| Reference Type | Journal (article/letter/editorial) |
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| Title | The metallographic structure of the iron meteorites Arltunga, Kopjes ,Vlei, Murnpeowie, Braunau, and Rancho de la Pila |
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| Journal | Mineralogical Magazine and Journal of the Mineralogical Society |
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| Authors | Axon, H. J. | Author |
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| Year | 1968 (December) | Volume | 36 |
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| Issue | 284 |
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| Publisher | Mineralogical Society |
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| Download URL | https://rruff.info/doclib/MinMag/Volume_36/36-284-1139.pdf+ |
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| DOI | doi:10.1180/minmag.1968.036.284.10Search in ResearchGate |
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| Generate Citation Formats |
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| Mindat Ref. ID | 6210 | Long-form Identifier | mindat:1:5:6210:1 |
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| GUID | 0 |
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| Full Reference | Axon, H. J. (1968) The metallographic structure of the iron meteorites Arltunga, Kopjes ,Vlei, Murnpeowie, Braunau, and Rancho de la Pila. Mineralogical Magazine and Journal of the Mineralogical Society, 36 (284) 1139-1142 doi:10.1180/minmag.1968.036.284.10 |
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| Plain Text | Axon, H. J. (1968) The metallographic structure of the iron meteorites Arltunga, Kopjes ,Vlei, Murnpeowie, Braunau, and Rancho de la Pila. Mineralogical Magazine and Journal of the Mineralogical Society, 36 (284) 1139-1142 doi:10.1180/minmag.1968.036.284.10 |
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| In | (1966) Mineralogical Magazine Vol. 36 (284) Mineralogical Society |
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| Abstract/Notes | SummaryFrom 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. |
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