We report the first resolved bispectrum speckle interferometry of the symbiotic binary CH Cyg .
The measured component separation , \rho = 42 \pm 2 mas , is consistent with the one derived from the known spectroscopic orbit and distance .
In particular , our result implies a total mass of the binary of M _ { t } = M _ { g } + M _ { wd } = 3.7 ^ { +3.5 } _ { -1.7 } M _ { \sun } , which is in good agreement with the value M _ { t } = 2.7 ^ { +1.2 } _ { -0.6 } M _ { \sun } derived from the spectroscopic orbit solution for the red giant and evolutionary contraints .
We also show that the radio jets and the bipolar outflow are not orthogonal to the orbital plane of the binary system .