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Multiple Origins of Alluvial Diamonds from New South Wales, Australia

机译:来自澳大利亚新南威尔士州的冲积钻石的多种来源

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In eastern Australia, diamonds occur in alluvial deposits overlying Phanerozoic basement. The origin of the diamonds is nut known. No feeder pipes of kimberlite or lamproite are known, and none of the usual diamond indicator minerals occurs in association with the diamonds.Alluvial diamonds from Wellington, Bingara, Copeton, and Airly Mountain in New South Wales form two distinct groups, here termed A and B. Group A diamonds are similar to those found in kimberlites and lamproites globally and are thought to have formed in Precambrian lithospheric mantle. Group B diamonds have unusual characteristics that indicate they formed in a subduction environment. Surface features of diamonds of both groups indicate that all were brought to the surface by magmas.Group A diamonds are similar in primary crystal form, internal structure, mineral inclusion composition (mainly peridotitic), and carbon isotopes to diamonds found in kimberlitic and lamproitic hosts in Archean and Proterozoic cratons worldwide. Re/Os ages (3.4 and 2.1 Ga; Pearson et al., 1998) of sulfide inclusions in two Group A diamonds constrain the origin of these diamonds to ancient mantle sources. This, along with the nature of the surface abrasion structures and radiation damage, suggests that the Group A diamonds represent an older group of diamonds that have been in secondary collectors for a significant time. If this is so, it is feasible that the Group A diamonds may have been derived from a number of primary sources, including possible sources in Antarctica.Group B diamonds are unlike any other diamond suites worldwide in their combination of shape, surface features, strained and irregular internal structures, ~(13)C-enrichment, and Ca-rich eclogitic mineral inclusions. The features are best explained as a product of diamond growth under varying P-T conditions in a high P/T dynamic environment such as a subducting slab. The diamonds may well have formed during arc-continent collision at the time of the development of the New England fold belt. This would explain why the major known concentration of Group B diamonds is within the New England fold belt at Copeton and Bingara, and is consistent with the Phanerozoic ages for diamond emplacement determined from mineral inclusions.
机译:在澳大利亚东部,钻石在上生代基底之上的冲积层中产生。钻石的来源尚不清楚。没有已知的金伯利岩或堇青石供料管,也没有与钻石相关的常见钻石指示剂矿物。来自惠灵顿,宾加拉,库珀顿和新南威尔士州的艾利山的冲积钻石分为两个不同的组,分别称为A和B. A组钻石与全球金伯利岩和斜长岩中的钻石相似,被认为是在前寒武纪岩石圈地幔中形成的。 B组钻石具有不寻常的特征,表明它们是在俯冲环境中形成的。两组钻石的表面特征都表明它们都是由岩浆带到地表的。A组钻石的初级晶体形式,内部结构,矿物包裹体成分(主要为橄榄岩)和碳同位素与金伯利岩岩体和南北岩系中的钻石相似。在全球的太古代和元古代克拉通中。两种A组钻石中硫化物夹杂物的Re / Os年龄(3.4和2.1 Ga; Pearson等人,1998)使这些钻石的起源局限于古老的地幔源。这与表面磨损结构和辐射损伤的性质一起,表明A组钻石代表了已在二手收藏家中使用了相当长一段时间的较旧的钻石组。如果是这样的话,那么A组钻石可能来自许多主要来源,包括南极洲的可能来源.B组钻石在形状,表面特征,拉力的组合方面与世界上任何其他钻石套件都不一样。和不规则的内部结构,〜(13)C富集和富含Ca的片状矿物包裹体。最好将这些特征解释为在高P / T动态环境(例如俯冲板)中,在不同的P-T条件下钻石生长的产物。钻石很可能是在新英格兰折叠带发展时的弧-陆碰撞中形成的。这可以解释为什么B组钻石的主要已知浓度集中在Copeton和Bingara的新英格兰褶皱带内,并且与由矿物包裹体确定的钻石时代的古生代时代相一致。

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