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The metallographic structure of the iron meteorites Arltunga, Kopjes ,Vlei, Murnpeowie, Braunau, and Rancho de la Pila

Published online by Cambridge University Press:  14 March 2018

H. J. Axon*
Affiliation:
Metallurgy Department, The University, Manchester 13

Summary

From a metallographic examination it is suggested that Rancho de la Pila is a shock-hardened octahedrite; Murnpeowie is a cosmically reheated meteorite of unusual composition; Kopjes Vlei may have been produced by the reheating of a shock-hardened hexahedrite either cosmically or on earth; Braunau shows signs of preterrestrial reheating but Arltunga is a nickel-rich ataxite with no signs of metabolic alteration.

Type
Research Article
Copyright
Copyright © The Mineralogical Society of Great Britain and Ireland 1968

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References

Axon, (H. J.), 1967. Metals and materials, vol. 1, pp. 8286.Google Scholar
El Goresy, (A.), 1965. Geochimic. Acta, vol. 29, pp. 11311151.CrossRefGoogle Scholar
Hey, (M. H.), 1966. Catalogue of meteorites, British Museum, London.Google Scholar
Perry, (S. H.), 1944. The metallography of meteoric iron, U.S. Nat. Mus. Bull. 184 Washington.Google Scholar
Smales, (A. A.), Mapper, (D.), and Fouché, (K. F.), 1967. Geochimic. Acta, vol. 31, pp. 673720.Google Scholar
Spencer, (L. J.), 1935. Min. Mag., vol. 24, pp. 13–2.Google Scholar