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.

Stable carbon isotopes in archaeobotanical remains and palaeoclimate

Es descriu una metodologia recent per a inferir la precipitació en el passat basada en l’anàlisi de la composició isotòpica del carboni (δ13C) en restes arqueobotàniques. Un cop descrita la base fisiològica de la tècnica, s’il·lustra l’aplicabilitat de δ13C mitjançant un exemple referent al NE peninsular. Hom pretén proporcionar una estimació quantitativa de l’evolució de la precipitació estacional (primavera) i anual al llarg dels darrers quatre mil anys basada en δ13C. Les mostres analitzades comprenen carbons (pi blanc) i llavors carbonitzades (blat i ordi), i s’obtenen estimes pluviomètriques superiors en el passat que actualment, amb una tendència gradual cap a condicions progressivament més àrides. No obstant això, aquesta tendència no esdevé uniforme, i es detecten dues fases de major precipitació (1800-900 aC; 300 aC - 300 dC) alternadament amb períodes relativament secs (900-300 aC; 900 dC - present). Dels resultats presentats també es desprèn que la importància relativa de la pluja primaveral en el passat fou variable. Des d’aproximadament el 300 aC en endavant, el període primaveral subministrà una major proporció de pluja anual que actualment. Contràriament, durant el període 1800-800 dC la seva contribució va esdevenir inferior, i va aparèixer una fase transitòria (800-300 aC) que mostra una recuperació sobtada en aportació primaveral. Posteriorment a aquesta fase la sincronia de canvis en δ13C en granes i carbons suggereix l’arribada del clima mediterrani a la regió.

Mantle- and crust-derived magmatism in the southern Fennoscandian Shield at c. 1.8 Ga; evidence from geochemistry, isotopes and geochronology

Geokemi och isotopsammansättningarna hos ca 1,8 Ga (miljarder år) gamla mafiska bergartsintrusioner studerades i två huvudområden: i) Transskandinaviska magmatiska bältet (TMB) i Bergslagen, Småland och Blekinge, södra Sverige, inklusive några prov från det ca 1,87 Ga gamla Hedesunda-komplexet i östra Bergslagen, samt ii) mindre, postkollisionala komplex i södra Finland och ryska Karelen. I det senare fallet var även tillhörande granitoider inkluderade i studierna. TMB-bergarterna skiljer sig avsevärt i utvecklingsgrad och omfattar sammansättningsmässigt bergarter från ultramafiter till kvartsdioriter. Dessa bergarters geokemi är kännetecknande för kontinentala öbågar. För sydligaste TMB och Hedesunda antyder geokemin en något mera oceanisk öbågekaraktär. Tillsammans med tidigare data antyder de av Rutanen analyserade Nd- och Sr-isotopförhållanden för TMB en ’milt utarmad’ mantelsammansättning. De mafiska bergarterna i södra Finland och ryska Karelen varierar från ultramafiska till monzodioritiska, men med avsevärt högre alkalihalter jämfört med TMB. Källan för all den studerade mafiska magmatismen kan beskrivas som en utarmad mantel som i varierande grad påverkats av fluider och smältor ur subducerande litosfärplattor. Geokemin antyder infiltrering och påverkning av H2O-dominerande fluider i övre manteln för TMB. Den mafiska ca 1,8 Ga gamla magmatismen österut avspeglar en ökande påverkan av sedimentderiverade karbonatfluider och smältor inom allt djupare mantelområden. Denna subduktionsrelaterade mantelanrikning skedde under den föregående öbågeutvecklingen i södra delarna av Finland och Sverige, samt ryska Karelen. Geokemin för en grupp granitoider, associerade med de ca 1,8 Ga gamla intrusionerna i södra Finland visar både vulkanisk öbåge och synkollisional granitoidkaraktär. Denna grupp har ett blandat magmatiskt och sedimentärt Svekofenniskt ursprung, vilket kan antas p.g.a. deras Nd- och Sr-isotopförhållanden. En annan grupp av granitoider ligger geokemiskt mellan vulkanisk öbåge- och intraplatt-granitoider, och har magmatiskt ursprung. Geokemin och isotoperna hos dessa intrusioner kan förklaras med hybridisering mellan de kraftigt anrikade, mantelderiverade magmorna, och granitmagmor från den äldre skorpan. Den ca 1,8 Ga gamla TMB-magmatismen i Sverige skedde vid sammanslutning av kontinentalrandbågar, med kontinuerlig subduktion mot öster i Bergslagen, och mot norr i de sydligare delarna. Samtidigt i öster intruderade de postkollisionala intrusionerna i skorpan omedelbart efter kollisionen med den Volgo-Sarmatiska kontinenten från sydost. Denna invecklade paleotektoniska konfiguration orsakade en tektonisk regim där litosfäriska mantelkällor levererade de starkt anrikade magmorna, vilkas uppstigning troligen möjliggjordes av djupgående postkollisionala skjuvzoner. Intrusionerna orsakade uppsmältning av den omgivande skorpan, vilket framkallade den associerade granitoidmagmatismen.

