EGU2018-10186, 2018 EGU General Assembly 2018 © Author(S) 2018

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EGU2018-10186, 2018 EGU General Assembly 2018 © Author(S) 2018 Geophysical Research Abstracts Vol. 20, EGU2018-10186, 2018 EGU General Assembly 2018 © Author(s) 2018. CC Attribution 4.0 license. Insights into the Oxidation State of Arc Magmas from the Xenolith Suite Sangeang Api Volcano, Eastern Indonesia. Ben Cooke, John Foden, and Alan Collins University of Adelaide, Earth Science, Adelaide, Australia ([email protected]) At ∆logQFM +2.5 ± 1 arc magmas are significantly more oxidized than MORB (∆logQFM 0 ± 0.5, Cottrell and Kelley, 2011). The origin of this oxidized state remains controversial, either due to oxidation of the mantle wedge source, or to processes operating as these volatile-rich magmas ascend to upper lithospheric pressures? Sangeang Api is an active volcano in the eastern Sunda Arc in the strait between the islands of Sumbawa and Flores. Its lavas are shoshonitic with silica undersaturated alkalic composition and transport abundant co-genetic, cumulate pyroxenite and gabbroic xenoliths. Lavas and xenoliths all contain pargasite to Mg-hastingite amphibole. Applying the formulations of Ridolfi, et. al. (2012) these yield a continuous range of pressure estimates from 975MPa to 340MPa representing crustal level crystallisation from the Moho at 34km up to 12km. Temperature estimates (1072-976˚C) and water content (6.51 to 3.15wt.% ) both decline continuously with depth. fO2 estimates range from ∆NNO+0.2 to +1.2 and show an initial trend of oxidation from the Moho up to ∼ 500MPa and then dominated by lava’s phenocrysts revert to a trend of reduction at the shallower depths. Cl in amphibole increases from the Moho up to 500MPa and then abruptly declines. The data imply continuous mixed CO2-H2O fluid saturation at all depths from the Moho up with declining CO2/H2O from the Moho up to ∼500 MPa. Magma bodies emplaced shallower than ∼17km exsolve a near pure hydrous fluid to which Cl and S strongly partition. We conclude that in this example arc magmas rise to the crust in a moderately oxidized state and then undergo complex oxidation histories coupled to volatile saturation..
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