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Pyroxenite and granulite xenoliths from beneath the Scottish Northern Highlands Terrane: evidence for lower-crust/upper-mantle relationships
Authors:B. Upton  P. Aspen  R. Hinton
Affiliation:Department of Geology and Geophysics, University of Edinburgh, Edinburgh EH9 3JW, UK,
Abstract:Xenolith suites from Permian host rocks in Orkney and the extreme NE of the Scottish mainland (Duncansby Ness) are described and compared to those from elsewhere in the Northern Highlands Terrane. Those from the Tingwall dyke, Orkney, comprise roughly equal proportions of ultramafic rocks (wehrlites, clinopyroxenites, websterites, hornblendites) and mafic to felsic rocks (gabbroic, noritic and dioritic granulites, with subordinate tonalites and trondhjemites). Those from Duncansby (45 km to the south) are dominantly olivine-poor ultramafic rocks (clinopyroxenites, pargasite pyroxenites, biotite-pyroxenites), together with granulites grading from gabbroic through to tonalites and trondhjemites. Most of the granulites are meta-igneous, comprising plagioclase and one- or two-pyroxene species with equilibration temperatures of 810-710 °C, and are regarded as samples of the lower crust. Absence of garnet and olivine, together with the association of relatively sodic plagioclase and aluminous pyroxenes, is consistent with derivation from depths corresponding to 5-10 kbar. Positive Eu anomalies in the granulites imply that most originated as plagioclase-rich cumulates from basaltic magmas. Scarce peraluminous quartzo-feldspathic xenoliths, such as a garnet-sillimanite-bearing sample from Duncansby, are regarded as metasedimentary in origin. Pyroxenes (and biotites) in the ultramafic xenoliths tend to have higher mg numbers than those of the granulites, reflecting higher temperatures of formation. Whereas the pyroxene-rich ultramafic rocks may be partly interleaved with the granulites in the lower crust, it is concluded that they also constitute a zone of substantial thickness at or around Moho level, separating the granulites from underlying peridotites, and that they originated as cumulates cognate to the granulites. They have, however, been variably metasomatised with formation of amphibole. This zone may constitute a density trap at which melt fractions, rich in K, Fe, Ti and OH and ascending from the asthenosphere, interact with the ultramafic cumulates, modifying them texturally and modally to produce a complex veined assemblage of clinopyroxene- and pargasite-rich rocks. The metasomatism involved an increase in LREE, HFSE and LILE contents. Some modal and cryptic metasomatism may also have affected the granulites, accounting for the presence of amphibole and relatively high LREE/HREE values (La/Lu 38-206). Since closely comparable xenolith assemblages also occur in Mull at the southwestern extremity of the Northern Highland Terrane, such metasomatised olivine- and orthopyroxene-deficient ultramafic rocks may characterise the shallowest part of the mantle beneath the entire terrane. The strongly bimodal character of the xenolith populations (either ultramafic or mafic grading to felsic) is taken to reflect the sharpness of the petrological Moho in this region.
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