Martian mantle mineralogy investigated by the Lu–Hf and Sm–Nd systematics of shergottites     

V. Debaille  Q.-Z. Yin  A.D. Brandon  B. Jacobsen 《Earth and Planetary Science Letters》2008,269(1-2):186-199

Chemical heterogeneities in the Martian mantle are believed to result from the crystallization of a magma ocean in the first 100 million years of its history. Shergottite meteorites from Mars are thought to retain a compositional record of such early differentiation and the resulting mineralogy at different depths. The coupled ¹⁷⁶Lu–¹⁷⁶Hf and ¹⁴⁷Sm–¹⁴³Nd isotope systematics in 9 shergottites are used here to investigate these issues. Three compositional groups in the shergottites display distinct isotope systematics. One group, commonly termed as depleted, is characterized by positive ¹⁷⁶Hf_i from + 46.2 to + 50.4 and ¹⁴³Nd_i from + 36.2 to + 39.1. Another, termed as enriched, has negative ¹⁷⁶Hf_i = − 16.5 to − 13.2 and ¹⁴³Nd_i = − 7.0 to − 6.5. The third group is intermediate between the depleted and enriched groups with positive ¹⁷⁶Hf_i = + 30.0 to + 33.4 and ¹⁴³Nd_i = + 16.9. Together, they describe mixing curves between ¹⁷⁶Hf/¹⁷⁷Hf, ¹⁴³Nd/¹⁴⁴Nd, Lu/Hf, and Sm/Nd, implying that they sample two distinct sources in the Martian mantle. All shergottites are characterized by (Sm/Nd)_source < (Sm/Nd)_sample, but (Lu/Hf)_source > (Lu/Hf)_sample. This decoupling can be explained by two successive partial melting episodes in the depleted shergottite source and localized in the Martian upper mantle. The genesis of shergottites can be modeled using non-modal equilibrium partial melting in a source initially composed of 60% olivine, 21% clinopyroxene, 9% orthopyroxene, and 10% garnet, with degrees of partial melting of 8.8% and 3.9%, respectively, for the two successive events. The enriched end-member of the shergottite mixing curve is best modeled by late-stage quenched residual melt resulting from the crystallization of a magma ocean. The depleted shergottite source may be modeled as a mixture of cumulates and residual melt, as convection in the Martian magma ocean is expected to reduce the incompatible trace element heterogeneity in the final solidified layers. Consequently, equilibrium crystallization is preferred to model the crystallization of the Martian magma ocean. The models that best explain the shergottite data are those where the magma ocean is at a depth of at least 1350 km in Mars.  相似文献   

汇聚板块边缘岩浆中金属和氯的地球化学性质研究   总被引：2，自引：0，他引：2  

孙卫东  胡艳华  丁兴  范安川  梁华英 《地学前缘》2007,14(2):139-148

总结了铜(Cu)、金(Au)、铼(Re)和氯(Cl)在汇聚板块边缘岩浆中的性质。在岛弧型的火山岩岩浆演化的早期,Cu、Au和Re均表现为中度不相容元素,含量随SiO2含量的增加而增加。在SiO2质量分数为58%时,多数岛弧型火山岩中Au、Cu的含量会突然大幅度下降。这一变化与铁和钛的变化是耦合的,铁和钛均由不相容元素变为相容元素,显示钛磁铁矿开始结晶了。进一步的研究表明,钛磁铁矿的结晶使硫酸根被还原为氢硫酸根,后者与Au、Cu形成氢硫酸根络合物,被萃取到流体相中,从而形成成矿流体。这一过程可以很好地解释Au、Cu矿床广泛分布于汇聚板块边缘的现象。与Au、Cu相反,Re的含量在SiO2质量分数为60%时才开始下降,而且是缓慢下降。这是因为Re通常比Au、Cu更亲石。此外,Re还具有强烈的挥发性。氯在东Manus岩浆中表现为高度不相容的特点。氯的性质主要受压力、初始水含量和岩浆演化分异程度的控制。计算结果显示,由于MORB和OIB含水量低,分异演化程度低,氯在上述岩浆中表现为高度不相容的特点。相比之下,氯在岛弧岩浆中的性质就复杂得多。随着水含量和岩浆房深度的不同,氯的性质可以从相容变到高度不相容。  相似文献   

