Elemental mixing systematics and Sr–Nd isotope geochemistry of mélange formation: Obstacles to identification of fluid sources to arc volcanics
Introduction
Analyses of arc volcanic rocks have long recognized the importance of metamorphic reactions and processes to arc magmatic petrogenesis and recycling to the mantle. However, despite igneous constraints, linking exact metamorphic processes to the development of distinct magmatic geochemical compositions has been ambiguous, especially since the geochemistry of metamorphic rocks beneath arcs is a combination of conjecture based on pre-subduction seafloor compositions (i.e. [1], [2], [3]) and the comparatively limited data for subduction-zone metamorphic rocks [4], [5], [6], [7], [8], [9], [10], [11], [12], [13]. Even more problematic is that data do not exist for the entire metamorphic suite produced within subduction zones, so our appreciation of the full spectrum of petrologic processes and their geochemical effects is incomplete. Most conspicuous among the missing data is a description of the geochemical ramifications of mélange formation.
Tectonic mélange is one of the most characteristic by-products of the subduction cycle, occurring in most orogenic belts. Styles and petrologic settings of mélange can range from highly deformed metasedimentary collages typical of incipient metamorphism within accretionary prisms (e.g. [14]) to chaotic hybridized mixtures of peridotite, basalt, and sediment produced at blueschist-, amphibolite-, or eclogite-facies conditions in forearc to sub-arc regions (e.g. [5], [6], [7], [15]). In all instances, mélange formation appears intimately linked to reactive fluid flow, indicating metasomatic processes are important in addition to mechanical deformation.
The extent and volumetric significance of mélange formation within deeper portions of subduction zones are debated, although anomalous geophysical results indicating deep subduction of hydrated material can be interpreted as measurement of mélange. Abers [16] reported seismic evidence for 1–7 km thick zones of anomalously slow material, interpreted by Abers [16] as hydrated oceanic crust along the surface of the subducting slab, in subduction zones worldwide. An intriguing alternative interpretation is that these seismically slow waveguides represent hydrated mélange zones dominated by chlorite + talc [7], a high-variance assemblage that will persist to the appropriate ∼ 250 km depths [4], [17]. This alternative interpretation suggests the possibility that mélange is an intrinsic feature of the slab–mantle interface and may play an important role in buffering fluid or melt compositions ultimately transferred to arc magma source regions in the mantle wedge.
Here, we explore the petrologic and geochemical diversity of mélange formed during active subduction in the Catalina Schist subduction complex exposed on Santa Catalina Island, CA. We report major element, trace element, and Sr–Nd isotope geochemistry for a large number of mélange samples spanning ranges in bulk composition and metamorphic grade. Our current dataset expands upon the more limited dataset of Bebout and Barton [7] for the Catalina Schist amphibolite-facies mélange by including a samples recording lawsonite–albite and lawsonite blueschist metamorphic conditions reminiscent of existing models for subduction-zone geothermal gradients. The focus of the current contribution is an investigation of geochemical effects stemming from mélange formation, as opposed to the petrogenetic modeling of Bebout and Barton [7].
Section snippets
Samples and analytical methods
The Catalina Schist has well-documented ranges in both bulk composition and metamorphic grade [4], [5], [6], [7], [18], [19]. Due to these factors and the expected variability stemming from mélange formation, we comprehensively analyzed a large population of mélange matrix samples formed at three metamorphic grades for major and trace elements (n = 58), while a representative subset were analyzed for Sr–Nd isotope ratios (n = 29). Samples of mélange were collected from zones of lawsonite–albite
Phenomenological model of mélange formation
Previous studies of the Catalina Schist have developed a model to explain the formation of mélange via the synergistic effects of fluid flow, metamorphism, and deformation occurring amongst the more “coherent” sedimentary, basaltic, and ultramafic blocks in the subduction complex; we briefly review this model here. Within the Catalina Schist, abundant subduction related fluid flow is evident, with the greatest extents of fluid–rock interaction and stable isotope homogenization occurring along
Major element geochemistry
Major element compositions for mélange matrix of the Catalina Schist reflect protolith contributions inferred from field relations. Variations for selected major elements, plotted as a function of MgO (Fig. 2), indicate fundamental distinctions between the dominantly binary ultramafic–mafic AM-facies mélange mixture and ternary protolith mixtures expected for LB- and LA-facies mélange. We choose to present major element variations as a function of MgO in that the predominance of an ultramafic
Sr–Nd isotope geochemistry
In this contribution we report Sr–Nd isotope ratios as age-corrected initial ratios based upon existing white mica Ar–Ar closure ages [18]. Unique ages for each sample are not available, so we have chosen to present maximum and minimum age corrections based on the range in Ar–Ar ages for each unit [18]. The range in age corrections spans 15 Ma in all cases.
When viewed on a εNd vs. 87Sr/86Sr isotope variation diagram, no firm array in the mélange data is evident (Fig. 7). However, the isotope
Mélange and the slab–mantle interface
Prior to any discussion of the geochemistry of the mélange zones of the Catalina Schist, it is worthwhile to briefly discuss why mélange will form in all subduction zones, and the physical role these mélange zones will have in the overall subduction system. Mélange must intrinsically form along the slab–mantle interface to form the chemical bridge between the depleted peridotites of the mantle wedge and the evolved components of the subducting slab. Across this interface, severe contrasts exist
The role of mélange in the subduction system
The dominant approach many utilize to resolve geochemical recycling during subduction is a comparison of subduction inputs vs. subduction outputs, usually to resolve what subducted lithologies are important contributors to the arc magmatic system or to constrain what proportion of subducted material is returned to the deep mantle (e.g. [1], [2], [3], [38], [56], [57], [58], [59], [60], [61]). Many of these studies are limited by our inadequate understanding of the physical processes
Conclusions
We have investigated the geochemical ramifications of subduction-zone mélange formation as recorded by the mélange matrix of the Catalina Schist, CA. The bulk compositions of these samples are consistent with their demonstrated petrogenesis and similar mélange zones are probably ubiquitous to subduction zones worldwide. Our major conclusions are:
- 1.
Mélange formation results in hybridized rock types that are not representative of the incoming subduction section, yet mélange commonly retains
Acknowledgments
We thank the many people who have participated in lively discussion of our data at meetings over the past three years. RLK would like to thank C. Sakaguchi for patience and guidance during TIMS analyses, all the members of the PML for constant support and criticism, and M. Walter for rational discussions of geochemistry and petrogenesis. Formal reviews by Jay Ague, Terry Plank, and the editorial handling of Ken Farley improved the manuscript, although they do not agree with all of our
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