Table 2
Theoretical and observational estimates of the evaporation rate Ṁ (g s−1) of the five planets reported in Fig. 9.
| Planet | This work | HD modelling | Observations |
|---|---|---|---|
| HD 189733b | 4 × 1011 |  |
 |
| HD 209458b | 2.5 × 1010 |  |
 |
| GJ 436b | 1.6 × 109 |  |
 |
| WASP-12b(5) | 1.3 × 1012 |  |
|
| 55 Cnc e(7) | 4.3 × 109 |  |
|
References. (1) Kubyshkina et al. (2018); (2) Lecavelier des Étangs et al. (2010); (3) Vidal-Madjar et al. (2003); (4) Ehrenreich et al. (2015); (5) the evaporation mass loss rate is uncertain (Haswell 2017); (6) Lai et al. (2010); (7) no observational rates are available.
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