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Low total REE zircon formed in equilibrium with hornblende in granulitized eclogites: Implications for exhumation rates 花岗闪长岩中与角闪石平衡形成的低总REE锆石:对剥蚀速率的影响
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-19 DOI: 10.1016/j.epsl.2024.119084
Jia-Min Wang , Daniela Rubatto , Pierre Lanari , Yu-Lu Tian , Yi Chen , Fu-Yuan Wu
Exhumation rates of high-pressure rocks are paramount in determining plate tectonic processes, which requires absolute chronology of metamorphic stages. U-Pb geochronology of zircon and other accessory minerals has proven successful in dating different metamorphic stages, thus constraining geological rates. A common strategy to link U-Pb ages to metamorphic stages uses rare earth element (REE) patterns in the dated minerals. In this study, the changes in the REE composition of accessory and rock-forming minerals in response to changing assemblages have been investigated in granulitized eclogites and gneisses from the Ama Drime Massif, central Himalaya. Phase equilibrium modelling shows that the eclogite-facies assemblage formed at 660–720 °C and 1.6–1.9 GPa (M1), was overprinted at high-pressure granulite-facies (M2) and then ultra-high temperature conditions of >900 °C and 0.8–1.1 GPa (M3) and finally re-equilibrated at conditions of 780–810 °C and 0.8–1.0 GPa (M4). In the countryrock orthogneisses, monazite records partial resetting during granulite-facies overprinting at 26–19 Ma and melt crystallisation at 16–13 Ma, supported by textures, mineral inclusions and trace elements. In the associated granulitized eclogites, zircon records only granulite/amphibolite facies overprinting at ∼14 Ma, and titanite and rutile record cooling to 580–630 °C at 12.5–9 Ma. Granulite/amphibolite facies zircon has a low total REE relative to the protolith zircon, primarily due to the growth of REE-rich hornblende (total REE 80–260 μg/g), which removed 67–92% of the REE from the system. The low total REE of granulite/amphibolite facies zircon is comparable to the flat HREE reported for garnet-rich eclogite-facies zircon, and distinguishing these zircon types requires quantitative mineral volume estimates and other criteria. These findings may imply slower exhumation rates for some eclogite-facies terranes, such as the Tso Morari Himalaya and Papua New Guinea, than previously reported.
高压岩石的剥蚀速率对于确定板块构造过程至关重要,这需要对变质阶段进行绝对的年代测定。锆石和其他附属矿物的铀-铅地质年代学已被证明可以成功地确定不同变质阶段的年代,从而制约地质速率。将 U-Pb 年龄与变质阶段联系起来的一个常见策略是利用已定年矿物中的稀土元素(REE)模式。本研究调查了喜马拉雅中部阿玛德里梅山块的花岗闪长岩和片麻岩中,附属矿物和成岩矿物的稀土元素组成随组合变化而发生的变化。相平衡模型显示,在 660-720 °C、1.6-1.9 GPa(M1)条件下形成的斜长岩-成因集合体,被高压花岗岩-成因集合体(M2)覆盖,然后在 >900 °C、0.8-1.1 GPa(M3)的超高温条件下形成,最后在 780-810 °C、0.8-1.0 GPa(M4)条件下重新平衡。在乡土岩正长片麻岩中,蒙脱石记录了花岗岩-成因叠压过程中的部分重置(26-19 Ma)和熔融结晶(16-13 Ma),并得到了纹理、矿物包裹体和微量元素的支持。在相关的花岗闪长岩中,锆石仅记录了14 Ma的花岗岩/闪长岩面叠加,榍石和金红石记录了12.5-9 Ma冷却至580-630 °C的过程。与原岩锆石相比,花岗岩/闪长岩面锆石的总REE较低,这主要是由于富含REE的角闪石(总REE为80-260 μg/g)的生长,从系统中去除了67-92%的REE。花岗岩/闪长岩岩相锆石的低总REE与富含石榴石的夕闪岩岩相锆石的平HREE相当,区分这些锆石类型需要定量的矿物体积估算和其他标准。这些发现可能意味着某些埃克洛辉石成因地层(如 Tso Morari 喜马拉雅山和巴布亚新几内亚)的掘起速度比以前报告的要慢。
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引用次数: 0
