Loading…

Ion microprobe investigation of plagioclase and orthopyroxene from lunar Mg-suite norites: Implications for calculating parental melt REE concentrations and for assessing postcrystallization REE redistribution

The lunar Mg-suite, which includes dunites, troctolites, and norites, makes up to 20–30% of the Moon's crust down to a depth of ∼ 60 km. The remainder is largely anorthosite. This report focuses on norites (which consist mostly of orthopyroxene and plagioclase) because we have found that both p...

Full description

Saved in:
Bibliographic Details
Published in:Geochimica et cosmochimica acta 1996-10, Vol.60 (20), p.3967-3978
Main Authors: Papike, J.J., Fowler, G.W., Shearer, C.K., Layne, G.D.
Format: Article
Language:English
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3
cites cdi_FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3
container_end_page 3978
container_issue 20
container_start_page 3967
container_title Geochimica et cosmochimica acta
container_volume 60
creator Papike, J.J.
Fowler, G.W.
Shearer, C.K.
Layne, G.D.
description The lunar Mg-suite, which includes dunites, troctolites, and norites, makes up to 20–30% of the Moon's crust down to a depth of ∼ 60 km. The remainder is largely anorthosite. This report focuses on norites (which consist mostly of orthopyroxene and plagioclase) because we have found that both phases are effective recorders of their parental melt compositions. In an earlier report, we analyzed orthopyroxene from twelve samples (three from Apollo 14, two from A-15, and seven from A-17) by SIMS for eight REE (La, Ce, Nd, Sm, Eu, Dy, Er, Yb). Inversion of these data to estimated melt compositions yielded extremely high REE concentrations similar to KREEP. In this study, we report SIMS REE data for plagioclase from these same twelve samples. The major objective of this study is to estimate parental REE concentrations from both orthopyroxene and plagioclase data to see if both data inversions produce concordant melt compositions and thus better constrain the composition of melts parental to Mg-suite norites. The estimated REE concentrations from both phases show some evidence of slight postcrystallization REE redistribution. Comparison of the observed ratio of REE for pyroxene/ plagioclase to the ratio of the Ds for pyroxene/plagioclase is consistent with REE redistribution which involves LREE diffusing from pyroxene into plagioclase and HREE diffusing from plagioclase into pyroxene. However, apparently these postcrystallization exchanges have not seriously affected our ability to estimate melt REE concentrations. The estimated melt REE concentrations using both plagioclase and orthopyroxene, are similar to high-K KREEP especially for melts parental to A-15 norites. This study provides support for mineral trace element inversion estimates for parental melts. Even though these lunar crustal lithologies experienced high temperature annealing, apparently the cores of plagioclase and pyroxene continue to carry a record of their igneous crystallization history.
doi_str_mv 10.1016/0016-7037(96)00212-8
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_26233600</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>0016703796002128</els_id><sourcerecordid>26233600</sourcerecordid><originalsourceid>FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3</originalsourceid><addsrcrecordid>eNp9kc1u1TAQhSMEEpfCG7DwCsEi4J_8skBC1YVeqQgJdW9NnMnFyLGDx6l6eUveCKe36pKNRx7Pd2yfUxSvBX8vuGg-8LyULVft2755x7kUsuyeFDvRtbLsa6WeFrvHkefFC6JfnPO2rvmu-HsIns3WxLDEMCCz_hYp2SMkmw_CxBYHRxuMA0IGfmQhpp9hOcVwhx7ZFMPM3Oohsm_HklabkPkQc6GP7DAvzpp7JWJTiMyAM6vLDX9kC0T0CRyb0SX2Y79nJniTW_EB2C7bICBConskUDLxRJly9s_5hRsYcbSUoh3WrfWyeDaBI3z1UC-Kmy_7m8ur8vr718Pl5-sSqpqnUgxT3SgzVH1XTRLHoa8aGEUjOzUoqMcRJwCpBIdRTtDW0JhRtFXfD7IdWlQXxZuzbPbt95o907Mlg86Bx7CSlo1UquE8D1bnwewxUcRJL9HOEE9acL3Fp7ds9JaN7rdNjk93Gft0xjD_4dZi1GQsZodGG9EkPQb7f4F_i6CpqA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>26233600</pqid></control><display><type>article</type><title>Ion microprobe investigation of plagioclase and orthopyroxene from lunar Mg-suite norites: Implications for calculating parental melt REE concentrations and for assessing postcrystallization REE redistribution</title><source>ScienceDirect Freedom Collection 2022-2024</source><creator>Papike, J.J. ; Fowler, G.W. ; Shearer, C.K. ; Layne, G.D.</creator><creatorcontrib>Papike, J.J. ; Fowler, G.W. ; Shearer, C.K. ; Layne, G.D.