SILICA-UNDERSATURATED SAPPHIRINE, SPINEL AND KORNERUPINE GRANULITE FACIES ROCKS, NE STRANGWAYS RANGE, CENTRAL AUSTRALIA

被引:48
作者
GOSCOMBE, B [1 ]
机构
[1] UNIV MELBOURNE,DEPT GEOL,PARKVILLE,VIC 3052,AUSTRALIA
关键词
ARUNTA BLOCK; GRANULITE FACIES ROCKS; KORNERUPINE; P-T PATHS; SAPPHIRINE;
D O I
10.1111/j.1525-1314.1992.tb00078.x
中图分类号
P5 [地质学];
学科分类号
0709 ; 081803 ;
摘要
Small pods of silica-undersaturated Al-rich and Mg-rich granulite facies rocks containing sapphirine, pleonastic spinel, kornerupine, cordierite, orthopyroxene, corundum, sillimanite and gedrite are scattered throughout the NE Strangways Range, Central Australia. These are divided into four distinct rock types, namely orthopyroxene-rich aluminous granofels and metapelitic gneisses containing sapphirine, spinel or kornerupine. Two granulite facies metamorphic events are recognized, of which only the first (M1) is considered in this paper. Peak metamorphic mineral parageneses indicate that the M1 thermal maximum occurred at approximately 900-950-degrees-C and 8-9 kbar. All samples are characterized by profuse and diverse coronitic and symplectic reaction textures. These are interpreted as evidence for the sequential crossing of the following reactions in the system FMAS: cordierite + spinel + corundum = sapphirine + sillimanite, cordierite + spinel = orthopyroxene + sapphirine + sillimanite, sapphirine + spinel + sillimanite = orthopyroxene + corundum, sapphirine + sillimanite = cordierite + orthopyroxene + corundum. Phase stability relationships in FMAS and MASH indicate an anticlockwise P-T path terminated by isobaric cooling. Such a path is exemplified by early low-P mineral parageneses containing spinel, corundum and gedrite and the occurrence of both prograde and retrograde corundum. Reaction textures preserve evidence for an increase in a(H2O) and a(B2O3) with progressive isobaric cooling. This hydrous retrogression resulted from crystallization of intimately associated M1 partial melt segregations. There is no evidence for voluminous magmatic accretion giving rise to the high M1 thermal gradient. The M1 P-T path may be the result of either lithospheric thinning after both crustal thickening and burial of the supracrustal terrane, or concomitant crustal thickening and mantle lithosphere thinning.
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页码:181 / 201
页数:21
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