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首页> 外文期刊>American Mineralogist >The behavior of Li and B in lunar mare basalts during crystallization, shock, and thermal metamorphism: Implications for volatile element contents of martian basalts
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The behavior of Li and B in lunar mare basalts during crystallization, shock, and thermal metamorphism: Implications for volatile element contents of martian basalts

机译:Li和B在月球母玄武岩结晶,冲击和热变质过程中的行为:对火星玄武岩中挥发性元素含量的影响

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摘要

Late-stage rims of magmatic pyroxenes from some martian basalts show decreases in Li and B contents relative to earlier-formed pyroxene cores. This behavior is different than expected from their documented incompatible element behavior. Previous workers interpreted such depletions to reflect the loss of several wt% magmatic water during basalt crystallization. This interpretation has profound implications for the nature of the martian mantle and recent exchange of volatiles between the martian mantle and atmosphere. To assess alternative mechanisms that may influence the behavior of Li and B in the absence of aqueous fluid activity, the effects of changing pyroxene composition during crystallization, shock pressure, and shock-associated thermal metamorphism were studied. Lithium and B depletions are documented in late-stage rims of pyroxenes from anhydrous lunar basalts indicating that mechanisms other than aqueous fluid activity must have influenced Li and B partitioning in these pyroxenes. Depletions of Li and B are most likely associated with changing pyroxene composition during crystallization, and occur in lunar and martian pyroxenes with late-stage Fe-enrichment. It is interesting that pyroxenes without late-stage Fe-enrichment show no concomitant Li and B increases. Lithium loss may occur during breakdown of metastable pyroxferroite. Additionally, changes in Cr content may influence the substitution mechanism involved for incorporating Li. Shock does not redistribute Li or B but may facilitate subsequent thermally driven diffusion by the introduction of mechanical defects in grains. Thermally metamorphosed pyroxenes exhibit higher Li and lower B contents relative to unheated pyroxenes. It is likely, therefore, that Li and B are redistributed through interactions between pyroxenes and surrounding zones of mesostasis during thermal metamorphism.
机译:与某些早期形成的 的岩浆辉石的后期边缘显示Li和B含量降低。此行为与 记录的不兼容元素行为不同。以前的工人 解释了这种消耗,以反映玄武岩结晶过程中几种wt% 岩浆水的损失。这种解释 对火星地幔 的性质以及火星地幔 和大气之间最近的挥发物交换具有深远的意义。为了评估在没有水流体活性的情况下可能影响Li和B行为的其他机制, 在结晶过程中改变辉石成分的影响, 的冲击压力和与冲击有关的热变质作用。在无水玄武岩中辉石的后期 轮缘中记录了锂和B的消耗,表明除水流体活动性以外的 机理必定影响了 Li和B在这些辉石中分配。 Li和 的耗尽最有可能与结晶过程中辉石组成的变化有关,并且发生在月相和火星的辉石中,并且在后期Fe-丰富。有趣的是,没有后期富铁的辉石 没有伴随的Li和 B的增加。在亚稳 pyferferroite分解过程中可能会发生锂损失。此外,Cr含量的变化可能会影响 掺入Li的取代机理。 Shock 不会重新分配Li或B,但可能会通过在晶粒中引入机械 缺陷来促进随后的 热驱动扩散。热变质的辉石相对于未加热的辉石显示 更高的Li和更低的B含量。 因此,Li和B可能通过 相互作用而重新分布热变质过程中辉石与介晶相变区 之间的关系。

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  • 来源
    《American Mineralogist》 |2006年第10期|1553-1564|共12页
  • 作者单位

    Institute of Meteoritics, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131-1126, U.S.A.;

    Institute of Meteoritics, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131-1126, U.S.A.;

    Institute of Meteoritics, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131-1126, U.S.A.;

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