Astronomical age constraints and extinction mechanisms of the Late Triassic Carnian crisis

Publication date

2017-06-01

Authors

Miller, Charlotte S.ISNI 0000000524240217
Peterse, FrancienORCID 0000-0001-8781-2826ISNI 0000000492917456
Da Silva, Anne-ChristineISNI 0000000456975704
Baranyi, Viktória
Reichart, G.-J.ISNI 0000000049622557
Kürschner, Wolfram MichaelISNI 0000000396347414

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Abstract

The geological record contains evidence for numerous pronounced perturbations in the global carbon cycle, some of which are associated with mass extinction. In the Carnian (Late Triassic), evidence from sedimentology and fossil pollen points to a significant change in climate, resulting in biotic turnover, during a time termed the 'Carnian Pluvial Episode' (CPE). Evidence from the marine realm suggests a causal relationship between the CPE, a global 'wet' period, and the injection of light carbon into the atmosphere. Here we provide the first evidence from a terrestrial stratigraphic succession of at least five significant negative C-isotope excursions (CIE)'s through the CPE recorded in both bulk organic carbon and compound specific plant leaf waxes. Furthermore, construction of a floating astronomical timescale for 1.09 Ma of the Late Triassic, based on the recognition of 405 ka eccentricity cycles in elemental abundance and gamma ray (GR) data, allows for the estimation of a duration for the isotope excursion(s). Source mixing calculations reveal that the observed substantial shift(s) in δ(13)C was most likely caused by a combination of volcanic emissions, subsequent warming and the dissociation of methane clathrates.

Keywords

SDG 13 - Climate Action, SDG 14 - Life Below Water

Citation

Miller, C S, Peterse, F, da Silva, A-C, Baranyi, V, Reichart, G J & Kürschner, W M 2017, 'Astronomical age constraints and extinction mechanisms of the Late Triassic Carnian crisis', Scientific Reports, vol. 7, no. 1, 2557. https://doi.org/10.1038/s41598-017-02817-7