Chemical Analysis of Iron Meteorites Using a Hand‐Held X‐Ray Fluorescence Spectrometer          下载免费PDF全文

Maurizio Gemelli  Massimo D'Orazio  Luigi Folco 《Geostandards and Geoanalytical Research》2015,39(1):55-69

We evaluate the performance of a hand‐held XRF (HHXRF) spectrometer for the bulk analysis of iron meteorites. Analytical precision and accuracy were tested on metal alloy certified reference materials and iron meteorites of known chemical composition. With minimal sample preparation (i.e., flat or roughly polished surfaces) HHXRF allowed the precise and accurate determination of most elements heavier than Mg, with concentrations > 0.01% m/m in metal alloy CRMs, and of major elements Fe and Ni and minor elements Co, P and S (generally ranging from 0.1 to 1% m/m) in iron meteorites. In addition, multiple HHXRF spot analyses could be used to determine the bulk chemical composition of iron meteorites, which are often characterised by sulfide and phosphide accessory minerals. In particular, it was possible to estimate the P and S bulk contents, which are of critical importance for the petrogenesis and evolution of Fe‐Ni‐rich liquids and iron meteorites. This study thus validates HHXRF as a valuable tool for use in meteoritics, allowing the rapid, non‐destructive (a) identification of the extraterrestrial origin of metallic objects (i.e., archaeological artefacts); (b) preliminary chemical classification of iron meteorites; (c) identification of mislabelled/unlabelled specimens in museums and private collections and (d) bulk analysis of iron meteorites.  相似文献   

西页1井龙潭组海陆过渡相页岩含气性分析   总被引：2，自引：0，他引：2  

王中鹏  张金川  孙睿  刘昌为  杜晓瑞  卢亚亚 《地学前缘》2015,22(2):243-250

目前,国内外在海陆过渡相页岩含气性方面的相关研究较少。位于贵州省毕节地区黔西县境内的页岩气参数调查井西页1井揭示了黔西北地区上二叠统龙潭组海陆过渡相黑色碳质页岩发育特征及其含气性特点。通过有机地球化学实验,获取了西页1井的有机地化参数:TOC含量分布范围为0.4%~17.85%,平均值为4.25%;Ro分布范围为2.68%~3.48%,平均值为3.06%。钻、录、测井资料分析显示该井钻遇上二叠统龙潭组富有机质页岩层系厚度为148.85m,在钻进过程中,共有6层出现气显示。利用测井资料、现场解吸和等温吸附实验数据分析和计算,认为龙潭组海陆过渡相页岩含气页岩层段多,具有良好的吸附能力,得到总含气量为1.40~19.60m3/t。通过以上结果分析表明:西页1井所揭示的上二叠统海陆过渡相龙潭组含气页岩具有层段数量多、单层厚度小、有机质分段富集、热演化成熟度偏高等特点,且含气性较好,故该区海陆过渡相龙潭组地层具有较大的页岩气资源潜力。  相似文献   

越南西北部Phan Si Pan地区Ngoi Chi岩组的锆石U-Pb年龄和Hf同位素组成     

HIEU Pham Trung 《地球学报》2015,36(6):755-760

本文对越南西北部Phan Si Pan地区变质地体中的一个Ngoi Chi片麻岩进行了锆石CL内部结构分析、LA-(MC)-ICP-MS锆石U-Pb定年和Hf同位素分析。CL图象和Th/U比值特征显示该片麻岩样品中的锆石主要为岩浆锆石,有少量窄的变质边。岩浆锆石的年龄为~2.9 Ga,表明该样品是越南西北部Phan Si Pan地区的基底岩石。它们的εHf(t)值为–4.70±0.92,二阶段Hf模式年龄为~3.5 Ga,表明其为更古老的(3.5 Ga)冥太古代地壳物质部分熔融作用形成。变质边部锆石给出了~1.8 Ga的年龄,表明变质作用发生在古元古代早期,Phan Si Pan地区在这一时期可能经历了一次重要的构造热事件。  相似文献   

页岩油资源定量评价中关键参数的选取与校正——以松辽盆地北部青山口组为例   总被引：1，自引：0，他引：1  

薛海涛  田善思  卢双舫  张文华  杜添添  穆国栋 《矿物岩石地球化学通报》2015,34(1)

