a JHU Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA b Institute for Astronomy, University of Hawai'i, 640 N. Aohaku Place, Hilo, HI 96720, USA c Ithaca College, Department of Physics, Ithaca, NY 14850, USA
Abstract:
We present observational evidence that carbonates and iron-rich clays are present on the surface of Ceres. These components are also present in CI chondrites and provide a means of explaining the unusual spectrum of this object as well as providing potential insight into its evolution.