汉诺坝玄武岩中熔体-捕虏体相互作用初步研究

汉诺坝新生代玄武岩捕获的地幔橄榄岩及其解体矿物橄榄石、单斜辉石、斜方辉石捕虏晶,普遍发育反应边结构,提供了玄武岩浆在上升穿越岩石圈地幔过程中橄榄岩-熔体相互作用的重要信息。橄榄石和单斜辉石捕虏晶反应边的成分变化一致,由核部富镁向边部富铁变化,趋同于玄武岩中相应斑晶的成分。斜方辉石捕虏晶反应边一般由橄榄石+单斜辉石+玻璃构成,多为双层结构,反应边矿物橄榄石、单斜辉石较相应的地幔矿物富铁,其富硅、碱的中酸性玻璃成分,为中国东部地幔矿物包裹体中存在的富硅、碱熔体的来源提供了重要信息。同时发现橄榄岩捕虏体中尖晶石颜色、成分的变化与温度的关系。地幔矿物捕虏晶反应边结构(非平衡结构)得以保存,暗示了玄武岩浆的快速上升。而大规模的熔体-捕虏体相互作用,改变着岩石圈地幔的性质。     

斜方辉石筛状反应边的成因机制及其对岩石圈地幔性质转变的意义

本文利用电子背散射衍射(EBSD)技术对河北张家口大麻坪汉诺坝玄武岩橄榄岩捕虏体中斜方辉石与玄武岩反应结构的显微构造进行了详细研究。研究结果表明: ① 其反应边具有复杂的多层筛状结构特征,包括玄武岩层、富橄榄石层以及橄榄石和单斜辉石交生层;② 由外至内,橄榄石的Mg值逐渐升高,而单斜辉石的Mg值变化不大;③ 反应边结构中的单斜辉石与斜方辉石残斑之间存在很好的结晶学拓扑关系,即(100)_opx//(100)_cpx、(010)_opx//(010)_cpx、(001)_opx//(001)_cpx;④ 橄榄石的结晶学取向无序且与斜方辉石和单斜辉石均无关。这个反应过程可以用贫硅熔体先与斜方辉石反应形成单斜辉石,并导致熔体富硅,从而橄榄石从反应熔体中结晶出来合理地解释。相对富硅熔体与橄榄岩的反应,贫硅熔体与橄榄岩的反应过程由于筛状反应边的存在可能更容易进行,筛状结构反应边可以为熔体在橄榄岩中沿颗粒边界运移提供通道,并使橄榄岩主要组成矿物发生细粒化和岩石结构变得松散,可以有效保证熔体上升过程中对橄榄岩的持续侵蚀和破坏,从而可能导致岩石圈地幔性质的迅速转变。     

地幔富硅交代与大陆岩石圈的演化

富硅交代是弧下地幔中熔体岩石相互作用的主要表现形式 ,是造成古老克拉通陆下岩石圈地幔富硅的主要机制。在弧下地幔捕掳体中 ,橄榄岩被来自俯冲洋壳物质部分熔融生成的含水富硅熔体交代后 ,斜方辉石含量的增加使全岩富集SiO2 ,斜方辉石显示异常低的Al2 O3和Cr2 O3,微量元素上表现为强烈富集LILE ,强烈亏损Nb ,Ta和Ti。在古老克拉通地幔岩样品中 ,方辉橄榄岩具过剩的斜方辉石 ,橄榄石的Ni含量与斜方辉石的组成含量成正比 ,而和橄榄石的x(Mg) /x(Mg +Fe2 +)值没有正比关系 ,被解释为亏损的地幔橄榄岩和来自俯冲板片的富硅熔体相互作用的结果。熔体岩石相互作用最终导致了陆下岩石圈地幔富集SiO2 ,这种被含水富硅熔体改造后的地幔岩石的部分熔融可能是造成陆壳富硅富镁的主要原因。含水富硅熔体对岩石圈地幔的影响程度也可能是大陆岩石圈增生或裂解、增厚或减薄的关键因素之一。     

