Loading…

Origin of the Pegmatitic Pyroxenite in the Merensky Unit, Bushveld Complex, South Africa

The genesis of the pegmatitic pyroxenite that often forms the base of the Merensky Unit in the Bushveld Complex is re-examined. Large (>1 cm) orthopyroxene grains contain tricuspidate inclusions of plagioclase, and chains and rings of chromite grains, which are interpreted to have grown by reacti...

Full description

Saved in:
Bibliographic Details
Published in:Journal of petrology 2006-08, Vol.47 (8), p.1509
Main Authors: R. GRANT CAWTHORN, Boerst, Kevin
Format: Article
Language:English
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue 8
container_start_page 1509
container_title Journal of petrology
container_volume 47
creator R. GRANT CAWTHORN
Boerst, Kevin
description The genesis of the pegmatitic pyroxenite that often forms the base of the Merensky Unit in the Bushveld Complex is re-examined. Large (>1 cm) orthopyroxene grains contain tricuspidate inclusions of plagioclase, and chains and rings of chromite grains, which are interpreted to have grown by reaction between small, primary orthopyroxene grains and superheated liquid. This superheated liquid may have been an added magma or be due to a pressure reduction as a result of lateral expansion of the chamber. There would then have been a period of non-accumulation of grains, permitting prolonged interaction with the crystal mush at the crystal-liquid interface. Crystal ageing and grain enlargement of original orthopyroxene grains would ensue. Only after the pegmatitic pyroxenite had developed did another layer of chromite and pyroxenite, with normal grain size, accumulate above it. Immiscible sulphide liquids formed with the second pyroxenite, but percolated down as a result of their density contrast, even as far as the footwall anorthosite in some cases. Whole-rock abundances of incompatible trace elements in the pegmatitic pyroxenite are comparable with or lower than those of the overlying pyroxenite, and so there is no evidence for addition and/or trapping of large proportions of interstitial liquid, or of an incompatible-element enriched liquid or fluid in the production of the pegmatitic rock. Because of the coarse-grained nature of the rock, modal analysis, especially for minor minerals, is unreliable. Annealing has destroyed primary textures, such that petrographic studies should not be used in isolation to distinguish cumulus and intercumulus components. Geochemical data suggest that the Merensky pyroxenite (both pegmatitic and non-pegmatitic) typically consists of about 70-80% cumulus orthopyroxene and 10-20% cumulus plagioclase, with a further 10% of intercumulus minerals, and could be considered to be a heteradcumulate.
doi_str_mv 10.1093/petrology/eg1017
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_219905342</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1107337501</sourcerecordid><originalsourceid>FETCH-LOGICAL-a120t-e99f4939b3819b40b8faa494b050e6930eb73cc892b2d932ae550eb85cd048043</originalsourceid><addsrcrecordid>eNotjUtLw0AURgdRMFb3LgfXjb3zSJtZ1mBVqLSgBXdlJrl51DQTJxNp_r0RXX1wDpyPkFsG9wyUmLXona1tMcywYMAWZyRgcg4hlyw6JwEA56GIBFySq647ALCRQ0A-Nq4qqobanPoS6RaLo_aVr1K6HZw9YVN5pKP_la_osOk-B7ob6ZQ-9F35jXVGE3tsazxN6ZvtfUmXuatSfU0ucl13ePO_E7JbPb4nz-F68_SSLNehZhx8iErlUgllRMyUkWDiXGuppIEIcK4EoFmINI0VNzxTgmuMRmHiKM1AxiDFhNz9dVtnv3rs_P5ge9eMl3vOlIJISC5-ABVIVNM</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>219905342</pqid></control><display><type>article</type><title>Origin of the Pegmatitic Pyroxenite in the Merensky Unit, Bushveld Complex, South Africa</title><source>Oxford Journals Online</source><creator>R. GRANT CAWTHORN ; Boerst, Kevin</creator><creatorcontrib>R. GRANT CAWTHORN ; Boerst, Kevin</creatorcontrib><description>The genesis of the pegmatitic pyroxenite that often forms the base of the Merensky Unit in the Bushveld Complex is re-examined. Large (&gt;1 cm) orthopyroxene grains contain tricuspidate inclusions of plagioclase, and chains and rings of chromite grains, which are interpreted to have grown by reaction between small, primary orthopyroxene grains and superheated liquid. This superheated liquid may have been an added magma or be due to a pressure reduction as a result of lateral expansion of the chamber. There would then have been a period of non-accumulation of grains, permitting prolonged interaction with the crystal mush at the crystal-liquid interface. Crystal ageing and grain