DEPTH AND DEGREE OF MELTING OF KOMATIITES

被引:254
作者
HERZBERG, C [1 ]
机构
[1] SUNY STONY BROOK, INST MINERAL PHYS, STONY BROOK, NY 11794 USA
关键词
D O I
10.1029/91JB03066
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
High pressure melting experiments have permitted new constraints to be placed on the depth and degree of partial melting of komatiites. Komatiites from Gorgona Island were formed by relatively low degrees of pseudoinvariant melting (< 30%) involving L + Ol + Opx + Gt on the solidus at 40 kbar, about 130 km depth. Munro-type komatiites were separated from a harzburgite residue (L + Ol + Opx) at pressures that are poorly constrained, but were probably around 50 kbar, about 165 km depth; the degree of partial melting was < 40%. Komatiites from the Barberton Mountain Land were formed by high degrees (approximately 50%) of pseudoinvariant melting (L + Ol + Gt + Cpx) of fertile mantle peridotite in the 80- to 100-kbar range, about 260- to 330- km depth. Secular variations in the geochemistry of komatiites could have formed in response to a reduction in the temperature and pressure of melting with time. The 3.5 Ga Barberton komatiites and the 2.7 Ga Munro-type komatiites could have formed in plumes that were hotter than the present-day mantle by 500-degrees and 300-degrees, respectively. When excess temperatures are this size, melting is deeper and volcanism changes from basaltic to komatiitic. The komatiites from Gorgona Island, which are Mesozoic in age, may be representative of komatiites that are predicted to occur in oceanic plateaus of Cretaceous age throughout the Pacific [Storey et al., 1991].
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页码:4521 / 4540
页数:20
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