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Comparison of Th, Sr, Nd and Pb Isotopes in Oceanic basalts: implications for Mantle heterogeneity and Magma genesis. Earth
, 2006
"... Abstract We report U-Th disequilibria data for a suite of 13 young basaltic samples from the Samoan Islands, which represent the endmember mantle component EM2, and 4 historic lavas from Mt. Erebus, typifying young HIMU. We interpret this observation in terms of differences in the melting regimes b ..."
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Abstract We report U-Th disequilibria data for a suite of 13 young basaltic samples from the Samoan Islands, which represent the endmember mantle component EM2, and 4 historic lavas from Mt. Erebus, typifying young HIMU. We interpret this observation in terms of differences in the melting regimes beneath mid-ocean ridges and ocean islands.
Frontiers in large igneous province research: Lithos, v
, 2005
"... Abstract Earth history is punctuated by events during which large volumes of mafic magmas were generated and emplaced by processes distinct from bnormalQ seafloor spreading and subduction-related magmatism. Large Igneous Provinces (LIPs) of Mesozoic and Cenozoic age are the best preserved, and comp ..."
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Abstract Earth history is punctuated by events during which large volumes of mafic magmas were generated and emplaced by processes distinct from bnormalQ seafloor spreading and subduction-related magmatism. Large Igneous Provinces (LIPs) of Mesozoic and Cenozoic age are the best preserved, and comprise continental flood basalts, volcanic rifted margins, oceanic plateaus, ocean basin flood basalts, submarine ridges, ocean islands and seamount chains. Paleozoic and Proterozoic LIPs are typically more deeply eroded and are recognized by their exposed plumbing system of giant dyke swarms, sill provinces and layered intrusions. The most promising Archean LIP candidates (apart from the Fortescue and Ventersdorp platformal flood basalts) are those greenstone belts containing tholeiites with minor komatiites. Some LIPs have a substantial component of felsic rocks. Many LIPs can be linked to regional-scale uplift, continental rifting and breakup, climatic shifts that may result in extinction events, and Ni-Cu-PGE (platinum group element) ore deposits. Some current frontiers in LIP research include: (1) Testing various mantle plume and alternative hypotheses for the origin for LIPs. (2) Characterizing individual LIPs in terms of (a) original volume and areal extent of their combined extrusive and intrusive components, (b) melt production rates, (c) plumbing system geometry, (d) nature of the mantle source region, and (e) links with ore deposits. (3) Determining the distribution of LIPs in time (from Archean to Present) and in space (after continental reconstruction). This will allow assessment of proposed links between LIPs and supercontinent breakup, juvenile crust production, climatic excursions, and mass extinctions. It will also allow an evaluation of periodicity in the LIP record, the identification of clusters of LIPs, and postulated links with the reversal frequency of the Earth's magnetic field. (4) Comparing the characteristics, origin and distribution of LIPs on Earth with planets lacking plate tectonics, such as Venus and Mars. Interplanetary comparison may also provide a better understanding of convective processes in the mantles of the inner planets. In order to achieve rapid progress in these frontier areas, a global campaign is proposed, which would focus on highprecision geochronology, integrated with paleomagnetism and geochemistry. Most fundamentally, such a campaign could
Homogeneous superchondritic 142 Nd/ 144 Nd in the mid-ocean ridge basalt and ocean island basalt
, 2012
"... [1] 146Sm decays to 142Nd with a relatively short half-life (68 Ma). The 142Nd/144Nd of modern terrestrial mantle-derived lavas is 18 5 ppm higher than the chondrite reservoir. The difference in 142Nd/144Nd between Earth and chondrites likely owes to Sm/Nd ratios 6 % higher in the accessible Earth ..."
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[1] 146Sm decays to 142Nd with a relatively short half-life (68 Ma). The 142Nd/144Nd of modern terrestrial mantle-derived lavas is 18 5 ppm higher than the chondrite reservoir. The difference in 142Nd/144Nd between Earth and chondrites likely owes to Sm/Nd ratios 6 % higher in the accessible Earth that arose within the first 30 million years following accretion. In order to constrain the early history of the mantle domains sampled by ocean island basalts (OIB) and mid-ocean ridge basalts (MORB), we present high-precision 142Nd/144Nd measurements on 11 different lavas from five hot spots, and one lava each from the Indian and Atlantic ridges. The lavas examined in this study bracket much of the known Sr-Nd-Pb-He isotopic variability the in mantle. These data complement existing high-precision 142Nd/144Nd data on MORB and OIB lavas. In agreement with previous studies, we find that MORB and OIB lavas examined for high-precision 142Nd/144Nd exhibit ratios that are indistinguishable from the terrestrial standard and are 15–20 ppm higher than the average obtained for ordinary and enstatite chondrites. The uniform, super-chondritic 142Nd/144Nd data in OIB and MORB are consistent with derivation from a common, early formed (<30 Ma after accretion) progenitor reservoir with Sm/Nd 6 % higher than chondrites. If there exists any variability in 142Nd/144Nd in the OIBs and MORBs examined to date, it is too small to be resolved with
Monte Carlo simulations of metasomatic enrichment in the lithosphere and implications for the source of alkaline basalts
- Journal of Petrology
, 2011
"... One hypothesis for the origin of alkaline lavas erupted on oceanic islands and in intracontinental settings is that they represent the melts of amphibole-rich veins in the lithosphere (or melts of their dehydrated equivalents if metasomatized lithosphere is recycled into the convecting mantle). Amph ..."
