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1.
Belal S. Amireh Joerg Mutterlose Mazen N. Amaireh Tobias Puettmann Abdulkader M. Abed 《Arabian Journal of Geosciences》2018,11(15):425
Three sections from the Al-Hisa Phosphorite Formation (AHP) were measured in the southeastern desert of Jordan: Batn El-Ghoul, Nagb Etayyeg, and Zgaimat Al-Hasah. A fourth section, Wadi Arfa, is added from a previous work. The three sections differ from the typical AHP Formation in central Jordan by having highly reduced thicknesses, omission/non-deposition of the underlying formations, rarity of fossils, abundant sand, and their stratigraphic ages. A Paleocene-Early Eocene age, based on calcareous nannofossils, has been assigned to the AHP Formation of the sections studied in the southeast desert. This Paleocene-Early Eocene age is younger than the Early Maastrichtian age of the AHP deposits in central Jordan. The published ages of the phosphorite deposits in the eastern Mediterranean countries suggest a younging to the east due to an interplay between paleodepositional environments and plate tectonics (paleohigh formation). The minor phosphorite deposits of Turkey and Iran are not involved in the discussion because they were not part of the Afro-Arabian Plate or the later Arabian Plate. The abovementioned differences between the southeastern desert phosphorites and the central Jordan deposits are here explained by the formation of paleohighs on the Neo-Tethys seafloor during the Late Cretaceous-Eocene. These include the Sirhan Paleohigh where the southeast desert phosphorites were deposited. The formation of the highs was due to the compression associated first, with the subduction of the Afro-Arabian Plate, below the Eurasian Plate and later with their collision. 相似文献
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A. H. Ruffell G. D. Price J. Mutterlose K. Kessels E. Baraboshkin D. R. Grcke 《Geological Journal》2002,37(1):17-33
A study of clay mineral and calcareous nannofossil abundances in late Jurassic–early Cretaceous sediments from the Volga Basin, SE Russia, is presented. From these results, we are able to compare some general patterns of mineralogical and palaeontological change for the Volga Basin to the palaeoclimate models developed for northern Europe and beyond. The two successions examined comprise calcareous mudstones with black organic‐rich shale horizons, overlain by a series of phosphatic silty sands. Clay mineralogical results show a progressive decrease in kaolinite and the concomitant increase of smectite and illite through the middle Volgian, followed by an abrupt increase in kaolinite in the late Volgian. The clay mineral evidence suggests increasing aridity at the end of the Jurassic, similar, in part, to many western European successions. Because of differential settling of clay minerals, superimposed upon this possible climatic signature is likely to be the effect of relative sea‐level change. Calcareous nannofossil analysis from a single section reveals a shift through the middle Volgian from low nutrient, warm water assemblages dominated by Watznaueria to cooler surface water and high nutrient assemblages dominated by Biscutum constans. These observations suggest that increased aridity is also associated with climatic cooling. Black shales are associated with increased productivity, higher sea levels and increases in smectite content. Hence, periods of low (chemical) hinterland weathering during semi‐arid conditions are paradoxically associated with relatively nutrient‐rich waters, and organic‐rich shales. Comparison of published carbon and oxygen stable isotope results from this and other sections to the clay mineral and nannofossil data confirms the palaeoclimatic interpretation. This study significantly improves the published biostratigraphically constrained clay mineral database for this time period, because other European and North American successions are either non‐marine (and thus poorly dated), absent (through penecontemporaneous erosion) or condensed. Copyright © 2002 John Wiley & Sons, Ltd. 相似文献
3.
Taniel Danelian Laurence Le Callonnec Jochen Erbacher David C. Mosher Mitchell J. Malone Debora Berti Karen L. Bice Helen Bostock Hans-Jürgen Brumsack Astrid Forster Felix Heidersdorf Jorijntje Henderiks Thomas J. Janecek Christopher Junium Ken MacLeod Philip A. Meyers Jörg H. Mutterlose Hiroshi Nishi Christine Glatz 《Comptes Rendus Geoscience》2005,337(6):609-616
Five sites located on a bathymetric transect of the distal Demerara Rise were studied by ODP Leg 207. Albian sediments of essentially terrigenous nature (clay, siltstone, sandstone) are the oldest drilled stratigraphic levels and form apparently the top of the synrift sequence. They are overlain by Cenomanian to Santonian finely laminated black shales, rich in organic matter of marine origin, which accumulated on a thermally subsiding ramp. Early Campanian hiatuses are thought to be the result of final disjunction of Demerara Rise (South America) from Africa and the onset of deep water communication between the two Atlantic basins (south and central). The overlying Uppermost Cretaceous–Oligocene chalk includes rich and diversified calcareous plankton assemblages, as well as two radiolarian-rich intervals (Late Campanian and Middle Eocene). A complex erosional surface developed during the Late Oligocene–Early Miocene. Sedimentation was impeded since then on the intermediate and deep sites of Demerara Rise, possibly due to the action of deep submarine currents. To cite this article: T. Danelian et al., C. R. Geoscience 337 (2005). 相似文献
4.