北部湾涠洲岛橄榄岩中熔体包裹体——大陆岩石圈地幔交代作用的新证据

根据北部湾涠洲岛晚更新世火山岩中尖晶石二辉橄榄岩的矿物化学和形成条件推测,它们是来自地下约40km-50km的大陆岩石圈地幔样品。涠洲岛地幔橄榄岩中同时出现高硅（64％～68％）和低硅（49％～57％）两种熔体成分,它们普遍富碱、Al2O3和H2O、CO2等挥发组分（2％-5％）。研究认为,两种熔体存在不同的成因机制。高硅熔体可能与软流圈上升的玄武质岩浆和斜方辉石反应或下地壳物质循环进入地幔后的部分熔融有关。低硅熔体直接提供了富硅熔体与橄榄石发生交代作用的证据。这可以用富SiO2熔体＋Ol→贫SiO2熔体＋Opx反应解释,其结果是消耗橄榄石生成斜方辉石。涠洲岛橄榄岩中两种熔体的发现,进一步提供了发生在大陆岩石圈地幔流（熔）体与橄榄岩交代作用的普遍性、复杂性,以及地幔熔体多样性的新证据。     

橄榄岩-熔体的相互作用:岩石圈地幔组成转变的重要方式

橄榄岩-熔体/岩浆的相互作用常被用来解释蛇绿岩套橄榄岩、造山带橄榄岩、超镁铁质侵入杂岩体、地幔橄榄岩捕虏体中某些具有不平衡结构和矿物组成的岩石的形成过程。橄榄岩-熔体的反应主要有两种方式,即消耗橄榄石(和单斜辉石)生成斜方辉石或消耗斜方辉石生成橄榄石(和单斜辉石)。反应的结果不仅造成矿物百分含量的变化,而且造成矿物组成的变化;后者更重要但未引起足够的重视。华北东部中生代玄武质岩石中具有环带状结构的橄榄石和辉石捕虏晶,特别是具有环带状结构的地幔橄榄岩捕虏体的发现,暗示这种橄榄岩-熔体的相互作用在华北东南部中生代岩石圈地幔中很可能普遍存在,为岩石圈地幔组成转变和快速富集的重要方式。这是全球首例由橄榄岩-熔体相互反应造成的岩石圈地幔大规模的组成变化。反应熔体来源途径主要有地壳来源和软流圈地幔来源。来源不同的熔体与橄榄岩的反应造成的组成变化完全不同。     

鹤壁新生代玄武岩源区及成因: 地球化学和Sr-Nd-Hf同位素证据

大陆碱性玄武岩是研究大陆地幔、软流圈和岩石圈、壳幔相互作用的窗口。鹤壁碱性玄武岩为华北中部新生代玄武岩重要组成部分,其源区和成因对了解新生代期间华北克拉通中部岩石圈地幔改造提供了重要依据。鹤壁新生代玄武岩主要为碱性玄武岩,贫硅(SiO₂=45.0%~47.8%)富镁(MgO=7.3%~8.5%)和全碱(Na₂O+K₂O=4.6%~6.3%),富集轻稀土元素,轻、重稀土元素强烈分馏,无明显Eu异常。富集大离子亲石元素(LILEs)和高场强元素(HFSEs)。在原始地幔标准化蛛网图上,具有明显的Nb、Ta正异常,其中Nb/U=35~48、La/Nb=0.4~0.7、Ba/Nb=3.6~11。 全岩的Sr、Nd、Hf同位素比值分别为⁸⁷Sr/⁸⁶Sr_i=0.7036~0.7044,ε_Nd(t)=+0.4~+5.4, ε_Hf(t)=+5.0~+9.7,显示鹤壁新生代玄武岩具有洋岛玄武岩(OIB)的地球化学特征和同位素组成。岩相学特征和地球化学特征表明鹤壁新生代玄武岩是软流圈地幔(>80km)小程度部分熔融形成的熔体与富集的岩石圈地幔相互作用后的结果,地壳物质混染和结晶分离作用不显著。     

