Q85834137

Summary

Q85834137 is an eruptive variable star^[1].

Key Facts

• Q85834137's instance of is recorded as eruptive variable star^[2].
• Q85834137's instance of is recorded as star^[3].
• Q85834137's instance of is recorded as near-infrared source^[4].
• Q85834137's constellation is recorded as Lyra^[5].
• Q85834137's spectral class is recorded as G2V^[6].
• Q85834137's child astronomical body is recorded as Q28855514^[7].
• Q85834137's catalog code is recorded as SPOCS 2987^[8].
• Q85834137's catalog code is recorded as Gaia DR2 2107114704928577792^[9].
• Q85834137's catalog code is recorded as KOI-22^[10].
• Q85834137's catalog code is recorded as KIC 9631995^[11].
• Q85834137's catalog code is recorded as 2MASS J18503111+4619240^[12].
• Q85834137's catalog code is recorded as Kepler-422^[13].
• Q85834137's catalog code is recorded as TOI-2176^[14].
• Q85834137's catalog code is recorded as Gaia DR3 2107114704928577792^[15].
• Q85834137's catalog code is recorded as TIC 123495874^[16].
• Q85834137's type of variable star is recorded as rotating variable star^[17].
• Q85834137's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.357'}^[18].
• Q85834137's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.126'}^[19].
• Q85834137's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.041'}^[20].
• Q85834137's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.642'}^[21].
• Q85834137's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.411342'}^[22].
• Q85834137's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.7282796'}^[23].
• Q85834137's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.15'}^[24].
• Q85834137's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.2894976'}^[25].
• Q85834137's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.24'}^[26].

Body

Definition and Type

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