共查询到20条相似文献，搜索用时 156 毫秒
1.
通过对燕辽成矿带东段冀东-辽西金矿床基础地质地球化学资料分析,结合区域构造演化和成矿时间及其分布空间的特异性,认为冀东-辽西金矿成矿物质具有相同的深来源特征,由于具体的构造背景不同而表现出矿床类型和就位空间的差异性,提出了燕辽裂陷槽是冀东-辽西金矿床空间分布的诱因,并提出冀东-辽西金成矿演化分为陆陆碰撞拼贴期(4.5～... 相似文献
2.
从变质作用演化、构造变形作用演化方面探讨了处于冀东与密云之间的兴隆地区太古宙变质岩系的变形变质构造演化史 相似文献
3.
铁矿是重要的大宗金属矿产资源,冀东地区作为我国重要的钢铁基地面临着后备资源不足的问题,亟待深入开展冀东地区铁矿成矿规律和找矿方向研究。本文在近年来冀东地区找矿实践的基础上,利用勘查区找矿预测理论方法体系,系统归纳冀东铁矿床特征,共划分5个成矿区带,分析了本区鞍山式沉积变质型铁矿含铁建造、变质变形空间分带规律及控矿构造特征,并总结该地区矿床成矿规律。提出滦县滦南铁矿成矿区带成矿构造受背形和断裂构造共同控制的观点,指出冀东地区“就矿找矿”预测要素可简化为矿体控制程度和地球物理标志两大类。认为冀东铁矿地质工作程度高,进一步找矿的2个主要方向:一是已有大中型矿山深部和外围“就矿找矿”,预测其仍有较大资源潜力;二是迁安铁矿成矿区带第三层硅铁建造,属新发现的成矿空间,具有重要的找矿意义。 相似文献
4.
峪耳崖金矿是冀东幔枝构造外国主折离带上盘盖层中,受反向铲状断层和次级折离带共同控制的典型金矿。突出表现为复合构造控制燕山花岗质岩体呈塔状展布,而次级折离带的持续折离滑脱使成岩后的岩床状花岗岩产生一系列缓倾裂隙,并成为主成矿期的主要储矿构造扩容带。文中探讨了冀东是区地质演化过程,分析了区域成矿构造特征,总结了成矿作用机理,归纳了成矿模式。认为深部找矿仍有较大远景。 相似文献
5.
由于太古宙克拉通活化、在克拉通内形成大小不等的构造岩浆活化带，华北陆台北缘中段已知的构造岩浆活地带有：冀东喜峰口一下板城构造岩浆活化带；张宣地区水泉沟构造岩浆活化带；丰宁一隆化构造岩浆后地带；喀喇沁一北票地区构造岩浆活化带．活化带内的深大断裂或剪切带，以及与其伴随的岩浆演出系列．给金矿的形成创造了良好条件．本文以冀东、张宣地区的构造岩浆活化带为例．介绍其地质特及其金矿床，并讨论了金矿床的成因模式。 相似文献
6.
冀东太古宙高级区主要由两个构造单元组成，以三屯营－洒河－金厂峪一线为界，北西侧为线性构造区，南东侧为卵形构造区。卵形构造是由紫苏花岗岩固态气球膨胀侵位形成的，之后又受到深部构造相韧性变形带的叠加，使卵形构造由东到西受改造的程度逐渐增大。线性构造则是中部构造相韧性变形带对深部构造相和卵形构造叠加的结果。尽管冀东地区南东、北西分异早于３５６３Ｍａ，但卵形构造区和线性构造区出现相对较晚（２５００Ｍａ）。 相似文献
7.
冀东太古宙高级区主要由两个构造单元组成，以三屯营－洒河－全厂峪一线为界，北西侧为线性构造区，南东侧为卵形构造区，卵形构造是由紫苏花岗岩固态气球膨胀侵位形成的，之后又受到深部构造相韧性变形带的叠加，使卵形构造由东到西受改造的程度逐渐增大，线性构造则是中部构造相韧性变形带对深部构造相和卵形构造叠加的结果，尽管冀东地区南东，北西分异早于３５６３Ｍａ，但卵形构造区和线性构造出现相对较晚。 相似文献
8.
作者研究了冀东地区构造特征及其成生联系,建立了构造体系。根据构造运动时期的鉴定,研究了构造演化过程,探讨了矿化与构造之间的关系。根据同成矿构造体系展布特点,分析了金矿的分布规律和富集部位,并对典型矿区进行了同成矿应力场的模拟实验,预测了隐状矿体。部分靶区经过工程验证,获得很大的经济效益. 相似文献
9.
冀东地区新发现一批产在中元古代碳酸盐岩层中的金矿床（点）,文中对该类矿床的容矿围岩特征及其成因、产出的区域构造背景进行了讨论,提出容矿角砾岩是液压致裂角砾岩,是一种矿控构造岩。 相似文献
10.
