Weathering of Fe-bearing minerals under extraterrestrial conditions, investigated by Mössbauer spectroscopy

The weathering of Fe-bearing minerals under extraterrestrial conditions was investigated by Mössbauer (MB) spectroscopy to gain insights into the role of water on the planet Mars. The NASA Mars Exploration Rovers Spirit and Opportunity each carry a miniaturized Mössbauer spectrometer MIMOS II for the in situ investigation of Martian soils and rocks as part of their payload. The MER flight instruments had to be modified in order to work over the Martian diurnal temperature range (180 K – 290 K) and within the unique electronic environment of the rovers. The modification required special calibration procedures. The integration time necessary to obtain a good quality Mössbauer spectrum with the MIMOS II flight instruments was reduced by 30 % through the design of a new collimator. The in situ investigation of rocks along the rover Spirit's traverse in Gusev crater revealed weakly altered olivine basalt on the plains and pervasively altered basalt in the Columbia Hills. Correlation plots of primary Fe-bearing minerals identified by MB spectroscopy such as olivine versus secondary Fe-bearing phases such as nanophase Fe oxides showed that olivine is the mineral which is primarily involved in weathering reactions. This argues for a reduced availability of water. Identification of the Fe-oxyhydroxide goethite in the Columbia Hills is unequivocal evidence for aqueous weathering processes in the Columbia Hills. Experiments in which mineral powders were exposed to components of the Martian atmosphere showed that interaction with the atmosphere alone, in the absence of liquid water, is sufficient to oxidize Martian surface materials. The fine-grained dust suspended in the Martian atmosphere may have been altered solely by gas-solid reactions. Fresh and altered specimens of Martian meteorites were investigated with MIMOS II. The study of Martian meteorites in the lab helped to identify in Bounce Rock the first rock on Mars which is similar in composition to basaltic shergottites, a subgroup of the Martian meteorites. The field of astrobiology includes the study of the origin, evolution and distribution of life in the universe. Water is a prerequisite for life. The MER Mössbauer spectrometers identified aqueous minerals such as jarosite and goethite. The identification of jarosite was crucial to evaluate the habitability of Opportunity's landing site at Meridiani Planum during the formation of the sedimentary outcrop rocks, because jarosite puts strong constrains on pH levels. The identification of olivine in rocks and soils on the Gusev crater plains provide evidence for the sparsity of water under current conditions on Mars. Ratios of Fe2+/Fe3+ were obtained with Mössbauer spectroscopy from basaltic glass samples which were exposed at a deep sea hydrothermal vent. The ratios were used as a measure of potential energy for use by a microbial community. Samples from Mars analogue field sites on Earth exhibiting morphological biosignatures were also investigated.

Petrographie und Geochemie des Eckfelder Maares und von Hillscheid und die Einbindung in den Hocheifelvulkanismus

