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Fig. 1

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Cumulative distributions of the semimajor axis N(≤a) of >100 km asteroids classified as CM-like, CI/IDP-like (including B types with the geometric albedo of pv < 0.1), and S-type. Vertical dotted lines mark major mean-motion resonances with Jupiter. CM-like objects exhibit an approximately symmetric distribution, whereas CIlike objects show a notably asymmetric distribution. Adapted from Anderson et al. (2025).

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