大兴安岭北部诺敏河地幔金云母及钾质地幔熔体研究

在大兴安岭北部诺敏河第四纪钾质火山岩携带的地幔捕虏体中,发现少量金云母矿物和富钾地幔熔体。金云母颗粒大小1~5mm,呈网脉状充填在橄榄石和辉石、石榴子石等地幔矿物间隙。电子探针研究表明地幔橄榄石、单斜辉石、斜方辉石和石榴石等矿物几乎不含钾质成分(K2O0.01%),而金云母矿物成分具有高钾(K2O~10%)、高钛(Ti O25.41%~7.74%)的特点,暗示区域地幔钾的富集与金云母矿物有密切关系。地幔金云母的成因往往与富钾地幔流体/熔体的交代作用有关,在地幔捕虏体矿物反应边的硅酸盐熔体(囊体)中,发现富硅、富钾的熔体,K2O 4%~8%。结合前人地幔熔体研究,认为区域地幔经历了多期、不同成分地幔熔体的富集作用,其中富钾熔体对地幔钾质成分的富集起到重要作用。诺敏钾质火山正是富钾地幔部分熔融的产物,钾质熔体成分的来源可能与俯冲再循环的壳源物质有关。     

橄榄岩—熔体相互作用过程中Re-Os体系的变化趋势: 对华北新生代地幔橄榄岩Re-Os年龄含义的启示

橄榄岩的Re-Os同位素体系作为探讨岩石圈地幔形成年龄的重要手段已受到人们越来越多的重视。然而,Re-Os体系是否会受到橄榄岩的低温蚀变如蛇纹石化和地幔交代作用或橄榄岩—熔体相互作用的影响并不十分清楚。本文在总结国际上典型造山带橄榄岩剖面研究和地幔橄榄岩捕虏体研究的基础上,发现橄榄岩的Re-Os同位素体系基本不受蛇纹石化等低温蚀变作用的影响; 但橄榄岩—熔体相互作用会造成橄榄岩的Re-Os体系的变化即Re或Os的带入。当熔体/岩石比例较小时(≤1),橄榄岩—熔体相互作用会造成橄榄岩的Re含量显著增加,而放射成因的Os同位素即¹⁸⁷Os增量有限。但当熔体/岩石比例很大时(≥1),会造成¹⁸⁷Os同位素显著增加。同时,橄榄岩的Re含量与中等程度不相容主、微量元素如Al、Ti、Yb的正相关关系可以通过橄榄岩的两阶段演化模式来解释,即早期的部分熔融残留和后期的橄榄岩—熔体相互作用共同影响的结果。橄榄岩的Re含量与Cr含量的正相关关系进一步说明了这一问题。上述结果对华北东部岩石圈地幔的演化过程有重要的启示作用。因为华北东部古生代时期的确存在太古宙岩石圈地幔,然而新生代时期地幔橄榄岩捕虏体普遍具有元古宙而非太古宙的事实证明橄榄岩—熔体的相互作用的确广泛存在,从而造成岩石圈地幔橄榄岩变年轻。因此,新生代地幔捕虏体的Re-Os同位素年龄并不是岩石圈地幔的形成年龄,而是混合作用的结果。汉诺坝地幔橄榄岩的Re含量和Sr、Nd同位素组成符合橄榄岩—多元熔体相互作用的混合趋势,其橄榄岩的全岩Al₂O₃含量和橄榄石Fo的反相关性能够通过橄榄岩—熔体相互作用来解释。     

