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Late Neoarchean–Paleoproterozoic granitoid basement serves as an effective helium source rock in cratonic basins 晚新太古代—古元古代花岗岩基底是克拉通盆地有效的氦源岩
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-09-11 DOI: 10.1016/j.precamres.2025.107905
Wenqi Li , Huichuan Liu , Greg Holland , Zheng Zhou , Jianfa Chen , Xiaoping Liu , Zhiqi Yu , Jian Li , Xiaobo Wang
The growing shortage of helium reserves presents a pressing worldwide concern. However, it remains ambiguous that how, when, and which type of tectonic environment the helium source rocks were formed. Recently, several helium-enriched gas fields have been discovered in the northern Ordos Block and confirmed to be crust-derived. Why late Neoarchean–Paleoproterozoic effective helium source rocks are distributed in the northern Ordos Block are still not clear. Detailed petrological, geochemical, geochronology, Sr-Nd isotopic and in-situ EPMA of U,-Th rich minerals studies were analyzed on the outcrops and drill cores of the basement of the northern Ordos Block to investigate the helium source rocks. The results show that (1) Late Neoarchean–Paleoproterozoic A-type granite and S-type granitoids are effective helium source rock types, and a large amount of U-Th rich accessory minerals (e.g., phosphate minerals, zircon, magnetite et al.) are preserved in alkaline feldspar and quartz. (2) The helium source rocks are classified into distinct temporal intervals: 2.60–2.45 Ga, 2.45–2.30 Ga and 1.95–1.80 Ga, respectively. 2.60–2.45 Ga granitoids exhibit compositional signatures of I-type granites, consistent with magmatic arc tectonic settings linked to subduction zones. 2.45–2.30 Ga granitoids display both A-type and I-type granitic affinities, indicating long live continental magmatic arc environment characteristics.1.95–1.80 Ga granitoids exhibit both A-type and S-type characteristics, suggesting formation in an extensional tectonic regime following continental collision. (3) 2.60–2.45 Ga period is late Archean subduction-accretion and arc magmatism, followed by arc-continent collision; 2.45–2.30 Ga period is a long-time arc-continental accretion process with multiple arc magmatism; 1.95–1.80 Ga period represents continent-continent collision to post-collisional extension setting. Thus, the long-term arc-continental accretion and multistage crustal recycling of terrigenous sediments with high U and Th content, comparable to Phanerozoic subduction-accretionary orogens, explain why effective helium source rocks are enriched in the northern Ordos Block. By the comparison of Khondalite Belts in North China Craton with global Khondalite Belts, global Khondalite belts could be favorable areas for predicting the worldwide distribution of helium source rocks.
氦储量的日益短缺是一个紧迫的全球性问题。然而,氦源岩是如何形成的、何时形成的、在何种构造环境中形成的,仍然是一个不明确的问题。近年来,在鄂尔多斯地块北部发现了几个富氦气田,并确认为壳源性气田。鄂尔多斯地块北部新太古代-古元古代有效氦源岩分布的原因尚不清楚。对鄂尔多斯地块北部基底露头和岩心进行了详细的岩石学、地球化学、年代学、Sr-Nd同位素和U、-Th富矿物原位EPMA研究,探讨了氦源岩。结果表明:(1)晚新太古代—古元古代a型花岗岩和s型花岗岩类是有效的氦源岩类型,碱性长石和石英中保存了大量富U-Th的副矿物(如磷矿物、锆石、磁铁矿等)。(2)氦源岩划分为2.60 ~ 2.45 Ga、2.45 ~ 2.30 Ga和1.95 ~ 1.80 Ga三个不同的时间段。2.60 ~ 2.45 Ga花岗岩具有i型花岗岩的组成特征,符合与俯冲带相关的岩浆弧构造背景。2.45 ~ 2.30 Ga花岗岩类具有a型和i型花岗岩亲和性,反映了长寿的大陆岩浆弧环境特征;1.95 ~ 1.80 Ga花岗岩类具有a型和s型花岗岩亲和性,表明形成于大陆碰撞后的伸展构造环境。(3) 2.60 ~ 2.45 Ga为晚太古宙俯冲-增生-弧岩浆作用期,其次为弧-陆碰撞期;2.45-2.30 Ga期为长时间弧陆吸积过程,多弧岩浆活动;1.95 ~ 1.80 Ga时期为大陆-大陆碰撞至碰撞后伸展环境。因此,与显生宙俯冲-增生造山带相当的高U、高Th含量陆源沉积物的长期弧陆增生和多期地壳再循环,解释了鄂尔多斯地块北部有效氦源岩富集的原因。通过华北克拉通孔雀岩带与全球孔雀岩带的对比,认为全球孔雀岩带是预测全球氦源岩分布的有利区域。
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引用次数: 0
Temporal and magmatic evolution of the Neoproterozoic ultramafic and mafic Ougda arc complex and associated granitoids (Western Tuareg Shield, Algeria) 阿尔及利亚西图阿雷格地盾新元古代超基性和基性奥格达弧杂岩及其花岗岩类的时间和岩浆演化
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-09-10 DOI: 10.1016/j.precamres.2025.107903
Chaouki Djallel Eddine Bendimerad , Abderrahmane Bendaoud , Julien Berger , Renaud Caby , Gaston Godard , Karel Schulmann
The Ougda area, located within the Tassendjanet terrane of the Western Tuareg Shield, hosts a large (ultra)mafic complex associated with granitoid intrusions. This magmatic complex represents a Neoproterozoic continental arc, active between 749 ± 2 Ma and 653 ± 4 Ma ago; during this time, various ultramafic and mafic (meta)cumulates (serpentinites, hornblendites, garnet amphibolites, amphibolites and leucogabbros) and non-cumulates (amphibole gabbros, quartz diorites, diorites) were emplaced. The latter exhibit a calc-alkaline affinity. Sr-Nd isotope data reveal a distinct contrast between North and South Ougda ultramafic and mafic units. The North Ougda units have a more juvenile signature (εNd = +6.3 to +9.4, ISr = 0.70248–0.70377) than the South Ougda units (εNd = +5.3 to +6.3, ISr = 0.70267–0.70400). Early arc construction is represented by the emplacement of the South Ougda units into a thinned juvenile crust at shallow crustal levels. In contrast, the younger and more juvenile North Ougda units were emplaced at deeper crustal levels, likely at the base of the arc crust.
