Made available in DSpace on 2015-03-13T17:08:28Z (GMT). No. of bitstreams: 1 MiriamTSM_DISSERT.pdf: 746109 bytes, checksum: 9993efc70026d11b86a511c7cf5aa9bc (MD5) Previous issue date: 2007-05-04 / Nd ISOTOPES IN THE PROVENANCE OF TERRIGENOUS AND CARBONATE ROCKS AND SEDIMENTS OF THE POTIGUAR BASIN, NORTHEASTERN BRAZIL. Mesozoic and Cenozoic rocks from the Potiguar Basin, including terrigenous and carbonate sediments have been investigated to identify their isotopic signature and source areas. Additionally, this study aims to determine the provenance of terrigenous and carbonate sediments on the Brazilian Continental shelf adjacent to Potiguar Basin. The Sm-Nd isotopic signatures of the rocks yielded model ages (TDM) in the range of 2,19- 2,88 Ga, indicating archean to paleoproterozoic sources from the basement. The terrigenous sediments yielded model ages (TDM) in the range of 2,31-2,26 Ga, from 17,5 to 0 cm depth. Despite the small number of samples, limited variations of provenance ages indicates the homogenization of the sediments, probably due to the strong influence of the basement, as the main source of sediments to the shelf. The Sm-Nd isotopic signatures of the carbonate sediments yielded model ages (TDM) in the range of 2,09-2,61 Ga, indicating archean to paleoproterozoic sources from the basement. The results also indicate that the shelf sediments are mainly derived from the A?u River or other small rivers from the Setentrional Sector of Rio Grande do Norte State. The littoral drift doesn?t seem to contribute with sediments from the Oriental Sector since isotopic signatures from this sector were not detected. / An?lises isot?picas Sm-Nd em rochas mesoz?icas e cenoz?icas da Bacia Potiguar, incluindo sedimentos terr?genos e carbon?ticos que aportam do Rio Piranhas-A?u, foram realizadas objetivando a caracteriza??o de suas assinaturas isot?picas e identifica??o de suas ?reas fonte. As assinaturas isot?picas Sm-Nd das rochas apresentaram idades modelo (TDM) variando de 2,88 a 2,19 Ga, indicando fontes, principalmente, paleoproteroz?icas e arquenas do embasamento. Os sedimentos terr?genos plataformais apresentaram idades modelo (TDM) de 2,31 Ga e 2,26 Ga, coletados, respectivamente, nas profundidades de 10-17,5 cm e 0-5 cm. Apesar do n?mero pequeno de amostras, a pequena varia??o na idade indica homogeneiza??o dos sedimentos, talvez devido a forte influ?ncia do embasamento como fonte de material para a plataforma. As assinaturas isot?picas Sm-Nd dos sedimentos carbon?ticos plataformais apresentaram idades modelo (TDM) variando de 2,61 a 2,09 Ga, indicando fontes do embasamento arqueano a paleoproteroz?ico. Estes resultados indicam ainda que os sedimentos terr?genos presentes na plataforma em estudo s?o ou foram trazidos principalmente pelo rio A?u, ou outros rios menores da por??o setentrional do Rio Grande do Norte. A deriva litor?nea aparentemente n?o tem compet?ncia para arrastar sedimentos da por??o oriental para a setentrional, tendo em vista que os valores ?Nd registrados n?o s?o compat?veis com as rochas da por??o oriental.

