Researches in Organic Geochemistry
Online ISSN : 2189-7891
Print ISSN : 1344-9915
ISSN-L : 1344-9915
Volume 32, Issue 2
Displaying 1-2 of 2 articles from this issue
Review
  • Ryosuke Saito
    2016 Volume 32 Issue 2 Pages 19-53
    Published: December 30, 2016
    Released on J-STAGE: April 04, 2017
    JOURNAL FREE ACCESS

    The mass extinction at the end of Permian was the severest crisis in the Earth’s history. Oceanic euxinia and acidification as well as global warming all have been hypothesized as causes for the mass extinction. However, oceanic euxinia occurred much earlier than the mass extinction, and oceanic acidification and global warming postdated. Accordingly, the cause for the end-Permian mass extinction is not fully understood. Organic geochemical studies have been the most extensively performed for the mass extinction event, and revealed important findings such as soil erosion, photic zone euxinia, and proliferation of cyanobacteria for the event. Recovery from the mass extinction was much delayed and took place in the Middle Triassic, after 5 million years from the mass extinction. Subsequently, the Early Triassic period is the transition interval from the mass extinction to the recovery. The environments in the Early Triassic were rather instable, and another mass extinctions and recoveries repeatedly occurred. Organic geochemical studies have suggested photic zone euxinia, stressful environments, and an occurrence of a previously undiscovered type of microbialite during the Early Triassic. In the present paper, I introduce the evidences of environmental and biotic changes through the end-Permian mass extinction to the Early Triassic.

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