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The effects of trivalent cations (Al and Fe) on the grain growth rates of bridgmanite 三价阳离子(铝和铁)对桥粒石晶粒长大速率的影响
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-05 DOI: 10.1016/j.epsl.2024.118983

Trivalent cations such as Al3+ and Fe3+ can be incorporated into the crystal structure of bridgmanite either by the charge-coupled mechanism forming the FeFeO3, AlAlO3, and FeAlO3 components or by the oxygen vacancy mechanism forming the MgAlO2.5 and MgFeO2.5 components. They may affect the physical properties of bridgmanite and thus affect lower mantle dynamics. In this study, we investigated the effects of Al and Fe3+ on the grain growth kinetics of bridgmanite at a pressure of 27 GPa and temperatures of 2000 – 2300 K by multi anvil experiments. The experimental results indicate that the FeFeO3, AlAlO3, and FeAlO3 components enhance the growth rate of bridgmanite, while the MgAlO2.5 and MgFeO2.5 components have negligible effects. However, due to the relatively low Fe3+ and Al3+ contents of bridgmanite in the lower mantle, none of them affect the lower mantle rheology significantly. In particular, the mid-mantle viscosity jump interpreted from geoid analysis is unlikely to be caused by the decreasing of MgAlO2.5 and MgFeO2.5 concentrations with increasing depth.

Al3+和Fe3+等三价阳离子可通过电荷耦合机制掺入桥芒石晶体结构,形成FeFeO3、AlAlO3和FeAlO3成分,或通过氧空位机制掺入桥芒石晶体结构,形成MgAlO2.5和MgFeO2.5成分。它们可能会影响桥芒石的物理性质,从而影响下地幔动力学。在本研究中,我们通过多砧实验研究了在压力为 27 GPa、温度为 2000 - 2300 K 的条件下,Al 和 Fe3+ 对桥芒石晶粒生长动力学的影响。实验结果表明,FeFeO3、AlAlO3 和 FeAlO3 成分能提高桥芒石的生长速度,而 MgAlO2.5 和 MgFeO2.5 成分的影响可以忽略不计。然而,由于下地幔中桥粒石的 Fe3+ 和 Al3+ 含量相对较低,它们都不会对下地幔流变学产生显著影响。特别是,根据大地水准面分析解释的中幔粘度跃变不太可能是由 MgAlO2.5 和 MgFeO2.5 浓度随深度增加而降低引起的。
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引用次数: 0
A threshold in submarine channel curvature explains erosion rate and type 海底河道曲率的临界值解释了侵蚀速度和类型
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-05 DOI: 10.1016/j.epsl.2024.118953

Submarine channels are conduits for sediment-laden flows called turbidity currents, which play a globally significant role in the offshore transport of sediment and organic carbon and pose a hazard to critical seafloor infrastructure. Time-lapse repeat surveys of active submarine channels have recently shown that upstream-migrating knickpoints can dominate channel evolution. This finding contrasts with many studies of ancient outcrops and subsurface geophysical data that inferred channel bends migrate laterally, as occurs in meandering rivers. Here, we aim to test these two contrasting views by analysing two high-resolution repeat seafloor surveys acquired 13 years apart across the entirety of an active submarine channel in Knight Inlet, British Columbia. We find that two main mechanisms control channel evolution, with the normalised channel radius of curvature (specifically, R* - channel radius of curvature normalised to channel width) explaining which of these mechanisms dominate. Pronounced outer bend migration only occurs at tight bends (R*<1.5). In contrast, at broader bends and straighter sections (R*>1.5), erosion is focused within the channel axis, where upstream-migrating knickpoints dominate. High centrifugal accelerations at tight bends promote super-elevation of flows on the outer channel flank, thus, enhancing outer bend erosion. At R*>1.5, flow is focused within the channel axis, promoting knickpoints that migrate upstream at an order of magnitude faster than the rate of outer bend erosion at tight bends. Despite the dominance of knickpoints in eroding the channel axis, their stratigraphic preservation is very low. In contrast, the lateral migration of channel bends results in much higher preservation via lateral accretion of deposits on the inner bend. We conclude that multiple mechanisms can control evolution at different channel reaches and that the role of knickpoints has been underestimated from past studies that focused on deposits due to their low preservation potential.

