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Reply to the discussion by Gell and Finlayson (2023) 对Gell和Finlayson讨论的回复(2023)
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-26 DOI: 10.1080/08120099.2023.2175908
R. Bourman, C. Murray-Wallace, Christopher J. Wilson, L. Mosley, J. Tibby, D. D. Ryan, E. D. De Carli, A. Tulley, A. Belperio, D. Haynes, A. Roberts, C. Westell, E. Barnett, S. Dillenburg, L. Beheregaray, P. Hesp
R. P. Bourman , C. V. Murray-Wallace , C. Wilson , L. Mosley , J. Tibby , D. D. Ryan , E. D. De Carli , A. Tulley , A. P. Belperio , D. Haynes , A. Roberts , C. Westell , E. J. Barnett , S. Dillenburg , L. B. Beheregaray and P. A. Hesp School of Earth, Atmospheric and Life Sciences, Faculty of Science, Medicine and Health, University of Wollongong, Wollongong, Australia; Department of Geography, Environment and Population, University of Adelaide, Adelaide, Australia; Beach and Dune Systems (BEADS) Laboratory, College of Science and Engineering, Flinders University, Bedford Park, Australia; College of Humanities Arts and Social Sciences, Flinders University, Bedford Park, Australia; Centre for Australian Biodiversity and Heritage (CABAH), Adelaide, Australia; School of Biological Sciences, University of Adelaide, Adelaide, Australia; Sprigg Geobiology Centre, University of Adelaide, Adelaide, Australia; Department of Geography and Environmental Science, University of Southampton, Southampton, UK; Copper Search Ltd., Norwood, Australia; School of Physical Sciences, University of Adelaide, Adelaide, Australia; Geosciences Institute, Federal University of Rio Grande do Sul, Porto Alegre, Brazil; Molecular Ecology Laboratory (MELFU), College of Science and Engineering, Flinders University, Bedford Park, SA, Australia
R.P.Bourman、C.V.Murray Wallace、C.Wilson、L.Mosley、J.Tibby、D.D.Ryan、E.D.De Carli、A.Tulley、A.P.Belperio、D.Haynes、A.Roberts、C.Westell、E.J.Barnett、S.Dillenburg、L.B.Beheregaray和P.A.Hesp地球、大气与生命科学学院,澳大利亚卧龙岗大学科学、医学与健康学院;澳大利亚阿德莱德阿德莱德大学地理、环境和人口系;澳大利亚贝德福德公园弗林德斯大学科学与工程学院海滩和沙丘系统实验室;弗林德斯大学人文艺术与社会科学学院,澳大利亚贝德福德公园;澳大利亚生物多样性和遗产中心,澳大利亚阿德莱德;澳大利亚阿德莱德,阿德莱德大学生物科学学院;斯普里格地质生物学中心,阿德莱德大学,澳大利亚阿德莱德;英国南安普顿南安普顿大学地理与环境科学系;澳大利亚诺伍德铜搜索有限公司;澳大利亚阿德莱德,阿德莱德大学物理科学学院;巴西阿雷格里港南里奥格兰德州联邦大学地球科学研究所;澳大利亚南部贝德福德公园弗林德斯大学科学与工程学院分子生态学实验室
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引用次数: 0
Discussion of Bourman, R. P., Murray-Wallace, C. V., Wilson, C., Mosley, L., Tibby, J., Ryan, D. D., De Carli, E. D., Tulley, A., Belperio, A. P., Haynes, D., Roberts, A., Westell, C., Barnett, E. J., Dillenburg, S., Beheregaray, L. B., Hesp, P. A. (2022). Holocene freshwater history of the Lower River Murray and its terminal lakes, Alexandrina and Albert, South Australia, and its relevance to contemporary environmental management. Australian Journal of Earth Sciences, 69(6), 605–629 讨论 Bourman, R. P., Murray-Wallace, C. V., Wilson, C., Mosley, L., Tibby, J., Ryan, D. D., De Carli, E. D., Tulley, A., Belperio, A. P., Haynes, D., Roberts, A., Westell, C., Barnett, E. J., Dillenburg, S., Beheregaray, L. B., Hesp, P. A. (2022).南澳大利亚墨累河下游及其末端湖泊亚历山大里纳湖和阿尔伯特湖的全新世淡水史及其与当代环境管理的相关性。Australian Journal of Earth Sciences, 69(6), 605-629
4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-26 DOI: 10.1080/08120099.2023.2175907
P. A. Gell, C. M. Finlayson
Click to increase image sizeClick to decrease image size Disclosure statementNo potential conflict of interest was reported by the author(s).
