Archaeology / Cultural Heritage / History

[Archaeology] [twocolumns]

Anthropology / Human Evolution / Linguistics

[Anthropology] [twocolumns]

Palaeontology / Palaeoclimate / Earth Sciences

[Palaeontology] [twocolumns]

Evolution / Genetics / Biology


Two strange planets: Neptune and Uranus

Uranus and Neptune both have a completely skewed magnetic field, perhaps due to the planets' special inner structures. But new experiments by ETH Zurich researchers now show that the mystery remains unsolved.

Two strange planets: Neptune and Uranus
Neptune and Uranus are the outermost two planets of our solar system
and two gas giants [Credit: NASA]

The two large gas planets Uranus and Neptune have strange magnetic fields. These are each strongly tilted relative to the planet's rotation axes and are significantly offset from the physical center of the planet. The reason for this has been a longstanding mystery in planetary sciences. 

Various theories assume that a unique inner structure of these planets could be responsible for this bizarre phenomenon. According to these theories, the skewed magnetic field is caused by circulations in a convective layer, which consists of an electrically conductive fluid. This convective layer in turn surrounds a stably layered, non-convective layer in which there is no circulation of the material due to its high viscosity and thus no contribution to the magnetic field.

Extraordinary states

Computer simulations show that water and ammonia, the main components of Uranus and Neptune, enter an unusual state at very high pressures and temperatures: a "superionic state," which has the properties of both a solid and a liquid. In this state, the hydrogen ions become mobile within the lattice structure formed by oxygen or nitrogen.

Two strange planets: Neptune and Uranus
The magnetic fields of Earth, Uranus and Neptune differ markedly
[Credit: ETH Zurich/T. Kimura]

Recent experimental studies confirm that superionic water can exist at the depth where, according to theory, the stably layered region is located. It could therefore be that the stratified layer is formed by superionic components. However, it is unclear whether the components are actually able to suppress convection, since the physical properties of the superionic state are not known.

High pressure in the smallest space

Tomoaki Kimura and Motohiko Murakami from the Department of Earth Sciences at ETH Zurich are now one step closer to finding the answer. The two researchers have conducted high-pressure and high-temperature experiments with ammonia in their laboratory. The aim of the experiments was to determine the elasticity of the superionic material. Elasticity is one of the most important physical properties that influences thermal convection in the planetary mantle. It is remarkable that the elasticity of the materials in their solid and liquid states is completely different.

Two strange planets: Neptune and Uranus
This is what the inner structure of the two gas planets could look like,
according to previous theories [Credit: ETH Zurich/T. Kimura]

For their investigations, the researchers used a high-pressure apparatus called a diamond anvil cell. In this apparatus, the ammonia is placed in a small container with a diameter of about 100 micrometers, which is then clamped between two diamond tips that compress the sample. This makes it possible to subject materials to extremely high pressures, such as those found inside Uranus and Neptune.

The sample is then heated to over 2,000 degrees Celsius with an infrared laser. At the same time, a green laser beam illuminates the sample. By measuring the wave spectrum of the scattered green laser light, the researchers can determine the elasticity of the material and the chemical bonding in the ammonia. The shifts in the wave spectrum at different pressures and temperatures can be used to determine the elasticity of ammonia at different depths.

A new phase discovered

In their measurements, Kimura and Murakami have discovered a new superionic ammonia phase (γ phase) that exhibits an elasticity similar to that of the liquid phase. This new phase may be stable in the deep interior of Uranus and Neptune and therefore occur there. However, the superionic ammonia behaves like a liquid and thus it would not be viscous enough to contribute to the formation of the non-convective layer.

Two strange planets: Neptune and Uranus
Schematic representation of the diamond anvil cell. The chemical structure can be determined with
the Raman spectrum, and the elasticity of the sample material with Brillouin scattering
[Credit: ETH Zurich/T. Kimura]

The question of what properties the superionic water has inside Uranus and Neptune is all the more urgent in light of the new results. For even now, the mystery of why the two planets have such an irregular magnetic field still remains unsolved.

The findings are published in Proceedings of the National Academy of Sciences.

Author: Felix Würsten | Source: ETH Zurich [March 31, 2021]

Support The Archaeology News Network with a small donation!


Post A Comment
  • Blogger Comment using Blogger
  • Facebook Comment using Facebook
  • Disqus Comment using Disqus

No comments :

Exhibitions / Travel

[Exhibitions] [bsummary]

Natural Heritage / Environment / Wildlife

[Natural Heritage] [list]

Astronomy / Astrobiology / Space Exploration

[Universe] [list]