The Equilibrium Configurations of the Restricted Problem of 2 + 2 Triaxial Rigid Bodies

Details The Equilibrium Configurations of the Restricted Problem of 2 + 2 Triaxial Rigid Bodies The Equilibrium Configurations of the Restricted Problem of 2 + 2 Triaxial Rigid Bodies

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cemda..63...81m&link_type=abstract

Celestial Mechanics & Dynamical Astronomy, Volume 63, Issue 1, pp.81-100

Astronomy and Astrophysics

Astronomy

2

Restricted 2+2 Rigid Body Problem, Equilibrium Solutions

Scientific paper

The restricted 2+2 body problem is considered. The infinitesimal masses are replaced by triaxial rigid bodies and the equations of motion are derived in Lagrange form. Subsequently, the equilibrium solutions for the rotational and translational motion of the bodies are detected. These solutions are conveniently classified in groups according to the several combinations which are possible between the translational equilibria and the constant orientations of the bodies.

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