Academic literature on the topic 'Lithophile trace elements'
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Journal articles on the topic "Lithophile trace elements"
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Barrat, J. A., B. Zanda, A. Jambon, and C. Bollinger. "The lithophile trace elements in enstatite chondrites." Geochimica et Cosmochimica Acta 128 (March 2014): 71–94. http://dx.doi.org/10.1016/j.gca.2013.11.042.
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Wood, Bernard J., and Ekaterina S. Kiseeva. "Trace element partitioning into sulfide: How lithophile elements become chalcophile and vice versa." American Mineralogist 100, no. 11-12 (November 2015): 2371–79. http://dx.doi.org/10.2138/am-2015-5358ccbyncnd.
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Ionov, Dmitri A., William L. Griffin, and Suzanne Y. O'Reilly. "Volatile-bearing minerals and lithophile trace elements in the upper mantle." Chemical Geology 141, no. 3-4 (September 1997): 153–84. http://dx.doi.org/10.1016/s0009-2541(97)00061-2.
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Porcelli, D. R., R. K. O'Nions, S. J. G. Galer, A. S. Cohen, and D. P. Mattey. "Isotopic relationships of volatile and lithophile trace elements in continental ultramafic xenoliths." Contributions to Mineralogy and Petrology 110, no. 4 (May 1992): 528–38. http://dx.doi.org/10.1007/bf00344086.
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Barrat, Jean-Alix, Albert Jambon, Akira Yamaguchi, Addi Bischoff, Marie-Laure Rouget, and Céline Liorzou. "Partial melting of a C-rich asteroid: Lithophile trace elements in ureilites." Geochimica et Cosmochimica Acta 194 (December 2016): 163–78. http://dx.doi.org/10.1016/j.gca.2016.08.042.
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Good, David J., and Peter C. Lightfoot. "Significance of the metasomatized lithospheric mantle in the formation of early basalts and Cu – platinum group element sulfide mineralization in the Coldwell Complex, Midcontinent Rift, Canada." Canadian Journal of Earth Sciences 56, no. 7 (July 2019): 693–714. http://dx.doi.org/10.1139/cjes-2018-0042.
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A diverse suite of tholeiitic to alkaline basalt and gabbroic intrusions located in the Coldwell Complex on the northern margin of the Midcontinent Rift exhibit unusual trace element signatures that show enriched large ion lithophile elements and light rare earth elements with negative Nb and Zr anomalies. These features are not typical of magmas derived by partial melting within or above a rising mantle plume, as might be expected in an early Midcontinent Rift magmatic event. In this paper, we provide a detailed geochemical study of a 500 m thick sequence of metabasalt that represents the earliest stage of magmatism in the Coldwell Complex. We show that contamination or crystallization processes or subsequent metasomatism cannot explain the trace element variations. Instead, we propose partial melting in a metasomatized Subcontinental Lithospheric Mantle source to explain the decoupled behavior of large ion lithophile elements from light rare earth elements and heavy rare earth elements and rare earth elements from high field strength elements and the enriched Nd isotope signature of metabasalt. Similar features occur in unit 5b of the Mamainse Point Volcanic Group located at the northern margin of the Rift. An objective of this paper is to relate Two Duck Lake gabbro, host rock for low-sulfur, high precious metal sulfide mineralization at the Marathon deposit, to the metabasalt sequence. The excellent match of trace element abundances in Two Duck Lake gabbro to metabasalt unit 3 confirms an early Coldwell Complex age for metabasalt and a Subcontinental Lithospheric Mantle source for Cu – platinum group element mineralized gabbros.
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Javed, Muhammad Babar, Iain Grant-Weaver, and William Shotyk. "An optimized HNO3 and HBF4 digestion method for multielemental soil and sediment analysis using inductively coupled plasma quadrupole mass spectrometry." Canadian Journal of Soil Science 100, no. 4 (December 1, 2020): 393–407. http://dx.doi.org/10.1139/cjss-2020-0001.
