Stable lifetime of compact, evenly-spaced planetary systems with non-equal masses

Compact planetary systems with more than two planets can undergo orbital crossings from planet-planet perturbations. The time which the system remains stable without orbital crossings has an exponential dependence on the initial orbital separations in units of mutual Hill radii. However when a multi...

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Veröffentlicht in:	arXiv.org 2023-02
Hauptverfasser:	Rice, David R, Steffen, Jason H
Format:	Artikel
Sprache:	eng
Schlagworte:	Chains Deviation Mathematics - Dynamical Systems Motion stability Orbital resonances (celestial mechanics) Perturbation Physics - Earth and Planetary Astrophysics Planetary systems
Online-Zugang:	Volltext
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