Resonances Required: Dynamical Analysis of the 24 Sex and HD 200964 Planetary Systems
Robert A. Wittenmyer, Jonathan Horner, C.G. Tinney

TL;DR
This study uses detailed dynamical simulations to demonstrate that the 24 Sextantis and HD 200964 planetary systems are only stable if their planets are in specific mean-motion resonances, explaining their current configurations.
Contribution
The paper provides the first detailed dynamical analysis showing that the observed planetary configurations are only feasible within narrow resonant stability zones.
Findings
Both systems' best-fit orbits are in narrow stable resonance zones.
Stability is highly sensitive to orbital inclination, collapsing with increased inclination.
Planets are only dynamically feasible if trapped in specific mean-motion resonances.
Abstract
We perform several suites of highly detailed dynamical simulations to investigate the architectures of the 24 Sextantis and HD 200964 planetary systems. The best fit orbital solution for the two planets in the 24 Sex system places them on orbits with periods that lie very close to 2:1 commensurability, while that for the HD 200964 system places the two planets therein in orbits whose periods lie close to a 4:3 commensurability. In both cases, the proposed best-fit orbits are mutually crossing - a scenario that is only dynamically feasible if the planets are protected from close encounters by the effects of mutual mean motion resonance. Our simulations reveal that the best fit orbits for both systems lie within narrow islands of dynamical stability, and are surrounded by much larger regions of extreme instability. As such, we show that the planets are only feasible if they are currently…
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