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Microtextural Studies of Feldspar in Ordinary Chondrites

机译:普通球粒长石的微观组织研究

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摘要

Ordinary chondrites contain an important record of events that took place during the earliest period of solar system evolution. These include primary processes, such as chondrule formation, and secondary processes, those that affected asteroids after accretion and modified primary components. Secondary processes include aqueous alteration, thermal metamorphism, and shock effects from impact events. Secondary minerals can provide insight into the chemical and physical conditions that affected their parent asteroids. Feldspar is known to be a secondary mineral that crystallized during thermal metamorphism. The goal of this work is to use the formation and evolution of feldspar to elucidate the conditions of secondary processing on the ordinary chondrite parent asteroids. I show the common occurrence of primary feldspar in chondrules and reveal ubiquitous evidence for widespread metasomatism recorded by feldspar, which has not been fully recognized previously.;Chapter 1 provides an overview of the effects of metamorphism in the L group of ordinary chondrites, as observed in feldspar as well as secondary phosphate minerals. I show that metamorphism of secondary minerals is similar in H, L, and LL groups of ordinary chondrites. Chapter 2 presents a study of the minimally metamorphosed ordinary chondrite Semarkona. I show that primary igneous plagioclase, with a wide range of compositions, is present within chondrules. Chapter 3 then follows the formation and alteration of feldspar in chondrules through the metamorphic sequence. I observe abundant evidence for metasomatism in feldspar, particularly in altered calcic plagioclase, crystallized secondary albite, and exsolved of K-feldspar from primary and secondary albite. I present a three-stage model of metasomatism involving prograde hydrous alteration, dehydration near peak metamorphism, and late-stage infiltration of anhydrous fluids. In Chapter 4, I examine fine-scale exsolution lamellae of K-feldspar in albite to determine cooling rates. I find fast cooling rates at high temperatures and discuss implications for thermal histories of ordinary chondrite parent bodies. Chapter 5 explores the development of porosity in chondrules. I show that pores in chondrules are the result of dissolution of feldspar and mesostasis glass, and that their existence facilitated fluid flow and chemical transport between chondrules and surrounding matrix.
机译:普通的球粒陨石包含在太阳系演化的最早时期发生的事件的重要记录。这些包括主要过程,例如软骨形成,以及次要过程,这些过程会在吸积后影响小行星并改变主要成分。次要过程包括水蚀,热变质和冲击事件引起的冲击作用。次生矿物可以洞悉影响其母体小行星的化学和物理条件。长石是热变质过程中结晶的次生矿物。这项工作的目的是利用长石的形成和演化来阐明普通球粒陨石母体小行星的二次加工条件。我展示了长粒石中长石的普遍发生,并揭示了长石记录的广泛的交代作用的普遍证据,这在以前尚未得到充分认识。;第1章概述了L组普通球粒陨石的变质作用。在长石以及二次磷酸盐矿中。我表明普通球粒陨石的H,L和LL组中次生矿物的变质作用相似。第2章介绍了对最小变形的普通球粒陨石Semarkona的研究。我表明,在软骨中存在具有广泛组成的原发性火成斜长石。第三章接着讨论了通过变质序列在软骨中长石的形成和变化。我观察到长石中有交代作用的大量证据,特别是钙斜长石改变,次生钠长石结晶以及从初生和次生钠长石中析出的钾长石。我提出了一个三阶段的交代模型,包括前期含水变化,接近峰值变质的脱水以及无水流体的后期渗透。在第4章中,我检查了钠长石中钾长石的细颗粒析晶片,以确定冷却速率。我发现高温下的冷却速度很快,并讨论了对普通球粒陨石母体热历史的影响。第5章探讨了软骨中孔隙的发展。我表明,软骨中的孔是长石和介晶玻璃溶解的结果,并且它们的存在促进了软骨和周围基质之间的流体流动和化学传输。

著录项

  • 作者

    Lewis, Jonathan A.;

  • 作者单位

    The University of New Mexico.;

  • 授予单位 The University of New Mexico.;
  • 学科 Planetology.;Geochemistry.;Mineralogy.
  • 学位 Ph.D.
  • 年度 2018
  • 页码 421 p.
  • 总页数 421
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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