  We analyze the morphologies of three core collapse supernova remnants
(CCSNRs) and the energy of jets in other CCSNRs and in Super Luminous
Supernovae (SLSNe) of type Ib/Ic/IIb, and conclude that these properties are
well explained by the last jets' episode as expected in the jet feedback
explosion mechanism of core collapse supernovae (CCSNe). The presence of two
opposite protrusions, termed ears, and our comparison of the CCSNR morphologies
with morphologies of planetary nebulae strengthen the claim that jets play a
major role in the explosion mechanism of CCSNe. We crudely estimate the energy
that was required to inflate the ears in two CCSNRs, and assume that the ears
were inflated by jets. We find that the energies of the jets that inflated ears
in 11 CCSNRs span a range that is similar to that of jets in some energetic
CCSNe (SLSNe), and that this energy, only of the last jets' episode, is much
less than the explosion energy. This finding is compatible with the jet
feedback explosion mechanism of CCSNe, where only the last jets, that carry a
small fraction of the total energy carried by earlier jets, are expected to
influence the outer parts of the ejecta. We reiterate our call for a paradigm
shift from neutrino-driven to jet-driven explosion models of CCSNe.
