Molecular organization of n-cyanobiphenyl liquid crystals on a molybdenite surface

The alignement and anchoring of liquid crystals on solid surfaces is a key problem for modern device technology that until now has been treated empirically, but that can now be tackled by atomistic computer simulations. Molecular dynamics (MD) simulations were used in this thesis work to study two films of 7 and 8 n-alkyl-4’cyanobiphenyl (7CB and 8CB) liquid crystals , with a thickness of 15 nm, confined between two (001) surfaces of MoS2 (molybdenite). The isotropic and nematic phases of both liquid crystals were simulated, and the resulting structures characterized structurally. A new force field was designed to model the interactions between the liquid crystal (LC) molecules and the surface of molybdenite, while an accurate force field developed previously was used to model the 7CB and 8CB molecules. The results show that the (001) molybdenite surface induces a planar orientation in both the liquid crystals. For the nematic phase of 8CB, one of the two solid/LC interfaces is composed of a first layer of molecules aligned parallel to the surface, followed by a second layer of molecules aligned perpendicular to the surface (also called, homeotropic). The effect of the surface appears to be local in nature as it is confined to the first 15 Angström of the LC film. Conversely, for the nematic phase of 7CB, a planar ordering is established into the LC film. The LC molecules at the interface with the molybdenite appear to align preferentially their alkyl chains toward the solid substrate. The resulting tilt angle of molecules was found to be in good agreement with experimental measurements available in literature. Despite the fact that the MD simulations spanned a time range of more than 100 ns, the nematic phases of both 7CB and 8CB were found not to be completely formed. In order to confirm the findings presented in this thesis, we propose to extend the current study.

Dissulfeto de molibdênio, um material multifuncional e surpreendente

The aim of this work is to review the chemical and physical properties of layered molybdenum disulfide. The three polymorphic/polytypic modifications of the compound were found, the polytypes 2H (molybdenite) and 3R are semiconductors while the polymorph 1T is an electronic conductor. 2H-MoS2 has several important industrial applications as hydrotreatment catalysts, energy storage devices, solar cells, solid lubricants, among others. When intercalated, the 2H phase changes to a distorted 1T phase, producing unstable intercalation compounds that can be exfoliated in solution, producing single layers and consequently nanocomposites. The direct synthesis of the 1T phase produces stable intercalation compounds. Recently molybdenum disulfide was prepared as nanotubes and fulerene-like structures that bring new insights in the investigation of this important material.

Estudo da dissolução oxidativa microbiológica de uma complexa amostra mineral contendo pirita (FeS2), Pirrotita (Fe1-xS) e Molibdenita (MoS2)

This work aims to study the oxidation of a complex molybdenite mineral which contains pyrite and pyrrotite, by Acidithiobacillus ferrooxidans. This study was performed by respirometric essays and bioleaching in shake flasks. Respirometric essays yielded the kinetics of mineral oxidation. The findings showed that sulfide oxidation followed classical Michaelis-Menten kinetics. Bioleaching in shake flasks allowed evaluation of chemical and mineralogical changes resulting from sulfide oxidation. The results demonstrated that pyrrotite and pyrite were completely oxidized in A. ferrooxidans cultures whereas molybdenite was not consumed. These data indicated that molybdenite was the most recalcitrant sulfide in the sample.

Estudo da oxidação dos sulfetos sintéticos molibdenita (MoS2) e covelita (CuS) por Acidithiobacillus ferrooxidans via respirometria celular

This paper analyses the oxidation of covellite and molybdenite by Acidithiobacillus ferrooxidans strain LR using respirometric experiments. The results showed that both sulfides were oxidized by A. ferrooxidans, however, the covellite oxidation was much higher than molybdenite. Regarding the kinetic oxidation, the findings revealed that just molybdenite oxidation followed the classical Michaelis-Menten kinetic. It is probably associated with the pathway which these sulfides react to chemistry-bacterial attack, what is influenced by its electronic structures. Besides, experiments conducted in the presence of Fe3+ did not indicate alterations in molybdenite oxidation. Thus, ferric ions seem not to be essential to the sulfide oxidations.

