胶南桃行超高压变质岩的氧同位素地球化学及其年代学制约     

龚冰郑永飞  吴元保 《岩石学报》2004,20(5):1097-1115

对苏鲁超高压变质带内诸城桃行地区榴辉岩及其花岗片麻岩围岩进行了单矿物氧同位素组成分析和锆石U-Pb定年。氧同位素组成显示出不均一亏损~(18)O的特征。石英-石榴石等高温矿物对的氧同位素温度为600～950℃,指示它们在榴辉岩相变质条件下达到并保存了氧同位素平衡。而部分石英-长石和白云母-金红石等矿物对的氧同位素温度为350～570℃,指示它们在峰期变质之后的角闪岩相退变质过程中达到并保存了同位素退化交换再平衡。锆石氧同位素组成低达-1.3‰～4.2‰,对这种低δ~(18)O值进行锆石U-Pb定年,分别得到762～834Ma的原岩年龄和202～249Ma的变质年龄。因此,桃行低δ~(18)O值锆石形成于新元古代(700～800Ma)的低δ~(18)O值岩浆。这种低δ~(18)O值岩浆是由于变质岩原岩经历新元古代高温大气降水热液蚀变后再部分熔融所形成。对于在角闪岩相退变质之后保存了封闭体系的花岗片麻岩样品(石英-长石矿物对温度为355～405℃),石榴石在榴辉岩相变质温度下达到并保存了氧同位素平衡(石英-石榴石矿物对温度为685℃),指示石榴石中Sm-Nd体系在同样的变质务件下也达到了平衡。因此,花岗片麻岩中石榴石-斜长石-全岩的Sm-Nd等时线年龄215±11Ma与锆石变质边的三叠纪年龄(202～249Ma)一样,代表了榴辉岩相峰期变质后的冷却年龄。而花岗片麻岩中石英-钾长石和石英-斜长石矿物对处于氧同位素不平衡状态,同时钾长石和斜长石相对于样品中其它矿物异常亏损~(18)O,指示在角闪岩相退变质之后体系曾经开放,岩石受到低~(18)O流体在低温和中温下(200～400℃)的热液蚀变。这种奈件下矿物氧同位素的退化交换是由表面反应机制控制,与Nd的扩散机制不同,因此氧同位素平衡无法制约Sm-Nd矿物等时线的有效性。  相似文献   

Chloritoid and barroisite-bearing pelitic schists from the eclogite unit in the Besshi district, Sanbagawa metamorphic belt     

Zaw Win Ko  M. Enami  M. Aoya   《Lithos》2005,81(1-4):79-100

The Sanbagawa metamorphic rocks in the Besshi district, central Shikoku, are grouped into eclogite and noneclogite units. Chloritoid and barroisite-bearing pelitic schists occur as interlayers within basic schist in an eclogite unit of the Seba area in the Sanbagawa metamorphic belt, central Shikoku, Japan. Major matrix phases of the schists are garnet, chlorite, barroisite, paragonite, phengite, and quartz. Eclogite facies phases including chloritoid and talc are preserved only as inclusions in garnet. P–T conditions for the eclogite facies stage estimated using equilibria among chloritoid, barroisite, chlorite, interlayered chlorite–talc, paragonite, and garnet are 1.8 GPa/520–550 °C. Zonal structures of garnet and matrix amphibole show discontinuous growth of minerals between their core and mantle parts, implying the following metamorphic stages: prograde eclogite facies stage→hydration reaction stage→prograde epidote–amphibolite stage. This metamorphic history suggests that the Seba eclogite lithologies were (1) juxtaposed with subducting noneclogite lithologies during exhumation and then (2) progressively recrystallized under the epidote–amphibolite facies together with the surrounding noneclogite lithologies.

