Rare Earth impurities in yb(6) and zrb(12).

We present data on the depression of the superconducting transition temperatures of YB(6) and ZrB(12) by rare earth impurities. These data show unusual features. Ce in YB(6) is in some ways analogous to Yb in ZrB(12), and this analogy also appears to hold between Ce in CeB(6) and YB in YbB(12).

Effect of rare earth dopants on structural and mechanical properties of nanoceria synthesized by combustion method

Structural characteristics of combustion synthesized, calcined and densified pure and doped nanoceria with tri-valent cations of Er, Y, Gd, Sm and Nd were analyzed by X-ray diffraction (XRD) and high resolution transmission electron microscopy (HRTEM). The results showed that the as-synthesized and calcined nanopowders were mesoporous and calculated lattice parameters were close to theoretical ion-packing model. The effect of dopants on elastic modulus, microhardness and fracture toughness of sintered pure and doped ceria were investigated. It was observed that tri-valent cation dopants increased the hardness of the ceria, whereas the fracture toughness and elastic modulus were decreased.

Multifunctional rare earth organic corrosion inhibitors

All rights reserved.Chromium (VI) compounds are commonly used in paint systems to provide corrosion protection, particularly for aerospace alloys. These compounds are toxic, carcinogenic and environmentally detrimental, therefore alternatives that are safe, environmentally benign and meet or exceed current levels of corrosion protection are vital. Multifunctional rare earth organic compounds incorporate known inhibitor species, achieving synergistic inhibition in corrosive environments. The mechanism, efficiency and surface interactions of these complexes are explored. The complexes were effective inhibitors for steel and aluminium alloys, through mixed inhibition. Advantages and limitations of these inhibitor complexes, along with applications and future research direction, are discussed.

Volcanology and petrology of submarine volcanoes of the New Hebrides island arc

The New Hebrides Island Arc, an intra-oceanic island chain in the southwest Pacific, is formed by subduction of the Indo-Australian Plate beneath the Pacific Plate. The southern end of the New Hebrides Island Arc is an ideal location to study the magmatic and tectonic interaction of an emerging island arc as this part of the island chain is less than 3 million years old. A tectonically complex island arc, it exhibits a change in relative subduction rate from ~12cm/yr to 6 cm/yr before transitioning to a left-lateral strike slip zone at its southern end. Two submarine volcanic fields, Gemini-Oscostar and Volsmar, occur at this transition from normal arc subduction to sinistral strike slip movement. Multi-beam bathymetry and dredge samples collected during the 2004 CoTroVE cruise onboard the RV Southern Surveyor help define the relationship between magmatism and tectonics, and the source for these two submarine volcanic fields. Gemini-Oscostar volcanic field (GOVF), dominated by northwest-oriented normal faults, has mature polygenetic stratovolcanoes with evidence for explosive subaqueous eruptions and homogeneous monogenetic scoria cones. Volsmar volcanic field (VVF), located 30 km south of GOVF, exhibits a conjugate set of northwest and eastwest-oriented normal faults, with two polygenetic stratovolcanoes and numerous monogenetic scoria cones. A deep water caldera provides evidence for explosive eruptions at 1500m below sea level in the VVF. Both volcanic fields are dominated by low-K island arc tholeiites and basaltic andesites with calcalkalic andesite and dacite being found only in the GOVF. Geochemical signatures of both volcanic fields continue the along-arc trend of decreasing K2O with both volcanic fields being similar to the New Hebrides central chain lavas. Lavas from both fields display a slight depletion in high field strength elements and heavy rare earth elements, and slight enrichments in large-ion lithophile elements and light rare earth elements with respect to N-MORB mantle. Sr and Nd isotope data correlate with heavy rare earth and high field strength element data to show that both fields are derived from depleted mantle. Pb isotopes define Pacific MORB mantle sources and are consistent with isotopic variation along the New Hebrides Island Arc. Pb isotopes show no evidence for sediment contamination; the subduction component enrichment is therefore a slab-derived enrichment. There is a subtle spatial variation in source chemistry which sees a northerly trend of decreasing enrichment of slab-derived fluids.