Establishing Winter Origins of Migrating Lesser Snow Geese Using Stable Isotopes

Increases in Snow Goose (Chen caerulescens) populations and large-scale habitat changes in North America have contributed to the concentration of migratory waterfowl on fewer wetlands, reducing resource availability, and enhancing risks of disease transmission. Predicting wintering locations of migratory individuals is critical to guide wildlife population management and habitat restoration. We used stable carbon (δ13C), nitrogen (δ15N), and hydrogen (δ2H) isotope ratios in muscle tissue of wintering Snow Geese to discriminate four major wintering areas, the Playa Lake Region, Texas Gulf Coast, Louisiana Gulf Coast, and Arkansas, and infer the wintering locations of individuals collected later during the 2007 and 2008 spring migrations in the Rainwater Basin (RWB) of Nebraska. We predicted the wintering ground derivation of migrating Snow Geese using a likelihood-based approach. Our three-isotope analysis provided an efficient discrimination of the four wintering areas. The assignment model predicted that 53% [95% CI: 37-69] of our sample of Snow Geese from the RWB in 2007 had most likely originated in Louisiana, 38% [23-54] had wintered on Texas Gulf Coast, and 9% [0-20] in Arkansas; the assessment suggested that 89% [73-100] of our 2008 sample had most likely come from Texas Gulf Coast, 9% [0-27] from Louisiana Gulf Coast, and 2% [0-9] from Arkansas. Further segregation of wintering grounds and additional sampling of spring migrating Snow Geese would refine overall assignment and help explain interannual variations in migratory connectivity. The ability to distinguish origins of northbound geese can support the development of spatially-adaptive management strategies for the midcontinent Snow Goose population. Establishing migratory connectivity using isotope assignment techniques can be extended to other waterfowl species to determine critical habitat, evaluate population energy requirements, and inform waterfowl conservation and management strategies.

Terrane transfer during the Grenville orogeny: tracing the Amazonian ancestry of southern Appalachian basement through Pb and Nd isotopes

