Loading…
Early Archean spherule beds; chromium isotopes confirm origin through multiple impacts of projectiles of carbonaceous chondrite type
Three Early Archean spherule beds from Barberton, South Africa, have anomalous Cr isotope compositions in addition to large Ir anomalies, confirming the presence of meteoritic material with a composition similar to that in carbonaceous chondrites. The extraterrestrial components in beds S2, S3, and...
Saved in:
Published in: | Geology (Boulder) 2003-03, Vol.31 (3), p.283-286 |
---|---|
Main Authors: | , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | cdi_FETCH-LOGICAL-a369t-71ff33f08e5c64f18c3da92ad9f3f37271891763c720c2848e6a0f10aff477053 |
container_end_page | 286 |
container_issue | 3 |
container_start_page | 283 |
container_title | Geology (Boulder) |
container_volume | 31 |
creator | Kyte, Frank T Shukolyukov, Alex Lugmair, Günter W Lowe, Donald R Byerly, Gary R |
description | Three Early Archean spherule beds from Barberton, South Africa, have anomalous Cr isotope compositions in addition to large Ir anomalies, confirming the presence of meteoritic material with a composition similar to that in carbonaceous chondrites. The extraterrestrial components in beds S2, S3, and S4 are estimated to be ∼1%, 50%-60%, and 15%-30%, respectively. These beds are probably the distal, and possibly global, ejecta from major large-body impacts. These impacts were probably much larger than the Cretaceous-Tertiary event, and all occurred over an interval of ∼20 m.y., implying an impactor flux at 3.2 Ga that was more than an order of magnitude greater than the present flux. |
doi_str_mv | 10.1130/0091-7613(2003)031<0283:EASBCI>2.0.CO;2 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_201156263</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>295718491</sourcerecordid><originalsourceid>FETCH-LOGICAL-a369t-71ff33f08e5c64f18c3da92ad9f3f37271891763c720c2848e6a0f10aff477053</originalsourceid><addsrcrecordid>eNpNkVGL1DAUhYsoOK7-h-CTIp29SdomdUUYy7guLMyD-hyy6c00Q9vUJEXm3R--7Y6IT5cL55x7OV-WXVPYUsrhGqCmuagof8cA-Hvg9BMwyT_ud9-_NHef2Ra2zeGGPcs2tC54zirJnmebf66X2asYTwC0KIXcZH_2OvRnsgumQz2SOHUY5h7JA7bxhpgu-MHNA3HRJz9hJMaP1oWB-OCObiRpEczHjgxzn9y0-NwwaZMi8ZZMwZ_QJNfj02p0ePCjNujnJabzYxtcQpLOE77OXljdR3zzd15lP7_ufzTf8vvD7V2zu881r-qUC2ot5xYklqYqLJWGt7pmuq0tt1wwQWVNRcWNYGCYLCRWGiwFbW0hBJT8Knt7yV1e-zVjTOrk5zAuJxUDSsuKVXwR3V5EJvgYA1o1BTfocFYU1EpArV2qtUu1ElALAbUSUBcCiilQzUGxJenDJemIPhqHo8HfPvTt_1dXPytrWfNHXQqN8w</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>201156263</pqid></control><display><type>article</type><title>Early Archean spherule beds; chromium isotopes confirm origin through multiple impacts of projectiles of carbonaceous chondrite type</title><source>GeoScienceWorld</source><creator>Kyte, Frank T ; Shukolyukov, Alex ; Lugmair, Günter W ; Lowe, Donald R ; Byerly, Gary R</creator><creatorcontrib>Kyte, Frank T ; Shukolyukov, Alex ; Lugmair, Günter W ; Lowe, Donald R ; Byerly, Gary R</creatorcontrib><description>Three Early Archean spherule beds from Barberton, South Africa, have anomalous Cr isotope compositions in addition to large Ir anomalies, confirming the presence of meteoritic material with a composition similar to that in carbonaceous chondrites. The extraterrestrial components in beds S2, S3, and S4 are estimated to be ∼1%, 50%-60%, and 15%-30%, respectively. These beds are probably the distal, and possibly global, ejecta from major large-body impacts. These impacts were probably much larger than the Cretaceous-Tertiary event, and all occurred over an interval of ∼20 m.y., implying an impactor flux at 3.2 Ga that was more than an order of magnitude greater than the present flux.