The Arabian–Nubian Shield (ANS) represents a major site of juvenile Neoproterozoic crustal addition on Earth and documents Neoproterozoic tectonics bracketed by two supercontinent cycles, namely the fragmentation of Rodinia and the amalgamation of Gondwana. There is general consensus that the ANS formed by juvenile magmatic arc accretion and subsequent shield–wide post–tectonic magmatism. However, detailed understanding about the timing of events and the nature of magma sources in parts of the shield are lacking. To date, there are no isotopic data from the Paleozoic sedimentary sequences of the ANS, except those from the northern part. New zircon U–Pb, δ18O and whole–rock Nd isotopes are presented for plutonic rocks from the eastern Ethiopia, Yemen and southernmost Arabian Shield in Saudi Arabia. This thesis also presents the first combined in situ zircon U–Pb–O–Hf isotope data on the Cambrian–Ordovician sandstones of the Arabian Shield. The results are used to elucidate the crustal evolution of these parts of the ANS and to evaluate terrane correlations. Specifically, the nature of crustal growth, i.e., relative proportions of juvenile magmatic additions vs. crustal reworking, nature of the magma source and mechanism of crust formation (plume material vs. subduction zone enrichment) and understanding the provenance of the Cambrian–Ordovician sandstone sequences were important research questions addressed. The results from Paper I suggest that the eastern Ethiopian Precambrian basement is dominated by reworking of pre-Neoproterozoic supracrustal material unlike contemporaneous rocks in the remaining parts of Ethiopia— indicating the presence of two distinct lithospheric blocks of contrasting isotopic compositions in Ethiopia. Metamorphic age distributions suggest that the eastern Ethiopian block was amalgamated with the juvenile Western Ethiopian Shield during ca. 580–550 Ma. Importantly, the suture between them may represent the northern continuation of a major suture identified further south in Africa along which Gondwana amalgamated. Similarly, the Abas terrane in Yemen (Paper II) is dominated by reworking of pre–Neoproterozoic crust and shows age and isotopic compositions that are inconsistent with the Afif terrane of Saudi Arabia, precluding correlation between the two regions. The trace element systematics of plutonic rocks from the southernmost Arabian Shield (paper III) point to enrichment due to subduction component, bear no evidence of a plume component, and are consistent with the adakite-like chemistry of some of the subduction–related plutonic samples. This reinforces the notion that the shield grew through juvenile magmatic arc additions. The combined zircon U–Pb–O–Hf data of the Cambrian–Ordovician sandstones (Paper IV) indicate their derivation from both the adjacent juvenile ANS and the more southerly crustal blocks that are dominated by reworking of pre–Neoproterozoic crust. The remarkable similarity in age spectra and homogeneity of Cambrian sandstones deposited across the northern margin of Gondwana point to continental–scale sediment mixing and dispersal regulated by the supercontinent cycle. / <p>At the time of the doctoral defense, the following papers were unpublished and had a status as follows: Paper 3: Manuscript. Paper 4: Manuscript.</p>

Rare earth elements (REEs) and their isotopes (such as Nd isotopes) can be potentially used to trace a wide range of oceanic processes in both modern and ancient oceans, but their successful application as tracers requires a comprehensive understanding of REE cycling in the modern ocean. Previous studies of REEs in seawater were largely constrained by analytical difficulties in generating accurate and precise REE data from seawater, which typically contain REE concentrations at a sub-ppt to ppt level. A new, and relatively simple, analytical method for precise and accurate determination of all dissolved REE concentrations in reasonably small (&Tilde;100 ml) seawater samples is presented in this thesis. With the application of the new method, this thesis reports the first full-depth, zonal ocean section of all dissolved REE concentrations, collected during the CoFeMUG cruise along &Tilde;12&deg;S in the South Atlantic. The section approach of this study places the distribution of dissolved REE concentrations in a well-constrained hydrographic context, allowing the first quantitative assessment (by an inverse model) of the relative importance of hydrographic controls resulting from advection/mixing of ocean circulation, together with non-conservative controls resulting from local particle scavenging and remineralization, in controlling the distribution of dissolved REEs in this region. A noteworthy decoupling of Ce and Mn with respect to their cycling in the water column was also observed in this study. The application of Nd isotopes as a tracer to reconstruct changes in ocean circulation in the NW European chalk shelf sea during rapid climatic events, including the mid-Cenomanian Event and oceanic anoxic event 2 (OAE 2), suggests a tight coupling between ocean circulation and transient climatic cooling during the general warm Late Cretaceous. An advected volcanic signal during OAE 2 was registered in the seawater Nd-isotope record from the English Chalk, probably suggesting a period of enhanced ocean ventilation/mixing at this time.

