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1.
Partial fusion hypotheses have been proposed for the origin of lherzolite-harzburgite alpine peridotite associations. Analyzed lherzolites from Othris, Ronda, Lanzo and Beni Bouchera, have light REE depleted to chondritic REE abundances, and clinopyroxenes contain most of the REE relative to depleted olivine and orthopyroxene. Variation in the level of REE enrichment within these lherzolites indicates mantle heterogeneity probably caused by partial melting processes. The Beni Bouchera spinel lherzolite and the Othris plagioclase lherzolite are the best candidates for relatively undepleted mantle based on REE studies. Fractional fusion calculations (15–25%) reveal that partial melts have REE characteristics somewhat similar to oceanic tholeiites. Conversely, computed source peridotites from oceanic tholeiites (Schilling, 1975) are similar to the alpine lherzolites reported here. Alpine lherzolites are, however, depleted in trace elements (K, Rb, Sr and Ba, Menzies and Murthy 1976). Since the lherzolites have an undepleted major, minor and REE chemistry close to that of pyrolite, the lost trace element-rich fraction must represent a small degree of melting. It is proposed that alpine lherzolites are residue left after the loss of a nephelinitic/alkalic fraction, ([Ce/Yb]N=2.0–4.01) representing a small degree of partial fusion. This labile fraction may have existed as an intergranular phase or hydrous mineral prior to melting.  相似文献   

2.
The author describes a new occurrence of garnet peridotite and garnet pyroxenite interlayered in the biotite-sillimanite-garnet gneisses at the top of the granulitic serie of the Monts du Lyonnais (Massif Central français). Its dimensions are rather significant for a crustal gisement (500×100 m). It is only composed of forsterite, enstatite, chromiferous diopside, pyrope and spinel peridotites with their products of retrograde transformations as kelyphites, amphiboles, chlorites, lizardite, ores, etc. The petrographic studies show the heterogeneity of the massif and the anteriority of the red spinel upon the garnet which always forms a corona around the spinel. The peridotites are intermingled with numerous streched and dislocated layers of garnet websterites with rare centimetric levels. These pyroxenites would be derived of particular magmatic processes (partial anatectic melting followed by cristallisation) developped from an upper mantle level in a primary pyrolitic lherzolitic (s. l) or garnet peridotitic material. The garnet peridotite of “Le Bois des Feuilles” would be, in fact, a “secondary garnet lherzolite” derived: - either from a spinel lherzolite intermingled with garnet websterite layers and their “dunitic” remnants, to form a “pseudo-garnet lherzolite” like this of Beni Bouchera described by Kornprobst; - or from a spinel lherzolite associated with garnet websterites and submitted temporarily, at the time of its diapiric rising movement from the mantle towards the crust to the conditions of the spinel garnet lherzolite facies. The plastic deformations and intense laminations form blastomylonites of mixed rocks recristallised ultimately under granulitic facies conditions. These rocks are, pro parte, not very different from the other crustal garnet peridotites, in spite of the frequency of the spinel inclusions in garnet. In corollary, it seems that numerous crustal garnet peridotites would have the same origin.  相似文献   

3.
Field and textural relationships have indicated the tectonic emplacement of the Norwegian garnet peridotites as relatively cold intrusions into their present environment. Mineralogical data demonstrate considerable heterogeneity. Olivines and orthopyroxenes in garnet rich peridotites are significantly more ferriferous than those in garnet free peridotites. Mineralogical features indicate that the mineral assemblages have been equilibrated at subsolidus temperatures. However, the hypothesis that these garnet peridotites have resulted from the eclogite facies metamorphism in deep levels of the crust of other peridotite mineral facies assemblages is considered and rejected.Statistical analysis of the bulk rock composition data has substantiated the existence of a very strong linear composition trend, two end members being sufficient to account for almost the whole range of composition variation.The hypothesis favoured is that these peridotites have been involved in partial melting processes in the upper mantle. The Kalskaret garnet peridotite occurrence is considered to represent a case where the picritic partial melt fraction has not been completely liberated but has remained trapped and mixed with the dunitic residual fraction.  相似文献   

