Q82138467

Summary

Q82138467 is a rotating variable star^[1].

Key Facts

• Q82138467's instance of is recorded as rotating variable star^[2].
• Q82138467's instance of is recorded as star^[3].
• Q82138467's instance of is recorded as near-infrared source^[4].
• Q82138467's constellation is recorded as Cygnus^[5].
• Q82138467's spectral class is recorded as G2^[6].
• Q82138467's child astronomical body is recorded as Q28502803^[7].
• Q82138467's child astronomical body is recorded as Q28502801^[8].
• Q82138467's catalog code is recorded as Gaia DR2 2087172999977491328^[9].
• Q82138467's catalog code is recorded as KIC 11521793^[10].
• Q82138467's catalog code is recorded as 2MASS J19521624+4924453^[11].
• Q82138467's catalog code is recorded as Kepler-143^[12].
• Q82138467's catalog code is recorded as KOI-352^[13].
• Q82138467's catalog code is recorded as Gaia DR3 2087172999977491328^[14].
• Q82138467's catalog code is recorded as TIC 28364164^[15].
• Q82138467's catalog code is recorded as SPOCS 4232^[16].
• Q82138467's type of variable star is recorded as rotating variable star^[17].
• Q82138467's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.590'}^[18].
• Q82138467's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.292'}^[19].
• Q82138467's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.223'}^[20].
• Q82138467's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.693681'}^[21].
• Q82138467's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.6975898'}^[22].
• Q82138467's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.354216'}^[23].
• Q82138467's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2219'}^[24].
• Q82138467's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-32.28'}^[25].
• Q82138467's metallicity is recorded as {'unit': '1', 'amount': '-0.073'}^[26].

Body

Definition and Type

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