Post-main-sequence planetary system evolution

TL;DR

This paper reviews the dynamical processes affecting planetary systems as their stars evolve beyond the main sequence, providing a theoretical foundation for interpreting observations of post-main-sequence systems.

Contribution

It offers a comprehensive review of the dynamical evolution of planetary systems during stellar post-main-sequence phases, integrating observations with theoretical models.

Findings

Diverse dynamical processes influence planetary bodies during stellar evolution.

The review aids in interpreting current and future observations of evolved planetary systems.

Provides a foundation for modeling post-main-sequence planetary system dynamics.

Abstract

The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical scrutiny. Here, I review the diverse dynamical processes which affect planets, asteroids, comets and pebbles as their parent stars evolve into giant branch, white dwarf and neutron stars. This reference provides a foundation for the interpretation and modelling of currently known systems and upcoming discoveries.