冀东地区内生金矿床成因类型不同,形成环境各异;但均受控于太古界地层、断裂构造及岩浆财,稳定同位素特征也极为相似,表明具有相同的物质一源和相似的成矿条件,区域上“三位一体”的地质环境是冀东地区内生金矿床的找矿方向。 相似文献
11.
有关地幔交代作用的研究始于７０年代早期。近２０年来研究工作的贡献是使人们对与地幔演化和不均一性有关的地幔交代作用特征和交代作用机制有了更多的了解。地幔交代作用很复杂，它取决于交代作用发生的时间、构造环境、交代介质的种类以及与不同深度地幔内各种地质事件有关的流体的组成。进一步深入开展有关交代作用成因、机制及其与各种地质事件关系的研究，对于深入认识岩石圈地幔的演化和不均一特征具有十分重要的意义。对不同构造环境中的不同包体类型进行深入研究，为地幔交代作用提供广泛约束。将传统的地质学、岩石学的研究与地球化学、地球物理学以及现代测试技术相结合，很可能为解决交代作用成因、机制及交代作用与岩浆作用之间的时间先后问题，交代作用与地质事件的关系问题提供有效的方法和途径。 相似文献
12.
有关地幔交代作用的研究始于７０年代早期。近２０年来研究工作的贡献是使人们对与地幔演化和不均一性有关的地幔交代作用特征和交代作用机制有了更多的了解，地幔交作用很复杂，它取决于交代作用发生的时间、构造环境、交代介质的种类以及与不同深度地幔内各种地质事件有关的流体的组成。进一步深入开发有关交代作用成因、机制及其与各种地质事件关系的研究，对于深入认识岩石圈地幔的演化和不均一特征具有十分重要的意义。对不同构 相似文献
13.
系统地介绍了近二十年来地幔地球化学在全球及区域地幔平均化学组成，地幔的化学不均一性及区域太产分布，地幔交代作用，化学地球动力学，地幔物理化学环境等五个方面的研究现状与进展。 相似文献
14.
The abundance of apatite in Phanerozoic mantle may be greatly underestimated. This study shows that apatite has a widespread occurrence in Phanerozoic lithospheric mantle and can be divided into two geochemically distinct types using halogen content, presence or absence of structural CO 2, Sr and trace element (especially U, Th, and light rare earth) ratios and abundances, and association with either metasomatised mantle wall-rock peridotites (Apatite A) or high-pressure magmatic crystallisation products (Apatite B). Apatite A is inferred to result from metasomatism by CO 2- and H 2O-rich fluids derived from a primitive mantle source region, while Apatite B compositions are consistent with crystallisation from magmas within the carbonate–silicate compositional spectrum. The presence of significant apatite in the lithospheric mantle is important not only for the geochemical budget but also for assessing heat production and heat flow in the mantle. The measured U and Th contents of mantle apatite average 60 and 200 ppm, respectively and 0.5% apatite would dominate heat production. Metasomatised mantle may also contain amphibole and mica with K2O and clinopyroxene with detectable U and Th. In lithospheric mantle with a thickness of 70 km, this abundance of apatite would result in mantle heat flow contribution of about 12 mW/m2, a significant proportion of the total “normal” mantle heat flow of about 18 mW/m2. 相似文献
15.
Spinel lherzolite xenoliths from Tertiary basaltic host magmas at Allyn River, eastern Australia reveal two distinct petrographic and geochemical types. One group is distinguished by xenoliths with undeformed, equilibrated microstructures and interstitial melt patches; The second group shows deformation and contains abundant fluid inclusions but no melt patches. Trace-element signatures of clinopyroxene in these xenoliths provide evidence for metasomatism by a silicate agent with hydrous component and by a carbonate-rich agent respectively. Melt patches in the undeformed xenoliths contain secondary minerals including clinopyroxene, olivine, feldspar, Mg- and Ca-rich carbonate, apatite, ilmenite and spinel. They are interpreted to represent volatile-rich melt captured shortly prior to entrainment in the host basalt. Sulfide globules, now recrystallised to discrete sulfide phases but inferred to be molten at lithospheric mantle T and P, are closely associated with the melt patches. The close association between sulfide and highly mobile, volatile-bearing fluid has important implications for the mobility of Re and Os, the use of their isotopes in dating mantle events, and the possible effect of volatile-bearing metasomatic agents on their composition. 相似文献
16.
