Replacing an irregular body by an equal-mass binary dumbbell converts its spin-orbit resonances into surrogate mean-motion resonances; for Quaoar the resulting maps show SORs play no relevant role in present ring dynamics.
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4 Pith papers cite this work, alongside 424 external citations. Polarity classification is still indexing.
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Pith papers citing it
424
external citations · OpenAlex
years
2026 4representative citing papers
A Hamiltonian framework maps coupled spin-orbit, spin-spin, and doubly synchronous resonances in ellipsoid binary asteroids and identifies a secondary resonance from nonlinear coupling between primary and secondary synchronous modes.
A central, velocity-dependent dissipative force preserves angular momentum and, at exponent d=3, turns planar central-configuration motion into a dissipative Kepler problem with no averaged apsidal precession.
Resolves six speculative companions into one giant planet, one eccentric brown dwarf, two low-mass stars, and two stars with no detectable companions.
citing papers explorer
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A circumbinary approach to the study of spin-orbit resonances around irregular shaped bodies. Application to the Quaoar system
Replacing an irregular body by an equal-mass binary dumbbell converts its spin-orbit resonances into surrogate mean-motion resonances; for Quaoar the resulting maps show SORs play no relevant role in present ring dynamics.
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Resonant Networks of Spin-Orbit Coupling in Ellipsoid-Ellipsoid Binary Asteroid Systems
A Hamiltonian framework maps coupled spin-orbit, spin-spin, and doubly synchronous resonances in ellipsoid binary asteroids and identifies a secondary resonance from nonlinear coupling between primary and secondary synchronous modes.
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An angular-momentum preserving dissipative model for the point-mass N -body problem
A central, velocity-dependent dissipative force preserves angular momentum and, at exponent d=3, turns planar central-configuration motion into a dissipative Kepler problem with no averaged apsidal precession.
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The Pan-Pacific Planet Search -- IX. A menagerie of companions orbiting evolved stars
Resolves six speculative companions into one giant planet, one eccentric brown dwarf, two low-mass stars, and two stars with no detectable companions.