Multidisciplinary Constraints on the Abundance of Diamond and Eclogite in the Cratonic Lithosphere

Garber Joshua M.; Maurya Satish; Hernandez Jean‐Alexis; Duncan Megan S.; Zeng Li; Zhang Hongluo L.; Faul Ulrich; McCammon Catherine; Montagner Jean‐Paul; Moresi Louis; Romanowicz Barbara A.; Rudnick Roberta L.; Stixrude Lars

摘要

Abstract > Some seismic models derived from tomographic studies indicate elevated shear‐wave velocities (≥4.7?km/s) around 120–150?km depth in cratonic lithospheric mantle. These velocities are higher than those of cratonic peridotites, even assuming a cold cratonic geotherm (i.e., 35?mW/m 2 surface heat flux) and accounting for compositional heterogeneity in cratonic peridotite xenoliths and the effects of anelasticity. We reviewed various geophysical and petrologic constraints on the nature of cratonic roots (seismic velocities, lithology/mineralogy, electrical conductivity, and gravity) and explored a range of permissible rock and mineral assemblages that can explain the high seismic velocities. These constraints suggest that diamond and eclogite are the most likely high‐ V <sub>s</sub> candidates to explain the observed velocities, but matching the high shear‐wave velocities requires either a large proportion of eclogite (50?vol.%) or the presence of up to 3?vol.% diamond, with the exact values depending on peridotite and eclogite compositions and the geotherm. Both of these estimates are higher than predicted by observations made on natural samples from kimberlites. However, a combination of ≤20?vol.% eclogite and ~2?vol.% diamond may account for high shear‐wave velocities, in proportions consistent with multiple geophysical observables, data from natural samples, and within mass balance constraints for global carbon. Our results further show that cratonic thermal structure need not be significantly cooler than determined from xenolith thermobarometry. </abstract> </span> <span class="z_kbtn z_kbtnclass hoverxs" style="display: none;">展开▼</span> </div> <div class="translation abstracttxt"> <span class="zhankaihshouqi fivelineshidden" id="abstract"> <span>机译：</span><Abstract Type =“Main”XML：Lang =“en”> <标题类型=“main”>抽象</ title> > 源自断层性研究的一些地震模型表示克拉特尼岩石地幔中升高的剪切波速度（≥4.7μm/ km）约为120-150 km深度。这些速度高于Cratonon恒星的速度，即使是假设冷爬脚地热（即35μm/ m 2 </ sup> 表面热通量，并占Cratonon PeridoTite Xenoliths中的组成异质性及其心制性的影响。我们审查了对克拉特尼根的性质（地震速度，岩性/矿物学，导电性和重力）的各种地球物理和岩石结构限制，并探索了一系列可解释高地震速度的允许岩石和矿物组装。这些约束表明钻石和eClogite是最可能的高度 - v </ i> <sub> s </ sub> 解释观察到的速度的候选者，但匹配高剪切波速度需要大量的eNlogite（＆ 50？Vol.％）或最多可存在的存在，或者百万钻，取决于确切的值橄榄石和eClogite组合物和地热。这些估计的两者都是高于通过来自Kimberlites的天然样本所取出的观察结果预测。但是，≤20？VOL。％Eclogite和〜2？VOL。％钻石可能考虑高剪切波速度，其比例与多个地球物理可观察品，来自天然样本的数据一致，以及全球碳的质量平衡约束。。我们的结果进一步表明，克拉固热结构不需要显着冷却，而不是由Xenolith Thermobometry确定的。 </ p> </摘要> </span> <span class="z_kbtn z_kbtnclass hoverxs" style="display: none;">展开▼</span> </div> </div> <div class="record"> <h2 class="all_title" id="enpatent33" >著录项</h2> <ul> <li> <span class="lefttit">来源</span> <div style="width: 86%;vertical-align: text-top;display: inline-block;"> <a href='/journal-foreign-23285/'>《Geochemistry, geophysics, geosystems》</a> <b style="margin: 0 2px;">|</b><span>2018年第7期</span><b style="margin: 0 2px;">|</b><span>共25页</span> </div> </li> <li> <div class="author"> <span class="lefttit">作者</span> <p id="fAuthorthree" class="threelineshidden zhankaihshouqi"> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Garber Joshua M.&option=202" target="_blank" rel="nofollow">Garber Joshua M.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Maurya Satish&option=202" target="_blank" rel="nofollow">Maurya Satish;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Hernandez Jean‐Alexis&option=202" target="_blank" rel="nofollow">Hernandez Jean‐Alexis;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Duncan Megan S.&option=202" target="_blank" rel="nofollow">Duncan Megan S.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Zeng Li&option=202" target="_blank" rel="nofollow">Zeng Li;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Zhang Hongluo L.&option=202" target="_blank" rel="nofollow">Zhang Hongluo L.