ORCID Profile
0000-0002-3883-5498
Current Organisation
Macquarie University
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Geology | Igneous And Metamorphic Petrology | Geotectonics | Geochemistry | Geochronology And Isotope Geochemistry | Tectonics | Igneous and Metamorphic Petrology | Isotope Geochemistry | Geophysics | Geochemistry Not Elsewhere Classified | Inorganic Geochemistry | Geodynamics | Geophysics Not Elsewhere Classified | Petroleum and Coal Geology | Earth Sciences Not Elsewhere Classified | Manufacturing Engineering not elsewhere classified | Sedimentology | Exploration Geochemistry | Marine Geoscience | Geochronology | Policy and Administration | Environmental Monitoring | Other Stratigraphy (Incl. Sequence Stratigraphy) | Geology Not Elsewhere Classified | Geomorphology | Seismology and Seismic Exploration | Palaeoclimatology | Simulation And Modelling | Optimisation | Climatology (Incl. Palaeoclimatology) | Earthquake Seismology | Electrical and Electromagnetic Methods in Geophysics | Other Earth Sciences | Research, Science and Technology Policy | Mathematical Sciences Not Elsewhere Classified | Environmental Sciences Not Elsewhere Classified |
Earth sciences | Expanding Knowledge in the Earth Sciences | Mineral Exploration not elsewhere classified | Mathematical sciences | Land and water management | Biological sciences | Environmental and resource evaluation not elsewhere classified | Climate change | Environmentally Sustainable Mineral Resource Activities not elsewhere classified | Other environmental aspects | Ceramics | Effects of Climate Change and Variability on Australia (excl. Social Impacts) | Oil and gas | Oil and Gas Exploration | Mineral Resources (excl. Energy Resources) not elsewhere classified | Exploration | Expanding Knowledge in the Chemical Sciences | Precious (Noble) Metal Ore Exploration | Expanding Knowledge in the Agricultural and Veterinary Sciences | Titanium Minerals, Zircon, and Rare Earth Metal Ore (e.g. Monazite) Exploration | Copper Ore Exploration | Other
Publisher: Elsevier BV
Date: 02-2016
Publisher: Springer Science and Business Media LLC
Date: 18-04-2022
Publisher: Elsevier BV
Date: 09-2022
Publisher: Elsevier BV
Date: 08-2006
Publisher: Springer Science and Business Media LLC
Date: 19-08-2012
Publisher: Elsevier BV
Date: 10-03-2009
Publisher: Springer Science and Business Media LLC
Date: 08-1995
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier
Date: 2011
Publisher: Elsevier BV
Date: 04-2014
Publisher: Elsevier BV
Date: 08-2009
Publisher: Elsevier BV
Date: 11-1980
Publisher: Elsevier BV
Date: 11-2009
Publisher: Geological Society of America
Date: 1987
Publisher: Mineralogical Society
Date: 07-2013
Publisher: Elsevier BV
Date: 04-1979
Publisher: Geological Society of London
Date: 1986
Publisher: Elsevier BV
Date: 02-2014
Publisher: Elsevier BV
Date: 10-2016
Publisher: Elsevier BV
Date: 10-2020
Publisher: Elsevier BV
Date: 04-2016
Publisher: Mineralogical Society
Date: 04-1997
DOI: 10.1180/MINMAG.1997.061.405.09
Abstract: The proton microprobe has been used to determine contents of Ca, Ti, Ni, Mn and Zn in the olivine of 54 spinel lherzolite xenoliths from Australian and Chinese basalts. These data are compared with proton-probe data for Ni, Mn and Zn in the olivine of 180 garnet peridotite xenoliths from African and Siberian kimberlites. Fe, Mn, Ni and Zn contents are well-correlated because the spinel lherzolite olivines have higher mean Fe contents than garnet peridotite olivines (average Fo 89.6 vs. Fo 90–92 ) they also have lower Ni and higher Mn contents. Zn and Fe are well-correlated in garnet peridotite olivine, but in spinel peridotites this relationship is perturbed by partitioning of Zn into spinel. None of these elements shows significant correlation with temperature. Consistent differences in trace-element contents of olivines in the two suites is interpreted as reflecting the greater degree of depletion of Archean garnet peridotites as compared to Phanerozoic spinel lherzolites. Ca and Ti contents of spinel-peridotite olivine are well correlated with one another, and with temperature as determined by several types of geothermometer. However, Ca contents are poorly correlated with pressure as determined by the Ca-in-olivine barometer of Köhler and Brey (1990). This reflects the strong T -dependence of this barometer: the uncertainty in pressure (calculated by this method) which is produced by the ±50°C uncertainty expected of any geothermometer is ca ± 8 kbar, corresponding to the entire width of the spinel-lherzolite field at 900–1200°C.
Publisher: Elsevier BV
Date: 02-2010
Publisher: Geological Society of America
Date: 2003
DOI: 10.1130/G19619.1
Publisher: Pleiades Publishing Ltd
Date: 10-2010
Publisher: Elsevier BV
Date: 07-2015
Publisher: MDPI AG
Date: 31-07-2020
DOI: 10.3390/MIN10080686
Abstract: Laser ablation MC-ICP-MS was used to measure the Os-isotope compositions of single sulfide grains, including laurite (RuS2) and pentlandite [(Fe,Ni)9S8], from two chromitite bodies and host lherzolites from ophiolites of North Andaman (Indo-Burma-Sumatra subduction zone). The results show isotopic heterogeneity in both laurite (n = 24) and pentlandite (n = 37), similar to that observed in other chromitites and peridotites from the mantle sections of ophiolites. Rhenium-depletion model ages (TRD) of laurite and pentlandite reveal episodes of mantle magmatism and/or metasomatism in the Andaman mantle predating the formation of the ophiolite (and the host chromitites), mainly at ≈0.5, 1.2, 1.8, 2.1 and 2.5 Ga. These ages match well with the main tectonothermal events that are documented in the continental crustal rocks of South India, suggesting that the Andaman mantle (or its protolith) had a volume of lithospheric mantle once underlaying this southern Indian continental crust. As observed in other oceanic lithospheres, blocks of ancient subcontinental lithospheric mantle (SCLM) could have contributed to the development of the subduction-related Andaman–Java volcanic arc. Major- and trace-element compositions of chromite indicate crystallization from melts akin to high-Mg IAT and boninites during the initial stages of development of this intra-oceanic subduction system.
Publisher: Elsevier BV
Date: 03-2010
Publisher: Springer Science and Business Media LLC
Date: 08-2005
DOI: 10.1038/NATURE03902
Abstract: Abyssal peridotites are assumed to represent the mantle residue of mid-ocean-ridge basalts (MORBs). However, the osmium isotopic compositions of abyssal peridotites and MORB do not appear to be in equilibrium, raising questions about the cogenetic relationship between those two reservoirs. However, the cause of this isotopic mismatch is mainly due to a drastic filtering of the data based on the possibility of osmium contamination by sea water. Here we present a detailed study of magmatic sulphides (the main carrier of osmium) in abyssal peridotites and show that the 187Os/188Os ratio of these sulphides is of primary mantle origin and can reach radiogenic values suggesting equilibrium with MORB. Thus, the effect of sea water on the osmium systematics of abyssal peridotites has been overestimated and consequently there is no true osmium isotopic gap between MORBs and abyssal peridotites.
Publisher: Elsevier BV
Date: 07-2011
Publisher: Elsevier
Date: 2007
Publisher: Elsevier BV
Date: 08-2006
Publisher: MDPI AG
Date: 10-2021
DOI: 10.3390/MIN11101083
Abstract: In this short communication, we present preliminary data on the Re-Os isotopic systematics of platinum-group minerals (PGM) recovered from different horizons in the Falcondo Ni-laterite in the Dominican Republic. The results show differences in the Os-isotope composition in different populations of PGM: (i) pre-lateritic PGM yield 187Os/188Os varying from 0.11973 ± 0.00134 to 0.12215 ± 0.00005 (2σ uncertainty) whereas (ii) lateritic PGM are more radiogenic in terms of 187Os/188Os (from 0.12390 ± 0.00001 to 0.12645 ± 0.00005 2σ uncertainty). We suggest that these differences reflect the opening of the Re-Os system in in idual grains of PGM during lateritic weathering. The implications of these results are twofold as they will help to (1) elucidate the small-scale mobility of noble metals in the supergene setting and therefore the possible formation of PGM at these very low temperatures, (2) better refine the Os-isotopic datasets of PGM that are currently being used for defining dynamic models of core–mantle separation, crustal generation, and fundamental plate-tectonic processes such as the opening of oceans.
Publisher: Elsevier BV
Date: 04-2003
Publisher: Wiley
Date: 02-2004
Publisher: Geological Society of America
Date: 2004
DOI: 10.1130/G20366.1
Publisher: Geological Society of London
Date: 2008
DOI: 10.1144/SP293.9
Publisher: Elsevier BV
Date: 05-2014
Publisher: American Journal of Science (AJS)
Date: 02-2014
DOI: 10.2475/02.2014.01
Publisher: Research Square Platform LLC
Date: 08-03-2022
DOI: 10.21203/RS.3.RS-1394420/V1
Abstract: Adiabatic decompressional melting of asthenosphere under spreading centers has been accepted to produce vertical compositional variations of oceanic lithospheric mantle. However, theoretical estimates of the compositional gradients are much smaller than those observed from ophiolites, clearly requiring additional processes. Here we conduct systematic high-density s ling and whole-rock and mineral compositional analyses of harzburgites in a Tibetan ophiolitic mantle section (~2 km thick), which shows a primary upward depletion (~12% difference over ~2 km) and local depleted anomalies. Thermodynamic modeling demonstrates that these features cannot be produced by decompressional melting or proportional compression of residual mantle. Instead, they can be explained by reaction between silica-undersaturated melts and peridotite with lateral melt/rock variations in the topmost asthenospheric upwelling column, showing stronger depletion in its melt-focusing center and local zones. This column will split from the center into two parts, which rotate in the mantle flow to become horizontal, thus forming the oceanic uppermost lithospheric mantle characterized by vertical depletion and local anomalies within a sub-spreading-center regime.
