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Planetary Interiors

All articles tagged with #planetary interiors

Earth-like cores may be the oddity in the galaxy's most common planets
science2 days ago

Earth-like cores may be the oddity in the galaxy's most common planets

A new study argues that the galaxy's most common planets—sub-Neptunes—may not have Earth-like layered interiors with a distinct metallic core and silicate mantle. If these planets accrete more than about 1% hydrogen by mass, hydrogen, iron, and silicate can mix into a single, homogeneous interior, changing how they cool, hold onto atmospheres, and evolve their radii. This could explain features like the radius gap and how radii relate to orbital period, and it offers testable predictions for JWST observations, though the model rests on extrapolations of material behavior under extreme pressures. In short, Earth-like cores might be the exception rather than the rule in the galaxy.

Helical Superionic Carbon-Hydrogen Emerges Inside Ice Giants
science1 month ago

Helical Superionic Carbon-Hydrogen Emerges Inside Ice Giants

New quantum simulations suggest carbon hydride (CH) can form a quasi-one-dimensional, spiral superionic state under extreme pressures (500–3,000 GPa) and temperatures (4,000–6,000 K) inside Uranus and Neptune, with hydrogen moving along corkscrew-like paths through a carbon lattice; this directional ion movement could affect heat and electrical transport and help explain the planets’ unusual magnetic fields.

Hidden Carbon-Hydrogen Phase May Shape Uranus and Neptune’s Interiors
space1 month ago

Hidden Carbon-Hydrogen Phase May Shape Uranus and Neptune’s Interiors

New computer simulations predict a quasi-1D superionic carbon-hydrogen phase inside Uranus and Neptune, where hydrogen atoms navigate spiral pathways through an ordered carbon lattice under 500–3,000 GPa and 4,000–6,000 K, potentially altering heat and electrical transport and helping explain the planets’ unusual magnetic fields.

Predicted Quasi-1D Carbon-Hydrogen State Inside Uranus and Neptune
science1 month ago

Predicted Quasi-1D Carbon-Hydrogen State Inside Uranus and Neptune

Scientists predict a quasi-one-dimensional superionic carbon–hydrogen phase under the extreme pressures and temperatures inside Uranus and Neptune, with hydrogen moving along helical pathways within an ordered carbon lattice. This could affect heat and electricity transport, influence magnetic field interpretation, and expand understanding of matter at high pressures relevant to planetary interiors and materials science.

Gold Becomes Reactive Under Megabar Pressures, Forms Stable Hydride
science3 months ago

Gold Becomes Reactive Under Megabar Pressures, Forms Stable Hydride

Researchers compressed gold in a hydrogen-rich environment to megabar pressures (>110 GPa) using a diamond anvil cell and, with ultrafast diffraction from the European XFEL, observed hydrogen incorporation into gold to form a stable gold hydride. The result shows gold’s noble behavior can break down under extreme planetary-core-like conditions, potentially altering models of gas giant interiors and suggesting new metallic hydride materials. The hydride persists only under high pressure; releasing pressure causes hydrogen to escape and gold to revert to its original state.

Reevaluating the Nature of Uranus and Neptune: Are They Really 'Ice Giants'?
science7 months ago

Reevaluating the Nature of Uranus and Neptune: Are They Really 'Ice Giants'?

New research suggests that Uranus and Neptune may not be 'ice giants' as previously thought, but could instead be 'rocky giants' with interiors dominated by rock rather than ice, due to limited data and a wide range of possible interior compositions. This challenges existing models of solar system formation and highlights the need for dedicated missions to better understand these planets.

"Bizarre Heat-Resistant Ice Discovered, Defying Conventional Melting Points"
science2 years ago

"Bizarre Heat-Resistant Ice Discovered, Defying Conventional Melting Points"

Scientists have discovered a new phase of superionic ice, called Ice XIX, which has a body-centered cubic structure and increased conductivity compared to its predecessor, Ice XVIII. Superionic ice is a strange form of ice that exists at extreme pressures and temperatures, such as those found in the interiors of Uranus, Neptune, and similar exoplanets. The enhanced conductivity of Ice XIX could explain the off-kilter magnetic fields observed in Uranus and Neptune, suggesting that these ice giants may have layers of superionic ice with differing conductivity, leading to the generation of multipolar magnetic fields. This discovery deepens our understanding of the unique properties of water in extreme environments and its role in shaping planetary interiors.