Abstract

Abstract. It is commonly accepted that the mass extinction associated with the Cretaceous–Paleogene (K–Pg) boundary (∼ 66 Ma) is related to the environmental effects of a large extraterrestrial impact. The biological and oceanographic consequences of the mass extinction are, however, still poorly understood. According to the Living Ocean model, the biological crisis at the K–Pg boundary resulted in a long-term reduction of export productivity in the early Paleocene. Here, we combine organic-walled dinoflagellate cyst (dinocyst) and benthic foraminiferal analyses to provide new insights into changes in the coupling of pelagic and benthic ecosystems. To this end, we perform dinocyst and benthic foraminiferal analyses on the recently discovered Tethyan K–Pg boundary section at Okçular, Turkey, and compare the results with other K–Pg boundary sites in the Tethys. The post-impact dominance of epibenthic morphotypes and an increase of inferred heterotrophic dinocysts in the early Paleocene at Okçular are consistent with published records from other western Tethyan sites. Together, these records indicate that during the early Paleocene more nutrients remained available for the Tethyan planktonic community, whereas benthic communities were deprived of food. Hence, in the post-impact phase the reduction of export productivity likely resulted in enhanced recycling of nutrients in the upper part of the water column, all along the western Tethyan margins.

Highlights

  • It is commonly accepted that the Cretaceous–Paleogene (K–Pg) boundary (∼ 66 Ma) mass extinction was associated with the impact of a large extraterrestrial body at Chicxulub, Yucatan, Mexico

  • Since export productivity was greatly reduced after the K–Pg boundary mass extinction, very little “new” organic matter reached the sea floor after the initial post-impact influx

  • Based on the succession of benthic faunal assemblages at a number of Tethyan margin sites, four phases can be recognized across the K–Pg boundary interval: the Maastrichtian or pre-impact phase (I), a disaster phase (II), a recovery phase (III), and an early Paleocene post-recovery phase (IV)

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Summary

Introduction

It is commonly accepted that the Cretaceous–Paleogene (K–Pg) boundary (∼ 66 Ma) mass extinction was associated with the impact of a large extraterrestrial body at Chicxulub, Yucatan, Mexico. The short- and long-term environmental implications of this impact resulted in the extinction of a large number of biological clades (Sepkoski, 1996). Paleontological records indicate that approximately 50 % of marine genera became extinct across the K–Pg boundary. This episode represents one of the largest mass-extinction events in Earth history (Sepkoski, 1996; D’Hondt, 2005). Apart from short-term global environmental consequences, such as an initial “impact winter” phase (Alvarez et al, 1980; Vellekoop et al, 2014, 2016), the event had major longterm biological consequences.

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