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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.1970.037.290.03</article-id>
<title-group>
<article-title>Pyroxenes from Non-carbonaceous Chondritic Meteorites</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Binns</surname>
<given-names>R. A.</given-names>
</name>
<aff>Department of Geology, University of New England, Armidale, New South Wales, Australia</aff></contrib></contrib-group>
<pub-date pub-type="ppub">
<month>6</month>
<year>1970</year>
</pub-date>
<volume>37</volume>
<issue>290</issue>
<fpage>649</fpage>
<lpage>669</lpage>
<history>
<date date-type="received">
<day>4</day>
<month>7</month>
<year>1969</year>
</date></history>
<copyright-statement>Copyright &#x00A9; 1970, The Mineralogical Society</copyright-statement>
<copyright-year>1970</copyright-year>
<abstract>
<title>Summary</title>
<p>Chemical, optical, and X-ray data are presented for pyroxenes from a representative selection of chondrites. The Mg-Fe pyroxenes originally crystallized above 1000-1200 &#x00B0;C as the protoenstatite-protohypersthene polymorph, and inverted on cooling to the polysynthetically twinned clinoenstatite-clinohypersthene polymorph. In most chondrites the latter became converted to orthopyroxene during recrystallization at temperatures ranging up to 900 to 950 &#x00B0;C. The contents of certain minor elements changed during the clino-ortho inversion. Ancestral protoenstatiteprotohypersthene may have been slightly non-stoichiometric. Accessory Ca-rich pyroxenes are discussed briefly.</p></abstract>
</article-meta>
</front>
</article>
