Q86843919

Summary

Q86843919 is a rotating variable star^[1].

Key Facts

• Q86843919's instance of is recorded as rotating variable star^[2].
• Q86843919's instance of is recorded as star^[3].
• Q86843919's instance of is recorded as near-infrared source^[4].
• Q86843919's instance of is recorded as eruptive variable star^[5].
• Q86843919's constellation is recorded as Cygnus^[6].
• Q86843919's spectral class is recorded as G7^[7].
• Q86843919's child astronomical body is recorded as Q28855512^[8].
• Q86843919's child astronomical body is recorded as Kepler-418 c^[9].
• Q86843919's catalog code is recorded as Gaia DR2 2052117923590073600^[10].
• Q86843919's catalog code is recorded as KIC 3247268^[11].
• Q86843919's catalog code is recorded as 2MASS J19374404+3821196^[12].
• Q86843919's catalog code is recorded as KOI-1089^[13].
• Q86843919's catalog code is recorded as Kepler-418^[14].
• Q86843919's catalog code is recorded as UCAC4 642-071962^[15].
• Q86843919's catalog code is recorded as Gaia DR3 2052117923590073600^[16].
• Q86843919's catalog code is recorded as TIC 377871791^[17].
• Q86843919's catalog code is recorded as SPOCS 3320^[18].
• Q86843919's type of variable star is recorded as rotating variable star^[19].
• Q86843919's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.493'}^[20].
• Q86843919's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.24'}^[21].
• Q86843919's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.10'}^[22].
• Q86843919's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.0'}^[23].
• Q86843919's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.636443'}^[24].
• Q86843919's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.689'}^[25].
• Q86843919's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.1229355'}^[26].

Body

Definition and Type

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