کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
6427066 | 1634700 | 2016 | 8 صفحه PDF | دانلود رایگان |
![عکس صفحه اول مقاله: High-pressure melting experiments on Fe-Si alloys and implications for silicon as a light element in the core High-pressure melting experiments on Fe-Si alloys and implications for silicon as a light element in the core](/preview/png/6427066.png)
- The melting phase relations in the Fe-FeSi binary system were studied to 127 GPa.
- The eutectic composition becomes depleted in silicon with increasing pressure.
- Silicon cannot be a single light element in the core.
We carried out melting experiments on Fe-Si alloys to 127 GPa in a laser-heated diamond-anvil cell (DAC). On the basis of textural and chemical characterizations of samples recovered from a DAC, a change in eutectic liquid composition in the Fe-FeSi binary system was examined with increasing pressure. The chemical compositions of coexisting liquid and solid phases were quantitatively determined with field-emission-type electron microprobes. The results demonstrate that silicon content in the eutectic liquid decreases with increasing pressure to less than 1.5±0.1 wt.% Si at 127 GPa. If silicon is a single light element in the core, 4.5 to 12 wt.% Si is required in the outer core in order to account for its density deficit from pure iron. However, such a liquid core, whose composition is on the Si-rich side of the eutectic point, crystallizes less dense solid, CsCl (B2)-type phase at the inner core boundary (ICB). Our data also show that the difference in silicon concentration between coexisting solid and liquid is too small to account for the observed density contrast across the ICB. These indicate that silicon cannot be the sole light element in the core. Previous geochemical and cosmochemical arguments, however, strongly require â¼6 wt.% Si in the core. It is possible that the Earth's core originally included â¼6 wt.% Si but then became depleted in silicon by crystallizing SiO2 or MgSiO3.
Journal: Earth and Planetary Science Letters - Volume 456, 15 December 2016, Pages 47-54