Larger asteroid families show higher incidence of fresh surface signatures (p_V/p_IR > 1.2) with Spearman correlations of 0.58 (S-complex) and 0.44 (C-complex).
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Size-Dependent Fresh Surface Signatures in Asteroid Families: Observational Evidence from Dual-Band Albedo Analysis
Larger asteroid families show higher incidence of fresh surface signatures (p_V/p_IR > 1.2) with Spearman correlations of 0.58 (S-complex) and 0.44 (C-complex).