Tertiäre Vulkanite aus dem Eckfelder Maar, dem Hillscheider Diatrem und dem Hillscheid Basalt (Schlot) wurden petrologisch und geochemisch untersucht. Bis auf tonige Klasten aus dem Bohrkern des Eckfelder Maares handelt es sich bei allen weiteren Proben um undifferenzierte basische Vulkanite. Die tonigen Klasten aus dem Bohrkern müssen der ehemaligen Landoberfläche vor der Eruption des Eckfelder Maares zugerechnet werden, in dessen Krater sie während der Eruption hineingefallen sind. Bis auf die Proben des Hillscheid Basaltes sind die Proben alteriert. Die Alteration zeigt sich an der Bildung von Zeolithen und Calcitmineralisationen, die primär und sekundär gebildete Hohlräume aufgefüllt haben oder an einer vertonten Grundmasse der Proben, die daneben Mineraleinschlüsse (Spinell) und kantige Fremdgesteinsbruchstücke enthalten können. Bei den Proben mit vertonter Grundmasse handelt es sich um Palagonite, Umwandlungsprodukte aus Sideromelan (basaltischem Glas). Geochemische Analysen an Grundmassepräparaten der alterierten bis vertonten Proben zeigen, dass außer den immobilen Elementen Ti, Nb, Zr, Y alle weiteren Elemente teilweise bis vollständig abgereichert worden sind. Eine Ausnahme bildet Barium (Ba), welches z.T. in beträchtlichen Mengen in Zeolithen (Harmotom) angereichert wurde. Bei den Proben aus dem Eckfelder Maar kann die Alteration bis Vertonung der Proben alleine mit der Palagonitisierung und Verwitterung erklärt werden. Es gibt keine Hinweise auf Materialzufuhr und damit für sich anschließende hydrothermale Prozesse. Die Proben des Hillscheider Diatrem sind wesentlich geringer alteriert (glasige Grundmasse). Neuste Erkenntnisse aus einer Bohrung im Sommer 1999 im vermuteten Zentrum des Hillscheider Diatrems beschränken das Diatrem maximal auf einen kleineren Bereich im Nordosten der bisherigen Lokation. Bei der Bohrung stieß man nach 20 Meter auf Anstehendes. Im Hangschutt darüber fand man Blöcke des Hillscheid Basaltes. Eine geringere Größe der Lokation zusammen mit der geringen Alteration könnten auf deren Entstehung mit einer initialen Maarphase gefolgt von Schlackentätigkeit hinweisen. Die Schlacken könnten die ersten Ablagerungen vor Verwitterung geschützt haben. Allerdings gibt es keine Funde die eine Schlackentätigkeit belegen. Beim sogenannten 'Hillscheider Diatrem' könnte es sich aber auch um Hangschutt aus der Randbreccie des Hillscheider Basaltes handeln. Zusammen mit Bruchstücken aus dem Schlot des Hillscheid Basaltes wären die Palagonite des sogenannten 'Hillscheider Diatrem' erst in jüngster Zeit im Bereich einer Uferböschung zur Ablagerung gekommen. Dies würde allerdings das sogenannte 'Hillscheider Diatrem' in seiner Existenz in Frage stellen. Vergleiche der Proben des Hillscheid Basaltes mit basischen Hocheifelvulkaniten deuten auf kogenetische Beziehung aller Proben untereinander und ordnen die Proben des Hillscheid Basaltes geochemisch dem Hocheifelvulkanismus zu. REE- und weitere Spurenelementgehalte und auch deren Elementverhältnisse weisen für alle tertiären Eifelvulkanite gemeinsam auf Mantelschmelzen aus dem Bereich eines Granatperidotits mit niedrigen Aufschmelzgraden um ein Prozent hin. Vergleich der Elementverhältnisse hochinkompatibler Elemente im Bezug auf die Bildung mafischer Schmelzen mit primitivem Mantel deuten darauf hin, dass der Mantel im Bereich der Hocheifel verarmt ist an K, Rb, Sr und angereichert an Ba und eventuell an Nb. Ursachen für diese von typisch primären Mantelzusammensetzung abweichenden Verhältnisse könnten durch Mischungen von Mantelschmelzen mit lithosphärischem Mantel (K-Anomalie) und durch Anreicherungen mit fluiden Phasen (Ba-Anomalie) oder auch Schmelzen aus einem tieferliegenden Plume (Kelberger Hoch) verursacht worden sein. Englischer Zusammenfassung:

Quantifizierung von Steinschlagrisiken an Straßen

Thema: Quantifizierung von Steinschlagrisiken an Straßen Die Einschätzung eines bestehenden Steinschlagrisikos an Verkehrswegen ist in Gebirgs- und Mittelgebirgsregionen seit jeher eine Aufgabe, die mit verschiedensten Methoden und unterschiedlichem Aufwand bearbeitet wird. In der vorliegenden Untersuchung werden die maßgebenden Parameter zur Beschreibung einer Böschung aufgenommen und bewertet. Es wurde ein Arbeitsblatt entwickelt, in dem festgelegte Parameter erfasst werden, die teils mit Ankreuztechnik, teils mit der Eingabe von Daten, im Computer notiert werden. Das Arbeitsblatt umfasst vier Themenbereiche: Allgemeine Daten, Angaben zur Geometrie der Böschung, Angaben zum Verkehr und Angaben zum Gestein und Gebirge. Ein Computerprogramm, das auf der Basis der Software Excel von Microsoft erstellt wurde, vergibt nach der Dateneingabe Bewertungspunkte (1. Bewertungsschritt). Es werden Summen gebildet und die Teilbereiche bewertet (2. Bewertungsschritt). Jeder Teilbereich besitzt drei Bewertungsklassen. Die Verknüpfung der Bewertung der Teilbereiche Geometrische Angaben und Angaben zum Gestein und Gebirge stellt die eigentliche Risikoeinschätzung dar (3. Bewertungsschritt). Es gibt drei Einstufungen zur Beschreibung des Risikos: ð Der Verkehr ist durch Steinschlag sehr gering gefährdet. ð Der Verkehr ist durch Steinschlag gering gefährdet. Eine Detailüberprüfung muss erfolgen, da eine Gefährdung nicht auszuschließen ist. ð Der Verkehr ist gefährdet. Es besteht ein hohes Steinschlagrisiko. Bewertungen und Hinweise zu den Teilbereichen Allgemeine Daten und Angaben zum Verkehr kann der Anwender nach eigenem Ermessen zusätzlich nutzen. Die abschließende Risikoeinschätzung erfolgt durch den Anwender bzw. einen Sachverständigen.

