Collection
On the modeling and exploitation of the co-orbital dynamics
The co-orbital motion plays a key role in the understanding of the three-body problem, to model the motion of natural bodies (asteroids, moons and planets) and eventually observe them, and to design spacecraft trajectories for exploration missions. The aim of the collection is to bring together mathematicians, planetary scientists and aerospace engineers to share their knowledge and experience as regards to mathematical tools, results and possible applications.
Please visit the Instruction for Authors web page for information on how to submit to this collection.
Editors
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Elisa Maria Alessi
Institute for applied mathematics and information technologies (IMATI) - CNR, Milano, Italy
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Sara Di Ruzza
University of Palermo, Italy
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Àngel Jorba
University of Barcelona, Spain
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Helena Morais
UNESP (Universidade Estadual Paulista), Brazil
