Petrogenesis of dunite, wehrlite and websterite xenoliths from Kimberley, South Africa: Origin as mantle peridotites of cumulates

Dunite, wehrlite and websterite xenoliths occur amongst a large abundance of mantle xenoliths in kimberlites of the Kimberley cluster in South Africa. Up to know they have mostly been neglected. On the basis of texture, major and trace elements, oxygen isotopes as well as Re-Os isotope characteristics, they can be subdivided into two groups. A coarse-grained mantle peridotite group, comprising dunite, wehrlite and websterite xenoliths, that are similar to fertile peridotites and represent upper mantle assemblages that are differently influenced by mantle metasomatism. And a cumulate group, containing fine-grained Fe-rich dunite xenoliths that represent cumulates of flood basalt magmatism related to ~183 Ma Karoo and ~2.7 Ga Ventersdorp events in southern Africa. Dunite, wehrlite and websterite xenoliths have preserved a complex history of melt depletion and metasomatic re-enrichment events, which gives information about the different re-enrichment stages of the subcratonic lithospheric mantle and the spatial differences within the Kaapvaal craton upper mantle. Websterite xenoliths comprise orthopyroxene (40-85 Vol. %), clinopyroxene (5-42 Vol. %), garnet (4-10 Vol. %) and subordinately olivine, while dunite and wehrlite xenoliths contain predominantly olivine (65-100 Vol %) and subordinately orthopyroxene, clinopyroxene and garnet. High melt depletion and a dunitic to harzburgitic protolith composition are reflected by high forsterite (Fo90-92) and high olivine NiO contents (2800-5000 ppm) and high orthopyroxene Mg# (Mg/(Mg+Fe)) of 0.91-0.93. Re-depletion ages of predominantly 2.9 Ga reflect a minimum age of melt depletion. Melt depletion ceased in conjunction with collision of the Kimberley block with the Witwatersrand block ~2.9 Ga ago. Subduction related re-fertilisation of the previously depleted mantle xenoliths is documented by i) amoeboid textured orthopyroxene, clinopyroxene and garnet, which crystallized in schlieren along olivine grain boundaries, ii) high whole-rock SiO2, Al2O3, CaO, TiO2, FeO contents, iii) low oxygen isotope ratios in clinopyroxene and garnet of 4.8-5.4 ‰ and 4.7-5.3 ‰, respectively and iv) trace element compositions of wehrlitic clinopyroxene and garnet in equilibrium with high-pressure partial melts of eclogite. Trace element disequilibrium of orthopyroxene with clinopyroxene and garnet indicates a separate origin for orthopyroxene, on one side as primary mantle orthopyroxene in dunite and wehrlite xenoliths and on the other side as reaction product with Si-rich melts produced by partial melting of eclogite. This reaction triggered replacement of olivine by orthopyroxene in the surrounding mantle and produced the typical Si-rich composition of Kaapvaal mantle peridotites. Partial melting of eclogite at higher temperatures produced a second metasomatic melt with lower SiO2, but higher Al2O3, CaO, FeO, Ti, Zr, Hf and a low oxygen isotope ratio. This melt triggered clinopyroxene and locally garnet and rutile crystallization in percolation veins, replacing olivine and orthopyroxene in the Kaapvaal upper mantle. Additionally, websterite xenoliths have experienced late stage cryptic metasomatism by the host kimberlite melt, changing the trace element composition of clinopyroxene, orthopyroxene and garnet to different extent. Hence websterite and most fertile lherzolite xenoliths have experienced three metasomatic events: i) reaction with high-Si melt, ii) percolation of subduction related silica melt with lower SiO2 content and iii) cryptic metasomatism by kimberlite. In contrast, dunite and wehrlite xenoliths have only experienced the second metasomatic event. They represent mantle lithologies further away from metasomatising agents. The Fe-rich dunites comprise olivine neoblasts with subordinate olivine porphyroclasts and parallel-orientated needles of ilmenite, which may enclose spinel. The lower forsterite and NiO contents of olivine in Fe-rich dunites compared to mantle peridotite xenoliths (Fo87-89 vs. Fo93-95 and 1300-2800ppm vs. 2200-3900 ppm, respectively), rules out a restitic origin. Cr-rich spinels are remnants of the original cumulate mineralogy that survived a late stage metasomatic overprint related to the production of the host kimberlite, producing ilmenite and phlogopite in some samples. Olivine porphyroclasts and neoblasts have different trace element compositions, the latter having high Ti, V, Cr and Ni and low Zn, Zr and Nb contents, indicating contrasting origins for neoblasts and porphyroclasts. The dunites have high 187Os/188Os ratios (0.11-0.15) indicating young (Phanerozoic) model ages for most samples, whereas three samples show isotopic mixtures between Phanerozoic neoblasts and ancient porphyroclastic material. Most Fe-rich dunite xenoliths can be interpreted as cumulates of fractional crystallization of Karoo magmatism, whereas the porphyroclasts are interpreted to be remnants from the much earlier Archaean Ventersdorp magmatism.

