4.6 Article

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

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ASTRONOMY & ASTROPHYSICS
卷 674, 期 -, 页码 -

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EDP SCIENCES S A
DOI: 10.1051/0004-6361/202346101

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celestial mechanics; planets and satellites: dynamical evolution and stability planets; and satellites: individual: Uranus; planets and satellites: individual: Ariel; planets and satellites: individual: Umbriel

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The orbits of Uranus' main satellites are expected to drift away gradually due to tides raised in the planet. The 5/3 mean motion resonance between Ariel and Umbriel was likely encountered in the past, and it has been challenging to explain why the eccentricities of the satellites must be larger than 0.01 to prevent entrapment in this resonance. Additionally, if the satellites experience temporary capture and escape, their inclinations rise to high values that are not observed today. Revisiting this problem, a study using a circular two-satellite model focused on inclination, showing that with an inclination of around 0.15 degrees at the time of the 5/3 resonance encounter, capture can be avoided in about 60% of cases.
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 Umbriel was likely encountered in the past. Previous studies have shown that, in order to prevent entrapment in this resonance, the eccentricities of the satellites must be larger than similar to 0.01 at the epoch, which is hard to explain. On the other hand, if the satellites experience some temporary capture and then escape, the inclinations rise to high values that are not observed today. We have revisited this problem both analytically and numerically focussing on the inclination, using a secular two-satellite model with circular orbits. We show that if the inclination of Umbriel was around 0.15 degrees at the time of the 5/3 resonance encounter, capture can be avoided in about 60% of the cases. Moreover, after the resonance crossing, the inclination of Umbriel drops to a mean value around 0.08 degrees, which is close to the presently observed one. The final inclination of Ariel is distributed between 0.01 degrees and 0.25 degrees with a nearly equal probability, which includes the present mean value of 0.02 degrees.

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