Lithologic Controls on Silicate Weathering Regimes of Temperate Planets
Kaustubh Hakim, Dan J. Bower, Meng Tian, Russell Deitrick, Pierre, Auclair-Desrotour, Daniel Kitzmann, Caroline Dorn, Klaus Mezger, Kevin Heng

TL;DR
This study models how different rock types influence silicate weathering rates on temperate planets, revealing lithology-dependent regimes and potential climate feedbacks crucial for planetary habitability.
Contribution
It introduces a thermodynamic and fluid-transport model to quantify lithology-specific weathering rates, highlighting the importance of mineral assemblages over individual minerals.
Findings
Weathering rates vary significantly between continental and oceanic crust lithologies.
Thermodynamics dominate weathering control at low CO2 or high temperatures.
Weathering regimes depend on lithology and can influence climate feedback mechanisms.
Abstract
Weathering of silicate rocks at a planetary surface can draw down CO from the atmosphere for eventual burial and long-term storage in the planetary interior. This process is thought to provide an essential negative feedback to the carbonate-silicate cycle (carbon cycle) to maintain clement climates on Earth and potentially similar temperate exoplanets. We implement thermodynamics to determine weathering rates as a function of surface lithology (rock type). These rates provide upper limits that allow estimating the maximum rate of weathering in regulating climate. This modeling shows that the weathering of mineral assemblages in a given rock, rather than individual minerals, is crucial to determine weathering rates at planetary surfaces. By implementing a fluid-transport controlled approach, we further mimic chemical kinetics and thermodynamics to determine weathering rates for three…
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