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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-837b.
Simulation parameters | |
---|---|
N◦ of Monte Carlo runs | 2 × 105 |
Seed formation time | 0.1–4.0 × 106 yr |
Disc lifetime | 5.0 × 106 yr |
Star, planet, and disc properties | |
Stellar mass | 1.109 M⊙ |
Disc mass | 0.06 M⊙ |
Disc characteristic radius Rc | 50.0 au |
Surface density @ Rc | 4.2 g cm−2 |
Temperature T0 @ 1 au | 200K |
Disc accretion coefficient, α | 0.01 |
Turbulent viscosity, αν | 0.0001 |
Pebble size | 1 mm−1 cm |
Seed mass | 0.01 M⊕ |
Initial envelope mass | 0.0 M⊕ |
Initial semimajor axis | 0.5–20.0au |
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