Multiple hydrothermal events at martian surface revealed by H and Cl isotope systematics of melt inclusions and hydrous minerals from chassignite NWA 2737 来自 NWA 2737 合欢岩的熔融包裹体和含水矿物的 H 和 Cl 同位素系统学揭示了火星表面的多重热液事件
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-16 DOI: 10.1016/j.epsl.2024.119072
Sen Hu , Mahesh Anand , Ian A. Franchi , Xuchao Zhao , Alice Stephant , Magali Bonifacie , Huicun He , Wei Yang , Jialong Hao , Yangting Lin
The chassignites and nakhlites could have co-magmatic origin but display distinct hydrogen and chlorine isotopic compositions, indicating that they may have experienced distinct hydrothermal activities on Mars. However, the details are not yet fully understood. Here, we performed H and Cl isotopic investigations on hydrous minerals (kaersutite and apatite) and glass-bearing melt inclusions from chassignite NWA 2737 to unravel the details of the hydrothermal events experienced by chassignites on Mars. Our results demonstrate that at least two hydrothermal events on Mars have been recorded in NWA 2737. A D- and 37Cl-rich martian crustal/underground fluid was added to the parent magma of NWA 2737 prior to the entrapment of melt inclusions and later interaction of the parent rock with a D-poor fluid, probably deriving from magma degassing. The notable high-δD values (up to 6239‰) of kaersutite in NWA 2737 are comparable with those recorded in younger shergottites, suggesting that the martian exchangeable water reservoir has retained a nearly constant δD value over the past 1.3 Ga.
恰西尼岩和纳克里特岩可能具有共同的岩浆起源,但显示出不同的氢和氯同位素组成,表明它们可能在火星上经历了不同的热液活动。然而,具体情况尚未完全明了。在这里,我们对来自霞石 NWA 2737 的含水矿物(高燧石和磷灰石)和含玻璃的熔融包裹体进行了氢和氯同位素研究,以揭示霞石在火星上经历的热液活动的细节。我们的研究结果表明,NWA 2737至少记录了火星上的两次热液事件。在NWA 2737的母岩浆中加入了富含D和37Cl的火星地壳/地下流体,然后夹杂了熔融包裹体,之后母岩与可能来自岩浆脱气的贫D流体相互作用。NWA 2737中高δD值(高达6239‰)显著的高闪长岩与较年轻的闪长岩中记录的δD值相当,这表明在过去的1.3 Ga中,火星可交换水储层保持了几乎恒定的δD值。
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引用次数: 0
2D numerical experiments on a plume-fed asthenosphere: Necessary preconditions and implications for geoid and dynamic topography 羽状天体层的二维数值实验:必要的先决条件及其对大地水准面和动态地形的影响
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-16 DOI: 10.1016/j.epsl.2024.119068
Ya-Nan Shi , Jason P. Morgan , Chao Shi
We explore the conditions necessary for mantle flow to include a plume-fed asthenosphere (PFA) as a key structure within its large-scale flow pattern. Using 2D finite element-based experiments, we examine temperature-dependent rheological effects of ridge accretion, plate cooling, and numerically well-resolved ∼10–30 km-thick asthenosphere dragdown by subducting slabs. We find that an average plume flux ∼1.2 times big as the average slab flux is needed to maintain a persistent PFA. These numerical experiments also demonstrate that, instead of generating dynamic topography on the sea floor, flow-induced dynamic relief due to sub-asthenospheric density anomalies will preferentially form at the buoyancy contrast associated with the base of a buoyant asthenosphere. This mode of dynamic internal relief may contribute significantly to near-surface density anomalies that are associated with Earth's low-order geoid, and local relief at the base of the asthenosphere near plumes, ridges, and trenches that can be imaged in seismic experiments.
