Earth and Planetary Science Letters最新文献

Southeast Tibet is characterized by low-relief surfaces at high-elevation, showing very little exhumation during the India–Asia collision, as well as deeply incised rivers valleys. Understanding how these low-relief surfaces adjacent to the plateau's edge survived from regressive fluvial erosion is still an enigma, which is key to understanding the formation of the plateau. In the Three Rivers Region around the Eastern Himalayan Syntaxis, the squeezing of the Salween, Mekong and Yangtze rivers’ drainage basins in their middlestream, where numerous thrusts parallel to the river channels are observed, has been invoked as the key factor driving the river evolution. More to the east, in the Great Bends Region, no such squeezing of the drainage basins has been observed; the Yalong and Yangtze rivers flow perpendicularly across northeast-trending thrust belts, generating huge (>100 km) river course bends with steep channel slopes. These faults have significantly contributed to construct the high plateau margin, including the Yalong Thrust Belt (YTB), active during the Eocene (∼35–25 Ma) and reactivated in the Miocene (15–12 Ma). By applying state-of-the-art landscape modelling (FastScape) to the Yalong River catchment, with simplified rock uplift scenario deduced from fault activities, we show that strong monsoonal precipitation on the plateau (∼1 m/yr), even during only a short period such as the Mid–Miocene Climatic Optimum (17–14 Ma), produces wide rivers and destroys the plateau edge. In contrast, modelling the orographic effect with weak net precipitation (∼0.2 m/yr) above ∼2700 or 4000 m, preserves the plateau edge and reproduces the slope of the Yalong River, but with a width larger than in nature. To reproduce both the slope and narrowness of the Yalong gorge just upstream of the YTB, a combination of a rapid Miocene rock uplift leading to a regional surface uplift, which creates a significant orographic effect and preserves interfluve low-relief surfaces close to the plateau edge, and a water inflow in upstream, which deeply incises downstream river valleys, is necessary. Such an amount of upstream water is collected from the flat and expansive headwater, inherited from the inland endorheic zone of the plateau interior, on which the hillslope processes dominate the landscape evolution.

This study reconstructs the upwelling history of the Southern Benguela Upwelling System (SBUS), examining its sensitivity to both regional and global climatic influences. We analyze planktic foraminiferal relative abundance and stable isotope data from ODP Site 1087 to investigate the history of SBUS since ∼ 6.1 Ma. During the latest Miocene-earliest Pliocene, the SBUS experienced increased productivity, fueled by wind-driven upwelling and an enriched global nutrient reservoir associated with the late Miocene biogenic bloom. The early Pliocene witnessed an apparent weakening of the SBUS due to the deepening of the global thermocline and weak trade winds. Significantly, our proxy records indicate strengthening of the SBUS beginning before the onset of intense northern hemisphere glaciation (iNHG) between 3.5 and 3 Ma. Despite contraction of upwelling cells after ∼ 3 Ma, our study challenges the notion of water column stability during the Matuyama Diatom Maximum event (3 to 2 Ma); we alternatively propose the existence of water column instability and probable presence of upwelling during this time. Post 2 Ma, the main upwelling cells shifted northward in response to the strengthening and equatorward migration of the Hadley cell, marked by long-term marginal upwelling. The SBUS achieved its modern state by ∼ 1 Ma with complete isolation from the coastal upwelling zone. Our observations indicate a strong correlation between the history of SBUS and global climatic events, with a strong correlation between them prior to the initiation of iNHG. Subsequently, local climatic influences have become more predominant, overshadowing the signals from global climatic events. The data also suggest linkages between shifts in the SBUS strengths and southwest African climate.

The extent of volatile elements on the surface and interior of the Moon remains a highly debated topic. Previous studies conducted on bulk lunar soil samples and solar wind samples collected by the Genesis mission indicate a discernible isotope mass- or non-mass-dependent fractionation of krypton and xenon. However, a detailed investigation of these processes is missing, particularly in determining the possible incorporation of cometary volatiles in the lunar regolith. New lunar soil samples returned by the Chang'e-5 mission provide a chance to answer these key questions. In this study, noble gas isotopes of nine subsamples from a Chang'e-5 scooped sample were analysed through stepwise-heating and total fusion laser extraction. The results reveal that a simple binary mixture of solar wind and cosmogenic components did not explain alone the isotopic composition of these samples. The Xe data shows insignificant amounts of atmospheric Xe and presents clear evidence of cometary contributions to the lunar regolith, with a significant depletion of ^134,136Xe compared to that in the solar wind. Additionally, a meteoritic component is identified. Compared to the Apollo results, our findings further validate the theory of Earth's atmospheric escape, substantiate the plausibility of these exogenous admixtures to elucidate the isotopic fractionation mechanisms of Kr and Xe within the lunar regolith, and provide novel insights into long-term constancy in the solar wind composition.

