用电厂水淬渣合成铁堇青石的实验研究

铸石是一种人造岩石,是以玄武岩、辉绿岩或某些工业废渣为原料,经配料、熔化、浇铸成型、结晶、退火而成的一种新工业材料。     

玄武岩纤维原料特征的统计及分析研究

玄武岩纤维是以玄武岩或他种成分相近的岩石为主要原料,经熔融后拉制而成的一种高性能纤维。天然矿石的成分波动会造成拉丝困难或纤维性能不稳定,本文收集了54组原料岩石以及114组玄武岩纤维样品的化学成分数据,研究归纳了玄武岩纤维所需原料的岩石学特征、参数指标特征和其他特征,分析提出了可拉丝岩石相关参数指标的最佳区间。适于生产玄武岩纤维的原料矿石,其特征可总结如下：岩石学方面,以基性岩以及SiO2含量为53%~57%的中性岩为佳,岩石类型最佳为玄武岩或安山玄武岩;岩石结构最佳为间隐结构、玻基斑状结构或玻璃质结构;构造的影响是间接的,主要为气孔或杏仁构造中可能含有的一些不利矿物的影响;矿物组成方面,蛇纹石、沸石等含水矿物会在熔融过程中产生气泡,影响纤维制备连续性的同时也有利于原料的充分熔融,镁橄榄石、磁铁矿等高熔点矿物会使原料在熔融阶段难以完全熔化,导致熔体不均匀并容易析晶。参数指标方面,可拉丝岩石的酸度系数（Mk）最佳区间为4.0~5.5;黏度系数（Mv）为2.0~3.0;硅铝氧化物与其他氧化物比值为1.5~3.0;氧化物组成的物质的量分数分布为n(RO)=20%~30%,n(RO2)=57%~70%,n(R2O3)=10%~16%（R为阳离子）。     

玄武岩纤维原料特征的统计及分析研究

玄武岩纤维是以玄武岩或他种成分相近的岩石为主要原料,经熔融后拉制而成的一种高性能纤维。天然矿石的成分波动会造成拉丝困难或纤维性能不稳定,笔者等收集了54组原料岩石以及114组玄武岩纤维样品的化学成分数据,研究归纳了玄武岩纤维所需原料的岩石学特征、参数指标特征和其他特征,分析提出了可拉丝岩石相关参数指标的最佳区间。适于生产玄武岩纤维的原料矿石,其特征可总结如下：岩石学方面,以基性岩以及SiO2含量为53%~57%的中性岩为佳,岩石类型最佳为玄武岩或安山玄武岩;岩石结构最佳为间隐结构、玻基斑状结构或玻璃质结构;构造的影响是间接的,主要为气孔或杏仁构造中可能含有的一些不利矿物的影响;矿物组成方面,蛇纹石、沸石等含水矿物会在熔融过程中产生气泡,影响纤维制备连续性的同时也有利于原料的充分熔融,镁橄榄石、磁铁矿等高熔点矿物会使原料在熔融阶段难以完全熔化,导致熔体不均匀并容易析晶。参数指标方面,可拉丝岩石的酸度系数（Mk）最佳区间为4. 0~5. 5;黏度系数（Mv）为2. 0~3. 0;硅铝氧化物与其他氧化物比值为1. 5~3. 0;氧化物组成的物质的量分数分布为n(RO)=20%~30%,n(RO2)=57%~70%,n(R2O3)=10%~16%（R为阳离子）。     

