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31.
《Chemie der Erde / Geochemistry》2015,75(1):1-28
Enstatite-rich meteorites include EH and EL chondrites, rare ungrouped enstatite chondrites, aubrites, a few metal-rich meteorites (possibly derived from the mantle of the aubrite parent body), various impact-melt breccias and impact-melt rocks, and a few samples that may be partial-melt residues ultimately derived from enstatite chondrites. Members of these sets of rocks exhibit a wide range of impact features including mineral-lattice deformation, whole-rock brecciation, petrofabrics, opaque veins, rare high-pressure phases, silicate darkening, silicate-rich melt veins and melt pockets, shock-produced diamonds, euhedral enstatite grains, nucleation of enstatite on relict grains and chondrules, low MnO in enstatite, high Mn in troilite and oldhamite, grains of keilite, abundant silica, euhedral graphite, euhedral sinoite, F-rich amphibole and mica, and impact-melt globules and spherules. No single meteorite possesses all of these features, although many possess several. Impacts can also cause bulk REE fractionations due to melting and loss of oldhamite (CaS) – the main REE carrier in enstatite meteorites. The Shallowater aubrite can be modeled as an impact-melt rock derived from a large cratering event on a porous enstatite chondritic asteroid; it may have been shock melted at depth, slowly cooled and then excavated and quenched. Mount Egerton may share a broadly similar shock and thermal history; it could be from the same parent body as Shallowater. Many aubrites contain large pyroxene grains that exhibit weak mosaic extinction, consistent with shock-stage S4; in contrast, small olivine grains in some of these same aubrites have sharp or undulose extinction, consistent with shock stage S1 to S2. Because elemental diffusion is much faster in olivine than pyroxene, it seems likely that these aubrites experienced mild post-shock annealing, perhaps due to relatively shallow burial after an energetic impact event. There are correlations among EH and EL chondrites between petrologic type and the degree of shock, consistent with the hypothesis that collisional heating is mainly responsible for enstatite-chondrite thermal metamorphism. Nevertheless, the apparent shock stages of EL6 and EH6 chondrites tend to be lower than EL3-5 and EH3-5 chondrites, suggesting that the type-6 enstatite chondrites (many of which possess impact-produced features) were shocked and annealed. The relatively young Ar–Ar ages of enstatite chondrites record heating events that occurred long after any 26Al that may have been present initially had decayed away. Impacts remain the only plausible heat source at these late dates. Some enstatite meteorites accreted to other celestial bodies: Hadley Rille (EH) was partly melted when it struck the Moon; Galim (b), also an EH chondrite, was shocked and partly oxidized when it accreted to the LL parent asteroid. EH, EL and aubrite-like clasts also occur in the polymict breccias Kaidun (a carbonaceous chondrite) and Almahata Sitta (an anomalous ureilite). The EH and EL clasts in Kaidun appear unshocked; some clasts in Almahata Sitta may have been extensively shocked on their parent bodies prior to being incorporated into the Almahata Sitta host. 相似文献
32.
Bernard Peybernès Marie-José Fondecave-Wallez Pierre-Jean Combes 《Comptes Rendus Geoscience》2003,335(3):335-344
The post-metamorphic breccias which underline the frontal overthrust of the ‘Marble Zone’ (Basque–Cantabrian Pyrenees, Province of Navarre, Spain), interpreted by P. Lamare as ‘mylonites’, correspond to sedimentary breccias of submarine canyon, filling former incised valleys dug within the metamorphic Jurassic/Early Cretaceous carbonates already folded and cleaved (Pyrenean Cretaceous tectorogen). Associated to microrhythmic hemipelagites containing Danian–Selandian planktonic foraminifera from the P1c–P3 interval, these breccias are now assigned to Palaeocene. Stratified and horizontal, they seal Late-Cretaceous structures, of which the overthrusting front of the ‘Marble Zone’ could be the principal regional element. 相似文献
33.
松辽盆地南部长岭断陷为古生界变质基底上发育的箕状断陷,沙河子组发育厚度较大的深湖相黒色泥岩,有机质丰度高,热演化程度高,生烃强度大,具备很好的天然气资源基础.断陷期发育2套火山岩,其中营城组爆发相、溢流相火山岩大面积分布,岩性以酸性流纹岩、凝灰岩、火山角砾岩等为主,孔洞发育,储集物性较好.长岭断陷东部发育2个大型古隆起,断裂发育,天然气运聚条件较好,目前已发现3个气藏3个含气构造,是寻找大型天然气藏的最有利地区. 相似文献
34.