The elastic interaction between an inclusion and its host is often employed to study metamorphic processes based on the assumption that the host is not affected by processes such as creep that irreversibly releases stress. However, it is not well understood how fast inelastic relaxation of stress may occur and under what conditions the elastic regime holds for each inclusion-host system. To provide new constraints for the widely used systems of quartz and zircon inclusions in garnet, we performed heating experiments on almandine-pyrope and spessartine garnets under graphite, N₂+H₂, or H₂O+Ar fluxed conditions at different temperatures. Raman spectroscopy was used to measure the same quartz and zircon inclusions after different heating times. The Raman-band wavenumbers undergo time-dependent decreases in quartz inclusions and increase in zircon inclusions under H₂O+Ar conditions and exhibit a greater final shift than under graphite and N₂+H₂ buffered conditions. Under graphite-buffered conditions, the wavenumbers of Raman bands measured on zircon and quartz stabilise after the first heating step, after which no change was observed. Electron backscatter diffraction results reveal greater misorientation around the heated inclusions compared to unheated inclusions, implying a greater dislocation density after heating. Raman mapping reveals that stress heterogeneity in the garnet host develops at an early stage of heating and fades away afterward, indicating dispersal of dislocations into the host. Fitting a visco-elastic model to the Raman data of garnet fluxed with N₂+H₂ or Ar+H₂O allows an estimate of flow-law parameters for garnet around quartz inclusions, similar to those obtained by conventional deformation experiments. The results demonstrate the weakening effect of aqueous fluid on garnet. The data also indicate that the garnet can hold inclusion pressure at elevated temperatures under a dry and reducing environment. This study provides information on the relaxation rate of pressurized inclusions in garnet at different temperatures and within different external environments. Furthermore, the use of inclusion-host pairs for studying creep processes offers a complementary approach to conventional deformation experiments to better understand the rheological behaviour of earth materials.

We report the H, C, and N isotopic compositions of microscale (0.2 to 2 µm) organic matter in samples of asteroid Ryugu and the Orgueil CI carbonaceous chondrite. Three regolith particles of asteroid Ryugu, returned by the Hayabusa2 spacecraft, and several fragments of Orgueil were analyzed by NanoSIMS isotopic imaging. The isotopic distributions of the Ryugu samples from two different collection spots are closely similar to each other and to the Orgueil samples, strengthening the proposed Ryugu-CI chondrite connection. Most individual sub-μm organic grains have isotopic compositions within error of bulk values, but 2–10 % of them are outliers exhibiting large isotopic enrichments or depletions in D, ¹⁵N, and/or ¹³C. The H, C and N isotopic compositions of the outliers are not correlated with each other: while some organic grains are both D- and ¹⁵N-enriched, many are enriched or depleted in one or the other system. This most likely points to a diversity in isotopic fractionation pathways and thus diversity in the local formation environments for the individual outlier grains. The observation of a relatively small population of isotopic outlier grains can be explained either by escape from nebular and/or parent body homogenization of carbonaceous precursor material or addition of later isotopic outlier grains. The strong chemical similarity of isotopically typical and isotopically outlying grains, as reflected by synchrotron x-ray absorption spectra, suggests a genetic connection and thus favors the former, homogenization scenario. However, the fact that even the least altered meteorites show the same pattern of a small population of outliers on top of a larger population of homogenized grains indicates that some or most of the homogenization occurred prior to accretion of the macromolecular organic grains into asteroidal parent bodies.

Seismic velocity changes in earthquake cycles have been observed over a wide range of timescales and may be a good indicator of the onset of future earthquakes. Understanding the effects of precursory velocity changes right before seismic and slow-slip events could potentially elucidate the onset and timing of fault failure. We use numerical models to simulate fully dynamic earthquake cycles in 2D strike-slip fault systems with antiplane geometry, surrounded by a narrow fault-parallel damage zone. By imposing S-wave velocity changes inside fault damage zones, we investigate the effects of these precursors on multiple stages of the seismic cycle, including nucleation, coseismic, postseismic, and interseismic stages. Our modeling results show a wide spectrum of fault slip behaviors including fast earthquakes, slow-slip events, and variable creep. One primary effect of the imposed velocity precursor is on the earthquake nucleation phase, and earlier onset of precursors causes earthquakes to nucleate sooner with a smaller nucleation size that is not predicted by theoretical equations. Furthermore, such precursors affect the nucleation of dynamic earthquakes and slow-slip events. Our results highlight the importance of short- and long-term monitoring of fault zone structures for better assessment of regional seismic hazard.