Syn-collisional granitoids, dated at 626 ± 5 Ma and 627 ± 4 Ma, intruded the Tassendjanet terrane and show a hybrid juvenile-crustal signature (εNd = +2.68 to −8.04, ISr = 0.70296–0.70743), interpreted as resulting from the partial melting of juvenile basaltic rocks in the lower crust of the Ougda arc, followed by the crustal contamination of primitive magmas. In addition, aplitic dykes crosscutting these granitoids display geochemical characteristics similar to those of the post-collisional granites that sealed the Panafrican orogeny in the Tuareg Shield. The Ougda continental arc complex is believed to have formed during the closure of an oceanic basin, leading to the amalgamation of West Gondwana and ultimately to the Pan-African orogeny observed across the Neoproterozoic NW African provinces.
奥格达地区位于西图阿雷格地盾的塔森珍妮特地块内,拥有一个与花岗岩类侵入有关的大型(超)基性复杂岩体。该岩浆杂岩为新元古代大陆弧,活动时间为749±2 Ma ~ 653±4 Ma;在此期间,各种超镁铁质和基性(变)堆积物(蛇纹岩、角闪岩、石榴石角闪岩、角闪岩和浅辉长岩)和非堆积物(角闪岩、石英闪长岩、闪长岩)被侵位。后者表现出钙碱性亲和力。Sr-Nd同位素数据揭示了南北奥格达超镁铁和基性单元的明显对比。北奥格达单元(εNd = +6.3 ~ +9.4, ISr = 0.70248 ~ 0.70377)比南奥格达单元(εNd = +5.3 ~ +6.3, ISr = 0.70267 ~ 0.70400)具有更明显的幼化特征。早期弧的构造表现为南奥格达单元在地壳浅层进入一个变薄的幼年地壳。相比之下,更年轻和更年轻的北奥格达单元位于更深的地壳水平,可能在弧壳的底部。同碰撞花岗岩类(626±5 Ma和627±4 Ma)侵入Tassendjanet地体,表现出幼体-地壳混合特征(εNd = +2.68 ~−8.04,ISr = 0.70296 ~ 0.70743),解释为奥格达弧下地壳幼体玄武岩部分熔融,然后是原始岩浆的地壳污染。此外,横切这些花岗岩的胶结脉显示出与图阿雷格地盾中封闭泛非造山作用的碰撞后花岗岩相似的地球化学特征。奥格达大陆弧复合体被认为是在一个海洋盆地闭合期间形成的,导致了西冈瓦纳的合并,并最终形成了横跨新元古代西北非洲省的泛非造山运动。
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引用次数: 0
Paired metamorphic belts in the Usagaran Orogen of Tanzania: evidence for one-sided oceanic subduction in the Palaeoproterozoic 坦桑尼亚乌萨加兰造山带的成对变质带:古元古代单侧大洋俯冲的证据
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-09-09 DOI: 10.1016/j.precamres.2025.107891
V. Schenk , T. Sarkar , D. Wiemer
Paired metamorphic belts (PMB) are the tectono-metamorphic expression of the one-sided subduction of oceanic lithosphere beneath continental margins and island arcs, which represents a key characteristic of terrestrial plate tectonics. PMB that are spatially and timely paired are mainly known from Phanerozoic orogenic belts, although the metamorphic rock record points to a duality of thermal regimes since the Palaeoproterozoic. Here we describe the tectono-metamorphic evolution of the Usagaran Orogen at the SE-margin of the Tanzania Craton, which includes PMB of Palaeoproterozoic age. The orogen’s lithological inventory reflects a Wilson cycle: (1) The passive margin sequence (Konse Group) was deposited during the Lomagundi carbon isotope excursion (2.22–2.06 Ga) and metamorphosed at 2.03 Ga during the Usagaran orogeny. (2) The precursors of most eclogites were ocean-floor basalts, but those of the Ky- and Opx-eclogites of boninite chemistry were related to subduction-initiation. Peak eclogite metamorphism at mantle depths (850–880 °C/18–19 kbar) was followed by transient granulite-facies conditions during exhumation (750–800 °C/6–10 kbar). High-T-P shear zones in Opx-eclogites and felsic mylonites formed at P < 15 > 10 kbar are related to exhumation. (3) High-P amphibolite-facies metamorphism of metasediments enveloping the eclogite belt (770 °C/13.2 kbar at 2.0 Ga) is attributed to an accretionary wedge setting. The concurrent evolutions and the preserved growth zonations in garnet of both units point to a shared short-lived metamorphism. (4) Low-P Grt-Crd-Sil-granulites, which overlie the accretionary wedge metasediments as a nappe, experienced a counter-clockwise P-T path at ca. 2.06 Ga (peak 820 °C/7.2 kbar) in an arc setting that predates the orogeny for 50–60 Myr. We attribute their protomylonitic texture to post-peak NW-thrusting towards the orogenic foreland during collision. Late-stage P-T paths of all units in the nappe stack (isobaric cooling at 20 km depth) are interrelated. Other Palaeoproterozoic PMB in orogens around the Congo Craton and in the Yangtze Craton, in addition to subduction-related eclogites in the Trans-North China Orogen, indicate that subduction of oceanic lithosphere and its partial exhumation after slab breakoff at mantle depths were already viable tectonic processes. Pre-Neoproterozoic eclogites representing exhumed oceanic crust are dominantly known from a short time interval (2.1–1.8 Ga), during which warm (12–14 °C/km) and cold (<11 °C/km) subduction zones existed, which both show the tectono-metamorphic characteristics akin to modern asymmetric one-sided oceanic subduction.