海底通道是被称为浊流的富含沉积物的水流的通道,在沉积物和有机碳的近海输送中发挥着全球性的重要作用,并对重要的海底基础设施造成危害。对活跃的海底通道进行的延时重复勘测最近表明,上游移动的节点可以主导通道的演变。这一发现与许多对古露头和地下地球物理数据的研究形成鲜明对比,后者推断河道弯曲是横向迁移的,就像蜿蜒的河流一样。在这里,我们通过分析在不列颠哥伦比亚省奈特湾(Knight Inlet)的整个活跃海底航道上两次相隔 13 年采集的高分辨率重复海底勘测数据,旨在检验这两种截然不同的观点。我们发现,有两种主要机制控制着海峡的演变,而归一化的海峡曲率半径(具体来说,R* - 归一化为海峡宽度的海峡曲率半径)可以解释其中哪种机制占主导地位。明显的外弯曲迁移只发生在狭小的弯曲处(R*<1.5)。相比之下,在较宽的弯道和较直的河段(R*>1.5),侵蚀集中在河道轴线内,上游迁移的节点在此占主导地位。急弯处的高离心加速度会促进河道外侧的水流超高,从而加剧弯道外侧的侵蚀。在 R*>1.5条件下,水流集中在河道轴线内,促使节点向上游迁移,其迁移速度比紧弯处的外弯侵蚀速度快一个数量级。尽管节理点在侵蚀河道轴线方面占主导地位,但其地层保存率非常低。与此相反,河道弯曲处的横向迁移通过内弯曲处沉积物的横向增生,使地层保存率高得多。我们的结论是,多种机制可以控制不同河道上游的演化,而过去以沉积物为重点的研究低估了节理点的作用,因为它们的保存潜力很低。
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引用次数: 0
Constraining the evaporative loss of zinc during impact processes using terrestrial impact glasses 利用陆地撞击玻璃模拟撞击过程中锌的蒸发损失
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-04 DOI: 10.1016/j.epsl.2024.118979

Evaporation can fractionate elements and their isotopes between the condensed and gas phases. The fractionation of zinc isotopes during impact-induced evaporation can be used to effectively determine the extent of volatile loss. A robust understanding of the Zn isotope system in assessing the volatile loss, however, relies on well-constrained empirical isotopic fractionation factors (α) during evaporation under a range of pressure and temperature conditions. In this study, Zn isotopic data for well-documented impact glasses from six sites (Darwin, Australia; Zhamanshin, Kazakhstan; El'gygytgyn, Russia; Boltysh, Ukraine; Lonar, India; and Ries, Germany) are reported to investigate the extent of Zn isotopic fractionation under conditions of impact-induced evaporation on Earth. Our findings suggest that the initial Zn isotopic composition in terrestrial impact glasses is comparable to that of continental crustal rocks, but this composition becomes progressively heavier as more isotopically light Zn is lost from the impact melt, reaching a maximum δ66Zn value of +1.1 ‰. The investigated samples show a statistically significant negative correlation between δ66Zn values and Zn contents, especially those from the Darwin crater (R2 = 0.90). These samples define an α value of 0.99971 ± 0.00005 (1SE). This α value is consistent with those previously estimated for melt glasses and fused sands (α = 0.9997 to 0.9998) from the Trinity nuclear detonation site, slightly higher than the value estimated from tektites (α = ∼0.998), and notably higher than that theoretically expected for evaporation into a vacuum (α = 0.985 to 0.993). This result highlights the limited fractionation of Zn isotopes during terrestrial impact processes. Moreover, the modelling suggests that the range of α values from 0.9997 to 0.9998 aligns with the observed compositions in lunar mare basalts and products from nuclear detonation, supporting α values close to but not exactly unity for Zn isotopic fractionation during various high-energy impact events. Utilizing the modelled fractionation factor (α = 0.9997), it is possible to reproduce the Zn concentration and isotopic composition of the lunar mare basalts, indicating a loss of about 98 % of the Moon's initial Zn inventory. Terrestrial impact glasses demonstrate that, under natural impact conditions, stable Zn isotopes can undergo evaporative fractionation to a degree comparable to lunar mare basalts and melted fallout glass and fused sands from nuclear detonation, suggesting an important contribution from impact to the volatile depletion of terrestrial planets.

