BY STUDYING ADDITIONAL CRATERS OF VARYING AGES WE WILL BE ABLE TO CHARACTERIZE THE EVOLUTION OF SUPERPOSED CRATERS AND THE EJECTA FACIES AND TERRAIN TYPES THEREBY CONSTRAINING THE RATES AT WHICH MATERIALS ARE HOMOGENIZED INTO REGOLITH.
$548,146FY2021National Aeronautics and Space AdministrationNASA
University Of California, Los Angeles