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1.
新疆巴里坤膨润土的红外光谱分析   总被引：3，自引：2，他引：1  
对巴里坤膨润土不同颜色的典型样品进行红外光谱测试分析,结果表明:巴里坤膨润土矿Ⅱ的膨润土的强吸收波谱出现在3627 cm-1(高频区)、1040 cm-1(中频区)、531 cm-1、470 cm-1(低频区)附近;5个代表样品的红外光谱曲线轮廓基本上一致,但仍存在一定的差异,不同颜色的膨润土因其化学成分的差异,在红外光谱曲线上有所不同,在3600 cm-1(高频区)附近,1#样品对红外光谱的吸收率较强,归属于Al—O—H的伸缩振动,说明1#样品蒙脱石的含量要高些;在797.64 cm-1(中频区)附近,1#、5#样品对红外光谱的吸收率要弱些,归属于Si—O—Si的反对称伸缩振动,说明SiO2的含量较低。  相似文献   

2.
不同亚类硅酸盐矿物的中红外光谱学特征   总被引：1，自引：0，他引：1  
利用热红外发射光谱研究了不同亚类硅酸盐矿物镁橄榄石、透闪石、蛇纹石和钠长石的红外发射光谱特征。在120oC时,通过对400～1650 cm-1的红外波段进行积分计算,发现硅酸盐矿物中镁橄榄石的发射率最高,可达到0.988,钠长石最低为0.947。硅酸盐矿物在850～1300cm-1区间均产生宽的低发射带,该发射带与硅氧四面体层中(Si,Al)-O的伸缩振动相关;在470 cm-1左右则形成相对尖锐的低发射带,与硅氧四面体层中(Si, Al)-O的弯曲振动相关。从岛状、链状、层状到架状硅酸盐矿物由于Si O2聚合程度依次增加,最强发射谷的位置依次向高频方向偏移,说明硅氧四面体中Si-O伸缩振动带的位置受到了n(Si)/n(O)比值的制约。此外,在辐射能量谱里,镁橄榄石、透闪石、蛇纹石和钠长石的最强辐射谷范围趋于变宽,依次为115、162、225和247 cm-1,反映了吸收的辐射能增加。综上可推测,硅酸盐矿物强的发射率可能与硅氧四面体中Si-O的振动模式、Si O2的聚合度、辐射能量谱中最强辐射谷的波长范围有关。  相似文献   

3.
马鞍山绿松石中水的振动光谱表征及其意义   总被引：8，自引：0，他引：8  
在室温和变温条件下对安徽马鞍山绿松石中水的结构特征进行红外吸收光谱和激光拉曼光谱分析研究,结果表明:绿松石中部分水分子与Cu2 结合成[Cu(H2O)4]2 水合离子,并在很大程度上制约了绿松石的颜色;马鞍山地区绿松石中结晶水的脱失温度约为303℃～310℃,结构水的脱失温度约为346℃～375℃。绿松石中H2O,OH-的振动是导致其水的激光拉曼光谱形成的主要原因,ν(OH)振动导致的强拉曼特征谱峰在3470 cm-1,3502 cm-1～3505 cm-1之间的弱谱峰则隶属3470 cm-1的次级谱峰,ν(H2O)的拉曼谱峰主峰位于3442 cm-1～3449 cm-1处。由ν(MFe,Cu-H2O)伸缩振动致平缓的拉曼谱峰主要分布在3074 cm-1～3303 cm-1附近。  相似文献   