The pelitic schists in the Seba eclogite unit contain paragonite of two generations: prograde phase of the eclogite facies included in garnet and matrix phase produced by local reequilibration of sodic pyroxene-bearing eclogite facies assemblages during exhumation. Paragonite is absent in the common Sanbagawa basic and pelitic schists, and is, however, reported from restricted schists from several localities near the proposed eclogite unit in the Besshi district. These paragonite-bearing schists could be lower-pressure equivalents of the former eclogite facies rocks and are also members of the eclogite unit. This idea implies that the eclogite unit is more widely distributed in the Besshi district than previously thought.  相似文献   

Pressure dependence and anisotropy of P-wave velocities in ultrahigh-pressure metamorphic rocks from the Dabie–Sulu orogenic belt (China): Implications for seismic properties of subducted slabs and origin of mantle reflections     

Qin Wang  Shaocheng Ji  Matthew H. Salisbury  Bin Xia  Mingbao Pan  Zhiqin Xu 《Tectonophysics》2005,398(1-2):67-99

The compressional wave velocities (Vp), pressure derivatives (Vp′) and anisotropy (A) of three types of eclogites and country rocks from the Dabie–Sulu ultrahigh-pressure (UHP) metamorphic belt, China, have been measured under confining pressures up to 800 MPa. Type-1 eclogites, which are coarse-grained and subjected to almost no retrograde metamorphism, experienced recovery-accommodated dislocation creep at peak metamorphic conditions (in the diamond stability field). Type-2 eclogites are fine-grained reworked Type-1 materials that experienced recrystallization-accommodated dislocation creep under quartz/coesite boundary conditions during the early stage of exhumation. Type-3 eclogites are retrogressed samples that were overprinted by significant amphibolite facies metamorphism during a late stage of exhumation within the crust. Type-1 eclogites are richer in Al₂O₃ and MgO but poorer in SiO₂ and Na₂O than Type-2 and Type-3 eclogites. Anisotropy of Type-1 and Type-2 eclogites is generally low (<4%) because volumetrically important garnet is elastically quasi-isotropic, while Type-3 eclogites can exhibit high anisotropy (>10%) due to the presence of strongly anisotropic retrograde minerals such as amphibole, plagioclase and mica. The transition of the pressure dependence of velocity from the poroelastic to elastic regimes occurs at a critical pressure (P_c), which depends mainly on the density and distribution of microcracks and in turn on the exhumation history of rocks. The Vp–pressure relationship can be expressed by Vp=a(lnP)²+blnP+c (P≤P_c) and Vp=V₀+DP (P≥P_c), where P is the confining pressure, a and b are constants describing the closure of microcracks below P_c, c is the velocity when P is equal to one (MPa), V₀ is the projected velocity of a crack-free sample at room pressure, and D is the intrinsic pressure derivative above P_c. When data are curve-fit, pressure derivatives and anisotropy as functions of pressure are determined. The average Vp of the eclogites in the linear regime is 8.42+1.41×10⁻⁴P for Type-1, 7.80+1.58×10⁻⁴P for Type-2, and 7.33+2.04×10⁻⁴P for Type-3, where Vp is in km/s and P in MPa. The decrease in V₀ and increase in D from Type-1 to Type-3 eclogites are attributed to a decrease in garnet content and an increase in retrograde minerals. The NE–SW trending, NW-dipping, slab-like high Vp anomaly (8.72 km/s at a depth of 71 km) which extends from the Moho to at least 110 km beneath the Dabie–Sulu region, can be interpreted as the remnant of a subducted slab which is dominated by Type-1 eclogites and has frozen in the upper mantle since about 200–220 Ma. Such relic crustal materials, subducted and preserved as eclogite layers intercalated with felsic gneiss, garnet–jadeite quartzite, marble and serpentinized peridotite, could be responsible for regionally observed seismic reflectors in the upper mantle.  相似文献   