长白山火山活动历史、岩浆演化与喷发机制探讨   总被引：18，自引：0，他引：18  

樊祺诚  隋建立  王团华  李霓  孙谦 《高校地质学报》2007,13(2):175-190

广义的长白山火山在我国境内包括著名的天池火山、望天鹅火山、图们江火山和龙岗火山,是我国最大的第四纪火山岩分布区。图们江火山和望天鹅火山活动都始于上新世,喷发活动分别介于上新世—中更新世（5.5~0.19 Ma）和上新世—早更新世（4.77 ~2.12 Ma）。天池火山和龙岗火山属于第四纪火山,喷发活动从早更新世（~2 Ma）持续到全新世。图们江火山岩为溢流式喷发的拉斑玄武岩,望天鹅火山、天池火山和龙岗火山母岩浆都是钾质粗面玄武岩,但经历了不同的演化过程。天池火山和望天鹅火山都经历了钾质粗面玄武岩造盾、粗面岩造锥和晚期碱性酸性岩浆（碱流岩和碱性流纹岩）的喷发;龙岗火山来自地幔的钾质粗面玄武岩浆则未经演化和混染直接喷出地表。图们江火山岩以溢流式喷发的拉斑玄武岩为主,少量玄武质粗安岩等。天池火山造盾之后,地壳岩浆房和地幔岩浆房具互动式喷发特点,来自地幔的钾质粗面玄武岩浆一方面在天池火山锥体内外形成诸多小火山渣锥,另一方面持续补给地壳岩浆房发生岩浆分离结晶作用和混合作用,分别导致双峰式火山岩分布特征和触发千年大喷发。火山岩微量元素和Sr-Nd-Pb同位素示踪揭示,长白山东（图们江火山、望天鹅火山和天池火山）、西（龙岗火山）两区显示地幔非均一性,东区岩浆源区具有软流圈地幔与富集岩石圈地幔混合特征,西区岩浆源区具有相对亏损的较原始地幔特征。西太平洋板块俯冲—东北亚大陆弧后引张是长白山火山活动的动力学机制。  相似文献   

北淮阳地区与斑岩型钼矿床相关岩浆岩的地质地球化学特征及成因   总被引：1，自引：0，他引：1  

王波华  张怀东  王萍  徐晓春  郝越进 《地学前缘》2016,23(4):46-62

位于秦岭-大别造山带东段的北淮阳地区分布有众多的斑岩型钼矿床,其成矿与岩浆作用紧密相关。对该区与斑岩型钼矿床密切相关的岩浆岩进行了系统的岩石化学、微量元素和同位素地球化学研究,深入探讨了其成因。研究认为,成矿岩体规模较小,岩性为花岗(斑)岩类,受北东向与北西向区域性断裂的次级构造控制。岩石化学成分以高硅、高钾、富碱为特征,为高钾钙碱性钾玄岩系列、准铝过铝质岩石。岩石微量、稀土元素特征相似并显示壳源特征。岩石Sr Nd Pb Hf同位素地球化学特征显示这些花岗质岩浆与整个大别地区白垩纪花岗岩的成岩物质来源一致,源于新元古界北大别片麻岩和扬子克拉通北缘TTG型岩浆,并混入一些古元古代扬子克拉通古老地壳物质(如崆岭杂岩)。在白垩纪发生的下地壳拆沉、软流圈上涌及大规模地壳伸展等机制下,扬子克拉通北缘的地壳熔融并提供了主要的成岩物质,幔源岩浆的上涌可能提供了热源,其物质的加入是次要的。该区与斑岩型钼矿床相关岩浆岩与东秦岭地区类似,属深源浅成型花岗岩类。  相似文献   

