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1.
Rare-earth abundances in chondritic meteorites   总被引：1，自引：0，他引：1  
Fifteen chondrites, including eight carbonaceous chondrites, have been analyzed for rare earth element (REE) abundances by isotope dilution. These analyses complement and extend earlier isotope dilution REE determinations in chondrites, performed in other laboratories, so that coverage of major chondrite classes is now complete. An examination of this body of precise and comparable REE data from individual chondrites reveals that only a small proportion of the analyses have flat, unfractionated REE patterns within experimental error. A statistical procedure is used to derive revised chondritic abundances of REE by selection of unfractionated patterns. A number of the remaining analyses show Eu anomalies and fractionated patterns consistent with magmatic fractionation as encountered in the products of planetary differentiation. However, many patterns exhibit features not readily explicable by known magmatic processes; in particular, positive Ce anomalies are often encountered. Abundance anomalies can be quantitatively determined by the use of a least-squares curve fitting procedure. The wide variety of anomalous patterns and the uncertainties in model parameters preclude detailed modeling of the origin of anomalies, but it is probable that at least some arise from fractional condensation in the solar nebula, as has been demonstrated for Allende inclusions. Elemental abundance anomalies are found in all major chondrite classes. If these anomalies are ignored, the range and nature of variation within chondrite classes are consistent with a parent body model, in which solid-liquid or solid-solid equilibria induce variations from an unfractionated bulk composition. Absolute abundances in the H, L and LL parent bodies are almost twice those of the E parent body.The persistence of anomalies in chondritic materials relatively removed from direct condensational processes implies that anomalous components are resistant to equilibration or were introduced at a late stage of chondrite formation. Large scale segregation of gas and condensate is also implied, and raises the possibility of bulk variations in REE abundances between planetary bodies.  相似文献   

2.
云南个旧碱性岩体主要的岩石类型有碱性正长岩和似长石正长岩,其中,似长石正长岩中出现大量似长石矿物霞石、方钠石和碱性暗色矿物。本文根据矿物成分及特征,将这些似长石正长岩进一步划分为黑榴霞石方钠正长岩、霞石方钠正长岩、霞石正长岩及方钠霞石正长岩4类。岩石地球化学结果表明,4类岩石的地球化学行为整体表现出过碱质岩的特征,K2O+Na2O含量很高,为钾玄岩系列,同时表现出钾质的特点。分异指数高,呈现高度分异演化特点。稀土元素变化大,轻重稀土元素分异明显,富集轻稀土元素,亏损重稀土元素。微量元素富集大离子亲石元素Th、U及Zr、Hf等高场强元素,亏损Ba、Sr大离子亲石元素,而P和高场强元素Ta、Ti亏损,同时Cr、Co、Ni含量非常低,具有中等的负Eu异常和微弱的负Ce异常。研究表明,似长石正长岩在岩浆演化过程中表现出明显的分离结晶作用特征,且岩浆起源温度较高,约为835℃,起源较深。个旧似长石正长岩为A型岩套A1亚型,结合构造判别图解,认为其可能来自角闪石或者金云母相矿物存在的富集地幔,形成于燕山晚期伸展的构造背景,岩浆在较高温度下高度结晶分异,并在侵位过程中伴随陆壳成分的混染。  相似文献   

3.
格尔木西山铜多金属矿的成矿岩体为似斑状二长花岗岩,位于昆中断裂与昆北断裂之间的秦祁昆晚加里东造山系内,其理论研究工作十分薄弱.以岩石地球化学、同位素年代学为手段进行研究,表明岩体属于高钾钙碱性系列过铝质花岗岩类.稀土、微量元素特征为轻稀土富集型,右倾式,具强负铕异常,富集大离子亲石元素（Th、U、K）,明显亏损高场强元素（如P、Ti）,相对于Rb和Th明显亏损Ba.岩浆为地壳来源,具弱分离结晶花岗岩特征.在似斑状二长花岗岩中获得岩浆锆石LA-ICP-MS U-Pb加权平均年龄（267.5±3.4 Ma）与谐和年龄（267.0±2.9 Ma）的数据,表明岩体形成于中二叠世的同时,也约束了成矿作用的下限.矿床类型应为与花岗质岩浆活动有关的构造热液型多金属矿.   相似文献   