Whole rock Pb isotope data can be used to determine the provenance of different blocks within the Rodinia supercontinent, providing a test for paleogeographic reconstructions. Calculated isotopic values for the source region of the Grenville-deformed SW Amazon craton (Rondonia, Brazil), anchored by published U-Pb zircon ages, are compared to those from the Grenville belt of North America and Grenvillian basement inliers in the southern Appalachians. Both the SW Amazon craton and the allochthonous Blue Ridge/Mars Hill terrane are defined by a similar Pb isotopic signature, indicating derivation from an ancient source region with an elevated U/Pb ratio. In contrast, the Grenville Province of Laurentia (extending from Labrador to the Llano Uplift of Texas) is characterized by a source region with a distinctly lower, time-integrated U/Pb ratio. Published U-Pb zircon ages (ca. 1.8 Ga) and Nd model ages (1.4-2.2 Ga) for the Blue Ridge/Mars Hill terrane also suggest an ancient provenance very different from the rest of the adjacent Grenville belt, which is dominated by juvenile 1.3-1.5 Ga rocks. The presence of mature continental material in rocks older than 1.15 Ga in the Blue Ridge/ Mars Hill terrane is consistent with characteristics of basement rocks from the SW Amazon craton. High-grade metamorphism of the Blue Ridge/Mars Hill basement resulted in purging of U, consistent with observations of the rest of the North American Grenville province. In contrast, the Grenvillian metamorphic history of the Amazon appears to have been much more heterogeneous, with both U enrichment and U depletion recorded locally. We propose that the Blue Ridge/ Mars Hill portion of the Appalachian basement is of Amazonian provenance and was transferred to Laurentia during Grenvillian orogenesis after similar to1.15 Ga. The presence of these Amazonian rocks in southeastern Laurentia records the northward passage of the Amazon craton along the Laurentian margin, following the original collision with southernmost Laurentia at ca. 1.2 Ga. (C) 2004 Elsevier B.V. All rights reserved.

A comparative study of aquifer systems occurring at the Paraná sedimentary basin, Brazil: U-isotopes contribution

The radioactivity due to 238U and 234U in three aquifer systems occurring within the Paraná sedimentary basin, South America, has been investigated. Uranium is much less dissolved from fractured igneous rocks than from the porous sedimentary rocks as indicated by the U-mobility coefficients between 7. 6 × 10-6 and 1. 2 × 10-3 g cm-3. These values are also compatible with the U preference ratios relative to Na, K, Ca, Mg and SiO2, which showed that U is never preferentially mobilized in the liquid phase during the flow occurring in cracks, fissures, fractures and faults of the igneous basaltic rocks. Experimental dissolution of diabase grains on a time-scale laboratory has demonstrated that the U dissolution appeared to be a two-stage process characterized by linear and second-order kinetics. The U dissolution rate was 8 × 10-16 mol m-2 s-1 that is within the range of 4 × 10-16-3 × 10-14 mol m-2 s-1 estimated for other rock types. The 234U/238U activity ratio of dissolved U in solutions was higher than unity, a typical result expected during the water-rock interactions when preferential 234U-leach from the rock surfaces takes place. Some U-isotopes data allowed estimating 320 ka for the groundwater residence time in a sector of a transect in São Paulo State. A modeling has been also realized considering all U-isotopes data obtained in Bauru (35 samples), Serra Geral (16 samples) and Guarani (29 samples) aquifers. The results indicated that the Bauru aquifer waters may result from the admixture of waters from Guarani (1. 5 %) and Serra Geral (98. 5 %) aquifers. © 2012 Springer-Verlag.

Growth and carbon isotopes of Mediterranean trees reveal contrasting responses to increased carbon dioxide and drought

Forest dynamics will depend upon the physiological performance of individual tree species under more stressful conditions caused by climate change. In order to compare the idiosyncratic responses of Mediterranean tree species (Quercus faginea, Pinus nigra, Juniperus thurifera) coexisting in forests of central Spain, we evaluated the temporal changes in secondary growth (basal area increment; BAI) and intrinsic water-use efficiency (iWUE) during the last four decades, determined how coexisting species are responding to increases in atmospheric CO2 concentrations (Ca) and drought stress, and assessed the relationship among iWUE and growth during climatically contrasting years. All species increased their iWUE (ca. +15 to +21 %) between the 1970s and the 2000s. This increase was positively related to Ca for J. thurifera and to higher Ca and drought for Q. faginea and P. nigra. During climatically favourable years the study species either increased or maintained their growth at rising iWUE, suggesting a higher CO2 uptake. However, during unfavourable climatic years Q. faginea and especially P. nigra showed sharp declines in growth at enhanced iWUE, likely caused by a reduced stomatal conductance to save water under stressful dry conditions. In contrast, J. thurifera showed enhanced growth also during unfavourable years at increased iWUE, denoting a beneficial effect of Ca even under climatically harsh conditions. Our results reveal significant inter-specific differences in growth driven by alternative physiological responses to increasing drought stress. Thus, forest composition in the Mediterranean region might be altered due to contrasting capacities of coexisting tree species to withstand increasingly stressful conditions. © 2013 Springer-Verlag Berlin Heidelberg.