4.
出露于饶拔寨一带的含尖晶石橄榄岩体是大别山区最大的一个上地幔残片,固态侵位于北大别深成片麻岩中,呈无根侵入体的形式产出。岩体内的石榴辉石岩和榴辉岩包体,具高温成因的特点。属于上地幔部分熔融的产物,在Pl-CIPW值对Al_2O_3图解上落于拉斑玄武岩区;榴辉岩、石榴辉石岩和含尖晶石橄榄岩的REE配分形式相似,均属平坦型,只是尖晶石橄榄岩的∑REE较低。在Ni-Co-Sc三组分图解上,石榴辉石岩投绘于深位玄武岩熔体的趋势线附近,而尖晶石橄榄岩的投点则接近超镁铁质残余的趋势,清楚揭示出地幔部分熔融的迹象。尖晶石的Cr~#=12～21,而共生橄榄石Fo=92～93,说明部分熔融程度不高,估计约15％。尖晶石贫TiO_2暗示熔融过程氧逸度低。饶拔赛含尖晶石橄榄岩的出现表明;伴随超高压岩石单元的折返和隆升,会有大陆地幔残片被携带上来。软流圈的上涌或板片的断离使侵出的岩石圈板片得以维持较高的温度,这也就是石榴辉石岩早期深位退变质为麻粒岩相的原因,是后续的进一步抬升,才出现以韭角闪石 斜长石组合为特征的高角闪岩相的退变质作用。  相似文献   

5.
IONOV  DMITRI 《Journal of Petrology》2004,45(2):343-367
Peridotite xenoliths in a Miocene picrite tuff from the Vitimvolcanic province east of Lake Baikal, Siberia, are samplesof the off-craton lithospheric mantle that span a depth rangefrom the spinel to garnet facies in a mainly fertile domain.Their major and trace element compositions show some scatter(unrelated to sampling or analytical problems), which is notconsistent with different degrees of partial melting or metasomatism.Some spinel peridotites and, to a lesser degree, garnet-bearingperidotites are depleted in heavy rare earth elements (HREE)relative to middle REE (MREE), whereas some garnet peridotitesare enriched in HREE relative to MREE, with Lu abundances muchhigher than in primitive mantle estimates. Clinopyroxenes fromseveral spinel peridotites have HREE-depleted patterns, whichare normally seen only in clinopyroxenes coexisting with garnet.Garnets in peridotites with similar modal and major elementcompositions have a broad range of Lu and Yb abundances. Overall,HREE are decoupled from MREE and Hf and are poorly correlatedwith partial melting indices. It appears that elements withhigh affinity to garnet were partially redistributed in theVitim peridotite series following partial melting, with feweffects for other elements. The Lu–Hf decoupling may disturbHf-isotope depletion ages and their correlations with meltingindices. KEY WORDS: garnet peridotite; lithospheric mantle; Lu–Hf isotope system; Siberia; trace elements  相似文献   

6.
Garnet-bearing mantle peridotites, occurring as either xenoliths in volcanic rocks or lenses/massifs in high-pressure and ultrahigh-pressure terrenes within orogens, preserve a record of deep lithospheric mantle processes. The garnet peridotite xenoliths record chemical equilibrium conditions of garnet-bearing mineral assemblage at temperatures (T) ranging from ~700 to 1,400°C and pressures (P) > 1.6–8.9 GPa, corresponding to depths of ~52–270 km. A characteristic mineral paragenesis includes Cr-bearing pyropic garnet (64–86 mol% pyrope; 0–10 wt% Cr2O3), Cr-rich diopside (0.5–3.5 wt% Cr2O3), Al-poor orthopyroxene (0–5 wt% Al2O3), high-Cr spinel (Cr/(Cr + Al) × 100 atomic ratio = 2–86) and olivine (88–94 mol% forsterite). In some cases, partial melting, re-equilibration involving garnet-breakdown, deformation, and mantle metasomatism by kimberlitic and/or carbonatitic melt percolations are documented. Isotope model ages of Archean and Proterozoic are ubiquitous, but Phanerozoic model ages are less common. In contrast, the orogenic peridotites were subjected to ultrahigh-pressure (UHP) metamorphism at temperature ranging from ~700 to 950°C and pressure >3.5–5.0 GPa, corresponding to depths of >110–150 km. The petrologic comparisons between 231 garnet peridotite xenoliths and 198 orogenic garnet peridotites revealed that (1) bulk-rock REE (rare earth element) concentrations in xenoliths are relatively high, (2) clinopyroxene and garnet in orogenic garnet peridotites show a highly fractionated REE pattern and Ce-negative anomaly, respectively, (3) Fo contents of olivines for off-cratonic xenolith are in turn lower than those of orogenic garnet and cratonic xenolith but mg-number of garnet for orogenic is less than that of off-cratonic and on-cratonic xenolith, (4) Al2O3, Cr2O3, CaO and Cr# of pyroxenes and chemical compositions of whole rocks are very different between these garnet peridotites, (5) orogenic garnet peridotites are characterized by low T and high P, off-cratonic by high T and low P, and cratonic by medium T and high P and (6) garnet peridotite xenoliths are of Archean or Proterozoic origin, whereas most of orogenic garnet peridotites are of Phanerozoic origin. Taking account of tectonic settings, a new orogenic garnet peridotite exhumation model, crust-mantle material mixing process, is proposed. The composition of lithospheric mantle is additionally constrained by comparisons and compiling of the off-cratonic, on-cratonic and orogenic garnet peridotite.  相似文献   

