Accretion and Uneven Depletion of the Main Asteroid Belt
Rogerio Deienno,
David Nesvorný,
Matthew S. Clement
et al.
Abstract:The main asteroid belt (MAB) is known to be primarily composed of objects from two distinct taxonomic classes, generically defined here as S- and C-complex. The former probably originated from the inner solar system (interior to Jupiter’s orbit), while the latter probably originated from the outer solar system. Following this definition, (4) Vesta, a V-type residing in the inner MAB (a < 2.5 au), is the sole D > 500 km object akin to the S-complex that potentially formed in situ. This provides a useful c… Show more
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