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Table 3
Input parameters used to run the MC modified GroMiT code to produce simulated planets and investigate the formation history of TOI-2443 b.
| Simulation parameters | |
|---|---|
| No. of Monte Carlo runs | 2×105 |
| Seed formation time | 0.0–3.0 Myr |
| Disk lifetime | 5.0 Myr |
| Star, planet, and disk properties | |
| Stellar mass | 0.642 M⊙ |
| Stellar luminosity at 1 Myr | 0.85 L⊙ |
| Disk mass | 0.03 M⊙ |
| Disk characteristic radius Rc | 30.0 au |
| Surface density at Rc | 6.05 g cm−2 |
| Temperature T0 at Rc | 45 K |
| Disk accretion coefficient, α | 0.0003–0.003 |
| Turbulent viscosity, αv | 0.0001 |
| Pebble size | 1 mm−1 cm |
| Dust-to-gas ratio | 0.0075 |
| Seed mass | 0.01 M⊕ |
| Initial envelope mass | 0.0 M⊕ |
| Initial semimajor axis | 0.1–30.0 au |
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