Orbital Dynamics in the Gravitational Field of Small Bodies

Nominated as an outstanding PhD thesis by the Tsinghua University in 2014Introduces qualitative methods of nonlinear dynamics into the study of orbits around solar system small bodies (SSSBs) with high-resolution mechanical modelsFocuses on the topological classification and evolution, showing the composition of the periodic motion set for a specific asteroidDescribes new methods for reproducing and measuring four typical types of motion in the vicinity of SSSBsIncludes supplementary material: sn.pub/extras

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