Non-Linear Stability Zones around Triangular Equilibria in the Plane Circular Restricted Three-Body Problem with Oblateness

Details Non-Linear Stability Zones around Triangular Equilibria in the Plane Circular Restricted Three-Body Problem with Oblateness Non-Linear Stability Zones around Triangular Equilibria in the Plane Circular Restricted Three-Body Problem with Oblateness

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.245..157m&link_type=abstract

Astrophysics and Space Science, Volume 245, Issue 1, pp.157-164

Astronomy and Astrophysics

Astrophysics

11

Scientific paper

Non-linear stability zones of the triangular Lagrangian points are computed numerically in the case of oblate larger primary in the plane circular restricted three-body problem. It is found that oblateness has a noticeable effect and this is identified to be related to the resonant cases and the associated curves in the mass parameter μ versus oblateness coefficientA 1 parameter space.

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