Speciation and fractionation of Ca and the REE in fresh and marine waters

This study is concerned with speciation and fractionation of the rare earth elements (REE) and calcium (Ca) in aqueous solutions. The aim is to investigate the chemical states and physical sizes in which these elements can be present. The REE (including neodymium) and Ca have contrasting geochemical behavior in aqueous solutions. Ca is a major dissolved element, while the REE are trace components and highly reactive with aquatic particles. The major interests of the five papers included in this thesis are the following: · Papers I and V deal with the behavior of neodymium (Nd) and its isotopes in the Kalix River and some marine waters. · The diffusive gradients in thin-films (DGT) method is developed for measuring Ca and Mg in Paper II. · Paper III presents a speciation and fractionation study of Ca in the Kalix and Amazonian rivers. · The rare earth elements and their carrier phases are investigated in the Kalix river in Paper IV. For most elements a detailed study of speciation and fractionation can not be performed using only one method. This is due to the overall heterogeneity of the material, considering both size and chemical composition, which is present in aquatic solutions. During this project the aquatic geochemistry of the REE and Ca has been studied using mainly three methods; cross-flow filtration (CFF), field-flow fractionation (FFF) and diffusive gradients in thin-films (DGT). Field work has to a large part been conducted in the Kalix River, in northern Sweden, which is one of the last pristine river systems in Europe. Some field work has also been conducted in the Baltic Sea and the Arctic Ocean. Results from Amazonian rivers are also presented. These are the main conclusions from this work: The DGT technique works equally well for measuring Ca and Mg in natural waters as previously reported for trace metal. A significant colloidal phase for Ca could be detected in the Kalix River and in different Amazonian rivers. This was concluded independently using both CFF and FFF. Variations in REE signatures in the Kalix River suggests two different pathways for the REE during weathering and release form soil profiles and transport in the river. No significant variation in Nd-isotopic composition could be detected in the Kalix River although concentrations varied by a factor of ~10. This suggests that there is one major source for Nd in the river although different pathways for the REE may exist. A study of Nd in the Kalix River, the Baltic Sea and the Arctic Ocean showed that the isotopic compositions in the diffusible fractions were similar to water samples. However, the relative amount of diffusible Nd increased with salinity, probably reflecting the lower concentration of colloidal and particulate material in marine waters.

Late Quaternary palaeoenvironmental reconstruction from Lakes Ohrid and Prespa (Macedonia/Albania border) using stable isotopes

