New Chemical Models Might Reveal Whether Icy Moons of Saturn and Jupiter Contain Life

Recent studies aim to determine the habitability of Saturn’s moon Enceladus using improved chemical models. These tools simulate how organic compounds interact with icy environments under extreme conditions. The research, led by Charity Phillips-Lander and Florent Bocher, focuses on phenomena such as organic-doped ice pores, replicating conditions found on icy moons.

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