Quantitative analysis of fluvial topography and sediment yield changes are often independently used to detect major river capture events and episodes of drainage reorganization. Here we use a unique set of geological and in situ ¹⁰Be cosmogenic data from Corsica, Western Mediterranean, to provide evidence of major river capture events affecting the former Paleo-Ostriconi river catchment during the Pliocene, and to illustrate how the landscape of Corsica is still reacting to the disequilibrium caused by the late Miocene uplift of Alpine Corsica. We found that ∼1280 km² of basin area originally draining towards the Ligurian Sea were abruptly connected to the Tyrrhenian Sea by the capturing Tavignano and Golo rivers, which led to the formation of a large Pliocene-Quaternary submarine fan offshore the Tyrrhenian coast. The increased sediment yield towards the Tyrrhenian margin after river capture in the Pliocene was three times greater than the average sediment yield in the same source-to-sink system during the Holocene (410±100 t·km⁻²·a ^{− 1} vs ∼131±8 t·km⁻²·a ^{− 1}) and greater magnitude than any subsequent peaks in sediment yield during late Pleistocene glaciations. ¹⁰Be-derived denudation rates reveal that focused erosion still affects retreating knickpoints near the sites of former river capture in central Corsica, suggesting persistence of landscape disequilibrium for several millions of years. Our results demonstrate the potentially large impact of river capture on the stratigraphic record and highlight the importance of full consideration of landscape response times to onshore disturbances for any reliable interpretation of the offshore sedimentary archive.

The subdivision and correlation of the Ediacaran System within the geologic timescale is desirable, but challenging. The Ediacaran Doushantuo Formation (∼635–550 Ma) in South China is one of the most important sedimentary successions for studying the co-evolution of Earth's environment and life at that time. However, its stratigraphic continuity is confusing and deserves scrutiny. In this study we evaluate stratigraphic continuity of the Doushantuo Formation from a key section deposited in an alleged deep-water “basinal” setting. Using litho-, chemo-, and chrono-stratigraphic data anchored by two new CA-ID-TIMS U-Pb zircon dates of 629.7 Ma and 556.4 Ma from two tuff layers, we reveal that this section contains a cryptic subaerial unconformity with a >44 Myr gap in the sedimentary record. The unconformity occurs immediately prior to the EN3/Shuram δ¹³C excursion in the mid-Ediacaran, and can be traced regionally and may be correlative to other mid-Ediacaran unconformities globally. We suggest that its development is related to glacio-eustatic sea-level changes during the mid-Ediacaran. This finding provides a critical stratigraphic boundary for future subdivision and correlation of the Ediacaran System in South China, and we advocate for a reconsideration of the completeness of the Ediacaran stratigraphic record in this area.

During International Ocean Discovery Program (IODP) Expedition 366 cores were recovered from three serpentinite mud volcanoes containing clasts that originate from the subduction-channel along the Philippine Sea Plate – Pacific Plate boundary. The drilled and sampled mud volcanoes (Yinazao, Fantangisña, and Asùt Tesoru) are located at distances of 55 to 72 km from the Mariana Trench. Mafic rock clasts, embedded within a serpentinite mud matrix, from the flanks and summits of both Asùt Tesoru and Fantangisña Seamounts were analyzed for reconstruction of their metamorphic and deformational overprint in order to reveal the tectono-metamorphic conditions at the metamorphic peak within the subduction channel and the subsequent low-grade overprint during exhumation. Several seamounts comprise clasts of lower plate metabasites with different metamorphic overprint (from low-grade sub-greenschist facies to lower blueschist facies). The metabasites are also associated with clasts of fossiliferous carbonates and cherts with different degrees of metamorphic and deformational overprint, that also originated from the Pacific lower Plate. This implies that these rocks were exhumed from different depths within the subduction channel before being regurgitated within a serpentinite mud matrix. The blueschist facies metamorphic rocks, being affected by metamorphic pressures in the range of 11 to 13.8 kbar at minimum, were very likely exhumed from greater depth within the subduction channel before being captured by uprising, localized serpentinite mudflows, indicating evidence that corner flow is actually taking place along the Mariana convergent margin, and that the high-pressure rocks were exhumed by corner flow in an active subduction zone. Final exhumation, however, is related to the embedding of the rocks within a serpentinite mud matrix and the buoyant ascent of serpentinite mudflows along forearc fracture zones extending from the plate boundary to the upper plate sea floor.

Fault asperities can produce concentrated slips during large earthquakes and intensify damage. However, how asperities control fault behavior during other phases of the earthquake cycle remains poorly known. Here, we conduct friction experiment on a laboratory fault featuring two prominent geometric asperities to directly image their influences on long-term and short-term seismicity, and the nucleation and propagation of the mainshock. The laboratory observations and supporting numerical simulations reveal that one asperity located in the fault interior behaves firstly as a mechanical attractor to long-term seismicity, then a barrier to preseismic slow slip, and ultimately a source of large coseismic slip. In contrast, another asperity located near the fault margin primarily undergoes persistent aseismic slip throughout most phases of the earthquake cycle. These results provide new insights into how asperities partition strain across a broad spatiotemporal domain, establishing a physical link between long-term and short-term fault behaviors and the occurrence of large earthquakes.