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Astrodynamics Vol. 2, No. 1, 69{86, 2018 https://doi.org/10.1007/s42064-017-0014-5 1;2 3 1 3 4 Yu Jiang (B), Jurgen Arno Schmidt , Hengnian Li , Xiaodong Liu , and Yue Yang 1. State Key Laboratory of Astronautic Dynamics, Xi'an Satellite Control Center, Xi'an 710043, China 2. School of Aerospace Engineering, Tsinghua University, Beijing 100084, China 3. Astronomy Research Unit, University of Oulu, Finland 4. School of Software Engineering, Xi'an Jiaotong University, Xi'an 710049, China ABSTRACT KEYWORDS We are interested in stable periodic orbits for spacecraft in the gravitational eld of minor asteroid celestial bodies. The stable periodic orbits around minor celestial bodies are useful not only comet for the mission design of the deep space exploration, but also for studying the long-time deep space exploration stability of small satellites in the large-size-ratio binary asteroids. The irregular shapes periodic orbits and gravitational elds of the minor celestial bodies are modeled by the polyhedral model. stability Using the topological classi cations of periodic orbits and the grid search method, the stable orbit design periodic orbits can be calculated and the topological cases can be determined. Furthermore, we nd ve di erent types of stable periodic orbits around minor celestial bodies: (1) stable
Astrodynamics – Springer Journals
Published: Mar 1, 2018
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