Feedbacks between climate, tectonics and erosion drive mineral dissolution in the subsurface and may provide strong controls on chemical weathering as a mechanism for modulating climate through CO2 drawdown. However, few quantitative evaluations of chemical weathering intensity or flux variations with time exist to support this hypothesized feedback. Trace element concentrations in colluvial sediment demonstrate that in unglaciated mid-latitude terrain, climate exerts a strong control on chemical weathering intensity and erosion over glacial-interglacial cycles by modulating the efficacy of abiotic and biotic processes. Weakly chemically altered sediment corresponds with high erosion rates during the Last Glacial interval (vice versa during the Holocene) such that we observe stable weathering rates despite variations in temperature and vegetation. Our results suggest that climate-weathering feedbacks in mid-latitude regions may be weaker than previously hypothesized and provide a new framework to explain stable solute fluxes over Milankovitch climate fluctuations. / 10000-01-01

Les modalités d’évolution d’une côte rocheuse granitique en contexte de marge passive restent encore mal connues à ce jour, du fait de leur évolution lente. L’objectif de l’étude du littoral granitique du sud-Finistère vise à mieux comprendre son développement et sa dynamique érosive sur une échelle de temps variant entre le Cénozoïque et le Quaternaire. Une cartographie Terre-Mer de détail a permis d’identifier plusieurs objets morphologiques : une rasa (≈15m), une terrasse marine (≈7m), une plateforme littorale (0-5m) et une plateforme rocheuse sous-marine (-70 à 0m). Ces objets témoignent de la variabilité spatiale et temporelle des processus tectoniques vs. eustatiques sur le littoral breton. L’architecture 3D de la zone révèle une plateforme rocheuse sous-marine très fracturée avec de grands accidents délimitant plusieurs micro-blocs et fonctionnant au Cénozoïque (compression pyrénéenne éocène, puis ouverture Atlantique Oligocène et extension au post-Oligocène avec l’ouverture continentale des grabens du Rhin). La Pointe SO de la zone d’étude se stabilise durant le tardi-Cénozoïque, révélant que les figures d’érosion aériennes (rasa et terrasse marine) ont été générées lors de plusieurs paléo-haut niveau marin. Les larges surfaces des objets terrestres s’expliquent par l’action combinée des purges eustatiques sur un matériel granitique très altéré. Il a été démontré que la morphologie de la zone littorale granitique a été façonnée a minima par deux épisodes de purges eustatiques durant le MIS 5 (120ka) et l’Holocène (10ka). Les taux d'érosions verticaux obtenus pour la terrasse marine et la plateforme littorale varient entre 3.35 ±0.32 m.Ma-1 et 6.20 ± 0.80 m.Ma-1. / The granitic rocky coast evolution, in passive margin context, is still not completely understood as its evolution is lower. The aim of the South-Finistère shore zone studying is to better understand its development and erosive dynamic on a time scale ranging between Cenozoic and Quaternary. A detailed onshore/offshore mapping has been realized, highlighting several erosional features. From land seaward, a rasa (≈15m-high), a marine terrace (≈7m-high), a shore platform (0-5 m-high) and a rocky marine platform (-70 à 0m) have been emphasized. These objects evidence temporal variations in the response of the tectonic or eustatic processes. The 3D architecture of rocky marine platform demonstrates a highly fractured domain with major faults bounding several micro-blocks, reactivated between the Eocene (Pyrenean compression) and Late / Post-Oligocene (Rhine continental transform zone activation). The quantitative geomorphology applied on the western part of studying zone reveals none late-Cenozoic uplift. Consequently, the rasa and marine terrace have been shaped during a high paleo-sea level. The granitic surface’s erosion produces horizontal joint planes, as a result of weathering processes. The combination between planar and horizontal granitic jointing and the marine eustatic purge explains the large width of granitic eroded surfaces.Two eustatic purges (MIS 5 and Holocene) have been shaped the granitic shore zone and the vertical erosion, rate obtained for various lateritic horizon in onshore and shore domains, is ranging between 3.35 ±0.32 m.Ma-1 and 6.20 ± 0.80 m.Ma-1.