蒸发可以在凝结相和气相之间对元素及其同位素进行分馏。锌同位素在撞击诱导蒸发过程中的分馏可用于有效确定挥发损失的程度。然而,在评估挥发损失过程中对锌同位素系统的深入了解有赖于在一系列压力和温度条件下蒸发过程中受到良好约束的经验同位素分馏系数(α)。本研究报告了来自六个地点(澳大利亚达尔文、哈萨克斯坦扎曼申、俄罗斯叶尔吉特金、乌克兰波尔蒂什、印度隆纳尔和德国里斯)的有据可查的撞击玻璃的锌同位素数据,以研究地球上撞击引起的蒸发条件下锌同位素分馏的程度。我们的研究结果表明,陆地撞击玻璃的初始锌同位素组成与大陆地壳岩石相当,但随着更多同位素轻的锌从撞击熔体中流失,这种组成逐渐变重,δ66Zn 的最大值为 +1.1 ‰。所调查的样本显示,δ66Zn 值与锌含量之间存在统计学意义上的显著负相关,尤其是来自达尔文陨石坑的样本(R2 = 0.90)。这些样本的 α 值为 0.99971 ± 0.00005(1SE)。这个α值与之前对特尼狄核爆现场的熔融玻璃和熔融砂的估计值(α = 0.9997 到 0.9998)一致,略高于对沸石的估计值(α = ∼ 0.998),并且明显高于理论上对蒸发到真空中的预期值(α = 0.985 到 0.993)。这一结果凸显了锌同位素在陆地撞击过程中的有限分馏。此外,建模表明,0.9997 至 0.9998 的 α 值范围与观测到的月兔玄武岩和核爆炸产物的成分相吻合,支持在各种高能撞击事件中锌同位素分馏的 α 值接近但不完全是统一值。利用模拟的分馏系数(α = 0.9997),可以再现月球赤泥玄武岩的锌浓度和同位素组成,表明月球初始锌存量损失了约 98%。陆地撞击玻璃表明,在自然撞击条件下,稳定的锌同位素会发生蒸发分馏,其程度可与月兔玄武岩和核爆熔化的落尘玻璃和熔砂相媲美,这表明撞击对陆地行星的挥发性耗竭有重要作用。
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引用次数: 0
Arctic Alaska deepwater organic carbon burial and environmental changes during the late Albian–early Campanian (103–82 Ma) 北极阿拉斯加深水有机碳埋藏与阿尔卑斯晚期-坎帕尼亚早期(103-82 Ma)的环境变化
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118948

The middle Cretaceous greenhouse period experienced profound environmental change including episodes of enhanced global burial of organic carbon marked by carbon isotopic excursions (CIEs). However, the role and response of polar regions like the newly formed, partially enclosed Arctic Ocean Basin during middle Cretaceous carbon burial remains enigmatic. We present the first Arctic deepwater CIE record that characterizes conditions offshore of the Alaska margin north of 75°N paleolatitude. Organic carbon isotopes (δ13Corg) and 103–82 Ma ash zircon U-Pb dates from the distal Hue Shale record multiple Albian–Campanian CIEs during slow ∼3–15 m/Myr sediment accumulation rates. Average total organic carbon (TOC) increased substantially during large 2–3 ‰ CIEs of the ∼101 Ma Albian-Cenomanian boundary event (from 7 to 18 % TOC) and ∼94 Ma Cenomanian-Turonian boundary event (5 to 10 % TOC). Turonian TOC remained elevated (8–13 %) during high global sea levels and temperatures of the Cretaceous Thermal Maximum, followed by an increase from 7 to 11 % TOC during the ∼90 Ma late Turonian event 1.5 ‰ CIE. Average TOC subsequently decreased in the Coniacian–Campanian, but relative maxima occurred during subtle 0.5–1 ‰ CIEs interpreted as the ∼87 Ma late Coniacian event (increase from 4 to 7 % TOC), ∼85 Ma Horseshoe Bay event (3.5 to 4.5 % TOC), and ∼84 Ma Santonian-Campanian boundary event (3.5 to 5 % TOC). Increases in hydrogen index and productivity proxies (P, Ba, Nd) that accompanied each CIE episode with enhanced TOC suggest a strong link between marine productivity and organic carbon burial at short-term CIE timescales. However, long-term (>5–8 Myr) changes in trace metal redox (Mo, Fe, V) and salinity (B/Ga) proxies suggest shifts in prevailing environmental conditions at timescales longer than the CIEs. Late Albian–middle Turonian marine salinity occurred during euxinic (103–98 Ma) and suboxic (98–90 Ma) conditions with deposition interpreted to have occurred within and beneath an oxygen minimum zone, respectively. In contrast, late Turonian–early Campanian (90–82 Ma) freshening and restricted euxinic basin conditions may signal the start of widespread restriction known to characterize the Paleogene Arctic. Overall, these results highlight that middle Cretaceous Arctic deepwater remained a productive marine carbon sink coupled to the global carbon cycle despite evolving Arctic greenhouse conditions.