Analyse genomischer Imbalancen in hepatozellulären Karzinomen und präneoplastischen Leberläsionen

Das hepatozelluläre Karzinom (HCC) ist mit ungefähr 1,000,000 neuen Fällen pro Jahr einer der häufigsten malignen Tumore weltweit. Es ist hauptsächlich in Südost-Asien und im südlichen Afrika verbreitet. Risikofaktoren sind chronische Infektionen mit Hepatitis Viren (HBV, HCV), Aflatoxin B1-Belastung und chronischer Alkoholkonsum. Um Veränderungen auf genomischer Ebene in HCCs zu untersuchen, wurden in der vorliegenden Untersuchung Frischgewebeproben von 21 Patienten mit HCCs und formalin-fixiertes, paraffineingebettetes Material von 6 Dysplastischen Knoten mittels Comparativer genomischer Hybridisierung (CGH) analysiert. In den untersuchten HCCs konnte Zugewinne auf 1q (12/21), 6p ( 6/21), 8q (11/21), 17q (6/21), 20q (6/21), sowie Verluste auf 4q (7/21), 6q (4/21), 10q (3/21), 13q (4/21), 16q (3/21) identifiziert werden. Die Validität der mit diesem Ansatz erzielten Ergebnisse konnte anhand von unabhängigen Kontrollexperimenten mit Interphase-FISH-Analyse nachgewiesen werden. Die in Dysplastische Knoten identifizierten Veränderungen sind Gewinne auf 1q (50% ) sowie Verluste auf 8p und 17p. Daher stellt 1q eine Kandidatenregion für die Identifizierung jener Gene dar, die bereits im frühem Stadium der Hepatokarzinogenese aktiviert sind. Die Gen-Expressionsanalyse eines HCCs mit Gewinnen auf 1q, 8q, und Xq zeigte die Überexpression von einigen Genen, die in den amplifizierten Regionen liegen. Daher kann spekuliert werden, dass die DNA-Amplifikation in der Hepatokarzinogenese bei einigen Genen ein Mechanismus der Aktivierung sein kann. Zusammengefasst konnte somit durch CGH-Analyse charakteristische, genomische Imbalances des HCC ermittelt werden. Der Vergleich mit Veränderungen bei prämalignen Läsionen erlaubt die Unterscheidung früher (prämaligner) und später (progressionsassoziierter) Veränderungen

