Seismic wave velocity and anisotropy of serpentinized peridotite in the Oman ophiolite

Shallow seismic measurements in harzburgite from the Oman ophiolite performed in a zone where the maximum horizontal anisotropy is expected (vertical foliation and horizontal lineation) point to a dominant dependence of seismic properties on fracturing.

Optical microscopy studies show that microcracks are guided by the serpentine (lizardite) penetrative network oriented subparallel to the harzburgite foliation and subperpendicular to the mineral lineation, and that serpentine (lizardite) vein filling has a maximum concentration of (001) planes parallel to the veins walls. The calculated elastic properties of the oriented alteration veins filled with serpentine in an anisotropic matrix formed by oriented crystals of olivine and orthopyroxene are compared with seismic velocities measured on hand specimens.

Laboratory ultrasonic data indicate that open microcracks are closed at 100 MPa pressure, e.g. (J. Geophys. Res. 65, (1960) 1083) and (Proc. ODP Sci. Results Leg 118, (1990) 227). Above this pressure, laboratory measurements and modeling show that P-compressional and S-shear wave velocities are mainly controlled by the mineral preferred orientation. Veins sealed with serpentine are effective in slightly lowering P and S velocities and increasing anisotropy. The penetrative lizardite network does not affect directly the geometry of seismic anisotropy, but contributes indirectly in the fact that this network controls the microcrack orientations.

Comparison between seismic measurements of peridotite and gabbro in the same conditions suggest that P- and S-waves anisotropies are a possible discriminating factor between the two lithologies in the suboceanic lithosphere.     

The ophiolite of Oman and United Arab Emirates

Marine Geophysical Research -     

Significance of gabbronorite occurrence in the crustal section of the Semail ophiolite

The eastern end of the Haylayn massif exposes a complex paleoridge structure interpreted as the tip of a northwestward propagating segment (Nicolas et al., this issue). The area, revisited from a petrostructural and geochemical viewpoint, offers the most documented exposures of the association of olivine gabbros and gabbronorites in Oman (Juteau et al., 1988). Gabbronorites were injected while the main gabbro unit was deforming in the magmatic state. Both units do not differ chemically, except for the SiO₂ enrichment of the orthopyroxene-rich gabbros relative to olivine-gabbro. In addition, they display the same trace element signature, which implies the same parent magma for both units. The extension of the stability field of orthopyroxene is assigned to increase of oxygen fugacity due to hydration. The source of hydration is the ridge axis hydrothermal circulation, suggesting hydrothermal/magma interaction at temperatures above the gabbro solidus. The distribution of gabbronorites at the scale of the entire ophiolite suggests a relation with ridge tectonics where high-T conditions of hydrothermal-magmatic interaction are met. Such conditions are met when propagating segments rotate the structures of the dying magma chamber.     

Emplacement of Semail–Emirates ophiolite at ridge–trench collision

The Oman‐Emirates is the largest and best‐exposed ophiolite; consequently, it has attracted significant interest among scientists, together with serious conflicts. Most geologists regard this ophiolite as having formed in an intra‐oceanic subduction zone before being accreted to the Arabian continent. Here, we propose an alternative scenario, supported by detailed field observations and integrated geophysics. The smaller Emirates part of the ophiolite was forced into a nearby continent, in the pre‐collision stage of Tethyan closure. The contraction led to the exhumation of the mantle floor of segmented basins accreted in a rifted system similar to the present‐day Gulf of California. The implied high temperature–high pressure metamorphism and the range of geochemical signatures were introduced during the process of rifting, whereas the larger Oman ophiolite was emplaced by obduction onto and along the subducting continental shore. This Ridge–Trench–Transform system might call for a new process to obduct over continents in particular Tethyan ophiolites.     

Minéraux serpentineux extraits de péridotites serpentinisées des Alpes Occidentales

Complete physical and chemical data presented concern serpentine minerals choosen from epizonal to non metamorphic domains. It is tried to correlate well-studied serpentine minerals, generally coming from particular outcrops with the rock-forming ones known only through the microscope.It appears that ribbons filling serpentine veins in a serpentinized dunite, the whole mesh-structure of a non metamorphic serpentine, and bastite lamellae are made of lizardite. Antigorite, only serpentine mineral present in metamorphic domains, shows no significative difference between high-pressure facies (glaucophane schist) and low-pressure facies (green-schist). The data allow a better understanding of the serpentinization process. The geochemically antinomic behaviour of iron and magnesium is emphasized.     

Inside the magma chamber of a dying ridge segment in the Oman ophiolite

For the first time, the crystallized remnant of an oceanic ridge magma chamber is documented in the Oman ophiolite. It exists in the centre of a 40 km long monoclinal ridge (Jebel Dihm, Wadi Tayin massif), exposing a full crustal section perpendicular to the spreading direction. New detailed mapping supported by U‐Pb zircon geochronology suggests that the active, fast‐spreading ridge that died just prior to detachment of the ophiolite is preserved and largely intact. Our observations provide insights into the crystallizing mush zone of a magma chamber, before it crosses the external walls and solidifies as deformed gabbros. Our data provide new constraints on the shape and internal dynamics of a magma chamber, including gabbro subsidence from the floor of a perched melt lens and the limited contribution of sills to crustal accretion. By locating precisely the palaeo‐ridge axis, prior full spreading rate estimates can be increased to ~140 km Ma^?1.     

