Quantification of Tides in Giant Planets from Observations
Val\'ery Lainey, Marco Zannoni, Vincent Robert, Tristan Guillot

TL;DR
This paper reviews recent advances in quantifying tidal effects on giant planets, highlighting measurements from the Cassini mission and discussing implications for both Solar System and exoplanet systems.
Contribution
It summarizes measurement techniques and results for Saturn's tidal parameters and discusses their extrapolation to other giant planets and exoplanets.
Findings
Measurements of Saturn's Love number and Q factor at different frequencies.
Summary of methods used to quantify tidal effects.
Discussion of tidal effects in exoplanet systems.
Abstract
Quantifying tidal effects on giant planets has recently made significant advances, thanks in particular to the Cassini space probe. During its thirteen-year orbit around Saturn, numerous measurements from different instruments made it possible to characterize fundamental parameters such as Saturn\'s Love number and quality factor at different frequencies. In this article, we summarize the various measurements and methods that have allowed to arrive at such a result, as well as the extrapolations that can be deduced for other systems. More generally, the state of the art concerning the four giant planets of the Solar System is presented, as well as the case of exoplanets.
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.
Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