4.
黄长煌 《地质通报》2017,36(10):1722-1739
台湾玉里带位于台湾东部,其主体为变质砂岩、千枚状泥岩夹绿帘片岩、阳起片岩、浅变质枕状玄武岩等(原岩为海相火山-陆源沉积岩),其次为高压相的蓝闪片岩。火山岩属钙碱性系列,具低Ba、Nb、Sr和高Pb丰度,稀土元素总量普遍较低,具有轻稀土元素弱富集、Eu无亏损的稀土元素配分模式;(含火山碎屑)变质砂岩的LA-ICP-MS锆石U-Pb年龄表明,~(206)Pb/~(238)U表面年龄有6个峰值:最新年龄23.3Ma(古近纪)为火山碎屑锆石年龄,也是成岩年龄;中生代—古生代年龄有96.7Ma(晚白垩世)、124.2Ma及130.6Ma(早白垩世)、214.1~228Ma(晚三叠世)、283.7Ma和289Ma(早二叠世)等,锆石为次棱角状或次圆状,代表了源岩的岩浆年龄;~(207)Pb/~(206)Pb表面年龄出现古元古代峰值(1769~1852Ma)和新太古代峰值(2506Ma和2530Ma),均为磨圆的碎屑变质或岩浆锆石,代表了不明古元古代变质基底的年龄。玉里带变质岩原岩可能形成于古近纪(23.3Ma),与南海扩张的白云运动同时,属白云运动有关的火山作用的产物。  相似文献   

5.
在攀西地区,自海西期以来出现两套与大陆裂谷作用有关的岩浆岩共生组合,即基性岩套与碱（酸）性岩套。与基性岩套有成因联系和紧密伴生的印支期碱性正长伟晶岩脉和碱性花岗伟晶岩脉等,普遍具稀有、稀土和铀钍矿化,有的已形成中小型铌钽矿床:碱（酸）性岩套以超基性碱性岩、碱性花岗岩为代表,并具与碱性花岗岩有关的稀有、稀土矿床和铀钍矿化。本文对上述碱性杂岩有关的成矿系列,划分了矿床成因类型,并对主要控制因素作了较为详细的探讨。  相似文献   

6.
Gough Island: Evaluation of a fractional crystallization model   总被引：3，自引：0，他引：3  
Gough Island is composed of an alkaline olivine basalt-trachyte series. A fractional crystallization model for the development of these rocks has been evaluated by correlating the geochemical trends of major and trace elements. Beginning with an alkali olivine basalt parent the major element abundances were used to determine the varying proportions of crystallizing minerals required to generate the various residual liquids. A least-squares computer model was used for this calculation. The modal proportions of cumulative minerals and trace element distribution coefficients were used to predict the trace element abundances in each rock type.Three significant trace element trends are observed in Gough Island rocks: (1) increasing rare earth (RE) abundance and relative light RE enrichment with increasing major element differentiation, (2) marked Eu, Sr, and Ba depletions in late stage trachytes, (3) Cr and M enrichment in picrite basalt.The trace element abundances predicted by the fractional crystallization model are in good agreement with these observed trends. A fractional crystallization process involving olivine, pyroxene, feldspar, and apatite accounts for all the significant major and trace element trends observed in Gough Island rocks.  相似文献   