汉诺坝玄武岩中熔体-捕虏体相互作用初步研究

汉诺坝新生代玄武岩捕获的地幔橄榄岩及其解体矿物橄榄石、单斜辉石、斜方辉石捕虏晶,普遍发育反应边结构,提供了玄武岩浆在上升穿越岩石圈地幔过程中橄榄岩-熔体相互作用的重要信息。橄榄石和单斜辉石捕虏晶反应边的成分变化一致,由核部富镁向边部富铁变化,趋同于玄武岩中相应斑晶的成分。斜方辉石捕虏晶反应边一般由橄榄石+单斜辉石+玻璃构成,多为双层结构,反应边矿物橄榄石、单斜辉石较相应的地幔矿物富铁,其富硅、碱的中酸性玻璃成分,为中国东部地幔矿物包裹体中存在的富硅、碱熔体的来源提供了重要信息。同时发现橄榄岩捕虏体中尖晶石颜色、成分的变化与温度的关系。地幔矿物捕虏晶反应边结构(非平衡结构)得以保存,暗示了玄武岩浆的快速上升。而大规模的熔体-捕虏体相互作用,改变着岩石圈地幔的性质。     

浙江嵊县—新昌盆地新生代玄武岩中橄榄石、辉石、斜长石矿物化学及演化的研究

浙江嵊县—新昌盆地新生代玄武岩为橄榄拉斑玄武岩—碱性橄榄玄武岩—碧玄岩组合。根据124个矿物电子探针分析资料研究了橄榄石、单斜辉石和斜长石的种属、成分相关性及演化。根据矿物组合、单斜辉石化学成分和演化趋势以及岩石化学特征,认为本区玄武岩属于碱性玄武岩系列。     

月球冷海玄武岩矿物成分研究

月海玄武岩的矿物组成反映了岩浆源区的化学成分以及岩石形成时的物理和化学环境,对月球热演化研究以及月球资源的开发利用都具有重要意义。本文选择延展范围长的冷海为研究区,基于月球矿物成像光谱仪(Moon Mineralogy Mapper,简称M3)数据研究其矿物的空间变化特征。综合利用光谱、地形、元素等多源遥感数据将冷海划分为25个地质单元。提取169条新鲜坑光谱曲线,获取吸收中心波长、波段面积比等光谱参数。通过光谱吸收特征分析,获得冷海玄武岩铁镁质矿物变化特征。东部冷海地层较老,铁镁质矿物主要为单斜辉石,辉石钙含量较月球样品单斜辉石钙偏低,与澄海以及雨海老的地层矿物组成类似。西部冷海和露湾的地质单元较为年轻,富含橄榄石。风暴洋和雨海年轻玄武岩的矿物也富含橄榄石。这种富含橄榄石、大面积分布的玄武岩反映了月球晚期热演化的独特性。尽管地理上冷海为一个独立的月海,其东西部玄武岩矿物组成的差异以及与其同位置周围月海矿物组成的类似性反映了冷海玄武岩源区与周围月海具有联系。     

内蒙锡盟新生代玄武岩的岩石学研究

依照地层顺序和火山机构的完好程度,内蒙锡盟新生代玄武岩可粗略划分为三期。各期玄武岩又可分出若干层(次)。玄武岩由含量不等的橄榄石、单斜辉石和斜长石斑晶及基质组成。部分玄武岩含有二辉橄榄岩等深源包体。斑晶矿物均具有成分环带。矿物化学、岩石化学资料揭示出本区玄武岩从原生岩浆到进化岩浆的主要演化机制是以橄榄石为主的分离结晶作用,同时在部分进化岩浆中还存在岩浆混合作用。稀土元素资料还指出了一个形成本区原生岩浆以及派生岩浆的原生母岩浆的重要机制:上地幔渐进的部分熔融作用。     

贝加尔裂谷带通京盆地呼兰霍博克火山的玄武岩岩石学和地球化学特征

位于贝加尔裂谷带西南端通京盆地的呼兰霍博克火山为玄武岩质碎屑锥,玄武岩由高拉长石、贵橄榄石、普通辉石和火山玻璃组成,其矿物组成及SiO2-（Na2O＋K2O）图和Hf-Th-Ta图指示为碱性玄武岩.CIPW标准矿物特征、岩石化学成分和单斜辉石化学成分特征表明岩石属碱性系列,钠质型.稀土元素和微量元素的地球化学特征表明岩石为裂谷初期玄武岩.初步推断原始岩浆来源于上地幔,斑晶可能于16.5 km深处的次生壳层岩浆房结晶.     