Soil biogenic emissions of nitric oxide from arid and semi-arid ecosystems

The biogenic production of NO in the soil accounts for between 10% and 40% of the global total. A large degree of the uncertainty in the estimation of the biogenic emissions stems from a shortage of measurements in arid regions, which comprise 40% of the earth’s land surface area. This study examined the emission of NO from three ecosystems in southern Africa which cover an aridity gradient from semi-arid savannas in South Africa to the hyper-arid Namib Desert in Namibia. A laboratory method was used to determine the release of NO as a function of the soil moisture and the soil temperature. Various methods were used to up-scale the net potential NO emissions determined in the laboratory to the vegetation patch, landscape or regional level. The importance of landscape, vegetation and climatic characteristics is emphasized. The first study occurred in a semi-arid savanna region in South Africa, where soils were sampled from 4 landscape positions in the Kruger National Park. The maximum NO emission occurred at soil moisture contents of 10%-20% water filled pore space (WFPS). The highest net potential NO emissions came from the low lying landscape positions, which have the largest nitrogen (N) stocks and the largest input of N. Net potential NO fluxes obtained in the laboratory were converted in field fluxes for the period 2003-2005, for the four landscape positions, using soil moisture and temperature data obtained in situ at the Kruger National Park Flux Tower Site. The NO emissions ranged from 1.5-8.5 kg ha-1 a-1. The field fluxes were up-scaled to a regional basis using geographic information system (GIS) based techniques, this indicated that the highest NO emissions occurred from the Midslope positions due to their large geographical extent in the research area. Total emissions ranged from 20x103 kg in 2004 to 34x103 kg in 2003 for the 56000 ha Skukuza land type. The second study occurred in an arid savanna ecosystem in the Kalahari, Botswana. In this study I collected soils from four differing vegetation patch types including: Pan, Annual Grassland, Perennial Grassland and Bush Encroached patches. The maximum net potential NO fluxes ranged from 0.27 ng m-2 s-1 in the Pan patches to 2.95 ng m-2 s-1 in the Perennial Grassland patches. The net potential NO emissions were up-scaled for the year December 2005-November 2006. This was done using 1) the net potential NO emissions determined in the laboratory, 2) the vegetation patch distribution obtained from LANDSAT NDVI measurements 3) estimated soil moisture contents obtained from ENVISAT ASAR measurements and 4) soil surface temperature measurements using MODIS 8 day land surface temperature measurements. This up-scaling procedure gave NO fluxes which ranged from 1.8 g ha-1 month-1 in the winter months (June and July) to 323 g ha-1 month-1 in the summer months (January-March). Differences occurred between the vegetation patches where the highest NO fluxes occurred in the Perennial Grassland patches and the lowest in the Pan patches. Over the course of the year the mean up-scaled NO emission for the studied region was 0.54 kg ha-1 a-1 and accounts for a loss of approximately 7.4% of the estimated N input to the region. The third study occurred in the hyper-arid Namib Desert in Namibia. Soils were sampled from three ecosystems; Dunes, Gravel Plains and the Riparian zone of the Kuiseb River. The net potential NO flux measured in the laboratory was used to estimate the NO flux for the Namib Desert for 2006 using modelled soil moisture and temperature data from the European Centre for Medium Range Weather Forecasts (ECMWF) operational model on a 36km x 35km spatial resolution. The maximum net potential NO production occurred at low soil moisture contents (<10%WFPS) and the optimal temperature was 25°C in the Dune and Riparian ecosystems and 35°C in the Gravel Plain Ecosystems. The maximum net potential NO fluxes ranged from 3.0 ng m-2 s-1 in the Riparian ecosystem to 6.2 ng m-2 s-1 in the Gravel Plains ecosystem. Up-scaling the net potential NO flux gave NO fluxes of up to 0.062 kg ha-1 a-1 in the Dune ecosystem and 0.544 kg h-1 a-1 in the Gravel Plain ecosystem. From these studies it is shown that NO is emitted ubiquitously from terrestrial ecosystems, as such the NO emission potential from deserts and scrublands should be taken into account in the global NO models. The emission of NO is influenced by various factors such as landscape, vegetation and climate. This study looks at the potential emissions from certain arid and semi-arid environments in southern Africa and other parts of the world and discusses some of the important factors controlling the emission of NO from the soil.

Evolution und historische Biogeographie von Senecio L. mit Fokus auf die Alte Welt

Senecio L., eine der größten Angiospermengattungen, entstand im mittleren Miozän in trockenen oder Winterregengebieten des südlichen Afrikas. Von dort ausgehend wurden die anderen Kontinente mehrmals unabhängig voneinander besiedelt. Die hohe Artenanzahl, das junge Alter und die was weltweite Verbreitung der Gattung stellt eine Besonderheit dar. Die meisten anderen jungen und schnellen Radiationen sind nicht so weit verbreitet. Es scheint, als wäre die hohe Artenanzahl und die weite Verbreitung das Ergebnis von einer guten Ausbreitungsfähigkeit, einem hohe Samenansatz sowie einer Präferenz für offene und gestörte Standorte.rnDie Paläarktis wurde zweimal unabhängig voneinander kolonisiert, beide Linien kommen in etwa in der gleichen Region vor, unterscheiden sich aber in ihrer Habitatpräferenz und Lebensdauer. Die eine Linie kommt zumeist entlang des Mittelmeeres vor und stammt am wahrscheinlichsten von annuellen Tieflandarten aus den trockenen oder Winterregengebieten des südlichen Afrikas ab. Die andere Linie stammt wahrscheinlich von Drakensbergarten ab und besiedelt auch bevorzugt bergige Regionen in der Paläarktis. Senecio ist außerdem die artenreichste Gattung in den tropisch afroalpinen Regionen Ostafrikas. Die Arten sind während des Pliozäns oder Pleistozäns entstanden und das Ergebnis von mehrfacher Einwanderung aus anderen temperaten Regionen, in situ Artbildung spielte nur eine untergeordnete Bedeutung. rn