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Fe-Ti oxide-silicate (QUIlF-type) equilibria in feldspathoid-bearing systems

Julian Schilling, B. Ronald Frost, Michael A. W. Marks, Thomas Wenzel and Gregor Markl
Fe-Ti oxide-silicate (QUIlF-type) equilibria in feldspathoid-bearing systems
American Mineralogist (January 2011) 96 (1): 100-110

Abstract

Silicate-oxide equilibria (abbreviated as QUIlF) have proven to be very powerful tools for reconstructing the temperature and oxygen fugacity evolution of magmatic systems containing magnetite and ilmenite with olivine, quartz, or pyroxenes. In this paper, we extend these QUIlF equilibria to include rocks where silica activity is controlled by equilibria between feldspars and feldspathoids. We present data on the orthomagmatic assemblage of titanomagnetite + ilmenite + feldspar + nepheline + compositionally variable olivine, which we call AUNIlF: NaAlSi (sub 3) O (sub 8 Albite) + 4Fe (sub 2) TiO (sub 4 Ulvospinel) =NaAlSiO (sub 4 Nepheline) + 4FeTiO (sub 3 Ilmenite) + 2Fe (sub 2) SiO (sub 4 Fayalite) . The AUNIlF reference curve (with unit activities for albite, nepheline, and fayalite) is stable at oxygen fugacities > or =2 log units below the QUIlF surface at temperatures of about 700 to 800 degrees C, temperatures typical of late-magmatic stages. At temperatures > approximately 800 degrees C, the AUNIlF reference assemblage would only be stable at unrealistically low f (sub O2) conditions more than 5 log units below FMQ (where FMQ is the fayalite-magnetite-quartz buffer), which explains the rarity or absence of orthomagmatic AUNIlF assemblages. We determine the most reduced conditions indicated by displaced AUNIlF assemblage from Mont Saint-Hilaire (Quebec, Canada) to be Delta FMQ=-1.15 at approximately 800 degrees C (olivine is Fa (sub 67) and a (sub SiO2) =0.41) and conclude that AUNIlF assemblages involving pure fayalite do not stably occur in terrestrial magmatic systems. The stability field of naturally occurring AUNIlF assemblages is a function of albite, nepheline, and olivine compositions and is controlled by the ratio of silica activity to fayalite activity (a (sub SiO2) /a (sub Fa) ). At values higher than approximately 0.77 for a (sub SiO2) /a (sub Fa) , olivine is Fa< approximately 70 when silica activity is buffered by the nepheline-albite equilibrium. In these situations, AUNIlF is stable at oxygen fugacities > or =-1.15 (Delta FMQ). At values below a (sub SiO2) /a (sub Fa) approximately 0.77, the AUNIlF equilibrium is shifted to lower oxygen fugacities and ilmenite becomes unstable relative to ulvospinel. Analogous to the construction and application of AUNIlF, a QUIlF-type reaction curve for potassic systems (KULIlF) involving leucite and alkali feldspar is presented and applied to naturally occurring assemblages. Potassic rocks invariably crystallize forsteritic olivine in the presence of ilmenite and magnetite, reflecting higher oxygen fugacities during crystallization than their sodic counterparts. As a result of low fayalite component in olivine, the a (sub SiO2) /a (sub Fa) ratio becomes > or =4 in assemblages of potassic systems consisting of alkali feldspar, magnetite, leucite, ilmenite, and olivine.


ISSN: 0003-004X
EISSN: 1945-3027
Coden: AMMIAY
Serial Title: American Mineralogist
Serial Volume: 96
Serial Issue: 1
Title: Fe-Ti oxide-silicate (QUIlF-type) equilibria in feldspathoid-bearing systems
Affiliation: Universitaet Tuebingen, Institut fuer Geowissenschaften, Tubingen, Germany
Pages: 100-110
Published: 201101
Text Language: English
Publisher: Mineralogical Society of America, Washington, DC, United States
References: 39
Accession Number: 2011-012695
Categories: General mineralogy
Document Type: Serial
Bibliographic Level: Analytic
Illustration Description: illus. incl. 4 tables
N45°00'00" - N63°00'00", W79°00'00" - W57°00'00"
Secondary Affiliation: University of Wyoming, USA, United States
Country of Publication: United States
Secondary Affiliation: GeoRef, Copyright 2017, American Geosciences Institute. Abstract, copyright, Mineralogical Society of America. Reference includes data from GeoScienceWorld, Alexandria, VA, United States
Update Code: 201108
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