</description><identifier>ISSN: 0091-7613</identifier><identifier>EISSN: 1943-2682</identifier><identifier>DOI: 10.1130/0091-7613(2003)031<0283:EASBCI>2.0.CO;2</identifier><language>eng</language><publisher>Boulder: Geological Society of America (GSA)</publisher><subject>Africa ; Archean ; Barberton greenstone belt ; carbonaceous chondrites ; chondrites ; chromium ; Cr-53/Cr-52 ; ejecta ; Fig Tree Group ; geochemical anomalies ; geochemistry ; Geological time ; impacts ; iridium ; isotope ratios ; Isotopes ; metals ; metamorphic rocks ; meteorites ; Paleoarchean ; platinum group ; Precambrian ; Southern Africa ; spherules ; stable isotopes ; stony meteorites ; Stratigraphy</subject><ispartof>Geology (Boulder), 2003-03, Vol.31 (3), p.283-286</ispartof><rights>GeoRef, Copyright 2020, American Geosciences Institute. Reference includes data supplied by the Geological Society of America @Boulder, CO @USA @United States</rights><rights>Copyright Geological Society of America Mar 2003</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-a369t-71ff33f08e5c64f18c3da92ad9f3f37271891763c720c2848e6a0f10aff477053</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.geoscienceworld.org/lithosphere/article-lookup?doi=10.1130/0091-7613(2003)031<0283:EASBCI>2.0.CO;2$$EHTML$$P50$$Ggeoscienceworld$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,38881,77824</link.rule.ids></links><search><creatorcontrib>Kyte, Frank T</creatorcontrib><creatorcontrib>Shukolyukov, Alex</creatorcontrib><creatorcontrib>Lugmair, Günter W</creatorcontrib><creatorcontrib>Lowe, Donald R</creatorcontrib><creatorcontrib>Byerly, Gary R</creatorcontrib><title>Early Archean spherule beds; chromium isotopes confirm origin through multiple impacts of projectiles of carbonaceous chondrite type</title><title>Geology (Boulder)</title><description>Three Early Archean spherule beds from Barberton, South Africa, have anomalous Cr isotope compositions in addition to large Ir anomalies, confirming the presence of meteoritic material with a composition similar to that in carbonaceous chondrites. The extraterrestrial components in beds S2, S3, and S4 are estimated to be ∼1%, 50%-60%, and 15%-30%, respectively. These beds are probably the distal, and possibly global, ejecta from major large-body impacts. These impacts were probably much larger than the Cretaceous-Tertiary event, and all occurred over an interval of ∼20 m.y., implying an impactor flux at 3.2 Ga that was more than an order of magnitude greater than the present flux.</description><subject>Africa</subject><subject>Archean</subject><subject>Barberton greenstone belt</subject><subject>carbonaceous chondrites</subject><subject>chondrites</subject><subject>chromium</subject><subject>Cr-53/Cr-52</subject><subject>ejecta</subject><subject>Fig Tree Group</subject><subject>geochemical anomalies</subject><subject>geochemistry</subject><subject>Geological time</subject><subject>impacts</subject><subject>iridium</subject><subject>isotope ratios</subject><subject>Isotopes</subject><subject>metals</subject><subject>metamorphic rocks</subject><subject>meteorites</subject><subject>Paleoarchean</subject><subject>platinum group</subject><subject>Precambrian</subject><subject>Southern Africa</subject><subject>spherules</subject><subject>stable isotopes</subject><subject>stony meteorites</subject><subject>Stratigraphy</subject><issn>0091-7613</issn><issn>1943-2682</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><recordid>eNpNkVGL1DAUhYsoOK7-h-CTIp29SdomdUUYy7guLMyD-hyy6c00Q9vUJEXm3R--7Y6IT5cL55x7OV-WXVPYUsrhGqCmuagof8cA-Hvg9BMwyT_ud9-_NHef2Ra2zeGGPcs2tC54zirJnmebf66X2asYTwC0KIXcZH_2OvRnsgumQz2SOHUY5h7JA7bxhpgu-MHNA3HRJz9hJMaP1oWB-OCObiRpEczHjgxzn9y0-NwwaZMi8ZZMwZ_QJNfj02p0ePCjNujnJabzYxtcQpLOE77OXljdR3zzd15lP7_ufzTf8vvD7V2zu881r-qUC2ot5xYklqYqLJWGt7pmuq0tt1wwQWVNRcWNYGCYLCRWGiwFbW0hBJT8Knt7yV1e-zVjTOrk5zAuJxUDSsuKVXwR3V5EJvgYA1o1BTfocFYU1EpArV2qtUu1ElALAbUSUBcCiilQzUGxJenDJemIPhqHo8HfPvTt_1dXPytrWfNHXQqN8w</recordid><startdate>20030301</startdate><enddate>20030301</enddate><creator>Kyte, Frank T</creator><creator>Shukolyukov, Alex</creator><creator>Lugmair, Günter W</creator><creator>Lowe, Donald R</creator><creator>Byerly, Gary R</creator><general>Geological Society of America (GSA)</general><general>Geological Society of America</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7UA</scope><scope>C1K</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope></search><sort><creationdate>20030301</creationdate><title>Early Archean spherule beds; chromium isotopes confirm origin through multiple impacts of projectiles of carbonaceous chondrite type</title><author>Kyte, Frank T ; Shukolyukov, Alex ; Lugmair, Günter W ; Lowe, Donald R ; Byerly, Gary