深源包体中的含水高压矿物组合

河北汉诺坝碱性玄武岩中的尖晶石二辉橄榄岩包体是一种粗粒结构的岩石。在其主要造岩矿物——橄榄石和二辉石矿物的颗粒之间,发现一种呈板状或填隙状的褐色含水细粒矿物集合体。这种集合体主要由含水镁硅酸盐和橄榄石的高压相——林伍德石(Ringwoodite)组成,其次分散着细粒的金红石和少量尖晶石等,组成了一种极为少见的含水高压矿物组合。     

黑龙江鸡西盆地新生代玄武岩大地构造环境探讨

鸡西盆地新生代玄武岩的岩石学、岩石化学和地球化学研究表明,岩石中发育橄榄石包裹体,且造岩矿物中也多含橄榄石晶体;δEu=0.87~0.94（大于0.7）,具基性岩浆分异特征.微量元素Nb^*值为0.91（接近1）、K^*值为1.09,略大于1,表明岩浆与消减作用相关不大,且有非地壳物质加入.总体分析,岩浆来源于上地幔,上升过程中遭受了壳源物质的混染.鸡西地区新生代玄武岩岩浆来源于上地幔,是裂谷作用的产物,为大陆裂谷型玄武岩,其形成与敦密断裂在上新世的拉张活动有关.     

Chemical anomalies of lunar plagioclase,described by substitution vectors and their relation to optical and structural properties

Lunar plagioclase posed an enigma because optical properties indicate slow cooling while structural properties suggest rapid quenching when compared directly to terrestrial plagioclase. If, however, the An-content is inferred from the Al/Si ratio rather than from the Ca/Na ratio, lunar plagioclase corresponds more closely to normal volcanic plagioclase. The differences between An=4(Al/(Al+Si))-1 and An=Ca/(Ca+Na+K) is caused by substitutions which appear so far to be unique to lunar feldspars. A vector representation of chemical composition makes it possible to single out several substitutions which account for the chemical peculiarities of lunar plagioclase. It permits to assign sites in the structure to various minor elements simply from the chemical analysis without having to rely on sophisticated spectroscopic techniques or an X-ray structure determination. 1. The deficiency in Al+Si (up to 0.06 per formula unit) is compensated for by Fe, Mg, and small amounts of Na or Ca occupying tetrahedral sites. The Ca/Na ratio is increased accordingly to balance the electric charge. This substitution accounts for most of the differences. 2. The vacancycoupled substitution Ca+□ → 2 Na (Weill et al., 1970) is another cause for the increased Ca/Na ratio. 3. The amount of alkali evaporation from plagioclase, if it occurred, is probably small. These unusual substitutions are an expression of special conditions on the moon during the crystallization of plagioclase. Crystallization at high temperatures, rapid cooling, and peculiar magma composition seem to be important factors, but experimental work and detailed study of terrestrial volcanic plagioclase are necessary to interpret the chemical composition quantitatively.     

铸石结晶过程中球体的发育特征

在火成岩、变质岩、混合岩中,“球状”岩石是不乏见的。“球状”岩石最早为伯奇(Buch)所描述,以后一直为岩石学家所注意。对“球状”岩石中球体的成因,有各种各样的解释莱维森(Leveson)。凯斯勒(Kesler)用电子探针研究了球状安山岩中球体和基质的化学成分特点,并据基思(Keith)假说,推测了球体形成温度为900-1000℃,球体生长速度为10^-6厘米/秒。     

