Q88332257

Summary

Q88332257 is a rotating variable star^[1].

Key Facts

• Q88332257's instance of is recorded as rotating variable star^[2].
• Q88332257's instance of is recorded as star^[3].
• Q88332257's instance of is recorded as near-infrared source^[4].
• Q88332257's instance of is recorded as eruptive variable star^[5].
• Q88332257's constellation is recorded as Lyra^[6].
• Q88332257's spectral class is recorded as M1V^[7].
• Q88332257's child astronomical body is recorded as Q28856545^[8].
• Q88332257's child astronomical body is recorded as Q15221253^[9].
• Q88332257's catalog code is recorded as Gaia DR2 2103377980301947264^[10].
• Q88332257's catalog code is recorded as KIC 5080636^[11].
• Q88332257's catalog code is recorded as 2MASS J19000314+4013147^[12].
• Q88332257's catalog code is recorded as KOI-1843^[13].
• Q88332257's catalog code is recorded as UCAC4 652-066547^[14].
• Q88332257's catalog code is recorded as Gaia DR3 2103377980301947264^[15].
• Q88332257's catalog code is recorded as TIC 120418600^[16].
• Q88332257's catalog code is recorded as Kepler-974^[17].
• Q88332257's type of variable star is recorded as rotating variable star^[18].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.951'}^[19].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.279'}^[20].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.056'}^[21].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.395094'}^[22].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.819'}^[23].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.776'}^[24].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.172'}^[25].
• Q88332257's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.295'}^[26].

Body

Definition and Type

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