Q86843980
rotating variable star in the constellation Lyra
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Q86843980
Summary
Q86843980 is a rotating variable star[1].
Key Facts
- Q86843980's instance of is recorded as rotating variable star[2].
- Q86843980's instance of is recorded as star[3].
- Q86843980's instance of is recorded as near-infrared source[4].
- Q86843980's constellation is recorded as Lyra[5].
- Q86843980's spectral class is recorded as G3[6].
- Q86843980's child astronomical body is recorded as Q28503124[7].
- Q86843980's child astronomical body is recorded as Q28503125[8].
- Q86843980's catalog code is recorded as Gaia DR2 2103671481186902912[9].
- Q86843980's catalog code is recorded as KIC 5941160[10].
- Q86843980's catalog code is recorded as 2MASS J18573837+4114148[11].
- Q86843980's catalog code is recorded as Kepler-200[12].
- Q86843980's catalog code is recorded as KOI-654[13].
- Q86843980's catalog code is recorded as Gaia DR3 2103671481186902912[14].
- Q86843980's catalog code is recorded as TIC 120252452[15].
- Q86843980's catalog code is recorded as SPOCS 3531[16].
- Q86843980's type of variable star is recorded as rotating variable star[17].
- Q86843980's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.871'}[18].
- Q86843980's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.580'}[19].
- Q86843980's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.455'}[20].
- Q86843980's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.940111'}[21].
- Q86843980's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.9023188'}[22].
- Q86843980's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.95519286'}[23].
- Q86843980's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5024'}[24].
- Q86843980's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-40.14'}[25].
- Q86843980's metallicity is recorded as {'unit': '1', 'amount': '-0.006'}[26].