A new mechanism of stability highlighted by the recent planetary system HD 73526

Details A new mechanism of stability highlighted by the recent planetary system HD 73526 A new mechanism of stability highlighted by the recent planetary system HD 73526

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sf2a.conf..407g&link_type=abstract

SF2A-2006: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: D. Barret, F. Casoli, G.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Dynamical stability of the recent planetary system HD 73526, in 2:1 mean motion resonance, is not without controversy. Whereas this system has been found at first stable for coplanar orbits, techniques of global dynamics analysis show a quite unstable behavior within its strict observational data. Nevertheless, we find a stabilizing mechanism involving the undetermined observational parameters, namely the orbital inclinations and the longitudes of nodes.

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