Structural contribution from the Oman ophiolite to processes of crustal accretion at the East Pacific Rise

A comprehensive model for the activity of the elementary accretion segment at fast‐spreading ridges relies on integration of structural data from the Oman ophiolite and geophysical results from the East Pacific Rise (EPR) around 9°N, which are of comparable size and spreading rates. The axial melt lens at shallow crustal level provides a link between Deval segmentation at the seafloor and a lower melt sill at Moho level, imaged at the EPR as a crustal melt zone (CMZ) and mapped in Oman as the Moho transition zone (MTZ). Both are attached to a mantle upwelling at the EPR, and to a frozen diapir in Oman. The physical link between diapiric mantle uprising at the Moho and Devals segmentation at the seafloor is the melt being injected from the mantle into the lower MTZ, ponding there, and then being released by powerful injections into the upper melt lens. The magma chamber covers the diapir at a distance of 5 km from the ridge axis.     

A conceptual hydrogeological model of ophiolite hard-rock aquifers in Oman based on a multiscale and a multidisciplinary approach

Ophiolites are found all over the world: from the Alps to the Himalayas, in Cuba, Papua-New Guinea, New Caledonia, Newfoundland, etc. They are composed of hard rocks—basalt, dolerite, gabbro and peridotite, which are formed at the mid-oceanic ridges, with specific ridge-related tectonic fracturing and intense hydrothermal alteration. Their geological and thus their hydrogeological properties differ from those of both granite or classical gabbro and classical basaltic lava. A conceptual hydrogeological model of these hard-rock aquifers was developed based on the convergent results of a multidisciplinary approach at several spatial scales, from rock-sample (centimetre) to catchment (kilometre), on well-preserved ophiolite rocks in Oman. In ophiolite rocks, groundwater circulation takes place mostly in the fissured near-surface horizon (50 m thick), and, to a lesser degree, in the tectonic fractures. Hydrograph analysis (Water Resour Res 34:233–240, 1977), interpretation of numerous pumping tests using both classical Theis and dual porosity models [Water Resour Res 32:2733–2745, 1996; Comput Geosci J (in press)], and mercury porosity and hydraulic conductivity lab-measurements support the aquifer parameter estimates. The hydraulic conductivity K of the fissured horizon is estimated at 10^–5 to 10^–6 m/s for gabbro and dolerite, and 10^–7 m/s for peridotite. The storage coefficient S of the peridotite aquifer is estimated at 10^–3 and appears to be controlled mainly by microcracks (20 to 100 m wide). Tectonic fractures in the ophiolite have similar hydrodynamic properties regardless of lithology (10^–1<T<10^–4 m²/s and 10^–1<S<10^–3) though the probability of obtaining productive wells is two to three times greater in gabbro and dolerite than in peridotite. Some of the tectonic fractures produce small hydrothermal, hyperalkaline springs in the peridotite. The water budget and hydrochemistry of the Oman ophiolite are characterized and support the conceptual hydrogeological model. Despite low annual rainfall, a relatively low hydraulic conductivity and a significant storage coefficient explain why most of the streams in peridotite are perennial.

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Résumé Les ophiolites se trouvent partout dans le monde : des Alpes à lHymalaya, à Cuba, Papouasie Nouvelle-Guinée, Nouvelle Calédonie, etc. Les ophiolites sont composées de roches dures basaltiques, de dolérites, gabbros et péridotites, qui sont formées aux rides mi-océaniques, avec, en relation avec les rides, une fracturation tectonique et une altération hydrothermale intense. Leurs propriétés géologiques et hydrogéologiques diffèrent de celles des granites ou des gabbros classiques ou des laves basaltiques classiques. Un modèle hydrogéologique conceptuel des aquifères de hard-rock a été développé sur les résultats convergents dune approche multidisciplinaire à différentes échelles spatiales, de léchantillon de roche de quelques centimètres à la taille du bassin versant en kilomètres, des ophiolites bien conservées dOman. Dans les roches ophiolitiques, la circulation des eaux souterraines est surtout localisée dans les fissures dun horizon de surface de plus dune cinquantaine de mètres et à un degré moindre dans les fractures tectoniques. Lanalyse des hydrographes (Water Resour Res 34:233–240, 1977), linterprétation des nombreux essais de pompage utilisant des modèles classiques de Theis et des modèles à double porosité (Water Resour Res 32:2733–2745, 1996; Comput Geosci J (Soumis), la porosité au mercure et la conductivité hydraulique calculée en laboratoire supportent lestimation des paramètres de laquifère. La conductivité hydraulique K de lhorizon fissuré est estimée entre 10^–5 et 10^–6 m/s pour les gabbros et les dolérites, et 10^–7 m/s pour les péridotites. Le coefficient demmagasinement S de laquifère de péridotite est estimé à 10^–3 et semble être contrôlé par les micro-fractures (20 à 100 m de largeur). Les fractures tectoniques dans les ophiolites possèdent des propriétés hydrodynamiques en regard de la lithologie (10-1<T<10-4 m²/s et 10-1/S/10-3) bien que la probabilité dobtenir des puits productifs est trois plus grand dans le grabbro et la dolérite que la péridétite. Quelques unes des fractures tectoniques produisent de petites sources hydrothermales hyperalcalines dans la péridotite. Le bilan hydrologique et hydrochimique de lophiolite dOman caractérise le modèle hydrogéologique conceptuel. Malgré des faibles précipitations annuelles, une relativement basse conductivité hydraulique et un coefficient demmagasinement significatif expliquent pourquoi la plus part des cours deau sur les péridotites ne sont jamais taris.

