Q85833824

Summary

Q85833824 is a rotating variable star^[1].

Key Facts

• Q85833824's instance of is recorded as rotating variable star^[2].
• Q85833824's instance of is recorded as star^[3].
• Q85833824's instance of is recorded as near-infrared source^[4].
• Q85833824's constellation is recorded as Cygnus^[5].
• Q85833824's spectral class is recorded as G5^[6].
• Q85833824's child astronomical body is recorded as Q28855670^[7].
• Q85833824's catalog code is recorded as Gaia DR2 2087191485516004224^[8].
• Q85833824's catalog code is recorded as KOI-356^[9].
• Q85833824's catalog code is recorded as KIC 11624249^[10].
• Q85833824's catalog code is recorded as 2MASS J19505673+4938137^[11].
• Q85833824's catalog code is recorded as Kepler-536^[12].
• Q85833824's catalog code is recorded as Gaia DR3 2087191485516004224^[13].
• Q85833824's catalog code is recorded as TIC 28234096^[14].
• Q85833824's catalog code is recorded as SPOCS 4244^[15].
• Q85833824's catalog code is recorded as Kepler-536A^[16].
• Q85833824's type of variable star is recorded as rotating variable star^[17].
• Q85833824's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.379'}^[18].
• Q85833824's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.988'}^[19].
• Q85833824's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.892'}^[20].
• Q85833824's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.801281'}^[21].
• Q85833824's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.03'}^[22].
• Q85833824's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.54685926'}^[23].
• Q85833824's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.965'}^[24].
• Q85833824's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.86'}^[25].
• Q85833824's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0724'}^[26].

Body

Definition and Type

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