我们探索了地幔流动的必要条件,即在其大尺度流动模式中包含一个作为关键结构的羽流星体层(PFA)。利用基于二维有限元的实验,我们研究了海脊增生、板块冷却以及俯冲板块在数值上很好地分辨的∼10-30 公里厚的星体层拖拽的温度相关流变效应。我们发现,要维持持久的PFA,平均羽流通量需要是板块平均通量的1.2倍。这些数值实验还证明,由亚对流层密度异常引起的流动诱导的动态浮雕不是在海底产生动态地形,而是优先在与浮力星体层底部相关的浮力对比处形成。这种内部动态地貌模式可能会极大地促进与地球低阶大地水准面相关的近地表密度异常,以及可在地震实验中成像的羽流、海脊和海沟附近的岩石圈底部的局部地貌。
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引用次数: 0
Water ice particles detected by SELENE's Spectral Profiler at lunar shadowed regions in various local times and latitudes SELENE 的光谱分析器在不同时间和纬度的月球阴影区探测到的水冰颗粒
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-15 DOI: 10.1016/j.epsl.2024.119065
Kosei Toyokawa , Junichi Haruyama , Takahiro Iwata , Hitoshi Nozawa
Processes of water (OH and H2O) migration on the Moon remain unclear, prompting active research. Understanding lunar water migration requires investigation of the trapping and diffusion properties of water at various latitudes and local times. This study analyzed visible to near-infrared spectral data obtained by the Spectral Profiler (SP) onboard SELENE for shadowed regions at various local times and latitudes, not limited to the polar permanently shadowed regions. We assessed SP data for shadowed regions in 60 areas, each spanning a 10° × 10° latitude–longitude grid. Of the 1,061,907 analyzed shadowed-region data, 41,385 at various latitudes exhibited significant absorption in the 1.25 and 1.5 µm bands, indicating water ice particles. Data with the two absorption features suggest the presence of a water ice frost layer covering the lunar surface or suspended water ice particles above the lunar surface, at various latitude shadowed regions. Our spectral simulations have quantified the ice particles as being 0.1–1 µm in diameter, with a column density of 10–4–10–3 kg/m2. The spectral parameters for band absorption at the 1.5 µm band show symmetry between morning and evening sides, which is potentially attributed to the absence of variations in ice grain size and quantity. The 1.5 µm band absorption shows an increasing trend toward terminator regions, indicating variation in the water ice distribution and likely reflecting temperature conditions for water retention. The latitudinal trend of ice grain size and quantity remains uncertain because of the observed noise levels. Observations of water ice particles in shadowed regions at various latitudes and local times can provide new constraints on trapping and diffusion processes of lunar water migration.
水(OH 和 H2O)在月球上的迁移过程仍不清楚,因此需要积极开展研究。要了解月球上水的迁移,就必须研究水在不同纬度和局部时间的捕获和扩散特性。本研究分析了 SELENE 星载光谱剖面仪(Spectral Profiler,SP)获得的可见光至近红外光谱数据,这些数据针对不同时间和纬度的阴影区域,而不局限于极地永久阴影区域。我们评估了 60 个区域的阴影区 SP 数据,每个区域的纬度网格为 10° × 10°。在分析的 1,061,907 个阴影区数据中,不同纬度的 41,385 个数据在 1.25 和 1.5 µm 波段有明显的吸收,表明有水冰颗粒。具有这两种吸收特征的数据表明,在不同纬度的阴影区,存在着覆盖在月球表面的水冰霜层或悬浮在月球表面的水冰颗粒。我们的光谱模拟确定冰粒直径为 0.1-1 微米,冰柱密度为 10-4-10-3 千克/平方米。1.5 µm 波段吸收的光谱参数在早晚两侧显示出对称性,这可能是由于冰粒的大小和数量没有变化。1.5 µm 波段的吸收率在终结者区域呈上升趋势,表明水冰分布的变化,也可能反映了水保留的温度条件。由于观测到的噪声水平,冰粒大小和数量的纬度趋势仍不确定。在不同纬度和局部时间观测阴影区域的水冰颗粒,可以为月球水迁移的捕获和扩散过程提供新的制约因素。
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引用次数: 0
Tracing hydrous eclogite melts in the source of sanukitoids 追踪萨努基托岩源中的含水蚀变岩熔体
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-15 DOI: 10.1016/j.epsl.2024.119067
L.M. Spencer , C. Albert , H.M. Williams , O. Nebel , I.J. Parkinson , R.H. Smithies , H. Bruno , M. Fowler , H. Moreira , C.J. Lissenberg , M.-A. Millet