中白垩世温室时期经历了深刻的环境变化,包括以碳同位素偏移(CIEs)为标志的全球有机碳埋藏增强事件。然而,像新形成的、部分封闭的北冰洋盆地这样的极地地区在中白垩世碳埋藏过程中的作用和反应仍然是个谜。我们首次展示了北极深水 CIE 记录,该记录描述了古北纬 75° 以北阿拉斯加边缘近海的情况。来自远端顺化页岩的有机碳同位素(δ13Corg)和 103-82 Ma 灰锆石 U-Pb 日期记录了多个阿尔卑斯-盎格鲁时期的 CIE,当时沉积物堆积速度缓慢,为 3-15 m/Myr。平均总有机碳(TOC)在∼101 Ma 的阿尔卑斯-震旦纪边界事件(TOC 从 7% 到 18%)和∼94 Ma 的震旦纪-都龙纪边界事件(TOC 从 5% 到 10%)的 2-3 ‰ CIE 期间大幅增加。在白垩纪热极盛时期的全球高海平面和高温度条件下,都龙纪的总有机碳保持在较高水平(8-13%),随后在 ∼90 Ma 的都龙纪晚期 1.5 ‰ CIE 事件中,总有机碳从 7% 上升到 11%。平均 TOC 随后在科尼阿克-坎帕尼亚期下降,但在 0.5-1 ‰ CIE 期间出现了相对最大值,被解释为 ∼87 Ma 晚科尼阿克事件(TOC 从 4% 增加到 7%)、 ∼85 Ma 马蹄湾事件(TOC 从 3.5% 增加到 4.5%)和 ∼84 Ma 桑顿-坎帕尼亚边界事件(TOC 从 3.5% 增加到 5%)。氢指数和生产力代用指标(P、Ba、Nd)的增加伴随着TOC增加的每一次CIE事件,表明在短期CIE时间尺度上,海洋生产力与有机碳埋藏之间存在密切联系。然而,痕量金属氧化还原(Mo、Fe、V)和盐度(B/Ga)代用指标的长期(5-8Myr)变化表明,在比CIE更长的时间尺度上,当时的环境条件发生了变化。晚白垩世-中都元世的海洋盐度发生在优氧(103-98 Ma)和亚氧(98-90 Ma)条件下,沉积分别被解释为发生在最小含氧区内和其下方。与此相反,晚都元世-早钟元世(90-82 Ma)的清新和受限的优氧海盆条件可能预示着北极古近纪已知的广泛限制的开始。总之,这些结果突出表明,尽管北极温室条件不断变化,但中白垩世北极深水仍然是一个与全球碳循环相耦合的高产海洋碳汇。
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引用次数: 0
Bayesian frameworks for integrating petrologic and geochronologic data 整合岩石学和地质年代数据的贝叶斯框架
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118963

Constraining the absolute time and duration of geologic processes is one of the great challenges and goals in Earth sciences. Increasingly, the integration of geochronologic constraints with petrologic information is being qualitatively applied to understanding the timescales of metamorphic, igneous, tectonic, and fluid-related processes. Many rocks and geochronometers preserve relative age constraints such as compositional zoning or cross cutting relationships. This prior information can be formalized in a Bayesian statistical framework to generate a probabilistic posterior chronology. As we show here, these “age-sequence” models can enhance precision on geochronologic dates and rates and insight into tectonic models. Bayesian modeling of complex, concentrically, zoned monazite from the northern Appalachian orogen was used to develop a detailed temperature-time history through the Acadian (∼405–395 Ma) and Neoacadian (∼380–350 Ma) orogenies with significantly reduced uncertainties (40–70 %). Modeling of zoned monazite from a southern Trans-Hudson orogen granulite yielded durations of 0.5+9/-0.4 Ma and 20+5/-8 Ma for biotite-dehydration melting and suprasolidus conditions, respectively. The relatively short intervals of heating and peak conditions are consistent with a back-arc tectonic setting. A complementary approach, Bayesian change point detection, provides a framework to constrain the timing of compositional changes that can be linked with metamorphic reactions. Applying this approach in the northern Appalachian orogen demonstrates contrasting durations of low-Y monazite crystallization (∼10 vs ∼30 myr) in regions with different pressure-temperature histories. Compositionally distinct monazite domains can be linked with garnet stability, which provides a key constraint on tectonic models. Bayesian statistical analysis represent a powerful tool that can be widely applied to refine the absolute time and duration of geologic processes. A more objective and reproducible set of interpretations are produced by this more formal, although not necessarily complex, statistical analysis.

确定地质过程的绝对时间和持续时间是地球科学的巨大挑战和目标之一。地质年代约束与岩石学信息的整合正越来越多地被定性地应用于了解变质、火成岩、构造和流体相关过程的时间尺度。许多岩石和地质年代计都保留了相对的年龄约束,如成分分带或横切关系。这种先验信息可以在贝叶斯统计框架中正规化,以生成概率后验年表。正如我们在这里所展示的,这些 "年龄序列 "模型可以提高地质年代和速率的精确性,并提高对构造模型的洞察力。通过对阿巴拉契亚造山带北部复杂的同心带状独居石进行贝叶斯建模,我们建立了阿卡迪亚造山带(405-395 Ma)和新阿卡迪亚造山带(380-350 Ma)的详细温度-时间历史,并显著降低了不确定性(40-70%)。通过对跨哈德逊造山带南部花岗岩中的带状独居石进行建模,得出生物脱水熔融和超固结条件的持续时间分别为0.5+9/-0.4 Ma和20+5/-8 Ma。相对较短的加热间隔和峰值条件与后弧构造环境相一致。贝叶斯变化点检测法是一种补充方法,它提供了一个框架来限制与变质反应有关的成分变化的时间。将这种方法应用于阿巴拉契亚造山带北部,可以发现在不同压力-温度历史的地区,低Y独居石结晶的持续时间(10 ∼ 30 myr)截然不同。成分上不同的独居石域可与石榴石的稳定性联系起来,这为构造模型提供了一个关键的约束条件。贝叶斯统计分析是一种强大的工具,可广泛应用于完善地质过程的绝对时间和持续时间。通过这种更加正式、但不一定复杂的统计分析,可以得出一套更加客观和可重复的解释。
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引用次数: 0
Hydraulically linked reservoirs simultaneously fed the 1975–1984 Krafla Fires eruptions: Insights from petrochemistry 1975-1984年克拉弗拉大火爆发时,水力相连的水库同时为大火提供了燃料:石油化学的启示
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118960

