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Axon, H. J., Waine, C. V. (1971) A metallographic study of the angra dos Reis (iron) meteorite. Mineralogical Magazine, 38 (293) 94-101 doi:10.1180/minmag.1971.038.293.13

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Reference TypeJournal (article/letter/editorial)
TitleA metallographic study of the angra dos Reis (iron) meteorite
JournalMineralogical Magazine
AuthorsAxon, H. J.Author
Waine, C. V.Author
Year1971 (March)Volume38
Issue293
PublisherMineralogical Society
Download URLhttps://rruff.info/doclib/MinMag/Volume_38/38-293-94.pdf+
DOIdoi:10.1180/minmag.1971.038.293.13Search in ResearchGate
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Mindat Ref. ID6438Long-form Identifiermindat:1:5:6438:9
GUID0
Full ReferenceAxon, H. J., Waine, C. V. (1971) A metallographic study of the angra dos Reis (iron) meteorite. Mineralogical Magazine, 38 (293) 94-101 doi:10.1180/minmag.1971.038.293.13
Plain TextAxon, H. J., Waine, C. V. (1971) A metallographic study of the angra dos Reis (iron) meteorite. Mineralogical Magazine, 38 (293) 94-101 doi:10.1180/minmag.1971.038.293.13
In(1971, March) Mineralogical Magazine Vol. 38 (293) Mineralogical Society
Abstract/NotesSummaryThe Angra dos Reis (iron) has been studied metallographically and an attempt has been made to discuss the circumstances under which the following elements of structure formed: clear etching and frosty etching kamacite, decorated Neumann lines, giant rhabdites, plate rbabdites, rhabdite clusters, microrhabdites, cohenite, and remelted troilite. The remelted troilite is taken to indicate a shock event. However, since there are no metallographically visible indications of shock in the kamacite and since the back reflection X-ray diffraction pattern shows only very faint Debye-Scherrer arcs superimposed on a pattern of sharp spots, it is concluded that the shock event took place at a temperature that allowed shock effects to anneal out of the kamacite almost completely. A submicroscopic precipitate in the metallic matrix is observable with the electron microscope and may represent the final precipitation of phosphide from shocked kamacite.


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