Heat from friction could power hydrothermal activity on Saturn's moon Enceladus for billions of years if the moon has a highly porous core, according to a new modeling study by European and U.S. researchers working on NASA's Cassini mission.

The study, published today in the journal Nature Astronomy, helps resolve a question scientist have grappled with for a decade:  Where does the energy to power the extraordinary geologic activity on Enceladus come from?

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One of the strongest chemical bonds in organic chemistry is formed between carbon and fluorine, giving unique properties to chemical compounds featuring this group. Pharmaceutical researchers are very interested in carbon-fluorine bond containing molecules because of the way they mimic certain behaviors of biological compounds. However, the strength of the carbon-fluorine bond makes it difficult to remove and replace fluorine atoms in a molecule, greatly limiting the structures and types of chemicals that can be made.

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