The release of zinc and lead from mine tailings

Mining and processing of metal ores are important causes of soil and groundwater contamination in many regions worldwide. Metal contaminations are a serious risk for the environment and human health. The assessment of metal contaminations in the soil is therefore an important task. A common approach to assess the environmental risk emanating from inorganic contaminations to soil and groundwater is the use of batch or column leaching tests. In this regard, the suitability of leaching tests is a controversial issue. In the first part of this work the applicability and comparability of common leaching tests in the scope of groundwater risk assessment of inorganic contamination is reviewed and critically discussed. Soil water sampling methods (the suction cup method and centrifugation) are addressed as an alternative to leaching tests. Reasons for limitations of the comparability of leaching test results are exposed and recommendations are given for the expedient application of leaching tests for groundwater risk assessment. Leaching tests are usually carried out in open contact with the atmosphere disregarding possible changes of redox conditions. This can affect the original metal speciation and distribution, particularly when anoxic samples are investigated. The influence of sample storage on leaching test results of sulfide bearing anoxic material from a former flotation dump is investigated in a long-term study. Since the oxidation of the sulfide-bearing samples leads to a significant overestimation of metal release, a feasible modification for the conduction of common leaching tests for anoxic material is proposed, where oxidation is prevented efficiently. A comparison of leaching test results to soil water analyzes have shown that the modified saturation soil extraction (SSE) is found to be the only of the tested leaching procedures, which can be recommended for the assessment of current soil water concentrations at anoxic sites if direct investigation of the soil water is impossible due to technical reasons. The vertical distribution and speciation of Zn and Pb in the flotation residues as well as metal concentrations in soil water and plants were investigated to evaluate the environmental risk arising from this site due to the release of metals. The variations in pH and inorganic C content show an acidification of the topsoil with pH values down to 5.5 in the soil and a soil water pH of 6 in 1 m depth. This is due to the oxidation of sulfides and depletion in carbonates. In the anoxic subsoil pH conditions are still neutral and soil water collected with suction cups is in equilibrium with carbonate minerals. Results from extended x-ray absorption fine-structure (EXAFS) spectroscopy confirm that Zn is mainly bound in sphalerite in the subsoil and weathering reactions lead to a redistribution of Zn in the topsoil. A loss of 35% Zn and S from the topsoil compared to the parent material with 10 g/kg Zn has been observed. 13% of total Zn in the topsoil can be regarded as mobile or easily mobilizable according to sequential chemical extractions (SCE). Zn concentrations of 10 mg/L were found in the soil water, where pH is acidic. Electron supply and the buffer capacity of the soil were identified as main factors controlling Zn mobility and release to the groundwater. Variable Pb concentrations up to 30 µg/L were observed in the soil water. In contrast to Zn, Pb is enriched in the mobile fraction of the oxidized topsoil by a factor of 2 compared to the subsoil with 2 g/kg Pb. 80% of the cation exchange capacity in the topsoil is occupied by Pb. Therefore, plant uptake and bioavailability are of major concern. If the site is not prevented from proceeding acidification in the future, a significant release of Zn, S, and Pb to the groundwater has to be expected. Results from this study show that the assessment of metal release especially from sulfide bearing anoxic material requires an extensive comprehension of leaching mechanisms on the one hand and on weathering processes, which influence the speciation and the mobility of metals, on the other hand. Processes, which may change redox and pH conditions in the future, have to be addressed to enable sound decisions for soil and groundwater protection and remediation.

