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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.1980.043.329.05</article-id>
<title-group>
<article-title>Petrogenesis of Aln&#x00D6;itic Rocks from Malaita, Solomon Islands, Melanesia</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Nixon</surname>
<given-names>Peter H.</given-names>
</name>
<aff>Geology Department, P.O. Box 4820, University, Papua New Guinea</aff></contrib>
<contrib contrib-type="author">
<name>
<surname>Mitchell</surname>
<given-names>Roger H.</given-names>
</name>
<aff>Geology Department, Lakehead University, Thunder Bay, Ontario, Canada</aff></contrib>
<contrib contrib-type="author">
<name>
<surname>Rogers</surname>
<given-names>Nicholas W.</given-names>
</name>
<aff>University of London Reactor Centre, Sunninghill, Ascot, Berks, U.K.</aff></contrib></contrib-group>
<pub-date pub-type="ppub">
<month>3</month>
<year>1980</year>
</pub-date>
<volume>43</volume>
<issue>329</issue>
<fpage>587</fpage>
<lpage>596</lpage>
<history>
<date date-type="received">
<day>28</day>
<month>6</month>
<year>1979</year>
</date>
<date date-type="rev-recd">
<day>17</day>
<month>9</month>
<year>1979</year>
</date></history>
<copyright-statement>Copyright &#x00A9; 1980, The Mineralogical Society</copyright-statement>
<copyright-year>1980</copyright-year>
<abstract>
<title>Summary</title>
<p>Aphanitic and fragmental aln&#x00F6;itic rocks from Malaita contain ultrabasic xenoliths and discrete nodules (megacrysts) of pyroxenes and garnets. Primary minerals in the aln&#x00F6;ites are olivine (Fo<sub>85</sub>), clinopyroxene (diopside-sahlite), natro-melilite (1/3 melilite-2/3 &#x00E5;kermanite), phlogopite (1&#x2013;9% TiO<sub>2</sub>), perovskite, spinel (ulv&#x00F6; spinel-magnetite series) and accessory nepheline, melanite, and apatite. Aln&#x00F6;ite olivines and clinopyroxenes are compositionally different from those phases in the xenoliths and megacrysts. Rare earth element distribution patterns are linear and indicate strong enrichment in the light rare earths (La/Yb = 42&#x2212;49). The aln&#x00F6;ites are possible primary melts of a pyrolite-type mantle formed by approximately 4% partial melting at depths greater than 120 km, under high carbon dioxide pressures. Despite containing a mantle xenolith assemblage similar to that found in kimberlites, the host Malaita rocks are minera-logically and geochemically different from kimberlite.</p></abstract>
</article-meta>
</front>
</article>
