I will review and present new results on the role of jets in shaping pre-SN outbursts, in driving and shaping the explosion of core collapse supernovae, and in powering super luminous supernovae. As many massive stars are in binary systems, many of these will undergo strong binary interaction before explosion. Such interaction are likely to lead to jets that form and shape the medium into which the supernova expands into.   I will present new results of the jet feedback explosion mechanism, including the jittering jets mechanism, and connect its predicted outcomes to the morphologies of supernova remnants, including the morphology of SN 1987A. I will make the connection between the jet feedback mechanism and super-energetic supernovae. I will present arguments for my call for a paradigm shift from the neutrino-driven to jet-driven explosion mechanism.