Q85833703

Summary

Q85833703 is a rotating variable star^[1].

Key Facts

• Q85833703's instance of is recorded as rotating variable star^[2].
• Q85833703's instance of is recorded as star^[3].
• Q85833703's instance of is recorded as near-infrared source^[4].
• Q85833703's instance of is recorded as eruptive variable star^[5].
• Q85833703's constellation is recorded as Lyra^[6].
• Q85833703's spectral class is recorded as K1V^[7].
• Q85833703's child astronomical body is recorded as Q28502862^[8].
• Q85833703's child astronomical body is recorded as Q28502861^[9].
• Q85833703's catalog code is recorded as Gaia DR2 2102046952760377728^[10].
• Q85833703's catalog code is recorded as 2MASS J19220395+4305017^[11].
• Q85833703's catalog code is recorded as KIC 7440748^[12].
• Q85833703's catalog code is recorded as Kepler-161^[13].
• Q85833703's catalog code is recorded as KOI-457^[14].
• Q85833703's catalog code is recorded as UCAC4 666-074979^[15].
• Q85833703's catalog code is recorded as Gaia DR3 2102046952760377728^[16].
• Q85833703's catalog code is recorded as TIC 159444082^[17].
• Q85833703's catalog code is recorded as SPOCS 3697^[18].
• Q85833703's type of variable star is recorded as rotating variable star^[19].
• Q85833703's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.767'}^[20].
• Q85833703's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.329'}^[21].
• Q85833703's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.246'}^[22].
• Q85833703's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.180068'}^[23].
• Q85833703's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.344'}^[24].
• Q85833703's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.4'}^[25].
• Q85833703's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.33968636'}^[26].

Body

Definition and Type

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