Dynamics of planetary rings under thermal forces

TL;DR

This paper introduces the Eclipse-Yarkovsky effect, a thermal torque affecting planetary rings, which can explain features like Saturn's sharp inner edges and influence ring evolution and satellite formation.

Contribution

It formulates and quantifies the EY effect within a continuum framework, revealing its role in ring dynamics and long-term evolution, including edge formation and outward transport.

Findings

EY effect produces positive angular momentum flux, driving outward ring material.

Different optical depth regimes lead to distinct evolutionary pathways.

Planetary thermal radiation can exert an opposing torque, affecting ring transport.

Abstract

Planetary rings provide natural laboratories for studying the fundamental processes that govern the evolution of planetary systems. However, several key features, such as the sharp inner edges of Saturn's rings remain unresolved. In this work, we introduce and quantify the Eclipse-Yarkovsky (EY) effect, a thermal torque arising from asymmetric thermal emission of particles during planetary eclipses, which is effective for particles larger than millimeters in size. We formulate this effect within a continuum framework appropriate for collisionally coupled planetary rings and derive the continuum evolution equation that includes the EY torque and viscous diffusion (Eq.26), constraining its magnitude using ring particle spin distributions obtained from N-body simulations. We find that the EY effect systematically produces a positive angular momentum flux that could overcome the viscous torque, driving ring material outward and leading to long-term decretion. The total EY torque principally depends on the optical depth, in which we identify three dynamical regimes: dense, transitional, and tenuous regimes, each exhibiting distinct evolutionary pathways. In the dense or transition regimes, the EY torque can produce a sharp inner edge such as that of Saturn's A ring. In the tenuous regime, it can drive an entire ring outward while preserving shape. This outward transport may also facilitate satellite formation beyond the Roche limit. We also quantitatively show that planetary thermal radiation on rings exerts an opposing torque, namely planetary-Yarkovsky effect, whose importance depends on planetary emissivity and ring-particle albedo, and may lead to inward transport in Saturn's close-in rings.