THE PYROCHLORE SUPERGROUP OF MINERALS: NOMENCLATURE

A new scheme of nomenclature for the pyrochlore supergroup, approved by the CNMNC-IMA, is based on the ions at the A, B and Y sites. What has been referred to until now as the pyrochlore group should be referred to as the pyrochlore supergroup, and the subgroups should be changed to groups. Five groups are recommended, based on the atomic proportions of the B atoms Nb, Ta, Sb, Ti, and W. The recommended groups are pyrochlore, microlite, romite, betafite, and elsmoreite, respectively. The new names are composed of two prefixes and one root name (identical to the name of the group). The first prefix refers to the dominant anion (or cation) of the dominant valence [or H(2)O or rectangle] at the Y site. The second prefix refers to the dominant cation of the dominant valence [or H(2)O or rectangle] at the A site. The prefix "" keno-"" represents "" vacancy"". Where the first and second prefixes are equal, then only one prefix is applied. Complete descriptions are missing for the majority of the pyrochlore-supergroup species. Only seven names refer to valid species on the grounds of their complete descriptions: oxycalciopyrochlore, hydropyrochlore, hydroxykenomicrolite, oxystannomicrolite, oxystibiomicrolite, hydroxycalcioromite, and hydrokenoelsmoreite. Fluornatromicrolite is an IMA-approved mineral, but the complete description has not yet been published. The following 20 names refer to minerals that need to be completely described in order to be approved as valid species: hydroxycalciopyrochlore, fluornatropyrochlore, fluorcalciopyrochlore, fluorstrontiopyrochlore, fluorkenopyrochlore, oxynatropyrochlore, oxyplumbopyrochlore, oxyyttropyrochlore-(Y), kenoplumbopyrochlore, fluorcalciomicrolite, oxycalciomicrolite, kenoplumbomicrolite, hydromicrolite, hydrokenomicrolite, oxycalciobetafite, oxyuranobetafite, fluornatroromite, fluorcalcioromte, oxycalcioromite, and oxyplumboromite. For these, there are only chemical or crystalstructure data. Type specimens need to be defined. Potential candidates for several other species exist, but are not sufficiently well characterized to grant them any official status. Ancient chemical data refer to wet-chemical analyses and commonly represent a mixture of minerals. These data were not used here. All data used represent results of electron-microprobe analyses or were obtained by crystal-structure refinement. We also verified the scarcity of crystal-chemical data in the literature. There are crystalstructure determinations published for only nine pyrochlore-supergroup minerals: hydropyrochlore, hydroxykenomicrolite, hydroxycalcioromite, hydrokenoelsmoreite, hydroxycalciopyrochlore, fluorcalciopyrochlore, kenoplumbomicrolite, oxycalciobetafite, and fluornatroromite. The following mineral names are now discarded: alumotungstite, bariomicrolite, bariopyrochlore, bindheimite, bismutomicrolite, bismutopyrochlore, bismutostibiconite, calciobetafite, ceriopyrochlore-(Ce), cesstibtantite, ferritungstite, jixianite, kalipyrochlore, monimolite, natrobistantite, partzite, plumbobetafite, plumbomicrolite, plumbopyrochlore, stannomicrolite, stetefeldtite, stibiconite, stibiobetafite, stibiomicrolite, strontiopyrochlore, uranmicrolite, uranpyrochlore, yttrobetafite-(Y), and yttropyrochlore-(Y).

Major- and trace-element composition of olivine, perovskite, clinopyroxene, Cr-Fe-Ti oxides, phlogopite and host kamafugites and kimberlites, Alto Paranaiba, Brazil

An integrated whole-rock petrographic and geochemical study has been carried out on kamafugites and kimberlites of the Late Cretaceous Alto Paranaiba igneous province, in Brazil, and their main minerals, olivine, clinopyroxene, perovskite, phlogopite, spinels and ilmenite. Perovskite is by far the dominant repository for light lanthanides, Nb, Ta, Th and U, and occasionally other elements, reaching concentrations up to 3.4 x 10(4) chondrite values for light lanthanides and 105 chondrite for Th. A very strong fractionation between light and heavy lanthanides (chondrite-normalized La/Yb from similar to 175 to similar to 2000) is also observed. This is likely the first comprehensive dataset on natural perovskite. Clinopyroxene has variable trace-element contents. likely due to the different position of this phase in the crystallization sequence; Sc reaches values as high as 200 ppm whereas the lanthanides show very variable enrichment in light over heavy REE, and commonly show a negative Eu anomaly. The olivine, phlogopite (and tetra-ferriphlogopite), Cr-Ti oxide and ilmenite are substantially barren minerals for lanthanides and most other trace elements, with the exception of Ba, Cs and Rb in mica, and V, Nb and Ta in ilmenite. Estimated mineral/whole-rock partition coefficients for lanthanides in perovskite are similar to previous determinations, though much higher than those calculated in experiments with synthetic compositions, testifying once more to the complex behavior of these elements in a natural environment. The enormous potential for exploitation of lanthanides, Th, U and high-field-strength elements in the Brazilian kamafugites, kimberlites and related rocks is clearly shown.

