The equilibria of the translational-rotational motion of two gyrostats in a Newtonian central field of forces

Details The equilibria of the translational-rotational motion of two gyrostats in a Newtonian central field of forces The equilibria of the translational-rotational motion of two gyrostats in a Newtonian central field of forces

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.196..125m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 196, no. 1, p. 125-142.

Astronomy and Astrophysics

Astrophysics

2

Equilibrium Equations, Newton Theory, Rotary Gyroscopes, Translational Motion, Two Body Problem, Artificial Satellites, Equations Of Motion, Three Body Problem

Scientific paper

A system consisting of two gyrostats moving in the field of a massive attracting body is considered theoretically to determine the equilibrium positions of the translational-rotational motion. The equilibria are determined and grouped in collinear and equilateral equilibria relative to the attracting body's Newtonian field of forces. The Routh-Hurwitz criterion is used to determine the stability of all equilibrium configurations.

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