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Evaporative fractionation of zinc during the first nuclear detonation

机译:第一次核爆中锌的蒸发分馏

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摘要

Volatile element and compound abundances vary widely in planets and were set during the earliest stages of solar system evolution. Experiments or natural analogs approximating these early conditions are limited. Using silicate glass formed from arkosic sands during the first nuclear detonation at the Trinity test site, New Mexico, we show that the isotopes of zinc were fractionated during evaporation. The green silicate glasses, termed “trinitite,” show +0.5 ± 0.1‰/atomic mass unit isotopic fractionation from ~200 m to within 10 m of ground zero of the detonation, corresponding to an α fractionation factor between 0.999 and 0.9995. These results confirm that Zn isotopic fractionation occurs through evaporation processes at high temperatures. Evidence for similar fractionations in lunar samples consequently implies a volatile-depleted bulk Moon, with evaporation occurring during a giant impact or in a magma ocean.
机译:挥发性元素和化合物的丰度在行星中变化很大,并且是在太阳系演化的最早阶段设定的。近似这些早期条件的实验或天然类似物是有限的。在新墨西哥的三位一体试验场中,在第一次核爆中,使用由方铁砂形成的硅酸盐玻璃,我们发现锌的同位素在蒸发过程中被分馏。绿色硅酸盐玻璃被称为“三亚硝酸盐”,在爆轰离零点约200 m至10 m以内显示+0.5±0.1‰/原子质量单位的同位素分馏,对应于0.999至0.9995之间的α分馏系数。这些结果证实锌同位素分馏通过高温下的蒸发过程发生。因此,在月球样品中进行类似分级分离的证据表明,月亮的挥发物已耗尽,在巨大撞击或岩浆海洋中会发生蒸发。

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