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Amphibole megacrysts as a probe into the deep plumbing system of Merapi volcano,Central Java,Indonesia
Authors:Email author" target="_blank">Stefan?T?M?PetersEmail author  Valentin?R?Troll  Franz?A?Weis  Luigi?Dallai  Jane?P?Chadwick  Bernhard?Schulz
Institution:1.Abteilung Isotopengeologie,Geowissenschaftliches Zentrum der Georg-August-Universit?t G?ttingen,G?ttingen,Germany;2.Faculteit der Aard- en Levenswetenschappen,Vrije Universiteit Amsterdam,HV Amsterdam,The Netherlands;3.Department of Earth Sciences, Section for Mineralogy, Petrology and Tectonics,Uppsala University,Uppsala,Sweden;4.Department of Geosciences,Swedish Museum of Natural History,Stockholm,Sweden;5.CNR-Istituto di Geoscienze e Georisorse,Pisa,Italy;6.Science Gallery, Trinity College Dublin,Dublin,Ireland;7.Institut für Mineralogie, TU Bergakademie Freiberg,Freiberg,Germany
Abstract:Amphibole has been discussed to potentially represent an important phase during early chemical evolution of arc magmas, but is not commonly observed in eruptive arc rocks. Here, we present an in-depth study of metastable calcic amphibole megacrysts in basaltic andesites of Merapi volcano, Indonesia. Radiogenic Sr and Nd isotope compositions of the amphibole megacrysts overlap with the host rock range, indicating that they represent antecrysts to the host magmas rather than xenocrysts. Amphibole-based barometry suggests that the megacrysts crystallised at pressures of >500 MPa, i.e., in the mid- to lower crust beneath Merapi. Rare-earth element concentrations, in turn, require the absence of magmatic garnet in the Merapi feeding system and, therefore, place an uppermost limit for the pressure of amphibole crystallisation at ca. 800 MPa. The host magmas of the megacrysts seem to have fractionated significant amounts of amphibole and/or clinopyroxene, because of their low Dy/Yb ratios relative to the estimated compositions of the parent magmas to the megacrysts. The megacrysts’ parent magmas at depth may thus have evolved by amphibole fractionation, in line with apparently coupled variations of trace element ratios in the megacrysts, such as e.g., decreasing Zr/Hf with Dy/Yb. Moreover, the Th/U ratios of the amphibole megacrysts decrease with increasing Dy/Yb and are lower than Th/U ratios in the basaltic andesite host rocks. Uranium in the megacrysts’ parent magmas, therefore, may have occurred predominantly in the tetravalent state, suggesting that magmatic fO2 in the Merapi plumbing system increased from below the FMQ buffer in the mid-to-lower crust to 0.6–2.2 log units above it in the near surface environment. In addition, some of the amphibole megacrysts experienced dehydrogenation (H2 loss) and/or dehydration (H2O loss), as recorded by their variable H2O contents and D/H and Fe3+/Fe2+ ratios, and the release of these volatile species into the shallow plumbing system may facilitate Merapi’s often erratic eruptive behaviour.
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