Ice-giant interiors support superionic water
An image of Neptune from Voyager 2. Credit: NASA/JPL-Caltech Deep inside Neptune and Uranus, temperatures and pressures are extreme enough to produce superionic water—a phase in which oxygen ions crystallize while highly mobile hydrogen ions float through interstitial spaces. Information about superionic water’s phase behavior would help planetary scientists model and understand the ice giants’ evolution, structure, and unusual magnetic fields. Theoretical and computational studies of superionic water’s structure and stability have supplemented scarce experimental data—the phase was observed for the first time in 2019. But those have yielded limited, and sometimes contradictory, results. Now Bingqing Cheng at the University of Cambridge and her collaborators have made predictions about superionic water’s lattice structure at planetary conditions by simulating the material using machine-learning potentials (MLPs) and an artificial neural-network architecture. Molecular-dyn...