TY - THES A1 - Wiersberg, Thomas T1 - Edelgase als Tracer für Wechselwirkungen von Krusten- und Mantelfluiden mit diamantführenden Gesteinen des östlichen Baltischen Schildes N2 - In der vorliegenden Arbeit werden anhand der Edelgaszusammensetzung von Kimberliten und Lamproiten sowie ihrer gesteinsbildenden Minerale die Wechselwirkungen dieser Gesteine mit Fluiden diskutiert. Die untersuchten Proben stammen vom östlichen Baltischen Schild, vom Kola-Kraton (Poria Guba und Kandalaksha) und vom karelischen Kraton (Kostamuksha). Edelgasanalysen nach thermischer oder mechanischer Gasextraktion von 23 Gesamtgesteinsproben und 15 Mineralseparaten ergeben folgendes Bild: Helium- und Neon-Isotopendaten der Fluideinschlüsse von Lamproiten aus Kostamuksha lassen auf den Einfluss einer fluiden Phase krustaler Herkunft schliessen. Diese Wechselwirkungen fanden wahrscheinlich schon während des Magmenaufstiegs statt, denn spätere Einflüsse krustaler Fluide auf die Lamproite und ihr Nebengestein (Quarzit) sind gering, wie anhand der C/36Ar-Zusammensetzung gezeigt wird. Auch sind die mit verschiedenen Datierungsmethoden (Rb-Sr, Sm-Nd, K-Ar) an Mineralseparaten und teilweise an Gesamtgestein ermittelten Alter konsistent und machen eine metamorphe Überprägung unwahrscheinlich. Aufgrund der Verteilung der primordialen Edelgasisotope zwischen Fluideinschlüssen und Gesteinsmatrix ist ein langsamer Magmenaufstieg anzunehmen, was die Möglichkeit der Kontamination mit einem krustalen Fluid während des Magmenaufstiegs erhöht. Die Gasextraktion aus Mineralseparaten erfolgte thermisch, wodurch eine Freisetzung der Gase ausschließlich aus Fluideinschlüssen nicht möglich ist. Hierbei zeigen Amphibol und Klinopyroxen, separiert aus Kostamuksha-Lamproiten, in ihrer Neon-Isotopenzusammensetzung im Vergleich zur krustalen Zusammensetzung (Kennedy et al., 1990) ein leicht erhöhtes Verhältnis von 20Ne/22Ne, was ein Hinweis auf Mantel-Neon sein könnte. Kalifeldspäte, Quarz und Karbonate enthalten dagegen nur Neon krustaler Zusammensetzung. Phlogopite haben sehr kleine Verhältnisse von 20Ne/22Ne und 21Ne/22Ne, zurückzuführen auf in-situ-Produktion von 22Ne in Folge von U- und Th-Zerfallsprozessen. Wie unterschiedliche thermische Entgasungsmuster für 40Ar und 36Ar zeigen, ist 36Ar in Fluideinschlüssen konzentriert. Das 40Ar/36Ar-Isotopenverhältnis der Fluideinschlüsse von Lamproiten aus Kostamuksha ist antikorreliert mit der durch thermische Extraktion bestimmten Gesamtmenge an 36Ar. Argon aus Fluideinschlüssen setzt sich daher aus zwei Komponenten zusammen: Einer Komponente mit atmosphärischer Argon-Isotopenzusammensetzung und einer krustalen Komponente mit einem Isotopenverhältnis 40Ar/36Ar > 6000. Diffusion von radiogenem 40Ar aus der Kristallmatrix in die Fluideinschlüsse spielt keine wesentliche Rolle. Kimberlite aus Poria Guba und Kandalaksha zeigen anhand der Helium- und z. T. auch der Neon-Isotopenzusammensetzung eine Mantelkomponente in den Fluideinschlüssen an. Bei einem angenommenen 20Ne/22Ne-Isotopenverhältnis von 12,5 in der Mantelquelle ergibt sich ein 21Ne/22Ne-Isotopenverhältnis von 0,073 ± 0,011 sowie ein 3He/4He-Isotopenverhältnis, welches im Vergleich zum subkontinentalem Mantel (Dunai und Baur, 1995) stärker radiogen geprägt ist. Solche Isotopensignaturen sind mit höheren Konzentrationen an Uran und Thorium in der Mantelquelle der Kimberlite zu erklären. Rb-Sr- und Sm-Nd-Altersbestimmungen erfolgten von russischer Seite (Belyatskii et al., 1997; Nikitina et al., 1999) und ergeben ein