Oxygen isotope compositions of iron oxides from high-grade BIF-hosted iron ore deposits of the Central Hamersley Province, Western Australia: Constraints on the evolution of hydrothermal fluids

The Hamersley province of northwest Australia is one of the world's premier iron ore regions with high-grade martite-microplaty hematite iron ore deposits mostly hosted within banded iron formation (BIF) sequences of the Brockman Iron Formations of the Hamersley Group. These high-grade iron ores contain between 60 and 68 wt percent Fe, and formed by the multistage interaction of hydrothermal fluids with the host BIF formation. The oxygen isotope compositions of magnetite and hematite from BIF, hydrothermal alteration assemblages, and high-grade iron Ore were analyzed from the Mount Tom Price, Paraburdoo, and Charmar iron ore deposits. The delta(18)O values of magnetite and hematite from hydrothermal alteration assemblages and high-grade iron ore range from -9.0 to -2.9 per mil, a depletion of 5 to 15 per mil relative to the host BIF. The delta(18)O values are spatially controlled by faults within the deposits, a response to higher fluid flux and larger influence the isotopic compositions by the hydrothermal fluids. The oxygen isotope composition of hydrothermal fluids (delta(18)O(fluid)) indicates that the decrease in the (18)O content of iron oxides was due to the interaction of both basinal brines and meteoric fluids with the original BIF. Late-stage talc-bearing ore at the Mount Tom Price deposit formed in the presence of a pulse of delta(18)O-enriched basinal brine, indicating that hydrothermal fluids may have repeatedly interacted with the BIFs during the Paleoproterozoic.

Ore genesis of Pb-Zn deposits in the Nappe zone of Northern Tunisia: Constraints from Pb-S-C-O isotopic systems

The Jalta and Jebel Ghozlane ore deposits are located in the extreme North of Tunisia, within the Nappe zone. The mineralization of Jalta, hosted in Triassic dolostones and the overlying Mio-Pliocene conglomerates, consists of abundant galena, barite, and cerussite with accessory sphalerite, pyrite, and jordanite. At Jebel Ghozlane, large Pb-Zn concentrations occur in the Triassic dolostones and Eocene limestones. The mineral association consists of galena, sphalerite, barite, and celestite and their oxidation products (cerussite, smithsonite, and anglesite). Lead isotope ratios in galena from both districts are relatively homogeneous ((206)Pb/(204)Pb = 18.702-18.823, (207)Pb/(204)Pb = 15.665-15.677, (208)Pb/(204)Pb = 38.725-38.875). The delta(34)S values for sulfates from both areas (+12.2 to +16.2 parts per thousand at Jalta and + 14.3 to + 19.4 parts per thousand at Jebel Ghozlane) are compatible with a derivation of sulfur from marine sulfates, possibly sourced from the Triassic evaporites. The delta(34)S values of the sulfides have a range between -10 and +12.5 parts per thousand at Jalta, and between -9.1 and +22.1 parts per thousand at Jebel Ghozlane. The large range of values suggests reduction of the sulfate by bacterial and/or thermochemical reduction of sulfate to sulfur. The high delta(34)S values of sulfides require closed-system reduction processes. The isotopically light carbon in late calcites (-6.3 to -2.5 parts per thousand) and authigenic dolomite (-17.6 parts per thousand) suggests an organic source of at least some of the carbon in these samples, whereas the similarity of the delta(18)O values between calcite (+24.8 parts per thousand) and the authigenic dolomite (+24.7 parts per thousand) of Jalta and their respective host rocks reflects oxygen isotope buffering of the mineralizing fluids by the host rock carbonates. The secondary calcite isotope compositions of Jalta are compatible with a hydrothermal fluid circulation at approximately 100 to 200 degrees C, but temperatures as low as 50 degrees C may be indicated by the late calcite of Jebel Ghozlane (delta(18)O of +35.9 parts per thousand). Given the geological events related to the Alpine orogeny in the Nappe zone (nappe emplacement, bimodal volcanism, and reactivation of major faults, such as Ghardimaou-Cap Serrat) and the Neogene age of the host rocks in several localities, a Late-Miocene age is proposed for the Pb-Zn ore deposits considered in this study. Remobilization of deep-seated primary deposits in the Paleozoic sequence is the most probable source for metals in both localities considered in this study and probably in the Nappe zone as a whole. (C) 2011 Elsevier B.V. All rights reserved.

Pollution and pollutant transport in the geosphere - An introduction to the symposium

Environmental research in earth sciences is focused on the geosphere, i.e. (1) waters and sediments of rivers, lakes and oceans, and (2) soils and underlying shallow rock formations,both water-unsaturated and -saturated. The subsurface is studied down to greater depths at sites where waste repositories or tunnels are planned and mining activities exist. In recent years, earth scientists have become more and more involved in pollution problems related to their classical field of interest, e.g. groundwater, ore deposits, or petroleum and non-metal natural deposits (gravel, clay, cement precursors). Major pollutants include chemical substances, radioactive isotopes and microorganisms. Mechanisms which govern the transport of pollutants are of physical, chemical (dissolution, precipitation, adsorption), or microbiological (transformation) nature. Land-use planning must reflect a sustainable development and sound scientific criteria. Today's environmental pollution requires working teams with an interdisciplinary background in earth sciences, hydrology, chemistry, biology, physics as well as engineering. This symposium brought together for the first time in Switzerland earth and soil scientists, physicists and chemists, to present and discuss environmental issues concerning the geosphere.