7.
低山头一带花岗岩体归属东昆仑弧盆系北昆仑岩浆弧带,位于东昆仑成矿带伯喀里克—香日德成矿亚带东昆仑造山带中段,岩石类型主要为石英闪长岩、正长花岗岩及二长花岗岩。为了加强该地区花岗岩体岩石地球化学与成岩成矿背景探讨,对花岗岩体开展了主量元素、微量元素及矿质元素研究。主量元素组成上,石英闪长岩具中硅（57.64%和58.47%）、富钠（Na2O/K2O均为2.57）特点,正长花岗岩具高硅（75.45%~75.99%）、富钾（Na2O/K2O为0.74~0.94）特点,二长花岗岩具高硅（66.80%~73.45%）、富钠（Na2O/K2O为1.50~2.13）特点;花岗岩体铝饱和指数A/CNK<1,为准铝质岩浆岩;碱饱和指数NK/A集中在0.26~0.69之间,属钙碱性岩石;里特曼组合指数σ43在1.18~2.31之间,属钙碱性类型。花岗岩体轻稀土元素相对重稀土元素富集,岩浆分异特征明显,大离子亲石元素（LILE）富集Rb、K、Ba、Th、Sr、Nd,仅正长花岗岩Sr亏损,高场强元素（HFSE）富集Zr、Hf、Ce,而Nb、P、Ti明显亏损,源区物质为壳幔混合物质,属挤压应力环境中同碰撞I型花岗岩。在岩体实测剖面中获得11种元素分析数据,与青海全省、东昆仑成矿带及其亚成矿带平均元素丰度值进行对比,初步划分不同岩性、不同类型、不同时代花岗岩,以及富集的含矿元素为Au、Zn、Y、Pb等。与区域有成矿事实且为I型花岗岩成因进行对比,认为研究区有较好的找矿前景。  相似文献   

8.
An ion probe study of rare earth element (REE) geochemistry of silicate inclusions in the Miles IIE iron meteorite was carried out. Individual mineral phases among inclusions have distinct REE patterns and abundances. Most silicate grains have homogeneous REE abundances but show considerable intergrain variations between inclusions. A few pyroxene grains display normal igneous REE zoning. Phosphates (whitlockite and apatite) are highly enriched in REEs (50 to 2000 × CI) with a relatively light rare earth element (LREE)-enriched REE pattern. They usually occurred near the interfaces between inclusions and Fe host. In Miles, albitic glasses exhibit two distinctive REE patterns: a highly fractionated LREE-enriched (CI normalized La/Sm ∼15) pattern with a large positive Eu anomaly and a relatively heavy rare earth element (HREE)-enriched pattern (CI-normalized Lu/Gd ∼4) with a positive Eu anomaly and a negative Yb anomaly. The glass is generally depleted in REEs relative to CI chondrites.The bulk REE abundances for each inclusion, calculated from modal abundances, vary widely, from relatively depleted in REEs (0.1 to 3 × CI) with a fractionated HREE-enriched pattern to highly enriched in REEs (10 to 100 × CI) with a relatively LREE-enriched pattern. The estimated whole rock REE abundances for Miles are at ∼ 10 × CI with a relatively LREE-enriched pattern. This implies that Miles silicates could represent the product of a low degree (∼10%) partial melting of a chondritic source. Phenocrysts of pyroxene in pyroxene-glassy inclusions were not in equilibrium with coexisting albitic glass and they could have crystallized from a parental melt with REEs of ∼ 10 × CI. Albitic glass appears to have formed by remelting of preexisting feldspar + pyroxene + tridymite assemblage. Yb anomaly played an important role in differentiation processes of Miles silicate inclusions; however, its origin remains unsolved.The REE data from this study suggest that Miles, like Colomera and Weekeroo Station, formed when a molten Fe ball collided on a differentiated silicate regolith near the surface of an asteroid. Silicate fragments were mixed with molten Fe by the impact. Heat from molten Fe caused localized melting of feldspar + pyroxene + tridymite assemblage. The inclusions remained isolated from one another during subsequent rapid cooling.  相似文献   

