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Tectonic controls on Ni and Cu contents of primary mantle-derived magmas for the formation of magmatic sulfide deposits

机译:用于岩浆硫化物沉积物形成的主要地幔衍生岩浆Ni和Cu含量的构造控制

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We have modeled the genesis of primary mantle-derived magma to explore the controls exerted on its Ni-Cu ore potential by water content, pressure, and mantle potential temperature (T-p). During decompression melting, Ni concentration in primary magma decreases with an increasing degree of melting, which is in contradiction to long-held understanding obtained from previous isobaric melting models. Pressure exerts a first-order control on the ore potential of primary plume-derived melt, such that plumes rising beneath thick lithosphere with melting paths terminating at relatively high pressure generate Ni-rich melts. Additionally, as plumes with higher T-p produce more Ni-rich melt at a higher pressure, the magmatism related to hotter plume-centers may have the greatest ore potential. On the other hand, the strong dependence of Cu behavior upon the presence or absence of residual sulfide is partly countered in decompression melting. Significant influences of mantle-contained water on Ni and Cu partitioning are restricted to low-degree melting. While release of H2O in lithosphere delamination may trigger voluminous magmatism, the Ni concentration in the melt is far lower than in melt generated from plumes. Furthermore, if isobaric melting dominates when the subcontinental litho spheric mantle (SCLM) is heated by underlying hotter plumes, the plume-lithosphere interaction plays no active role in the Ni ore potential of primary magma because derived melt volumes are relatively small. In subduction zones, flux-melting of the mantle wedge tends to generate cool Ni-poor melts, however hot subduction zones may produce magmas with increased metal concentrations. Overall, the anticipated ranges of Ni contents in primary melts are strongly controlled by tectonic setting, with a range of 100-300 ppm in subduction zones, 230-450 ppm in mid-ocean ridges, and 500-1300 ppm in plume suites. There are only minor differences in the Cu concentrations of primitive magmas generated from diverse tectonic settings, despite the variations in Cu partitioning behaviors.
机译:我们已经建模了主要地幔源性岩浆的成因,以探讨通过含水量,压力和地幔潜在温度(T-P)对其Ni-Cu矿势施加的对照。在减压熔融期间,初级岩浆中的Ni浓度随着熔化程度的增加而降低,这与从先前的异教熔化模型获得的长期理解矛盾。压力对主羽流衍生的熔体的矿石电位施加了一流的控制,使得在厚的岩石圈下升的羽毛在相对高的压力下终止于富含Ni的熔体。另外,由于具有较高T-P的羽流,在更高的压力下产生更丰富的Ni的熔体,与更热的羽流相关的岩浆可能具有最大的矿石潜力。另一方面,Cu行为在存在或不存在残留硫化物时的强烈依赖性部分地抵消了减压熔化。含有碎片含水对Ni和Cu分配的显着影响仅限于低度熔化。虽然在岩石圈分层中释放H2O可以触发大量的岩浆,但熔体中的Ni浓度远低于从羽毛产生的熔体中的浓度远低于熔体。此外,如果通过潜在的较热羽毛加热亚型Litho球形罩(SCLM),因此羽毛岩石圈相互作用在初级岩浆的Ni矿石电位中发挥了不良作用,因此由于衍生的熔体量相对较小,因此在潜在的熔融熔融偏离。在俯冲区域中,披风楔的熔融膨胀趋于产生凉爽的Ni熔体熔体,但是热俯冲区可以产生具有增加的金属浓度的磁带。总体而言,初级熔体中的Ni含量的预期范围受到构造环境的强烈控制,俯冲区的100-300ppm,中海脊230-450ppm,500-1300ppm在羽流套件中。尽管Cu分区行为的变化,从不同的构造环境产生的原始磁带的Cu浓度只有微小的差异。

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