安徽沿江地区古生代—中生代地层发育较为完整,印支构造变形表现最为强烈。印支晚期南象运动已成为公认的事实,而早期金子运动存在与否及其地质界面一直存在较大的争议。本文通过关键界面的考查、角砾岩特征及成因,以及岩相古地理的演化的分析,初步认为安徽沿江地区印支运动早期金子运动确实存在,其构造界面位于周冲村组与黄马青组之间,以平行不整合或微角度不整合接触关系为表现形式,其构造样式以构造抬升为主,盆地边界以宽缓的褶皱变形为辅。该运动与南象运动(大规模的褶皱造山)共同控制了沿江地区构造格架的形成和发展。 相似文献
35.
Three types of periglacial deposits (breccias, stratified breccias and grèzes litées are described from Córdoba Province in southern Spain. Their physico-chemical properties, in particular clay mineralogy in relation to terra rossas in the area, indicate two different ages for these deposits. Younger terra rossas and younger periglacial deposits contain illite and kaolinite whereas older terra rossas and older periglacial deposits contain vermiculite and kaolinite. Geomorphological evidence (altitude and relationships to the surfaces described by earlier authors in southern Spain) indicate approximate ages for the deposits. Secondary carbonate from one of the younger breccias gave a uranium series date of 80 000 yr BP, suggesting that some of the younger breccias were deposited in a periglacial climate before 80 000 BP. © 1997 John Wiley & Sons, Ltd. 相似文献
36.
Alain Blot 《Comptes Rendus Geoscience》2002,334(12):909-915
There are many small ferruginous outcrops of different facies, often breccia-like, in the Neoproterozoic sedimentary formations in northern Burkina. These outcrops are made up of goethite and quartz, and are often along with high grades of various elements. It could be a question of gossans. Their large distribution in this part of the Taoudéni Basin offers it prospects as a province geochemically rich in Cu, Pb, Zn, Mo, As, Cd, Co... This basin would be a geochemical bin for ancient formations, which would have been evacuated before the Neoproterozoic. The ironstones would be the mark of further concentrations. To cite this article: A. Blot, C. R. Geoscience 334 (2002) 909–915. 相似文献
37.
《Chemie der Erde / Geochemistry》2019,79(4):125532
For the bulk rocks of CI chondrites, various values are given for the modal abundance of matrix (95–100 vol%) and the accompanying mineral constituents. Here, we have determined the modal abundance of phases >5 μm in the CI chondrites Orgueil, Ivuna, Alais, and Tonk. Considering this cut-off grain-size to distinguish between matrix and coarse-grained constituents, then, we find the modal abundance of the minor phases magnetite, pyrrhotite, carbonate, olivine, and pyroxene to be 6 vol% in total, and these phases are embedded within the fine-grained, phyllosilicate-rich matrix, making up 94 vol%. The values vary slightly from meteorite to meteorite. Considering all four chondrites, the most abundant phase is - by far - magnetite (4.3 vol%) followed by pyrrhotite (∼1.1 vol%). All four CI chondrites are complex breccias, and their degree of brecciation decreases in the sequence: Orgueil > Ivuna > Alais ∼ Tonk. Because these meteorites contain clasts with highly variable modal abundances, we therefore also studied individual clasts with high abundances of specific coarse-grained phases. In this respect, in Orgueil we found a fragment with a 21.5 vol% of magnetite as well as a clast having 31.8 vol% phosphate. In Ivuna, we detected an individual clast with a 21.5 vol% of carbonates. Thus, since the CI composition is used as a geochemical standard for comparison, one also should keep in mind that sufficiently large sample masses are required to reveal a homogeneous CI composition. Small aliquots with one dominating lithology may significantly deviate from the suggested standard CI composition. 相似文献
38.
