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Transition metal rutiles and titanates from the Deadhorse Creek diatreme complex, northwestern Ontario, Canada
- R. Garth Platt, Roger H. Mitchell
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- Journal:
- Mineralogical Magazine / Volume 60 / Issue 400 / June 1996
- Published online by Cambridge University Press:
- 05 July 2018, pp. 403-413
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The main mineralized zone of the West subcomplex of the Deadhorse Creek diatreme complex, northwestern Ontario possesses an exotic mineralogy. Mineralization involves the first-order transition metals (principally Sc, Ti, V, Cr, Mn, and Fe), the second-order transition metals (principally Zr and Nb), the lanthanides, the actinides (principally Th and U), Be, Ba and Sr. Minerals include phenacite, zircon, uraninite, thorite, monazite-(Ce), xenotime-(Y), barylite, thortveitiite, hollandite, tyuyamunite, a number of unknown and as yet undescribed species, and those minerals more specifically described in this paper. These are Cr-V-Nb rutile, V-rich members of the crichtonite series, and a titanate of general composition (Cr,V3+,Fe3+)2(Ti,V4+,Nb)O5.
Similar to rutiles reported from alkaline rocks in general, the Deadhorse Creek rutiles are enriched in Cr and Nb, with the latter element attaining some of the highest recorded values. V contents are also unusually high and this element is thought to exist in both the tri- and tetravalent states.
The V-rich crichtonites are essentially vanadium analogues of crichtonite and lindsleyite. M-site Nb and V are the highest yet recorded. A-site cations are dominated by Ba and Sr with an inverse relationship together with lesser but significant amounts of Ca and Pb. Although not of upper mantle origin, they plot in the upper mantle LIMA quadrant of TiO2vs. FeO + Fe2O3 + MgO (Haggerty, 1991).
(Cr,V3+,Fe3+)2(Ti,V4+,Nb)O5 is thought to be a member of an homologous series of type (Cr,V3+,Fe3+)2p(Ti,V4+,Nb)2p+qO5p+4q with p = 1 and q = 0 and a V3O5-type structure. Whether this structure is ultimately derived from that of rutile or from α-PbO2 by crystallographic shear is not known.
The rutiles and titanates discussed here are thought to have formed from hydrous alkaline solutions which have scavenged the necessary elements from a mafic/ultramafic source. The origin of the solutions is not specifically known although the magmatic activity associated with the spatially related Coldwell alkaline complex and/or the Prairie Lake complex are both potential sources. Both complexes contain the necessary mafic/ultramafic rocks.
The Peralkaline Nepheline Syenites of the Junguni Intrusion, Chilwa Province, Malawi
- Alan R. Woolley, R. Garth Platt
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- Journal:
- Mineralogical Magazine / Volume 52 / Issue 367 / September 1988
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- 05 July 2018, pp. 425-433
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The mineralogy of the highly peralkaline Junguni nepheline syenite intrusion of the Chilwa alkaline province has been investigated. The rocks comprise alkali feldspar, very abundant nepheline, locally exceptionally abundant sodalite, sodic pyroxenes, scarce biotite, rare amphibole, and an extensive range of accessory minerals. Electron microprobe analyses indicate that the pyroxenes define an evolutionary trend from salite through aegirine-augite to aegirine, which is unusual in its broadness and ill-definition. This is explained by a series of overlapping trends produced by fluctuating Fe3+/Fe2+ ratios caused by variations in alkali content of the magma, probably produced by periodic alkali loss by surface de-gassing. Much of the sodalite occurs as a primary liquidus phase, but the paragenesis of certain ramifying sodalite veins is more problematical. It is possible that such ramifying masses are the product of coupled migration of alkalis and volatiles by diffusion in a gravitation field under pressure gradients generated by eruptive events, or by the formation of immiscible Na- and Cl-rich liquids. Both early calcic and late mangan-fluor eckermannitic/arfvedsonitic amphiboles occur. The micas vary from biotites with Mg: Fe ratios < 0·5 to almost pure annites; they are fluor-micas and characterized by high Mn contents. Analyses of niobian rutile, mangan ilmenite, ferroan pyrophanite, manganese-rich eucolite, låvenite, mangan-titan låtvenite, rosenbuschite, wöhlerite, pyrochlore, eudialyte and what is believed to be only the second occurrence of kupletskite are given. Many of these minerals are rich in Zr, Nb, Na and Mn and thus typical of the assemblages found in extreme agpaitic complexes such as Ilimaussaq and Lovozero.
The mafic mineralogy of the peralkaline syenites and granites of the Mulanje complex, Malawi
- R. Garth Platt, Alan R. Woolley
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- Journal:
- Mineralogical Magazine / Volume 50 / Issue 355 / March 1986
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- 05 July 2018, pp. 85-99
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Studies of the mafic mineralogy of the Mulanje granite-quartz-syenite-syenite Massif of southern Malawi delineate two mineralogically distinct complexes—the Main complex and the Chambe complex. Each complex is associated with its own trend of pyroxene evolution. The Main complex pyroxenes exhibit initial enrichment in hedenbergite before subsequent enrichment in acmite (i.e. sodic-salite-sodic-hedenbergite-aegirine-hedenbergite-aegirine), whereas the Chambe pyroxenes display constantly increasing acmite content with no significant enrichment in hedenbergite (i.e. sodic-salite-aegirine-augite-aegirine). This phenomenon is also reflected in the more Mg-rich amphiboles and biotites of the Chambe rocks when compared to those of the Main complex.
