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Equilibrium thallium isotope fractionation and its constraint on Earth’s late veneer 被引量:3
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作者 Tong Fang Yun Liu 《Acta Geochimica》 EI CAS CSCD 2019年第4期459-471,共13页
Equilibrium isotope fractionation of thallium(Tl) includes the traditional mass-dependent isotope fractionation effect and the nuclear volume effect(NVE). The NVE dominates the overall isotope fractionation, especiall... Equilibrium isotope fractionation of thallium(Tl) includes the traditional mass-dependent isotope fractionation effect and the nuclear volume effect(NVE). The NVE dominates the overall isotope fractionation, especially at high temperatures. Heavy Tl isotopes tend to be enriched in oxidized Tl^3+-bearing species. Our NVE fractionation results of oxidizing Tl^+ to Tl^3+ can explain the positive enrichments observed in ferromanganese sediments. Experimental results indicate that there could be0.2–0.3 e-unit fractionation between sulfides and silicates at 1650 ℃. It is consistent with our calculation results,which are in the range of 0.17–0.38 e-unit. Importantly,Tl’s concentration in the bulk silicate Earth(BSE) can be used to constrain the amount of materials delivered to Earth during the late veneer accretion stage. Because the Tl concentration in BSE is very low and its Tl isotope composition is similar with that of chondrites, suggesting either no Tl isotope fractionation occurred during numerous evaporation events, or the Tl in current BSE was totally delivered by late veneer. If it is the latter, the Tl-contentbased estimation could challenge the magnitude of late veneer which had been constrained by the amount of highly siderophile elements in BSE. Our results show that the lateaccreted mass is at least five-times larger than the previously suggested magnitude, i.e., 0.5 wt% of current Earth’s mass. The slightly lighter 205 Tl composition of BSE relative to chondrites is probable a sign of occurrence of Tlbearing sulfides, which probably were removed from the mantle in the last accretion stage of the Earth. 展开更多
关键词 EQUILIBRIUM TL isotope fractionation Nuclear volume effect TL fractionations between SILICATES and sulfides late veneer First-principles calculation
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地球早期演化的Hf-W同位素制约 被引量:4
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作者 梅清风 杨进辉 《岩石学报》 SCIE EI CAS CSCD 北大核心 2018年第1期207-216,共10页
^(182)Hf-^(182)W作为短周期放射性衰变体系,可有效约束地球早期演化吸积增生和内部分异过程。本文通过系统总结、归纳太阳系形成初期地球核幔分异过程中Hf-W同位素变化规律、月球与地球硅酸盐的W同位素组成,提出利用^(182)Hf-^(182)W... ^(182)Hf-^(182)W作为短周期放射性衰变体系,可有效约束地球早期演化吸积增生和内部分异过程。本文通过系统总结、归纳太阳系形成初期地球核幔分异过程中Hf-W同位素变化规律、月球与地球硅酸盐的W同位素组成,提出利用^(182)Hf-^(182)W体系测定地球核幔分异时间不确定性的主要原因是地球核幔分异的持续性及开放性,大碰撞时间的^(182)Hf-^(182)W同位素限定主要受控于硅酸盐地球和硅酸盐月球的Hf/W比值,讨论了地幔W同位素不均一性的形成机制,与现代地幔不同的^(182)W/^(184)W组成可能代表了后增生作用之前整体硅酸盐地球的W同位素组成,也可能是^(182)Hf未完全灭绝时形成的区域性Hf/W比值差异经^(182)Hf衰变形成的结果。这些结论为探索类地行星形成与演化提供了重要制约。 展开更多
关键词 灭绝核素 核幔分异 形成月球大碰撞 后增薄层模型
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亲铁元素异常——后增薄层模型 被引量:1
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作者 朱丹 高振敏 +3 位作者 罗泰义 李晓彪 柏坚 普传杰 《矿物岩石地球化学通报》 CAS CSCD 2003年第1期65-68,共4页
地幔中铂族元素丰度是基于地球形成理论所得计算值的两三百倍,无论是地幔中还是球粒陨石中,铂族元素之间的比值是相近的;对于这一现象有很多解释,其中被普遍接受的是:地核形成后(核幔分异完成后),大约占现在地球质量0.5%~1%的球粒陨石... 地幔中铂族元素丰度是基于地球形成理论所得计算值的两三百倍,无论是地幔中还是球粒陨石中,铂族元素之间的比值是相近的;对于这一现象有很多解释,其中被普遍接受的是:地核形成后(核幔分异完成后),大约占现在地球质量0.5%~1%的球粒陨石物质加入地幔,即可造成现在地幔中的铂族元素在丰度与比值方面的特征,这就是后增薄层模型(Late veneermodel)。但是,这一模型受到很多地幔样品铂族元素具非球粒陨石比值和高压下Co、Ni亲铁性测定结果的挑战。最近的地幔橄榄岩各相铂族元素精确测定、高压下Pt、Pd金属相与硅酸盐分配系数的测定,以及Re Os同位素的研究都支持后增薄层模型。 展开更多
关键词 铂族元素 地慢 橄榄岩 亲铁元素 锇同位素 后增薄层假说 球粒陨石
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