Impact of recent coastal development and human activities on Nha Trang Bay, Vietnam : evidence from a Porites lutea geochemical record

Nha Trang Bay (NTB) is located on the Central Vietnam coast, western South China Sea. Recent coastal development of Nha Trang City has raised public concern over an increasing level of pollution within the bay and degradation of nearby coral reefs. In this study, multiple proxies (e.g., trace metals, rare earth elements (REEs), and Y/Ho) recorded in a massive Porites lutea coral colony were used to reconstruct changes in seawater conditions in the NTB from 1995 to 2009. A 14-year record of REEs and other trace metals revealed that the concentrations of terrestrial trace metals have increased dramatically in response to an increase in coastal development projects such as road, port, and resort constructions, port and river dredging, and dumping activities since 2000. The effects of such developmental processes are also evident in changes in REE patterns and Y/Ho ratios through time, suggesting that both parameters are critical proxies for marine pollution.

Controls on mid-Holocene fringing reef growth and termination in a high latitude, estuarine setting, Wellington Point, Southeast Queensland

Several fringing coral reefs in Moreton Bay, Southeast Queensland, some 300 km south of the Great Barrier Reef (GBR), are set in a relatively high latitude, estuarine environment that is considered marginal for coral growth. Previous work indicated that these marginal reefs, as with many fringing reefs of the inner GBR, ceased accreting in the mid-Holocene. This research presents for the first time data from the subsurface profile of the mid-Holocene fossil reef at Wellington Point comprising U/Th dates of in situ and framework corals, and trace element analysis from the age constrained carbonate fragments. Based on trace element proxies the palaeo-water quality during reef accretion was reconstructed. Results demonstrate that the reef initiated more than 7,000 yr BP during the post glacial transgression, and the initiation progressed to the west as sea level rose. In situ micro-atolls indicate that sea level was at least 1 m above present mean sea level by 6,680 years ago. The reef remained in "catch-up" mode, with a seaward sloping upper surface, until it stopped aggrading abruptly at ca 6,000 yr BP; no lateral progradation occurred. Changes in sediment composition encountered in the cores suggest that after the laterite substrate was covered by the reef, most of the sediment was produced by the carbonate factory with minimal terrigenous influence. Rare earth element, Y and Ba proxies indicate that water quality during reef accretion was similar to oceanic waters, considered suitable for coral growth. A slight decline in water quality on the basis of increased Ba in the later stages of growth may be related to increased riverine input and partial closing up of the bay due to either tidal delta progradation, climatic change and/or slight sea level fall. The age data suggest that termination of reef growth coincided with a slight lowering of sea level, activation of ENSO and consequent increase in seasonality, lowering of temperatures and the constrictions to oceanic flushing. At the cessation of reef accretion the environmental conditions in the western Moreton Bay were changing from open marine to estuarine. The living coral community appears to be similar to the fossil community, but without the branching Acropora spp. that were more common in the fossil reef. In this marginal setting coral growth periods do not always correspond to periods of reef accretion due to insufficient coral abundance. Due to several environmental constraints modern coral growth is insufficient for reef growth. Based on these findings Moreton Bay may be unsuitable as a long term coral refuge for most species currently living in the GBR.

A vibrational spectroscopic study of the silicate mineral normandite – NaCa(Mn2+,Fe2+)(Ti,Nb,Zr)Si2O7(O,F)2

We have studied the mineral normandite using a combination of scanning electron microscopy with energy dispersive spectroscopy and vibrational spectroscopy. The mineral normandite NaCa(Mn2+,Fe2+)(Ti,Nb,Zr)Si2O7(O,F)2 is a crystalline sodium calcium silicate which contains rare earth elements. Chemical analysis shows the mineral contains a range of elements including Na, Mn2+, Ca, Fe2+ and the rare earth element niobium. No Raman bands are observed above 1100 cm−1. The mineral is characterised by Raman bands observed at 724, 748, 782 and 813 cm−1. Infrared bands are broad; nevertheless bands may be resolved at 723, 860, 910, 958, 933, 1057 and 1073 cm−1. Intense Raman bands at 454, 477 and 513 cm−1 are attributed to OSiO bending modes. No Raman bands are observed in the hydroxyl stretching region, but low intensity infrared bands are observed at 3191 and 3450 cm−1. This observation brings into question the true formula of the mineral.

