Fast numerical computation of Lissajous and quasi-halo libration point trajectories
Visualitza/Obre
Estadístiques de LA Referencia / Recolecta
Inclou dades d'ús des de 2022
Cita com:
hdl:2117/17854
Tipus de documentText en actes de congrés
Data publicació2012
Condicions d'accésAccés obert
Llevat que s'hi indiqui el contrari, els
continguts d'aquesta obra estan subjectes a la llicència de Creative Commons
:
Reconeixement-NoComercial-SenseObraDerivada 3.0 Espanya
Abstract
In this paper we present a methodology for the automatic generation of quasi–periodic libration point trajectories
(Lissajous and quasi–halo) of the Spatial, Circular Restricted Three–Body Problem. This methodology is based
on the computation of a mesh of orbits which, using interpolation strategies, gives an accurate quantitative representation
of the full set of libration point orbits. This representation, when combined with the one obtained using
Poincar´e maps, provides a useful tool for the design of missions to libration points fulfilling specific requirements.
The same methodology applies to stable and unstable manifolds as well. This paper extends and improves results
presented in [10].
CitacióMondelo, J. M. [et al.]. Fast numerical computation of Lissajous and quasi-halo libration point trajectories. A: International Astronautical Congress. "63rd International Astronautical Congress". Naples: 2012, p. 1-12.
ISBN1995-6258
Fitxers | Descripció | Mida | Format | Visualitza |
---|---|---|---|---|
iac12_paper-v02.pdf | 1,058Mb | Visualitza/Obre |