1966年邢台地震静态库仑应力触发分析     

李守勇  邹立晔  孙晴  赵爱平 《大地测量与地球动力学》2016,36(10):918-921

通过分析1966年邢台5次地震的静态库仑应力触发情况发现,前2次地震对后面的地震有较好的触发,而MS7.2以后地震的触发不理想。从而认为,随着地震的发生和震源深度的增加,岩浆活动对地壳介质的影响越来越大,地壳介质弹性性能越来越弱,即该区域浅部可以用均匀弹性半空间来近似,而深部在岩浆等因素的影响下,用均匀弹性半空间来近似存在较大的误差,不适合用弹性位错理论计算地震的触发关系。这从侧面反映了该地区岩浆活动的剧烈性和超壳断层存在的客观性。  相似文献   

冲绳海槽岩浆物理化学性质及其地质意义     

黄朋  李安春  胡宁静 《海洋学报》2008,30(3):85-94

借助冲绳海槽火山岩地球化学分析结果,讨论了海槽不同区段岩浆的温度、压力、密度和黏度等物理化学参数,以确定海槽岩浆的物理性质及其对海槽不同区段岩浆演化过程的影响.海槽北段的岩浆相对于中段表现出高压力、低温度的特征.由于海槽岩浆挥发分含量较高,北段岩浆的密度和黏度要高于中段的.但总的来说,海槽岩浆具有低密度、低黏度的特点,因此岩浆更容易穿透岩石圈,而且有利于岩浆结晶分异作用的进行.对海槽岩浆相对运移速度的研究显示,在外部条件及含水量相同的前提下,在海槽中段岩浆上升速度要大于北段的,这从岩浆物理化学性质的角度解释了为何海槽中段火山活动要强于北段的.  相似文献   

Formation and mechanics of magma reservoirs in Iceland     

Agust Gudmundsson 《Geophysical Journal International》1987,91(1):27-41

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Zircon U–Pb age and Hf isotope evidence for contrasting origin of bimodal protoliths for ultrahigh-pressure metamorphic rocks from the Chinese Continental Scientific Drilling project     

R.-X. CHEN  Y.-F. ZHENG  Z.-F. ZHAO  J. TANG  F.-Y. WU  X. M. LIU 《Journal of Metamorphic Geology》2007,25(8):873-894

A combined study of zircon morphology, U–Pb ages and Hf isotopes as well as whole‐rock major and trace elements was carried out for ultrahigh‐pressure (UHP) eclogite and felsic gneiss from the main hole (MH) of the Chinese Continental Scientific Drilling (CCSD) project in the Sulu orogen. The results show contrasting Hf isotope compositions for bimodal UHP metaigneous rocks, pointing to contrasting origins for their protoliths (thus dual‐bimodal compositions). The samples of interest were from two continuous core segments from CCSD MH at depths of 734.21–737.16 m (I) and 929.67–932.86 m (II) respectively. Zircon U–Pb dating for four samples from the two core segments yields two groups of ages at 784 ± 17 and 222 ± 3 Ma, respectively, corresponding to protolith formation during supercontinental rifting and metamorphic growth during continental collision. Although the Triassic UHP metamorphism significantly reset the zircon U–Pb system of UHP rocks, the Hf isotope compositions of igneous zircon can be used to trace their protolith origin. Contrasting types of initial Hf isotope ratios are, respectively, correlated with segments I and II, regardless of their lithochemistry. The first type shows positive ?_Hf(t) values of 7.8 ± 3.1 to 6.0 ± 3.0, with young Hf model age of 1.03 and 1.11 Ga. The second type exhibits negative ?_Hf(t) values of ?6.9 ± 1.6 to ?9.1 ± 1.1, with old Hf model ages of 2.11 and 2.25 Ga. It appears that the UHP rocks from the two segments have protoliths of contrasting origin. Consistent results are also obtained from their trace element compositions suggesting that mid‐Neoproterozoic protoliths of bimodal UHP metaigneous rocks formed during supercontinental rifting at the northern margin of the South China Block. Thus, the first type of bimodal magmatism formed by rapid reworking of juvenile crust, whereas the second type of bimodal magmatism was principally generated by rift anatexis of Paleoproterozoic crust. Melting of orogenic lithosphere has potential to bring about bimodal magmatism with contrasting origins. Because arc–continent collision zones are the best place to accumulate both juvenile and ancient crusts, the contrasting types of bimodal magmatism are proposed to occur in an arc–continent collision orogen during the supercontinental rifting, in response to the attempted breakup of the supercontinent Rodinia at c. 780 Ma.  相似文献   