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A robust and reliable analytical procedure for the determination of trace (mg∙kg−1) and ultra-trace elements (μg∙kg−1) in soil and sediments by inductively coupled plasma quadrupole mass spectrometry (ICP-QMS) was optimized. Aliquots of ∼200 mg of two certified reference materials (IAEA Soil-7, soil and IAEA SL-1, lake sediments) were digested in nitric acid (HNO3) purified twice by sub-boiling distillation using a microwave-heated high-pressure autoclave. Incremental addition of tetrafluoroboric acid (HBF4, 0.1–2 mL) to HNO3 was evaluated for yield. The selection of appropriate proportions of digestion acids was crucial to obtain accurate results. Digested samples were analyzed for a range of trace elements including those that are potentially toxic (Ag, Cd, Pb, Sb, and Tl), plant micronutrients (Cu, Fe, Mn, and Zn), those enriched in bitumen (Mo, Ni, and V), and lithophile elements (Al, Ba, Co, Cr, Rb, Sr, Th, Ti, Y, and Zr). Nitric acid alone proved to be sufficient to completely liberate Cd, Co, Cr, Fe, Mn, Ni, Pb, V, and Zn in both soil and sediments (87%–120% recovery). For almost all the other elements, addition of HBF4 was needed for improved recovery. A combination of 3 mL of HNO3 and 1.5 mL of HBF4 was optimal to fully liberate an extended list of elements including Ba, Sb, and Sr from both the reference materials. Conservative lithophile elements (Th, Ti, Y, and Zr) could not be completely recovered with the proposed method, requiring hydrofluoric acid for complete dissolution of recalcitrant minerals.
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Duran, Charley J., Sarah-Jane Barnes, Eduardo T. Mansur, Sarah A. S. Dare, L. Paul Bédard, and Sergey F. Sluzhenikin. "Magnetite Chemistry by LA-ICP-MS Records Sulfide Fractional Crystallization in Massive Nickel-Copper-Platinum Group Element Ores from the Norilsk-Talnakh Mining District (Siberia, Russia): Implications for Trace Element Partitioning into Magnetite." Economic Geology 115, no. 6 (September 1, 2020): 1245–66. http://dx.doi.org/10.5382/econgeo.4742.
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Abstract Mineralogical and chemical zonations observed in massive sulfide ores from Ni-Cu-platinum group element (PGE) deposits are commonly ascribed to the fractional crystallization of monosulfide solid solution (MSS) and intermediate solid solution (ISS) from sulfide liquid. Recent studies of classic examples of zoned orebodies at Sudbury and Voisey’s Bay (Canada) demonstrated that the chemistry of magnetite crystallized from sulfide liquid was varying in response to sulfide fractional crystallization. Other classic examples of zoned Ni-Cu-PGE sulfide deposits occur in the Norilsk-Talnakh mining district (Russia), yet magnetite in these orebodies has received little attention. In this contribution, we document the chemistry of magnetite in samples from Norilsk-Talnakh, spanning the classic range of sulfide composition, from Cu poor (MSS) to Cu rich (ISS). Based on textural features and mineral associations, four types of magnetite with distinct chemical composition are identified: (1) MSS magnetite, (2) ISS magnetite, (3) reactional magnetite (at the sulfide-silicate interface), and (4) hydrothermal magnetite (resulting from sulfide-fluid interaction). Compositional variability in lithophile and chalcophile elements records sulfide fractional crystallization across MSS and ISS magnetites and sulfide interaction with silicate minerals (reactional magnetite) and fluids (hydrothermal magnetite). Estimated partition coefficients for magnetite in sulfide systems are unlike those in silicate systems. In sulfide systems, all lithophile elements are compatible and chalcophile elements tend to be incompatible with magnetite, but in silicate systems some lithophile elements are incompatible and chalcophile elements are compatible with magnetite. Finally, comparison with magnetite data from other Ni-Cu-PGE sulfide deposits pinpoints that the nature of parental silicate magma, degree of sulfide evolution, cocrystallizing phases, and alteration conditions influence magnetite composition.
