Q78608956

Summary

Q78608956 is a rotating variable star^[1].

Key Facts

• Q78608956's instance of is recorded as rotating variable star^[2].
• Q78608956's instance of is recorded as star^[3].
• Q78608956's instance of is recorded as near-infrared source^[4].
• Q78608956's constellation is recorded as Lyra^[5].
• Q78608956's spectral class is recorded as K5V^[6].
• Q78608956's child astronomical body is recorded as Q28857053^[7].
• Q78608956's catalog code is recorded as Gaia DR2 2117344732912435968^[8].
• Q78608956's catalog code is recorded as KIC 8210018^[9].
• Q78608956's catalog code is recorded as KOI-2762^[10].
• Q78608956's catalog code is recorded as 2MASS J18420282+4409336^[11].
• Q78608956's catalog code is recorded as Kepler-1341^[12].
• Q78608956's catalog code is recorded as Kepler-1341A^[13].
• Q78608956's catalog code is recorded as Gaia DR3 2117344732912435968^[14].
• Q78608956's catalog code is recorded as TIC 123126460^[15].
• Q78608956's catalog code is recorded as KOI-2762A^[16].
• Q78608956's type of variable star is recorded as rotating variable star^[17].
• Q78608956's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.285'}^[18].
• Q78608956's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.782'}^[19].
• Q78608956's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.636'}^[20].
• Q78608956's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.00422'}^[21].
• Q78608956's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.35'}^[22].
• Q78608956's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.20231038'}^[23].
• Q78608956's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.71'}^[24].
• Q78608956's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.785'}^[25].
• Q78608956's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0788'}^[26].

Body

Definition and Type

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