Alter von 1,23 Ga für den Lamproitvulkanismus in Kostamuksha. Eigene K-Ar-Datierungen an Phlogopiten und Kalifeldspäten stimmen mit einem Alter von 1193 ± 20 Ma fast mit den Rb-Sr- und Sm-Nd-Altern überein. Die K-Ar-Datierung an einem Phlogopit aus Poria Guba, separiert aus dem Kimberlit PGK 12a, ergibt ein Alter von 396 Ma, ebenfalls in guter Übereinstimmung mit Rb-Sr-und Sm-Nd-Altern (ca. 400 Ma, Lokhov, pers. Mitteilung). K-Ar-Altersbestimmungen an Gesamtgestein aus Poria Guba erbrachten kein schlüssiges Alter. Die Rb-Sr- und Sm-Nd-Alter des Lamproitmagmatismus in Poria Guba betragen 1,72 Ga (Nikitina et al., 1999). Vergleiche von gemessenen mit berechneten Edelgaskonzentrationen aus in-situ-Produktion zeigen weiterhin, dass in Abhängigkeit vom Alter der Probe Diffusionsprozesse stattgefunden haben, die zu unterschiedlichen und z. T. erheblichen Verlusten an Helium und Neon führten. Diffusionsverluste an Argon sind dagegen kaum signifikant. Unterschiedliche Diffusionsverluste in Abhängigkeit von Alter und betrachtetem Edelgas zeigen auch die primordialen Edelgase. N2 - In the present thesis, interactions of kimberlites and lamproites as well as their constituent minerals with fluids are discussed based on noble gas compositions. The samples originate from the eastern Baltic Shield, more specifically from the Kola craton (Poria Guba and Kandalaksha) and the Karelia craton (Kostamuksha). Gas was extracted by stepwise heating and crushing from 23 whole rock samples and 15 mineral separates. These two techniques allow differential extraction of gas from fluid inclusions (crushing technique) and from the bulk sample (stepwise heating). The noble gas analyses provide the following information: Helium and neon isotopic compositions of fluid inclusions in lamproites reveal the presence of a crustal fluid phase. Fluid interaction probably ocurred already during the process of magma ascent. Interaction after lamproite emplacement seems unlikely. The lamproites and their host rock differ in the degree of fluid-rock interaction, as demonstrated by the C/36Ar composition. In addition, various dating methods (Rb-Sr, Sm-Nd, K-Ar) yield almost the same age within analytical error. Thus, a metamorphic overprint can be excluded. The distribution of primordial noble gases between fluid inclusions and crystal lattice suggests a relatively slow magma ascent, making an interaction of the lamproitic magma with crustal fluids even more likely. Since noble gases from mineral separates were extracted only by the stepwise heating method, gases stored in fluid inclusions could not be released separately. Amphibole and clinopyroxene separates yielded a higher 20Ne/22Ne ratio in comparison to crustal composition (Kennedy et al., 1990). This presumably is an indication of a mantle derived fluid phase. On the other hand, neon isotopic composition of K-feldspar, quartz and carbonate separates are indistinguishable from the crustal composition. In comparison to other mineral separates, phlogopite yields very low ratios of 20Ne/22Ne and 21Ne/22Ne due to in situ production of 22Ne, which is a result of nuclear reactions. The distinct thermal gas release patterns of 40Ar and 36Ar indicates that 36Ar is concentrated in fluid inclusions. The 40Ar/36Ar isotopic ratio in fluid inclusions shows a negative correlation with the total amount of 36Ar released by thermal extraction. Therefore, argon from fluid inclusions is a simple 2-component mixture of air and a crustal component with an 40Ar/36Ar ratio > 6000. It