MELTING AND SUBSOLIDUS PHASE-RELATIONS IN THE MGSIO3-MGCO3 SYSTEM AT HIGH-PRESSURES - IMPLICATIONS TO EVOLUTION OF THE EARTHS ATMOSPHERE

被引:110
作者
KATSURA, T
ITO, E
机构
[1] Institute for Study of the Earth's Interior, Okayama University, Misasa, Tottori-ken
关键词
D O I
10.1016/0012-821X(90)90074-8
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Melting and subsolidus phase relations in the MgSiO3MgCO3 system were investigated at 8 and 15 GPa and temperatures up to 2100°C and at 26 GPa and 1600°C using a uniaxial split-sphere anvil apparatus. Mineral assemblages of enstatite + magnesite and perovskite + magnesite are stable at 8 and 15 GPa and at 26 GPa, respectively, under subsolidus conditions. The melting temperature of magnesite increases with increasing pressure. Melting of the system shows a simple eutectic relation; the eutectic point shifts to lower MgCO3 content and to higher temperature with increasing pressure. Carbon dioxide is no longer a volcatile component at a depth of 140-720 km in the mantle and is retained as magnesite. A considerable amount of CO2 has been stored in the Earth's mantle for a long period of the Earth's history and is successively released through volcanism. © 1990.
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页码:110 / 117
页数:8
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