Automation of High-Fidelity Pump-Down Flyby Tours at Saturn

Abstract An efficient new framework for automating the search for multiple-body high-fidelity pump-down tours is presented. An existing pathfinding method for same-body transfer sequences is extended to include inter-moon transfers in patched conics. A separate algorithm analyzes each multiple-body sequence to determine how many legs can be efficiently converted to high-fidelity and optimized. The sequences are pruned, and patched conics searches are repeated from the terminal conditions of the high-fidelity trajectories. Frequent corrections in the high-fidelity model allow the optimization scheme to exploit, rather than fight, the high-fidelity perturbations. The process is automated and returns a Pareto optimal trade space of high-fidelity multiple-body pump-down tours. The method is used to create integrated trajectories starting at Titan arrival conditions and terminating with capture at Enceladus. The resulting Pareto front ranges from 900-1030 days time of flight and 410-550 m/s $$\Delta v$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>Δ</mml:mi> <mml:mi>v</mml:mi> </mml:mrow> </mml:math> , and leads to a compelling case for sending an orbiter to Enceladus.

Authors

Publication Details

Journal
The Journal of the Astronautical Sciences
Published
2026-06-17
DOI
https://doi.org/10.1007/s40295-026-00601-2
Primary Topic
Spacecraft Dynamics and Control
Type
article
Field-Weighted Citation Impact
0.00

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article

Automation of High-Fidelity Pump-Down Flyby Tours at Saturn

Matthew Shaw, Ryan P. Russell, William Brandenburg
The Journal of the Astronautical Sciences
Spacecraft Dynamics and Control
article

Automation of High-Fidelity Pump-Down Flyby Tours at Saturn

Matthew Shaw, Ryan P. Russell, William Brandenburg
article en

Abstract

Abstract An efficient new framework for automating the search for multiple-body high-fidelity pump-down tours is presented. An existing pathfinding method for same-body transfer sequences is extended to include inter-moon transfers in patched conics. A separate algorithm analyzes each multiple-body sequence to determine how many legs can be efficiently converted to high-fidelity and optimized. The sequences are pruned, and patched conics searches are repeated from the terminal conditions of the high-fidelity trajectories. Frequent corrections in the high-fidelity model allow the optimization scheme to exploit, rather than fight, the high-fidelity perturbations. The process is automated and returns a Pareto optimal trade space of high-fidelity multiple-body pump-down tours. The method is used to create integrated trajectories starting at Titan arrival conditions and terminating with capture at Enceladus. The resulting Pareto front ranges from 900-1030 days time of flight and 410-550 m/s $$\Delta v$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>Δ</mml:mi> <mml:mi>v</mml:mi> </mml:mrow> </mml:math> , and leads to a compelling case for sending an orbiter to Enceladus.

The Journal of the Astronautical SciencesVol. 73(4)
National Aeronautics and Space Administration, Lockheed Martin
Openalex Percentile: Top 3%
Spacecraft Dynamics and Control
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