NOBLE-GASES IN H-CHONDRITES AND POTENTIAL DIFFERENCES BETWEEN ANTARCTIC AND NON-ANTARCTIC METEORITES

被引:86
作者
SCHULTZ, L
WEBER, HW
BEGEMANN, F
机构
[1] Max-Planck-Institut für Chemie (Otto-Hahn-Institut)
关键词
D O I
10.1016/0016-7037(91)90399-P
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
Thirty-one Antarctic H-chondrites from the Allan Hills have been analyzed for their noble gases. Seven of the specimens contain solar gases; thirteen have a cosmic-ray exposure age around 8 Ma. Both fractions are as observed for H-chondrites from the rest of the world. Scrutiny of the data for "paired samples" yields a minimum number of 17 independent falls, with 6 falls required for the 8 Ma peak of exposure age. The distribution of exposure ages as well as that of radiogenic He-4 and Ar-40 yield no evidence that H-chondrites from the Allan Hills regions represent a mixture of populations that is different from that brought to moderate latitudes of the Earth in more recent times.
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页码:59 / 66
页数:8
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