Tag

Ice Giants

All articles tagged with #ice giants

New Model Recasts Uranus and Neptune as Magma-Ocean Giants
space-and-spaceflight18 days ago

New Model Recasts Uranus and Neptune as Magma-Ocean Giants

A UC-led study proposes Uranus and Neptune may harbor well-mixed magma oceans with dissolved hydrogen beneath a hydrogen-dominated envelope, suggesting they’re magma-ocean giants rather than ice giants and potentially explaining their densities. The model, submitted to The Astrophysical Journal, challenges the traditional three-layer interior picture and could inform the study of sub-Neptune exoplanets, though the idea remains under debate without a dedicated mission to these distant planets.

New Study Hints Uranus and Neptune Hide Magma Oceans, Not Ice
space18 days ago

New Study Hints Uranus and Neptune Hide Magma Oceans, Not Ice

A UCLA-led study using computer models proposes that Uranus and Neptune may have interior magma oceans rather than icy mantles, with a layered structure of a hydrogen/helium atmosphere, a boundary layer containing H/He/Mg/SiO/O, and a bottom magma ocean of silicate and iron. This challenges the long-standing “ice giants” label and has implications for understanding similar sub-Neptune exoplanets, while noting proposed future missions (Uranus Orbiter and Probe, Neptune Odyssey) and ongoing interest in these worlds.

Two Lost Ice Giants May Have Shaped the Early Solar System
space1 month ago

Two Lost Ice Giants May Have Shaped the Early Solar System

A new study based on 122 simulations suggests the early outer solar system may have hosted two additional ice-giant planets with masses between Earth and Neptune that were later ejected. Depending on whether the system started with five or six giants, Jupiter’s moons remained stable in the presence of two extra ice giants, while Uranus’s moons stayed stable with only one extra; Miranda’s ice content hints at past moon collisions. The findings imply a far bardziej crowded infancy for the solar system than previously thought, and the team notes further simulations are needed to pin down the exact number and masses of the missing planets. The work was published online in Icarus (2026).

Rocks in the Ice Giants? Uranus and Neptune May Be More Rocky Than Thought
space2 months ago

Rocks in the Ice Giants? Uranus and Neptune May Be More Rocky Than Thought

A new Astronomy & Astrophysics study models Uranus and Neptune and finds their outer shells may be composed largely of rocks rather than being purely icy, implying their atmospheres could be littered with rocky material and suggesting a possible reclassification from “ice giants” to a term like “minor giants,” though the authors caution this isn’t definitive.

A Quasi-1D Superionic Phase Could Lurk Inside Uranus and Neptune
science2 months ago

A Quasi-1D Superionic Phase Could Lurk Inside Uranus and Neptune

Researchers using first-principles simulations predict a new quasi-1D superionic phase in a carbon–hydrogen compound that could exist inside ice giants Uranus and Neptune at extreme pressures and temperatures. In this phase, hydrogen diffuses along a carbon lattice that forms a helical structure, producing anisotropic heat and electrical conduction. This could influence our understanding of the planets’ unusual magnetic fields and guides how such materials might behave under the extreme conditions found in their interiors.

Reevaluating Uranus and Neptune: Are They Really Ice Giants?
science6 months ago

Reevaluating Uranus and Neptune: Are They Really Ice Giants?

A new computational model suggests that Uranus and Neptune may have rockier interiors than previously thought, challenging the traditional classification of these planets as 'ice giants' and potentially explaining their complex magnetic fields. The study combines physics-based and observational data to propose that their cores contain significant rock content, which could influence their magnetic properties. Further research and dedicated space missions are needed to confirm these findings.

Reevaluating the Nature of Uranus and Neptune: Are They Really 'Ice Giants'?
science9 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.

Exploring Uranus: Insights from the KISS Workshop
science1 year ago

Exploring Uranus: Insights from the KISS Workshop

NASA's proposed Uranus Orbiter and Probe (UOP) mission aims to explore Uranus and its moons, marking it as a top priority for 2023-2032. The mission seeks to enhance understanding of ice giants, focusing on Uranus' interior, atmosphere, rings, and moons. This exploration could provide transformative insights into planetary formation and evolution, potentially influencing our knowledge of exoplanets. The mission also considers the astrobiological potential of Uranus' moons, which may harbor liquid oceans beneath their surfaces.

"Uranus Unveils Unexpected Gas Composition"
science2 years ago

"Uranus Unveils Unexpected Gas Composition"

New research suggests Uranus may contain significantly more methane than previously thought, challenging existing models of its composition. Scientists propose that organic-rich materials in the outer solar system could have triggered chemical reactions during the planet's formation, leading to higher methane levels. Further observations are needed to confirm these findings and refine our understanding of Uranus and Neptune.

"Revealing the Surprising Composition of Uranus and Neptune"
astronomy2 years ago

"Revealing the Surprising Composition of Uranus and Neptune"

A new study suggests that Uranus and Neptune may contain tons of methane ice in addition to frozen water, challenging previous beliefs about their composition. The findings could help solve the puzzle of how these icy worlds formed, as they coalesced from planetesimals rich in carbon. The study's authors built models of the planets' interiors and found that those with methane fit their criteria, with the methane forming a thick layer between the hydrogen-helium envelope and the water layer. This discovery could provide greater insight into these little-understood planets, although confirming their methane content would be challenging and may require future space missions.