页岩油资源评价过程中,常用热解参数(S1)反映含油性。由于实验关系,所测得的S1存在轻烃、重烃的损失,为更准确的对页岩油资源进行定量评价,本文通过有机质成烃动力学研究以及对样品抽提前后的热解参数进行对比,对S1进行轻、重烃补偿校正,获得泥页岩总含油率参数,根据泥页岩排烃门限确定其可动油含量参数(S1/TOC)。研究结果表明,松辽盆地北部青山口组泥页岩S1校正前后相差2~3倍,排烃门限对应的S1/TOC=75mg/g TOC,结合黏土矿物含量(表征可压裂性),优选出页岩油勘探开发有利区:青一段有利区主要集中在齐家古龙凹陷中北部及龙虎泡大安阶地中部,青二、三段集中在龙虎泡大安阶地中部与齐家古龙凹陷中南部。  相似文献   

花岗岩的成岩时代、地球化学特征和成因青海祁漫塔格地区虎头崖矿床Ⅵ矿带     

姚磊  吕志成  于晓飞  庞振山  蔡煜琦  刘鹏  刘长城  王凤兰 《吉林大学学报(地球科学版)》2015,(3)

利用 LA ICP MS 锆石 U Pb 法,测得与成矿有关的青海祁漫塔格地区虎头崖矿床Ⅵ矿带花岗岩的成岩年龄为(233.6±1.8)Ma(MSWD=1.2,n=17)。地球化学特征显示：花岗岩属高钾钙碱性、弱过铝质花岗岩;样品的稀土元素组成以总体右倾,轻、重稀土分异明显和具明显的负铕异常为特征;微量元素具有富集 Rb、Th、U、La、Nd 等大离子亲石元素,亏损 Ba、Sr、Nb、P、Ti 等元素的特点。Sr Nd 同位素组成特征显示,花岗岩的源区可能是富集岩石圈地幔。初步研究认为,虎头崖矿床Ⅵ矿带花岗岩可能形成于中、晚三叠世碰撞后碰撞的构造背景下。  相似文献   

花岗岩的成岩时代、地球化学特征和成因青海祁漫塔格地区虎头崖矿床Ⅵ矿带     

姚磊  吕志成  于晓飞  庞振山  蔡煜琦  刘鹏  刘长城  王凤兰 《吉林大学学报(地球科学版)》2015,(3):743-758

利用 LA ICP MS 锆石 U Pb 法,测得与成矿有关的青海祁漫塔格地区虎头崖矿床Ⅵ矿带花岗岩的成岩年龄为(233.6±1.8)Ma(MSWD=1.2,n=17)。地球化学特征显示：花岗岩属高钾钙碱性、弱过铝质花岗岩;样品的稀土元素组成以总体右倾,轻、重稀土分异明显和具明显的负铕异常为特征;微量元素具有富集 Rb、Th、U、La、Nd 等大离子亲石元素,亏损 Ba、Sr、Nb、P、Ti 等元素的特点。Sr Nd 同位素组成特征显示,花岗岩的源区可能是富集岩石圈地幔。初步研究认为,虎头崖矿床Ⅵ矿带花岗岩可能形成于中、晚三叠世碰撞后碰撞的构造背景下。  相似文献   

Correlation of main physicochemical parameters of some groundwater in northern Serbia     

Sanja Mrazovac  Mirjana Vojinović-Miloradov 《Journal of Geochemical Exploration》2011

The geothermal waters of the first and the shallowest groundwater system of the Province of Vojvodina in northern Serbia, south part of the Pannonian Basin, are characterized by elevated temperatures (between 25 and 85 °C) and elevated gas content (above 1 Nm³/m³) with a high methane content (average about 94% of total gases). These methane-containing waters are particularly abundant in the Central part of the province between Danube and Tisa rivers. Dominant ions in these waters are sodium and bicarbonate, but the waters also contain significant amounts of calcium, magnesium, potassium, chloride, and ammonium. Components that are of balneological significance include iodine, bromine, fluorine, strontium, lithium, barium, and metasilicic and metaboric acids. Based on statistical analysis, a strong positive correlation is generally observed in about 9.2% cases. A slightly lower correlation appears in about 42.2%, and negative correlation coefficient appears in about 48.6% cases. The dendrogram of the cluster analysis built on the wells shows three main groups. There is the cluster of (Na⁺)_aq, (Cl⁻)_aq and (HCO₃⁻)_aq. The second aggregation is (NH₄⁺)_aq/(NH₃)_aq. The third group includes (Mg²⁺)_aq, (Ca²⁺)_aq, (Fe³⁺)_aq, (Sr²⁺)_aq, (Pb²⁺)_aq, and (Zn²⁺)_aq.  相似文献   

巴丹吉林沙漠高大沙山粒度组成及其意义     

赵景波  张冲  董治宝  邵天杰  李恩菊 《地质学报》2011,85(8):1389-1398

选取巴丹吉林沙漠东南部全球高差最大(约420m)的诺尔图湖东大沙山和较高的苏木巴润吉林湖西大沙山(高差约400m),对其迎风坡沉积物进行系统采样分析,讨论了高大沙山迎风坡沉积物粒度成分特点、变化规律、原因及其活动性.结果表明,全球高差最大的诺尔图东沙山和苏木巴润吉林湖西沙山迎风坡沉积物具有双层结构,表层沉积物的粒度组成...  相似文献   

