  We identify jet-shaped morphology in the core-collapse supernova remnant
(SNR) CTB 1 that includes two opposite structural features. We identify these
as the imprints of a pair of jets that were among the last jets to explode the
massive stellar progenitor of CTB 1. We find the projected angle between the
jets' axis and the direction of the pulsar velocity, which is the neutron star
natal kick, to be 78 degrees. We tentatively identify possible signatures of a
second pair of opposite jets along a different direction. If this
identification holds, SNR CTB 1 has a point-symmetric structure. The morphology
and large angle of the jets' axis to kick velocity are expected in the
jittering jets explosion mechanism (JJEM) of core-collapse supernovae.
