Loading…

The I-Xe chronometer

129Xe, from the decay of the now-extinct 16.7 Ma129I, accumulates in iodine-bearing sites and since most iodine host phases are secondary, the I-Xe system is typically a chronometer for post-formational processes. The validity of the I-Xe chronometer is confirmed by comparison with Pb-Pb ages on pho...

Full description

Saved in:
Bibliographic Details
Published in:Academy Proceedings in Earth and Planetary Sciences 1998-12, Vol.107 (4), p.413-423
Main Authors: HOHENBERG, C. M, BRAZZLE, R. H, PRAVDIVTSEVA, O. V, MESHIK, A. P
Format: Article
Language:English
Subjects:
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-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13
cites cdi_FETCH-LOGICAL-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13
container_end_page 423
container_issue 4
container_start_page 413
container_title Academy Proceedings in Earth and Planetary Sciences
container_volume 107
creator HOHENBERG, C. M
BRAZZLE, R. H
PRAVDIVTSEVA, O. V
MESHIK, A. P
description 129Xe, from the decay of the now-extinct 16.7 Ma129I, accumulates in iodine-bearing sites and since most iodine host phases are secondary, the I-Xe system is typically a chronometer for post-formational processes. The validity of the I-Xe chronometer is confirmed by comparison with Pb-Pb ages on phosphate and feldspar separates from twelve meteorites. Phosphate separates are found to be concordant with Pb-Pb for all six samples in which useful I-Xe data were obtained. Feldspar is a better iodine host than apatite in H chondrites, typically providing good I-Xe isochrons. These too are concordant with the Pb-Pb ages of the corresponding phosphates for five out of six feldspar separates. The exception is Allegan whose feldspar yields one of the oldest I-Xe ages observed, similar to those for CI and CM magnetites. We attribute this to a more primary mineralization, predating the secondary phosphate from which the comparison Pb-Pb age was obtained. Absolute I-Xe ages, found using the reported Pb-Pb age of Acapulco phosphate provide an absolute I-Xe age of 4.566 ± 0.002 Ga for both Shallowater and Bjurböle irradiation standards. This allows relative I-Xe ages to be interpreted in the context of absolute ages.
doi_str_mv 10.1007/BF02841607
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_741061841</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2105654301</sourcerecordid><originalsourceid>FETCH-LOGICAL-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13</originalsourceid><addsrcrecordid>eNpFj01LAzEURYMoWKsb8QcUcSVE35t8vMxSi9VCwU2F7kImk9CWdqYm04X_viMtdHXf4rx7OYzdI7wgAL2-T6AwEjXQBRtASYITycVlfxdKcImFvmY3Oa8BhDZUDtjDfBlGU74II79MbdNuQxfSLbuKbpPD3SmH7GfyMR9_8dn353T8NuNOgOm4MBF1kJEUGQW1rIwGJVVdGS8IsArKOSQKEJQPHmSsaiGjIEISRR1RDNnjsXeX2t99yJ1dt_vU9JOWJILGXqWHno-QT23OKUS7S6utS38Wwf5L27N0Dz-dGl32bhOTa_wqnz9KlFBocQBBB1Jg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>741061841</pqid></control><display><type>article</type><title>The I-Xe chronometer</title><source>Springer Link</source><creator>HOHENBERG, C. M ; BRAZZLE, R. H ; PRAVDIVTSEVA, O. V ; MESHIK, A. P</creator><creatorcontrib>HOHENBERG, C. M ; BRAZZLE, R. H ; PRAVDIVTSEVA, O. V ; MESHIK, A. P</creatorcontrib><description>129Xe, from the decay of the now-extinct 16.7 Ma129I, accumulates in iodine-bearing sites and since most iodine host phases are secondary, the I-Xe system is typically a chronometer for post-formational processes. The validity of the I-Xe chronometer is confirmed by comparison with Pb-Pb ages on phosphate and feldspar separates from twelve meteorites. Phosphate separates are found to be concordant with Pb-Pb for all six samples in which useful I-Xe data were obtained. Feldspar is a better iodine host than apatite in H chondrites, typically providing good I-Xe isochrons. These too are concordant with the Pb-Pb ages of the corresponding phosphates for five out of six feldspar separates. The exception is Allegan whose feldspar yields one of the oldest I-Xe ages observed, similar to those for CI and CM magnetites. We attribute this to a more primary mineralization, predating the secondary phosphate from which the comparison Pb-Pb age was obtained. Absolute I-Xe ages, found using the reported Pb-Pb age of Acapulco phosphate provide an absolute I-Xe age of 4.566 ± 0.002 Ga for both Shallowater and Bjurböle irradiation standards. This allows relative I-Xe ages to be interpreted in the context of absolute ages.