  We identify a point-symmetric morphology of the supernova remnant (SNR)
Cassiopeia A compatible with shaping by at least two, and more likely more than
four, pairs of opposite jets, as expected in the jittering jets explosion
mechanism (JJEM) of core-collapse supernovae. Using an old X-ray map of argon,
we identify seven pairs of opposite morphological features that we connect with
lines that cross each other at the same point on the plane of the sky. The
opposite morphological features include protrusions, clumps, filaments, and
funnels in the main SNR shell. In addition to these seven symmetry axes, we
find two tentative symmetry axes (lines). These lines form a point-symmetric
wind-rose. We place this point-symmetric wind-rose on a new JWST and X-ray
images of Cassiopeia A. We find other morphological features and one more
symmetry axis that strengthen the identified point-symmetric morphology. Not
all symmetry axes correspond to jets; e.g., some clumps are formed by the
compression of ejecta between two jet-inflated lobes (bubbles). The robust
point-symmetric morphology in the iconic Cassiopeia A SNR strongly supports the
JJEM and poses a severe challenge to the neutrino-driven explosion mechanism.
