火花源质谱法定量分析岩石样品

叙述了一种定量分析岩石中微量元素的火花源质谱法。大约10～25毫克绝缘粉末样品直接压在T型电极上。在选定的分析条件下进行单曝光摄谱。用AGV—1做标准样品,计算相对灵敏度因子。此方法可分析24个元素。相对标准偏差为±20％。做了地幔和月岩等样品分析。     

太空(FeNi)金属熔体凝固的时空图象和结晶机理研究

岩庄陨石冲击重熔再结晶(FeNi)金属颗粒的微结构研究发现,四同心环生长结构是远离热力学平衡态的太空(FeNi)金属熔体凝固的基本时空图象。四同心环结构的快速生长和相互作用导致八面体(FeNi)金属枝晶的形成。四同心环晶体生长方式可能是太空环境下(FeNi)金属熔体结晶形成八面体铁陨石的一种基本方式。     

RAMAN SPECTROSCOPY OF C,H,L AND LL CHONDRITES AND ITS SIGNIFICANCE IN EXPLORING THE FORMATION ENVIRONMENTS OF METEORITES AND THEIR TAXONOMY

The comparison of Raman spectra of the chondrites (C, H, L, LL) has confirmed thatthere exist two types of meteorite carbon: one is the primary carbon present in carbonaceouschondrites (c) and the other is the secondary carbon contained in ordinary chondrites (H, L,LL). The parameter of order (I_G/I_D intensity ratio, similarly hereinafter) of primary car-bon tends to decrease with increasing petrologic type and it can reflect the temperature ofdust carrier at the time plasma gases in the early nebula were condensed to form primarycarbonaceous material and the hydrogen content in primary carbonaceous material. This kindof primary carbonaceous material maybe has not experienced late stage thermometamorphismwithin the parent body of chondrites, indicating that the carbonaceous chondrites wereformed and retained in the low temperature region of the solar system. The parameter oforder of the secondary carbon tends to increase with increasing petrologic type and it can re-flect the degree of graphitization o     

C,H,L,LL球粒陨石的Raman光谱研究及对陨石形成环境与分类的意义

本文对球粒陨石(C,H,L,LL)的Raman光谱比较研究证明,存在两种类型的陨石碳质:一是碳质球粒陨石(C)的原生碳质,它的有序参量(I_G/I_D强度比,下同)随岩石学类型升高而减小;另一是普通球粒陨石(H,L,LL)的次生碳质,它的有序参量随岩石学类型升高而增大,这些事实支持碳质球粒陨石起源于彗星和Alfven等人的由等离子体星云到行星的假说。