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Faul Ulrich&option=202" target="_blank" rel="nofollow">Faul Ulrich;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=McCammon Catherine&option=202" target="_blank" rel="nofollow">McCammon Catherine;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Montagner Jean‐Paul&option=202" target="_blank" rel="nofollow">Montagner Jean‐Paul;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Moresi Louis&option=202" target="_blank" rel="nofollow">Moresi Louis;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Romanowicz Barbara A.&option=202" target="_blank" rel="nofollow">Romanowicz Barbara A.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Rudnick Roberta L.&option=202" target="_blank" rel="nofollow">Rudnick Roberta L.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Stixrude Lars&option=202" target="_blank" rel="nofollow">Stixrude Lars;</a> </p> <span class="z_kbtnclass z_kbtnclassall hoverxs" id="zkzz" style="display: none;">展开▼</span> </div> </li> <li> <div style="display: flex;"> <span class="lefttit">作者单位</span> <div style="position: relative;margin-left: 3px;max-width: 639px;"> <div class="threelineshidden zhankaihshouqi" id="fOrgthree"> <p>Department of Earth ScienceUniversity of CaliforniaSanta Barbara CA USA;</p> <p>Institut de Physique du Globe de ParisParis France;</p> <p>Laboratoire LULIEcole PolytechniquePalaiseau France;</p> <p>Geophysical LaboratoryCarnegie Institution of WashingtonWashington DC USA;</p> <p>Department of Earth and Planetary SciencesHarvard UniversityCambridge MA USA;</p> <p>Department of Geophysics and Planetary SciencesUniversity of Science and Technology of ChinaHefei China;</p> <p>Department of Earth Atmospheric and Planetary SciencesMassachusetts Institute of TechnologyCambridge MA USA;</p> <p>Bayerisches GeoinstitutUniversity of BayreuthBayreuth Germany;</p> <p>Institut de Physique du Globe de ParisParis France;</p> <p>School of Earth SciencesUniversity of MelbourneParkville Victoria Australia;</p> <p>Department of Earth and Planetary ScienceUniversity of CaliforniaBerkeley CA USA;</p> <p>Department of Earth ScienceUniversity of CaliforniaSanta Barbara CA USA;</p> <p>Department of Earth SciencesUniversity College LondonLondon UK;</p> </div> <span class="z_kbtnclass z_kbtnclassall hoverxs" id="zhdw" style="display: none;">展开▼</span> </div> </div> </li> <li > <span class="lefttit">收录信息</span> <span style="width: 86%;vertical-align: text-top;display: inline-block;"></span> </li> <li> <span class="lefttit">原文格式</span> <span>PDF</span> </li> <li> <span class="lefttit">正文语种</span> <span>eng</span> </li> <li> <span class="lefttit">中图分类</span> <span><a href="https://www.zhangqiaokeyan.com/clc/163.html" title="地球物理学">地球物理学;</a></span> </li> <li class="antistop"> <span class="lefttit">关键词</span> <p style="width: 86%;vertical-align: text-top;"> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=cratonic lithosphere&option=203" rel="nofollow">cratonic lithosphere;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=diamond&option=203" rel="nofollow">diamond;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=eclogite&option=203" rel="nofollow">eclogite;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=seismic tomography&option=203" rel="nofollow">seismic tomography;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=petrologic modeling&option=203" rel="nofollow">petrologic modeling;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=electrical conductivity&option=203" rel="nofollow">electrical conductivity;</a> </p> <div class="translation"> 机译：克拉廷岩石圈;钻石;eClogite;地震层析成像;碳化岩层;电导率; </div> </li> </ul> </div> </div> <div class="literature cardcommon"> <div class="similarity "> <h3 class="all_title" id="enpatent66">相似文献</h3> <div class="similaritytab clearfix"> <ul> <li class="active" >外文文献</li> <li >中文文献</li> <li >专利</li> </ul> </div> <div class="similarity_details"> <ul > <li> <div> <b>1. </b><a class="enjiyixqcontent" href="/journal-foreign-detail/0704023360732.html">Multidisciplinary Constraints on the Abundance of Diamond and Eclogite in the Cratonic Lithosphere</a> <b>[J]</b> . <span> <a 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