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New models rethink the insides of Uranus and Neptune — Level B2 — a tent in the snow with mountains in the background

New models rethink the insides of Uranus and NeptuneCEFR B2

15 Dec 2025

Adapted from U. Zurich, Futurity CC BY 4.0

Photo by ruedi häberli, Unsplash

Level B2 – Upper-intermediate
5 min
277 words

Scientists at the University of Zurich have presented a new numerical framework that challenges the traditional view of Uranus and Neptune as clearly "ice-rich" worlds. Led by PhD student Luca Morf and initiated by professor Ravit Helled, the team combined physics-based and empirical approaches to produce interior models that are both physically consistent and deliberately "agnostic" about prior assumptions.

The method begins with a random density profile for a planet's interior. For each profile the team computes the gravitational field that best matches observational data, then infers a compatible composition. They repeat this cycle many times and retain solutions that fit the observations. The resulting range of models shows the two blue planets need not be dominated by ice (usually represented by water); some solutions are rock-rich while others are water-rich. Helled notes the idea was first suggested nearly 15 years ago, and the new framework can now demonstrate it numerically.

The study also offers a plausible account of the planets' unusual magnetic fields. The models include so-called "ionic water" layers that generate magnetic dynamos in positions that explain the observed non-dipolar, multi-pole fields. The team finds that Uranus' magnetic field originates deeper than Neptune's. However, uncertainty about how materials behave under the extreme pressures and temperatures inside these planets could affect the conclusions. The authors say current data cannot distinguish the models and call for dedicated missions to Uranus and Neptune to reveal their true nature. The research appears in Astronomy & Astrophysics; source: University of Zurich.

  • New modelling combines physics and empirical data.
  • Interiors could be rock-rich or water-rich.
  • Models help explain non-dipolar magnetic fields.

Difficult words

  • frameworka system of methods and ideas used
  • agnosticnot committed to one belief or assumption
  • densityamount of mass per unit volume
  • gravitational fieldregion where gravity affects objects around a body
  • compositionthe substances or materials that form something
  • ionic waterwater in a charged, electrically conducting state
  • dynamoa mechanism that generates a magnetic field
    dynamos
  • distinguishto recognize or show a difference between things

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Discussion questions

  • Why do the authors call for dedicated missions to Uranus and Neptune, and what could such missions reveal?
  • How might uncertainty about material behaviour at extreme pressures and temperatures change the study's conclusions?
  • If you planned a mission to test these interior models, which measurements would you prioritise and why?

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