We present new radial velocities for 306 bright (R < 16) galaxies in a 77 d
eg(2) region of the Shapley supercluster, measured with the FLAIR-II spectr
ograph on the UK Schmidt Telescope. The galaxies we measured were uniformly
distributed over the survey area, in contrast to previous samples which we
re concentrated in several rich Abell clusters. Most of the galaxies (230)
were members of the Shapley supercluster: they trace out two previously unk
nown sheets of galaxies linking the Abell clusters of the supercluster. In
a 44 deg2 area of the supercluster excluding the Abell dusters, these sheet
s alone represent an overdensity of a factor of 2.0+/-0.2 compared to a uni
form galaxy distribution. The supercluster is not flattened in the Declinat
ion direction as has been suggested in previous papers. Within our survey a
rea the new galaxies contribute an additional 50% to the known contents of
the Shapley supercluster, with a corresponding increase in its contribution
to the motion of the Local Group.