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Smith, Alan D. "Geochemistry and tectonic setting of volcanics from the Anyox mining camp, British Columbia." Canadian Journal of Earth Sciences 30, no. 1 (January 1, 1993): 48–59. http://dx.doi.org/10.1139/e93-005.
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Volcanogenic massive sulphide deposits at Anyox in the Tracy Arm terrane of the Canadian Cordillera are associated with a sequence of tholeiitic basalts with minor intercalated basaltic andesite tuffs and siliceous sediments. Sm–Nd and Pb–Pb systematics indicate an Early to Middle Jurassic age. The tholeiites are characterized by normal mid-ocean-ridge basalt to weak island-arc tholeiite trace element signatures with slight enrichment in large-ion lithophile elements and depletion in high-field-strength elements, high 207Pb/204Pb, and εNd(170 Ma) values of +8.2 to +8.4. The mineralized sequence is conformably overlain by argillaceous sediments and minor limestones. These features, combined with the location of the strata and similarities with the Spider Peak Formation of the Methow terrane, indicate an origin in a narrowing marginal basin that once separated superterranes I and II.
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Morrison, A. D., and A. Reay. "Geochemistry of Ferrar Dolerite sills and dykes at Terra Cotta Mountain, south Victoria Land, Antarctica." Antarctic Science 7, no. 1 (March 1995): 73–85. http://dx.doi.org/10.1017/s0954102095000113.
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At Terra Cotta Mountain, in the Taylor Glacier region of south Victoria Land, a 237 m thick Ferrar Dolerite sill is intruded along the unconformity between basement granitoids and overlying Beacon Supergroup sedimentary rocks. Numerous Ferrar Dolerite dykes intrude the Beacon Supergroup and represent later phases of intrusion. Major and trace element data indicate variation both within and between the separate intrusions. Crystal fractionation accounts for much of the geochemical variation between the intrusive events. However, poor correlations between many trace elements require the additional involvement of open system processes. Chromium is decoupled from highly incompatible elements consistent with behaviour predicted for a periodically replenished, tapped and fractionating magma chamber. Large ion lithophile element-enrichment and depletion in Nb, Sr, P and Ti suggests the addition of a crustal component or an enriched mantle source. The trace element characteristics of the Dolerites from Terra Cotta Mountain are similar to those of other Ferrar Group rocks from the central Transantarctic Mountains and north Victoria Land, as well as with the Tasmanian Dolerites. This supports current ideas that the trace element signature of the Ferrar Group is inherited from a uniformly enriched mantle source region.
Dissertations / Theses on the topic "Lithophile trace elements"
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Júnior, Eduardo Reis Viana Rocha. "Sistemática isotópica de Os-Nd-Pb-Sr e geoquímica de elementos traço litófilos e siderófilos de basaltos da Província Magmática do Paraná." Universidade de São Paulo, 2011. http://www.teses.usp.br/teses/disponiveis/14/14132/tde-02022011-203512/.