Dispersion of natural arsenic in the Malcantone watershed, Southern Switzerland: field evidence for repeated sorption-desorption and oxidation-reduction processes

In recent years, elevated arsenic concentrations have been found in waters and soils of many, countries, often resulting in a health threat for the local population. Switzerland is not an exception and this paper deals with the release and subsequent fate of arsenic in a 200-km(2) mountainous watershed, characterized by crystalline silicate rocks (gneisses, schists, amphibolites) that contain abundant As-bearing sulfide ore deposits, some of which have been mined for iron and gold in the past. Using analytical methods common for mineralogical, ground water and soil studies (XRD, XRF, XAS-XANES and -EXAFS, electron microprobe, extraction, ICP, AAS with hydride generator, ion chromatography), seven different field situations and related dispersion processes of natural arsenic have been studied: (1) release by rock weathering, (2) transport and deposition by water and ice; (3) release of As to the ground and surface water due to increasing pH; (4) accumulation in humic soil horizons; (5) remobilization by reduction in water-saturated soils and stagnant ground waters; (6) remobilization by using P-rich fertilizers or dung and (7) oxidation, precipitation and dilution in surface waters. Comparison of the results with experimental adsorption studies and speciation diagrams from the literature allows us to reconstruct and identify the typical behavior of arsenic in a natural environment under temperate climatic conditions. The main parameters identified are: (a) once liberated from the primary minerals, sorption processes on Fe-oxy-hydroxides dominate over Al-phases, such as Al-hydroxides or clay minerals and limit the As concentrations in the spring and well waters between 20 and 300 mug/l. (b) Precipitation as secondary minerals is limited to the weathering domain, where the As concentrations are still high and not yet too diluted by rain and soils waters. (c) Although neutral and alkaline pH conditions clearly increase the mobility of As, the main factor to mobilize As is a low redox potential (Eh close or below 0 mV), which favors the dissolution of the Fe-oxy-hydroxides on which the As is sorbed. (d) X-ray absorption spectroscopy (XAS) of As in water-logged humic forest soils indicates that the reduction to As III only occurs at the solid-water interface and that the solid contains As as As V (e) A and Bh horizons of humic cambisols can effectively capture As when As-rich waters flow through them. Complex spatial and temporal variation of the various parameters in a watershed results in repeated mobilization and immobilization of As, which continuously transports As from the upper to the lower part of a watershed and ultimately to the ocean. (C) 2004 Elsevier B.V. All rights reserved.

Minerais, métaux, isotopes : recherches archéométriques sur les mines de plomb et d'argent en Valais, Suisse

