A parametric analysis of relative equilibrium stability in a gravitational field.

Details A parametric analysis of relative equilibrium stability in a gravitational field. A parametric analysis of relative equilibrium stability in a gravitational field.

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..664b&link_type=abstract

Kosmicheskie Issledovaniia, Tom 28, Vyp. 5, p. 664 - 675

Physics

5

Two-Body Problem: Stability, Two-Body Problem: Binaries, Two-Body Problem: Gravitational Field

Scientific paper

The problem of planar motion of a system from two gravitationally attracting bodies, one of which is a sphere, is considered. The stability of stationary motions is studied. The main point of the paper is a parametric analysis of conditions for transfer from stability to instability and/or gyroscopic stability. The results may be applied to an analysis of dynamics of double stars. A brief review of previous publications dealing with these questions is given.

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