Highlight
Open Access

Fig. 5.

image

Asteroid orbital parameter distributions inside the Solar asteroid belt (blue) and our reconstructed primordial model belt (orange). Top: asteroid semi-major axes distribution. Bottom: asteroid inclinations as a function of the semi-major axes. In both panels, the Kirkwood gaps are clearly visible in the Solar asteroid belt.

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.