Origin and significance of cosmogenic signatures in vesicles of lunar basalt 15016

Bekaert David V.; Avice Guillaume; Marty Bernard

摘要

Abstract > Lunar basalt 15016 (~3.3?Ga) is among the most vesicular (50% by volume) basalts recovered by the Apollo missions. We investigated the possible occurrence of indigenous lunar nitrogen and noble gases trapped in vesicles within basalt 15016, by crushing several cm‐sized chips. Matrix/mineral gases were also extracted from crush residues by fusion with a <fc>CO</fc> <sub>2</sub> laser. No magmatic/primordial component could be identified; all isotope compositions, including those of vesicles, pointed to a cosmogenic origin. We found that vesicles contained ~0.2%, ~0.02%, ~0.002%, and ~0.02% of the total amount of cosmogenic 21 Ne, 38 Ar, 83 Kr, and 126 Xe, respectively, produced over the basalt's 300?Myr of exposure. Diffusion/recoil of cosmogenic isotopes from the basaltic matrix/minerals to intergrain joints and vesicles is discussed. The enhanced proportion of cosmogenic Xe isotopes relative to Kr detected in vesicles could be the result of kinetic fractionation, through which preferential retention of Xe isotopes over Kr within vesicles might have occurred during diffusion from the vesicle volume to the outer space through microleaks. This study suggests that cosmogenic loss, known to be significant for 3 He and 21 Ne, and to a lesser extent for 36 Ar (Signer et?al. [Signer P., 1977]), also occurs to a negligible extent for the heaviest noble gases Kr and Xe. </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 XMLNS =“http://www.wiley.com/namespaces/wiley”type =“main”xml：id =“maps13069-abs-0001”xml：lang =“en”> <标题类型=“main”>抽象</ title> > 月球玄武岩15016（〜3.3？GA）是Apollo任务恢复的最凹凸（50％（50％）的基础之一。通过粉碎几个CM尺寸的芯片，我们调查了截留在玄武岩15016内的囊泡中的土着月球氮和惰性气体的可能出现。通过融合，还通过融合中提取基质/矿物气体通过熔化残留物 <FC> CO </ FC> <sub> 2 </ sub> 激光。无法识别岩浆/原始组件;所有同位素组合物，包括囊泡的那些，指向富含念头。我们发现囊泡含有约0.2％，〜0.02％，〜0.002％，〜0.02％的宇宙中含量 21 </ sup> 鼻子， 38 </ sup> ar， 83 </ sup> KR，和 126 </ sup> XE分别在玄武岩300？曝光中产生的。讨论了来自玄武岩基质/矿物质的玄武岩基质同位素的扩散/反馈，并进行了整形接头和囊泡。相对于在囊泡中检测到的Kr的增强比例可以是动力学分馏的结果，通过它在通过微框中的囊泡体积的扩散期间可能发生囊泡内kr上的Xe同位素的优先保留。该研究表明，富裕的损失，已知是重要的 3 </ sup> 他和 21 </ sup> NE，以及较小程度 36 </ sup> AR（签名者等等。[签名者P.，1977]），也发生在最重最大的惰性气体KR和XE的程度上。 </ 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-24922/'>《Meteoritics & planetary science》</a> <b style="margin: 0 2px;">|</b><span>2018年第6期</span><b style="margin: 0 2px;">|</b><span>共14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=Bekaert David V.&option=202" target="_blank" rel="nofollow">Bekaert David V.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Avice Guillaume&option=202" target="_blank" rel="nofollow">Avice Guillaume;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Marty Bernard&option=202" target="_blank" rel="nofollow">Marty Bernard;</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>Centre de Recherches Pétrographiques et GéochimiquesUMR 7358 CNRS—Université de Lorraine15 rue Notre Dame des Pauvres BP 20 54501 Vandoeuvre‐lès‐Nancy France;</p> <p>Centre de Recherches Pétrographiques et GéochimiquesUMR 7358 CNRS—Université de Lorraine15 rue Notre Dame des Pauvres BP 20 54501 Vandoeuvre‐lès‐Nancy France;</p> <p>Centre de Recherches Pétrographiques et GéochimiquesUMR 7358 CNRS—Université de Lorraine15 rue Notre Dame des Pauvres BP 20 54501 Vandoeuvre‐lès‐Nancy France;</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/161.html" title="天文学">天文学;</a></span> </li> <li class="antistop"> <span class="lefttit">关键词</span> <p style="width: 86%;vertical-align: text-top;"> </p> </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/0704023665079.html">Origin and significance of cosmogenic signatures in vesicles of lunar basalt 15016</a> <b>[J]</b> . <span> <a 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