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O objetivo primário deste estudo é aprimorar o conhecimento acerca das fontes do manto e dos mecanismos envolvidos na gênese dos basaltos da Província Magmática do Paraná, que constitui uma das maiores manifestações de basaltos continentais do mundo. Para tanto, foram determinadas as concentrações de terras raras (La, Ce, Nd, Sm, Eu, Tb, Yb e Lu), outros elementos traço (Cs, Rb, Ba, U, Th, Ta, Hf, Co e Sc) e elementos altamente siderófilos (Os, Ir, Ru, Pt, Pd e Re), juntamente com razões isotópicas dos sistemas Rb-Sr, Sm-Nd, U-Th-Pb e Re-Os em basaltos com alto-Ti (Paranapanema e Pitanga) que ocorrem no norte da PMP. Além disso, foram determinadas as concentrações de elementos altamente siderófilos e as razões isotópicas de 187Os/188Os amostras representativas de basaltos com baixo-Ti (Esmeralda) do sul da PMP. Os dados geoquímicos e as razões isotópicas de Sr, Nd e Pb obtidos são consistentes com dados da literatura, porém, refinam as variações (extremos) isotópicas dos magmas-tipo Paranapanema e Pitanga. Esses dados, juntamente com as concentrações de elementos altamente siderófilos e das razões isotópicas de Os, inéditas na literatura, sugerem que as fontes dos basaltos (astenosfera ou manto litosférico subcontinental) sofreram metassomatismo significativo, com a intrusão de veios piroxeníticos, relacionado a antigas subducções e/ou processos de delaminação.The primary goal of this study is to improve the understanding about the mantle sources and the mechanisms involved in the basalt genesis from Paraná Magmatic Province (PMP), which is one of the largest known continental flood basalts of the world. Therefore, the concentrations of rare earths (La, Ce, Nd, Sm, Eu, Tb, Yb and Lu), other trace elements (Cs, Rb, Ba, U, Th, Ta, Hf, Co and Sc) and highly siderophile elements (Os, Ir, Ru, Pt, Pd and Re) were determined, along with isotope ratios regarding Rb-Sr, Sm-Nd, U-Th-Pb e Re-Os systematics in high-Ti basalts (Paranapanema and Pitanga) from northern PMP. In addition, the highly siderophile element concentrations, as well as 187Os/188Os isotope ratios, were measured in selected samples of low-Ti basalts (Esmeralda) from southern PMP. The geochemical and Sr-Nd-Pb isotope results of the present study are consistent with literature data, but refine the isotope variations (extreme) for the Paranapanema and Pitanga magma-types. These data, along with the concentrations of highly siderophile elements and Os isotope ratios suggest that the basalt mantle sources (asthenosphere or subcontinental lithospheric mantle) were affected by significant metasomatism (piroxenitic vein hybridization), related with old subduction and/or delamination processes.
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D'Souza, Rameses Joseph. "Controls on the sources and distribution of chalcophile and lithophile trace elements in arc magmas." Thesis, 2018. https://dspace.library.uvic.ca//handle/1828/9005.
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Volcanic arcs have been the locus of continental growth since at least the Proterozoic eon. In this dissertation, I seek to shine more light on arc processes by inferring the lower crustal mineralogy of an ancient arc by geochemical and structural modelling of its exposed levels. Arcs characteristically have high concentrations of incompatible elements, thus I also experimentally assess the ability of alkaline melts and fluids associated with sediment melting to carry lithophile and chalcophile elements in the sub-arc.
I measured the chemical composition of 18 plutonic samples from the Bonanza island arc, emplaced between 203 and 164 Ma on the Wrangellia terrane on Vancouver Island, British Columbia. Models using trace elements with Nd and Sr isotopes indicate < 10% assimilation of the Wrangellia basement by the Bonanza arc magmas. The Bonanza arc rare earth element geochemistry is best explained as two lineages, each with two fractionation stages implicating < 15% garnet crystallization. My inference of garnet-bearing cumulates in the unexposed lower crust of the Bonanza arc, an unsuspected similarity with the coeval Talkeetna arc (Alaska), is consistent with estimates from geologic mapping and geobarometry indicating that the arc grew to > 23 km total thickness. The age distribution of the Bonanza arc plutons shows a single peak at 171 Ma whereas the volcanic rock age distribution shows two peaks at 171 and 198 Ma, likely due to sampling and/or preservation bias. Numerous mechanisms may produce the E-W separation of young and old volcanism and this does not constrain Jurassic subduction polarity beneath Wrangellia.
Although a small component of arc magmatism, alkaline arc rocks are associated with economic concentrations of chalcophile elements. The effect of varying alkalinity on S Concentration at Sulfide Saturation (SCSS) has not been previously tested. Thus, I conducted experiments on hydrous basaltic andesite melts with systematically varied alkalinity at 1270°C and 1 GPa using piston-cylinder apparatus. At oxygen fugacity two log units below the fayalite magnetite quartz buffer, I find SCSS is correlated with total alkali concentration, perhaps a result of the increased non-bridging oxygen associated with increased alkalinity. A limit to the effect of alkalis on SCSS in hydrous melts is observed at ~7.5 wt.% total alkalis. Using my results and published data, I retrained earlier SCSS models and developed a new empirical model using the optical basicity compositional parameter, predicting SCSS with slightly better accuracy than previous models.