The Rumuruti chondrite group     

Addi Bischoff  Nadia Vogel  Julia Roszjar 《Chemie der Erde / Geochemistry》2011,(2):101-133

Since 1994, the Rumuruti (R) chondrites have been recognized as a new, well-established chondrite group differing from carbonaceous, ordinary, and enstatite chondrites. The first R chondrite, Carlisle Lakes, was found in Australia in 1977. Meanwhile, the number has increased to 107 (December, 2010). This group is named after the Rumuruti meteorite, the first and so far the only R chondrite fall. Most of the R chondrites are breccias containing a variety of different clasts embedded in a clastic matrix. Some textural and mineralogical characteristics can be summarized as follows: (a) the chondrule abundance in large fragments and in unbrecciated rocks is ∼35–50 vol%; (b) Ca,Al-rich inclusions are rare; (c) the olivine abundance is typically 65–78 vol%; (d) the mean chondrule diameter is ∼400 μm; (e) in unequilibrated R chondrites, low-Ca pyroxene is dominating, whereas in equilibrated R chondrites it is Ca-rich pyroxene; (f) the typical olivine in a metamorphosed lithology is ∼Fa_38–40; (g) matrix olivine in unequilibrated, type 3 fragments and rocks has much higher Fa (∼45–60 mol%) compared to matrix olivines in type 4–6 lithologies (∼Fa_38–41); (h) spinels have a high TiO₂ of ∼5 wt%; (i) abundant different noble metal-bearing phases (metals, sulfides, tellurides, arsenides) occur. The exception is the metamorphosed, type 5/6 R chondrite La Paz Icefield 04840 which contains hornblende, phlogopite, and Ca-poor pyroxene, the latter phase typically occurring in low-grade metamorphosed R chondrites only.In bulk composition, R chondrites have some affinity to ordinary chondrites: (a) the absence of significant depletions in Mn and Na in R chondrites and ordinary chondrites is an important feature to distinguish these groups from carbonaceous chondrites; (b) total Fe (∼24 wt%) of R chondrites is between those of H and L chondrites (27.1 and 21.6 wt%, respectively); (c) the average CI/Mg-normalized lithophile element abundances are ∼0.95 × CI, which is lower than those for carbonaceous chondrites (≥1.0 × CI) and slightly higher than those for ordinary chondrites (∼0.9 × CI); (d) trace element concentrations such as Zn (∼150 ppm) and Se (∼15 ppm) are much higher than in ordinary chondrites; (e) the whole rock Δ¹⁷O of ∼2.7 for R chondrites is the highest among all meteorite groups, and the mean oxygen isotope composition is δ¹⁷O = 5.36 ± 0.43, δ¹⁸O = 5.07 ± 0.86, Δ¹⁷O = +2.72 ± 0.31; (f) noble gas cosmic ray exposure ages of R chondrites range between ∼0.1 and ∼70 Ma. More than half of the R chondrites analyzed for noble gases contain implanted solar wind and, thus, are regolith breccias. The 43 R chondrites from Northern Africa analyzed so far for noble gases seem to represent at least 16 falls. Although the data base is still scarce, the data hint at a major collision event on the R chondrite parent body between 15 and 25 Ma ago.  相似文献   

拉萨市夏季大气降尘单颗粒矿物组成及其形貌特征   总被引：3，自引：0，他引：3       下载免费PDF全文

张学磊  邬光剑  岳雅慧  张成龙 《岩石矿物学杂志》2011,30(1):127-134

应用带能谱的电子扫描电镜(SEM-EDX)对拉萨市夏季正常天气下收集的大气自然沉降气溶胶样品进行分析,研究了拉萨市大气降尘矿物组成和各种物相形貌特征信息。拉萨市大气颗粒物含有硅酸盐颗粒、富钙颗粒、富铁颗粒、富碳颗粒(燃煤飞灰颗粒和燃油飞灰颗粒)和植物残体颗粒。根据颗粒物数量统计发现拉萨市大气颗粒物以硅酸盐颗粒为主,富钙颗粒和富铁颗粒次之,需要指出的是以燃油飞灰为主的富碳颗粒已占到一定比重,说明以燃油为主的机动车尾气对拉萨大气污染在加强。研究结果表明,大气降尘矿物成分及其形貌特征可以用作判定污染物来源的重要标志,拉萨大气中颗粒来源的多样性决定了治理措施也应综合进行。  相似文献