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Fig. 1


Left: cloud structures for changing C/O = 0.43 (blue), 1.1 (red), 1.5 (gray) 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: input Tgas [K] and pgas [bar], 2nd panel: nucleation rate log J [cm-3 s-1], 3rd panel: cloud particle number density log nd [cm-3], and 4th panel: mean cloud particle radius log ⟨ a [μm]. Right: changing material composition, Vs/Vtot [%] (relative volume fractions of solid species s) of the cloud particles with changing C/O ratio.

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