Q86844316

Summary

Q86844316 is an eclipsing binary star^[1].

Key Facts

• Q86844316's instance of is recorded as eclipsing binary star^[2].
• Q86844316's instance of is recorded as star^[3].
• Q86844316's instance of is recorded as near-infrared source^[4].
• Q86844316's instance of is recorded as rotating variable star^[5].
• Q86844316's constellation is recorded as Cygnus^[6].
• Q86844316's spectral class is recorded as G2V^[7].
• Q86844316's child astronomical body is recorded as Q85078428^[8].
• Q86844316's catalog code is recorded as SPOCS 3076^[9].
• Q86844316's catalog code is recorded as Gaia DR2 2129671220332872192^[10].
• Q86844316's catalog code is recorded as KOI-760^[11].
• Q86844316's catalog code is recorded as KIC 11138155^[12].
• Q86844316's catalog code is recorded as 2MASS J19284009+4843393^[13].
• Q86844316's catalog code is recorded as Kepler-1976^[14].
• Q86844316's catalog code is recorded as Gaia DR3 2129671220332872192^[15].
• Q86844316's catalog code is recorded as TIC 26584326^[16].
• Q86844316's type of variable star is recorded as rotating variable star^[17].
• Q86844316's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.12'}^[18].
• Q86844316's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.80'}^[19].
• Q86844316's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.815'}^[20].
• Q86844316's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.245373'}^[21].
• Q86844316's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.44'}^[22].
• Q86844316's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.15'}^[23].
• Q86844316's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.1206473'}^[24].
• Q86844316's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.02'}^[25].
• Q86844316's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.09'}^[26].

Body

Definition and Type

Recorded instance of include eclipsing binary star^[2], star^[3], near-infrared source^[4], and rotating variable star^[5].