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引用次数: 0
Dolomitisation under an arid climate at low sea-level: a case study of the Lei 4 Member of the Middle Triassic Leikoupo Formation, Western Sichuan Depression, China 低海平面干旱气候下的白云化作用——以川西坳陷中三叠统雷口坡组雷四段为例
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-23 DOI: 10.1080/08120099.2023.2173653
Y. Qing, S. Li, Z. Liao, Y. Li, Z. Lv, X. Song, Q. Cao
Abstract The origin of dolostones from the Lei 4 Member (T2l4) of the Middle Triassic Leikoupo Formation in the Western Sichuan Depression is unclear. The occurrence and genetic evolution of dolostones in T2l4 were analysed by polarised thin-sections and cathodoluminescence, major- and trace-element, scanning electron microscope, and carbon, oxygen and strontium isotope analyses. The study results are summarised as follows. (1) The dolostones were mainly precipitated in three stages of <40 °C, 40–60 °C and 60–80 °C, corresponding with three paleodepth ranges of 167–300 m, 433–1000 m and 1067–1433 m. The micritic dolostones and the fabric-retentive dolostones (algal dolostone, granular dolostone) mainly formed in a near-surface–shallow-burial environment, and the crystalline dolostones were mainly formed under intermediate burial conditions. (2) 87Sr/86Sr ratios are equivalent to that of the Middle Triassic seawater, Sr/Ba and V/Ni ratios >1, Na notably higher than that in coexisting limestones of T2l4, and the dolostones always coexist with evaporative minerals such as gypsum, indicating that dolomitisation fluids mainly originated from evaporative concentrated seawater. (3) The dolostones mainly inherit materials from precursor limestones based on trace-element distribution patterns, and carbon and oxygen isotope values that are consistent with coexisting limestones of T2l4. (4) Mediated by micro-organisms during the syngenetic period, micritic dolostones and some algal dolostones were formed by replacing aragonites and calcites. During shallow burial, concentrated seawater rich in Mg2+ from the supratidal–intertidal zone flowed downward owing to gravity along the platform and replaced the underlying carbonate rocks, promoting continuous growth of the early dolomites. In the intermediate burial period, the Mg2+-depleted dolomitisation fluid caused the early micritic and silt-crystalline dolostones to recrystallise into silt- or fine-crystalline dolostones with larger crystals and altered the fabric-retentive dolostones into crystalline dolostones. (5) The evaporative dolostones deposited in the near-surface environment are characterised by maximal enrichment of Fe, Sr and Na, the highest δ18O values, the lowest order degree and the highest Ca/Mg ratios. The reflux dolostones formed in a shallow-burial environment characterised by the lowest Fe, medium δ18O values and the lowest order degree. The burial dolostones that developed in the intermediate burial environment are characterised by relative enrichment of Fe and Mn, minimal Na, the lowest δ18O values, the highest order degree and medium Ca/Mg ratios. KEY POINTS The fabric-retentive dolostones mainly formed in a near-surface–shallow-burial environment, and the crystalline dolostones mainly formed under intermediate burial conditions. Dolomitisation fluids mainly originated from the evaporative concentrated seawater, and the dolostones inherit materials from the precursor limestones. Micritic
摘要川西坳陷中三叠统雷口坡组雷4段(T2l4)白云岩的成因尚不清楚。通过偏光薄片和阴极发光、主元素和微量元素、扫描电子显微镜以及碳、氧和锶同位素分析,分析了T2l4中白云岩的发生和成因演化。研究结果总结如下。(1) 白云岩主要在1、Na三个阶段沉淀,Na明显高于共存的T2l4石灰岩,白云岩始终与石膏等蒸发矿物共存,表明白云石化流体主要来源于蒸发浓缩海水。(3) 根据微量元素分布模式以及与T2l4共存石灰岩一致的碳和氧同位素值,白云岩主要继承了前体石灰岩的物质。(4) 在同生期微生物的介导下,微晶白云岩和一些藻类白云岩是通过取代文石和方解石形成的。浅埋过程中,潮上带-潮间带富含Mg2+的浓缩海水由于重力沿平台向下流动,取代了下伏的碳酸盐岩,促进了早期白云岩的持续生长。在中期埋藏期,Mg2+贫化的白云石化流体导致早期泥晶白云岩和粉砂质结晶白云岩重结晶为具有较大晶体的粉砂质或细晶白云岩,并将组构保持白云岩变为结晶白云岩。(5) 在近地表环境中沉积的蒸发白云岩具有Fe、Sr和Na富集最大、δ18O值最高、有序度最低和Ca/Mg比值最高的特征。回流白云岩形成于浅埋环境中,其特征是Fe最低,δ18O值中等,有序度最低。在中等埋藏环境中发育的埋藏白云岩具有Fe和Mn相对富集、Na含量最低、δ18O值最低、有序度最高和Ca/Mg比值中等的特征。要点组构保持白云岩主要形成于近地表浅埋环境,结晶白云岩主要在中等埋藏条件下形成。白云岩流体主要来源于蒸发浓缩海水,白云岩继承了前体石灰岩的物质。泥质白云岩是由蒸发白云石化作用形成的;藻类白云岩和粒状白云岩是由蒸发白云石化和回流白云石化形成的;粉砂质结晶白云岩由回流白云石化和埋藏白云石化形成。
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引用次数: 0
Petrogenesis of the Kalka, Ewarara and Gosse Pile layered intrusions, Musgrave Province, South Australia, and implications for magmatic sulfide prospectivity 南澳穆斯格雷夫省Kalka、Ewarara和Gosse桩层状侵入体的岩石成因及岩浆硫化物找矿意义
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-19 DOI: 10.1080/08120099.2023.2173292
W. Maier, B. Wade, S. Barnes, R. Dutch
