High-order resonant orbit manifold expansions for mission design in the planar circular restricted 3-body problem

In recent years, stable and unstable manifolds of invariant objects (such as libration points and periodic orbits) have been increasingly recognized as an efficient tool for designing transfer trajectories in space missions. However, most methods currently used in mission design rely on using eigenv...

Full description

Saved in:
Bibliographic Details
Published in:Communications in nonlinear science & numerical simulation Vol. 97; p. 105691
Main Authors: Kumar, Bhanu, Anderson, Rodney L., de la Llave, Rafael
Format: Journal Article
Language:English
Published: Amsterdam Elsevier B.V 01.06.2021
Elsevier Science Ltd
Subjects:
ISSN:1007-5704, 1878-7274
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:In recent years, stable and unstable manifolds of invariant objects (such as libration points and periodic orbits) have been increasingly recognized as an efficient tool for designing transfer trajectories in space missions. However, most methods currently used in mission design rely on using eigenvectors of the linearized dynamics as local approximations of the manifolds. Since such approximations are not accurate except very close to the base invariant object, this requires large amounts of numerical integration to globalize the manifolds and locate intersections. In this paper, we study hyperbolic resonant periodic orbits in the planar circular restricted 3-body problem, and transfer trajectories between them, by: 1) determining where to search for resonant periodic orbits; 2) developing and implementing a parameterization method for accurate computation of their invariant manifolds as Taylor series; and 3) developing a procedure to compute intersections of the computed stable and unstable manifolds. We develop and implement algorithms that accomplish these three goals, and demonstrate their application to the problem of transferring between resonances in the Jupiter-Europa system.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 14
ISSN:1007-5704
1878-7274
DOI:10.1016/j.cnsns.2021.105691