Cation distribution in orthopyroxenes from S?o Jo?o Nepomuceno iron meteorite inferred from        <sup xmlns='http://www.wiley.com/namespaces/wiley'>5757        Fe M?ssbauer spectroscopy: Implications for thermal history and origin of IVA parent body

Dos Santos Edivaldo; Scorzelli Rosa B.; Varela Maria E.

摘要

Abstract > S?o Jo?o Nepomuceno (SJN) is an IVA iron meteorite, found in Minas Gerais state (Brazil) in 1960, that consists of Fe‐Ni metal matrix and coarse‐grained silicate inclusions. In spite of the extensive work performed on the IVA irons, there is still no consensus about their origin and thermal history. Their particular chemistry and range in metallographic cooling rates are difficult to explain using conventional models. Furthermore, metal–silicate mixing of the IVA group remains a complex issue. In this work, the 57 Fe M?ssbauer spectroscopy was applied for measuring the intracrystalline Fe‐Mg distribution in orthopyroxenes extracted from SJN. The M?ssbauer data associated with Ganguly's cooling rate numerical model were used to investigate the thermal history of SJN meteorite. The results are the background for discussions about the IVA formation models, aiming to improve the understanding of the origin of IVA iron meteorite group. </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 =“maps13121-abs-0001”XML：lang =“en”> <标题类型=“main”>抽象</ title> > s？o jo？o nepomuceno（sjn）是1960年在Minas Gerais国家（巴西）的IVA铁陨石，由Fe-Ni金属基质和粗粒硅酸盐夹杂物组成。尽管对IVA IRONS进行了广泛的工作，但仍然没有关于他们的起源和热历史的共识。它们的特定化学和金相冷却速率的范围难以使用常规模型来解释。此外，IVA组的金属硅酸盐混合仍然是复杂的问题。在这项工作中， 57 </ sup> 施用Fe m？Ssbauer光谱法测量从SJN提取的矫形器中的脑内Fe-Mg分布。与Ganguly的冷却速率数值模型相关的M？SSBauer数据探讨SJN陨石的热历史。结果是关于讨论IVA形成模型的背景，旨在改善对IVA铁陨石群的起源的理解。 </ 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10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=Dos Santos Edivaldo&option=202" target="_blank" rel="nofollow">Dos Santos Edivaldo;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Scorzelli Rosa B.&option=202" target="_blank" rel="nofollow">Scorzelli Rosa B.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Varela Maria E.&option=202" target="_blank" rel="nofollow">Varela Maria E.;</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>Instituto de Ciência e Tecnologia—ICT/UFVJMRodovia MGT 367—km 583 n° 5000 39100‐000 Minas Gerais Brazil;</p> <p>Centro Brasileiro de Pesquisas Físicas—CBPFRua Dr. Xavier Sigaud 150 22290‐180 Rio de Janeiro Brazil;</p> <p>Instituto de Ciencias Astronómicas de la Tierra y del Espacio—ICATE/CONICETAv Espa?a 1512 sur San Juan Argentina;</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/0704023664724.html">Cation distribution in orthopyroxenes from S?o Jo?o Nepomuceno iron meteorite inferred from <sup xmlns="http://www.wiley.com/namespaces/wiley">5757 Fe M?ssbauer spectroscopy: Implications for thermal history and origin of IVA parent body</a> <b>[J]</b> . <span> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Dos Santos Edivaldo&option=202" target="_blank" rel="nofollow" class="tuijian_auth tuijian_authcolor">Dos Santos Edivaldo,</a> <a 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Cation distribution in orthopyroxenes from S?o Jo?o Nepomuceno iron meteorite inferred from 5757 Fe M?ssbauer spectroscopy: Implications for thermal history and origin of IVA parent body

摘要

Cation distribution in orthopyroxenes from S?o Jo?o Nepomuceno iron meteorite inferred from ^{5757 Fe M?ssbauer spectroscopy: Implications for thermal history and origin of IVA parent body}