大兴安岭地幔橄榄岩中熔体的多样性及其成因

本文报道了大兴安岭第四纪火山岩中的地幔橄榄岩中橄榄石、单斜辉石和斜方辉石颗粒内部熔体产状(囊体、包裹体和反应边)和成分(低硅熔体和高硅熔体)的多样性,初步讨论了不同熔体的成因。低硅熔体囊体是在地幔深部玄武岩浆与橄榄岩中单斜辉石发生交代反应的产物,斜方辉石反应边的高硅熔体是橄榄岩被捕获上升过程中玄武岩浆与斜方辉石反应的产物,高硅熔体包裹体是地幔中存在的交代熔体。     

滇西富碱斑岩及其中包体岩石的深部地质过程探讨

自新生代以来，伴随深部地质作用，滇西地区多处发育富含深源包体的富碱斑岩体。文章从寄主岩石和包体岩石的岩石化学研究入手，认为交代主岩和包体岩石的流体富含碱质（Na₂O+K₂O）和硅质（SiO₂），是与富碱岩浆同源的来自富集地幔源区的地幔流体，这种地幔流体交代作用的功能和能量明显优于一般意义上的地壳流体作用，对富碱斑岩的成岩和成矿发挥了重要的先导作用。     

Some implications of xenolith glasses for the mantle sources of alkaline mafic magmas

The assumption that mafic alkaline magmas are derived from mantle sources with a lherzolite mineralogy has become entrenched in the petrologic literature. Although it is commonly assumed that highly alkaline magmas require metasomatised mantle sources, there is little understanding of the spatial relation of such sources with respect to those of associated more Si-rich transitional magmas. Glasses developed in mantle xenoliths represent natural experiments which may provide some insight on this problem. Highly silica undersaturated glasses developed in the amphibole-garnet clinopyroxenite portion of a composite xenolith from Nunivak Island, Alaska, become quartz normative where they penetrate adjacent spinel lherzolite. A comparison of glass compositions in mantle pyroxenite and lherzolite xenoliths reveals that glasses developed in amphibole pyroxenite xenoliths are in general more silica undersaturated than those in lherzolite xenoliths. This suggests that some highly silica undersaturated magmas such as nephelinites may in fact be derived by the preferential melting of amphibole or amphibole-garnet pyroxenite veins and that the spectrum from nephelinite to transitional alkaline basalt that characterizes many individual alkaline volcanic suites is produced by mixing with melt derived from the host lherzolite as the degree of partial melting increases.     

Dissolution of orthopyroxene in basanitic magma between 0.4 and 2 GPa: further implications for the origin of Si-rich alkaline glass inclusions in mantle xenoliths