</creatorcontrib><description>The lunar Mg-suite, which includes dunites, troctolites, and norites, makes up to 20–30% of the Moon's crust down to a depth of ∼ 60 km. The remainder is largely anorthosite. This report focuses on norites (which consist mostly of orthopyroxene and plagioclase) because we have found that both phases are effective recorders of their parental melt compositions. In an earlier report, we analyzed orthopyroxene from twelve samples (three from Apollo 14, two from A-15, and seven from A-17) by SIMS for eight REE (La, Ce, Nd, Sm, Eu, Dy, Er, Yb). Inversion of these data to estimated melt compositions yielded extremely high REE concentrations similar to KREEP. In this study, we report SIMS REE data for plagioclase from these same twelve samples. The major objective of this study is to estimate parental REE concentrations from both orthopyroxene and plagioclase data to see if both data inversions produce concordant melt compositions and thus better constrain the composition of melts parental to Mg-suite norites. The estimated REE concentrations from both phases show some evidence of slight postcrystallization REE redistribution. Comparison of the observed ratio of REE for pyroxene/ plagioclase to the ratio of the Ds for pyroxene/plagioclase is consistent with REE redistribution which involves LREE diffusing from pyroxene into plagioclase and HREE diffusing from plagioclase into pyroxene. However, apparently these postcrystallization exchanges have not seriously affected our ability to estimate melt REE concentrations. The estimated melt REE concentrations using both plagioclase and orthopyroxene, are similar to high-K KREEP especially for melts parental to A-15 norites. This study provides support for mineral trace element inversion estimates for parental melts. Even though these lunar crustal lithologies experienced high temperature annealing, apparently the cores of plagioclase and pyroxene continue to carry a record of their igneous crystallization history.</description><identifier>ISSN: 0016-7037</identifier><identifier>EISSN: 1872-9533</identifier><identifier>DOI: 10.1016/0016-7037(96)00212-8</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><ispartof>Geochimica et cosmochimica acta, 1996-10, Vol.60 (20), p.3967-3978</ispartof><rights>1996 Elsevier Science Ltd</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3</citedby><cites>FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3</cites></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>Papike, J.J.</creatorcontrib><creatorcontrib>Fowler, G.W.</creatorcontrib><creatorcontrib>Shearer, C.K.</creatorcontrib><creatorcontrib>Layne, G.D.</creatorcontrib><title>Ion microprobe investigation of plagioclase and orthopyroxene from lunar Mg-suite norites: Implications for calculating parental melt REE concentrations and for assessing postcrystallization REE redistribution</title><title>Geochimica et cosmochimica acta</title><description>The lunar Mg-suite, which includes dunites, troctolites, and norites, makes up to 20–30% of the Moon's crust down to a depth of ∼ 60 km. The remainder is largely anorthosite. This report focuses on norites (which consist mostly of orthopyroxene and plagioclase) because we have found that both phases are effective recorders of their parental melt compositions. In an earlier report, we analyzed orthopyroxene from twelve samples (three from Apollo 14, two from A-15, and seven from A-17) by SIMS for eight REE (La, Ce, Nd, Sm, Eu, Dy, Er, Yb). Inversion of these data to estimated melt compositions yielded extremely high REE concentrations similar to KREEP. In this study, we report SIMS REE data for plagioclase from these same twelve samples. The major objective of this study is to estimate parental REE concentrations from both orthopyroxene and plagioclase data to see if both data inversions produce concordant melt compositions and thus better constrain the composition of melts parental to Mg-suite norites. The estimated REE concentrations from both phases show some evidence of slight postcrystallization REE redistribution. Comparison of the observed ratio of REE for pyroxene/ plagioclase to the ratio of the Ds for pyroxene/plagioclase is consistent with REE redistribution which involves LREE diffusing from pyroxene into plagioclase and HREE diffusing from plagioclase into pyroxene. However, apparently these postcrystallization exchanges have not seriously affected our ability to estimate melt REE concentrations. The estimated melt REE concentrations using both plagioclase and orthopyroxene, are similar to high-K KREEP especially for melts parental to A-15 norites. This study provides support for mineral trace element inversion estimates for parental melts. Even though these lunar crustal lithologies experienced high temperature annealing, apparently the cores of plagioclase and pyroxene continue to carry a record of their igneous crystallization history.</description><issn>0016-7037</issn><issn>1872-9533</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><recordid>eNp9kc1u1TAQhSMEEpfCG7DwCsEi4J_8skBC1YVeqQgJdW9NnMnFyLGDx6l6eUveCKe36pKNRx7Pd2yfUxSvBX8vuGg-8LyULVft2755x7kUsuyeFDvRtbLsa6WeFrvHkefFC6JfnPO2rvmu-HsIns3WxLDEMCCz_hYp2SMkmw_CxBYHRxuMA0IGfmQhpp9hOcVwhx7ZFMPM3Oohsm_HklabkPkQc6GP7DAvzpp7JWJTiMyAM6vLDX9kC0T0CRyb0SX2Y79nJniTW_EB2C7bICBConskUDLxRJly9s_5hRsYcbSUoh3WrfWyeDaBI3z1UC-Kmy_7m8ur8vr718Pl5-sSqpqnUgxT3SgzVH1XTRLHoa8aGEUjOzUoqMcRJwCpBIdRTtDW0JhRtFXfD7IdWlQXxZuzbPbt95o907Mlg86Bx7CSlo1UquE8D1bnwewxUcRJL9HOEE9acL3Fp7ds9JaN7rdNjk93Gft0xjD_4dZi1GQsZodGG9EkPQb7f4F_i6CpqA</recordid><startdate>19961001</startdate><enddate>19961001</enddate><creator>Papike, J.J.