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《科学》 2026年10月1日 · 中文解读

气泡—金属化合物将大气组分带入行星岩浆洋

Incorporation of atmospheric components in planetary magma oceans through bubble–metal compounds · F. Gaillard et al.
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法国奥尔良地球科学研究所的法布里斯·盖亚尔等人通过高温高压实验发现,在岩浆洋中气泡会牢固附着在金属液滴上形成复合体,从而抵抗金属与硅酸盐的分离。这种机制能让小行星等小天体在低重力下把碳、氢、氮等大气元素封存到内部,并可能解释地球地幔中铂族元素过剩而无需依赖“晚期薄层”假说。
原文开头
Fabrice Gaillard1*, Luiz Pereira2, Laurent Arbaret1, Giada Iacono- Marziano1, Emmanuel Le Trong1, Fabien Bernadou1,3, Yves Marrocchi4 Atmophile elements (carbon, hydrogen, and nitrogen) were thought to accrete late during planetary formation, yet cosmochemical and astrophysical evidence suggests that they were already present while small bodies, such as Vesta, were forming. High- temperature magmatic events on small bodies, however, should have outgassed these ultravolatile elements because gravity would have been insufficient to retain them. In this study, experiments reveal that gas bubbles strongly attach to metal droplets in magma ocean–like mixtures, forming compounds that resist segregation. early flotation of such compounds would have enhanced mantle siderophile endowment, eliminating the need for late accretion. …
摘自《科学》(Science)2026年10月1日,F. Gaillard et al.。仅引用开头一小段供了解文章,版权归原刊所有,全文请阅读原刊。
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