Q90955841
eclipsing binary star
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Q90955841
Summary
Q90955841 is an eclipsing binary star[1].
Key Facts
- Q90955841's instance of is recorded as eclipsing binary star[2].
- Q90955841's instance of is recorded as star[3].
- Q90955841's instance of is recorded as near-infrared source[4].
- Q90955841's instance of is recorded as rotating variable star[5].
- Q90955841's instance of is recorded as eruptive variable star[6].
- Q90955841's constellation is recorded as Lyra[7].
- Q90955841's spectral class is recorded as K2III[8].
- Q90955841's catalog code is recorded as Gaia DR2 2106751007097870976[9].
- Q90955841's catalog code is recorded as KIC 8803882[10].
- Q90955841's catalog code is recorded as 2MASS J18591126+4505567[11].
- Q90955841's catalog code is recorded as KOI-2659[12].
- Q90955841's catalog code is recorded as UCAC4 676-066943[13].
- Q90955841's catalog code is recorded as Gaia DR3 2106751007097870976[14].
- Q90955841's catalog code is recorded as TIC 164785576[15].
- Q90955841's catalog code is recorded as SPOCS 3870[16].
- Q90955841's type of variable star is recorded as rotating variable star[17].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.489'}[18].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.013'}[19].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.910'}[20].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.941487'}[21].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.693'}[22].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.988'}[23].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.666'}[24].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.263'}[25].
- Q90955841's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.219'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], star[3], near-infrared source[4], rotating variable star[5], and eruptive variable star[6].