Alkaline magmatism in the Amambay area, NE Paraguay: The Cerro Sarambi complex

The Early Cretaceous alkaline magmatism in the northeastern region of Paraguay (Amambay Province) is represented by stocks, plugs, dikes, and dike swarms emplaced into Carboniferous to Triassic-Jurassic sediments and Precambrian rocks. This magmatism is tectonically related to the Ponta Pora Arch, a NE-trending structural feature, and has the Cerro Sarambi and Cerro Chiriguelo carbonatite complexes as its most significant expressions. Other alkaline occurrences found in the area are the Cerro Guazu and the small bodies of Cerro Apua, Arroyo Gasory, Cerro Jhu, Cerro Tayay, and Cerro Teyu. The alkaline rocks comprise ultramafic-mafic, syenitic, and carbonatitic petrographic associations in addition to lithologies of variable composition and texture occurring as dikes; fenites are described in both carbonatite complexes. Alkali feldspar and clinopyroxene, ranging from diopside to aegirine, are the most abundant minerals, with feldspathoids (nepheline, analcime), biotite, and subordinate Ti-rich garnet; minor constituents are Fe-Ti oxides and cancrinite as the main alteration product from nepheline. Chemically, the Amambay silicate rocks are potassic to highly potassic and have miaskitic affinity, with the non-cumulate intrusive types concentrated mainly in the saturated to undersaturated areas in silica syenitic fields. Fine-grained rocks are also of syenitic affiliation or represent more mafic varieties. The carbonatitic rocks consist dominantly of calciocarbonatites. Variation diagrams plotting major and trace elements vs. SiO(2) concentration for the Cerro Sarambi rocks show positive correlations for Al(2)O(3), K(2)O, and Rb, and negative ones for TiO(2), MgO, Fe(2)O(3), CaO, P(2)O(5), and Sr, indicating that fractional crystallization played an important role in the formation of the complex. Incompatible elements normalized to primitive mantle display positive spikes for Rb, La, Pb, Sr, and Sm, and negative for Nb-Ta, P, and Ti, as these negative anomalies are considerably more pronounced in the carbonatites. Chondrite-normalized REE patterns point to the high concentration of these elements and to the strong LRE/HRE fractionation. The Amambay rocks are highly enriched in radiogenic Sr and have T(DM) model ages that vary from 1.6 to 1.1 Ga. suggesting a mantle source enriched in incompatible elements by metasomatic events in Paleo-Mesoproterozoic times. Data are consistent with the derivation of the Cerro Sarambi rocks from a parental magma of lamprophyric (minette) composition and suggest an origin by liquid immiscibility processes for the carbonatites. (C) 2011 Elsevier Ltd. All rights reserved.

Transformações de ordem-desordem no sistema ixiolita-columbita-wodginita

O mineral columbita-tantalita (muitas vezes chamado simplesmente columbita,para Nb>Ta,ou tantalita,paraNb

Estudo, desenvolvimento e caracterização de revestimentos do tipo super-rede de dureza

