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Inclination of Miranda as a Constraint on the Tidal Dissipation of Uranus

  • Authors: Maryame El Moutamid, Matija Ćuk

Maryame El Moutamid and Matija Ćuk 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Representative SIMPL integration for (k2,M, k2,A) = (1.0, 0.1) with QU = 600. The coupled dynamical evolution again avoids a Miranda–Ariel 5:3 resonance encounter. Instead, Umbriel becomes involved in both the Miranda–Umbriel 3:1 and Ariel–Umbriel 5:3 resonances, with the latter interaction governing the long-term evolution of the system.

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