Sanukitoids are unique Archean and early Proterozoic igneous rocks. They contain high amounts of Mg, Ni and Cr, showing they are mantle-derived melts, while they are also enriched in Sr and Ba and have relatively high K contents, requiring the involvement of an incompatible element-enriched component likely derived from recycled crustal material. The appearance of sanukitoids in the geological record coincides with a shift in continental crust composition, and both events have been linked to a change in geodynamic processes on Earth. However, uncertainties remain about sanukitoid petrogenesis, in particular whether their mantle source was metasomatised by a metabasite-derived silicate melt or by an aqueous fluid. Titanium (Ti) stable isotopes can trace magmatic processes where silicate melts are in equilibrium with Fe-Ti oxides and amphibole but are insensitive to fluid-driven processes, making them a suitable tool to investigate not only the formation of sanukitoid magmas but also their subsequent evolution. Here we present Ti isotope data (δ49Ti) for a series of Neoarchean sanukitoids from the Yilgarn Craton that continuously covers the full compositional range of sanukitoids. These are complemented by Mesoarchean sanukitoids and Paleoarchean “sanukitoid-like” rocks from the Pilbara Craton, and by Paleoproterozoic sanukitoids from the São Francisco Craton/Paleocontinent. In addition, we analysed Paleozoic high Ba-Sr granite suites from Scotland, which are proposed to be Phanerozoic sanukitoid analogues.
Evolved sanukitoids, which formed after Fe-Ti oxide saturation, show a more muted δ49Ti increase during differentiation compared to currently analysed modern calc-alkaline suites. This difference is best explained by removal of significant proportions of Ti during sanukitoid differentiation by magmatic hornblende, which fractionates Ti isotopes less strongly than Fe-Ti oxides. Combined with early oxide saturation at high Mg#, this suggests that sanukitoid parental magmas had H2O contents and fO2 at least as high as modern arc magmas. Primitive (pre-oxide saturation) sanukitoids, however, have significantly higher δ49Ti (0.11–0.20‰) than modern arc basalts, the depleted mantle and the bulk silicate Earth (BSE). Their elevated δ49Ti values cannot be explained by aqueous fluids alone in their mantle source, and instead require the involvement of a hydrous eclogite melt component formed in equilibrium with residual rutile. We favour generation of this metasomatic melt by fluid-fluxed eclogite partial melting, demonstrating that both metabasite melts and aqueous fluids are important for sanukitoid formation. The Ti isotope compositions of Archean and Paleoproterozoic sanukitoids therefore favour formation of the sanukitoid mantle source by a subduction-like process at least ∼2.7 Ga.
萨努基托岩是一种独特的阿新世和新生代早期火成岩。它们含有大量的镁、镍和铬,表明它们是地幔熔体,同时还富含锶和钡,钾含量也相对较高,这就要求有不相容元素富集的成分参与其中,而这些不相容元素富集的成分很可能来自回收的地壳物质。地质记录中出现萨努基多岩的时间与大陆地壳成分的变化相吻合,这两个事件都与地球地球动力过程的变化有关。然而,萨努基托岩成岩过程仍存在不确定性,特别是它们的地幔源是由新元古代硅酸盐熔体还是由水流体变质而成。钛(Ti)稳定同位素可以追踪硅酸盐熔体与铁钛氧化物和闪石处于平衡状态的岩浆过程,但对流体驱动过程不敏感,因此钛同位素不仅是研究萨努基特类岩浆形成过程的合适工具,也是研究其后续演化过程的合适工具。在这里,我们展示了来自伊尔加恩克拉通的一系列新元古代萨努基特岩的钛同位素数据(δ49Ti),这些数据连续涵盖了萨努基特岩的全部成分范围。皮尔巴拉克拉通的中新世砂岩和古新世 "类砂岩 "以及圣弗朗西斯科克拉通/古陆的古近纪砂岩对这些岩石进行了补充。此外,我们还分析了来自苏格兰的古生代高钡锶花岗岩套件,这些套件被认为是新生代sanukitoid的类似物。与目前分析的现代钙碱性套件相比,在铁钛氧化物饱和之后形成的进化sanukitoids在分化过程中显示出更为柔和的δ49Ti增加。这种差异的最佳解释是,岩浆角闪石在三绢云母分异过程中去除了大量的Ti,而角闪石对Ti同位素的分馏作用不如Fe-Ti氧化物强烈。结合高 Mg# 时的早期氧化物饱和,这表明三琉球母岩的 H2O 含量和 fO2 至少与现代弧岩浆一样高。然而,原始(氧化物饱和前)萨努基托岩浆的δ49Ti(0.11-0.20‰)明显高于现代弧玄武岩、贫化地幔和大块硅酸盐地球(BSE)。它们升高的δ49Ti值不能仅用地幔源中的水性流体来解释,而需要与残余金红石平衡形成的含水闪长岩熔体成分的参与。我们倾向于通过流体通量的斜长岩部分熔融来生成这种偏闪长岩熔体,从而证明偏闪长岩熔体和水成流体对于砂岩的形成都很重要。因此,阿新世和古新生代沙努基托岩的Ti同位素组成倾向于沙努基托岩地幔源是通过至少∼2.7 Ga的类似俯冲过程形成的。
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引用次数: 0