对变质带(PMB)是大洋岩石圈在大陆边缘和岛弧下单向俯冲的构造变质表现,是陆地板块构造的一个重要特征。虽然变质岩记录显示了古元古代以来的二元热机制,但在空间和时间上配对的PMB主要来自显生宙造山带。本文描述了坦桑尼亚克拉通东南缘Usagaran造山带的构造变质演化,其中包括古元古代的PMB。(1)被动边缘层序(Konse群)在Lomagundi碳同位素漂移时期(2.22 ~ 2.06 Ga)沉积,在Usagaran造山带2.03 Ga变质。(2)大部分榴辉岩的前体为海底玄武岩,而宝钢化学的Ky-和opx -榴辉岩的前体则与俯冲起生有关。在地幔深度(850-880°C/ 18-19 kbar)的榴辉岩变质作用达到峰值,随后是挖掘过程中(750-800°C/ 6-10 kbar)的瞬态麻粒岩相条件。在P <; 15 >; 10 kbar形成的opx榴辉岩和长英质糜棱岩的高t -P剪切带与发掘有关。(3)包裹榴辉岩带的变质沉积物(770℃/13.2 kbar, 2.0 Ga)的高磷角闪岩相变质作用属于楔形增生环境。这两个单位在石榴石中的同步演化和保存下来的生长带表明它们共同经历了短暂的变质作用。(4)低磷grt - crd - si -麻粒岩在约2.06 Ga(峰值820°C/7.2 kbar)的弧形环境中经历了逆时针P-T路径,早于50-60 Myr的造山运动。其原糜棱岩结构是碰撞过程中造山前陆向北西逆冲的峰后构造。推覆层各单元的后期P-T路径(20 km深度等压冷却)是相互关联的。刚果克拉通和扬子克拉通周围造山带的其他古元古代PMB,以及跨华北造山带中与俯冲有关的榴辉岩,表明大洋岩石圈的俯冲及其在地幔深处板块断裂后的部分掘出已经是可行的构造过程。前新元古代榴辉岩主要是在短时间间隔(2.1 ~ 1.8 Ga)内发现的,在此期间存在温暖(12 ~ 14℃/km)和寒冷(<11℃/km)的俯冲带,具有类似于现代不对称单边海洋俯冲的构造变质特征。
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引用次数: 0
Late Mesoproterozoic mafic magmatism in the southwestern Yangtze Block and its implications for reconstructing the Rodinia supercontinent 扬子地块西南晚中元古代基性岩浆活动及其对罗迪尼亚超大陆重建的意义
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-09-09 DOI: 10.1016/j.precamres.2025.107904
Dongxue Li , Mingguo Zhai , Lu Xiang , Hailong He , Junping Liu , Hanlin Chen
Late Mesoproterozoic igneous rocks are traditionally considered a key hallmark of the Grenvillian Orogeny and have been widely utilized in reconstructing the Rodinia supercontinent. Despite increasing attention to Late Mesoproterozoic magmatism in the southwestern Yangtze Block, the tectonic evolution of this region during that time still remains unresolved, leading to ongoing debate regarding the role of the Yangtze Block in Rodinia assembly. Here, we report two suites of ca. 1085 Ma mafic rocks from the Dongchuan area in the SW Yangtze Block to investigate their petrogenesis and assess their implications for reconstructing the Yangtze Block in the Rodinia supercontinent. The studied mafic rocks are characterized by high TiO2 content (1.49–4.49 wt%) and low Mg# values (22–56), exhibiting slight enrichment in light rare earth elements, with (La/Yb)N ratios ranging from 1.65 to 5.24, and displaying trace element patterns analogous to E-MORB, without significant Nb-Ta or Zr-Hf anomalies. Their zircon εHf(t) and whole-rock εNd(t) values range from 1.9 to 9.4 and 0.7 to 4.9, respectively, indicating that their primary magmas were derived from the partial melting of a depleted mantle source. In contrast, their zircon δ18O values vary from 5.50 ± 0.29 ‰ to 6.78 ± 0.39 ‰, likely reflecting the involvement of subducted oceanic mafic crust in the magma source. Moreover, their geochemical characteristics, such as high Zr/Y ratios and elevated Ti concentrations, are consistent with formation in an intra-continental rifting environment. Integrated with the presence of other 1.2–1.0 Ga intraplate magmatism in the SW Yangtze Block, we propose that the block most possibly remained an independent landmass during 1.2–1.1 Ga and began drifting toward Rodinia between 1.1 and 1.0 Ga, ultimately positioning itself on the periphery rather than at the core of the supercontinent.
