Table B.1
Spectral characteristics of primitive asteroid families.
| Family | NSDSS | NECAS | Albedo (%) | SVIS (g−i) (μm−1) | NUV abs. (μm−1) | SNIR1 (Y−J) (μm−1) | SNIR2 (J−Ks) (μm−1) | Qhyd (%) |
|---|---|---|---|---|---|---|---|---|
| IMB | ||||||||
| Polana–Eulalia | 368 | 8 | 6.5 ± 2.8 | 7(1) | ||||
| Erigone (h) | 127 | 0 | 5.4 ± 1.2 | 58(2) | ||||
| Clarissa | 6 | 1 | 5.6 ± 1.5 | − | − | 9(3) | ||
| Sulamitis (h) | 16 | 0 | 5.4 ± 1.4 | − | − | 60(3) | ||
| Klio (h) | 40 | 0 | 6.7 ± 1.8 | − | − | 23(4) | ||
| Chaldaea | 21 | 1 | 6.6 ± 1.7 | 79(4) | ||||
| MMB | ||||||||
| Nemesis | 57 | 3 | 8.4 ± 2.7 | 0(5) | ||||
| Adeona (h) | 251 | 1 | 6.3 ± 1.7 | 69(6) | ||||
| Padua | 76 | 1 | 7.2 ± 1.4 | 0(5,6) | ||||
| Chloris (h) | 43 | 1 | 8.1 ± 3.6 | |||||
| Misa (h) | 37 | 0 | 6.1 ± 1.7 | − | − | |||
| Dora (h) | 179 | 0 | 5.6 ± 1.7 | 83(6) | ||||
| Astrid (h) | 12 | 0 | 5.6 ± 1.9 | − | − | 20(6) | ||
| Konig (h) | 13 | 0 | 5.0 ± 1.6 | − | ||||
| Hoffmeister | 82 | 0 | 5.0 ± 1.4 | 0(5,6) | ||||
| Vibilia (h) | 15 | 0 | 6.4 ± 1.0 | − | ||||
| Phaeo | 20 | 1 | 5.8 ± 1.5 | − | − | |||
| Mitidika | 103 | 2 | 7.2 ± 2.0 | |||||
| Karma | 9 | 0 | 5.8 ± 1.0 | − | − | |||
| Postrema | 9 | 0 | 5.2 ± 2.3 | − | − | |||
| Pallas | 20 | 1 | 13.0 ± 3.3 | − | − | 0(7) | ||
| Brucato (h) | 44 | 0 | 6.5 ± 1.4 | − | ||||
| OMB | ||||||||
| Hygiea | 381 | 3 | 7.8 ± 2.6 | 0–15(6,8) | ||||
| Themis | 536 | 19 | 7.7 ± 2.4 | 11–13(6,8) | ||||
| Sylvia | 13 | 2 | 6.3 ± 1.7 | − | − | |||
| Meliboea (h) | 53 | 3 | 6.3 ± 1.7 | 78(6) | ||||
| Emma (h) | 46 | 0 | 4.8 ± 1.6 | |||||
| Veritas (h) | 85 | 0 | 6.8 ± 1.9 | 75–77(6,8) | ||||
| Naema (h) | 22 | 0 | 6.8 ± 1.9 | − | ||||
| Lixiaohua | 68 | 0 | 4.4 ± 1.0 | 0(8) | ||||
| Theobalda | 39 | 1 | 7.4 ± 2.3 | |||||
| Beagle | 17 | 1 | 7.2 ± 1.6 | − | − | |||
| Fringilla | 17 | 0 | 5.1 ± 1.5 | − | − | |||
| Ursula | 136 | 1 | 6.5 ± 2.2 | 0(8) | ||||
| Inarradas (h) | 10 | 0 | 7.2 ± 1.5 | − | − | |||
| Euphrosyne | 150 | 0 | 5.8 ± 1.9 | |||||
| Alauda | 176 | 2 | 7.2 ± 2.7 | |||||
| Luthera | 14 | 0 | 5.1 ± 1.0 | − | ||||
Notes. Numbers in the brackets of SNIR are numbers of samples from the MOVIS-C catalog by Popescu et al. (2016), Qhyd is the fraction of family members with the 0.7 μm band from previous studies (see the references under the table). The notation of “(h)” indicates presence of the 0.7-μm absorption based on the positive HYD value.
References. (1) de León et al. (2016); (2) Morate et al. (2016); (3) Morate et al. (2018); (4) Morate et al. (2019); (5) Morate et al. (2021); (6) Mothé-Diniz et al. (2005); (7) de León et al. (2010); (8) De Prá et al. (2020b).
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