U–Pb apatite geochronology is increasingly recognized as a valuable tool for constraining the age of mid-crustal ductile shear zones. The crustal-scale Outer Hebrides Fault Zone (OHFZ) within the Laurentian foreland of the Scottish Caledonides has long been of uncertain age and tectonic significance. Earliest deformation within the OHFZ was associated with top-to-the-NW ductile thrusting that formed a belt of greenschist facies mylonites within host Archean−Paleoproterozoic basement gneisses. Previous estimates for the timing of thrusting vary between c . 1600 Ma and c . 430 Ma. The mylonitic fabrics are defined by a recrystallized assemblage of quartz + albite/oligoclase + sericite + actinolite + epidote + apatite ± calcite, consistent with deformation temperatures of 400–500°C and within the range of reported closure temperatures for Pb diffusion in apatite. U–Pb (LA−ICP−MS) dating of two texturally distinct apatite grain types within the mylonites has yielded ages mostly in the range c . 1100–900 Ma. The OHFZ is therefore interpreted as a Grenville–Sveconorwegian structure that formed during the tripartite collision of Laurentia, Baltica, and Amazonia and the assembly of Rodinia. Supplementary material : U–Pb isotopic data (Table S1), trace element data (Table S2) and laser ablation spot images are available at https://doi.org/10.6084/m9.figshare.c.7084925
Abstract The Himalayan-Tibetan system is growing upward and outward, influenced by mid-lower crustal melting and flow. This study offers a missing geochemical perspective on current geophysics, linking mid-crustal melting beneath SE Tibet to the initiation of transcurrent tectonics that have facilitated the ongoing southeastward extrusion of the Tibetan plateau. New zircon U-Pb data reveal a pulse of Miocene felsic magmatism southeast of the Eastern Himalayan Syntaxis. These have high SiO2, variable but low ɛHf(t) and high δ18O which strongly suggest metasedimentary anatexis. Moderate La/Yb and Sr/Y, with high 87Sr/86Sr(i) and low ɛNd(t) are comparable with mid-lower crust biotite-bearing granitic gneisses. Together with biotite and zircon thermobarometry, these characteristics suggest biotite-dehydration anatexis in the middle crust. Experimental and rheological data suggest melt fractions (> 10%) sufficient to reduce crustal viscosity and allow rheological accommodation for Miocene extrusion of the plateau, and the continued presence of mid-crustal melt is supported by current geophysical data.
Crustal evolution is currently governed by plate tectonics and it has been shown that between the Archean and the Phanerozoic major changes in subduction styles occured. Among others, the chemistry of different plutonic rocks through time and the understanding of their petrogenesis have helped to define different stages in the evolution of plate tectonics. An important change around 2.7 Ga led to the genesis of rocks that are the result of a metasomatized mantle wedge: the sanukitoids. This event is interpreted as the result of the evolution from a shallow to a steep subduction style. Modern plate tectonics is now generally generating calc-alkaline suites but exceptions can occur such as the Caledonian (Palaeozoic) high Ba-Sr plutons in northern Scotland. The latter have been interpreted as a modern analogue of the sanukitoids. In this contribution, we aim to study this Caledonian sanukitoid-like suite from northern Scotland. Whole rock chemistry (trace elements and stable isotopes) of these rocks ranging from appinitic to granitoid in composition are well constrained but it has been argued that careful study of accessory phases can give more information on the petrogenesis of the plutons. The incorporation of trace elements and more particularly rare earth elements (REE) into their structures make them ideal to understand petrogenetic processes. Here, we present a detailed petrographic study and systematic analysis of trace elements of apatite, titanite and zircon in a range of plutonic rocks from appinitic to granitoid compositions. Trace elements in these accessory phases give direct access to the crystallisation history of these plutons. With these data, we suggest that apatite and titanite record in-situ crystal fractionation and mixing processes. Whole-rock reverse modelling, using single grain apatite or titanite trace element compositions, give reliable results. These results also highlight the relationship between the appinite and granitoid rocks and their petrogenetic history.
Abstract Uranium-lead (U-Pb) zircon dating establishes a late Cambrian (Drumian) protolith age of 503 ± 2 Ma for a trondhjemitic gneiss of the calc-alkaline Strathy Complex, northern Scottish Caledonides. Positive εHf and εNd values from trondhjemitic gneisses and co-magmatic amphibolites, respectively, and an absence of any inheritance in zircon populations support published geochemistry that indicates a juvenile origin distal from Laurentia. In order to account for its present location within a stack of Laurentia-derived thrust sheets, we interpret the complex as allochthonous and located along a buried suture. We propose that a microcontinental ribbon was detached from Laurentia during late Neoproterozoic to Cambrian rifting; the intervening oceanic tract closed by subduction during the late Cambrian and formed a juvenile arc, the protolith of the Strathy Complex. The microcontinental ribbon was reattached to Laurentia during the Grampian orogeny, which transported the Strathy Complex as a tectonic slice within a nappe stack. Peak metamorphic conditions for the Strathy Complex arc (650–700 °C, 0.6–0.75 GPa) are intermediate in pressure between those published previously for Grampian mineral assemblages in structurally overlying low-pressure migmatites (670–750 °C, <0.4 GPa) that we deduce to have been derived from an adjacent backarc basin, and structurally underlying upper amphibolite rocks (650–700 °C, 1.1–1.2 GPa) that we interpret to represent the partially subducted Laurentian margin. This scenario compares with that of the northern Appalachian Mountains and Norway where microcontinental blocks are interpreted to have their origins in detachment from passive margins of the Iapetus Ocean during Cambrian rifting and to have been re-amalgamated during Caledonian orogenesis.