Table A.11
NEOs predicted to be associated with an S-complex taxonomy from the analysis of this work and the results of Simion et al. (2021).
| Number | Designation | i (°) | e | a (au) | q (au) | TJ | H |
|---|---|---|---|---|---|---|---|
| 2017 AF5 | 20.91 | 0.95 | 2.48 | 0.12 | 2.50 | 17.78 | |
| 2019 NF6 | 19.76 | 0.92 | 2.19 | 0.17 | 2.80 | 20.10 | |
| 431760 | 2008 HE | 9.83 | 0.95 | 2.26 | 0.11 | 2.70 | 18.10 |
| 2010 JG87 | 16.91 | 0.95 | 2.76 | 0.15 | 2.30 | 19.20 | |
| 2000 LK | 16.58 | 0.94 | 2.18 | 0.12 | 2.80 | 18.30 | |
| 2013 YC | 2.80 | 0.94 | 2.50 | 0.14 | 2.50 | 21.40 | |
| 2012 US68 | 25.80 | 0.96 | 2.50 | 0.11 | 2.40 | 18.30 | |
| 2021 LM1 | 29.54 | 0.95 | 2.31 | 0.13 | 2.60 | 20.45 | |
| 399457 | 2002 PD43 | 26.04 | 0.96 | 2.51 | 0.11 | 2.40 | 19.10 |
Although 2002 PD43 (Jewitt 2013) has optical colours that do not match those of an S-complex asteroid, we have not ruled it out as more taxonomic data are required to accept or reject the prediction criteria.
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