Publisher: Elsevier BV
Date: 12-2018
Publisher: Springer Science and Business Media LLC
Date: 19-08-2023
DOI: 10.1038/S43247-023-00956-6
Abstract: Rare earth element ore deposits associated with carbonatite derived from Earth’s mantle supply half of the world’s rare earth element. However, the formation of carbonatite and initial enrichment and transport of rare earth element in the mantle, is unclear. Here, we image the lithospheric architecture of a Cenozoic rare earth element ore belt in southwestern China by integrating seismic tomography with geochemical data. The subduction of the Indian continent caused vertical upwelling and lateral flow of the asthenosphere, which triggered the melting of the overlying subcontinental lithospheric mantle to generate carbonatites. Such a mantle source that previously metasomatized by fluids from recycled marine sediments is a precursor process critical for forming a giant rare earth element system. For the studied ore belt, three key factors are prerequisites to generating ore-forming carbonatites: thick lithosphere with a continental root prior fertilization of the subcontinental lithospheric mantle and trans-lithospheric weakness for magma ascent.
Publisher: Elsevier BV
Date: 05-2018
Publisher: Wiley
Date: 19-11-2010
Publisher: Elsevier BV
Date: 12-2012
Publisher: Mineralogical Society
Date: 08-1999
Abstract: Diamonds from alluvial deposits near Wellington, New South Wales, have been characterized on the basis of morphological features, mineral inclusions, C isotope signatures, N content and aggregation state and internal structure. The diamonds are of two types. The larger group (Group A) is indistinguishable from diamonds found worldwide from kimberlitic and l roitic host rocks. This group is inferred to have formed in a peridotitic mantle source in Pre-Cambrian subcratonic lithosphere. The second group (Group B) is unique in its internal structures (which show evidence of growth in a stress field and non-planar facets), has unusually heavy C isotopic compositions and contains Ca-rich eclogitic inclusions. This group is inferred to have formed in a subducting slab. Diamonds of both groups have external features (corrosion structures and polish) indicating transport to the surface by l roitic-like magmas. The diamonds show evidence of long residence at the earth's surface and significant alluvial reworking: they are not accompanied by typical diamond indicator minerals.
Publisher: Oxford University Press (OUP)
Date: 25-01-2021
DOI: 10.1093/PETROLOGY/EGAA115
Abstract: Harzburgite–dunite associations in the Yushigou ophiolitic complex (North Qilian suture, NW China) offer insights into melt migration and melt–rock interaction above a subduction zone. Based on detailed petrographic and in situ analyses, we propose a three-stage model to describe the history of melt channel formation in oceanic arc mantle. In the first stage, high-degree melt extraction was followed by widespread infiltration of small-volume melts, which formed the harzburgite that makes up most of the Yushigou complex. The Yushigou harzburgites thus have highly refractory major-element compositions (olivine Fo = 91·1–93·2, spinel Cr# [atomic 100 × Cr/(Cr + Al)] = 55·2–62·9, whole-rock Mg# = 90·5–92·0, Al2O3 = 0·29–0·74 wt%, CaO = 0·35–0·54 wt%, and low Na2O = 0·02–0·05 wt%) but slight enrichment in the light rare earth elements (LREE). In the second stage, high-volume focused melts infiltrated into the mantle wedge and produced two types of dunite, with high-Cr# (mainly 63·1–73·6) versus low-Cr# (23·6–33·7) spinel. In the low-Cr# dunites, spinels have significantly fewer inclusions and lower Fo values (88·7–90·1) in olivine than in the high-Cr# dunite (Fo = 89·9–90·5), together with higher modal abundances of interstitial sulfides. The two groups of dunite show similar extremely low TiO2 (& ·01 wt%) but different igneous clinopyroxene trace-element patterns (ΣLREE/ΣHREE ≈ 1 in low-Cr# dunite versus ΣLREE/ΣHREE & in high-Cr# dunite), indicating distinct differences in the infiltrating melts. The low-Cr# dunite is a cumulate from an anhydrous Al- and S-enriched basaltic melt, whereas the high-Cr# dunite was produced by reaction of harzburgite with a carbon-bearing, alkaline hydrous silicate magma. The confluence of these melt migrations finally formed a channelized dunite network, and later magmatic activity was restricted to these channels. Pulsated melt supply after chromite crystallization formed pervasive sieve-textured rims around spinel in both kinds of dunite, but these are rare in the harzburgite. The third stage was marked by fluid-dominated metasomatism recorded by millimeter-scale veined conduits, which contain carbonate (dolomite and magnesite), hibole, phlogopite and compound crystal assemblages in both kinds of dunite. CH4–N2–graphite-dominated fluid inclusions are widespread in all lithologies, recording the volatiles transported during the last metasomatic event. The Yushigou complex thus provides a detailed ex le of interaction between multiple batches of melt or fluid and a lithospheric mantle wedge dunitic channel system. The results of this study further suggest that the formation of podiform chromite requires melt participation, and the nature and origins of the melts can be erse.
Publisher: Wiley
Date: 18-05-2019
DOI: 10.1111/GGR.12265
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 02-1986
Publisher: Elsevier BV
Date: 05-2018
Publisher: Elsevier BV
Date: 11-2006
Publisher: Oxford University Press (OUP)
Date: 07-2009
Publisher: Geological Society of America
Date: 2006
DOI: 10.1130/G22569.1
Publisher: Elsevier BV
Date: 03-2020
Publisher: Geological Society of America
Date: 02-2015
DOI: 10.1130/G36245.1
Publisher: Springer Science and Business Media LLC
Date: 10-05-2019
Publisher: Springer Science and Business Media LLC
Date: 26-07-2023
Publisher: Elsevier BV
Date: 10-2019
Publisher: Springer Science and Business Media LLC
Date: 02-2022
Publisher: Geological Society of London
Date: 2010
DOI: 10.1144/SP337.1
Publisher: Springer Science and Business Media LLC
Date: 11-08-2018
Publisher: Elsevier BV
Date: 10-2007
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 10-2017
Publisher: Elsevier BV
Date: 12-1990
Publisher: Oxford University Press (OUP)
Date: 04-07-2009
Publisher: Elsevier BV
Date: 03-2008
Publisher: Springer Science and Business Media LLC
Date: 08-05-2007
Publisher: Geological Society of America
Date: 31-12-2018
DOI: 10.1130/G45362.1
Publisher: Elsevier BV
Date: 04-2002
Publisher: Oxford University Press (OUP)
Date: 08-10-2007
Publisher: Elsevier BV
Date: 09-2015
Publisher: Springer Science and Business Media LLC
Date: 1984
DOI: 10.1007/BF00373055
Publisher: Elsevier BV
Date: 2000
Publisher: Informa UK Limited
Date: 08-2001
Publisher: Elsevier BV
Date: 08-2003
Publisher: Elsevier BV
Date: 30-03-2006
Publisher: Geological Society of America
Date: 2006
DOI: 10.1130/G22282.1
Publisher: Springer Science and Business Media LLC
Date: 19-03-2020
Publisher: Elsevier BV
Date: 03-1994
Publisher: Geological Society of America
Date: 08-2010
DOI: 10.1130/G31219.1
Publisher: Elsevier BV
Date: 09-2004
Publisher: Elsevier BV
Date: 05-2011
Publisher: Elsevier BV
Date: 07-2001
Publisher: Mineralogical Society of America
Date: 04-2021
DOI: 10.2138/AM-2021-7714
Abstract: An intensive study of the geochemical characteristics (including the volatile elements Cl and S) of apatite associated with porphyry deposits was undertaken to address the debate about the crust- or mantle-derivation of their copper and gold and to better understand the controls on the transport of metals in magmatic fluids in post-subduction settings. New geochemical data on apatite reveal parameters to discriminate mineralized porphyry systems across Iran and western China (Tibet and Yunnan), from coeval barren localities across this post-subduction metallogenic belt. Apatites in fertile porphyries have higher Cl and S concentrations (reflecting water-rich crystallization conditions) than those from coeval barren ones. Our new isotopic data also indicate these volatiles are likely derived from pre-enriched sub-continental lithospheric mantle, metasomatized by previous oceanic subduction. This study demonstrates that refertilization of suprasubduction lithospheric mantle during previous collision events is a prerequisite for forming post-subduction fertile porphyries, providing an evidence-based alternative to current ore-enrichment models.
Publisher: Elsevier BV
Date: 09-2004
Publisher: Elsevier BV
Date: 09-2004
Publisher: Elsevier BV
Date: 11-2003
Publisher: American Geophysical Union (AGU)
Date: 11-2002
DOI: 10.1029/2001GC000287
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 05-2021
Publisher: American Geophysical Union (AGU)
Date: 04-2010
DOI: 10.1029/2008TC002428
Publisher: European Association of Geochemistry
Date: 09-2018
Publisher: Royal Society of Chemistry (RSC)
Date: 2005
DOI: 10.1039/B501374G
Publisher: Informa UK Limited
Date: 23-02-2022
Publisher: MDPI AG
Date: 19-12-2018
DOI: 10.3390/MIN8120601
Abstract: The new mineral species carmeltazite, ideally ZrAl2Ti4O11, was discovered in pockets of trapped melt interstitial to, or included in, corundum xenocrysts from the Cretaceous Mt Carmel volcanics of northern Israel, associated with corundum, tistarite, anorthite, osbornite, an unnamed REE (Rare Earth Element) phase, in a Ca-Mg-Al-Si-O glass. In reflected light, carmeltazite is weakly to moderately bireflectant and weakly pleochroic from dark brown to dark green. Internal reflections are absent. Under crossed polars, the mineral is anisotropic, without characteristic rotation tints. Reflectance values for the four COM wavelengths (Rmin, Rmax (%) (λ in nm)) are: 21.8, 22.9 (471.1) 21.0, 21.6 (548.3), 19.9, 20.7 (586.6) and 18.5, 19.8 (652.3). Electron microprobe analysis (average of eight spot analyses) gave, on the basis of 11 oxygen atoms per formula unit and assuming all Ti and Sc as trivalent, the chemical formula (Ti3+3.60Al1.89Zr1.04Mg0.24Si0.13Sc0.06Ca0.05Y0.02Hf0.01)Σ=7.04O11. The simplified formula is ZrAl2Ti4O11, which requires ZrO2 24.03, Al2O3 19.88, and Ti2O3 56.09, totaling 100.00 wt %. The main diffraction lines, corresponding to multiple hkl indices, are (d in Å (relative visual intensity)): 5.04 (65), 4.09 (60), 2.961 (100), 2.885 (40), and 2.047 (60). The crystal structure study revealed carmeltazite to be orthorhombic, space group Pnma, with unit-cell parameters a = 14.0951 (9), b = 5.8123 (4), c = 10.0848 (7) Å, V = 826.2 (1) Å3, and Z = 4. The crystal structure was refined to a final R1 = 0.0216 for 1165 observed reflections with Fo 4σ(Fo). Carmeltazite exhibits a structural arrangement similar to that observed in a defective spinel structure. The name carmeltazite derives from Mt Carmel (“CARMEL”) and from the dominant metals present in the mineral, i.e., Titanium, Aluminum and Zirconium (“TAZ”). The mineral and its name have been approved by the IMA Commission on New Minerals, Nomenclature and Classification (2018-103).