Abstract The Musgrave Province of central Australia was the focus of long-lived mantle upwelling that produced large volumes of magnesian basaltic to tholeiitic magma and their felsic derivatives. The Musgrave Province contains one of the greatest concentrations of mafic–ultramafic layered intrusions globally, grouped as the Giles intrusions. In the present paper, we study the magmatic ore potential of the Kalka, Gosse Pile and Ewarara layered intrusions located in South Australia. Ewarara and Gosse Pile appear to have relatively low potential for platnium-group element (PGE) reefs and magmatic Ni–Cu, based on lack of evident metal enrichment and the absence of a mafic–ultramafic transition zone that hosts most PGE reefs globally. However, mafic–ultramafic pipes within the intrusions that could have higher ore potential have not been studied by us. At Kalka, the mafic–ultramafic transition interval is exposed, rendering this intrusion potentially more prospective for PGE reefs. However, based on the available data, this zone appears to be barren. Instead, there are signs of PGE enrichment and metal ratio variation in the magnetite-bearing upper portion of the intrusion suggestive of undiscovered PGE reefs. This interpretation is consistent with subtle Cu–Pd enrichment of soils adjacent to the upper portion of the intrusion. KEY POINTS First assessment of magmatic ore potential of Kalka, Ewarara and Gosse Pile layered intrusions in South Australia. Kalka shows signs of PGE enrichment in upper, magnetite-bearing portion of intrusion, suggesting enhanced potential for a PGE reef. Ewarara and Gosse Pile appear to be less prospective for PGE–Ni–Cu, but picrite pipes remain unstudied.
澳大利亚中部的马斯格雷夫省是长期地幔上涌的焦点,产生了大量镁质玄武岩到拉斑岩浆及其长英质衍生物。马斯格雷夫省拥有全球最集中的基性-超基性层状侵入体之一,被归类为吉尔斯侵入体。本文研究了南澳大利亚Kalka、Gosse桩和Ewarara层状侵入体的岩浆成矿潜力。Ewarara和Gosse Pile的铂族元素(PGE)礁和岩浆Ni-Cu礁的潜力相对较低,这主要是由于缺乏明显的金属富集和镁铁质-超镁铁质过渡带,而镁铁质-超镁铁质过渡带是全球大多数PGE礁的栖息地。然而,侵入体中可能具有较高找矿潜力的镁铁质-超镁铁质管道尚未被研究。在Kalka,暴露了基性-超基性过渡层,使得这种入侵具有潜在的PGE礁前景。然而,根据现有的数据,这个区域似乎是贫瘠的。相反,在含磁铁矿的侵入体上部有PGE富集和金属比变化的迹象,提示未发现的PGE生物礁。这一解释与侵入体上部邻近土壤的微量Cu-Pd富集相一致。南澳大利亚Kalka、Ewarara和Gosse桩层状侵入体岩浆成矿潜力首次评价。在岩体上部含磁铁矿部分,Kalka显示出PGE富集的迹象,表明PGE礁的可能性增强。Ewarara和Gosse Pile似乎对PGE-Ni-Cu的前景不太乐观,但苦橄岩管道仍未被研究。
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引用次数: 0
Late Quaternary geological history of the Sydney estuary, Australia 澳大利亚悉尼河口晚第四纪地质史
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-17 DOI: 10.1080/08120099.2023.2139756
G. Birch, S. Lound
Abstract The present study provides valuable new information on the evolution of Sydney estuary by tracing the development of the complete marine–estuarine–fluvial system through a full glacial cycle (Last Interglacial, LIG, to the present Interglacial). Extensive seismic (361.3-line km) and sedimentological studies provided a sound foundation for production of a detailed litho- and seismic-stratigraphic record for the estuary. In the absence of reliable age data, a relative chronology was constructed based on Quaternary flooding surface elevations constrained by a recent local relative sea-level record supported by other global studies. A thick, ubiquitous estuarine unit deposited during the LIG period (MIS 5.5; 130–115 ka BP) was an important chronological marker horizon and played a critical role in controlling seismic interpretation and correlation throughout the estuary. Deposition during the MIS 5.1/5.3 interstadial period (100–80 ka BP) resulted in deposition of fine-grained, estuarine sediments in the lower estuary and time-equivalent, fluvial-sourced estuarine and channel sediments, and marsh sediments in the upper and central estuary, respectively. The MIS 3 interstadial event did not play a significant role in sedimentation in Sydney estuary. An eolian dune field formed adjacent to the southern shores of the estuary during the last glacial (31–24 ka BP) when most of the sediment in the lower estuary had been removed by fluvial erosion. Transgressive marine sand, which deposited in the lower paleovalley after the ocean re-entered the estuary, experienced repeated erosion and infilling by laterally migrating paleoriver channels. A marine flood-tide delta now occupies the estuary mouth, and the lower and upper/central estuary are mantled in a veneer (mean 7 m) of Holocene sand and mud, respectively. KEY POINTS A relative chronology was based on Quaternary flooding surface elevations constrained by relative sea-level. First geological history of the Sydney estuary with a complete marine–estuarine–fluvial system. A late Quaternary estuary evolution through a full glacial cycle. Geological history includes an interstadial (MIS 5.3/5.1) estuarine sequence.
