
- Q88477922's catalog code is recorded as KIC 9154866[6].
- Q88477922's catalog code is recorded as 2MASS J19273722+4532052[7].
- Q88477922's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7258'}[8].
- Q88477922's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.219'}[9].
- Q88477922's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.744'}[10].
- Q88477922's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.666'}[11].
- Q88477922's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4271'}[12].
- Q88477922's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-0.6'}[13].
- Q88477922's metallicity is recorded as {'unit': '1', 'amount': '-0.28'}[14].
- Q88477922's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2341.37'}[15].
- Q88477922's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.90507956194330'}[16].
- Q88477922's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.53480027001584'}[17].
- Q88477922's epoch is recorded as J2000.0[18].
- Q88477922's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4977'}[19].
- Q88477922's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.889'}[20].
- Q88477922's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.045'}[21].
Body
Definition and Type
Q88477922's instance of is recorded as star[2].