Fig. 10

Upper panel: theoretical distribution of masses and semi-major axes
(or incident fluxes) of planets at 10 Gyr with various initial masses and water mass
fractions. Crosses (red) represent planets that lost their water envelopes completely
in 10 Gyr, while open squares (blue) represent planets that survive significant loss
of the water envelopes via photo-evaporation. The green line is the minimum threshold
masses, . Here, we have
adopted ε = 0.1. Lower panel: distribution of masses
and semi-major axes (or incident fluxes) of detected exoplanets compared to the
minimum threshold mass,
, derived in
this study (see Sect. 3.3 for definition). We have shown three
relationships for different
heating efficiencies: ε = 1 (solid line), ε = 0.1
(dashed line), and ε = 0.01 (dotted line). Filled circles with error
bars represent observational data (from http://exoplanet.org (Wright et al. 2011)) for planets orbiting host
stars with effective temperature of 5000–6000 K (relatively early K-type stars and
G-type stars). Planets are colored according to their zero-albedo equilibrium
temperatures in K. In the planet names, “CoR” and “Kep” stand for CoRoT and
Kepler, respectively.
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