Q83203784

Summary

Q83203784 is a rotating variable star^[1].

Key Facts

• Q83203784's instance of is recorded as rotating variable star^[2].
• Q83203784's instance of is recorded as star^[3].
• Q83203784's instance of is recorded as near-infrared source^[4].
• Q83203784's constellation is recorded as Lyra^[5].
• Q83203784's child astronomical body is recorded as Q28855986^[6].
• Q83203784's child astronomical body is recorded as Q28855987^[7].
• Q83203784's child astronomical body is recorded as Q28855985^[8].
• Q83203784's child astronomical body is recorded as KOI-1108 e^[9].
• Q83203784's catalog code is recorded as Gaia DR2 2099980386293545216^[10].
• Q83203784's catalog code is recorded as KIC 3218908^[11].
• Q83203784's catalog code is recorded as 2MASS J19055770+3822296^[12].
• Q83203784's catalog code is recorded as KOI-1108^[13].
• Q83203784's catalog code is recorded as Kepler-770^[14].
• Q83203784's catalog code is recorded as Gaia DR3 2099980386293545216^[15].
• Q83203784's catalog code is recorded as TIC 120891972^[16].
• Q83203784's type of variable star is recorded as rotating variable star^[17].
• Q83203784's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.391'}^[18].
• Q83203784's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.010'}^[19].
• Q83203784's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.923'}^[20].
• Q83203784's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.9'}^[21].
• Q83203784's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.584625'}^[22].
• Q83203784's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.0280354'}^[23].
• Q83203784's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.94'}^[24].
• Q83203784's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.1863834'}^[25].
• Q83203784's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0594'}^[26].

Body

Definition and Type

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