Preprints
https://doi.org/10.5194/cp-2021-180
https://doi.org/10.5194/cp-2021-180

  20 Dec 2021

20 Dec 2021

Review status: this preprint is currently under review for the journal CP.

Climate and Ocean Circulation in the Aftermath of a Marinoan Snowball Earth

Lennart Ramme1,2 and Jochem Marotzke1,3 Lennart Ramme and Jochem Marotzke
  • 1Max-Planck-Institute for Meteorology, Hamburg, Germany
  • 2International Max Planck Research School on Earth System Modelling, Hamburg, Germany
  • 3Center for Earth System Research and Sustainability (CEN), Universität Hamburg, Germany

Abstract. When a snowball Earth deglaciates through a very high atmospheric CO2 concentration, the resulting inflow of freshwater leads to a stably stratified ocean, and the strong greenhouse conditions drive the climate into a very warm state. Here, we use a coupled atmosphere-ocean general circulation model, applying different scenarios for the evolution of atmospheric CO2, to conduct the first simulation of the climate and the three-dimensional ocean circulation in the aftermath of the Marinoan snowball Earth. The simulations show that the strong freshwater stratification breaks up on a timescale in the order of 103 years, mostly independent of the applied CO2 scenario. This is driven by the upwelling of salty waters in high latitudes, mainly the northern hemisphere, where a strong circumpolar current dominates the circulation. In the warmest CO2 scenario, the simulated Marinoan supergreenhouse climate reaches a global mean surface temperature of about 30 °C under an atmospheric CO2 concentration of 15 × 103 parts per million by volume, which is a moderate temperature compared to previous estimates. Consequently, the thermal expansion of seawater causes a sea-level rise of only 8 m, with most of it occurring during the first 3000 years. Our results imply that the surface temperatures of that time were potentially not as threatening for early metazoa as previously assumed. Furthermore, the short destratification timescale found in this study implies a very rapid accumulation of Marinoan cap dolostones, given that they were deposited in a freshwater environment.

Lennart Ramme and Jochem Marotzke

Status: open (until 14 Feb 2022)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on cp-2021-180', Anonymous Referee #1, 17 Jan 2022 reply

Lennart Ramme and Jochem Marotzke

Model code and software

Publication data for “Ramme and Marotzke: Climate and Ocean Circulation in the Aftermath of a Marinoan Snowball Earth” Lennart Ramme https://cera-www.dkrz.de/WDCC/ui/cerasearch/entry?acronym=DKRZ_LTA_033_ds00011

Lennart Ramme and Jochem Marotzke

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Short summary
After the Marinoan snowball Earth, the climate warmed rapidly due to enhanced greenhouse conditions, and the freshwater inflow of melting glaciers caused a strong stratification of the ocean. Our climate simulations reveal a potentially only moderate global temperature increase and a break up of the stratification within just a few thousand years. The findings give insights into the environmental conditions relevant for the geological and biological evolution during that time.