Nos últimos 10 anos, o desenvolvimento de técnicas de deposição e seus equipamentos permitiu o surgimento de novos tipos de filmes finos, principalmente voltados para aplicações mecânicas e tribológicas, que são multicamadas nanoestruturadas. Esses revestimentos apresentam propriedades que não são diretamente ligadas as propriedades das camadas individuais de cada material, geralmente apresentando valores de dureza extremamente elevados relacionados a um período de modulação crítico ΛC. Esses filmes demonstram um claro potencial para aplicações tribológicas mesmo com o seu comportamento de dureza ainda não completamente esclarecido. O objetivo deste trabalho é produzir multicamadas nanoestruturadas do tipo metal / nitreto pela técnica de magnetron sputtering usando Nb, Ta e TiN, visando obter uma estrutura com valores de dureza extremamente elevados, tipicamente observados em revestimentos do tipo super-redes. A estrutura periódica dos revestimentos com baixo valor de Λ (< 10 nm) foi caracterizada por XRR (Refletividade por Difração de Raios X) e por RBS (Espectrometria por Retroespalhamento Rutherford) para os valores altos de Λ. As propriedades mecânicas dos revestimentos foram avaliadas por testes instrumentados de dureza usando um equipamento Fischerscope HV100. Todas as multicamadas foram produzidas com sucesso e apresentaram uma periodicidade bem definida, o que foi confirmado pelos resultados de RBS e XRR. Os valores de dureza medidos apresentaram um comportamento tipicamente observado em superredes com um valor máximo maior que 50 GPa sempre relacionado a uma valor crítico de Λ. O valor ΛC foi 8 nm para as amostras de Nb/TiN e 4 nm para as amostras de Ta/TiN. A razão H/E indicou que o revestimento nanoestruturado mais adequado para aplicações tribológicas foram as multicamadas com maior valor de dureza. Esses resultados mostraram claramente a possibilidade de aplicação industrial destes revestimentos.

A Gagarinita e fases associadas no Granito Madeira (Pitinga, Amazonas)

O trabalho descreve a ocorrência de gagarinita-(Y) das porções mineralizadas de criolita da base do Depósito Criolítico Maciço associado à subfácies albita granito do Granito Madeira (1.8Ma) na jazida de Pitinga (Sn, Nb, Ta e criolita), onde o Y e ETR serão explorados como co-produtos. A gagarinita forma cristais anédricos de até 7mm, intersticiais ou inclusos na criolita, de cristalização anterior à criolita dos bolsões. Todos os cristais apresentam texturas típicas de exsolução, pela primeira vez descritas em fluoretos. Os padrões de exsolução são variados. Os cristais exsolvidos têm até 0,4mm, são incolores, as cores de interferência são de primeira ordem, com birrefringência 0,005-0,007, são U(-), com retardo de 150 a 210nm. A fase exsolvida distribui-se uniformemente em toda a extensão dos grãos da gagarinita-(Y), inclusive na borda; segue uma ou mais orientações preferenciais e tem dimensões semelhantes. Podem ocorrer coalescência de diferentes cristais exsolvidos, resultando em strings e stringlets. Mais raramente, a orientação é menos evidente e as dimensões dos cristais são mais variáveis No contato gagarinita/criolita, reconhece-se a formação da fase exsolvida como anterior à cristalização da criolita. A análise modal de uma população de grãos de gagarinita-(Y) com os diversos padrões texturais de exsolução fornece o valor médio de 25,8% (considerado estatisticamente representativo) de proporção de fase exsolvida em relação à fase hospedeira. Os parâmetros cristalinos da gagarinita-(Y) determinados a partir de análises por DRX são compatíveis com os da literatura. Análises por MSE, FRX e MEV da gagarinita-(Y) mostram uma composição bastante homogênea. A fórmula estrutural média calculada na base de 2(ETR+Y+Ca) é Na0,24Ca0,58Y1,01ETR0,39F5,81. O padrão de ETR normalizado ao condrito é caracterizado por enriquecimento em ETRP e anomalia negativa em Eu. A composição da fase exsolvida obtida por MSE, calculada para um total de cátions igual a 1, é Ce0,53-0,66 La0,09-0,26 Nd0,08-0,26 Sm0,01-0,04 Eu0,01Y0-0,03 F3,3-4,14. Esta fórmula é semelhante à da fluocerita, cujos picos característicos, entretanto, não ocorrem nos difratogramas. O padrão de ETR mostra um fracionamento contínuo dos ETR com empobrecimento em ETRP e discreta anomalia positiva em Eu. A composição da gagarinita inicial foi reconstituída considerando-se as proporções modais das fases hospedeira e exsolvida, obtendo-se Na0,19Ca0,48Y0,83ETR0,69F6,27. O padrão de ETR é plano com anomalia negativa em Eu menos acentuada que na gagarinita hospedeira Antes da exsolução, o sistema mineral comportava-se provavelmente como uma solução sólida com a substituição - + 2ETR3+<=> Na+ + Ca2+ + Y3+ . Formou-se, assim, uma gagarinita inicial excepcionalmente rica em ETRL (cátions relativamente grandes) cuja presença foi compensada por vacâncias, notadamente no sítio de coordenação VI. A diminuição da temperatura desestabilizou a estrutura mineral que exsolveu os cátions de ETR com raio iônico maior que o do Sm. A gagarinita hospedeira preservou os conteúdos de Y, ETRP (com exceção do Sm que se repartiu entre ela e a fase exsolvida) e Na (e Ca), constituindo uma estrutura estável, menos afetada por vacâncias e com um balanço de cargas bastante equilibrado. A fase exsolvida é um fluoreto com razão cátions/flúor= 1/3, correspondendo à composição da fluocerita. Sua estrutura não pôde ser determinada: picos da fluocerita não foram identificados e uma estrutura semelhante à da gagarinita (razão cátions/flúor= 1/2) parece pouco provável. Estudos subseqüentes poderão definir se trata-se de um novo mineral, polimorfo da fluocerita.