7.
Samples of ten eclogites in gneiss, one eclogite in dunite-peridotite, three dunites and four garnet- and dunite-peridotites from the Nordfjord-Molde area, west Norway were analysed for La, Ce, Nd, Sm, Eu, Gd, Tb, Yb and Lu by radiochemical neutron activation analysis.The chondrite normalized REE patterns of eclogites in gneisses show mostly slight enrichment of the heavy REE, which converge towards a value about ten times above the average chondrite. It is suggested that the light REE scatter is due to the original mineralogical composition of the rocks.One garnet-peridotite shows a distribution pattern similar to those reported for high-temperature peridotites while the two others could be compared with that of Lac de Lherz and Still water peridotite.Two of the dunites taken from the same locality show a difference in the individual REE content by a factor of one order of magnitude. This is explained by the higher content of tremolite in the most REE-enriched sample.  相似文献   

8.
The layered cumulus rocks of the Marum ophiolite complex in northern Papua New Guinea range from highly magnesian dunite, wehrlite, and lherzolite through pyroxenite to norite-gabbro with minor anorthosite and ferronorite-gabbro near the top of the sequence. Most of the cumulates, particularly the gabbroic rocks, are characterised by recrystallised adcumulus textures and all intercumulus melt (mesostasis) has been expelled. Trends in the cumulate sequence from Mg-rich to more Fe-, Ca- and Al-rich compositions are consistent with the formation of the layered sequence by magmatic accumulation from mafic tholeiitic magmas with varying degrees of differentiation. The cumulates are characterised by extremely low levels of ‘incompatible’ elements (K, Ba, Rb, P, Zr, Nb, Hf, Y and REE) at all levels of differentiation. REE patterns are strongly depleted in LREE; HREE abundances range from ≦0.3 chondrites in peridotite to 3 x chondrites in the norite-gabbros. The Marum cumulates resemble low-Ti peridotites and gabbros found in other orthopyroxene-bearing ophiolite sequences. The parent magmas of the Marum cumulates are inferred to have been strongly depleted in ‘incompatible’ trace elements (～ 2,000 ppm Ti, ～20 ppm Zr, 6–9 x chondrites HREE with LaN/SmN～0.5). These abundances are lower than found in typical MORB and back-arc basin basalts or their picritic parents. The dissimilarity of trace element abundances of the inferred Marum parent magmas with MORB-type high-alumina olivine tholeiites supports the conclusion drawn previously from the petrology of the cumulates that the parent magmas to the Marum ophiolite were not of MORB composition but resembled the strongly depleted, Ni-rich magnesian olivine-poor tholeiites and quartz tholeiites of the Upper Pillow Lavas of the Troodos ophiolite. The Marum parent magmas are believed to have been formed by shallow melting of refractory peridotite, and are chemically and genetically distinct from the LREE-enriched high-Ti lavas (Tumu River basalts) which occur in faulted contact. The geochemical data do not permit unequivocal assignment of a tectonic environment for the formation of either the Tumu River basalts or the plutonic suite; their juxtaposition results from thrust emplacement.  相似文献   