中元古代晚期火成岩被认为是格林尼治造山运动的重要标志,并被广泛用于重建罗丁尼亚超大陆。尽管人们对扬子地块西南部晚中元古代岩浆活动的关注越来越多,但该地区在这一时期的构造演化仍未得到解决,因此关于扬子地块在Rodinia组合中的作用的争论仍在继续。本文报道了西南扬子地块东川地区两套约1085 Ma的基性岩,探讨了它们的成因,并评价了它们对Rodinia超大陆扬子地块重建的意义。研究的基性岩石具有TiO2含量高(1.49 ~ 4.49 wt%)、Mg#值低(22 ~ 56)的特征,轻稀土元素轻度富集,(La/Yb)N比值在1.65 ~ 5.24之间,微量元素模式与E-MORB相似,Nb-Ta和Zr-Hf无明显异常。锆石εHf(t)和全岩εNd(t)值分别在1.9 ~ 9.4和0.7 ~ 4.9之间,表明其原生岩浆来源于衰竭地幔源的部分熔融作用。锆石δ18O值变化范围为5.50±0.29‰~ 6.78±0.39‰,可能反映了洋基俯冲地壳参与岩浆源作用。高Zr/Y比值、高Ti浓度等地球化学特征与陆内裂陷环境相一致。结合扬子地块西南段1.2 ~ 1.0 Ga板块内岩浆活动的存在,我们认为该地块在1.2 ~ 1.1 Ga期间很可能是一个独立的陆块,并在1.1 ~ 1.0 Ga之间开始向Rodinia漂移,最终定位于超大陆的外围而非核心。
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引用次数: 0
U–Pb zircon geochronology and geochemistry of Um Genud layered mafic intrusion in the northern tip of the Arabian-nubian shield: implications for the genesis of the plutonic crust of neoproterozoic immature intra-oceanic arc 阿拉伯-努比亚盾北端Um Genud层状基性侵入体的U-Pb锆石年代学和地球化学:对新元古代未成熟洋内弧深部地壳成因的启示
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-09-05 DOI: 10.1016/j.precamres.2025.107915
Tarek H. Abu El-Kheir , Keda Cai , Ayman E. Maurice , Kai Wang , Hairuo Wang , Maher Dawoud
The Um Genud Neoproterozoic layered mafic intrusion, located in the South Eastern Desert of Egypt, represents the northwestern tip of the juvenile crust of the Arabian-Nubian Shield (ANS). This intrusion is composed of olivine gabbro, gabbro, noritic-gabbro and hornblende gabbro. Zircon U–Pb data constrain the emplacement age of the intrusion to 718 Ma, coinciding with the island arc stages of the ANS. The trace element patterns of pyroxenes, amphiboles, whole-rock samples and calculated melts in equilibrium with clinopyroxene and amphibole show marked Nb-Ta and Zr-Hf troughs and prominent peak of Pb. These features, along with the trace element abundances and ratios in zircon, suggest that the parental magma was generated in an intra-oceanic island arc setting from a depleted mantle source metasomatized by subducted slab-derived aqueous fluids. Textural features, mineral compositions of olivine, pyroxene and plagioclase, whole-rock geochemical characteristics, the calculated ƒO2 values (FMQ + 1 – FMQ + 1.6), and the estimated water content (5.9 – 9.1 wt%) of melt indicate that the Um Genud gabbroic rocks represent cumulates differentiated from oxidized hydrous low-K tholeiitic magma, essentially by fractional crystallization. The estimated pressure of crystallization (∼3 to ∼ 3.5 kbar; ∼10 km depth), the low-K tholeiitic nature of parental magma and the relative abundance of the exposed gabbroic and granitic arc rocks in the study area are consistent with intrusion emplacement within the lower crust of an immature oceanic arc. This implies that even arcs with thin crust can develop considerable plutonic layers and contribute to continental crust growth through vertical accretion.
位于埃及沙漠东南部的Um Genud新元古代层状基性侵入岩,代表了阿拉伯-努比亚盾(ANS)幼壳的西北端。该侵入岩由橄榄辉长岩、辉长岩、北辉长岩和角闪辉长岩组成。锆石U-Pb资料限定了该岩体的侵位年龄为718 Ma,与ANS的岛弧阶段一致,辉石、角闪石、整岩样品以及与斜辉石和角闪孔平衡的计算熔体微量元素模式显示出明显的Nb-Ta和Zr-Hf槽,Pb峰明显。这些特征以及锆石中微量元素的丰度和比值表明,母岩浆是在洋内岛弧背景下由俯冲板源水交代的衰竭地幔源形成的。构造特征、橄榄石、辉石和斜长石矿物组成、全岩地球化学特征、熔体ƒO2值(FMQ + 1 ~ FMQ + 1.6)计算和熔体含水量(5.9 ~ 9.1 wt%)估算表明,Um Genud辉长岩主要是由氧化含水低钾拉斑岩浆分异而成。估计结晶压力(~ 3 ~ ~ 3.5 kbar; ~ 10 km深度)、母岩浆的低钾拉斑性质以及研究区内暴露的辉长岩和花岗质弧岩的相对丰度与未成熟洋弧下地壳的侵入侵位一致。这意味着即使是地壳薄的弧也可以发育相当大的深成层,并通过垂直增生促进大陆地壳的增长。
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引用次数: 0
Kilometer-scale hook-shaped Type2/Type3 folds due to refolding and transpressional strike-slip reversal in the Egyptian Nubian Shield, east African orogenic belt 东非造山带埃及-努比亚盾逆转走滑作用下的千米尺度钩状2/ 3型褶皱
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-09-05 DOI: 10.1016/j.precamres.2025.107912
Mohamed A. Abd El‑Wahed , Ahmed M. Eldosouky , Osama M.K. Kassem , Ahmed Abdelhady Abo-Rayan , Mohamed Attia
This study combines remote sensing, aeromagnetic data, and field investigations to provide the initial identification of hook-shaped Type 2/Type 3 folds within the Egyptian Nubian Shield. The Western Allaqi shear belt (WASB) exhibits remarkable refolded structures that are distinctly observable from space. This belt primarily comprises ophiolite slices, metavolcanics, and volcanoclastic metasediments, which have been intruded by syn- (729–635 Ma) and post-tectonic granites (610–543 Ma). The WASB region experienced significant compression during the N-S shortening (830–720 Ma), leading to the formation of east–west oriented folds and foliation and N-dipping thrust imbrications. The interference patterns of the folds predominantly display Type 2 and Type 3 refolds characterized by wavelengths on the order of kilometers. The geological observation reveals a complex history of deformation, with refolded folds linked to dextral shear zones, ductile and brittle fabrics, and opposing movement directions. The fold interference structures were formed through the reactivation of NW-trending sinistral strike-slip shear zones, combined with shear-related folding of the initial F1 folds, and NE-SE compression (625–565 Ma). The subsequent development of NW-trending Haseierbah folds (F2) was accompanied by a shift in stress orientation from NE-SW to E-W (620–580), resulting in a reversal of shear sense and the reactivation of NW-trending shear zones into dextral strike-slip shear zones, which in turn formed the N-trending El-Quleib fold (F3) and the NE-trending Haimur and Shilman folds (F4). This reversal in shear sense contributes to the formation of Type 2 and Type 3 fold interference patterns and the distinctive hook-shaped fold structures observed within the WASB. This study provides a detailed description of refolding and transpressional strike-slip reversal in the WASB, highlighting the innovative tectonic evolution and urging a reassessment of the entire Allaqi-Heinai suture and the major shear zones in the Egyptian Nubian Shield.
