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Table A.2.
Fiducial parameters used in simulations.
| Stellar (Solar-type) | ||
|---|---|---|
| Mass | M⋆ | 1.0 M⊙ |
| Radius | R⋆ | 1.0 R⊙ (0.00465 au) |
| Disrupted Jupiter-like planet | ||
| Total mass | Mp | 0.99 MJup |
| Layers (atmosphere / mantle / core) | Mi | 0.65 / 0.32 / 0.02 MJup |
| Disruption radii (Roche) | r0, i = RRoche, i | 0.012 / 0.009 / 0.0056 au |
| VEPs (volatile-enriched planets) | ||
| Mass | Mp | 1, 10 M⊕ |
| Semi-major axis | a | 0.04, 0.07 au |
| Hill radius | RH = a (Mp/3M⋆)1/3 | 4.0 × 10−4 au (1 M⊕) |
| 1.5 × 10−4 au (10 M⊕) | ||
| Capture radius | Rcap = 0.2 RH | 8.0 × 10−5 au (1 M⊕) |
| 3.0 × 10−5 au (10 M⊕) | ||
| Disc and hydrodynamic simulation | ||
| Kinematic viscosity | ν | 7 × 1013 cm2 s−1 |
| Radial domain | [rin, rout] | [0.001, 0.10] au |
| Resolution | (Nr, Nϕ) | (720, 1024) |
| Equation of state | locally isothermal | |
| Kelvin–Helmholtz contraction | ||
| Rosseland mean opacity | κR | 1 cm2 g−1 |
| Exponent 1 − 1/q′ | −2.5 | |
| Exponent s/q′ | 1 | |
| Time-scale | tKH | ∼ 108 (Mcore/M⊕)−2.5 yr |
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