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The noble gas concentrations of the Martian meteorites GRVGRV 99027 and paired NWANWA 7906/ NWANWA 7907

机译：火星陨石的惰性气体浓度 grv grv 99027并配对 nwa nwa 7906 / nwa nwa 7907

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Abstract > Here we present the isotopic concentrations of He, Ne, Ar, Kr, and Xe for the three Martian meteorites, namely Grove Mountains 99027 (GRV 99027), Northwest Africa 7906 ( <fc>NWA</fc> 7906), and Northwest Africa 7907 ( <fc>NWA</fc> 7907). The cosmic ray exposure (CRE) age for <fc>GRV</fc> 99027 of 5.7?±?0.4?Ma (1σ) is consistent with <fc>CRE</fc> ages for other poikilitic basaltic shergottites and suggests that all were ejected in a single event ~5.6?Ma ago. After correcting for an estimated variable sodium concentration, the <fc>CRE</fc> ages for <fc>NWA</fc> 7906 and <fc>NWA</fc> 7907 of 5.4?±?0.4 and 4.9?±?0.4?Ma (1σ), respectively, are in good agreement with the <fc>CRE</fc> age of ~5?Ma favored by Cartwright et?al. ([Cartwright J. A., 2014]) for <fc>NWA</fc> 7034. The data, therefore, support the conclusion that all three basaltic regolith breccias are paired. The 40 Ar gas retention age for <fc>NWA</fc> 7907 of ~1.3?Ga is in accord with Cartwright et?al. ([Cartwright J. A., 2014]). For <fc>NWA</fc> 7906, we were unable to determine a 40 Ar gas retention age. The 4 He gas retention ages for <fc>NWA</fc> 7906 and 7907 are in the range of 200?Ma and are much shorter than the 40 Ar gas retention age of <fc>NWA</fc> 7907, indicating that about 86–88% of the radiogenic 4 He has been lost. The Kr and Xe isotopic concentrations in <fc>GRV</fc> 99027 are composed almost exclusively of Martian interior (MI) gases, while for <fc>NWA</fc> 7906 and <fc>NWA</fc> 7907, they indicate gases from the MI, elementally fractionated air, and possibly Martian atmosphere. </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 =“maps12950-abs-0001”> <标题类型=“main”>抽象</ title> > 在这里，我们介绍了他，NE，AR，KR和XE的同位素浓度，即三个火山陨石，即Grove Mountains 99027（Grv 99027），非洲7906（ <FC> NWA </ FC> 7906）和西北非洲7907（ <FC> NWA </ FC> 7907）。宇宙射线曝光（CRE）年龄 <FC> GRV </ FC> 99027的5.7？±0.4？ma（1σ）一致 <FC> CRE </ FC> 其他波西尼玄武岩玄武梯的年龄既表明所有人都在一次事件中被射出〜5.6？MA前。纠正估计可变钠浓度后， <FC> CRE </ FC> 年龄段 <FC> NWA </ FC> 7906和 <FC> NWA </ FC> 7907分别为5.4？±0.4和4.9？±0.4？mA（1σ）与之吻合 <FC> CRE </ FC> 年龄〜5？MA由Cartwright等人青睐。 （[咖啡册J. A.，2014]）为 <FC> NWA </ FC> 因此，数据支持所有三种玄武岩概述Breccias配对的结论。这 40 </ sup> AR气体保留年龄 <FC> NWA </ FC> 7907的〜1.3？GA符合Cartwright等。 （[咖啡册J.A.，2014]）。为了 <FC> NWA </ FC> 7906，我们无法确定一个 40 </ sup> AR气体保留年龄。这 4 </ sup> 他燃气保留年龄 <FC> NWA </ FC> 7906和7907在200？ma的范围内，比 40 </ sup> AR气体保留年龄 <FC> NWA </ FC> 7907，表明约86-88％的辐射性 4 </ sup> 他已经迷失了。 KR和XE同位素浓度 <FC> GRV </ FC> 99027几乎完全由火星内部（MI）气体组成，同时 <FC> NWA </ FC> 7906和 <FC> NWA </ FC> 7907，它们表明来自MI，元素分级的空气和可能是火星氛围的气体。 </ 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>2017年第12期</span><b style="margin: 0 2px;">|</b><span>共16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=Stephenson Peter C.&option=202" target="_blank" rel="nofollow">Stephenson Peter C.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Lin Yangting&option=202" target="_blank" rel="nofollow">Lin Yangting;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Leya Ingo&option=202" target="_blank" rel="nofollow">Leya Ingo;</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>Physical InstituteUniversity of Bern3012 Bern Switzerland;</p> <p>Key Laboratory of Earth and Planetary PhysicsChinese Academy of SciencesBeijing 100864 China;</p> <p>Physical InstituteUniversity of Bern3012 Bern Switzerland;</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 >专利</li> </ul> </div> <div class="similarity_details"> <ul > <li> <div> <b>1. </b><a class="enjiyixqcontent" 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