NEW DATA ON THE ABUNDANCE OF PALLADIUM IN METEORITES

被引:18
作者
MERMELENGAS, N
DELAETER, JR
ROSMAN, KJR
机构
[1] Department of Physics, Western Australian Institute of Technology, South Bentley
关键词
D O I
10.1016/0016-7037(79)90258-8
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
The concentration of Pd in 7 carbonaceous chondrites, 18 ordinary chondrites, 3 achondrites, 29 iron meteorites and other samples has been determined by stable isotope dilution using solid source mass spectrometry. The Cl chondrite Orgueil gives a 'cosmic' abundance for Pd of 1.5 (Si = 106 atoms), in good agreement with the currently accepted value. The concentration of Pd shows little variation among the carbonaceous chondrites, but in ordinary chondrites decreases from the H to L to LL groups. Pd in achondrites is approx 100 times lower than in chondrites. Data for iron meteorites plot around the 'cosmic' Pd Ni ratio; however the Pd data falls into distinct groups, corresponding to the chemical group classification. These results support the hypothesis that at least two fractionation processes have occurred during the formation of iron meteorites. © 1979.
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页码:747 / 753
页数:7
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