Mediterranean-type climate in the South Aegean (Eastern Mediterranean) during the Late Miocene: Evidence from isotope and element proxies

The present-day climate in the Mediterranean region is characterized by mild, wet winters and hot, dry summers. There is contradictory evidence as to whether the present-day conditions (“Mediterranean climate”) already existed in the Late Miocene. This thesis presents seasonally-resolved isotope and element proxy data obtained from Late Miocene reef corals from Crete (Southern Aegean, Eastern Mediterranean) in order to illustrate climate conditions in the Mediterranean region during this time. There was a transition from greenhouse to icehouse conditions without a Greenland ice sheet during the Late Miocene. Since the Greenland ice sheet is predicted to melt fully within the next millennia, Late Miocene climate mechanisms can be considered as useful analogues in evaluating models of Northern Hemispheric climate conditions in the future. So far, high resolution chemical proxy data on Late Miocene environments are limited. In order to enlarge the proxy database for this time span, coral genus Tarbellastraea was evaluated as a new proxy archive, and proved reliable based on consistent oxygen isotope records of Tarbellastraea and the established paleoenvironmental archive of coral genus Porites. In combination with lithostratigraphic data, global 87Sr/86Sr seawater chronostratigraphy was used to constrain the numerical age of the coral sites, assuming the Mediterranean Sea to be equilibrated with global open ocean water. 87Sr/86Sr ratios of Tarbellastraea and Porites from eight stratigraphically different sampling sites were measured by thermal ionization mass spectrometry. The ratios range from 0.708900 to 0.708958 corresponding to ages of 10 to 7 Ma (Tortonian to Early Messinian). Spectral analyses of multi-decadal time-series yield interannual δ18O variability with periods of ~2 and ~5 years, similar to that of modern records, indicating that pressure field systems comparable to those controlling the seasonality of present-day Mediterranean climate existed, at least intermittently, already during the Late Miocene. In addition to sea surface temperature (SST), δ18O composition of coral aragonite is controlled by other parameters such as local seawater composition which as a result of precipitation and evaporation, influences sea surface salinity (SSS). The Sr/Ca ratio is considered to be independent of salinity, and was used, therefore, as an additional proxy to estimate seasonality in SST. Major and trace element concentrations in coral aragonite determined by laser ablation inductively coupled plasma mass spectrometry yield significant variations along a transect perpendicular to coral growth increments, and record varying environmental conditions. The comparison between the average SST seasonality of 7°C and 9°C, derived from average annual δ18O (1.1‰) and Sr/Ca (0.579 mmol/mol) amplitudes, respectively, indicates that the δ18O-derived SST seasonality is biased by seawater composition, reducing the δ18O amplitude by 0.3‰. This value is equivalent to a seasonal SSS variation of 1‰, as observed under present-day Aegean Sea conditions. Concentration patterns of non-lattice bound major and trace elements, related to trapped particles within the coral skeleton, reflect seasonal input of suspended load into the reef environment. δ18O, Sr/Ca and non-lattice bound element proxy records, as well as geochemical compositions of the trapped particles, provide evidence for intense precipitation in the Eastern Mediterranean during winters. Winter rain caused freshwater discharge and transport of weathering products from the hinterland into the reef environment. There is a trend in coral δ18O data to more positive mean δ18O values (–2.7‰ to –1.7‰) coupled with decreased seasonal δ18O amplitudes (1.1‰ to 0.7‰) from 10 to 7 Ma. This relationship is most easily explained in terms of more positive summer δ18O. Since coral diversity and annual growth rates indicate more or less constant average SST for the Mediterranean from the Tortonian to the Early Messinian, more positive mean and summer δ18O indicate increasing aridity during the Late Miocene, and more pronounced during summers. The analytical results implicate that winter rainfall and summer drought, the main characteristics of the present-day Mediterranean climate, were already present in the Mediterranean region during the Late Miocene. Some models have argued that the Mediterranean climate did not exist in this region prior to the Pliocene. However, the data presented here show that conditions comparable to those of the present-day existed either intermittently or permanently since at least about 10 Ma.