9.
BECKER  HARRY 《Journal of Petrology》1996,37(4):785-810
Gamet-bearing high-temperature peridotite massifs in lower Austriawere exhumed during Carboniferous plate convergence in the Bohemianmassif. The peridotite massifs contain garnet pyroxenite layers,most of which are high-pressure cumulates that crystallizedin the deep lithosphere during ascent and cooling of hot asthenosphericmelts. Many of the pyroxenites have negative Eu anomalies andhigh LREE abundances in pyroxenes and bulk rocks, 87Sr/86Sr(335 Ma) as high as 0.7089, and Nd (335 Ma) as low as –4.8(leached clinopyroxenes and garnets). These pyroxenites alsoshow strong depletions in Rb, K, Ta, P and Ti compared withthe REE Equilibrium melt compositions calculated from the cumulatecompositions have very high LREE abundances (Lan = 300–600)and show strong LREEfractionation [(La/Sm)n = 7–47)].Trace element abundances, the Ca–Al-rich composition ofthe cumulates and possible Ti saturation in the melts suggestthat these melts were of primitive carbonatitic–meliliticor lamprophyrt-like composition. Other garnet pyroxenites suchas Al-rich garnet-kyanite clinopyroxemtes with positive Eu anomaliesprobably represent metamorphosed crustal rocks which were subductedand accreted to the lithospheric mantle. The high 87Sr/86Sr,low Nd (335 Ma) and negative Eu anomalies of the high-pressurecumulates can be explained if their equilibrium melts containeda component derived from subducted upper-crustal rocks. Thehigh equilibration pressures of the host peridotites (3–3.5GPa) and the high equilibration temperatures of the pyroxenites(1100–1400C) indicate that these melts are likely tobe derived from the sub-lithospheric mantle. There, meltingmay have been triggered by small amounts of melt or fluids derivedfrom a subducting slab at greater depth. KEY WORDS: garnet pyroxenites; geochemistry; lower Austria; ultramafic massifs; subduction  相似文献   

10.
We report new textural and chemical data for 10 garnet peridotite xenoliths from the Udachnaya kimberlite and examine them together with recent data on another 21 xenoliths from the 80–220 km depth range. The samples are very fresh (LOI near zero), modally homogeneous and large (>100 g). Some coarse-grained peridotites show incipient stages of deformation with <10 % neoblasts at grain boundaries of coarse olivine. Such microstructures can only be recognized in very fresh rocks, because fine-grained interstitial olivine is strongly affected by alteration, and may have been overlooked in previous studies of altered peridotite xenoliths in the Siberian and other cratons. Some of the garnet peridotites are similar in composition to low-opx Udachnaya spinel harzburgites (previously interpreted as pristine melt extraction residues), but the majority show post-melting enrichments in Fe and Ti. The least metasomatized coarse peridotites were formed by 30–38 % of polybaric fractional melting between 7 and 4 GPa and ≤1–3 GPa. Our data together with experimental results suggest that garnet in these rocks, as well as in some other cratonic peridotites elsewhere, may be a residual mineral, which has survived partial melting together with olivine and opx. Many coarse and all deformed garnet peridotites from Udachnaya underwent modal metasomatism through interaction of the melting residues with Fe-, Al-, Si-, Ti-, REE-rich melts, which precipitated cpx, less commonly additional garnet. The xenoliths define a complex geotherm probably affected by thermal perturbations shortly before the intrusion of the host kimberlite magmas. The deformation in the lower lithosphere may be linked to metasomatism.  相似文献   

