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arXiv · 1506.06632

Dynamics of a small planetoid in Newtonian gravity field of Lagrangian configuration of three primaries

Sergey V. Ershkov·Dmytro Leshchenko·Alla Rachinskaya
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Abstract

Novel method for semi-analytical solving of equations of a trapped dynamics for a planetoid m4 close to the plane of mutual motion of main bodies around each other (in case of a special type of Bi-Elliptic Restricted 4-Bodies Problem) is presented. We consider here three primaries m1, m2, m3 orbiting around their center of mass on elliptic orbits which are permanently forming Lagrangian configuration of an equilateral triangle. Our aim is to obtain appoximate coordinates of quasi planar trajectory of the infinitesimal planetoid m4, when the primaries have masses equal to 1/3. Results are as follows: 1) equations for coordinates {x, y} are described by system of coupled 2-nd order ordinary differential equations with respect to true anomaly f, 2) expression for z stems from solving second order Riccati ordinary differential equation that determines the quasi-periodical oscillations of planetoid m4 not far from invariant plane {x, y, 0}.

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Sergey V. Ershkov, Dmytro Leshchenko, Alla Rachinskaya. 2015-06-12. Dynamics of a small planetoid in Newtonian gravity field of Lagrangian configuration of three primaries. https://doi.org/10.1155/2015%2F615029

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