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Fig. 3

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Modelled temperature profiles at different longitudes, averaged in latitude (thick lines). The light lines represent the temperature profiles at each latitude (spaced every 3.75°). (a) Cloudless simulation at solar metallicity. (b) With Mg2SiO4 clouds of 1 μm at solar metallicity. (c) Cloudless at 10× solar metallicity. (d) With Mg2SiO4 clouds of 1 μm at 10x solar metallicity. The solid grey line represents the condensation curves of Mg2SiO4 at solar metallicity, and the dashed grey line is the condensation curve of Mg2SiO4 at 10× solar metallicity.

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