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      Thermodynamic and Energetic Limits on Continental Silicate Weathering Strongly Impact the Climate and Habitability of Wet, Rocky Worlds

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          Abstract

          The "liquid water habitable zone" (HZ) concept is predicated on the ability of the silicate weathering feedback to stabilize climate across a wide range of instellations. However, representations of silicate weathering used in current estimates of the effective outer edge of the HZ do not account for the thermodynamic limit on concentration of weathering products in runoff set by clay precipitation, nor for the energetic limit on precipitation set by planetary instellation. We find that when the thermodynamic limit is included in an idealized coupled climate/weathering model, steady-state planetary climate loses sensitivity to silicate dissolution kinetics, becoming sensitive to temperature primarily through the effect of temperature on runoff and to pCO\(_2\) through an effect on solute concentration mediated by pH. This increases sensitivity to land fraction, CO\(_2\) outgassing, and geological factors such as soil age and lithology, all of which are found to have a profound effect on the position of the effective outer edge of the HZ. The interplay between runoff sensitivity and the energetic limit on precipitation leads to novel warm states in the outer reaches of the HZ, owing to the decoupling of temperature and precipitation. We discuss strategies for detecting the signature of silicate weathering feedback through exoplanet observations in light of insights derived from the revised picture of weathering.

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          Author and article information

          Journal
          29 April 2020
          Article
          2004.14058
          6a309825-5afe-413a-840c-eed9f3132055

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          27 pages excluding references, 8 figures. Submitted to ApJ, revised, resubmitted
          astro-ph.EP

          Planetary astrophysics
          Planetary astrophysics

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