Free Access

Fig. B.1


Panel a: Portion of the domain of definition of the initial orbital parameters є, r0, and rcir,p involved in the Keplerian two-body problem (shaded in grey). The blue and brown surfaces depict limiting cases. Panel b: A closer view of the lower boundary of this domain (brown surface). It allows for a greater appreciation of the values of the initial orbital energy, rcir,p, below which the initial relative velocity, ν0, is not defined.

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.