11.
The authors report a redox profile based on Mössbauer data of spinel and garnet to a depth of 210 km from mantle xenoliths of the northern (N) and southeastern (SE) Slave craton (northern Canada). The profile transects three depth facies of peridotites that form segments of different bulk composition, represented by spinel peridotite, spinel–garnet peridotite, low-temperature garnet peridotite, high-temperature garnet peridotite, and pyroxenite. The shallow, more depleted N Slave spinel peridotite records lower oxygen fugacities compared to the deeper, less depleted N Slave spinel–garnet peridotite, consistent with their different spinel Fe3+ concentrations. Garnet peridotites show a general reduction in log fO2 (FMQ)s with depth, where values for garnet peridotites are lower than those for spinel–garnet peridotites. There is a strong correlation between depletion and oxygen fugacity in the spinel peridotite facies, but little correlation in the garnet peridotite facies. The strong decrease in log fO2 (FMQ) with depth that arises from the smaller partial molar volume of Fe3+ in garnet, and the observation of distinct slopes of log fO2 (FMQ) with depth for spinel peridotite compared to spinel–garnet peridotite strongly suggest that oxygen fugacity in the cratonic peridotitic mantle is intrinsically controlled by iron equilibria involving garnet and spinel.
C. McCammonEmail: Phone: +49-921-553709Fax: +49-921-553769
  相似文献   

12.
The metamorphic core of the Betic-Rif orogenic chain (Alboran Domain) is made up of lower crustal rocks forming the envelope of the Ronda (Spain) and Beni Bousera (Morocco) peridotites. The deepest sections of the crustal envelopes are made of migmatitic granulites associated with diffuse acidic magmatic products, making these exposure and ideal site to investigate the textural and petrological connection between crustal anatexis and granite magmatism in the contintental crust. However, still debated is the timing of intracrustal emplacement of the peridotite bodies, with models proposing either Alpine (early Miocene) or Hercynian ages, and still uncertain is the linkage between peridotite emplacement and crustal anatexis. In this study, by combining rock textures with whole-rock geochemistry, metamorphic thermobarometry, the U-Pb zircon geochronology and the analysis of the garnet and zircon REE chemistry, we document the P-T-t evolution of the granulite facies migmatites that form the immediate envelope of the Beni Bousera peridotites of the Rif belt. A main episode of Permo-Carboniferous (ca. 300–290 Ma) deep crustal anatexis, melt extraction and migration is documented that we link to the crustal emplacement of the Beni Bousera peridotites during collapse of the Hercynian orogen. Correlation at a regional scale suggests that the Beni-Bousera section can be tentatively correlated with the pre-Alpine (Permo-Carboniferous) basement units tectonically interleaved within the orogenic structure of the Alpine chain. The results of this study provide ultimate constraints to reconstruct the tectono-metamorphic evolution of the Alboran Domain in the Western Mediterranean and impose re-assessment of the modes and rates through which Alpine orogenic construction and collapse occurred and operated in the region.  相似文献   

13.
豆英状铬铁矿按其矿物化学组分分为高铝型(Cr#值为20～ 60)和高铬型(Cr#值为60～80)两类(Thayer,1970),在全球已报道的豆英状铬铁矿中普遍为在一岩体内只存一种类型的矿体,而在同一岩体内发现两种类型的铬铁矿体较少见.位于雅鲁藏布江缝合带西段普兰岩体中首次发现同时存在高铬型和高铝型铬铁矿,岩体由地幔橄榄岩、辉长辉绿岩、火山岩等组成.地幔橄榄岩主要为方辉橄榄岩、纯橄岩和少量二辉橄榄岩.在方辉橄榄岩中发现7处透镜状的铬铁矿矿体露头,矿石类型主要有致密块状、稠密浸染状和稀疏浸染状等.矿体长2～6m,厚0.5～2m,矿体的最大延伸方向为北西-南东向,与岩体的展布方向一致,矿石的Cr#=52～88,高铬型铬铁矿包括Cr-2～5矿体,Cr#值为63～89,高铝型铬铁矿有Cr-1和Cr-6矿体,Cr#=52 ～55.矿石中脉石矿物主要为橄榄石、角闪石、蛇纹石等.普兰地幔橄榄岩的矿物结构显示,岩体经历了强烈的部分熔融以及塑性变形作用,地幔橄榄岩的地球化学特征显示岩体形成于MOR,后受到SSZ环境的改造.并且依据铬尖晶石-橄榄石/单斜辉石的矿物化学成分,识别出普兰地幔橄榄岩至少经历了3次不同的部分熔融,包括早期部分熔融(～10％)、晚期部分熔融(20％～30％)和局部的减压部分熔融作用(～15％).对比其他铬铁矿矿体和地幔橄榄岩的矿物组合,矿物化学和地球化学等,显示普兰豆荚状铬铁矿矿体与典型高铬型、高铝型铬铁矿具相似性,并存在较大的找矿空间.  相似文献   

