Subducting volcaniclastic-rich upper crust supplies fluids for shallow megathrust and slow slip

Recurring slow slip along near-trench megathrust faults occurs at many subduction zones, but for unknown reasons, this process is not universal. Fluid overpressures are implicated in encouraging slow slip; however, links between slow slip, fluid content, and hydrogeology remain poorly known in natural systems. Three-dimensional seismic imaging and ocean drilling at the Hikurangi margin reveal a widespread and previously unknown fluid reservoir within the extensively hydrated (up to 47 vol % H2O) volcanic upper crust of the subducting Hikurangi Plateau large igneous province. This ~1.5 km thick volcaniclastic upper crust readily dewaters with subduction but retains half of its fluid content upon reaching regions with well-characterized slow slip. We suggest that volcaniclastic-rich upper crust at volcanic plateaus and seamounts is a major source of water that contributes to the fluid budget in subduction zones and may drive fluid overpressures along the megathrust that give rise to frequent shallow slow slip

Tying seismic data to geologic information from core data: an example from ODP Leg 177

The integration of seismic data with core data provides ground-truth toa structural interpretation of seismic data.The most important difficulty that arises in an integration effort isthe correct translation between the different scales of the core dataand the seismic data.In the absence of check-shots, detailed knowledge of the velocitystructure at the drilling locations is required, either from downholelogging measurements, velocity analysis of the seismic data, or directmeasurements on core samples.Three of the seven drill-sites during ODP (Ocean Drilling Program) Leg177 in the south-eastern Atlantic were located on the Agulhas Ridge andconnected through eight seismic profiles.Synthetic seismograms created from velocity and density measurements onselected core samples generally show a good agreement with real seismicdata with respect to amplitude and waveform, whereas timing of theevents is troublesome.The use of velocity profiles with inaccurate sections along cores, afalse depth scale due to recovery problems, and inaccuracies in thepositioning during both seismic and coring operations are the mainshortcomings of this method.The main reflectors identified on seismic data correspond to hiatuses orperiods of reduced sedimentation rates, and correlate well with densityvariations.In this way the cored data provide a calibration tool for the overallgeological interpretation of the seismic sections

Stabilists strike again

ON page 412 of this issue1, Sugden and colleagues announce that glacier ice in the Dry valleys of East Antarctica seems to have survived for over 8 million years under a thin layer of sediment. This, they argue, testifies that stable polar conditions have persisted for at least that time

Orbitally induced oscillations in the East Antarctic ice sheet at the Oligocene/Miocene boundary

Between 34 and 15 million years (Myr) ago, when planetary temperatures were 3–4 °C warmer than at present and atmospheric CO2 concentrations were twice as high as today1, the Antarctic ice sheets may have been unstable2, 3, 4, 5, 6, 7. Oxygen isotope records from deep-sea sediment cores suggest that during this time fluctuations in global temperatures and high-latitude continental ice volumes were influenced by orbital cycles8, 9, 10. But it has hitherto not been possible to calibrate the inferred changes in ice volume with direct evidence for oscillations of the Antarctic ice sheets11. Here we present sediment data from shallow marine cores in the western Ross Sea that exhibit well dated cyclic variations, and which link the extent of the East Antarctic ice sheet directly to orbital cycles during the Oligocene/Miocene transition (24.1–23.7 Myr ago). Three rapidly deposited glacimarine sequences are constrained to a period of less than 450 kyr by our age model, suggesting that orbital influences at the frequencies of obliquity (40 kyr) and eccentricity (125 kyr) controlled the oscillations of the ice margin at that time. An erosional hiatus covering 250 kyr provides direct evidence for a major episode of global cooling and ice-sheet expansion about 23.7 Myr ago, which had previously been inferred from oxygen isotope data (Mi1 event5)