enlargement of original orthopyroxene grains would ensue. Only after the pegmatitic pyroxenite had developed did another layer of chromite and pyroxenite, with normal grain size, accumulate above it. Immiscible sulphide liquids formed with the second pyroxenite, but percolated down as a result of their density contrast, even as far as the footwall anorthosite in some cases. Whole-rock abundances of incompatible trace elements in the pegmatitic pyroxenite are comparable with or lower than those of the overlying pyroxenite, and so there is no evidence for addition and/or trapping of large proportions of interstitial liquid, or of an incompatible-element enriched liquid or fluid in the production of the pegmatitic rock. Because of the coarse-grained nature of the rock, modal analysis, especially for minor minerals, is unreliable. Annealing has destroyed primary textures, such that petrographic studies should not be used in isolation to distinguish cumulus and intercumulus components. Geochemical data suggest that the Merensky pyroxenite (both pegmatitic and non-pegmatitic) typically consists of about 70-80% cumulus orthopyroxene and 10-20% cumulus plagioclase, with a further 10% of intercumulus minerals, and could be considered to be a heteradcumulate.</description><identifier>ISSN: 0022-3530</identifier><identifier>EISSN: 1460-2415</identifier><identifier>DOI: 10.1093/petrology/eg1017</identifier><language>eng</language><publisher>Oxford: Oxford Publishing Limited (England)</publisher><ispartof>Journal of petrology, 2006-08, Vol.47 (8), p.1509</ispartof><rights>Copyright Oxford University Press(England) Aug 2006</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>R. GRANT CAWTHORN</creatorcontrib><creatorcontrib>Boerst, Kevin</creatorcontrib><title>Origin of the Pegmatitic Pyroxenite in the Merensky Unit, Bushveld Complex, South Africa</title><title>Journal of petrology</title><description>The genesis of the pegmatitic pyroxenite that often forms the base of the Merensky Unit in the Bushveld Complex is re-examined. Large (&gt;1 cm) orthopyroxene grains contain tricuspidate inclusions of plagioclase, and chains and rings of chromite grains, which are interpreted to have grown by reaction between small, primary orthopyroxene grains and superheated liquid. This superheated liquid may have been an added magma or be due to a pressure reduction as a result of lateral expansion of the chamber. There would then have been a period of non-accumulation of grains, permitting prolonged interaction with the crystal mush at the crystal-liquid interface. Crystal ageing and grain enlargement of original orthopyroxene grains would ensue. Only after the pegmatitic pyroxenite had developed did another layer of chromite and pyroxenite, with normal grain size, accumulate above it. Immiscible sulphide liquids formed with the second pyroxenite, but percolated down as a result of their density contrast, even as far as the footwall anorthosite in some cases. Whole-rock abundances of incompatible trace elements in the pegmatitic pyroxenite are comparable with or lower than those of the overlying pyroxenite, and so there is no evidence for addition and/or trapping of large proportions of interstitial liquid, or of an incompatible-element enriched liquid or fluid in the production of the pegmatitic rock. Because of the coarse-grained nature of the rock, modal analysis, especially for minor minerals, is unreliable. Annealing has destroyed primary textures, such that petrographic studies should not be used in isolation to distinguish cumulus and intercumulus components. Geochemical data suggest that the Merensky pyroxenite (both pegmatitic and non-pegmatitic) typically consists of about 70-80% cumulus orthopyroxene and 10-20% cumulus plagioclase, with a further 10% of intercumulus minerals, and could be considered to be a heteradcumulate.