(Shoemaker, et al., 1994, Pieters et al., 1994); 8) 
improved understanding of the lunar photometric 
function (McEwen, 1996); and 9) the discovery of 
five broad compositional-altimetric units (Lucey et 
al, 1996). Many additional results are expected 
following completion of systematic processing efforts, 
now underway. 
References: 
Nozette, S., et al., 1994, Science 266, 1835. 
Davies, M.E., et al, 1994, The unified lunar control 
network: 1994 version. J. Geophys. Res. 99, 
23,211-23,214. 
Duxbury, T., et al, 1994, Clementine global 
geodetic/cartographic accuracy. Bull Am 
Astron. Soc. 26, 1097. 
McEwen, A.S., et al., 1995, Global albedo map of the 
Moon: Clementine 750-nm observations 
(abstract), LPSC XXV, 931-932. 
Oberst, J. et al, 1995, Clementine Stereo Data 
Analysis (abstract), LPSC XXV, 1067-1068. 
Zuber, M.T., et al, 1994, The shape and internal 
structure of the Moon from the Clementine 
Mission, Science, 266, 1839-43. 
Spudis, P.D. et al., 1994, Ancient multiring basins on 
the Moon revealed by Clementine laser 
altimetry, Science, 266, 1848-1851. 
Lucey et al, et al., 1995, Abundance and distribution 
of Iron on the Moon, Science, 268, 1150- 
1153. 
Moore, J.M. and A.S. McEwen, 1996, The abundance 
of large, Copernican-age craters on the 
Moon (abstract), LPSC XXVI, in press. 
McEwen, A.S., et al., 1994, Clementine observations 
of the Aristarchus region of the Moon, 
Science, 266, 1858-1862. 
Shoemaker, E.M., et al., 1994, The south pole region 
of the Moon as seen by Clementine, 
Science, 266, 1851-1854. 
Pieters, C.M., et al., 1994, A sharper view of impact 
craters fron Clementine data, Science, 266, 
1844-1848. 
McEwen, A.S., A precise lunar photometric function 
(abstract), LPSC XXVI, in press. 
Lucey, PG., et al., 1994, Topographic-compositional 
units on the Moon and the early evolution of 
the lunar crust, Science, 266, 1855-1858. 
703 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B4. Vienna 1996