Table 6
Asteroid families in the individual parts of the MB according to Brož et al. (2013).
| Region | Family | DPB (km) |
|---|---|---|
| Inner | Erigone | 114 |
| Eulalia | 100–160 | |
| Polana | ? | |
| Middle | Maria | 120–130 |
| Padua | 106 | |
| Misa | 117 | |
| Dora | 165 | |
| Merxia | 121 | |
| Teutonia | 120 | |
| Gefion | 100–150 | |
| Hoffmeister | 134 | |
| Pristine | Koronis | 170–180 |
| Fringilla | 130–140 | |
| Outer | Themis | 380–430 |
| Meliboea | 240–290 | |
| Eos | 381 | |
| Ursula | 240–280 | |
| Veritas | 100–177 | |
| Lixiaohua | 220 | |
| High-Inclination | Alauda | 290–330 |
Notes. DPB is the parent body diameter inferred from SPH simulations (Durda et al. 2007). We only consider families with DPB > 100 km and MLR∕MPB < 0.5. In the case of parent bodies with a wide range of diameters we took a mean value, while in the case of Polana we adopted a parent body size of 115 km.
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