Clumped-isotope geochemistry deals with the state of ordering of rare isotopes in molecules, in particular with their tendency to form bonds with other rare isotopes rather than with the most abundant ones. Among its possible applications, carbonate clumped-isotope thermometry is the one that has gained most attention because of the wide potential of applications in many disciplines of the earth sciences. In particular, it allows reconstructing the temperature of formation of carbonate minerals without knowledge of the isotopic composition of the water from which they were formed. In addition, the O isotope composition of the waters from which they were formed can be calculated using the δ18O of the same carbonate sample. This feature offers new approaches in paleoclimatology for reconstructing past global geochemical cycles. In this contribution two applications of this method are presented. First the potential of a new analytical method of measurement of clumped isotopes on small samples of foraminifera, for high-resolution SST and seawater δ18O reconstructions from marine sediments is shown. Furthermore the potential of clumped isotope analysis of belemnites, for reconstructing seawater δ18O and temperatures in the Cretaceous is shown. 相似文献
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This study focuses on the morphometry and taxonomy of the Late Cretaceous coccolith genus Arkhangelskiella. Sixty samples from the Campanian–Maastrichtian interval of DSDP Hole 390A (Blake Nose) were investigated for their contents of Arkhangelskiella spp. In each sample one hundred specimens of Arkhangelskiella spp. were examined by measuring the coccolith length and width, as well as the length and width of the central area. In the samples investigated the Arkhangelskiella group exhibits a large size variation, specimens length varies from 4.95 μm to 14.52 μm. Former taxonomic concepts, based on morphometry, subdivided the Arkhangelskiella group into three species: Arkhangelskiella maastrichtiana, Arkhangelskiella confusa and Arkhangelskiella cymbiformis. Our data show a large variability of the morphometric data (coccolith length, width of the outer rim). There is no indication for three independant species; two of the quoted taxa (1. thick outer rim = Arkhangelskiella maastrichtiana; 2. very thin outer rim = Arkkhangelskiella cymbiformis) seem to be extreme forms of a continuous morphometric lineage. The lower part of the investigated succession (139.92–133.42 mbsf) is dominated by small specimens with an average length of 6.8 μm whereas the upper part (132.86–126.15 mbsf) is characterized by larger specimens (mean 8.7 μm). In DSDP Hole 390A the size increase appears to be very abrupt, within two samples (samples 133.42 mbsf, 132.86 mbsf) the mean size increases by 1.51 μm. Previous morphometric studies of Arkhangelskiella indicate a more continuous size increase throughout the late Campanian–Maastrichtian. The abrupt size increase observed here hints toward a minor hiatus in DSDP Hole 390A separating upper Campanian from lower Maastrichtian sediments. It seems likely that the size increase of Arkhangelskiella reflects changes of various environmental factors like nutrient supply and sea water chemistry (Mg/Ca ratio; Ca concentration). A comparison of morphometric results with previous palaeoecological studies documents a nutrient control for the growth of Arkhangelskiella. Small specimens can be related to more mesotrophic conditions whereas large specimens are linked to oligotrophic surface waters. 相似文献
6.
