  The source of the very bright Gamma-Ray Burst GRB 030329 is close enough to
us for there to be a hope to measure or significantly constrain its putative
superluminal motion. Such a phenomenon is expected in the ``Cannonball'' (CB)
model of GRBs. Recent precise data on the optical and radio afterglow of this
GRB --which demonstrated its very complex structure-- allow us to pin down the
CB-model's prediction for the afterglow-source position as a function of time.
It has been stated that (the unpublished part of) the new radio data
``unequivocably disprove'' the CB model. We show how greatly exaggerated that
obituary announcement was, and how precise a refined analysis of the data would
have to be, to be still of interest.
