Table 1
Properties of the asteroid families in terms of center ac and slope K of their V-shapes.
| Name | ac (au) | K (au−1 km−1) | Reference |
|---|---|---|---|
| Low albedo | |||
| Klio | 2.362 | 2.65 | 1 |
| PrimordialL | 2.367 | 0.59 | 2 |
| Erigone | 2.376 | 9.22 | 1 |
| Chaldea | 2.376 | 1.99 | 1 |
| PrimordialR | 2.400 | 0.59 | 2 |
| Clarissa | 2.406 | 33.65 | 1 |
| Polana | 2.420 | 1.10 | 2 |
| Chimaera | 2.460 | 6.14 | 1 |
| Sulamitis | 2.463 | 5.02 | 1 |
| Svea | 2.476 | 6.14 | 1 |
| Eulalia | 2.490 | 1.70 | 2 |
| High albedo | |||
| Flora | 2.200 | 1.60 | 2 |
| Baptistina | 2.260 | 11.90 | 3 |
| Euterpe | 2.347 | 7.67 | 1 |
| Primordial | 2.363 | 0.68 | 4 |
| Vesta | 2.370 | 2.97 | 1 |
| Athor | 2.380 | 1.72 | 3 |
| Massalia | 2.400 | 14.12 | 1 |
| Hertha1 | 2.412 | 8.36 | 5 |
| Hertha2 | 2.426 | 31.35 | 5 |
Notes. For the low-albedo primordial family of Delbo et al. (2017), we give the inward (left) and outward (right) borders. The former is indicated with the L, while the latter with the R as a suffix to the family name.
References. (1) Nesvorný et al. (2015), (2) Delbo et al. (2017), (3) Delbo et al. (2019), (4) Delbo et al. (in prep.), and (5) Dykhuis & Greenberg (2015).
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