Q87706626

Summary

Q87706626 is a rotating variable star^[1].

Key Facts

• Q87706626's instance of is recorded as rotating variable star^[2].
• Q87706626's instance of is recorded as star^[3].
• Q87706626's instance of is recorded as near-infrared source^[4].
• Q87706626's constellation is recorded as Lyra^[5].
• Q87706626's spectral class is recorded as G6V^[6].
• Q87706626's child astronomical body is recorded as Q92357176^[7].
• Q87706626's child astronomical body is recorded as Q85078492^[8].
• Q87706626's catalog code is recorded as Gaia DR2 2106371744306291328^[9].
• Q87706626's catalog code is recorded as KIC 8804283^[10].
• Q87706626's catalog code is recorded as 2MASS J19000866+4504158^[11].
• Q87706626's catalog code is recorded as KOI-1276^[12].
• Q87706626's catalog code is recorded as Kepler-1991^[13].
• Q87706626's catalog code is recorded as Gaia DR3 2106371744306291328^[14].
• Q87706626's catalog code is recorded as TIC 164831457^[15].
• Q87706626's catalog code is recorded as SPOCS 3863^[16].
• Q87706626's type of variable star is recorded as rotating variable star^[17].
• Q87706626's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.539'}^[18].
• Q87706626's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.194'}^[19].
• Q87706626's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.07'}^[20].
• Q87706626's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.708344'}^[21].
• Q87706626's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.048'}^[22].
• Q87706626's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.94'}^[23].
• Q87706626's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.7647252'}^[24].
• Q87706626's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.96'}^[25].
• Q87706626's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.98'}^[26].

Body

Definition and Type

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