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Tilting Styx and Nix but not Uranus with a Spin-Precession-Mean-motion resonance
A Hamiltonian model is constructed for the spin axis of a planet perturbed by a nearby planet with both planets in orbit about a star. We expand the planet-planet gravitational potential perturbation to first order in orbital inclinations and eccentricities, finding terms describing spin resonances...
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| Publicat a: | Celest Mech Dyn Astron |
|---|---|
| Autors principals: | , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
2018
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7485118/ https://ncbi.nlm.nih.gov/pubmed/32924029 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1007/s10569-017-9804-6 |
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