4.
内蒙古嘎仙矿床为大兴安岭北段与岩浆作用有关的大型低品位镍钴硫化物矿床,成矿作用主要与花岗质岩浆作用有关。文章主要对矿区内矿体下盘的花岗岩类(花岗斑岩、长石斑岩、伟晶状花岗岩、黑云母花岗岩)进行了锆石LA-ICP-MS U-Pb定年,获得花岗斑岩的谐和线年龄(125.3±1.1)Ma～(127.5±4.5)Ma,长石斑岩的谐和线年龄为(128.1±2.2)Ma,伟晶状花岗岩的谐和线年龄为(127.9±2.3)Ma,黑云母花岗岩的谐和线年龄为(127.9±1.4)Ma,说明这些花岗岩类主要形成于中生代早白垩世。通过对矿化超镁铁岩、科马提岩、镁铁岩(辉绿岩、玄武岩)、长英质岩(闪长岩、长石斑岩、斜长花岗岩、花岗斑岩、伟晶状花岗岩、黑云母花岗岩)及围岩(大理岩)的主量、微量元素地球化学测试分析,结果表明,与吉峰科马提岩成分相比较,矿化超镁铁岩具有较高的w(SiO_2)(40.53%～54.96%)、w(TiO_2)(0.24%～0.86%)、w(Al_2O_3)(3.58%～10.47%)、w(FeO)(5.30%～8.80%)、w(CaO)(7.35%～13.66%)、w(Na_2O)(0.01%～0.76%)、w(K_2O)(0.02%～0.66%)和w(P_2O_5)(0.06%～0.61%);镁铁岩(包括辉绿辉长岩、玄武岩)铝含量较高,w(Al_2O_3)=16.34%～17.74%;长英质岩类也富铝质(Al_2O_3/(CaO+Na_2O+K_2O)=1.34～1.63),多数岩石属于钙碱性系列。闪长岩与镁铁岩相比,具有较高的硅、铝、钾、钠,较低的铁、镁和钙,微量元素具有大离子亲石元素富集,高场强元素相对亏损的右倾模式;稀土元素具有轻稀土元素富集,重稀土元素相对亏损特征,超镁铁岩类成分点位于N-MORB与OIB范围之间,而镁铁岩和长英质岩类成分点位于E-MORB和OIB之间。镁铁岩落入火山弧玄武岩范围,长英质岩落入火山弧花岗岩+同碰撞花岗岩范围,同属于造山后花岗岩的范围,因此镁铁质岩的形成应属于俯冲-碰撞环境,而长英质岩的形成应属于造山后伸展环境。根据各岩类所含成矿元素和亲流体元素分析,认为含矿热液来自矿区西部的深部,并且构建了嘎仙矿床的成矿模型,即超镁铁岩先期侵位,后期经历了区域的变质变形,最后发生燕山期大规模花岗质岩浆活动及成矿流体的蚀变矿化。  相似文献   

5.
通过固相法合成了一系列氯羟磷灰石(ClHAp)固溶体,经FTIR表征发现,纯羟基磷灰石(HAp)的羟基振动频率为3572cm-1和632cm-1。当Cl-进入HAp晶体结构后,在3494cm-1和673cm-1处各出现新的吸收谱带,说明在其通道结构中形成[Cl…HO]氢键,导致羟基的伸缩振动向低频偏移,弯曲振动向高频偏移。与氟羟磷灰石的FTIR谱比较可知:ClHAp的羟基振动谱带的位置与数量主要受氢键和周围结构环境变化程度影响。  相似文献   

6.
磷氯铅矿(Pyromorphite)在我国比较罕见,2001年在广西岛坪发现的磷氯铅矿结晶较好,运用XRD、XRFI、R和UV/Vis等分析方法对黄色和绿色样品进行了研究。结果表明,二者XRD谱只是峰强有所不同。在它们的红外吸收谱带中,除了标准的PO43-吸收峰外,在670~800 cm-1之间和430 cm-1左右出现的两组肩峰为SiO44-振动峰。黄色样品的振动频率偏高、半峰宽偏窄、透射率与绿色样品相比较高。通过XRF分析发现黄色晶体比绿色晶体含有更多的Fe3 ,而Fe3 常使矿物呈现黄色,同时证实了黄色磷氯铅矿的红外吸收峰频率偏高是因为它的铅含量低于绿色矿。UV/Vis进一步说明在可见光区的吸收不同是使二者颜色差异的主要原因,Fe离子含量较大使磷氯铅矿呈现黄色。  相似文献   