A large body of recent work has linked the origin of Si-Al-rich alkaline glass inclusions to metasomatic processes in the upper mantle. This study examines one possible origin for these glass inclusions, i.e., the dissolution of orthopyroxene in Si-poor alkaline (basanitic) melt. Equilibrium dissolution experiments between 0.4 and 2 GPa show that secondary glass compositions are only slightly Si enriched and are alkali poor relative to natural glass inclusions. However, disequilibrium experiments designed to examine dissolution of orthopyroxene by a basanitic melt under anhydrous, hydrous and CO₂-bearing conditions show complex reaction zones consisting of olivine, ± clinopyroxene and Si-rich alkaline glass similar in composition to that seen in mantle xenoliths. Dissolution rates are rapid and dependent on volatile content. Experiments using an anhydrous solvent show time dependent dissolution rates that are related to variable diffusion rates caused by the saturation of clinopyroxene in experiments longer than 10 minutes. The reaction zone glass shows a close compositional correspondence with natural Si-rich alkaline glass in mantle-derived xenoliths. The most Si-and alkali-rich melts are restricted to pressures of 1 GPa and below under anhydrous and CO₂-bearing conditions. At 2 GPa glass in hydrous experiments is still Si-␣and alkali-rich whereas glass in the anhydrous and CO₂-bearing experiments is only slightly enriched in SiO₂ and alkalis compared with the original solvent. In the low pressure region, anhydrous and hydrous solvent melts yield glass of similar composition whereas the glass from CO₂-bearing experiments is less SiO₂ rich. The mechanism of dissolution of orthopyroxene is complex involving rapid incongruent breakdown of the orthopyroxene, combined with olivine saturation in the reaction zone forming up to 60% olivine. Inward diffusion of CaO causes clinopyroxene saturation and uphill diffusion of Na and K give the glasses their strongly alkaline characteristics. Addition of Na and K also causes minor SiO₂ enrichment of the reaction glass by increasing the phase volume of olivine. Olivine and clinopyroxene are transiently stable phases within the reaction zone. Clinopyroxene is precipitated from the reaction zone melt near the orthopyroxene crystal and redissolved in the outer part of the reaction zone. Olivine defines the thickness of the reaction zone and is progressively dissolved in the solvent as the orthopyroxene continues to dissolve. Although there are compelling reasons for supporting the hypothesis that Si-rich alkaline melts are produced in the mantle by orthopyroxene – melt reaction in the mantle, there are several complications particularly regarding quenching in of disequilibrium reaction zone compositions and the mobility of highly polymerized melts in the upper mantle. It is considered likely that formation of veins and pools of Si-rich alkaline glass by orthopyroxene – melt reaction is a common process during the ascent of xenoliths. However, reaction in situ within the mantle will lead to equilibration and therefore secondary melts will be only moderately siliceous and alkali poor. Received: 24 August 1998 / Accepted: 2 December 1998     

Mantle-Melt Interaction Recorded in Spinel Lherzolite Xenoliths from the Alligator Lake Volcanic Complex, Yukon, Canada

Magmas which have equilibrated with the Earth's upper mantleare generally assumed to be compositionally buffered by spinellherzolite as represented by Cr-diopside series xenoliths foundin alkaline lavas. The fact that the mineral equilibria preservedin such xenoliths typically reflect re-equilibration at sub-solidusmantle conditions, however, has discouraged attempts to usethe compositional variation observed in spinel lherzolite xenolithsto constrain the compositions of melts extracted from the uppermantle. A suite of mantle-derived xenoliths from the AlligatorLake volcanic center in the southern Yukon, Canada, exhibitsa bimodal xenolith population consisting of lherzolites, themost fertile of which approach pyrolite in composition, andrelatively depleted harzburgites. If a source-residue relationshipis assumed between the two, then the extracted melt was a picriticmagma (17 wt. per cent MgO, 23 Mg cation units) with low Febut relatively high Si contents, similar to picritic lavas associatedwith subduction margins. The compositional variation within the lherzolite xenoliths,however, is not towards the majority of the harzburgite xenoliths,but towards relatively rare, Fe-rich harzburgites. Reactionsobserved between the xenoliths and their alkaline host lavasmay provide an analogue for the upper mantle process which producedthis trend. The observed reactions result in the loss of anAl and Si-rich melt associated with the preferential destructionof pyroxene and spinel and a concomitant rise in the Fe contentof residual olivine. The result of such an interaction in theupper mantle would be the development of a Fe and oli vine-richresidue similar to the observed Fe-rich harzburgites. In turn,the magma responsible would be forced to evolve towards moreSi-rich, but Fe-poor compositions than would otherwise be possibleby closed system, crystal fractionation. A comparison with other mantle xenolith suites indicates thatthe compositional spectra of many of those associated with continentalalkaline basalts can be interpreted in terms of the extractionof picritic magmas similar to that calculated for AlligatorLake. Xenolith suites from oceanic islands such as Hawaii, incontrast, contain fertile lherzolites which are considerablymore Fe-rich than pyrolite. The associated refractory xenoliths,however, are similar to those at Alligator Lake and their derivationfrom such fertile lherzolites would require the extraction ofa picritic melt which was both Fe and Si-rich, similar to theobserved tholeiitic picritcs of the shield-building stage ofHawaiian volcanism. Alternately, the Fe-rich lherzolites mayrepresent samples of upper mantle which have reacted extensivelywith the relatively Fe-rich Hawaii magmas. Xenolith suites fromkimberlites, on the otheT hand, are dominated by refractoryharzburgites which are richer in Si but poorer in Fe than theAlligator Lake harzburgites. They suggest that the lower continentallithosphere is both more orthopyroxene-rich and more depletedthan the upper mantle sampled by alkaline basalts. In general,the derivation of depleted harzburgite xenoliths by the partialmelting of a pyrolite mantle source seems to require the extractionof picritic magmas. If the majority of terrestrial basalticmagmas are not derived from picritic parental magmas, they requirethe existence of mantle source regions more Fe-rich than standardpyrolite models.     

