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The behaviour of Ni and its isotopes during early diagenesis of Mn oxide-rich abyssal sediments 富氧化锰深海沉积物早期成岩过程中镍及其同位素的行为
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-07 DOI: 10.1016/j.gca.2025.12.007
Sarah Fleischmann , Jianghui Du , Brian Haley , James McManus , Mingzhao Sun , Derek Vance
The use of nickel (Ni) and its isotope system as biogeochemical tracers of past ocean environments requires a sound understanding of the oceanic mass balance and the sinks that control output fluxes. Recent efforts have focused in particular on quantifying and understanding the size and Ni isotope composition of the most complicated and largest sink of Ni from the dissolved oceanic pool, the output to oxic Mn-rich sediments. The precise processes controlling Ni and its isotopes during early diagenesis in oxic sediments are not yet fully understood, but could impact estimates of the net oxic sink used in oceanic mass balance calculations. To address this issue, we present Ni concentration and isotope data from fully oxic Mn-rich sediments and corresponding porewater samples from 3 stations in the Equatorial North Pacific, south of Hawai’i.
As in other abyssal Mn-rich sediments, Ni is well correlated with Mn in the solid phase, suggesting that Mn oxides are the dominant vector by which Ni is supplied to these sediments. Authigenic Ni isotope compositions in the solid phase are isotopically lighter than global deep seawater Ni (∼1.33 ‰) and range from 0.52 to 1.06 ‰, within the range of other abyssal Mn-rich sediments (0.26 to 1.08 ‰). At all three stations, the porewater results indicate the presence of a reactive Ni pool that is mobilised into the aqueous phase near the top of the cores. Nickel concentrations in the porewaters are significantly higher at the core top (30–63 nM) than in seawater (∼8 nM), decrease to seawater concentrations downcore, and correlate with porewater DOC concentrations. Additionally, porewater Ni isotopes are heaviest (∼1.8 ‰) near the sediment–water interface, where DOC levels are highest, and decrease monotonically to values that are close to, but slightly lower than, the deep ocean Ni isotope composition (∼1.3 ‰) further down in the cores. The relationship between Ni concentration, isotopes and DOC in the porewater suggests that Ni is remobilised into porewater from Mn oxides due to lowering of pH as a result of the remineralisation of organic matter. The heavy isotope composition of porewater Ni is likely controlled by isotope fractionation between residual solid Mn oxide Ni (light) and organically-complexed heavy aqueous Ni. This isotopically heavy pore fluid Ni leaves the sediment via a diffusive benthic flux. Despite this reactive zone very close to the sediment–water interface, these diagenetic processes barely impact sediment geochemistry, suggesting that the buried sink of Ni to Mn oxide-rich sediments is accessible via analysis of solid sediment in the upper few 10 s of cm at such sites.
使用镍(Ni)及其同位素系统作为过去海洋环境的生物地球化学示踪剂,需要对海洋质量平衡和控制输出通量的汇有充分的了解。最近的工作主要集中在量化和理解溶解海洋池中最复杂和最大的Ni汇的大小和Ni同位素组成,输出到富锰的富氧沉积物。在含氧沉积物早期成岩过程中控制镍及其同位素的精确过程尚未完全了解,但可能影响用于海洋质量平衡计算的净氧汇的估计。为了解决这一问题,我们提供了来自夏威夷以南赤道北太平洋3个站点的全氧富锰沉积物和相应孔隙水样品的Ni浓度和同位素数据。
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引用次数: 0
Impact of strong redox shifts and manganese cycling on sedimentary molybdenum isotopes in stratified hypoxic/euxinic basins 强氧化还原移位和锰循环对层状缺氧/含氧盆地沉积钼同位素的影响
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-20 DOI: 10.1016/j.gca.2025.12.042
Martin Wille , Olaf Dellwig , Florian Kurzweil , Helge W. Arz , Leo Armingeon , Qasid Ahmad
<div><div>Molybdenum concentrations and stable isotope compositions have been extensively applied to marine sediments for palaeo-redox reconstruction. While the open ocean Mo isotope signature is conservative on time scales of several million years, and depends on the changing global isotopic mass balance between input and output fluxes, large Mo isotope variability over smaller time scales has been identified in organic-rich sediments. In addition to changing dissolved sulfide levels and deep-water ventilation times, the varying extent of Fe and Mn oxide shuttling is also considered to be a cause of short-term variability in Mo isotopes. Here we present the Mo isotope composition of well-dated sediments from the redox-stratified Landsort Deep (Baltic Sea) covering the current warm period and the medieval climate anomaly. These modern sediments provide the unique opportunity to directly link water column redox conditions, derived from instrumental time-series, to the sedimentary Mo isotope record. We observe an overall lower Mo isotopic composition (av. δ<sup>98</sup>Mo −0.21 ‰) during longer-lasting bottom water hypoxia between ∼ 1955 and 2000 CE than during weakly sulfidic interruptions and sapropel formation since ∼ 2000 CE (av. δ<sup>98</sup>Mo + 0.63 ‰). Such lower δ<sup>98</sup>Mo signatures during hypoxia benefitted from intense Mn oxide-shuttling near the sediment/water interface. Sedimentary δ<sup>98</sup>Mo values as low as −0.94 ‰ compared to seawater, most likely required intense Mo isotope fractionation via repeated Mn oxide shuttling, aided by incomplete thiolation at a weakly sulfidic sediment/water interface, before Mo was finally sequestered from strongly sulfidic porewaters. Such combined Mo isotope fractionation is also seen in the weakly sulfidic and hypoxic water columns of the Landsort and Gotland Deeps, which suggests significant changes in Mo cycling depending on the presence of dissolved sulfide and Mn oxide. Based on comparable geochemical variations, similar redox dynamics could be also attested for the Landsort Deep sediments deposited during the medieval climate anomaly.</div><div>In comparison to other modern O<sub>2</sub>-deficient marine settings ranging from mildly reducing to strongly sulfidic conditions, the Landsort Deep sediments deposited during fluctuating sulfidic-hypoxic periods with intense shuttling of Mn oxides act as a distinct sink of isotopically light Mo from the ocean with overall lower δ<sup>98</sup>Mo compared to the marine Mo input flux. Widespread occurrence of Mn ores in organic matter-rich sediments throughout Earth’s history implies that dynamic redox conditions comparable to those in the Landsort Deep were more frequent. This could be particularly true for past periods of global warming, when the flooding of shelf areas promoted expansion of reducing bottom waters in epicontinental seas. Finally, the coupled Mo-Mn-S cycling during fundamental redox changes in such epicontinental settings, a
钼浓度和稳定同位素组成已被广泛应用于海相沉积物的古氧化还原重建。虽然开放海洋的Mo同位素特征在数百万年的时间尺度上是保守的,并且取决于输入和输出通量之间不断变化的全球同位素质量平衡,但在更小的时间尺度上,在富有机物沉积物中发现了较大的Mo同位素变异。除了改变溶解的硫化物水平和深水通风时间外,Fe和Mn氧化物穿梭的不同程度也被认为是Mo同位素短期变化的一个原因。本文介绍了波罗的海陆深氧化还原层状沉积物的Mo同位素组成,这些沉积物覆盖了当前暖期和中世纪气候异常。这些现代沉积物提供了独特的机会,可以直接将仪器时间序列得出的水柱氧化还原条件与沉积Mo同位素记录联系起来。我们观察到,在~ 1955年至2000年期间,在较长时间的底水缺氧期间,Mo同位素组成(δ98Mo−0.21‰)总体上低于自~ 2000年以来的弱硫化物中断和火山冲积形成期间(δ98Mo + 0.63‰)。低氧条件下δ98Mo特征的降低与沉积物/水界面附近Mn氧化物的强烈穿梭有关。与海水相比,沉积δ98Mo值低至- 0.94‰,很可能需要在弱硫化物沉积/水界面的不完全硫化作用下,通过重复的Mn氧化物来回移动进行强烈的Mo同位素分馏,然后Mo才最终从强硫化物孔隙水中隔离出来。在Landsort和Gotland deep的弱硫化物和缺氧水柱中也可以看到这种组合的Mo同位素分异,这表明Mo循环的显著变化取决于溶解硫化物和氧化锰的存在。基于可比较的地球化学变化,类似的氧化还原动力学也可以在中世纪气候异常时期沉积的Landsort Deep沉积物中得到证实。与其他现代海洋缺氧环境(从轻度还原到强硫化氢)相比,在波动的硫化氢-缺氧时期沉积的陆地深层沉积物具有强烈的锰氧化物往返,与海洋Mo输入通量相比,其δ98Mo总体较低,是一个同位素轻Mo的独特汇。在整个地球历史中,富含有机质的沉积物中广泛存在锰矿石,这意味着与陆地深层类似的动态氧化还原条件更为频繁。在过去的全球变暖时期尤其如此,当时陆架地区的洪水促进了大陆表层海洋底部水的扩张,减少了海底水的数量。最后,在这种陆表环境中,在基本氧化还原变化期间的耦合Mo- mn - s循环,类似于在现代陆地深层观测到的情况,可能会显著影响全球海洋Mo收支。
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引用次数: 0
Discovery of young submarine volcanism in the Cook Islands: New constraints on the location of the Rarotonga hotspot 库克群岛年轻海底火山活动的发现:拉罗汤加热点位置的新限制
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-29 DOI: 10.1016/j.gca.2025.12.058
Yifan Du , Matthew G. Jackson , Brian Jicha , Andrew Kylander-Clark , Benjamin L. Byerly , Michael Bizimis , Sæmundur Ari Halldórsson , Gareth G.E. Seward , Olivia E. Anderson , Matthew Rioux , Kevin Konrad , Sunna Harðardóttir , Ruixia Bai , Andrea Giuliani , Douglas A. Wiens , S. Shawn Wei , Gerald McCormack , John Michael Parianos
A multiple-hotspot origin has been proposed for the Cook–Austral volcanic lineament in the southwest (SW) Pacific. One candidate, the Rarotonga hotspot, is associated with volcanism on only two islands: Rarotonga (1.157 ± 0.003 to 1.697 ± 0.055 Ma) and Aitutaki (youngest stage: 1.382 ± 0.058 to 1.941 ± 0.035 Ma), located ∼250 km apart in a north–south (N–S) direction. Their overlapping eruption ages and lack of clear age progression preclude a robust evaluation of a hotspot origin. This study identifies and investigates a new volcanic feature, Tama Seamount—located ∼80 km east–southeast (ESE) of Rarotonga Island along a Pacific plate flowline—potentially associated with the Rarotonga hotspot. New ages from two lavas (40Ar/39Ar groundmass ages: 0.664 ± 0.027 and 0.816 ± 0.020 Ma) and from a nepheline syenite xenolith—including zircon U–Pb dating (weighted mean age: 0.74 ± 0.02 Ma) and a biotite 40Ar/39Ar age (0.730 ± 0.007 Ma)—constrain Tama’s age. These ages align with a Rarotonga hotspot age progression based on Pacific plate motion, and support a Rarotonga hotspot origin for Tama. We also report on the first lava samples dredged from the submarine flanks of Rarotonga Island, which exhibit geochemical fingerprints and an age (1.493 ± 0.007 Ma) consistent with those of previous Rarotonga samples. Furthermore, radiogenic isotopes of Tama samples in this study overlap with existing Rarotonga Island data, supporting a genetic relationship between Tama Seamount and Rarotonga Island. Together, these new results suggest Tama Seamount represents the youngest known expression of the Rarotonga hotspot.