7.
富镁和贫镁坡缕石及其酸浸蚀产物的红外吸收光谱研究   总被引：9，自引：1，他引：8  
本文对两个富镁和贫镁坡缕石的红外吸收光谱高频区的拟合结果表明,富镁坡缕石(p0)和贫镁坡缕石(g0)的八面体离子的配置有区别,前者除出现Mg3OH振动外,MgM2口OH振动的比例比AlM2口OH振动的大,后者则反之。经酸短时间浸蚀的和未经浸蚀的坡缕石红外吸收光谱相比,除部分吸收峰(如3560cm^-1)的峰形发生明显变化外,其余各吸收峰的峰形相似、强度稍有变化,且Siu-O-SiD的不对称振动吸收峰向低波数方向偏移、对称吸收峰向高波数方向偏移;坡缕石中790cm^-1左右的吸收峰的归属是不明确的,据实验确认它是由Siu-O-SiD的对称吸收所致;由985cm^-1、1030cm^-1、1080cm^-1和1200cm^-1左右4个吸收峰组成Si-O骨架振动吸收带的峰形、强度和峰位移反映了酸浸蚀过程中坡缕石的结构改变。两个坡缕石经360h盐酸浓度为1mol／L和3mol／L浸蚀后,所得产物的粉末X射线衍射谱虽仍具有坡缕石的衍射线,但它们的红外吸收光谱却只有与表面OH振动、物理吸附水相关的OH振动和几个SiO振动吸收峰,而无代表八面体振动、硅氧骨干中的大部分SiO振动和晶格中的结晶水的振动,说明酸对坡缕石浸蚀的最后产物是以硅氧为主。  相似文献   

8.
对特提斯喜马拉雅带中段中侏罗统遮拉组玄武岩进行了系统的岩石学、地球化学和同位素地球化学研究.结果表明:①遮拉组玄武岩以高钛[平均w(TiO2)=2.57%]、高铁[平均w(TFe2O3)=11.58%]、低镁[平均w(MgO)=4.06%]、富集LREE和高场强元素{[w(La)/w(Yb)]N、w(Nb)、w(Zr)平均分别为8.61,32.67×10-6,331.33×10-6}为特征,w(Ti)/w(V)(62.74～80.26)、w(Ti)/w(Y)(218.71～665.20)和w(Zr)/w(Y)(10.89～11.09)比值高,具有与OIB相似的主量元素和微量元素组成特征,同位素组成以高Sr{[n(87Sr)/n(86Sr)]i为0.712 763～0.714 765}、低Nd{[n(143Nd)/n(144Nd)]i为0.512 417～0.512 458}为特点;②遮拉组玄武岩为一套产于大陆边缘裂谷背景下的碱性玄武岩,没有经历地壳混染;③遮拉组玄武岩是地幔热柱或热点物质与岩石圈地幔物质相互作用的结果,对了解与雅鲁藏布江洋盆构造演化有关的一些关键地质问题可能具有重要意义.  相似文献   

9.
二叠纪是塔里木盆地热-构造演化史上最重要的时期,这一时期在塔里木盆地中部和西北部发生了大规模的基性-中酸性岩浆活动.对塔里木盆地西北部瓦吉里塔格超镁铁岩的地球化学反演表明:瓦吉里塔格超镁铁岩(包括角砾和胶结物)是由残余岩浆和橄榄石、单斜辉石不同比例混合的产物,其中角砾主要由橄榄石和残余岩浆组成,其比例达到了72∶28.与角砾中橄榄石(平均Fo=0.82)平衡的熔体的w(MgO)为9.06%、w(FeOt)为11.77%,是由w(MgO)为11.46%、w(FeOt)为12.12%的原始岩浆经7.3%的橄榄石(Fo=0.82)分异而成的.其原始岩浆并不属于高镁岩浆,而是地幔石榴子石橄榄岩低程度(<5%)部分熔融的产物,初始熔融温度约1 150～1 250 ℃,压力约2.2 GPa,深度约70 km.结合前人研究成果认为,塔里木盆地二叠纪岩浆活动的形成可能与软流圈上涌导致的软流圈-岩石圈的相互作用有关,目前尚没有直接的岩石地球化学证据表明有地幔柱活动的参与.  相似文献   

