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Table 1
Simulations of the young Solar System.
| Planets born in orbit around an isolated star (see Sects. 3.2 and 4.2.2) | |
|---|---|
| Designation | Simulations E |
| Simulations | Twelve simulations to study the internal planetary dynamics and their response to the local asteroids |
| Star | Single 1 M⊙ with 4 planets, 2000 asteroids |
| Planets | Four planets in almost circular orbits (e < 0.006) in the plane (i < 0.1°) with Jupiter, Saturn, Neptune, and Uranus in orbits with semi-major axes of 5.1, 9.5, 19.2, and 30.1 au. We performed two more simulations with initial semi-major axes of 3.75, 5.953, 9, 449, and 15.0 au |
| Asteroids | Two-thousand asteroids in circular orbits in a thick Q = 25 disk in the ecliptic plane of the planets between 3 au and 50 au |
| Numerics | Huayno (Pelupessy et al. 2012) |
| Computer | Run on a 192 core Intel-Xeon workstation |
| Duration | Simulation performed for a duration of 50 Myr |
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