14.
内蒙古天和永新生代玄武岩成因及其地质意义   总被引：1，自引：0，他引：1       下载免费PDF全文
天和永玄武岩为碧玄岩,至少可以划分出3种矿物共生组合类型。天和永玄武岩总体具有贫硅(w(SiO2)=43.97%～45.68%)、富碱(w(K2O+Na2O)=5.91%～7.65%)、富钾(w(K2O)=2.04%～2.89%)、高钛(w(TiO2)=2.18%～2.37%)、高Mg值(Mg#=68～76)的特征;稀土元素含量高(∑REE=(246.62～329.82)×10-6),稀土配分曲线呈右倾平滑直线,强烈富集轻稀土,轻重稀土强烈分馏((La/Yb)N>30),无明显的Eu(δEu=0.90～1.02)和Ce异常(δCe=0.96～1.00);强烈富集不相容元素,其中高场强元素(HFSE)Nb、Ta和Th出现峰值,具有近似OIB配分型式的特征;玄武岩富含相容元素Co((39.1～48.9)×10-6)、Ni((130～257)×10-6)、Cr((138～320)×10-6)。上述所有特征以及岩石结晶程度低、富含橄榄岩包体和少量捕虏晶、元素变异关系等均表明,天和永玄武岩是原生玄武岩质岩浆固结的产物。微量元素比值Ba/Rb(12～35)和碱金属的变化暗示源区可能遭受过流体的交代作用,源岩可能是富集的二辉橄榄岩。岩石成因模拟表明,形成天和永玄武岩的原生岩浆是在变压、部分熔融的条件下富集地幔源区岩石非实比熔融的产物,变压熔融柱穿切了Sp/Gt二辉橄榄岩相边界。岩浆形成于源区岩石的低度(约<5%)部分熔融,其中石榴石二辉橄榄岩部分熔融约为1%,尖晶石二辉橄榄岩部分熔融2%～5%。综合分析显示,源区部分熔融的触发机制是边际驱动的地幔对流,因而其形成深度大于东部的集宁玄武岩和汉诺坝玄武岩。  相似文献   

15.
The Red Hills peridotite in the Dun Mountain ophiolite of SouthIsland, New Zealand, is assumed to have been produced in a paleo-mid-oceanridge tectonic setting. The peridotite is composed mostly ofharzburgite and dunite, which represent residual mantle andthe Moho transition zone (MTZ), respectively. Dunite channelswithin harzburgite blocks of various scales represent the MTZcomponent. Plagioclase- and clinopyroxene-bearing dunites occursporadically within common dunites. These dunites representproducts of melt–wall-rock interaction. Chondrite-normalizedrare earth element (REE) patterns of MTZ clinopyroxenes showa wide compositional range. Clinopyroxenes in plagioclase dunitesare extremely depleted in light REE (LREE) ([Lu/La]N >100),and are comparable with clinopyroxenes in abyssal peridotitesfrom normal mid-ocean ridges. Interstitial clinopyroxenes inthe common dunite have flatter patterns ([Lu/La]N 2) comparablewith those for dunite in the Oman ophiolite. Clinopyroxenesin the lower part of the residual mantle harzburgites are evenmore strongly depleted in LREE ([Lu/La]N = 100–1000) thanare mid-ocean ridge peridotites, and rival the most depletedabyssal clinopyroxenes reported from the Bouvet hotspot. Incontrast, those in the uppermost residual mantle harzburgiteand harzburgite blocks in the MTZ are less LREE depleted ([Lu/La]N= 10–100), and are similar to those in plagioclase dunite.Clinopyroxenes in the clinopyroxene dunite in the MTZ are similarto those reported from mid-ocean ridge basalt (MORB) cumulates,and clinopyroxenes in the gabbroic rocks have compositions similarto those reported from MORB. Strong LREE and middle REE (MREE)depletion in clinopyroxenes in the harzburgite suggests thatthe harzburgites are residues of two-stage fractional melting,which operated initially in the garnet field, and subsequentlycontinued in the spinel lherzolite field. The early stage meltingproduced the depleted harzburgite. The later stage melting wasresponsible for the gabbroic rocks and dunite. Strongly LREE–MREE-depletedclinopyroxene in the lower harzburgite and HREE-enriched clinopyroxenein the upper harzburgite and plagioclase dunite were formedby later reactive melt migration occurring in the harzburgite. KEY WORDS: clinopyroxene REE geochemistry; Dun Mountain ophiolite; Moho transition zone; orogenic peridotite; Red Hills  相似文献   

