Ready for Their Close-up: Insights about Occator’s Bright Faculae Derived from New, Highest Resolution Observations of Ceres
Jennifer E. C. Scully1, David A Williams2, Debra Buczkowski3, Paul Schenk4, Britney Schmidt5, Hanna Sizemore6, Margaret E Landis7, Michael Sori8, Jan Hendrik Pasckert9, Adrian Neesemann10, David P O'Brien11, Julie C Castillo1, Carol A Raymond12, Christopher T Russell13, Ralf Jaumann14, Katrin Stephan15, Mark V Sykes11 and The Dawn Team, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)Arizona State University, Tempe, AZ, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (4)Lunar and Planetary Institute, USRA, Houston, TX, United States, (5)Cornell University, Astronomy and Earth & Atmospheric Sciences, Ithaca, United States, (6)Planetary Science Institute, Tuscon, United States, (7)Planetary Science Institute Albuquerque, Albuquerque, NM, United States, (8)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (9)University of Münster, Münster, Germany, (10)FU, Berlin, Germany, (11)Planetary Science Institute, Tucson, AZ, United States, (12)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (13)University of California Los Angeles, Los Angeles, United States, (14)German Aerospace Ctr, Berlin, Germany, (15)German Aerospace Center, Berlin, Germany
