NO LIQUID IMMISCIBILITY IN THE SYSTEM MGSIO3-SIO2 AT 5.0 GPA

Citation
Ja. Dalton et Dc. Presnall, NO LIQUID IMMISCIBILITY IN THE SYSTEM MGSIO3-SIO2 AT 5.0 GPA, Geochimica et cosmochimica acta, 61(12), 1997, pp. 2367-2373
Citations number
28
Categorie Soggetti
Geochemitry & Geophysics
ISSN journal
00167037
Volume
61
Issue
12
Year of publication
1997
Pages
2367 - 2373
Database
ISI
SICI code
0016-7037(1997)61:12<2367:NLIITS>2.0.ZU;2-P
Abstract
Liquidus phase relationships in the system MgSiO3-SiO2 at 5.0 GPa have been determined using a multianvil apparatus. Compared to phase relat ionships at 1 atm, the MgSiO3-SiO2 phase diagram at 5.0 GPa is signifi cantly different in two respects. First, the composition of the eutect ic between MgSiO3 and SiO2 moves from 65.0 wt% SiO2 at 1 atm/1547 degr ees C (protoenstatite-cristobalite eutectic; Bowen and Andersen, 1914) to 68.8 wt% SiO2 (orthoenstatite-coesite eutectic) at 5.0 GPa/1930 de grees C. Second, no stable two-liquid held is present in the MgSiO3-Si O2 system at 5.0 GPa. The unbroken coesite liquidus curve is inflected indicating the presence of a submerged, metastable miscibility gap be low the liquidus. Thus, although the temperature of the solvus critica l point is likely to increase with pressure, the dT/dP slope of the Si O2 liquidus is much steeper and as a result, the immiscibility dome ha s become submerged completely. The reduction in liquid immiscibility i n the MgSiO2-SiO2 system at 5.0 GPa implies that in more complex syste ms relevant to the Earth, immiscibility will also be suppressed at hig h pressures. Copyright (C) 1997 Elsevier Science Ltd.