The 1975–1984 Krafla Fires in northeast Iceland was the first plate-boundary rifting episode to be tracked using seismic and geodetic monitoring. Geophysical observations from this episode have inspired conceptual models of magma transport during plate spreading, but a lack of complementary petrologic insights has hindered a holistic understanding of the events. To address this knowledge gap, we studied the petrochemistry of all nine Krafla Fires basaltic eruptions. Our large dataset of new whole-rock, matrix glass and mineral analyses from samples collected during or shortly after each eruption reveal a clear compositional bimodality in the erupted magmas that persisted across the episode, with evolved quartz tholeiite (MgO = 5.7–6.4 wt.%) erupted inside Krafla caldera, and more primitive (usually olivine-normative) tholeiite (MgO = 6.4–8.7 wt%) erupted north of the caldera margin. Barometric calculations indicate tapping of these magmas from distinct reservoirs: a primitive lower-crustal reservoir at a most probable depth of ∼14–19 km, and a more evolved, shallower reservoir at a most probable depth of ∼7–9 km beneath the caldera. These reservoirs were tapped simultaneously in several of the nine eruptions, and in three events the two magma types mixed near the northern caldera margin. Varying levels of trace element depletion in the deep-sourced primitive melts reflect incomplete mixing of diverse mantle-derived melts at depth; the most enriched of these melts could be parental to evolved inside-caldera magma via fractional crystallization. Clinopyroxene rims on gabbroic nodules from primitive September 1984 lavas record lower crustal pressures, while diffusion models suggest that these rims grew up to within a few months before eruption. Ascent of the primitive magma from the lower crust thus occurred over timescales much shorter than eruptive repose periods, without prolonged stalling at shallow depths. These observations are inconsistent with the view that the eruptions were entirely fed by lateral magma outflow from the shallow reservoir. They instead require some decoupling of the flow paths of the two magma types: the primitive magma either bypassed the sub-caldera reservoir laterally or ascended vertically beneath the northern vents. The two reservoirs nonetheless shared a hydraulic connection and jointly responded to rifting. Comparison of the Krafla Fires with other rifting events and eruptions highlights the complexity and diversity of magma transport during plate boundary rifting events, which is not yet captured by a generalizable model. Integration of petrologic, geochemical and geophysical data is essential to provide a holistic view of future rifting events in Iceland and at other spreading centres.

冰岛东北部 1975-1984 年的克拉弗拉大火是利用地震和大地测量监测跟踪的第一个板块边界断裂事件。从这一事件中观察到的地球物理现象启发了人们建立板块扩张过程中岩浆运移的概念模型,但由于缺乏补充的岩石学知识,人们对这一事件的整体理解受到了阻碍。为了弥补这一知识空白,我们研究了所有九次克拉弗拉大火玄武岩喷发的岩石化学。我们从每次喷发期间或喷发后不久采集的样本中获得了大量新的全岩、基质玻璃和矿物分析数据集,这些数据集揭示了喷发岩浆中明显的成分双峰性,这种双峰性在整个事件中持续存在,进化的石英透辉石(MgO = 5.7-6.4 wt.%)在克拉弗拉火山口内喷发,而更原始(通常为橄榄石常态)的透辉石(氧化镁=6.4-8.7 wt%)则在火山口边缘以北喷发。气压计算表明,这些岩浆是从不同的储层中喷发出来的:一个原始的下地壳储层,最可能的深度为14-19千米;另一个较新的、较浅的储层,最可能的深度为火山口下7-9千米。在九次喷发中,有几次同时开采了这些储层,在三次喷发中,这两种岩浆在火山口北缘附近混合。深源原始熔体中不同程度的微量元素贫化反映了不同地幔源熔体在深部的不完全混合;这些熔体中最富集的可能是通过部分结晶而演化成破火山口内部岩浆的亲代。1984年9月原始熔岩的辉长岩结核上的霞石边缘记录了较低的地壳压力,而扩散模型表明,这些边缘是在喷发前几个月内形成的。因此,原始岩浆从下地壳上升的时间比喷发休止期要短得多,没有在浅层长时间停滞。这些观察结果与喷发完全由浅层储层的横向岩浆流出提供动力的观点不一致。相反,它们要求两种岩浆的流动路径有所分离:原始岩浆要么横向绕过火山口下储层,要么在北部喷口下方垂直上升。尽管如此,这两个岩浆库仍有共同的水力联系,并共同对断裂做出反应。将克拉弗拉大火与其他断裂事件和火山爆发进行比较,突出了板块边界断裂事件期间岩浆运移的复杂性和多样性,而这种复杂性和多样性尚未被一个通用模型所捕捉。整合岩石学、地球化学和地球物理数据对于全面了解冰岛和其他扩张中心未来的断裂事件至关重要。
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引用次数: 0
Neogene surface uplift of the Lunpola Basin in Central Tibet: Implications for uplifting and flattening of orogenic plateaus 西藏中部伦坡拉盆地新近纪地表隆起:造山高原隆起和变平的影响
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118961