Low-frequency high-temperature internal friction in Ti-13Nb-13Zr alloy

Recent studies have been done to achieve biomedical alloys containing non-toxic elements and presenting low elastic moduli. It has been reported that Ti-Nb-Zr alloys rich in beta phase, especially Ti-13Nb-13Zr, have potential characteristics for substituting conventional materials such as Ti-6Al-4V, stainless steel and Co alloys. The aim of this work is to study the internal friction (IF) of Ti-13Nb-13Zr (TNZ) alloy due to the importance of the absorption impacts in orthopedic applications. The internal friction of this alloy produced by arc melting was measured using an inverted torsion pendulum with the free decay method. The measurements were performed from 77 to 700 K with heating rate of 1 K/min, in a vacuum better than 10-5 mBar. The results show a relaxation structure at high temperature strongly dependent on microstructure of the material. Qualitative discussions are presented for the experimental results, and the possibility of using the TNZ as a high damping material is briefly mentioned.

O grupo araxá na região sul-sudoeste do estado de goiás

In the S - SW region of Goiás State, Brazil, the Araxá Group is constituted of a metasedimentary sequence containing schistose and gneissic (garnet-biotite-quartz schists, feldspatic garnet-biotite-quartz schists, garnet-biotite-quartz paragneisses, with muscovite and locally amphibole, epidote, kyanite and staurolite. This sequence presents intercalations of metaul-tramafc rocks (serpentinite, actinolite schist, talc schist, chlorite schist), metamafc ones (amphibolite, amphibole schist containing or not garnet, garnet amphibolite) and associated granitic bodies. Chemically, the Araxá Group metasediments present peraluminous composition, showing enrichment in LILE, when compared with HFSE and REE, and displaying negative anomalies of Nb, Ta, Sr, P and Ti. Their chemical composition is that of greywake and the chemical characteristics of the sediments are generated in magmatic arcs. Isotopic data for Sm/Nd - model ages (TDM) between 1,04 - 1,51 and 1,76 - 2,26 Ga - and U/Pb (predominance of zircon with ages < 900 Ma) suggest that these metasediments have Neoproterozoic rocks as the source rocks. Chemical and isotopic characteristics of the studied metasediments suggest that their source are rocks originated in magmatic arcs and that they were deposited in a fore arc basin developed in the margins of Neoproterozoic island arcs.

Intrusão Alcalina de Morro Preto (go): Geologia, Petrografia e Geoquímica

A intrusão alcalina de Morro Preto, localizada ao norte da cidade de Piranhas (GO), corresponde a um corpo irregular a subcircular com aproximados 3,34 km2 alojado em gnaisses atribuídos ao Arco Magmático de Goiás. É constituída principalmente por carbonatitos e lamprófiros com graus variados de laterização e silicificação, além de silexitos e, em menor expressão, por sienito ferruginizado e basalto alcalino. Quimicamente mostram baixas concentrações em Cs, K, Na, Rb e altas concentrações em elementos como TR, Nb, Ba, Th e U. Isto aparenta resultar de processos de laterização/silicificação e da formação de fases minerais raras (ou neoformação de fases minerais), como fosfatos com alta concentração de TR e Th, oxi-hidróxidos de Fe, Ba, Mn, e oxi e/ou silico-fosfatos de ETR, Nb, Ta, dentre outros, e a formação de barita. A presença de rochas carbonatíticas com alto P2O5 e o enriquecimento acentuado em TR sugere a possibilidade de mineralizações destes componentes, similar às observadas em outros complexos alcalinos de Goiás e de Minas Gerais, como Catalão e Araxá. A distribuição de elementos menores, traços e TR mostram que as rochas são produtos de alteração de rochas ígneas alcalinas como carbonatitos, lamprófiros e basaltos alcalinos, rochas já enriquecidas em elementos como Th, U, TR (principalmente em ETRL), Nb e Ta. Os teores anormalmente altos são resultado do processo de enriquecimento supérgeno (processos de intemperismo como silicificação e laterização) e/ou alteração hidrotermal com baixa temperatura.