10.
吉林红旗岭镁铁-超镁铁质侵入岩群位于中亚造山带东段南缘,由3个北西向岩带(I、II、III)组成,包括30多个小岩株,其中I-岩带的部分岩体伴有铜镍矿化,并且其1和7号岩体分别形成了中型和大型岩浆铜镍硫化物型矿床。矿床主要容矿岩石为辉橄岩、橄辉岩、斜方辉石岩、二辉石岩、苏长岩和辉长岩。主量元素方面,红旗岭岩群具有富镁(w(MgO)=20.7%～31.1%)、低钛(w(TiO2)=0.33%～0.79%)、低碱(w(K2O+Na2O)=0.60%～2.29%)和硅(w(SiO2)=40.0%～53.0%)变化范围大的特征;微量元素方面,红旗岭岩群呈现弱富集LREE和LILE(Th)以及亏损HREE和HFSE(Nb-Ta-Ti)。岩相学、地球化学和矿物(橄榄石、斜方辉石、单斜辉石、尖晶石、斜长石和角闪石)主微量元素特征表明,红旗岭岩群明显不同于洋岛型玄武岩、阿拉斯加型环状杂岩和科马提岩,但与岛弧玄武岩以及中亚造山带西段的“黄山西”和“黄山东”铜镍硫化物矿床的容矿超镁铁质岩相似,其母岩浆是一种富Mg、亏损...  相似文献   

11.
This investigation deals with the Nigerian iron-formations and their host rocks and is based on about 560 mineral analyses (electron-microprobe) and 93 whole-rock analyses (64 iron-formations and 29 host rocks). The manganese-rich and Al-bearing iron-formations occurring in various schist belts of the northern and southern part of West-Nigeria consist of the magnetite-free silicate, the magnetite–silicate and the quartz-rich hematite facies.Iron-formations and host rocks originated from submarine-volcanogenic exhalations enriched in Fe, Mn and CO2 and from Al2O3, SiO2 and alkali (K2O and Na2O)-rich continental-derived pelitic to psammitic material. From these sources and their interaction and controlled by the volcanogenic activity, differently composed protoliths were deposited in the marine basin during the Birimian time. Subsequent metamorphism of greenschist to low amphibolite facies conditions during the Eburnian time led to the formation of the metaprotoliths of the magnetite–silicate (consisting of predominantly magnetite and quartz and subordinate of garnet and amphibole), the silicate facies (consisting of garnet, amphibole and rarely Mn-bearing ilmenite and quartz) and the metasediment phyllite. Garnets are predominantly almandine–spessartine solid solutions, whereas amphiboles are Mn and Ca-bearing grunerite–cummingtonite solid solutions. In the course of a second tectono-metamorphic event of Pan-African age, the magnetite–silicate facies iron-formation/phyllite association was transformed into the hematite facies and muscovite/biotite schists, whereas the silicate facies is characterized by extensive silicification features. The hematite facies and the silicified silicate facies are restricted to southern Nigeria where the second and heterogeneous tectono-metamorphic event is more pronounced (amphibolite facies conditions) than in northern Nigeria.The genesis, summarized as the metamorphic model, shows that the carbonate-rich (siderite, rhodochrosite and subordinate magnesite and calcite) protoliths were metamorphically transformed into the silicate and magnetite–silicate facies. The separation of Mn and Fe, leading to manganese-bearing iron-formations and iron-bearing manganese-formations was explained by varying pH-conditions, under which siderite (pH: 6.8–9.4) and rhodochrosite (pH: 9–11) precipitated.Similar to the Gunfit and Biwabik iron-formations of Minnesota, USA, the iron-formation of Bingi (Maru schist belt), now present in the form of the fayalite bearing silicate facies, was overprinted by contact metamorphism caused by a gabbro intrusion.  相似文献   

