Baig, S. and McInnes, C. R. (2009) Artificial halo orbits for low-thrust propulsion spacecraft. Celestial Mechanics and Dynamical Astronomy, 104(4), pp. 321-335. (doi: 10.1007/s10569-009-9215-4)
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Publisher's URL: http://dx.doi.org/10.1007/s10569-009-9215-4
Abstract
We consider periodic halo orbits about artificial equilibrium points (AEP) near to the Lagrange points L 1 and L 2 in the circular restricted three body problem, where the third body is a low-thrust propulsion spacecraft in the Sun–Earth system. Although such halo orbits about artificial equilibrium points can be generated using a solar sail, there are points inside L 1 and beyond L 2 where a solar sail cannot be placed, so low-thrust, such as solar electric propulsion, is the only option to generate artificial halo orbits around points inaccessible to a solar sail. Analytical and numerical halo orbits for such low-thrust propulsion systems are obtained by using the Lindstedt Poincaré and differential corrector method respectively. Both the period and minimum amplitude of halo orbits about artificial equilibrium points inside L 1 decreases with an increase in low-thrust acceleration. The halo orbits about artificial equilibrium points beyond L 2 in contrast show an increase in period with an increase in low-thrust acceleration. However, the minimum amplitude first increases and then decreases after the thrust acceleration exceeds 0.415 mm/s2. Using a continuation method, we also find stable artificial halo orbits which can be sustained for long integration times and require a reasonably small low-thrust acceleration 0.0593 mm/s2.
Item Type: | Articles |
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Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | McInnes, Professor Colin |
Authors: | Baig, S., and McInnes, C. R. |
College/School: | College of Science and Engineering > School of Engineering > Systems Power and Energy |
Journal Name: | Celestial Mechanics and Dynamical Astronomy |
Publisher: | Springer Verlag |
ISSN: | 0923-2958 |
ISSN (Online): | 1572-9478 |
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