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Observation of Hexagonal Close-Packed Water Ice at Conditions in Ice Giant Planetary Interiors

Alexis Forestier1,2,*, Gunnar Weck1,2, Sandra Ninet3, Gaston Garbarino4, Mohamed Mezouar4, Frédéric Datchi3, and Paul Loubeyre1,2

  • *Contact author: alexis.forestier@cea.fr

Phys. Rev. Lett. 137, 114101 – Published 9 September, 2026

DOI: https://doi.org/10.1103/sdrk-3m4t

Abstract

Using synchrotron x-ray diffraction in laser-heated diamond anvil cells, we report the observation of a hexagonal close-packed (hcp) phase of water ice at high pressure and temperature conditions. Above 200 GPa and 1800 K, the hcp phase becomes dominant upon entering the superionic regime, as evidenced by anomalous thermal expansion. Observations are consistent with the hcp phase becoming thermodynamically more stable than the face-centered cubic (fcc) phase via a martensitic transition extending across the 130–200 GPa pressure range, within the superionic regime. Hcp ice is also observed to emerge from stacking disorder developing within the fcc oxygen lattice upon cooling, during its reversion to the body-centered cubic phase. The presence of an fcc-hcp martensitic transition in the superionic regime of warm dense ice may have implications for planetary models of Uranus and Neptune.

Physics Subject Headings (PhySH)

synopsis

Making Uranian and Neptunian Ice on Earth

Published 9 September, 2026

Researchers crushed and heated ice between diamond anvils to confirm the existence of a phase of ice that could be present in the warm mantles of ice giants.

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