Marine snowstorm during the Permian–Triassic mass extinction

Author:

Grasby Stephen E.1ORCID,Ardakani Omid H.1,Liu Xiaojun1,Bond David P.G.2,Wignall Paul B.3,Strachan Lorna J.4

Affiliation:

1. 1Geological Survey of Canada, 3303 33rd Street NW Calgary, AB T2L-2A7, Canada

2. 2School of Environmental Sciences, University of Hull, Hull HU6 7RX, UK

3. 3School of Earth and Environment, University of Leeds, Woodhouse Lane, Leeds LS2 9JT, UK

4. 4School of Environment, University of Auckland, Auckland, 1142, New Zealand (Aotearoa)

Abstract

Abstract 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.

Publisher

Geological Society of America

Subject

Geology

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