Q85834140

Summary

Q85834140 is a rotating variable star^[1].

Key Facts

• Q85834140's instance of is recorded as rotating variable star^[2].
• Q85834140's instance of is recorded as star^[3].
• Q85834140's instance of is recorded as near-infrared source^[4].
• Q85834140's constellation is recorded as Lyra^[5].
• Q85834140's spectral class is recorded as G6^[6].
• Q85834140's child astronomical body is recorded as Q28502950^[7].
• Q85834140's child astronomical body is recorded as Q28502951^[8].
• Q85834140's catalog code is recorded as Gaia DR2 2117317829237452160^[9].
• Q85834140's catalog code is recorded as KIC 8344004^[10].
• Q85834140's catalog code is recorded as 2MASS J18450713+4418559^[11].
• Q85834140's catalog code is recorded as Kepler-188^[12].
• Q85834140's catalog code is recorded as KOI-573^[13].
• Q85834140's catalog code is recorded as Gaia DR3 2117317829237452160^[14].
• Q85834140's catalog code is recorded as TIC 123235018^[15].
• Q85834140's catalog code is recorded as SPOCS 3797^[16].
• Q85834140's type of variable star is recorded as rotating variable star^[17].
• Q85834140's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.536'}^[18].
• Q85834140's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.197'}^[19].
• Q85834140's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.144'}^[20].
• Q85834140's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.620576'}^[21].
• Q85834140's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.0363429'}^[22].
• Q85834140's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.0223525'}^[23].
• Q85834140's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0241'}^[24].
• Q85834140's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-19.52'}^[25].
• Q85834140's metallicity is recorded as {'unit': '1', 'amount': '+0.003'}^[26].

Body

Definition and Type

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