  I suggest that the recently observed hot-dust elongated structure that likely
engulfs the neutron star (NS) remnant of supernova (SN) 1987A was shaped by
jets that the NS launched shortly after it acquired its natal kick velocity. I
take the axis of the two post-kick jets to be along the long dimension of the
hot-dust elongated structure, which I term the bipolar lobe. The jittering jets
explosion mechanism accounts for the misalignment of the post-kick jets axis
and the main-jets axis of the ejecta. For post-kick jets to shape the bipolar
lobe their energy should have been about equal to the energy of the ejecta
inner to the outer edge of the lobe, E(2j)~E(ej,lobe)~4.6e48erg. For an
efficiency of 0.01-0.1 to convert accretion energy to post-kick jets' energy I
estimate that the post-kick accreted mass was Macc~0.0002-0.002Mo. The negative
jets feedback mechanism, where jets remove some of the mass that could have
been accreted, accounts for the limited amount of accreted mass. This study
adds to the growing recognition of the importance of jets in core collapse
supernovae, including post-explosion jets.
