Left: end states of the escaped Vesta fragments, represented as the percentage with respect to the total number of ejected fragments as a function of time. The different curves indicate the end states reached by the fragments, which are the ejection from the Solar System or a collision with the Sun. Right: escape routes from the MB of Vesta fragments, represented as the percentage with respect to the total number of escaped fragments as a function of time. The escape routes are the 3:1 MMR and the ν6 secular resonance.