9.
The major rock-forming mineral phases (pyroxenes, plagioclase, garnet, hornblende) of a suite of granulite-facies gneisses from the Scourian complex, NW Scotland, have been analyzed for their rare earth element (REE) content. Although host rock compositions range from felsic to ultramafic, REE abundances and patterns for each mineral group show only limited variation. The REEs exhibit regular and consistent distribution patterns for each mineral which suggest, together with major element and textural considerations, that the observed distribution coefficients approach equilibrium. Total REE content follows the sequence hornblende>clinopyroxene>garnet>plagioclase >orthopyroxene and mass balance calculations show that even in the felsic gneisses>60% of the REEs reside in the major rock-forming minerals. Comparisons of both relative REE abundances and distribution coefficients with those in other rock types reveal a striking resemblance with patterns observed in mineral-liquid pairs of dacitic rocks. These similarities may have arisen during a partial melting episode in which granite-granodiorite melts were generated and removed from the Scourian complex; leaving a residuum which is severely depleted in the incompatible elements, including the REEs.  相似文献   

10.
通过野外调研发现,秦岭造山带山阳地区水沟口组黑色岩系主要由黑灰色微晶灰岩、炭质泥板岩、灰白色粘土岩、黑灰色含炭-钙质硅板岩、灰黑色含炭泥质硅板岩及浅红色硅质板岩组成;岩系中磷结核及重晶石纹层常见。采用等离子质谱仪(ICP-MS)方法对岩系的稀土元素及微量元素测定,结果显示岩系中成矿物质含量丰富(如V、Mo、Ni、Ba、Pb、Zn、U、Ag、Cu、Cd、Tl、Bi和Cr等元素的平均含量是地壳丰度的几倍到几十倍),稀土元素和微量元素的含量与磷质、炭质以及钡关系密切;稀土模式曲线基本平行显示其成因相同;泥质和硅质岩类是主要的含矿岩性;不同程度的δEu正异常、中到弱的δCe负异常及相应的稀土、微量元素比值如Ce/La、V/(V+Ni)等指示岩石形成于干燥缺氧环境并有热水物质加入,La/Yb-Ce/La图解及La/Yb-REE图解表明岩系与海相沉积及基性岩成因关系密切。结合岩系的地质特征认为:山阳地区水沟口组黑色岩系形成于被动陆缘的一种干燥缺氧的深水-半深水滞留断陷局限海盆,期间热液(水)活动频繁、低等浮游生物发育,对岩系中矿物质的富集具有非常重要的意义。  相似文献   

11.
班康姆铜金矿床是近年来发现的大型铜金矿床,矿体主要赋存于中基性火山岩之中,其微量元素特征、玄武岩类的Ti-Zr-Y、Ti-Zr判别图、花岗岩类在Nb-Y(A)、Rb-(Y+Ta)判别图均表明成矿构造环境为岛弧环境,火山岩属于中钾钙碱性系列.岩浆岩稀土总量较低,标准化模式曲线均为略富集轻稀土的平坦型,Eu几乎不存在异常,说明火山岩、侵入岩为同源不同期的产物,岩浆热液来源于地幔或下地壳,热液活动划分为火山喷发期、热液叠加期,其成矿物质来源于安山岩,矿(化)体受NNE断裂构造、岩浆岩控制,矿床类型为与岩浆岩密切相关的复合型热液矿床.  相似文献   

12.
郗山和龙宝山稀土矿具有相似的成矿地质背景、控矿岩体特征及矿床地质特征。燕山早期碱性侵入岩与稀土矿关系密切,稀土矿体主要赋存于杂岩体内及其附近围岩中;稀土元素和同位素研究表明,含矿质的富碱岩浆可能属壳幔混源型,碱性岩浆及成矿物质最初可能都来源于上地幔同一部位,而在岩浆上侵过程中同化混染了地壳物质。郗山稀土矿为单一富轻稀土矿床,矿脉类型以含稀土石英重晶石碳酸盐脉为主,含稀土矿物以氟碳铈矿和氟碳钙铈矿为主,碳酸铈钠矿和菱钙锶铈矿属国内首次发现。龙宝山稀土矿为稀土、金共生矿,矿脉类型主要为石英脉和硅化角砾岩;含稀土矿物主要有氟碳铈矿、氟碳铈镧矿、氟碳钙铈矿;金矿物有自然金、银金矿等。成矿时代稍晚于岩浆岩形成时代,属中生代燕山晚期;矿床成因类型为碱性岩浆期后中-低温热液稀土矿床。  相似文献   

