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Rb-Sr and Sm-Nd isotopic variations in dissected crustal xenoliths

dc.contributor.authorDer-Chuen Lee,en_US
dc.contributor.authorHalliday, Alexander N.en_US
dc.contributor.authorHunter, Robert H.en_US
dc.contributor.authorHolden, Peteren_US
dc.contributor.authorUpton, Brian G. J.en_US
dc.date.accessioned2006-04-10T15:57:26Z
dc.date.available2006-04-10T15:57:26Z
dc.date.issued1993-01en_US
dc.identifier.citationDer-Chuen Lee, , Halliday, Alex N., Hunter, Robert H., Holden, Peter, Upton, Brian G. J. (1993/01)."Rb-Sr and Sm-Nd isotopic variations in dissected crustal xenoliths." Geochimica et Cosmochimica Acta 57(1): 219-230. <http://hdl.handle.net/2027.42/31064>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V66-488Y4J7-1BF/2/afd72a9b05dd7e37ceb9436a76da3743en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/31064
dc.description.abstractFour crustal xenoliths from Scotland have been dissected in order to evaluate the effects of magma-xenolith interaction on Rb-Sr and Sm-Nd isotopic systematics, and hence the use of the xenoliths for accurate determination of source compositions. Each xenolith was sampled from the edge to the center. The Nd isotopic compositions are virtually uniform across each xenolith; however, there are significant variations in Rb, Sr, and REE concentration, as well as Rb/Sr and Sm/Nd ratios and Sr isotopic composition. Most of this variation appears to be inherited from the protolith. However, one sample shows systematic variations in Rb and Sr concentration and Sr isotopic composition with distance from the xenolith edges due to interaction with the host magma. This sample displays petrographic evidence for grain boundary melt infiltration. These data are consistent with theoretical considerations of transport times and diffusivities that place limits on the amount of modification that is possible via diffusion alone. The calculated effects of transport of even large amounts of crustal xenoliths on the compositions of xenoliths and host magmas will be small, provided transport times are short.Overall, the isotopic variations within the xenolith suite mirror the source rocks from which they were extracted and are inferred to reflect variations in the deep crust of Scotland. However, small samples, such as most crustal xenoliths, may be of little use in defining meaningful crustal residence ages because of modal variations in metamorphic minerals and isotopic re-equilibration. The one xenolith studied has extremely variable Sm/Nd ratios due to the presence of garnet and yields a broad range of geologically meaningless Nd model ages, but yields an Sm-Nd isochron age of 396 +/- 49 Ma. The Loch Roag xenolith has a large range of Rb/Sr ratio, and the Sr isotopic data define an isochron age of 416+/-28 Ma. Both ages are taken to represent the timing of metamorphism and/or cooling from 600[deg]C at the end of the Caledonian Orogeny in Scotland.en_US
dc.format.extent1690000 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleRb-Sr and Sm-Nd isotopic variations in dissected crustal xenolithsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeology and Earth Sciencesen_US
dc.subject.hlbsecondlevelChemistryen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Geological Sciences, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumDepartment of Geological Sciences, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherDepartment of Earth Sciences, University of Liverpool, Liverpool, L69 3BX, UKen_US
dc.contributor.affiliationotherDepartment of Earth and Space Sciences, University of California at Los Angeles, Los Angeles, CA 90024, USAen_US
dc.contributor.affiliationotherDepartment of Geology and Geophysics, University of Edinburgh, Edinburgh, EH9 3JW, UKen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/31064/1/0000741.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0016-7037(93)90480-Ken_US
dc.identifier.sourceGeochimica et Cosmochimica Actaen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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