Reviews in Mineralogy & Geochemistry Vol. 60, pp. 83-219, 2006 2 Copyright © Mineralogical Society of America Understanding the Lunar Surface and Space-Moon Interactions Paul Lucey1, Randy L. Korotev2, Jeffrey J. Gillis1, Larry A. Taylor3, David Lawrence4, Bruce A. Campbell5, Rick Elphic4, Bill Feldman4, Lon L. Hood6, Donald Hunten7, Michael Mendillo8, Sarah Noble9, James J. Papike10, Robert C. Reedy10, Stefanie Lawson11, Tom Prettyman4, Olivier Gasnault12, Sylvestre Maurice12 1University of Hawaii at Manoa, Honolulu, Hawaii, U.S.A. 2Washington University, St. Louis, Missouri, U.S.A. 3University of Tennessee, Knoxville, Tennessee, U.S.A. 4Los Alamos National Laboratory, Los Alamos, New Mexico, U.S.A. 5Smithsonian Institution, Washington D.C., U.S.A. 6Lunar and Planetary Laboratory, Univ. of Arizona, Tucson, Arizona, U.S.A. 7University of Arizona, Tucson, Arizona, U.S.A. 8Boston University, Cambridge, Massachusetts, U.S.A. 9Brown University, Providence, Rhode Island, U.S.A. 10University of New Mexico, Albuquerque, New Mexico, U.S.A. 11 Northrop Grumman, Van Nuys, California, U.S.A. 12Centre d’Etude Spatiale des Rayonnements, Toulouse, France Corresponding authors e-mail: Paul Lucey <
[email protected]> Randy Korotev <
[email protected]> 1. INTRODUCTION The surface of the Moon is a critical boundary that shapes our understanding of the Moon as a whole. All geologic mapping and remote sensing techniques utilize only the outermost portion of the Moon. Before leaving the Moon for study in our laboratories, all lunar samples that have been studied existed at or very near the surface. With the exception of the deeply probing geophysical techniques, our understanding of the interior of the Moon is derived from surficial, but not superficial, information, coupled with geologic reasoning.