4.7 Article

Cooling-driven oceanic anoxia across the Smithian/Spathian boundary (mid-Early Triassic)

Journal

EARTH-SCIENCE REVIEWS
Volume 195, Issue -, Pages 133-146

Publisher

ELSEVIER
DOI: 10.1016/j.earscirev.2019.01.009

Keywords

Organic carbon burial; Carbon isotopes; Sulfur isotopes; Primary productivity; South China

Funding

  1. Natural Science Foundation of China [41872033, 41402302, 41530414, 41661134047]
  2. Research Program the State Key Laboratory of Palaeobiology and Stratigraphy [143106]
  3. Natural Science Foundation of Hubei [2017CFB610]
  4. Sedimentary Geology and Paleobiology program of the U.S. National Science Foundation
  5. NASA Exobiology program
  6. State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences-Wuhan
  7. Agouron
  8. U.S. National Science Foundation
  9. IGCP Projects [572, 630]

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The Smithian/Spathian boundary (SSB) represents a major climatic-oceanic-biotic event within the similar to 5-Myr-long recovery interval of the Early Triassic following the end-Permian mass extinction. The SSB was associated with pronounced cooling following the middle Smithian hyper-greenhouse, a similar to +2 to + 8 parts per thousand positive carbon isotope excursion, and a second-order mass extinction, yet its underlying cause(s) remain poorly understood. Here, we review oceanic environmental changes during the middle Smithian to early Spathian interval and their potential mechanisms. In addition, we undertook an analysis of the carbon-sulfur-iron (C-S-Fe) systematics of the South Majiashan section, which was located on the paleo-western margin of the South China Craton during the Early Triassic, to better understand the causation of these environmental changes. This analysis revealed low delta C-13(carb)(ie., the N3 minimum) in the middle Smithian but rapidly rising delta C-13(carb) (i.e., to the P3 maximum) and delta S-34(CAS) within the SSB interval (i.e., late Smithian-earliest Spathian). Both the middle Smithian and SSB intervals are marked by development of marine euxinia, which we hypothesize had fundamentally different causes. The middle Smithian was associated with hyperwarming (the Smithian Thermal Maximum), which was probably triggered by a peak in magmatic activity of the Siberian Traps LIP. In contrast, the SSB interval was associated with global climatic cooling, which may have stimulated oceanic overturning circulation and upwelling on continental margins, leading to transient local increases in marine productivity and expansion of oceanic oxygen-minimum zones (OMZs). The concurrent positive excursions in delta C-13(carb) and delta S-34(CAS) at South Majiashan and other sections worldwide are evidence of enhanced burial of organic carbon and pyrite on a regional or global scale, as well as of a concurrent decline in atmospheric pCO(2) that may have positively re-enforced the SSB cooling event.

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