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Geological Society, London, Special Publications; 2003; v. 216; p. 491-503;
DOI: 10.1144/GSL.SP.2003.216.01.32
© 2003 Geological Society of London

Deep Subsurface Sediment Mobilization

Boron and boron isotopes as tracers for diagenetic reactions and depth of mobilization, using muds and authigenic carbonates from eastern Mediterranean mud volcanoes

A. Deyhle1, Achim J. Kopf1 & G. Aloisi2

1 SCRIPPS Institution of Oceanography, UCSD, 9500 Gilman Drive, La Jolla, CA 92093-0212, USA akopf{at}ucsd.edu
2 GEOMAR Research Centre, University Kiel, Wischhofstrasse 1-3, 24148 Kiel, Germany

Authigenic carbonates and muds from six mud volcanoes in the eastern Mediterranean Sea were recovered during the French/Dutch MEDINAUT cruise utilizing the submersible Nautile in November 1998. The mud volcanoes are active seafloor vents in two areas at the plate boundary between the converging African and Eurasian Plates: the Mediterranean Ridge accretionary prism near Crete (Greece) and the Anaximander Mountains south of Turkey. B contents and {delta}11B signatures were measured with the aim of identifying the diagenetic processes and source depths of the material in the collision zone. B concentrations of the carbonate precipitates cover a range of 8–45 ppm and vary isotopically from +15.6 to +22.9{per thousand} (corresponding to a parent solution of 34.9–42.2{per thousand} at pH 7). Both the B-enrichment and a {delta}11B valve slightly lower than seawater suggest the mud domes originate from a moderately deep fluid source, with local admixture of seawater. B contents and {delta}11B of the mud show distinct differences between the areas: the Mediterranean Ridge mud domes have lower B contents and higher {delta}11B (average 3.9{per thousand}) compared to Anaximander Mountains mud volcanoes ({delta}11B average –0.6{per thousand}). These B results attest the release of structurally-bound B from clay mineral lattices, probably due to stronger deformation near Turkey. These mudstones, which had previously been affected by deep-seated thrusting beneath the Antalya Complex, may have been liquefied and remobilized in their present setting. By contrast, the mud on the Mediterranean Ridge represents offscraped clay-rich strata that was incorporated into the large accretionary wedge.