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A Whole-planet Model of the Earth without Life for Terrestrial Exoplanet Studies

  • Authors: Samantha Gilbert-Janizek, Rory K. Barnes, Peter E. Driscoll, Nicholas F. Wogan, Avi M. Mandell, Jessica L. Birky, Ludmila Carone, Rodolfo Garcia

Samantha Gilbert-Janizek et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Properties of the ocean as a function of time. (a) After 4.5 Gyr, 1 TO has entered the mantle, ultimately leaving 1 TO on the surface. (b) The concentration of CO2 in the oceans tracks closely with the atmospheric CO2 inventory, following Henry’s law. (c) Prior to equilibration, the pH initially spikes because the initial concentrations of carbonate and bicarbonate in the calcite-saturated oceans are also very high. Following equilibration, the pH gradually becomes more alkaline as the abundance of CO2 in the atmosphere and ocean gradually decreases. (d) The total DIC at the ocean surface, which includes aqueous CO2, carbonate, and bicarbonate, tracks closely with the atmospheric CO2 budget. On all plots, dots represent measurements of PIE (4.5 Gyr) properties with uncertainties.

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