Journal Article The Late Cretaceous Impact of the Trindade Mantle Plume: Evidence from Large-volume, Mafic, Potassic Magmatism in SE Brazil Get access S. A. GIBSON, S. A. GIBSON * 1DEPARTMENT OF GEOLOOICAL SCIENCES, UNIVERSITY OF DURHAMSOUTH ROAD, DURHAM DH1 3LE, UK Corresponding author Search for other works by this author on: Oxford Academic Google Scholar R. N. THOMPSON, R. N. THOMPSON 1DEPARTMENT OF GEOLOOICAL SCIENCES, UNIVERSITY OF DURHAMSOUTH ROAD, DURHAM DH1 3LE, UK Search for other works by this author on: Oxford Academic Google Scholar O. H. LEONARDOS, O. H. LEONARDOS 2DEPARTMENTO DE GEOQUIMICA E RECURSOS MINERAIS, INSTITUTO DE GEOCIENCIASUNIVERSIDADE DE BRASILIA, 70910 BRASILIA DF, BRAZIL Search for other works by this author on: Oxford Academic Google Scholar A. P. DICKIN, A. P. DICKIN 3DEPARTMENT OF GEOLOGY, McMASTER UNIVERSITY1280 MAIN STREET WEST, HAMILTON, ONTARIO, CANADA L83 4M1 Search for other works by this author on: Oxford Academic Google Scholar J. G. MITCHELL J. G. MITCHELL 4DEPARTMENT OF PHYSICS, THE UNIVERSITY, NEWCASTLEUPON TYNE NE1 7RU, UK Search for other works by this author on: Oxford Academic Google Scholar Journal of Petrology, Volume 36, Issue 1, February 1995, Pages 189–229, https://doi.org/10.1093/petrology/36.1.189 Published: 01 February 1995 Article history Received: 07 February 1994 Revision received: 05 July 1994 Published: 01 February 1995
The Late-Cretaceous Alto Paranaíba Igneous Province (APIP) comprises a variety of ultrapotassic rock-types, including kimberlites, lamproites and large volumes of kamafugites, in addition to a number of carbonatite-bearing plutonic alkaline complexes. Phlogopite-picrites are ultramafic fine-grained rocks typically composed of olivine phenocrysts set in a groundmass of phlogopite, carbonate, perovskite, apatite and chromite. They occur as dyke swarms in the carbonatite complexes, but are also scattered throughout the Province. The phlogopite-picrites represent the peralkaline, ultrapotassic, carbonate-rich, silicate magmas parental to the carbonatite-bearing complexes, and have strong chemical affinity with kamafugites. Together with petrographic similarities observed between silicate rocks from the carbonatite complexes and xenoliths occurring in APIP kamafugites, this provides a strong link between kamafugitic and carbonatitic magmatism in the Province.
WALL, F. & ZAITSEV, A. N. (eds) 2004. Phoscorites and Carbonatites from Mantle to Mine: the Key Example of the Kola Alkaline Province. The Mineralogical Society Series no. 10. xv + 498 pp. London: The Mineralogical Society of Great Britain and Ireland. Price £89.00 (hard covers); introductory price £49.00. ISBN 0 903056 22 4 - Volume 143 Issue 1
The physicochemical characteristics of sub-volcanic magma storage regions have important implications for magma system dynamics and pre-eruptive behaviour. The architecture of magma storage regions located directly above high buoyancy flux mantle plumes (such as Kīlauea, Hawai’i and Fernandina, Galápagos) are relatively well understood. However, far fewer constraints exist on the nature of magma storage beneath ocean island volcanoes that are distal to the main zone of mantle upwelling or above low buoyancy flux plumes, despite these systems representing a substantial proportion of ocean island volcanism globally. To address this, we present a detailed petrological study of Isla Floreana in the Galápagos Archipelago, which lies at the periphery of the upwelling mantle plume and is thus characterised by an extremely low flux of magma into the lithosphere. Detailed in situ major and trace element analyses of crystal phases within exhumed cumulate xenoliths, lavas and scoria deposits, indicate that the erupted crystal cargo is dominated by disaggregated crystal-rich material (i.e., mush or wall rock). Trace element disequilibria between cumulus phases and erupted melts, as well as trace element zoning within the xenolithic clinopyroxenes, reveals that reactive porous flow (previously identified beneath mid-ocean ridges) is an important process of melt transport within crystal-rich magma storage regions. In addition, application of three petrological barometers reveal that the Floreana mush zones are located in the upper mantle, at a depth of 23.7±5.1 km. Our barometric results are compared to recent studies of high melt flux volcanoes in the western Galápagos, and other ocean island volcanoes worldwide, and demonstrate that the flux of magma from the underlying mantle source represents a first-order control on the depth and physical characteristics of magma storage.