Identification of a 4.3 billion year old asteroid family and planetesimal population in the Inner Main Belt

Open Access

Fig. 1

Proper orbital elements of the inner main asteroid belt. Only bodies with p_V greater than 0.123 are shown. The y-axis is shared for the top two panels, while the x-axis is shared for the left two panels. Clusters of objects correspond to some of the most preeminent asteroid families.

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