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Isotopic variations with distance and time in the volcanic islands of the Cameroon line: evidence for a mantle plume origin

dc.contributor.authorLee, Der-Chuenen_US
dc.contributor.authorHalliday, Alexander N.en_US
dc.contributor.authorFitton, J. Godfreyen_US
dc.contributor.authorPoli, Giamperoen_US
dc.date.accessioned2006-04-10T18:10:21Z
dc.date.available2006-04-10T18:10:21Z
dc.date.issued1994-05en_US
dc.identifier.citationLee, Der-Chuen, Halliday, Alex N., Fitton, J. Godfrey, Poli, Giampero (1994/05)."Isotopic variations with distance and time in the volcanic islands of the Cameroon line: evidence for a mantle plume origin." Earth and Planetary Science Letters 123(1-3): 119-138. <http://hdl.handle.net/2027.42/31599>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V61-46YCVHP-X/2/b50427ac2d26371c642344b557ac866fen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/31599
dc.description.abstractThe oceanic sector of the Cameroon line consists of three volcanic islands: Principe, Sao Tome and Pagalu. New 40Ar---39Ar data for Pagalu basalts, combined with published K---Ar ages for Principe and Sao Tome, indicate that all three islands have been active in the past 5 Ma. They have similar petrogenetic histories, with basements of basaltic flows capped by more evolved rocks. However, the age of the earliest exposed volcanic rocks decreases oceanward from Principe (31 Ma) to Sao Tome (13 Ma) to Pagalu (4.8 Ma). This age progression is consistent with the suggested motion of the African plate over this period of time. The average incompatible trace element compositions of 87Sr/86Sr)t increases from 0.7029 to 0.7037 and (206Pb/204Pb)t decreases from 20.2 to 18.9 from Principe through Sao Tome to Pagalu for all samples younger than 10 Ma. In addition to the overall spatial isotopic variations, Principe and Sao Tome display temporal isotopic variations, with Pb isotopic ratios becoming progressively more radiogenic. Pagalu shows no temporal geochemical or isotopic differences and the island has the least radiogenic Pb but most radiogenic Sr. These distinctive Pb, Sr and Nd isotopic compositions are also found in the early tholeiitic hyaloclastite breccia from Principe (31 Ma). Similarly, the Nd and Sr isotopic compositions are identical to those of the earliest Sao Tome lavas (13 Ma) and the Pb isotopic compositions of early Sao Tome samples are only slightly radiogenic relative to Pagalu. Therefore, it is probable that all these islands were initiated from a common source, similar to that of Pagalu, that migrated relative to the melt zone of each island with time. Since their initiation, the magma conduits at Principe and Sao Tome have been gradually modified by the introduction of a HIMU component. The common source from which the islands were initially derived probably represents ambient upper mantle, entrained with the plume head during ascent. This entrained component is like `PREMA', but the Nd and Sr isotopic data indicate that it represents variably mixed depleted and enriched components, such as DMM and EMI. The HIMU component is probably representative of a lower mantle source from which the plume head was derived. The long-lived episodic magmatism on Principe provides evidence that the initial melt migration paths from the upper mantle form a hot zone that can be re-activated after long periods (107 yr) of apparent quiescence. The progression to HIMU characteristics within each island probably reflects the gradual flattening of the contaminated plume head within this hot zone, near the base of the lithosphere, and the melting of a stem composed of relatively uncontaminated HIMU mantle.en_US
dc.format.extent1434050 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleIsotopic variations with distance and time in the volcanic islands of the Cameroon line: evidence for a mantle plume originen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeology and Earth Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Geological Sciences, University of Michigan, 1006 C.C. Little Building, Ann Arbor, MI 48109-1063, USAen_US
dc.contributor.affiliationumDepartment of Geological Sciences, University of Michigan, 1006 C.C. Little Building, Ann Arbor, MI 48109-1063, USAen_US
dc.contributor.affiliationotherDepartment of Geology and Geophysics, University of Edinburgh, Edinburgh, EH9 3JW, UKen_US
dc.contributor.affiliationotherDepartment of Earth Science, University of Perugia, I-06100, Perugia, Italyen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/31599/1/0000528.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0012-821X(94)90262-3en_US
dc.identifier.sourceEarth and Planetary Science Lettersen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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