Petrology of highly aluminous xenoliths from kimberlites of Yakutia     

Z.V. Spetsius   《Lithos》2004,77(1-4):525-538

Highly aluminous xenoliths include kyanite-, corundum- and coesite-bearing eclogites, grospydites and alkremites. These xenoliths are present in different kimberlites of Yakutia but have most often been found in Udachnaya and other pipes of the central Daldyn–Alakitsky region. Kimberlites of this field also contain eclogite-like xenoliths with kyanite and corundum that originate in the lower crust or the lower crust–upper mantle transition zone. Petrographic study shows that two rock groups of different structure and chemistry can be distinguished among kyanite eclogites: fine- to medium-grained with mosaic structure and coarse-grained with cataclastic structure. Eclogites with mosaic structure are characterized by the occurrences of symplectite intergrowths of garnet with kyanite, clinopyroxene and coesite; only in this group do grospydites occur. In cataclastic eclogites, coarse-grained coesite occurs, corresponding in size to other rock-forming minerals. Highly aluminous xenoliths differ from bimineralic eclogites in their high content of Al₂O₃ and total alkali content. Coesite-bearing varieties are characterized by low MgO content and higher Na/K and Fe²⁺/Fe³⁺ ratios, as well as high contents of Na₂O. Geochemical peculiarities of kyanite eclogites and other rocks are exhibited by a sloping chondrite-normalized distribution of rare earth elements (REE) in garnets and low Y/Zr ratio, in contrast to bimineralic rocks. Coesite is found in more than 20 kyanite eclogites and grospydites from Udachnaya. Grospydites with coesite from Zagadochnaya pipe are described. Three varieties of coesite in these rocks are distinguished: (a) subhedral grains with size of 1.0–3.0 mm; (b) inclusions in the rock-forming minerals; (c) sub-graphic intergrowths with garnet. The presence and preservation of coesite in eclogites indicate both high pressure of formation (more than 30 kbar) and set a number of constraints on the timing of xenolith cooling during entrainment and transport to the surface. Different ways of formation of the highly aluminous eclogites are discussed. Petrographic observations and geochemistry suggest that some highly aluminous rocks have formed as a result of crystallization of anorthosite rocks in abyssal conditions. δ¹⁸O-estimations and other petrologic evidence point out the possible origin of some of these xenoliths as the result of subduction of oceanic crust. Diamondiferous samples have been found in all varieties except alkremites. Usually these eclogites contain cubic or coated diamonds. However, two sample corundum-bearing eclogites with diamonds from the Udachnaya pipe contain octahedra that show evidence of resorption.  相似文献   

Kimberlite AT-56: a mantle sample from the north central Superior craton, Canada     

K.A. Armstrong  T.E. Nowicki  G.H. Read 《Lithos》2004,77(1-4):695-704

Kimberlite AT-56, discovered in February 2001, represents the most recent addition to the Attawapiskat kimberlite cluster, located in the James Bay Lowlands of Ontario, Canada. AT-56 is a small kimberlite body with a surface diameter of approximately 40 m and a steep southeastern plunge. It consists of a medium to coarse-grained matrix supported kimberlite with abundant olivine, clinopyroxene, garnet, ilmenite and mica macrocrysts in a green-black to orange-black matrix. The kimberlite is classified as a hypabyssal facies sparsely macrocrystic calcite kimberlite. Heavy mineral concentrates from two representative samples of AT-56 have been analyzed to characterize the mantle sampled by the kimberlite. Both samples yielded large heavy mineral concentrates comprised of roughly equal proportions of Mg-ilmenite, Cr-diopside, high-Cr garnet and low-Cr garnet. Mg-chromite is also present in quantities an order of magnitude less than the other constituents.

The high-Cr peridotitic garnet macrocrysts are only slightly more abundant than the low-Cr varieties, the population being dominated by G9 (lherzolitic) types with only a few (less than 10%) weakly sub-calcic G10 (probable harzburgitic) garnets present. Ni thermometry results for a representative selection of G9 and G10 garnets indicate that the majority equilibrated at temperatures ranging from 1000 to 1250 °C. A significant proportion of the low-Cr garnet population derived from AT-56 is characterized by relatively low-Ti (0.2 to 0.4 wt.% TiO₂) and elevated Na (0.07 to 0.13 wt.% Na₂O) contents characteristic of Group 1, diamond inclusion type eclogite garnets. These sodic garnets have elevated Cr₂O₃ contents (typically 1 to 2 wt.% Cr₂O₃), suggesting they may be websteritic in origin rather than eclogitic. Comparison of AT-56 garnet compositions with published data available for other Attawapiskat kimberlites suggests websteritic mantle has also been sampled by kimberlite bodies elsewhere in the Attawapiskat cluster and it may be an important diamond reservoir in this area.  相似文献   

Integrated models of diamond formation and craton evolution   总被引：4，自引：0，他引：4  

Steven B. Shirey  Stephen H. Richardson  Jeffrey W. Harris   《Lithos》2004,77(1-4):923-944

