Noble gases in the Finero phlogopite-peridotites, western Italian Alps

Takuya Matsumoto*, Tomoaki Morishita, Jun Ichi Matsuda, Toshiyuki Fujioka, Masamichi Takebe, Koshi Yamamoto, Shoji Arai

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    29 Citations (Scopus)

    Abstract

    Here we report results from an investigation of noble gases in a specimen with layers of very fine-grained apatite and orthopyroxene from the Finero ultramafic complex, western Italian alps. We have also examined fresh olivine grains separated from phlogopite-harzburgites without an apatite layer. Fluid inclusions of these olivine separates appeared rich in radiogenic components such as 4He, 21Ne and 40Ar, suggesting the derivation of fluids from a crust-like reservoir. Such a crust-like component also appeared to be contained in the samples with the apatite-opx layer, however, an additional isotopically distinct component is necessary to explain progressive increases in 3He concentration and decreases in 40Ar/36Ar ratios observed approaching the apatite-rich layer. High 3He contents and low 40Ar/36Ar ratios are consistent with the signature expected for slab-derived metasomatic fluids. There is a clear mixing trend defined in a 3He/36Ar vs. 40Ar/36Ar diagram with crustal and slab-derived fluids as end-member compositions, suggesting that the complex was metasomatised by fluids derived from geochemically distinct regions and distinct geotectonic settings. The parent melt or fluids responsible for the formation of the apatite-rich layer should be derived from the slab-derived component, which is consistent with the notion that the Finero mantle was once in the mantle wedge. An in situ component produced in the previously metasomatised portion of lithospheric mantle, or fluid released from surrounding metamorphic rocks during exhumation are possible sources for the crust-like component.

    Original languageEnglish
    Pages (from-to)130-145
    Number of pages16
    JournalEarth and Planetary Science Letters
    Volume238
    Issue number1-2
    DOIs
    Publication statusPublished - 30 Sept 2005

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