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One hypothesis for the origin of alkaline lavas erupted on oceanic islands and in intracontinental settings is that they represent the melts of amphibole-rich veins in the lithosphere (or melts of their dehydrated equivalents if metasomatized lithosphere is recycled into the convecting mantle). Amphibole-rich veins are interpreted as cumulates produced by crystallization of low-degree melts of the underlying asthenosphere as they ascend through the lithosphere. We present the results of trace-element modelling of the formation and melting of veins formed in this way with the goal of testing this hypothesis and for predicting how variability in the formation and subsequent melting of such cumulates (and adjacent cryptically and modally metasomatized lithospheric peridotite) would be manifested in magmas generated by such a process. Because the high-pressure phase equilibria of hydrous near-solidus melts of garnet lherzolite are poorly constrained and given the likely high variability of the
Petrogenesis of Latest Miocene^Quaternary Continental IntraplateVolcanism along the Northern Dead Sea Fault System (Al Ghab^HomsVolcanic Field),Western Syria: Evidence for Lithosphere^Asthenosphere Interaction
, 2009
"... Late Miocene to Quaternary intraplate basaltic volcanism in the Al ..."
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Late Miocene to Quaternary intraplate basaltic volcanism in the Al
Models for Noble Gases in Mantle Geochemistry: Some Observations and Alternatives
, 2004
"... Models for noble gases in the Earth's mantle are evaluated against a number of observational constraints: 1) high 3He/4He ratios do not correlate with high (initial) 3He concentrations, 2) MORB and OIB 3He/4He data do not represent two different distributions [Anderson 2001], 3) globally robust ..."
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Models for noble gases in the Earth's mantle are evaluated against a number of observational constraints: 1) high 3He/4He ratios do not correlate with high (initial) 3He concentrations, 2) MORB and OIB 3He/4He data do not represent two different distributions [Anderson 2001], 3) globally robust correlations between 3He/4He ratios and lithophile isotopic systems are not observed, 4) diverse local correlations exist that are broadly linear, 5) large, local geographical 3He/4He variations are observed, which are inconsistent with a strongly localized (i.e. plume-stem) flux of high-3He/4He material, and 6) dramatic temporal 3He/4He variations are observed on very short time scales (102 years). Layered (reservoir) models for noble gases, in which a deep and radially constrained region of the Earth’s mantle preserves unradiogenic He and Ne isotopic compositions because of a high noble gas concentration, do not seem consistent with these observations. Heterogeneous (non-layered) mantle models for noble gases, in which the carrier of unradiogenic He is a relatively noble-gas-poor component scattered in the (upper) mantle, appear more consistent with the constraints.
DoWe Really Need Mantle Components to Define Mantle Composition?
, 2006
"... We discuss the concept of components in the Earth’s mantle starting from a petrological and geochemical approach, but adopting a new method of projection of geochemical and isotopic data.This allows the compositional variability of magmatic associations to be evalu-ated in multi-dimensional space, t ..."
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We discuss the concept of components in the Earth’s mantle starting from a petrological and geochemical approach, but adopting a new method of projection of geochemical and isotopic data.This allows the compositional variability of magmatic associations to be evalu-ated in multi-dimensional space, thus simultaneously accounting for a large number of compositional variables.We demonstrate that ocean island basalts (OIB) and mid-ocean ridge basalts (MORB) are derived from a marble-cake mantle, in which different degrees of partial melting of recycled lithosphere, which are heterogeneous in age and composition, contribute to the magma genesis. This view is supported by the variability in the geochemical and isotopic signa-tures of OIB that are observed on the scale of a single ocean island as well as on that of an ocean, mostly varying between two extreme com-positions, that are not strictly related to the commonly accepted mantle components (DMM, EMI, EMII, HIMU). Rather they
Final Magma Storage Depth Modulation of Explosivity andTrachyte^Phonolite Genesis at an IntraplateVolcano: a Case Study from Ulleung Island, South Korea
, 2013
"... Ulleung Island is the top of a 3000 m (from sea floor) intraplate al-kalic volcanic edifice in the East Sea/Sea of Japan. The emergent 950 m consist of a basaltic lava and agglomerate succession (Stage 1, 1·37^0·97Ma), intruded and overlain by a sequence of trachytic lavas and domes, which erupted i ..."
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Ulleung Island is the top of a 3000 m (from sea floor) intraplate al-kalic volcanic edifice in the East Sea/Sea of Japan. The emergent 950 m consist of a basaltic lava and agglomerate succession (Stage 1, 1·37^0·97Ma), intruded and overlain by a sequence of trachytic lavas and domes, which erupted in two episodes (Stage 2, 0·83^ 0·77Ma; Stage 3, 0·73^0·24Ma). The youngest eruptions, post 20 ka BP, were explosive, generating thick tephra sequences of phonoli-tic composition (Stage 4), which also entrained phaneritic, porphy-ritic and cumulate accidental lithics. Major element chemistry of the evolved products shows a continuous spectrum of trachyte to phonolite compositions, but these have discordant trace element trends and distinct isotopic characteristics, excluding a direct genetic relationship between the two end-members. Despite this, the Stage 3 trachytes and some porphyritic accidental lithics have chemical char-acteristics transitional between Stage 2 trachytes and Stage 4 phono-
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, 2006
"... www.elsevier.com/locate/epsl Os isotope heterogeneity of the upper mantle: Evidence from the Mayarí–Baracoa ophiolite belt in eastern Cuba ..."
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www.elsevier.com/locate/epsl Os isotope heterogeneity of the upper mantle: Evidence from the Mayarí–Baracoa ophiolite belt in eastern Cuba