New asteroid clusters and evidence of collisional fragmentation in the L5 Trojan cloud of Mars

Open Access

Fig. 1

Distribution of L₅ MTs in libration width (L) vs. inclination (I_P) space (top) and eccentricity e_P vs. inclination I_P (bottom). Red points correspond to new asteroid clusters identified in this work. Plotted errors correspond to 2σ formal uncertainties and are smaller than the symbol size for the libration width L.

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