Jupiter and Saturn: a new theoretical model of giant magnetospheres

News

3 April 2024

The giant planets in our Solar System are extremely complex systems. They are first characterized by their intense magnetic field, which creates a magnetic cavity, the magnetosphere, protecting their direct surroundings against solar wind and extending to tens of planetary radii. In addition, their fast rotation, with a period of approximately 9 to 10h (compared to 24h at Earth), induces a strong forcing in the magnetosphere. In the regions closest to the planet, (cryo-)volcanic moons, Enceladus at Saturn and Io at Jupiter, continuously inject gas and plasma in the system. This plasma is picked up by the magnetic field and strongly accelerated by the planetary rotation. It is transported outwards, resulting in a feedback onto the gas giant in the form of field-aligned current loops.

How exactly does this plasma transport in the system occur, knowing that, according to physical principles, it must conserve mass, energy and momentum ? A study carried out by a young PhD student at IRAP, based on fundamental magneto-hydrodynamic laws, resulted in a theoretical model describing this phenomenon in its full complexity. Published in the Journal of Geophysical Research, this work shows that, considering only the global movement of plasma, it can be understood simply as… a competition between various rotation resistances !

Schematic view of the Jovian system. The moon Io expells gas in the form of a torus around Jupiter. This gas is then ionized and picked-up by the magnetic field, rotating with the planet. It is transported outwards and forms a disk. Part of the plasma escapes along field lines towards the planet, resulting in field-aligned current loops.

Rather general, this model could apply to the understanding of finer dynamical processes taking place in the gas giant magnetospheres, with always greater precision and complexity. It is the first model able to take into account most of the observed asymetries in the fast rotating magnetospheres. It will enable the analysis of data from probes orbiting in those systems : “retired” Cassini (Saturn) and Galileo (Jupiter), active Juno (Jupiter) and soon JUICE and Europa Clipper, which will provide a two observers’ view of the Jovian magnetosphere from 2031.

Further Resources

  • Publication : Devinat, M., Blanc, M., & André, N. (2024). A self-consistent model of radial transport in the magnetodisks of gas giants including interhemispheric asymmetries. Journal of Geophysical Research: Space Physics, 129, e2023JA032233. https://doi.org/10.1029/2023JA032233

IRAP Contacts

More news

ESO signs agreement for MOSAIC instrument on the ELT

Today, ESO has signed an agreement with a large international consortium for the design and construction of the Multi-Object Spectrograph (MOSAIC), an instrument for ESO’s Extremely Large Telescope (ELT). Able […]

Electric discharges detected on Mars for the first time

Electric discharges have for the first time been recorded within the storms and whirlwinds of dust – known as dust devils – that sweep across the surface of Mars. Captured […]

MACIV nodes: an exceptional seismological network on the volcanoes of the Massif Central

As part of the MACIV project, funded by the French National Research Agency (ANR), a team of scientists deployed the largest mobile seismological network ever installed by a university team […]

Search