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Titel 87/86Sr, 143/144Nd, HFSE, REE, and PGE variations across the K-Pg boundary at Site 1259, ODP Leg 207 (Western Atlantic)
VerfasserIn A. Deutsch, J. Berndt, K. Mezger, P. Schulte
Konferenz EGU General Assembly 2009
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 11 (2009)
Datensatznummer 250023815
 
Zusammenfassung
The exceptionally well preserved, not bio-turbated, about 2- to 3-cm-thick spherule layer occurring in 6 of 13 cores from ODP Leg 207 (Demerara Rise, ~4500 km off the Chicxulub crater center) is ideally suited for tracing chemical changes related to the deposition of Chicxulub ejecta at the Cretaceous-Paleogene (K-Pg) boundary. We have analyzed Sr-Nd isotope systematics on hand-picked separates (spherules, matrix; Site 1259B) using TIMS, and the variation of 34 trace elements in the upper 5 mm of the ejecta sequence at Site 1259C using La-ICP-MS with a spot size of 235 µm (Inst. f. Mineralogie WWU). The micro-chemical study allows separation of the different components that have contributed to this spectacular layer. These are (i) projectile matter exemplified in the maximum Pt and Ir concentrations of ~0.1 and 0.04 ppm, respectively, in the uppermost one millimeter of the spherule layer, (ii) ejected mafic material, identified by low Ni/Cr ratios and rather flat chondrite-normalized REE, (iii) ejected silica-rich material (shocked quartz, feldspar, and lithic clasts), (iv) ejected carbonate clasts, (v) wash-off from the nearby Guayana cration, recognized by strongly negative time-corrected epsilon(Nd) of -17, and very exotic Zr/Hf and Nb/Ta ratios of 20.5 +- 1.0, and 5.4 +- 0.8, respectively, as well as by steeper REE patterns, and (vi) the contemporaneous seawater, given by Sr isotope ratios around 0.708. The time-span contained in this layer is constrained by the settling time of the larger spherules (about 2 days), and the residence times of Nd in the ocean (200 to 1000 yrs.; HFSE may a residence time on the same order of magnitude); alteration of the spherules to smectite, and uptake of Sr from the ocean may have happened later. Our reconnaissance study demonstrates the extraordinary potential of isotope studies with a high spatial resolution for unravelling the complexities of ejecta layers.