Abstract
METALLIC meteorites are composed in, varying proportions of two iron–nickel metallic solid solutions, kamacite, which has a low nickel content, and taenite, which has a higher nickel content. The structure and distribution of these phases have been extensively examined on a macro- and on a micro-scale. Many iron meteorites also contain non-metallic inclusions of an iron–nickel phosphide (schreibersite) or an iron–nickel sulphide (troilite). Troilite has not been subject to very detailed microscopic examination for two reasons. First, it shows a great tendency to chip and disintegrate during preparation and, secondly, it is very reactive towards most etching agents ; hence, when metallic meteorites are deeply etched for museum exhibition the troilite is usually protected from the etching agent by a suitable stopping-off compound.
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References
Perry, S. H., “The Metallography of Meteoritic Iron”, pl. 6 (Smithsonian Institution, Washington, 1944).
Williams, R. S., and Homerberg, V. O., “Principles of Metallography”, 234 (McGraw-Hill, 1948).
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AXON, H. The Sulphide Phase in Some Iron Meteorites. Nature 187, 406–407 (1960). https://doi.org/10.1038/187406a0
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DOI: https://doi.org/10.1038/187406a0
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