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Resumen Las rocas ofiolitas se encuentran en muchas partes del mundo desde los Alpes a los Himilaya, Newfoundland, Nueva Caledonia etc. Son rocas duras compuestas de basalto, dolerita, gabro y peridotita que son formadas por los cordones medio-oceánicos y por fracturación relacionada con los cordones tectónicos específicos y alteración hidrotermal intensa. La geología y los propiedades hidrogeológicas varian entre las de granito y gabro clásico y lava de basalto clásico. Se desarrolló un modelo conceptual de los acuíferos de las rocas duras Basado en los resultados convergentes de un enfoce multidisciplinario a varias escalas a partir de muestras de roca (centímetro) a cuenca kilómetro) enfocado en las rocas ofilíticas bien preservados en Oman. En las rocas ofiolíticas la circulación de agua ocurre principalmente en el horizonte de fisuras cercanas a la superficie (>50 m de espesor) y en un grado menos importante en fracturas tectónicas. Los estimados de los parámetros de estos acuíferos se basan en análisis de hidrógrafos (Water Resour Res 34:233–240, 1977), en la interpretación de pruebas de bombeo usando los modelos clásicos de Theis y de porosidad doble (Hamm y Bidaux 1996; Lods y Gouze, [en prensa]), y porosidad de mecurio y conductividad hidraúlica medida en el laboratorio. La conductividad hidraúlica K del horizonte fisurado se estima en 10E-5 a 10E-6 m-s para gabro y dolerita y 10E-7 para peridotita. El coeficiente de abastecimiento S del acuífero peridotita se estima en 10–3 y parece ser controlado principalmente por microfracturas (20 to 100 m de ancho). Las fracturas tectónicas en la ofiolita tienen propiedades hidrodinámicas similares independientes de la litología (10–1<T<10–4 m²/s and 10–1<S<10–3) pero la probabilidad de obtener pozos productivos es dos o tres veces mayor en gabro que en dolerita o peridotita. Algunas de las fracturas tectónicas producen pequeñas descargas de agua hidrotermal hiperalcalina en la peridotita. El presupuesto e hidroquímica de las ofilitas de Omán se caracteriza y apoya en el modelo conceptual hidrogeológico. La baja lluvia anual, una conductividad hidraúlica relativamente baja y un coeficiente de abastecimiento importante explican porqué la mejoría de los drenajes en peridotita es peremne.

     

Dike distribution in the Oman-United Arab Emirates ophiolite

Mafic dikes and dunite veins are observed in the mantle section of the Oman – United Arab Emirates (O-UAE) ophiolites, as well as diabase dikes and hydrothermal veins in the crust section. They have been systematically measured during the mapping of this ophiolite and are represented by their trajectories in the folded map 3 in the back of this volume, and by local stereoplots included in this study. Mafic dikes in the mantle section correspond to basaltic melt being injected at decreasing temperatures from above or at peridotite solidus, down to below 450°C. Hydrothermal veins associated with dioritic dikes issued from hydrous melting of host gabbros are observed down to the base of the crust, bearing evidence for sea water penetration into basal gabbros at or above 900°C, that is very close to the ridge axis. Dike orientations record the stress field at the time of their injection. In most places, all types of dikes are dominantly parallel to the general trend of the nearest sheeted dike complex; thus the stress field has not visibly changed from melt injection in the asthenosphere below the ridge of origin to injection in a lithosphere up to a few Myr old, at distances beyond 100 km from the axis. Local preferred orientations, when they are considered in the frame of the paleo-ridge system of O-UAE, result in a coherent model throughout the belt: the sheeted dike complex dips moderately away from the presumed ridge axis and the mantle dikes, toward this axis. These opposite directions are explained by the presumed effect of subsidence toward the axis for the sheeted dikes and by the central feeding from an asthenospheric uprise for the mantle dikes.