摘要本研究通过追踪完整的海洋-河口-河流系统在整个冰川周期(最后一次冰间期,LIG,到现在的冰间期)的发展,为悉尼河口的演变提供了有价值的新信息。广泛的地震(361.3线km)和沉积学研究为河口详细的岩石和地震地层记录提供了坚实的基础。在缺乏可靠的年龄数据的情况下,根据第四纪洪泛面高程构建了相对年表,该高程受其他全球研究支持的最近当地相对海平面记录的限制。LIG时期沉积的厚而普遍的河口单元(MIS 5.5;130–115 ka BP)是一个重要的年代标志层,在控制整个河口的地震解释和对比方面发挥了关键作用。MIS 5.1/5.3辐射间期间的沉积(100–80 ka BP)分别导致下河口的细粒河口沉积物和时间等价物、河流来源的河口和河道沉积物以及上河口和中河口的沼泽沉积物的沉积。MIS 3中层间事件对悉尼河口的沉积作用不显著。在最后一次冰川期(31-24 ka BP),当时下河口的大部分沉积物已被河流侵蚀清除。海洋重新进入河口后沉积在古河谷下游的海进海沙,经历了横向迁移的古河道的反复侵蚀和填充。一个海洋洪潮三角洲现在占据了河口,下河口和上河口/中央河口被覆盖在一个单板中(平均7 m) 全新世的沙子和泥土。关键点相对年表基于受相对海平面约束的第四纪洪泛面高程。悉尼河口完整的海洋-河口-河流系统的第一个地质历史。第四纪晚期河口经过一个完整的冰川周期的演变。地质历史包括一个中层间(MIS 5.3/5.1)河口序列。
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引用次数: 0
Petrogenesis and tectonic setting of Early Cretaceous mafic dykes in the North Qinling Orogenic Belt, central China: constraints on the lithospheric lower crust delamination 北秦岭造山带早白垩世基性岩脉的成因与构造背景:对岩石圈下地壳拆沉的制约
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-16 DOI: 10.1080/08120099.2023.2172609
Y. N. Huang, D. Li, A. Xiao, S. M. Xu
Abstract Late Mesozoic mafic dykes, which are widely developed in the North Qinling Orogenic Belt (NQOB), include abundant geodynamic information. This paper describes the mafic dykes that intrude the Late Jurassic granite in the Dayu and Kuyu areas, and reports important petrological constraints for the late Mesozoic tectonic transition from compression to extension in the NQOB. Three zircon U–Pb results show that the minimum ages of the mafic dykes are 139.8 ± 1.4 Ma, 137.4 ± 1.7 Ma and 133.4 ± 0.9 Ma, indicating that the emplacement age of the Dayu and Kuyu mafic dykes is 140–133 Ma. Petrogeochemical analyses suggest that the mafic dykes belong to the high-K calc-alkaline shoshonite series with low SiO2 (46.93–56.73 wt%), MgO (1.88–9.10 wt%) and TiO2 (1.17–1.82 wt%), and high Al2O3 (13.98–17.46 wt%), TFe2O3 (7.81–10.92 wt%) and K2O (1.28–4.78 wt%). The mafic dykes are enriched in large ion lithophile elements (e.g. Rb, Ba, K, La, Sr) and depleted in high-field-strength elements (e.g. Nb, Ta, Zr, Ti). These samples have the right-sloping chondrite-normalised rare earth element patterns, which suggest light rare earth element enrichment and heavy rare earth elements depletion with no obvious Eu anomalies (δEu = 0.94–1.11). The I Sr, ε Nd(t), ε Hf (t) and T DM2(crust) values are 0.7056–0.7060, −10.60 to −5.98, −14.1 to −2.8, and 1382.4 ± 25.1 to 2081.9 ± 47.6 Ma, respectively. Both elemental and isotopic geochemistry show that the formation of Dayu and Kuyu mafic dykes is due to the partial decompression melting of previously enriched lithospheric mantle during a delamination process. The mafic dykes have undergone fractionation crystallisation of Mg–Fe phase minerals during magma ascent, accompanied by some crustal contamination. Combined with the regional tectonic setting, we suggested that the NQOB experienced intra-continental extension during the Early Cretaceous. KEY POINTS Early Cretaceous (140–133 Ma) mafic dykes have been discovered in the middle part of the North Qinling Orogenic Belt. The remote effect of the Paleo-Pacific Plate subduction has reached the middle of the North Qinling Orogenic Belt. The North Qinling Orogenic Belt entered the extensional stage in the Early Cretaceous (140–133 Ma).
