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首页> 外文期刊>Meteoritics & planetary science >Aqueous alteration of the Martian meteorite Northwest Africa 817: Probing fluid–rock interaction at the nakhlite launch site
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Aqueous alteration of the Martian meteorite Northwest Africa 817: Probing fluid–rock interaction at the nakhlite launch site

机译：Martian Meteorite Northwest Afroma的水改变817：Nakhlite发射部位探测流体岩石互动

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Abstract > The nakhlite meteorites characteristically contain iddingsite, a hydrous iron–magnesium silicate that formed by aqueous alteration on Mars. Iddingsite is most abundant in Northwest Africa ( <fc>NWA</fc> ) 817, and alteration products in this meteorite also have the lowest deuterium/hydrogen ratio of any nakhlite. Taken together, these distinctive properties could be interpreted to show that <fc>NWA</fc> 817 was altered under different physico‐chemical conditions than the other nakhlites and by liquid water from a separate reservoir. Here this interpretation is tested through a petrographic, mineralogical, chemical, and isotopic study of <fc>NWA</fc> 817. We find that its iddingsite occurs as olivine‐hosted veins of nanocrystalline smectite and Fe‐oxyhydroxide. Strong similarities in the mineralogy of iddingsite between <fc>NWA</fc> 817 and other nakhlites suggest that these meteorites were altered under comparable physico‐chemical conditions, with the Fe‐rich composition of <fc>NWA</fc> 817 olivine grains rendering them especially susceptible to aqueous alteration. Analyses of <fc>NWA</fc> 817 bulk samples by stepwise pyrolysis confirm that its iddingsite has unusually low deuterium/hydrogen ratios, but owing to terrestrial weathering of this meteorite, the hydrogen isotopic data cannot be used with confidence to infer the origin of Martian aqueous solutions. <fc>NWA</fc> 817 was most probably altered along with the other nakhlites over a short time period and in a common aqueous system. One interpretation of a correlation between the eruption ages of three of the nakhlites and the chemical composition of their iddingsite is that water originated from close to the surface of Mars and flowed through the nakhlite lava pile under the influence of gravity. </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 =“maps13136-abs-0001”xml：lang =“en”> <标题类型=“main”>抽象</ title> > Nakhlite Meteorites特征性地含有IDDingsite，一种通过MARS水溶液形成的含水铁 - 镁硅酸盐。 Iddingsite在西北非洲最丰富（ <FC> NWA </ FC> ）817，这种陨石中的改变产物也具有任何Nakhlite的最低氘/氢比。连同，这些独特的属性可以被解释为表明这一点 <FC> NWA </ FC> 817在不同的物理化学条件下比其他Nakhlites和来自单独的储存器的液态水改变。在这里，这种解释是通过岩体，矿物学，化学和同位素研究来测试的 <FC> NWA </ FC> 817.我们发现其Iddingsite作为纳米晶蒙脱石和Fe-羟基氧化物的橄榄石托管静脉发生。 inddingsite矿物质中的强烈相似之处 <FC> NWA </ FC> 817和其他Nakhlites表明这些陨石在可比较的物理化学条件下改变，具有富含费用的组合物 <FC> NWA </ FC> 817个橄榄石颗粒使它们特别容易受到水性改变的影响。分析 <FC> NWA </ FC> 通过逐步热解的817个散装样品证实，其Iddingsite具有异常低的氘/氢气量，但由于这种陨石的陆地风化，氢同位素数据不能置信，以便推断火星水溶液的起源。 <FC> NWA </ FC> 在短时间内和常见的水系统中，最多可能与其他纳克莱斯一起改变817。一种解释纳克莱特三个爆发衰龄和其念特的化学成分之间的相关性是，水源于火星的表面，并在重力的影响下流过Nakhlite Lava堆。 </ 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11期</span><b style="margin: 0 2px;">|</b><span>共18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=Lee M. R.&option=202" target="_blank" rel="nofollow">Lee M. R.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Daly L.&option=202" target="_blank" rel="nofollow">Daly L.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Cohen B. E.&option=202" target="_blank" rel="nofollow">Cohen B. E.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Hallis L. J.&option=202" target="_blank" rel="nofollow">Hallis L. J.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Griffin S.&option=202" target="_blank" rel="nofollow">Griffin S.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Trimby P.&option=202" target="_blank" rel="nofollow">Trimby P.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Boyce A.&option=202" target="_blank" rel="nofollow">Boyce A.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Mark D. F.&option=202" target="_blank" rel="nofollow">Mark D. F.;</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>School of Geographical and Earth SciencesUniversity of GlasgowGregory Building Lilybank Gardens Glasgow G12 8QQ UK;</p> <p>School of Geographical and Earth SciencesUniversity of GlasgowGregory Building Lilybank Gardens Glasgow G12 8QQ UK;</p> <p>School of Geographical and Earth SciencesUniversity of GlasgowGregory Building Lilybank Gardens Glasgow G12 8QQ UK;</p> <p>School of Geographical and Earth SciencesUniversity of GlasgowGregory Building Lilybank Gardens Glasgow G12 8QQ UK;</p> <p>School of Geographical and Earth SciencesUniversity of GlasgowGregory Building Lilybank Gardens Glasgow G12 8QQ UK;</p> <p>Oxford Instruments NanoanalysisHigh Wycombe HP12 3SE UK;</p> <p>Scottish Universities Environmental Research CentreRankine Avenue Scottish Enterprise Technology Park East Kilbride G75 0QF UK;</p> <p>Scottish Universities Environmental Research CentreRankine Avenue Scottish Enterprise Technology Park East Kilbride G75 0QF 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/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> </ul> </div> <div class="similarity_details"> <ul > <li> <div> <b>1. </b><a class="enjiyixqcontent" href="/journal-foreign-detail/0704023664733.html">Aqueous alteration of the Martian meteorite Northwest Africa 817: Probing fluid–rock interaction at the nakhlite launch site</a> <b>[J]</b> . <span> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Lee M. 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