Le flux de météorites vers la Terre peut être déterminé en observant des bolides, ou en étudiant des collections de météorites. Pour estimer l’intensité et la composition du flux, nous avons collecté et classifié une collection de 213 météorites issues du désert de l’Atacama (Chili). Nous avons développé un protocole chimique afin d’extraire des nucléides cosmogéniques de chondrites ordinaires. La fraction métallique est d’abord séparée de la météorite. Les échantillons sont ensuite dissouts dans l’acide, et les éléments utiles sont extraits et purifiés grâce à des résines échangeuses d’ions et des précipitations contrôlées. Après la mesure par SMA, les concentrations de nucléides cosmogéniques nous permettent de calculer l’âge terrestre, le rayon pré-atmosphérique et la profondeur dans le météoroide, en utilisant l'approche développée par Leya & Masarik (2009). En combinant le nombre de météorites par unité de surface et les spectres d’âge terrestre, nous pouvons déterminer un flux de 218 météorites>10g/Ma/km2 sur une période de 700 ka avec la méthode 41Ca.Dans le cadre d’une collaboration avec l’Université de Bern (Suisse), nous avons aussi mesuré les concentrations en gaz rares dans certaines de ces météorites. Les concentrations en gaz rares et en nucléides radiogéniques ont ensuite été étudiées avec le modèle développé par Ammon et al. (2009), afin de déterminer le temps d’exposition dans l’espace, l’âge terrestre, le rayon pré-atmosphérique et la profondeur dans le météoroide. / Meteorite flux to the Earth can be determined using observations of fireballs or studying meteorites collections. To estimate the intensity and the composition of the flux, we collected and classified a 213 samples collection from the Atacama desert (Chile). We developed a mathematical model to help pairing of meteorites, and hence get a reliable number of falls per unit of surface. A chemical procedure to extract the cosmogenic nuclides 10Be, 26Al, 36Cl and 41Ca from ordinary chondrites was developed. The metallic fraction was extracted from the bulk meteorite. Samples were dissolved into acid and the elements of interest were extracted and purified using ion-exchange resins and pH controlled precipitation. After measurements using the Accelerator Mass Spectrometry (AMS) technique, the cosmogenic nuclides concentrations enable us to calculate terrestrial age, pre-atmospheric radius and shielding depth, using the Leya & Masarik (2009) model. Combining the number of meteorites per km2 and the terrestrial ages spectrum, we determine a flux of 218 meteorites > 10g/Ma/km2 over 700 ka with the 41Ca calculation method. Applying the same procedure as described above, we studied a selection of iron meteorites in which noble gases (He, Ne and Ar isotopes) concentrations were measured in collaboration with the University of Bern (Switzerland). Stable and radiogenic nuclides concentration results were then used according to the Ammon et al. (2009) model to determine Cosmic Ray Exposure (CRE) ages, terrestrial ages, pre-atmospheric radii and shielding depths.

Indiana University-Purdue University Indianapolis (IUPUI) / Subglacial chemical processes in Antarctica are potentially significant contributors to global geochemical cycles, but current understanding of their scale and nature is limited. A sequential chemical extraction procedure was developed and tested to investigate the utility of meteoric 10Be as a tracer for chemical weathering processes beneath the East Antarctic Ice Sheet. Subglacial meltwater is widely available under the Antarctic Ice Sheet and chemical constituents within it have the potential to drive geochemical weathering processes in the subglacial environment. Meteoric 10Be is a cosmogenic nuclide with a half-life of 1.39×106 years that is incorporated into glacier ice, therefore its abundance in the subglacial environment in Antarctica is meltwater dependent. It is known to adsorb to fine-grained particles in aqueous solution, precipitate with amorphous oxides, and/or be incorporated into authigenic clay structures during chemical weathering. The presence of 10Be in weathering products derived from beneath the ice therefore indicates chemical weathering processes in the subglacial environment. Freshly emerging subglacial sediments from the Mt. Achernar blue ice moraine were subject to chemical extractions where these weathering phases were isolated and 10Be concentrations therein quantified. Optimization of the phase isolation was developed by examining the effects of each extraction on the sample mineralogy and chemical composition. Experiments on 10Be desorption revealed that pH 3.2-3.5 was optimal for the extraction of adsorbed 10Be. Vigorous disaggregation of the samples before grain size separations and acid extractions is crucial due to the preferential fractionation of the nuclide with clay-sized particles. 10Be concentrations of 2-22×107 atoms g-1 measured in oxides and clay minerals in freshly emerging sediments strongly indicate subglacial chemical weathering in the catchment of the Mt. Achernar moraine. Sediment-meltwater contact in the system was calculated to be on the order of thousands of years, based on total 10Be sample concentrations, local basal melt rates, and 10Be ice concentrations. Strong correlation (R = 0.96) between 10Be and smectite abundance in the sediments indicate authigenic clay formation in the subglacial environment. This study shows that meteoric 10Be is a useful tool to characterize subglacial geochemical weathering processes under the Antarctic Ice Sheet.

