On the planar motion in the full two-body problem with inertial symmetry
Relative motion of binary asteroids, modeled as the full two-body planar problem, is studied, taking into account the shape and mass distribution of the bodies. Using the Lagrangian approach, the equations governing the motion are derived. The resulting system of four equations is nonlinear and coup...
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Veröffentlicht in: | Celestial mechanics and dynamical astronomy 2013-11, Vol.117 (3), p.263-277 |
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Format: | Artikel |
Sprache: | eng |
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