提出了西南太平洋Cook-Austral火山线的多热点起源。一个候选人,拉罗汤加热点,在只有两个岛屿与火山活动有关:拉罗汤加(1.157 ± 0.003到1.697 ±0.055  Ma)和Aitutaki(最小的阶段:1.382 ± 0.058到1.941 ±0.035  Ma),位于∼250 公里在南北方向(n)。它们重叠的喷发年龄和缺乏明确的年龄进展妨碍了对热点起源的可靠评估。这项研究确定并调查了一个新的火山特征,Tama海山——位于拉罗汤加岛东南偏东(ESE)约80 公里处,沿着太平洋板块流线——可能与拉罗汤加热点有关。新时代从两个熔岩(40 ar / 39 ar石基年龄:0.664 ±  0.027和0.816±0.020  Ma)和霞石正长岩xenolith-including锆石U-Pb约会(加权平均年龄:0.74 ±0.02  Ma)和黑云母40 ar / 39 ar年龄(0.730 ±0.007  Ma),抑制了一只名叫阿玉的年龄。这些年龄与基于太平洋板块运动的拉罗汤加热点年龄进展一致,并支持塔摩的拉罗汤加热点起源。我们还报道了从拉罗汤加岛海底侧翼打捞的第一批熔岩样本,这些样本显示了地球化学指纹,年龄(1.493 ± 0.007 Ma)与以前的拉罗汤加样品一致。此外,本研究中Tama样品的放射性成因同位素与现有的Rarotonga岛数据重叠,支持Tama海山与Rarotonga岛之间的遗传关系。总之,这些新的结果表明,塔玛海山代表了已知的拉罗汤加热点最年轻的表达。
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引用次数: 0
Photochemical behavior between oxalate and Sb(V)/As(V)-bearing jarosite: Reaction mechanism, mineral transformation, and elemental fate 草酸盐与含Sb(V)/As(V)黄铁矾的光化学行为:反应机理、矿物转化和元素命运
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2026-01-11 DOI: 10.1016/j.gca.2026.01.010
Qi Huang , Guining Lu , Xiaohu Jin , Xiaodong Du , Xiaofei Li , Qian Yao , Lijuan Zeng , Xueqin Tao , Jianmin Zhou , Zhi Dang
Jarosite is a common metastable iron mineral in acid sulfate-rich environments, which is known to retain antimony (Sb) and arsenic (As). Sunlight has emerged as a critical driver for the dissolution of iron minerals, especially in the presence of dissolved organic matter (DOM). However, the mechanisms governing jarosite dissolution and associated Sb/As migration under the coexistence of sunlight and DOM remain poorly understood. Here, we employed a series of techniques, including in situ attenuated total reflection-Fourier transform infrared spectroscopy (ATR-FTIR), scanning transmission electron microscopy (STEM), and chemical extraction, to investigated the photochemical behavior of Sb(Ⅴ)/As(Ⅴ)-bearing jarosite with the representative DOM-oxalate (OA) under simulated sunlight. The results indicated that OA was predominantly adsorbed onto the jarosite surface via mononuclear bidentate (MB) binding geometry. Under light irradiation, OA underwent photolysis on the jarosite surface, thereby inducing reductive dissolution of the mineral. The dissolution rate of jarosite was faster under anoxic conditions than under oxic conditions, and both rates increased with increasing OA dosage. Notably, high OA dosage (2.5 mM) induced jarosite transformation to humboldtine under anoxic conditions and to lepidocrocite under oxic conditions. This difference in transformation gave rise to distinct mobility of Sb and As, as the results demonstrated that the formed lepidocrocite exhibited a superior capability to fix Sb and As compared to humboldtine. Additionally, the photoaged Sb preferentially partitioned into the poorly crystalline phase, whereas As tended to adsorb onto the mineral surface. These findings provide new insights into the photochemical interactions between iron minerals and DOM, and reveal the differences in the photochemical transformation of jarosite under anoxic and oxic environments. These are crucial for predicting the behavior of Sb and As in sunlit environments.
黄钾铁矾是富酸性硫酸盐环境中常见的亚稳铁矿物,具有锑(Sb)和砷(As)的特性。阳光已经成为铁矿物溶解的关键驱动力,特别是在溶解有机物(DOM)存在的情况下。然而,在阳光和DOM共存的情况下,黄铁矾溶解和相关Sb/As迁移的机制尚不清楚。本文采用原位衰减全反射-傅里叶变换红外光谱(ATR-FTIR)、扫描透射电子显微镜(STEM)和化学萃取等一系列技术,研究了含Sb(Ⅴ)/As(Ⅴ)黄钾铁矾与代表性的dom -草酸盐(OA)在模拟阳光下的光化学行为。结果表明,OA主要通过单核双齿结合结构吸附在黄钾铁矾表面。在光照射下,OA在黄钾铁矾表面发生光解作用,从而诱导矿物的还原性溶解。缺氧条件下黄钾铁矾的溶解速率比缺氧条件下快,且随OA用量的增加而增加。值得注意的是,高剂量的OA (2.5 mM)诱导黄铁矾在缺氧条件下转化为洪堡石,在缺氧条件下转化为鳞铁石。这种转变的差异导致Sb和As的迁移率明显,结果表明,形成的鳞片石比洪堡石具有更强的固定Sb和As的能力。此外,光老化的Sb优先分配到低晶相,而As倾向于吸附在矿物表面。这些发现为研究铁矿物与DOM之间的光化学相互作用提供了新的思路,揭示了缺氧和缺氧环境下黄钾铁矾光化学转化的差异。这些对于预测Sb和As在阳光环境中的行为至关重要。
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引用次数: 0
Modeling extreme nitrogen isotope variability in Neoarchean diamonds from Knee Lake, Superior Craton 苏必利尔克拉通膝湖新太古代钻石氮同位素极端变异模型
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-19 DOI: 10.1016/j.gca.2025.12.039
Andrea Pezzera, Long Li, Richard A. Stern, D. Graham Pearson
<div><div>The nitrogen (N) isotope composition of world-wide diamonds shows considerable variability that is uncorrelated with carbon isotopes. Most of this variability is currently explained by different compositions of the N sources, although fractionation processes can nonetheless play a role. Because N in Earth’s mantle is overprinted by subduction as time progresses, we examined the N isotope composition of the Knee Lake diamond suite, hosted in volcaniclastic rocks erupted in the Neoarchean at ∼2.73 Ga, to try to obtain an older glimpse of N isotope variability. Secondary ion mass spectrometry analyses of 186 Knee Lake diamonds revealed extraordinarily varied N isotope compositions, expanding from the lowest (−46.8 ‰) to the highest (+31.8 ‰) values measured for terrestrial diamonds, strongly clustered around a median of −0.7 ‰. The median value advocate for a heavier-than modern δ<sup>15</sup>N composition of the Archean mantle, suggesting a secular change from a <sup>15</sup>N-enriched primordial composition. Whether some of the δ<sup>15</sup>N variability in the Knee Lake diamonds could have been inherited by crustal recycled or unmixed primordial sources, the range and discontinuous distribution of the most extreme values rule out an overall explanation as being formed by mixing of heterogeneous N sources and suggests the involvement of fractionation processes. The