Lyapunov times are a measure of the stability of dynamical systems, specifically indicating the time it takes for nearby trajectories in phase space to diverge or converge. In the context of multiplanet systems, Lyapunov times help assess the long-term stability of planetary orbits, reflecting how small changes in initial conditions can lead to vastly different outcomes over time. Understanding these times is crucial for predicting whether a system will remain stable over astronomical time scales.
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