Abstract Details

USING THERMAL INFRARED OBSERVATIONS TO CHARACTERIZE THE THERMOPHYSICAL AND COMPOSITIONAL PROPERTIES OF THE LACUS MORTIS REGION OF THE MOON

WILLIAMS, Jean-Pierre1, GREENHAGEN, Benjamin T.2, BENNETT, Kristen A.3, PAIGE, David1, KUMARI, Nandita4, AHRENS, Caitlin J.5, RUBANENKO, Lior6, POWELL, Tyler1, PREM, Parvathy7, BLEWETT, David T.7, RUSSELL, Patrick8, HAYNE, Paul O.9 and SULLIVAN, Mark T.1, (1)Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095, (2)Johns Hopkins Applied Physics Laboratory, 11101 Johns Hopkins Rd, Laurel, MD 20723, (3)US Geological Survey, 2255 N Gemini Dr, Flagstaff, AZ 86001-1698, (4)Department of Geosciences, Stony Brook University, Stony Brook, NY 11794, (5)Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, (6)Department of Geological Sciences, Stanford University, Mail Code 2115, Stanford, CA 94305, (7)Johns Hopkins University Applied Physics Laboratory, 11101 Johns Hopkins Rd, Laurel, MD 20723, (8)Earth, Planetary, and Space Sciences, UCLA, Los Angeles, CA 90095, (9)Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, 2000 Colorado Ave, Boulder, CO 80305