Add to ORKGThesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Science, 1972.Vita.Bibliography: 90-92.Ph.D
In the Solar System is widely accepted that most distant region of stability for prograde and retrog...
Context. Saturn’s mid-sized moons (satellites) have a puzzling orbital configuration with trapping i...
Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into ...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric and Planetary Sc...
Several examples of satellite dynamics are presented where significant progress has been made in und...
Massachusetts Institute of Technology. Dept. of Aeronautics and Astronautics. Thesis. 1969. Ph.D.MIC...
In this thesis, we study the origin and evolution of planets, rings, and moons in the context of orb...
textThe existence of the exact commensurability between the periods of rotation and revolution of a ...
Context. The stability of satellites in the solar system is affected by the so-called evection reson...
In stable solar systems, planets remain in nearly elliptical orbits around their stars. Over longe...
Astronomy and Astrophysics, 453, pp. 341-348, http://dx.doi.org./10.1051/0004-6361:20054655Internati...
International audienceThis paper discusses the effect of tides raised by Saturn on its co-orbital sa...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Earth and Planetary Sciences, 1...
Thesis. 1976. Ph.D.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Mi...
Tidal dissipation inside giant planets is important for the orbital evolution of their natural satel...
In the Solar System is widely accepted that most distant region of stability for prograde and retrog...
Context. Saturn’s mid-sized moons (satellites) have a puzzling orbital configuration with trapping i...
Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into ...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric and Planetary Sc...
Several examples of satellite dynamics are presented where significant progress has been made in und...
Massachusetts Institute of Technology. Dept. of Aeronautics and Astronautics. Thesis. 1969. Ph.D.MIC...
In this thesis, we study the origin and evolution of planets, rings, and moons in the context of orb...
textThe existence of the exact commensurability between the periods of rotation and revolution of a ...
Context. The stability of satellites in the solar system is affected by the so-called evection reson...
In stable solar systems, planets remain in nearly elliptical orbits around their stars. Over longe...
Astronomy and Astrophysics, 453, pp. 341-348, http://dx.doi.org./10.1051/0004-6361:20054655Internati...
International audienceThis paper discusses the effect of tides raised by Saturn on its co-orbital sa...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Earth and Planetary Sciences, 1...
Thesis. 1976. Ph.D.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Mi...
Tidal dissipation inside giant planets is important for the orbital evolution of their natural satel...
In the Solar System is widely accepted that most distant region of stability for prograde and retrog...
Context. Saturn’s mid-sized moons (satellites) have a puzzling orbital configuration with trapping i...
Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into ...