Geology of the Sand Creek porphyry molybdenum prospect /

The Sand Creek Prospect is located within the eastern exposed margin of the Coast Plutonic Complex. The occurrence is a plug and dyke porphyry molybdenum deposit. The rock types, listed in decreasing age: 1) metamorphlc schists and gneisses; 2) diorite suite rocks - diorite, quartz diorite, tonalite; 3) rocks of andesitic composition; 4) granodiorites, coarse porphyritic granodiorite, quartzfeldspar porphyry, feldspar porphyry; and 5) lamprophyre. Hydrothermal alteration is known to have resulted from emplacement of the hornblende-feldspar porphyry through to the quartz-feldspar porphyry. Molybdenum mineralization is chiefly associated with the quartz-feldspar porphyry. Ore mineralogy is dominated by pyrite with subordinate molybdenite, chalcopyrite, covelline, sphalerite, galena, scheelite, cassiterite and wolframite. Molybdenite exhibits a textural gradation outward from the quartz-feldspar porphyry. That is, disseminated rosettes and rosettes in quartz veins to fine-grained molybdenite in quartz veins and potassic altered fractures to fine-grained molybdenite paint or 6mears in the peripheral zones. The quartz-feldspar porphyry dykes were emplaced in an inhomogeneous stress field. The trend of dykes, faults and shear zones is 0^1° to 063° and dips between 58° NW and 86* SE. Joint Pole distribution reflects this fault orientation. These late deformatior maxima are probably superimposed upon annuli representing diapiric emplacement of the plutons. A model of emplacement involving two magmatic pulses is given in the following sequence: Diorite pulse (i) dioritequartz diorite, (ii) tonalites; granodiorite pulse (iii) hornblende-fildspar microporphyry, hornblende/biotite porphyry, (iv) coarse grained granodiorite, (v) quartz-feldspar porphyry, (vi) feldspar porphyry, and (vii) lamprophyre. The combination of plutonic and coarse porphyritic textures, extensive propylitic overprinting of potassic alteration assemblages suggests that the. prospect represents the lower reaches of a porphyry system.

Estudo da oxidação dos sulfetos sintéticos molibdenita (MoS2) e covelita (CuS) por Acidithiobacillus ferrooxidans via respirometria celular

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Estudo da dissolução oxidativa microbiológica de uma complexa amostra mineral contendo pirita (FeS2), pirrotita (Fe 1-XS) e molibdenita (MoS2)

This work aims to study the oxidation of a complex molybdenite mineral which contains pyrite and pyrrotite, by Acidithiobacillus ferrooxidans. This study was performed by respirometric essays and bioleaching in shake flasks. Respirometric essays yielded the kinetics of mineral oxidation. The findings showed that sulfide oxidation followed classical Michaelis-Menten kinetics. Bioleaching in shake flasks allowed evaluation of chemical and mineralogical changes resulting from sulfide oxidation. The results demonstrated that pyrrotite and pyrite were completely oxidized in A. ferrooxidans cultures whereas molybdenite was not consumed. These data indicated that molybdenite was the most recalcitrant sulfide in the sample.

Estudo da oxidação de covelita (CuS) e molibdenita (MoS2) sintéticas por Acidithiobacillus ferrooxidans

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Estudos isotópicos (Pb, O, H, S) em zonas alteradas e mineralizadas do depósito cupro-aurífero Visconde, Província Mineral de Carajás