南海新生代碱性玄武岩中斜长石矿物的化学成分及意义

南海新生代碱性玄武岩中存在两种不同粒径的斜长石矿物.其一为斜长石斑晶,常见熔蚀麻点,是岩浆上升、压力降低时发生熔蚀作用并在骤冷条件下形成的;其二斜长石微晶,半定向或杂乱分布于火山玻璃中,其中空骸晶结构表明斜长石微晶是在淬冷条件下迅速结晶形成的.斜长石斑晶具弱成分环带,斑晶边部的An值稍高或接近于斜长石微晶.微晶斜长石An值与岩浆喷出后的水深以及喷发位置距离岩浆主通道的远近存在一定联系.本区的斜长石斑晶形成温度明显低于冲绳海槽地区,而类似于东海陆架地区;斜长石微晶的结晶温度类似于冲绳海槽,表明两地区在岩浆喷出海底后淬火结晶的物理化学条件相似.结合同样品中橄榄石斑晶研究结果以及已有的地球物理学和岩石学方面的资料,可能反映了地幔柱快速上涌使早期部分熔融及结晶分异作用较弱,岩浆本身温度高提供了早期结晶形成的斑晶与寄主岩浆进一步充分反应的热量.计算的斜长石斑晶温度不能反映源区温度特征,后者应高于本文所计算的斜长石斑晶的结晶温度.     

Origin of ultramafic xenoliths containing exsolved pyroxenes from Hualalai Volcano,Hawaii

Hualalai Volcano, Hawaii, is best known for the abundant and varied xenoliths included in the historic 1800 Kaupulehu alkalic basalt flow. Xenoliths, which range in composition from dunite to anorthosite, are concentrated at 915-m elevation in the flow. Rare cumulate ultramafic xenoliths, which include websterite, olivine websterite, wehrlite, and clinopyroxenite, display complex pyroxene exsolution textures that indicate slow cooling. Websterite, olivine websterite, and one wehrlite are spinel-bearing orthopyroxene +olivine cumulates with intercumulus clinopyroxene +plagioclase. Two wehrlite samples and clinopyroxenite are spinel-bearing olivine cumulates with intercumulus clinopyroxene+orthopyroxene + plagioclase. Two-pyroxene geothermometry calculations, based on reconstructed pyroxene compositions, indicate that crystallization temperatures range from 1225° to 1350° C. Migration or unmixing of clinopyroxene and orthopyroxene stopped between 1045° and 1090° C. Comparisons of the abundance of K₂O in plagioclase and the abundances of TiO₂ and Fe₂O₃in spinel of xenoliths and mid-ocean ridge basalt, and a single ⁸⁷Sr/ ⁸⁶Sr determination, indicate that these Hualalai xenoliths are unrelated to mid-ocean ridge basalt. Similarity between the crystallization sequence of these xenoliths and the experimental crystallization sequence of a Hawaiian olivine tholeiite suggest that the parental magma of the xenoliths is Hualalai tholeiitic basalt. Xenoliths probably crystallized between about 4.5 and 9 kb. The 155°–230° C of cooling which took place over about 120 ka — the age of the youngest Hualalai tholeiitic basalt — yield maximum cooling rates of 1.3×10^–3–1.91×10^–3 °C/yr. Hualalai ultramafic xenoliths with exsolved pyroxenes crystallized from Hualalai tholeiitic basalt and accumulated in a magma reservoir located between 13 and 28 km below sealevel. We suspect that this reservoir occurs just below the base of the oceanic crust at about 19 km below sealevel.     

Lunar anorthosite 60025, the petrogenesis of lunar anorthosites,and the composition of the Moon

Systematic variations of the mineral chemistry of ferroan anorthosite 60025, which is probably a mixture of closely related materials, suggest that lunar anorthosites formed by strong fractional crystallization and near-perfect adcumulate growth, without trapping liquid. The parent liquid for the most primitive samples was saturated with olivine, plagioclase, pigeonite, and chromite, and evolved to one saturated with plagioclase, pigeonite, high-Ca pyroxene, and ilmenite. The parent liquid also had a very low Na₂O content, and combined with strong fractional crystallization this explains the steep trend of anorthosites on an Mg1 (atomic 100 × Mg/(Mg + Fe)) v. An diagram. The mineral and chemical data for other anorthosites are consistent with such a model. Near-perfect adcumulation can occur if growth takes place at the crystal-liquid interface without the physical accumulation of crystals grown elsewhere, and is encouraged by the shifts in phase boundaries with pressure.Anorthosites are probably the remnants of a crust floating on, and crystallizing at the surface of, a magma ocean originally of bulk Moon composition. Mineralogical and trace element data suggest that the parental liquid for the most primitive anorthosites had previously crystallized no plagioclase and some but perhaps very little pyroxene. Hence the bulk Moon appears to be similar to that proposed by Ringwood (1976) but to have even lower alkalis, a subchondritic $\text{Ca}\text{Al}$ ratio, and REE abundances and patterns close to chondritic. The mare basalt sources are not directly complementary to the feldspathic crust, because experimental and trace element data indicate that they are too magnesian and contain too much high-Ca pyroxene. Other crustal rocks, such as the Mg-suite samples, are not closely related to anorthosites; in addition to their chemical differences they have a different crystallization sequence: ol → plag → px, in contrast with the ol → px → plag inferred for anorthosite parental liquid evolution.     

