Add to ORKGMost of the orbital resonances among the satellites of the major planets are thought to be assembled by differential tidal expansion of their orbits. Why this has not occurred for the Uranus system can be investigated by determining the resonances which would be encountered for various values of Uranus' tidal effective Q. The comparison and the possible escape of Ariel-Umbriel from the 5:3 resonance mean that it is not unreasonable that no orbital resonances are found among these satellites
A diversity of 2:1 resonance configurations can be expected in extrasolar planetary systems, and the...
DERMOTT and Gold have proposed a resonance model for the rings of Uranus. They assume the rings are,...
We assess the multi-planet systems discovered by the Kepler satellite in terms of current ideas abou...
The orbits of the main satellites of Uranus are expected to slowly drift away owing to tides raised ...
For significant dissipation in Ariel, the past existence of an orbital resonance to force and mainta...
Several examples of satellite dynamics are presented where significant progress has been made in und...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric and Planetary Sc...
Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into ...
Satellite systems around giant planets are immersed in a region of complex resonant configurations. ...
Uranus and its complex and unexpected system of moons are still today a mystery of the solar system....
The satellites of Uranus all have significant non-zero eccentricities and in the case of Miranda a s...
Mean motion commensurabilities in multi-planet systems are an expected outcome of protoplanetary dis...
The inner moons of Jupiter and Saturn migrate outwards due to tidal energy dissipation within the pl...
The multiple-planet systems discovered by the Kepler mission show an excess of planet pairs with per...
(Abridged) A diversity of 2:1 resonance configurations can be expected in extrasolar planetary syste...
A diversity of 2:1 resonance configurations can be expected in extrasolar planetary systems, and the...
DERMOTT and Gold have proposed a resonance model for the rings of Uranus. They assume the rings are,...
We assess the multi-planet systems discovered by the Kepler satellite in terms of current ideas abou...
The orbits of the main satellites of Uranus are expected to slowly drift away owing to tides raised ...
For significant dissipation in Ariel, the past existence of an orbital resonance to force and mainta...
Several examples of satellite dynamics are presented where significant progress has been made in und...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric and Planetary Sc...
Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into ...
Satellite systems around giant planets are immersed in a region of complex resonant configurations. ...
Uranus and its complex and unexpected system of moons are still today a mystery of the solar system....
The satellites of Uranus all have significant non-zero eccentricities and in the case of Miranda a s...
Mean motion commensurabilities in multi-planet systems are an expected outcome of protoplanetary dis...
The inner moons of Jupiter and Saturn migrate outwards due to tidal energy dissipation within the pl...
The multiple-planet systems discovered by the Kepler mission show an excess of planet pairs with per...
(Abridged) A diversity of 2:1 resonance configurations can be expected in extrasolar planetary syste...
A diversity of 2:1 resonance configurations can be expected in extrasolar planetary systems, and the...
DERMOTT and Gold have proposed a resonance model for the rings of Uranus. They assume the rings are,...
We assess the multi-planet systems discovered by the Kepler satellite in terms of current ideas abou...