Table 2
The final parameters of the simulations in the inner Solar System.
| Set | mtot | ƒemb | ƒpl,J | ƒemb,J | ƒa>7 | 〈memb〉 |
|---|---|---|---|---|---|---|
| 232 | 3.88 | 30 | 41 | 14 | 11 | 0.045 |
| 233 | 3.72 | 20 | 29 | 20 | 17 | 0.027 |
| 234 | 3.34 | 15 | 27 | 27 | 20 | 0.022 |
| 315 | 3.15 | 15 | 5.8 | 12 | 30 | 0.025 |
| 334 | 3.23 | 34 | 31 | 17 | 15 | 0.043 |
| 335 | 3.84 | 18 | 15 | 30 | 31 | 0.025 |
| 222g4 | 2.96 | 36 | 26 | 8.9 | 19 | 0.050 |
| 232g5 | 3.04 | 39 | 25 | 15 | 26 | 0.051 |
Notes. The first column is the total remaining mass in embryos and planetesimals (in M⊕), ƒemb = memb/mtot is the average fraction of total mass in embryos, ƒpl,J = mpl,J/mtot is the same for Jovian group planetesimals that are in the inner Solar System (i.e. a < 5 au), ƒemb,J = memb,j/memb,tot is the average mass fraction of Jovian group material incorporated into the embryos, and ƒa>7 is the fraction of planetesimals in the inner Solar System that come from beyond 7 au. All of these are in units of percent [%]. The final column is the average individual embryo mass (in M⊕).
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