Les poussières atmosphériques naturelles jouent un rôle complexe dans le système climatique global étant à la fois un facteur affectant le climat et variant en fonction de ce dernier. Notre compréhension des différentes interactions entre les poussières atmosphériques et le climat est limitée par l’importante variabilité spatiale et temporelle des celles-ci. À l’aide de tourbières ombrotrophes, la variabilité spatiale et temporelle des dépôts de poussières atmosphériques holocènes au Québec boréal fut caractérisée en lien avec les fluctuations climatiques. Les flux de poussières atmosphériques furent reconstruits à l’aide des concentrations en terres rares. Les isotopes du Nd et Pb en combinaison avec les terres rares ont été utilisés afin de déterminer la source des particules déposées dans les tourbières. Afin d’évaluer les liens entre les flux de poussières et la variabilité climatique, les changements temporels dans les flux de poussières et l’isotopie du Nd furent comparés à la taille des particules déposée et des reconstitutions écohydrologiques basées sur l’analyse des macrorestes végétaux et des thécamoebiens. Dans les deux premiers volets de l’étude, les flux de poussières atmosphériques furent reconstruits dans deux tourbières de la Côte-Nord alors que les particules déposées dans celles-ci furent caractérisées à l’aide des concentrations des terres rares (REE), des isotopes du néodyme et du plomb ainsi que la granulométrie. Les deux profils présentent des valeurs de Nd similaires, ce qui s’explique soit par une source commune des poussières atmosphériques ou encore des sources distinctes, mais possédant des valeurs de Nd similaires dans les deux régions. Les deux sites étudiés montrent des tendances différentes dans les flux de poussières. La tourbière IDH montre peu de variations dans les flux de poussières, ce qui s’explique en partie par l’emplacement du site d’étude, qui prévient les apports de poussières atmosphérique. La tourbière Baie quant à elle, montre deux périodes de flux de poussières plus élevés soit 1700-1000 et 650-100 cal a BP correspondant avec des périodes de refroidissement du climat documentées. Les REE, le Nd et les tailles de particules suggèrent qu’au cours des 2000 dernières années, la tourbières de Baie a reçu une proportion accrue de poussières atmosphériques provenant de sources locales. Ces deux périodes ont été identifiées comme des épisodes d’instabilité climatique en réponse à une instabilité hydroclimatique régionale et une plus grande variabilité des températures (principalement contrôlée par l’activité solaire). Un changement du régime des vents dans la région a aussi probablement influencé ces les variations observées. Dans le troisième chapitre, les mêmes analyses furent réalisées sur des carottes de tourbe d’une tourbières de la Baie James, La Grande 2 (LG2). Des apports accrus de poussières furent observés lors de différentes période : 4000 à 3000, 2600 à 2000, 1600 à 1000, 800 à 650 cal a BP et de 1960 à 1990AD. Au moins trois sources distinctes constituent les apports de poussières dans le temps: les sédiments marins à la base de la tourbières, la moraine de Sakami, deux sources locales, ainsi qu’une source probablement plus régionale dont l’origine est non-identifiée. La période allant de 7000 à 4100 cal a BP montre des valeurs près des sources locales (Nd : -36 à -29). Une augmentation graduelle des valeurs de Nd à partir de 4100 cal a BP suggère une diminution des apports locaux de poussière à la faveur d’une source non identifiée. La majorité des périodes d’apports accrus de poussières identifiées correspondent à des périodes documentées comme étant froides et sèches probablement lié à des intrusions de masses d’air arctiques. La présence de certains de ces pics de poussières lors de minimums solaires suggère que la variabilité solaire joue aussi un rôle dans la variabilité climatique de la région. / Mineral dust plays an important role in the global climate system having effects on the radiation budget and the chemical composition of the atmosphere. Our understanding of the exact role of dust in the Earth’s climate system is still poorly constrained mostly due to a lack of data reflecting the high spatial and temporal variability of dust. Using peat bogs, spatial and temporal variability of Holocene dust deposition in boreal Quebec was investigated in relation to climate fluctuations. Dust fluxes were reconstructed using rare earth elements (REE) concentrations in bulk peat, while Nd and Pb isotopes in combination with REE were used to identify the source of dust particles deposited into these bogs. In order to evaluate the relationship between dust fluxes and climate variability, temporal changes in dust flux, and Nd isotopes were compared to dust grain size and ecohydrological reconstructions derived from testate amoebae and plant macrofossils. In two peat bogs from the North Shore region of the St. Lawrence Estuary (Baie bog) and Gulf (IDH bog), atmospheric dust