RESUME Les nombreuses mines de plomb et d'argent du Valais témoignent d'une activité minière importante par le passé, sans toutefois dévoiler ni l'importance des minéralisations, ni l'ancienneté de l'exploitation. La présente recherche a pour but de comprendre pourquoi les grandes mines sont concentrées dans une région, et de déterminer la chronologie de leur exploitation. L'originalité de ce travail réside dans son interdisciplinarité, plus précisément dans l'application des méthodes minéralogiques pour résoudre une problématique historique. Afin d'évaluer les ressources minières en plomb et en argent du Valais, 57 mines et indices ont été repérés et échantillonnés. Les signatures isotopiques du Pb (74 analyses) et les compositions chimiques élémentaires (45 analyses) ont été déterminées. Les plus grandes exploitations se situent dans la nappe de Siviez-Mischabel, au Sud d'une ligne Vallée du Rhône / Val de Bagnes ainsi que dans le Lötschental. Elles sont liées, d'après leur signature isotopique de plomb, à des minéralisations d'âge calédonien (408 à 387 Ma) ou tardi-hercynien (333 à 286 Ma). À ces périodes, l'ancien continent est très lourd et subit une subsidence thermique. Des premières fractures d'extrême importance se forment. Comme il s'agit d'accidents tectoniques majeurs, des gisements de grande extension peuvent se former dans ce contexte. D'autres minéralisations se situent dans les domaines helvétiques (Massif des Aiguilles Rouges, Massif du Mont Blanc et couverture sédimentaire), couvrant une région au Nord de la Vallée du Rhône et du Val d'Entremont. D'âge post-hercynien à tardi-alpin (notons qu'il n'y a pas de minéralisations d'âge tertiaire), elles sont pour la plupart liées à des intrusions granitiques, sources de plomb juvénile. Les mines situées dans ces unités tectoniques sont nettement moins étendues que celles de la nappe de Siviez-Mischabel, ce qui permet de penser que les minéralisations correspondantes le sont également. Les périodes d'exploitation des mines peuvent être déterminées par quatre approches différentes l'archéologie minière, la lecture des textes historiques, l'étude des déchets métallurgiques et la comparaison de la signature isotopique du plomb, que l'on mesure dans un objet archéologique bien daté (monnaie, bijoux etc.), avec celles des minerais. Cette dernière méthode a été appliquée et développée dans le cadre de la présente recherche. Pour ce faire, 221 échantillons d'objet en plomb ou en argent datés entre l'Âge du Fer et le Moyen Age ont été analysés par la méthode des isotopes de plomb et comparés à environ 1800 signatures isotopiques de minerais des gisements les plus importants en Suisse et en Europe. Avant l'époque romaine et jusqu'au 1 er siècle de cette époque, le plomb provient principalement des mines de la péninsule ibérique alors en pleine activité. Un apport des mines d'Europe tempérée, notamment des Vosges, reste à confirmer. A partir du 1" siècle de notre ère, le plomb a principalement été importé en Suisse occidentale de grands centres de productions situées en Allemagne du Nord (région d'Eifel). Les mines de plomb valaisannes, notamment celles de Siviez, débutent leur exploitation en même temps, principalement pour couvrir les besoins locaux, mais également pour l'exportation jusque dans l'arc lémanique et, dans une moindre importance, au-delà. À partir du 4ème siècle, le besoin en plomb a été couvert par un apport des mines locales et par la refonte d'objets anciens. Ce changement d'approvisionnement est probablement lié aux tensions créées par les invasions germaniques durant la seconde moitié du 3' siècle ; le marché suisse n'est dès lors plus approvisionné par le nord, c'est-à-dire par la vallée du Rhin. Quant à l'argent, l'exploitation de ce métal est attestée à partir de la fin du La Tène, peu après l'apparition de ce métal dans la région valaisanne. L'échantillonnage ne couvrant pas l'époque romaine, rien n'est connu pour cette période. A partir du 5" siècle, une exploitation d'argent est de nouveau attestée. Cependant, l'exploitation d'argent des mines locales ne gagne en importance qu'à partir du Moyen Âge avec les frappes monétaires, notamment les frappes carolingiennes et épiscopales valaisannes. Les sources d'argent sont différentes selon leur utilisation : à part quelques exceptions notamment vers la fin du La Tène et au tardo-antique, les bijoux et objets de cultes ont été souvent créés à partir d'argent refondu, contrairement aux monnaies pour lesquelles l'argent provient des mines locales. On note un approvisionnement différent de ce métal pour les objets, notamment les monnaies, selon leur lieu de fabrication : on peut clairement distinguer les objets valaisans de ceux du Plateau Suisse. SUMMARY The many lead and silver mines of the Valais testify of an important mining activity in the past, without however revealing neither the importance of the mineralizations, nor the era of the exploitation. The purpose of this research is to understand why the large mines are concentrated in one region, and to determine the history of their exploitation. The uniqueness of this work lies in its interdisciplinarity, more precisely in the application of mineralogical methods to solve historical problems. In order to evaluate the lead and silver mining resources of the Valais region, 57 mines and ore deposits were located and sampled. The isotope signatures of Pb (74 analyses) and the compositions of the chemical elements (45 analyses) were determined. The largest activities are in the Siviez-Mischabel area, located in the South of the boundary formed by the Rhone, Bagnes and Lotschental valleys. According to their lead isotope signatures, they are linked to mineralizations of the Caledonian (408 to 387 my) or tardi-Hercynian (333 to 286 my) orogenies. In those times, the old continent was very heavy and underwent a thermal subsidence. First fractures of great significance were formed. Through these major tectonic events, large extended ore deposits can be formed. Other mineralizations are found in the helvetic regions situated north of the Rhone and the Entremont valley (the Aiguilles Rouges basement, Mount Blanc basement and the covering sediment). Because they are from post-hercynien to tardi-alpine age (there are no mineralizations of tertiary age), they are mainly linked to granite intrusions, the sources of juvenile lead. The mines found in these tectonic units are significantly less extensive than those of the Siviez-Mischabel area, leading to the assumption that the respective mineralizations extend accordingly. The history of exploitation of the mines can be determined by four different sources: