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Image for: Frictional Heat Powers Hydrothermal Activity on Enceladus


Surface, ocean and core of Saturn's moon Enceladus. Computer simulation shows how the icy moon heats water in a porous rock core.
Surface, ocean and core of Saturn's moon Enceladus. Computer simulation shows how the icy moon heats water in a porous rock core.

Source: Surface – NASA/JPL-Caltech/Space Science Institute; Core – Choblet et al (2017); Graphic composition – ESA

(1791 KB, 4267 x 3200 pixels)

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