Abstract. Here we present stable isotope data from three sediment records from lakes that lie along the Macedonian- Albanian border (Lake Prespa: 1 core, and Lake Ohrid: 2 cores). The records only overlap for the last 40 kyr, although the longest record contains the MIS 5/6 transition (Lake Ohrid). The sedimentary characteristics of both lakes differ significantly between the glacial and interglacial phases. At the end of MIS 6 Lake Ohrid’s water level was low (high �18Ocalcite) and, although productivity was increasing (high calcite content), the carbon supply was mainly from inorganic catchment rock sources (high �13Ccarb). During the last interglacial, calcite and TOC production and preservation increased, progressively lower �18Ocalcite suggest increase in humidity and lake levels until around 115 ka. During ca. 80 ka to 11 ka the lake records suggest cold conditions as indicated by negligible calcite precipitation and low organic matter content. In Lake Ohrid, �13Corg are complacent; in contrast, Lake Prespa shows consistently higher �13Corg suggesting a low oxidation of 13C-depleted organic matter in agreement with a general deterioration of climate conditions during the glacial. From 15 ka to the onset of the Holocene, calcite and TOC begin to increase, suggesting lake levels were probably low (high �18Ocalcite). In the Holocene (11 ka to present) enhanced productivity is manifested by high calcite and organic matter content. All three cores show an early Holocene characterised by low �18Ocalcite, apart from the very early Holocene phase in Prespa where the lowest �18Ocalcite occurs at ca. 7.5 ka, suggesting a phase of higher lake level only in (the more sensitive) Lake Prespa. From 6 ka, �18Ocalcite suggest progressive aridification, in agreement with many other records in the Mediterranean, although the uppermost sediments in one core records low �18Ocalcite which we interpret as a result of human activity. Overall, the isotope data present here confirm that these two big lakes have captured the large scale, low frequency palaeoclimate variation that is seen in Mediterranean lakes, although in detail there is much palaeoclimate information that could be gained, especially small scale, high frequency differences between this region and the Mediterranean.

Evidence for extinct Cs-135 from Ba isotopes in Allende CAIs?

he abundance and distribution of isotopes throughout the Solar System can be used to constrain the number and type of nucleosynthetic events that contributed material to the early nebula. Barium is particularly well suited to quantifying the degree of isotope heterogeneity in the Solar System because it comprises seven stable isotopes that were synthesized by three different nucleosynthetic processes (s-, r-, and p-processes), all of which contributed material to the Solar System. There is also potential contribution to 135Ba from short-lived radioisotope 135Cs, conclusive evidence for which is yet to be reported. Four Allende (CV3) Ca,Al-rich inclusions (CAI 1, CAI 2, CAI 4, CAI 5) and one Allende dark inclusion (DI) were analyzed for Ba isotope variability. Two CAIs (CAI 2 and CAI 5) display 135Ba excesses that are not accompanied by 137Ba anomalies. Calcium–aluminum-rich inclusion 1 displays a 135Ba excess that is possibly coupled with a 137Ba excess, and the remaining refractory inclusions (CAI 2 and DI) have terrestrial Ba isotope compositions. These Ba isotope data are presented in conjunction with published whole rock Ba isotope data from individual Allende CAIs. The enrichment in 135Ba and absence of coupled 137Ba excesses in CAI 2 and CAI 5 is interpreted to indicate that the anomalies are not purely nucleosynthetic in origin but also contain contributions (16–48 ppm) from the decay of short-lived 135Cs. The majority of Allende CAIs studied to date may also have similar contributions from 135Cs on the basis of higher than expected 135Ba excesses if the Ba isotope anomalies were purely nucleosynthetic in origin. The 135Ba anomalies appear not to be coupled with superchondritic Cs/Ba, which may imply that the contribution to 135Ba did not occur via in situ decay of live 135Cs. However, it is feasible that the CAIs had a superchondritic Cs/Ba during decay of 135Cs, but Cs was subsequently removed from the system during aqueous alteration on the parent body. An alternative scenario is the potential existence of a transient high-temperature reservoir having superchondritic Cs/Ba in the early Solar System while 135Cs was extant, which enabled a radiogenic 135Ba signature to develop in some early condensates. The nucleosynthetic source of 135Cs can be determined by reconciling the predicted astrophysical 135Cs abundance with its measured abundance in meteorites. Further, the currently accepted initial 135Cs/133Cs of the Solar System, [135Cs/133Cs]0, may be underestimated because the spread of Cs/Ba among samples is small and the range of excess 135Ba is limited thus leading to inaccuracies when estimating [135Cs/133Cs]0. If the initial meteoritic abundance of 135Cs was indeed higher than is currently thought, the most probable stellar source of short-lived radioisotopes was a nearby core-collapse supernova and/or the Wolf–Rayet wind driven by its progenitor.