12.
Mass balance of incompatible elements was analyzed for different inferred reservoirs of the bulk silicate Earth. It was shown that the lower mantle, as well as the primitive mantle, includes an MORB-source depleted mantle component and material with a high content of incompatible elements. Contribution of the continental crust was found to be subordinate. The predominant part of the enriched mantle formed through differentiation of the mantle itself. Enriched material was supplied into the deep-seated zones of silicate shell through delamination of subcontinental lithospheric blocks affected by mantle metasomatism and their subsequent involvement in the mantle convective system. The osmium isotope composition of the plunged lithospheric material is modified in the lower mantle by the infiltration of sulfide melts.  相似文献   

13.
The Dhofar 280 lunar highland meteorite is the first one in which native silicon was identified in association with iron silicides. This association is surrounded by silicate material enriched in Si, Na, K, and S and occurs within an impact-melt matrix. Compared to the meteorite matrix, the objects with native Si and the silicate material around them show high Al-normalized concentrations of volatile elements and/or elements with low sensitivity to oxygen but are not any significantly enriched in refractory lithophile elements. Some lithophile elements (V, U, Sm, Eu, and Yb) seem to be contained in reduced forms, and this predetermines REE proportions atypical of lunar rocks and a very low Th/U ratio. The admixture of siderophile elements (Ni, Co, Ge, and Sb) suggests that the Si-bearing objects were contaminated with meteorite material and were produced by the impact reworking of lunar rocks. The high concentrations of volatile elements suggest that the genesis of these objects could be related to the condensation of silicate vapor generated during meteorite impacts. The reduction of silicon and other elements could take place in an impact vapor cloud, with the subsequent condensation of these elements together with volatile components. On the other hand, condensates of silicate vapor could be reduced by impact reworking of impact breccias. Impact-induced vaporization and condensation seem not to play any significant role in forming the composition of the lunar crust, but the contents of the products of such processes can be locally relatively high. The greatest amounts of silicate vapor were generated during significant impact events. For example, more than 70% of the total mass of lunar material evaporated in the course of impact events should have resulted from the collision of the Moon with a cosmic body that produced the Moon??s largest South Pole-Aitken basin.  相似文献   

14.
In this study, the compressive and tensile behavior of polymer treated sulfate contaminated CL soil was investigated. Based on the information in the literature, a field soil was contaminated with up to 4 % (40,000 ppm) of calcium sulfate in this study. In addition to characterizing the behavior of sulfate contaminated CL soil, the effect of treating the soil with a polymer solution was investigated and the performance was compared to 6 % lime treated soil. In treating the soil, acrylamide polymer solution (15 g of polymer dissolved in 85 g of water) content was varied up to 15 % (by dry soil weight). Addition of 4 % calcium sulfate to the soil decreased the compressive and tensile strengths of the compacted soils by 22 and 33 % respectively with the formation of calcium silicate sulfate [ternesite Ca5(SiO4)2SO4)], magnesium silicate sulfate (Mg5(SiO4)2SO4) and calcium-magnesium silicate (merwinite Ca3Mg(SiO4)2). With the polymer treatment the strength properties of sulfate contaminated CL soil was substantially improved. Polymer treated sulfate soils had higher compressive and tensile strengths and enhanced compressive stress–strain relationships compared to the lime treated soils. Also polymer treated soils gained strength more rapidly than lime treated soil. With 10 % of polymer solution treatment, the maximum unconfined compressive and splitting tensile strengths for 4 % of calcium sulfate soil were 625 kPa (91 psi) and 131 kPa (19 psi) respectively in 1 day of curing. Similar improvement in the compressive modulus was observed with polymer treated sulfate contaminated CL soil. The variation of the compacted compressive strength and tensile strength with calcium sulfate concentrations for the treated soils were quantified and the parameters were related to calcium sulfate content in the soil and polymer content. Compressive stress–strain relationships of the sulfate soil, with and without lime and polymer treatment, have been quantified using two nonlinear constitutive models. The constitutive model parameters were sensitive to the calcium sulfate content and the type of treatment.  相似文献   