O depósito cupro-aurífero Visconde está localizado na Província Mineral de Carajás, a cerca de 15 km a leste do depósito congênere de classe mundial Sossego. Encontra-se em uma zona de cisalhamento de direção WNW-ESE, que marca o contato das rochas metavulcanossedimentares da Bacia Carajás com o embasamento. Nessa zona ocorrem outros depósitos hidrotermais cupro-auríferos com características similares (Alvo 118, Cristalino, Jatobá, Bacaba, Bacuri, Castanha), que têm sido enquadrados na classe IOCG (Iron Oxide Copper-Gold), embora muitas dúvidas ainda existam quanto a sua gênese, principalmente no que diz respeito à idade da mineralização e fontes dos fluidos, ligantes e metais. O depósito Visconde está hospedado em rochas arqueanas variavelmente cisalhadas e alteradas hidrotermalmente, as principais sendo metavulcânicas félsicas (2968 ± 15 Ma), o Granito Serra Dourada (2860 ± 22 Ma) e gabros/dioritos. Elas registram diversos tipos de alteração hidrotermal com forte controle estrutural, destacando-se as alterações sódica (albita + escapolita) e sódico-cálcica (albita + actinolita ± turmalina ± quartzo ± magnetita ± escapolita), mais precoces, que promoveram a substituição ubíqua de minerais primários das rochas e a disseminação de calcopirita, pirita, molibdenita e pentlandita. Dados isotópicos de oxigênio e hidrogênio de minerais representativos desses tipos de alteração mostram que os fluidos hidrotermais foram quentes (410 – 355°C) e ricos em ¹⁸O (δ¹⁸O_H2O= +4,2 a 9,4‰). Sobreveio a alteração potássica, caracterizada pela intensa biotitização das rochas, a qual ocorreu concomitantemente ao desenvolvimento de foliação milonítica, notavelmente desenhada pela orientação de palhetas de biotita, que precipitaram de fluidos com assinatura isotópica de oxigênio similar à dos estágios anteriores (δ¹⁸O_H2O entre +4,8 e +7,2‰, a 355°C). Microclina e alanita são outras fases características desse estágio, além da calcopirita precipitada nos planos da foliação. A temperaturas mais baixas (230 ± 11°C), fluidos empobrecidos em ¹⁸O (δ¹⁸O_H2O = -1,3 a +3,7‰) geraram associações de minerais cálcico-magnesianos (albita + epidoto + clorita ± calcita ± actinolita) que são contemporâneas à mineralização. Valores de δ¹⁸D_H2O e δO_H2O indicam que os fluidos hidrotermais foram inicialmente formados por águas metamórficas e formacionais, a que se misturou alguma água de fonte magmática. Nos estágios tardios, houve considerável influxo de águas superficiais. Diluição e queda da temperatura provocaram a precipitação de abundantes sulfetos (calcopirita ± bornita ± calcocita ± digenita), os quais se concentraram principalmente em brechas tectônicas - os principais corpos de minério - que chegam a conter até cerca de 60% de sulfetos. Veios constituídos por minerais sódico-cálcicos também apresentam comumente sulfetos. A associação de minerais de minério e ganga indica uma assinatura de Cu-Au- Fe-Ni-ETRL-B-P para a mineralização. Os valores de δ³⁴S (-1,2 a +3,4‰) de sulfetos sugerem enxofre de origem magmática (proveniente da exsolução de magmas ou da dissolução de sulfetos das rochas ígneas pré-existentes) e precipitação em condições levemente oxidantes. Datação do minério por lixiviação e dissolução total de Pb em calcopirita forneceu idades de 2736 ± 100 Ma e 2729 ± 150 Ma, que indicam ser a mineralização neoarqueana e, a despeito dos altos erros, permite descartar um evento mineralizador paleoproterozoico. A idade de 2746 ± 7 Ma (MSDW=4,9; evaporação de Pb em zircão), obtida em um corpo granítico não mineralizado (correlacionado à Suíte Planalto) que ocorre na área do depósito, foi interpretada como a idade mínima da mineralização. Assim, a formação do depósito Visconde teria relação com o evento transpressivo ocorrido entre 2,76 e 2,74 Ga, reponsável pela inversão da Bacia Carajás e pela geração de magmatismo granítico nos domínios Carajás e de Transição. Esse evento teria desencadeado reações de devolatilização em rochas do Supergrupo Itacaiúnas, ou mesmo, provocado a expulsão de fluidos conatos salinos aprisionados em seus intertícios. Esses fluidos teriam migrado pelas zonas de cisalhamento e reagido com as rochas (da bacia e do embasamento) pelas quais se movimentaram durante a fase dúctil. As concentrações subeconômicas do depósito Visconde devem ser resultado da ausência de grandes estruturas que teriam favorecido maior influxo de fluidos superficiais, tal como ocorreu na formação dos depósitos Sossego e Alvo 118.

Depósito Cu-Au Visconde, Carajás (PA): geologia e alteração hidrotermal das rochas encaixantes

Distante 15 km a leste da mina Sossego (Canaã de Carajás, no Pará), o depósito Visconde jaz na zona de contato entre o Supergrupo Itacaiúnas (2,76 Ga) e o embasamento (> 3.0 Ga). No depósito e arredores, ocorrem, principalmente, o granito Serra Dourada, riodacitos e gabrodioritos, variavelmente deformados e hidrotermalizados. A Suíte Intrusiva Planalto, também identificada, não mostra feições de alteração das demais rochas. Diques máficos e félsicos cortam o pacote rochoso. Sob condições dúctil-rúpteis iniciais a rúpteis, subsequentemente, a alteração hidrotermal evoluiu de sódico-cálcica (albita, escapolita e anfibólios) precoce e ubíqua para potássica (K-feldspato e Cl-biotita), retomando, em seguida, o caráter sódico-cálcico de efeito local (albita, epidoto, apatita, turmalina e fluorita), para, finalmente, assumir caráter cálcio-magnesiano (clinocloro, actinolita, carbonatos e talco subordinado). No granito Serra Dourada, albitização, epidotização e turmalinização são mais proeminentes e se contrapõem à escapolitização, biotitização, anfibolitização e magnetitização, muito expressivas nos gabros/quartzodioritos, e à K-feldspatização, mais comum nos riodacitos. Os principais corpos de minério são representados por veios e brechas, constituídos por calcopirita-bornita, além de disseminações (calcopirita + pirita ± molibdenita ± pentlandita). A suíte metálica básica é Fe-Cu-Au ± ETR. Abundante sulfeto foi precipitado na transição da alteração potássica para a cálcio-magnesiana, tendo apatita, escapolita, actinolita, epidoto, magnetita, turmalina, calcita, gipsita e fluorita como os principais minerais de ganga. Os metais foram transportados por fluidos hidrotermais ricos em Na, Ca, K, Fe e Mg, além de P, B, F e espécies de S. As similaridades se sobrepõem às diferenças, o que permite considerar os depósitos Visconde e Sossego cogenéticos.

