Free Access

Fig. 1


Illustration of the circular restricted three-body problem with oblateness. The origin of the synodic coordinate is in the barycentre. The primary m1 is the rotational ellipsoid whose coordinate is (−μ2, 0, 0), while m2 is the point mass located at (μ1, 0, 0).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.