Orogenic plateaus are known for their high and flat interiors, but the mechanism by which the high-elevation, low-relief topography is formed remains controversial. The Tibetan Plateau, which may have had a broad central valley along the Bangong suture zone during the Eocene, is a valuable research target to test potential driving mechanisms. In this study, we report both stable and clumped isotopes of lacustrine carbonates of the Lunpola Basin to better constrain the paleoelevation history of the Bangong suture zone in Central Tibet. Covariations of the stable oxygen and carbon isotopes indicate increasing evaporative enrichment of lake water reflecting enhanced aridity from the middle Eocene to early Miocene. After removing altered samples using multiple diagenesis screening methods and the potential influence of global cooling, our clumped isotope temperatures indicate consistent paleoelevations of 2.2 ± 1.1 km at 40–20 Ma, followed by an abrupt 1.4 ± 0.8 km surface uplift at 20–19 Ma and an additional 1.0 ± 0.7 km surface uplift between 16 Ma and the present to achieve the current high elevation of ∼4.6 km. These new paleoelevation results suggest that the Neogene was the primary period of topographic growth for the Lunpola Basin, which contradicts previous inferences emphasizing Paleogene growth. We argue that the Bangong suture zone in Central Tibet was probably a broad low-elevation valley throughout the Paleogene and uplifted mainly during the Neogene by multiple subsurface geodynamic processes, including convective removal of the lower lithosphere and middle–lower crustal flow. A comparison with the north-central Tibet Hoh Xil Basin and South American Altiplano indicates that these subsurface geodynamic processes may be common for uplifting and flattening orogenic plateaus.

众所周知,造山运动形成的高原内部高而平坦,但高海拔、低起伏地形的形成机制仍存在争议。青藏高原在始新世时期可能沿班公错缝合带有一个宽阔的中央谷地,它是检验潜在驱动机制的一个有价值的研究目标。在本研究中,我们报告了伦坡拉盆地湖相碳酸盐岩的稳定同位素和团块同位素,以更好地解释西藏中部班公错缝合带的古海拔历史。稳定氧同位素和碳同位素的变异表明,湖水蒸发富集程度不断增加,反映了中新世中期至中新世早期的干旱加剧。在使用多种成岩筛选方法剔除了蚀变样品以及全球变冷的潜在影响之后,我们的团块同位素温度表明,40-20Ma时期的古海拔高度一致为2.2 ± 1.1千米,随后在20-19Ma时期地表突然抬升了1.4 ± 0.8千米,16Ma至今地表又抬升了1.0 ± 0.7千米,从而达到了目前4.6千米的高海拔高度。这些新的古海拔结果表明,新近纪是伦坡拉盆地地形增长的主要时期,这与之前强调古近纪增长的推论相矛盾。我们认为,西藏中部的班公断裂带在整个古近纪很可能是一个宽阔的低海拔山谷,在新近纪主要通过多种地下地球动力学过程(包括下岩石圈的对流剥离和中下地壳流动)而隆起。与西藏中北部的呼日勒盆地和南美高原的比较表明,这些次表层地球动力过程可能是造山高原隆起和变平的常见过程。
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引用次数: 0
Evolution of rift faulting in incipient, magma-poor divergent plate boundaries: New insights from the Okavango-Makgadikgadi Rift Zone, Botswana 岩浆贫乏的发散板块边界初期断裂的演变:博茨瓦纳奥卡万戈-马卡迪卡迪断裂带的新发现
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118957