该研究结合了遥感、航磁数据和实地调查,初步确定了埃及努比亚盾内的2/ 3型钩形褶皱。西阿拉奇剪切带(WASB)表现出非凡的折叠式结构,从太空中可以清楚地观察到。该带主要由蛇绿岩片、变质火山和火山碎屑沉积组成,曾被syn- (729-635 Ma)和后构造花岗岩(610-543 Ma)侵入。830 ~ 720ma南北向缩短期,WASB区域经历了明显的挤压作用,形成了东西向的褶皱、片理和向n倾斜的逆冲叠瓦构造。褶皱的干涉图案主要显示波长在千米量级的2型和3型折痕。地质观测揭示了一个复杂的变形历史,与右旋剪切带、韧性和脆性织物以及相反的运动方向有关的再折叠褶皱。褶皱干涉构造是由北西向左旋走滑剪切带的重新激活、F1初始褶皱的剪切相关褶皱和NE-SE挤压作用(625 ~ 565 Ma)共同形成的。随着北西向Haseierbah褶皱(F2)的发育,应力方向由NE-SW向E-W转变(620-580),导致剪切意义逆转,北西向剪切带重新活化为右旋走滑剪切带,进而形成n向El-Quleib褶皱(F3)和ne向Haimur和Shilman褶皱(F4)。这种剪切意义上的反转有助于形成2型和3型褶皱干涉模式,并在WASB内观察到独特的钩状褶皱结构。该研究详细描述了WASB的折叠式走滑反转和转压式走滑反转,强调了构造演化的创新性,并敦促对整个Allaqi-Heinai缝合带和埃及努比亚盾的主要剪切带进行重新评估。
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引用次数: 0
Origin of the Brunovistulian microcontinent: Geochemical and Sr–Nd–Pb–Hf isotope evidence 布鲁诺维斯纪微大陆的起源:地球化学和Sr-Nd-Pb-Hf同位素证据
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-08-26 DOI: 10.1016/j.precamres.2025.107902
Simona Krmíčková , Lukáš Krmíček , Martin J. Timmerman , Jiří Sláma , Jitka Míková
The Brunovistulian microcontinent (BVM) represents the largest (up to 30 000 km2) geological unit of Proterozoic provenance in the eastern part of the Variscan collision zone in Central Europe. We present whole-rock, mineral and Sr–Nd–Pb–Hf isotope compositions of representative samples from exposures and deep boreholes (up to 3 km in depth) situated in the Czech part of the BVM. The oldest rocks are ∼ 740 Ma Tonian basic metavolcanic rocks and associated felsic dykes and metatuffs of the Metavolcanic Zone. Geochemical and isotope characteristics of these felsic rocks confirm that their parent melts were derived from the upper mantle, similar to their metabasite hosts. The Tonian (Pan-African) age of the Metavolcanic Zone and its MORB-like geochemical and isotope signature (87Sr/86Sr = 0.7027; ɛNd = +5.6; ɛHf = +10) reflect the main phase of rifting during breakup of Rodinia and subsequent formation of volcanic island arcs. Granitoids forming the two principal domains of the BVM, the Slavkov Domain situated to the NE, and the Thaya domain situated to the SW, both intruded during the dominant magmatic activity at ∼ 600 Ma. The Sr–Nd–Pb–Hf isotope compositions of granitoids of the Slavkov Domain are typical of relatively primitive volcanic arc magmas. Thus, the Slavkov Domain may represent an eroded relic of a juvenile Neoproterozoic volcanic arc that developed above a subduction zone, very probably at an active Gondwanan margin of the Tornquist Ocean. Possibility of slab breakoff during arc formation cannot be ruled out. In contrast, the Thaya Domain originated by melting of Proterozoic mature continental crust above the same subducting slab at the Gondwanan margin. During subduction, significantly older remnants of an island arc (∼655 Ma Metadiorite Zone) and MORB-like volcanic rocks (∼740 Ma Metavolcanic Zone) were accreted to the continental margin, leading to the assemblage of the Brunovistulian microcontinent. Based on the depleted mantle Nd model ages, the lithosphere of the BVM has retained an isotope signature similar to Avalonia.
