A Probabilistic Approach to Determination of Ceres' Average Surface Composition From Dawn Visible‐Infrared Mapping Spectrometer and Gamma Ray and Neutron Detector Data

The Visible‐Infrared Mapping Spectrometer (VIR) on board the Dawn spacecraft revealed that aqueous secondary minerals—Mg‐phyllosilicates, NH4‐bearing phases, and Mg/Ca carbonates—are ubiquitous on Ceres. Ceres' low reflectance requires dark phases, which were assumed to be amorphous carbon and/...

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Bibliographic Details
Published inJournal of geophysical research. Planets Vol. 125; no. 12
Main Authors Kurokawa, H., Ehlmann, B. L., De Sanctis, M. C., Lapôtre, M. G. A., Usui, T., Stein, N. T., Prettyman, T. H., Raponi, A., Ciarniello, M.
Format Journal Article
LanguageEnglish
Published 01.12.2020
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