can be shown that diffusion of 40Ar from the matrix into fluid inclusions is negligible. In contrast to lamproites, whole rock kimberlite samples from Poria Guba and Kandalaksha show clear evidence in helium and, to a certain extentalso in neon isotope ratios, of interaction with a mantle derived fluid phase. Assuming a 20Ne/22Ne ratio of 12.5 for the mantle endmember, a 21Ne/22 Ne ratio of 0.073 ± 0.011 can be calculated. Likewise, the resulting 3He/4He ratio is more strongly influenced by radiogenic helium in comparison to the mean subcontinental mantle (Dunai und Baur, 1995). Such behaviour reflects higher concentrations of uranium and thorium in the magma source of kimberlites than the subcontinental mantle. Rb-Sr and Sm-Nd age determinations (Belyatskii et al., 1997; Nikitina et al., 1999) yield 1.23 Ga for the lamproite magmatism in Kostamuksha. K-Ar dating of phlogopite and K-feldspar provides similar ages (1.19 Ga). K-Ar dating of a single phlogopite separate from the Kimberlite sample PGK12a from Poria Guba, yields an age of 396 Ma which corresponds well with Rb-Sr and Sm-Nd ages. Depending on sample age, distinct and partly extensive diffusive loss of helium and neon has occurred, as shown by comparison of measured and calculated concentrations of in situ produced isotopes. Diffusion loss is negligible for argon. This is also strongly supported by primordial noble gas composition. KW - Geochemie KW - Edelgase KW - Mantel KW - Kruste KW - Fluid KW - Helium KW - Neon KW - Argon KW - noble gas KW - mantle KW - geochemistry KW - crust KW - fluid KW - helium KW - neon KW - argon Y1 - 2001 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-0000218 ER - TY - JOUR A1 - Wilke, Franziska Daniela Helena A1 - Vasquez, Monica A1 - Wiersberg, Thomas A1 - Naumann, Rudolf A1 - Erzinger, Jörg T1 - On the interaction of pure and impure supercritical CO2 with rock forming minerals in saline aquifers: An experimental geochemical approach JF - Applied geochemistry : journal of the International Association of Geochemistry and Cosmochemistry N2 - The aim of this experimental study was to evaluate and compare the geochemical impact of pure and impure CO2 on rock forming minerals of possible CO2 storage reservoirs. This geochemical approach takes into account the incomplete purification of industrial captured CO2 and the related effects during injection, and provides relevant data for long-term storage simulations of this specific greenhouse gas. Batch experiments were conducted to investigate the interactions of supercritical CO2, brine and rock-forming mineral concentrates (albite, microcline, kaolinite, biotite, muscovite, calcite, dolomite and anhydrite) using a newly developed experimental setup. After up to 42 day (1000 h) experiments using pure and impure supercritical CO2 the dissolution and solution characteristics were examined by XRD, XRF, SEM and EDS for the solid, and ICP-MS and IC for the fluid reactants, respectively. Experiments with mixtures of supercritical CO2 (99.5 vol.%) and SO2 or NO2 impurities (0.5 vol.%) suggest the formation of H2SO4 and HNO3, reflected in pH values between 1 and 4 for experiments with silicates and anhydrite and between 5 and 6 for experiments with carbonates. These acids should be responsible for the general larger amount of cations dissolved from the mineral phases compared to experiments using pure CO2. For pure CO2 a pH of around 4 was obtained using silicates and anhydrite, and 7-8 for carbonates. Dissolution of carbonates was observed after both pure and impure CO2 experiments. Anhydrite was corroded by approximately 50 wt.