The distribution of elevations on the moon determined by Clementine de
viates strongly from a normal distribution, suggesting that several ge
ologic processes have influenced the topography. The hypsograms for th
e near side and far side of the moon are distinctly different, and the
se differences correlate with differences in composition as determined
by Apollo orbital geochemistry, Clementine global multispectral imagi
ng, and groundbased spectroscopy. The hypsograms and compositional dat
a indicate the presence of at least five compositional-altimetric unit
s. The lack of fill of the South Pole-Aitken Basin by mare basalts sug
gests poor production efficiency of mare basalt in the mantle of this
area of the moon.