盐津地区峨眉山玄武岩地球化学特征及成因分析

峨眉山火成岩省东部盐津地区玄武岩的岩石地球化学分析结果表明,盐津玄武岩w(SiO2)为47.97%~52.33%,w(Na2O+K2O)为3.35%~6.57%,Ti/Y值为496.29~567.80,w(TiO2)为3.60%~4.14%,属于钙碱性高钛玄武岩(HT)。岩石LREE/HREE值为7.34~7.88,轻稀土元素富集,分馏程度高,总体亏损Ba,K,Sr,P。高场强元素Nb/U比值为26.39,Ce/Y-Sm/Y和Th/Nb-Ce/Nb等比值均呈明显正相关系,表明盐津地区峨眉山玄武岩受到了明显地壳混染作用。Nb-Nb/Y和La-La/Sm图解中样品投点呈倾斜直线,表明盐津玄武岩岩浆受分离结晶作用影响较弱,δEu值为0.86~0.93,CaO/Al2O3与Mg#无明显相关关系,以及镜下观察均表明仅有少量斜长石、单斜辉石的分离结晶。盐津玄武岩与盐源和越西等地高钛玄武岩地球化学特征相似,具地幔柱成因特征,岩浆可能起源于富集地幔。分配系数相近的强不相容元素Ce/Sm比值为25.50,La/Yb-Sm/Yb图解中样品靠近石榴石尖晶石二辉橄榄岩区域,表明岩浆源区为石榴石尖晶石二辉橄榄岩。     

一个与铬铁矿富集有关的巨型实验

现在岩石学、矿床学的实验一般用样品是几十毫克、甚至十几毫克,其目的是要精确化。但是许多事实说明,这种精密的实验工作并不能完全解决矿床的成因。要解决矿床成因的问题,至少必须回答下面三个问题:(1)有用金属矿物是在什么条件下形成的;(2)有用金属矿物是如何富集为矿石的;(3)矿石如何具有一定的量,并达到经济上可开采的要求。实验岩石学和实验矿床学的资料一般只说明了第一个问题。     

Quench textures in pillow basalt from the Andaman-Nicobar Islands,Bay of Bengal,India

Tholeiitic pillow basalt from the South Andaman island, an integral part of the outer sedimentary arc of the Sunda-Burmese double chain arc system in the Bay of Bengal, is characterized by the occurrence of several morphologies of quenched crystals of plagioclase and pyroxene. Plagioclase shows a swallow tail, belt-buckle, rosette and closely spaced fan-spherulites pattern while pyroxene has elongate parallel chain, dendritic, spherulitic and finely ornamented feathery spherulitic habit. Most of these textures are identical to those reported from submarine basalts, lunar basalts, spinifex textured rocks and experimentally produced textures. The occurrence of these quench textures in the Andaman basalt suggests that they were formed by rapid cooling at 30–70°C/h in a submarine environment.     

