Trajectory design in the Earth-Moon system and lunar South Pole coverage

Spacecraft trajectory design is evolving and innovation is increasingly driven by computational methods. As new regimes are explored, numerical techniques are most often developed to cope with undesirable behavior in sensitive dynamical systems. Nonlinear systems with sensitive dynamics are ubiquito...

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Main Author: Grebow, Daniel J
Other Authors: Howell, Kathleen C.
Format: Text
Language:English
Published: Purdue University 2010
Subjects:
Online Access:https://docs.lib.purdue.edu/dissertations/AAI3413892
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spelling ftpurdueuniv:oai:docs.lib.purdue.edu:dissertations-9687 2023-07-02T03:33:44+02:00 Trajectory design in the Earth-Moon system and lunar South Pole coverage Grebow, Daniel J Howell, Kathleen C. 2010-01-01T08:00:00Z https://docs.lib.purdue.edu/dissertations/AAI3413892 ENG eng Purdue University https://docs.lib.purdue.edu/dissertations/AAI3413892 Theses and Dissertations Available from ProQuest Aerospace engineering text 2010 ftpurdueuniv 2023-06-12T21:43:17Z Spacecraft trajectory design is evolving and innovation is increasingly driven by computational methods. As new regimes are explored, numerical techniques are most often developed to cope with undesirable behavior in sensitive dynamical systems. Nonlinear systems with sensitive dynamics are ubiquitous spacecraft trajectory modeling, where the models include, for example, perturbations due to an aspherical central body, multi-body perturbations, and solar wind. Numerical techniques are particularly useful in designing trajectories for lunar south pole coverage. Dual-spacecraft constellations include either two spacecraft in lunar "frozen" orbits or in multi-body orbits near the libration points of the Earth-Moon Restricted 3-Body Problem (R3BP). Alternatively, single spacecraft constellations, or "pole-sitters," require only one spacecraft for continuous surveillance and a control source for displacing the vehicle below the trans- or cis-lunar libration point. The control source might originate from a solar sail or an electric thruster. A spacecraft equipped with an electric thruster has an added advantage in that it can be deployed immediately and is eventually inserted into a larger constellation for continued surveillance. The following investigation includes many numerical techniques that are useful for trajectory design. The methods are applied for a thorough analysis of motion in the Earth-Moon R3BP, including dual-spacecraft and pole-sitter missions for lunar south pole coverage, where continuous line-of-sight access between a lunar ground station and the Earth is required. The various options for coverage are explored in higher-fidelity models and evaluated in terms of elevation angle and altitude from the Shackleton crater near the lunar south pole. The choice of constellation is driven by the mission requirements. Text South pole Purdue University: e-Pubs Shackleton Sitter ENVELOPE(10.986,10.986,64.529,64.529) South Pole
institution Open Polar
collection Purdue University: e-Pubs
op_collection_id ftpurdueuniv
language English
topic Aerospace engineering
spellingShingle Aerospace engineering
Grebow, Daniel J
Trajectory design in the Earth-Moon system and lunar South Pole coverage
topic_facet Aerospace engineering
description Spacecraft trajectory design is evolving and innovation is increasingly driven by computational methods. As new regimes are explored, numerical techniques are most often developed to cope with undesirable behavior in sensitive dynamical systems. Nonlinear systems with sensitive dynamics are ubiquitous spacecraft trajectory modeling, where the models include, for example, perturbations due to an aspherical central body, multi-body perturbations, and solar wind. Numerical techniques are particularly useful in designing trajectories for lunar south pole coverage. Dual-spacecraft constellations include either two spacecraft in lunar "frozen" orbits or in multi-body orbits near the libration points of the Earth-Moon Restricted 3-Body Problem (R3BP). Alternatively, single spacecraft constellations, or "pole-sitters," require only one spacecraft for continuous surveillance and a control source for displacing the vehicle below the trans- or cis-lunar libration point. The control source might originate from a solar sail or an electric thruster. A spacecraft equipped with an electric thruster has an added advantage in that it can be deployed immediately and is eventually inserted into a larger constellation for continued surveillance. The following investigation includes many numerical techniques that are useful for trajectory design. The methods are applied for a thorough analysis of motion in the Earth-Moon R3BP, including dual-spacecraft and pole-sitter missions for lunar south pole coverage, where continuous line-of-sight access between a lunar ground station and the Earth is required. The various options for coverage are explored in higher-fidelity models and evaluated in terms of elevation angle and altitude from the Shackleton crater near the lunar south pole. The choice of constellation is driven by the mission requirements.
author2 Howell, Kathleen C.
format Text
author Grebow, Daniel J
author_facet Grebow, Daniel J
author_sort Grebow, Daniel J
title Trajectory design in the Earth-Moon system and lunar South Pole coverage
title_short Trajectory design in the Earth-Moon system and lunar South Pole coverage
title_full Trajectory design in the Earth-Moon system and lunar South Pole coverage
title_fullStr Trajectory design in the Earth-Moon system and lunar South Pole coverage
title_full_unstemmed Trajectory design in the Earth-Moon system and lunar South Pole coverage
title_sort trajectory design in the earth-moon system and lunar south pole coverage
publisher Purdue University
publishDate 2010
url https://docs.lib.purdue.edu/dissertations/AAI3413892
long_lat ENVELOPE(10.986,10.986,64.529,64.529)
geographic Shackleton
Sitter
South Pole
geographic_facet Shackleton
Sitter
South Pole
genre South pole
genre_facet South pole
op_source Theses and Dissertations Available from ProQuest
op_relation https://docs.lib.purdue.edu/dissertations/AAI3413892
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