Q87810996
rotating variable star in the constellation Lyra
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Q87810996
Summary
Q87810996 is a rotating variable star[1].
Key Facts
- Q87810996's instance of is recorded as rotating variable star[2].
- Q87810996's instance of is recorded as star[3].
- Q87810996's instance of is recorded as near-infrared source[4].
- Q87810996's instance of is recorded as eruptive variable star[5].
- Q87810996's constellation is recorded as Lyra[6].
- Q87810996's spectral class is recorded as G7[7].
- Q87810996's child astronomical body is recorded as Q28502886[8].
- Q87810996's child astronomical body is recorded as Q28502888[9].
- Q87810996's catalog code is recorded as Gaia DR2 2104098950692667264[10].
- Q87810996's catalog code is recorded as 2MASS J18580508+4137465[11].
- Q87810996's catalog code is recorded as KIC 6266741[12].
- Q87810996's catalog code is recorded as Kepler-170[13].
- Q87810996's catalog code is recorded as KOI-508[14].
- Q87810996's catalog code is recorded as UCAC4 659-068540[15].
- Q87810996's catalog code is recorded as Gaia DR3 2104098950692667264[16].
- Q87810996's catalog code is recorded as TIC 120253745[17].
- Q87810996's type of variable star is recorded as rotating variable star[18].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.143'}[19].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.773'}[20].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.677'}[21].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.334707'}[22].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.161'}[23].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.303'}[24].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.898'}[25].
- Q87810996's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.521'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].