Sulfur isotope distribution in Late Silurian volcanic‐hosted massive sulfide deposits of the Hill End Trough,eastern Lachlan Fold Belt,New South Wales     

P. M. Downes  P. K. Seccombe 《Australian Journal of Earth Sciences》2013,60(1):123-139

Volcanic‐hosted massive sulfide (VHMS) deposits of the eastern Lachlan Fold Belt of New South Wales represent a VHMS district of major importance. Despite the metallogenic importance of this terrane, few data have been published for sulfur isotope distribution in the deposits, with the exception of previously published studies on Captains Flat and Woodlawn (Captains Flat‐Goulburn Trough) and Sunny Corner (Hill End Trough). Here is presented 105 new sulfur isotope analyses and collation of a further 92 analyses from unpublished sources on an additional 12 of the VHMS systems in the Hill End Trough. Measured δ³⁴S values range from ‐7.4% to 38.3%, mainly for massive and stockwork mineralisation. Sulfur isotope signatures for polymetallic sulfide mineralisation from the Lewis Ponds, Mt Bulga, Belara and Accost deposits (group 1) are all very similar and vary from ‐1.7% to 5.9%. Ore‐forming fluids for these deposits were likely to have been reducing, with sulfur derived largely from a magmatic source, either as a direct magmatic contribution accompanying felsic volcanism or indirectly through dissolution and recycling of rock sulfide in host volcanic sequences. Sulfur isotope signatures for sulfide mineralisation from the Calula, Commonwealth, Cordillera and Kempfield deposits, Peelwood mine and Sunny Corner (group 2) are similar and have average δ³⁴S values ranging from 5.4% to 8.1%. These deposits appear to have formed from ore fluids that were more oxidising than group 1 deposits, representing a mixed contribution of sulfur derived from partial reduction of seawater sulfate, in addition to sulfur from other sources. The δ³⁴S values for massive sulfides from the John Fardy deposit are the highest in the present study and have a range of 11.9–14.5%, suggesting a greater component of sulfur of seawater origin compared to other VHMS deposits in the Hill End Trough. For barite the sulfur isotope composition for samples from the Commonwealth, Stringers and Kempfield deposits ranges from 12.6% to 38.3%. More than 75% of barite samples have a sulfur isotope composition between 23.4 and 30.6%, close to the previously published estimates of the composition of seawater sulfate during Late Silurian to earliest Devonian times, providing supporting evidence that these deposits formed concurrently with the Late Silurian volcanic event. Sulfur isotope distribution appears to be independent of the host rock unit, although there appears to be a relation linking the sulfur isotope composition of different deposits to defined centres of felsic volcanism. The Mt Bulga, Lewis Ponds and Accost systems are close to coherent felsic volcanic rocks and/or intrusions and have sulfur isotope signatures with a stronger magmatic affinity than group 2 deposits. By contrast, group 2 deposits (including John Fardy) are characterised by ³⁴S‐enrichment and a lesser magmatic signature, are generally confined to clastic units and reworked volcanogenic sediments with lesser coherent volcanics in the local stratigraphy, and are interpreted to have formed distal from the magmatic source. An exception is the Belara deposit, which is hosted by reworked felsic volcanic rocks and has a more pronounced magmatic sulfur isotope signature.  相似文献   

Stratigraphy,sedimentology, structure and tectonics of Lower Ordovician and Devonian strata of South Mootwingee,Darling Basin,western New South Wales     

G. Neef 《Australian Journal of Earth Sciences》2013,60(1):15-29

K‐Ar age measurements using the ⁴⁰Ar/³⁹Ar total fusion technique on nephrite from two occurrences in the Great Serpentine Belt southeast of Tamworth yielded ages of 273 ± 5.8 and 280 ± 5.6 m.y. The K‐Ar ages indicate that tectonic emplacement, during which the nephrite was produced as a reaction product between ultra‐mafic rock and country rock, occurred early in the Permian about 275–280 m.y. ago.  相似文献   

