Q90113532
star in the constellation Cygnus
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Q90113532
Summary
Q90113532 is a star[1].
Key Facts
- Q90113532's instance of is recorded as star[2].
- Q90113532's instance of is recorded as rotating variable star[3].
- Q90113532's instance of is recorded as near-infrared source[4].
- Q90113532's constellation is recorded as Cygnus[5].
- Q90113532's spectral class is recorded as F5[6].
- Q90113532's child astronomical body is recorded as Q28856590[7].
- Q90113532's catalog code is recorded as Gaia DR2 2125896459478159360[8].
- Q90113532's catalog code is recorded as 2MASS J19310175+4325368[9].
- Q90113532's catalog code is recorded as KIC 7755636[10].
- Q90113532's catalog code is recorded as KOI-1921[11].
- Q90113532's catalog code is recorded as Kepler-1015[12].
- Q90113532's catalog code is recorded as Gaia DR3 2125896459478159360[13].
- Q90113532's catalog code is recorded as TIC 63373862[14].
- Q90113532's catalog code is recorded as SPOCS 3723[15].
- Q90113532's type of variable star is recorded as rotating variable star[16].
- Q90113532's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.887'}[17].
- Q90113532's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.713'}[18].
- Q90113532's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.684'}[19].
- Q90113532's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.749828'}[20].
- Q90113532's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+3.276706'}[21].
- Q90113532's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.49'}[22].
- Q90113532's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.3886747'}[23].
- Q90113532's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2787'}[24].
- Q90113532's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.0766'}[25].
- Q90113532's metallicity is recorded as {'unit': '1', 'amount': '-0.028'}[26].