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Fig. 3

image

Size frequency distributions of the Jupiter Trojans in the case of Rmin = 100 km and Rexp = 250 km (top histogram) and for Rmin = 10 km and Rexp = 100 km (bottom histogram). The histograms show the number of Trojans in mass bins (bottom x-axis). In the upper x-axes we show the correspondent radius bins (we assumed a density of the Trojans of 1.5 g cm−3). In cyan we highlight the part of the distributions that we substituted into the Trojan swarms as massive bodies. The black arrow indicates the mass of asteroid (624) Hektor, which is the most massive Jupiter Trojan.

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