Unexpected Near-Resonant and Metastable States of Young Multi-Planet Systems

TL;DR

This study examines the dynamical states of young multi-planet systems, revealing most are near resonance with circulating angles, making them prone to chaos and potential instability, thus shedding light on early planetary evolution.

Contribution

It provides new insights into the near-resonant and metastable states of young multi-planet systems, highlighting their susceptibility to chaos and transitional dynamical phases.

Findings

Most planet pairs are near resonance with circulating angles.

Young systems are more susceptible to dynamical chaos.

Eccentricities of 0.04 to 0.08 can lead to instability.

Abstract

Recent observations suggest that the incidence of near-resonant planets declines as planetary systems age, making young planetary systems key signposts of early dynamical evolution. Here we investigate the dynamical states of three of the youngest multi-transiting planetary systems: AU Mic (3-planet, $\sim$20-Myr-old), V1298 Tau (4-planet, $\sim$23-Myr-old), and TOI-2076 (4-planet, $\sim$200-Myr-old). We find that most planet pairs in these systems lie near resonance with circulating rather than librating resonant angles. As a result, they are more susceptible to dynamical chaos than systems that are either securely locked in resonance or far removed from it. Even modest eccentricities of 0.04 to 0.08 may drive them to instability on timescales of tens to hundreds of Myr. Moreover, the observed orbital architectures are vulnerable to eccentricity excitation through mechanisms such as divergent resonance crossing triggered by planetesimal scattering. The observed near-resonant state may represent a transitional phase between a librating resonant chains and a mature non-resonant planetary system. Finally, we briefly discuss mechanisms that could give rise to the observed near-resonant configurations, including overstable libration, disk turbulence, and receding disk inner edge.