Angiolini, L.

Brand, U.

Eisenhauer, Anton

Flögel, Sascha

Garbelli, C.

Gutjahr, Marcus

Jurikova, Hana

Liebetrau, Volker

Posenato, R.

Wallmann, Klaus

OceanRep

Goldschmidt2017 Abstract  Decoupled δ11B and δ13C during the Late Permian: Implications for carbon cycle perturbations during the mass extinction event H. JURIKOVA1*, M. GUTJAHR1, K. WALLMANN1, V. LIEBETRAU1,  S. FLÖGEL1, U. BRAND2, R. POSENATO3, C. GARBELLI4, L. ANGIOLINI5 AND A. EISENHAUER1 1GEOMAR Helmholtz-Zentrum für Ozeanforschung Kiel, Germany (*correspondence: hjurikova@geomar.de) 2Department of Earth Sciences, Brock University, St. Catharines, Ontario, Canada 3Dipartimento di Scienze della Terra, Università di Ferrara, Polo Scientifico-tecnologico, Ferrara, Italy 4State Key Laboratory of Paleobiology and Stratigraphy, Nanjing Institute of Geology and Palaeontology, Chinese Academy of Sciences, Jiangsu, P.R. China 5Dipartimento di Scienze della Terra, Università di Milano, Milan, Italy  The Permian-Triassic boundary (PTB) witnessed the most severe environmental and biotic crisis identified in the Earth’s geological record. Current lines of evidence on causation point towards massive flood-basalt volcanism from Siberian traps, involving a combination of global warming by ~6°C, substantial input of relatively light carbon to the atmosphere, sporadic anoxia or euxinia, and ocean acidification. In order to reconstruct potential changes in seawater chemistry during this time interval, we examined the boron isotope composition (δ11B) of pristine brachiopod shells. Although to date hardly applied in Paleozoic settings such as the PTB [1], the δ11B of marine calcium carbonate is considered to be one of the most reliable paleo-pH proxies [e.g. 2], providing the archive is free from post-depositional diagenetic alterations. Using selected δ11B to pH relationships and bulk seawater δ11B scenarios, we present a high-resolution seawater pH record for the Western Tethys covering ~10 ky [3] during the latest phase of the Permian extinction [4]. This interval recorded a negative δ13C excursion (CIE) in excess of ~4 ‰ preceding the extinction event by a few millennia [5]. Our δ11B results show a maximum variation between 12.9 and 14.3 ‰ throughout the record, yet suggesting none to minor pH change during the CIE. Given the very good preservation of our specimens, this finding may argue against pronounced ocean acidification or point to pH buffering mechanisms associated with CIE. Combined with a quantitative modelling approach we delineate potential atmospheric and oceanic conditions and changes in the carbon budget involved.   [1] Clarkson et al. (2015) Science 348, 229-232. [2] Foster (2008) EPSL 271, 254-266. [3] Posenato (2010) Geol. J. 45, 195-215. [4] Song et al. (2012) Nat. Geosci. 6, 52-56. [5] Brand et al. (2012) Chem. Geol. 323, 121-144. 

Decoupled δ11B and δ13C during the Late Permian: Implications for Carbon Cycle Perturbations during the Mass Extinction Event

http://oceanrep.geomar.de/45927/1/1899.pdf

Decoupled δ11B and δ13C during the Late Permian: Implications for Carbon Cycle Perturbations during the Mass Extinction Event

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