15.
The Plainview. Texas, meteorite is a polymict-brecciated H-group chondrite composed of recrystallized light-colored portions embedded in a well-compacted, dense, somewhat recrystallized, dark-colored matrix. Both portions consist of equilibrated silicates (H5 classification), but a small number of silicate grains and unequilibrated lithic fragments not compatible with equilibrated ordinary H-group material are present in the dark-colored matrix. Lithic fragments include: (i) dark-colored, more or less altered, type II carbonaceous chondrites. (ii) unequilibrated ordinary chondrites and (iii) light-colored, unequilibrated and equilibrated fragments, some of which are compositionally similar to the host. Also present are fragment-like dark areas that are highly-shocked host material and not true lithic fragments (pseudo-fragments). Conclusions: Plainview represents a complex regolith breccia formed by repeated impact episodes. Recrystallized, light-colored portions represent surface or near-surface material of a small (asteroidal-sized) parent body. Impacts broke up this material to form fine-grained, dark material which enclosed light-colored protolith. Lithic fragments (i-iii) and some unequilibrated silicate grains and chondrules (apparently derived from unequilibrated chondrites) were embedded in the dark matrix during these repeated impacts. Xenolitlils of carbonaceous and unequilibrated ordinary chondrites are either residues of projectiles that impacted the Plainview parent body, or material from coexisting regoliths impact-splashed into Plainview regolith. Chondrules and silicate grains in the dark matrix which differ from H-group material are likely related to these xenoliths and their regoliths. Light-colored lithic fragments may represent shock-melted chondritic material, sometimes compositionally-modified, or new, achondritic meteoritic types. Unequilibrated and carbonaceous lithic fragments in the dark-colored host matrix indicate that equilibration of the host occurred before incorporation of the fragments and that compaction and lithification of the Plainview regolith to form a coherent meteorite must have occurred at temperatures below 300°C and/or on a short time scale.  相似文献   

16.
吴朱敏  吕擎峰  王生新 《岩土力学》2016,37(Z2):301-308
进行压汞试验和SEM-EDS试验研究复合改性前后水玻璃加固黄土,分析其孔隙分布特征、颗粒和孔隙形态以及胶结物形态和化学元素含量,探讨宏观力学特性与微观特征的联系。压汞测试结果表明,改性前后加固黄土具有相近的孔隙分布特征,入口孔径主要分布在0.06～8 ?m之间,大、中、小和微孔隙分界值分别为8、2、0.06 ?m,加固时生成的凝胶填充作用不显著。SEM-EDS测试结果表明,改性后黄土仍保持其粒状、架空、接触-胶结结构不变,但加入硅酸钾材料后黄土颗粒表面变得粗糙并吸附有絮状物,EDS数据显示K元素含量随着硅酸钾掺入量的增加而增大,且试样无侧限强度与K元素百分含量正相关。研究还表明,土的颗粒联结强度和结构形态特征是导致黄土宏观力学性质差异的本质原因,在复合改性水玻璃加固黄土时在保持黄土架空孔隙基本不变的前提下,生成的含K凝胶在改变颗粒表面形态的同时强化了骨架颗粒之间的连接强度,从而改善了土体的强度。  相似文献   

17.
The groundwater quality detoriation due to various geochemical processes like saline water intrusion, evaporation and interaction of groundwater with brines is a serious problem in coastal environments. Understanding the geochemical evolution is important for sustainable development of water resources. A detailed investigation was carried out to evaluate the geochemical processes regulating groundwater quality in Cuddalore district of Tamilnadu, India. The area is entirely underlined by sedimentary formations, which include sandstone, clay, alluvium, and small patches of laterite soils of tertiary and quaternary age. Groundwater samples were collected from the study area and analyzed for major ions. The electrical conductivity (EC) value ranged from 962 to 11,824 μS/cm, with a mean of 2802 μS/cm. The hydrogeochemical evolution of groundwater in the study area starts from Mg-HCO3 type to Na-Cl type indicating the cation exchange reaction along with seawater intrusion. The Br/Cl ratio indicates the evaporation source for the ion. The Na/Cl ratios indicate groundwater is probably controlled by water-rock interaction, most likely by derived from the weathering of calcium-magnesium silicates. The plot of (Ca+Mg) versus HCO3 suggests ions derived from sediment weathering. The plot of Na+K over Cl reflects silicate weathering along with precipitation. Gibbs plot indicates the dominant control of rock weathering. Factor analysis indicates dominance of salt water intrusion, cation-exchange and anthropogenic phenomenon in the study.  相似文献   