Sediment melts contribute to the trace element signature of arcs and the chalcophile elements, compatible in redox-sensitive sulfide, are of particular interest. I conducted experiments at 3 GPa, 950 – 1050°C on sediment melts, determined fluid concentrations by mass balance and report the first fluid-melt partition coefficients (Dfluid/melt) for sediment melting. Compared to oxidized, anhydrite-bearing melts, I observe high Dfluid/melt for chalcophile elements and low values for Ce in reduced, pyrrhotite-bearing melts. Vanadium and Sc are unaffected by redox. The contrasting fluid-melt behaviour of Ce and Mo that I report indicates that melt, not fluid, is responsible for elevated Mo in the well-studied Lesser Antilles arc.Graduate
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Gleißner, Philipp [Verfasser]. "Petrogenesis of anorthosites of the Mesoproterozoic Kunene Intrusive Complex, NW Namibia: evidence from stable and radiogenic isotope and lithophile and highly siderophile trace element composition / vorgelegt von Philipp Gleißner." 2011. http://d-nb.info/1012215547/34.
Full textBooks on the topic "Lithophile trace elements"
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Trieloff, Mario. Noble Gases. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.30.
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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Although the second most abundant element in the cosmos is helium, noble gases are also called rare gases. The reason is that they are not abundant on terrestrial planets like our Earth, which is characterized by orders of magnitude depletion of—particularly light—noble gases when compared to the cosmic element abundance pattern. Indeed, such geochemical depletion and enrichment processes make noble gases so versatile concerning planetary formation and evolution: When our solar system formed, the first small grains started to adsorb small amounts of noble gases from the protosolar nebula, resulting in depletion of light He and Ne when compared to heavy noble gases Ar, Kr, and Xe: the so-called planetary type abundance pattern. Subsequent flash heating of the first small mm to cm-sized objects (chondrules and calcium, aluminum rich inclusions) resulted in further depletion, as well as heating—and occasionally differentiation—on small planetesimals, which were precursors of larger planets and which we still find in the asteroid belt today from where we get rocky fragments in form of meteorites. In most primitive meteorites, we even can find tiny rare grains that are older than our solar system and condensed billions of years ago in circumstellar atmospheres of, for example, red giant stars. These grains are characterized by nucleosynthetic anomalies and particularly identified by noble gases, for example, so-called s-process xenon.While planetesimals acquired a depleted noble gas component strongly fractionated in favor of heavy noble gases, the sun and also gas giants like Jupiter attracted a much larger amount of gas from the protosolar nebula by gravitational capture. This resulted in a cosmic or “solar type” abundance pattern, containing the full complement of light noble gases. Contrary to Jupiter or the sun, terrestrial planets accreted from planetesimals with only minor contributions from the protosolar nebula, which explains their high degree of depletion and basically “planetary” elemental abundance pattern. Indeed this depletion enables another tool to be applied in noble gas geo- and cosmochemistry: ingrowth of radiogenic nuclides. Due to heavy depletion of primordial nuclides like 36Ar and 130Xe, radiogenic ingrowth of 40Ar by 40K decay, 129Xe by 129I decay, or fission Xe from 238U or 244Pu decay are precisely measurable, and allow insight in the chronology of fractionation of lithophile parent nuclides and atmophile noble gas daughters, mainly caused by mantle degassing and formation of the atmosphere.Already the dominance of 40Ar in the terrestrial atmosphere allowed C. F v. Weizsäcker to conclude that most of the terrestrial atmosphere originated by degassing of the solid Earth, which is an ongoing process today at mid ocean ridges, where primordial helium leaves the lithosphere for the first time. Mantle degassing was much more massive in the past; in fact, most of the terrestrial atmosphere formed during the first 100 million years of Earth´s history, and was completed at about the same time when the terrestrial core formed and accretion was terminated by a giant impact that also formed our moon. However, before that time, somehow also tiny amounts of solar noble gases managed to find their way into the mantle, presumably by solar wind irradiation of small planetesimals or dust accreting to Earth. While the moon-forming impact likely dissipated the primordial atmosphere, today´s atmosphere originated by mantle degassing and a late veneer with asteroidal and possibly cometary contributions. As other atmophile elements behave similar to noble gases, they also trace the origin of major volatiles on Earth, for example, water, nitrogen, sulfur, and carbon.