Mantle xenoliths and xenocrysts were retrieved from three of the 88–86 Ma Buffalo Hills kimberlites (K6, K11, K14) for a reconnaissance study of the subcontinental lithospheric mantle (SCLM) beneath the Buffalo Head Terrane (Alberta, Canada). The xenoliths include spinel lherzolites, one garnet spinel lherzolite, garnet harzburgites, one sheared garnet lherzolite and pyroxenites. Pyroxenitic and wehrlitic garnet xenocrysts are derived primarily from the shallow mantle and lherzolitic garnet xenocrysts from the deep mantle. Harzburgite with Ca-saturated garnets is concentrated in a layer between 135–165 km depth. Garnet xenocrysts define a model conductive paleogeotherm corresponding to a heat flow of 38–39 mW/m 2. The sheared garnet lherzolite lies on an inflection of this geotherm and may constrain the depth of the lithosphere–asthenosphere boundary (LAB) beneath this region to ca 180 km depth. A loss of >20% partial melt is recorded by spinel lherzolites and up to 60% by the garnet harzburgites, which may be related to lithosphere formation. The mantle was subsequently modified during at least two metasomatic events. An older metasomatic event is evident in incompatible-element enrichments in homogeneous equilibrated garnet and clinopyroxene. Silicate melt metasomatism predominated in the deep lithosphere and led to enrichments in the HFSE with minor enrichments in LREE. Metasomatism by small-volume volatile-rich melts, such as carbonatite, appears to have been more important in the shallow lithosphere and led to enrichments in LREE with minor enrichments in HFSE. An intermediate metasomatic style, possibly a signature of volatile-rich silicate melts, is also recognised. These metasomatic styles may be related through modification of a single melt during progressive interaction with the mantle. This metasomatism is suggested to have occurred during Paleoproterozoic rifting of the Buffalo Head Terrane from the neighbouring Rae Province and may be responsible for the evolution of some samples toward unradiogenic Nd and Hf isotopic compositions. Disturbed Re–Os isotope systematics, evident in implausible model ages, were obtained in situ for sulfides in several spinel lherzolites and suggest that many sulfides are secondary (metasomatic) or mixtures of primary and secondary sulfides. Sulfide in one peridotite has unradiogenic 187Os/188Os and gives a model age of 1.89±0.38 Ga. This age coincides with the inferred emplacement of mafic sheets in the crust and suggests that the melts parental to the intrusions interacted with the lithospheric mantle. A younger metasomatic event is indicated by the occurrence of sulfide-rich melt patches, unequilibrated mineral compositions and overgrowths on spinel that are Ti-, Cr- and Fe-rich but Zn-poor. Subsequent cooling is recorded by fine exsolution lamellae in the pyroxenes and by arrested mineral reactions. If the lithosphere beneath the Buffalo Head Terrane was formed in the Archaean, any unambiguous signatures of this ancient origin may have been obliterated during these multiple events. 相似文献
17.
We present petrography and mineral chemistry for both phlogopite,from mantle-derived xenoliths(garnet peridotite,eclogite and clinopyroxene-phlogopite rocks)and for megacryst,macrocryst and groundmass flakes from the Grib kimberlite in the Arkhangelsk diamond province of Russia to provide new insights into multi-stage metasomatism in the subcratonic lithospheric mantle(SCLM)and the origin of phlogopite in kimberlite.Based on the analysed xenoliths,phlogopite is characterized by several generations.The first generation(Phil)occurs as coarse,discrete grains within garnet peridotite and eclogite xenoliths and as a rock-forming mineral within clinopyroxene-phlogopite xenoliths.The second phlogopite generation(Phl2)occurs as rims and outer zones that surround the Phil grains and as fine flakes within kimberlite-related veinlets filled with carbonate,serpentine,chlorite and spinel.In garnet peridotite xenoliths,phlogopite occurs as overgrowths surrounding garnet porphyroblasts,within which phlogopite is associated with Cr-spinel and minor carbonate.In eclogite xenoliths,phlogopite occasionally associates with carbonate bearing veinlet networks.Phlogopite,from the kimberlite,occurs as megacrysts,macrocrysts,microcrysts and fine flakes in the groundmass and matrix of kimberlitic pyroclasts.Most phlogopite grains within the kimberlite are characterised by signs of deformation and form partly fragmented grains,which indicates that they are the disintegrated fragments of previously larger grains.Phil,within the garnet peridotite and clinopyroxene-phlogopite xenoliths,is characterised by low Ti and Cr contents(TiO_21 wt.%,Cr_2 O_31 wt.