Publisher: Elsevier BV
Date: 02-1990
Publisher: Springer Science and Business Media LLC
Date: 08-11-2011
Publisher: Elsevier BV
Date: 07-2003
Publisher: Elsevier BV
Date: 11-2017
Publisher: Springer Science and Business Media LLC
Date: 16-11-2012
Publisher: Oxford University Press (OUP)
Date: 05-2018
Publisher: Elsevier BV
Date: 08-1987
Publisher: Elsevier BV
Date: 09-2004
Publisher: Geological Society of America
Date: 02-2015
DOI: 10.1130/G36231.1
Publisher: Oxford University Press (OUP)
Date: 29-06-2018
Publisher: Springer Science and Business Media LLC
Date: 10-2000
DOI: 10.1038/35038049
Abstract: The abundances of highly siderophile (iron-loving) elements (HSEs) in the Earth's mantle provide important constraints on models of the Earth's early evolution. It has long been assumed that the relative abundances of HSEs should reflect the composition of chondritic meteorites--which are thought to represent the primordial material from which the Earth was formed. But the non-chondritic abundance ratios recently found in several types of rock derived from the Earth's mantle have been difficult to reconcile with standard models of the Earth's accretion, and have been interpreted as having arisen from the addition to the primitive mantle of either non-chondritic extraterrestrial material or differentiated material from the Earth's core. Here we report in situ laser-ablation analyses of sulphides in mantle-derived rocks which show that these sulphides do not have chondritic HSE patterns, but that different generations of sulphide within single s les show extreme variability in the relative abundances of HSEs. Sulphides enclosed in silicate phases have high osmium and iridium abundances but low Pd/Ir ratios, whereas pentlandite-dominated interstitial sulphides show low osmium and iridium abundances and high Pd/Ir ratios. We interpret the silicate-enclosed sulphides as the residues of melting processes and interstitial sulphides as the crystallization products of sulphide-bearing (metasomatic) fluids. We suggest that non-chondritic HSE patterns directly reflect processes occurring in the upper mantle--that is, melting and sulphide addition via metasomatism--and are not evidence for the addition of core material or of 'exotic' meteoritic components.
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 04-1995
Publisher: Elsevier BV
Date: 06-2011
Publisher: Geological Society of America
Date: 2004
DOI: 10.1130/G20133.1
Publisher: Science China Press., Co. Ltd.
Date: 2005
DOI: 10.1360/982004-808
Publisher: Elsevier BV
Date: 03-2019
Publisher: Elsevier BV
Date: 02-2010
Publisher: Springer Science and Business Media LLC
Date: 16-07-2004
Publisher: Schweizerbart
Date: 10-10-2017
Publisher: Elsevier BV
Date: 2011
Publisher: Science China Press., Co. Ltd.
Date: 2004
DOI: 10.1360/04WD0137
Publisher: Elsevier BV
Date: 02-2017
Publisher: Springer Science and Business Media LLC
Date: 14-08-2009
Publisher: Elsevier BV
Date: 04-2017
Publisher: Elsevier BV
Date: 02-2018
Publisher: Elsevier BV
Date: 08-2010
Publisher: Springer Science and Business Media LLC
Date: 23-11-2015
DOI: 10.1038/SREP16878
Abstract: To understand the behavior of Li in zircon, we have analyzed the abundance and isotopic composition of Li in three zircon standards (Plešovice, Qinghu and Temora) widely used for microbeam analysis of U-Pb ages and O-Hf isotopes. We have mapped Li concentration ([Li]) on large grains, using a Cameca 1280HR Secondary Ion Mass Spectrometer (SIMS). All zircons have a rim 5–20 μm wide in which [Li] is 5 to 20 times higher than in the core. Up to ~20‰ isotopic fractionation is observed on a small scale in the rims of a single zircon grain. The measured δ 7 Li values range from –14.3 to 3.7‰ for Plešovice, –22.8 to 1.4‰ for Qinghu and –4.7 to 16.1‰ for Temora zircon. The [Li] and δ 7 Li are highly variable at the rims, but relatively homogenous in the cores of the grains. From zircon rim to core, [Li] decreases rapidly, while δ 7 Li increases, suggesting that the large isotopic variation of Li in zircons could be caused by diffusion. Our data demonstrate that homogeneous δ 7 Li in the cores of zircon can retain the original isotopic signatures of the magmas, while the bulk analysis of Li isotopes in mineral separates and in bulk-rock s les may produce misleading data.
Publisher: Elsevier BV
Date: 09-2020
Publisher: Wiley
Date: 12-2015
Publisher: Elsevier BV
Date: 12-2013
Publisher: Springer Science and Business Media LLC
Date: 10-10-2017
DOI: 10.1038/S41467-017-00821-Z
Abstract: Gold enrichment at the crustal or mantle source has been proposed as a key ingredient in the production of giant gold deposits and districts. However, the lithospheric-scale processes controlling gold endowment in a given metallogenic province remain unclear. Here we provide the first direct evidence of native gold in the mantle beneath the Deseado Massif in Patagonia that links an enriched mantle source to the occurrence of a large auriferous province in the overlying crust. A precursor stage of mantle refertilisation by plume-derived melts generated a gold-rich mantle source during the Early Jurassic. The interplay of this enriched mantle domain and subduction-related fluids released during the Middle-Late Jurassic resulted in optimal conditions to produce the ore-forming magmas that generated the gold deposits. Our study highlights that refertilisation of the subcontinental lithospheric mantle is a key factor in forming large metallogenic provinces in the Earth’s crust, thus providing an alternative view to current crust-related enrichment models.
Publisher: Elsevier BV
Date: 09-2000
Publisher: Elsevier BV
Date: 04-2006
Publisher: Elsevier BV
Date: 11-2008
Publisher: Elsevier BV
Date: 11-2016
Publisher: Elsevier BV
Date: 10-2018
Publisher: Geological Society of London
Date: 09-2021
DOI: 10.1144/M56-2020-13
Abstract: We present a summary of peridotite in the Subantarctic (46–60° S) surrounding the Antarctic Plate. Peridotite xenoliths occur on the Kerguelen Islands and Auckland Islands. The Kerguelen Islands are underlain by a plume, whereas the Auckland Islands are part of continental Zealandia, which is a Gondwana-rifted fragment. Small amounts of serpentinized peridotite has been dredged from fracture zones on the Southeast Indian Ridge, Southwest Indian Ridge and Pacific Antarctic Ridge, and represent upwelled asthenosphere accreted to form lithosphere. Suprasubduction-zone peridotite was collected from two locations on the Sandwich Plate. Peridotites from most subantarctic occurrences are moderately to highly depleted, and many show signs of subsequent metasomatic enrichment. Os isotopes indicate that subantarctic continental and oceanic lithospheric mantle contains ancient fragments that underwent depletion long before formation of the overlying crust.
Publisher: Elsevier BV
Date: 12-2019
Publisher: Oxford University Press (OUP)
Date: 10-2016
Publisher: Wiley
Date: 16-11-2022
Publisher: Society of Economic Geologists
Date: 09-2010
Publisher: Elsevier BV
Date: 12-2012
Publisher: Elsevier BV
Date: 03-2003
Publisher: Elsevier BV
Date: 03-2017
Publisher: Springer Science and Business Media LLC
Date: 19-12-2012
Publisher: Elsevier BV
Date: 06-2009
Publisher: Elsevier BV
Date: 10-2002
Publisher: Oxford University Press (OUP)
Date: 02-1984
Publisher: Oxford University Press (OUP)
Date: 21-11-2006
Publisher: Elsevier BV
Date: 05-2008
Publisher: Elsevier BV
Date: 12-2023
Publisher: Springer Science and Business Media LLC
Date: 1991
DOI: 10.1007/BF00687203
Publisher: Mineralogical Society of America
Date: 04-2019
DOI: 10.2138/AM-2019-6949
Publisher: Wiley
Date: 12-2015
Publisher: Elsevier BV
Date: 07-2004
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 09-2015
Publisher: Elsevier BV
Date: 04-2008
Publisher: Springer Science and Business Media LLC
Date: 05-09-2011
Publisher: Informa UK Limited
Date: 09-1980
DOI: 10.1071/EG980121
Publisher: Elsevier BV
Date: 2012
Publisher: Elsevier BV
Date: 06-2009
Publisher: Springer Science and Business Media LLC
Date: 1973
DOI: 10.1007/BF00373880
Publisher: Elsevier BV
Date: 05-2004
Publisher: Elsevier BV
Date: 06-2009
Publisher: Elsevier BV
Date: 06-2009
Publisher: Elsevier BV
Date: 11-2009
Publisher: Science China Press., Co. Ltd.
Date: 2003
DOI: 10.1360/03WD0028
Publisher: Springer Berlin Heidelberg
Date: 06-04-2012
Publisher: Geological Society of London
Date: 2010
DOI: 10.1144/SP337
Publisher: Springer Science and Business Media LLC
Date: 07-1997
DOI: 10.1038/40606
Publisher: Institute of Earth's Crust, Siberian Branch of the Russian Academy of Sciences
Date: 2017
Publisher: Oxford University Press (OUP)
Date: 11-2017
Publisher: Oxford University Press (OUP)
Date: 03-09-2007
Publisher: American Geophysical Union (AGU)
Date: 31-08-2023
DOI: 10.1029/2023GL104951
Abstract: A diffuse magmatic province covering central‐eastern Asia continent displays a compositional transition at 120–100 Ma and probably reflects melting initiation in isotopically enriched lithospheric mantle, followed by melting of the asthenosphere. However, the cause for the transition across such a vast landmass remains poorly constrained. Here, analyses of newly found Chaoge basalts (∼95 Ma, central Asia) and compiled data from across the basaltic province are combined to reveal the factors controlling the basalt dichotomy. The Chaoge basalts are considered to originate from a hot pyroxenite‐bearing asthenosphere with potential temperatures of ∼1,450°C, overlapping the source thermochemical conditions for most post‐transition basaltic rocks. The asthenosphere in 120–100 Ma is suggested to be hotter and to have controlled the compositional transition in the studied basaltic province. We suggest that asthenospheric warming resulted from prolonged continental thermal blanketing and can account for other diffuse igneous provinces with similar compositional variations and tectonic histories.
