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The effect of oxygen fugacity and volatile content on Martian and terrestrial magmatic evolution.

机译:氧气逸度和挥发物含量对火星和陆地岩浆演化的影响。

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摘要

This dissertation addresses the role of water and oxygen fugacity in magmatic systems on Mars and the earth by correlating analyses of eruptive products with laboratory studies that are designed to reproduce the conditions necessary to replicate the observed features. The first two chapters of this dissertation focus on the oxygen fugacity (fO2) variations of Martian magmas as recorded by elemental fractionations in the Martian meteorite pyroxenes. The multivalent cations europium and iron were calibrated for use as oxybarometers in the meteoritic pyroxenes. The results indicate that variations on the order of three log units oxygen fugacity are recorded in the meteorites. Several processes have been proposed to explain the origin of this fO2 range, the majority of which involve assimilation of an oxidized source. A potential correlation between new pyroxene data (an early crystallizing phase) from this study and recent data from late-crystallizing Fe-Ti oxides, however, is consistent with the idea that intrinsic fO2 differences in the magma source region are responsible for the measured f O2 variation. This implies that the Martian meteorite source region, the mantle or lithosphere, may be heterogeneous in nature. It should be noted, however, that early assimilation events that took place before crystallization commenced cannot be ruled out.; The third chapter explores the effects of water on phase equilibria and ascent rate of a terrestrial dacitic magma from Black Butte, a flank dome of Mount Shasta, California. The pre-eruption storage conditions were determined through phase equilibria experiments and analytical petrography. The phenocryst assemblage was reproduced experimentally at 900°C, 300 MPa, X H2O = 1, and fO2 = NNO+1. Magma ascent rate was quantified using amphibole breakdown rim and plagioclase microlite crystal size distribution (CSD) measurements in both the natural and experimentally decompressed samples. Ascent rates calculated from both the amphibole and plagioclase methods indicate similar ascent rates (0.002 m/s) for the Black Butte magma, similar to effusive extrusion rates calculated for other subduction zone volcanic systems.
机译:本文通过将喷发产物的分析与旨在重现观测特征的必要条件的实验室研究相关联,探讨了水和氧逸度在火星和地球岩浆系统中的作用。本论文的前两章着重于火星陨石辉石中元素分馏所记录的火星岩浆的氧逸度(fO2)变化。对多价阳离子euro和铁进行了校准,以便用作陨石辉石中的氧饱和度计。结果表明,在陨石中记录了三个对数单位氧逸度的变化。已经提出了几种方法来解释该fO 2范围的来源,其中大多数涉及氧化源的同化。然而,这项研究中新的辉石数据(早期结晶阶段)与后期结晶的Fe-Ti氧化物最新数据之间的潜在相关性与以下观点一致:岩浆源区中固有的fO2差异是所测f的原因。 O2变化。这意味着火星陨石的源区,地幔或岩石圈在性质上可能是异质的。但是,应该指出,不能排除在结晶开始之前发生的早期同化事件。第三章探讨了水对黑沙丘(加利福尼亚山沙斯塔山顶)的陆生damagtic岩浆的相平衡和上升速率的影响。通过相平衡实验和分析岩相学确定了喷发前的储存条件。在900°C,300 MPa,X H2O = 1和fO2 = NNO + 1的条件下,通过实验复制了表晶混合物。在天然和实验减压样品中,均使用闪石击穿边缘和斜长石微晶晶体尺寸分布(CSD)测量来量化岩浆上升速率。从闪石和斜长石方法计算出的上升速率表明,黑But岩浆的上升速率(0.002 m / s)与其他俯冲带火山系统的渗出挤压速率相似。

著录项

  • 作者

    McCanta, Molly Colleen.;

  • 作者单位

    Brown University.;

  • 授予单位 Brown University.;
  • 学科 Geology.; Geochemistry.; Mineralogy.
  • 学位 Ph.D.
  • 年度 2004
  • 页码 228 p.
  • 总页数 228
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地质学;地质学;矿物学;
  • 关键词

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