No liquid immiscibility in the system MgSiO3-SiO2 at 5.0 GPa

被引:21
作者
Dalton, JA
Presnall, DC
机构
[1] Magmalogy Laboratory, Department of Geosciences, University of Texas at Dallas, Richardson
关键词
D O I
10.1016/S0016-7037(97)00072-0
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
Liquidus phase relationships in the system MgSiO3-SiO2 at 5.0 GPa have been determined using a multianvil apparatus. Compared to phase relationships at 1 atm, the MgSiO3-SiO2 phase diagram at 5.0 GPa is significantly different in two respects. First, the composition of the eutectic between MgSiO3 and SiO2 moves from 65.0 wt% SiO2 at 1 atm/1547 degrees C (protoenstatite-cristobalite eutectic; Bowen and Andersen, 1914) to 68.8 wt% SiO2 (orthoenstatite-coesite eutectic) at 5.0 GPa/1930 degrees C. Second, no stable two-liquid held is present in the MgSiO3-SiO2 system at 5.0 GPa. The unbroken coesite liquidus curve is inflected indicating the presence of a submerged, metastable miscibility gap below the liquidus. Thus, although the temperature of the solvus critical point is likely to increase with pressure, the dT/dP slope of the SiO2 liquidus is much steeper and as a result, the immiscibility dome has become submerged completely. The reduction in liquid immiscibility in the MgSiO2-SiO2 system at 5.0 GPa implies that in more complex systems relevant to the Earth, immiscibility will also be suppressed at high pressures. Copyright (C) 1997 Elsevier Science Ltd.
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页码:2367 / 2373
页数:7
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