Q85257109
eclipsing binary star in the constellation Cygnus
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Q85257109
Summary
Q85257109 is an eclipsing binary star[1].
Key Facts
- Q85257109's instance of is recorded as eclipsing binary star[2].
- Q85257109's instance of is recorded as star[3].
- Q85257109's instance of is recorded as near-infrared source[4].
- Q85257109's instance of is recorded as rotating variable star[5].
- Q85257109's constellation is recorded as Cygnus[6].
- Q85257109's spectral class is recorded as F6IV[7].
- Q85257109's child astronomical body is recorded as Q76087115[8].
- Q85257109's child astronomical body is recorded as Q76071397[9].
- Q85257109's catalog code is recorded as Gaia DR2 2085204015173031552[10].
- Q85257109's catalog code is recorded as KIC 9117416[11].
- Q85257109's catalog code is recorded as 2MASS J20011589+4529434[12].
- Q85257109's catalog code is recorded as Kepler-1921[13].
- Q85257109's catalog code is recorded as Gaia DR3 2085204015173031552[14].
- Q85257109's catalog code is recorded as TIC 239287963[15].
- Q85257109's catalog code is recorded as SPOCS 3911[16].
- Q85257109's catalog code is recorded as KOI-3425[17].
- Q85257109's type of variable star is recorded as rotating variable star[18].
- Q85257109's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.897'}[19].
- Q85257109's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.610'}[20].
- Q85257109's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.514'}[21].
- Q85257109's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.973302'}[22].
- Q85257109's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.1'}[23].
- Q85257109's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+4.350041'}[24].
- Q85257109's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.17'}[25].
- Q85257109's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+2.22'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], star[3], near-infrared source[4], and rotating variable star[5].