Water, when pushed to the most extreme conditions found deep within giant planets, transforms into a superionic state—an exotic, electricity-conducting solid. This unusual form, believed to be abundant in celestial bodies like Uranus and Neptune, is now understood to possess an atomic structure far more complex than scientists previously imagined, offering new insights into how these planets generate their powerful magnetic fields.

For decades, researchers have hypothesized the existence of superionic water, where oxygen atoms lock into a rigid crystal lattice while hydrogen ions move freely through it, conducting electricity. This unique behavior makes it a prime candidate for explaining the enigmatic magnetic fields of “ice giants.” The recent findings, detailed by institutions including the University of Rostock, challenge prior assumptions about its internal order.

The implications extend beyond our solar system, influencing models for exoplanets. Understanding this strange form of water is crucial because it could be the most common type of water in the universe, shaping the evolution and characteristics of countless worlds. The latest experiments provide unprecedented clarity on its microscopic arrangement.

New insights into superionic water’s complex structure

Previous models suggested that the oxygen atoms in superionic water would arrange themselves into one of two simple cubic patterns: body-centered cubic or face-centered cubic. However, groundbreaking experiments, as reported by ScienceDaily on January 13, 2026, reveal a much messier reality. Instead of a single, orderly pattern, the oxygen atoms form a mixed structure combining face-centered cubic regions with hexagonal close-packed layers. This hybrid arrangement creates widespread structural disorder.

Scientists leveraged powerful X-ray lasers at facilities like the Matter in Extreme Conditions (MEC) instrument at LCLS in the US and the HED-HIBEF instrument at European XFEL. These advanced tools allowed them to subject water to pressures exceeding 1.5 million atmospheres and temperatures of several thousand degrees Celsius, capturing atomic snapshots within trillionths of a second. The precision of these measurements uncovered the irregular, hybrid sequence of oxygen atoms.

This structural complexity is analogous to ordinary ice, which also exists in numerous crystal phases depending on specific temperature and pressure conditions. The discovery reinforces that water, despite its apparent simplicity, continues to surprise researchers with its remarkable behaviors under extreme environments. The findings align with the most advanced computer simulations, validating the experimental approach.

Reshaping models of giant planets’ magnetic fields

The existence of superionic water deep within Uranus and Neptune has long been a key hypothesis for their unusual magnetic fields. Unlike Earth’s field, which is largely dipolar and aligned with its rotational axis, the magnetic fields of these ice giants are highly tilted and offset from their centers. The newly revealed “messy” atomic structure of superionic water provides a more nuanced understanding of the fluid dynamics and electrical conductivity within their interiors.

This refined understanding of superionic water’s properties is critical for improving models of planetary internal structure and long-term evolution. Researchers from the University of Rostock and a large international collaboration, supported by the German Research Foundation (DFG) and the French ANR, contributed to this significant advance. Their work suggests that the dynamic interplay between these mixed crystal patterns could be fundamental to generating the complex magnetic fields observed around these distant worlds.

Ultimately, this research helps us better comprehend not only our own solar system’s mysterious giants but also the myriad of similar exoplanets believed to populate the cosmos. The ongoing exploration of water under such extreme conditions continues to unveil its hidden complexities, fundamentally changing our perspective on planetary science and the potential for life beyond Earth.