The core accretion theory of planetary formation does not predict that super-Jupiters will form beyond the snow line of a low mass stars .
We present a discovery of 3.9 \pm 1.2 ~ { } M _ { Jup } mass planet orbiting the 0.59 \pm 0.17 ~ { } M _ { \odot } star using the gravitational microlensing method .
During the event , the projected separation of the planet and the star is 3.9 \pm 1.0 ~ { } { AU } i.e. , the planet is significantly further from the host star than the snow line .
This is a fourth such planet discovered using the microlensing technique and challenges the core accretion theory .