Table 1
Simulation parameters.
| Set | minner | mouter | Change | Gap (range) | Bodies |
|---|---|---|---|---|---|
| 232 | 2 | 3 | 2 | – | 35k |
| 233 | 2 | 3 | 3 | – | 47k |
| 234 | 2 | 3 | 4 | – | 30k |
| 315 | 3 | 1 | 5 | – | 22k |
| 334 | 3 | 3 | 4 | – | 19k |
| 335 | 3 | 3 | 5 | – | 35k |
| 222g4 | 2 | 2 | 4 | 2–4 | 35k |
| 232g5 | 2 | 3 | 5 | 2–5 | 30k |
Notes. The masses are total planetesimal masses in Earth masses. The column ‘Change’ implies at what distance (in au) I consider the composition of the planetesimals to be predominantly inner versus outer Solar System. The fourth column indicates whether there is an empty region, and where (in au). The last column is self-explanatory.
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