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Thermodynamic models for eclogitic mantle lithosphere

机译:地幔幔岩石圈的热力学模型

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Cratonic mantle eclogite xenoliths occur with diamond-bearing kimberlite. The modes and mineral compositions of eclogite contain important information on their origin, physical-chemical conditions of formation, and their geophysical properties. We have used the pseudosection option of the program PERPLEX to explore how mineral assemblage, abundance, and composition vary with bulk composition, temperature (T) and pressure (P). We considered a range of protolith compositions, including: fresh unaltered basalt, altered seafloor basalt, cumulates resulting from high-pressure crystallization of basaltic melts, and metasomatically altered (SiO_2-depleted) basalt. Stable mineral assemblages and associated geophysical properties for each protolith were calculated at P–T conditions found along the mantle geotherm for the Slave craton. At depths greater than 90 km, the predicted modal mineralogy of eclogite for all protoliths changes little along the geotherm. Within the diamond stability field of cratonic mantle, eclogite has a single mineral assemblage that reflects protolith composition. We recognize three basic classes: (1) a silica-oversaturated assemblage indicated by the presence of coesite, (2) a silica-saturated assemblage distinguished by the absence of coesite and olivine, and (3) a silica-undersaturated assemblage containing olivine. Within the diamond stability field for the Slave geotherm, kyanite is stable only in extremely Al-enriched protoliths. Most kimberlite-hosted eclogite belongs to class 2 and our results show that it cannot derive from either fresh or altered seafloor basalt. We suggest an origin involving mantle metasomatism (SiO2 depletion) operating on subducted basalt although we cannot rule out an origin from cumulates of metaluminous, subalkaline magmas. Predicted seismic velocities of model eclogite are higher than corresponding velocities for peridotite and most crustal rocks and therefore may be distinctive in regional seismic surveys. However, the only class of eclogite that could be distinguished from seismic data is the oversaturated assemblage (class 1). The quartz–coesite transition produces sharp changes in both P and S wave velocities at depths of about 90 km along the ambient mantle geotherm.
机译:克拉通时期的榴辉岩闪长岩与含金刚石的石英岩一起出现。榴辉岩的形态和矿物成分包含有关其来源,形成的物理化学条件及其地球物理性质的重要信息。我们使用了PERPLEX程序的伪截面选项来研究矿物组合,丰度和组成随体积组成,温度(T)和压力(P)的变化。我们考虑了一系列的原生石成分,包括:未变质的新鲜玄武岩,改变后的海底玄武岩,由玄武质熔体的高压结晶产生的堆积物以及变质变(贫SiO_2的玄武岩)。在沿奴隶克拉通地幔地热发现的P–T条件下,计算了每种原生岩的稳定矿物组合和相关的地球物理特性。在深度大于90 km时,所有原型岩的榴辉岩的预测模态矿物学沿地热变化不大。在克拉通地幔的钻石稳定领域内,榴辉岩具有单一矿物组合,反映了原生岩的组成。我们认识到三个基本类别:(1)硅藻土的存在表明存在二氧化硅过度饱和的组合,(2)硅藻土和橄榄石不存在引起的二氧化硅饱和的组合,以及(3)包含橄榄石的二氧化硅不饱和的组合。在奴隶地热的钻石稳定性领域内,蓝晶石仅在极富铝的原石中稳定。大多数由金伯利岩主持的榴辉岩属于2类,我们的结果表明,它既不能来自新鲜的海底玄武岩,也不能来自改变后的海底玄武岩。尽管我们不能从成矿的,亚碱性的岩浆岩中排除一个起源,但我们建议一个涉及在俯冲玄武岩上进行地幔交代作用(SiO2耗竭)的成因。模型榴辉岩的预测地震波速要高于橄榄岩和大多数地壳岩石的对应波速,因此在区域地震勘探中可能具有独特性。但是,唯一可以与地震数据区分开的榴辉岩是过饱和组合物(1类)。在沿地幔地热的约90 km深度处,石英-柯氏体转变在P波和S波速度上均产生急剧变化。

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