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Journal Title

Title of Journal: Celestial Mech Dyn Astr

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Abbravation: Celestial Mechanics and Dynamical Astronomy

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Kluwer Academic Publishers

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DOI

10.1007/s12206-013-0525-9

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ISSN

1572-9478

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Dynamics of two satellites in the 2/1 Mean–Motion

Authors: N Callegari T Yokoyama
Publish Date: 2007/04/05
Volume: 98, Issue: 1, Pages: 5-30
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Abstract

The dynamics of a pair of satellites similar to Enceladus–Dione is investigated with a twodegreesoffreedom model written in the domain of the planar general threebody problem Using surfaces of section and spectral analysis methods we study the phase space of the system in terms of several parameters including the most recent data A detailed study of the main possible regimes of motion is presented and in particular we show that besides the two separated resonances the phase space is replete of secondary resonances

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Other Papers In This Journal:
  1. A note on the dynamics around the Lagrange collinear points of the Earth–Moon system in a complete Solar System model
  2. Universal unfolding of symmetric resonances
  3. A sixth-order accurate scheme for solving two-point boundary value problems in astrodynamics
  4. Single lunation N -observation orbits
  5. Explicit algorithmic regularization in the few-body problem for velocity-dependent perturbations
  6. Tidal friction in close-in satellites and exoplanets: The Darwin theory re-visited
  7. Spacecraft trajectories to the L 3 point of the Sun–Earth three-body problem
  8. The local standard of rest and the well in the velocity distribution
  9. Three-dimensional multi-tethered satellite formation with the elements moving along Lissajous curves
  10. Analysis of the Chaotic Behaviour of Orbits Diffusing along the Arnold Web
  11. Analytic estimates and topological properties of the weak stability boundary
  12. On constructing the general Earth’s rotation theory
  13. Secular tidal changes in lunar orbit and Earth rotation
  14. Bifurcating families around collinear libration points
  15. Sensitivity of the orbital content of a model stellar system to the potential approximation used to describe it
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