Two decades of diamond research in southern Africa allow the age, average N content and carbon composition of diamonds, and the dominant paragenesis of their syngenetic silicate and sulfide inclusions to be integrated on a cratonwide scale with a model of craton formation. Individual eclogitic sulfide inclusions in diamonds from the Kimberley area kimberlites, Koffiefontein, Orapa and Jwaneng have Re–Os isotopic ages that range from circa 2.9 Ga to the mid-Proterozoic and display little correspondence with the prominent variations in the P-wave velocity (±1%) that the mantle lithosphere shows at depths within the diamond stability field (150–225 km). Silicate inclusions in diamonds and their host diamond compositions for the above kimberlites, Finsch, Jagersfontein, Roberts Victor, Premier, Venetia, and Letlhakane show a regional relationship to the seismic velocity of the lithosphere. Mantle lithosphere with slower P-wave velocity relative to the craton average correlates with a greater proportion of eclogitic vs. peridotitic silicate inclusions in diamond, a greater incidence of younger Sm–Nd ages of silicate inclusions, a greater proportion of diamonds with lighter C isotopic composition, and a lower percentage of low-N diamonds. The oldest formation ages of diamonds support a model whereby mantle that became part of the continental keel of cratonic nuclei first was created by middle Archean (3.2–3.3 Ga or older) mantle depletion events with high degrees of melting and early harzburgite formation. The predominance of eclogitic sulfide inclusions in the 2.9 Ga age population links late Archean (2.9 Ga) subduction–accretion events to craton stabilization. These events resulted in a widely distributed, late Archean generation of eclogitic diamonds in an amalgamated craton. Subsequent Proterozoic tectonic and magmatic events altered the composition of the continental lithosphere and added new lherzolitic and eclogitic diamonds to the already extensive Archean diamond suite. Similar age/paragenesis systematics are seen for the more limited data sets from the Slave and Siberian cratons.  相似文献   

Nature of diamonds in Yakutian eclogites: views from eclogite tomography and mineral inclusions in diamonds   总被引：1，自引：0，他引：1  

Mahesh Anand  Lawrence A. Taylor  Kula C. Misra  William D. Carlson  Nikolai V. Sobolev 《Lithos》2004,77(1-4):333-348

We have performed dissections of two diamondiferous eclogites (UX-1 and U33/1) from the Udachnaya kimberlite, Yakutia in order to understand the nature of diamond formation and the relationship between the diamonds, their mineral inclusions, and host eclogite minerals. Diamonds were carefully recovered from each xenolith, based upon high-resolution X-ray tomography images and three-dimensional models. The nature and physical properties of minerals, in direct contact with diamonds, were investigated at the time of diamond extraction. Polished sections of the eclogites were made, containing the mould areas of the diamonds, to further investigate the chemical compositions of the host minerals and the phases that were in contact with diamonds. Major- and minor-element compositions of silicate and sulfide mineral inclusions in diamonds show variations among each other, and from those in the host eclogites. Oxygen isotope compositions of one garnet and five clinopyroxene inclusions in diamonds from another Udachnaya eclogite (U51) span the entire range recorded for eclogite xenoliths from Udachnaya. In addition, the reported compositions of almost all clinopyroxene inclusions in U51 diamonds exhibit positive Eu anomaly. This feature, together with the oxygen isotopic characteristics, is consistent with the well-established hypothesis of subduction origin for Udachnaya eclogite xenoliths. It is intuitive to expect that all eclogite xenoliths in a particular kimberlite should have common heritage, at least with respect to their included diamonds. However, the variation in the composition of multiple inclusions within diamonds, and among diamonds, from the same eclogite indicates the involvement of complex processes in diamond genesis, at least in the eclogite xenoliths from Yakutia that we have studied.  相似文献   

