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Fig. 1

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Cryovolcanic features on Ceres' surface. The materials that form Cerealia Tholus (A), Ahuna Mons (B), and the exposed parts of Liberalia Mons (C), revealed by the impact of the Xevioso crater, are notable for their bright colour spectrum, which contrasts sharply with the darker tones of the average surface of Ceres. Credit: NASAZJPL-CaltechZUCLAZMPSZDLRZIDAZPSI. Image numbers: PIA20350 and PIA21907.

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