13.
陈焕元  贾飞 《地质学报》2021,95(11):3352-3365
浙江省内发育着众多中-大型萤石矿,但是对成矿岩体的研究相对较弱,制约着对区域成矿过程的认识.本文首次对安吉统里地区萤石成矿花岗岩体进行了系统的锆石U-Pb年代学和地球化学研究.锆石U-Pb测年结果显示小圩坞花岗闪长岩形成于146～140 Ma,而五房里细粒二长花岗岩形成于135 Ma,二者均形成于早白垩世早期,与华南地区大规模爆发的晚中生代岩浆作用时代相一致.全岩主微量元素地球化学表明统里地区花岗岩体可以划分为钙碱性Ⅰ型花岗岩和高分异Ⅰ型花岗岩两类,二者均显示高硅、富铝、贫铁和镁等特征,在地球化学上属于准铝质-过铝质岩石系列.其中小圩坞花岗闪长岩相对富集轻稀土元素和大离子亲石元素,亏损重稀土元素和高场强元素,而五房里细粒二长花岗岩则显示明显的中稀土元素亏损.研究认为小圩坞Ⅰ型花岗岩是变火成岩中下地壳熔融的产物,而五房里高分异Ⅰ型花岗岩是花岗质岩浆在浅层岩浆房内经历广泛结晶分异作用的产物.结合华南地区晚中生代岩浆作用由陆向海迁移的趋势,本文研究认为古太平洋板块俯冲过程中的板片回转过程是统里地区花岗岩侵入最为合理的深部动力学机制.  相似文献   

14.
山东张里金矿床是与碱性次火山岩有关的、赋存于隐爆角砾岩体内的石英－ 冰长石－ 萤石型中低温热液矿床。岩石化学、稀土元素和同位素分析结果表明: 控矿岩石系列分为: ①高钾钙碱性岩石系列,SiO2 平均含量为57. 6%,稀土总量为373. 98 × 10 － 6 ～ 297. 43 × 10 － 6,δEu 为0. 85 ～ 0. 82,Sr = 0. 704 41; ②高钾碱性岩系列,SiO2 平均含量为56. 65%,稀土总量为371. 19 × 10 － 6 ～ 41. 62 × 10 － 6, δEu 为0. 89 ～ 0. 93,Sr = 0. 717 11。这两种控矿岩石系列分别由两个不同的幔源岩浆在上升过程中,各自经过长时期的分异作用,并且混染了部分壳源物质而成,其含矿热液来自碱性次火山岩。  相似文献   