</description><issn>0022-3530</issn><issn>1460-2415</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNotjUtLw0AURgdRMFb3LgfXjb3zSJtZ1mBVqLSgBXdlJrl51DQTJxNp_r0RXX1wDpyPkFsG9wyUmLXona1tMcywYMAWZyRgcg4hlyw6JwEA56GIBFySq647ALCRQ0A-Nq4qqobanPoS6RaLo_aVr1K6HZw9YVN5pKP_la_osOk-B7ob6ZQ-9F35jXVGE3tsazxN6ZvtfUmXuatSfU0ucl13ePO_E7JbPb4nz-F68_SSLNehZhx8iErlUgllRMyUkWDiXGuppIEIcK4EoFmINI0VNzxTgmuMRmHiKM1AxiDFhNz9dVtnv3rs_P5ge9eMl3vOlIJISC5-ABVIVNM</recordid><startdate>20060801</startdate><enddate>20060801</enddate><creator>R. GRANT CAWTHORN</creator><creator>Boerst, Kevin</creator><general>Oxford Publishing Limited (England)</general><scope>7UA</scope><scope>8BQ</scope><scope>8FD</scope><scope>C1K</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>JG9</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope></search><sort><creationdate>20060801</creationdate><title>Origin of the Pegmatitic Pyroxenite in the Merensky Unit, Bushveld Complex, South Africa</title><author>R. GRANT CAWTHORN ; Boerst, Kevin</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a120t-e99f4939b3819b40b8faa494b050e6930eb73cc892b2d932ae550eb85cd048043</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>R. GRANT CAWTHORN</creatorcontrib><creatorcontrib>Boerst, Kevin</creatorcontrib><collection>Water Resources Abstracts</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy &amp; Non-Living Resources</collection><collection>Materials Research Database</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of petrology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>R. GRANT CAWTHORN</au><au>Boerst, Kevin</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Origin of the Pegmatitic Pyroxenite in the Merensky Unit, Bushveld Complex, South Africa</atitle><jtitle>Journal of petrology</jtitle><date>2006-08-01</date><risdate>2006</risdate><volume>47</volume><issue>8</issue><spage>1509</spage><pages>1509-</pages><issn>0022-3530</issn><eissn>1460-2415</eissn><abstract>The genesis of the pegmatitic pyroxenite that often forms the base of the Merensky Unit in the Bushveld Complex is re-examined. Large (&gt;1 cm) orthopyroxene grains contain tricuspidate inclusions of plagioclase, and chains and rings of chromite grains, which are interpreted to have grown by reaction between small, primary orthopyroxene grains and superheated liquid. This superheated liquid may have been an added magma or be due to a pressure reduction as a result of lateral expansion of the chamber. There would then have been a period of non-accumulation of grains, permitting prolonged interaction with the crystal mush at the crystal-liquid interface. Crystal ageing and grain enlargement of original orthopyroxene grains would ensue. Only after the pegmatitic pyroxenite had developed did another layer of chromite and pyroxenite, with normal grain size, accumulate above it. Immiscible sulphide liquids formed with the second pyroxenite, but percolated down as a result of their density contrast, even as far as the footwall anorthosite in some cases. Whole-rock abundances of incompatible trace elements in the pegmatitic pyroxenite are comparable with or lower than those of the overlying pyroxenite, and so there is no evidence for addition and/or trapping of large proportions of interstitial liquid, or of an incompatible-element enriched liquid or fluid in the production of the pegmatitic rock. Because of the coarse-grained nature of the rock, modal analysis, especially for minor minerals, is unreliable. Annealing has destroyed primary textures, such that petrographic studies should not be used in isolation to distinguish cumulus and intercumulus components. Geochemical data suggest that the Merensky pyroxenite (both pegmatitic and non-pegmatitic) typically consists of about 70-80% cumulus orthopyroxene and 10-20% cumulus plagioclase, with a further 10% of intercumulus minerals, and could be considered to be a heteradcumulate.</abstract><cop>Oxford</cop><pub>Oxford Publishing Limited (England)</pub><doi>10.1093/petrology/eg1017</doi></addata></record>
fulltext fulltext
identifier ISSN: 0022-3530
ispartof Journal of petrology, 2006-08, Vol.47 (8), p.1509
issn 0022-3530
1460-2415
language eng
recordid cdi_proquest_journals_219905342
source Oxford Journals Online
title Origin of the Pegmatitic Pyroxenite in the Merensky Unit, Bushveld Complex, South Africa
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-26T12%3A20%3A53IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Origin%20of%20the%20Pegmatitic%20Pyroxenite%20in%20the%20Merensky%20Unit,%20Bushveld%20Complex,%20South%20Africa&rft.jtitle=Journal%20of%20petrology&rft.au=R.%20GRANT%20CAWTHORN&rft.date=2006-08-01&rft.volume=47&rft.issue=8&rft.spage=1509&rft.pages=1509-&rft.issn=0022-3530&rft.eissn=1460-2415&rft_id=info:doi/10.1093/petrology/eg1017&rft_dat=%3Cproquest%3E1107337501%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a120t-e99f4939b3819b40b8faa494b050e6930eb73cc892b2d932ae550eb85cd048043%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=219905342&rft_id=info:pmid/&rfr_iscdi=true