mining archaeology, historical texts, metallurgical waste, and the comparison of the isotope signature of the lead from accurately dated archaeological objects (currency, jewels etc), with those of the ores. This last approach was applied and developed within the framework of this research. The lead isotope signatures of 221 lead or silver objects from the Iron Age to the Middle Age were compared with approximately 1800 samples of ore of the most important ore deposits in Switzerland and Europe. Before the Roman time up to the 1st century, lead comes mainly from the mines of the Iberian Peninsula then in full activity. A contribution of the mines of Central Europe, in particular of the Vosges, remains to be confirmed. From the 1st century on, lead was mainly imported into Western Switzerland from Northern Germany (Eiffel region). The lead mines in the Valais region, in particular those of Siviez, begin their exploitation at the same time, mainly to meet the local needs, but also for export to the lemanic basin and of lesser importance, beyond. As from the 4th century, the need of lead was met by the production from local mines and the recycling of old objects. This change of supply is probably related to the tensions created by the Germanic invasions during second half of the 3rd century; as a consequence, the Swiss market is not supplied any more by the north, i.e. the Rhine valley. Silver production is confirmed starting from the end of La Tene, shortly after the appearance of this metal in the Valais region. Since no objects of Roman origin were analyzed, nothing is known for this period. From the 5th century on, silver production is again confirmed. However, significant silver production from local mines starts only in the Middle Age with the coinage, in particular Carolingian and Episcopal minting from the Valais region. The sources of silver differ according to their use: besides some exceptions in particular towards the end of La Tene and the tardi-Roman, the jewels and objects of worships were often created from recycled silver, contrary to the coins the silver for which comes from the local mines. A different source of silver is observed according to the location of coin manufacture: Objects originating from the Valais region are clearly distinguished from those from the Plateau Suisse. ZUSAMMENFASSUNG Die grosse Zahl von Blei- und Silberminen im Wallis ist Zeugnis einer bedeutenden Bergbautätigkeit, es fehlen aber Hinweise über ihren Umfang und den Zeitraum ihrer Ausbeutung. Die vorliegende Arbeit sucht zu ergründen, warum grosse Minen sich in einer eng begrenzten Region häufen und in welchem Zeitraum sie genutzt wurden. Die Besonderheit der Studie liegt in ihrer Interdisziplinarität, genauer in der Anwendung von mineralogischen Methoden zur Beantwortung historischer Fragestellungen. Zur Beurteilung der Lagerstätten wurden von 57 Minen und Aufschlüssen Proben entnommen oder Nachweise erbracht und mittels 74 Isotopen-Analysen von Blei und 45 chemischen Gesamtanalysen ausgewertet. Die wichtigsten Vorkommen liegen in der Siviez- Mischabel- Decke südlich der Linie Rhonetal- Val de Bagnes, sowie im Lötschental. Die Bleiisotopen- Alter weisen ihre Entstehung der kaledonischen (408 - 387 Mio. J.) oder der spät- herzynischen (333 - 286 Mio. J.) Gebirgsbildungsphase zu. In dieser Periode ist die kompakte Landmasse sehr schwer und erfairt eine thermische Absenkung. Es bilden sich tektonische Brüche von kontinentaler Ausdehnung. Die grossen tektonischen Bewegungen ermöglichen die Bildung von ausgedehnten Lagerstätten. Andere Vorkommen finden sich im Bereich der Helvetischen Alpen (Aiguilles Rouges Massiv, Mont-Blanc-Massiv und Sediment-Decken) im Gebiet nördlich des Rhonetales bis zum Val d'Entremont. Altersmässig sind sie der nach-hercynischen bis zur spät-alpidischen Orogenese zuzuweisen (auffällig ist das Fehlen von Vorkommen im Tertiär) und haben sich meist in der Folge von Granit- Intrusion, dem Ursprung von primärem Blei ausgebildet. Die Bergwerke in diesem Bereich sind deutlich weniger ausgedehnt als jene in der Siviez-Mischabel-Decke und entsprechen wahrscheinlich dem geringen Umfang der zugehörigen Vorkommen. Die Nutzungsperioden der Minen können mit vier verschiedenen Methoden bestimmt werden: Minenarchäologie, Historische Quellen, Auswertung von metallischen Abfällen (Schlacken) und Vergleich der Bleiisotopen-Zusammensetzung von Erzen mit jener von zeitlich gut datierbaren archäologischen Gegenständen (Münzen, Schmuckstücke). Die letztere Methode wurde im Rahmen der vorliegenden Forschungsarbeit entwickelt und angewendet. Zu diesem Zweck wurden an 221 Proben von Blei- oder Silberobjekten, die in die Periode zwischen Eisenzeit und Mittelalter eingestuft werden können, Bleiisotopen- Analysen durchgeführt und mit ca. 1800 Proben aus den wichtigsten Lagerstätten der Schweiz und Europas verglichen. Vor der Römerzeit und bis ins 1. Jahrh. stammt das Blei vornehmlich aus den in jener Zeit in voller Ausbeutung begriffenen Minen der Iberischen Halbinsel. Der Beitrag von Mitteleuropa, besonders der Vogesen, muss noch bestätigt werden. Ab dem 1. Jahrh. nach Chr. wurde die Westschweiz hauptschlich mit Blei aus den grossen Produktionszentren Norddeutschlands, vorwiegend der Eifel, versorgt. In dieser Periode setzt die Ausbeutung der Bleiminen des Wallis, besonders von Siviez, ein. Sie dienen der Deckung des örtlichen Bedarfs aber auch der Ausfuhr in das Gebiet des Genfersees und in einem bescheidenen Rahmen sogar darüber hinaus. Ab dem 4. Jahrhundert wurden vermehrt alte Objekte eingeschmolzen. Dieser Wechsel der Versorgungsquellen war vermutlich eine Folge der Wölkerwanderung in der zweiten Hälfte des 3. Jahrhunderts. Ab diesem Zeitpunkt war Helvetien der Zugang zu den Versorgungsquellen des Nordens, besonders des Rheinlandes, verwehrt. Der Abbau von Silber ist ab dem Ende des La Tène nachgewiesen, nur wenig nach dem Auftreten dieses Metalls im Wallis. Über die Römerzeit können wegen dem Fehlen entsprechender Proben keine Aussagen gemacht werden. Eine erneute Abbauperiode ist ab dem 5. Jahrhundert nachgewiesen. Die Produktion der örtlichen Minen erreicht aber erst im Mittelalter eine gewisse Bedeutung mit der Prägung von Mnzen durch die Karolinger und die Walliser Bischöfe. Die Herkunft des Silbers ist abhängig von dessen Verwendung. Mit wenigen Ausnahmen in der Zeit des La Tène und der späteren Römerzeit wurde für Kunst- und Kult- Gegenstände rezykliertes Silber verwendet, für Münzprägungen neues Silber aus den örtlichen Minen. Von Einfluss auf die Herkunft war auch der Produktionsstandort: Die Objekte aus dem Wallis unterscheiden sich deutlich von jenen des Mittellandes.

