Saved in:
Bibliographic Details
Main Authors: Martinez-Ruiz, Francisca C, Kastner, Miriam, Paytan, Adina, Ortega-Huertas, M, Bernasconi, Stefano M
Format: Dataset Open Access
Language:en
Published: PANGAEA 2000
Subjects:
Online Access:https://doi.org/10.1594/PANGAEA.738508
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1867169500960391168
author Martinez-Ruiz, Francisca C
Kastner, Miriam
Paytan, Adina
Ortega-Huertas, M
Bernasconi, Stefano M
author_facet Martinez-Ruiz, Francisca C
Kastner, Miriam
Paytan, Adina
Ortega-Huertas, M
Bernasconi, Stefano M
collection Datos científicos de ciencias marinas y ambientales
contents The geochemistry of the youngest Mediterranean sapropel layer suggests changes in productivity and water column oxygen conditions during sapropel deposition. The Ba-enriched interval is broader than the organic-carbon-rich interval of this sapropel. We suggest that the Ba-enriched horizon records the original thickness of the sapropel prior to subsequent partial oxidation. The main carrier of Ba is barite, as microcrystals (0.5-5 µm ) having a morphology characteristic of marine barite, particularly abundant beneath high productivity regions. Ba concentrations do not change at the sapropel layer oxidation front and diagenetic barite crystals are absent, thus the Ba-enriched layer reflects original oceanic conditions of increased biological productivity during sapropel deposition and not diagenetic Ba remobilization. Paleoredox indicators point to restricted oxygenated bottom water but not to fully anoxic conditions. Detrital elements within this layer indicate a lower eolian terrigenous input, enhanced humidity, and increased precipitation/runoff, thus likely higher nutrient supply.
format Dataset Open Access
id pangaea_https___doi_org_10_1594_PANGAEA_738508
institution PANGAEA
language en
publishDate 2000
publisher PANGAEA
record_format pangaea
spellingShingle Geochemistry on sapropel deposition in the eastern Mediterranean from cores TTR-GL94 and M25/4-KL11
Martinez-Ruiz, Francisca C
Kastner, Miriam
Paytan, Adina
Ortega-Huertas, M
Bernasconi, Stefano M
25/4-11; GC; Gravity corer; KL; M25/4; M25/4-KL11; Mediterranean Sea; Meteor (1986); Piston corer (BGR type); TTR-GL94
The geochemistry of the youngest Mediterranean sapropel layer suggests changes in productivity and water column oxygen conditions during sapropel deposition. The Ba-enriched interval is broader than the organic-carbon-rich interval of this sapropel. We suggest that the Ba-enriched horizon records the original thickness of the sapropel prior to subsequent partial oxidation. The main carrier of Ba is barite, as microcrystals (0.5-5 µm ) having a morphology characteristic of marine barite, particularly abundant beneath high productivity regions. Ba concentrations do not change at the sapropel layer oxidation front and diagenetic barite crystals are absent, thus the Ba-enriched layer reflects original oceanic conditions of increased biological productivity during sapropel deposition and not diagenetic Ba remobilization. Paleoredox indicators point to restricted oxygenated bottom water but not to fully anoxic conditions. Detrital elements within this layer indicate a lower eolian terrigenous input, enhanced humidity, and increased precipitation/runoff, thus likely higher nutrient supply.
title Geochemistry on sapropel deposition in the eastern Mediterranean from cores TTR-GL94 and M25/4-KL11
topic 25/4-11; GC; Gravity corer; KL; M25/4; M25/4-KL11; Mediterranean Sea; Meteor (1986); Piston corer (BGR type); TTR-GL94
url https://doi.org/10.1594/PANGAEA.738508