Raman and infrared spectroscopic study of kamphaugite-(Y)

We have studied the carbonate mineral kamphaugite-(Y)(CaY(CO3)2(OH)·H2O), a mineral which contains yttrium and specific rare earth elements. Chemical analysis shows the presence of Ca, Y and C. Back scattering SEM appears to indicate a single pure phase. The vibrational spectroscopy of kamphaugite-(Y) was obtained using a combination of Raman and infrared spectroscopy. Two distinct Raman bands observed at 1078 and 1088cm(-1) provide evidence for the non-equivalence of the carbonate anion in the kamphaugite-(Y) structure. Such a concept is supported by the number of bands assigned to the carbonate antisymmetric stretching mode. Multiple bands in the ν4 region offers further support for the non-equivalence of carbonate anions in the structure. Vibrational spectroscopy enables aspects of the structure of the mineral kamphaugite-(Y) to be assessed.

Chemical and mineralogical characterization of micro-inclusions in diamonds

Secondary-ion mass spectrometry (SIMS), electron probe analysis (EPMA), analytical scanning electron microscopy (SEM) and infrared (IR) spectroscopy were used to determine the chemical composition and the mineralogy of sub-micrometer inclusions in cubic diamonds and in overgrowths (coats) on octahedral diamonds from Zaire, Botswana, and some unknown localities.

The inclusions are sub-micrometer in size. The typical diameter encountered during transmission electron microscope (TEM) examination was 0.1-0.5 µm. The micro-inclusions are sub-rounded and their shape is crystallographically controlled by the diamond. Normally they are not associated with cracks or dislocations and appear to be well isolated within the diamond matrix. The number density of inclusions is highly variable on any scale and may reach 10^(11) inclusions/cm^3 in the most densely populated zones. The total concentration of metal oxides in the diamonds varies between 20 and 1270 ppm (by weight).

SIMS analysis yields the average composition of about 100 inclusions contained in the sputtered volume. Comparison of analyses of different volumes of an individual diamond show roughly uniform composition (typically ±10% relative). The variation among the average compositions of different diamonds is somewhat greater (typically ±30%). Nevertheless, all diamonds exhibit similar characteristics, being rich in water, carbonate, SiO_2, and K_2O, and depleted in MgO. The composition of micro-inclusions in most diamonds vary within the following ranges: SiO_2, 30-53%; K_2O, 12-30%; CaO, 8-19%; FeO, 6-11%; Al_2O_3, 3-6%; MgO, 2-6%; TiO_2, 2-4%; Na_2O, 1-5%; P_2O_5, 1-4%; and Cl, 1-3%. In addition, BaO, 1-4%; SrO, 0.7-1.5%; La_2O_3, 0.1-0.3%; Ce_2O_3, 0.3-0.5%; smaller amounts of other rare-earth elements (REE), as well as Mn, Th, and U were also detected by instrumental neutron activation analysis (INAA). Mg/(Fe+Mg), 0.40-0.62 is low compared with other mantle derived phases; K/ AI ratios of 2-7 are very high, and the chondrite-normalized Ce/Eu ratios of 10-21 are also high, indicating extremely fractionated REE patterns.

SEM analyses indicate that individual inclusions within a single diamond are roughly of similar composition. The average composition of individual inclusions as measured with the SEM is similar to that measured by SIMS. Compositional variations revealed by the SEM are larger than those detected by SIMS and indicate a small variability in the composition of individual inclusions. No compositions of individual inclusions were determined that might correspond to mono-mineralic inclusions.

IR spectra of inclusion- bearing zones exhibit characteristic absorption due to: (1) pure diamonds, (2) nitrogen and hydrogen in the diamond matrix; and (3) mineral phases in the micro-inclusions. Nitrogen concentrations of 500-1100 ppm, typical of the micro-inclusion-bearing zones, are higher than the average nitrogen content of diamonds. Only type IaA centers were detected by IR. A yellow coloration may indicate small concentration of type IB centers.