systematics of N concentration ([N]) and δ<sup>15</sup>N variations for most of the Knee Lake diamonds are permissive of a Rayleigh distillation process. Rayleigh distillation during kinetic isotope fractionation associated with the decomposition of N-phases could even produce the most <sup>15</sup>N-enriched compositions and the uncorrelated [N] and δ<sup>13</sup>C variability. However, Ryleigh fractionation cannot produce the most <sup>15</sup>N-depleted compositions. The extreme N isotope compositions in the Knee Lake diamond suite are correlated with crystal shape, the most negative δ<sup>15</sup>N values occurring in cuboid and the most positive in octahedral crystals. This suggests the operation of kinetic N fractionation processes related to different growth-surface structures or growth conditions. Despite the recognition of distinct N isotope compositions in different growth sectors in synthetic crystals, two mixed-habit Knee Lake diamonds show only a small growth-sector related N isotope variability. The only process we can model that is capable of producing the most <sup>15</sup>N-depleted values is diffusion along chemical gradients, whether pre-existing in the growth environment or generated by crystal growth under diffusion-limited conditions as indicated by the re-entrant, fibrous shape of some cuboid crystals. These observations highlight the complexity of nitrogen isotope geochemistry in the Earth mantle, and suggest that various kinetic effects may play a role in fractionating the N isotope compositions of some diamonds during their growth. The possibility of
世界范围内钻石的氮(N)同位素组成显示出与碳同位素无关的相当大的变异性。尽管分选过程仍然可以发挥作用,但大多数这种变异目前可以用氮源的不同组成来解释。由于地幔中的N随着时间的推移被俯冲覆盖,我们研究了膝湖钻石套件的N同位素组成,该套件位于新太古代约2.73 Ga喷发的火山碎屑岩中,试图获得更古老的N同位素变化。对186颗膝湖钻石的二次离子质谱分析显示,N同位素组成变化非常大,从最低(- 46.8‰)到最高(+31.8‰)的陆地钻石测量值,强烈聚集在−0.7‰的中位数附近。中值表明太古宙地幔的δ15N成分重于现代,表明太古宙地幔的δ15N成分与富15n的原始成分发生了长期变化。无论膝关节湖钻石中的某些δ15N变率是否可能由地壳再循环或未混合的原始源继承,最极端值的范围和不连续分布排除了由非均质N源混合形成的整体解释,并表明分馏过程的参与。大多数Knee Lake钻石的N浓度([N])和δ15N变化系统允许瑞利蒸馏过程。在动力学同位素分馏过程中,与N相分解相关的瑞利蒸馏甚至可以产生最富15n的成分和不相关的[N]和δ13C变率。然而,Ryleigh分馏不能产生最缺15n的组分。膝湖钻石组的极端N同位素组成与晶体形状相关,负δ15N值在长方体晶体中出现最多,正δ15N值在八面体晶体中出现最多。这表明动力学N分馏过程的操作与不同的生长表面结构或生长条件有关。尽管在合成晶体的不同生长扇区中发现了不同的N同位素组成,但两颗混合习性的Knee Lake钻石仅显示出与生长扇区相关的小N同位素变异。我们能够模拟的唯一能够产生最多15n耗尽值的过程是沿着化学梯度的扩散,无论是在生长环境中预先存在的,还是在扩散限制条件下晶体生长产生的,如一些长方体晶体的重新进入,纤维状形状所表明的那样。这些观测结果突出了地幔中氮同位素地球化学的复杂性,并表明各种动力学效应可能在某些钻石生长过程中对氮同位素组成的分异起作用。钻石生长过程中N同位素分馏的可能性表明,在存在极端值的情况下,即使在地幔的高温下,也要谨慎使用同位素示踪剂。
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引用次数: 0
Organic carbon cycling in hemipelagic and turbidite sediments of Santa Monica Basin, California Borderland 圣莫尼卡盆地半深海和浊积岩沉积物中的有机碳循环
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-27 DOI: 10.1016/j.gca.2025.12.053
David J. Burdige , Tomoko Komada
We examined carbon cycling in the upper ∼ 1.2 m of sediments from the center of Santa Monica Basin (SMB) CA using a reaction-transport model applied to dissolved organic carbon (DOC) and dissolved inorganic carbon (DIC) concentration and isotope signature profiles (δ13C and Δ14C). The sediments here consist of ∼ 20 cm of laminated hemipelagic sediment and a ∼ 1 m thick layer containing sand-silt turbidites. Linear solute profiles of inorganic reactants or products of anoxic remineralization in the turbidite layer suggest that this is largely a diffusion-dominated zone. Model results support this interpretation showing that remineralization in the turbidite sediments is ∼ 2 % of that in the upper hemipelagic sediments.
Benthic fluxes of DOC from SMB sediments contain both “labile” and “refractory” components, as has also been observed in studies of nearby Santa Barbara Basin (SBB) sediments. When the two sets of results are compared, there appears to be a larger flux of labile DOC from SMB versus SBB sediments. Differences in the nature of iron redox cycling in the surface sediments of the two basins may explain these observations.
If the relative amounts of refractory DOC in the total benthic DOC fluxes from SMB and SBB sediments are representative of continental margin sediments globally, then the integrated flux of sediment-derived refractory DOC represents ∼ 3–160 % of the refractory DOC added to the oceans. At its high end, this suggests that some of the refractory DOC which leaves these anoxic sediments as a benthic flux may be remineralized in oxic marine waters on time scales shorter than ocean mixing.
Model results from SMB and SBB provide evidence that sediments are a potential source of both refractory and pre-aged (14C-depleted) DOC to the oceans. Specifically, the benthic flux of refractory DOC from both basins includes components with Δ14C signatures that range from around −300‰ to −400‰, or even lower. This occurs because some fraction of the refractory DOC produced in the sediments (and ultimately added to the water column as a benthic flux) is either “pre-aged” in the sediments based on its pre-depositional OM source, or is produced by remineralization of less reactive OM whose 14C content decreases with sediment age and burial. At the same time, SMB and SBB sediments are not representative, in general, of continental margin and coastal sediments, and the broader relevance of the benthic flux of 14C depleted DOC (and its impact on the radiocarbon signature of deep ocean DOC) will require further studies in a wider range of sedimentary environments.
