Open Access

Fig. 7


Relationship between the initial planetary mass and the fraction of the initial water envelope that is lost via photo-evaporation in 5 Gyr for six initial water mass fractions of Xwt,0 = 1% (solid, red), 3% (long-dashed, green), 10% (dotted, blue), 30% (dash-dotted, purple), 50% (dot-dashed, light blue), and 60% (dashed, black). We have assumed L0 = 1 × 1024  erg  s-1, a = 0.1 AU, and ε = 0.1.

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