两类榴辉岩的石榴石变形特征差异——来自TEM研究的证据   总被引：9，自引：4，他引：9  

刘祥文金振民  金淑燕曲晶　徐薇 《岩石学报》2005,21(2):411-420

大陆碰撞造山带中超高压榴辉岩从变形程度上通常可以分为面理化榴辉岩和块状榴辉岩两类。本文利用透射电子显微镜对中国大陆科学钻探主孔岩心中面理化榴辉岩和块状榴辉岩的石榴石变形特征进行了比较研究。结果表明:(1)面理化榴辉岩中石榴石的位错密度比块状榴辉岩中石榴石的位错密度高大约3个数量级,位错密度达1.2×1010/cm2。并且有水分子团与高密度位错共存,表明主导石榴石发生强烈塑性变形的机制为水弱化的位错滑移。(2)块状榴辉岩中石榴石的位错密度低,没有观察到水分子团,虽然在局部发现有位错网,但总体上仍呈刚性。(3)两类榴辉岩的石榴石中占主导地位的位错滑移系都是1/2<111>{110},其次为<100>{010}。本文对变形石榴石晶体中水的赋存状态、水弱化机制及变形石榴石形态优选方位与晶格优选方位不协调问题进行了讨论:(1)水在石榴石晶体中有三种可能赋存状态:第一种是吸附于位错管道中的极化水分子;第二种是通过晶体表面以及位错管道扩散进入晶格的间隙水分子;第三种是以4OH-替代SiO44-形式的结构水。(2)石榴石水弱化机制有两种可能:一种是水弱化促进的位错滑移机制,在面理化榴辉岩石榴石的塑性变形中起主导作用;另一种是水弱化促进的扩散和颗粒边界滑移机制,在面理化榴辉岩石榴石的塑性变形中只起次要作用。(3)变形石榴石不产生明显的LPO是由其晶体结构本身特征所决定的,并不能排除其主导变形机制仍然是位错滑移的可能性。  相似文献   

苏北青龙山超高压变质榴辉岩流体包裹体特征与流体演化   总被引：3，自引：7，他引：3  

翟伟孙晓明  徐莉张泽明  梁金龙梁业恒 沈昆 《岩石学报》2005,21(2):482-488

根据青龙山超高压变质榴辉岩中流体包裹体的化学成分、矿物中的分布特征将岩石中的流体包裹体分为五类,即富N2包裹体、高盐度(22.4-略大于23.2wt%NaCl)的NaCl CaCl2 H2O体系流体包裹体、中高盐度(12.6-16.0wt%NaCl)的含Mg2 或Fe2 的NaCl H2O体系流体包裹体、中等盐度(6.4-10.5wt%NaCl)水溶液包裹体和低盐度(3.3-0.2wt%NaCl)的水溶液包裹体。富N2包裹体形成于超高压变质峰期阶段,高盐度的流体包裹体形成于超高压变质岩折返早期固体出溶体出溶阶段,中高盐度的流体包裹体形成于高压变质重结晶作用阶段,中等盐度的流体包裹体形成于角闪岩相变质重结晶作用阶段,低盐度的流体包裹体形成于折返晚期的绿片岩退变质作用阶段。超高压变质峰期阶段和折返早期的高盐度流体和中高盐度的流体主要来自继承原岩中的流体(如含NH4 矿物分解或片麻岩原岩中的有机质分解,名义上无水矿物中羧基水的出溶),晚期角闪岩相退变质阶段的中等盐度的流体除名义上无水矿物中羟基水的出溶外还有外来流体的加入,绿片岩相退变质作用阶段的流体主要为外来流体。  相似文献   

大别-苏鲁区超高压变质岩的多期构造变质演化   总被引：3，自引：0，他引：3  

索书田  钟增球周汉文游振东 《岩石学报》2005,21(4):1175-1188

对大别-苏鲁地区超高压(UHP)变质岩的详细构造和岩石学研究揭示了其复杂的构造变质演化历史。除前超高压事件外,至少可识别出5个相继发育的构造变质事件或阶段(D_1-D_5)。D_1和 D_2同超高压事件与三叠纪(250～230Ma)中朝克拉通和扬子克拉通间的大陆深俯冲及碰撞有关,而超高压后的 D_3和 D_4韧性变形及其伴生的减压部分熔融作用和退变质作用事件,则是超高压岩石向中上地壳折返过程中(230～140Ma)发生的。碰撞后形成的 D_4构造,主导了大别-苏鲁超高压和高压变质带区域尺度的构造格架。第5阶段的构造以摩擦或摩擦-粘性过渡性变形机制为主,并伴随有大规模的未变形的花岗质岩体就位,该期构造热事控制了现今大别-苏鲁地区的地貌学特征。新的构造和岩石学资料并结合可利用的地质年代学和地球化学等资料,提出一个涉及中朝与扬子克拉通间三叠纪大陆深俯冲、碰撞及相继超高压变质岩石向地表的多期折返构造变质演化模式。  相似文献