Q89860771

Summary

Q89860771 is a rotating variable star^[1].

Key Facts

• Q89860771's instance of is recorded as rotating variable star^[2].
• Q89860771's instance of is recorded as star^[3].
• Q89860771's instance of is recorded as near-infrared source^[4].
• Q89860771's instance of is recorded as eruptive variable star^[5].
• Q89860771's constellation is recorded as Cygnus^[6].
• Q89860771's spectral class is recorded as G3^[7].
• Q89860771's child astronomical body is recorded as Q28855398^[8].
• Q89860771's child astronomical body is recorded as Q28855400^[9].
• Q89860771's catalog code is recorded as Gaia DR2 2134773160443224192^[10].
• Q89860771's catalog code is recorded as KIC 11358389^[11].
• Q89860771's catalog code is recorded as 2MASS J19423038+4907495^[12].
• Q89860771's catalog code is recorded as KOI-2163^[13].
• Q89860771's catalog code is recorded as UCAC4 696-069337^[14].
• Q89860771's catalog code is recorded as Gaia DR3 2134773160447382656^[15].
• Q89860771's catalog code is recorded as TIC 27530849^[16].
• Q89860771's catalog code is recorded as Kepler-365^[17].
• Q89860771's type of variable star is recorded as rotating variable star^[18].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.484'}^[19].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.155'}^[20].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.145'}^[21].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.27727'}^[22].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.477'}^[23].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.637'}^[24].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.069'}^[25].
• Q89860771's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.758'}^[26].

Body

Definition and Type

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