Mossbauer studies of Soltmany and Shisr 176 meteorites - comparison with other ordinary chondrites

被引：18

作者：

Galazka-Friedman, J. ^{[1
]}

Szlachta, K. ^{[1
]}

Karwowski, L. ^{[2
]}

Wozniak, M. ^{[3
]}

机构：

[1] Warsaw Univ Technol, Fac Phys, PL-00662 Warsaw, Poland

[2] Univ Silesia, Fac Earth Sci, Sosnowiec, Poland

[3] Univ Warsaw, Fac Biol, Warsaw, Poland

来源：

HYPERFINE INTERACTIONS | 2014年 / 226卷 / 1-3期

关键词：

Ordinary chondrites; Classification of meteorites; Soltmany meteorite; Shisr; 176; meteorite; SPECTROSCOPY;

D O I：

10.1007/s10751-013-0944-0

中图分类号：

O64 [物理化学（理论化学）、化学物理学]; O56 [分子物理学、原子物理学];

学科分类号：

070203 ; 070304 ; 081704 ; 1406 ;

摘要：

Two ordinary chondrites type L6: Soltmany and Shisr 176, were recently investigated in our laboratory. The distribution of iron in the 4 main iron bearing mineral phases (olivine, pyroxene, kamacite and troilite) determined by Mossbauer spectroscopy in Soltmany and Shisr 176 meteorites was very different from that in the Baszkowka meteorite (type L5). To explain the cause of this difference, a comparison of the distribution of iron among the main mineral phases present in other type L and H meteorites was performed. Our studies have shown that the Baszkowka meteorite is not a good point of reference for Soltmany and Shisr 176 meteorites.

引用

页码：593 / 600

页数：8

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