Publisher: Pleiades Publishing Ltd
Date: 06-2009
Publisher: Geological Society of America
Date: 17-09-2021
DOI: 10.1130/B36041.1
Abstract: New trace-element, radiogenic Sr-Nd-Pb isotopic and geochronological data from Middle-Late Cretaceous Zagros ophiolites of Iran give new insights into the tectono-magmatic history of these supra-subduction zone (SSZ)-type ophiolites. The distribution of Middle-Late Cretaceous SSZ-type ophiolites in Iran comprises two parallel belts: (1) the outer Zagros ophiolitic belt and (2) the inner Zagros ophiolitic belt. These Middle-Late Cretaceous ophiolites were generated by seafloor spreading in what became the fore-arc and back-arc during the subduction initiation event and now define a ~3000-km-long belt from Cyprus to Turkey, Syria, Iran, the UAE, and Oman. The Zagros ophiolites contain complete (if disrupted) mantle and crustal sequences. Mantle sequences from both outer-belt and inner-belt ophiolites are dominated by dunites, harzburgites, and lherzolites with minor chromitite lenses. Peridotites are also intruded by gabbros and a variety of mafic to minor felsic (plagiogranite and dacite) dikes. Crustal rocks comprise ultramafic-mafic cumulates as well as isotropic gabbros, sheeted dike complexes, pillowed and massive lavas, and felsic rocks. Our new zircon U-Pb ages indicate that the outer-belt and inner-belt ophiolites formed near coevally during the Middle-Late Cretaceous 100–96 Ma for the outer belt and 105–94 Ma for the inner belt. Both incompatible-element ratios and isotopic data confirm that depleted mantle and variable contributions of subduction components were involved in the genesis of outer-belt and inner-belt rocks. Our data for the outer belt and inner belt along with those from better-studied ophiolites in Cyprus, Turkey, the UAE, and Oman lead to the conclusion that a broad, ~3000-km-long swath of fore-arc lithosphere was created during Middle-Late Cretaceous time.
Publisher: Wiley
Date: 10-2001
Publisher: Elsevier BV
Date: 08-2006
Publisher: European Association of Geochemistry
Date: 11-2016
Publisher: Elsevier BV
Date: 03-2011
Publisher: Elsevier BV
Date: 07-2004
Publisher: Elsevier BV
Date: 07-2004
Publisher: Elsevier BV
Date: 07-2004
Publisher: Springer Science and Business Media LLC
Date: 28-10-2010
Publisher: Elsevier BV
Date: 1985
Publisher: Elsevier BV
Date: 12-2017
Publisher: Elsevier BV
Date: 11-2017
Publisher: Elsevier BV
Date: 07-2001
Publisher: Oxford University Press (OUP)
Date: 06-2017
Publisher: Wiley
Date: 10-2020
Publisher: Informa UK Limited
Date: 08-2008
Publisher: Springer Science and Business Media LLC
Date: 07-2001
DOI: 10.1007/BF02900604
Publisher: Elsevier BV
Date: 11-2007
Publisher: Elsevier BV
Date: 09-2017
Publisher: Elsevier BV
Date: 07-2000
Publisher: Elsevier BV
Date: 2012
Publisher: American Geophysical Union (AGU)
Date: 07-2006
DOI: 10.1029/2005GC001120
Publisher: Informa UK Limited
Date: 23-11-2018
Publisher: Elsevier BV
Date: 10-2012
Publisher: Elsevier BV
Date: 10-2015
Publisher: Elsevier BV
Date: 11-2011
Publisher: Elsevier BV
Date: 08-2005
Publisher: Elsevier BV
Date: 10-2012
Publisher: Elsevier BV
Date: 02-2015
Publisher: Elsevier BV
Date: 06-2009
Publisher: Elsevier BV
Date: 03-2004
Publisher: Elsevier BV
Date: 06-2009
Publisher: Oxford University Press (OUP)
Date: 1991
Publisher: Elsevier BV
Date: 10-2010
Publisher: Elsevier BV
Date: 03-2022
Publisher: Elsevier BV
Date: 11-2016
Publisher: Springer Science and Business Media LLC
Date: 17-06-2008
Publisher: Oxford University Press (OUP)
Date: 31-03-2006
Publisher: Springer Science and Business Media LLC
Date: 14-06-2009
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier BV
Date: 08-2006
Publisher: Oxford University Press (OUP)
Date: 04-2016
Publisher: Elsevier BV
Date: 11-2016
Publisher: Elsevier BV
Date: 06-2018
Publisher: Springer Science and Business Media LLC
Date: 16-12-2012
Publisher: Geological Society of America
Date: 2007
DOI: 10.1130/G23092A.1
Publisher: Geological Society of America
Date: 2011
Publisher: Elsevier BV
Date: 05-2022
Publisher: Mineralogical Society
Date: 04-2002
Abstract: The Pingtan and Tonglu igneous complexes in SE China are typical of the calc-alkaline series developed at active continental margins. These two complexes are dominated by felsic rocks, temporally and spatially associated with minor mafic rocks. Morphological and trace-element studies of zircon populations in rocks from each of these complexes show that the zircon populations may be ided into 3–4 distinct growth stages, characterized by different distributions of morphological indices ( I pr , I py and I el ), and different contents of the substituting elements (Hf, U, Th, Y and P). The four growth stages recognized in the zircons are believed to have formed successively in the magma chamber, during the emplacement, and in the early and later stages of magma consolidation, respectively. All four stages are recognized in the plutonic Pingtan complex, whereas the stages 3 and 4 are less developed in the volcanic/subvolcanic Tonglu complex. Based on the chemistry and morphology of the different zircon populations of the Pingtan and Tonglu complexes, it is suggested that basaltic magmas underplating at the boundary between crust and mantle caused partial melting of the mid–lower crust and produced granitoid magmas. Subsequently, mixing between magmas was important.
Publisher: Mineralogical Society of America
Date: 09-2021
DOI: 10.2138/AM-2021-7680
Abstract: Xenocrysts and xenoliths in Upper Cretaceous pyroclastics on Mount Carmel (northern Israel) represent a series of similar magma-fluid systems at different stages of their evolution, recording a continuous decrease in oxygen fugacity (fO2) as crystallization proceeded. Corundum coexisting with Fe-Mg-Cr-Al spinels, other Fe-Mg-Al-Na oxides, and Fe-Ni alloys in apparent cumulates crystallized at fO2 values near the iron-wüstite (IW) buffer (fO2 = IW±1) and is zoned from high-Cr cores to lower-Cr rims, consistent with fractional crystallization trends. The reconstructed parental melts of the cumulates are Al-Cr-Fe-Mg oxides with ca. 2 wt% SiO2. Corundum in other possible cumulates that contain Cr-Fe (Fe 45 wt%) alloys has low-Cr cores and still lower-Cr rims. Corundum coexisting with Cr0 (fO2 = IW-5) in some possible cumulates has low-Cr cores, but high-Cr rims (to & % Cr2O3). These changes in zoning patterns reflect the strong decrease in the melting point of Cr2O3, relative to Al2O3, with decreasing fO2. The electron energy loss spectroscopy (EELS) analyses show that all Cr in corundum that coexists with Cr0 is present as Cr3+. This suggests that late in the evolution of these reduced melts, Cr2+ has disproportionated via the reaction 3Cr2+(melt) → 2Cr3+(Crn) + Cr0. The most Cr-rich corundum crystallized together with β-alumina phases including NaAl11O17 (diaoyudaoite) and KAl11O17 (kahlenbergite) and β″-alumina phases residual melts crystallized a range of (K,Mg)2(Al,Cr)10O17 phases with the kahlenbergite structure. The parental melts of these assemblages appear to have been Al-Cr-K-Na-Mg oxides, which may be related to the Al-Cr-Fe-Mg oxide melts mentioned above, through fractional crystallization or liquid immiscibility. These s les are less reduced (fO2 from IW to IW-5) than the assemblages of the trapped silicate melts in the more abundant xenoliths of corundum aggregates (fO2 = IW-6 to IW-10). They could be considered to represent an earlier stage in the fO2 evolution of an “ideal” Mt. Carmel magmatic system, in which mafic or syenitic magmas were fluxed by mantle-derived CH4+H2 fluids. This is a newly recognized step in the evolution of the Mt. Carmel assemblages and helps to understand element partitioning under highly reducing conditions.
