Paleomagnetism of the Marble Bar Chert Member, Western Australia: Implications for apparent polar wander path for Pilbara craton during Archean time
The Archean Biosphere Drilling Project (ABDP) drilled a continuous 270 m long oriented core from the Towers Formation, which includes the Marble Bar Chert Member (3456.1–3476.0 Ma) in the Pilbara craton, northwestern Australia. A paleomagnetic study of 261 discrete specimens, collected from a 158.5...
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Veröffentlicht in: | Earth and planetary science letters 2006-12, Vol.252 (3), p.360-371 |
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creator | Suganuma, Yusuke Hamano, Yozo Niitsuma, Sachiko Hoashi, Masamichi Hisamitsu, Toshio Niitsuma, Nobuaki Kodama, Kazuto Nedachi, Munetomo |
description | The Archean Biosphere Drilling Project (ABDP) drilled a continuous 270 m long oriented core from the Towers Formation, which includes the Marble Bar Chert Member (3456.1–3476.0 Ma) in the Pilbara craton, northwestern Australia. A paleomagnetic study of 261 discrete specimens, collected from a 158.5 to 182.0 m section of the Marble Bar Chert Member, revealed two distinct magnetic components (LT and MT). The MT component yields seven different mean paleomagnetic directions clustered as MB1 to MB7. These, together with the published paleomagnetic poles of early Archean rocks from the Pilbara craton, draw a continuous paleomagnetic pole path, which likely to be regarded as the early to late Archean apparent polar wander path (APWP) for the Pilbara craton. The APWP implies that the Pilbara craton underwent a latitudinal drift of about 21° during the interval when the magnetization of the Marble Bar Chert Member was acquired. The estimated speed of the lateral drift is 12–112 cm/yr (120–1120 km/Myr), which is large compared with current plate motion velocities, suggesting that continents might have moved during the Archean faster than in the Phanerozoic. |
doi_str_mv | 10.1016/j.epsl.2006.10.003 |
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The estimated speed of the lateral drift is 12–112 cm/yr (120–1120 km/Myr), which is large compared with current plate motion velocities, suggesting that continents might have moved during the Archean faster than in the Phanerozoic.</description><subject>apparent polar wander path</subject><subject>Archean</subject><subject>Marble Bar Chert</subject><subject>paleomagnetism</subject><subject>Pilbara craton</subject><issn>0012-821X</issn><issn>1385-013X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNp9kUFvEzEQhS1EJULhD3DyiROb2ut4s4u4hAhopVb0UERv1qw92zjy2svYacX_6A9mQzgjjTTSzHtPevoYeyfFUgrZXOyXOOWwrIVo5sNSCPWCLaRqdSWkun_JFkLIumpref-Kvc55L2ahbroFe76FgGmEh4jF55GngZcd8hugPiD_DMS3O6TCb3DskT7wn5gLUuSbQy4EwcNHfjVOwVsoPsXMh0QcpgkIY-FTCnPAE0SHxCcou7_vWx96IOCWoKTI3YF8fOAbsjuEyIsf8Q07GyBkfPtvn7MfX7_cbS-r6-_frrab6wpWtShVI1F3rdLYOdkPutUOpW5UJ-QwuG6tdOeUG_SqGVZS2BbEqtfOrtt2nk5Zpc7Z-1PuROnXYW5mRp8thgAR0yGbWmit1qqZhfVJaCnlTDiYifwI9NtIYY4AzN4cAZgjgONtBjCbPp1MOFd49EgmW4_RovOEthiX_P_sfwAft5Dx</recordid><startdate>20061215</startdate><enddate>20061215</enddate><creator>Suganuma, Yusuke</creator><creator>Hamano, Yozo</creator><creator>Niitsuma, Sachiko</creator><creator>Hoashi, Masamichi</creator><creator>Hisamitsu, Toshio</creator><creator>Niitsuma, Nobuaki</creator><creator>Kodama, Kazuto</creator><creator>Nedachi, Munetomo</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20061215</creationdate><title>Paleomagnetism of the Marble Bar Chert Member, Western Australia: Implications for apparent polar wander path for Pilbara craton during Archean time</title><author>Suganuma, Yusuke ; Hamano, Yozo ; Niitsuma, Sachiko ; Hoashi, Masamichi ; Hisamitsu, Toshio ; Niitsuma, Nobuaki ; Kodama, Kazuto ; Nedachi, Munetomo</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a420t-61e59835e9d1bf585de1563901ffd97359d3df546f410c8a04b5dc78878893c33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>apparent polar wander path</topic><topic>Archean</topic><topic>Marble Bar Chert</topic><topic>paleomagnetism</topic><topic>Pilbara craton</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Suganuma, Yusuke</creatorcontrib><creatorcontrib>Hamano, Yozo</creatorcontrib><creatorcontrib>Niitsuma, Sachiko</creatorcontrib><creatorcontrib>Hoashi, Masamichi</creatorcontrib><creatorcontrib>Hisamitsu, Toshio</creatorcontrib><creatorcontrib>Niitsuma, Nobuaki</creatorcontrib><creatorcontrib>Kodama, Kazuto</creatorcontrib><creatorcontrib>Nedachi, Munetomo</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Earth and planetary science letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Suganuma, Yusuke</au><au>Hamano, Yozo</au><au>Niitsuma, Sachiko</au><au>Hoashi, Masamichi</au><au>Hisamitsu, Toshio</au><au>Niitsuma, Nobuaki</au><au>Kodama, Kazuto</au><au>Nedachi, Munetomo</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Paleomagnetism of the Marble Bar Chert Member, Western Australia: Implications for apparent polar wander path for Pilbara craton during Archean time</atitle><jtitle>Earth and planetary science letters</jtitle><date>2006-12-15</date><risdate>2006</risdate><volume>252</volume><issue>3</issue><spage>360</spage><epage>371</epage><pages>360-371</pages><issn>0012-821X</issn><eissn>1385-013X</eissn><abstract>The Archean Biosphere Drilling Project (ABDP) drilled a continuous 270 m long oriented core from the Towers Formation, which includes the Marble Bar Chert Member (3456.1–3476.0 Ma) in the Pilbara craton, northwestern Australia. A paleomagnetic study of 261 discrete specimens, collected from a 158.5 to 182.0 m section of the Marble Bar Chert Member, revealed two distinct magnetic components (LT and MT). The MT component yields seven different mean paleomagnetic directions clustered as MB1 to MB7. These, together with the published paleomagnetic poles of early Archean rocks from the Pilbara craton, draw a continuous paleomagnetic pole path, which likely to be regarded as the early to late Archean apparent polar wander path (APWP) for the Pilbara craton. The APWP implies that the Pilbara craton underwent a latitudinal drift of about 21° during the interval when the magnetization of the Marble Bar Chert Member was acquired. The estimated speed of the lateral drift is 12–112 cm/yr (120–1120 km/Myr), which is large compared with current plate motion velocities, suggesting that continents might have moved during the Archean faster than in the Phanerozoic.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.epsl.2006.10.003</doi><tpages>12</tpages></addata></record> |
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subjects | apparent polar wander path Archean Marble Bar Chert paleomagnetism Pilbara craton |
title | Paleomagnetism of the Marble Bar Chert Member, Western Australia: Implications for apparent polar wander path for Pilbara craton during Archean time |
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