The absorption due to the micro-inclusions in all diamonds produces similar spectra and indicates the presence of hydrated sheet silicates (most likely, Fe-rich clay minerals), carbonates (most likely calcite), and apatite. Small quantities of molecular CO_2 are also present in most diamonds. Water is probably associated with the silicates but the possibility of its presence as a fluid phase cannot be excluded. Characteristic lines of olivine, pyroxene and garnet were not detected and these phases cannot be significant components of the inclusions. Preliminary quantification of the IR data suggests that water and carbonate account for, on average, 20-40 wt% of the micro-inclusions.

The composition and mineralogy of the micro-inclusions are completely different from those of the more common, larger inclusions of the peridotitic or eclogitic assemblages. Their bulk composition resembles that of potassic magmas, such as kimberlites and lamproites, but is enriched in H_2O, CO_3, K_2O, and incompatible elements, and depleted in MgO.

It is suggested that the composition of the micro-inclusions represents a volatile-rich fluid or a melt trapped by the diamond during its growth. The high content of K, Na, P, and incompatible elements suggests that the trapped material found in the micro-inclusions may represent an effective metasomatizing agent. It may also be possible that fluids of similar composition are responsible for the extreme enrichment of incompatible elements documented in garnet and pyroxene inclusions in diamonds.

The origin of the fluid trapped in the micro-inclusions is still uncertain. It may have been formed by incipient melting of a highly metasomatized mantle rocks. More likely, it is the result of fractional crystallization of a potassic parental magma at depth. In either case, the micro-inclusions document the presence of highly potassic fluids or melts at depths corresponding to the diamond stability field in the upper mantle. The phases presently identified in the inclusions are believed to be the result of closed system reactions at lower pressures.

Geochemical characterization of the fire-fountain fed deposits of Las Herrerias volcano (Campo de Calatrava Volcanic Field, Ciudad Real)

The Las Herrerias volcano (Bolanos de Calatrava, Campo de Calatrava Volcanic Field) is characterized by the great amount and variety of fire-fountain fed deposits. All these deposits are compositionally similar, being constituted by magnesium-rich (MgO = 11.58-4.19%), aluminium-poor (Al2O3 = 9.64-10.99%) highly sodic (Na2O = 2.24-3.81%) melanephelinites, with high contents in rare earth-elements (10x-200x chondrite), particularly in light-rare earth elements with respect to the heavy ones [(La/Lu)(N) = 32-35]. Contrary to the equivalent melanephelinites of this volcanic field, the relatively low contents in Ni (233-286 ppm), Cr (393-520 ppm) and magnesium number (Mg* = 45-54) indicate that these rocks do not correspond with primary melts. On the other hand, the variable distribution of clinopyroxene in the magma during eruption would be responsible for the slight compositional differences observed in the studied samples. Finally, we argue that these fire fountains were developed in a continental intraplate setting.

Interações do lantânio e cério com microalgas dos gêneros Monoraphidium e Scenedesmus

