The Kaidun meteorite: Composition and origin of inclusions in the metal of an enstatite chondrite clast

被引:25
作者
Ivanov, AV
MacPherson, GJ
Zolensky, ME
Kononkova, NN
Migdisova, LF
机构
[1] SMITHSONIAN INST,DEPT MINERAL SCI,WASHINGTON,DC 20560
[2] NASA,LYNDON B JOHNSON SPACE CTR,DIV EARTH SCI & SOLAR SYST EXPLORAT,HOUSTON,TX 77058
来源
METEORITICS & PLANETARY SCIENCE | 1996年 / 31卷 / 05期
关键词
D O I
10.1111/j.1945-5100.1996.tb02034.x
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
Metal nodules are one of the major textural components of Kaidun sample #01.3.06 EH3-4. In terms of structure, the nodules are of three types: (1) globular, (2) zoned with a massive core and globular mantle, and (3) nodules with no internal structure. The size and composition of the globules in the nodules and grains of metal of the matrix are almost identical: no greater than 20 mu m and Ni, 5.95; Si, 3.33 wt%. The nodules contain small (usually <5 mu m) inclusions of SiO2; albitic glass; enstatite; roedderite; and a mixture of SiO2 and Na2S2. This is the first reported occurrence of a simple sulfide of an alkaline metal in nature. The formation of the inclusions appears to be related to condensation of material onto the surfaces of metal grains. The nodules appear to have formed by aggregation of separate grains (globules) of metal, with conservation of condensates on the grain surfaces as inclusions. The inclusions probably condensed over a significant temperature range from 1400 to 600 K. The aggregation of metal grains and formation of the nodules probably occurred simultaneously with condensation.
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页码:621 / 626
页数:6
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