Table 1
Simulation resuts for each simulation.
| Run | N | AMD | RMC | Mplanets | MMars | aMars |
|
|
||||||
| Normal migration | ||||||
| Test31 | 5 | 0.0085 | 32.69 | 2.10 | 0.56 | 1.52 |
| Test43 | 3 | 0.0011 | 45.51 | 1.85 | 0.59 | 1.41 |
| Ran1 | 3 | 0.0035 | 58.77 | 1.82 | 0.43 | 1.42 |
| Ran3 | 4 | 0.0017 | 38.95 | 1.93 | 0.52 | 1.52 |
| Ran4 | 3 | 0.0023 | 42.09 | 1.71 | 0.14 | 1.71 |
| Ran7 | 3 | 0.0011 | 50.30 | 1.76 | 0.78 | 1.29 |
| Double asteroids | ||||||
| Test61 | 3 | 0.0023 | 42.38 | 1.82 | 0.59 | 1.43 |
| Test62 | 3 | 0.0014 | 66.43 | 1.83 | – | – |
| Double embryos | ||||||
| Test54 | 4 | 0.0011 | 40.53 | 1.90 | 0.06 | 1.88 |
| Perfect migration | ||||||
| PM21 | 4 | 0.0016 | 40.87 | 1.93 | 0.46 | 1.41 |
| PM22 | 3 | 0.0113 | 51.34 | 1.72 | 0.33 | 1.37 |
| PM24 | 6 | 0.0076 | 25.93 | 2.06 | 0.36 | 1.43 |
| MVEM | 4 | 0.0014 | 89.9 | 1.88 | 0.11 | 1.52 |
Notes. Included are the number of planets N, the angular momentum deficit (AMD) and the radial mass concentration (RMC) for each system of planets, the total mass of the planets Mplanets, and Mars analog MMars in Earth Masses, and the semimajor axis of the Mars analogs aMars. The entry MVEM is data for the current terrestrial planets. Note that Test31 and PM24 each had one embryo stranded in the asteroid belt region, with a > 2.0 AU, which are counted in their N, but not used to calculate RMC or AMD.
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