Q86853723
eclipsing binary star in the constellation Lyra
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Q86853723
Summary
Q86853723 is an eclipsing binary star[1].
Key Facts
- Q86853723's instance of is recorded as eclipsing binary star[2].
- Q86853723's instance of is recorded as star[3].
- Q86853723's instance of is recorded as near-infrared source[4].
- Q86853723's instance of is recorded as eruptive variable star[5].
- Q86853723's constellation is recorded as Lyra[6].
- Q86853723's spectral class is recorded as F5[7].
- Q86853723's child astronomical body is recorded as Q28856926[8].
- Q86853723's catalog code is recorded as Gaia DR2 2119130163697443840[9].
- Q86853723's catalog code is recorded as KIC 9753154[10].
- Q86853723's catalog code is recorded as 2MASS J18491229+4630583[11].
- Q86853723's catalog code is recorded as KOI-2457[12].
- Q86853723's catalog code is recorded as Kepler-1244[13].
- Q86853723's catalog code is recorded as UCAC4 683-066277[14].
- Q86853723's catalog code is recorded as Gaia DR3 2119130163697443840[15].
- Q86853723's catalog code is recorded as TIC 123447592[16].
- Q86853723's catalog code is recorded as SPOCS 3991[17].
- Q86853723's type of variable star is recorded as rotating variable star[18].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.503'}[19].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.351'}[20].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.269'}[21].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.317146'}[22].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.323'}[23].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.325'}[24].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.567'}[25].
- Q86853723's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.384'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], star[3], near-infrared source[4], and eruptive variable star[5].