Q86844030

Summary

Q86844030 is a rotating variable star^[1].

Key Facts

• Q86844030's instance of is recorded as rotating variable star^[2].
• Q86844030's instance of is recorded as star^[3].
• Q86844030's instance of is recorded as near-infrared source^[4].
• Q86844030's instance of is recorded as eruptive variable star^[5].
• Q86844030's constellation is recorded as Cygnus^[6].
• Q86844030's child astronomical body is recorded as Q28503854^[7].
• Q86844030's child astronomical body is recorded as Kepler-256 d^[8].
• Q86844030's child astronomical body is recorded as Q28503853^[9].
• Q86844030's child astronomical body is recorded as Q28503856^[10].
• Q86844030's catalog code is recorded as Gaia DR2 2128250926189039488^[11].
• Q86844030's catalog code is recorded as 2MASS J19301930+4605506^[12].
• Q86844030's catalog code is recorded as KIC 9466668^[13].
• Q86844030's catalog code is recorded as Kepler-256^[14].
• Q86844030's catalog code is recorded as KOI-939^[15].
• Q86844030's catalog code is recorded as UCAC4 681-070148^[16].
• Q86844030's catalog code is recorded as Gaia DR3 2128250926189039488^[17].
• Q86844030's catalog code is recorded as TIC 63362772^[18].
• Q86844030's catalog code is recorded as SPOCS 3949^[19].
• Q86844030's type of variable star is recorded as rotating variable star^[20].
• Q86844030's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.824'}^[21].
• Q86844030's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.496'}^[22].
• Q86844030's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.42'}^[23].
• Q86844030's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.002748'}^[24].
• Q86844030's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.946'}^[25].
• Q86844030's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.84785527'}^[26].

Body

Definition and Type

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