Pierre-Jean Combes Bernard Peybernès Marie-José Fondecave-Wallez 《Eclogae Geologicae Helvetiae》2004,97(2):155-174
In the Eastern part of French Pyrenees, the Cucugnan area (Southern Corbières) corresponded during the early/Mid-Paleocene (Danian/Selandian) to a narrow transitional zone between the sea to the South (Pyrenean Paleocene Trough) and the continent (fluvio-palustrine and lacustrine Vitrollian deposits) to the North. To the South, in the North-Pyrenean Zone, the polygenic marine breccias and the associated Dano-Selandian Globigerinid-bearing hemipelagites have been preserved within successive paleokarsts superimposed onto the carbonate substratum (ante-Albian). Four paleosurfaces are recognized, principally filled by marine internal sediments with proximal and distal facies. To the North, in the Sub-Pyrenean Zone, a continental foreland basin is characterized by four formations of variegated Microcodium-bearing marls and channelized conglomerates, separated by erosional paleosurfaces underlining well-marked unconformities. An event correlation (chronodiagrams) between the marine realm to the South and the continental realm to the North is proposed, using the successive paleosurfaces and the lithological sequences (same number within the two realms). Our paleogeographic reconstruction shows, to the North, the Lake of Cucugnan and, to the South, a calcareous mountainous zone broken by the juxtaposition of deep paleocanyons (eroded in a continental context) later converted into rias submitted to marine oscillations. Several palinspastic transects are reconstructed: they show the polyphase control of the Frontal North-Pyrenean Overthrust on the Paleocene sedimentation and the importance of the successive intra-Vitrollian compressions/ transpressions (phase fini-crétacée auct.) inducing, within the two juxtaposed realms, emersions, erosions and karstic features which give a very contrasted paleogeography during a period characterized by plate convergence and creation of steep topographies.Manuscrit reçu le 25 septembre 2003 Révision acceptée le 4 mai 2004 相似文献
39.
MIL090036 is a previously unknown meteorite （a feldspathic lunar breccia） that was discovered in Antarctica. The detailed petrography and mineralogy of this meteorite forms the subject of this paper. It has a typical clastic texture that consists of various types of rock debris （e.g. anorthosite, gabbroic anorthosite, gabbro, regolith breccia, troctolite, microporphyritic crystalline impact melt and compound clasts）, mineral crystal fragments （e.g. pyroxenes, plagioclase, olivine and ilmenite） and feldspathic glass clasts. The ifne-grained recrystallized minerals and mineral clasts are cemented together in a glassy groundmass. The anorthite content of plagioclase in the gabbro （An81-83） and anorthosite （An88-93） both have relatively low calcium content compared to those from other breccias （An90-98）. The pyroxene composition （Fs12-35 Wo3-44 En22-79） in the rock debris, crystal mineral clasts and anorthositic glass clasts are relatively iron-deifcient compared to those from gabbro debris with melt glass （Fs37-65 Wo10-29 En21-49） and groundmass （Fs18-69 Wo3-45 En14-50）. In contrast, the pyroxene grains in the gabbroic anorthosite display a narrow compositional range （Fs24-27 Wo7-14 En59-69）. Olivine grains in mineral fragments and the groundmass have a wider compositional range （Fo57-79） than those in the rock debris （Fo67-77）. The Fe/Mn ratio in olivine is in the range of 47 to 83 （average 76） and 76 to 112 （average 73） in pyroxenes, and hence classify within the lunar ifeld. The characteristics of texture, mineral assemblage and compositions suggest that MIL090036 possibly originated from a region beyond that of the Apollo and Luna samples. Further study of MIL090036 is therefore likely to lead to a better understanding of the geological processes on the Moon and the chemical composition of the lunar crust. 相似文献
40.
川滇黔交界地区铅锌矿床含矿角砾岩特征及其构造意义 总被引：3，自引：1，他引：2
川滇黔交界地区的铅锌矿床中普遍发育含矿角砾岩。文章综述了角砾岩的成因分类,在重点矿床野外地质调查的基础之上,对川滇黔交界地区的铅锌矿床含矿角砾岩进行了详细研究。结果表明:大部分含矿角砾岩显示张性角砾岩的特点,仅个别矿床同时出现挤压角砾岩。综合区域地质构造演化特征和典型铅锌矿床的同位素测年数据,可大致推断出,从中二叠世茅口期以来该铅锌成矿区伸展构造至少有2期:一期发生在铅锌矿化之前或同时,即早二叠世/晚二叠世的升降运动(东吴运动)与晚二叠世峨眉山玄武岩喷发期间,此次伸展作用形成的角砾岩为成矿流体提供了大量的容矿空间,并最终导致成矿流体沿断裂运移并充填沉淀而形成角砾状或网脉状-脉状构造的矿石;另一期发生在铅锌矿化之后,即白垩纪—古近纪,发育一系列正断层,并有可能破坏了铅锌矿体的连续性。 相似文献