Simulations suggest that Saturn’s smallest, innermost moon could have an expanding, geologically young ocean. When a Southwest Research Institute scientist discovered surprising evidence that Saturn’s smallest, innermost moon could generate the right amount of heat to support a liquid internal ocean, colleagues began studying Mimas’ surface to understand how its interior may have evolved. Numerical simulations of the moon’s Herschel impact basin, the most striking feature on its heavily cratered surface, determined that the basin’s structure and the lack of tectonics on Mimas are compatible with a thinning ice shell and geologically young ocean.
“In the waning days of NASA’s Cassini mission to Saturn, the spacecraft identified a curious libration, or os...
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