The viscosity of a partially molten layer in a paleo-orogenic plateau 古成因高原部分熔融层的粘度
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-15 DOI: 10.1016/j.epsl.2024.119060
Z. Molitor , T. Mittal , O. Jagoutz
Orogenic plateaus (e.g., Tibet, Altiplano) are characterized by broad, flat-top topography at high elevation and significantly increased crustal thickness. Partial melt is thought to weaken the middle crust of orogenic plateaus, and thus reduce the viscosity of the crust; however, the amount of partial melt and the magnitude of associated weakening remain unconstrained. The New England Appalachians represent an exposed mid- to lower crustal section of a paleo-orogenic plateau, similar to modern-day Tibet. In this study, we utilize the relationship between the spacing of deformation bands and the compaction length to constrain mid-crustal shear viscosity in a late Devonian migmatite. We find that the viscosity of the middle orogenic crust in the paleo-orogenic plateau of the New England Appalachians is 1017–18 Pa∙s at ∼3–9% melt. This finding is consistent with geophysical models of orogenic channel flow and provides field-based evidence for a significant rheologic transition at low melt-fraction. Our results suggest that the key elements for the formation of a weak, mid-crustal layer in orogenic plateaus are an influx of water and temperatures near the hydrous granite solidus.
造山运动高原(如西藏、高原)的特点是海拔高,顶部平坦,地壳厚度显著增加。部分熔融被认为会削弱造山运动高原的中地壳,从而降低地壳的粘度;然而,部分熔融的数量和相关削弱的程度仍未确定。新英格兰阿巴拉契亚山脉是古造山运动高原中下地壳裸露部分,类似于现代西藏。在这项研究中,我们利用变形带间距与压实长度之间的关系来约束泥盆纪晚期伟晶岩的中地壳剪切粘度。我们发现,在新英格兰阿巴拉契亚山脉古成因高原,熔融度为 3-9% 的情况下,中间造山地壳的粘度为 1017-18 Pa∙s。这一发现与造山通道流的地球物理模型一致,并为低熔融分率时的显著流变转变提供了实地证据。我们的研究结果表明,在造山高原中形成薄弱的中岩壳层的关键因素是水的涌入和含水花岗岩固结点附近的温度。
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引用次数: 0
Detection of a ULVZ in the Central Pacific using high frequency Sdiff postcursors 利用高频 Sdiff 后验器探测中太平洋的超低海流区
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-14 DOI: 10.1016/j.epsl.2024.119028
Carl Martin , Stuart Russell , Sanne Cottaar
In recent decades, ultra-low velocity zones (ULVZs) – thin patches of strongly reduced seismic velocity atop the core-mantle boundary (CMB) – have been inferred from observations of a variety of seismic phases. One such phase is Sdiff and its out-of-plane postcursory energy, Sdiff+. In this study, we present a high quality dataset of Sdiff and Sdiff+ which shows evidence of a ULVZ in the central Pacific, roughly between Hawaii and Marquesas. The observed Sdiff+ have an unusually short dominant period (5–12 seconds) compared to previous Sdiff+ observations, which is indicative of a ULVZ that is approximately 10–15 km thick. We analyse this high frequency dataset using the 2D Wavefront Tracker (2DWT) Bayesian inversion methodology to generate a probabilistic ensemble of ULVZ models. As a result of the uniazimuthal coverage of data, there is a strong southwest-northeast trade-off, but there is a slight preference for the ULVZ to be located just outside the Pacific large low velocity province (LLVP) boundary, roughly centred 20° north of Marquesas and 20° southeast of Hawaii. The 2DWT inversion of Sdiff+ travel times suggest that the ULVZ can be approximated as a cylindrical structure; either as a larger and weaker anomaly (radius 280 km, dVs -20%) close to the LLVP, or a smaller and stronger anomaly (radius 180 km, dVs -30%) further away from the LLVP. Unlike previous broad-scale ULVZs modelled with Sdiff+, this ULVZ is thinner, might lie outside of an LLVP, and lacks a potential relationship to a mantle plume.