</creator><creator>Fowler, G.W.</creator><creator>Shearer, C.K.</creator><creator>Layne, G.D.</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19961001</creationdate><title>Ion microprobe investigation of plagioclase and orthopyroxene from lunar Mg-suite norites: Implications for calculating parental melt REE concentrations and for assessing postcrystallization REE redistribution</title><author>Papike, J.J. ; Fowler, G.W. ; Shearer, C.K. ; Layne, G.D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Papike, J.J.</creatorcontrib><creatorcontrib>Fowler, G.W.</creatorcontrib><creatorcontrib>Shearer, C.K.</creatorcontrib><creatorcontrib>Layne, G.D.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geochimica et cosmochimica acta</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Papike, J.J.</au><au>Fowler, G.W.</au><au>Shearer, C.K.</au><au>Layne, G.D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Ion microprobe investigation of plagioclase and orthopyroxene from lunar Mg-suite norites: Implications for calculating parental melt REE concentrations and for assessing postcrystallization REE redistribution</atitle><jtitle>Geochimica et cosmochimica acta</jtitle><date>1996-10-01</date><risdate>1996</risdate><volume>60</volume><issue>20</issue><spage>3967</spage><epage>3978</epage><pages>3967-3978</pages><issn>0016-7037</issn><eissn>1872-9533</eissn><abstract>The lunar Mg-suite, which includes dunites, troctolites, and norites, makes up to 20–30% of the Moon's crust down to a depth of ∼ 60 km. The remainder is largely anorthosite. This report focuses on norites (which consist mostly of orthopyroxene and plagioclase) because we have found that both phases are effective recorders of their parental melt compositions. In an earlier report, we analyzed orthopyroxene from twelve samples (three from Apollo 14, two from A-15, and seven from A-17) by SIMS for eight REE (La, Ce, Nd, Sm, Eu, Dy, Er, Yb). Inversion of these data to estimated melt compositions yielded extremely high REE concentrations similar to KREEP. In this study, we report SIMS REE data for plagioclase from these same twelve samples. The major objective of this study is to estimate parental REE concentrations from both orthopyroxene and plagioclase data to see if both data inversions produce concordant melt compositions and thus better constrain the composition of melts parental to Mg-suite norites. The estimated REE concentrations from both phases show some evidence of slight postcrystallization REE redistribution. Comparison of the observed ratio of REE for pyroxene/ plagioclase to the ratio of the Ds for pyroxene/plagioclase is consistent with REE redistribution which involves LREE diffusing from pyroxene into plagioclase and HREE diffusing from plagioclase into pyroxene. However, apparently these postcrystallization exchanges have not seriously affected our ability to estimate melt REE concentrations. The estimated melt REE concentrations using both plagioclase and orthopyroxene, are similar to high-K KREEP especially for melts parental to A-15 norites. This study provides support for mineral trace element inversion estimates for parental melts. Even though these lunar crustal lithologies experienced high temperature annealing, apparently the cores of plagioclase and pyroxene continue to carry a record of their igneous crystallization history.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/0016-7037(96)00212-8</doi><tpages>12</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0016-7037
ispartof Geochimica et cosmochimica acta, 1996-10, Vol.60 (20), p.3967-3978
issn 0016-7037
1872-9533
language eng
recordid cdi_proquest_miscellaneous_26233600
source ScienceDirect Freedom Collection 2022-2024
title Ion microprobe investigation of plagioclase and orthopyroxene from lunar Mg-suite norites: Implications for calculating parental melt REE concentrations and for assessing postcrystallization REE redistribution
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T02%3A34%3A56IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Ion%20microprobe%20investigation%20of%20plagioclase%20and%20orthopyroxene%20from%20lunar%20Mg-suite%20norites:%20Implications%20for%20calculating%20parental%20melt%20REE%20concentrations%20and%20for%20assessing%20postcrystallization%20REE%20redistribution&rft.jtitle=Geochimica%20et%20cosmochimica%20acta&rft.au=Papike,%20J.J.&rft.date=1996-10-01&rft.volume=60&rft.issue=20&rft.spage=3967&rft.epage=3978&rft.pages=3967-3978&rft.issn=0016-7037&rft.eissn=1872-9533&rft_id=info:doi/10.1016/0016-7037(96)00212-8&rft_dat=%3Cproquest_cross%3E26233600%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a450t-1bf563cb4984f2edb946ad16283b3a5ddefaa2310ad2fa75a6cd17499b27b7e3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=26233600&rft_id=info:pmid/&rfr_iscdi=true