Tidal evolution of the Uranian satellites: I. Passage of Ariel and Umbriel through the 5:3 mean-motion commensurability
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Cited by (70)
Early impact chronology of the icy regular satellites of the outer solar system
2021, IcarusCitation Excerpt :Wong et al. (2019) did not study the Saturnian satellites because there are many controversies about the tidal evolution of that system (e.g., Lainey et al. 2012, 2020; Meyer and Wisdom 2008), the interior evolution of the satellites (e.g., Neveu and Rhoden 2017, 2019), their origin (e.g., Charnoz et al. 2011; Crida and Charnoz 2010; Ćuk et al. 2016) and their crater surface ages (e.g., Zahnle et al. 2003; Kirchoff and Schenk 2010; Kirchoff and Marchi 2019). In contrast, the evolution of the Jovian and Uranian systems appear more straightforward (e.g., Tittemore and Wisdom 1988, 1989, 1990) and Callisto, Umbriel, Titania and Oberon appear to have undergone little resurfacing which makes tying their crater densities to their ages easier (Zahnle et al. 1998, 2003). We also include the irregular satellites as a source of impacts.
Elastic thickness and heat flux estimates for the uranian satellite Ariel
2015, IcarusCitation Excerpt :The present-day uranian system differs from the Galilean and saturnian systems in that none of its satellites are currently in stable orbital resonances. Past papers on Ariel have investigated potential mean motion resonance configurations with the other satellites to isolate a heat source that could explain the inferred resurfacing (Dermott et al., 1988; Tittemore and Wisdom, 1989; Tittemore, 1990). However, below we conclude that neither Ariel’s present eccentricity, nor radioactive heating, nor any of the previously calculated ancient resonances (2:1 with Umbriel, 5:3 with Miranda, or 4:1 with Titania) are sufficient to explain the inferred heat fluxes.
Geology before Pluto: Pre-encounter considerations
2015, IcarusCitation Excerpt :No preferred orientations for the resulting rifts and graben are predicted, and an absence of an organized pattern could be taken as circumstantial evidence for ocean freezing. The tectonic evidence may not be as spectacular as that found on Ariel (Fig. 19), a satellite that may have been tidally heated during resonance passage (Tittemore and Wisdom, 1988), but it should still be notable. In Charon’s case, even without an ocean, extensional tectonics may also prevail; global cooling of a solid body produces a radius decrease, but the thermoelastic contraction of the icy lithosphere is generally more important (Hillier and Squyres, 1991).
Dynamical Interactions and Mass Loss within the Uranian System
2023, Planetary Science Journal