近几十年来,根据对各种地震相位的观测,推断出了超低速度区(ULVZs)--地核-地幔边界(CMB)上地震速度强烈减弱的薄片。其中一个相位是 Sdiff 及其平面外后发能量 Sdiff+。在这项研究中,我们展示了一个高质量的 Sdiff 和 Sdiff+ 数据集,该数据集显示了在太平洋中部(大致在夏威夷和马克萨斯群岛之间)存在超低变区的证据。与之前的 Sdiff+ 观测结果相比,观测到的 Sdiff+ 的主周期(5-12 秒)异常短,这表明超低频带的厚度约为 10-15 千米。我们利用二维波前跟踪器(2DWT)贝叶斯反演方法分析了这一高频数据集,生成了一个超低频谱区概率模型集合。由于数据的单方位角覆盖,西南-东北方向有很强的权衡,但超低压带略微偏向于位于太平洋大低速区(LLVP)边界之外,大致以马克萨斯群岛以北 20° 和夏威夷东南 20° 为中心。Sdiff+ 移动时间的 2DWT 反演表明,超低强度区可以近似为一个圆柱形结构;或者是靠近低纬度带的一个较大且较弱的异常(半径 280 千米,dVs -20%),或者是远离低纬度带的一个较小且较强的异常(半径 180 千米,dVs -30%)。与以前用 Sdiff+ 模拟的大尺度超低变异区不同,这个超低变异区更薄,可能位于 LLVP 之外,而且与地幔羽流缺乏潜在关系。
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引用次数: 0
Ring faulting and piston collapse in the mantle sustained the largest submarine eruption ever documented 地幔中的环状断层和活塞塌陷维持了有史以来最大的海底火山爆发
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-11 DOI: 10.1016/j.epsl.2024.119026
E. Jacques , R. Hoste-Colomer , N. Feuillet , A. Lemoine , J. van der Woerd , W.C. Crawford , C. Berthod , P. Bachèlery
The basaltic submarine eruption offshore the island of Mayotte between July 2018 and January 2021 is one of the largest documented underwater eruptions. One of the most striking differences between this eruption and most documented eruptions is the exceptional depth of the associated seismicity, which is limited almost exclusively to the lithospheric mantle. This seismicity probably outlines magma reservoirs and dyking zones.
In order to better understand the deep processes driving the eruption, we analyze precise earthquake locations and focal mechanisms associated with this event. We present a set of 2677 accurate earthquake relocations and 300 focal mechanisms determined from data collected over the first 9 months of ocean bottom seismometer deployments, starting in February 2019.
Our relocations refine the structure of two swarms (Proximal and Distal with respect to Mayotte), and reveal well-defined mantle structures between 20 and 55 km below sea level, which we interpret as a ring-fault zone and a dyke, respectively. The Proximal swarm outlines a ring-fault zone as the locus of a large piston collapse caused by the deflation of an underlying magma reservoir. Deformation around the piston is driven by normal faulting on a set of inward dipping patches surrounding the piston. Locally, collapse of the conical shaped piston causes a radial extensional stress field with strike-slip and normal faulting ruptures accommodating the relaxation of the damaged zone around the piston.
This piston collapse allowed the transfer of lava to the eruption site via the dyke highlighted by the Distal earthquake swarm. The link between the swarms is thus magmatic, in agreement with petrological analyses of lava from the new volcano.
This is the first time that piston collapse and localized dyking have been documented in the mantle. The pattern of deformation documented here could apply to shallower, crustal piston collapses, such as in Iceland.