Copper and zinc stable isotope ratios as tracers of biogeochemical processes, sources and transport of Cu and Zn in soils

Copper and Zn are essential micronutrients for plants, animals, and humans; however, they may also be pollutants if they occur at high concentrations in soil. Therefore, knowledge of Cu and Zn cycling in soils is required both for guaranteeing proper nutrition and to control possible risks arising from pollution.rnThe overall objective of my study was to test if Cu and Zn stable isotope ratios can be used to investigate into the biogeochemistry, source and transport of these metals in soils. The use of stable isotope ratios might be especially suitable to trace long-term processes occurring during soil genesis and transport of pollutants through the soil. In detail, I aimed to answer the questions, whether (1) Cu stable isotopes are fractionated during complexation with humic acid, (2) 65Cu values can be a tracer for soil genetic processes in redoximorphic soils (3) 65Cu values can help to understand soil genetic processes under oxic weathering conditions, and (4) 65Cu and 66Zn values can act as tracers of sources and transport of Cu and Zn in polluted soils.rnTo answer these questions, I ran adsorption experiments at different pH values in the laboratory and modelled Cu adsorption to humic acid. Furthermore, eight soils were sampled representing different redox and weathering regimes of which two were influenced by stagnic water, two by groundwater, two by oxic weathering (Cambisols), and two by podzolation. In all horizons of these soils, I determined selected basic soil properties, partitioned Cu into seven operationally defined fractions and determined Cu concentrations and Cu isotope ratios (65Cu values). Finally, three additional soils were sampled along a deposition gradient at different distances to a Cu smelter in Slovakia and analyzed together with bedrock and waste material from the smelter for selected basic soil properties, Cu and Zn concentrations and 65Cu and 66Zn values.rnMy results demonstrated that (1) Copper was fractionated during adsorption on humic acid resulting in an isotope fractionation between the immobilized humic acid and the solution (65CuIHA-solution) of 0.26 ± 0.11‰ (2SD) and that the extent of fractionation was independent of pH and involved functional groups of the humic acid. (2) Soil genesis and plant cycling causes measurable Cu isotope fractionation in hydromorphic soils. The results suggested that an increasing number of redox cycles depleted 63Cu with increasing depth resulting in heavier 65Cu values. (3) Organic horizons usually had isotopically lighter Cu than mineral soils presumably because of the preferred uptake and recycling of 63Cu by plants. (4) In a strongly developed Podzol, eluviation zones had lighter and illuviation zones heavier 65Cu values because of the higher stability of organo-65Cu complexes compared to organo-63Cu complexes. In the Cambisols and a little developed Podzol, oxic weathering caused increasingly lighter 65Cu values with increasing depth, resulting in the opposite depth trend as in redoximorphic soils, because of the preferential vertical transport of 63Cu. (5) The 66Zn values were fractionated during the smelting process and isotopically light Zn was emitted allowing source identification of Zn pollution while 65Cu values were unaffected by the smelting and Cu emissions isotopically indistinguishable from soil. The 65Cu values in polluted soils became lighter down to a depth of 0.4 m indicating isotope fractionation during transport and a transport depth of 0.4 m in 60 years. 66Zn values had an opposite depth trend becoming heavier with depth because of fractionation by plant cycling, speciation changes, and mixing of native and smelter-derived Zn. rnCopper showed measurable isotope fractionation of approximately 1‰ in unpolluted soils, allowing to draw conclusions on plant cycling, transport, and redox processes occurring during soil genesis and 65Cu and 66Zn values in contaminated soils allow for conclusions on sources (in my study only possible for Zn), biogeochemical behavior, and depth of dislocation of Cu and Zn pollution in soil. I conclude that stable Cu and Zn isotope ratios are a suitable novel tool to trace long-term processes in soils which are difficult to assess otherwise.rn

Diversity of lithologic components at Meridiani Planum, Mars: Insights from Mössbauer spectroscopic investigations

