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Evolution of Saturn’s Mid-Sized Moons
The orbits of Saturn’s inner mid-sized moons (Mimas, Enceladus, Tethys, Dione, and Rhea) have been notably difficult to reconcile with their geology. Here, we present numerical simulations coupling thermal, geophysical, and simplified orbital evolution for 4.5 billion years that reproduce observed c...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
2019
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6662725/ https://www.ncbi.nlm.nih.gov/pubmed/31360776 http://dx.doi.org/10.1038/s41550-019-0726-y |