本文研究了圣莫尼卡盆地(SMB) CA中心沉积物上部~ 1.2 m的碳循环,采用反应-输移模型,应用于溶解有机碳(DOC)和溶解无机碳(DIC)浓度和同位素特征剖面(δ13C和Δ14C)。这里的沉积物由~ 20厘米的层状半深海沉积物和~ 1米厚的砂粉浊积层组成。浊积层中无机反应物或缺氧再矿化产物的线性溶质剖面表明,这主要是一个以扩散为主的区域。模型结果支持这一解释,表明浊积岩沉积物中的再矿化作用是上半深海沉积物中的再矿化作用的2%。SMB沉积物中DOC的底栖生物通量既含有“不稳定”成分,也含有“难降解”成分,这在附近的圣巴巴拉盆地(SBB)沉积物的研究中也观察到。当两组结果进行比较时,SMB比SBB沉积物的不稳定DOC通量更大。两个盆地表面沉积物中铁氧化还原循环性质的差异可能解释了这些观察结果。如果SMB和SBB沉积物的底栖DOC总通量中难降解DOC的相对量代表了全球大陆边缘沉积物,那么沉积源难降解DOC的综合通量代表了海洋中添加的难降解DOC的~ 3 - 160%。在其高端,这表明一些难降解的DOC离开这些缺氧沉积物作为底栖生物通量可能在缺氧海水中再矿化,时间尺度比海洋混合时间短。SMB和SBB的模型结果提供了证据,表明沉积物是海洋中难降解和预老化(14c耗尽)DOC的潜在来源。具体来说,这两个盆地的难熔DOC底栖通量包括Δ14C特征组分,范围在- 300‰至- 400‰左右,甚至更低。这是因为沉积物中产生的难降解DOC(最终作为底栖生物通量添加到水柱中)的一部分要么是根据沉积前OM的来源在沉积物中“预老化”的,要么是由活性较低的OM再矿化产生的,其14C含量随着沉积物年龄和埋藏而降低。同时,SMB和SBB沉积物一般不具有大陆边缘和沿海沉积物的代表性,14C耗尽DOC的底栖生物通量(及其对深海DOC放射性碳特征的影响)的更广泛相关性将需要在更广泛的沉积环境中进一步研究。
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引用次数: 0
Reprocessing of lunar crust at ∼4.3 Ga inferred from in situ U-Pb isotopic and trace element investigation of Northwest Africa 11479 从非洲西北部U-Pb原位同位素和微量元素调查推断的月球地壳在~ 4.3 Ga的再处理11479
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2026-01-11 DOI: 10.1016/j.gca.2026.01.007
Jingyou Chen , Shaolin Li , Shiyong Liao , Jian Chen , Alexander Nemchin , Katherine H. Joy , Xiaochao Che , Weibiao Hsu , Menghua Zhu
The increasing identification of magnesian anorthosites (MAN) in lunar meteorites, along with inferences from remote sensing techniques, has intensified research interest in understanding their role in lunar crust formation. However, the lack of robust geochronological constraints for MAN impeded our comprehension of the timeline of crustal evolution. The lunar feldspathic breccia meteorite, Northwest Africa (NWA) 11479, is composed primarily of Mg-rich, KREEP-poor (K, rare earth elements, and P) highland lithic fragments, predominantly consisting of magnesian anorthositic lithologies (including anorthosite noritic/troctolitic anorthosites, and the associated magnesian granulites). The close chemical match between the bulk rock and lunar remote sensing data supports a farside origin, providing evidence for the presence of MAN in the Feldspathic Highlands Terrane (FHT).
Zircon and apatite grains have been discovered within the small Mg-rich anorthositic clasts in NWA 11479. Notably, the occurrence of these highly evolved accessory minerals contrasts with the depletion of incompatible trace elements in the coexisting silicates, suggesting their formation via interactions between the anorthositic crust and a later-stage KREEPy metasomatic melt. In-situ U-Pb isotopic analysis of the zircon and apatite yields a well-defined discordia line, with an upper intercept date of 4328 ± 9 Ma (2σ), and a lower intercept date of 140 ± 64 Ma (2σ). The younger age likely reflects a more recent impact event, whereas the upper intercept is consistent with both the concordant U-Pb zircon date (4327 ± 12 Ma, 2σ) and the weighted average 207Pb/206Pb date of the zircon and apatite (4326 ± 8 Ma, 2σ). This ∼ 4.33 Ga age is interpreted as the timing of metasomatism responsible for the formation of the zircon and apatite, or an impact event. Importantly, this age obtained from the putative-origin meteorite coincides with the period (4.3–4.35 Ga) of the active secondary magmatism recorded in nearside-collected Apollo samples, the proposed formation age of the giant South Pole–Aitken (SPA) basin. These temporal correlations suggest that this epoch represents a major phase of global reworking of the primordial lunar crust, likely driven by the overturn of mantle cumulates, and further associated with basin‑scale impact events, or both.
月球陨石中越来越多的镁质斜长岩(MAN)的发现,以及遥感技术的推断,加强了对其在月球地壳形成中的作用的研究兴趣。然而,对MAN缺乏强有力的年代学约束阻碍了我们对地壳演化时间的理解。西北非洲(NWA) 11479月长石角砾岩主要由富镁、贫钾(K、稀土元素和P)的高原岩屑组成,主要由镁质斜长岩岩性组成(包括镁长石/硅长石斜长岩和伴生的镁质粒粒岩)。大块岩石与月球遥感数据之间的密切化学匹配支持了远侧起源,为长石高地Terrane (FHT)中存在MAN提供了证据。
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引用次数: 0
A novel experimental V-Sc olivine-melt oxybarometer for arc magmas 一种新型的实验性V-Sc橄榄石熔体氧气压表
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-15 DOI: 10.1016/j.gca.2025.12.025
Enzo-Enrico Cacciatore, Ivano Gennaro, Kalin Kouzmanov, Alexandra Tsay, Zoltán Zajacz
<div><div>Redox conditions significantly affect phase equilibria, the availability and mobility of heterovalent elements, including volatiles (e.g., S) and metals (e.g., Fe, Cu) in silicate melts. Gaining a deeper understanding of the initial redox state of magmas may help better understand magmatic ore fertility, volcanic degassing, and the redox evolution of Earth’s crust and atmosphere.</div><div>This study reports optimized V and novel V-Sc olivine-melt oxybarometers, developed using existing V-partitioning data and new results from a series of fractional crystallization experiments. Experiments were conducted in a rapid-quench molybdenum-hafnium carbide pressure vessel apparatus equipped with a custom-designed hydrogen membrane for flexible, precise, and accurate oxygen fugacity (<em>f</em>O<sub>2</sub>) control. In some experiments, solid buffers were additionally applied. They were performed at constant pressure (<em>P</em> = 200 <!