Q85833831

Summary

Q85833831 is an eclipsing binary star^[1].

Key Facts

• Q85833831's instance of is recorded as eclipsing binary star^[2].
• Q85833831's instance of is recorded as star^[3].
• Q85833831's instance of is recorded as near-infrared source^[4].
• Q85833831's instance of is recorded as rotating variable star^[5].
• Q85833831's constellation is recorded as Lyra^[6].
• Q85833831's spectral class is recorded as K1^[7].
• Q85833831's child astronomical body is recorded as Q28855590^[8].
• Q85833831's catalog code is recorded as Gaia DR2 2102468134431912064^[9].
• Q85833831's catalog code is recorded as KOI-201^[10].
• Q85833831's catalog code is recorded as KIC 6849046^[11].
• Q85833831's catalog code is recorded as 2MASS J19083133+4221005^[12].
• Q85833831's catalog code is recorded as Kepler-491^[13].
• Q85833831's catalog code is recorded as Gaia DR3 2102468134431912064^[14].
• Q85833831's catalog code is recorded as TIC 158388163^[15].
• Q85833831's catalog code is recorded as SPOCS 3639^[16].
• Q85833831's type of variable star is recorded as eclipsing binary star^[17].
• Q85833831's type of variable star is recorded as rotating variable star^[18].
• Q85833831's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.746'}^[19].
• Q85833831's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.426'}^[20].
• Q85833831's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.354'}^[21].
• Q85833831's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.949793'}^[22].
• Q85833831's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.8251914'}^[23].
• Q85833831's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.04'}^[24].
• Q85833831's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.0317457'}^[25].
• Q85833831's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5621'}^[26].

Body

Definition and Type

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