4.7 Article

Syn-volcanic cannibalisation of juvenile felsic crust: Superimposed giant 18O-depleted rhyolite systems in the hot and thinned crust of Mesoproterozoic central Australia

Journal

EARTH AND PLANETARY SCIENCE LETTERS
Volume 424, Issue -, Pages 15-25

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.epsl.2015.05.005

Keywords

O-18-depleted rhyolite; Mesoproterozoic; supervolcano; juvenile crustal addition; central Australia; Musgrave Province

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Eruptions of voluminous O-18-depleted rhyolite provide the best evidence that the extreme conditions required to produce and accumulate huge volumes of felsic magma can occur in the upper 10 km of the crust. Mesoproterozoic bimodal volcanic sequences from the Talbot Sub-basin in central Australia contain possibly the world's most voluminous accumulation of O-18-depleted rhyolite. This volcanic system differs from the better known, but geochemically similar, Miocene Snake River Plain Yellow-stone Plateau of North America. Both systems witnessed 'super' sized eruptions from shallow crustal chambers, and produced O-18-depleted rhyolite. The Talbot system, however, accumulated over a much longer period (>30 Ma), at a single depositional centre, and from a magma with mantle-like isotopic compositions that contrast strongly with the isotopically evolved basement and country-rock compositions. Nevertheless, although the Talbot rhyolites are exclusively O-18-depleted, the unavoidable inference of an O-18-undepleted precursor requires high-temperature rejuvenation of crust in an upper-crustal chamber, and in this respect the evolution of the Talbot rhyolites and O-18-depleted rhyolites of the Snake River Plain - Yellowstone Plateau is very similar. However, instead of older crustal material, the primary upper-crustal source recycled into Talbot rhyolites was comagmatic (or nearly so) felsic rock itself derived from a contemporaneous juvenile basement hot-zone. Whereas giant low delta O-18 volcanic systems show that voluminous melting of upper crust can occur, our studies indicate that felsic magmas generated at lower crustal depths can also contribute significantly to the thermal and material budget of these systems. The requirement that very high-temperatures be achieved and sustained in the upper crust means that voluminous low delta O-18 magmatism is rare, primarily restricted to bimodal tholeiitic, high-K rhyolite (A-type) magmatic associations in highly attenuated lithosphere. In the case of the Talbot system, at least, our data suggest that an unusually hot pre-history might also be required to thermally prime the crust. Crown Copyright (C) 2015 Published by Elsevier B.V. All rights reserved.

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