N-body simulations show proposed exomoons around Kepler-1625, Kepler-1708, and HD 23079 are mostly orbitally stable, while submoons destabilize above about 40 degrees inclination and show a secular 13:2 precession resonance feature.
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Orbital Stability of Hierarchical 3 and 4-Body Systems with Inclination: Results for Kepler-1625, 1708, and HD 23079
N-body simulations show proposed exomoons around Kepler-1625, Kepler-1708, and HD 23079 are mostly orbitally stable, while submoons destabilize above about 40 degrees inclination and show a secular 13:2 precession resonance feature.