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Exploring S-type orbits in the Pluto-Charon binary system
(Wiley-Blackwell, 2010-05-01)
This work generates, through a sample of numerical simulations of the restricted three-body problem, diagrams of semimajor axis and eccentricity which defines stable and unstable zones for particles in S-type orbits around ...
Exploring S-type orbits in the Pluto-Charon binary system
(Wiley-Blackwell, 2010-05-01)
This work generates, through a sample of numerical simulations of the restricted three-body problem, diagrams of semimajor axis and eccentricity which defines stable and unstable zones for particles in S-type orbits around ...
Why isn't Pluto a planet anymore?
(Youtube, 2011)
Why isn't Pluto a planet anymore?
(Youtube, 2016)
Small particles in Pluto's environment: Effects of the solar radiation pressure
(2013-05-02)
Impacts of micrometeoroids on the surfaces of the plutonian small satellites Nix and Hydra can generate dust particles. Even in this region so far from the Sun these tiny ejected particles are under the effects of the solar ...
Small particles in Pluto's environment: Effects of the solar radiation pressure
(2013-05-02)
Impacts of micrometeoroids on the surfaces of the plutonian small satellites Nix and Hydra can generate dust particles. Even in this region so far from the Sun these tiny ejected particles are under the effects of the solar ...
Stable regions around Pluto
(2013-05-02)
In a previous work, GiuliattiWinter et al. found several stable regions for test particles in orbit around Pluto associated with families of periodic orbits obtained in the circular, restricted three-body problem. They ...
A peculiar stable region around Pluto
(Oxford University Press, 2014-04-01)
Giuliatti Winter et al. found several stable regions for a sample of test particles located between the orbits of Pluto and Charon. One peculiar stable region in the space of the initial orbital elements is located at a = ...