EGU24-20588, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-20588
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Marine snowstorm during the Permian−Triassic mass extinction  

Stephen Grasby, Omid Ardakani, Xiaojun Liu, David Bond, Paul Wignall, and Lorna Strachan
Stephen Grasby et al.
  • Geological Survey of Canada, Calgary, Canada (steve.grasby@canada.ca)

The Permian−Triassic mass extinction (PTME) interval is marked by major excursions in both inorganic and organic carbon (C) isotopes. Carbon cycle models predict that these trends were driven by large increases in productivity, yet organic C−rich rocks are not recorded in most PTME shelf sedimentary successions. Anomalous C-rich facies have been reported from rare abyssal plains records now exposed in Japan and New Zealand, where black shales at the PTME are extraordinarily organic-rich units. We examined organic matter at the Waiheke, New Zealand, section, and results show that these deposits are dominated by lamalginites composed of unicellar solitary or colonial phytoplankton produced during algal blooms that falls as “marine snow.” We modeled the impact of ash fall from eruptions in the Siberian Traps large igneous province and argue that they fertilized the Panthalassa Ocean with P and Fe, leading to a marine “snowstorm” and significant C drawdown marking this major biobloom during the PTME.

How to cite: Grasby, S., Ardakani, O., Liu, X., Bond, D., Wignall, P., and Strachan, L.: Marine snowstorm during the Permian−Triassic mass extinction  , EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-20588, https://doi.org/10.5194/egusphere-egu24-20588, 2024.