CARBON SULFUR IRON SYSTEMATICS OF THE UPPERMOST DEEP-WATER SEDIMENTS OF THE BLACK-SEA

被引:170
作者
LYONS, TW [1 ]
BERNER, RA [1 ]
机构
[1] YALE UNIV,DEPT GEOL & GEOPHYS,NEW HAVEN,CT 06511
基金
美国国家科学基金会;
关键词
D O I
10.1016/0009-2541(92)90028-4
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Box cores recovered during Leg 4 of the 1988 R/V "Knorr" Black Sea Oceanographic Expedition from deep-water regions of the basin were dominated by coccolith-rich, microlaminated (Unit 1) sediment and muddy, gray turbidite layers. Both organic carbon (OC) and pyrite sulfur values for Unit 1 display narrow ranges, with mean concentrations of 5.3 +/- 1.1 (1sigma) wt% and 1.3 +/- 0.3 wt%, respectively. Unit 1 is not enriched in pyrite-S relative to sediments deposited under oxygenated bottom waters (normal marine sediments) with comparable OC concentrations. Carbon-sulfur relationships (evaluated on a calcium carbonate-free basis to avoid spurious correlations resulting from dilution effects) demonstrate that OC and pyrite-S are essentially decoupled. These observations, combined with the persistence of elevated pore-water sulfide to depth and a strong correlation between pyrite-S and the detrital Fe component argue strongly for limitation of pyrite formation in Unit 1 by the availability of reactive Fe. Unit-1 Fe limitation is further indicated by degree-of-pyritization (DOP) studies (a measure of the extent to which the original potentially reactive Fe has been transformed to pyrite). These studies show sulfidation of reactive Fe ranging from 57% to 78%, with DOP values independent of OC concentration. Unit-1 DOP profiles suggest that the majority of the pyrite is formed in the sulfidic water column and/or very close to the sediment-water interface. Pyrite-S concentrations of Unit 1, when compared with the particulate reduced sulfur fluxes measured in time-series sediment traps, are compatible with predominantly water-column pyrite formation. Because of the limitations in the supply of reactive Fe associated with the comparatively high supply of OC, the microlaminated sediment is characterized by C/S ratios greater than those typical of Holocene oxically deposited sediments. The turbidite muds of the deep basin display high reduced S values (relative to Holocene normal marine sediments) in samples with low OC concentrations (low C/S ratios). This reflects pyrite formation under anoxic-sulfidic bottom-water conditions in a probable upper-slope source region, as well as during transport and final deposition. Intermediate DOP values for the turbidites, in part a product of their rapid rate of deposition, reveal that Fe limitation is ultimately not a factor and that further pyrite should form during burial. However, the very rapid rate at which Unit-1 pyrite forms suggests fundamental differences between the overall reactivities of the Fe phases associated with the microlaminated and turbiditic sediments. The signature of water-column anoxia with regard to sedimentary pyrite formation is clearly indicated by the high DOP values of Unit 1 and the comparatively high levels of S associated with the low concentrations of OC of the turbidite muds. This agrees with similar conclusions based on studies of ancient sedimentary rocks.
引用
收藏
页码:1 / 27
页数:27
相关论文
共 94 条
[1]  
ALBERT DB, 1988, T AM GEOPHYS UNION, V69, P1241
[2]   C-S-FE RELATIONSHIPS AND THE ISOTOPIC COMPOSITION OF PYRITE IN THE NEW ALBANY SHALE OF THE ILLINOIS BASIN, USA [J].
ANDERSON, TF ;
KRUGER, J ;
RAISWELL, R .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1987, 51 (10) :2795-2805
[3]  
[Anonymous], 1977, SOC EC PALEONTOLOGIS, DOI DOI 10.2110/PEC.77.25
[4]  
ARTHUR MA, 1988, TEMPORAL SPATIAL VAR, P109
[5]  
BEIER JA, 1989, GEOL SOC AM BULL, V101, P774, DOI 10.1130/0016-7606(1989)101<0774:GAIEFP>2.3.CO
[6]  
2
[7]  
BEIER JA, 1990, T AM GEOPHYS UNION, V71, P151
[8]   SEDIMENTARY PYRITE FORMATION [J].
BERNER, RA .
AMERICAN JOURNAL OF SCIENCE, 1970, 268 (01) :1-&
[9]   BURIAL OF ORGANIC-CARBON AND PYRITE SULFUR IN SEDIMENTS OVER PHANEROZOIC TIME - A NEW THEORY [J].
BERNER, RA ;
RAISWELL, R .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1983, 47 (05) :855-862
[10]  
BERNER RA, 1984, GEOLOGY, V12, P365, DOI 10.1130/0091-7613(1984)12<365:CMFDFF>2.0.CO