Celestial Mechanics and Dynamical Astronomy

, Volume 88, Issue 3, pp 245–257 | Cite as

Special Families of Orbits in the Direct Problem of Dynamics

  • M.-C. Anisiu
  • C. Blaga
  • G. Bozis


The direct problem of dynamics in two dimensions is modeled by a nonlinear second-order partial differential equation, which is therefore difficult to be solved. The task may be made easier by adding some constraints on the unknown function γ = f y /f x , where f(x, y) = c is the monoparametric family of orbits traced in the xy Cartesian plane by a material point of unit mass, under the action of a given potential V(x, y). If the function γ is supposed to verify a linear first-order partial differential equation, for potentials V satisfying a differential condition, γ can be found as a common solution of certain polynomial equations.

The various situations which can appear are discussed and are then illustrated by some examples, for which the energy on the members of the family, as well as the region where the motion takes place, are determined. One example is dedicated to a Hénon—Heiles type potential, while another one gives rise to families of isothermal curves (a special case of orthogonal families). The connection between the inverse/direct problem of dynamics and the possibility of detecting integrability of a given potential is briefly discussed.

integrability inverse and direct problem of dynamics special families of orbits 


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Copyright information

© Kluwer Academic Publishers 2004

Authors and Affiliations

  • M.-C. Anisiu
    • 1
  • C. Blaga
    • 2
  • G. Bozis
    • 3
  1. 1.T. Popoviciu Institute of Numerical AnalysisRomanian AcademyCluj-NapocaRomania
  2. 2.Faculty of Mathematics and Computer ScienceBabes-Bolyai UniversityCluj-NapocaRomania
  3. 3.Department of PhysicsAristotle University of ThessalonikiThessalonikiGreece

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