R</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a369t-71ff33f08e5c64f18c3da92ad9f3f37271891763c720c2848e6a0f10aff477053</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><topic>Africa</topic><topic>Archean</topic><topic>Barberton greenstone belt</topic><topic>carbonaceous chondrites</topic><topic>chondrites</topic><topic>chromium</topic><topic>Cr-53/Cr-52</topic><topic>ejecta</topic><topic>Fig Tree Group</topic><topic>geochemical anomalies</topic><topic>geochemistry</topic><topic>Geological time</topic><topic>impacts</topic><topic>iridium</topic><topic>isotope ratios</topic><topic>Isotopes</topic><topic>metals</topic><topic>metamorphic rocks</topic><topic>meteorites</topic><topic>Paleoarchean</topic><topic>platinum group</topic><topic>Precambrian</topic><topic>Southern Africa</topic><topic>spherules</topic><topic>stable isotopes</topic><topic>stony meteorites</topic><topic>Stratigraphy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kyte, Frank T</creatorcontrib><creatorcontrib>Shukolyukov, Alex</creatorcontrib><creatorcontrib>Lugmair, Günter W</creatorcontrib><creatorcontrib>Lowe, Donald R</creatorcontrib><creatorcontrib>Byerly, Gary R</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Geology (Boulder)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kyte, Frank T</au><au>Shukolyukov, Alex</au><au>Lugmair, Günter W</au><au>Lowe, Donald R</au><au>Byerly, Gary R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Early Archean spherule beds; chromium isotopes confirm origin through multiple impacts of projectiles of carbonaceous chondrite type</atitle><jtitle>Geology (Boulder)</jtitle><date>2003-03-01</date><risdate>2003</risdate><volume>31</volume><issue>3</issue><spage>283</spage><epage>286</epage><pages>283-286</pages><issn>0091-7613</issn><eissn>1943-2682</eissn><abstract>Three Early Archean spherule beds from Barberton, South Africa, have anomalous Cr isotope compositions in addition to large Ir anomalies, confirming the presence of meteoritic material with a composition similar to that in carbonaceous chondrites. The extraterrestrial components in beds S2, S3, and S4 are estimated to be ∼1%, 50%-60%, and 15%-30%, respectively. These beds are probably the distal, and possibly global, ejecta from major large-body impacts. These impacts were probably much larger than the Cretaceous-Tertiary event, and all occurred over an interval of ∼20 m.y., implying an impactor flux at 3.2 Ga that was more than an order of magnitude greater than the present flux.</abstract><cop>Boulder</cop><pub>Geological Society of America (GSA)</pub><doi>10.1130/0091-7613(2003)031<0283:EASBCI>2.0.CO;2</doi><tpages>4</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0091-7613 |
ispartof | Geology (Boulder), 2003-03, Vol.31 (3), p.283-286 |
issn | 0091-7613 1943-2682 |
language | eng |
recordid | cdi_proquest_journals_201156263 |
source | GeoScienceWorld |
subjects | Africa Archean Barberton greenstone belt carbonaceous chondrites chondrites chromium Cr-53/Cr-52 ejecta Fig Tree Group geochemical anomalies geochemistry Geological time impacts iridium isotope ratios Isotopes metals metamorphic rocks meteorites Paleoarchean platinum group Precambrian Southern Africa spherules stable isotopes stony meteorites Stratigraphy |
title | Early Archean spherule beds; chromium isotopes confirm origin through multiple impacts of projectiles of carbonaceous chondrite type |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T13%3A10%3A42IST&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=Early%20Archean%20spherule%20beds;%20chromium%20isotopes%20confirm%20origin%20through%20multiple%20impacts%20of%20projectiles%20of%20carbonaceous%20chondrite%20type&rft.jtitle=Geology%20(Boulder)&rft.au=Kyte,%20Frank%20T&rft.date=2003-03-01&rft.volume=31&rft.issue=3&rft.spage=283&rft.epage=286&rft.pages=283-286&rft.issn=0091-7613&rft.eissn=1943-2682&rft_id=info:doi/10.1130/0091-7613(2003)031%3C0283:EASBCI%3E2.0.CO;2&rft_dat=%3Cproquest_cross%3E295718491%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a369t-71ff33f08e5c64f18c3da92ad9f3f37271891763c720c2848e6a0f10aff477053%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=201156263&rft_id=info:pmid/&rfr_iscdi=true |