摘要北秦岭造山带广泛发育的晚中生代镁铁质岩脉具有丰富的地球动力学信息。本文描述了大禹、库峪地区晚侏罗世花岗岩中侵入的镁铁质岩脉,并报道了晚中生代构造从挤压向伸展过渡的重要岩石学制约因素。三个锆石U–Pb结果表明,镁铁质岩脉的最小年龄为139.8 ± 1.4 马,137.4 ± 1.7 马和133.4 ± 0.9 Ma,表明大禹和库峪镁铁质岩脉的侵位年龄为140–133 马。岩石地球化学分析表明,镁铁质岩脉属于低SiO2(46.93–56.73 wt%)、MgO(1.88–9.10 wt%)和TiO2(1.17–1.82 wt%)和高Al2O3(13.98–17.46 wt%),TFe2O3(7.81–10.92 wt%)和K2O(1.28–4.78 wt%)。镁铁质岩脉富含大离子亲石元素(如Rb、Ba、K、La、Sr),而贫含高场强元素(如Nb、Ta、Zr、Ti)。这些样品具有右旋球粒陨石归一化稀土元素模式,表明轻稀土元素富集和重稀土元素贫化,没有明显的Eu异常(δEu=0.94–1.11)。I Sr、εNd(t)、εHf(t)和t DM2(地壳)值分别为0.7056–0.7060、−10.60至−5.98、−14.1至−2.8和1382.4 ± 25.1至2081.9 ± 47.6 马。元素地球化学和同位素地球化学都表明,大禹和库豫镁铁质岩脉的形成是由于先前富集的岩石圈地幔在分层过程中部分减压熔融。镁铁质岩脉在岩浆上升过程中经历了镁铁相矿物的分馏结晶,并伴有一些地壳污染。结合区域构造环境,我们认为NQOB在早白垩世经历了陆内伸展。关键点早白垩世(140–133 在北秦岭造山带中部发现了镁铁质岩脉。古太平洋板块俯冲的遥远作用已到达北秦岭造山带的中部。北秦岭造山带在早白垩世(140–133)进入伸展阶段 马)。
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引用次数: 1
A geophysically constrained crustal element map of East Antarctica between Enderby Land and Princess Elizabeth Land 南极洲东部恩德比地和伊丽莎白公主地之间的地球物理约束地壳元素图
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-08 DOI: 10.1080/08120099.2023.2169957
Y. Giri, P. Betts, M. Radhakrishna, M. McLean, T. K. Biswal, R. Armit
Abstract East Antarctica along with Greater India played a vital role in the accretion and breakup of the Indo-Antarctic landmasses during the supercontinents Nuna, Rodinia and Gondwana. Without geophysical potential field methods, interpreting the architecture of the ice-covered geological provinces of Antarctica is impossible. We present here a crustal element map of East Antarctica between Enderby Land and Princess Elizabeth Land (Indo-Antarctica tectonic element) using aerogeophysical data interpretation. The data reveal distinct anastomosing geophysical provinces that correlate with sparse geological data. Our crustal element map shows the Oygarden Province and the Northern and Southern Rayner provinces are arcuate belts that wrap around the Archean Napier Province. These provinces represent the remnants of an accretionary tectonic margin, which evolved between ca 1300 Ma and 900 Ma. The arcuate geometry of these Meso- to Neoproterozoic provinces formed during the collision with the Napier Province, which represents a microcontinent. This collision triggered widespread extension and ultra-high temperature metamorphism in the Northern and Southern Rayner provinces. The southernmost provinces include the Fisher Province, Lambert Province and a transition zone. The provinces are truncated by a suture zone with the Archean Ruker Province, following north-dipping subduction during the Meso- to Neoproterozoic. Our interpretation provides a template upon which to correlate geological provinces with the terranes on the conjugate eastern Indian margin. KEY POINTS An aeromagnetic interpretation is given for Enderby Land and Princess Elizabeth Land of East Antarctica. Napier Province is a microcontinent that collided with the Rayner Province during a ca 1000 Ma orogenic event. A new interpretation of potential field data suggests anastomosing provinces accreted as part of a collisional event. New structures/piercing points are identified at the Mawson Coast and in Kemp Land.