从地壳上地幔构造看大陆碰撞带岩石圈的克拉通化   总被引：1，自引：0，他引：1  

杨文采  于常青 《地质论评》2014,60(4):721-740

本篇讨论超级大陆汇聚后逐渐变为克拉通或扩大克拉通的作用过程,即指经及大陆碰撞地体汇聚后新形成的大陆块逐渐转变为刚性克拉通的作用过程。增生大陆岩石圈的克拉通化的作用后果,包括大陆地壳密度的增加,岩石圈地幔的增厚和大地热流值的下降,使大陆岩石圈逐渐刚性强化。大陆碰撞后形成的大陆块必须经过克拉通化的过程,才能逐渐成为刚性克拉通。作用过程主要包括:①上地壳沉积碎屑岩石结晶岩化和中地壳岩石角闪岩化;②下地壳岩石基性化;③大陆碰撞带下凹莫霍面的磨平;④岩石圈地幔底侵加厚形成陆根。从大陆碰撞带转变为克拉通的过程也是岩石圈地幔不断增厚而地壳缓慢变硬变冷的过程。这个过程包含以下作用:区域变质作用,交代作用和岩石圈幔源岩浆的底侵。这个过程时间尺度比碰撞造山作用大一个级次。长期的底侵作用使地壳岩石密度和强度不断加大,改变岩层的矿物成分和局部结构。当大陆岩石圈克拉通化到一定程度之后,由于下方软流圈的热能供应逐渐减缓,使岩石圈地温梯度缓慢下降,最终结果会形成大陆根。由于显生宙大陆碰撞带岩石圈强度弱,大陆碰撞时更容易造成岩石圈变形,因此大陆碰撞的板内效应主要发生在大陆内的显生宙碰撞带。显生宙大陆碰撞带如果再次受到大陆碰撞板内效应的作用,其克拉通化的过程必然会推迟。  相似文献   

青藏高原东北缘柳坪新生代苦橄玄武岩地球化学及其大陆动力学意义   总被引：3，自引：2，他引：1  

赖绍聪  秦江锋  赵少伟  朱韧之 《岩石学报》2014,30(2):361-370

柳坪苦橄玄武岩出露在青藏高原东北缘特殊的构造部位,位于青藏、华北和扬子三大构造域的交接转换区域。岩石形成年龄在23~7.1Ma之间,属于新近纪火山岩。岩石SiO2介于41.72%~42.82%之间,Na2OK2O,K2O/Na2O平均0.51,为一套典型的幔源钠质碱性玄武岩类。岩石微量及稀土元素具板内火山岩特征,Th、Rb等元素呈较明显的富集状态,而岩石显著的低K2O特征(0.48%~0.90%)明显不同于青藏高原北缘新生代钾质-超钾质火山岩系列。岩石87Sr/86Sr(0.704158~0.704668)、143Nd/144Nd(0.512831~0.513352)、206Pb/204Pb(18.729871~18.779184)、207Pb/204Pb(15.591395~15.602454)和208Pb/204Pb(39.097372~39.181458)等同位素变化特征具有显著的混源属性,投影点位于EMI、EMII、BSE及PREMA等典型地幔储库的过渡部位,并可能存在HIUM地幔源的部分参与,明显不同于单一地幔源局部熔融形成的玄武岩的同位素组成特征。表明新生代期间青藏东缘西秦岭-松潘地区受青藏、扬子及华北三大构造体系域的控制,西秦岭-松潘构造结处于从下部地幔到上部陆壳物质的总体汇聚拼贴阶段,地幔具有显著的混合特征。柳坪苦橄玄武岩正是在这种特定的构造背景下,由于新生代青藏高原软流圈地幔物质向东的流动,诱发西秦岭-松潘构造结多源混合的地幔橄榄岩局部熔融而形成。  相似文献