Transfers from the Earth to L2 Halo orbits in the Earth-Moon bicircular problem

Fecha de publicación

2022-02-25T11:48:52Z

2022-12-03T06:10:27Z

2021-12-03

2022-02-25T11:48:53Z

Resumen

This paper deals with direct transfers from the Earth to Halo orbits related to the translunar point. The gravitational influence of the Sun as a fourth body is taken under consideration by means of the Bicircular Problem (BCP), which is a periodic time dependent perturbation of the Restricted Three Body Problem (RTBP) that includes the direct effect of the Sun on the spacecraft. In this model, the Halo family is quasi-periodic. Here we show how the effect of the Sun bends the stable manifolds of the quasi-periodic Halo orbits in a way that allows for direct transfers.

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Springer Verlag

Documentos relacionados

Versió postprint del document publicat a: https://doi.org/10.1007/s10569-021-10054-4

Celestial Mechanics and Dynamical Astronomy, 2021, vol. 133, num. 55

https://doi.org/10.1007/s10569-021-10054-4

info:eu-repo/grantAgreement/EC/H2020/734557/EU//TraX

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(c) Springer Verlag, 2021

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