在努纳、罗迪尼亚和冈瓦纳超大陆时期,东南极洲和大印度在印度-南极大陆块的增生和分裂中起了至关重要的作用。如果没有地球物理势场方法,就不可能解释南极洲被冰覆盖的地质省份的结构。本文利用航空地球物理资料解释,绘制了Enderby Land和Princess Elizabeth Land(印-南极洲构造元素)之间的东南极洲地壳元素图。这些数据揭示了与稀疏的地质数据相关的独特的吻合的地球物理省。我们的地壳元素图显示,Oygarden省和Rayner省的北部和南部是环绕太古宙Napier省的弧形带。这些省份代表了一个增生构造边缘的残余,在大约1300 Ma和900 Ma之间演化。这些中至新元古代省的弧形几何形状是在与纳皮尔省碰撞时形成的,代表了一个微大陆。这次碰撞在雷纳省北部和南部引发了广泛的伸展和超高温变质作用。最南端的省份包括费舍尔省、兰伯特省和一个过渡区。中-新元古代北倾俯冲,与太古宙鲁克省形成缝合带。我们的解释提供了一个模板,在此基础上将地质省与共轭东印度边缘的地体联系起来。给出了东南极洲恩德比岛和伊丽莎白公主岛的航磁解译。纳皮尔省是一个微大陆,在大约1000 Ma的造山活动中与雷纳省碰撞。对势场数据的一种新的解释表明,重合的省份是碰撞事件的一部分。在莫森海岸和坎普地发现了新的构造/刺穿点。
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引用次数: 1
Shale gas potential of Ordovician marine Pingliang shale and Carboniferous–Permian transitional Taiyuan-Shanxi shales in the Ordos Basin, China 鄂尔多斯盆地奥陶系海相平凉页岩和石炭-二叠系过渡太原-山西页岩的页岩气潜力
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-05 DOI: 10.1080/08120099.2023.2170466
H. Nie, Q. Chen, P. Li, W. Dang, J. C. Zhang
Abstract The assessment of shale gas potential for the Ordovician Pingliang Formation and Carboniferous–Permian Taiyuan and Shanxi formations in the northwest margin of Ordos Basin, China provides insight into how fluctuation in depositional environments has a significant role on lithofacies and shale gas potential. To investigate the shale gas potential, a series of measurements (i.e. Rock-Eval pyrolysis, maceral composition analyses and X-ray powder diffraction, etc.) on representative outcrop samples were conducted to characterise shale properties. The organic matter from marine Pingliang shale is predominantly type I with a strong predominance of sapropelinite, whereas the transitional Taiyuan-Shanxi shales are dominated by types II to III kerogen. Furthermore, the Pingliang shale is characterised as a ‘poor’ source rock mainly owing to the lower total organic carbon (TOC) content (average 0.79 wt%) and higher maturity [average 1.78% in vitrinite reflectance (R o)], while the transitional Taiyuan-Shanxi shales are mostly characterised as ‘fair’ source rocks, and some samples with high TOC content (more than 2.0 wt%) present good source rocks. It is also found that the sedimentary environment, as a key factor determining the organic matter and TOC content, inevitably influences the type and content of minerals in shale, and controls the shale gas potential. For example, the transitional argillaceous Taiyuan-Shanxi shales are significantly different from the siliceous Pingliang shales, specifically, total clay content for the former is more than 50 wt%, while the latter is rich in quartz content (more than 70 wt%). Additionally, the quartz and clay contents of the Taiyuan shale range widely, especially the smectite content of I–S ML. The barrier coastal facies in the Taiyuan Formation are more conducive to the enrichment and preservation of organic matter because the Shanxi shale was deposited in shallow delta facies with a greater terrestrial influence. Conclusively, the Taiyuan and Shanxi formations have relatively good exploitation potential for shale gas, especially the relatively high TOC content (average 2.45 wt%) and moderate R o value (average 1.25%). For future exploration, selecting areas with relatively large shale thickness, high brittle mineral content, stable tectonics and better preservation conditions are key to optimising favourable exploration areas for shale gas. KEY POINTS The shale gas potentials of the argillaceous Taiyuan-Shanxi shales and siliceous Pingliang shale are compared. The influence of sedimentary facies on reservoir parameters of marine and transitional shales is established. This is a first detailed comparison of the marine and transitional shale gas potential in the northwest margin of Ordos Basin, China.