地幔捕虏体中的流体-熔体包裹体

地幔流体的研究现已成为国内外前沿课题。地幔岩捕虏体中的流体-熔体包裹体是地幔流体的直接证据,通过对它们的研究可以直接获取地授流体的信息。包裹体按相态特征主要有三类：二氧化碳流体包裹体、二氧化碳-硅酸盐熔体包裹体、硫化物-熔体流体包裹体。本总结了地幔岩中流体-熔体包裹体的基本特征、微量元素地球化学、硫化物-熔体包裹体和二氧化碳流体包裹体稳定同位素特征的研究进展状况。讨论认为：地幔流体是由C、H、O、S等元素的挥发份和硅酸盐熔体组成;上地幔流体在化学成分上明显富含CO2、硫化物、LILE和BEE,它引起地幔交代作用和地授部分熔融;上地授流体的分布存在不均匀性,其组成也存在地区性差异。     

滇西富碱斑岩中特殊包体岩石的流体包裹体幔源不混溶特征

滇西地区沿金沙江-哀牢山断裂带产出了一套新生代富碱斑岩,其中发现了与镁铁-超镁铁质深源包体岩石共生的含石英的方解石包晶(体)、石英钠长石伟晶岩包体和含玻璃包裹体的纯石英包晶(体)以及富铁熔浆包体.流体包裹体地球化学研究表明,该四类特殊包体的形成与富含CO2流体持续减压而造成的不混溶作用有关;而玻璃包裹体与水溶液包裹体以...     

Metasomatism and sulfide mobility in lithospheric mantle beneath eastern Australia: Implications for mantle Re–Os chronology

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.     

Fluid inclusions in mantle xenoliths

Fluid inclusions in olivine and pyroxene in mantle-derived ultramafic xenoliths in volcanic rocks contain abundant CO₂-rich fluid inclusions, as well as inclusions of silicate glass, solidified metal sulphide melt and carbonates. Such inclusions represent accidentally trapped samples of fluid- and melt phases present in the upper mantle, and are as such of unique importance for the understanding of mineral–fluid–melt interaction processes in the mantle. Minor volatile species in CO₂-rich fluid inclusions include N₂, CO, SO₂, H₂O and noble gases. In some xenoliths sampled from hydrated mantle-wedges above active subduction zones, water may actually be a dominant fluid species. The distribution of minor volatile species in inclusion fluids can provide information on the oxidation state of the upper mantle, on mantle degassing processes and on recycling of subducted material to the mantle. Melt inclusions in ultramafic xenoliths give information on silicate–sulphide–carbonatite immiscibility relationships within the upper mantle. Recent melt-inclusion studies have indicated that highly silicic melts can coexist with mantle peridotite mineral assemblages. Although trapping-pressures up to 1.4 GPa can be derived from fluid inclusion data, few CO₂-rich fluid inclusions preserve a density representing their initial trapping in the upper mantle, because of leakage or stretching during transport to the surface. However, the distribution of fluid density in populations of modified inclusions may preserve information on volcanic plumbing systems not easily available from their host minerals. As fluid and melt inclusions are integral parts of the phase assemblages of their host xenoliths, and thus of the upper mantle itself, the authors of this review strongly recommend that their study is included in any research project relating to mantle xenoliths.     

