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Melting and undercooled crystallisation of felsic xenoliths from minor intrusions (Jebilet massif, Morocco) |
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| Authors: | J Bouloton and D Gasquet |
| Institution: | a Département de Géologie and URA 10 CNRS, Université Blaise Pascal, 5 rue Kessler, 63038, Clermont-Ferrand Cedex, France b CRPG-CNRS, BP 20, 54501 Vandœuvre-lès-Nancy and Ecole Nationale Supérieure de Géologie, BP 452, 54001, Nancy Cedex, France |
| Abstract: | Granitic and gneissic xenoliths within microdiorite dykes from the Palaeozoic Jebilet massif (Morocco) contain up to 40% of granophyric intergrowths that occur as films along quartz-feldspar contacts and form an interconnected grain boundary network. The composition of the feldspar megacrysts — i.e. large embayed crystals surrounded by the granophyric intergrowths — implies high-temperature crystallisation (T >900 °C) and the sievetexture (or finger-print texture) indicates that these crystals underwent incipient melting. Moreover, the microstructural position and bulk composition of the granophyre are similar to that of glass in partly molten felsic xenoliths from lavas or pyroclastics. It is argued that the granophyre originated after partial melting of the xenoliths when incorporated into the dioritic magma. Crystallisation of that melt resulted in most cases in the formation of vermicular and/or cuneiform granophyre, which testifies to moderate degrees of undercooling. A few occurrences of plumose granophyre i.e. very thin intergrowths that are close to quartz-bearing spherulites, indicate that some xenoliths crystallised at higher degrees of undercooling. Together with granophyric xenoliths, a number of microgranular inclusions also occur. These are characterized by phenocrysts of quartz and feldspar in a microgranular groundmass. Finger-print texture in feldspar suggests that these inclusions, like the granophyric xenoliths, underwent ultra-metamorphism and melting. The microgranular groundmass is most probably indicative of crystallisation at lower degrees of undercooling, but the relationships between the two types of xenoliths still remain to be explored in detail. |
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