15.
Abstract: Systematic data of rare earth elements (REEs) are presented in order to put some constraints on the origin of hydrothermal fluids responsible for two contrastive skarn deposits in Japan; the Kamioka Zn-Pb and Yoshiwara-Sannotake Cu(-Fe) deposits. Carbon and oxygen isotopic studies have demonstrated that the hydrothermal fluids responsible for the Kamioka Zn-Pb deposits are of meteoric water origin whereas those for the Yoshiwara-Sannotake Cu(-Fe) deposits are of magmatic water origin. The REE abundances of epidote skarn derived from aluminous rocks, garnet and clinopyroxene in calcic exoskarn derived from limestone, and interstitial calcite associated with sulfide minerals were determined for these contrastive skarn deposits by inductively-coupled plasma mass spectrometry (ICP-MS). A significant difference in the REE concentrations is not found between epidote skarn and aluminous original rock (plagioclase-clinopyroxene rock, called Inishi rock) from the Kamioka Zn-Pb deposits, indicating that the REEs are generally immobile during the formation of epidote skarn, and that the REE concentrations of the hydrothermal fluid are considerably low relative to the aluminous original rock. In contrast, the epidote skarn exhibits enrichment of Eu with increasing total REE concentrations relative to the aluminous original rock (quartz diorite) in the Yoshiwara-Sannotake Cu(-Fe) deposits, implying a contribution of magmatic fluid derived from granitoids during the skarn formation. Limestone generally has much lower REE concentrations related to surrounding aluminous rocks, and thus the REE concentrations of garnet and clinopyroxene in calcic exoskarn, originated from limestone, are variable due to the interaction with the hydrothermal fluids. The chondrite-normalized REE patterns of garnet, clinopyroxene, and interstitial calcite exactly provide useful information on origins of hydrothermal fluids. The REE patterns of these minerals from the Kamioka Zn-Pb deposits show lower (Pr/Yb)cn ratios, and negative Ce and Eu anomalies inherited from limestone with the decrease of This suggests that the hydrothermal fluids responsible for the Kamioka Zn-Pb deposits were depleted in REEs, and were not magmatic water in origin, but presumably meteoric one. In striking contrast, the REE patterns of exoskarn minerals and calcite from the Yoshiwara-Sannotake Cu(-Fe) deposits exhibit a positive Eu anomaly, and high (Pr/Yb)cn ratios with the considerable increase of σREE and the disappearance of negative Ce anomaly, implying that the fluids were dominantly of magmatic origin. The REE indices are very likely to be an excellent indicator to origins of the skarn deposits.  相似文献   

16.
为了解由早期(伟晶、巨晶)斑状二长花岗岩、中期(细粒)花岗岩和晚期花岗(斑)岩脉组成的马鞍山杂岩体的成因, 采用SHRIMP和LA-ICP-MS锆石U-Pb法厘定其侵入时代, 年龄显示伟晶斑状二长花岗岩为132.2±1.6 Ma, 巨晶斑状二长花岗岩为127. 7±1.2 Ma, 细粒花岗岩为128.3±1.1 Ma, 花岗斑岩脉为127.4±1.8 Ma.岩石地球化学研究结果表明岩体从早到晚具有从钾玄岩系列向高钾钙碱系列演变特征, 分异演化程度逐渐变高; 斑状二长花岗岩具有高REE含量, 轻重稀土分异较为明显, 具较强负铕异常和弱右倾的配分曲线特征, 富集K、Th、U、Rb等元素, 弱亏损Ba、Sr、P、Nb、Ta、Ti等元素; 细粒花岗岩及花岗(斑)岩脉具有较低REE含量, 轻重稀土分异不明显, 具强负铕异常和"V"型配分曲线特征, 富集K、Th、U、Rb等元素, 强亏损Ba、Sr、P、Nb、Ti等元素.马鞍山岩体为浙西北-皖南地区早白垩世俯冲造山后陆内拉张作用环境下下地壳部分熔融的同源岩浆侵位结晶分异作用形成的产物, 具有高分异I型花岗岩的特征.   相似文献   

17.
Coupled with a petrographical study, I carried out an ion probe study of rare earth element microdistributions in mineral phases of silicate inclusions from the Colomera IIE iron meteorite. Most mineral grains have homogeneous REEs, but show considerable inter-grain variations by a factor of 2 to 100. The whole rock REE abundances for Colomera,estimated by combining REE data with modal abundances, are relatively LREE-enriched with REEs of～10’CI, which suggest that Colomera silicates were highly differentiated and might represent a low degree partial melt (-10%) of a chondritic source. REE geochemistry of Colomera silicate inclusions points to an origin that involves differentiation,dynamic mixing, remelting, reduction, recrystallization, and subsequent rapid cooling near the surface of a planetary body.  相似文献   