2018 年 7 月至 2021 年 1 月间马约特岛近海的玄武岩海底喷发是有记录的最大水下喷发之一。这次喷发与大多数记录在案的喷发之间最显著的区别之一是相关地震的深度特别大,几乎只限于岩石圈地幔。为了更好地了解驱动此次喷发的深层过程,我们分析了与此次事件相关的精确地震位置和聚焦机制。我们从 2019 年 2 月开始,通过前 9 个月的海底地震仪部署所收集的数据,确定了一组 2677 次精确地震定位和 300 个焦点机制。我们的定位完善了两个震群(相对于马约特岛的近端震群和远端震群)的结构,并揭示了海平面以下 20 至 55 千米之间定义明确的地幔结构,我们将其分别解释为环状断层带和堤坝。近端岩浆群勾勒出的环状断层带是一个大型活塞塌陷的位置,该活塞塌陷是由地下岩浆储层的膨胀引起的。活塞周围的变形是由活塞周围一组向内倾斜的斑块上的正断层驱动的。在局部,锥形活塞的坍塌造成了径向伸展应力场,而走向滑动和正断层的断裂适应了活塞周围受损区域的松弛。因此,地震群之间的联系是岩浆作用,这与新火山熔岩的岩石学分析结果一致。这里记录的变形模式可能适用于较浅的地壳活塞塌陷,如冰岛的活塞塌陷。
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引用次数: 0
Lithium isotope stratigraphy and Ordovician weathering 锂同位素地层学与奥陶纪风化作用
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-11 DOI: 10.1016/j.epsl.2024.119030
Y. Datu Adiatma , Matthew R. Saltzman , Xiao-Ming Liu , Xi-Kai Wang , Cole T. Edwards
Understanding the role of silicate weathering in controlling the long-term carbon cycle is essential in exploring multi-million-year scale climate variabilities and links to tectonics and changes in biodiversity. The lithium isotopic composition of carbonate rocks (δ7Li) is a non-traditional proxy that offers a more comprehensive understanding of silicate weathering dynamics in the geologic past in combination with traditional weathering proxies such as strontium isotopes (87Sr/86Sr). However, questions related to the effects of diagenesis and the relationship between changes in δ7Li and CO2 consumption during silicate rock weathering hamper the use of this novel proxy to its full potential. Here we present measurements of bulk carbonate δ7Li that span the Ordovician Period from six sections across the Laurentian paleocontinent. Using a rigorous textural and geochemical screening, we produce the first high-resolution seawater δ7Li (δ7Lisw) curve that spans the Tremadocian to Sandbian of the Ordovician Period (∼487 – 453 Ma). The δ7Lisw curve produced in this study exhibits a ∼4‰ negative shift during the Early to Middle Ordovician. Using comparisons to existing weathering proxies and a numerical modeling approach, we suggest a progressive change toward a low-intensity, congruent weathering regime was a likely driver for the observed trend. This finding highlights potential links between island arc migration toward the tropics, global increase in exposed landmass, possible terrestrialization by non-vascular land plants and changes in silicate weathering.