Esk Trough—Yarraman Block contact,an unconformity: Its nature and implications for regional tectonics     

E. C. Willey 《Australian Journal of Earth Sciences》2013,60(1):139-152

Detailed field study in southeast Queensland has resulted in the interpretation of an unconformity at the base of the Esk Trough sequence at its contact with the Yarraman Block (Maronghi Creek beds and associated intrusions). Previously this contact had been considered to be faulted. The nature of the unconformity is very variable with the Esk Formation resting on freshly eroded surfaces, on mature palaeosols and on an immature palaeosol. Immediately above the unconformity, the Esk Formation variably comprises scree breccia, fluvial conglomerate and arenite, and alluvial fan conglomerate and arenite. North‐northwest‐south‐southeast‐striking faults are associated with the unconformity. Where the unconformity parallels these faults, it retains a relatively constant character, but where it is cut by these faults, it shows greater variability, a relationship interpreted to result from contemporaneous tectonism. The Glen Howden Fault extends into structurally disturbed areas previously described as ‘fractured anticlines’ and ‘complex anticlines’, which are here interpreted as flower structures and associated features. The south‐southeast extension of the Glen Howden Fault strikes obliquely across the Esk Trough to finally pass into the South Moreton Anticline previously interpreted as a positive flower structure, and resolves structural and stratigraphic observations that previously appeared anomalous. Inferred strike‐slip movement in the Esk Trough resulted from Early to Middle Triassic north‐northwest‐south‐southeast oblique transtension followed by Late Triassic transpression, and similar tectonism probably affected adjacent portions of the Yarraman Block.  相似文献   

The Early Devonian Coopers Creek Limestone: A deep‐water redeposited limestone in the Melbourne Trough,southeastern Australia     

M. W. Rehfisch  J. A. Webb 《Australian Journal of Earth Sciences》2013,60(6):575-589

The Coopers Creek Limestone represents an Early Devonian redeposited carbonate accumulation and records the evolution of a carbonate slope in the southeastern portion of the Melbourne Trough. During the earliest Devonian, the underlying Boola Formation was deposited, probably as turbidites, in a moderately deep‐water setting. The presence of chert and greenstone clasts in the top of the formation indicates exposure of an area of Cambrian greenstones in this part of the Melbourne Trough, as a result of uplift associated with the earliest Devonian Bowning Orogeny. This uplift provided ideal conditions for carbonate production along the margin of the exposed landmass. The periodic transportation of carbonate material downslope resulted in the accumulation of the Coopers Creek Limestone. Initially, in the early Pragian, turbidity currents deposited clayey biomicrites and biopelmicrites on a relatively gentle slope. However, the rapid build‐up of carbonate sand banks at the shelf margin steepened the gradient from the shelf into the basin and a bypass margin began to develop. Grainflows deposited pelsparites and biopelsparites and the presence of debris flow breccias indicates erosion of lithified limestone by channelling. Continued carbonate build‐up led to the development of a rimmed reef margin in the earliest Emsian, with a steep fore‐reef gradient. Large blocks of reefal limestone fell or rolled to the base of the slope, to accumulate as reefal megabreccias at the top of the Coopers Creek Limestone. Carbonate production abruptly ceased in the early Emsian, due to the uplift of a quartzo‐micaceous source to the east during the initial stages of the Tabberabberan Orogeny. This uplift supplied abundant terrigenous material into the Melbourne Trough to be deposited as the turbidites of the Walhalla Group, which deeply buried the limestone accumulation.  相似文献   

