期刊名称:Proceedings of the National Academy of Sciences
印刷版ISSN:0027-8424
电子版ISSN:1091-6490
出版年度:2020
卷号:117
期号:18
页码:9747-9754
DOI:10.1073/pnas.1917448117
出版社:The National Academy of Sciences of the United States of America
摘要:Sub-Neptunes are common among the discovered exoplanets. However, lack of knowledge on the state of matter in H 2 O-rich setting at high pressures and temperatures ( P − T ) places important limitations on our understanding of this planet type. We have conducted experiments for reactions between S i O 2 and H 2 O as archetypal materials for rock and ice, respectively, at high P − T . We found anomalously expanded volumes of dense silica (up to 4%) recovered from hydrothermal synthesis above ∼24 GPa where the C a C l 2 -type (Ct) structure appears at lower pressures than in the anhydrous system. Infrared spectroscopy identified strong OH modes from the dense silica samples. Both previous experiments and our density functional theory calculations support up to 0.48 hydrogen atoms per formula unit of ( S i 1 − x H 4 x ) O 2 ( x = 0.12 ) . At pressures above 60 GPa, H 2 O further changes the structural behavior of silica, stabilizing a niccolite-type structure, which is unquenchable. From unit-cell volume and phase equilibrium considerations, we infer that the niccolite-type phase may contain H with an amount at least comparable with or higher than that of the Ct phase. Our results suggest that the phases containing both hydrogen and lithophile elements could be the dominant materials in the interiors of water-rich planets. Even for fully layered cases, the large mutual solubility could make the boundary between rock and ice layers fuzzy. Therefore, the physical properties of the new phases that we report here would be important for understanding dynamics, geochemical cycle, and dynamo generation in water-rich planets.
关键词:silica ; water ; sub-Neptunes ; waterworlds ; exoplanets