Q86794723
rotating variable star in the constellation Lyra
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Q86794723
Summary
Q86794723 is a rotating variable star[1].
Key Facts
- Q86794723's instance of is recorded as rotating variable star[2].
- Q86794723's instance of is recorded as star[3].
- Q86794723's instance of is recorded as near-infrared source[4].
- Q86794723's constellation is recorded as Lyra[5].
- Q86794723's spectral class is recorded as K1V[6].
- Q86794723's child astronomical body is recorded as Q83207767[7].
- Q86794723's child astronomical body is recorded as Q86455755[8].
- Q86794723's catalog code is recorded as Gaia DR2 2119409512668086656[9].
- Q86794723's catalog code is recorded as KIC 10252275[10].
- Q86794723's catalog code is recorded as 2MASS J18425005+4719410[11].
- Q86794723's catalog code is recorded as Kepler-1907[12].
- Q86794723's catalog code is recorded as Gaia DR3 2119409512668086656[13].
- Q86794723's catalog code is recorded as TIC 123130285[14].
- Q86794723's catalog code is recorded as KOI-3130[15].
- Q86794723's catalog code is recorded as SPOCS 4063[16].
- Q86794723's type of variable star is recorded as rotating variable star[17].
- Q86794723's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.268'}[18].
- Q86794723's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.809'}[19].
- Q86794723's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.726'}[20].
- Q86794723's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.720085'}[21].
- Q86794723's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.989'}[22].
- Q86794723's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.23'}[23].
- Q86794723's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.23099793'}[24].
- Q86794723's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.831'}[25].
- Q86794723's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.647'}[26].