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Experimental Constraints on the Origin of the 1991 Pinatubo Dacite
Authors:PROUTEAU  GAELLE; SCAILLET  BRUNO
Institution:1 UMR 6538, UNIVERSITÉ DE BRETAGNE OCCIDENTALE, 6 AVENUE LE GORGEU, BP 29285, BREST, FRANCE
2 INSTITUT DES SCIENCES DE LA TERRE D'ORLÉANS, CNRS, 1A RUE DE LA FÉROLLERIE, 45071 ORLÉANS CEDEX 2, FRANCE
Abstract:Crystallization (dacite) and interaction (dacite–peridotite)experiments have been performed on the 1991 Pinatubo dacite(Luzon Island, Philippines) to constrain its petrogenesis. Inthe dacite–H2O system at 960 MPa, magnetite and eitherclinopyroxene (low H2O) or amphibole (high H2O) are the liquidusphases. No garnet is observed at this pressure. Dacite–peridotite interaction at 920 MPa produces massive orthopyroxenecrystallization, in addition to amphibole ± phlogopite.Amphibole crystallizing in dacite at 960 MPa has the same compositionas the aluminium-rich hornblende preserved in the cores of amphibolephenocrysts in the 1991 dacite, suggesting a high-pressure stageof dacite crystallization with high melt H2O contents (>10wt %) at relatively low temperature (<950°C). The compositionsof plagioclase, amphibole and melt inclusion suggest that thePinatubo dacite was water-rich, oxidized and not much hotterthan 900°C, when emplaced into the shallow magma reservoirin which most phenocrysts precipitated before the onset of the1991 eruption. The LREE-enriched REE pattern of the whole-rockdacite demands garnet somewhere during its petrogenesis, whichin turn suggests high-pressure derivation. Partial melting ofsubducted oceanic crust yields melts unlike the Pinatubo dacite.Interaction of these slab melts with sub-arc peridotite is unableto produce a Pinatubo type of dacite, nor is a direct mantleorigin conceivable on the basis of our peridotite–daciteinteraction experimental results. Dehydration melting of underplatedbasalts requires unrealistically high temperatures and doesnot yield dacite with the low FeO/MgO, and high H2O, Ni andCr contents typical of the Pinatubo dacite. The most plausibleorigin of the Pinatubo dacite is via high-pressure fractionationof a hydrous, oxidized, primitive basalt that crystallized amphiboleand garnet upon cooling. Dacite melts produced in this way weredirectly expelled from the uppermost mantle or lower crust toshallow-level reservoirs from which they erupted occasionally.Magmas such as the Pinatubo dacite may provide evidence forthe existence of particularly H2O-rich conditions in the sub-arcmantle wedge rather than the melting of the young, hot subductingoceanic plate. KEY WORDS: Pinatubo dacite; slab melt; experimental petrology; arc magmas
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