Os elementos de terras raras, representados em sua maioria pelos lantanídeos, ocorrem principalmente como constituintes-traço da maioria dos minerais de rochas comuns (monazita, apatita) e também estão presentes em alguns minérios. Tais elementos foram largamente usados por décadas como fertilizantes na China. Na área das inovações tecnológicas, a demanda por esses metais vem crescendo por conta das suas aplicações em diversos campos. Consequentemente, grandes quantidades desses elementos são acumulados em ambientes aquáticos atingindo o fitoplâncton. Assim, as microalgas que são organismos ecologicamente importantes na cadeia alimentar têm sido frequentemente usadas em estudos ambientais para avaliar a toxicidade relativa de várias descargas químicas e são largamente estudadas na detecção dos primeiros impactos no ecossistema. Somado a isso, são biomassas que possuem boa capacidade de biossorção de metais devido à presença de ligantes na sua estrutura que promovem a captação deles quando em solução. Dessa forma, as interações entre as microalgas verdes Monoraphidium e Scenedesmus e os íons La3+ e Ce3+ foram investigadas neste trabalho. Para isso, foram avaliados o efeito tóxico e a bioacumulação do La3+ pelas duas microalgas verdes. Adicionalmente, estudos em batelada da biossorção do La3+ e Ce3+ em soluções contendo os elementos isoladamente ou em combinação foram realizados. No estudo de toxicidade e de bioacumulação o meio de cultivo utilizado foi o ASM-1, com e sem presença de La3+ (10 mg.L-1 a 100 mg.L-1), onde o efeito tóxico do metal foi monitorado por análises micro e macroscópica das células e também pela quantificação do crescimento celular baseada em medidas da massa seca. A bioacumulação do metal foi avaliada da mesma forma para ambas as microalgas. Os resultados obtidos mostraram que o efeito tóxico do metal foi presente em concentrações iônicas de 50 e 100 mg.L-1 e que houve uma bioconcentração do La3+ em ambas espécies de microalgas, principalmente quando a concentração inicial do La3+ foi de 10 e 25 mg.L-1, mostrando que houve uma relação direta entre a bioconcentração e a toxicidade do La3+. O gênero Monoraphidium bioconcentrou mais metal que o gênero Scenedesmus. Os resultados da biossorção dos metais em solução monoelementar mostraram que as microalgas apresentaram grande capacidade de captação do La3+ (20,7 mmol.g-1 para Monoraphidium sp. e 17,8 mmol.g-1 para Scenedesmus sp.) e do Ce3+ (25,7 mmol.g-1 para Monoraphidium sp. e 11,5 mmol.g-1 para Scenedesmus sp.). Os resultados obtidos revelaram que os dados melhor se ajustaram ao modelo de Freundlich, na maioria dos casos. Em sistema binário, notou-se que houve uma menor captação de cada um individualmente, evidenciando uma competição entre eles pelos mesmos sítios ligantes e que ambas apresentaram maior afinidade pelo Ce3+

稀土元素生物效应的蛋白质组学研究

蛋白质组学是研究细胞内全部蛋白的动态表达及其相互关系的新兴学科，是功能基因组学研究的重要组成部分和战略制高点，广泛应用于生命科学的各个领域，研究对象涵盖微生物、动物和植物等。 　　稀土元素（rare earth elements），亦称镧系元素（lanthanides），是性质相似的15种金属元素。随着稀土元素在工业、农牧业和医疗等领域的应用日益深入，它们对生物体的作用机制亟待研究。生物固氮作用为生命世界提供75%的绿色氮源，根瘤菌是重要的固氮微生物，具有基因组结构简单、培养周期短等特点。酿酒酵母是与人类关系最密切的一种酵母，不仅因为传统上其用于制作食品及酿酒，而且是现代分子生物学和细胞生物学中的真核模式生物。为了全面地了解稀土元素对细胞的作用，我们运用高分辨率的蛋白质双向电泳分离技术和高通量的蛋白质质谱分析手段以及生物信息学等方法，分析了稀土元素钆（Gadolinium，Gd）在原核生物费氏中华根瘤菌（Sinorhizobium fredii）USDA205和真核生物酿酒酵母（Saccharomyces cerevisiae）YM4271的生物效应。 　　结果表明，经1mM Gd(NO3)3处理12小时后，费氏中华根瘤菌USDA205中 22个蛋白质表达有差异。这些蛋白质可根据功能分为8类，包括转运蛋白、胁迫相关蛋白、代谢相关蛋白等。其中13个蛋白质表达量增加，9个蛋白质表达量下降。膜蛋白在差异蛋白中占有很大比重。另外，我们分析了不同浓度的钆处理后蛋白质表达的变化情况，发现蛋白质组的变化是与处理浓度密切相关的。研究中还发现同种浓度的钆与另一种稀土元素铒（Erbium，Er）相比，离子半径较小的铒离子对根瘤菌的抑制作用更加明显。 　　比较不同浓度的钆对酿酒酵母YM4271的影响，发现酵母对稀土元素的反应不及根瘤菌敏感，对数生长初期的酵母经钆处理12小时或24小时后均无显著变化。 　　本研究首次用蛋白质组学的方法研究稀土元素对微生物的作用，鉴定了一些有价值的蛋白质，并得到了它们的表达特点和相关数据，为更好地理解稀土元素的生物效应提供了有力的分子生物学证据。