Q85293704
eclipsing binary star in the constellation Cygnus
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Q85293704
Summary
Q85293704 is an eclipsing binary star[1].
Key Facts
- Q85293704's instance of is recorded as eclipsing binary star[2].
- Q85293704's instance of is recorded as near-infrared source[3].
- Q85293704's instance of is recorded as rotating variable star[4].
- Q85293704's instance of is recorded as eruptive variable star[5].
- Q85293704's constellation is recorded as Cygnus[6].
- Q85293704's spectral class is recorded as G0V[7].
- Q85293704's child astronomical body is recorded as Q113594235[8].
- Q85293704's catalog code is recorded as KIC 9032900[9].
- Q85293704's catalog code is recorded as 2MASS J19422078+4521539[10].
- Q85293704's catalog code is recorded as KOI-134[11].
- Q85293704's catalog code is recorded as Gaia DR2 2079971473693847168[12].
- Q85293704's catalog code is recorded as UCAC4 677-072171[13].
- Q85293704's catalog code is recorded as Gaia DR3 2079971473693847168[14].
- Q85293704's catalog code is recorded as TIC 271772050[15].
- Q85293704's catalog code is recorded as SPOCS 3895[16].
- Q85293704's type of variable star is recorded as rotating variable star[17].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.628'}[18].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.413'}[19].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.322'}[20].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.619514'}[21].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.575'}[22].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.611'}[23].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.933'}[24].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.75'}[25].
- Q85293704's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.283'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], near-infrared source[3], rotating variable star[4], and eruptive variable star[5].