--> <!-->MPa) and variable temperatures (<em>T</em> = 1019–920 °C), under water-saturated conditions at <em>f</em>O<sub>2</sub> ranging from −1<!--> <!-->to + 3.5<!--> <!-->log<!--> <!-->units relative to the FMQ buffer. The impact of the system’s composition (<em>X</em>) was evaluated by comparing two distinct liquid lines of descent (medium-K-calk-alkaline and shoshonitic) through simultaneous experiments using two capsules in parallel. The results show that the partition coefficient of V between olivine and melt <span><math><mrow><mo>(</mo><msubsup><mtext>D</mtext><mrow><mtext>V</mtext></mrow><mtext>[Ol/melt]</mtext></msubsup><mo>)</mo></mrow></math></span> is not systematically affected by varying <em>P</em>-<em>T</em>-<em>X</em> and highly correlates with changing <em>f</em>O<sub>2</sub>, thus suggesting that the minor variations observed on a global <em>f</em>O<sub>2</sub> scale rather reflect analytical and experimental uncertainties. The updated empirical calibrations allow the determination of log<em>f</em>O<sub>2</sub> as ΔFMQ from measured 1)<!--> <span><math><msubsup><mtext>D</mtext><mrow><mtext>V</mtext></mrow><mtext>[Ol/melt]</mtext></msubsup></math></span> and 2)<!--> <span><math><msubsup><mtext>K</mtext><mrow><mtext>D</mtext><mtext>[V/Sc]</mtext></mrow><mtext>[Ol/melt]</mtext></msubsup></math></span>, expressed by the following equations: <span><math><mrow><mrow><mn>1</mn><mo>)</mo><mspace></mspace><mi>Δ</mi><mi>F</mi><mi>M</mi><mi>Q</mi><mo>=</mo><mo>-</mo><mn>1.723</mn><mspace></mspace><mo>±</mo><mspace></mspace><mn>0.047</mn><mo>-</mo></mrow><mfenced><mrow><mfrac><mrow><msub><mi>log</mi><mn>10</mn></msub><mrow><mo>[</mo><mrow><mo>(</mo><mn>1.230</mn><mspace></mspace><mo>-</mo><msubsup><mtext>log(D</mtext><mrow><mtext>V</mtext></mrow><mtext>[Ol/melt]</mtext></msubsup><mo>)</mo></mrow><mo>)</mo></mrow><mo>/</mo><mrow><mo>(</mo><msubsup><mtext>log(D</mtext><mrow><mtext>V</mtext></mrow><mtext>[Ol/melt]</mtext></msubsup><mo>)</mo></mrow><mo>+</mo><mn>3.119</mn><mspace></mspace><mrow><mo>)</mo><mo>]
氧化还原条件显著影响硅酸盐熔体中相平衡、异价元素的可用性和迁移率,包括挥发物(如S)和金属(如Fe、Cu)。对岩浆初始氧化还原状态的深入了解,有助于更好地理解岩浆矿石肥力、火山脱气以及地壳和大气的氧化还原演化。本研究报告优化V和新型V- sc橄榄石熔体氧压计,利用现有的V-分配数据和一系列分数结晶实验的新结果开发。实验在快速淬火碳化钼铪压力容器装置中进行,该装置配备了定制的氢膜,用于灵活、精确和准确地控制氧逸度(fO2)。在一些实验中,还添加了固体缓冲液。实验在恒压(P = 200 MPa)和变温度(T = 1019-920℃)下进行,水饱和条件下,相对于FMQ缓冲液,fO2在−1到+ 3.5 log单位之间。通过同时使用两个胶囊进行平行实验,通过比较两种不同的液体下降线(中钾钙碱性和松石质)来评估系统成分(X)的影响。结果表明,橄榄石和熔体之间的V分配系数(DV[Ol/melt])不受P-T-X变化的系统影响,而与fO2的变化高度相关,从而表明在全球fO2尺度上观测到的微小变化反映了分析和实验的不确定性。更新的经验校准允许从测量的1)DV[Ol/melt]和2)KD[V/Sc][Ol/melt]中测定logfO2为ΔFMQ,用以下公式表示:1)ΔFMQ=-1.723±0.047-log10[(1.230-log(DV[Ol/melt]))/(log(DV[Ol/melt])+3.119)]-0.099±0.002对于NBO/T(每个四面配位离子的非桥接氧)≤0.6:2)ΔFMQ=(log(KD[V/Sc][Ol/melt])+0.981±0.022)/-0.206±0.012。在与弧岩浆作用有关的FMQ -1至FMQ + 3.5的logfO2范围内,以及在含水条件下,两种氧压计的2σ校准不确定度均低于0.5 log单位。更新和新的基于v的氧气压计增强了在广泛的P-T-X-fO2范围内的稳健性,能够准确量化岩浆系统的氧化还原状态。反过来,它们可以应用于从玄武岩到安山岩组成的火山岩,通过使用合适的橄榄石硅酸盐熔融包裹体来重建俯冲带深部岩浆储层的氧化还原历史。此外,我们证实了橄榄石熔体FeT- mg交换系数(其中FeT是用FeO表示的总铁)与fO2的变化相关,可以作为本研究校准范围内的Fe-Mg氧晴雨表。由于铁在橄榄石中的快速扩散,这种方法可以记录快速氧化还原波动,并为更强大的v基氧气压计提供补充约束。
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Experiments were conducted in a rapid-quench molybdenum-hafnium carbide pressure vessel apparatus equipped with a custom-designed hydrogen membrane for flexible, precise, and accurate oxygen fugacity (&lt;em&gt;f&lt;/em&gt;O&lt;sub&gt;2&lt;/sub&gt;) control. In some experiments, solid buffers were additionally applied. They were performed at constant pressure (&lt;em&gt;P&lt;/em&gt; = 200 &lt;!--&gt; &lt;!--&gt;MPa) and variable temperatures (&lt;em&gt;T&lt;/em&gt; = 1019–920 °C), under water-saturated conditions at &lt;em&gt;f&lt;/em&gt;O&lt;sub&gt;2&lt;/sub&gt; ranging from −1&lt;!--&gt; &lt;!--&gt;to + 3.5&lt;!--&gt; &lt;!--&gt;log&lt;!--&gt; &lt;!--&gt;units relative to the FMQ buffer. The impact of the system’s composition (&lt;em&gt;X&lt;/em&gt;) was evaluated by comparing two distinct liquid lines of descent (medium-K-calk-alkaline and shoshonitic) through simultaneous experiments using two capsules in parallel. The results show that the partition coefficient of V between olivine and melt &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;msubsup&gt;&lt;mtext&gt;D&lt;/mtext&gt;&lt;mrow&gt;&lt;mtext&gt;V&lt;/mtext&gt;&lt;/mrow&gt;&lt;mtext&gt;[Ol/melt]&lt;/mtext&gt;&lt;/msubsup&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; is not systematically affected by varying &lt;em&gt;P&lt;/em&gt;-&lt;em&gt;T&lt;/em&gt;-&lt;em&gt;X&lt;/em&gt; and highly correlates with changing &lt;em&gt;f&lt;/em&gt;O&lt;sub&gt;2&lt;/sub&gt;, thus suggesting that the minor variations observed on a global &lt;em&gt;f&lt;/em&gt;O&lt;sub&gt;2&lt;/sub&gt; scale rather reflect analytical and experimental uncertainties. The updated empirical calibrations allow the determination of log&lt;em&gt;f&lt;/em&gt;O&lt;sub&gt;2&lt;/sub&gt; as ΔFMQ from measured 1)&lt;!