Résumé
At slow spreading ridges, axial detachment faults exhume mantle-derived peridotites. Their interaction with seawater-derived hydrothermal fluids causes serpentinization down to 2-3 km from the fault, as inferred from seismic velocity models. It is commonly proposed that fractures allow penetration of seawater into the fault's footwall. At the microscopic scale, the hydration front progresses from a microfracture network toward the center of olivine relicts and forms the serpentine mesh texture. The origin of these microfractures is a matter of debate: tectonic, anisotropic thermal contraction of olivine during peridotite cooling or hierarchical fracturing of the olivine due to volume increase during serpentinization. In this presentation we use petrology and geochemistry to analyze the links between microfractures and serpentinization in a set of highly serpentinized peridotites dredged along the melt-starved easternmost part of the Southwest Indian Ridge (Smoothseafloor cruise). Our observations suggest that thermal contraction of olivine combines with tectonic stresses to fracture fresh peridotite in the brittle lithosphere. These approximately 60 mu m-spaced microfractures constitute the initial sample-scale permeability network for fluid penetration, onset of serpentinization and formation of additional hierarchical fractures. As serpentinization proceeds, the volume increase closes the least-developed planes and preferential pathways for fluid circulation become more distant, forming the 200-500 mu m-wide polygonal pattern typical of the serpentine mesh texture. In about 20% of the recovered samples the mesh serpentine is partially recrystallized forming rims next to later microfractures and serpentine veins. The spacing of these rims, and the limited proportion of affected samples suggest that the scales of the efficient permeability network in the serpentinites at this stage had increased to decimetric and greater scales. We use geochemical constrains to derive temperature conditions associated with this serpentinization history and to discuss the nature of serpentinizing fluids, based on a comparison with published work on serpentinites from the Mid-Atlantic Ridge. delta (super 18) O values decrease from 5.98 ppm to 1.91 ppm, from mesh texture serpentine to the later recrystallized serpentines. These values probably correspond to temperatures on the order of 200-300 degrees C and to a progressive equilibration with serpentinizing fluid values due to increasing water-rock ratios. Fluid-rock interactions produce serpentine minerals that are enriched in fluid-mobile elements (B, As, Sb, U, Cu) compared to primary minerals in the peridotites and present occasional Eu anomalies that may reflect variable redox conditions during serpentinization.