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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 A8.

Probability plot showing the effect of planetary hypsometry for Earth-like and Venus-like instellations. Higher probabilities imply that the model is more likely to reach temperatures above 400 K. Models with Earth-like hypsometry and instellation are shown in blue shades, and models with Venus-like hypsometry and instellation are shown in orange shades, similar to Figure 7. Models with Earth-like hypsometry but Venus-like instellation are denoted by shades of gray. Lighter shades of any color denote the surface-dependent deep-water cycle.

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