16.
《Geodinamica Acta》2013,26(1):49-50
New structural data and P–T estimates of syn-deformational assemblages within the Beni Bousera peridotites and their crustal envelope are used to explain their Alpine exhumation. The Beni Bousera peridotites occur as thin sheets within high grade crustal units of the lower Sebtides (inner Rif, Morocco) and are composed of weakly deformed spinel lherzolite in the core of the massif and garnet-spinel mylonite at the rim. The main foliation trajectories in both the peridotites and overlying crustal units show systematic rotation towards their mutual contact, indicating a kilometer-scale top to the NW shearing with a dextral component along this crust/mantle contact. Widespread top to the NW shear criteria within the crustal units overlying the peridotite support this feature. Available ages constrain the development of the main foliation in both the peridotites and crustal rocks between 25 and 20 Ma. New P–T data from the peridotites show that deformation occurs during decompression from ≈ 22 kbar, 1050°C to ≈ 9-15 kbar, 800°C. As a consequence, exhumation of the Beni Bousera peridotites takes place during the Oligo-Miocene lithosphere thinning in the footwall of a lithospheric extensional shear zone. The exceptional preservation of garnet within the mylonitic peridotites results from rapid cooling of the border of the massif due to the juxtaposition with colder crustal rocks along this shear zone. Uplifting of the hot mantle rocks simultaneously induces high temperature metamorphism in the overlying crustal units. These new findings allow us to reconstruct the deformation history of the Beni Bousera region and the Alboran domain in the framework of the western Mediterranean geodynamics during the last 40 Myrs.  相似文献   

17.
Basanites and alkali basalts from Oberon, NSW, Australia contain variable abundances of small Cr-diopside lherzolite xenoliths. Despite a limited range in (metamorphic) textures and modal mineralogy, there is significant variation in mineral chemistry. Mineral thermometric data applied to the geotherm of O'Reilly and Griffin (1985) suggests equilibration over a narrow pressure interval corresponding to depths of 30–45 km. These data show that significant compositional variations exist over a small depth interval in the subcontinental mantle.Basaltic host rocks show near-primary chemical characteristics. Mildly and strongly incompatible element (i.e. D< 1 and D1 respectively) concentrations have been used to constrain the modal amounts of clinopyroxene and garnet in a presumed garnet peridotite mantle source. Estimated proportions of (ol+opx)=73%; cpx=16%; gar= 11% closely resemble source compositions for other basaltic rocks of eastern Australia. Batch partial melting of this source in the range F=9.5–15% applied to the available REE data suggests the source is enriched relative to chondrite 8–10 × La, 2.1–2.4 × Tb and 2.5–3.7 × Yb.  相似文献   

18.
ABUNDANCE AND DISTRIBUTION OF PLATINUM-GROUP ELEMENTS (PGE) IN PERIDOTITE FROM THE DAGZHUKA OPHIOLITE IN TIBET:IMPLICATIONS FOR MANTLE METASOMATISM  相似文献   