--&gt; &lt;span&gt;&lt;math&gt;&lt;msubsup&gt;&lt;mtext&gt;D&lt;/mtext&gt;&lt;mrow&gt;&lt;mtext&gt;V&lt;/mtext&gt;&lt;/mrow&gt;&lt;mtext&gt;[Ol/melt]&lt;/mtext&gt;&lt;/msubsup&gt;&lt;/math&gt;&lt;/span&gt; and 2)&lt;!--&gt; &lt;span&gt;&lt;math&gt;&lt;msubsup&gt;&lt;mtext&gt;K&lt;/mtext&gt;&lt;mrow&gt;&lt;mtext&gt;D&lt;/mtext&gt;&lt;mtext&gt;[V/Sc]&lt;/mtext&gt;&lt;/mrow&gt;&lt;mtext&gt;[Ol/melt]&lt;/mtext&gt;&lt;/msubsup&gt;&lt;/math&gt;&lt;/span&gt;, expressed by the following equations: &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mi&gt;Δ&lt;/mi&gt;&lt;mi&gt;F&lt;/mi&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;mi&gt;Q&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mo&gt;-&lt;/mo&gt;&lt;mn&gt;1.723&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;±&lt;/mo&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mn&gt;0.047&lt;/mn&gt;&lt;mo&gt;-&lt;/mo&gt;&lt;/mrow&gt;&lt;mfenced&gt;&lt;mrow&gt;&lt;mfrac&gt;&lt;mrow&gt;&lt;msub&gt;&lt;mi&gt;log&lt;/mi&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;/msub&gt;&lt;mrow&gt;&lt;mo&gt;[&lt;/mo&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mn&gt;1.230&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mo&gt;-&lt;/mo&gt;&lt;msubsup&gt;&lt;mtext&gt;log(D&lt;/mtext&gt;&lt;mrow&gt;&lt;mtext&gt;V&lt;/mtext&gt;&lt;/mrow&gt;&lt;mtext&gt;[Ol/melt]&lt;/mtext&gt;&lt;/msubsup&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;mo&gt;/&lt;/mo&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;msubsup&gt;&lt;mtext&gt;log(D&lt;/mtext&gt;&lt;mrow&gt;&lt;mtext&gt;V&lt;/mtext&gt;&lt;/mrow&gt;&lt;mtext&gt;[Ol/melt]&lt;/mtext&gt;&lt;/msubsup&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;mo&gt;+&lt;/mo&gt;&lt;mn&gt;3.119&lt;/mn&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;mrow&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;mo&gt;]","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"415 ","pages":"Pages 106-129"},"PeriodicalIF":5.0,"publicationDate":"2026-02-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145786148","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Heterogeneous distribution of moderately volatile elements in the Moon determined from Apollo 15 and 17 pyroclastic glass beads 由阿波罗15号和17号火山碎屑玻璃珠测定的中等挥发性元素在月球上的非均匀分布
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-30 DOI: 10.1016/j.gca.2025.12.059
Eleanor C. McIntosh, James M.D. Day
The Apollo 17 high-Ti orange (74220) and Apollo 15 low-Ti green (15426) lunar pyroclastic glasses are some of the most primitive igneous samples from the Moon and are considered critical for understanding the volatile content of the lunar interior. The orange and green glass deposits are petrologically distinct, containing both holohyaline (glassy) and crystallized beads. In this study, edge and center analyses on holohyaline beads representative of the deposits were conducted by laser ablation inductively coupled plasma mass spectrometry to constrain the distribution of moderately volatile elements (MVE: K, Cu, Zn, Cs, Ga, Ge, Rb, Cd, and Pb), and trace element images were produced of the beads in 74220. Bead edges have elevated MVE abundances compared to centers in the larger (107 µm average diameter) low-Ti Apollo 15 green glasses, likely resulting from syn-eruptive processes. Leaching experiments of 15426 bulk beads support a large fraction of Na, K, Zn, Cu, Cd and Pb on their outer surfaces. The smaller (42 µm average diameter) high-Ti Apollo 17 orange glasses have a greater extent of overlap in MVE contents between bead edges and centers. Orange and green glass bead centers offer approximations of melt MVE abundances, indicating ∼500 µg/g K, ≤20 µg/g Zn, ∼6 µg/g Cu, <4 µg/g Ga, ≤ 1 µg/g Rb, <0.1 µg/g Pb and ≤ 100 µg/g K, ≤1 µg/g Zn, ≤2.5 µg/g Cu, <2 µg/g Ga, ≤ 0.5 µg/g Rb and Pb, respectively. These estimates are as much as ten times lower than bulk bead MVE abundances within the pyroclastic glass deposits, are depleted compared to terrestrial mid-ocean ridge basalts, and are similar to, or lower than, bulk silicate Earth (BSE) concentration estimates. Partial melting estimates for the source of the pyroclastic glass beads indicate similarities with tholeiitic and komatiite lavas on Earth and between ∼10 and 30 % melting of their mantle source, consistent with high mantle potential temperatures at ∼3.5 billion years ago in the Moon. The estimated MVE composition of the orange glass bead mantle source is marginally higher than the green glass mantle source, and both are within or lower than bulk silicate Moon estimates. More shallowly derived mare basalts have been shown to be yet more MVE depleted, indicating that the lunar interior had a heterogeneous distribution of volatile elements, with a deep interior with volatile abundances ∼10 times lower than BSE sampled by the pyroclastic glass beads, volatile-poor upper magma ocean cumulates, and an incompatible volatile-enriched KREEP reservoir.
