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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >The origin of volatile element depletion in early solar system material: Clues from Zn isotopes in chondrules
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The origin of volatile element depletion in early solar system material: Clues from Zn isotopes in chondrules

机译:早期太阳系材料中挥发性元素耗尽的起源:软骨中Zn同位素的线索

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摘要

Volatile lithophile elements are depleted in the different planetary materials to various degrees, but the origin of these depletions is still debated. Stable isotopes of moderately volatile elements such as Zn can be used to understand the origin of volatile element depletions. Samples with significant volatile element depletions, including the Moon and terrestrial tektites, display heavy Zn isotope compositions (i.e. enrichment of Zn-66 vs. Zn-64), consistent with kinetic Zn isotope fractionation during evaporation. However, Luck et al. (2005) found a negative correlation between delta Zn-66 and 1/[Zn] between CI, CM, CO, and CV chondrites, opposite to what would be expected if evaporation caused the Zn abundance variations among chondrite groups.
机译:挥发性碎石元素在不同的行星材料中耗尽到各种程度,但这些耗尽的起源仍然讨论。 中等挥发性元素如Zn的稳定同位素可用于理解挥发性元素耗尽的起源。 具有显着的挥发性元素耗尽的样品,包括月球和地球赛牙,显示重Zn同位素组合物(即Zn-66对Zn-64的富集),与蒸发过程中的动力学Zn同位素分馏一致。 但是,幸运等人。 (2005)发现CI,CM,CO和CV Chondrites之间的Delta Zn-66和1 / Zn之间的负相关性,与蒸发在填充群中引起Zn丰度变异的预期相反。

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