Publisher: Informa UK Limited
Date: 12-1973
Publisher: Oxford University Press (OUP)
Date: 05-1999
Publisher: Springer Science and Business Media LLC
Date: 11-05-2018
Publisher: Informa UK Limited
Date: 06-1991
DOI: 10.1071/EG991295
Publisher: Elsevier BV
Date: 12-2009
Publisher: Springer Science and Business Media LLC
Date: 12-2015
Publisher: Elsevier BV
Date: 03-1989
Publisher: Elsevier BV
Date: 06-1991
Publisher: Wiley
Date: 03-1983
Publisher: Oxford University Press (OUP)
Date: 02-08-2006
Publisher: Royal Society of Chemistry (RSC)
Date: 1998
DOI: 10.1039/A707972I
Publisher: Elsevier BV
Date: 11-2018
Publisher: Springer Science and Business Media LLC
Date: 20-06-2014
Publisher: Elsevier BV
Date: 09-1997
Publisher: Wiley
Date: 03-06-2015
DOI: 10.1111/TER.12157
Publisher: Elsevier BV
Date: 07-1996
Publisher: Springer Science and Business Media LLC
Date: 2007
Publisher: Springer Science and Business Media LLC
Date: 11-03-2006
Publisher: Elsevier BV
Date: 02-2020
Publisher: Elsevier BV
Date: 09-2013
Publisher: Elsevier BV
Date: 05-2013
Publisher: Elsevier BV
Date: 09-1999
Publisher: American Geophysical Union (AGU)
Date: 10-2005
DOI: 10.1029/2005GC000978
Publisher: Elsevier BV
Date: 11-1983
Publisher: Mineralogical Society
Date: 24-05-2023
DOI: 10.1180/MGM.2023.36
Publisher: Geological Society of America
Date: 1994
Publisher: Elsevier BV
Date: 07-2004
Publisher: Springer Science and Business Media LLC
Date: 23-05-2017
Publisher: Elsevier BV
Date: 06-2004
Publisher: Elsevier BV
Date: 06-1984
Publisher: Geological Society of America
Date: 2002
Publisher: Elsevier BV
Date: 11-2015
Publisher: Oxford University Press (OUP)
Date: 26-10-2005
Publisher: Oxford University Press (OUP)
Date: 20-10-2005
Publisher: Springer Science and Business Media LLC
Date: 21-11-2014
Publisher: Scientific Societies
Date: 03-2020
DOI: 10.1094/PHYTO-08-19-0320-R
Abstract: The root lesion nematode Pratylenchus thornei causes economic losses in wheat and barley internationally through both reduced grain yield and grain quality. This study investigated the relationships between the presowing P. thornei density and grain yield and the postharvest nematode densities. Four field experiments were conducted at the same site between 2010 and 2014. A range of presowing P. thornei densities was established in the first year by growing three cereal cultivars that ranged from resistant to susceptible. In the following year, plots were sown with the five same cereal cultivars. A linear relationship was observed between the natural log of the presowing P. thornei density and grain yield across all seasons. The results showed that grain yield losses varied between cultivars and seasons. The importance of season was significant, with this study conducted over several seasons, and it highlighted the variability in yield losses between seasons, which will need further investigation. The greatest yield losses observed were 25 to 28% when the maximum presowing P. thornei densities ranged between 150 and 250 P. thornei g of soil −1 . An analysis of the relationship between the presowing and postharvest nematode densities revealed that increased presowing nematode densities resulted in decreased multiplication rates in all seasons and in all cultivars. Nematode multiplication rates also varied between seasons. These results explain why it is difficult to predict nematode levels based on cropping history, and additionally, they highlight the importance of growing resistant cultivars to maintain low levels of P. thornei to minimize risk of yield losses.
Publisher: Sociedad Geologica Mexicana
Date: 28-11-2020
DOI: 10.18268/BSGM2020V72N3A080420
Abstract: Chromitites hosted in the serpentinized harzburgite bodies from Los Congos and Los Guanacos (Eastern P ean Ranges, north Argentina) record a complex metamorphic evolution. The hydration of chromitites during the retrograde metamorphism, their subsequent dehydration during the prograde metamorphism and the later-stage cooling, have resulted in a threefold alteration of chromite: i) Type I is characterized by homogeneous Fe3+- and Cr-rich chromite ii) Type II chromite contains exsolved textures that consist in blebs and fine lamellae of a magnetite-rich phase hosted in a spinel-rich phase iii) Type III chromite is formed by variable proportions of magnetite-rich and spinel-rich phases with symplectitic texture. Type I chromite shows lower Ga and higher Co, Zn and Mn than magmatic chromites from chromitites in suprasubduction zone ophiolites as a consequence of the redistribution of these elements between Fe3+-rich non-porous chromite and silicates during the prograde metamorphism. Whereas, the spinel-rich phase in Type III chromite is enriched in Co, Zn, Sc, and Ga, but depleted in Mn, Ni, V and Ti with respect to the magnetite-rich phase, due to the metamorphic cooling from high-temperature conditions. The pseudosection calculated in the fluid-saturated FCrMACaSH system, and contoured for Cr# and Mg#, allows us to constrain the temperature of formation of Fe3+-rich non-porous chromite by the diffusion of magnetite in Fe2+-rich porous chromite at ºC and 20 kbar. The subsequent dehydration of Fe3+-rich non-porous chromite by reaction with antigorite and chlorite formed Type I chromite and Mg-rich olivine and pyroxene at ºC and 10 kbar. The ultimate hydration of silicates in Type I chromite and the exsolution of Type II and Type III chromites would have started at ~600 ºC. These temperatures are in the range of those estimated for ocean floor serpentinization ( ºC and kbar), the regional prograde metamorphism in the granulite facies (800 ºC and kbar), and subsequent retrogression to the hibolite facies (600 ºC and 4-6.2 kbar) in the host ultramafic rocks at Los Congos and Los Guanacos. A continuous and slow cooling from granulite to hibolite facies produced the exsolution of spinel-rich and magnetite-rich phases, developing symplectitic textures in Type III chromite. However, the discontinuous and relatively fast cooling produced the exsolution of magnetite-rich phase blebs and lamellae within Type II chromite. The P-T conditions calculated in FCrMACaSH system and the complex textural and geochemical fingerprints showed by Type I, Type II and Type III chromites leads us to suggest that continent-continent collisional orogeny better records the fingerprints of prograde metamorphism in ophiolitic chromitites.
Publisher: Elsevier BV
Date: 08-2004
Publisher: Elsevier BV
Date: 08-2004
Publisher: Elsevier BV
Date: 11-2001
Publisher: Elsevier BV
Date: 11-2010
Publisher: Elsevier BV
Date: 2017
Publisher: Elsevier BV
Date: 04-2008
Publisher: Geological Society of America
Date: 2003
Publisher: Elsevier BV
Date: 06-2004
Publisher: Elsevier BV
Date: 10-2022
Publisher: Elsevier BV
Date: 03-2021
Publisher: Elsevier BV
Date: 10-2005
Publisher: Elsevier BV
Date: 02-2020
Publisher: Elsevier BV
Date: 08-2018
Publisher: Geological Society of America
Date: 1999
Publisher: Elsevier BV
Date: 06-2010
Publisher: Elsevier BV
Date: 10-2009
Publisher: American Geophysical Union (AGU)
Date: 07-2019
DOI: 10.1029/2018JB016582
Abstract: This study analyzes the microstructures and deformational characteristics of spinel peridotite xenoliths from the Nógrád‐Gömör Volcanic Field (NGVF), located on the northern margin of a young extensional basin presently affected by compression. The xenoliths show a wide range of microstructures, bearing the imprints of heterogeneous deformation and variable degrees of subsequent annealing. Olivine crystal preferred orientations (CPOs) have dominantly [010]‐fiber and orthorhombic patterns. Orthopyroxene CPOs indicate coeval deformation with olivine. Olivine J indices correlate positively with equilibration temperatures, suggesting that the CPO strength increases with depth. In contrast, the intensity of intragranular deformation in olivine varies as a function of the s ling locality. We interpret the microstructures and CPO patterns as recording deformation by dislocation creep in a transpressional regime, which is consistent with recent tectonic evolution in the Carpathian‐Pannonian region due to the convergence between the Adria microplate and the European platform. Postkinematic annealing is probably linked to percolation of metasomatism by mafic melts through the upper mantle of the NGVF prior to the eruption of the host alkali basalt. Elevated equilibration temperatures in xenoliths from the central part of the volcanic field are interpreted to be associated with the last metasomatic event, which only shortly preceded the ascent of the host magma. Despite well‐developed olivine CPOs in the xenoliths, which imply a strong seismic anisotropy, the lithospheric mantle alone cannot account for the shear wave splitting delay times measured in the NGVF, indicating that deformation in both the lithosphere and the asthenosphere contributes to the observed shear wave splitting.
Publisher: Informa UK Limited
Date: 15-11-2019
Publisher: Elsevier BV
Date: 08-2004
Publisher: Elsevier BV
Date: 12-2013
Publisher: Elsevier BV
Date: 03-2022
Publisher: American Geophysical Union (AGU)
Date: 2017
DOI: 10.1002/2016GC006585
Publisher: Elsevier BV
Date: 15-11-2000
Publisher: Society of Economic Geologists
Date: 1998
DOI: 10.5382/REV.11.13
Publisher: Informa UK Limited
Date: 02-2006
Publisher: Elsevier BV
Date: 03-2019
Publisher: Oxford University Press (OUP)
Date: 12-2014
Publisher: Elsevier BV
Date: 09-2016
Publisher: Elsevier BV
Date: 05-2018
Publisher: Elsevier BV
Date: 20-08-2008
Publisher: Elsevier BV
Date: 03-2002
Publisher: Geological Society of America
Date: 02-2009
DOI: 10.1130/GES00179.1
Publisher: Elsevier BV
Date: 12-1995
Publisher: Elsevier
Date: 2019
Publisher: Elsevier BV
Date: 08-2010
Publisher: Elsevier BV
Date: 06-2012
Publisher: Elsevier BV
Date: 10-2014
Publisher: Elsevier BV
Date: 09-2012
Publisher: Elsevier BV
Date: 05-2001
Publisher: Mineralogical Society of America
Date: 20-12-2012
DOI: 10.2138/AM.2013.4179
Publisher: Wiley
Date: 05-2019
Publisher: Mineralogical Society of America
Date: 02-2019
DOI: 10.2138/AM-2019-6733
Publisher: Geological Society of America
Date: 07-2012
DOI: 10.1130/G33064.1
Publisher: Geological Society of London
Date: 05-02-2023
DOI: 10.1144/JGS2018-076
Publisher: Springer Berlin Heidelberg
Date: 2005
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier BV
Date: 09-2013
Publisher: Elsevier BV
Date: 10-2011
Publisher: Pleiades Publishing Ltd
Date: 02-2009
Publisher: Elsevier BV
Date: 05-2016
Publisher: American Geophysical Union (AGU)
Date: 03-2017
DOI: 10.1002/2016GC006681
Publisher: Informa UK Limited
Date: 09-2005
DOI: 10.1071/EG05266
Publisher: American Geophysical Union (AGU)
Date: 10-2012
DOI: 10.1029/2012GC004250
Publisher: Elsevier BV
Date: 08-2013
Publisher: Wiley
Date: 10-2001
Publisher: Elsevier BV
Date: 03-2014
Publisher: Oxford University Press (OUP)
Date: 09-09-2004
Abstract: Laser ablation microprobe data are presented for olivine, orthopyroxene and clinopyroxene in spinel harzburgite and lherzolite xenoliths from La Palma, Hierro, and Lanzarote, and new whole-rock trace-element data for xenoliths from Hierro and Lanzarote. The xenoliths show evidence of strong major, trace element and Sr isotope depletion (87Sr/86Sr ≤ 0·7027 in clinopyroxene in the most refractory harzburgites) overprinted by metasomatism. The low Sr isotope ratios are not compatible with the former suggestion of a mantle plume in the area during opening of the Atlantic Ocean. Estimates suggest that the composition of the original oceanic lithospheric mantle beneath the Canary Islands corresponds to the residues after 25–30% fractional melting of primordial mantle material it is thus significantly more refractory than ‘normal’ mid-ocean ridge basalt (MORB) mantle. The trace element compositions and Sr isotopic ratios of the minerals least affected by metasomatization indicate that the upper mantle beneath the Canary Islands originally formed as highly refractory oceanic lithosphere during the opening of the Atlantic Ocean in the area. During the Canarian intraplate event the upper mantle was metasomatized the metasomatic processes include cryptic metasomatism, resetting of the Sr–Nd isotopic ratios to values within the range of Canary Islands basalts, formation of minor amounts of phlogopite, and melt–wall-rock reactions. The upper mantle beneath Tenerife and La Palma is strongly metasomatized by carbonatitic or carbonaceous melts highly enriched in light rare earth elements (REE) relative to heavy REE, and depleted in Zr–Hf and Ti relative to REE. In the lithospheric mantle beneath Hierro and Lanzarote, metasomatism has been relatively weak, and appears to be caused by high-Si melts producing concave-upwards trace element patterns in clinopyroxene with weak negative Zr and Ti anomalies. Ti–Al–Fe-rich harzburgites/lherzolites, dunites, wehrlites and clinopyroxenites formed from mildly alkaline basaltic melts (similar to those that dominate the exposed parts of the islands), and appear to be mainly restricted to magma conduits the alkali basalt melts have caused only local metasomatism in the mantle wall-rocks of such conduits. The various metasomatic fluids formed as the results of immiscible separations, melt–wall-rock reactions and chromatographic fractionation either from a CO2-rich basaltic primary melt, or, alternatively, from a basaltic and a siliceous carbonatite or carbonaceous silicate melt.