</description><identifier>ISSN: 0253-4126</identifier><identifier>EISSN: 0973-774X</identifier><identifier>DOI: 10.1007/BF02841607</identifier><language>eng</language><publisher>Bangalore: Indian Academy of Sciences</publisher><subject>Age ; Apatite ; Chondrites ; Chronometers ; Cosmochemistry. Extraterrestrial geology ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; Feldspars ; Geochronology ; Iodine ; Irradiation ; Isotope geochemistry. Geochronology ; Lead ; Measuring instruments ; Meteorites. Tectites. Impactites ; Mineralization ; Phosphates ; Radiometric dating ; Xenon 129</subject><ispartof>Academy Proceedings in Earth and Planetary Sciences, 1998-12, Vol.107 (4), p.413-423</ispartof><rights>1999 INIST-CNRS</rights><rights>Indian Academy of Sciences 1998.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13</citedby><cites>FETCH-LOGICAL-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>309,310,314,776,780,785,786,23909,23910,25118,27901,27902</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=1914026$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>HOHENBERG, C. M</creatorcontrib><creatorcontrib>BRAZZLE, R. H</creatorcontrib><creatorcontrib>PRAVDIVTSEVA, O. V</creatorcontrib><creatorcontrib>MESHIK, A. P</creatorcontrib><title>The I-Xe chronometer</title><title>Academy Proceedings in Earth and Planetary Sciences</title><description>129Xe, from the decay of the now-extinct 16.7 Ma129I, accumulates in iodine-bearing sites and since most iodine host phases are secondary, the I-Xe system is typically a chronometer for post-formational processes. The validity of the I-Xe chronometer is confirmed by comparison with Pb-Pb ages on phosphate and feldspar separates from twelve meteorites. Phosphate separates are found to be concordant with Pb-Pb for all six samples in which useful I-Xe data were obtained. Feldspar is a better iodine host than apatite in H chondrites, typically providing good I-Xe isochrons. These too are concordant with the Pb-Pb ages of the corresponding phosphates for five out of six feldspar separates. The exception is Allegan whose feldspar yields one of the oldest I-Xe ages observed, similar to those for CI and CM magnetites. We attribute this to a more primary mineralization, predating the secondary phosphate from which the comparison Pb-Pb age was obtained. Absolute I-Xe ages, found using the reported Pb-Pb age of Acapulco phosphate provide an absolute I-Xe age of 4.566 ± 0.002 Ga for both Shallowater and Bjurböle irradiation standards. This allows relative I-Xe ages to be interpreted in the context of absolute ages.</description><subject>Age</subject><subject>Apatite</subject><subject>Chondrites</subject><subject>Chronometers</subject><subject>Cosmochemistry. Extraterrestrial geology</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Feldspars</subject><subject>Geochronology</subject><subject>Iodine</subject><subject>Irradiation</subject><subject>Isotope geochemistry. Geochronology</subject><subject>Lead</subject><subject>Measuring instruments</subject><subject>Meteorites. Tectites. Impactites</subject><subject>Mineralization</subject><subject>Phosphates</subject><subject>Radiometric dating</subject><subject>Xenon 129</subject><issn>0253-4126</issn><issn>0973-774X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1998</creationdate><recordtype>article</recordtype><recordid>eNpFj01LAzEURYMoWKsb8QcUcSVE35t8vMxSi9VCwU2F7kImk9CWdqYm04X_viMtdHXf4rx7OYzdI7wgAL2-T6AwEjXQBRtASYITycVlfxdKcImFvmY3Oa8BhDZUDtjDfBlGU74II79MbdNuQxfSLbuKbpPD3SmH7GfyMR9_8dn353T8NuNOgOm4MBF1kJEUGQW1rIwGJVVdGS8IsArKOSQKEJQPHmSsaiGjIEISRR1RDNnjsXeX2t99yJ1dt_vU9JOWJILGXqWHno-QT23OKUS7S6utS38Wwf5L27N0Dz-dGl32bhOTa_wqnz9KlFBocQBBB1Jg</recordid><startdate>19981201</startdate><enddate>19981201</enddate><creator>HOHENBERG, C. M</creator><creator>BRAZZLE, R. H</creator><creator>PRAVDIVTSEVA, O. V</creator><creator>MESHIK, A. P</creator><general>Indian Academy of Sciences</general><general>Springer Nature B.V</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7UA</scope><scope>7XB</scope><scope>88I</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>M2P</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PYCSY</scope><scope>Q9U</scope></search><sort><creationdate>19981201</creationdate><title>The I-Xe chronometer</title><author>HOHENBERG, C. M ; BRAZZLE, R. H ; PRAVDIVTSEVA, O. V ; MESHIK, A. P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1998</creationdate><topic>Age</topic><topic>Apatite</topic><topic>Chondrites</topic><topic>Chronometers</topic><topic>Cosmochemistry. Extraterrestrial