Brunovistulian微大陆(BVM)是中欧Variscan碰撞带东部最大的元古代物源地质单元(面积达3万平方公里)。我们展示了位于BVM捷克部分的暴露和深钻孔(深达3公里)的代表性样品的全岩、矿物和Sr-Nd-Pb-Hf同位素组成。最古老的岩石是变质火山带的~ 740 Ma - Tonian基性变质火山岩及其伴生的长英质岩脉和变质岩。这些长英质岩石的地球化学和同位素特征证实了它们的母熔体来源于上地幔,与它们的变质岩宿主相似。变质火山带的Tonian(泛非)年龄及其类似morb的地球化学和同位素特征(87Sr/86Sr = 0.7027; Nd = +5.6; Hf = +10)反映了Rodinia断裂和火山岛弧形成的主要裂陷阶段。花岗岩类形成了BVM的两个主要域,位于东北方向的Slavkov域和位于西南方向的Thaya域,它们都是在约600 Ma的主导岩浆活动期间侵入的。斯拉夫科夫域花岗岩类的Sr-Nd-Pb-Hf同位素组成具有相对原始的火山弧岩浆特征。因此,Slavkov域可能代表了新元古代幼火山弧的侵蚀遗迹,该火山弧在俯冲带之上发育,很可能位于Tornquist洋的活跃冈瓦南边缘。不能排除弧形成过程中板坯断裂的可能性。而塔雅域则是由冈瓦南缘同一俯冲板块上元古代成熟大陆地壳的熔融作用形成的。在俯冲过程中,明显更古老的岛弧(~ 655 Ma变质长岩带)和morb样火山岩(~ 740 Ma变质火山带)的残余被增生到大陆边缘,导致了布鲁诺维斯微大陆的组合。根据枯竭地幔Nd模式年龄,BVM岩石圈保留了类似Avalonia的同位素特征。
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引用次数: 0
Petrogenesis of the Wuhe complex, southeastern margin of the North China Craton: implications for the Meso-Neoarchean crustal growth and evolution 华北克拉通东南缘五河杂岩的岩石成因:对中-新太古代地壳生长演化的启示
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-08-25 DOI: 10.1016/j.precamres.2025.107901
Hai-Yan Su , Yang Yang , Yi-Can Liu , Chris Yakymchuk
Archean granitoids and mafic igneous rocks are crucial records of the generation and differentiation of Archean continental crust. New U–Pb zircon geochronological data from granitoids, sanukitoids and mafic igneous rocks from the Wuhe complex, southeastern margin of the North China Craton (NCC) constrain the processes of early crustal growth and evolution in the Meso-Neoarchean period. Magmatic zircons from two granitoid gneisses yield weighted mean 207Pb/206Pb ages of 2986 ± 24 Ma and 2935 ± 11 Ma, followed by metamorphism at ca. 2.5 Ga and ca. 1.85 Ga. Sanukitoid gneisses have protolith crystallization ages of 2739 ± 5 Ma with zircon overgrowth rims at 2501 ± 22 Ma. Amphibolite yields a weighted mean 207Pb/206Pb age of 2500 ± 39 Ma, with metamorphism at 1846 ± 17 Ma. The granitoid gneisses show that they are characterized by steep rare earth element (REE) patterns, obviously negative Nb, Ta, Ti anomalies and positive Eu anomalies, high Sr/Y and (La/Yb)N ratios, and positive εHf(t) (+5.4 to +7.5) values. Their chemical compositions are similar to those of the TTG-like melts derived from juvenile mafic crust in the deep crust, implying a crustal growth event at ca. 3.0 Ga. The sanukitoid gneisses exhibit high MgO, Cr and Ni concentrations but relatively low (La/Yb)N values, positive εHf(t) values (+0.6 to +3.0). They were most likely originated from partial melting of mantle peridotite, which was significantly metasomatized by slab-derived granitoid melts, i.e. they plot on an evolution line. The amphibolites display the depleted mantle-derived geochemistry with positive εHf(t) (+1.2 to +3.2) values. Geochemical and zircon Hf isotopic compositions suggest that amphibolite was derived from partial melting of a depleted mantle with minor crustal contamination. Based on comparison of the spatial–temporal distribution and geochemical features of 3.0–2.9, ∼2.7 Ga and ∼2.5 Ga granitoids and amphibolites in the NCC, we propose that the Meso-Neoarchean crustal evolution of the Wuhe complex is similar to the whole NCC, which recorded significant crustal growth and reworking events at 3.0–2.9, 2.7 Ga and 2.5 Ga.
