Open Access

Fig. 2

image

Download original image

Cumulative distributions of the initial semi-major axis of Hungaria, Vesta, and Hebe analogues in the Grand Tack (GT), EJS, and depleted disc (DD) models. The asteroids have equal probability of originating from anywhere in the disc for the Grand Tack model, while their formation locations are more restricted in the EJS model and the depleted disc model.

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.