Parametric dependence of the stationary solutions in the restricted 2 + 2 body problem

Details Parametric dependence of the stationary solutions in the restricted 2 + 2 body problem Parametric dependence of the stationary solutions in the restricted 2 + 2 body problem

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.259...77k&link_type=abstract

Astrophysics and Space Science, v. 259, Issue 1, p. 77-90 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The restricted gravitational 2 + 2 body problem, is a particular case of the N body problem and it may be used to approximate the dynamical behaviour of binary asteroids or dual sattelites moving in the gravitational field of two primaries Pi, i = 1,2. By considering oblate primaries, five parameters are needed to describe the model, namely the reduced mass μ of the primary P2, the reduced masses μ1 and μ2 of the minor bodies and the oblatenesses Ii, i = 1,2 of the primaries. This work deals with the effect of those parameters on the location of the stationary solutions.

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