Silicate mineralogy of martian meteorites

Basalts and basaltic cumulates from Mars (delivered to Earth as meteorites) carry a record of the history of that planet - from accretion to initial differentiation and subsequent volcanism, up to recent times. We provide new microprobe data for plagioclase, olivine, and pyroxene from 19 of the martian meteorites that are representative of the six types of martian rocks. We also provide a comprehensive WDS map dataset for each sample studied, collected at a common magnification for easy comparison of composition and texture. The silicate data shows that plagioclase from each of the rock types shares similar trends in Ca-Na-K, and that K₂O/Na₂O wt% of plagioclase multiplied by the Al content of the bulk rock can be used to determine whether a rock is “enriched” or “depleted” in nature. Olivine data show that meteorite Y 980459 is a primitive melt from the martian mantle as its olivine crystals are in equilibrium with its bulk rock composition; all other olivine-bearing Shergottites have been affected by fractional crystallization. Pyroxene quadrilateral compositions can be used to isolate the type of melt from which the grains crystallized, and minor element concentrations in pyroxene can lend insight into parent melt compositions.In a comparative planetary mineralogy context, plagioclase from Mars is richer in Na than terrestrial and lunar plagioclase. The two most important factors contributing to this are the low activity of Al in martian melts and the resulting delayed nucleation of plagioclase in the crystallizing rock. Olivine from martian rocks shows distinct trends in Ni-Co and Cr systematics compared with olivine from Earth and Moon. The trends are due to several factors including oxygen fugacity, melt compositions and melt structures, properties which show variability among the planets. Finally, Fe-Mn ratios in both olivine and pyroxene can be used as a fingerprint of planetary parentage, where minerals show distinct planetary trends that may have been set at the time of planetary accretion.Although the silicate mineralogical data alone cannot support one specific model of martian magmatism over another, the data does support the basic igneous reservoirs proposed for Mars, and may also be used to constrain some aspects of specific petrogenetic models. Examples include enriched and depleted reservoirs that can be identified by plagioclase K, Na and Al composition, multivalent element partitioning in olivine and pyroxene (V, Cr) elucidates oxygen fugacity conditions of the reservoirs, and minor element concentrations (i.e., Cr in pyx) show that proposed fractional crystallization models linking Y 980459 to QUE 94201 will not work.     

Mineralogy,petrology and chemistry of lithic fragments from Luna 20 fines: origin of the cumulate ANT suite and its relationship to high-alumina and mare basalts

Bulk analyses of 157 lithic fragments of igneous origin and analyses of their constituent minerals (plagioclase, pyroxene, olivine, Mg-Al spinel, chromite, ilmenite, armalcolite, baddeleyite, zirkelite, K-feldspar, interstitial glass high in SiO₂ and K₂O) have been used to characterize the lunar highland rock suites at the Luna 20 site. The predominant suite is composed of ANT (anorthositic-noritic-troctolitic) rocks, as found at previous Apollo and Luna sites. This suite consists of an early cumulate member, spinel troctolite, and later cumulate rocks which are gradational from anorthosite to noritic and troctolitic anorthosite to anorthositic norite and troctolite; anorthositic norite is the most abundant rock type and its composition is close to the average composition for the highland rocks at this site. Spinel troctolite is a distinctive member of this suite and is characterized by the presence of Mg-Al spinel, magnesian olivine (average, Fo₈₃), and plagioclase. High-alumina basalt with low alkali content is another important rock type and melt of this composition may be parental to the cumulate ANT suite. Alkalic high-alumina basalt (KREEP) was not found in our sample, but may be genetically related to the ANT suite in that it may have formed by partial melting of rocks similar to those of the ANT suite. Fractional crystallization of low alkali, high-alumina basalt probably cannot produce alkalic high-alumina basalt because the enrichment in KREEP component is many times greater than the simultaneous change in major element components. Formation of alkalic high-alumina basalt by mechanical mixing of ANT rocks with very KREEP-rich components is not likely because the high-alumina basalt suite falls on a cotectic in the anorthiteolivine-silica system. Mare basalts may also be genetically related in that they may have been derived by remelting of rocks formed from residual liquids of fractional crystallization of parental low-alkali, high-alumina basalt, plus mafic cumulate crystals; the resultant melt would have a negative Eu anomaly and high $\text{Fe}\text{Mg}$ and $\text{pyroxene}\text{plagioclase}$ ratios.