Layered convection as the origin of Saturn's luminosity anomaly
J\'er\'emy Leconte, Gilles Chabrier

TL;DR
This paper proposes that layered convection within Saturn's interior, caused by compositional gradients, can explain its unexpectedly high luminosity without additional energy sources, challenging traditional models of giant planet interiors.
Contribution
It introduces planetary evolution models showing layered convection as a key factor in Saturn's luminosity, revising the standard homogeneous interior paradigm.
Findings
Layered convection reduces Saturn's cooling rate.
It can account for Saturn's observed luminosity without extra energy.
Implications for understanding exoplanet radii.
Abstract
As they keep cooling and contracting, Solar System giant planets radiate more energy than they receive from the Sun. Applying the first and second principles of thermodynamics, one can determine their cooling rate, luminosity, and temperature at a given age. Measurements of Saturn's infrared intrinsic luminosity, however, reveal that this planet is significantly brighter than predicted for its age. This excess luminosity is usually attributed to the immiscibility of helium in the hydrogen-rich envelope, leading to "rains" of helium-rich droplets. Existing evolution calculations, however, suggest that the energy released by this sedimentation process may not be sufficient to resolve the puzzle. Here, we demonstrate using planetary evolution models that the presence of layered convection in Saturn's interior, generated, like in some parts of Earth oceans, by the presence of a…
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.