Ibtisam Beik Victor Giraldo Gómez Olaf G. Podlaha Jörg Mutterlose 《Arabian Journal of Geosciences》2017,10(15):346
The purpose of this study is to better understand the depositional setting of Late Cretaceous to Early Paleocene oil shales from southeast and central-east Jordan. One core from both the Jafr and the Azraq-Hamza Basins was logged, and their lithology, texture, and ichnofabrics were recorded. A total of 79 thin sections were analyzed petrographically, and eight microfacies types recognized. Both cores show lithologic and petrographic similarities. The oil shales are Maastrichtian to Danian in age and can be described as organic matter and calcite-rich mudrocks. The most abundant granular components are foraminifera and various types of phosphatic bio- and lithoclasts. Macrofossils (bivalves, ostracods, echinoderms) were recorded in some intervals. The current results were compared with data from a previous publication on Maastrichtian oil shales from the Jafr Basin. A new model explaining the deposition of the oil shales of the Jafr and Azraq-Hamza Basins is proposed. The onset of the Maastrichtian oil shale deposition in both basins coincides with the early Maastrichtian transgression in this region. The organic matter-rich sediments were deposited in a mid to outer ramp setting below the storm wave base. Younger oil shales of Late Maastrichtian to Danian age were deposited in a shallower environment, below the fair weather wave base. The Cretaceous/Paleogene boundary is marked by a hiatus in both cores. The Danian oil shales show relatively lower “total organic carbon” content than the Maastrichtian ones. The former are believed to have been deposited in more oxygenated bottom waters of a mid-ramp zone. 相似文献
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The fracture-bound deposit at the Sieringhoek (Bentheim) bitumen mine in NW Germany has yielded a substantial quantity of bitumen ore. Emplacement of the bitumen into the fracture system occurred under high pressure, causing brecciation and impregnation of the host Gildehaus Sandstone. Subsequently the bitumen was brecciated and cemented by calcite and calcite-entrained sand. Bitumen injection followed fracturing into a hydro-carbon reservoir at depth, generated from a Jurassic/Cretaceous source rock. Diagenesis of the host rock was largely completed by the time of bitumen injection, reflecting the long time gap during which source rock maturation occurred. Impurities in the bitumen include large quantities of rock fragments, abraded during injection, and crystals of metal oxides and sulphides. 相似文献
9.
Nannoplankton successions in the northern Red Sea during the last glaciation (60 to 14.5 ka BP): Reactions to climate change 总被引：1，自引：0，他引：1
Heiko-Lars Legge Jrg Mutterlose Helge W. Arz Jürgen Ptzold 《Earth and Planetary Science Letters》2008,270(3-4):271-279
Due to its restricted connection with the Indian Ocean, the desert-enclosed Red Sea is extremely sensitive to global sea level changes and thus ideally suited for paleoceanographic studies of what occurred during the last glaciation. The understanding of its glacial history is, however, still limited. A serious obstacle to obtain satisfactory paleoecological information has been the rarity of microfossil proxy species caused by high salinities. Here, we present a continuous and well-dated calcareous nannoplankton record from the northern Red Sea, covering the interval from 60–14.5 ka BP. Our investigation shows that the composition of the calcareous nannoplankton community varied between 32 ka BP and 14.5 ka BP in response to rapid environmental changes which are closely correlated to climatic fluctuations described from the North Atlantic region. Heinrich events H3, H2 and H1 are dominated by Emiliania huxleyi. Gephyrocapsa oceanica and especially Gephyrocapsa ericsonii are abundant between H3–H2 and H2–H1. A less pronounced response of the calcareous nannoplankton to the high latitudinal climatic oscillations is documented prior to 32 ka BP, suggesting that a strong atmospheric coupling between the northern Red Sea and the North Atlantic realm was established in the late Marine Isotope Stage 3. In contrast to the previously held view of a sea level related salinity increase as the major cause for changes of the plankton communities within the glacial Red Sea, we interpret the documented variations as being caused by local hydrographic changes under the atmospheric control from the extratropics. Temperature changes and especially variations of the water stratification appear to be critical selective factors for the calcareous nannoplankton composition. 相似文献
10.
Marine sediments of Early Cretaceous age (Berriasian–Albian) have a widespread distribution in the Lower Saxony Basin of northern Germany. This basin, which is about 400 km long and 100 km wide, formed the southernmost extension of the North Sea Basin. Sediments attaining a maximum thickness of up to several hundred metres are represented by shallow marine siliciclastics in the west, south and easternmost part of the basin. These interfinger with the basin facies represented by dark mudstones up to 2000 m thick. The distribution and facies patterns of the sediments as well as thicknesses are related to three factors: differential subsidence, local tectonics and sea-level changes. For various parts of the basin and certain stratigraphic intervals it is possible to distinguish between these causes. Sedimentary thicknesses are clearly a result of differential subsidence from Kimmeridgian to Albian times onwards, being controlled by tectonic movements along northwest–southeast trending faults. These result in an asymmetric trough, bound to the north and south by synsedimentary faults with sedimentation rates highest in the north. Local tectonics are clearly caused by salt diapirs mainly in the eastern part of the basin and along the western, southern and eastern margins. These areas in particular include parts of the western Emsland and the Salzgitter area. Sedimentary patterns vary considerably over less than a kilometre, showing an extreme range of different lithologies. This is ideally observed in the Salzgitter area. Sea-level changes finally are reflected by widespread facies patterns and particularly by fossils of different provenance. The following sea-level-related events can be followed throughout the basin: the Wealden regressive phase, the Early Valanginian transgression, the early Late Valanginian transgression, the mid Hauterivian transgression, the Barremian regression, deposition of the Early Aptian anoxic sediments, and accumulation of the mid Albian hemipelagic marls. 相似文献