fluxes were reconstructed using REE concentration while the geochemical composition of deposited dust was characterized using Nd and Pb isotopes combined with REE and grain size. Both peat bogs present similar Nd values, which suggests either a common source or sources with similar signatures in both regions. In terms of dust flux, the two study sites display distinct tendencies. IDH bog show few variations in dust flux, which can be explained by its geographical setting, where a tree fringe and higher altitude likely partially prevent dust from reaching the peat bog. Two dust events were recorded in the Baie bog from 1750 to 1000 cal BP and 600 to 100 cal BP and correspond to documented cold periods. These two periods have been found to occur at the same time as periods of high variability in the macrofossil record (i.e. successive layers dominated by Sphagnum or Ericaceae). REE elements, Nd and grain-size distribution suggest that, over the last 2000 years, the Baie bog received more local dust. The two periods were identified as periods of increased local storminess in response to regional hydroclimatic instability and temperature variations mainly controlled by solar activity. These episodes of climatic instability could also have been caused by changes in the wind regime. The same set of analyses were performed in a third peatland located in the James Bay region, the La Grande 2 bog (LG2). Increases in dust flux were reconstructed from 4000-3000, 2600-2000, 1600-1000, 800-650 cal BP and from 1960-1990AD. The Nd values show a large variability from -37 to -12, identifying a least three sources: local marine sediment, the Sakami moraine and another unidentified source likely from a more regional origin. Between 7000 and 4100 cal BP, Nd values resemble those localsources (-36 to -29). A gradual increase in Nd signature is observed from 4100 to 1500 cal BP suggesting a decreasing influence of local sources in favor of a yet unidentified source. The occurrence of increased dust deposition during cold periods in two of the three studied bogs suggests that dust fluxes can be used as an indicator of cold and dry climatic conditions in boreal Quebec. In northeastern Canada, these cold and dry conditions are usually the results of the intrusion of Arctic air masses. The exact mechanism controlling these incursion is yet unknown, but the similar timing of solar minima and dust peaks suggest that solar irradiance may also have played a role. The fact that both Baie and LG2 sites display similar tendencies during the last 2000 years reveals that both regions were likely controlled by the same climatic processes.

Global climate is controlled by two factors, the amount of heat energy received from the sun (solar insolation) and the way that heat is distributed Earth's surface. Solar insolation varies on timescales of 10s to 100s of thousands of years due to changes in the path of Earth's orbit about the sun (Milankovitch cycles). Earth's internal boundary conditions, such as paleogeography, the presence/absence of polar icecaps, atmospheric/oceanic chemistry and sea level, provide distribution and feedback mechanisms for the incoming heat. Variations in these internal boundary conditions may happen abruptly or, as in the case of plate tectonics, take millions of years. We use geochemical and sedimentological techniques to investigate the response of ocean chemistry, regional aridity and atmospheric and oceanic circulation patterns to climate change during both greenhouse and icehouse climates. To explore the connection between orbitally-forced changes in solar insolation, continental aridity and wind, we generated a high-resolution dust record for ~58 Myr old deep-sea sediments from Shatsky Rise. Our data provide the first evidence of a correlation between dust flux to the deep sea and orbital cycles during the Early Paleogene, indicating dust supply (regional aridity) responded to orbital forcing during the last major interval of greenhouse climate. The change in dust flux was comparable to that during icehouse climates implying subtle variations in solar insolation have a similar impact on climate during intervals of over-all warmth as they do during glacial-interglacial states. The Carboniferous Period (359-299 Ma) marks a critical time in Earth's history when a series of tectonic and biological events caused a shift in the mean climate state from a global "greenhouse" to an "icehouse". Geochemical records extracted from sedimentary rocks deposited in shallow epicontinental seaways are increasingly being used to infer relationships between tectonism, carbon cycling and climate and therefore are assumed to reflect global ocean processes. We analyzed radiogenic isotopes in biogenic apatite along a North American transect to constrain the degree of geochemical coupling between the epicontinental seas and the open ocean. Our results argue strongly for decoupling of North American seaways from the open ocean by latest Mississippian time.