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Geodynamic impact on the stable isotope signatures in a shallow epicontinental sea
Author(s) -
Harzhauser Mathias,
Piller Werner E.,
Latal Christine
Publication year - 2007
Publication title -
terra nova
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.353
H-Index - 89
eISSN - 1365-3121
pISSN - 0954-4879
DOI - 10.1111/j.1365-3121.2007.00755.x
Subject(s) - geology , seawater , stable isotope ratio , paleontology , precipitation , geodynamics , ocean current , oceanography , tethys ocean , isotopes of oxygen , isotope , paleoceanography , tectonics , geochemistry , subduction , physics , quantum mechanics , meteorology
Analyses were made of a mollusc‐based meta dataset of 859 δ 13 C and δ 18 O data of Miocene nearshore settings in the European Paratethys Sea and its descendant Lake Pannon. The observed trends document a strong tie to geodynamics, which are largely decoupled from Miocene open ocean isotope curves. Semi‐ to fully enclosed, initially marine water bodies such as the Paratethys Sea are prone to switching seawater isotope signatures because they respond rapidly to changes in the evaporation/precipitation ratio. Two phases of positive deviations of oxygen isotope values of water (relative to the modern ocean value, SMOW) occurred during the Middle Miocene; both were initiated by tectonic constrictions of the seaways and became amplified by global warming and regionally decreasing precipitation. With the final disintegration of the Paratethys, the marine isotope signatures vanish. Instead, the observed isotope trends suggest a comparably simple system of an alkaline lake with steadily declining salinity. The ‘ocean‐derived’ Paratethys Sea may thus act as a key for understanding isotope trends in epicontinental seas.