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
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.
引用
收藏
页码:1403 / 1405
页数:4
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