Ortsaufgelöste Speziation von Schwermetallen in geogenen Proben mit Röntgenabsorptionsspektrometrie (my-XAS)

Die Vergesellschaftung und Bindungsform von Arsen in Düngekalk wurde durch chemische und mineralogische Analysen sowie XANES/EXAFS-Messungen untersucht. Die durch-schnittliche As-Konzentration im Düngekalk (70 mg/kg) überschreitet den Grenzwert der DüMV (40 mg/kg). Arsen ist in Mn- (Romanechit) und Fe-Dendriten (Goethit, Ferrihydrit) angereichert. Seine Oxidationsstufe ist jeweils 5+. µ-EXAFS-Untersuchungen ergaben Hin-weise auf zweizähnige und einzähnige mononukleare Durchdringungskomplexe mit Eisen-oxid. Das Mobilisierungsverhalten von Arsen wurde durch sequentielle Extraktion des Dün-gekalks und Mobilisierungsversuche mit wassergesättigtem Boden untersucht. Die Lösung erfolgte vorwiegend im dritten Extraktionsschritt gemeinsam mit kristallinen Eisenoxiden. Unter moderat anoxischen Bedingungen war im Boden keine zusätzliche Mobilisierung von Arsen aus dem Düngekalk nachweisbar. Erhöhte As-Konzentrationen und As3+-Anteile im Porenwasser traten bei niedrigem Eh unabhängig von Kalkzugabe auf. Eine Kopplung des Arsen-Grenzwerts an den Eisenoxidgehalt erscheint sinnvoll. Ein Messaufbau für Mikro-XAS Imaging wurde in Betrieb genommen. Er ermöglicht die si-multane Erfassung einer Probenfläche von 26,6×6,6 mm² wahlweise im Transmissions- oder Fluoreszenzmodus mit der räumlichen Auflösung 52×52 µm² durch eine CCD-Kamera. Zur Datenverarbeitung wurden IDL-Programme sowie die Fernerkundungssoftware ENVI ver-wendet. Die Messergebnisse zeigen weniger Störungen und Rauschen als die Ergebnisse frü-herer Messungen mit einem Prototyp. Die Ergebnisse und Erfahrungen der Messungen liefern Hinweise für die weitere erfolgreiche Nutzung des Messaufbaus.

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.