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Libration point orbit characterization in the Earth–Moon system
Article first published online: 1 OCT 2012
DOI: 10.1111/j.1365-2966.2012.21585.x
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Issue

Monthly Notices of the Royal Astronomical Society
Volume 426, Issue 2, pages 1212–1222, 21 October 2012
Additional Information
How to Cite
Pergola, P. and Alessi, E. M. (2012), Libration point orbit characterization in the Earth–Moon system. Monthly Notices of the Royal Astronomical Society, 426: 1212–1222. doi: 10.1111/j.1365-2966.2012.21585.x
Publication History
- Issue published online: 24 SEP 2012
- Article first published online: 1 OCT 2012
- Manuscript Accepted: 22 JUN 2012
- Manuscript Received: 1 JUN 2012
- Abstract
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Keywords:
- celestial mechanics;
- eclipses;
- Earth;
- Moon
ABSTRACT
Recently, new efforts have been made to explore the lunar environment, with missions aimed at collecting vast amounts of data in view of a future human installation. In this context, several authors have proposed the exploitation of the neighbourhood of the equilibrium point L1 in the Earth–Moon system for various objectives. The purpose of this study is to provide effective criteria that can be applied to choosing a nominal orbit operable to these ends. We consider as key parameters the lunar surface coverage, Earth and Moon eclipses and orbit maintenance costs. By considering sets of periodic and quasi-periodic orbits at various energy levels, we provide parametric analyses that can be used to identify a specific orbit according to mission constraints. In general, a quasi-periodic orbit is preferable to a periodic one, owing to the larger number of parameters that characterize quasi-periodic orbits.

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