Book chapters on the topic "Lithophile trace elements"
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Mueller, Barbara. "The Provenance of Arsenic in Southeast Asia Discovered by Trace Elements in Groundwater from the Lowlands of Nepal." In Trace Metals in the Environment - New Approaches and Recent Advances. IntechOpen, 2021. http://dx.doi.org/10.5772/intechopen.83014.
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Arsenic concentrations in groundwater extracted from quaternary alluvial sediments pose a serious health issue for inhabitants living in several countries in Southeast Asia. A widely approved hypothesis states that reductive dissolution of Fe-bearing minerals releases As oxyanions to ground water and the original source of As has to be located in mafic rocks occurring across the entire Himalayan belt. Yet, recent trace element analyses of ground water from the lowlands (Terai) of Nepal show a clear decoupling of As and Fe. The positive correlation of K, Na, and trace elements like Li, B, and Mo with arsenic points out to clay minerals hosting the toxic element. This pattern of trace elements found in the ground water of the Terai also advocates against an original source of As in mafic rocks. The lithophile elements like Li, B, P, Br, Sr, and U reflect trace element composition typical for felsic rocks as an origin of As. All the mentioned elements are components of clay minerals found ubiquitously in some of the most characteristic felsic rocks of the Nepal Himalaya: metapelites and leucogranites—all these rocks exhibiting a high abundance of especially B, P, and As besides Cd and Pb.
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Bianchi, Thomas S. "Trace Metal Cycling." In Biogeochemistry of Estuaries. Oxford University Press, 2006. http://dx.doi.org/10.1093/oso/9780195160826.003.0024.
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Like many other elements, natural background levels of trace elements exist in crustal rocks, such as shales, sandstones, and metamorphic and igneous rocks (Benjamin and Honeyman, 2000). In particular, the majority of trace metals are derived from igneous rocks, simply based on the relative fraction of igneous rocks in comparison with sedimentary and metamorphic rocks in the Earth’s crust. The release of trace metals from crustal sources is largely controlled by the natural forces of physical and chemical weathering of rocks, notwithstanding large-scale anthropogenic disturbances such as mining, construction, and coal burning (release of fly ash). As discussed later in the chapter, adjustments can be made for anthropogenic loading to different ecosystems based on an enrichment factor which compares metal concentrations in the ecosphere to average crustal composition. Biological effects of weathering, such as plant root growth and organic acid release associated with respiration also contribute to these weathering processes. As some trace metals are more volatile than others, release due to volcanic activity represents another source of metals with such properties (e.g., Pb, Cd, As, and Hg). Just as Goldschmidt (1954) grouped elements (e.g., siderophiles, chalcophiles, lithophiles, andatomophiles) based on similarities in geochemical properties, trace metals also represent a group of elements with similar chemical properties. One particularly important distinguishing feature of these elements is their ability to bond reversibly to a broad spectrum of compounds (Benjamin and Honeyman, 2000). Thus, the major inputs of trace metals to estuaries are derived from riverine, atmospheric, and anthropogenic sources. Although trace elements typically occur at concentrations of less than 1 ppb (part per billion) (or μg L−1, also reported in molar units), these elements are important in estuaries because of their toxic effects, as well as their importance as micronutrients for many organisms. The fate and transport of trace elements in estuaries are controlled by a variety of factors ranging from redox, ionic strength, abundance of adsorbing surfaces, and pH, just to name a few (Wen et al., 1999).