geology</topic><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Feldspars</topic><topic>Geochronology</topic><topic>Iodine</topic><topic>Irradiation</topic><topic>Isotope geochemistry. Geochronology</topic><topic>Lead</topic><topic>Measuring instruments</topic><topic>Meteorites. Tectites. Impactites</topic><topic>Mineralization</topic><topic>Phosphates</topic><topic>Radiometric dating</topic><topic>Xenon 129</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>HOHENBERG, C. M</creatorcontrib><creatorcontrib>BRAZZLE, R. H</creatorcontrib><creatorcontrib>PRAVDIVTSEVA, O. V</creatorcontrib><creatorcontrib>MESHIK, A. P</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central</collection><collection>Agricultural &amp; Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>ProQuest Natural Science Collection</collection><collection>Earth, Atmospheric &amp; Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>ProQuest Central Student</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy &amp; Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) Professional</collection><collection>ProQuest Science Journals</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric &amp; Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><jtitle>Academy Proceedings in Earth and Planetary Sciences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>HOHENBERG, C. M</au><au>BRAZZLE, R. H</au><au>PRAVDIVTSEVA, O. V</au><au>MESHIK, A. P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The I-Xe chronometer</atitle><jtitle>Academy Proceedings in Earth and Planetary Sciences</jtitle><date>1998-12-01</date><risdate>1998</risdate><volume>107</volume><issue>4</issue><spage>413</spage><epage>423</epage><pages>413-423</pages><issn>0253-4126</issn><eissn>0973-774X</eissn><abstract>129Xe, from the decay of the now-extinct 16.7 Ma129I, accumulates in iodine-bearing sites and since most iodine host phases are secondary, the I-Xe system is typically a chronometer for post-formational processes. The validity of the I-Xe chronometer is confirmed by comparison with Pb-Pb ages on phosphate and feldspar separates from twelve meteorites. Phosphate separates are found to be concordant with Pb-Pb for all six samples in which useful I-Xe data were obtained. Feldspar is a better iodine host than apatite in H chondrites, typically providing good I-Xe isochrons. These too are concordant with the Pb-Pb ages of the corresponding phosphates for five out of six feldspar separates. The exception is Allegan whose feldspar yields one of the oldest I-Xe ages observed, similar to those for CI and CM magnetites. We attribute this to a more primary mineralization, predating the secondary phosphate from which the comparison Pb-Pb age was obtained. Absolute I-Xe ages, found using the reported Pb-Pb age of Acapulco phosphate provide an absolute I-Xe age of 4.566 ± 0.002 Ga for both Shallowater and Bjurböle irradiation standards. This allows relative I-Xe ages to be interpreted in the context of absolute ages.</abstract><cop>Bangalore</cop><pub>Indian Academy of Sciences</pub><doi>10.1007/BF02841607</doi><tpages>11</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0253-4126
ispartof Academy Proceedings in Earth and Planetary Sciences, 1998-12, Vol.107 (4), p.413-423
issn 0253-4126
0973-774X
language eng
recordid cdi_proquest_journals_741061841
source Springer Link
subjects Age
Apatite
Chondrites
Chronometers
Cosmochemistry. Extraterrestrial geology
Earth sciences
Earth, ocean, space
Exact sciences and technology
Feldspars
Geochronology
Iodine
Irradiation
Isotope geochemistry. Geochronology
Lead
Measuring instruments
Meteorites. Tectites. Impactites
Mineralization
Phosphates
Radiometric dating
Xenon 129
title The I-Xe chronometer
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-09T07%3A03%3A17IST&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=The%20I-Xe%20chronometer&rft.jtitle=Academy%20Proceedings%20in%20Earth%20and%20Planetary%20Sciences&rft.au=HOHENBERG,%20C.%20M&rft.date=1998-12-01&rft.volume=107&rft.issue=4&rft.spage=413&rft.epage=423&rft.pages=413-423&rft.issn=0253-4126&rft.eissn=0973-774X&rft_id=info:doi/10.1007/BF02841607&rft_dat=%3Cproquest_cross%3E2105654301%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a308t-38f16e4f757850d4b860545db8c3701be5aa177e0e5cec04fbd34f3771732df13%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=741061841&rft_id=info:pmid/&rfr_iscdi=true