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The dynamics of a spacecraft propelled by a continuous radial thrust resembles that of a nonlinear oscillator. This is analyzed in this work with a novel method that combines the definition of a suitable homotopy with a classical perturbation approach, in which the low thrust is assumed to be a perturbation of the nominal Keplerian motion. The homotopy perturbation method provides the analytical (approximate) solution of the dynamical equations in polar form to estimate the corresponding spacecraft propelled trajectory with a short computational time. The accuracy of the analytical results was tested in an orbital-targeting mission scenario.


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Application of homotopy perturbation method to the radial thrust problem

Show Author's information Lorenzo Niccolai( )Alessandro A. QuartaGiovanni Mengali
Department of Civil and Industrial Engineering, University of Pisa, I-56122, Italy

Abstract

The dynamics of a spacecraft propelled by a continuous radial thrust resembles that of a nonlinear oscillator. This is analyzed in this work with a novel method that combines the definition of a suitable homotopy with a classical perturbation approach, in which the low thrust is assumed to be a perturbation of the nominal Keplerian motion. The homotopy perturbation method provides the analytical (approximate) solution of the dynamical equations in polar form to estimate the corresponding spacecraft propelled trajectory with a short computational time. The accuracy of the analytical results was tested in an orbital-targeting mission scenario.

Keywords: radial thrust, nonlinear oscillator, homotopy perturbation method, trajectory approximation

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Publication history

Received: 24 May 2022
Accepted: 04 August 2022
Published: 23 November 2022
Issue date: June 2023

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© The Author(s) 2022

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