太古宙花岗岩和基性火成岩是太古宙大陆地壳生成和分异的重要记录。华北克拉通东南缘五河杂岩中花岗岩类、岩浆岩类和基性火成岩的新锆石U-Pb年代学资料约束了中-新太古代早期地壳的生长演化过程。两个花岗质片麻岩的岩浆锆石加权平均207Pb/206Pb年龄分别为2986±24 Ma和2935±11 Ma,其次是约2.5 Ga和约1.85 Ga的变质作用。Sanukitoid片麻岩的原岩结晶年龄为2739±5 Ma,锆石过度生长的边缘为2501±22 Ma。角闪岩的207Pb/206Pb加权平均年龄为2500±39 Ma,变质期为1846±17 Ma。花岗岩类片麻岩具有稀土元素(REE)模式陡峭,Nb、Ta、Ti负异常明显,Eu正异常明显,Sr/Y和(La/Yb)N高,εHf(t)正(+5.4 ~ +7.5)。它们的化学成分与来自深地壳幼年基性地壳的ttg类熔体相似,暗示了约3.0 Ga的地壳生长事件。类麻岩的MgO、Cr、Ni浓度较高,但La/Yb N值较低,εHf(t)值为正(+0.6 ~ +3.0)。它们极有可能起源于地幔橄榄岩的部分熔融,而地幔橄榄岩的部分熔融主要是由板状花岗岩类熔体交代的,即它们在一条演化线上。角闪岩的εHf(t)为正(+1.2 ~ +3.2),具有贫幔源地球化学特征。地球化学和锆石Hf同位素组成表明角闪岩起源于贫地幔的部分熔融,地壳污染较小。通过对比北陆3.0 ~ 2.9、~ 2.7 Ga和~ 2.5 Ga花岗岩类和角闪岩的时空分布和地球化学特征,认为中-新太古代五河杂岩的地壳演化与整个北陆相似,在3.0 ~ 2.9、2.7 Ga和2.5 Ga发生了显著的地壳生长和改造事件。
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引用次数: 0
Linking borate remobilization and mineralization to ∼1.85 Ga post-tectonic granitic magmatism in the northern North China Craton: Constraints from in-situ monazite, baddeleyite U-Pb and molybdenite Re-Os ages 华北克拉通北部硼酸盐再活化和成矿作用与~ 1.85 Ga构造后花岗质岩浆活动的联系:原位独居石、坏辉钼矿U-Pb和辉钼矿Re-Os年龄的制约
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-08-18 DOI: 10.1016/j.precamres.2025.107890
Li-Xing Li , Jian-Wei Zi , Yu Liu , Hou-Min Li , Yi Wang
Precambrian borate deposits are generally considered to have formed by multiple stages of metamorphic-hydrothermal events subsequent to boron-rich evaporite deposition, but determining the ages of hydrothermal overprinting and remobilization has proven to be challenging. The lack of robust geochronology data has hindered understanding of the geological controls on this type of mineralization. The Houxianyu boron deposit and Wengquangou boron-iron deposit, hosted in 2.05–1.93 Ga metamorphosed evaporites in northern North China Craton, represent the largest occurrences of Precambrian borate deposits. Monazite, molybdenite, baddeleyite and apatite are intergrown with borate minerals of szaibelyite and ludwigite, and thus can be dated to constrain the timing of boron-iron mineralization. In situ U-Pb and Re-Os geochronology yielded consistent Paleoproterozoic ages of 1854 ± 11 Ma (U-Pb monazite age), 1815 ± 4 Ma (U-Pb baddeleyite age) and 1825 ± 22 Ma (Re-Os molybdenite age) related to borate mineralization. These ages constrain the timing of boron and boron-iron mineralization to 1.86–1.81 Ga, which is younger than the ∼1.90 Ga regional metamorphism but contemporaneous with the ∼1.85 Ga post-tectonic granitic magmatism. This interpretation is further supported by field relationships which show that hydrothermal quartz-tourmalinite veins cross-cut the schistosity of the leptynites, and by the granitoid-affiliated accessory mineral assemblage (molybdenite, monazite and uraninite). Additionally, chondrite-normalized rare earth element (REE) patterns of apatite intergrown with ludwigite from borate ores show enrichment of LREEs relative to HREEs and strong negative Eu anomalies. These chemical features are similar to those of apatite from ∼1.85 Ga granites but distinct from those of apatite in metamorphosed rocks. Therefore, we propose that 1.86–1.81 Ga borate mineralization resulted from hydrothermal remobilization associated with the ∼1.85 Ga granitic magmatism. Our results negate the previously proposed genetic link between borate mineralization and ∼1.90 Ga regional metamorphism. These results, combined with previously published data, allow us to establish a hydrothermal B-Fe-U-Nb-Ta-Co-Ni metallogenic belt in relation to the ∼1.85 Ga post-tectonic granitic magmatism in northern North China Craton, potentially valuable for future exploration efforts.
