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Search for sulfates on the surface of Ceres
DOI: 10.1111/maps.13024 Bibcode: 2018M&PS...53.1946B

McFadden, L. A.; Ruesch, O.; Li, J. -Y. +3 more

The formation of hydrated salts is an expected consequence of aqueous alteration of Main Belt objects, particularly for large, volatile-rich protoplanets like Ceres. Sulfates, present on water-bearing planetary bodies (e.g., Earth, Mars, and carbonaceous chondrite parent bodies) across the inner solar system, may contribute to Ceres' UV and IR spe…

2018 Meteoritics and Planetary Science
ISO 10