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Geochemistry of a new enriched mantle type locality in the northern hemisphere: Implications for the origin of the EM-I source
Authors:Jörg Geldmacher  Kaj Hoernle  Andreas Klügel  Paul van den Bogaard  Ilya Bindeman
Institution:1. Department of Earth Science, University of California, Santa Barbara, USA;2. Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA;3. Department of Marine Geology and Geophysics, Woods Hole Oceanographic Institution, 266 Woods Hole Road, Woods Hole, MA 02543, USA;4. Geological and Planetary Sciences Division, California Institute of Technology, Pasadena, CA 91125, USA;5. School of Earth Sciences, The University of Melbourne, Victoria 3010, Australia;1. Dipartimento di Ingegneria & Geologia (InGeO), Università G. D''Annunzio di Chieti-Pescara, Via dei Vestini 31, 66100 Chieti, Italy;2. Institute for Mineralogy, Leibniz University of Hannover, Callinstrasse 3, Hannover D-30167, Germany;3. Istituto Nazionale di Geofisica e Vulcanologia, INGV, Via di Vigna Murata 605, 00143 Roma, Italy;4. Dipartimento di Scienze della Terra, Sapienza Università di Roma, Piazzale A. Moro 5, 00185 Roma, Italy;1. NIRVANA Laboratories, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA;2. Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA;3. Institut für Geowissenschaften, Goethe Universität Frankfurt, Altenhöferalle 1, 60438 Frankfurt am Main, Germany;4. Seafloor Hydrothermal Activity Laboratory of the Key Laboratory of Marine Geology and Environment, Institute of Oceanology, Chinese Academy of Sciences, Qingdao, Shandong 266071, China;5. University of Chinese Academy of Sciences, Beijing 100049, China;6. School of Earth & Space Exploration, Arizona State University, Tempe, AZ 85287, USA;7. Department of Solid Earth Geochemistry, Japan Agency for Marine-Earth Science and Technology, Yokosuka 237-0061, Japan
Abstract:Late Cretaceous (66.2 ± 0.5 Ma amphibole and 66.7 ± 0.2 Ma phlogopite 40Ar/39Ar ages) nephelinitic volcanic rocks from Godzilla Seamount in the eastern North Atlantic (34°N latitude) have trace element and Sr–Nd–Pb–Hf-isotope compositions similar to the Enriched Mantle I (EM-I) endmember, except for their low 207Pb/204Pb relative to 206Pb/204Pb ratios (206Pb/204Pbin = 17.7, 207Pb/204Pbin = 15.34) plotting below the Northern Hemisphere Reference Line on the uranogenic Pb isotope diagram. O isotope data on amphibole separates are mantle-like (δ18O = 5.6–5.8‰). Age and location of the isolated Godzilla Seamount, however, preclude it from being derived from the Madeira or Canary hotspots, making a lower-mantle origin unlikely. Therefore we propose derivation from a shallow (lithospheric/asthenospheric) melting anomaly. As observed in mid-ocean-ridge and ocean-island basalts, there is a systematic decrease of 207Pb/204Pb ratios (and Δ7/4) in the individual EM-I endmember type localities towards northern latitudes with Godzilla lying on the extension of this trend. This trend is mirrored in ultra-potassic volcanic rocks such as lamproites and kimberlites, which reflect the composition of enriched subcontinental lithospheric mantle. Therefore, a global pattern in 207Pb/204Pb ratios and Δ7/4 is suggested. The geochemical composition of EM-I endmember type localities, including Godzilla lavas, and the enriched (DUPAL) anomaly in the southern hemisphere could reflect derivation from ancient, metasomatized subcontinental lithospheric mantle. We propose a two-stage model to explain the trace element and isotopic composition of the EM-I mantle endmember localities worldwide: 1) during the early history of the Earth, subcontinental lithosphere was metasomatized by melts from subducted slabs along convergent margins generating high μ (238U/204Pb) sources, and 2) as the Earth cooled, hydrous fluids replaced hydrous melts as the main slab component metasomatizing the subcontinental lithospheric mantle (generating EM-I sources with lower μ). In accordance with this model, the global variations in 207Pb/204Pb ratios and Δ7/4 could reflect geographic differences in μ and/or the age at which the transition from stages 1 to 2 took place in the Archaean lithosphere. The model would require a re-definition of the EM-I endmember to low 206Pb/204Pb, high 208Pb/204Pb (positive Δ8/4) but variable 207Pb/204Pb (positive and negative Δ7/4).
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