Hydrocarbon biomarkers in the Topla-Mezica zinc-lead deposits, northern Karavanke/Drau Range, Slovenia: Paleoenvironment at the site of ore formation

The Mississippi Valley-type zinc and lead deposits at Topla (250,150 metric tons (t) of ore grading 1.0 wt % Zn and 3.3 wt % Pb) and Mezica (19 million metric tons (Mt) of ore grading 5.3 wt % Pb and 2.7 wt % Zn) occur within the Middle to Upper Triassic platform carbonate rocks of the northern Karavanke/Drau Range geotectonic units of the Eastern Alps, Slovenia. The ore and host rocks of these deposits have been investigated by a combination of inorganic and organic geochemical methods to determine major, trace, and rare earth element (REE) concentrations, hydrocarbon distribution, and stable isotope ratios of carbonates, kerogen, extractable organic matter, and individual hydrocarbons. These data combined with sedimentological evidence provide insight into the paleoenvironmental conditions at the site of ore formation. The carbonate isotope composition, the REE patterns, and the distribution of hydrocarbon biomarkers (normal alkanes and steranes) suggest a marine depositional environment. At Topla, a relatively high concentration of redox sensitive trace elements (V, Mo, U) in the host dolostones and REE patterns parallel to that of the North American shale composite suggest that sediments were deposited in a reducing environment. Anoxic conditions enhanced the preservation of organic matter and resulted in relatively higher total organic carbon contents (up to 0.4 wt %). The isotopic composition of the kerogen (delta C-13(kerogon) = -29.4 to -25.0 parts per thousand, delta N-15(kerogen) = -.13.6 to 6.8 parts per thousand) suggests that marine algae and/or bacteria were the main source of organic carbon with a very minor contribution from detrital continental plants and a varying degree of alteration. Extractable organic matter from Topla ore is generally depleted in C-13 compared to the associated kerogen, which is consistent with an indigenous source of the bitumens. The mineralization correlates with delta N-15(kerogen) values around 0 per mil, C-13 depleted kerogen, C-13 enriched n-heptadecane, and relatively high concentrations of bacteria] hydrocarbon biomarkers, indicating a high cyanobacterial biomass at the site of ore formation. Abundant dissimilatory sulfate-reducing bacteria, feeding on the cyanobacterial remains, led to accumulation of biogenic H2S in the pore water of the sediments. This biogenic H2S was mainly incorporated into sedimentary organic matter and diagenetic pyrite. Higher bacterial activity at the ore site also is indicated by specific concentration ratios of hydrocarbons, which are roughly correlated with total Pb plus Zn contents. This correlation is consistent with mixing of hydrothermal metal-rich, fluids and local bacteriogenic sulfide sulfur. The new geochemical data provide supporting evidence that Topla is a low-temperature Mississippi Valley-type deposit formed in an anoxic supratidal saline to hypersaline environment. A laminated cyanobacterial mat, with abundant sulfate-reducing bacteria was the main site of sulfate reduction.

Sr, C and O isotope systematics in the Pucara Basin, central Peru - Comparison between Mississippi Valley-type deposits and barren areas

