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arXiv · 0712.3239

Orbital Stability of Planets in Binary Systems: A New Look at Old Results

J. Eberle·M. Cuntz·Z. E. Musielak
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Abstract

About half of all known stellar systems with Sun-like stars consist of two or more stars, significantly affecting the orbital stability of any planet in these systems. This observational evidence has prompted a large array of theoretical research, including the derivation of mathematically stringent criteria for the orbital stability of planets in stellar binary systems, valid for the "coplanar circular restricted three-body problem". In the following, we use these criteria to explore the validity of results from previous theoretical studies.

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J. Eberle, M. Cuntz, Z. E. Musielak. 2008-02-15. Orbital Stability of Planets in Binary Systems: A New Look at Old Results. https://doi.org/10.1017/s1743921308017043

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