Abstract
Anoxic hypersaline basins have been found in two different tectonic
environments in the eastern Mediterranean. Within the Tyro area (the
western Strabo Trench) there are three pull apart basins: the Tyro
Basin, presently filled with anoxic hypersaline bottomwater, and the
Poseidon and Kretheus Basins, thought to have been anoxic and filled
with hypersaline water in
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the past. The Mediterranean Ridge shows a
"cobblestone topography" (Camerlenghi, 1990). The Bannock Basin is
the largest depression found within this area and is divided into nine
sub-basins. Tectonic deformations of Messinian evaporites are thought
to be the major processes involved in the formation of these anoxic
hypersaline basins.
The interstitial water chemistry of sediments from these basins have
been studied. The fact that the Poseidon and Kretheus Basins have
been filled with hypersaline bottomwater is reflected by an increase of
the CI and Na concentration in the pore waters downcore. These brines
are thought to have been similar to that of the Tyro Basin. A diffusionadvection
model has been applied to the CI profiles. From time
calculations it was possible to estimate the time elapsed since
hypersaline conditions in the Poseidon and Kretheus Basins changed
into normal saline conditions. A renewal time between 2000 - 3000
years was found.
Organic matter reaching the sediments is decomposed by sulphate
reducing bacteria. Despite the high salinity (260 %0) in the Tyro and
Bannock Basins, sulphate reduction rates are higher than in the
sediments from the Poseidon and Kretheus Basins. These higher
sulphate reduction rates could be related to a better "preservation" of
the organic matter in the anoxic brine. The release of inorganic
metabolites, such as ammonium, alkalinity, phosphate and sulphide
leads to the formation of authigenic minerals in these sediments such
as dolomite, gypsum and sulphides.
The sulphur chemistry in the anoxic hypersaline sediments from the
Tyro and Bannock Basins have been studied in detail. Despite the
difference in major element chemistry of the brines (De Lange et aI.,
1990a) their sulphur chemistry in the sediments is very similar. The
following sulphur species have been determined and quantified:
elemental sulphur, Acid Volatile Sulphur (AVS), organic polysulphides,
humic sulphur (0.5 M NaOH extractable) and pyritic sulphur. Pyritic
sulphur was found to be the main phase of the inorganic reduced
sulphur (50 - 80% of the total sulphur pool) and was at the same level
(250 pmoles per gram dry weight) in both cores. Remarkably, humic
sulphur was found to account for 17 to 28% of the total sulphur pool in the Tyro Basin and for 10 - 43 % in the Bannock Basin. Sulphur
isotope data show negative 634S values for both pyritic sulphur (-16 to
-40 %0) and humic sulphur (-16 to -30 %0). Pyritic and humic sulphur are
thought to be mainly formed at the interface of oxic seawater and
anoxic hypersaline bottom water. At this interface material is captured
due to the large density difference. Higher amounts of particulate and
dissolved organic carbon have been observed at these interfaces as
well as sulphate reduction and sulphide oxidation processes. Turbiditic
deposition transports pyritic and humic sulphur compounds to the
sediments in the Tyro and Bannock Basins.
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