Seismology of Giant Planets
Patrick Gaulme, Benoit Mosser, Francois-Xavier Schmider, Tristan, Guillot, Jason Jackiewicz

TL;DR
Seismology of giant planets offers a promising way to uncover their internal structures and compositions, utilizing techniques adapted from helioseismology and new methods like ring seismology, with recent observational advances fueling ongoing research.
Contribution
This paper reviews the potential of seismology to study giant planets, discussing methods, recent results, and future prospects in planetary interior research.
Findings
Detection of Jupiter's acoustic oscillations with SYMPA.
Indirect detection of Saturn's f-modes in its rings.
Development of new ground-based and space instruments for planetary seismology.
Abstract
Seismology applied to giant planets could drastically change our understanding of their deep interiors, as it has happened with the Earth, the Sun, and many main-sequence and evolved stars. The study of giant planets' composition is important for understanding both the mechanisms enabling their formation and the origins of planetary systems, in particular our own. Unfortunately, its determination is complicated by the fact that their interior is thought not to be homogeneous, so that spectroscopic determinations of atmospheric abundances are probably not representative of the planet as a whole. Instead, the determination of their composition and structure must rely on indirect measurements and interior models. Giant planets are mostly fluid and convective, which makes their seismology much closer to that of solar-like stars than that of terrestrial planets. Hence, helioseismology…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