18.
东昆仑造山带发育大量花岗质岩浆岩,对其研究不仅能为东昆仑的岩浆、构造提供新的信息,且对探讨古特提斯的构造-演化过程具重要意义。本文报道东昆仑西段落雁山花岗闪长斑岩体的两组锆石U-Pb年龄和地球化学数据,并对其成因及构造意义进行探讨。两组落雁山花岗闪长斑岩体锆石206Pb/238U-年龄分别为(312.4±2.0)Ma、(312.4±2.2)Ma,形成于晚石炭世。岩石地球化学特征显示,该岩体具高钾钙碱性准铝质花岗岩特征,稀土元素标准分布曲线呈右倾,富集轻稀土,轻、重稀土分异明显,微量元素中大离子亲石元素(LILE:Rb,Ba)相对富集;高场强元素(HFSE:Nb,P,Ti)亏损。锆石Hf同位素特征和岩石成因物源研究表明,落雁山花岗闪长斑岩为少量幔源岩浆参与的壳幔混源I型花岗岩。据区域构造研究,落雁山花岗闪长斑岩形成于晚石炭世古特提斯洋壳俯冲作用背景下的岛弧晚期岩浆活动。  相似文献   

19.
达达肯乌拉山位于柴达木盆地北缘中东部,区内发育闪长岩体,以小岩株形式产出。通过对达达肯乌拉山闪长岩岩石LA-ICP-MS锆石U-Pb定年和地球化学特征的研究,获得闪长岩体的年龄为(240.5±1.7) Ma,属早印支期。闪长岩体的w(K_2O)较高,为2.03%～2.30%,w(Na2O)含量较低,为3.2%～3.44%,为一套准铝质及弱过铝质高K、低Na的高钾钙碱性型I型花岗岩。岩石稀土元素总量为158.35×10~(-6)～200.41×10~(-6),球粒陨石标准化曲线向右倾斜,重稀土元素曲线呈水平状,轻稀土元素富集,但负铕异常不明显,岩浆分异程度不高。岩石的La/Ta(54.32～68.51)、Sm/Nd(0.18～0.19)及Rb/Sr(0.11～0.19)比值特征反映该岩体岩浆具有壳幔混合的特点。通过构造判别,反映达达肯乌拉山岩体可能形成于俯冲陆壳断离、幔源岩浆底侵的地球动力学背景,在中央造山带早中生代统一的板块碰撞与挤压构造体制下,以滩间山蛇绿岩带为基础,发生陆壳俯冲和断离作用,并诱发幔源岩浆的底侵和下地壳物质的部分熔融,沿火山机构侵位形成达达肯乌拉山岩体。  相似文献   

20.
李屯铁矿为近年在山东省齐河—禹城地区发现的隐伏富磁铁矿床,为空白区地质找矿新发现。本文通过详细野外调查、室内镜下观察及地球化学分析测试,对矿床地质、地球化学特征进行了系统研究,初步揭示矿床成因。磁铁矿体赋存于李屯岩体与石炭纪—二叠纪地层接触带附近的砂泥岩地层内。李屯铁矿中岩体微量元素分配模式具有较好的一致性,均不同程度地富集Rb、Ba、Sr等大离子亲石元素,亏损Zr、Nb、Ta等高场强元素,磁铁矿石中富集大离子亲石元素Sr,亏损K;高场强元素富集U、P、Hf、Ta,亏损Nb、Ti。岩体与磁铁矿石稀土元素均表现出轻稀土富集、重稀土亏损的右倾型配分模式。李屯铁矿形成于岩石圈大规模快速减薄期,成矿构造背景应为板块伸展扩张环境。李屯岩体的岩浆来源为壳幔混源,尖晶石相二辉橄榄岩发生部分熔融产生的的岩浆熔体;成矿物质来源于深源岩浆及其形成的岩浆岩。磁铁矿成矿与李屯岩体关系密切,矿床成因类型应是接触交代型矽卡岩铁矿床。  相似文献   

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