摘要通过对鄂尔多斯盆地西北缘奥陶系平凉组、石炭-二叠系太原组和山西组页岩气潜力的评价,可以深入了解沉积环境的波动对岩相和页岩气潜力有何重要影响。为了研究页岩气潜力,对代表性露头样品进行了一系列测量(即岩石蒸发热解、显微组分分析和X射线粉末衍射等),以表征页岩性质。平凉海相页岩有机质以Ⅰ型为主,以腐泥岩为主,而太原-山西过渡页岩以Ⅱ-Ⅲ型干酪根为主。此外,平凉页岩的特征是“贫”烃源岩,主要是由于总有机碳(TOC)含量较低(平均0.79 wt%)和更高的成熟度[镜质组反射率(R o)平均1.78%],而太原-山西过渡页岩的特征主要是“中等”烃源岩,一些样品的TOC含量高(超过2.0 wt%)存在良好的烃源岩。沉积环境作为决定有机质和TOC含量的关键因素,不可避免地影响着页岩中矿物的类型和含量,并控制着页岩气的潜力。例如,过渡泥质太原-山西页岩与硅质平凉页岩有显著差异,特别是前者的总粘土含量超过50 wt%,而后者富含石英含量(超过70 wt%)。此外,太原页岩的石英和粘土含量范围很广,尤其是I–S ML的蒙脱石含量。由于山西页岩沉积在受陆地影响较大的浅三角洲相,太原组障壁海岸相更有利于有机质的富集和保存。综上所述,太原组和山西组页岩气具有较好的开发潜力,特别是TOC含量较高(平均2.45 wt%)和中等R o值(平均1.25%)。对于未来的勘探,选择页岩厚度相对较大、脆性矿物含量较高、构造稳定和保存条件较好的区域是优化页岩气有利勘探区域的关键。重点对比了太原-山西泥质页岩和平凉硅质页岩的页岩气潜力。建立了沉积相对海相和过渡期页岩储层参数的影响。这是对中国鄂尔多斯盆地西北缘海相和过渡期页岩气潜力的首次详细比较。
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引用次数: 0
New age constraints for the Tommy Creek Domain of the Mount Isa Inlier, Australia 新时代的限制,为汤米溪领域的伊萨山Inlier,澳大利亚
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-02-05 DOI: 10.1080/08120099.2023.2171124
A. Brown, C. Spandler, T. Blenkinsop, C. Fergusson
Abstract The Tommy Creek Domain is a complex, yet little studied, terrane in the Eastern Subprovince of the Mount Isa Province, northwest Queensland Australia. In this study, we take advantage of modern low-cost and rapid geochronology techniques to undertake an iterative dating approach integrated with detailed fieldwork to define the ages and extents of numerous lithologies and units of the Tommy Creek Domain. This includes some units not previously identified, lithologies previously grouped together based on field observations but now shown to have multiple distinct ages and dates not commonly represented in Mount Isan time–space plots. We identify an episode of felsic magmatism at ca 1640 Ma, and multimodal intrusions (ca 1615 Ma) immediately preceding the onset of the Isan Orogeny. A major rock package of the Tommy Creek Domain, the Milo beds, are characterised here as the youngest pre-Isan Orogeny sedimentary unit in the Eastern Subprovince (1660–1620 Ma), confirming that sedimentation and possibly rifting continued after deposition of the Soldiers Cap, Mount Albert and Kuridala groups (ca 1690–1650 Ma) before the onset of the Isan Orogeny (ca 1600 Ma). The Milo beds are thus age equivalent to the Mount Isa and McNamara groups of the Western Succession. There is evidence of a compositional shift in sedimentation coincident with the ca 1640 Ma Riversleigh Inversion event, previously only observed in the Western Subprovince in the Lawn Hill Platform. The application of geochronology as part of the mapping workflow can assist with differentiating geological units in terranes where field evidence is ambiguous and can aid in the focusing of objectives for field campaigns to enable the best possible interpretations to be made. KEY POINTS New ages constrain the Milo beds in the Tommy Creek Domain as the youngest stratigraphy in the Eastern Subprovince of the Mount Isa Province. The Milo beds are age equivalents of the McNamara and Mount Isa groups of the Western Subprovince of the inlier. Recognition of felsic and mafic intrusions with ca 1640 Ma and ca 1615 Ma ages. Evidence for Riversleigh Inversion event ca 1640 in the Eastern Subprovince.
