Table 1
Nature of the discard events of planetesimals and embryos.
Accreted | Final inner | Remaining mass | ||
---|---|---|---|---|
Index | by giants | Ejected | eccentricity | in M⊕ |
or the star | (min-max) | (max) | ||
2_01 | 51.9% | 48.1% | 0.228 (0.132-0.291) | 0.033 (0.055) |
2_02 | 44.3% | 55.7% | 0.143 (0.034-0.196) | 0.061 (0.115) |
2_03 | 43.6% | 56.4% | 0.385 (0.186-0.528) | 0.110 (0.285) |
2_04 | 82.6% | 17.4% | 0.430 (0.311-0.553) | 0.000 |
2_05 | 57.9% | 42.1% | 0.070 (0.026-0.194) | 0.183 (0.168) |
2_06 | 65.5% | 34.5% | 0.406 (0.203-0.716) | 0.0003 |
3_01 | 47.0% | 53.0% | 0.410 (0.087-0.855) | 0.000 |
3_02 | 43.2% | 56.8% | 0.434 (0.186-0.784) | 0.009 (0.580) |
3_03 | 90.9% | 9.1% | 0.329 (0.081-0.823) | 0.101 (0.313) |
2_07 | 37.0% | 63.0% | 0.155 (0.077-0.279) | 1.348 (0.925) |
2_08 | 8.8% | 91.2% | 0.105 (0.041-0.186) | 1.851 (1.180) |
2_09 | 22.2% | 77.8% | 0.160 (0.064-0.384) | 1.626 (1.283) |
3_04 | 51.8% | 48.2% | 0.331 (0.139-0.774) | 0.023 (0.198) |
3_05 | 33.1% | 66.9% | 0.233 (0.097-0.569) | 0.099 (0.688) |
Notes. For the nine runs per configuration (index in the first column), the average percentage of collisions with a giant or the star is given in the second column and that of ejections in the third column. The fourth column shows the average final eccentricity of the innermost giant planet for the nine runs per configuration, while the minimum and maximum values are given in brackets. The last column indicates the average remaining mass (in M⊕) of the terrestrial disc after 100 Myr, while the maximum mass of the formed terrestrial planets in each set is indicated in brackets.
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