The classification of micrometeorites

被引:243
作者
Genge, M. J. [1 ,2 ]
Engrand, C. [3 ]
Gounelle, M. [3 ]
Taylor, S. [4 ]
机构
[1] Univ London Imperial Coll Sci Technol & Med, IARC, Dept Earth Sci & Engn, London SW7 2AZ, England
[2] Nat Hist Museum, London SW7 2BT, England
[3] Univ Paris 11, Ctr Spectrometrie Nucl & Spectrometrie Masse, CNRS, IN2P3, F-91405 Orsay, France
[4] USA, Cold Reg Res & Engn Lab, Hanover, NH 03755 USA
关键词
D O I
10.1111/j.1945-5100.2008.tb00668.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
Due to their small size, the mineralogical and chemical properties of micrometeorites (MMs) are not representative of their parent bodies on the centimeter to meter scales that are used to define parent body groups through the petrological Study of meteorites. Identifying which groups Of MM are derived From the same type of parent body is problematic and requires particles to be rigorously grouped on the basis of mineralogical, textural, and chemical properties that reflect the fundamental genetic differences between meteorite parent bodies, albeit with minimal bias towards preconceived genetic models. Specifically, the interpretation of MMs requires a rigorous and meaningful classification scheme. At present the classification of MMs is, however, at best ambiguous. A unified petrological-chemical classification scheme is proposed in the current Study and is based on observations of several thousand MMs collected from Antarctic ice.
引用
收藏
页码:497 / 515
页数:19
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