Q88478416
star in the constellation Cygnus
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Q88478416
Summary
Q88478416 is a star[1].
Key Facts
- Q88478416's instance of is recorded as star[2].
- Q88478416's constellation is recorded as Cygnus[3].
- Q88478416's spectral class is recorded as G5III-IVp[4].
- Q88478416's catalog code is recorded as Gaia DR2 2126538780427219328[5].
- Q88478416's catalog code is recorded as KIC 9221215[6].
- Q88478416's catalog code is recorded as 2MASS J19320745+4536520[7].
- Q88478416's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.5207'}[8].
- Q88478416's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.007'}[9].
- Q88478416's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.500'}[10].
- Q88478416's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.427'}[11].
- Q88478416's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1084'}[12].
- Q88478416's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-128.3'}[13].
- Q88478416's metallicity is recorded as {'unit': '1', 'amount': '-0.64'}[14].
- Q88478416's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.03108736215586'}[15].
- Q88478416's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.61445434119500'}[16].
- Q88478416's epoch is recorded as J2000.0[17].
- Q88478416's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4986'}[18].
- Q88478416's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+360'}[19].
- Q88478416's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.209'}[20].
- Q88478416's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.462'}[21].
Body
Definition and Type
Q88478416's instance of is recorded as star[2].