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<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.1968.036.284.10</article-id>
<title-group>
<article-title>The Metallographic Structure of the Iron Meteorites Arltunga, Kopjes Vlei, Murnpeowie, Braunau, and Rancho De La Pila</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Axon</surname>
<given-names>H. J.</given-names>
</name>
<aff>Metallurgy Department, The University, Manchester 13</aff></contrib></contrib-group>
<pub-date pub-type="ppub">
<month>12</month>
<year>1968</year>
</pub-date>
<volume>36</volume>
<issue>284</issue>
<fpage>1139</fpage>
<lpage>1142</lpage>
<history>
<date date-type="received">
<day>11</day>
<month>6</month>
<year>1968</year>
</date></history>
<copyright-statement>Copyright &#x00A9; 1968, The Mineralogical Society</copyright-statement>
<copyright-year>1968</copyright-year>
<abstract>
<title>Summary</title>
<p>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.</p></abstract>
</article-meta>
</front>
</article>
