Fig. 9
Evolution of carbon reservoirs for a stagnant-lid planet with an initial mantle temperature of 1900 K and (a) CO2 -dependent weathering model with α = 0.23 and (b) Tp -dependent weathering model. The accumulated degassed CO2 (magenta) is distributed between the carbonated crust (red), the atmosphere (blue), and the volatile CO2 reservoir in the crustal matrix (yellow).
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