我国南海历史性水域线的地质特征   总被引：3，自引：1，他引：2  

夏戡原  夏综万  赵明辉  孙珍 《海洋学报》2014,36(5):77-89

40a的海洋地质、地球物理实测研究表明,九段线不仅是显示我国南海主权的历史性水域线,而且总体上也是南海与东部、南部和西部陆区及岛区的巨型地质边界线。根据实测数据,本文将从地质成因、来源、演化的角度论述此南海历史性水域线的合理性。主要结论包括:历史性水域线的东段在地形上基本与马尼拉海沟一致,海沟西侧为南海中央海盆洋壳区,东侧为菲律宾群岛。根据国际地质研究的资料,菲律宾群岛始新世以前位于较偏南的纬度,后来于中晚中新世(距今16~10Ma)仰冲于南海中央海盆之上,因此菲律宾群岛是一个外来群岛。而黄岩岛在马尼拉海沟以西,是中央海盆洋壳区的一个岛礁,与菲律宾群岛成因不同。南海历史性水域线的南段在地形上基本与南沙海槽一致,伴随南沙地块由北部陆缘向南裂离,古南海洋壳沿此海槽以南俯冲至加里曼丹岛陆壳之下,因此南沙地块与加里曼丹陆块为两个来历不同的地块。南海历史性水域线西段的分布在地形上与越东巨型走滑断裂带基本一致,可能与西沙地块、中沙地块、南沙地块从南海北部陆缘向南滑移有关。南沙地块北缘陡直的正断层结构,突显中央海盆是拉裂形成,其基底和中新生代地层与北部珠江口盆地的地层结构可以对比,说明南沙岛礁原属我国华南大陆南缘,后因南海的形成裂离至现今的位置。  相似文献   

南海南部海域浮游介形类新种——南沙深海浮萤*     

尹健强  李开枝  谭烨辉 《热带海洋学报》2022,41(2):193-197

文章描述了发现于南海南沙海槽的一新种——南沙深海浮萤(Bathyconchoecia nanshaensis sp. nov.)。该种个体小,壳长度(CL<1.0mm)和壳高度(~70% CL)与小深海浮萤(Bathyconchoecia paulula)和太平洋深海浮萤(Bathyconchoecia pacifica)非常相似。但是, 根据不对称腺体开口的位置、下颌骨的臀齿边缘的结构, 以及第六肢的位置可以把该种和这两个相似的物种区分开。  相似文献   

Formational history of the Wicklow Trough: a marine-transgressed tunnel valley revealing ice flow velocity and retreat rates for the largest ice stream draining the late-Devensian British–Irish Ice Sheet     

Mark Coughlan  Zsuzsanna TÓth  Katrien J. J. Van Landeghem  Stephen Mccarron  Andrew J. Wheeler 《第四纪科学杂志》2020,35(7):907-919

The Wicklow Trough is one of several Irish Sea bathymetric deeps, yet unusually isolated from the main depression, the Western Trough. Its formation has been described as proglacial or subglacial, linked to the Irish Sea Ice Stream (ISIS) during the Last Glacial Maximum. The evolution of the Wicklow Trough and neighbouring deeps, therefore, help us to understand ISIS dynamics, when it was the main ice stream draining the former British–Irish Ice Sheet. The morphology and sub-seabed stratigraphy of the 18 km long and 2 km wide Wicklow Trough is described here from new multibeam echosounder data, 60 km of sparker seismic profiles and five sediment cores. At a maximum water depth of 82 m, the deep consists of four overdeepened sections. The heterogeneous glacial sediments in the Trough overlay bedrock, with indications of flank mass-wasting and subglacial bedforms on its floor. The evidence strongly suggests that the Wicklow Trough is a tunnel valley formed by time-transgressive erosional processes, with pressurised meltwater as the dominant agent during gradual or slow ice sheet retreat. Its location may be fault-controlled, and the northern end of the Wicklow Trough could mark a transition from rapid to slow grounded ice margin retreat, which could be tested with modelling.  相似文献   

