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The core accretion theory of planetary formation does not predict thatsuper-Jupiters will form beyond the snow line of a low mass stars. We present adiscovery of 3.9 +- 1.2 M_Jup mass planet orbiting the 0.59 +- 0.17 M_Sun starusing the gravitational microlensing method. During the event, the projectedseparation of the planet and the star is 3.9 +- 1.0 AU i.e., the planet issignificantly further from the host star than the snow line. This is a fourthsuch planet discovered using the microlensing technique and challenges the coreaccretion theory.

Super-massive planets around late-type stars - the case of OGLE-2012-BLG-0406Lb