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Fig. 5

image

Left: cloud structures for changing C/O = 3.0 (pink), 10.0 (orange) for a prescribed Drift-Phoenix (Tgas, pgas) structure for a giant gas planet with Teff = 2000 K, log (g) = 3.0, initial solar element abundances. 1st panel: nucleation rate log J [cm-3 s-1], 2nd panel: cloud particle number density log nd [cm-3], and 3rd panel: mean cloud particle radius log ⟨ a [μm]. Right: 1st panel changing material composition, Vs/Vtot [%] (relative volume fractions of solid species s) of the cloud particles for C/O ratios = 3.0 and 10.0.

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