南海西沙海槽盆地地质构造特征   总被引：2，自引：0，他引：2  

钟广见  冯常茂  韦振权 《海洋地质与第四纪地质》2012,(3):63-68

西沙海槽盆地是一个发育在南海北部陆坡深水区的新生代沉积盆地,接受了厚1 500～8 000m的沉积,沉积层中部厚,南北薄,呈南北分带特征。地震剖面上表现出下断上拗的特点,盆地裂陷期的构造样式以"多米诺式半地堑"或"地堑"为特征,控制半地堑发育的主要断层有F1、F2、F3、F4、F5。盆地发育经历了古新世—渐新世断陷和中新世—第四纪拗陷两个主要演化阶段,断陷阶段发育陆相河湖相沉积,拗陷阶段发育浅海-半深海沉积。  相似文献   

24ka来冲绳海槽北部沉积物来源的高分辨率常量元素记录   总被引：3，自引：0，他引：3  

徐兆凯  常凤鸣  李铁刚  南青云  蒋富清  李安春 《海洋地质与第四纪地质》2012,(4):73-82

为进一步了解冲绳海槽北部24ka来柱状沉积物的常量元素组成特征及其物源和古环境指示意义,对PC-1孔进行了402个常量元素和粒度及344个浮游有孔虫氧同位素的综合分析,其平均样品分辨率高达百年时间尺度。结果表明:沉积物中的主要常量元素含量表现出明显的3段式垂向变化特征,并记录到了7.3和12.7cal.kaBP时的两次火山事件;物源判别图解及R型因子分析则揭示出主要氧化物含量在垂向上的变化主要受控于附近陆源物质输入,而热液活动和海洋生物沉积作用及火山物质的影响较小。特别是不同陆源物质对研究区的影响表现出明显的变化规律,与海平面波动及对马暖流形成演化间具有良好的耦合关系,但期间的典型古气候事件却并未明显改变沉积物中的陆源物质组成,从而为揭示24ka来冲绳海槽北部地区陆源物质输入演化历史,及其主要控制因素提供了新的高分辨率资料。  相似文献   

Contributions of slab fluid and sediment melt components to magmatism in the Mariana Arc–Trough system: Evidence from geochemical compositions and Sr,Nd, and noble gas isotope systematics          下载免费PDF全文

Yasuo Ikeda  Keisuke Nagao  Teruaki Ishii  Daisuke Matsumoto  Robert J. Stern  Hiroo Kagami  Makoto Arima  Sherman H. Bloomer 《Island Arc》2016,25(4):253-273

This study presents new major and trace element, mineral, and Sr, Nd, and noble gas isotope geochemical analyses of basalts, gabbro, and clinopyroxenite from the Mariana Arc (Central Islands and Southern Seamount provinces) including the forearc, and the Mariana Trough (Central Graben and Spreading Ridge). Mantle source compositions beneath the Mariana Arc and the Mariana Trough indicate a mantle source that is depleted in high field strength elements relative to MORB (mid‐oceanic ridge basalt). Samples from the Mariana Arc, characterized by high ratios of Ba/Th, U/Th, ⁸⁴Kr/⁴He and ¹³²Xe/⁴He, are explained by addition of fluid from the subducted slab to the mantle wedge. Correlations of noble gas data, as well as large ion lithophile elements, indicate that heavy noble gases (Ar, Kr, and Xe) provide evidence for fluid fluxing into the mantle wedge. On the other hand, major elements and Sr, Nd, He, and Ne isotopic data of basalts from the Mariana Trough are geochemically indistinguishable from MORB. Correlations of ³He/⁴He and ⁴⁰Ar/³⁶Ar in the Mariana Trough samples are explained by mixing between MORB and atmosphere. One sample from the Central Graben indicates extreme enrichment in ²⁰Ne/²²Ne and ²¹Ne/²²Ne, suggesting incorporation of solar‐type Ne in the magma source. Excess ¹²⁹Xe is also observed in this sample suggesting primordial noble gases in the mantle source. The Mariana Trough basalts indicate that both fluid and sediment components contributed to the basalts, with slab‐derived fluids dominating beneath the Spreading Ridge, and that sediment melts, characterized by high La/Sm and relatively low U/Th and Zr/Nb, dominate in the source region of basalts from the Central Graben.  相似文献