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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 2.

Precipitation estimated analytically for different surface temperatures assuming wind-driven evaporation limits (lines, R. T. Pierrehumbert 2010) is compared to the weighted average of precipitation from GCM runs of arid planets (dots, M. J. Way & A. D. Del Genio (2020; and square markers, D. M. Glaser et al. 2025). The average surface temperature associated with the calculated wind-driven precipitation and the GCM outputs are represented by a color heatmap. The M. J. Way & A. D. Del Genio (2020) GCM models tested five discrete land fractions, resulting in the five distinct dot groups. Broadly speaking the analytic precipitation-limited estimate of precipitation agrees with or overestimates precipitation from the GCMs.

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