Magmatic–hydrothermal molybdenum isotope fractionation and its relevance to the igneous crustal signature

We analysed the Mo isotope composition of a comprehensive series of molybdenite samples from the porphyry- type Questa deposit (NM, USA), as well as one rhyolite and one granite sample, directly associated with the Mo mineralization. The δ98Mo of the molybdenites ranges between −0.48‰ and +0.40‰, with a median at −0.05‰. The median Mo isotope composition increases from early magmatic (−0.29‰) to hydrothermal (−0.05‰) breccia mineralization (median bulk breccia = −0.17‰) to late stockwork veining (+0.22‰). Moreover, variations of up to 0.34‰ are found between different molybdenite crystals within an individual hand specimen. The rhyolite sample with 0.12 μg g−1 Mo has δ98Mo = −0.57‰ and is lighter than all molybde- nites from the Questa deposit, interpreted to represent the igneous leftover after aqueous ore fluid exsolution. We recognize three Mo isotope fractionation processes that occur between about 700 and 350 °C, affecting the Mo iso- tope composition of magmatic–hydrothermal molybdenites. Δ1Mo: Minerals preferentially incorporate light Mo isotopes during progressive fractional crystallization in subvolcanic magma reservoirs, leaving behind a melt enriched in heavy Mo isotopes. Δ2Mo: Magmatic–hydrothermal fluids preferentially incorporate heavy Mo iso- topes upon fluid exsolution. Δ3Mo: Light Mo isotopes get preferentially incorporated in molybdenite during crys- tallization from an aqueous fluid, leaving behind a hydrothermal fluid that gets heavier with progressive molybdenite crystallization. The sum of all three fractionation processes produces molybdenites that record heavier δ98Mo compositions than their source magmas. This implies that the mean δ98Mo of molybdenites published so far (~0.4‰) likely represents a maximum value for the Mo isotope composition of Phanerozoic igneous upper crust.

Experimental dissolution of molybdenum-sulphides at low oxygen concentrations: A first-order approximation of late Archean atmospheric conditions

The abundance of atmospheric oxygen and its evolution through Earth's history is a highly debated topic. The earliest change of the Mo concentration and isotope composition of marine sediments are interpreted to be linked to the onset of the accumulation of free O2 in Earth's atmosphere. The O2 concentration needed to dissolve significant amounts of Mo in water is not yet quantified, however. We present laboratory experiments on pulverized and surface-cleaned molybdenite (MoS2) and a hydrothermal breccia enriched in Mo-bearing sulphides using a glove box setup. Duration of an experiment was 14 days, and first signs of oxidation and subsequent dissolution of Mo compounds start to occur above an atmospheric oxygen concentration of 72 ± 20 ppmv (i.e., 2.6 to 4.6 × 10−4 present atmospheric level (PAL)). This experimentally determined value coincides with published model calculations supporting atmospheric O2 concentrations between 1 × 10−5 to 3 × 10−4 PAL prior to the Great Oxidation Event and sets an upper limit to the molecular oxygen needed to trigger Mo accumulation and Mo isotope variations recorded in sediments. In combination with the published Mo isotope composition of the rock record, this result implies an atmospheric oxygen concentration prior to 2.76 Ga of below 72 ± 20 ppmv.

Chemical composition of bottom sediments from the Discovery Deep, Red Sea rift zone

Hot brines in depressions of the central Red Sea contain thousands of times more iron, manganese and other metals than . After removal of salts, approximately half of sediments from these depressions consists of iron hydroxides and they are enriched in zinc, copper, lead and molybdenum. Hydrothermal deposits with the same complex of metals, located along the coast of the Red Sea, are correlated with faults and may be due to occurrences of Tertiary volcanism. Brines of similar composition are known in the Cheleken Peninsula. Certain geological and geochemical data indicate that such brines are of relatively deep origin.

Composition of Fe-Mn nodules and crusts from the Cape Basin

Facies zonation of the Cape basin with respect to Fe-Mn nodules based on data from Cruise 43 of R/V Akademik Kurchatov and published data is presented. Three facies regions are distinguished: the southern end of the Walvis Ridge and seamounts, the continental slope of the Southwest Africa and the deep-water Cape Basin. Iron-manganese nodules in the first of these areas are predominantly sedimentary, those in the second area are diagenetic and those in the third are sedimentary-diagenetic. Chemical characteristics and type of metallogenic specialization for each of the regions are identified.