Tommy Creek域是一个复杂的,但很少被研究的地体,位于澳大利亚昆士兰州西北部的伊萨山省东部亚省。在这项研究中,我们利用现代低成本和快速的地质年代学技术,采用迭代测年方法,结合详细的野外工作,确定Tommy Creek域众多岩性和单元的年龄和范围。这包括一些以前未确定的单元,以前根据实地观察组合在一起的岩性,但现在显示出具有多个不同的年龄和日期,这些年龄和日期在伊桑山的时空图中通常没有表示。我们确定了大约1640 Ma的长英质岩浆活动,以及在伊桑造山运动开始之前的多模态侵入(大约1615 Ma)。Tommy Creek域的一个主要岩石包,Milo层,在这里被描述为东部亚省最年轻的前伊桑造山运动沉积单元(1660-1620 Ma),证实了在伊桑造山运动开始(约1600 Ma)之前,Soldiers Cap、Mount Albert和Kuridala组(约1690-1650 Ma)沉积之后,沉积和可能的裂谷作用仍在继续。因此,米洛地层的年龄相当于西演替时期的伊萨山和麦克纳马拉群。有证据表明,在1640年左右的马河利反转事件中,沉积的成分发生了变化,以前只在Lawn Hill台地的西部亚省观测到。将地质年代学作为制图工作流程的一部分,有助于在实地证据不明确的地形中区分地质单元,并有助于确定实地活动的目标,以便作出尽可能最佳的解释。新时代约束了Tommy Creek地区的Milo层,使其成为伊萨山省东部亚省最年轻的地层。Milo层的年龄相当于河西亚省的McNamara和Mount Isa组。1640 Ma和1615 Ma花岗岩和镁质花岗岩的识别。1640年东副省里弗斯利逆温事件的证据。
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引用次数: 0
Foliation boudinage structures in the Mount Isa Cu system 伊萨-Cu山体系中的褶皱构造
IF 1.2 4区 地球科学 Q2 Earth and Planetary Sciences Pub Date : 2023-01-30 DOI: 10.1080/08120099.2022.2153384
B. J. Williams, T. Blenkinsop, R. Lilly, M. Thompson, P. Ava, C. Fergusson
Abstract Small-scale foliation boudinage structures occur in rocks that were sampled in drill core from the Mount Isa Cu deposit, northwest Queensland. The necks of foliation boudinage structures plunge gently to the north and south as a result of layer normal shortening and layer parallel extension of the steeply west-dipping Urquhart Shale. Detailed petrographic analysis of the foliation boudinage structures has identified an initial rim of quartz and dolomite, followed by infill and replacement by pyrrhotite and minor chalcopyrite. Foliation boudinage structures formed after dolomitisation and silicification of the shale. They occur most commonly in the unaltered Urquhart Shale where the anisotropy and homogeneity provided by the shale layering is still intact. Infilling of the structures occurred during protracted silica-dolomite alteration, pyrrhotite and chalcopyrite mineralisation. The paragenesis of the foliation boudinage structures is consistent with the established paragenesis of the main Cu mineralisation. Foliation boudinage structures formed over the period from shortening during D4a through to the main Cu mineralisation during D4b west-northwest–east-southeast sinistral-reverse shortening. The timing of foliation boudinage is consistent with a current kinematic model for the Mount Isa system. KEY POINTS First record of foliation boudinage structures at Mount Isa. Foliation boudinage structures with sulfide-dominated infills. Foliation boudinage structures formed as a result of progressive deformation from a D4a dextral-reverse through to D4b sinistral-reverse slip. Foliation boudinage structures are associated with the timing and kinematics of Cu mineralisation at Mount Isa.
摘要:在昆士兰西北部伊萨山铜矿的岩芯中取样的岩石中,出现了小规模的叶理boudinage结构。叶理boudinage结构的颈部缓慢地向北和向南倾斜,这是急剧向西倾斜的Urquhart页岩的层正常缩短和层平行延伸的结果。对叶理boudinage结构的详细岩相分析已经确定了石英和白云石的初始边缘,随后是磁黄铁矿和少量黄铜矿的填充和置换。在页岩的白云石化和硅化作用之后形成的叶理凝灰岩结构。它们最常见于未改变的厄克特页岩中,页岩分层提供的各向异性和均匀性仍然完好无损。在长期的二氧化硅-白云石蚀变、磁黄铁矿和黄铜矿矿化期间,结构发生了填充。叶理boudinage结构的共生作用与主要铜矿化的既定共生作用一致。从D4a缩短到D4b西北偏西-东南偏东左旋反向缩短期间的主要铜矿化,形成了叶理-凝灰岩结构。叶理隆起的时间与伊萨山系统的当前运动学模型一致。要点伊萨山叶理构造的首次记录。具有硫化物为主填充物的叶理构造。由D4a右旋逆滑到D4b左旋逆滑的渐进变形,形成了叶理构造。叶理构造与伊萨山铜矿化的时间和运动学有关。
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引用次数: 1
期刊
Australian Journal of Earth Sciences
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