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Carbon Cycle Imbalances on Arid Terrestrial Planets with Implications for Venus

  • Authors: Haskelle T. White-Gianella, Joshua Krissansen-Totton

Haskelle T. White-Gianella and Joshua Krissansen-Totton 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure A4.

Similar to Figure 6, but additionally including sensitivity tests where only the crust can be hydrated (“crustal hydration only,” pink lines). Albedo is constant at α = 0.3, and escape processes are included for Earth-like instellation and hypsometry. Even with limited or no ingassing, small initial surface reservoirs result in an imbalanced carbon cycle that leads to uninhabitable surfaces.

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