<?xml version="1.0"?>
<!DOCTYPE article SYSTEM "journalpublishing.dtd">
<article article-type="research-article">
<front>
<journal-meta>
<journal-id journal-id-type="archive">gsminmag</journal-id>
<journal-title>Mineralogical Magazine</journal-title>
<abbrev-journal-title abbrev-type="full">Mineralogical Magazine</abbrev-journal-title>
<issn pub-type="ppub">0026-461X</issn>
<publisher>
<publisher-name>Mineralogical Society</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.1180/minmag.1971.038.293.13</article-id>
<title-group>
<article-title>A Metallographic Study of the Angra Dos Reis (Iron) Meteorite</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Axon</surname>
<given-names>H. J.</given-names>
</name></contrib>
<contrib contrib-type="author">
<name>
<surname>Waine</surname>
<given-names>C. V.</given-names>
</name></contrib>
<aff>Metallurgy Department, The University, Manchester, M13 9PL</aff></contrib-group>
<pub-date pub-type="ppub">
<month>3</month>
<year>1971</year>
</pub-date>
<volume>38</volume>
<issue>293</issue>
<fpage>94</fpage>
<lpage>101</lpage>
<history>
<date date-type="received">
<day>2</day>
<month>3</month>
<year>1970</year>
</date></history>
<copyright-statement>Copyright &#x00A9; 1971, The Mineralogical Society</copyright-statement>
<copyright-year>1971</copyright-year>
<abstract>
<title>Summary</title>
<p>The 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.</p></abstract>
</article-meta>
</front>
</article>