前寒武纪硼酸盐矿床通常被认为是由富含硼的蒸发岩沉积后的多期变质热液事件形成的,但确定热液叠印和再活化的年龄已被证明是具有挑战性的。缺乏可靠的地质年代学资料阻碍了对这类成矿的地质控制的认识。华北克拉通北部2.05 ~ 1.93 Ga变质蒸发岩中赋存的后仙峪硼矿床和翁泉沟硼铁矿床是前寒武纪硼酸盐矿床的最大产状。独居石、辉钼矿、坏辉钼矿和磷灰石与辉钼矿和绿辉钼矿的硼酸矿物共生,可以对硼铁成矿时间进行定年。原位U-Pb和Re-Os年代学结果显示,与硼酸矿化有关的古元古代年龄分别为1854±11 Ma (U-Pb独居石年龄)、1815±4 Ma (U-Pb坏辉钼矿年龄)和1825±22 Ma (Re-Os辉钼矿年龄)。这些年龄限制了硼和硼铁成矿的时间为1.86 ~ 1.81 Ga,比~ 1.90 Ga区域变质作用年轻,但与~ 1.85 Ga构造后花岗质岩浆作用同时发生。这一解释进一步得到了现场关系的支持,这些关系表明热液石英-电气石脉与瘦斑岩的片岩相交叉,以及花岗岩类附属矿物组合(辉钼矿、独居石和铀矿)。此外,硼酸矿石中与镁辉石共生的磷灰石球粒陨石归一化稀土元素(REE)模式显示lree相对hree富集,且Eu负异常明显。这些化学特征与~ 1.85 Ga花岗岩中的磷灰石相似,但与变质岩中的磷灰石不同。因此,我们认为1.86-1.81 Ga硼酸盐矿化是由与~ 1.85 Ga花岗质岩浆活动相关的热液再活化引起的。我们的结果否定了先前提出的硼酸矿化与~ 1.90 Ga区域变质作用之间的遗传联系。这些结果与之前发表的数据相结合,使我们能够在华北克拉通北部建立与~ 1.85 Ga构造后花岗岩岩浆活动有关的热液B-Fe-U-Nb-Ta-Co-Ni成矿带,对未来的勘探工作具有潜在的价值。
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引用次数: 0
Subduction-induced crustal growth in the Neoproterozoic continental magmatic arc: Evidence from arc-type high-Mg# diorites and adakitic granitoids in the western Yangtze Block, South China 新元古代大陆岩浆弧俯冲诱发地壳生长:来自扬子地块西部弧型高镁闪长岩和埃达克花岗岩类的证据
IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-08-15 DOI: 10.1016/j.precamres.2025.107892
Rui-Yang Liu , Shao-cong Lai , Yu Zhu , Ren-Zhi Zhu , Min Liu , Jiang-Feng Qin , Fang-yi Zhang , Hang Yang
The coexistence of normal arc-type mafic-intermediate rocks and adakitic granodiorites can provide significant insights into the subduction-induced crustal growth. In this study, we present the comprehensive study of petrology, mineralogy, zircon U-Pb geochronology, bulk rock major and trace elements, Sr-Nd isotopes, zircon Lu-Hf isotopes, and electron microprobe (plagioclase, amphibole, biotite, and clinopyroxene) for the newly identified Neoproterozoic high-Mg# diorites (HMA) and adakitic granodiorites from the Kangding area along the western margin of the Yangtze Block (South China), to explore the subduction-induced crustal growth in the Neoproterozoic continental arc magma. The results show that the high-Mg# diorites formed at 792.9 Ma, and have much andesines, labradorites, high magnesium biotites and iron hornblendes, and are characterized by variably high MgO (3.62 ∼ 5.82 wt%) contents and Mg# (58.36 ∼ 60.49) values, showing the positive bulk rock εNd(t) (+0.84 ∼ +2.19) and zircon εHf(t) (+4.18 ∼ +9.44) values. The adakitic granodiorites formed at 793.5 Ma, and have much mineral of quartz, plagioclase, biotite as well as minor pyroxene and iron calcium magnesium amphibole. They contain high Sr (463.14 ∼ 494.44 ppm) and Y (10.41 ∼ 13.81 ppm) contents as well as Sr/Y (35.69 ∼ 47.49) ratios, indicating the adakitic dffinity. Theses adakitic granodiorites display positive εNd(t) (+1.52 ∼ +1.83) and zircon εHf(t) (+3.45 ∼ +7.14) values. Both types of rocks are enriched in LREEs (Light rare earth elements) and LILEs (Large ion lithophile elements) and depleted in Nb, Ta and Ti. We suggest that these high-Mg# diorites were derived from the partial melting of metasomatized mantle source enriched by subduction-related fluids, and the adakitic granodiorites were formed by partial melting of thickened juvenile mafic lower crust, which can reveal the subduction-induced crustal growth.
Combined with 860 ∼780 Ma mafic-intermediate-felsic rocks and 800 ∼750 Ma adakitic granitoids, we support that the Neoproterozoicc crustal growth were induced by metasomatized mantle-derived magmas. The subduction-induced crustal growth is vital for moulding the geochemical characteristics of arc magmatic rock types.
正弧型基性-中间岩与埃达克质花岗闪长岩的共存,对研究俯冲作用下的地壳生长具有重要意义。本文对扬子地块西缘康定地区新发现的新元古代高镁闪长岩(HMA)和阿达基花岗闪长岩进行了岩石学、矿物学、锆石U-Pb年代学、块状岩石主微量元素、Sr-Nd同位素、锆石Lu-Hf同位素和电子探针(斜长石、角闪洞、黑云母、斜辉石)等综合研究。探讨新元古代大陆弧岩浆中俯冲引起的地壳生长。结果表明:高Mg#闪长岩形成于792.9 Ma,含有大量安山岩、labradorites、高镁黑云母和铁角闪石,具有变高的MgO (3.62 ~ 5.82 wt%)含量和Mg#(58.36 ~ 60.49)值,呈现正的体岩εNd(t)(+0.84 ~ +2.19)和锆石εHf(t)(+4.18 ~ +9.44)值。易达质花岗闪长岩形成于793.5 Ma,矿物以石英、斜长石、黑云母为主,并有少量辉石和铁钙镁角闪洞。它们含有较高的Sr (463.14 ~ 494.44 ppm)和Y (10.41 ~ 13.81 ppm)含量以及Sr/Y(35.69 ~ 47.49)的比值,表明其同源性。阿达基花岗闪长岩的εNd(t)为正(+1.52 ~ +1.83),锆石的εHf(t)为正(+3.45 ~ +7.14)。两类岩石均富集轻稀土元素(lree)和大离子亲石元素(LILEs),亏损Nb、Ta和Ti。我们认为,这些高mg #闪长岩是俯冲相关流体富集的交代地幔源的部分熔融形成的,而阿达克质花岗闪长岩则是增厚的幼基性下地壳的部分熔融形成的,反映了俯冲引起的地壳生长。结合860 ~ 780 Ma的基性-中长英质岩石和800 ~ 750 Ma的埃达质花岗岩,我们认为新元古代的地壳生长是由交代幔源岩浆引起的。俯冲诱发的地壳生长对塑造弧岩浆岩石类型的地球化学特征至关重要。
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Precambrian Research
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