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Large gem diamonds from metallic liquid in Earth's deep mantle
被引:273
|作者:
Smith, Evan M.
[1
]
Shirey, Steven B.
[2
]
Nestola, Fabrizio
[3
]
Bullock, Emma S.
[4
]
Wang, Jianhua
[2
]
Richardson, Stephen H.
[5
]
Wang, Wuyi
[1
]
机构:
[1] Gemol Inst Amer, New York, NY 10036 USA
[2] Carnegie Inst Sci, Dept Terr Magnetism, 5241 Broad Branch Rd NW, Washington, DC 20015 USA
[3] Univ Padua, Dept Geosci, I-35131 Padua, Italy
[4] Carnegie Inst Sci, Geophys Lab, 5251 Broad Branch Rd NW, Washington, DC 20015 USA
[5] Univ Cape Town, Dept Geol Sci, ZA-7701 Rondebosch, South Africa
来源:
基金:
美国国家科学基金会;
欧洲研究理事会;
关键词:
II DIAMONDS;
IRON CARBIDE;
INCLUSIONS;
STABILITY;
MELT;
D O I:
10.1126/science.aal1303
中图分类号:
O [数理科学和化学];
P [天文学、地球科学];
Q [生物科学];
N [自然科学总论];
学科分类号:
07 ;
0710 ;
09 ;
摘要:
The redox state of Earth's convecting mantle, masked by the lithospheric plates and basaltic magmatism of plate tectonics, is a key unknown in the evolutionary history of our planet. Here we report that large, exceptional gem diamonds like the Cullinan, Constellation, and Koh-i-Noor carry direct evidence of crystallization from a redox-sensitive metallic liquid phase in the deep mantle. These sublithospheric diamonds contain inclusions of solidified iron-nickel-carbon-sulfur melt, accompanied by a thin fluid layer of methane +/- hydrogen, and sometimes majoritic garnet or former calcium silicate perovskite. The metal-dominated mineral assemblages and reduced volatiles in large gem diamonds indicate formation under metal-saturated conditions. We verify previous predictions that Earth has highly reducing deep mantle regions capable of precipitating a metallic iron phase that contains dissolved carbon and hydrogen.
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页码:1403 / 1405
页数:4
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