First-principles simulations predict that metallic liquid H3O, stabilized at 450-600 GPa, forms a thin conducting shell near the cores of Uranus and Neptune that can power their anomalous magnetic fields.
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Metallic liquid H3O in a thin-shell zone inside Uranus and Neptune
First-principles simulations predict that metallic liquid H3O, stabilized at 450-600 GPa, forms a thin conducting shell near the cores of Uranus and Neptune that can power their anomalous magnetic fields.