Earth escape from a sun-earth halo orbit using unstable manifold and lunar swingbys
Earth escape from a sun-earth halo orbit using unstable manifold and lunar swingbys
This paper investigates the Earth escape for spacecraft in a Sun-Earth halo orbit. The escape trajectory consists of first ejecting to the unstable manifold associated with the halo orbit, then coasting along the manifold until encountering the Moon, and finally performing lunar-gravity-assisted escape. The first intersection of the manifold tube and Moon's orbit results in four intersection points. These four manifold-guided encounters have different relative velocities (v∞) to the Moon; therefore, the corresponding lunar swingbys can result in different levels of characteristic energy (C3) with respect to the Earth. To further exploit these manifold-guided lunar encounters, subsequent swingbys utilizing solar perturbation are considered. A graphical method is introduced to reveal the theoretical upper limits of the C3 achieved by double and multiple swingbys. The numerically solved Sun-perturbed Moon-to-Moon transfers indicate that a second lunar swingby can efficiently increase C3. Compared to the direct low-energy escape along the manifold, applying a portion of the lunar swingbys before escape is shown to be more advantageous for deep-space mission design.
Circular restricted three-body problem, Earth escape, Graphical method, Invariant manifolds, Luni-solar gravity assists
269-277
Chen, Hongru
8286469d-afe1-46e5-b107-694017de4d97
Kawakatsu, Yasuhiro
ac1d6736-32d7-45ea-b65c-b446a8557a11
Hanada, Toshiya
6a914261-4634-4e52-8605-7c7579869145
2016
Chen, Hongru
8286469d-afe1-46e5-b107-694017de4d97
Kawakatsu, Yasuhiro
ac1d6736-32d7-45ea-b65c-b446a8557a11
Hanada, Toshiya
6a914261-4634-4e52-8605-7c7579869145
Chen, Hongru, Kawakatsu, Yasuhiro and Hanada, Toshiya
(2016)
Earth escape from a sun-earth halo orbit using unstable manifold and lunar swingbys.
Transactions of the Japan Society for Aeronautical and Space Sciences, 59 (5), .
(doi:10.2322/tjsass.59.269).
Abstract
This paper investigates the Earth escape for spacecraft in a Sun-Earth halo orbit. The escape trajectory consists of first ejecting to the unstable manifold associated with the halo orbit, then coasting along the manifold until encountering the Moon, and finally performing lunar-gravity-assisted escape. The first intersection of the manifold tube and Moon's orbit results in four intersection points. These four manifold-guided encounters have different relative velocities (v∞) to the Moon; therefore, the corresponding lunar swingbys can result in different levels of characteristic energy (C3) with respect to the Earth. To further exploit these manifold-guided lunar encounters, subsequent swingbys utilizing solar perturbation are considered. A graphical method is introduced to reveal the theoretical upper limits of the C3 achieved by double and multiple swingbys. The numerically solved Sun-perturbed Moon-to-Moon transfers indicate that a second lunar swingby can efficiently increase C3. Compared to the direct low-energy escape along the manifold, applying a portion of the lunar swingbys before escape is shown to be more advantageous for deep-space mission design.
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Published date: 2016
Keywords:
Circular restricted three-body problem, Earth escape, Graphical method, Invariant manifolds, Luni-solar gravity assists
Identifiers
Local EPrints ID: 490992
URI: http://eprints.soton.ac.uk/id/eprint/490992
ISSN: 0549-3811
PURE UUID: 1c0ecce7-7f64-491e-9167-d6e6a49c5279
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Date deposited: 11 Jun 2024 16:33
Last modified: 12 Jun 2024 02:11
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Contributors
Author:
Hongru Chen
Author:
Yasuhiro Kawakatsu
Author:
Toshiya Hanada
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