Notice: This is an archived and unmaintained page. For current information, please browse

What We Talk About When We Talk About Reverse Weathering

Presenter: Noah Planavsky, Yale University
When: November 6, 2018 3PM PST

Despite a Sun with lowered luminosity, the early Earth was marked by apparent climate stability, with rare catastrophic glaciations. I will make a case that elevated rates of reverse weathering-the consumption of alkalinity and the release of acidity accompanying clay authigenesis-releases a flux of CO2 to the atmosphere that would have sustained a significantly elevated pCO2 baseline. Although dampened by sluggish kinetics today, more prolific rates of reverse weathering persisted under the pervasively silica-rich conditions that dominated early oceans. As little as 20-30% of marine dissolved silica burial through the reverse weathering sink would have successfully maintained the equable and ice-free environment that characterized most of the Precambrian. Further, during this time, a dynamic negative feedback in which marine pH controlled authigenic clay formation would have prevented large swings in atmospheric CO2 concentrations. The ecological rise of siliceous organisms would have removed this reverse weathering buffer, destabilizing Earth’s climate system, and lowering baseline CO2 levels. We likely need to incorporate reverse weathering into the framework we use to think about planetary habitability and the habitable lifespan of a planet.

University of Washington Seminars

  • The University of Washington seminar series is hosted by the NAI Virtual Planetary Lab (VPL) team live from the University of Washington campus in Seattle.
  • Subscribe to this series

Other Seminars in this Series