We present polarization-phase awe measurements and analysis for three basal
t samples: fresh, dark red varnished, and dark gray varnished. Each sample
displays a prominent opposition surge, countering the widely held notion th
at only particulate surfaces, and not bare rock, will display this phenomen
on. The most likely cause of the opposition surge is coherent backscatterin
g, but the width of the surge suggests that other mechanisms may also contr
ibute. The photopolarimetric properties of the samples; especially the nega
tive branch parameters, are most comparable to those of C-class asteroids,
(C) 1999 Academic Press.