Q90050611
rotating variable star in the constellation Lyra
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Q90050611
Summary
Q90050611 is a rotating variable star[1].
Key Facts
- Q90050611's instance of is recorded as rotating variable star[2].
- Q90050611's instance of is recorded as star[3].
- Q90050611's instance of is recorded as near-infrared source[4].
- Q90050611's constellation is recorded as Lyra[5].
- Q90050611's spectral class is recorded as G0.5V[6].
- Q90050611's child astronomical body is recorded as Q28857406[7].
- Q90050611's child astronomical body is recorded as Q21067504[8].
- Q90050611's catalog code is recorded as Gaia DR2 2101689061725421312[9].
- Q90050611's catalog code is recorded as KIC 6364582[10].
- Q90050611's catalog code is recorded as 2MASS J19280049+4147130[11].
- Q90050611's catalog code is recorded as Gaia DR3 2101689061725421312[12].
- Q90050611's catalog code is recorded as TIC 137408775[13].
- Q90050611's catalog code is recorded as SPOCS 3588[14].
- Q90050611's catalog code is recorded as KOI-3456[15].
- Q90050611's catalog code is recorded as Kepler-1505[16].
- Q90050611's type of variable star is recorded as rotating variable star[17].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.402'}[18].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.913'}[19].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.810'}[20].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.697'}[21].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.830'}[22].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.497'}[23].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.406'}[24].
- Q90050611's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.917766'}[25].
- Q90050611's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.288442'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], and near-infrared source[4].