Aplicação de cavacos de titânio para produção de revestimentos resistentes ao desgaste

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Ortognaisses peraluminosos associados ao Grupo Araxá na região de Mairipotaba-Prof. Jamil Safady, Goiás

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Geoquímica e geocronologia U-Pb e ­Sm-Nd dos ortognaisses da região de Pontalina (GO), Brasil

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Biocompatibility of experimental Ti-30Ta implants with compromised primary stability: effect of TEA

Purpose: Ti-Ta alloys have high potential for dental application due to a good balance between high strength and low modulus. Absence of primary anchoring may occur when dental implants are installed immediately after tooth extraction. Tranexamic acid (TEA) is used to reduce fibrin degradation and can prevent early blood clot breakdown. The aim of this study was to evaluate the biocompatibility of Ti-30Ta implants associated or not with tranexamic acid and installed with compromised primary stability. Methods and materials: Fabricated were 20 implants of titanium ASTM F67 (Grade 4) and 20 implants of Ti-30Ta alloy with dimensions of 2.1 mm × 2.8 mm Ø. They were divided (n = 10) into Group I (Ti machined), Group II (Ti machined/tranexamic acid), Group III (Ti-30Ta alloy) and Group IV (Ti-30Ta/tranexamic acid) and were implanted in tibia (defects with 2.5 mm × 3.2 mm Ø) of 40 male rats (250 g). The surgical sites were rinsed with 5% tranexamic acid solution in Groups II and IV. The animals were euthanized at 45 days postoperative. The pieces were processed in methyl methacrylate (Stevenel's blue/Alizarin red). The percentage of peri-implant tissue repair was analyzed via images obtained by an optical microscope coupled to a digital camera using Leica software and Adobe Photoshop QWin. Data were analyzed statistically with a significance level of 5%. Results: Histomorphometric results showed 97.16% of bone-implant contact for group IV, 89.78% of bone contact for group III, 70.89% for group II and 61.59% of bone contact for group I. The statistical analyses demonstrated significant differences (P < 0.05) among group I and other groups. Conclusion: The results suggest that (a) Ti-30Ta promoted an increase of bone healing and apposition around implant; (b) tranexamic acid favored the stabilization of blood clot and bone formation.

Ortognaisses peraluminosos associados ao grupo Araxá na região de Rochedo, Goiás

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Petrogenesis of Cenozoic volcanic rocks in the NW sector of the Gharyan volcanic field, Libya

The north-western sector of the Gharyan volcanic field (northern Libya) consists of trachytic-phonolitic domes emplaced between similar to 41 and 38 Ma, and small-volume mafic alkaline volcanic centres (basanites, tephrites. alkali basalts. hawaiites and rare benmoreites) of Middle Miocene-Pliocene age (similar to 12-2 Ma). Two types of trachytes and phonolites have been recognized on the basis of petrography, mineralogy and geochemistry. Type-1 trachytes and phonolites display a smooth spoon-shaped REE pattern without negative Europium anomalies. Type-2 trachytes and phonolites show a remarkable Eu negative anomaly, higher concentration in HFSE (Nb-Ta-Zr-Hf), REE and Ti than Type-1 rocks. The origin of Type-1 trachytes and phonolites is compatible with removal of clinopyroxene, plagioclase, alkali feldspar, amphibole. magnetite and titanite starting from benmoreitic magmas. found in the same outcrops. Type-2 trachytes and phonolites could be the result of extensive fractional crystallization starting from mafic alkaline magma, without removal of titanite. In primitive mantle-normalized diagrams, the mafic rocks (Mg#= 62-68, Cr up to 514 ppm, Ni up to 425 ppm) show peaks at Nb and Ta and troughs at K. These characteristics, coupled with low Sr-87/Sr-86(i) (0.7033-0.7038) and positive epsilon(Nd) (from +4.2 to + 5.3) features typical of the mafic anorogenic magmas of the northern African plate and of HIMU-OIB-like magma in general. The origin of the mafic rocks is compatible from a derivation from low degree partial melting (3-9%) shallow mantle sources in the spinel/gamet facies. placed just below the rigid plate in the uppermost low-velocity zone. The origin of the igneous activity is considered linked to passive lithospheric thinning related to the development of continental rifts like those of Sicily Channel (e.g.. Pantelleria and Linosa) and Sardinia (e.g., Campidano Graben) in the Central-Western Mediterranean Sea. (C) 2012 Elsevier B.V. All rights reserved.