Fig. 11

Molar ratio of atoms O, C, N, and S relative to the total mass of gas
H2 in
planets as a function of the total mass of
planets and mass ratio of solids
relative to total planetary mass
, for
all models. Horizontal gray lines represent abundances of atoms adopted in the
ISM. Gray dots J and S represent,
respectively, the abundances for Jupiter and Saturn. Data for Jupiter and Saturn
provided by Wong et al. (2004), Flasar et
al. (2005), Orton et al. (2005), and Briggs & Sackett (1989). The light
gray area on the right corresponds to the zone where the mass of planets is higher
than 13 Jovian masses and where there could be more brown dwarfs than giant
planets.
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