A combined Sr, O and C isotope study has been carried out in the Pucara basin, central Peru, to compare local isotopic trends of the San Vicente and Shalipayco Zn-Pb Mississippi Valley-type (MVT) deposits with regional geochemical patterns of the sedimentary host basin. Gypsum, limestone and regional replacement dolomite yield Sr-87/Sr-86 ratios that fall within or slightly below the published range of seawater Sr-87/Sr-86 values for the Lower Jurassic and the Upper Triassic. Our data indicate that the Sr isotopic composition of seawater between the Hettangian and the Toarcian may extend to lower Sr-87/Sr-86 ratios than previously published values. An Sr-87-enrichment is noted in (1) carbonate rocks from the lowermost part of the Pucara basin, and (2) different carbonate generations at the MVT deposits. This indicates that host rocks at MVT deposits and in the lowermost part of the carbonate sequence interacted with Sr-87-enriched fluids. The fluids acquired their radiogenic nature by interaction with lithologies underlying the carbonate rocks of the Pucara basin. The San Ramon granite, similar Permo-Triassic intrusions and their elastic derivatives in the Mitu Group are likely sources of radiogenic Sr-87. The Brazilian shield and its erosion products are an additional potential source of radiogenic Sr-87. Volcanic rocks of the Mitu Group are not a significant source for radiogenic Sr-87; however, molasse-type sedimentary rocks and volcaniclastic rocks cannot be ruled out as a possible source of radiogenic Sr-87. The marked enrichment in Sr-87 of carbonates toward the lower part of the Pucara Group is accompanied by only a slight decrease in delta(18)O values and essentially no change in delta(13)C values, whereas replacement dolomite and sparry carbonates at the MVT deposits display a coherent trend of progressive Sr-87-enrichment, and O-18- and C-13-depletion. The depletion in O-18 in carbonates from the MVT deposits are likely related to a temperature increase, possibly coupled with a O-18-enrichment of the ore-forming fluids. Progressively lower delta(13)C values throughout the paragenetic sequence at the MVT deposits are interpreted as a gradually more important contribution from organically derived carbon. Quantitative calculations show that a single fluid-rock interaction model satisfactorily reproduces the marked Sr-87-enrichment and the slight decrease in delta(18)O values in carbonate rocks from the lower part of the Pucara Group. By contrast, the isotopic covariation trends of the MVT deposits are better reproduced by a model combining fluid mixing and fluid-rock interaction. The modelled ore-bearing fluids have a range of compositions between a hot, saline, radiogenic brine that had interacted with lithologies underlying the Pucara sequence and cooler, dilute brines possibly representing local fluids within the Pucara sequence. The composition of the local fluids varies according to the nature of the lithologies present in the neighborhood of the different MVT deposits. The proportion of the radiogenic fluid in the modelled fluid mixtures interacting with the carbonate host rocks at the MVT deposits decreases as one moves up in the stratigraphic sequence of the Pucara Group.

Organic and inorganic geochemistry of Ljubija siderite deposits, NW Bosnia and Herzegovina

The Ljubija siderite deposits, hosted by a Carboniferous sedimentary complex within the Inner Dinarides, occur as stratabound replacement-type ore bodies in limestone blocks and as siderite-sulfides veins in shale. Three principal types of ore textures have been recognized including massive dark siderite and ankerite, siderite with zebra texture, and siderite veins. The ore and host rocks have been investigated by a combination of inorganic (major, trace, and rare earth element concentrations), organic (characterization of hydrocarbons including biomarkers), and stable isotope geochemical methods (isotope ratios of carbonates, sulfides, sulfates, kerogen, and individual hydrocarbons). New results indicate a marine origin of the host carbonates and a hydrothermal-metasomatic origin of the Fe mineralization. The differences in ore textures (e.g., massive siderite, zebra siderite) are attributed to physicochemical variations (e.g., changes in acidity, temperature, and/or salinity) of the mineralizing fluids and to the succession and intensity of replacement of host limestone. Vein siderite was formed by precipitation from hydrothermal fluids in the late stage of mineralization. The equilibrium fractionation of stable isotopes reveals higher formation temperatures for zebra siderites (around 245A degrees C) then for siderite vein (around 185A degrees C). Sulfur isotope ratios suggest Permian seawater or Permian evaporites as the main sulfur source. Fluid inclusion composition confirms a contribution of the Permian seawater to the mineralizing fluids and accord with a Permian mineralization age. Organic geochemistry data reflect mixing of hydrocarbons at the ore site and support the hydrothermal-metasomatic origin of the Ljubija iron deposits.

Carbon and oxygen isotope study of hydrothermal carbonates in the zinc-lead deposits of the San Vicente district, central Peru: A quantitative modeling on mixing processes and CO2 degassing

Carbon and oxygen isotope studies of the host and gangue carbonates of Mississippi Valley-type zinc-lead deposits in the San Vicente District hosted in the Upper Triassic to Lower Jurassic dolostones of the Pucara basin (central Peru) were used to constrain models of the ore formation. A mixing model between an incoming hot saline slightly acidic radiogenic (Pb, Sr) fluid and the native formation water explains the overall isotopic variation (delta(13)C = - 11.5 to + 2.5 parts per thousand relative to PDB and delta(18)O = + 18.0 to + 24.3 parts per thousand relative to SMOW) of the carbonate generations. The dolomites formed during the main ore stage show a narrower range (delta(13)C = - 0.1 to + 1.7 parts per thousand and delta(18)O = + 18.7 to + 23.4 parts per thousand) which is explained by exchange between the mineralizing fluids and the host carbonates combined with changes in temperature and pressure. This model of fluid-rock interaction explains the pervasive alteration of the host dolomite I and precipitation of sphalerite I. The open-space filling hydrothermal white sparry dolomite and the coexisting sphalerite II formed by prolonged fluid-host dolomite interaction and limited CO2 degassing. Late void-filling dolomite III (or calcite) and the associated sphalerite III formed as the consequence of CO2 degassing and concomitant pH increase of a slightly acidic ore fluid. Widespread brecciation is associated to CO2 outgassing. Consequently, pressure variability plays a major role in the ore precipitation during the late hydrothermal events in San Vicente. The presence of native sulfur associated with extremely carbon-light calcites replacing evaporitic sulfates (e.g., delta(13)C = - 11.5 parts per thousand), altered native organic matter and heavier hydrothermal bitumen (from - 27.0 to - 23.0 parts per thousand delta(13)C) points to thermochemical reduction of sulfate and/or thiosulfate. The delta(13)C- and delta(18)O-values of the altered host dolostone and hydrothermal carbonates, and the carbon isotope composition of the associated organic matter show a strong regional homogeneity. These results coupled with the strong mineralogical and petrographic similarities of the different MVT occurrences perhaps reflects the fact that the mineralizing processes were similar in the whole San Vicente belt, suggesting the existence of a common regional mineralizing hydrothermal system with interconnected plumbing.