The two Mars Exploration Rovers (MER), Spirit and Opportunity, landed on the Martian surface in January 2004 and have since collected a wealth of information about their landing sites. As part of their payload, the miniaturised Mössbauer spectrometer MIMOS II contributes to the success of the mission by identifying Iron-bearing minerals and by determining Iron oxidation states in them. The basis of this work is the data set obtained at Opportunity’s landing site at Meridiani Planum. A portion of this data set is evaluated with different methods, with the aim to thoroughly characterize lithologic components at Meridiani Planum and possible relations between them.rnMIMOS II is able to measure Mössbauer spectra at different energies simultaneously, bearing information from different sampling depths of the investigated target. The ability of depth-selective Mössbauer spectroscopy to characterize weathered surface layers is illustrated through its application to two suitable rock targets that were investigated on Mars. In both cases, an enhanced concentration of Iron oxides at the rock surface was detected, pointing to a low degree of aqueous alteration. rnThe mineral hematite (α-Fe2O3) is present in the matrix of outcrop rocks and in spherules weathering from the outcrop. Simultaneous fitting of Mössbauer spectra was applied to data sets obtained on both target types to characterize the hematite component in detail. This approach reveals that two hematite populations are present, both in the outcrop matrix as well as in spherules. The hematite component with a comparably high degree of crystallinity and/or chemical purity is present in the outcrop matrix. The investigation of hematite at Meridiani Planum has shown that simultaneous fitting is a suitable and useful method to evaluate a large, correlated set of Mössbauer spectra.rnOpportunity encountered loose, cm-sized rocks along its traverse. Based on their composition and texture, these “cobbles” can be divided into three different groups. Outcrop fragments are impact-derived ejecta from local outcrop rocks. Cobbles of meteoritic origin contain the minerals kamacite (Fe,Ni) and troilite (FeS) and exhibit high Ni contents. Melt-bearing impact breccias bear similarities to local outcrop rocks and basaltic soil, with a phase composition and texture consistent with a formation scenario involving partial melting and inclusion of small, bright outcrop clasts. rnIron meteorites on the Martian surface experience weathering through the presence of even trace amounts of water due to their metallic nature. Opportunity encountered and investigated four Iron meteorites, which exhibit evidence for physical and chemical weathering. Discontinuous coatings contain Iron oxides, pointing to the influence of limited amounts of water. rnA terrestrial analogue site for Meridiani Planum is the Rio Tinto basin in south-west Spain. With its deposits of sulfate- and iron-oxide-bearing minerals, the region provides an adequate test bed for instrumentation for future Mars missions. In-situ investigations at Rio Tinto were carried out with a special focus on the combined use of Mössbauer spectroscopy with MIMOS II and Raman spectroscopy with a field-portable instrument. The results demonstrate that the two instruments provide complementary information about investigated samples.

Process-based modelling of lichens and bryophytes and their role in global biogeochemical cycles

This thesis presents a process-based modelling approach to quantify carbon uptake by lichens and bryophytes at the global scale. Based on the modelled carbon uptake, potential global rates of nitrogen fixation, phosphorus uptake and chemical weathering by the organisms are estimated. In this way, the significance of lichens and bryophytes for global biogeochemical cycles can be assessed. The model uses gridded climate data and key properties of the habitat (e.g. disturbance intervals) to predict processes which control net carbon uptake, namely photosynthesis, respiration, water uptake and evaporation. It relies on equations used in many dynamical vegetation models, which are combined with concepts specific to lichens and bryophytes, such as poikilohydry or the effect of water content on CO2 diffusivity. To incorporate the great functional variation of lichens and bryophytes at the global scale, the model parameters are characterised by broad ranges of possible values instead of a single, globally uniform value. The predicted terrestrial net uptake of 0.34 to 3.3 Gt / yr of carbon and global patterns of productivity are in accordance with empirically-derived estimates. Based on the simulated estimates of net carbon uptake, further impacts of lichens and bryophytes on biogeochemical cycles are quantified at the global scale. Thereby the focus is on three processes, namely nitrogen fixation, phosphorus uptake and chemical weathering. The presented estimates have the form of potential rates, which means that the amount of nitrogen and phosphorus is quantified which is needed by the organisms to build up biomass, also accounting for resorption and leaching of nutrients. Subsequently, the potential phosphorus uptake on bare ground is used to estimate chemical weathering by the organisms, assuming that they release weathering agents to obtain phosphorus. The predicted requirement for nitrogen ranges from 3.5 to 34 Tg / yr and for phosphorus it ranges from 0.46 to 4.6 Tg / yr. Estimates of chemical weathering are between 0.058 and 1.1 km³ / yr of rock. These values seem to have a realistic order of magnitude and they support the notion that lichens and bryophytes have the potential to play an important role for global biogeochemical cycles.