No description available.

<p>Chemical weathering of highly reactive mafic and ultramafic igneous rocks may be a key sink in the global carbon cycle. Understanding how uplift of these rocks during arc-arc and arc-continent collisions through earth history has affected the evolution of global climate, including the onset of icehouse periods, requires improved constraints on the relative sensitivity of their weathering rates to physical erosion vs. climate. If weathering rates depend chiefly on erosion, then tectonic uplift of mafic and ultramafic rocks may have a strongly destabilizing effect on global climate. Conversely, if weathering rates are limited primarily by temperature or runoff, then a negative feedback mechanism between weathering and climate may attenuate the effects of rock uplift. This work characterizes the relationship between chemical weathering rates, physical erosion rates, and climate in tropical, montane watersheds in Puerto Rico that are underlain by volcanic arc rocks and associated ophiolitic serpentinite. Key to this analysis are new constraints on long-term erosion rates on these rocks from cosmogenic Cl-36 produced <em>in situ</em> in magnetite. These cosmogenic erosion rates are paired with classical measurements of stream solute fluxes and sediment geochemistry across runoff gradients to quantify the limits to volcanic arc rock and serpentinite weathering rates. </p> <p><br></p> <p>This work is divided into three chapters. Chapter 2 constrains the altitude scaling behavior of Cl-36 production in magnetite. This allows erosion rates to be determined more accurately in watersheds near sea level in Puerto Rico. Chapter 3 demonstrates that volcanic arc rock weathering rates in the humid tropics are more strongly limited by physical erosion than by climatic factors. However, a positive correlation between erosion and runoff observed in this landscape may enhance the coupling between climate and weathering rates. Chapter 4 finds that, in contrast to volcanic arc rocks, serpentinite weathering is strongly limited by runoff and weakly limited by erosion. These results are presented as empirical power-law relationships that can be readily applied in global carbon cycle modeling.  </p>

No description available.

No description available.

No description available.

Rising sea levels present an ongoing threat to communities and resources around the Chesapeake Bay, east coast, USA, where tide gauges indicate that the relative rise of sea level is approximately twice the rate of average, eustatic sea-level rise. This has significantly compromised the health and viability of salt marsh habitat on the Eastern Shore during the 20th century, and the biologists who are charged with managing coastal resources in the coming decades need to understand the nature and causes of high rates of regional sea-level rise to develop suitable adaptation plans. Dated geologic deposits and geophysical models suggest that sea-level rise is relatively high on mid-Atlantic coastlines because the land surface is subsiding due to a collapsing glacial forebulge following the Last Glacial Maximum (LGM). To fully understand this process, past sea-level indicators such as dated shoreline deposits are needed to reconstruct regional sea-level behavior in the past, but rigorous age control on geologic deposits is largely restricted to the Holocene and to marine isotope stage (MIS) 5, so the rates and timescales over which these processes operate remain unknown. This research provides long-term paleoenvironmental records from ancient environments under east-central Chesapeake Bay to place the current sea-level threats into the context of a long geologic history of sea-level fluctuations. First, the Pleistocene geologic framework of the region is reconstructed through borehole drilling. Sediments from boreholes provided material for interpreting depositional environments, and for establishing age control for deposits, so that the entire stratigraphy was constrained both in space and time. The geologic framework and ages indicate that Chesapeake Bay alternated between a deeply incised fluvial system and a filled estuary repeatedly in response to major climate fluctuations since at least the early Pleistocene, ~2 Ma. The ages and sedimentology indicate that the field area was submerged intermittently in a shallow estuary until nearly the end of marine isotope stage 3. Because global sea-level proxies suggest that sea level was ~40-80 meters lower than present at that time, these ages suggest that the penultimate glacial forebulge must have remained significantly lowered for nearly 100 ky following the retreat of ice. The implication of this time lag is that mid-Atlantic coastlines are still in a relatively early state of forebulge collapse, and subsidence following retreat of ice from the Last Glacial Maximum will likely continue for the foreseeable future. Ongoing subsidence will continue to exacerbate projected eustatic sea-level rise due to changing global climate, and coastal adaptation plans must remain focused on encouraging the migration of vital habitat toward higher elevations in the landscape.