Magmatic-dominated fluid evolution in the Jurassic Nambija gold skarn deposits (southeastern Ecuador)

The Jurassic (approximately 145 Ma) Nambija oxidized gold skarns are hosted by the Triassic volcanosedimentary Piuntza unit in the sub-Andean zone of southeastern Ecuador. The skarns consist dominantly of granditic garnet (Ad(20-98)) with subordinate pyroxene (Di(46-92)Hd(17-42)Jo(0-19)) and epidote and are spatially associated with porphyritic quartz-diorite to granodiorite intrusions. Endoskarn is developed at the intrusion margins and grades inwards into a potassic alteration zone. Exoskarn has an outer K- and Na-enriched zone in the volcanosedimentary unit. Gold mineralization is associated with the weakly developed retrograde alteration of the exoskarn and occurs mainly in sulfide-poor vugs and milky quartz veins and veinlets in association with hematite. Fluid inclusion data for the main part of the prograde stage indicate the coexistence of high-temperature (500A degrees C to > 600A degrees C), high-salinity (up to 65 wt.% eq. NaCl), and moderate- to low-salinity aqueous-carbonic fluids interpreted to have been trapped at pressures around 100-120 MPa, corresponding to about 4-km depth. Lower-temperature (510-300A degrees C) and moderate- to low-salinity (23-2 wt.% eq. NaCl) aqueous fluids are recorded in garnet and epidote of the end of the prograde stage. The microthermometric data (Th from 513A degrees C to 318A degrees C and salinity from 1.0 to 23 wt.% eq. NaCl) and delta(18)O values between 6.2aEuro degrees and 11.5aEuro degrees for gold-bearing milky quartz from the retrograde stage suggest that the ore-forming fluid was dominantly magmatic. Pressures during the early retrograde stage were in the range of 50-100 MPa, in line with the evidence for CO(2) effervescence and probable local boiling. The dominance of magmatic low-saline to moderately saline oxidizing fluids during the retrograde stage is consistent with the depth of the skarn system, which could have delayed the ingression of external fluids until relatively low temperatures were reached. The resulting low water-to-rock ratios explain the weak retrograde alteration and the compositional variability of chlorite, essentially controlled by host rock compositions. Gold was precipitated at this stage as a result of cooling and pH increase related to CO(2) effervescence, which both result in destabilization of gold-bearing chloride complexes. Significant ingression of external fluids took place after gold deposition only, as recorded by delta(18)O values of 0.4aEuro degrees to 6.2aEuro degrees for fluids depositing quartz (below 350A degrees C) in sulfide-rich barren veins. Low-temperature (< 300A degrees C) meteoric fluids (delta(18)O(water) between -10.0aEuro degrees and -2.0aEuro degrees) are responsible for the precipitation of late comb quartz and calcite in cavities and veins and indicate mixing with cooler fluids of higher salinities (about 100A degrees C and 25 wt.% eq. NaCl). The latter are similar to low-temperature fluids (202-74.5A degrees C) with delta(18)O values of -0.5aEuro degrees to 3.1aEuro degrees and salinities in the range of 21.1 to 17.3 wt.% eq. CaCl(2), trapped in calcite of late veins and interpreted as basinal brines. Nambija represents a deep equivalent of the oxidized gold skarn class, the presence of CO(2) in the fluids being partly a consequence of the relatively deep setting at about 4-km depth. As in other Au-bearing skarn deposits, not only the prograde stage but also the gold-precipitating retrograde stage is dominated by fluids of magmatic origin.

An evaluation of the inorganic and organic geochemistry of the San Vicente Mississippi Valley-type zinc-lead district, central Peru: Implications for ore fluid composition, mixing processes, and sulfate reduction

