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首页> 外文期刊>Meteoritics & planetary science >Ambient and cold‐temperature infrared spectra and XRD patterns of ammoniated phyllosilicates and carbonaceous chondrite meteorites relevant to Ceres and other solar system bodies
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Ambient and cold‐temperature infrared spectra and XRD patterns of ammoniated phyllosilicates and carbonaceous chondrite meteorites relevant to Ceres and other solar system bodies

机译：环境和冷温红外光谱和氨化的神经硅酸盐和碳质浮石陨石与CER和其他太阳系体有关

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摘要

Abstract > Mg‐phyllosilicate‐bearing, dark surface materials on the dwarf planet Ceres have NH <sub>4</sub> ‐bearing materials, indicated by a distinctive 3.06?μm absorption feature. To constrain the identity of the Ceres NH <sub>4</sub> ‐carrier phase(s), we ammoniated ground particulates of candidate materials to compare their spectral properties to infrared data acquired by Dawn's Visible and Infrared (VIR) imaging spectrometer. We treated Mg‐, Fe‐, and Al‐smectite clay minerals; Mg‐serpentines; Mg‐chlorite; and a suite of carbonaceous meteorites with NH <sub>4</sub> ‐acetate to exchange ammonium. Serpentines and chlorites showed no evidence for ammoniation, as expected due to their lack of exchangeable interlayer sites. Most smectites showed evidence for ammoniation by incorporation of NH <sub>4</sub> + into their interlayers, resulting in the appearance of absorptions from 3.02 to 3.08?μm. Meteorite samples tested had weak absorptions between 3.0 and 3.1?μm but showed little clear evidence for enhancement upon ammoniation, likely due to the high proportion of serpentine and other minerals relative to expandable smectite phases or to NH <sub>4</sub> + complexing with organics or other constituents. The wavelength position of the smectite NH <sub>4</sub> absorption showed no variation between IR spectra acquired under dry‐air purge at 25?°C and under vacuum at 25?°C to ?180?°C. Collectively, data from the smectite samples show that the precise center wavelength of the characteristic ~3.05?μm v <sub> 3 </sub> absorption in NH <sub>4</sub> is variable and is likely related to the degree of hydrogen bonding of NH <sub>4</sub> ‐H <sub>2</sub> O complexes. Comparison with Dawn VIR spectra indicates that the hypothesis of Mg‐saponite as the ammonium carrier phase is the simplest explanation for observed data, and that Ceres dark materials may be like Cold Bokkeveld or Tagish Lake but with proportionally more Mg‐smectite. </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 =“maps13103-abs-0001”XML：lang =“en”> <标题类型=“main”>抽象</ title> > Mg-phyllosinalate ud，Dwarf Planet Ceres上的深色表面材料有NH <sub> 4 </ sub> - 挤成材料，由独特的3.06？μm吸收特征表示。约束CERES NH的身份 <sub> 4 </ sub> - 载波相，我们氨化候选材料的研磨颗粒，将它们的光谱特性与黎明可见和红外（VIR）成像光谱仪获得的红外数据进行比较。我们处理了Mg-，Fe-和Al-蒙脱石粘土矿物质; Mg-蛇形; Mg-Chlorite;和一套碳质陨石套 <sub> 4 </ sub> - 交换铵。蛇纹石和氯化物没有由于他们缺乏可交换的中间位点而显示氨的证据。大多数椎间夹显示通过掺入NH的氨的证据 <sub> 4 </ sub> + </ sup> 进入其中间层，导致从3.02到3.08μm的吸收外观。测试的陨石样品在3.0和3.1之间的吸收较弱，但在氨化量上提高了明确的证据，可能是由于蛇形和其他矿物相对于可扩张的蒙脱土阶段或NH的高比例 <sub> 4 </ sub> + </ sup> 络合有机物或其他成分。蒙脱石NH的波长位置 <sub> 4 </ sub> 吸收显示在干燥空气吹扫下在25Ω·℃下在25Ω℃下获得的IR光谱之间没有变化，在25℃至180℃下真空。统称，来自蒙脱石样品的数据表明特性的精确中心波长〜3.05？μm v </ i> <sub> 3 </ i> </ sub> NH的吸收 <sub> 4 </ sub> 是可变的，并且可能与NH的氢键程度有关 <sub> 4 </ sub> -H <sub> 2 </ sub> o复合物。与黎明Vir光谱的比较表明，Mg-Saponite作为铵载体相位的假设是观察到数据的最简单的解释，并且Ceres暗材料可能就像冷的Bokkeveld或Tagish Lake，但用比例的mg-晶体。 </ 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>2018年第9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=Ehlmann Bethany L.&option=202" target="_blank" rel="nofollow">Ehlmann Bethany L.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Hodyss Robert&option=202" target="_blank" rel="nofollow">Hodyss Robert;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Bristow Thomas F.&option=202" target="_blank" rel="nofollow">Bristow Thomas F.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Rossman George R.&option=202" target="_blank" rel="nofollow">Rossman George R.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Ammannito Eleonora&option=202" target="_blank" rel="nofollow">Ammannito Eleonora;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=D Sanctis M. Cristina&option=202" target="_blank" rel="nofollow">D Sanctis M. Cristina;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Raymond Carol A.&option=202" target="_blank" rel="nofollow">Raymond Carol A.;</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>Division of Geological &</p> <p>Planetary SciencesCalifornia Institute of TechnologyPasadena California 91125 USA;</p> <p>Jet Propulsion LaboratoryPasadena California 91125 USA;</p> <p>Exobiology BranchNASA Ames Research CenterMoffett Field California 94035 USA;</p> <p>Division of Geological &</p> <p>Planetary SciencesCalifornia Institute of TechnologyPasadena California 91125 USA;</p> <p>Department of Earth Planetary and Space SciencesUniversity of CaliforniaLos Angeles California 90095–1567 USA;</p> <p>Istituto di Astrofisica e Planetologia SpazialiIstituto Nazionale di Astrofisica00133 Rome Italy;</p> <p>Italian Space Agency (ASI)00133 Rome Italy;</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/0704023664696.html">Ambient and cold‐temperature infrared spectra and XRD patterns of ammoniated phyllosilicates and carbonaceous chondrite meteorites relevant to Ceres and other solar system bodies</a> <b>[J]</b> . <span> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Ehlmann Bethany L.&option=202" target="_blank" rel="nofollow" class="tuijian_auth tuijian_authcolor">Ehlmann Bethany L.,</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Hodyss Robert&option=202" target="_blank" rel="nofollow" class="tuijian_auth tuijian_authcolor">Hodyss Robert,</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Bristow Thomas F.&option=202" target="_blank" rel="nofollow" class="tuijian_auth tuijian_authcolor">Bristow Thomas F.,</a> <a href="/journal-foreign-24922/" target="_blank" rel="nofollow" class="tuijian_authcolor">Meteoritics & planetary science .</a> <span>2018</span><span>,第9期</span> </span> </div> <p class="zwjiyix translation" style="max-width: initial;height: auto;word-break: break-all;white-space: initial;text-overflow: initial;overflow: initial;"> <span>机译：环境和冷温红外光谱和氨化的神经硅酸盐和碳质浮石陨石与CER和其他太阳系体有关</span> </p> </li> <li> <div> <b>2. </b><a class="enjiyixqcontent" href="/journal-foreign-detail/0704024739840.html">Infrared Spectroscopy of Carbonaceous-chondrite Inclusions in the Kapoeta Meteorite: Discovery of Nanodiamonds with New Spectral Features and Astrophysical Implications</a> <b>[J]</b> . <span> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Yassir A. 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