31/08/2026
Far beneath the clouds of Uranus and Neptune, matter may behave in a way unlike anything we experience on Earth.
New computer simulations by Carnegie researchers Cong Liu and Ronald Cohen suggest that the extreme interiors of the ice giants could support an unusual superionic form of carbon hydride, a state that behaves partly like a solid and partly like a fluid.
The team recreated conditions reaching roughly 30 million times Earth’s atmospheric pressure and temperatures near 6,000 kelvin. Under those extremes, the carbon atoms are predicted to form a stable hexagonal framework, while hydrogen atoms remain mobile, moving through narrow spiral shaped channels inside the structure.
That unusual motion could strongly affect how heat and electrical charge travel through the deep interiors of Uranus and Neptune. It may also help scientists understand one of their greatest mysteries: both planets possess unusually tilted and displaced magnetic fields that are very different from the more symmetric fields of Earth, Jupiter and Saturn.
The implications may extend beyond planetary science. If these exotic phases can eventually be reproduced or studied in laboratory conditions, they could reveal entirely new ways that simple elements behave under extreme pressure.
What looks like an ordinary mixture of carbon and hydrogen may become something completely different deep inside an ice giant.
📄 Research paper
📌 Liu et al., Prediction of Thermally Driven Quasi One Dimensional Superionic States in Carbon Hydride Under Giant Planetary Conditions, Nature Communications, 2026.