(Table 2) B/Ca, d11B, Mg/Ca and d18O record for ODP Hole 130-806B samples

We present the first continuous records from 0 to 5 Ma (in 0.333 m.y. integrated time steps) of paired boron/calcium (B/Ca) ratios and boron isotopes (d11B) in the planktonic foraminifera Globogerinoides sacculifer (without sacc) from a site in the western equatorial Pacific Ocean (Ocean Drilling Program Site 806). These measurements, the first made in conjunction with calcification temperature (magnesium/calcium ratios) and average shell mass measurements, indicate that pH is not the sole environmental variable controlling B in planktonic foraminiferal calcite. Our data are consistent with calcification temperature exerting a primary control on B concentration and isotopic composition in planktonic foraminifera. If so, calcification temperature must be taken into account if pH for past oceans and atmospheric pCO2 are to be estimated from B isotope measurements in foraminiferal calcite. Doing so will substantially increase the uncertainty of pH estimates. Although this work was designed as a temporal study, its results define new aspects of calibrating the d11B paleo-pH tracer.

Boron isotopes, pH and pCO2 calculation for one Fiji coral specimen Porites (1898-1998), 2012

delta11B results and deduced pH, pCO2 and omega values obtained for a tropical coral specimen Porites collected in 1998 at Yasawa (16°48'S- 177°27'E) on the western side of the Fiji archipelago, location in the north western part of the Pacific Warm Pool. Such Porites specimen grew during the XXth century (1898-1998). Boron isotopes results allowed the reconstruction of surface ocean acidification in the vincinity of Fiji Islands with strong interdecadal influence of the ENSO at regional scale. pHT calculation parameters (Hönisch et al., 2007): a=0 PER MIL; alpha=0.9804; delta11B=39.5 PER MIL; salinity=35.02; pKB from Dickson (1990). pCO2 and omega calculation parameters: TA= 2350 µM; Ca= 10.2 mM; Dickson et al.(2007); Mucci 1983.

Element contents, sulfur and oxygen isotopes, and molecular biomarkers of phosphatic crust samples from the Chimbote Platform of the shelf off Peru

Authigenic phosphatic laminites enclosed in phosphorite crusts from the shelf off Peru (10°01' S and 10°24' S) consist of carbonate fluorapatite layers, which contain abundant sulfide minerals including pyrite (FeS2) and sphalerite (ZnS). Low d34Spyrite values (average -28.8 per mill) agree with bacterial sulfate reduction and subsequent pyrite formation. Stable sulfur isotopic compositions of sulfate bound in carbonate fluorapatite are lower than that of sulfate from ambient sea water, suggesting bacterial reoxidation of sulfide by sulfide-oxidizing bacteria. The release of phosphorus and subsequent formation of the autochthonous phosphatic laminites are apparently caused by the activity of sulfate-reducing bacteria and associated sulfide-oxidizing bacteria. Following an extraction-phosphorite dissolution-extraction procedure, molecular fossils of sulfate-reducing bacteria (mono-O-alkyl glycerol ethers, di-O-alkyl glycerol ethers, as well as the short-chain branched fatty acids i/ai-C15:0, i/ai-C17:0 and 10MeC16:0) are found to be among the most abundant compounds. The fact that these molecular fossils of sulfate-reducing bacteria are distinctly more abundant after dissolution of the phosphatic laminite reveals that the lipids are tightly bound to the mineral lattice of carbonate fluorapatite. Moreover, compared with the autochthonous laminite, molecular fossils of sulfate-reducing bacteria are: (1) significantly less abundant and (2) not as tightly bound to the mineral lattice in the other, allochthonous facies of the Peruvian crusts consisting of phosphatic coated grains. These observations confirm the importance of sulfate-reducing bacteria in the formation of the phosphatic laminite. Model calculations highlight that organic matter degradation by sulfate-reducing bacteria has the potential to liberate sufficient phosphorus for phosphogenesis.