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. Author manuscript; available in PMC: 2018 May 30.
Published in final edited form as: J Geophys Res Planets. 2016 Sep 9;121(10):1865–1884. doi: 10.1002/2016JE005128

Figure 13.

Figure 13

Processes involved in space weathering of Ceres. Because the environment is so unlike that at 1 AU, the dominant processes are distinctly different and include contamination and mixing with exogenic material as well as formation of a surficial lag deposit as volatile materials sublimate or are lost.