Extended Data Fig. 6: Influence of the surface pressure and internal heat flux. | Nature

Extended Data Fig. 6: Influence of the surface pressure and internal heat flux.

From: A cool runaway greenhouse without surface magma ocean

Extended Data Fig. 6

a) Profiles for Venus gravity and insolation 4.5 Gyrs ago. b) Profiles for an Earth gravity with an ISR of 378 Wm−2 and T-1 spectrum. At ϕint = 0 both cases have an OTR of 378 Wm−2. Dashed lines indicate convective layers. Dots indicate the surface of each individual profile.

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