19.
The paper discusses the petrography, mineralogy, petrochemical affinities, P/T crystallization regimes and genetic aspects of four garnet clinopyroxenite inclusions from diatremes in the Gloucester area, New South Wales. Inclusion mineral assemblages (which generally display textural evidence of annealing) include garnet-plagioclase-(sulphur-rich scapolite)-clinopyroxene, garnet-hornblende-orthopyroxene-clinopyroxene and garnet-hornblende-clinopyroxene. The garnet-plagioclase clinopyroxenite inclusion possesses an essentially alkali basaltic chemistry. It probably represents a crystallized basaltic liquid whereas the petrochemical affinities of the two garnet pyroxenites carrying amphiboles are more appropriate to subcalcie clinopyroxenites with variable Mg/Fe ratios. Experimental and other data suggest that the Gloucester garnet clinopyroxenite suite crystallized at pressures of the order of 10–14 kb and temperatures in the vicinity of 1000° C. The chemical compositions of many garnet pyroxenites, occurring either as inclusions in alkali basaltic rocks or as localized facies within some alpine-type peridotites, such as those in the western Mediterranean region, suggest that they can be interpreted as lower temperature heteromorphs of “primitive” subcalcic clinopyroxenites, variable in Al contents and hy/di ratios, but retaining consistently low Ti, Na, K and P. It is suggested that many inclusions of garnet (-spinel) pyroxenite and subcalcie Clinopyroxenite, restricted to alkali basaltic rocks and their associates, originally may have been interleaved with upper mantle aluminous peridotites and that they represent partial melt products of their aluminous peridotitic hosts.  相似文献   

20.
The Ronda orogenic peridotite (southern Spain) contains a varietyof pyroxene-rich rocks ranging from high-pressure garnet granulitesand pyroxenites to low-pressure plagioclase–spinel websterites.The ‘asthenospherized’ part of the Ronda peridotitecontains abundant layered websterites (‘group C’pyroxenites), without significant deformation, that occur asswarms of layers showing gradual modal transitions towards theirhost peridotites. Previous studies have suggested that theselayered pyroxenites formed by the replacement of refractoryspinel peridotites. Here, we present a major- and trace-element,and numerical modelling study of a layered outcrop of groupC pyroxenite near the locality of Tolox aimed at constrainingthe origin of these pyroxenites after host peridotites by pervasivepyroxene-producing, refertilization melt–rock reactions.Mg-number [= Mg/(Mg + Fe) cationic ratio] numerical modellingshows that decreasing Mg-number with increasing pyroxene proportion,characteristic of Ronda group C pyroxenites, can be accountedfor by a melt-consuming reaction resulting in the formationof mildly evolved, relatively low Mg-number melts (0·65)provided that the melt fraction during reaction and the time-integratedmelt/rock ratio are high enough (>0·1 and > 1,respectively) to balance Mg–Fe buffering by peridotiteminerals. This implies strong melt focusing caused by melt channellingin high-porosity domains resulting from compaction processesin a partial melted lithospheric domain below a solidus isothermrepresented by the Ronda peridotite recrystallization front.The chondrite-normalized rare earth element (REE) patterns ofgroup C whole-rocks and clinopyroxenes are convex-upward. Numericalmodeling of REE variations in clinopyroxene produced by a pyroxene-forming,melt-consuming reaction results in curved trajectories in the(Ce/Nd)N vs (Sm/Yb)N diagram (where N indicates chondrite normalized).Based on (Ce/Nd)N values, two transient, enriched domains betweenthe light REE (LREE)-depleted composition of the initial peridotiteand that of the infiltrated melt may be distinguished in thereaction column: (1) a lower domain characterized by convex-upwardREE patterns similar to those observed in Ronda group C pyroxenite–peridotite;(2) an upper domain characterized by melts with strongly LREE-enrichedcompositions. The latter are probably volatile-rich, small-volumemelt fractions residual after the refertilization reactionsthat generated group C pyroxenites, which migrated throughoutthe massif—including the unmelted lithospheric spinel-tectonitedomain. The Ronda mantle domains affected by pyroxenite- anddunite- or harzburgite-forming reactions (the ‘layeredgranular’ subdomain and ‘plagioclase-tectonite’domain) are on average more fertile than the residual, ‘coarsegranular’ subdomain at the recrystallization front. Thisindicates that refertilization traces the moving boundariesof receding cooling of a thinned and partially melted subcontinentallithosphere. This refertilization process may be widespreadduring transient thinning and melting of depleted subcontinentallithospheric mantle above upwelling asthenospheric mantle. KEY WORDS: subcontinental mantle; refertilization; pyroxenite; peridotite; websterite; melt–rock reaction; plagioclase; trace elements  相似文献   

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