Publisher: Geological Society of America
Date: 08-11-2016
DOI: 10.1130/G38466.1
Publisher: Elsevier BV
Date: 12-2014
Publisher: Springer Science and Business Media LLC
Date: 04-1998
DOI: 10.1007/BF02883644
Publisher: Oxford University Press (OUP)
Date: 08-09-2012
Publisher: Elsevier BV
Date: 2010
Publisher: Elsevier BV
Date: 09-2019
Publisher: Elsevier BV
Date: 12-1995
Publisher: Springer Berlin Heidelberg
Date: 2005
Publisher: American Geophysical Union (AGU)
Date: 07-2003
DOI: 10.1029/2002GC000420
Publisher: Springer Science and Business Media LLC
Date: 28-01-2021
DOI: 10.1038/S41598-020-79739-4
Abstract: Aggregates of corundum crystals with skeletal to hopper morphology occur in pyroclastic rocks erupted from Cretaceous basaltic volcanoes on Mt Carmel, N. Israel. The rapid growth of the crystals trapped volumes of the parental Al 2 O 3 -supersaturated melt phenocrysts of tistarite (Ti 2 O 3 ) in the trapped melts indicate crystallization at oxygen fugacities 6–7 log units below the Iron-Wüstite buffer ( f O 2 = ΔIW − 6 to − 7), induced by fluxes of mantle-derived CH 4 -H 2 fluids. Cathodoluminescence images reveal growth zoning within the in idual crystals of the aggregates, related to the substitution of Ti 3+ in the corundum structure. Ti contents are 0.3 wt% initially, then increase first linearly, then exponentially, toward adjacent melt pockets to reach values 2 wt%. Numerical modelling indicates that the first skeletal crystals grew in an open system, from a moving magma. The subsequent linear increase in Ti reflects growth in a partially closed system, with decreasing porosity the exponential increase in Ti close to melt pockets reflects closed-system growth, leading to dramatic increases in incompatible-element concentrations in the residual melts. We suggest that the corundum aggregates grew in melt/fluid conduits diffusion modelling implies timescales of days to years before crystallization was terminated by explosive eruption. These processes probably operate in explosive volcanic systems in several tectonic settings.
Publisher: Elsevier BV
Date: 2008
Publisher: Elsevier BV
Date: 09-2012
Publisher: Springer Science and Business Media LLC
Date: 29-01-1998
Publisher: Mineralogical Society of America
Date: 05-2021
DOI: 10.2138/AM-2021-7292
Abstract: Silicate melt inclusions (SMI) containing several daughter minerals, residual glass, and a CO2 bubble were analyzed to constrain the composition and evolution of the metasomatic melt present in the upper mantle beneath the Nógrád-Gömör Volcanic Field (NGVF), northern Hungary to southern Slovakia. The SMI were analyzed with a combination of Raman spectroscopy, FIB-SEM, and LA-ICP-MS to identify phases and obtain their volume proportions and major- and trace-element geochemistry. Slicing through the entire volume of the inclusions and collecting geochemical information at each slice with FIB-SEM allowed us to model the 3D appearance of the phases within the SMI and to use this information to calculate bulk major-element compositions. The partially crystallized SMI are hosted in clinopyroxene in a lherzolite xenolith that shows evidence of a metasomatic event that altered the lherzolites to produce wehrlites. Based on bulk compositions, the SMI trapped the metasomatic melt linked to wehrlite formation in the NGVF. The melt is enriched in Fe and has an OIB-like trace-element pattern, which suggests an intraplate mafic melt similar to the host basalt, but with slightly different chemistry. Pre-entrapment evolution and reaction with the lherzolite wall rock produced an intermediate melt composition. Petrogenetic modeling indicates that the melt was generated as a result of a very small degree of partial melting of a garnet lherzolite source. Following entrapment, a volatile bubble exsolved from the residual melt during ascent to shallow depths as suggested by consistent densities of CO2 in vapor bubbles. Small crystals, including sulfates and mica, that formed at the boundary of the bubble and the glass indicate that the exsolved fluid originally contained S and H2O, in addition to CO2.
Publisher: Springer Science and Business Media LLC
Date: 11-1984
DOI: 10.1007/BF00371413
Publisher: Elsevier BV
Date: 11-2007
Publisher: Springer Science and Business Media LLC
Date: 26-11-1996
Publisher: Elsevier BV
Date: 08-2006
Publisher: Informa UK Limited
Date: 08-2008
Publisher: Elsevier BV
Date: 10-2022
Publisher: Elsevier BV
Date: 08-2017
Publisher: Geochemical Society
Date: 2020
Publisher: Elsevier BV
Date: 2001
Publisher: Elsevier BV
Date: 04-2005
Publisher: Elsevier BV
Date: 09-1993
Publisher: Elsevier BV
Date: 10-2020
Publisher: Elsevier BV
Date: 04-2005
Publisher: Elsevier BV
Date: 12-2003
Publisher: Pleiades Publishing Ltd
Date: 12-2010
Publisher: Elsevier BV
Date: 15-07-2006
Publisher: Elsevier BV
Date: 08-2006
Publisher: International Union of Geological Sciences
Date: 06-2021
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier BV
Date: 02-1988
Publisher: Springer Science and Business Media LLC
Date: 03-2015
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier BV
Date: 09-2012
Publisher: Geological Society of America
Date: 09-2010
DOI: 10.1130/G30944.1
Publisher: Elsevier BV
Date: 11-2022
Publisher: Elsevier BV
Date: 08-2006
Publisher: Informa UK Limited
Date: 10-1998
Publisher: American Geophysical Union (AGU)
Date: 04-2021
DOI: 10.1029/2021JB021663
Abstract: Intraplate small‐volume mafic magmatism is spatially and temporally widespread in central and eastern Asia, but the relevant melting dynamics have remained enigmatic. Here, we report Ar‐Ar ages, mineral and whole‐rock compositions on newly found ∼81 Ma l rophyre dykes from central Asia, aiming to constrain the source characteristics and the melting dynamics in this intraplate setting. Mineral chemistry of the l rophyres shows that pre‐emplacement magmas equilibrated at 970–1060°C (probably at the base of the crust) and contained 1.4–2.1 wt% water. The source region of the l rophyres is shown to have H contents equivalent to H 2 O = ∼150 ppm, and to be lithologically heterogeneous with silica‐deficient pyroxenite embedded in peridotite. Because of the thermodynamic complexities involved in calculating melting scenarios with major elements for such mantle domains, we have conducted a grid search with a forward‐modeling methodology that can simulate the adiabatic decompression melting of a lithologically heterogeneous mantle using incompatible trace elements. The modeling results indicate that original melting occurred at a potential temperature of ∼1400°C under a thinned lithosphere (∼70 km, corresponding to a final melting pressure of 2.3 GPa). Combining these conditions with constraints from regional geology and the tectonic history, the l rophyres are inferred to have formed by decompression melting induced by small‐scale asthenospheric upwellings due to the edge effects under a corrugated lithospheric lower boundary. We suggest that this scenario has global relevance and represents a likely mechanism for the initiation of relatively small‐scale intraplate magmatism within continents.
