The effect of a biosphere on the habitable timespan of stagnant-lid planets and implications for the atmospheric spectrum

Open Access

Fig. 1

Resulting atmospheric CO₂ from our interior-atmosphere model. We show model results of an abiotic planet (a), a biotic planet (b), and the difference between them (c). The planet parameters are $f_{O_{2}} = IW- 0.2$ ${f_{{{\rm{O}}_2}}} = {\rm{IW}}\,{\rm{ - 0}}.2$ , T₀=1900 K, and η_ref = 10²¹ Pa s.

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