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The Implementation of Hori–Deprit Method to the Construction Averaged Planetary Motion Theory by Means of Computer Algebra System Piranha

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Abstract

This article is related to the problem of the construction of planetary motion theory. We have expanded the Hamiltonian of the four-planetary problem into the Poisson series in osculating elements of the second Poincare system. The series expansion is constructed up to the third degree of the small parameter. The averaging procedure of the Hamiltonian is performed by the Hori–Deprit method. It allows to eliminate short-periodic perturbations and sufficiently increase time step of the integration of the equations of motion. This method is based on Lie transformation theory. The equations of motion in averaged elements are constructed as the Poisson brackets of the averaged Hamiltonian and corresponding orbital element. The transformation between averaged and osculating elements is given by the change-variable functions, which are obtained in the second approximation of the Hori–Deprit method. We used computer algebra system Piranha for the implementation of the Hori–Deprit method. Piranha is an echeloned Poisson series processor authored by F. Biscani. The properties of the obtained series are discussed. The numerical integration of the equations of motion is performed by Everhart method for the Solar system’s giant planets.

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Acknowledgements

This work is funded by RFBR according to the research Project No. 18-32-00283.

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  1. Ural Federal University, 51 Lenin Avenue, Yekaterinburg, Russia

    A. S. Perminov & E. D. Kuznetsov

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  1. A. S. Perminov
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  2. E. D. Kuznetsov
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Correspondence to A. S. Perminov.

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This work is funded by RFBR according to the research Project No. 18-32-00283.

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Perminov, A.S., Kuznetsov, E.D. The Implementation of Hori–Deprit Method to the Construction Averaged Planetary Motion Theory by Means of Computer Algebra System Piranha. Math.Comput.Sci. 14, 305–316 (2020). https://doi.org/10.1007/s11786-019-00441-4

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