Radiogenic helium in xenoliths from Simcoe, Washington, USA: implications for metasomatic processes in the mantle wedge above subduction zones

We report ³He/⁴He ratios from 10 peridotite xenoliths considered to represent samples of the uppermost mantle wedge above the downgoing Juan de Fuca Plate. Helium isotopic ratios in all but two of the xenoliths are similar to many arc magmas, roughly 7 Ra (1 Ra=atmospheric value). Based on decoupling of He from Sr, Nd and Os in these samples, similar He ratios in olivines from rims of larger xenoliths, and modeling of helium exchange between xenoliths and magmas, we interpret this ratio as that of helium in the host basalt. ³He/⁴He ratios as low as 4.2 Ra are found in olivines from the cores of the two largest xenoliths. These results cannot be reasonably explained by interaction with crustal material or post-eruptive ingrowth of ⁴He, but have been produced by interaction between mantle peridotite and a ⁴He-rich melt or fluid. Either ⁴He already present in the subducting oceanic crust has been retained to significant depths below Simcoe and then directly released behind the arc to interact with the mantle wedge, or, more likely, ⁴He has been produced by decay of U and Th in metasomatized mantle directly above the slab; a He-rich fluid or melt from this source has then ascended and modified the region of mantle represented by the xenoliths. This latter model is supported by estimates of residence time for the Simcoe metasomatic agent from U–Th–Pb isotopic systematics of pyroxenes from the Simcoe peridotites, estimated U and Th concentrations in the source of the fluid or melt, and commonly assumed patterns of helium behavior. This model is also consistent with higher ³He/⁴He ratios typically measured in arc samples; the portion of sub-arc mantle with such low He isotope ratios may be quite small, but the Simcoe xenoliths record a much larger volumetric contribution of the He-rich metasomatic agent than do arc lavas.     

兴蒙造山带北部岩石圈地幔橄榄岩氧逸度特征研究

在大兴安岭北部的诺敏和科洛地区的新生代玄武岩中发现了尖晶石相的橄榄岩包体。地幔橄榄岩中橄榄石的Mg~#说明了研究区上地幔具有部分难熔的特点。在橄榄石含量与Fo图解中,有一部分橄榄岩包体落在太古代和元古代的地幔区域,揭示了研究区的岩石圈地幔存在古老岩石圈地幔的残余。研究区方辉橄榄岩与二辉橄榄岩有显示高氧逸度值FMQ+1.95～3.01,这与一般情况下相对还原的古老岩石圈地幔的低氧逸度值形成鲜明对比,可能为古生代的古亚洲洋以及中生代的古太平洋相继俯冲到了兴蒙造山带之下,导致当时岩石圈地幔的氧化所致。在地幔包体的反应边中发现了富钾熔体(K20 1%-6%),这被认为研究区地幔经历了多期富钾流体活动,富钾流体的来源可能与俯冲再循环的壳源物质有关。     

鲁西纯橄岩捕虏体中富硅质熔（流）体的交代作用：对中生代岩石圈地幔减薄的意义

鲁西中生代辉长-闪长质岩石中纯橄岩捕虏体的岩石学、矿物化学及微量元素地球化学研究表明,纯橄岩捕虏体代表了古老岩石圈地幔的残留;地幔纯橄岩捕虏体中存在两种类型的交代作用,一是以填隙型金云母为代表的早期富含CO_2和H_2O的不活动流体的交代作用;二是以斜方辉石交代脉和网络状斜方辉石为代表的晚期富硅质熔(流)体的交代作用。后者代表了起源于软流圈的富硅质熔(流)体对古老岩石圈地幔的一种化学侵蚀。这对认识华北地块东部中生代岩石圈地幔的性质以及岩石圈减薄机制具有重要意义。