Late stage slope failure in the wake of the 1929 Grand Banks earthquake

Small volume (<15 km³) debris flows which were triggered by the 1929 earthquake postdate the period of high velocity turbidity current flow resulting from that earthquake. They thus could not have contributed sediment to the 1929 cable-breaking turbidity currents. Both the proposed “Grand Banks Slump” and another large scale debris flow also attributed to the 1929 event, are shown to be autochthonous. In light of the limited volume and late-stage timing of mass wasting on the upper Laurentian Fan in 1929, an additional mechanism must have existed which supplied further sediment to the turbidity current in 1929.     

Conditions during syntectonic vein formation in the footwall of the Absaroka Thrust Fault, Idaho–Wyoming–Utah fold and thrust belt

The Twin Creek Limestone in the footwall of the Absaroka thrust sheet contains three sets of bed-normal syntectonic calcite veins. Vein formation occurred during Cretaceous motion along the Absaroka thrust fault as indicated by (1) crosscutting relationships among these vein sets, (2) a previously dated solution cleavage, and (3) calcite twin analysis. Fluid inclusions in the veins and overburden estimates constrain inclusion entrapment temperatures to be between 175 °C and 328 °C. Results from stable oxygen isotopes indicate that the host and vein fluid compositions were in near isotopic equilibrium. Applying both reasonable geothermal gradients and constraints on overburden temperature yields fluid pressures during vein precipitation that are near hydrostatic. All data taken together suggest both that vein formation within the Twin Creek Formation occurred in a relatively closed system, and that the veins filled near hydrostatic fluid pressure. Because the veins fill precursory cracks, vein filling might not reflect the maximum fluid pressure that existed during the complete vein forming process.     

Arm hooks of coleoid cephalopods from the Jurassic succession of the Wessex Basin,Southern England

The Jurassic succession of the Wessex Basin – especially that cropping out within the Dorset and East Devon Coast World Heritage Site – contains important lagerstätten for coleoid cephalopods. The Blue Lias and Charmouth Mudstone formations of West Dorset, the Oxford Clay Formation of North Wiltshire and the Kimmeridge Clay Formation of Purbeck have provided large numbers of important body fossils that inform our knowledge of coleoid palaeobiology, including the hooks present in the arms. Isolated hooks are also found in the processed residues studied by micropalaeontologists and these occurrences can be used – in some cases – to record the presence of key taxa in the absence of well-preserved body fossils. While some hook morphotypes can be attributed to known species, there are many forms of hook described where the parent animal remains unknown. The present state of our knowledge of the Jurassic assemblages in the Wessex Basin is presented and remaining issues identified.     

Antecedent aeolian dune topographic control on carbonate and evaporite facies: Middle Jurassic Todilto Member,Wanakah Formation,Ghost Ranch,New Mexico,USA

The Middle Jurassic Todilto Member of the Wanakah Formation is a carbonate and gypsum unit inset into the underlying aeolian Entrada Sandstone in the San Juan Basin. Field and thin section study of the uppermost Entrada and Todilto at Ghost Ranch, New Mexico, identified Todilto facies and their relationship to remnant Entrada dune topography. Results support the previous interpretation that the Entrada dunes, housed in a basin below sea level, were rapidly flooded by marine waters. Mass wasting of the dunes gave rise to sediment‐gravity flows that largely buried remnant dune topography, leaving ca 12 m of relief that defined the antecedent condition for Todilto deposition. Previously interpreted as seasonal varves deposited in a stratified water body, the Todilto is reinterpreted as a microbial biolaminite. Most diagnostic are organic‐rich laminae with structures characteristic of filamentous microbes and containing trapped aeolian silt, and clotted‐texture laminae with a fabric associated with calcification of extracellular polymeric substances. The spatial arrangement of Todilto facies is controlled by the dune palaeotopography. A continuous basal laminated mudstone thickens over the dune crest, reflecting the optimum conditions for microbial mat development, and is interpreted to have been deposited when marine waters submerged the topography. Subsequent drying caused emergence of the crestal area, and formation of tepee structures and a dissolution breccia. Gypsiferous mudflats and periodic ponds occupied the dune flanks and interdune area, with gypsum concentrated within the interdune area. Entrada sands remained unstable during Todilto deposition with common injection structures into the Todilto, and a remnant slope caused the downslope movement and folding of Todilto strata on the upper lee face. Although some expansion of the gypsum occurred in the subsurface, facies architecture fostered development of a dissolution front adjacent to the interdune gypsum body with section collapse of gypsiferous limestone on the dune flanks.     

Palaeoglaciation of Parque Natural Lago de Sanabria, northwest Spain

Detailed geomorphological mapping provides evidence for at least three phases of glaciation in the Parque Natural Lago de Sanabria, in northwest Spain. The most extensive glaciation was characterised by a large plateau ice cap. A combination of geomorphological evidence and glacier modelling indicates that this ice cap covered an area of more than 440 km², with a maximum ice thickness of c. 300 m and outlet glaciers reaching as low as 1000 m. This represents the largest ice mass in Iberia outside the Pyrenees and one of the largest in the mountains of southern Europe and the Mediterranean region. Radiocarbon dates from the base of lacustrine sequences appear to suggest that the most extensive phase of ice-cap glaciation occurred during the last cold stage (Weichselian) with deglaciation occurring before 14–15 ka ¹⁴C BP. A second phase of glaciation is recorded by the moraines of valley glaciers, which may have drained small plateau ice caps; whilst a final phase of glaciation is recorded by moraines in the highest cirques.     

An examination of groundwater within the Hawara Pyramid,Egypt

The Hawara Pyramid is an outstanding monument. However, the mudbrick structure shows signs of erosion, and the passages and chambers are currently submerged. The problem of water ingress has mainly arisen since the 1880s. In this study, an initial assessment of the pyramid structure was made and causes of water ingress were investigated through analysis of water samples. Stable oxygen isotope measurements indicate that the source of water within the pyramid is the Bahr Selah canal. Water within the pyramid is highly saline compared to the Bahr Selah, and evaporation can only partly account for this high salinity. The composition of dissolved ions suggests that dissolution of salts in soils and from bedrock in the vicinity of the pyramid has enhanced the salinity of water percolating into the pyramid structure. Water ingress and salt deposition are at present the main threat to the integrity of the monument. © 2007 Wiley Periodicals, Inc.