Q86174846
rotating variable star in the constellation Lyra
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Q86174846
Summary
Q86174846 is a rotating variable star[1].
Key Facts
- Q86174846's instance of is recorded as rotating variable star[2].
- Q86174846's instance of is recorded as star[3].
- Q86174846's instance of is recorded as near-infrared source[4].
- Q86174846's constellation is recorded as Lyra[5].
- Q86174846's spectral class is recorded as F8IV-V[6].
- Q86174846's child astronomical body is recorded as Q92356968[7].
- Q86174846's catalog code is recorded as Gaia DR2 2099957605786905344[8].
- Q86174846's catalog code is recorded as KIC 3098810[9].
- Q86174846's catalog code is recorded as 2MASS J19045357+3815294[10].
- Q86174846's catalog code is recorded as KOI-1878[11].
- Q86174846's catalog code is recorded as Kepler-1773[12].
- Q86174846's catalog code is recorded as Gaia DR3 2099957605786905344[13].
- Q86174846's catalog code is recorded as TIC 120763491[14].
- Q86174846's catalog code is recorded as SPOCS 3314[15].
- Q86174846's type of variable star is recorded as rotating variable star[16].
- Q86174846's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.970'}[17].
- Q86174846's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.753'}[18].
- Q86174846's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.692'}[19].
- Q86174846's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.933461'}[20].
- Q86174846's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.085'}[21].
- Q86174846's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.16'}[22].
- Q86174846's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.41'}[23].
- Q86174846's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5008'}[24].
- Q86174846's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-15.7'}[25].
- Q86174846's metallicity is recorded as {'unit': '1', 'amount': '+0.19'}[26].