Continental rifts are thought to transition from a power-law fault length distribution during the juvenile stages of extension, to an exponential distribution during break-up and oceanic spreading. However, fault scaling relationships have rarely been quantified in natural incipient rifts, particularly in the absence of magmatic influence. We address this knowledge-gap in the incipient Okavango-Makgadikgadi Rift Zone, Northern Botswana, consisting of the amagmatic Okavango Rift Basin (ORB) and Makgadikgadi Rift Basin (MRB). We utilize high-resolution satellite topography data (12.5 m TanDEM-X and 30 m SRTM) and aeromagnetic data to image and map faults across the rift zones and generate a new robust fault map for the region. Further, we analyze the length-frequency distribution of faults using a two-sample Kolmogorov-Smirnov test. The results show that the Makgadikgadi Rift Basin exhibits an exponential distribution associated with a nucleating rift as it exhibits diffuse faulting and lacks a border-fault, whereas the Okavango Rift Basin exhibits a power-law distribution that is consistent with its relatively more evolved rift structure with established border faults. Thus, we propose that continental divergent plate boundaries commonly nucleate with an initial exponential distribution of fault lengths which subsequently transition into a power-law distribution as the rift evolves into its stretching phase, and may again transition into an exponential distribution as break-up initializes.

人们认为,大陆裂谷在延伸的初级阶段会从幂律断层长度分布过渡到断裂和海洋扩张期间的指数分布。然而,在自然的新生断裂中,尤其是在没有岩浆影响的情况下,断层的比例关系很少被量化。我们在博茨瓦纳北部奥卡万戈-马卡迪卡迪断裂带的萌生期填补了这一知识空白,该断裂带由岩浆型奥卡万戈断裂盆地(ORB)和马卡迪卡迪断裂盆地(MRB)组成。我们利用高分辨率卫星地形数据(12.5 米 TanDEM-X 和 30 米 SRTM)和航空磁数据对整个裂谷带的断层进行成像和测绘,并为该地区绘制了新的稳健断层图。此外,我们还利用双样本 Kolmogorov-Smirnov 检验分析了断层的长度-频率分布。结果表明,马卡迪卡迪裂谷盆地呈现指数分布,这与正在形成的裂谷有关,因为该盆地呈现弥漫性断层,缺乏边界断层;而奥卡万戈裂谷盆地则呈现幂律分布,这与该盆地相对更成熟的裂谷结构以及已形成的边界断层相一致。因此,我们认为,大陆分异板块边界的成核断层长度通常呈初始指数分布,随着裂谷演化到伸展阶段,断层长度随之过渡到幂律分布,随着断裂的初始化,断层长度可能再次过渡到指数分布。
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引用次数: 0
A failed search for concordancy across multiple isotopic systems in lunar impactites: Implications for testing the Late Heavy Bombardment hypothesis 对月球撞击岩中多个同位素系统一致性的失败探索:对检验晚期重轰炸假说的影响
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118943
Investigations of Apollo-returned samples radically altered our understanding of lunar history which has important implications for terrestrial habitability and Solar System evolution. Radiometric dating of those samples inspired the hypothesis that Moon experienced a Late Heavy Bombardment (LHB) at ∼3.9 Ga. The LHB concept has come under several recent challenges, including the concern that 40Ar/39Ar step-heating dates of Apollo impactites had been misinterpreted. Ultraviolet laser ablation (UVLAMP) 40Ar/39Ar dates – with their capacity for much higher spatial resolution and thus potential to avoid dating near-ubiquitous clasts in impact melt rocks – should in principle provide more interpretable results. Here we compare new ion microprobe 207Pb/206Pb accessory mineral dates for two Apollo 17 impactites for which UVLAMP 40Ar/39Ar dates had been previously obtained. Our results are consistent with a single accessory phase growth event for each sample, though the two samples yielded statistically different mean ages of ca. 3.974±0.013 and 3.928±0.003 Ga. Both can reasonably be interpreted as dating an impact event, but the 207Pb/206Pb dates are older than the associated 40Ar/39Ar dates by several hundred million years. We interpret that the age differences result from subsequent thermal disturbances. The discordancy between impact ages inferred from lunar impactites using two different radiometric systems suggests caution in acceptance of the LHB hypothesis without the benefit of both larger lunar datasets and more multichronometric studies. Even with such information, our capacity to know the lunar bombardment history is likely limited by compositional and thermal effects which appear to restrict growth of impact-produced accessory minerals to a small fraction of the lunar surface. Using currently available datasets, the LHB hypothesis may be effectively untestable.
对阿波罗返回样本的研究从根本上改变了我们对月球历史的认识,这对陆地宜居性和太阳系的演化具有重要影响。对这些样本进行的辐射测年激发了月球在 ∼3.9 Ga经历了晚期重型轰炸(LHB)的假说。LHB 概念最近受到了一些挑战,包括对阿波罗撞击岩的 40Ar/39Ar 阶跃加热日期的误读。紫外线激光烧蚀法(UVLAMP)的 40Ar/39Ar 年代测定,空间分辨率要高得多,因此可以避免对撞击熔融岩中几乎无处不在的碎屑进行年代测定,原则上应该可以提供更多可解释的结果。在这里,我们比较了两块阿波罗 17 号撞击岩的新的离子微探针 207Pb/206Pb 附属矿物的年代,这些撞击岩以前曾获得过 UVLAMP 40Ar/39Ar 的年代。我们的结果与每个样品的单一附属相生长事件相一致,尽管这两个样品的平均年龄在统计上存在差异,分别约为 3.974±0.013 Ga 和 3.928±0.003 Ga。两者都可以被合理地解释为一个撞击事件的年代,但是 207Pb/206Pb 年代比相关的 40Ar/39Ar 年代要早几亿年。我们认为这些年龄差异是由随后的热扰动造成的。使用两种不同的辐射测量系统从月球撞击岩中推断出的撞击年龄之间的不一致表明,在没有更大的月球数据集和更多的多时间测量研究的情况下,接受 LHB 假设需要谨慎。即使有了这些信息,我们了解月球轰击历史的能力也很可能受到成分和热效应的限制,这些效应似乎将撞击产生的附属矿物的生长限制在月球表面的一小部分。利用目前可用的数据集,LHB 假设可能实际上是无法检验的。
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引用次数: 0
Long-term evolution of the Sulzberger Ice Shelf, West Antarctica: Insights from 74-year observations and 2022 Hunga-Tonga volcanic tsunami-induced calving 南极洲西部苏尔茨伯格冰架的长期演变:从 74 年的观测和 2022 年洪加-通加火山海啸引发的断裂中获得的启示
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-09-02 DOI: 10.1016/j.epsl.2024.118958