Publisher: Oxford University Press (OUP)
Date: 21-09-2011
Publisher: Elsevier BV
Date: 06-2008
Publisher: Springer Science and Business Media LLC
Date: 08-06-2008
DOI: 10.1038/NGEO226
Publisher: Wiley
Date: 2016
DOI: 10.1111/JMG.12170
Publisher: Elsevier BV
Date: 09-2004
Publisher: Elsevier BV
Date: 02-2000
Publisher: Springer Science and Business Media LLC
Date: 30-07-2014
Publisher: Springer Science and Business Media LLC
Date: 21-11-1995
Publisher: Oxford University Press (OUP)
Date: 06-04-2012
Publisher: Elsevier BV
Date: 12-2009
Publisher: Springer Science and Business Media LLC
Date: 06-2015
Publisher: Mineralogical Society of America
Date: 04-2021
DOI: 10.2138/AM-2020-7347
Abstract: Controversies on the origin of zircon, corundum, titanomagnetite, and quartz megacrysts in alkali basalts mostly reflect the lack of direct evidence of a “melt reservoir” required for their formation. Various mineral megacrysts are carried up by Cenozoic (mostly younger than 25 Ma) alkali basalts that extend more than 4000 km along eastern China. Here we report unusual inclusions in corundum megacrysts from Changle, and we attribute their origin to the existence of a FeO*-SiO2-Al2O3-ZrO2-rich melt. The inclusions, analyzed using electron microprobe and Raman microscopy, may be ided into two types. Type I inclusions are dominated by glassy materials, may exhibit a dark part in backscattered eletron (BSE) images composed of quartz, corundum, and an amorphous substance (AS-1), and a bright part in BSE images composed of baddeleyite and a second distinct amorphous substance (AS-2). Compared with AS-1, AS-2 has higher concentrations of ZrO2 and FeO* but lower concentrations of Al2O3 and SiO2. We argue that the formation temperature of Type I inclusions is ~1200 °C, and the generation of their bright and dark parts in BSE images may be attributed to the coexistence of immiscible melts. Type II inclusions are composed of zircon, quartz, and an amorphous substance (AS-3). Both types of inclusions might be derived from a similar parent melt, which is FeO*-SiO2-Al2O3-ZrO2-rich. New secondary ion mass spectroscopy (SIMS) in situ U-Pb ages of 18 Ma and 13–14 Ma for zircon inclusions suggest that the corundum megacrysts, occurring in basaltic host rocks distributed along the middle segment of the north and south-trending Tanlu fault zone, formed from precursor residual magmas related to underplating basalts stalled at the crust-mantle boundary, and were brought to the surface by entrainment in later basalts. This study provides new insights into the genesis of the corundum-related megacryst suite.
Publisher: Geological Society of America
Date: 2017
Publisher: Elsevier BV
Date: 12-2012
Publisher: Springer Science and Business Media LLC
Date: 22-05-2011
Publisher: Elsevier BV
Date: 11-2020
Publisher: American Geophysical Union (AGU)
Date: 10-2018
DOI: 10.1029/2018JB015520
Publisher: Elsevier BV
Date: 02-2014
Publisher: Springer Science and Business Media LLC
Date: 25-06-2010
Publisher: Elsevier BV
Date: 02-2014
Publisher: Elsevier BV
Date: 10-2018
Publisher: Elsevier BV
Date: 03-2007
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 07-2002
Publisher: Springer Science and Business Media LLC
Date: 20-02-2007
Publisher: Springer Science and Business Media LLC
Date: 09-2006
Publisher: Elsevier BV
Date: 02-1988
Publisher: Oxford University Press (OUP)
Date: 24-07-2020
DOI: 10.1093/PETROLOGY/EGAA079
Abstract: Transformation of refractory cratonic mantle into more fertile lithologies is the key to the fate of cratonic lithosphere. This process has been extensively studied in the eastern North China Craton (NCC) while that of its western part is still poorly constrained. A comprehensive study of newly-found pyroxenite xenoliths from the Langshan area, in the northwestern part of this craton is integrated with a regional synthesis of pyroxenite and peridotite xenoliths to constrain the petrogenesis of the pyroxenites and provide an overview of the processes involved in the modification of the deep lithosphere. The Langshan pyroxenites are of two types, high-Mg# [Mg2+/(Mg2++Fe2+)*100 = ∼90, atomic ratios] olivine-bearing websterites with high equilibration temperatures (880–970 oC), and low-Mg# (70–80) plagioclase-bearing websterites with low equilibration temperatures (550–835 oC). The high-Mg# pyroxenites show trade-off abundances of olivine and orthopyroxene, highly depleted bulk Sr–Nd (εNd = +11·41, 87Sr/86Sr = ∼0·7034) and low clinopyroxene Sr isotopic ratios (mean 87Sr/86Sr = ∼0·703). They are considered to reflect the reaction of mantle peridotites with silica-rich silicate melts derived from the convective mantle. Their depletion in fusible components (e.g., FeO, TiO2 and Na2O) and progressive exhaustion of incompatible elements suggest melt extraction after their formation. The low-Mg# pyroxenites display layered structures, convex-upward rare earth element patterns, moderately enriched bulk Sr–Nd isotopic ratios (εNd = -14·20– -16·74, 87Sr/86Sr = 0·7070–0·7078) and variable clinopyroxene Sr-isotope ratios (87Sr/86Sr = 0·706–0·711). They are interpreted to be crustal cumulates from hypersthene-normative melts generated by interaction between the asthenosphere and heterogeneous lithospheric mantle. Combined with studies on regional peridotite xenoliths, it is shown that the thinning and refertilization of the lithospheric mantle was accompanied by crustal rejuvenation and that such processes occurred ubiquitously in the northwestern part of the NCC. A geodynamic model is proposed for the evolution of the deep lithosphere, which includes long-term mass transfer through a mantle wedge into the deep crust from the Paleozoic to the Cenozoic, triggered by subduction of the Paleo-Asian Ocean and the Late Mesozoic lithospheric extension of eastern Asia.
Publisher: Elsevier BV
Date: 03-2009
Publisher: Elsevier BV
Date: 07-2014
Publisher: Elsevier BV
Date: 04-0004
Publisher: Elsevier BV
Date: 02-2020
Publisher: Elsevier BV
Date: 04-2013
Publisher: Elsevier BV
Date: 07-1998
Publisher: Elsevier BV
Date: 10-2004
Publisher: Elsevier BV
Date: 08-2007
Publisher: Elsevier BV
Date: 04-2009
Publisher: Elsevier BV
Date: 2010
Publisher: Wiley
Date: 05-1991
Publisher: Elsevier BV
Date: 11-2017
Publisher: American Geophysical Union (AGU)
Date: 12-03-2005
DOI: 10.1029/2004TC001652
Publisher: Wiley
Date: 16-06-2020
DOI: 10.1111/TER.12471
Publisher: Virtual Explorer Pty Ltd.
Date: 2003
Publisher: Geological Society of America
Date: 12-04-2011
DOI: 10.1130/B30253.1
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 12-2012
Publisher: Elsevier BV
Date: 04-2020
Publisher: Elsevier BV
Date: 07-2011
Publisher: Springer Science and Business Media LLC
Date: 14-11-2022
DOI: 10.1038/S41467-022-34781-W
Abstract: Decompressional melting of asthenosphere under spreading centers has been accepted to produce oceanic lithospheric mantle with vertical compositional variations, but these gradients are much smaller than those observed from ophiolites, which clearly require additional causes. Here we conduct high-density s ling and whole-rock and mineral analyses of peridotites across a Tibetan ophiolitic mantle section (~2 km thick), which shows a primary upward depletion (~12% difference) and local more-depleted anomalies. Thermodynamic modeling demonstrates that these features cannot be produced by decompressional melting or proportional compression of residual mantle, but can be explained by melt-peridotite reaction with lateral melt/rock ratio variations in an upwelling asthenospheric column, producing stronger depletion in the melt-focusing center and local zones. This column splits symmetrically and flows to become the horizontal uppermost lithospheric mantle, characterized by upward depletion and local anomalies. This model provides insights into melt extraction and uppermost-mantle origin beneath spreading centers with high melt fluxes.
Publisher: Elsevier BV
Date: 12-2007
Publisher: Elsevier BV
Date: 06-2007
Publisher: Mineralogical Society of America
Date: 11-2020
DOI: 10.2138/AM-2020-7375
Abstract: Titanium diboride (TiB2) is a minor but common phase in melt pockets trapped in the corundum aggregates that occur as xenoliths in Cretaceous basaltic volcanoes on Mt. Carmel, north Israel. These melt pockets show extensive textural evidence of immiscibility between metallic (Fe-Ti-C-Si) melts, Ca-Al-Mg-Si-O melts, and Ti-(oxy)nitride melts. The metallic melts commonly form spherules in the coexisting oxide glass. Most of the observed TiB2 crystallized from the Fe-Ti-C silicide melts and a smaller proportion from the oxide melts. The parageneses in the melt pockets of the xenoliths require fO2 ≤ ΔIW-6, probably generated through interaction between evolved silicate melts and mantle-derived CH4+H2 fluids near the crust-mantle boundary. Under these highly reducing conditions boron, like carbon and nitrogen, behaved mainly as a siderophile element during the separation of immiscible metallic and oxide melts. These parageneses have implications for the residence of boron in the peridotitic mantle and for the occurrence of TiB2 in other less well-constrained environments such as ophiolitic chromitites.
Publisher: Mineralogical Society of America
Date: 05-2005
DOI: 10.2138/AM.2005.1706
Publisher: Oxford University Press (OUP)
Date: 03-09-2009
Publisher: Wiley
Date: 20-11-2012
DOI: 10.1111/JMG.12011
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 11-2018
Publisher: Elsevier BV
Date: 08-2006
Publisher: Elsevier BV
Date: 05-2005
Publisher: American Geophysical Union (AGU)
Date: 12-2002
DOI: 10.1029/2002GC000298
Publisher: Elsevier BV
Date: 05-2005
Publisher: Elsevier BV
Date: 2019
Publisher: Elsevier BV
Date: 06-2010
Publisher: Springer Science and Business Media LLC
Date: 30-07-2015
Publisher: Mineralogical Society of America
Date: 06-2016
DOI: 10.2138/AM-2016-5611
Publisher: Elsevier BV
Date: 2013
Publisher: Society of Economic Geologists
Date: 2002
Publisher: Elsevier BV
Date: 03-1995
Publisher: Elsevier BV
Date: 09-2007
Publisher: Geological Society of America
Date: 05-2013
DOI: 10.1130/G34003.1
Publisher: Elsevier BV
Date: 04-2020
Publisher: Elsevier BV
Date: 06-2004
Publisher: Elsevier BV
Date: 02-2006
Publisher: Springer Science and Business Media LLC
Date: 06-10-2013
Publisher: Elsevier BV
Date: 09-2007
Publisher: Elsevier BV
Date: 08-2013
Publisher: Elsevier BV
Date: 10-2016
Publisher: Elsevier BV
Date: 05-2015
Publisher: Elsevier BV
Date: 11-2007
Publisher: Springer Science and Business Media LLC
Date: 07-2006
Publisher: Elsevier BV
Date: 05-2002
Publisher: Elsevier BV
Date: 11-2010
Publisher: Elsevier BV
Date: 07-2007
Publisher: Oxford University Press (OUP)
Date: 30-01-2018
Publisher: Geological Society of America
Date: 17-08-2016
DOI: 10.1130/G37910.1
Publisher: Elsevier BV
Date: 12-2000
Publisher: Geological Society of America
Date: 2008
DOI: 10.1130/G24868A.1
Publisher: Springer Science and Business Media LLC
Date: 13-10-2013
DOI: 10.1038/NGEO1954
Publisher: Springer Science and Business Media LLC
Date: 07-2014
Publisher: Springer Science and Business Media LLC
Date: 13-11-2015
DOI: 10.1038/SREP16484
Abstract: Investigations of the Mantle Transition Zone (MTZ 410–660 km deep) by deformation experiments and geophysical methods suggest that the MTZ has distinct rheological properties, but their exact cause is still unclear due to the lack of natural s les. Here we present the first direct evidence for crystal-plastic deformation by dislocation creep in the MTZ using a chromitite from the Luobusa peridotite (E. Tibet). Chromite grains show exsolution of diopside and SiO 2 , suggesting previous equilibration in the MTZ. Electron backscattered diffraction (EBSD) analysis reveals that olivine grains co-existing with exsolved phases inside chromite grains and occurring on chromite grain boundaries have a single pronounced crystallographic preferred orientation (CPO). This suggests that olivine preserves the CPO of a high-pressure polymorph (wadsleyite) before the high-pressure polymorph of chromite began to invert and exsolve. Chromite also shows a significant CPO. Thus, the fine-grained high-pressure phases were deformed by dislocation creep in the MTZ. Grain growth in inverted chromite produced an equilibrated microstructure during exhumation to the surface, masking at first sight its MTZ deformation history. These unique observations provide a window into the deep Earth and constraints for interpreting geophysical signals and their geodynamic implications in a geologically robust context.
