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20232026
most citedDynamical evolution of the Uranian satellite system II. Crossing of the 5/3 Ariel-Umbriel mean motion resonance

6 citations · 18 across the 7 of their papers we have counts for

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astro-ph.EP2026

CHEOPS observations of V1298 Tau: updated planetary densities and implications on the early evolution of the young system

Hinna Shivkumar, Sérgio Gomes, Jean-Michel Désert +9

The young (10-30 Myr) multi-planet system V1298 Tau presents a unique opportunity to probe the early formation and evolution of young systems. We present new CHEOPS observations of…

astro-ph.EP2026

Dynamical evolution of the Uranian satellite system III. The passage through the7/4 MMR between Miranda and Ariel

Sérgio R. A. Gomes, Tibi Keizer

The passage through the mean-motion resonance between Ariel and Umbriel, two of Uranus's largest moons, still raises several open questions. Previous studies suggest that, in…

astro-ph.EP2025

Capture and escape from the 2:1 resonance between Ariel and Umbriel in a fast-migration scenario of the Uranian system

M. Rossi, G. Lari, M. Falletta +3

Recent measurements suggest that Uranus may exhibit a higher tidal dissipation than previously assumed. This enhanced dissipation leads to a faster orbital migration of its five ma…

astro-ph.EP2024★ 6 cited

Dynamical evolution of the Uranian satellite system II. Crossing of the 5/3 Ariel-Umbriel mean motion resonance

Sérgio R. A. Gomes, Alexandre C. M. Correia

At present, the main satellites of Uranus are not involved in any low order mean motion resonance (MMR). However, owing to tides raised in the planet, Ariel and Umbriel most likely…

astro-ph.EP2024★ 6 cited

Dynamical evolution of the Uranian satellite system I. From the 5/3 Ariel-Umbriel mean motion resonance to the present

Sérgio R. A. Gomes, Alexandre C. M. Correia

Mutual gravitational interactions between the five major Uranian satellites raise small quasi-periodic fluctuations on their orbital elements. At the same time, tidal interactions…

astro-ph.EP2023★ 1 cited

Stability maps for the 5/3 mean motion resonance between Ariel and Umbriel with inclination

Sérgio R. A. Gomes, Alexandre C. M. Correia

The evolution of the five largest satellites of Uranus during the crossing of the 5/3 mean motion resonance between Ariel and Umbriel is strongly affected by chaotic motion. Studie…

astro-ph.EP2023★ 5 cited

Effect of the inclination in the passage through the 5/3 mean motion resonance between Ariel and Umbriel

Sérgio R. A. Gomes, Alexandre C. M. Correia

The orbits of the main satellites of Uranus are expected to slowly drift away owing to tides raised in the planet. As a result, the 5/3 mean motion resonance between Ariel and Umbr…