Published January 1, 2014 | Version v1
Journal article Open

Petrology of Quaternary volcanic rocks and related plutonic xenoliths from Golcuk volcano, Isparta Angle, Turkey: Origin and evolution of the high-K alkaline series

  • 1. Univ Paris Sud, UMR CNRS 8148, Lab GEOPS, F-91405 Orsay, France
  • 2. Suleyman Demirel Univ, Dept Geothermal Energy & Mineral Ressources, TR-32260 Isparta, Turkey
  • 3. CEA CNRS UVSQ, Lab Sci Climat & Environm, UMR 8212, F-91191 Gif Sur Yvette, France

Description

The Quaternary volcanism of Isparta, south-western Anatolia, belongs to the post-collisional alkalipotassic to ultrapotassic magmatism, active since Miocene, from Afyon to Isparta. In the so-called Isparta Angle, the magmatism is contemporaneous with the Aegean extensional regime initiated during the Late Miocene and active throughout the Pliocene and Quaternary. The Golcuk volcano-forming stages consist of three main eruptive cycles: Cycle I comprising 200 m-thick pyroclastic flow deposits; Cycle II consisting of tephriphonolitic lava dome-flows extruded throughout the caldera; and Cycle III characterized by tuff-ring deposits related to the last phreatoplinian events. These late explosive events sampled plutonic xenoliths that allow to better constrain magma fractionation processes that operated at depth in the magma chamber. Magma evolution was first controlled by accumulation of clinopyroxene, phlogopite and apatite, then by phlogopite, amphibole and feldspars, with apatite, magnetite, titanite and zircon as accessories. Crystallization of clinopyroxene, phlogopite and amphibole probably controlled the silica-saturation trend of the whole series and faithfully reflect intensive H2O variations in the magma that were responsible of explosive cyclic events. The parental magma may have had a lamprophyric-tephritic composition. Trace element and isotope ratios indicate a prevalent asthenospheric source versus lithospheric one. Geochemical features, such as strong enrichment of LILE, REE, HFSE in the Golcuk magma point to the involvement of a asthenospheric OIB-type melt with a possible carbonatitic component, that interacted with remnants of the delaminated lithosphere during upwelling. (C) 2014 Elsevier Ltd. All rights reserved.

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