The general evolutionary trend of the Main complex amphiboles is katophorite → ferroricherite → arfvedsonite which broadly correlates with a change in rock type from syenite to granite. Superimposed on this trend is an essentially similar, yet less extensive trend of the more Mg-rich Chambe amphiboles. The micas of both complexes show a general evolution to more iron-rich compositions with relatively constant Al content. Those of the Main complex, however, display extreme iron enrichment with ultimate formation of essentially pure ferrous annite.
Aenigmatite, astrophyllite, fayalite, chevkinite, yttrofluorite, and unidentified RE minerals are characteristic of the Main complex rocks but totally absent from those of the Chambe complex. Ilmenite constitutes the only iron oxide phase in the Main complex rocks whereas titaniferous magnetite (now unmixed) and ilmenite are both present in the rocks of Chambe.
The differences between the two complexes are explained in terms of oxygen fugacity, silica activity, crystallization interval, and the relative rates of development of peralkalinity. In essence, the Chambe magmas are considered to have crystallized under high fO2 conditions with an earlier development of peralkaline tendencies when compared to those of the Main complex magmas. Moreover, a lower initial silica activity, a smaller alkali to alumina ratio, and a correspondingly smaller crystallization interval could account for the lack of highly evolved granitic magmas in the Chambe complex, whereas such magmas are integral in the evolution of the Main complex.
Perovskite, loparite and Ba-Fe hollandite from the Schryburt Lake carbonatite complex, northwestern Ontario, Canada
- R. Garth Platt
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- Journal:
- Mineralogical Magazine / Volume 58 / Issue 390 / March 1994
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- 05 July 2018, pp. 49-57
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Within a suite of felsic-free, mica-rich alkaline ultramafic rocks of the Schryburt Lake carbonatite complex of northwestern Ontario, loparite and Ba-Fe hollandite occur in intimate association with perovskite. The host rocks have variable modal proportions of Mg-olivine, phlogopite, magnetite, ilmenite, apatite and carbonate (generally calcite) with minor Mg-salite. Thus, they correspond to ultramafic lamprophyres (i.e. aillikites), in the sense of Rock (1990) or the lamprophyric facies of the melilitite clan, in the sense of Mitchell (1993).
Perovskite is the principal titanate phase, forming both euhedral and anhedral grains, the latter showing evidence of marginal resorption. It exhibits complex zonal patterns due principally to variations in the light rare earth elements, Na and Nb. In the nomenclature suggested, they may be termed perovskite and cerian perovskite. Loparite forms as small euhedral overgrowths on corroded perovskite cores. Chemically they are essentially solid solutions of loparite, lueshite and perovskite. Consequently, they may be termed calcian-loparite, calcian niobian loparite, niobian calcian loparite, loparite and niobian loparite. Titanates of the hollandite group are rare accessory minerals whose composition closely approach that of the septatitanate BaFe2+Ti7O16.
The complex zoning of the perovskite grains has been attributed to the periodic introduction of carbonatite-derived fluids enriched in REE, Na and Nb into the silicate system during perovskite crystallization. Subsequent reaction of the early perovskite with F-bearing fluids leads to a localized environment enriched in Ti, Na, Nb and REE derived from both the fluid phase and the unstable perovskite. Loparite subsequently crystallizes from these micro-chemical environments.
The mineralogy of nepheline syenite complexes from the northern part of the Chilwa Province, Malawi
- Alan R. Woolley, R. Garth Platt
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- Journal:
- Mineralogical Magazine / Volume 50 / Issue 358 / December 1986
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- 05 July 2018, pp. 597-610
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The mineralogy, including the accessory phases låvenite, rosenbuschite, and catapleiite, and consequent petrogenetic implications have been investigated for a group of four overlapping nepheline syenite complexes (Chikala, Chaone, Mongolowe, and Chinduzi) and for spatially associated silica-saturated and over-saturated perthosites, from the northern part of the Chilwa Alkaline Province, Malawi.
The complexes are thought to have formed by injection into high-level chambers of magma pulses genetically related to a common source magma at depth. Evidence for the source magma is preserved in salitic cores observed in the pyroxenes and a trend to more hedenbergite-rich compositions is believed to have formed by evolution of this magma. Subsequent trends of acmite enrichment followed magma injection into the higher-level chambers; the actual pyroxene trend associated with each individual complex is a function of the evolution attained by the source magma, oxidation potential, and perhaps even alkali activity. On the basis of such a two-stage model, the pyroxene data suggest emplacement of the Chaone and Mongolowe magmas somewhat earlier than that of Chikala, with the Chinduzi magma migrating even later.
Amphiboles and biotites are believed to have formed after high-level injection of the magmas. Their compositions broadly reflect the nature of the crystallizing pyroxenes in that magnesian hastingsitic hornblendes and more Mg-rich biotites are associated with more Mg-rich sodic pyroxenes, whereas katophorites and annite-rich micas are generally associated with sodic pyroxenes somewhat richer in hedenbergite. Sub-solidus crystallization in some of the complexes is represented by aegirine and magnesio-arfvedsonite. Nepheline compositions indicate broadly similar crystallization temperatures within the complexes, namely 950 to 750°C. Oxygen fugacities for these magmas obtained from biotite/annite compositions vary from 10−19 to 10−14 bars for this temperature range. Mineralogical data, particularly from pyroxenes and amphiboles, strongly suggest that the perthosites, spatially associated with the nepheline syenite complexes, are genetically unrelated.