Figure 11.
Chemical gas composition at the substellar point (θ = 0°, ϕ = 0°) HD 189733b (left) and HD 209458b (right) in a collisionally dominated, inner (deeper) atmosphere. Shown are the number densities of atoms and molecules linked to the elements (O, Al, S, Mg, Ti Fe, Si Ca) involved in cloud formation.

Chemical gas composition at the substellar point (θ = 0°, ϕ = 0°) HD 189733b (left) and HD 209458b (right) in a collisionally dominated, inner (deeper) atmosphere. Shown are the number densities of atoms and molecules linked to the elements (O, Al, S, Mg, Ti Fe, Si Ca) involved in cloud formation.

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