Mississippi Tialley-type zinc-lead deposits and ore occurrences in the San Vicente belt are hosted in dolostones of the eastern Upper Triassic to Lower Jurassic Pucara basin, central Peru. Combined inorganic and organic geochemical data from 22 sites, including the main San Vicente deposit, minor ore occurrences, and barren localities, provide better understanding of fluid pathways and composition, ore precipitation mechanisms, Eh-pH changes during mineralization, and relationships between organic matter and ore formation. Ore-stage dark replacement dolomite and white sparry dolomite are Fe and rare earth element (REE) depleted, and Mn enriched, compared to the host dolomite. In the main deposit, they display significant negative Ce and probably Eu anomalies. Mixing of an incoming hot, slightly oxidizing, acidic brine (H2CO3 being the dominant dissolved carbon species), probably poor in REE and Fe, with local intraformational, alkaline, reducing waters explains the overall carbon and oxygen isotope variation and the distributions of REE and other trace elements in the different hydrothermal carbonate generations. The incoming ore fluid flowed through major aquifers, probably basal basin detrital units, with limited interaction with the carbonate host rocks. The hydrothermal carbonates show a strong regional chemical homogeneity, indicating access of the ore fluids by interconnected channelways near the ore occurrences. Negative Ce anomalies in the main deposit, that are absent at the district scale, indicate local ore-fluid chemical differences. Oxidation of both migrated and indigenous hydrocarbons by the incoming fluid provided the local reducing conditions necessary for sulfate reduction to H2S, pyrobitumen precipitation, and reduction of Eu3+ to Eu2+. Fe-Mn covariations, combined with the REE contents of the hydrothermal carbonates, are consistent with the mineralizing system shifting from reducing/rock-dominated to oxidizing/fluid-dominated conditions following ore deposition. Sulfate and sulfide sulfur isotopes support sulfide origin from evaporite-derived sulfate by thermochemical organic reduction; further evidence includes the presence of C-13-depleted calcite cements (similar to-12 parts per thousand delta(13)C) as sulfate pseudomorphs, elemental sulfur, altered organic matter in the host dolomite, and isotopically heavier, late, solid bitumen. Significant alteration of the indigenous and extrinsic hydrocarbons, with absent bacterial membrane biomarkers (hopanes) is observed. The light delta(34)S of sulfides from small mines and occurrences compared to the main deposit reflect a local contribution of isotopically light sulfur, evidence of local differences in the ore-fluid chemistry.

Genesis of the Jurassic carbonate-hosted Pb-Zn deposits of Jebel Ressas (North-eastern Tunisia): Evidence from mineralogy, petrography and trace metal contents and isotope (O, C, S, Pb) geochemistry

The Jebel Ressas Pb-Zn deposits in North-Eastern Tunisia occur mainly as open-space fillings (lodes, tectonic breccia cements) in bioclastic limestones of the Upper Jurassic Ressas Formation and along the contact of this formation with Triassic rocks. The galena-sphalerite association and their alteration products (cerussite, hemimorphite, hydrozincite) are set within a calcite gangue. The Triassic rocks exhibit enrichments in trace metals, namely Pb, Co and Cd enrichment in clays and Pb, Zn, Cd, Co and Cr enrichment in carbonates, suggesting that the Triassic rocks have interacted with the ore-bearing fluids associated with the Jebel Ressas Pb-Zn deposits. The delta(18)O content of calcite associated with the Pb-Zn mineralization suggests that it is likely to have precipitated from a fluid that was in equilibrium with the Triassic dolostones. The delta(34)S values in galenas from the Pb-Zn deposits range from -1.5 to +11.4%, with an average of 5.9% and standard deviation of 3.9%. These data imply mixing of thermochemically-reduced heavy sulfur carried in geothermal- and fault-stress-driven deep-seated source fluid with bacterially-reduced light sulfur carried in topography-driven meteoric fluid. Lead isotope ratios in galenas from the Pb-Zn deposits are homogenous and indicate a single upper crustal source of base-metals for these deposits. Synthesis of the geochemical data with geological data suggests that the base-metal mineralization at Jebel Ressas was formed during the Serravallian-Tortonian (or Middle-Late Miocene) Alpine compressional tectonics.

Apparent stable-isotope heterogeneities in gangue carbonates of the Mississippi Valley-type Zn-Pb deposits of San-Vicente, Central Peru

The aim of the present communication is to emphasize that some variations of the measured delta(13)C and delta(18)O values are apparent, and due to analytical interferences caused by the presence of sulfur and organosulfur compounds in the analyzed carbonates. This is particularly relevant for isotopic studies on carbonate-hosted mineral deposits, where the nearly ubiquitous association of the host carbonates with organic matter and sulfides can certainly affect the metallogenetic interpretations. In this work two methods were used to overcome the disturbing effects of sulfides and organic matter: (1) sample pretreatment following the method proposed by Charef and Sheppard (1984), combining the oxidation of organic matter with sodium hypochlorite and trapping of the sulfur species with silver phosphate; and (2) laser-based microprobe extraction. Apparent isotopic variations in sparry dolomite from a single hand sample of zebra ore from the MVT Zn-Pb deposit, San Vicente, central Peru, are as large as 6 parts per thousand delta(13)C and 4 parts per thousand delta(18)O. These variations are reduced to several tenths of a per mil when the samples are pretreated. A careful examination of the effects of treatment with NaOCl and/or Ag3PO4 in relation to the concentration of sulfide inclusions indicates that the main disturbing effects for delta(13)C values are the presence of sulfur species and organic matter, whereas the delta(18)O values are mainly affected by the presence of sulfides. Fine- and medium-grained replacement carbonates from MVT and other sediment-hosted base metal deposits are potentially the most affected during isotope analysis, due to the common presence of organic matter and sulfides. Using in situ laser microprobe techniques, it is possible to determine isotopic variations at a sub-millimeter scale. Our results show that laser extraction analysis allows a more precise sampling of the carbonate minerals, and minimizes contamination of the sample with sulfides and to some extent with intergrown organic matter. However, there is an isotopic shift associated with the laser extraction technique, of the order of 0.5-1 parts per thousand for delta(13)C and delta(18)O values.