% and Mg# = 100 × Mg/(Mg+ Fe)92)typical of primary peridotite phlogopite in mantle peridotite xenoliths from global kimberlite occurrences.They formed during SCLM metasomatism that led to a transformation from garnet peridotite to clinopyroxene-phlogopite rocks and the crystallisation of phlogopite and high-Cr clinopyroxene megacrysts before the generation of host-kimberlite magmas.One of the possible processes to generate low-Ti-Cr phlogopite is via the replacement of garnet during its interaction with a metasomatic agent enriched in K and H_2O.Rb-Sr isotopic data indicates that the metasomatic agent had a contribution of more radiogenic source than the host-kimberlite magma.Compared with peridotite xenoliths,eclogite xenoliths feature low-Ti phlogopites that are depleted in Cr_2O_3 despite a wider range of TiO_2 concentrations.The presence of phlogopite in eclogite xenoliths indicates that metasomatic processes affected peridotite as well as eclogite within the SCLM beneath the Grib kimberlite.Phl2 has high Ti and Cr concentrations(TiO_22 wt.%,Cr_2O_31 wt.% and Mg# = 100× Mg/(Mg + Fe)92)and compositionally overlaps with phlogopite from polymict brecc:ia xenoliths that occur in global kimberlite formations.These phlogopites are the product of kimberlitic magma and mantle rock interaction at mantle depths where Phl2 overgrew Phil grains or crystallized directly from stalled batches of kimberlitic magmas.Megacrysts,most macrocrysts and microcrysts are disintegrated phlogopite fragments from metasomatised peridotite and eclogite xenoliths.Fine phlogopite flakes within kimberlite groundmass represent mixing of high-Ti-Cr phlogopite antecrysts and high-Ti and low-Cr kimberlitic phlogopite with high Al and Ba contents that may have formed individual grains or overgrown antecrysts.Based on the results of this study,we propose a schematic model of SCLM metasomatism involving phlogopite crystallization,megacryst formation,and genesis of kimberlite magmas as recorded by the Grib pipe. 相似文献
18.
The assembly of supercontinents should impact mantle flow fields significantly, affecting the distribution of subduction, upwelling plumes, lower mantle chemical heterogeneities, and thus plausibly contributing to voluminous volcanism that is often associated with their breakup. Alternative explanations for this volcanism include insulation by the continent and thus elevated subcontinental mantle temperatures. Here we model the thermal and dynamic impact of supercontinents on Earth-like mobile-lid convecting systems. We confirm that insulating supercontinents (over 3000 km extent) can impact mantle temperatures, but show the scale of temperature anomaly is significantly less for systems with strongly temperature-dependent viscosities and mobile continents. Additionally, for continents over 8000 km, mantle temperatures are modulated by the development of small-scale convecting systems under the continent, which arise due to inefficient lateral convection of heat at these scales. We demonstrate a statistically robust association between rising plumes supercontinental interiors for a variety of continental configurations, driven largely by the tendency of subducting slabs to lock onto continental margins. The distribution of slabs also affects the spatial positioning of deep mantle thermochemical anomalies, which demonstrate stable configurations in either the sub-supercontinent or intraoceanic domains. We find externally forced rifting scenarios unable to generate significant melt rates, and thus the ultimate cause of supercontinent breakup related volcanism is probably related to dynamic continental rifting in response to mantle reconfiguration events. 相似文献
19.
Mantle plumes originating from the Core-Mantle Boundary(CMB) or the Mantle Transition Zone(MTZ) play an important role in material transfer through Earth's interior.The hotspot-related plumes originate through different mechanisms and have diverse processes of material transfer.Both the Morganian plumes and large low shear wave velocity provinces(LLSVPs) are derived from the D " layer in the CMB,whereas the Andersonian plumes originate from the upper mantle.All plumes have a plume head at the Moho,although the LLSVPs have an additional plume head at the MTZ.We compare the geochemical characteristics of various plumes in an attempt to evaluate the material exchange between the plumes and mantle layers.The D" layer,the LLSVPs and the Morganian plumes are consisted of subducted slab and post-perovskite from the lower mantle.Bridgmanite would crystallize during the upwelling process of the LLSVPs and the Morganian plumes in the lower mantle,and the residual is a basalt-trachyte suite.Unlike the Morganian plumes,the crystallization in the LLSVPs is insufficient that material accumulates beneath the MTZ to form a plume head.Typically,the secondary plumes above the plume head occur at the edge of the LLSVPs because it is easier for bridgmanite crystal separating from the plume head at the edge,and the residual material with low density upwells to form the secondary plumes.Meanwhile,Na and K are enriched during the long-term crystallization process,and then the basalt-phonolite suite appears in the LLSVPs.The geochemical characteristics of Andersonian plumes suggest that the basalt-rhyolite suite is the major component in the upper mantle.Meanwhile the basalt-rhyolite suite also appears in the LLSVPs and the Morganian plumes because of the assimilation and contamination in the plume head beneath the Mono. 相似文献
20.
通过地幔粘滞性及粘滞结构、地幔热状态、地幔热生成三个方面，探讨了地幔物质发生对流的物理背景，并归纳出地幔对流模式热动力系统，在此基础上剖柏了地幔对流和现代板块构造的直接联系。 相似文献
|
