RARE EARTH CONTRIBUTION TO ORIGIN OF HAWAIIAN LAVAS

被引:108
作者
SCHILLING, JG
WINCHEST.JW
机构
[1] Graduate School of Oceanography, University of Rhode Island, Kingston, 02881, Rhode Island
[2] Department of Meteorology and Oceanography, University of Michigan, Ann Arbor, 48104, Michigan
关键词
D O I
10.1007/BF00371330
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
Rare earth abundances were determined by neutron activation in twenty Hawaiian lavas and one diabase of known chemical and mineralogical compositions. These results demonstrate a systematic relationship between the absolute or relative rare earth abundances and the petrochemistry of these rocks. Three distinct lava groups are recognized. These correspond to: (1) tholeiites, (2) alkali series, (3) nepheline-melilite basalts. Based on rare earths: a) The hawaiites and mugearite of the alkali series represent residual melts derived from alkali olivine basalts, most likely by fractional crystallization; the trachyte, however, seems to have a more complicated history. b) Fractional crystallization models linking nephelinites or alkali olivine basalts to tholeiites are possible. However, production of these three lava groups, independently, by various degrees of partial melting of the mantle is equally likely and cannot be distinguished from these fractional crystallization models. c) Daly limestone syntexis hypothesis to produce the nephelinites is unlikely. © 1969 Springer-Verlag.
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页码:27 / +
页数:1
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