SULFUR ISOTOPIC EVIDENCE FOR CHEMOCLINE UPWARD EXCURSIONS DURING THE END-PERMIAN MASS EXTINCTION

dc.contributor.authorRiccardi A.L.
dc.contributor.authorArthur M.A.
dc.contributor.authorKump L.R.
dc.date.accessioned2024-09-04T09:55:42Z
dc.date.available2024-09-04T09:55:42Z
dc.date.issued2006
dc.description.abstractThe latest Permian was a time of major change in ocean chemistry, accompanying the greatest mass extinction of the Phanerozoic. To examine the nature of these changes, samples from two well-studied marine sections that span the Permian-Triassic boundary have been analyzed: the Meishan and Shangsi sections located in Southern China. Isotopic analysis of the carbonate-associated sulfate in these samples provides a detailed record of several isotopic shifts in δ34SCAS approaching and across the PTB, ranging from +30 to -15‰ (VCDT), with repeated asynchronous fluctuations at the two locations. We interpret the patterns of isotopic shifts, in conjunction with other data, to indicate a shallow unstable chemocline overlying euxinic deep-water which periodically upwelled into the photic zone. These chemocline upward excursion events introduced sulfide to the photic zone stimulating a bloom of phototrophic sulfur oxidizing bacteria. We hypothesize that elemental sulfur globules produced by these organisms and 34S-depleted pyrite produced in the euxinic water column were deposited in the sediment; later oxidation led to incorporation as CAS. This created the large changes to the δ34SCAS observed in the latest Permian at these locations. © 2006 Elsevier Inc. All rights reserved.
dc.identifierhttps://www.elibrary.ru/item.asp?id=31357241
dc.identifier.citationGeochimica et Cosmochimica Acta, 2006, 70, 23 SPEC. ISS., 5740-5752
dc.identifier.doi10.1016/j.gca.2006.08.005
dc.identifier.issn0016-7037
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/44942
dc.subject.ageМезозой::Триасовая
dc.subject.ageПалеозой::Пермская
dc.subject.ageMesozoic::Triassic
dc.subject.agePaleozoic::Permian
dc.titleSULFUR ISOTOPIC EVIDENCE FOR CHEMOCLINE UPWARD EXCURSIONS DURING THE END-PERMIAN MASS EXTINCTION
dc.typeСтатья

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