Q94488214

Summary

Q94488214 is an eclipsing binary star^[1].

Key Facts

• Q94488214's instance of is recorded as eclipsing binary star^[2].
• Q94488214's instance of is recorded as star^[3].
• Q94488214's instance of is recorded as near-infrared source^[4].
• Q94488214's instance of is recorded as eruptive variable star^[5].
• Q94488214's constellation is recorded as Cygnus^[6].
• Q94488214's child astronomical body is recorded as Q28856721^[7].
• Q94488214's child astronomical body is recorded as Q85930709^[8].
• Q94488214's catalog code is recorded as Gaia DR2 2076598687419100800^[9].
• Q94488214's catalog code is recorded as KIC 5546761^[10].
• Q94488214's catalog code is recorded as 2MASS J19415549+4043551^[11].
• Q94488214's catalog code is recorded as KOI-2160^[12].
• Q94488214's catalog code is recorded as UCAC4 654-076235^[13].
• Q94488214's catalog code is recorded as Gaia DR3 2076598687419100800^[14].
• Q94488214's catalog code is recorded as TIC 184009076^[15].
• Q94488214's catalog code is recorded as Kepler-1125^[16].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.694'}^[17].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.31'}^[18].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.24'}^[19].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.879403'}^[20].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.674'}^[21].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.929'}^[22].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.311'}^[23].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.061'}^[24].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.785'}^[25].
• Q94488214's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.971'}^[26].

Body

Definition and Type

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