On January 15, 2022, the eruption of the Hunga-Tonga volcano unleashed a tsunami that rapidly traversed the Pacific Ocean, soon reaching the Sulzberger Ice Shelf (SIS), West Antarctica. In the aftermath, the West Sulzberger Ice Shelf (WSIS) experienced a significant calving event, shedding 106 km2 of ice and reducing its size to the smallest recorded since 1948. To investigate the potential association between this calving event and the tsunami, and to elucidate the long-term evolution of the WSIS, this study employed tide gage records and remote sensing data for an extensive cross-cycle observation spanning 74 years. The results indicate that post-2014, the WSIS exhibited heightened instability, manifesting as an increased frequency of calving events, a shift from an expanding to a contracting shelf area, and accelerated ice flow velocities (Video S1). The critical rift, instrumental in the 2022 calving, also displayed an accelerated widening rate post-2014, culminating in rapid expansion upon the tsunami's arrival, completing the final 2% of the iceberg's detachment boundary. Modeling results quantify the tsunami induced flexural strains on the ice shelf, with peak values occurring near the region of the subsequent calving event. Notably, multiple calving events during the study period coincided with local minima in landfast sea ice extent, underscoring its protective role for the ice shelf. Furthermore, a significant decline in landfast sea ice near the SIS had been observed over the past two decades, suggesting a weakening of this protective effect. A combination of modeling results and comparative analysis with other similar calving events suggests that tsunamis tend to expedite ice shelf calving predominantly when the shelf is already teetering on instability, which casts a shadow on the SIS's future resilience against natural hazards.

2022 年 1 月 15 日,Hunga-Tonga 火山喷发引发的海啸迅速席卷太平洋,并很快抵达南极洲西部的苏兹伯格冰架(SIS)。其后,西苏尔兹伯格冰架(WSIS)经历了一次重大的冰裂解事件,106 平方公里的冰块脱落,其面积缩小到 1948 年以来的最小记录。为了探究这次塌冰事件与海啸之间的潜在联系,并阐明西苏尔兹贝格冰架的长期演变情况,本研究采用了潮汐测量仪记录和遥感数据,进行了长达 74 年的跨周期观测。研究结果表明,2014 年后,WSIS 表现出更高的不稳定性,表现为断裂事件发生频率增加、大陆架面积从扩大到收缩以及冰流速度加快(视频 S1)。对 2022 年冰山崩解起关键作用的临界裂缝在 2014 年后也出现了加速扩大的趋势,并在海啸来临时达到了快速扩张的顶峰,完成了冰山脱离边界的最后 2%。建模结果量化了海啸诱发的冰架挠曲应变,其峰值出现在随后的挤压事件区域附近。值得注意的是,在研究期间发生的多次崩塌事件与当地陆地海冰范围的最小值相吻合,这突出表明了海冰对冰架的保护作用。此外,在过去二十年里,SIS 附近的陆地海冰出现了明显的减少,表明这种保护作用正在减弱。综合建模结果以及与其他类似冰架断裂事件的比较分析表明,海啸往往会加速冰架断裂,主要是在冰架已经濒临不稳定的情况下,这给小岛屿冰架未来抵御自然灾害的能力蒙上了阴影。
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引用次数: 0
期刊
Earth and Planetary Science Letters
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