Publisher: Geological Society of America
Date: 2006
DOI: 10.1130/G22725.1
Publisher: Elsevier BV
Date: 08-2020
Publisher: Geological Society of America
Date: 15-10-2019
DOI: 10.1130/B35065.1
Abstract: How new subduction zones form is an ongoing scientific question with key implications for our understanding of how this process influences the behavior of the overriding plate. Here we focus on the effects of a Late Cretaceous subduction-initiation (SI) event in Iran and show how SI caused enough extension to open a back-arc basin in NE Iran. The Late Cretaceous Torbat-e-Heydarieh ophiolite (THO) is well exposed as part of the Sabzevar-Torbat-e-Heydarieh ophiolite belt. It is dominated by mantle peridotite, with a thin crustal sequence. The THO mantle sequence consists of harzburgite, clinopyroxene-harzburgite, plagioclase lherzolite, impregnated lherzolite, and dunite. Spinel in THO mantle peridotites show variable Cr# (10–63), similar to both abyssal and fore-arc peridotites. The igneous rocks (gabbros and dikes intruding mantle peridotite, pillowed and massive lavas, hibole gabbros, plagiogranites and associated diorites, and diabase dikes) display rare earth element patterns similar to MORB, arc tholeiite and back-arc basin basalt. Zircons from six s les, including plagiogranites and dikes within mantle peridotite, yield U-Pb ages of ca. 99–92 Ma, indicating that the THO formed during the Late Cretaceous and was magmatically active for ∼7 m.y. THO igneous rocks have variable εNd(t) of +5.7 to +8.2 and εHf(t) ranging from +14.9 to +21.5 zircons have εHf(t) of +8.1 to +18.5. These isotopic compositions indicate that the THO rocks were derived from an isotopically depleted mantle source similar to that of the Indian Ocean, which was slightly affected by the recycling of subducted sediments. We conclude that the THO and other Sabzevar-Torbat-e-Heydarieh ophiolites formed in a back-arc basin well to the north of the Late Cretaceous fore-arc, now represented by the Zagros ophiolites, testifying that a broad region of Iran was affected by upper-plate extension accompanying Late Cretaceous subduction initiation.
Publisher: Elsevier BV
Date: 04-2021
Publisher: Elsevier BV
Date: 03-2008
Publisher: Elsevier BV
Date: 11-2020
Publisher: Informa UK Limited
Date: 12-1990
Publisher: Elsevier BV
Date: 2013
Publisher: Springer Science and Business Media LLC
Date: 17-09-2008
Publisher: MDPI AG
Date: 18-07-2021
DOI: 10.3390/MIN11070780
Abstract: Titanium oxynitrides (Ti(N,O,C)) are abundant in xenolithic corundum aggregates in pyroclastic ejecta of Cretaceous volcanoes on Mount Carmel, northern Israel. Petrographic observations indicate that most of these nitrides existed as melts, immiscible with coexisting silicate and Fe-Ti-C silicide melts some nitrides may also have crystallized directly from the silicide melts. The TiN phase shows a wide range of solid solution, taking up 0–10 wt% carbon and 1.7–17 wt% oxygen these have crystallized in the halite (fcc) structure common to synthetic and natural TiN. Nitrides coexisting with silicide melts have higher C/O than those coexisting with silicate melts. Analyses with no carbon fall along the TiN–TiO join in the Ti–N–O phase space, implying that their Ti is a mixture of Ti3+ and Ti2+, while those with 1–3 at.% C appear to be solid solutions between TiN and Ti0.75O. Analyses with at% C have higher Ti2+/Ti3+, reflecting a decrease in fO2. Oxygen fugacity was 6 to 8 log units below the iron–wüstite buffer, at or below the Ti2O3–TiO buffer. These relationships and coexisting silicide phases indicate temperatures of 1400–1100 °C. Ti oxynitrides are probably locally abundant in the upper mantle, especially in the presence of CH4–H2 fluids derived from the deeper metal-saturated mantle.
Publisher: Elsevier BV
Date: 03-2016
Publisher: Research Square Platform LLC
Date: 08-12-2021
DOI: 10.21203/RS.3.RS-986686/V1
Abstract: Diamonds are erupted at Earth’s surface in volatile-rich magmas called kimberlites 1,2,3 . These enigmatic magmas, originating from depths exceeding 150 kilometres in Earth’s mantle 1 , occur in stable cratons and in pulses broadly synchronous with supercontinent cyclicity 4 . Whether their mobilization is driven by mantle plumes 5 or mechanical weakening of cratonic lithosphere 4,6 remains unclear. Here we show that most kimberlites spanning the past billion years erupted approximately 25 million years after the onset of continental fragmentation, suggesting an association with rifting processes. Our dynamic models show that physically steep lithosphere-asthenosphere boundaries formed during terminal rifting (necking) generate convective instabilities in the asthenosphere that slowly migrate many hundreds of kilometres inboard of the rift, causing destabilization of cratonic mantle keel tens of kilometres thick. Displaced lithosphere is replaced by hot, upwelling asthenosphere in the return flow, causing partial melting of carbonated mantle and variable assimilation of lithospheric material. The resulting small-volume kimberlite magmas ascend rapidly and adiabatically, exsolving amounts of carbon dioxide (CO 2 ) that are consistent with independent constraints 7 . Our model reconciles diagnostic kimberlite features including association with cratons and geochemical characteristics that implicate a common asthenospheric mantle source contaminated by cratonic lithosphere 8 . Together, these results provide a quantitative and mechanistic link between kimberlite episodicity and supercontinent cycles via progressive disruption of cratonic keels.
Start Date: 2020
End Date: 2024
Funder: Australian Research Council
View Funded ActivityStart Date: 2004
End Date: 2006
Funder: Australian Research Council
View Funded ActivityStart Date: 2009
End Date: 2011
Funder: Australian Research Council
View Funded ActivityStart Date: 2003
End Date: 2003
Funder: Australian Research Council
View Funded ActivityStart Date: 2007
End Date: 2009
Funder: Australian Research Council
View Funded ActivityStart Date: 2014
End Date: 2016
Funder: Australian Research Council
View Funded ActivityStart Date: 2016
End Date: 2016
Funder: Australian Research Council
View Funded ActivityStart Date: 2011
End Date: 2017
Funder: Australian Research Council
View Funded ActivityStart Date: 2002
End Date: 2006
Funder: Australian Research Council
View Funded ActivityStart Date: 2008
End Date: 2011
Funder: Australian Research Council
View Funded ActivityStart Date: 2003
End Date: 2003
Funder: Australian Research Council
View Funded ActivityStart Date: 2008
End Date: 2012
Funder: Australian Research Council
View Funded ActivityStart Date: 2004
End Date: 2006
Funder: Australian Research Council
View Funded ActivityStart Date: 2014
End Date: 2015
Funder: Australian Research Council
View Funded ActivityStart Date: 2007
End Date: 2007
Funder: Australian Research Council
View Funded ActivityStart Date: 2007
End Date: 2010
Funder: Australian Research Council
View Funded ActivityStart Date: 2010
End Date: 2010
Funder: Australian Research Council
View Funded ActivityStart Date: 2013
End Date: 2013
Funder: Australian Research Council
View Funded ActivityStart Date: 2006
End Date: 2006
Funder: Australian Research Council
View Funded ActivityStart Date: 2005
End Date: 2005
Funder: Australian Research Council
View Funded ActivityStart Date: 2007
End Date: 2008
Funder: Australian Research Council
View Funded ActivityStart Date: 2005
End Date: 12-2005
Amount: $495,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2009
End Date: 12-2011
Amount: $397,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2007
End Date: 12-2009
Amount: $151,249.00
Funder: Australian Research Council
View Funded ActivityStart Date: 10-2010
End Date: 12-2012
Amount: $700,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2004
End Date: 12-2006
Amount: $450,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2004
End Date: 06-2007
Amount: $120,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 03-2016
End Date: 06-2019
Amount: $648,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 03-2008
End Date: 09-2013
Amount: $6,000,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2007
End Date: 12-2010
Amount: $690,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2002
End Date: 12-2003
Amount: $190,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2021
End Date: 12-2024
Amount: $375,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 10-2014
End Date: 12-2018
Amount: $474,334.00
Funder: Australian Research Council
View Funded ActivityStart Date: 06-2006
End Date: 06-2007
Amount: $350,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2007
End Date: 12-2011
Amount: $700,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2007
End Date: 12-2010
Amount: $314,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 03-2009
End Date: 06-2012
Amount: $355,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 02-2013
End Date: 12-2015
Amount: $390,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2002
End Date: 12-2007
Amount: $1,355,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2022
End Date: 11-2025
Amount: $490,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2014
End Date: 12-2016
Amount: $3,600,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2003
End Date: 12-2004
Amount: $10,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 06-2011
End Date: 12-2018
Amount: $12,400,000.00
Funder: Australian Research Council
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