阿波罗17号的高钛橙色(74220)和阿波罗15号的低钛绿色(15426)月球火山碎屑玻璃是来自月球的一些最原始的火成岩样品,被认为是了解月球内部挥发性成分的关键。橙色和绿色的玻璃矿床在岩石学上是独特的,含有全透明(玻璃状)和结晶珠。本研究采用激光烧蚀电感耦合等离子体质谱法对具有代表性的全息玻璃微珠进行了边缘和中心分析,以限制中等挥发性元素(MVE: K、Cu、Zn、Cs、Ga、Ge、Rb、Cd和Pb)的分布,并对74220微珠进行了微量元素图像分析。与较大的低钛阿波罗15号绿色玻璃(平均直径107µm)的中心相比,珠状玻璃边缘的MVE丰度更高,这可能是由于同喷发过程造成的。15426颗粒珠的浸出实验表明,颗粒珠的外表面含有大量的Na、K、Zn、Cu、Cd和Pb。较小(平均直径42µm)的高钛阿波罗17号橙色玻璃在玻璃头边缘和中心之间的MVE含量重叠程度更大。橙色和绿色玻璃珠中心提供熔体MVE丰度的近似值,分别表示~ 500µg/g K,≤20µg/g Zn, ~ 6µg/g Cu, <4µg/g Ga,≤1µg/g Rb, <;0.1µg/g Pb和≤100µg/g K,≤1µg/g Zn,≤2.5µg/g Cu, <2µg/g Ga,≤0.5µg/g Rb和Pb。这些估算值比火山碎屑玻璃矿床中的整体珠状MVE丰度低10倍之多,与陆地中海脊玄武岩相比已经枯竭,与整体硅酸盐土(BSE)浓度估算值相似或更低。火山碎屑玻璃珠来源的部分熔融估计表明,它们与地球上的拉斑岩和科玛蒂岩熔岩相似,其地幔来源的熔点在~ 10%至30%之间,与~ 35亿年前月球上的高地幔电位温度一致。橙色玻璃珠幔源的MVE组成估价值略高于绿色玻璃幔源,两者均低于或低于“月球”估算值。更浅层衍生的海玄武岩已被证明更缺乏MVE,这表明月球内部挥发性元素的分布不均匀,深层内部的挥发性丰度比火山碎屑玻璃珠取样的BSE低10倍,挥发性差的上部岩浆海洋堆积,以及一个不相容的富含挥发物的KREEP储层。
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引用次数: 0
Experimental and theoretical investigation of antimony isotope fractionation during Sb(III) adsorption on iron (oxyhydr)oxides under anaerobic environment 厌氧环境下Sb(III)吸附铁(氧)氧化物过程中锑同位素分馏的实验与理论研究
IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2026-02-15 Epub Date: 2025-12-02 DOI: 10.1016/j.gca.2025.11.050
Wenju Wang , Hai-Bo Qin , Jian-Ming Zhu , Hongtao He , Decan Tan , Peng Zhao , Yan Zhang , Chengshuai Liu , Yoshio Takahashi , Mingshi Wang
Antimony (Sb) isotopes have emerged as reliable proxies for tracing pollutant sources, elucidating geochemical processes, and reconstructing paleoredox conditions. However, Sb isotope fractionation during Sb(III) adsorption on Fe (oxyhydr)oxides under anaerobic conditions is not yet fully understood, particularly concerning fractionation factors and molecular-scale mechanisms, which constrains the broader application of Sb isotopes. Here we systematically examined the adsorption behavior and isotopic fractionations for Sb(III) adsorption on goethite, lepidocrocite, and ferrihydrite in anaerobic systems, by combining Sb isotope measurements, X-ray absorption fine structure (XAFS) spectroscopy, and first-principles calculations. Results showed that Sb isotope fractionation (Δ123Sbaqueous-adsorbed) ranged from + 0.25 ‰ to + 0.41 ‰ during adsorption, with lighter Sb isotopes preferentially enriched in the adsorbed phase regardless of solution pH and mineral surface coverage. The comparable fractionation magnitudes induced by the adsorption of goethite, lepidocrocite, and ferrihydrite are likely attributed to the formation of bidentate edge-sharing (2E) and bidentate corner-sharing (2C) inner-sphere complexes revealed by XAFS analyses. The first-principles calculations further demonstrated that structural distortions in 2C and 2E complexes on the goethite (1 1 0) facet, particularly changes in their O-Sb-O bond angle, critically govern Sb isotope fractionation during Sb(III) adsorption. Our findings elucidate molecular-scale mechanisms driving Sb isotopic fractionation during Sb(III) adsorption on Fe (oxyhydr)oxides in anaerobic systems, and highlight the Sb isotope as a potential proxy for deciphering the microscopic geochemical processes at mineral–water interfaces. This work advances the understanding of Sb cycling in natural systems and provides a theoretical foundation for applying Sb isotopic signatures to trace geochemical processes and reconstruct paleoenvironment.
锑(Sb)同位素已成为追踪污染源、阐明地球化学过程和重建古氧化还原条件的可靠指标。然而,在厌氧条件下,Sb(III)吸附在Fe(氧)氧化物上时,Sb同位素的分馏尚未完全了解,特别是关于分馏因素和分子尺度机制,这限制了Sb同位素的广泛应用。本文通过结合Sb同位素测量、x射线吸收精细结构(XAFS)光谱和第一性原理计算,系统地研究了厌氧系统中Sb(III)在针铁矿、蛭石和水合铁上的吸附行为和同位素分异。结果表明:吸附过程中Sb同位素分异(Δ123Sbaqueous-adsorbed)范围为+ 0.25‰~ + 0.41‰,与溶液pH和矿物表面覆盖度无关,较轻的Sb同位素优先富集于吸附相;由针铁矿、绢云母和水合铁的吸附引起的相当的分选幅度可能归因于XAFS分析显示的双齿共边(2E)和双齿共角(2C)内球配合物的形成。第一线原理计算进一步表明,2C和2E配合物在针铁矿(11 - 10)面上的结构畸变,特别是它们的O-Sb-O键角的变化,对Sb(III)吸附过程中Sb同位素的分馏起关键作用。我们的研究结果阐明了厌氧系统中Sb(III)吸附在Fe(氧)氧化物上时Sb同位素分馏的分子尺度机制,并强调了Sb同位素作为解读矿物质-水界面微观地球化学过程的潜在代理。本研究促进了对自然系统中锑循环的认识,为应用锑同位素特征追踪地球化学过程和重建古环境提供了理论基础。
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Geochimica et Cosmochimica Acta
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