Basalt thicknesses in mare basins have been determined using assumptio
ns about the premare topography of partly buried craters and by compar
ison to the Orientale basin. Differences in those assumptions have led
to a factor of 4 difference in mare thickness estimates. Further, kno
wledge of thickness is restricted to areas in which buried craters are
present. Using mixing models applied to multispectral images acquired
by the Clementine spacecraft, we have shown that craters in the mare
sometimes excavate highland material from below the mare cover. Using
such craters and assumptions about their depth of excavation, we obtai
n independent estimates of basalt thickness. Our results are in agreem
ent with the lowest of previous thickness estimates. We derive a volum
e of 40,000 km(3) for basalts in Mare Humorum, considerably less than
the similar to 110,000 km(3) from previous estimates. We also confirm
a diameter of 425 km for the Humorum multiring basin based on the Clem
entine gridded global topography, assuming an original morphology like
Orientale.