了解硅酸盐风化在控制长期碳循环中的作用,对于探索数百万年尺度的气候变异以及与构造和生物多样性变化的联系至关重要。碳酸盐岩的锂同位素组成(δ7Li)是一种非传统的代用指标,与锶同位素(87Sr/86Sr)等传统的风化作用代用指标相结合,可以更全面地了解地质历史上硅酸盐风化作用的动态。然而,有关硅酸盐岩风化过程中成岩作用的影响以及δ7Li的变化与二氧化碳消耗之间的关系等问题,阻碍了这一新型代用指标充分发挥其潜力。在这里,我们展示了横跨奥陶纪的、来自劳伦森古大陆六个剖面的大块碳酸盐岩δ7Li的测量结果。通过严格的纹理和地球化学筛选,我们首次绘制了横跨奥陶纪(487 - 453 Ma)Tremadocian 至 Sandbian 的高分辨率海水 δ7Li (δ7Lisw)曲线。本研究绘制的δ7Lisw曲线在早奥陶世至中奥陶世期间呈现出∼4‰的负偏移。通过与现有的风化代用指标和数值模拟方法的比较,我们认为,向低强度、同向风化机制的渐进变化可能是观测到的趋势的驱动因素。这一发现凸显了岛弧向热带迁移、全球裸露陆地面积的增加、非维管束陆生植物可能的陆地化以及硅酸盐风化变化之间的潜在联系。
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引用次数: 0
Rhenium isotope variations in Icelandic groundwaters and hydrothermal systems 冰岛地下水和热液系统中的铼同位素变化
IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-10-10 DOI: 10.1016/j.epsl.2024.119046
Wenhao Wang , Alexander J. Dickson , Mathieu Dellinger , Kevin W. Burton , Deirdre E. Clark , Guðjón Helgi Eggertsson , Íris Eva Einarsdóttir , Heimir Ingimarsson , Kiflom Gebrehiwot Mesfin , Robert G. Hilton , Julie Prytulak
The isotopic composition of rhenium (Re) has potential for use as a proxy to infer changes in seafloor redox and/or global oxidative weathering intensity. Despite an emerging dataset on this nascent isotope system in Earth's surficial environments, very little is known about processes that control Re isotope fractionation, nor the isotopic composition of hydrothermal systems. Here we present Re concentrations and Re isotopic compositions (reported as δ187Re, relative to NIST 3143) of groundwaters and hydrothermal fluids from three Icelandic settings. First, we show that high-temperature fluids that have experienced vapour-phase segregation (boiling) from the Reykjanes peninsula and the Hengill volcanic system have the highest δ187Re values (−0.01 to +0.34 ‰) observed to date, inferred to result from Re isotope fractionation during incorporation of Re into secondary reduced minerals. Second, we examine the Mývatn area in northern Iceland, which has both cold and warm groundwaters. Cold groundwaters (< 10 °C) have δ187Re values indistinguishable from Icelandic basalts (−0.36 to −0.32 ‰) whilst warm waters have higher δ187Re (−0.31 to +0.19 ‰) which increase with increasing temperature (up to 45 °C). The variation of δ187Re in Mývatn groundwaters is closely mirrored by variations in δ98Mo, consistent with mixing between compositionally distinct water end-members. Finally, geothermal waters from the Geysir field have variable Re concentrations and δ187Re values (−0.23 to +0.34 ‰), likely reflecting multiple physico-chemical processes. Using these results, we show that hydrothermal activity is unlikely to exert a large net impact on the seawater Re budget, nor the secular changes in seawater δ187Re. These findings also point toward developing a novel Re isotope tracer for redox processes.
铼(Re)的同位素组成有可能被用作推断海底氧化还原和/或全球氧化风化强度变化的替代物。尽管有关地球表面环境中这一新生同位素系统的数据集正在不断涌现,但人们对控制铼同位素分馏的过程以及热液系统的同位素组成知之甚少。在这里,我们介绍了冰岛三种环境中地下水和热液的 Re 浓度和 Re 同位素组成(以 δ187Re 报告,相对于 NIST 3143)。首先,我们展示了雷克雅未克半岛和亨吉尔火山系统中经历过汽相分离(沸腾)的高温流体具有迄今为止观测到的最高δ187Re值(-0.01 至 +0.34‰),推断这是由于Re在融入二次还原矿物的过程中发生了同位素分馏。其次,我们考察了冰岛北部的 Mývatn 地区,该地区既有冷地下水,也有暖地下水。冷地下水(< 10 °C)的δ187Re值与冰岛玄武岩无异(-0.36 至 -0.32 ‰),而暖地下水的δ187Re值则更高(-0.31 至 +0.19 ‰),并随着温度的升高而增加(最高可达 45 °C)。Mývatn 地下水中 δ187Re 的变化与 δ98Mo 的变化密切相关,这与成分不同的水末端分子之间的混合是一致的。最后,盖希尔气田的地热水具有不同的 Re 浓度和 δ187Re 值(-0.23 至 +0.34‰),可能反映了多种物理化学过程。利用这些结果,我们表明热液活动不太可能对海水 Re 预算产生巨大的净影响,也不太可能对海水 δ187Re 的长期变化产生巨大的净影响。这些发现也为开发氧化还原过程的新型 Re 同位素示踪剂指明了方向。
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引用次数: 0
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Earth and Planetary Science Letters
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