% and gypsum precipitated during experiments with supercritical CO2 + NO2. Silicates do not exhibit visible alterations during all experiments but released an increasing amount of cations in the reaction fluid during experiments with impure CO2. Nonetheless, precipitated secondary carbonates could not be identified. Y1 - 2012 U6 - https://doi.org/10.1016/j.apgeochem.2012.04.012 SN - 0883-2927 VL - 27 IS - 8 SP - 1615 EP - 1622 PB - Elsevier CY - Oxford ER - TY - JOUR A1 - Toy, Virginia Gail A1 - Sutherland, Rupert A1 - Townend, John A1 - Allen, Michael J. A1 - Becroft, Leeza A1 - Boles, Austin A1 - Boulton, Carolyn A1 - Carpenter, Brett A1 - Cooper, Alan A1 - Cox, Simon C. A1 - Daube, Christopher A1 - Faulkner, D. R. A1 - Halfpenny, Angela A1 - Kato, Naoki A1 - Keys, Stephen A1 - Kirilova, Martina A1 - Kometani, Yusuke A1 - Little, Timothy A1 - Mariani, Elisabetta A1 - Melosh, Benjamin A1 - Menzies, Catriona D. A1 - Morales, Luiz A1 - Morgan, Chance A1 - Mori, Hiroshi A1 - Niemeijer, Andre A1 - Norris, Richard A1 - Prior, David A1 - Sauer, Katrina A1 - Schleicher, Anja Maria A1 - Shigematsu, Norio A1 - Teagle, Damon A. H. A1 - Tobin, Harold A1 - Valdez, Robert A1 - Williams, Jack A1 - Yeo, Samantha A1 - Baratin, Laura-May A1 - Barth, Nicolas A1 - Benson, Adrian A1 - Boese, Carolin A1 - Célérier, Bernard A1 - Chamberlain, Calum J. A1 - Conze, Ronald A1 - Coussens, Jamie A1 - Craw, Lisa A1 - Doan, Mai-Linh A1 - Eccles, Jennifer A1 - Grieve, Jason A1 - Grochowski, Julia A1 - Gulley, Anton A1 - Howarth, Jamie A1 - Jacobs, Katrina A1 - Janku-Capova, Lucie A1 - Jeppson, Tamara A1 - Langridge, Robert A1 - Mallyon, Deirdre A1 - Marx, Ray A1 - Massiot, Cécile A1 - Mathewson, Loren A1 - Moore, Josephine A1 - Nishikawa, Osamu A1 - Pooley, Brent A1 - Pyne, Alex A1 - Savage, Martha K. A1 - Schmitt, Doug A1 - Taylor-Offord, Sam A1 - Upton, Phaedra A1 - Weaver, Konrad C. A1 - Wiersberg, Thomas A1 - Zimmer, Martin T1 - Bedrock geology of DFDP-2B, central Alpine Fault, New Zealand JF - New Zealand journal of geology and geophysics : an international journal of the geoscience of New Zealand, the Pacific Rim, and Antarctica ; NZJG N2 - During the second phase of the Alpine Fault, Deep Fault Drilling Project (DFDP) in the Whataroa River, South Westland, New Zealand, bedrock was encountered in the DFDP-2B borehole from 238.5–893.2 m Measured Depth (MD). Continuous sampling and meso- to microscale characterisation of whole rock cuttings established that, in sequence, the borehole sampled amphibolite facies, Torlesse Composite Terrane-derived schists, protomylonites and mylonites, terminating 200–400 m above an Alpine Fault Principal Slip Zone (PSZ) with a maximum dip of 62°. The most diagnostic structural features of increasing PSZ proximity were the occurrence of shear bands and reduction in mean quartz grain sizes. A change in composition to greater mica:quartz + feldspar, most markedly below c. 700 m MD, is inferred to result from either heterogeneous sampling or a change in lithology related to alteration. Major oxide variations suggest the fault-proximal Alpine Fault alteration zone, as previously defined in DFDP-1 core, was not sampled. KW - Alpine Fault KW - New Zealand KW - scientific drilling KW - mylonite KW - cataclasite Y1 - 2017 U6 - https://doi.org/10.1080/00288306.2017.1375533 SN - 0028-8306 SN - 1175-8791 VL - 60 IS - 4 SP - 497 EP - 518 PB - Taylor & Francis CY - Abingdon ER -