A computational population study evaluating atmospheric retention using the cosmic shoreline framework and energy-limited escape modeling across 5,000 simulated planet-star systems.
| Planet | v_esc (km/s) | Fluence Ratio | T_eq (K) | Status |
|---|---|---|---|---|
| TOI-6716 b | 11.2 | 0.030 | 358 | Retained |
| TRAPPIST-1 e | 9.7 | 0.061 | 326 | Retained |
| TRAPPIST-1 f | 11.2 | 0.020 | 284 | Retained |
| TRAPPIST-1 g | 12.0 | 0.010 | 258 | Retained |
| LHS 1140 b | 16.8 | 0.001 | 273 | Retained |
| Proxima Cen b | 11.5 | 0.023 | 343 | Retained |
| GJ 1132 b | 12.9 | 0.210 | 721 | Retained |
| GJ 486 b | 15.0 | 0.120 | 768 | Retained |
| Gliese 12 b | 11.0 | 0.027 | 363 | Retained |