Ice under cover: Using bulk spatial and physical properties of probable ground ice driven mass wasting features on Ceres to better understand its surface
Kynan Hughson1, Steven J Schwartz2, Britney Schmidt3, Heather Chilton4, Jennifer E. C. Scully5, Julie C Castillo5, Jean Philippe Combe6, Eleonora Ammannito7, Hanna Sizemore8, Thomas Platz8,9, Shane Byrne10, Andreas Nathues9 and Carol A Raymond11, (1)University of Alaska Anchorage, Anchorage, AK, United States, (2)University of California Los Angeles, Department of Earth, Planetary and Space Sciences, Los Angeles, CA, United States, (3)Cornell University, Astronomy and Earth & Atmospheric Sciences, Ithaca, United States, (4)California State University Fullerton, Fullerton, CA, United States, (5)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (6)Bear Fight Institute, Winthrop, WA, United States, (7)University of California Los Angeles, Los Angeles, United States, (8)Planetary Science Institute Tucson, Tucson, AZ, United States, (9)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (10)University of Arizona, Tucson, AZ, United States, (11)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