18.
The mineralogy and bulk compositions of the matrices of the CR chondrites MET 00426 and QUE 99177 have been studied using a combination of SEM, EPMA, and TEM techniques. The matrices of these two chondrites are texturally, chemically, and mineralogically similar and are characterized by significant FeO-enrichments with respect to other CR chondrite matrices, nearly flat refractory lithophile patterns, variable volatile element patterns, and a simple mineral assemblage dominated by amorphous silicate material and Fe,Ni sulfides. Fine-grained, crystalline silicate phases such as olivine and pyroxene appear to be extremely rare in the matrices of both meteorites. Instead, the mineralogy of matrices and fine-grained rims of both meteorites consists of abundant amorphous FeO-rich silicate material, containing nanoparticles of Fe,Ni sulfides (troilite, pyrrhotite, and pentlandite). Secondary alteration minerals that are characteristic of other CR chondrites (e.g., Renazzo and Al Rais), such as phyllosilicates, magnetite, and calcite are also rare. The texture and mineralogy of the matrices of MET 00426 and QUE 99177 share many features with matrices in the primitive carbonaceous chondrites ALH A77307 (CO3.0) and Acfer 094 (unique). These observations show that MET 00426 and QUE 99177 are very low petrologic type 3 chondrites that have escaped the effects of aqueous alteration, unlike other CR chondrites, which are typically classified as petrologic type 2. We suggest that these meteorites represent additional samples of highly primitive, but extremely rare carbonaceous chondrites of petrologic type 3.00, according to the classification scheme of Grossman and Brearley (2005). The highly pristine nature of MET 00426 and QUE 99177 provides important additional insights into the origins of fine-grained materials in carbonaceous chondrites. Based on our new observations, we infer that the amorphous silicate material and nanosulfide particles that dominate the matrices of these meteorites formed in the solar nebula by rapid condensation of material following high-temperature events, such as those that formed chondrules.  相似文献   

19.
In order to decipher information about the local coordination environments of Na in anhydrous silicates from 23Na nuclear magnetic resonance spectroscopy (NMR), we have collected 23Na magic angle spinning (MAS) NMR spectra on several sodium-bearing silicate and aluminosilicate crystals with known structures. These data, together with those from the literature, suggest that the 23Na isotropic chemical shift correlates well with both the Na coordination and the degree of polymerization (characterized by NBO/T) of the material. The presence of a dissimilar network modifier also affects the 23Na isotropic chemical shift. From these relations, we found that the average Na coordinations in sodium silicate and aluminosilicate liquids of a range of compositions at 1 bar are nearly constant at around 6–7. The average Na coordinations in glasses of similar compositions also vary little with Na content (degree of polymerization). However, limited data on ternary alkali silicate and aluminosilicate glasses seem to suggest that the introduction of another network-modifier, such as K or Cs, does cause variations in the average local Na coordination. Thus it appears that the average Na coordination environments in silicate glasses are more sensitive to the presence of other network-modifiers than to the variations in the topology of the silicate tetrahedral network. Further studies on silicate glasses containing mixed cations are necessary to confirm this conclusion.  相似文献   

20.
微生物对硅酸盐矿物风化作用研究进展   总被引：6，自引：1，他引：6  
微生物对硅酸盐矿物风化的影响研究取得了一系列重要进展。在贫营养环境中,微生物风化硅酸盐矿物获取营养物质,加速了硅酸盐矿物的风化;由于微生物的作用,矿物的风化会不遵循正常的矿物化学风化序列,表现出稳定矿物比不稳定矿物更易风化的特征。微生物风化硅酸盐矿物时会在硅酸盐矿物表面留下痕迹,即富集或转移相应的元素和矿物,而且还能改变硅酸盐矿物的化学组成和结构。微生物的上述行为受营养基质含量、有机酸、生物膜、胞外聚合物以及氧化还原作用的影响。  相似文献   

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